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1995 Tectonic Subsidence of the Cretaceous Western Interior Basin, United States. Ming Pang Louisiana State University and Agricultural & Mechanical College
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Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. TECTONIC SUBSIDENCE OF THE CRETACEOUS WESTERN INTERIOR BASIN, UNITED STATES
A Dissertation
Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy
in
The Department of Geology and Geophysics
by Ming Pang B.S., Chengdu College of Geology, 1982 M.S., China University of Geosciences, 1985 May 1995
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Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ACKNOWLEDGMENTS
I would like to express my sincere thanks to members of my dissertation committee,
Dr. Roy Dokka, Dr. Joseph Hazel, Dr. Richard Kesel, Dr. Juan Lorenzo, Dr. C. M.
Molenaar, Dr. Jeffrey Nunn, and Dr. Andrew Schedl, and especially my advisor, Dr.
Dag Nummedal for their interest, encouragement, and constructive criticism.
Dr. Dag Nummedal's guidance was most instrumental to the completion of this
dissertation. Many of the ideas presented in this dissertation came about as the result of
discussions and arguments with him. Because of his careful reviewing and editing, the
structure and clarity of the manuscript has been greatly improved.
Discussions with Dr. Andrew Schedl on many aspects of foreland basins were very
helpful in early stages of this dissertation. Dr. Joseph Hazel taught me the essence of
biostratigraphy and generously provided me his own research results. Dr. Jeffrey Nunn's
knowledge of sedimentary basin mechanisms led to many significant improvements in the
approach taken in this study. Discussions with Dr. Roy Dokka on many occasions were
very constructive to the analysis of the subsidence data. His insights on the tectonics of
foreland basins resulted in improvements in this dissertation. "K" Molenaar helped me in
many ways throughout my work. Much of the subsurface data used in this dissertation
was obtained with his help and guidance at the USGS at Denver. More important, his
expertise and knowledge of the Cretaceous stratigraphy proved most valuable to the
compilation of the stratigraphic data base of my work.
Discussions with fellow students at LSU have also been constructive to this
dissertation. In particular, I recognize with appreciation Drs. Greg Riley, Mark Pasley,
Mr. Xiaogong Xie, and Mr. Mingji Chu for their interest and support of my work.
I would like to thank all those extremely helpful people at the Office of the
Department of Geology and Geophysics, especially Liz Keller and Thea Burchell.
I wish to thank Drs. R. Johnson, K. Franczyk, T. Fouch, and T. Dyman of the
USGS at Denver, each of whom contributed to my dissertation by making available their
ii
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. own research results on the Cretaceous stratigraphy of the Western Interior basin. The
American Association of Petroleum Geologists is thanked for a grant-in-aid.
iii
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. TABLE OF CONTENTS
Acknowledgments ...... ii
List of tables ...... vi
List of figures ...... vii
A bstract...... xi
Chapter
1. Introduction ...... 1 A statement of work ...... 1 The Cretaceous Western Interior basin, a tectonic overview ...... 4 Objectives...... 7 Dissertation structure ...... 8
2. The tectonic framework of the Cretaceous Western Interior basin, U.S.A 10 Introduction ...... 10 Precambrian basins and provinces ...... 11 Archean Provinces ...... 11 Proterozoic basins ...... 14 Late Proterozoic rifting ...... 15 Basement faults ...... 19 Paleozoic orogenies ...... 21 The early Paleozoic passive margin ...... 21 The Antler orogeny ...... 21 The ancestral rocky Mountain deformation ...... 23 Transformation into an active margin ...... 25 The Sevier orogeny ...... 25 Style of deformation ...... 25 Times of movement ...... 27 Magnitude of thrust loads ...... 37 Basement controls on the Sevier thrusting ...... 38 The overlap province and buttressing ...... 38 Inferred buttresses and their consequences ...... 40
3. Stratigraphy of the Upper Cretaceous rocks, the U.S. Western Interior basin ...... 44 Introduction ...... 44 Depositional setting ...... 46 The molluscan biostratigraphic time scale ...... 51 Transgressive-regressive cycles ...... 54 Neocomian to Aptian ...... 57 The Kiowa-Skull Creek cycle...... 57 The Greenhorn cycle...... 60 The Niobrara cycle...... 66 The Claggett cycle ...... 69 The Bearpaw cycle...... 70 Stratigraphic correlations ...... 71 Data...... 71 Correlation method ...... 72 Study interval ...... 73
iv
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. A note on the cross sections...... 74 Regional stratigraphic cross sections ...... 75 Cross sections 1 and 2: western Montana to North and South Dakotas ...... 75 Cross sections 3 and 4: western Wyoming to South Dakota and Nebraska...... 84 Cross sections 5: central Utah to Denver Basin ...... 92 Cross sections 6: Kaiparowits region-San Juan Basin-Raton Basin-Pueblo ...... 99
4. Backstripping analysis ...... 108 Introduction ...... 108 Airy backstripping ...... 109 Flexural unloading sedimen ...... I l l Decompaction of sediment ...... 117 Sea level corrections and the meaning of subsidence ...... 123 Water depth corrections ...... 124 A note on error sources ...... 125 Results...... 126
5. Flexural subsidence and basement tectonics ...... 127 Introduction ...... 127 Previous work ...... 128 Subsidence patterns in space and time ...... 132 Subsidence profiles ...... 132 Subsidence curves ...... 134 Modeling flexural subsidence ...... 136 Model description...... 136 Method ...... 138 Model results ...... 138 A note on the lithosphere’s elastic thickness...... 141 Discussion ...... 144 Complexities of foreland basin subsidence ...... 144 Basement structures and their influences on lithospheric flexure 145
6. Residual subsidence and speculations on its causes ...... 152 Introduction ...... 152 Nature of the residual subsidence ...... 154 Epeirogenic subsidence mechanisms...... 158 Sublithospheric loading and cooling ...... 160 Continental tilting ...... 161 Mantle dynamic topography ...... 164
7. Conclusions ...... 167
References ...... 171
Appendix: Wireline logs used in the stratigraphic cross-sections 1 to 6 ...... 214
Vita...... 218
v
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. LIST OF TABLES
1. Empirical constants in the exponential porosity-depth relationships
vi
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. LIST OF FIGURES
I. The Cretaceous Western Interior Seaway during late Campanian time ...... 3
2 a: Generalized stratigraphic cross section of the Western Interior basin by King (1977). Also shown are tectonic" zones" proposed by Kauffman (1985). 2 b: foreland basin subsidence model ...... 5
3. Precambrian tectonic elements of the North American craton ...... 12
4. Protrozoic basins along the Cordillera. Dashed patterns in northwest part of craton indicate possible extension of craton ...... 13
5. Isopach maps of: a, Precambrian and Lower Cambrian rocks; b, Cambrian, Ordovician, and Silurian rocks ...... 16
6. Inferred crustal profile of the western North American continental margin prior to the initial terrane-accretion in the Late Devonian ...... 17
7. Tectonic subsidence curve showing the early Paleozoic passive margin subsidence history of western North America ...... 18
8. Normal faults and lineaments along the Sevier thrust front or the Cordilleran hingeline ...... 20
9. A generalized stratigraphic crosss section of the Antler foreland basin ...... 22
10. Principal tectonic elements of the Ancestral Rocky Mountain orogeny during Middle and Late Pennsylvanian time ...... 24
II. Sketch map of the Cordilleran region showing the Cretaceous Sevier orogenic belt relative to the Laramide trend and other tectonic elements at the time of the Mesozoic/Cenozoic boundary ...... 26
12. Chart showing the thrust chronology at three segments of the Sevier belt 28
13. Schematic map showing the major structural features of western Montana 30
14. Timing of major thrust faults in the Idaho-Wyoming salient and the contemporaneous uplift and fault in the adjacent foreland ...... 32
15. Generalized tectonic map of the Idaho-Wyoming salient showing the locations and extent of the major thrust faults ...... 33
16. A structural cross section of west-central Utah ...... 36
17. a: Location of the overlap province between the Cordilleran thrust belt and the Rocky Mountain foreland, b: A cross section of the overlap province.. . . 39
18. An interpretative structural block diagram showing the inferred relationship between the Proterozoic Willow Creek fault, the transverse zone, and frontal ramps of the Helena salient ...... 42
vii
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 19. Map showing the extent of the Cretaceous outcrops (shaded) in the U.S. Western Interior ...... 45
20. Map showing the distribution of Laramide structural basins in the U.S. Western Interior ...... 47
21. Generalized map of the Western Interior Seaway during the maximum transgression in the Late Cretaceous ...... 48
22. Restored Cretaceous isopach patterns in the Western Interior, a: Albian through Santonian strata and b: Campanian and Maastrichtian strata. Isopach contours in 1000 ft interval ...... 50
23. Molluscan time scale and reference sequences of the Western Interior Basin 52
24. Late Jurassic to Early Cretaceous correlation chart for parts of the Western Interior basin ...... 55
25. Transgressive-regressive depositional cycles of the North American Cretaceous Western Interior ...... 56
26. Early Cretaceous drainage pattern in the Western Interior ...... 58
27. Generalized stratigraphic section for the Rock Canyon anticline area, northwestern Pueblo quadrangle, Colorado, showing principlal lithologies and zonal fossils of the Dakota, Greenhorn, Carlile, Niobrara, and lower Pierre Shale...... 61
28. Map showing the extent of the Cretaceous Western Interior Sea Ways at three different times...... 62
29. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from northwestern Montana to North Dakota ...... 76
30. Regional stratigraphic cross section 1 of the lower Upper Cretaceous rocks from northwestern Montana to North Dakota ...... 77
31. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from southwestern Montana to South Dakota ...... 78
32. Regional stratigraphic cross section 2 of the lower Upper Cretaceous rocks from southwestern Montana to South Dakota ...... 79
33. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from northwestern Wyoming to South Dakota ...... 85
34. Regional stratigraphic cross section 3 of the lower Upper Cretaceous rocks from northwestern Wyoming to South Dakota ...... 86
35. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from southwestern Wyoming to Nebraska ...... 87
36. Regional stratigraphic cross section 4 of the lower Upper Cretaceous rocks from southwestern Wyoming to Nebraska ...... 88
viii
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 37. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from Uinta to Denver Basins ...... 94
38. Regional stratigraphic cross section 5 of the lower Upper Cretaceous rocks from central Utah to western Nebraska ...... 95
39. Generalized time-stratigraphic correlation chart for Upper Cretaceous strata from Kaiparowits region to Raton Basin ...... 100
40. Regional stratigraphic cross section 6 of the lower Upper Cretaceous rocks from southern Utah to western Kansas ...... 101
41. Illustration and comparison of Airy and flexural backstripping schemes 110
42. Subsidence profiles (b and c) in response to the loading of a sedimentary wedge (a). The wedge represents the real geometry of strata on the regional stratigraphic cross section 5 of this study ...... 115
43. Tectonic subsidence profiles resulting from different backstripping schemes: a. Airy backstripping; b. flexural backstripping ...... 116
44. Exponential porosity -depth relationships used in decompacting the Cretaceous rocks of the Western Interior basin ...... 120
45. Effects of the underlying rocks on results of flexural backstripping. Profile a was obtained by ignoring the compaction of the underlying strata; profile b by decompacting the underlying strata. A siltsone lithology was used in calculations ...... 121
46. Qualitative representation of the flexural responses to loading. Curve 1 depicts flexure resulting from initial emplacement of a load, or an elastic response. Curves 2 and 3 dipict flexure involving viscous relaxation under a constant load ...... 130
47. Flexurally backstripped subsidence profiles across basin ...... 133
48. Temporal subsidence trends at six locations 100-150 km east of the thrust belt... 135
49. Flexural half wave-length as a function of lithosphere's elastic thickness...... 137
50. Best-fitting flexural profiles for the backstripped subsidence profiles across the Wyoming foreland ...... 139
51. Bi-modal distribution of continental lithospheric elastic thickness ...... 142
52. Distribution of continental elastic thickness Te versus age of lithosphere at the time of loading ...... 143
53. Interpretative diagram showing differential crustal shortening as a result of buttressing near Uinta Mt. and in southwestern Montana ...... 147
54. Diagramatic sketch of the paleotectonic blocks during the middle Proterozoic time...... 148
ix
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 55. Spatial variations in the present day lithospheric elastic thickness across parts of Idaho, Wyoming, and Utah ...... 150
56. Diagram illustrating the two main subsidence components in the Western Interior basin: flexural subsidence to the west and residual subsidence over the entire basin ...... 153
57. Eustatic sea level curve (heavy line) of Haq et al. (1988) and predicted sea level curves by Engebreston et al. (1992) using global spreading rate data (dashed lines) ...... 157
58. Vertical continental movements during the past 180 Ma ...... 159
59. Continental tilt model by Mitrovica et al. (1989). A. Schematic illustration of the net effect of Late Cretaceous subsidence and Tertiary uplift across Wyoming. B. The proposed tilting mechanism resulting from subduction and mantle convection ...... 162
60. Diagram showing changes in continental topography relative to sea surface during continental breakup ...... 165
x
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ABSTRACT
The tectonic subsidence history recorded in middle Cenomanian to early Campanian
(96 to 80 Ma) strata in the U.S. Cretaceous Western Interior basin was studied by
applying two-dimensional flexural backstripping techniques to six regional stratigraphic
sections across different segments of the basin. Results indicate that tectonic subsidence
over the 16 m.y. study interval consists of two distinct components: a westward-
increasing flexural subsidence confined within a few hundred kilometers of the thrust
belt, and a spatially uniform "residual" subsidence that affected the entire basin. The
residual subsidence does not represent signals of eustatic sea level changes but instead
reflects epeirogenic movements specific to the North American Western Interior. The
flexural component exhibits significant spatial and temporal variations along the strike of
the Sevier thrust belt. The greatest cumulative subsidence occurred in southwestern
Wyoming and northern Utah, whereas concurrent subsidence in northwestern Montana
and southern Utah was insignificant. Temporal trends in subsidence also show a distinct
regional pattern. From middle Cenomanian to late Turanian (96 to 90 Ma), subsidence
rates were high in Utah and much lower in Wyoming and Montana. In contrast, during
the Coniacian and Santonian stages (90 to 85 Ma) subsidence accelerated rapidly in
Wyoming, increased slightly in Montana, and decreased in Utah. The observed variations
in flexural subsidence were probably manifestations of basement structures, particularly
those zones of crustal weakness inherited from the Precambrian rifting and early
Paleozoic passive margin development.
xi
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 1 INTRODUCTION
A STATEMENT OF WORK
The past three decades have witnessed significant progress in our understanding of
the evolution of sedimentary basins. Plate tectonic concepts, particularly knowledge of
the physics of lithospheric processes, provide an elegant conceptual framework within
which to synthesize formerly separate geological data and comprehend the causes of
sedimentary basins. This theoretical breakthrough together with improved seismic,
gravity, borehole, biostratigraphic, and other geologic data has led to the development of
quantitative geophysical models for a great number and variety of basins. In such
models, basin subsidence history can be predicted according to theories of lithospheric
flexure or thermal cooling. In conjunction with backstripping techniques for data
reduction, the models have served as a powerful analytic tool furnishing valuable insights
into the tectonic mechanisms of various basins.
Foreland basins are distinct asymmetrical depressions coupled with orogenic belts.
Our understanding of these basins has been greatly enhanced by the use of quantitative
models (e.g., Stockmal et al., 1986; Beaumont et al., 1987). These models consider the
evolution of foreland basins as a result of lithospheric flexure under the loading of
orogenic belts. Such models have been used to predict foreland basin subsidence history,
or inversely, to extract information on the kinematics of orogenic belts or the attributes of
the lithosphere from basin stratigraphic records. In recent years, the burgeoning interest
in foreland basins and unprecedented computing capabilities have lead to the development
of highly integrated stratigraphic models (Flemings and Jordan, 1990; Jordan and
Flemings, 1991; Sinclair et al., 1991; Jervey, 1992). In these models, the kinematics of
orogenic belts, the resultant lithospheric flexure, sea level changes, and sedimentation
and erosion are all coupled together as independent variables that interact to determine the
1
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 2
stratal stacking pattern and facies distribution. To field geologists, these models promise
to provide a theoretical framework to guide observations of particular stratigraphic,
sedimentologic, and structural expressions that are otherwise hidden or difficult to
comprehend.
As attention focused on the development of quantitative foreland basin models,
however, inadequate efforts went into collecting geologic data to document basin
subsidence history and patterns. More often than not, quantitative models are developed,
but their viability and geologic relevance go unchecked. The models, though impressively
capable in predicting particular stratal architectures, appear to be outstripping the data
needed to calibrate and test them. Unless deliberate efforts are taken to address this
discrepancy, further progress in developing realistic basin models will be hindered.
This dissertation is an effort pointed toward bridging the gap between foreland basin
models and observations. It focuses on the regional tectonic subsidence history and
mechanisms of the U.S. Western Interior basin during the Cretaceous Period (Fig. 1).
Although arguably one of the best understood foreland basins in the world, the Western
Interior basin has not been systematically studied with respect to its subsidence history on
sufficiently large spatial and refined temporal scales. Hence, many attributes and
complexities of this 'classic' foreland basin remain poorly understood. The overall
objective of this dissertation is to document basin subsidence history as preserved in the
stratigraphic record across different parts of the basin so that relevant basin models can be
evaluated. To achieve this, a regional stratigraphic data base was first compiled by
integrating a large amount of surface and subsurface stratigraphic data from the U.S.
Western Interior. Then, flexural backstripping techniques were applied to extract the
tectonic subsidence history from this stratigraphic data base. On the basis of this
documentation, possible tectonic mechanisms of basin formation and evolution were
evaluated. Results of this study present significant new data and insights into the tectonic
control on the development of the Western Interior basin. Beyond the immediate concern
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ,___ ARCTIC OCEAN
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Figure 1. The Cretaceous Western Interior Seaway during late Campanian time From Gill and Cobban (1973).
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 4
on this basin, these results are also of value in the generation of more realistic models in
the future.
THE CRETACEOUS WESTERN INTERIOR BASIN, A TECTONIC OVERVIEW
The interior of western North America was occupied by a large epeiric seaway during
much of the Cretaceous (Fig. 1). At its peak, the seaway connected the Arctic ocean and
the Gulf of Mexico, a longitudinal distance of more than 5,000 km, and reached a width
of 1,000 km or more. Lithofacies deposited proximal to the Cordilleran fold and thrust
belt on the western side of the basin are composed of intertonguing non- and marginal
marine sandstone and marine shale, and those on the eastern platform of the basin are
dominated by marine limestones and shale.
The Western Interior basin is an excellent locale for understanding the coupled
relationships between tectonic factors and foreland basin development (Price, 1973;
Bond, 1976; Kauffman, 1977a; Cross and Pilger, 1978; Cross, 1986; Beaumont, 1981;
Jordan, 1981; Heller et al., 1986; Mitrovica et al., 1989; Gumis, 1990). There are two
important reasons for this. First, there are abundant biostratigraphic and lithostratigraphic
data for the Western Interior basin. These data have made the Western Interior basin a
fertile ground for the development and testing of many stratigraphic as well as
sedimentologic concepts (Kauffman and Caldwell, 1993). Secondly, the structures in the
Cordilleran fold and thrust belt are fairly well preserved for direct observational
information (Armstrong, 1968; Price, 1973; Royse et al., 1975). Therefore, information
on the styles of thrusting and amount of crustal shortening can be integrated into foreland
basin models.
Many plausible models bearing directly or indirectly on the Western Interior basin
have been proposed. In general, they emphasize in different manner the roles of tectonic
loading, sublithospheric processes, eustatic, and sedimentary factors. Figure 2 is a
generalized stratigraphic cross section accompanied by a simple illustration of a foreland
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. LA -IOWA- 3 0 0 0 m Stable Eastern Platform □ Marineshale Limestoneand chalk NEBRASKA JCANSAS AND. ********** A kAAAAAAAAAA kAAAAAAAAAA A A] AAAAAAAAAAA AAAAAAAAAAA A] _6l sandstone Fox H illsss Marine/coastal "HingeZone": Moderate Subsidence i mudstone Non-marine -COLORADO- Zoneof High Subsidence Non-marine Conglomerate [Frontier Fi Foreland Basin Foreland Fill Flexural Subsidence Belt Zoneof Max. Subsidence ^_^.Thrust -UTAH- tectonic zones"" proposed by Kauffman (1985). 2 b: foreland basin subsidence model. Figure 2 a: Generalized stratigraphic cross section ofthe Western Interioirbasin by King (1977). Also shown are b a
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 6
basin model. Price (1973) first hypothesized that the Western Interior foreland basin
resulted from isostatic flexural subsidence in response to the vertical loading of
supracrustal rocks tectonically thickened by thrusting. This mechanical linkage between
basin and thrust belt was subsequently tested in the framework of quantitative
lithospheric flexural models by Jordan (1981) and Beaumont (1981). Their models
demonstrated that the asymmetrical stratigraphic architecture observed within a few
hundred miles of the thrust belt can be explained by lithospheric flexure. Since then,
these models have served as a useful guide to understanding the tectonic control on
foreland basin stratigraphy in the Western Interior and other basins.
Despite the impact of these studies, a growing body of evidence suggests that the
Cretaceous Western Interior basin can only be partially described by flexural models. For
example, the basin is much wider than the flexural depressions predicted by any model.
This anomaly is reflected in nearly 1 km of Cretaceous rocks deposited in the cratonic
interior, as far as 1000 km away from the Sevier thrust belt (Fig. 2 a). Lithospheric
flexure under thrust loading, unaccompanied by additional mechanisms, can not explain
such a broad basin dimension. Finding a viable complementary tectonic mechanism has
not been an easy task. Furthermore, previous studies have essentially treated flexural
mechanisms of the Western Interior foreland basin as a two-dimensional case. Although
this generalization is a reasonable first order approximation, its usefulness beyond the site
of observational controls is questionable. Recent studies of foreland basins have
documented that spatial variations in the flexural subsidence may be the norm rather than
the exception (Waschbusch and Royden, 1992).
Drawing on the general lithofacies pattern of the observed basin fill and foreland
basin models, Kauffman (1985) proposed that spatial variations in basin subsidence
divided the Western Interior basin into a series of longitudinal zones (Fig. 2 a). These
zones occur from west to east in the following order: a western foredeep zone of
maximum subsidence, a west-median trough of high subsidence, an east-median hinge of
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 7
moderate subsidence, and an eastern platform of low subsidence. Because of its
speculative nature, however, this characterization of the spatial subsidence pattern has yet
to be corroborated by quantitative subsidence and detailed stratigraphic data.
Cross (1986) provided a regional synthesis on the development of the Cretaceous
Western Interior basin in the context of Farallon Plate subduction beneath North America
Plate. He suggested that lithospheric flexure by thrust loading was most effective in the
early phase of the basin subsidence history during early Late Cretaceous. With the onset
of low-angle subduction of the Farallon Plate in the Late Cretaceous, Cross (1986)
argued, a broad downwarping centered in Wyoming and Colorado occurred in response
to sublithospheric loading and cooling, which dominated over the lithospheric flexure
caused by thrust loading.
Although these and other works collectively enhanced our understanding of the basin,
a coherent explanation of basin development that can accommodate separate facets of the
basin stratigraphy and tectonic setting remains elusive. The quest for such a
comprehensive model demands a thorough and accurate understanding of basin
subsidence history.
OBJECTIVES
The first objective of this dissertation is to provide an improved documentation of the
subsidence history of the Western Interior basin in both spatial extent and temporal
refinement, a step that is long overdue. To do this, two-dimensional flexural
backstripping techniques were applied to six regional stratigraphic cross sections
extending east-west across the basin from Montana and North Dakota to southern Utah
and New Mexico. These sections were constructed with subsurface data and
biostratigraphically calibrated with outcrop megafossil data. The approach and scope
taken here enables sampling of the temporal and spatial variations in basin subsidence on
many different scales.
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 8
The second objective of this dissertation is to explore the tectonic mechanisms of the
observed subsidence in the framework of foreland basin models. The objective consists
of two parts. First, tectonic subsidence observed in the foreland area is evaluated both
quantitatively in terms of an elastic lithospheric flexural model and qualitatively in the
context of basement tectonics. This provides a perspective on the spatial and temporal
significance of lithospheric flexure and thrust loading in the Western Interior basin.
Secondly, with the flexural subsidence identified and separated, th e" residual"
component of subsidence observed in the eastern cratonic interior can then be evaluated.
This regional subsidence component, indistinguishable from a eustatic sea level rise if
considered in isolation, has long been overlooked in previous studies. In view of this,
this study demonstrates its significance to the development of the Western Interior basin
and suggests that it may originate in the dynamic topographic effects of mantle convection
and subduction.
DISSERTATION STRUCTURE
This dissertation consists of seven chapters including this introductory chapter.
Chapter 2 provides a literature review of the tectonic history of the western North
American craton from the Precambrian to the Tertiary. Attention is focused on the tectonic
events and processes that shaped basement heterogeneity, and the styles and timing of
thrusting during the Cretaceous. This information is essential for discussion of flexural
subsidence and its relation to the basement and thrust tectonics. Chapter 3 describes the
stratigraphic data base as well as the procedures used in constructing the regional cross
sections. Chapter 4 discusses the concepts and application of backstripping techniques.
The procedures of two-dimensional flexural backstripping techniques are discussed with
reference to the Cretaceous stratigraphic data. Chapter 5 presents an analysis of the
flexural subsidence both in terms of lithospheric flexural models and in the context of the
basement and thrust tectonics. Chapter 6 discusses the pattern of the platform subsidence
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. and its probable causes. Conclusions are given in Chapter 7. The seven chapters
complement each other and present a coherent analysis of the subsidence history of the
Cretaceous Western Interior basin.
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CHAPTER 2
THE TECTONIC FRAMEWORK OF THE CRETACEOUS WESTERN INTERIOR BASIN, U.S.A.
INTRODUCTION
Prior to the development of the Cretaceous Western Interior basin, the western North
American continent had been shaped by a succession of distinct tectonic episodes dating
back to the Precambrian. In highly generalized terms, these include early Proterozoic
crustal accretion in southwestern U.S., late Proterozoic rifting, early Paleozoic passive
margin development, middle Paleozoic accretionary tectonics, Pennsylvanian-Permian
Ancestral Rocky Mountain deformation, and the early Mesozoic transformation into an
active margin. Each episode brought about profound changes in the tectonic regime and
depositional setting. Tectonic features acquired in an earlier episode commonly persisted
to exert influence on subsequent tectonic and sedimentary patterns.
Fundamentally, the Cretaceous Western Interior basin is a consequence of the
accelerated sea floor spreading and subduction in the late Mesozoic following the break
up of Pangaea. Subduction of the Farallon Plate beneath the North American Plate
initiated a north-south trending orogenic belt, the Cordillera fold-thrust belt. The Western
Interior basin was formed in response to the crustal shortening and loading by this b elt.
Though a direct consequence of Mesozoic orogenic loading, the Western Interior
basin was also affected by older tectonic features such as the geometry of basement
trends and faults/lineaments inherited from the latest Proterozoic rifting. Therefore,
analysis of the Cretaceous subsidence history requires knowledge of the pre-existing
tectonic conditions. This chapter provides a literature review of the tectonic history of the
western North American continent as it evolved from Precambrian to the late Mesozoic.
In composing this review an effort was made to maintain the continuity of the tectonic
history as presented. However, emphasis was placed on those aspects thought to be of
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greatest relevance to the Cretaceous subsidence history. Essentially, they include
basement structural features that had persistent effects on Phanerozoic sedimentation and
the styles and timing of thrusting in different sectors of the Sevier belt.
Because of the enormous scope and intrinsic complexity of this subject, much of the
discussion is stripped to bare essentials and, inevitably, certain important views or
references on a particular issue may be overlooked. Limited as it is, this document
provides an independent source of constraints for subsequent analysis of subsidence
data.
PRECAMBRIAN PROVINCES AND BASINS
Archean Provinces
The Phanerozoic sedimentary cover of the North American Western Interior is
underlain by Precambrian metamorphic and plutonic rocks that comprise several
lithotectonic provinces (Fig. 3). The nuclei of these provinces are generally considered to
have been separate Archean microcontinents, which were gradually assembled into a
coherent craton during the Early Proterozoic by collisional orogens and by crustal
accretion along their margins (Bickford, 1988a; Hoffman, 1989; Reed et al., 1993). The
Wyoming Province, which includes parts of Wyoming, Montana, eastern Idaho, and
northernmost Utah, is one of the oldest and largest Precambrian provinces in the U.S. It
is bordered to the east by the Superior Province and to the north by the Heame Province.
The boundary between the Wyoming and Superior Provinces is an Early Proterozoic
collisional zone that extends across North and South Dakota. This boundary is known as
the Trans-Hudson orogen or the Dakota mobile belt (Bickford, 1988a). The boundary
between the Wyoming and Heame Provinces is concealed from direct observation, but it
is inferred to be a northeast-southwest trending Early Proterozoic crustal discontinuity
named the Great Falls tectonic zone (Hoffman, 1989). South of the Wyoming Province,
in Colorado, southern Nebraska, Kansas, and New Mexico, basement rocks are early
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. VN»
-GFi SUPERIOR^',/. * * t * **rmMS±t kr^
Archean greenstone 2.3-2.1 Ga 2.0-1.8 Ga 1.9-1.8 Ga granite-gneiss provinces Juvenile(?) crust thrust-fold belts Juvenile crust
2.0-1.8 Ga ].8-1.6Ga 1.3-1.0 1.1 Ga magmatic arcs Juvenile crust imbricated crust continental rift
Figure 3. Precambrian tectonic elements of the North American craton. BH, Black Hills inlier; CH, Cheyenne belt; GF, Great Falls tectonic zone; KR, Keweenawan rift; THO, Trans-Hudson orogen; VN, Vulcan tectonic zone. Archean rocks are undifferentiated. Modified from Hoffman (1989).
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. //////✓✓////✓✓XX// //////////////////////// ////✓✓/////////////////////////✓ ✓///////✓////////////✓////////✓/////// ///////////////✓////✓/✓//./✓/✓//////// //// //////✓//////✓////////////✓✓/✓/////////// //////////////////////////////// ///////✓///////✓///✓/////// ////////////✓ ////// //////////// /////
N orth
American///i
~ ^ [ates
Craton
Figure 4. Protrozoic basins along the Cordillera. Dashed patterns in northwest part of craton indicate possible extension of craton. From Harrison et al. (1974).
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 14
Proterozoic in age. These rocks have been interpreted as arc-affiliated oceanic rocks
accreted to the Archean Wyoming Province during the early Proterozoic (Bickford,
1988b; Hoffman, 1989; Tonnsen, 1986). The boundary between the Wyoming Province
and these younger, accreted Proterozoic rocks is a major crustal discontinuity or suture
zone, named as the Cheyenne belt (Duebendorfer and Houston, 1986,1987).
Proterozoic basins
During the Middle Proterozoic, widespread extensional tectonics attenuated the crust
along the western margin of the Heame and Wyoming Provinces and resulted in several
large Proterozoic basins (Fig. 4; Harrison et al., 1974; Link, 1993; Hoffman, 1989;
Tonnsen, 1986). Strata deposited in these basins range in age from 1.8 Ga to 0.8 Ga,
including the Belt Supergroup, Big Cottonwood Formation, Uinta Mountain Group,
Grand Canyon Supergroup, and the Apache Group (Link et al., 1993).
The Belt basin, which extends from southern British Columbia to the Snake River
plain, accumulated some 18 km of fine-grained, quartz-rich, clastic sediments and
subordinate carbonates. These sediments are mostly Middle Proterozoic in age and are
collectively known as the Belt Supergroup. The southernmost part of the basin extended
inland into central Montana, forming the Helena embayment or rift system (Winston,
1986; Oldow, 1989). Southwest of the Belt basin in central Idaho was a major
Proterozoic landmass referred to as the Belt Island (Ruppel, 1986). The Belt basin has
been interpreted to have formed on attenuated Archean crust in an intracratonic rift
(Winston, 1986) or remnant back-arc basin setting (Hoffman, 1989).
In northern Utah, the Proterozoic Uinta Basin (Uinta trough or aulacogen) developed
in close contemporaneity with the Belt basin. The basin fill strata, named the Uinta
Mountain Group or Big Cottonwood Formation, are Middle or early Late Proterozoic in
age (Link, 1993; Hoffman, 1989). The Uinta Mountain Group is found only in
northeastern Utah, where it consists of up to 7 km of quartzites and shale and lies
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 15
unconformably on the early Proterozoic metasediments. These quartzite-rich sediments
form the core of the Uinta Mountain today. Immediately to the west in the Wasatch
Mountains, the Big Cottonwood Formation consists of as much as 4 km of more
metamorphosed quartzites and shale. Sediments of the Uinta Mountain Group and Big
Cottonwood Formation outline a west-east trending aulacogen located near the western
extension of the Cheyenne belt (Fig. 3 and 4).
Late Proterozoic rifting
The Late Proterozoic marked a period of intensified continental rifting before the
development of a passive margin in the early Paleozoic. Sedimentary rocks of this age are
fairly extensive in Canada, as represented by the Windermere Group, but only
sporadically preserved in the U.S. (Stewart, 1972; Stewart and Poole, 1974; Hoffman,
1989; Link et al., 1993). These rocks consist mainly of immature glaciogenic elastics and
volcaniclastics marking episodic rifting events. They form a narrow, westward
thickening belt along the west margin of the North American craton (Fig. 5a).
Toward the end of the Proterozoic, a continental fragment was rifted away from the
western margin of the North American craton during the breakup of the Proterozoic
supercontinent (Stewart, 1972; Armin and Mayer, 1983; Bond and Kominz, 1984). This
rifting event resulted in a passive margin that persisted virtually uninterrupted until the
Devonian (Fig. 6). Figure 7 is a tectonic subsidence curve by Kominz and Bond (1991)
showing the subsidence history of the Western U.S. from Cambrian to Pennsylvanian
time. This curve depicts the thermal subsidence on a newly developed passive margin.
The boundary between the attenuated passive margin crust and the cratonic crust
defines an important tectonic feature, the Cordilleran hingeline (Fig. 6; Picha, 1986;
Picha and Gibson, 1985; Allmendinger et al., 1987,1986). The Cordilleran hingeline
largely coincides with the much younger Sevier thrust front in Utah (Allmendinger et al.,
1987,1986). West of the hingeline, late Proterozoic and Paleozoic strata thicken
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'-"V"
t—
-----1
j — 100 200 300 mi 300 Km
Figure 5. Isopach maps of: a, Precambrian and Lower Cambrian rocks; b, Cambrian, Ordovician, and Silurian rocks. Contours are in feet. From Stewart (1972).
Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. HINGELINE' '^CONTINENTALCRUST \\\ \ N\ NS\\\\\\S\\\ N\ \ \\\ Nevada WEDGE'~~~x~~ X v v v R I F T STAGE CRUST ,,S///////////mOGE Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. oo 250 PERM. 300400 350 450 ORDOVICIAN SEL. DEVONIAN MISS PENN. 500 CAMBRIAN 550 Ma “ - 5 0 0 - NorthAmerica. Thecurve is representative ofnorthern Utah. From Kominz andBond (1991). Figure 7. Tectonic subsidencecurve showing the early Paleozoic passive margin subsidence history ofwestern 1500 - 1000 2000 meters Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 19 markedly, whereas east of it, platform sedimentation accompanied by subdued tectonic activities prevailed through much of the Phanerozoic (Fig. 5a and b). Basement faults The normal faults associated with the latest Proterozoic rifting and those associated with the earlier Belt basin development shaped the geometry of the Precambrian basement in the western North America. Most of these faults were formed at high angles to the Cordilleran hingeline (Fig. 8), creating promontories and embayments along the passive margin strike (Kulik and Schmidt, 1988). During the late Mesozoic Sevier orogeny, these old passive margin promontories and embayments might have been an important factor controlling the style and orientation of the thrust belt (Kulik and Schmidt, 1988; Allmendinger et al., 1983). The faults themselves also served as long-lived crustal fractures that were periodically reactivated during the Phanerozoic to affect the lithofacies and thickness patterns of sediments deposited nearby. A few such structures are particularly noteworthy. In Montana, the east-west trending Perry (Willow Creek) and Garnet faults along the periphery of the Helena embayment were periodically reactivated to influence not only Paleozoic and Mesozoic sedimentation, but also the formation of lateral thrust ramps during the Sevier orogeny (Harrison et al., 1974; Fryxell and Smith, 1986; Winston, 1986; Peterson, 1986; Kulik and Schmidt, 1988; Wallace et al., 1990). In northern Utah, the boundary-normal faults of the Proterozoic Uinta trough marked the western extension of the Cheyenne belt. These faults were intermittently active during the Proterozoic and Paleozoic, affecting the sedimentation on opposite side of the faults (Bruhn et al., 1986; Bryant and Nichols, 1988). In the Tertiary, however, they were tectonically inversed into reverse faults creating the Uinta Mountain (Gries, 1983). In central Utah, Picha and Gibson (1985) and Picha (1986) identified not only a major north-south trending Precambrian normal fault, the Ancient Ephraim Fault, but also four other northeast- and east-trending lineaments Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ~~1— Lineaments or normal faults of probable Precambrian age Lineaments or faults of Mesozoic age 100 200 miles Figure 8. Normal faults and lineaments along the Sevier thrust front or the Cordilleran hingeline. Modified from Kulik and Schmidt (1988) and Picha and Gibson (1985). 1: Lemhi Arch; 2: Lewis & Clark lineament; 3: Transverse zone; 4: Ancestral Cache Creek fault; 5: Uinta trough margin faults; 6: Leamington lineament; 7: Scipio lineament; 8: Cove Fork lineament; 9: Paragona lineament; 10: Ancient Ephraim fault. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 21 (Fig. 8). These lineaments were interpreted to be zones of crustal weakness associated with the latest Proterozoic rifting. They were reactivated as tear faults in the late Mesozoic to sever the continuity of the Sevier thrust belt. PALEOZOIC OROGENIES The early Paleozoic passive margin The passive margin setting initiated by the latest Proterozoic rifting became well established in the early Paleozoic. From the Cambrian to the Devonian, sedimentation on this passive margin proceeded largely uninterrupted with deposition of extensive clastic and carbonate shelf sediments. These sediments assume the form of an elongated, westward-thickening wedge subparallel to the Cordilleran hingeline (Fig. 5b; Peterson and Smith, 1986). Contemporaneous tectonic activities in the cratonic interior were insignificant; the only known large-scale structure is the Transcontinental Arch, a northeast-southwest trending paleotopographic high that was most evident from the early Paleozoic sedimentation patterns (Sloss, 1988). The Antler orogeny In Middle Devonian time, a volcanic arc formed offshore and migrated toward the western North American passive margin (Speed et al., 1988). In Early Mississippian time, oceanic rocks of the Roberts Mountains allochthon, derived from this arc, were emplaced eastward over the continental shelf of the Paleozoic passive margin. This event, widely known as the Antler orogeny, marked the advent of accretionary tectonics in western North America (Poole, 1974; Dickinson, 1977; Nilsen and Stewart, 1980; Speed and Sleep, 1982; Dorobek et al., 1991). In response to the tectonic loading of the emplaced allochthon, an elongated foreland basin parallel with the Cordilleran hingeline was formed by lithospheric flexure on the former passive margin (Speed and Sleep, 1982). On the gentle, eastern side of the foreland basin near the Cordilleran hingeline, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. to to EAST BASIN W1LLISTON Big Snowy Group 5;W 5;W o W Madison Ls gSfif 3 SHELF CRATONIC Mission Canyon Ls LOWER SHELFMARGIN Lodgepole Ls MIOGEOCLINE CORDILLERAN I 50 km White Knob & MonroeCanyon Ls M cGowanCreek Fm Middle Canyon Fm IDAHO I MONTANA 300 m Figure 9. A generalized stratigraphicModified fromcrosss Rose section (1976). ofthe Antler foreland basin. UPPER SHELF MARGIN ANTLER HIGHLAND WEST Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 23 fine-grained clastic and carbonate sediments dominated (Fig. 9). On the steep, western part of the basin, coarse clastic sediments shed from the rising Antler highland rest on outer shelf or slope facies of the early Paleozoic passive margin. Subsidence analysis by Dorobek et al. (1991) indicates that the flexure across the Antler foreland basin was complicated by differential subsidence associated with the reactivation of Precambrian faults/lineaments. Specifically, isopach maps and sections across Idaho and western Montana indicate that the subsidence across the basin was highly variable, exhibiting apparent reversals of basement movement at different times. The locations of major troughs in the Antler foreland coincide largely with the Precambrian faults/lineaments, suggesting that the crustal heterogeneity inherited from Precambrian tectonics played an important role in distorting the Antler flexural subsidence pattern. The Ancestral Rocky Mountain deformation From Late Mississippian through Pennsylvanian time, tectonic activities propagated from the plate boundary into the cratonic interior. This intracratonic tectonic interval, limited to the accreted early Proterozoic crusts in Colorado, Utah and adjacent areas, is referred to as the Ancestral Rocky Mountains deformation (Fig. 10; Kluth, 1986). The dominant tectonic elements are uplifts bounded by high-angle faults of both normal and reverse types, some of which had Precambrian ancestry (Stevenson and Baars, 1986). The main uplifts are the Uncompahgre and Front Range highlands, and the major basins include the Paradox and Central Colorado troughs. The origin of the Ancestral Rocky Mountains deformation has been difficult to decipher chiefly because much of the evidence for its existence, severely overprinted by the Laramide orogeny, has been derived from stratigraphic studies (Oldow et al., 1989). Eardley (1962) hypothesized that the Ancestral Rocky Mountains deformation was related to the coeval collisional tectonics in the Ouachita Mountains. Kluth and Coney (1981) and Kluth (1986) further suggested that this tectonic episode probably took place in a transpressional tectonic regime driven Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. m m Apishipa Highland TOl w y . Arkose ^ » rafA Evapontes 200 mi I I 200 km Figure 10. Principal tectonic elements of the Ancestral Rocky Mountain orogeny during Middle and Late Pennsylvanian time. From Lindsey et al. (1986), modified from Mckee et al. (1975). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 25 by the continental collision between South and North American. Regardless of its exact cause, there is little doubt that as a result of the Ancestral Rocky Mountains deformation the basement rigidity was further weakened by its block faulting along pre-existing or new faults/lineaments. Transformation into an active margin In Late Permian time, another volcanic arc was migrating from offshore toward the North American plate. In Early Triassic time, arc-affiliated oceanic rocks of the Golconda allochthon were emplaced eastward across the continental shelf of the Nevada continental margin and onto the earlier Roberts Mountains allochthon. This is the so-called Sonoma orogeny. Unlike the Antler orogeny, the Sonoma orogeny generated no conspicuous foreland basin on the cratonic side (Speed and Sleep, 1982). Following the Sonoma orogeny, the western margin of the North American continent began a dramatic reorganization. An active margin was formed in Late Triassic time. From that time to the Late Cretaceous, over a span of 100 m.y., east-dipping subduction proceeded along this active margin in a manner analogous to many modem subduction zones (Atwater, 1989). THE SEVIER OROGENY Style of deformation As a result of the convergence between the North American and Farallon plates in the late Mesozoic, a north-south trending fold-thrust belt, the Cordilleran orogenic belt, was formed inland of the Sierra Nevada-Klamath volcanic arc on the western margin of the North American craton (Fig. 11). The U.S. part of the Cordillera is referred to as the "Sevier orogenic belt" (Armstrong and Oriel, 1965; Armstrong, 1968; Beutner, 1977). The eastern front of the Sevier belt follows closely the Cordilleran hingeline or "the Wasatch Line" of Utah (Allmendinger et al., 1983; Cross, 1986; Picha, 1986; Kulik and Schmidt, 1988). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. •?77?77i7i .*.• .*.• . • .* ,• .* ,• .* .< . ,*;• .*;• .*;• . •*. *v. • .*.*•.*;• •.*. •.*. •/. .*;• • .• •: *••• •: •.* ■. Major late Mesozoic //VA, ‘V** batholiths(Sierra Nevada ■*« /.* .**•. and Klamath arcs) 0 • ••• •.*’ ••• v> \% «.V *.• *•.*•..* »/Mrf>T7Vf'.V v' V ; •;.*V / / ' •«*, • *, • *, • •*, v ,« *. •*.*. ■*.*. •*. »v. •'*. • ••• •. ;:*V>vy/:.:y>y;y;y,‘v-v. v«.v;^v**v^v^/.'V./.v •v. ., *.*. •' •. .* % • V; V.« ».’• V; *.'• V>V/ *•••;.v • •*.* • •• •*.* .*.• •*.• .*.• .%• • •V. •/.• .*-* .*.* .*,• *.*• «.*• •/. •}. ■.*. •’.* •*.* •*.*. *. •/.• .*A >. *. • *.*• *.■ .*:• Laramide uplifts 500 km Figure 11. Sketch map of the Cordilleran region showing the Cretaceous Sevier orogenic belt relative to the Laramide trend and other tectonic elements at the time of the Mesozoic/Cenozoic boundary. From Dickinson and Snyder (1978). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 27 The Sevier belt is characterized by east-vergent thrusting and folding in the Paleozoic and Mesozoic sedimentary cover above gently west-dipping ddcollements in weak horizons (Armstrong, 1968; Armstrong and Oriel, 1965; Royse et al., 1975; Royse, 1993; Wiltschko and Dorr, 1983). Thrust sheets cut successively younger rocks as they moved eastward along the dgcollements. Generally, the youngest thrust is structurally the lowest and closest to the foreland. Multiple episodes of thrusting and folding led to progressive eastward-directed crustal shortening in excess of 100 km in many places across the orogenic belt (Elison, 1991). The shortening was accommodated entirely within the sedimentaiy cover by displacement along stair-step thrust faults, by folding of thrust plates, or by internal shortening in sedimentary rocks (Wiltschko and Dorr, 1983). Because decollements separate the shortened sedimentary rocks above from the undeformed crystalline basement below, this style of deformation has been widely referred to as the 'thin-skinned' in contrast to the 'basement-involved' Laramide tectonic style that characterized the latest Cretaceous-early Tertiary foreland (Cross, 1986). Times o f Movement Thrusting along the Sevier belt proceeded through time in a discrete, sequential manner (Fig. 12). The initial thrusting probably occurred between latest Jurassic and Early Cretaceous. A recent estimate by Heller et al. (1986) based on subsidence analysis placed the initial thrusting as late as Aptian age. Despite this ambiguity, thrusting was probably in full progress by Late Cretaceous time along the Sevier belt. Possible exceptions may exist in western Montana, where no unequivocal evidence exists to indicate so (Ruppel and Lopez, 1984). Overall, thrusting remained active throughout the Late Cretaceous and well into the Tertiary, a period of more than 50 m.y. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. N> 00 Hollow Smoky ; Canyon :fy/; w id e Pm North North £ w South £ [vGroup ;VvV [vGroup CodyShale W. WYOMING ...*.■ M esavetde Fra ,W.* %’• S**\\\',\ ,W.* %’• .jwGamet Thrusts Thrusts m m Limestone •. » • . : •. .*». shorn Fm sandstone and conglomerate Conglomerate Unconformity Q aggett Shale ’V* V* V*V«V» V»V*i*. V»V*i*. V*V«V» V* ’V* - .VA-.V.V.V.-.vT’ JudithRiver fin ^ North £ ^ South W. MONTANA Shale m nonmanne Marineand Nonmarine sandstone Silicious Thrusts Aptian Albian Turanian Barremian Coniacian Santonian Campanian Cenomanian Maastnchian SP=Sapphire, GH= Grasshopper, EH=Elkhom, P=Paris, M=Meade, C=Crawford, A=Absaroka, D=Darby, CR= Canyon thepossible duration ofthrustinga event. Generalizedbasin stratigraphy eachat segment is shownin west-east trending cross-sectional columns. Compiled from authors mentioned Abbreviationsthein text. for thrusts: ML= Medicine Lodge, Range, PI andP2=Pavant, P&G=Paxton and Gunnison. Figure 12. Chart showing the thrust chronology atthree segments ofthe Sevierbelt. The length the blockof barrepresents 80 90 70 120 110 Ma 100 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 29 Montana: The fold and thrust belt in western Montana is broken up into three segments by the east-west trending Lewis and Clark Lineament and the Transverse Zone (or the Perry Line; the Willow Creek Fault) (Fig. 8 and 13; Schmidt et al., 1988; Eldredge et al., 1988). These lineaments represent zones of crustal weakness inherited from the Precambrian Belt Basin. They were reactivated intermittently since then and eventually became tear faults during the development of the Sevier belt (Ruppel and Lopez, 1984; Kulik and Schmidt, 1988). North of the Lewis and Clark Lineament is a series of thrust faults collectively known as "Disturbed Belt" (Mudge, 1970). These thrusts were emplaced from west to east in early Tertiary time, equivalent in age to the easternmost thrust faults in the Idaho-Wyoming salient, such as the Darby thrust (Mudge and Earhart, 1980). The cumulative horizontal displacement across the Disturbed Belt is estimated at between 60 - 80 km (Mudge and Earhart, 1980). Between the Lewis and Clark Lineament and the Transverse Zone is the Helena Salient, where two major thrust systems are recognizable: the Sapphire to the west and those curved thrusts in the Helena Salient to the east, such as the Lombard thrust (Fig. 13). Movement on the Sapphire thrust is estimated to be Santonian to early Campanian in age, with a total displacement of 50 - 65 km (Ruppel et al. 1981; Ruppel and Lopez, 1984; Mudge and Earhart, 1980; Elison 1991). The Lombard thrust lying to the east of the Sapphire thrust is dated roughly as Campanian to Maastrichtian (75-73 Ma) (Cross, 1986). South of the Transverse Zone, structural relationships of the east-directed thrust faults become even more complex. The added complexity stems from involvement of the foreland basement (Kulik and Schmidt, 1988). Ruppel (1978) and Ruppel et al. (1981, 1984) mapped two major thrust systems and many associated imbricate thrust faults in southwestern Montana: the Grasshopper thrust system, which is structurally lower and younger, and the Medicine Lodge thrust system, which is structurally higher and much Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. o WYOMING HELENA EMBAYMENT TransverseZone Plate K Snake RiverPlai CANADA MONTANA Boulder Batholith^ J J > ite ite f Grassh Sapphire Idaho '%'Batholith Idaho Batholith too 50 km LO IDAHO Snowcrest Uplift. Modified from Schmidtet al. (1988) and Kulikand Schmidt (1988). Figure Schematic13. map showing the majorstructural features ofwestern Montana. BSU is Blacktail Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 31 larger (Fig. 13). Movements on individual thrusts of the two thrust systems are poorly dated. According the postulated age of the synorogenic conglomerates of the Beaverhead Formation presumably derived from these thrusts, Ruppel and Lopez (1984) inferred that thrust movements could span the entire Late Cretaceous. However, a new palynological study of the Beaverhead Formation suggests that thrusting in southwestern Montana did not begin until early Campanian (Nichols et al., 1985, see the correlation chart by Johnson and Sears, 1988, p. 232). Ruppel and Lopez (1984) considered the Grasshopper thrust system to be partially equivalent to the Sapphire thrust system to the north. Wvominp-Idaho: The timing of Sevier thrusting is better constrained in the Idaho and Wyoming salient, where several discrete episodes of thrusting, ranging in age from Late Jurassic to early Eocene, have been recognized and dated over the years (Fig. 12,14; Armstrong and Oriel, 1965; Royse et al., 1975; Wiltschko and Dorr, 1983; Oriel and Armstrong, 1986; Coogan, 1992; DeCelles et al., 1993). The Sevier thrust belt in Idaho-Wyoming-Utah forms a broad, eastward-convex salient that is 320 km long and 100 km wide (Fig. 15). From west to east, in order of progressively younger ages, the major thrusts are: Paris, Meade-Crawford, Absaroka, Hogsback- Darby, and Prospect. These thrusts have been studied in great details by many authors with respect to the timing and the amount of crustal shortening (Armstrong and Oriel, 1965; Jordan, 1981; Wiltschko et al., 1983; Oriel and Armstrong, 1986). As a result, their movements are the best understood along the entire Sevier belt. The Paris thrust of southeastern Idaho has the longest history of movement (Fig. 12, 13). Its initial movement is indicated by the synorogenic conglomerates in the late Jurassic lower Ephraim Formation of the Gannet Group. Marine mollusks have been reported in the lower, pre-orogenic Ephraim Formation. These, along with other evidence Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. to East West 120 140 100 80 40 ■60 Albian A ptian Eocene Santonian T uranian Paleocene C oniacian N eocom ian C am panian Maastrichtian C enom anian JURASSIC and fault in the adjacent foreland. Modified from Oriel and Armstrong (1986) and Craddock, Kopania, and Figure Timing14. ofmajor thrust faults in the Idaho-Wyoming salientand the contemporaneousuplift Wiltschko (1988). ! i Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 7T77 ------VTeton Range £Snake ^River w (% Gros Ventre ^Plain Range \ \V (Jackson'4A/s‘\\ gj Quaternary and Tertiary volcanic rocks □ Precambrian rocks Thrust fault SO km 'Kemmerer Coalville Salt Lake City Figure 15. Generalized tectonic map of the Idaho-Wyoming salient showing the locations and extent of the major thrust faults. Modified from Oriel and Armstrong (1986). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 34 reviewed by Armstrong and Oriel (1965), date the initial movement of the Paris thrust as latest Jurassic/early Cretaceous time. Subsequent movements on the Paris thrust are also indicated by deposition of several other synorogenic clastic wedges described in their paper. The Paris thrust dies out southward in northern Utah, where the Willard thrust has been considered its equivalent (Royse et al., 1975). However, Bryant et al. (1988) pointed out that the Willard thrust may connect with the younger Meade thrust. The cessation of the Paris thrusting is poorly constrained because the oldest sedimentary rocks above the Paris fault trace are of Pliocene age. Nevertheless, the major movements on the Paris thrust probably occurred in the early Cretaceous (Wiltschko and Dorr, 1983). Directly east of the Paris thrust are the Meade and the Crawford thrusts (Fig. 15). The traces of the two thrusts occupy the same structural and stratigraphic position, and therefore they have been considered as two segments of one thrust system (Royse et al., 1975). Closely related as they were, however, estimates of their timing of movement differ. Based on palynologic data and interpreted ages of the synorogenic clastic deposits, the initial movement on the Meade thrust was estimated to be either of Albian (Oriel and Armstrong, 1986) or Coniacian age (Wiltschko and Dorr, 1983), and that on the Crawford thrust Coniacian or earliest Santonian age (Jacobson and Nichols, 1982; Wiltschko and Dorr, 1983). Recently, a reexamination of the Meade and the Crawford thrusts by DeCelles et al. (1993) suggests that the Meade thrust is part of the Paris thrust, unrelated to the Crawford thrust. They argued that the initial Meade thrusting occurred in Aptian time. Cessation of the Meade and the Crawford thrusting is less certain because the oldest rocks overlying them are of Miocene-Pliocene age. Nevertheless, structural analysis suggests that the Meade and Crawford thrusts were followed by the Absaroka thrust, which is fairly well dated as late Campanian or earliest Maastrichtian in age (Jacobson and Nichols, 1982). Given these data, it is reasonable to assume that the Meade and Crawford thrusts spanned the Aptian to Santonian interval with little temporal Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 35 overlapping by immediately adjacent thrusts. This interpretation places the Meade and Crawford thrust system largely contemporaneous with the Greenhorn and Niobrara cycles (see Chapter 3). Central Utah: The Sevier thrust belt continues southwestward into Utah, where it displays structural styles similar to those in the Idaho-Wyoming salient. In part because of erosion, post- Cretaceous tectonic overprints, and burial by derivative sediments, the Sevier thrusts in Utah were for a long time poorly documented and dated. As a result of subsurface drilling, seismic profiling, coupled with surface mapping and detailed sedimentologic analysis, a succession of major thrust faults have been recognized in west-central Utah and occasionally dated (Royse, 1993; Villien and Kligfield, 1986; Lawton, 1985; Allmendinger et al., 1986; Armstrong 1968; Heller et al.; 1986). Elsewhere in Utah, much work is needed to identify and map the distribution of Sevier thrust faults. The major thrust faults in west-central Utah, in progressive sequential order, are: the Canyon Range, Pavant, Paxton, and Gunnison thrusts (Fig. 16). Total, cumulative crustal shortening on these thrust faults is about 120 km (Royse, 1993). Because structurally well-juxtaposed synorogenic clastic wedges are not abundant and reliable paleontologic data are rare, most of these thrust faults are not well dated. Generally, they range from Early Cretaceous (Albian) to middle Eocene (Heller et al., 1986). In west-central Utah, the earliest and structurally highest thrust is the Canyon Range thrust (Allmendinger, 1986; Royse, 1993). Its movement is recorded by the synorogenic conglomerates in the Lower Cretaceous Cedar Mountain Formation (Lawton, 1986), or the Canyon Range Fanglomerate (Armstrong, 1968). Palynomorphs collected from the lower part of the Canyon Range Fanglomerate on the Gunnison Plateau yielded an age between Neocomian and Albian (Standlee, 1982). This suggests that the Canyon Range thrust was broadly contemporaneous with the Paris-Willard thrust to the north. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. n O Plateau Wasatch AncientEphraim A ult 20km TK TK P-TR : p z V i - l • ///////////////// Pavant Range R Hraore Arch u t :L_-PZ. PVT. Mountains Cricket .in'; CRX p z - l •■ Canyon Range P ts Figure 16. A structural cross section ofwest-central Utah. P' s= Proterozoic sediments; LPz= lowerPaleozoic; P-TR= upperPaleozoic and Triassic; J=Jurassic; K= Cretaceous; PVT=Pavant Range Thrust; PAX= Paxton thrust;the locationsG= Gunnison ofwells thrust. used Vertical in constructing lines are the cross section. Modified fromRoyce (1993). TK= lowerTertiary andUpper Cretaceous; UT= upperTertiary; CRT= Canyon RangeThrust; PEs UT House Range PCs L-PZ P-TK ‘ Range Confusion 10 k m Cross section Cross Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 37 According to the estimate by Royse (1993), displacement on the Canyon Range thrust is about 50 km. East of the Canyon Range thrust is the Pavant thrust (Fig. 16), which Villien and Kligfield (1986) inferred had two separate phases of movement. The early phase of the Pavant thrust is recorded by synorogenic conglomerates equivalent to the Sanpete Formation. Palynomorphs collected from these rocks suggest an age between late Albian and Turanian time. The late phase of the Pavant thrust is recorded by synorogenic conglomerates interpreted as being equivalent to the Sixmile Formation, which Fouch et al. (1983) assigned a late Santonian to early Campanian age by correlations with better dated strata in the distal foreland. The ages of the synorogenic conglomerates, though somewhat tenuous, date the movements on the Pavant thrust roughly as Late Cretaceous. The Paxton and Gunnison thrusts occurred in the latest Cretaceous (Royse, 1993). Their movements were probably recorded by the widespread conglomerates of Campanian to Maastrichtian age found throughout central Utah. However, because of lack of precise age constraints, the initiation and cessation of their movements are essentially uncertain. Magnitude of thrust loads Viewed as a single tectonic entity, the Sevier belt can be characterized as an east- tapering wedge of sedimentary rocks migrating inland along the west-dipping decollements above the passive basement crystalline rocks. Crustal shortening across the thrust belt amounted to 200 km in the Canadian Rockies and 100 to 150 km in the U.S., where the smaller shortening may have been counterbalanced in the foreland by the Laramide orogeny (Elison, 1991). Crustal shortening, and therefore vertical thickening, generates supracrustal loads that require isostatic balance by lithospheric flexure in the foreland (Barrell, 1914; Price, 1973). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 38 A useful reference for the magnitude of the supracrustal load is available from the southern Canadian Rockies, where a supracrustal wedge more than 370 km wide and up to 15 km thick was horizontally shortened by more than 50 percent (Price, 1973). More detailed work on the crustal shortening was carried out by Jordan (1981) in the Idaho- Wyoming salient. On the basis of seismically controlled structural cross sections (Royse et al., 1975), she reconstructed the amount of excess mass associated with the Paris, Meade-Crawford, and Absaroka thrusts, respectively. The Paris thrust amounted to a relatively small and narrow crustal load, 30 km wide and 1.5 km thick. The Meade- Crawford thrust system was a substantially larger thrust load. It is up to 100 km wide and over 4 km thick. BASEMENT CONTROLS ON THE SEVIER THRUSTING The Overlap Province and buttressing Toward the end of the Cretaceous and continuing into the early Tertiary, widespread basement faulting occurred in the Western Interior foreland basin. This tectonic style, named the Laramide orogeny, is characterized by deep-rooted reverse faults. The Laramide orogeny ended the domination of the thin skinned Sevier thrusting and eventually broke the Western Interior foreland basin into the Laramide structural basins and intervening uplifts in their present form (Cross, 1986; Dickinson et al., 1988). Initially, the Sevier and Laramide orogenies were considered as two contrasting styles of deformation that were partitioned in two distinct provinces and succeeded each other in time (Armstrong, 1968). Subsequently, however, it was found that the Laramide deformation and Sevier thrusting partly overlapped in time (Armstrong, 1974; Wiltschko and Dorr, 1983; Cross, 1986; Dickinson et al., 1988). Still later, it was found that in addition to the temporal overlap, the two tectonic styles developed in tandem since at least the middle Late Cretaceous in a so called "overlap province" (Fig. 17; Schmidt and Perry, 1988). Although the precise tectonic mechanisms of both the Sevier and Laramide Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. VO foreland RockyMountain Overlap Province .Sevier thrust belt. Figure a: 17. Location oftheoverlap province between Cordilleran the thrustbelt andthe Rocky Mountainb: foreland,Across section ofthe overlap province. Arrowscrustal indicate shortening. From Kulikand Schmidt (1988). 100 200 miles Major faults ofthe Rocky Mountain foreland ■Overlap Province Sevier thrust front ----- T a I I Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 40 orogenies still remain controversial, there is a growing consensus that they were not mutually exclusive of each other in either spatial or temporal domains. The overlap province refers to a north-south elongated region 100 to 150 km wide along the Cordilleran hingeline, where zones of crustal weakness inherited from the Precambrian were concentrated (Fig. 8,17; Kulik and Schmidt, 1988). The interactions between the thin-skinned thrusting and coeval basement uplifting in this region took place primarily in the form of buttressing (Schmidt and Perry, 1988). Buttressing involves impingement of eastward-advancing thrust sheets against uplifted basement blocks or other pre-existing basement irregularities, such as the inferred basement promontories and embayments along the Cordilleran hingeline (Beutner, 1977, Schmidt et al., 1988, Kulik and Schmidt, 1988). The complex alternating reentrants and salients along the strike of the Sevier belt have been attributed to buttressing (Beutner, 1977, Couples and Lewis, 1988). Perhaps more important, buttressing against pre-existing basement irregularities could be an effective mechanism of generating along-strike variations in crustal shortening, which may find expressions in the foreland basin subsidence patterns (Craddock et al., 1988, Beutner, 1977). Below is a description of those structures that have been mentioned as candidates for buttressing of coeval thrusting. Inferred buttresses and their consequences Along the length of the Sevier belt from Montana to Utah, thrust sheets were emplaced onto basement rocks that display different degrees of complexity (Fig. 8). In the Idaho-Wyoming salient, Sevier thrusting progressed on a gently westward-dipping stable platform established since Precambrian time (Picha, 1986). North and south of the Idaho-Wyoming salient, in contrast, Sevier thrusting progressed across complexly faulted margins of the North American craton inherited from Precambrian continental rifting (Skipp, 1988; Picha, 1986). These basement variations determined to a large extent the distribution of buttressing. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 41 The Blacktail-Snowcrest uplift in southwestern Montana provides a well documented case of buttressing (Fig. 13). Structural as well as stratigraphic evidence suggests that this basement-cored uplift, though spatially restricted, was active as early as Coniacian time (Nichols et al., 1985; Ryder and Scholten, 1973). It has been suggested that because of this and nearby buttresses, the contemporaneous eastward Sevier thrusting was restrained, leading to the formation of the southwestern Montana reentrant (Beutner, 1977; Perry et al., 1988). Northeast of the Blacktail-Snowcrest uplift, the formation of the Helena salient might also be the result of buttressing (Beutner, 1977; Kulik and Schmidt, 1988; Schmidt et al., 1988). The Helena salient is connected to the reentrant to the south by the Willow Creek fault zone or Transverse zone, which was probably the southern boundary fault of the Proterozoic Belt basin. Schmidt et al. (1988) developed a lateral thrust ramp model for the thrust styles in the Helena salient (Fig. 18). North of the Transverse zone in the Helena salient, a ddcollement was developed deep within the Proterozoic sedimentary rocks of the Belt basin and thrusts progressed to the east and up. South of the Transverse zone, in contrast, the Archean crystalline rocks acted as a buttress to thrust propagation. Paleomagnetic data obtained near the Helena salient have documented local rotations of thrust sheets along the margin of the salient possibly due to buttressing (Eldredge and Van der Voo, 1988). Evidence for buttressing also exists in the ancestral Teton-Gros Ventre uplift in northwestern Wyoming (Fig. 15). This tectonic feature was inferred to be uplifted along the Cache Creek thrust contemporaneously with the early phase of Sevier thrusting during Coniacian time (Kulik and Schmidt, 1988), or even Albian time (Craddock et al., 1988). As thrust sheets approached from the west, buttressing by this uplift may have caused the deflection of thrust sheets away from the uplift initiating rotations of frontal thrusts (Craddock et al., 1988). Paleomagnetic data obtained near the Teton-Gros Ventre uplift have documented rotations of rocks presumably in response to this buttressing (Hunter, 1988; Eldredge and Van der Voo, 1988). Structural analysis by Craddock et al. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Figure 18. An interpretative structural block diagram showing the inferred relationship between the Proterozoic Willow Creek fault, the transverse zone, and frontal ramps of the Helena salient. From Schmidt et al. (1988). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. (1988) also indicate that thrust displacements on the Paleocene-Eocene Prospect and Darby thrusts increase toward the south, away from the Teton-Gros Ventre uplift. Farther south, in northern Utah, deflections of thrusts around the western edge of the Uinta Uplift has been interpreted as a result of buttressing by relatively rigid quartzites deposited in the Proterozoic Uinta trough (Beutner, 1977). However, the same structural pattern has been explained by post-thrusting bending effects (Crittenden, 1969). In other words, the apparent deflection patterns of thrusts in question is due to subsequent erosion following the doming of the Uinta Uplift in the Tertiary. Because of these basement buttresses, eastward thrust translation along the Sevier thrust belt was not uniform. In the case of the Idaho-Wyoming salient, more thrust translation occurred between the Uinta trough in the south and the ancestral Teton-Gros Ventre uplift and the uplifts in the southwestern Montana foreland to the north. As a result, the Idaho-Wyoming salient was the site where disproportionally greater crustal shortening was accommodated. The implication of this thrusting style to basin subsidence is discussed in Chapter 5. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 3 STRATIGRAPHY OF THE UPPER CRETACEOUS ROCKS, THE U.S. WESTERN INTERIOR BASIN INTRODUCTION Cretaceous rocks comprise one of the most important systems in the North American Western Interior. They represent highly diverse marine and nonmarine facies, many of which contain a rich fossil record. They host many types of economically valuable deposits such as coal, oil, gas, and uranium. During the Tertiary Laramide orogeny, many areas in the Western Interior were uplifted, resulting in extensive outcrops across the Rocky Mountains and many areas of the Great Plains (Fig. 19). Most Cretaceous rocks, however, are buried in the subsurface of the Tertiary Laramide structural basins that were once part of the much larger Cretaceous Western Interior foreland basin. Because of economic and academic interest, Cretaceous rocks have been studied extensively by generations of geologists with respect to their sedimentary characteristics, paleontologic records, and regional stratigraphic relationships. These studies augmented the exploration activities in the region, which in turn provided studies of the Cretaceous rocks with a steady input of subsurface data. As a result of the extensive studies and prolonged exploration activities, an enormously large body of stratigraphic data has accumulated over time. This includes wireline logs, seismic sections, outcrop litho- and biostratigraphic sections, subsurface cross sections, and numerous publications devoted to the study of Cretaceous rocks. This body of data not only makes the Western Interior basin a thoroughly explored region with respect to economic resources but also ranks it as one of the world's best studied foreland basins that provides many textbook examples for stratigraphic analysis. The abundant litho- and biostratigraphic data available in the Western Interior basin present an excellent opportunity for restoring basin subsidence history. This study 44 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Bismarck [Hot Spings Rawlins] K cm m crcr North Platte • Denver I G ran d ] Junction C edar C it' 0 100 200 300 km Figure 19. Map showing the extent of the Cretaceous outcrops (shaded) in the U.S. Western Interior. Oblique hatches denote uplifted Precambrian basement rocks. From Cobban and Reeside (1952a). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 46 applied two-dimensional flexural backstripping techniques to six regional stratigraphic cross sections crossing different parts of the basin, from Montana and the Dakotas to Utah and New Mexico (Fig. 20). Each cross section, portraying lateral changes in stratal thickness and lithofacies, was compiled by integrating subsurface and surface stratigraphic data. The stratigraphic interval emphasized on the sections is the "middle Cretaceous" or in more formal terms, the lower part of the Upper Cretaceous succession. This chapter reviews the Cretaceous stratigraphy and describes the stratigraphic data base that supports the subsequent flexural backstripping analysis. The first half of this chapter provides a brief overview of the depositional setting, biostratigraphic framework, and the transgressive-regressive cycles. Because of the scope of the subject, this review is highly generalized and by no means complete. The second half of this chapter describes the regional stratigraphic cross sections and the specific procedures and data that were used to compile them. Discussion focuses on the major lithologic units involved, age-diagnostic fossils, and chronostratigraphic correlations along the length of the cross sections. DEPOSITIONAL SETTING Rapid sea floor spreading and subduction during the Cretaceous led to the flooding of a sizable portion of the world’s continental areas (Hays and Pitman, 1973; Kominz, 1984). As part of this flooding, the North American craton underwent the largest marine incursion since the Paleozoic and developed a large western interior epeiric seaway (Fig. 21). The Cretaceous Western Interior seaway, as it is commonly called, was confined between the Cordilleran fold and thrust belt to the west and the drainage divide of the low-relief cratonic interior to the east. At times of maximum flooding, it connected the Arctic ocean and the Gulf of Mexico, a longitudinal distance of more than 5000 km, and reached a width of 1000 km or more in many places (Williams and Stelck, 1975). Toward the end of the Cretaceous, this marine basin was brought to an end by the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. — I— -T- 110 "TI5 100 95 -50 50- ^ T \ Willistoti M*"01 Devils Lake \ Great Falls Bismarck -4 5 Billings Livingston 4 5 - heridan •Hot Spmgs Rawlins Kemmc North Platte Lincoln . 4 0 - Denve Junction d arC it Wichita Pueblo Durango Trinidad Flagstafr Santa Fc 0 100 200 300 km 110 105 190 — I— JL Figure 20. Map showing the distribution of Laramide structural basins in the U.S. Western Interior. The east-west trending lines numbered from 1 to 6 are the locations of the regional stratigraphic cross sections compiled in this study. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ARCTIC OCEAN M£*lC0 \\cpj, r ? 500 1000 miles Sand and silt Dark gray muds: Pure carbonate Impure clayey deposits: nearshore offshore muds: offshore carbonate muds: offshore Figure 21. Generalized map of the Western Interior Seaway during the maximum transgression in the Late Cretaceous. From Kauffman (1977a). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 49 withdrawal of marine water and by the onset of the Laramide orogeny, which broke the basin apart and created numerous uplifts and intervening structural basins (Dickinson and Snyder, 1978; Cross, 1986). Great quantities of clastic sediments were shed into the seaway from the rising Cordilleran highlands and deposited in shallow marine and nonmarine environments (Fig. 21). Easterly-derived clastic sediments are less significant and restricted to the easternmost part of the cratonic platform and most has been removed by Tertiary erosion. Lithofacies proximal to the Cordillera were composed of intertongued non/marginal- marine sandstone and marine shale. Towards the east, these predominantly shallow marine clastic deposits become finer and thinner, eventually grading into relatively uniform calcareous shale or carbonate-dominated sediments deposited in open marine environments on the broad cratonic platform. Overall, the basin fill thickness assumes a distinctive asymmetrical foreland basin pattern, varying from as much as 5000 meters proximal to the thrust belt to a few hundred meters or less in the Great Plains (Fig. 22). In contrast to a passive continental margin setting, the Cretaceous Western Interior seaway represents a foreland ramp type depositional setting (Nummedal et al., 1989), where the bathymetry was shallow and gentle. In this depositional setting, sediments deposited in the seaway are predominantly of shallow marine origin. However, partly because of lack of a modem analog for such a basin, the precise water depth has been difficult to determine. Attempts have been made to estimate water depth on the basis of the distribution of benthic Foraminifera (Eicher, 1969), reconstruction of depositional clinoform topography (Asquith, 1970), physical evidence for shelf, slope, and basin models ( Weimer, 1983), and sedimentologic model (Kauffman, 1969; 1977a; Hattin, 1975). The consequent estimates of maximum water depth vary considerably, from a high of 600 meters (Eicher, 1969; Asquith, 1970) to a low of 100 to 300 meters (Kauffman, 1969, 1977a; Hattin, 1975; Weimer, 1983). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. o T - > 4 - n- outcrops Limitof UK 300 ml 300 km j ----- i andb: Campanian andMaastrichtian strata. Isopachcontours in 1000 ft interval. From Cross andPilger (1978). Figure 22. RestoredCretaceous isopachpatterns in theWestern Interior, a: Albian through Santonian strata ! i i ! Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 51 Episodic contractions and expansions of the seaway left a cyclic stratigraphic record in the basin. The cycles occur on varied temporal and spatial scales, ranging from those major transgressive-regressive depositional cycles that are recognizable over much of the basin to individual sandstone/mudstone tongues that represent episodes of local strandplain progradation and retreat (Weimer, 1962; McGookey et al., 1975; Kauffman, 1977b; Peterson, 1977; Molenaar, 1983; Ryer, 1977,1993). The typical lithostratigraphic units and the age-diagnostic fossils of the five major transgressive- regressive cycles are discussed later in this chapter. THE MOLLUSCAN BIOCHRONOSTRATIGRAPHIC SCALE The Cretaceous rocks of the North American Western Interior have one of the most refined biostratigraphic systems among the Mesozoic rocks around the world. This system is based primarily on rapidly evolving molluscan lineages, in particular ammonites and various groups of bivalves. Based on several decades of stratigraphic and systematic paleontologic research by many workers, such as W. A. Cobban, over 70 thoroughly tested molluscan biozones have now been established for the Upper Cretaceous series alone (Fig. 23; Cobban, 1993; Obradovich, 1993). These molluscan biozones offer exceptional chronostratigraphic resolution and reliability. Moreover, the Cretaceous rocks of the Western Interior contain numerous volcanic ash beds useful for radiometric dating, and numerical ages have been assigned to many of these biozones. Using single crystal Ar40 /Ar39 dating techniques, Obradovich (1993) obtained over 30 closely-spaced radiometric ages from volcanic ash beds in the Upper Cretaceous sequence of the Western Interior. These radiometric age data, which commonly have an analytical error bar of less than 0.5 m.y., allow the molluscan biozones of the Western Interior to be calibrated quantitatively (Kauffman and Caldwell, 1993). A standard reference sequence for the Upper Cretaceous rocks of the U.S. Western Interior is shown on Figure 23. This particular sequence is largely based on rock Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reference Sequences, U. Cretaceous Ammonite zones Western Interior, U.S.A. Stages Eastern Colorado -M — Scaphitcs Ic c i- 32 Desmoscaphites baaleri TT _33„Dcsmosc ophites erdmonni .Santonian 85- -Clioscaphitcs chotcaucnsis M 35 Clioscaphitcs vcrmiformis Smoky Hill Shale Mbr 36 Clioscaphitcs saxitonianus u 37 Scaphitcs dcprcssus Coniacian- M- -48—Scaphitcs ventricosua- Corresponding bivalve 39 Scaphites preventricosus Fort Hays *40“ Forreslcria peruana ------39 Inoceramusdcformis Limestone Mbr 41 S. corvcnsis, P. germari “42™Scaphitcs nigricollensis" Unnamed Shale Mbr ^>Ir»occramus pciplexus 43 Scaphites whitfiddi -u- 4 ) “54” Scaphites fcrroncnsis *«3 Juana Lopez Mbr 45 Scaphitcs warreni 90 ^>Inoccram us dimidius CO 46 Prionocyclus macombi 4 6 ' £ ^ Codell Ss Mbr -47— Prionocyclus hyatli ------j^M ytiloides mytiloidci Blue Hill Shale Mbr 48 Prionocyclus pcrcarinatus <3 Turanian M' U Fairport Shale Mbr ,4a__ColIignoniccras woollgari 50 Mammites nodosoidcs i Bridge Creek 51 Vascoccras birchbyi 4 $Neocardioccrasjuddii- 52 Pscudaspidoccras flcxuosum R Limestone Mbr 53 Watinoccrasdcvoncnsc x: 5 4 "Nigcriccras 8 Vascoccras diartiamim 56 Burroccras clydenae u 57 Euomphaloccras septcmacriatum ^ ______Duvcnganoccras conaitum a Dunveganoccras aJbcrtcnsc Hartland Shale Mbr Dunveganoceras problcmaticum Dunveaanoceras oondi Lincoln Mbr Plctriacanthoccras wvomingcrc 95 Acamhoccrasbcucnse Acanthoccras muldooncnsc Acamnoccras grancroscnsc M Cenomanian Conlinoccrasgilbcrti _____ Graneros Shale 52 Watinoccrascoloradocnsc 55 v > Sciponoceras gracile 5 9 ' 69 Ncogastroplites macicami 55 ^ Pycnodontc ncwbcrryi 70 Ncogastroplitesamcricanu Mowry Shale 7T Ncogastroplites mucllcri ^M elolcoccras mosbyense „22,..Ncoga J Sandstone 100 Albian "74,MInoccramus bcllvucnsis Skull Creek Shale 75 Inoccramuscomanchcanus Figure 23. Molluscan time scale and reference sequences of the Western Interior Basin. Based on Obradovich (1993), Cobban (1993), and Kauffman et al. (1993), Scott (1969), Gill and Cobban (1966b, 1973), McGookey et al. (1972). (figure con'd.) Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reference Sequences, U. Cretaceous Ammonite zones Western Interior, U.S.A. Stages N.E. Wyoming W. Montana South Dakota Hell Creek / Lance Formation U 3 Dtacoscapfcitea roaacrais, H. nicciJeti Fox Hills Sandstone Maastrichtian 4 Hoploscaphiics spaff. H.nicollcli Elk Butte Mbr 5 Baculitesclinolobatus Upper Mobridge Mbr L 6 Baculilcs grandis unnamed shale unit 7 Baculitesbacuius Virgin Creek 8 Baculilcs cliasi Mbr 9 Bactiliicsjcnscni 10 Baculilcs reesidci Bearpaw Verendrye Mbr Shale 11 Baculilcs cuneatus Lower unnamed IT 12 Baculilcs compressus shale unit (Tepee Butte zone) DeGrey Mbr 14 Exitdocerasjcnncyi IS Didymoccrasstevcnsoni Gow Creek Mbr 16 Didymoccras ncbrasccnsc 17 Baculitcsscolli Campanian 18 Baculilcs gregorycnsis, B. reduncus Judith River Red Bird Gregory Mbr Sandstone 19 Baculilcs perplexus(late form) Silty Mbr M 20 Baculilcs gilhcni 21 Baculilcs perplexus (early form) ------Mitten Black ------Shale Mbr T\ Baculilcs aspcriformis Sharon ------Springs Mbr Sharon Claggett Shale Springs Mbr 26 Baculilcs sp. (weak flank ribs) 27 Baculilcs sp. (smooth 1) ....2R Scaphitcs hippocrcpis 111 Gammon 29 Scaphitcs hippocicpisll L Ferruginous Eagle Sandstone Mbr 30 Scaphites hlppocrcpisl 1 1 | Pierre Shale Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 54 formations exposed in the eastern and central part of the Western Interior basin, particularly eastern Colorado and contiguous areas ( Cobban and Reeside, 1952; Gill and Cobban, 1966 b; Kauffman, 1977b). In this part of the basin, Upper Cretaceous rocks are highly fossiliferous and biostratigraphically better constrained than elsewhere. Because of the distinctive, short-ranging, fossil assemblages these formations possess, they have in practice been used as biostratigraphic or chronostratigraphic units in regional stratigraphic correlations for many years. The Lower Cretaceous series is excluded in Figure 5 because it is thin, poorly constrained and mostly nonmarine. For an updated reference, a recent correlation chart of the Lower Cretaceous rocks compiled by Heller and Paola (1989) is shown instead in Figure 24. TRANSGRESSIVE-REGRESSIVE CYCLES It is widely recognized among stratigraphers that the Cretaceous stratigraphy of the North American Western Interior reflects a succession of major transgressive-regressive depositional cycles. In the U.S. Western Interior, five transgressive-regressive depositional cycles have long been recognized in Albian to Maastrichtian strata (Weimer, 1960; Kauffman, 1969,1977a and b; McGookey et al., 1972; Kauffman and Caldwell, 1993). They have been named in ascending order as: the Kiowa-Skull Creek, Greenhorn, Niobrara, Claggett, and Bearpaw cycles (Fig. 25). Where fully developed, these cycles, or cyclothems, generally consist of transgressive marine shales or limestones overlain by subsequent regressive marine and marginal marine shales, siltstones, and sandstones. These cycles are not periodic; their duration ranges from 5 to 10 m.y. Some cycles are apparently provincial, confined to the Western Interior or only part of it, whereas others such as the Greenhorn cycle can be correlated with most world-wide Cretaceous transgression-regression records (Hancock and Kauffman, 1979; Matsumoto, 1980). It should be noted that the current knowledge of these cycles is generalized and heavily influenced by the stratigraphic records in the type areas where the cycles were Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. LA CO ------Beaver Beaver 7TV1 Mines Fm Mines Cadomin Fm. Fm. Cadomin Gladstone Fm Gladstone Kootenay Group Mill Creek Fm Creek Mill CANADA m m Femie Gp SOUTHERN MONTANA WESTERN ColoradoSh KootenaiFm Swift Fm Morrison Fm Morrison CreekSh FusonFm Fall RiverSs cul S. DAKOTA NewcastleSs BLACK HILLS 999999999^ , r Sundance Fm Sundance Morrison Fm Morrison 11/ Rusty Beds Muddy Ss CENTRAL C]ove^ly_Fm Greybull Ss Mowry Sh. Mowry Sh. WYOMING r Thermopolis Sh ^— — Peterson Ls Ls Peterson U^phraim Lower Ephraim Draney Ls Ls Draney Fm Bechler congl. Smoot Sh Sh Smoot WEST Aspen Sh WYOMING BearRiver Ss South Lytle Fm PlatteFin Mowry Sh COLORADO COLORADO Ralston FmRalston Fm Stump N. FRONT RANGE FRONT N. Morrison Fm Morrison Fm cooel_ Plainview Ss Glencaim Sh ''Purgatoffe'’ CENTRAL MowiySh COLORADO 9793^9665190 Burro CanyonFn l Morrison Fm Morrison Summerville Fm Summerville M _J L_ 1 Mbr ormation Buckhom UTAH UTAH COLORADO F Cedar CENTRAL WESTERN WESTERN CENTRAL 152 156 144 124 131 138 113 119 Ma 97 Barr. Bern Haul. Valan. Aptian Albian Kinun. Oxford Tithon. STAGE c o o .2 *5 55 TheMowry AspenShale Shale and arenow assigned Cretaceousthe Upperto Cenomanian) (lower (Cobban and Kennedy, 1989). Figure24. Late toJurassic Early correlation Cretaceous chartpartsfor of Western the InteriorPaolaHellerFrom basin. and (1989). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. REFERENCE SEQUENCE OF STUDY STAGES T-R CYCLES U.S. WESTERN INTERVAL M a INTERIOR Fox Hills Sandstone/ Hell Creek Fm Maastrichtian Elk Butte Mbr. 70 - Bearpaw Virgin Creek Mbr. Verendrye Mbr. -PsQrev MbL__ Crow Creek Mbr. Campanian Gregory Mbr Claggett 80 - Sharon Springs Mbr Eagle Sandstone Telegraph Creek Fm Santonian Niobrara Niobrara Fm. Coniacian 90 - Turonian Carlile Shale Greenhorn Greenhorn Fm. Graneros/Belle Cenomanian Fourche Shale Mowry Shale ioo - Newcastle Sandstone Regression Skull Creek Shale Albian Kiowa-Skull Creek Transgression Fall River Sandstone Figure 25. Transgressive-regressive depositional cycles of the North American Cretaceous Western Interior. Selected stratigraphic intervals on the six regional cross sections of this study are shown by arrows. From McGookey et al., (1972); Kauffman (1977b, 1985). Time scale based on Obradovich (1993). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 57 first defined. The Kiowa-Skull Creek, Greenhorn, and Niobrara cycles were defined in the eastern and central parts of the basin, including Colorado, western Kansas and adjacent areas, whereas the Claggett and Bearpaw cycles were established in Montana and South Dakota. The following is a generalized description of these cycles in terms of their lithologic successions and associated fossils found in their type areas. No attempt is made to compare systematically equivalent strata of these cycles in every part of the Western Interior with those in the type areas. Neocomian to Aptian During much of Early Cretaceous time, the U.S. Western Interior was a broad fluvial drainage basin, where the overall drainage direction was to the north and most sediments were derived from the incipient Sevier orogenic belt (Fig. 26). Rocks of Neocomian to Aptian age are distinguished by the presence of abundant and widespread nonmarine conglomerates displaying rapid lateral changes in lithofacies, stratal thickness, and age. Figure 24 summarizes the main Lower Cretaceous lithostratigraphic units from different regions and their probable age relations (Heller and Paola, 1989). The nonmarine, conglomeratic Lower Cretaceous rocks rest with a regional unconformity of uncertain duration on the Morrison Formation of Late Jurassic age ( Peterson, 1994). These conglomeratic units, including the Ephraim Conglomerate in western Wyoming, the Cloverly Formation in central Wyoming, the Kootenai Formation in western Montana, and the Lakota Sandstone in the Black Hills, form a 100-200 meter thick blanket of conglomeratic sandstones and variegated mudstones over much of the Western Interior. The Kiowa-Skull Creek cycle The Kiowa-Skull Creek cycle, the first marine incursion into the U.S. Western Interior in the Cretaceous, was Albian in age and lasted nearly 10 m.y. (Fig. 25). Strata associated with the Kiowa-Skull Creek cycle are well described in the central-eastern part Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 110 105 100 95 Kootenai Fm C loverly Fm 40 Lytle Fm Burro Canyon Fm 35 0 1 0 0 200300 km 105 Figure 26. Early Cretaceous drainage pattern in the Western Interior. Modified after Young (1970). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 59 of the U.S. Western Interior (Haun and Weimer, 1959; Waage, 1959; Franks, 1975; Young, 1970; MacKenzie, 1971). The Kiowa-Skull Creek transgression was represented by the Fall River Sandstone and its correlatives, including the Rusty Beds in central Wyoming and the Plainview Sandstone in Colorado (Fig. 24). These rocks rest unconformably on the pre-Albian fluvial deposits of the Cloverly Formation and its correlatives. They occur as an extensive sheet of marine or marginal marine sandstones, siltstones, shales, and thin coals that measure in thickness from a few meters to tens of meters. Other than plant remains and trace fossils, few age-diagnostic fossils have been reported from these transgressive deposits. Conformably overlying the Fall River SaBdstone is the Skull Creek Shale and its correlatives, the Kiowa Shale in Western Kansas and Nebraska, and the Thermopolis Shale in Wyoming and Colorado. These rocks, deposited during the peak of the Kiowa- Skull Creek transgression, consist of dark-gray marine shale and siltstone and are generally less than 60 meters in thickness. Marine fossils, including mollusks (Waage, 1959; MacKenzie, 1971) and foraminifera (Eicher, 1960), have been widely reported from these deposits, albeit with low diversity and abundance. Among them, lnoceramus comancheanus Cragin has proved to be a very reliable late Albian guide fossil to date the Kiowa-Skull Creek marine deposits throughout the U.S. Western Interior. The Kiowa-Skull Creek regression in late Albian time was recorded by several closely contemporaneous sandy units, including the Newcastle Sandstone in the Black Hills, the Bear River Sandstone in western Wyoming, and the Muddy Sandstone in central Wyoming and Colorado. These rocks consist of interbedded sandstone, siltstone, and shale deposited in deltaic or estuarine environments. Their thickness is rarely in excess of 50 meters. Fossil records from them are sparse and restricted to plant remains, vertebrate fragments, and trace fossils. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 60 The Greenhorn cycle The Greenhorn cycle spans the time interval from latest Albian-earliest Cenomanian through middle Turanian time, a period of nearly 10 m.y. The standard section of the Greenhorn cycle is located at Pueblo, Colorado (Fig. 27). Its lithostratigraphy and biostratigraphy have been thoroughly described by Scott (1969), Cobban and Scott (1972), and Kauffman (1977b). In western Kansas, complementary sections of the Greenhorn cycle have also been described in great detail by Hattin (1962,1965a, 1969, 1971,1975b). In these places as well as many others, the Greenhorn cycle assumes a more or less symmetrical sequence in terms of the duration of the transgressive phase and the ensuing regressive phase. The transgressive phase consists of, in ascending order, the Mowry Shale, Graneros Shale, and Greenhorn Formation; the regressive phase is represented by the Carlile Shale and the Codell Sandstone. The Mowry Shale The Mowry Shale was deposited in a marine embayment during the initial Greenhorn transgression as the sea advanced from the north in the early Cenomanian (Fig. 28a). It occurs as an extensive blanket of siliceous shales and bentonite beds overlying the Newcastle Sandstone and its correlatives (Fig. 24) in the northern and central parts of the Western Interior. It grades laterally into marginal marine and nonmarine sandstones towards the basin margins, such as the undifferentiated Cedar Mountain Formation and the Dakota Sandstone in central and southern Utah (Molenaar and Cobban, 1991). The thickness of the Mowry shale is usually less than 100 m in the central part of the basin and diminishes towards the basin margin. Abundant fish remains exist in the Mowry, but other fossils are scarce. Only a very limited early Cenomanian fauna, including Neogastroplites americanus and Neogastroplites comutus, have been widely reported from the Mowry (Reeside and Cobban, 1960). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 61 B a c u l i t e s o b tu s u s Thickness (meters) Apache Creek Sandstone Mbr B a c u l i u s s p (w eak ribbed) Pierre Shale Transition M br 'B a c u I U e s s p (smooth) -y uppercfMUc y — X illlit / Ccncrctiotnry uboail I n o c e r a m u s s im p s o n l Upper chalk shale unit Inoceramus piatinus CO I n o c e r a m u s cfJ. patootensis Inoceramus cordiformis Niobrara Formation Inoceramus undulatoplicatus M iddle shate unit 11.6 Lower limestone unit Lower shate unit Inoceramus invdutus 17.1 _ / Shale and 'Ss - limestone unit - 7 I n o c e r a m u s d e fo r m is Fort Hays I n o c e r a m u s e r e c tu s 12.2 Limestone Mbr " X ju a n a Lopez Mbc^" >*ssJScaphitfs whitfieldi Pionocyclus wyomingensis - V N / I VTodcll Sandstone/ I n o c e r a m u s h o w e lli Prionocyclus hyatti 30.8 Carlile Blue Hilt Shale Shale Mbr Fairport chalky 30.2 shale M br Collignoniceras woollgari Bridge Creek Inoceramus labiatus Limestone Mbr Sciponoccras gracile Greenhorn Haitland Shale Mbr Formation Inoceramus pictus Lincoln Lim estone M b 11.4 Graneros Shale — Conlinoceras sp. 31.4 Dakota ' Sandstone Figure 27. Generalized stratigraphic section for the Rock Canyon anticline area, northwestern Pueblo quadrangle, Colorado, showing principled lithologies and zonal fossils of the Dakota, Greenhorn, Carlile, Niobrara, and lower Pierre Shale. From Scott (1969). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. time .Embayment' 'Mississippi ; ] Scaphites. hippocrepis Early Early Campanian Seas is now consideredto be early Cenomanian time Watinoceras Early Early Turanian Seas (Neogastroplites comutus Late Late Albian Seas by Cobban and Kennedy, 1989) FromWilliams and Stelck (1975). Figure 28. Map showing the extent ofthe Cretaceous Western Interior SeaWays atthree differenttimes. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 63 In both outcrops and the subsurface, the Mowry Shale occurs as a distinct lithologic unit that contrasts with both the overlying and underlying rocks. In eastern Montana and Wyoming, a bentonite bed, the Clay Spur Bentonite, occurs near the top of the Mowry Shale. Radiometric dating of this bentonite bed in the Black Hills yielded an age of 97 Ma, or early Cenomanian (Obradovich, 1993). The Graneros Shale The Mowry is succeeded without a depositional break by the Graneros Shale (Fig. 25). In Colorado and Western Kansas, the Graneros Shale is a dark, organic-rich shale deposited in a open marine environment. Thickness of the Graneros Shale is variable, ranging from around 10 m in western Kansas to 50 meters in much of Colorado. In the Black Hills, near the junction of Montana, South Dakota, and Wyoming, the Belle Fourche Shale overlies the Mowry shale as the lateral equivalent of the Graneros Shale. Marine fossils are sparse in the lower part of the Graneros Shale and its correlatives, but are comparatively abundant in the upper part, including ammonites and inoceramid bivalves. Cobban and Scott (1972) established four middle Cenomanian ammonite zones in the upper Graneros Shale, which, in ascending order, are Calycoceras gilberti, Acanthoceras granerosense, Acanthoceras muldoonense, and Acanthoceras amphibolum. Bentonite beds of varying thickness are common throughout the Graneros Shale. The most prominent one, the X bentonite, occurs at the top of the Graneros Shale and lies within the Acanthoceras amphibolum zone. It is nearly a meter in thickness and can be traced northward into the Alberta foreland. Because of its extent, it has been widely used as a marker bed in surface and subsurface correlation. The Greenhorn Formation In Colorado, Kansas, and adjacent areas, the Greenhorn Formation comprises three distinct lithologic units which, in ascending order, are the Lincoln Limestone, Hartland Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 64 Shale, and Bridge Creek Limestone Members (Fig. 27). Their cumulative thickness is usually less than 70 m. The Lincoln Limestone consists of calcareous shale, limestone, and numerous thin bentonite beds. Its thickness varies from 10 m at the Pueblo to less than 1 m in Bunker Hill, Kansas. Abundant ammonites and inoceramid bivalves have been collected from the Lincoln Limestone. Late middle Cenomanian zonal fossil Acanthoceras amphibolum occurs at its base, and the late Cenomanian zonal fossil Dunveganoceras pondi is found at its top (Cobban and Scott, 1972; Sageman, 1985; Sageman and Johnson, 1985). Overlying the Lincoln Limestone Member, the Hartland Shale Member is composed of organic-rich, well-laminated calcareous shale and numerous thin bentonite beds. At Pueblo, the Hartland Shale Member is 17 m thick and contains Inoceramus pictus Sowerby, which ranges from the basal Lincoln Limestone Member to the lower part of the Bridge Creek Limestone Member. In the northern part of the Western Interior, the Hartland Shale and its correlatives encompass the early late Cenomanian Dunveganoceras conditum and Dunveganoceras albertense zones (Metoicoceras mosbyense zone; Cobban and Scott, 1972). The Hartland Shale Member is succeeded by the Bridge Creek Limestone Member, which records the peak of the Greenhorn transgression and the maximum areal extent reached by the Western Interior seaway (Fig. 28b). At Pueblo, it is 15 m thick and consists of many rhythmic limestone- shale couplets and laterally persistent bentonite beds. These lithofacies are widespread in the eastern and central part of the Western Interior basin. In western Kansas, the Bridge Creek Limestone is divided into a lower Jetmore Chalk Member and an upper Pfeifer Shale Member (Hattin, 1971b). Marine fossils are abundant and diverse in the Bridge Creek Limestone, and fossil zonations are well established. Four ammonite zones, ranging in age from middle late Cenomanian to earliest middle Turanian, are defined in the Bridge Creek Limestone by Cobban and Scott (1972). These are the Sciponoceras gracile, Watinoceras coloradoense, Mammites nodosoides, and Collignoniceras woollgari zones. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 65 The Cariile Shale Conformably overlying the Bridge Creek Limestone Member of the Greenhorn Formation is an upward coarsing succession of shale, siltstone, and sandstone that comprise the Cariile Shale (Fig. 27). The Cariile Shale is divided into, in ascending order, the Fairport Chalky Shale, Blue Hill Shale, Codell Sandstone, and Juana Lopez Members (Hattin, 1971a; Hattin and Cobban, 1977). Its total thickness ranges from less than 15 m to more than 60 m (Weimer, 1986). The Fairport Member is a calcareous shale and siltstone unit (Scott, 1969; Glenister and Kauffman, 1985). Marine fossils in the Fairport are low in diversity and poorly preserved. The early middle Turanian zonal index fossil Collignoniceras woollgari, which is best documented in the Pool Creek Member of the Cariile Shale in the Black Hills, occurs as flattened impressions (Cobban, 1984). The Blue Hill Member is composed of non-calcareous, silty shale. At Pueblo, the Blue Hill is 30 m thick; the lower half consists of silty shale and the upper half of sandy siltstone. Marine fossils are sparse and poorly preserved in the Blue Hill Shale Member. In north-central Kansas, however, the Blue Hill contains many specimens of the ammonite Prionocyclus hyatti (Cobban, 1984). The Codell Sandstone Member is a fine grained shallow marine sandstone unit deposited during the terminal regression of the Greenhorn cycle (Glenister and Kauffman, 1985; Weimer, 1986). It occurs sporadically on the eastern side of the basin and is usually less than 10 m thick. Its contact with the Blue Hill Member is either conformable, as at Pueblo (Glenister and Kauffman, 1985), or disconformable, as in parts of the Denver basin (Weimer, 1986). Its contact with the overlying Juana Lopez Member, the basal transgressive deposits of the Niobrara cycle, is disconformable. Marine fossils found in the Codell Sandstone Member include the middle Turanian Prionocyclus hyatti and Inoceramus howelli (Scott, 1969). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 6 6 The Niobrara cycle The Niobrara cycle spans the time interval from the latest Turonian to early Campanian, a period of more than 9 m.y. (Fig. 25). Like the Greenhorn cycle, the standard section of the Niobrara cycle is also located at Pueblo (Fig. 27; Scott and Cobban, 1964; Scott, 1969). As defined by Kauffman et al. (1977b), strata deposited during this period of time include the upper part of the Cariile Shale or Mancos Shale {e.g., the Juana Lopez Member), the Niobrara Formation, and the Transition member and the lower part of the Apache Creek Sandstone Member of the Pierre Shale. Similar to the Greenhorn cycle, strata of the Niobrara cycle are distinguished by domination of limestones and calcareous shales. The transgressive phase of the Niobrara cycle is thin; the peak transgressive deposits rest unconformably on regressive facies of the Greenhorn cycle (Codell Sandstone or Blue Hill Shale Members). The regressive phase, on the other hand, has a long and well developed rock record. The Juana Lopez Member At Pueblo, Colorado, the initial transgression of the Niobrara cycle is represented by three lithologic units, which, in ascending order, are: 1) a 25-cm-thick silty shale unit of the upper Cariile Shale lying disconformably on the Codell Sandstone (not shown on Fig. 23,27), 2) a calcarenite-calcareous shale unit of the Juana Lopez Member, and 3) a shale unit equivalent to the Sage Breaks Member of the Cariile Shale in Wyoming (Fisher et al., 1985). Among them, the Juana Lopez Member is the most laterally persistent and lithologically distinct unit that records the initial transgression of the Niobrara cycle in New Mexico, Colorado, and Utah. Time-equivalent rocks include part of the Turner Sandy Member of the Cariile Shale in northeastern Wyoming and Montana, and the Wall Creek Member of the Frontier Formation in central and southeastern Wyoming. The type section of the Juana Lopez Member is located near Cerrillos, Santa Fe County, New Mexico (Rankin, 1944). At a reference section in the southeastern part of the San Juan Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 67 basin, New Mexico, the Juana Lopez Member is 30 m thick and composed of interbedded calcarenites, fine-grained sandstones, and shales (Dane et al., 1966; Hook and Cobban, 1980; Molenaar, 1983). There, the Juana Lopez Member has a conformable contact with both the overlying and underlying Mancos Shale. Its top has been considered a time-parallel surface that can be traced over long distances in the subsurface (Dane, 1960a; Molenaar, 1973). In the eastern part of the Western Interior basin, the Juana Lopez Member occurs only locally. Where preserved, it is rarely more than 1 m thick, and unconformably bounded between the underlying regressive deposits of the Greenhorn cycle and the overlying transgressive deposits of the Niobrara cycle. The Juana Lopez Member and its equivalents are generally fossiliferous, lying within the late Turanian Inoceramus dimidius, Scaphites warreni , Prionocyclus wyomingensis, and Prionocyclus macombi zones (Hook and Cobban, 1980). The Niobrara Formation The Niobrara Formation is a dominantly chalky unit that constitutes the bulk of the Niobrara cycle in much of the Great Plains, from the North and South Dakotas to Colorado and western Kansas (Fig. 27). It is best exposed in Colorado, western Kansas, and neighboring areas. For this reason, the stratigraphy of the Niobrara Formation has been studied in detail by Hattin (1981,1982) in western Kansas, by Scott and Cobban (1964) at Pueblo, Colorado, and by Scott et al. (1986) in the Raton basin, New Mexico. Kauffman (1977b) identified as many as four successive transgressive pulses, separated by regressive episodes, in the Niobrara Formation at Pueblo, Colorado. In Colorado, western Kansas, and adjacent areas, the Niobrara Formation comprises a lower Fort Hays Limestone Member and an upper Smoky Hill Shale Member. These two members are lithologically distinct and can be recognized either in outcrops or in the subsurface over a large area. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 68 The Fort Hays Limestone unconformably overlies the Cariile Shale and records the inception of the Niobrara transgression (Kauffman, 1977b; Scott and Cobban, 1964). It consists of about 10 to 20 m of limestone beds and intervening shale. The limestone beds are micritic and contain abundant inoceramids. Locally, the basal part of the Fort Hays Limestone contains quartz sands reworked from the underlying Codell Sandstone. The Fort Hays Limestone is laterally persistent and forms an excellent time-parallel marker bed in the subsurface. In the western part of the basin, age-equivalent rocks include the uppermost part of the Frontier Formation of Wyoming, and the upper part of the Gallup Sandstone and the lower part of the Tocito Sandstone in New Mexico. To the north and west, the Fort Hays Limestone thins and becomes shaly by facies changes. At Pueblo, three latest Turonian-early Coniacian Inoceramus zones span the Fort Hays Limestone, which, from the bottom to the top, are the Inoceramus perplexus, Inoceramus erectus, Inoceramus deformis (Scott and Cobban, 1964). In the Raton basin, only one latest Turanian ammonite zone, that of Prionocyclus germari, is present (Scott et al., 1986). The Smoky Hill Shale Member consists of alternating units of calcareous shale and chalk or limestone (Scott and Cobban, 1964; Hattin, 1981,1982). In the northern Great Plains, the equivalent of the Smoky Hill Shale is unnamed chalk and calcareous shale in the Niobrara Formation (Shurr and Rice, 1986). At Pueblo, the Smoky Hill Shale is about 212 m thick and is divided into seven lithologic units (Scott and Cobban, 1964). These are, in ascending order, the shale and limestone unit; the lower shale unit; the lower limestone unit; the middle shale unit; the middle chalk unit; the upper chalky shale unit; and the upper chalk unit (Fig. 27). Kauffman (1977b) identified the lower limestone unit, the middle chalk unit, and the upper chalk unit as the three additional transgressive pulses of the Niobrara cycle. Throughout the section, marine fossils, particularly inoceramids, are abundant and diverse. The section encompasses the following zonal fossils ranging in age from middle Coniacian to lower Campanian; Inoceramus deformis, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 69 Inoceramus involutes, Scaphites depressus, Inoceramus undulatoplicatus-Clioscaphites saxitonianus, Clioscaphites vermiformis , Clioscaphites choteauensis, Scaphites hippocrepis, Baculites sp zones (smooth) (Scott and Cobban, 1964). Pierre Shale During the regressive phase of the Niobrara cycle, following the deposition of the Smoky Hill Shale Member, the Western Interior seaway became greatly reduced in areal extent (Fig. 28c). The regression of the Niobrara cycle is represented by the basal Pierre Shale lying below the earliest middle Campanian zonal fossil Baculites obtusus (Kauffman, 1977b). This interval includes the Transition member and the lower part of the Apache Creek Sandstone Member of the Pierre Shale at Pueblo (Fig. 27), the Gammon Member of the Pierre Shale in the Dakotas, and the Telegraph Creek Formation and Eagle Sandstone in Montana (Fig. 23). The contact between the Pierre Shale and the underlying Niobrara Formation at Pueblo and Raton basin is gradational, lying between the fossil zones of Scaphites hippocrepis II and Scaphites hippocrepis III (Scott et al., 1986). In the Denver basin and the Black Hills region, the contact has been inferred to be a regional unconformity (LeRoy and Schultz, 1958; DeGraw, 1975; Weimer, 1983). The Claggett cycle The Claggett cycle spans the middle Campanian, a period of about 5 m.y. (Fig. 25). The stratigraphic signature of the Claggett cycle is well defined in the northern part of the U.S. Western Interior. However, in central and southern parts of the Western Interior, the transgressive-regressive patterns in the contemporaneous rocks display complex and diachronous relationships. The stratigraphy of the Claggett cycle and the trends of the contemporaneous strandline movements have been described by Gill and Cobban (1973) in the northern part of the basin. In that region, the Claggett cycle consists of a Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 70 transgressive phase represented by the Claggett shale, and a regressive phase represented by the Judith River Formation. The Claggett Shale is a noncalcareous bentonic unit deposited during a period of intensive volcanic activity. The basal part of the Claggett Shale contains the Ardmore Bentonite, a bentonite bed that is locally one meter thick and can be traced throughout the Dakotas, Montana, and Wyoming. This bentonite bed lies between the two successive ammonite zones: the latest early Campanian Baculites sp. (weak flank ribs) and the earliest middle Campanian Baculites obtusus. Radiometric dating of the Ardmore Bentonite yielded an age of 80.5 Ma (Obradovich, 1993). The Claggett shale overlying the Ardmore Bentonite Bed contains many early middle Campanian ammonites, including, Baculites obtusus, Baculites macleami, and Baculites asperiformis (Gill and Cobban, 1973). The Claggett Shale is overlain by the eastward-thinning regressive clastic wedge of the Judith River Formation. The basal part of the Judith River Formation is a shallow marine sandstone unit named the Parkman Sandstone Member. Overlying the Parkman Sandstone are non-marine deposits rich in coarse volcanic material. The proportion of volcanic material in the Judith River Formation increases towards the western source areas in the Elkhom Mountains. The Judith River regression took place during the span of six ammonite zones. In ascending order, they are: the Baculites sp. (smooth), Baculites perplexus (early), Baculites gilberti, Baculites perplexus (late), Baculites gregoryensis, and Baculites scotti (Gill and Cobban, 1973). The Bearpaw cycle The Bearpaw cycle marks the conclusion of marine sedimentation in the Cretaceous Western Interior basin. Like the preceding Claggett cycle, the Bearpaw cycle is well developed in the northern part of the U.S. Western Interior, where it is bounded by the Judith River Formation at the base and the Fox Hills Sandstone at the top. The Bearpaw Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 71 Shale overlies the Judith River Formation to form the transgressive phase of the Bearpaw cycle. It spans about six late Campanian ammonite zones, ranging, in ascending order, from the Didymoceras nebrascense, Didymoceras stevensoni, Exiteloceras jenneyi, Didymoceras cheyennense, Baculites compressus, to Baculites cuneatus. Marine water finally withdrew from the Western Interior during the succeeding Fox Hills regression. The withdrawal began in the late Campanian during zones of Baculites compressus and Baculites cuneatus. STRATIGRAPHIC CORRELATIONS Data The regional stratigraphic cross sections of this study were constructed with data available in the public domain. These data consist of wireline logs and various reports of outcrop fossil collections. Within most Laramide structural basins and across much of the Great Plains, such data are readily available. Over 300 well logs were collected from different parts of the basin for the purpose of subsurface correlation. In addition, many subsurface log cross sections in Laramide basins were also collected from various publications. They were either referred to or incorporated selectively in the present stratigraphic cross sections with or without modifications. The names and locations of the wells incorporated in the cross sections are given in the Appendix. The most common and valuable biostratigraphic data in the Cretaceous Western Interior are the ammonite and bivalve collections made by geologists of the U.S. Geological Survey, most notably W. A. Cobban and his colleagues. Over the decades, these collections have been made at many fossil-bearing outcrops in the Western Interior. As a result, an extremely large body of age-diagnostic fossil data are available for stratigraphic correlations. This constitutes a significant advantage for constraining the chronostratigraphic relationships of Cretaceous rocks in widely separated areas. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 72 One particular problem in handling subsurface data is the variance in the nomenclature attached to the Cretaceous rocks. In some cases, multiple names, dictated by local lithofacies, were applied to single rock units in different places (e.g., Cody, Hilliard, Baxter Shales); in others, a formation name was extended to an unrelated rock unit in different areas (e.g., the Emery Sandstone in central and southern Utah). Yet, a more serious problem is produced by differences in the designation of lithologic subdivisions in different areas based on local lithofacies patterns. These problems are more annoying than serious, but they highlight the importance of proper biostratigraphic data in chronostratigraphic correlations. Correlation method Chronostratigraphic correlations in the Upper Cretaceous series can be carried out by two complementary methods. Regional correlations are best carried out with the support of ammonite and bivalve fossil data. This is particularly important across areas where Cretaceous rocks have been stripped away by uplift and erosion due to the Laramide orogeny. The other method is based on the physical continuity of certain time-parallel marker beds, such as limestone and bentonite beds. Such marker beds generate distinctive log patterns that can be traced laterally for tens or hundreds of miles. In some places, the log patterns are so laterally persistent that they can be correlated from one Laramide basin to the next. In planning each cross section, care was taken to maximize the integration of outcrop fossil data and wireline log correlations. To achieve this, the location of the cross sections in Figure 2 was dictated to a large extent by the availability and distribution of the fossil- bearing outcrops. In selecting wireline logs, priority was given to those located as close as possible to the outcrop sections where age-diagnostic fossils have been reported. In many places, logs can be found from wells within a few to tens of miles of the outcrops. Because Cretaceous fossil-bearing rocks are invariably marine, the lithofacies change Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 73 little over this distance. Therefore, prominent lithologic units or marker beds can readily be correlated to the log sections. By matching prominent lithologic units between outcrop sections and log sections, fossil occurrences on outcrop sections can then be projected into the subsurface and allow wireline log correlations to be biostratigraphically constrained and dated. Because of the widespread fossil-bearing outcrops, each cross section usually contains multiple wireline logs tied to outcrop sections. Between the foredeep and the cratonic interior, 12 to 33 wireline logs were selected as individual stratigraphic columns along each cross section. In many cases, however, correlations on each cross section are supported by additional logs not listed in the Appendix. The selected logs are usually spaced tens of miles or less in Laramide basins, and up to hundreds of miles across Laramide uplifts. Such large spacings between logs may not be suited for detailed lithostratigraphic analysis, but because correlations are performed at the formation or larger scale and supported by biostratigraphic data they are well-suited to this study. Study interval Strata presented on the six cross sections encompass the lower and middle part of the Upper Cretaceous Series, ranging in age from middle Cenomanian to early Campanian. This time interval corresponds to the Greenhorn and Niobrara cycles (Fig. 25). Selection of this stratigraphic interval carries several advantages as far as correlations are concerned. First, strata of this interval are better preserved than younger ones. Therefore, correlations can be made over wider areas and with more data points. Second, unlike the overlying complexly intertongued marine and nonmarine formations, this interval consists of predominantly marine rocks distinguished by exceptional lateral lithofacies consistency. Third, rocks of this interval contain many marker beds recognizable over large areas. For example, the Mowry Shale, the 'X' and Ardmore Bentonite Beds, the Juan Lopez Member, and many of the limestone beds of the Greenhorn and Niobrara Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 74 Formations can be traced continuously for several hundreds of miles ( Zelt, 1985; Kirkland, 1991; Elder et al., 1994). These and other beds serve as ideal markers for chronostratigraphic correlations. Fourth, strata of the Greenhorn and the Niobrara cycles are highly fossiliferous. A large body of ammonite and bivalve data have been collected from this interval throughout the Western Interior. They can be readily integrated into subsurface correlations. Finally, although spanning a period of 16 m.y., this interval represents more than half of the preserved Upper Cretaceous series in many places. A note on the cross sections The six regional litho-stratigraphic cross sections show stratal thickness, lithofacies, and age relationships across different parts of the U.S. Western Interior, from Montana and the Dakotas to southern Utah, New Mexico, Colorado, and Western Kansas. Each litho-stratigraphic cross section is accompanied by a generalized chronostratigraphic section crossing approximately the same segment of the Western Interior basin. Such sections show generalized lateral stratigraphic relationships between individual Laramide basins and include younger Cretaceous rocks. The remainder of this chapter is devoted to the discussion of the litho-stratigraphic cross sections. Several procedural remarks need to be made in advance. First, discussion extends only to the formations within the range of the cross sections of this study; age-equivalent formations that exist in the thrust belt, where they assume different lithofacies and different nomenclature, are not considered. Second, the following discussion will focus on strata deposited in the western part of the basin Inasmuch as those in the central and eastern parts have been described to some extent in the preceding section on the stratigraphy of the cycles. In addition, the Cretaceous lithofacies and fossil records in the central and eastern part of the basin are fairly consistent, whereas those in the western part of the basin show great variations and therefore deserve special attention. Finally, the terms "Greenhorn" and "Niobrara" cycles were used in a chronostratigraphic sense in the following discussions of the cross Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 75 sections. This usage was adopted merely for the purpose of organizing age-equivalent strata from widely separated regions. Apart from the convenience provided by the two chronostratigraphic units, the time they represent may be discrete periods of time possibly related to the ultimate tectonic forces that also drive basin subsidence. REGIONAL STRATIGRAPHIC CROSS SECTIONS Cross sections 1 and 2: west Montana to North and South Dakotas Upper Cretaceous rocks are not as fully exposed in Montana and the Dakotas as farther south because of lack of major Laramide uplifts. However, for the same reason, these rocks are better preserved in the subsurface. Because subsurface data are abundant, closely spaced wells logs can be used in stratigraphic correlations. Upper Cretaceous rocks in western Montana consist of, in ascending order, the Marias River Formation/Cody Shale, the Telegraph Creek Formation, the Eagle Sandstone, the Claggett Shale, the Judith River Formation, the Bearpaw Shale, the Fox Hills Sandstone, and the latest Cretaceous nonmarine formations that overly the Fox Hills Sandstone (Figs, 29,31; Cobban and Reeside, 1952a; Cobban, 1955a; Gill et al., 1972a; Gill and Cobban, 1973; Rice and Shurr, 1983; Roberts, 1972). These formations generally amount to less than 2000 meters in total thickness. In contrast, equivalent beds in western Wyoming and central Utah can be twice as thick. The lower part of the Upper Cretaceous succession, including the Marias River Formation/Cody Shale, and the Telegraph Creek Formation, is conspicuously dominated by marine shale. The upper part of the Upper Cretaceous succession, from the Eagle Sandstone to the Fox Hills Sand stone, comprises intertongued marine/nonmarine sandstone and shale. Towards the east, the Upper Cretaceous succession as a whole thins and grades into marine shales by facies changes. In eastern Montana and the Dakotas, this succession is a monotonously uniform marine shale sequence composed of, in ascending order, the Belle Fourche Shale, the Greenhorn Formation, the Cariile Shale, the Niobrara Formation, and the Pierre Shale. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. -j ON ' -1 , 29 unconformity North Dakota North marine sandstone Mowiy Shale GreenhornF m .u '223^23 mmmm nonmarinerocks coastal and N.Montana E. t : it j . ^ <* - x " , If- - -1 r ,-T---1-- , I Tir . v vrjk'«rr -4' P manne limestone tv ~ ir 7 i - 1 gg»m»Mosby Ss gg»m»Mosby Montana N. Central * -* — tt” -' n ; ffiw n j: |lr \ . ‘S< . 11 I,*'' ' ■ ■ ^ ir ^ ir - ' 023 Arch interbeddedlimestone shale Sweetgrass Montanato North Dakota. Figure Generalized 29. time-stratigraphic correlation chartUpperfor Cretaceous strata from northwestern Albian Turanian Coniacian Santonian Campanian Cenomanian marine shale calcareous shale with siliceousmarine Maastrichtian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. MONTANA— Swettgrass Havre Glasgow Arch 6 7 Ardmore Bentonite Bed r ^vvV^A;VvV'-;ivV^ meters • */• m* * • * 5 j ? 5 3 ? 5 J 5 3 5 3 E » *•*■ ♦+ *»+ *•«**• * * * + «► ■*■ «► **T*•►«4» • ♦ 4* 4t^.+ ♦♦♦♦ + * N id ra n ! ilcS ha Si^**.1 7 nternFB ;^.jg elfnFoiirc Howcrec^^T 33,35,38,39,49,57.58,60: Mhr ^ : Cobban, 1951a; Cobbanetal., 1958,1959 Marine calcareous Undifferentiated marine and Marine shale 1000 - shale or limestone nonmarine sandstone Figure 30. Regional stratigraphic cross section 1 of lower Upper Cretaceous rocks from northwestern P (see Appendix for name and location). Projected fossil occurrences are marked by small triangles follo\ section is shown in Figure 20. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. f------NORTH DAKOTA Glasgow ------Williston Basin ------* Cavalier 10 11 12 13 14 15 16 0 100 200 km ■ i n e a n d , ______i______, > n e ;ks from northwestern Montana to North Dakota. Vertical lines and the numbers above represent individual wells by small triangles followed by numbers that correspond to the ammonite zones in Figure 23. Location of the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 00 Central N. Dakota m m Black Hills ibraraFra. *1 m C C immonShale G G eenbomFm. Ci Shale rltle B< leFourcbeS Mowry Shale Montana S-central W m m m . tamSDEEB -Ji tamSDEEB ’.FrootierF Livingston area Figure 31. Generalized time-stratigraphiccorrelation chartfor Upper Cretaceous stratafrom southwestern Montanato South Dakota. Albian Turanian Coniacian Santonian Campanian Cenomanian Maastrichtian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. MONTANA Bozeman Roundup Boyes ?&%?I 1 *•••.*.• *.* .**• .*.• .*.• *.*»•.*„• /.• Sandstone •.%•/.•/.**,*.•/.♦.*.».*.♦.*.»•-»•*- • *. ,* • ,• \ • * .. . *. . • . . *Ty - yfyfy^..... ^Niobrara! 29: Cobban (1969) 35: Cobban (1951b)55* 39- 49, and 60 were projected from the column 34 on cross section C of Rice (1976, 1977) 1000 37: Robert (1972) Figure 32. Regional stratigraphic cross section 2 of lower Upper Cretaceous rocks from southweste individual wells (see Appendix A for name and location). Projected fossil occurrences are marked b in Figure 23. Location of the section is shown in Figure 20. See Figure 30 for legends. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. SOUTH DAKOTA -Williston Basin- N. Black Hills Pierre Ardmore Niobrara Fmj The age of the Clay Spur Bentonite is dated as 97 Ma, ourchc Sha and that of the Ardmore Bentonite 50: Cobban (1951a) 35 80 5 Ma (obdoroch>1993) jrojected from the on C of Rice (1976, 1977) 25,27,45: Rice (1976), Robinson et al. (1964) 29: Cobban (1969) 100 2 0 0 km jtaceous rocks from southwestern Montana to South Dakota. Vertical lines and the numbers above represent fossil occurrences are marked by small triangles followed by numbers that correspond to the ammonite zones ire 30 for legends. Reproduced w«h p e n n o n of .he copyright owner Further reproduction prohibited whhout permission Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 80 Cross sections 1 and 2 extend from western Montana to the Dakotas (Figs. 30,32). They were composed by combining and modifying four different subsurface cross sections from Montana and the Dakotas that were originally compiled by Rice (1976,1977). Where possible, molluscan fossil data collected within short distances of these two cross sections were projected in to constrain correlations. Strata included on the two cross sections are those of the Greenhorn and the Niobrara cycles, bounded below by the Mowry Shale and above by the Ardmore Bentonite Bed. This interval encloses many distinct marker beds whose log patterns can be traced continuously along the length of the entire cross sections. Based on the fossil data available, four time lines were drawn on the two cross sections for the purpose of backstripping. Inasmuch as the lithofacies and stratigraphic architecture of Upper Cretaceous rocks along the two cross sections are nearly identical, their discussion is combined. Greenhorn age The Mowry Shale consists of marine and nearshore marine shale and siltstone deposited during the initial Greenhorn transgression. It measures up to 150 meters in thickness in central Montana and decreases to less than 50 meters in much of the Dakotas. The relatively high siliceous content gives the Mowry Shale a distinct log response recognizable over much of the Western Interior (Reeside and Cobban, 1960; McGookey et al., 1972; Vuke, 1984; Molenaar and Cobban, 1991). For this reason, the top of the Mowry Shale, where recognizable, was chosen as the oldest horizon in subsequent backstripping analysis. In northwestern Montana, the correlative of the Mowry Shale consists of 30 m of interbedded sandstone and shale assigned to the Bootlegger Member of the Blackleaf Formation (Cobban et al., 1976; Rice, 1976; Rice and Cobban, 1977). In northwestern Montana, the Mowry Shale is overlain conformably by the Marias River Formation, a predominantly marine shale and siltstone unit that averages about 200 m in thickness (Figs. 29,30). The Marias River Formation is divided into the Floweree, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 81 Cone, Ferdig, and Kevin Members (Cobban et al., 1976). The Floweree Member, the Cone Member, and the lower part of the Ferdig Member are of Greenhorn age, whereas the upper part of the Ferdig Member, and the Kevin Member fall into Niobrara age. The Marias River Formation as a whole passes eastward into calcareous and noncalcareous shale assigned to the Belle Fourche Shale, Greenhorn Formation, Carlile Shale, and Niobrara Formation. Many molluscan zonal fossils have been collected in members of the Marias River Formation. On the Sweetgrass Arch, the late Cenomanian zonal fossil Metoicoceras mosbyense occurs in the upper part of the Floweree Member, and another younger late Cenomanian zonal fossil Sciponoceras gracile in the overlying Cone Member (Cobban et al., 1976). The former is a guide fossil of the Hartland Shale and the latter is a guide fossil of the basal part of the Bridge Creek Limestone in Colorado and western Kansas. In the overlying Ferdig Member, middle Turanian ammonites Prionocyclus hyatti, and, perhaps, Collignoniceras woollgari are present (Cobban et al., 1976). In southwestern Montana, the Mowry Shale is overlain by the Frontier Formation (Figs. 31,32; Roberts, 1972; Rice, 1976). An eastward-thinning sandstone wedge of limited extent, the Frontier Formation is composed of marine and nonmarine sandstone and is less than 100 meters thick. It grades eastward rapidly into the marine Belle Fourche Shale by facies changes. Overlying the Frontier Formation is the Cody Shale, a silty shale interval that correlates with the Greenhorn Formation, Carlile Shale, and Niobrara Formation in eastern Montana and the Dakotas. The lower part of the Cody Shale falls into the Greenhorn cycle. Fossils from both the Frontier Formation and the lower Cody Shale are sparse. In eastern Montana and the Dakotas, strata of the Greenhorn cycle consists of the Belle Fourche Shale, Greenhorn Formation, and lower part of the Carlile Shale. The Belle Fourche Shale is a noncalcareous shale unit and averages about 30-100 meters in thickness. It is in gradational contact with both the underlying Mowry Shale and the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 8 2 overlying Greenhorn Formation. Unlike its equivalent, the Graneros Shale in Colorado, the Belle Fourche Shale is barren of age-diagnostic fossils. The overlying Greenhorn Formation is a calcareous shale unit containing locally interbedded thin limestone units, and averaging 40 meters in thickness. In central Montana, the lower 10 m of the Greenhorn Formation is a fossiliferous sandstone unit named the Mosby Sandstone member (Cobban, 1951a; Rice, 1976). The Mosby contains late Cenomanian ammonites Dunveganoceras albertense and Metoicoceras mosbyense (Cobban, 1951a, 1953b). These fossils are guide fossils found in the Hartland Shale Member of Colorado and western Kansas. In the northern Black Hills, the Greenhorn Formation contains Inoceramus fragilis (?) at the base and Inoceramus labiatus (early Turanian) at the top (Cobban, 1951a). Overlying the Greenhorn Formation, the Carlile Shale is a noncalcareous shale unit. It represents the transition between the Greenhorn regression and the Niobrara transgression. In South Dakota, a sandy unit of limited extent, named the Codell Sandstone, occurs in the middle of the Carlile Shale and passes into shales to the west (Fig. 32; Rice, 1977). A second sandy unit named the Turner Sandy Member also occurs in the Carlile Shale. The ages of these sandy units are uncertain because of lack of age-diagnostic fossils. Possibly, they are correlatives of the Codell Sandstone of Colorado and record the final regression of the Greenhorn cycle. Niobrara age In northwestern Montana, strata of the Niobrara cycle consists of the upper part of the Ferdig Member and the Kevin Member of the Marias River Formation, the Telegraph Creek, and the Eagle Sandstone Formations (Figs. 29,30). The Kevin Member of the Marias River Formation is composed of marine shales. It grades eastward into the calcareous shales in the Niobrara Formation and southward into the upper Cody Shale. Many molluscan zonal fossils of Niobrara age have been found in the Kevin Member. On the Sweetgrass Arch, early and middle Coniacian zonal fossil Inoceramus erectus, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 83 middle Coniacian Scaphites preventricosus, and Inoceramus deformis occur at its base, and late Coniacian Inoceramus involutus, Scaphites ventricosus, and Scaphites depressus occur in its middle part, and Santonian Clioscaphites choteauensis, Desmoscaphites erdmanni, Desmoscaphites bassleri, and Scaphites lee are found in its upper part (Cobban, 1955a and b; Cobban et al., 1976). These are all guide fossils of the Niobrara Formation in Colorado. In southwestern Montana, the equivalent of the Kevin Member is the upper part of the Cody Shale (Figs. 31,32). To the east, the upper part of the Cody Shale becomes increasingly calcareous and grades into the Niobrara Formation. The Niobrara Formation in Montana and the Dakotas is generally barren of age-diagnostic fossils, but the Cody Shale has yielded a few molluscan zonal fossils in the Livingston area of southwestern Montana. These fossils include the latest Coniacian-earliest Santonian Inoceramus involutus, and Scaphites depressus in a sandy unit in the middle of the Cody Shale (Roberts, 1972; Cobban et al., 1958), and middle Santonian ammonite Clioscaphites vermiformis in the upper part of the Cody Shale (Cobban, 1951b). The Telegraph Creek Formation is a upward-coarsing succession of shale, siltstone, and sandstone in western and central Montana. It is transitional from the underlying Kevin Member of the Marias River Formation or the Cody Shale to the overlying Eagle Sandstone. To the east, it grades into the Gammon Shale. Fossils are sparse and poorly preserved in the Telegraph Creek Formation, but on the Kevin-Sunburst dome (Column 1, Fig. 30), the late Santonian zonal fossil Desmoscaphites bassleri and the early Campanian Scaphites hippocrepis (DeKay) have been reported from it (Cobban, 1951a, 1955a, 1955b; Cobban et al., 1976). These are guide fossils for the uppermost part of the Niobrara Formation in Colorado. The Eagle Sandstone is a major wedge of regressive marine and nonmarine sandstone that mark the end of the Niobrara cycle. Its lower part is a marine sandstone bed called the Virgelle Sandstone. Its upper part consists of predominantly nonmarine sandstone. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 84 The contact between the Eagle Sandstone and the overlying Claggett Shale is a sharp surface that lies within meters of the Ardmore Bentonite Bed. To the east, the Eagle Sandstone thins and grades into marine, noncalcareous shale in the Gammon Shale. The Eagle Sandstone is sparsely fossiliferous, but Scaphites hippocrepis II was reported from the Virgelle Sandstone at its base (Cobban 1955a, b). In the northern Black Hills the upper part of the Gammon Shale yielded early Campanian zonal fossils Scaphites hippocrepis and Scaphites sp. (smooth) (Cobban, 1951a, 1969). Cross sections 3 and 4: western Wyoming to south Dakota and Nebraska The Upper Cretaceous series in Wyoming has a greater average thickness than almost anywhere else in the Western Interior basin. In western Wyoming, over 4000 meters of Upper Cretaceous rocks accumulated, composing a complexly intertongued succession of marine and nonmarine strata. The major lithostratigraphic units include the Frontier, the Cody/Hilliard, and the Mesaverde Formations (Figs. 33, 35). To varying degrees, these formations demonstrate lateral changes in stratal thickness, lithology, and age. In eastern Wyoming and adjacent states, Upper Cretaceous rocks are comprised predominantly of shale. In ascending order this succession consists of: the Belle Fourche Shale, Greenhorn Formation, Carlile Shale, Niobrara Formation, and Pierre Shale (Gill and Cobban, 1966a, 1966b, 1973; Merewether, 1972,1980; Merewether et al., 1977). Because the Upper Cretaceous stratigraphic succession is similar over much of Wyoming, discussion of the two cross sections is combined (Figs. 34,36). The northern cross section extends from the Jackson Hole area across the southern rim of the Bighorn basin, the Powder River basin, the Black Hills, and ends in central South Dakota (Fig. 34). As on the Montana sections, strata represented here encompass the Greenhorn and the Niobrara cycles, bounded below by the top of the Mowry Shale and above by the Ardmore Bentonite Bed. Included are the Frontier Formation and the Cody Shale in the Jackson Hole area and the Bighorn basin. East of the Powder River Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 00 Central S. Dakota Black Hills V 7 7 7 7 7 7 7 , Buffalo WallCreek Thermopolis Jackson Hole Figure Generalized 33. time-stratigraphic correlation chart forUpperCretaceous fromstrata northwestern Wyoming to SouthDakota. Albian Turom an Coniacian Santonian Campanian Cenomanian Maastrichtian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. S. BIGHORN BASIN- -POWDER RIVER BASIN- Jackson Hole Thermopolis Bighom Mts Buffalo N.W 1 10 11 meters Shannon Ss sry<-j mm /* Cody Shale r/OAVV;^v*vy I Colui 23,2 Mere Column 8: 25,27,39, *14-43,49,52,62,64: Merewether etal. (1977) Column S: •V;..;.: 30: Cobbari (1969) 24,25, 27,37: Keefer (1972) ontier Pm* 39: Merewether etal. (1975) 27: Gill and Cobban (1966a) Column 3: 30: Cobban (1969) 39: Keefer (1972) Column 2: Column 6: 37: Cobban (195lb) 43,62: Merewether et al. (1975) Column 7: | Column 1: 25,27: Keefer (1972) ! 39,49: Cobban and Reeside 2000 - (1952b) and Love (1956) Figure 34. Regional stratigraphic cross section 3 of lower Upper Cretaceous rocks from northwestern > represent individual wells (see Appendix for name and location). Projected fossil occurrences are mark to the ammonite zones in Figure 23. Location of the section is shown in Figure 20. See Figure 30 for le Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. POWDER RIVER BASIN— «------S. DAKOTA Its Buffalo N.W. Black Hills 12 13 141516 t! ! ! ! L , ?Ardmore Bentonite; ‘Shannon Sa] .Niobrara Fr iCarlile Shale* ysmmm v v v ■Belle Fourche Shal Colum n 16: 23,26,30,40 44,62,65: Merewether et al. (1977), Robinson et al. (1964) Column 8: 25,27,39, <14-43,49,52,62,64: Merewethe r et al. (1977) 30: Cobban (1969) 72) 75) a) 1.(1975) >er Cretaceous rocks from northwestern Wyoming to South Dakota. Vertical lines and the numbers above n). Projected fossil occurrences are marked by small triangles followed by numbers that correspond shown in Figure 20. See Figure 30 for legends. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 00 cSieenbornn Nebraska Medicine Bow Rawlins W T |l IlHlflililll m m m m m U plift Rock Springs M M Pii! Thrust B ek Figure 35. Generalized time-stratigraphic correlation chartforUpper Cretaceous fromstrata southwesternWyoming to Nebraska. Albian Santonian Coniacian Turoman Campanian Maastrichtian Cenomanian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. GREATER GREEN LARAP RIVER BASIN BASH Moxa Rock Springs Rawlins Medicine Lararr Arch Uplift Bow |<»or Jl 7 8 9 1 0 11 1 1 'li '.B ail Blair si-V'-V'/vV-V. meters ; A j** *■ ' ‘ • ; ’ f, Hilliard Shale •* c* r ^ ’irPl* 't - . I - , ' Column 13: s m t a 42,43: Merewethe V v--V ’» M erewether and C HM j Colum n 11: ' 39,43,47,62: Cobban (1951b] 1000- Colum n 10: 39,43,47,63: Merewether (1983b) Column 9: (composite): 30,32,35: Smith (1965) VjToniicrFnr Column Smith Column Merewether .•Aspen Column 1 2000-1 40: Merewether (1983b) Figure 36. Regional stratigraphic cross section 4 of lower Upper Cretaceous rocks from so represent individual wells (see Appendix for name and location). Projected fossil occurrenc to the ammonite zones in Figure 23. Location of the section is shown in Figure 20. See Figi Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. LARAMIE DENVER TO NEBRASKA BASIN BASIN Medicine Laramie Cheyenne Bow 18 15i 16i 17i <2?*v V 4 { .*. .- + '- ^ -t I i i i I i i—I i i i I i i i i I i i jj-.i- • L .-r ~*~t t t t t + ti-t -t- -f- ■*■ t ^ ^ ■ Front er Belle Fourche Soil Column 16: 25: Kitely (1978) Column 13: 42,43: Merewether et al. (1979) Merewether and Cobban (1972) I Column 11: ' 39,43,47,62: Cobban (1951b) 100 200 km mn 10: 3,47,63: Merewether (1983b) (composite): Smith (1965) pper Cretaceous rocks from southwestern Wyoming to Nebraska. Vertical lines and the numbers above on). Projected fossil occurrences are marked by small triangles followed by numbers that correspond s shown in Figure 20. See Figure 30 for legends. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 89 basin, equivalent strata consist of the Belle Fourche Shale, Greenhorn Formation, Carlile Shale, Niobrara Formation, and lower part of the Steele Shale. Four time lines are drawn on the basis of fossil data and lithologic marker beds. The southern cross section begins near Kemmerer, crosses the Rock Springs Uplift, and ends near the northeast margin of the Denver basin (Fig. 36). Strata included here are late Cenomanian to Santonian in age; early Campanian strata in the upper part of the Niobrara cycle are excluded because of insufficient age-diagnostic fossil data. In lithostratigraphic terms, this interval consists of the Frontier Formation and the Hilliard Shale in the Kemmerer area; the Frontier Formation and the lower part of the Baxter Shale in the Rock Springs Uplift area; the Frontier Formation and the Niobrara Formation in Laramie and Denver basins; and the Graneros/Belle Fourche Shale, Greenhorn Formation, Carlile Shale, and Niobrara Formation in Nebraska. Three time lines are drawn on the cross section on the basis of fossil data and lithologic marker beds. Greenhorn age The Frontier Formation and its temporal equivalents elsewhere, such as the Ferron Sandstone of central Utah, represent a major regressive clastic wedge along the western part of the Western Interior basin (Cobban and Reeside, 1952b). As defined in western Wyoming, the Frontier Formation consists of those strata that lie between the top of the hard siliceous marine shale of the Aspen or Mowry Shale, and the top of the highest sandstone below the soft black marine shale of the Cody/Hilliard Shale. The Frontier Formation, of both marine and nonmarine origin, comprises an alternating succession of sandstone and shale with minor amounts of bentonite and coal beds. The thickness of the Frontier Formation ranges from less than 50 meters on the Rock Springs uplift to more than 700 meters near the thrust belt (Figs. 34,36). Inasmuch as the sandstone that defines the top of the formation intertongues and passes into shale to the east, the lithological boundaries of the Frontier Formation become progressively older in that Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 90 direction. The Frontier Formation is gradational with both the underlying Mowry Shale and the overlying Cody/Hilliard Shale. However, internally, the Frontier Formation is punctuated by several unconformities (Merewether and Cobban, 1986). The Frontier Formation is in excess of 300 meters thick in Jackson Hole area, about 150 meters on the southern flank of the Bighorn basin, and nearly 180 meters in the Powder River basin (Fig. 34). Its lithofacies changes laterally from interbedded marine and nonmarine sandstone and shale in Jackson Hole area to fully marine shale and sandstone in the Powder River basin, where it is divided into the Belle Fourche Shale, the Wall Creek Sandstone, and the intervening "unnamed Member" (Merewether et al., 1977,1979). In the Black Hills, the correlative of the Frontier Formation consists of the Belle Fourche Shale, the Greenhorn Formation, and the Carlile Shale. Ammonites and bivalves have been found in the upper part of the Frontier Formation; they are sparse to absent at most other horizons. The reported collections of zonal fossils include: Collignoniceras woollgari from the Jackson Hole area (Cobban and Reeside, 1952b; Love, 1956), Dunveganoceras pondi from the eastern flank of the Bighorn Mountains (Merewether et al., 1975), and Dunveganoceras pondi and Collignoniceras woollgari from the western flank (Merewether et al., 1977). These are late Cenomanian to early Turonian guide fossils of the Greenhorn Formation in Colorado. In and east of the Powder River basin, late Turonian-early Coniacian molluscan zonal fossils Dunveganoceras pondi through Inoceramus erectus have been found in abundance in the Frontier Formation or its equivalent (Merewether and Cobban, 1986; Cobban, 1958a). At its type locality at Cumberland (about 30 miles southwest of Column 1, Fig. 36), the Frontier Formation consists of 700 meters of sandstone, siltstone, mudstone, and minor amounts of coal and bentonite beds (Cobban and Reeside, 1952b). The lower half of the Frontier Formation consists of nonmarine sandstone and mudstone, whereas the upper half consists of interbedded, predominantly marine sandstone and shale. The Frontier Formation thins to the east and grades into increasingly marine rocks with fewer Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 91 and thinner sandstones beds. Near Rawlins, the Frontier Formation is a fully marine succession totaling 150 to 200 meters in thickness. It comprises the Belle Fourche Shale, the Wall Creek Sandstone, and the intervening "unnamed Member" (Merewether and Cobban, 1972; Merewether et al., 1979). Fossils are generally sparse in the Frontier Formation. However, the early-middle Turonian zonal fossils Mammites nodosoides and Collignoniceras woollgari have been reported from the upper part of the Frontier Formation (Allen Hollow Member and the Oyster Ridge Sandstone) in the Kemmerer area (Merewether, 1983b; Merewether and Cobban, 1986). In southeastern Wyoming, late Turonian to early Coniacian zonal fossils Scaphites whitfieldi, Inceramus erectus, and Prionocyclus quadratus have been collected from the Wall Creek Sandstone (Merewether et al., 1979). The Frontier Formation in western Wyoming spans much of the Greenhorn cycle. The transgressive phase of the Greenhorn cycle was recorded by the regressive sandstone and interbedded siltstone in the lower part of the Frontier Formation in western and central Wyoming, and by the lower part of the Belle Fourche Shale in eastern Wyoming and beyond. The Greenhorn regression is recorded by one or more unconformities in the Frontier Formation. According to Merewether (1983b), Merewether et al. (1975,1976, 1984), and Merewether and Cobban (1973,1985,1986), a regional unconformity may be found in the upper Frontier Formation throughout Wyoming, separating the upper predominantly marine sandstones (Wall Creek) from the lower marine and nonmarine sandstones and shales. Niobrara age In western Wyoming, strata of the Niobrara cycle are represented by the uppermost marine and nonmarine Frontier sandstone, the overlying marine shale, and the lower part of the Mesaverde Formation (Figs. 33,35). Many names have been given to this marine shale unit (Gill et al., 1970). In southwestern Wyoming, it is named the Hilliard or Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 92 Baxter Shale. In the remainder of Wyoming and Montana, it is called the Cody Shale. Where the Niobrara limestone beds can be recognized, the marine shale above the Niobrara Formation is named the Steele Shale, as in eastern Wyoming, or the Pierre Shale, as in eastern Colorado, Nebraska, and western Kansas. The Cody/Hilliard Shale consists of shale and minor amounts of thin bentonitic, calcareous, and fine-grained sandstones and siltstone beds. It intertongues extensively with the overlying marine and nonmarine sandstones of the Mesaverde Formation. As a result, the upper boundary of the Cody/Hilliard Shale rises stratigraphically eastward as successively younger Mesaverde sandstone tongues pass into shales (Figs. 33,34,35). The Ardmore Bentonite Bed can be recognized on wireline logs in northern Wyoming, but its lithologic identity becomes lost in southern Wyoming. The Cody/Hilliard Shale is moderately fossiliferous at some horizons. These fossils permit stratigraphic correlations in this otherwise nondescript shale unit. Reported collections of molluscan zonal fossils include: the late Coniacian Scaphites depressus from the flanks of the Bighorn basin (Cobban, 1951b, Keefer, 1972), the middle Santonian Clioscaphites vermiformis and late Santonian Desmoscaphites bassleri in the Rock Springs Uplift and Rawlins area (Smith, 1961,1965; Cobban and Reeside, 1951; Gill et al., 1970), the early Campanian Scaphites hippocrepis and Baculites sp. (weak flank ribs) in the Black Hills (Cobban, 1969; Robinson et al., 1964). Cross sections 5: central Utah to Denver Basin Upper Cretaceous rocks are well exposed in central Utah and northern Colorado. Regionally, they display similar intertonguing facies relationships to those in Wyoming. However, a different set of lithostratigraphic nomenclature has been applied (Fisher et al., 1960; Fouch et al., 1983; Molenaar and Rice, 1988). Near the Sevier thrust belt in central Utah, the bulk of the Upper Cretaceous rocks are composed of synorogenic conglomerates of the Indianola Group. The Indianola Group, aggregating over 4000 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 93 meters locally, grades rapidly eastward into a series of sandstone beds that intertongue with the marine Mancos Shale farther to the east. The Mancos Shale consists of marine shale and siltstone and correlates broadly to the Hilliard/Cody Shale in Wyoming. It attains a thickness over 1 km in many areas of eastern Utah and western Colorado. In eastern-central Utah, the major sandstone units intertonguing with the Mancos Shale are the Ferron Sandstone, Emery Sandstone, Star Point Sandstone, Blackhawk Formation, and Castlegate Sandstone (Fig. 37). These sandstone tongues break the Mancos Shale into the Tununk Shale, lower Blue Gate Shale, and upper Blue Gate Shale members. Most of these coastal sandstones pinch out in northwestern Colorado. There, the Mancos Shale is a monotonously uniform shale succession containing only the Juana Lopez siltstone bed near its base and the sandy Mancos B zone in its upper part. Farther east, in the Denver basin, the Upper Cretaceous rocks are distinguished by abundant calcareous marine shale and limestone beds much like those in the Pueblo area in terms of lithology and nomenclature. This cross section (Fig. 38) extends across three Laramide basins: the Uinta, Piceance Creek, and Denver basins (Fig. 20). Strata selected on this cross section span not only the Greenhorn and Niobrara cycles, but also the early phase of the Claggett cycle. This package is bounded by the Mowry Shale and the top of the Castlegate Sandstone or its correlative strata to the east (within the Baculites gilberti or Baculites perplexus zones). Correlations of these rocks between basins are reasonably well constrained owing to the available subsurface as well as surface data. Six time lines were established along the cross section by using lithologic marker beds and fossil data where available. Greenhorn age The Mowry Shale deposited during the initial Greenhorn transgression is confined to areas north of northeastern Utah and central Colorado (Fig. 28 a). Rocks in eastern Utah Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 4^ VO F m V * V A W GreenhornFm Niobrara ' t ' i 'w * *- * £r« .miner kRid and K«» I I DenverBasin irfox'fflllsSs'- «.> irfox'fflllsSs'- /Hygiene as/Hygiene Kremling Front Range Kremlu s MancosShale fuahaLopez Mbr Douglas Arch BuckTong l*kkhi*k I m Emery Ss, egatess. UintaBasin Figure 37. Generalized time-stratigraphic correlation chartUpperfor Cretaceous fromstrata Uinta to Denver Basins. Albian Turonian Coniacian Santonian Campanian Cenomanian Maastrichtian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. —PICEANCE CREEK-*. _N. PA UINTA BASIN- BASIN BAS Salina Sunnyside Douglas Arch Meeker Kremlin 7 8 9 10 12 1314 15 16 171819 2021 22 unu a* meters erreS ht "v Mancos S lu le -o r/ 'V-1 * 1000 - 2 1 ,2 3 ,2 4 Izett et al. 39 and 43- i3 7 an d 4 6 : 40,44: Iz< P 24, and 26 Cullins (1969) ^ B lu c G itc S Gill and Hail (1975) | 21 and 23: ! i i i i i i i Gill and Hail (1975)| i i i i ! 29,' 3 2 ,3 5 ,3 7 ,3 8 ,4 4 ,4 6 ,4 7 , 21,24,25, and i 49, and 63: Fisher et al. (1960) 26: Hail (1974) 63: Katich (1954) 2000H i29 and 35: Cobban (1976) i 44 and 47: Esher et al. (1960) Tununk Shale 55-56: Zelt (1985) M m - Figure 38. Regional stratigraphic cross section 5 of lower Upper Cretaceous rocks from central Utah to western IS (see Appendix for name and location). Projected fossil occurrences are marked by small triangles followed by nun section is shown in Figure 20. See Figure 30 for legends. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. NCE CREEK — _N. PARK DENVER BASIN- \SIN BASIN Meeker Kremling Boulder 16 17>8 19 2021 22 23 24 25 26 28 29 30 31 Kremling .Ss £ N io b ram F CSrlfleSha Orccnboro F m IM owrySna Ptenr Shale 20 (21?), 2 3 ,2 4 , and 25 Scotland Cobban (1965) 34,39, and 43: Scott (1963) * 62: Scott (i9 6 2 ) 21,23,24,25, and 26: Izett etal. (1971) 39 and 43-45: Hail (1968) 40,44: Izett (1968) 200 km fail (1975) • 21,24,25, and 26: Hail (1974) i rocks from central Utah to western Nebraska. Vertical lines and the numbers above represent individual wells ;ed by small triangles followed by numbers that correspond to the ammonite zones in Figure 23. Location of the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 96 that are correlative with the Mowry Shale include the nonmarine sandstones in the upper part of the undifferentiated Dakota Sandstone and the Cedar Mountain Formation of Aptian to early Cenomanian age (Molenaar and Cobban, 1991). In much of northern Colorado and northeastern Utah, the Mowry Shale retains its distinct lithology and log patterns, but it is only about 20 meters thick, considerably thinner than to the north. In east-central Utah, the oldest fully marine unit resulting from the Greenhorn transgression is the Tununk Shale Member of the Mancos Shale. The Tununk Shale consists of shale, siltstone, and minor amounts of bentonite beds. Many bentonite beds can be traced laterally over long distances (Zelt, 1985). Its contact with the underlying Dakota Sandstone is conformable. The contact with the overlying Ferron Sandstone is also gradational. The thickness of the Tununk Shale decreases rapidly to the northeast, from over 200 m on the Wasatch Plateau to only 30 m near the Utah-Colorado state line (Ryer and McPhilips, 1983). Molluscan fossils are fairly abundant in the Tununk Shale. In eastern Utah, the late Cenomanian bivalve Pycnodonte newberryi (formerly Gryphaea newberryi) has been widely reported in beds a few meters above its base (Dane, 1935; Katich, 1954; Young, 1960; Fisher and others, 1960); the middle Turonian zonal fossil Collignoniceras woollgari has been found in a sandy unit (Coon Spring Sandstone) in the middle of the Tununk Shale (Molenaar and Cobban, 1991); and the late middle Turonian zonal fossil Prionocyclus hyatti in the basal beds of the overlying Ferron Sandstone (Cobban, 1976; Cobban and Hook, 1980; Molenaar and Cobban, 1991). Near the Colorado state line, the slightly older late Cenomanian zonal fossil Duvenganocems albertense has been found in the basal part of the Mancos Shale (Fouch et al., 1983). In central Utah, Collignoniceras woollgari was also found in the basal beds of the Ferron- equivalent strata of the Funk valley Formation (Ryer and McPhilips, 1983). These fossils indicate that the base of the Tununk Shale becomes progressively younger and its top progressively older to the west. In general terms, the total Tununk Shale is approximately correlative with the Bridge Creek Limestone and the Carlile Shale of Colorado. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 97 The regressive phase of the Greenhorn cycle is represented in eastern Utah by the lower Ferron Sandstone Member, an eastward-thinning sandstone wedge contemporaneous with the upper part of the Frontier Formation in Wyoming. The Ferron Member is nearly 300 m thick on the Wasatch Plateau, but pinches out rapidly eastward. The upper part of the Ferron grades into the marine siltstone and shale of the Juana Lopez Member (Molenaar and Cobban, 1991). The Ferron Sandstone Member consists of sandstones interbedded with minor amount of shales, and coal beds. The basal Ferron Sandstone is a coastal sandstone unit gradationally overlying the Tununk Shale. The upper Ferron Sandstone, sharply overlain by the main body of the Mancos Shale and confined west of Price, consists of interbedded deltaic/fluvial sandstone and shale that thin and become increasingly marine to the east (Molenaar and Cobban, 1991; Ryer and McPhilips, 1983). Many ammonites and bivalves have been collected from the marine beds in the Ferron Sandstone Member and from its correlative to the east, the Juana Lopez Member. They span three or four molluscan fossil zones, ranging from the middle Turanian Prionocyclus hyatti to late Turanian Inocemmus perplexus (Fisher et al., 1960; Molenaar and Cobban, 1991). These fossils indicate partial equivalence of the Ferron Sandstone to the Codell Sandstone and Juana Lopez Member in eastern Colorado and western Kansas (Fig. 37). Niobrara age Strata of the Niobrara cycle are represented by the upper part of the Ferron Sandstone, Blue Gate Shale Member of the Mancos Shale, the Star Point Sandstone, and the Blackhawk Formation in central and eastern Utah; by the main body of the Mancos Shale in northwestern Colorado; and by the Niobrara Formation and the lower part of the Pierre Shale in northeastern Colorado. The Blue Gate Shale Member conformably overlies the Ferron Sandstone Member and underlies the Star Point Sandstone and the Blackhawk Formation. It is separated into Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 98 a lower tongue and an upper tongue (or the Masuk Shale) by an eastward thinning sandstone wedge, the Emery Sandstone. Where the Emery Sandstone pinches out, the marine shale equivalent to the Blue Gate Shale is called the Mancos Shale. The total thickness of the Blue Gate Shale Member, including that of the intervening Emery Sandstone, averages about 1 km in central Utah. Toward the thrust belt, the Blue Gate decreases in thickness as it grades to the sandstone and conglomerate of the Funk Valley Formation (Molenaar and Rice, 1988). The upper boundary of the Blue Gate rises stratigraphically eastward with the pinchout of successively younger sandstone beds in the Star Point Sandstone and the Blackhawk Formation. On the Douglas Arch and in the western Piceance Creek basin, the Mancos Shale contains in its upper part a regionally extensive sandy unit locally called the "Mancos B" (Kellogg, 1977; Cole and Young, 1991). This sandy interval was formerly correlated with the Emery Sandstone in central Utah (Fouch et al., 1983), but correlations of this study suggest that it correlates with the younger Star Point Sandstone. Molluscan fossils are moderately abundant in the Blue Gate Shale Member. In central Utah, early Coniacian Scaphites preventricosus and middle Coniacian Inoceramus deformis have been reported in the basal Blue Gate Shale Member; middle Santonian Clioscaphites vermiformis and late Santonian Desmoscaphites bassleri in the basal Emery Sandstone; and early Campanian Scaphites hippocrepis in the upper Blue Gate Shale Member (Fisher et al., 1960; Cobban, 1976). These limited fossil collections indicate that the Blue Gate and the intervening Emery Sandstone are the temporal equivalent of the Niobrara Formation in eastern Colorado and western Kansas. The Star Point Sandstone is the oldest sandstone tongue overlying the Blue Gate Shale. It is less than 100 m thick on the Wasatch Plateau and pinches out rapidly to the east. No age-diagnostic fossils have been collected from the Star Point Sandstone, but Fouch et al. (1983) assigned the Star Point Sandstone to the latest Santonian and early Campanian through correlation to ammonite bearing beds along the Book Cliffs. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 99 Overlying the Star Point Sandstone, the Blackhawk Formation is a succession of nonmarine and marine sandstones comprising as many as six eastward-thinning sandstone tongues or members (Young, 1955). Each tongue thins and becomes increasingly marine to the east. Together, successively younger tongues step farther basinward. The contact between the Blackhawk Formation and the overlying Castlegate Sandstone is a major unconformity in Utah but becomes conformable towards the Colorado state line, where the youngest Blackhawk sandstones pinch out. The Castlegate Sandstone is areally the most extensive sandstone tongue in the Mancos Shale. It thins and becomes increasingly marine to the east. It pinches out east of the Colorado State line in the Piceance Creek basin. Its contact with the overlying Mancos Shale is a sharp but conformable surface. Because of sufficient wireline log control and a fair amount of fossil data, this surface has been correlated as far east as the Denver basin. The Castlegate Sandstone and the shale immediately below and above have yielded many ammonite zonal fossils, particularly along the Book Cliffs (Gill and Hail, 1975). These include lower middle Campanian Baculites macleami and Baculites asperiformis in the Castlegate Sandstone and the underlying shale, and the middle Campanian Baculites perplexus at the base of the overlying Buck Tongue of the Mancos Shale. Cross section 6: Kaiparowits region-San Juan Basin-Raton Basin-Pueblo Upper Cretaceous rocks are only sporadically preserved in the southern part of the Western Interior basin as a result of widespread post-Cretaceous uplift and erosion. Areas with extensive Upper Cretaceous deposits include: the Kaiparowits Plateau, the Henry Mountains region, the Black Mesa, San Juan, and Raton basins (Fig. 20). Upper Cretaceous rocks vary with location in thickness, lithofacies, and stratigraphic nomenclature (Fig. 39). On the Kaiparowits Plateau, the Upper Cretaceous series is about 2350 m in total preserved thickness. Its lower 600 meters is a predominantly marine unit composed of the Dakota Sandstone and the Tropic Shale, and the remainder Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. r 8 Vc rroc Vc Raton Basin ^ |♦ ... » QitlaodFm/yy San Juan Basin SW U plift M onum ent Henry region M ountains rowitsFm Drip TankDrip Mbr S.W. Kaiparowits Kaiparowits regionto Raton Basin. Figure Generalized 39. time-stratigraphic correlation chartUpperfor Cretaceous from strata Albian Turanian Coniacian Santonian Campanian Cenomanian Maastrichtian Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. KAIPAROWITS HENRY MTS SAN Jl REGION REGION BASI] Cedar City Hatch Mt Ellen Ship Rock 1 2 0 meters \\i'\lA•*.% i:y:y.y •* *.*•’> AV^V^V*‘V*.V*.' John Henry M b r\ •*.*.•>. •'/.•*. y.Sinujjju CIilT»Fn>\%;’.V ^ v T j 7 . » 7 ; |.;,'.1,'.Ferron&>.*.■ ■ f . ^ *' '« ^46n,<7 Br d jc Creek La Turn nk V p a k o to & \j< ...... 32,35,39,44-47: Reeside (1924) 32,35,37,46-47,51, and 55- 44-47: Dane et al. (1966), SVM* Peterson and Ryder (1975) Hook and Cohhan ( 19801 59,62: Cobban et al. (198‘ 1000 - * 58-60: Cobban and Hook (1984) 38,46-47: Peterson (1969) 49 and 55-58: Lawrence (1965), Peterson and Kirk (1977), Zelt (1985) 49: Lessard (1973) 55-58: Moir (1974) Figure 40. Regional stratigraphic cross section 6 of lower Upper Cretaceous rocks from southern Utah to (see Appendix for name and location). Projected fossil occurrences are marked by srnall triangles folio wet section is shown in Figure 20. See Figure 30 for legends. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. SAN JUAN RATON BASIN BASIN Ship Rock El Vado Trinidad 10 11 To Alwood, KS * Mancos * v «44-47 CanileSba f ' Juana LopezK 33,35,38,41,42: Scott et al. (1986) 50,62: Kauffman et al. (1969) ...... i t 'i ‘ I i i ^ 32,35,39,44-47: 25: Cobban, Landis, and Dane (1974) Reeside (1924) 30: Cobban (1969) 44-47: Dane et al. (1966), 38,39,44: King (1974) and Dane (1960) Hnok and Cobban (10801 59,62: Cobban et al. (1989) 50,59: Landis et al. (1973) 100 200 km . i.. :eous rocks from southern Utah to western Kansas. Vertical lines and the numbers above represent individual wells marked by small triangles followed by numbers that correspond to the ammonite zones in Figure 23. Location of the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 1 0 2 of the section is a predominantly nonmarine unit comprising the Straight Cliffs and the Wahweap Formations (Peterson, 1969). In the Henry Mountains region, Upper Cretaceous rocks were more deeply eroded, preserving only the lower 1300 meters. The section here comprises the Dakota Sandstone, Tununk Shale, Ferron Sandstone, and Mancos Shale. In the San Juan basin, over 2000 meters of Upper Cretaceous rocks are preserved (Molenaar, 1983). In the southwest part of the basin, rocks are predominantly nonmarine sandstone and shale. To the northeast, they pass into the marine shale of the Mancos and Lewis Shales by facies changes (Molenaar et al., in press). Because of the complex intertonguing marine and nonmarine formations across the basin, stratigraphic nomenclature varies with location. In the Raton basin, the lithofacies and stratigraphic nomenclature of the Upper Cretaceous rocks are similar to those at Pueblo, Colorado (Kauffman et al., 1969; Scott et al., 1986). This cross section begins in the Kaiparowits Plateau, crosses the Henry Mountains, San Juan and Raton basins, and ends in western Kansas (Fig. 40). The interval selected is that of the Greenhorn cycle and the early and middle part of the Niobrara cycle. Because of the absence of Mowry Shale, the initial Greenhorn transgressive surface at the top of the Dakota Sandstone was chosen as the oldest horizon in the subsequent backstripping analysis. Four time lines were established along the cross section on the basis of lithologic marker beds and fossil records. These lines are well constrained by fossil data in and east of the San Juan basin. However, uncertainties exist in correlations of strata of the Niobrara age in the Kaiparowits Plateau and the Henry Mountains region because of erosion, increased amount of nonmarine strata, and the scarcity of age- diagnostic fossils. Greenhorn age The Greenhorn sea did not flood the southwestern part of the Western Interior basin until near its peak transgression in the late Cenomanian-early Turanian. Therefore, in the Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 103 Kaiparowits, Henry, and much of the San Juan basins, early transgressive deposits of the Greenhorn cycle equivalent to the Mowry Shale are absent. The oldest rocks of the Greenhorn age are probably the Dakota Sandstone of late Cenomanian age. The Dakota Sandstone in these basins is commonly less than 100 meters thick and consists of nearshore marine sandstone in its uppermost part and nonmarine sandstone and shale in the rest of the section. It unconformably overlies the Lower Cretaceous Cedar Mountain and Burro Canyon Formations or older rocks, and is overlain conformably by the marine Mancos Shale. In the Kaiparowits Plateau and Henry Mountains region, the late Cenomanian zonal fossil Pycnodonte newberryi has been found at the top of the Dakota Sandstone or the base of the overlying shale (Peterson and Ryder, 1975; Moir, 1974; Lawrence 1965). In the San Juan basin, where a greater part of the Dakota is of marine origin, middle and late Cenomanian zonal fossils, from Acanthoceras amphibolum to Dunveganoceras pondi, have been reported (Molenaar et al., in press). These fossils indicate that the Dakota Sandstone in these areas is approximately contemporaneous with the Belle Fourche/Graneros Shale and the lower part of the Greenhorn Formation at Pueblo. On the cross section in Fig. 40, the oldest time line follows the top of the Dakota Sandstone in the Kaiparowits, Henry, and much of the San Juan basins. In and east of the Raton basin, this line follows the top of the Graneros Shale; the Dakota Sandstone here is Albian-early Cenomanian in age and much older than to the west. The marine shale overlying the Dakota Sandstone is called the Tropic Shale in the Kaiparowits Plateau region and the Tununk Shale in the Henry Mountains region (Peterson, 1969; Peterson et al., 1980; Peterson and Ryder, 1975; Zelt, 1985). The Tropic/Tununk Shale thins eastward from over 300 meters in the Kaiparowits Plateau region to less than 200 meters in the Henry Mountains region. In the San Juan basin, equivalent rocks are the basal Mancos Shale sandwiched between the Dakota Sandstone and the Juana Lopez Member, including the Bridge Creek Limestone Member and the Gallup Sandstone (Molenaar, 1983 ; Molenaar et al., in press). The average thickness of Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 104 this interval is about 200 meters. Molluscan zonal fossils are fairly abundant at many horizons in the Tropic/Tununk Shale and their equivalents. The lower part of the Tropic Shale in the Kaiparowits Plateau has yielded the late Cenomanian Sciponceras gracile and the middle Turanian Collignoniceras woollgari (Lawrence, 1965; Moir, 1964; Zelt, 1985). In the Henry Mountains region, the Tununk Shale yielded the early Turanian Mytiloides mytiloides in its lower middle part, the middle Turanian Collignoniceras woollgari in its middle part, and the early late Turanian Prionocyclus macombi in its upper part (Peterson and Ryder, 1975). In the San Juan basin, molluscan zonal fossils Sciponceras gracile through Collignoniceras woollgari have been collected in the correlative interval (Molenaar et al., in press). Bentonite beds ranging in thickness from centimeters to tens of centimeters are quite abundant in the Tropic Shale and its lateral equivalents to allow correlations between basins. On this cross section, correlations in the Kaiparowits Plateau region relied on the work of bentonite correlations by Zelt (1985). Overlying the Tropic Shale in the Kaiparowits Plateau is the Straight Cliffs Formation, a predominantly nonmarine succession of sandstone, mudstone, and coal with an aggregate thickness of over 500 meters. The Straight Cliffs Formation comprises, in ascending order, the Tibbet Canyon, Smoky Hollow, John Henry, and Drip Tank Members (Peterson, 1969; Peterson and Kirk, 1977). The Tibbet Canyon Member is a nearshore marine sandstone unit transitional between the underlying marine Tropic Shale and the overlying nonmarine Smoky Hollow Member. It averages about 30 meters in thickness and contains the early middle Turanian bivalve Inoceramus howelli of thePrionocyclus hyatti zone (Peterson, 1969). The Smoky Hollow Member is a unit composed of nonmarine sandstone, mudstone, and coal. Its thickness is highly variable, from 30 meters in southern Kaiparowits Plateau to 300 meters in northern Kaiparowits Plateau. No age-diagnostic fossils have been found in the Smoky Hollow Member, but because it is conformable with the underlying Tibbet Canyon Member, it is probably only slightly younger. The Smoky Hollow Member is unconformably overlain by the John Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 105 Henry Member, a succession of intertongued marine and nonmarine rocks. Above the unconformity, the late Coniacian bivalve Inoceramus stantoni or kleini has been found in the lower westward-thinning marine shale tongue of the John Henry Member (Peterson, 1969). This fossil and the Inoceramus howelli from the Tibbet Canyon Member suggest that this unconformity could span late Turanian to middle Coniacian. It probably correlates with the regional unconformity of lesser magnitude near the top of the Frontier Formation in Wyoming. In the Henry Mountains region, strata equivalent to the Tibbet Canyon and Smoky Hollow Members are represented by the Ferron Sandstone, the lateral extension of the Ferron Sandstone in central-eastern Utah. The Ferron Sandstone averages about 80 meters and consists of marine sandstones in the lower part and nonmarine sandstones, mudstones, and coals in the upper part. It is in gradational contact with the Tununk Shale below but separated from the Blue Gate Shale by an unconformity (Peterson and Ryder, 1975). Below the unconformity, the lower marine part of the Ferron Sandstone has yielded the middle Turanian zonal fossil Inoceramus howelli. Above the unconformity, the basal part of the Blue Gate Shale contains the late Coniacian inoceramids, either Inoceramus stantoni or 7. kleini. This unconformity correlates with the one separating the Smoky Hollow Member from the John Henry Member in the Kaiparowits Plateau (Peterson and Kirk, 1977). In the southwestern San Juan Basin, strata correlative with the Ferron Sandstone are the Tres Hermanos Formation, a northeast-thinning wedge of nonmarine and nearshore marine sandstones. Middle to late Turanian fossils such as Collignoniceras woollgari and Lopha lugubris have been reported from the Tres Hermanos Formation (Molenaar et al., in press). Because the cross section in Fig. 40 crosses the San Juan Basin farther north, it does not include the Tres Hermanos Formation. Instead, only its offshore equivalent Mancos Shale is shown. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 106 The Niobrara age Initial transgressive strata of the Niobrara cycle, such as the Juana Lopez Member of the Mancos Shale and the Fort Hayes Limestone Member of the Niobrara Formation in Colorado, are not present in the Kaiparowits Plateau and Henry Mountains region (Fig. 39). This period of time was probably recorded by the predominantly regressive, nonmarine deposits of the Smoky Hollow Member, the upper nonmarine Ferron Sandstone, and the unconformities above them. In the Kaiparowits Plateau, strata deposited during the remainder of the Niobrara include the John Henry and Drip Tank Members of the Straight Cliffs Formation, and possibly part or all of the overlying Wahweap Formation (Peterson and Kirk, 1977). These rocks are predominantly nonmarine sandstones, mudstones and coals. Their total thickness averages about 600 meters. Owing to the scarcity of age-diagnostic fossils, considerable uncertainties exist with respect to their ages. In the Henry Mountains region, strata of the Niobrara cycle includes the Mancos Shale and the Muley Canyon Sandstone. The Mancos Shale in that area averages about 450 meters in thickness. It has yielded several Coniacian and Santonian molluscan zonal fossils, including Scaphites depressus, Clioscaphites vermiformis, and Desmoscaphites bassleri (Peterson and Ryder, 1975). Conformably overlying the Mancos Shale, the Muley Canyon Sandstone is a regressive sandstone unit and averages about 90 meters in thickness. Its lower part consists of nearshore marine sandstone and the upper part is composed of nonmarine sandstone. The Muley Canyon Sandstone here is stratigraphically unrelated to the Emery Sandstone in central Utah. According to Peterson et al. (1980) and Maxfield (1976), the Muley Canyon Sandstone in the Henry Mountains region is of early Campanian age and correlate with the Star Point Sandstone and the lower Blackhawk Formation in east-central Utah (Fig. 37). Unlike in the Kaiparowits Plateau and the Henry Mountains region, strata of the Niobrara age are well preserved in the San Juan basin and contain molluscan fossils (Fig. 40). However, considerable difference exists between the local stratal stacking pattern Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 107 and the transgressive-regressive trends observed elsewhere (Fig. 39). On the western side of the San Juan basin, the early phase of the Niobrara cycle is recorded by the Juana Lopez Member and the predominantly regressive nearshore marine sandstones of the Gallup Sandstone. It is noteworthy that the Gallup Sandstone has no lateral correlatives in the Kaiparowits Plateau and Henry Mountains region (Molenaar, 1983; Peterson and Kirk, 1977). The remainder of the Niobrara cycle in the western San Juan basin was recorded by the northeast-thinning wedges of the Crevasse Canyon Formation, the Point Lookout Sandstone, and the intervening southwest-thinning Mulatto and Satan Tongues of the Mancos Shale (Molenaar et al., in press). On the cross section in Fig. 40, which is seaward of these intertonguing units, these formations are represented by their offshore equivalents in the Mancos Shale. In the northeastern San Juan basin, strata of the Niobrara cycle consists of the Juana Lopez Member and the overlying Mancos Shale. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 4 BACKSTRIPPING ANALYSIS INTRODUCTION With few exceptions, stratigraphic successions attaining significant thickness reflect continued tectonic subsidence. Determination of tectonic subsidence from basin stratigraphy constitutes an important aspect of basin analysis. Early studies generally relied on isopach maps or rock thickness-time diagrams to portray the trends of tectonic subsidence. Although fairly effective in portraying the long term trends and dominant patterns of tectonic subsidence, raw sediment thickness is not an accurate measure of tectonic subsidence for detailed quantitative subsidence analysis. Sleep (1971) discussed the complicating effects on subsidence analysis due to such factors as isostasy of sedimentation, compaction, eustatic changes, and differences in sedimentary facies. These concepts were later integrated into what is now known as the backstripping techniques. The quantitative procedures of backstripping techniques were formulated by Watts and Ryan (1976). Since then, they have been widely used as a powerful means of extracting tectonic subsidence from stratigraphic records in many sedimentary basins around the world (e.g., Steckler and Watts, 1978; Sclater and Christie, 1980; Bond and Kominz, 1984). Compared to the use of gross rock thickness, backstripping techniques provide a more rigorous quantity that relates to with calculations of various basin models. Furthermore, backstripping analysis facilitates comparison of results from different areas, or basins. Indeed, since it was first formulated a little more than a decade ago, the backstripping technique has been instrumental to the improved understanding of many sedimentary basins. This chapter briefly outlines the principles of backstripping and discusses step by step the procedures of flexural backstripping as applied in the Cretaceous Western Interior 108 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 109 basin. These procedures include flexural unloading of sediments, decompaction, and correction for water depths. At the end of this chapter, a brief discussion is given of the errors arising from various possible sources. AIRY BACKSTRIPPING Backstripping techniques were invented to extract tectonic subsidence from stratigraphic records, i.e., that part of subsidence not attributable to sediment loading, compaction, sea level changes, and paleowater depths. According to the types of isostasy taken to calculate sediment loading (Airy, 1855; Barrell, 1914), two types of backstripping analysis are generally recognized in the literature: Airy backstripping and flexural backstripping (Fig. 41). Following Steckler and Watts (1978), the general formula of Airy backstripping is: Y = s pm1pi+W d_ ASL_P=_ (1) pm - pw pm - p« where S is the decompacted sediment thickness, Wd is the water depth, ASL is eustatic sea level change (positive for a rise), and p m , p s , and p * are the mantle, bulk sediment, and water densities respectively. The above Airy backstripping scheme applies to individual stratigraphic columns. It requires that a stratigraphic column, either an outcrop or wireline log section, be broken down into a succession of stratigraphic units or intervals according to faunal data, radiometric ages, or by correlation with a well- established section. In calculations, stratigraphic units are successively stripped off, causing the basement to rise isostatically and the underlying units to expand or decompact to the original thickness in the absence of overburden. This procedure is repeated until the oldest unit is removed. Airy backstripping simplifies lithospheric response to sediment loading by assuming that lithosphere has no lateral strength (Fig. 41). Although unsupported by geophysical Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 110 Loaded Unloaded a. ______ASL Water column W Sediment column S Fully compacted sedimentary rocks 4 Mantle Sediment load Lithosphere Sediment C. load >Ps / / < / / t / / » Lithosphere N N ' NX ✓ / i' NX*/ / XX f \ / X / ' / X ✓ X✓ Figure 41. Illustration and comparison of Airy and flexural backstripping schemes. Steckler and Watts's (1978) backstripping diagram includes an uncorrected geologic column and "backstripped" (unloaded) column (a.). Airy isostasy assumes no lateral strength for lithosphere (b.). In contrast, flexural isostasy recognizes lithosphere's lateral strength (c.). From Angevine et al. (1990) Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. I l l evidence, the simplifying assumption is often necessary and, in certain circumstances, justifiable. For example, Airy backstripping can be applied with little hesitation in fault dominated basins, especially those supported by a young and less rigid lithosphere marking the early phase of rifting. In these situations, because flexural effects tend to be spatially limited, Airy backstripping could provide adequate approximation to the actual sediment loading. Also, Airy backstripping can be considered a viable method in cratonic basins where strata extend for hundreds of kilometers without significant thickness variation. Inasmuch as the dimension of such a spatially uniform sediment load can greatly exceed the flexural wavelength of the lithosphere, sediments can be considered in Airy isostatic compensation except at basin margins. In practice, however, Airy backstripping has often been used indiscriminately with respect to the size of the basin, stratal geometry, and the nature of the lithosphere. This is partly due to the fact that the stratigraphic data it requires can be easily compiled and calculations are quite simple and fast. As a potential hazardous consequence, however, the resultant tectonic subsidence may be exaggerated, such as near basin flanks where little has actually occurred, or underestimated, such as in the basin interior where certain amount of tectonic subsidence is incorrectly attributed to sediment loading by Airy isostasy (Angevine et al., 1990). Because of these limitations, flexural backstripping schemes generally produce better estimates of regional tectonic subsidence patterns (Watts, 1988; Watts and Thome, 1992; Steckler et al., 1988; Zhou, 1993). FLEXURAL UNLOADING OF SEDIMENT The Cretaceous Western Interior basin is a highly asymmetrical foreland basin, the stratal geometry of which is a westward-thickening wedge (see Chapter 3). From a theoretical point of view, this stratal geometry invalidates Airy backstripping. Despite this, most workers resorted to Airy backstripping to calculate tectonic subsidence history in the Cretaceous Western Interior basin (Cross, 1986; Heller et al., 1986; Steidtmann et Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 112 al., 1991; Devlin et al., 1993; Johnson, 1992). This approach, though not unreasonable considering the purposes of these works, fail to account for the potentially significant flexural effects of sediment loading. In view of the shortcoming of Airy backstripping, this study therefore adopted a two-dimensional flexural backstripping scheme. Flexural backstripping calculates and removes sediment loading from the decompacted sediment thickness according to lithospheric flexure theory instead of Airy isostasy (Fig. 41). The data format required is regional stratigraphic cross sections, composed of a series of individual stratigraphic columns of wireline logs, or alternatively, high quality seismic profiles. The stratigraphic data for this study consists of six biostratigraphically calibrated subsurface cross sections. Strata bounded by time lines comprise a succession of discrete sediment sheet or wedge loads. On each cross section, the interval thickness, lithology, age range, and water depth were specified for each stratal layer and at each control point. The flexural subsidence in response to sediment loads were calculated using the same mathematical procedures as those used in lithospheric flexure modeling (e.g., Turcotte, 1979; Watts 1982; Jordan, 1981; Beaumont, 1978). For simplicity, an elastic flexural model with constant flexural rigidity is used in this study. As described in Turcotte (1979), the flexural deflection, w(x), of an infinite, elastic thin beam overlying a fluid medium in response to loading in two dimensions is described by the differential equation: (2) where D is flexural rigidity, N is horizontal stress, Ap are density contrast between mantle and the basin fill, g is gravitational acceleration, and p(x) is the load function. Elastic thickness T is related to the flexural rigidity D by: Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 113 where E is Young's modulus, and v is Poisson's ratio. Because only sediment loading is considered, the horizontal stress N is ignored. Unless necessitated by geologic evidence, the flexural rigidity D can be held as a constant so that the level of mathematical involvement is greatly reduced. The simplified equation is: + Ap • g • w = p(x) (4) dx where p(x) is the thrust load function in foreland basin modeling and is the sediment load function in flexural backstripping. Analytical solutions of this equation for certain geometrically simple loads can be found in Nadai (1963) and Turcotte (1979). Generally, transform methods are applied to express flexure in the frequency domain. To calculate flexure, the Fourier transform can be taken to yield a solution for (4) in the frequency domain (Watts et al., 1983; Banks et al., 1977): w(k) = 0 (k L p(k) (5) A p g f Dk4 '"' o = 1+- (6) Ap where k is wave number, p(k) is the Fourier transform of p(x) or load spectrum, and 4>is basement response function. Then, the flexural deflection, w(x), can be calculated by inverse Fourier transform of w(k) in (5). The flexural backstripping scheme of this study adopts a hybrid finite-difference method previously used in the literature (Jordan 1981; Flemings and Jordan, 1989). This Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 114 scheme discretizes the sediment layers into evenly spaced line loads, and then uses an efficient algorithm in Angevine et al. (1990) for solving flexure under line loads to calculate the flexural deflection due to each load element. Sediment thickness between control points is calculated by piecewise-linear interpolation of the decompacted thicknesses. To account for lateral changes in lithologies along the cross sections, a stepwise interpolation was used to assign sediment densities for each interval according to the decompacted mean bulk sediment density at control points. At each point, flexure due to sediment loading is obtained by summing the contributions from each individual line load. To reduce the flexural edge effect at basin margins, the cross section was extended for an additional 50 to 100 kilometers on both ends. The flexural rigidity used in calculation is lxlO24 Nm, a typical value for continental lithosphere (Watts, 1992). Figure 42 compares the amount of sediment loading calculated by applying Airy and flexural backstripping schemes respectively to one of the cross sections used in this study (cross section 5, Chapter 3). Airy isostasy predicts that the basement subsidence in response to a sediment wedge (Fig. 42 a) assumes a similar but subdued form to that of the original sediment geometry (Fig. 42 b). In contrast, flexural isostasy predicts a rather different basement subsidence profile from that of the original sediment geometry (Fig. 42 c). As a result of this difference, the tectonic subsidence patterns calculated by the two schemes differ significantly, as demonstrated in Figure 43. This demonstration highlights the inadequacy of Airy backstripping in foreland basins like the U.S. Western Interior. The Cretaceous rocks exhibit gross thickness variations not only across the basin but also along the basin axis. However, a two-dimensional flexural backstripping scheme considers only the flexural effects arising from changes in sediment thickness across the basin. Apparently, even though the flexural effects across the basin are likely to be far greater than along the basin axis, a two-dimensional scheme is inherently unsatisfactory. A still better approach would be a three-dimensional flexural backstripping scheme. A three-dimensional scheme, though conceptually desirable, is difficult to implement. The Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 115 a. Original strata thickness pattern (cross section 5) 2000 b. Airy sediment unloading C. Flexural sediment unloading Figure 42. Subsidence profiles (b and c) in response to the loading of a sedimentary wedge (a). The wedge represents the real geometry of strata on the regional stratigraphic cross section 5 of this study. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 116 a. 0 km 200 400 600 800 1000 JT, 500 1000 b . 0 km 200 400 600 800 1000 / ' s * 500 / s ' f /// // 1000 Figure 43. Tectonic subsidence profiles resulting from different backstripping schemes: a. Airy backstripping; b. flexural backstripping. The profiles are derived by subtracting the sediment loading (Fig. 42) from the decompacted thickness. Dashed lines, To to Ts, show progressive subsidence of an original horizontal datum (top of Mowry Shale) during successively deeper burial. Underlying strata was decompacted. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 117 main difficulty lies in the preparation of a suitable data base, which would take the form of a series of isochron maps over the entire basin. Until the Cretaceous rocks are systematically correlated along closely spaced grids to generate such maps, the mathematical merit of a three-dimensional flexural backstripping scheme will be undermined by the added difficulties and uncertainties that come with its numerical implementation. As the stratigraphic data of the Cretaceous Western Interior steadily accumulates and improves, however, a three-dimensional scheme may be employed in future studies. DECOMPACTION OF SEDIMENT Decompaction restores a rock column to its original, depositional thickness in the absence of overburden according to certain porosity-depth relationships presumably followed by sediments. Given a porosity-depth relationship and the assumption that the rock grain volume is conserved during compaction, decompaction is a rather straightforward process (Sclater and Christie, 1980; Angevine et al., 1990). The relation between sediment thickness and porosity is as follows: So(l — (po) = Sn(l — (pn) (7) where So and cpo denote the original sediment thickness and porosity respectively, and Sn and Given the porosity value of sediments at a certain depth, the decompacted thickness can easily be calculated. To decompact a stratigraphic section composed of multiple lithologies, the porosity-depth relationship for each lithology needs to be specified. However, determination of meaningful porosity-depth relationships for different lithologies found in a specific basin is seldom if ever an easy task. What is needed is porosity data for each lithology obtained over a wide range of burial depths. Because this is not the case in most basins, empirical porosity-depth relationships are commonly used as a first order approximation. The empirical porosity-depth relationships obtained by Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 118 Sclater and Christie (1980) from the North Sea are among the most widely used. These empirical relationships assume an exponential form: where determined compaction constant, and z is the burial depth corresponding to the porosity value cpn (Table 1). The porosity-depth relationships for these lithologies are shown graphically in Figure 44. Decompaction is usually performed only on the stratal interval under investigation. In reality, compaction was not just limited to these strata; rather it could occur over the entire sedimentary cover above the crystalline basement. Unless the underlying strata are thin or had been sufficiently compacted, failure to take the underlying strata into consideration results in overestimation of tectonic subsidence. Stated explicitly, compaction of the underlying strata in response to the overburden of younger sediments leads to greater depositional thickness than attributable to tectonic mechanisms. The additional thickness resulting from this compaction is otherwise indistinguishable from the flexural subsidence driven by supracrustal loading. In the Western Interior basin, the additional step of including the lower Mesozoic and Paleozoic strata in decompaction is particularly called for because of their great thickness. More important, because the overall thickness of the Pre-Cretaceous strata increases westward, their compaction may have contributed to the asymmetrical geometry displayed by the Cretaceous rocks (Sloss, 1988). To decompact the Pre-Cretaceous strata, published Phanerozoic isopach maps for the U.S. Western Interior were used to obtain their thickness (McGookey et al., 1972; Peterson and Smith, 1986) and a siltstone lithology was used. This choice of lithology may not be a good representation of these older strata, many of which have a high percentage of carbonate rocks. Nevertheless, it provides an upper bound on the effect of their compaction under the overburden of the Cretaceous rocks. Figure 45 compares subsidence profiles obtained by including and excluding the underlying strata during Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Table 1. Empirical constants in the exponential porosity-depth relationships cpo C x10'5 p s fcnr1) (a/cm3) Shale .63 .51 2.72 Sand .49 .27 2.65 Chalk .70 .71 2.71 Shaly sand .56 .39 2.68 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. without prohibited reproduction Further owner. copyright the of permission with Reproduced -10000 Depth (meters) Cretaceous rocks of the Western Interior basin. From Sclater and Christie (1980). Sclater andChristie basin. From Interior Western of the rocks Cretaceous the in used decompacting relationships -depth porosity Exponential 44. Figure -8000- -6000- -4000- - 2000 2 4 6 8 100 80 60 40 20 0 - Silt Sand ooiy%) Porosity(% Shale Chalk 0 2 1 to 1000 '7 7 . 600 800 400 200 siltsone lithology usedwas in calculations. Flexural rigidity D=l.E+24 Nm. Basedon the regional cross section 5. ignoringthe compaction oftheunderlying strata;profile b by decompactingtheunderlying strata. A Figure45. Effectsofthe underlying rocks on resultsof flexural backstripping. Profilea was obtained by 0 0 Km 2000 1000 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 1 2 2 decompaction, respectively. By ignoring the underlying strata, a greater amount of tectonic subsidence is predicted than if they are taken into account (Fig. 45 a and b). Clearly, the compaction of underlying strata during deposition of the Cretaceous rocks could potentially contribute to their accommodation and asymmetrical geometry. Although the decompaction procedure is mathematically precise, the geologic database has several uncertainties and errors. Among the uncertainties pertaining to decompaction are the porosity-depth relationships, the complicating factors such as cementation, and the present burial depth of tectonically elevated rocks. First and foremost, it is important not to lose sight of the fact that the current porosity-depth relationships are empirical by nature. They may not accurately represent the actual compaction process in the Western Interior basin. As more precise depth-porosity data become available for the Cretaceous rocks in the future, decompaction may be improved accordingly. The decompaction procedure applied here assumes that reduction of sediment porosity is due only to mechanical compaction. This assumption certainly is a simplistic approximation chosen more out of convenience than thoughtful considerations. Sediment porosity is dependent not only on its burial depth, but also diagenesis. However, little is known about the quantitative details of the interactions between chemical cementation and mechanical compaction in the Western Interior basin. Consequently, chemical cementation can not be easily incorporated into decompaction procedures. For this reason, this decompaction procedure implicitly assumes that sediment porosity reduction during burial is depth dependent and controlled by mechanical compaction alone. By attributing the present thickness to compaction alone, the decompacted sediment thickness is certainly greater than the original, depositional sediment thickness if chemical cementation played an important role. Nevertheless, the errors introduced by this assumption are systematic and distributed evenly over the rock columns where backstripping is conducted. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 123 Finally, added to the above complexities is the fact that during Laramide tectonics and ensuing erosion, Cretaceous rocks in many places were tectonically elevated or exposed while retaining their low porosity and high density indicative of the previous burial depth at which they were fully compacted and lithified. Therefore, the present day burial depth of these rocks needs to be adjusted before decompaction can be carried out. By comparing outcrop sections with adjacent subsurface ones, it is found that the difference between subsurface thickness and adjacent outcrop thickness of the same stratigraphic unit is usually less than 5% -10 %. This suggests that once Cretaceous rocks were fully compacted and lithified at maximum burial depth, they did not incur significant thickness expansion during subsequent uplift. In light of this, the present day burial depth of the strata preserved near uplift areas is corrected according to the average burial depth of the same strata in adjacent areas where a relatively complete sequence of Cretaceous rocks are preserved. SEA LEVEL CORRECTIONS AND THE MEANING OF SUBSIDENCE As shown in equation (1), the backstripping technique was designed to determine tectonic subsidence from the stratigraphic record. This goal requires that both water depth and eustatic sea level changes through time can be independently determined. Uninhibited by this requirement, many have made attempts towards this straightforward use of backstripping technique to obtain "tectonic subsidence". Under the scrutiny of the cautious, however, the fragility of this approach betrays itself. The main reason lies in the difficulty and complexity of the subject of eustatic sea level changes. Although some highly commendable results of eustatic sea level estimates, including the Exxon cycle chart (Haq et al., 1988), have been published, their acceptance is not without skepticism and reservations (Watts et al., 1982; Burton et al., 1987; Miall 1992). Given the difficulties and controversies concerning the subject, it is hardly justifiable to consider the current sea level curves as a known variable in backstripping analysis. With no solution Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 124 of these controversies in sight, this study made no attempt to correct for eustatic sea level changes. To circumvent this step, equation (1) was rearranged by combining the tectonic subsidence and eustatic sea level terms to form a composite unknown term R l: R1 = Y + ASL——— = + Wd (9) pm - pw pm - p«r This approach has been taken previously by Bond and Kominz (1988). Although referred to as "subsidence" in the discussion, the resulting quantity is actually a composite of tectonic subsidence, contemporaneous eustatic sea level change, and the consequent effects of water loading. WATER DEPTH CORRECTIONS Tectonic subsidence is recorded by deposition of sediments as well as by changes in water depth. Correction for changes in water depth is therefore an important step in backstripping analysis. In general, water depth estimation is difficult for deep marine deposits, much less so for shelf sediments, and quite accurate for deltaic and nonmarine deposits. The commonly used criteria for estimating water depth range from sedimentary facies characteristics, fossil assemblages indicative of certain water depths, to the reconstruction of depositional topography or bathymetry. These criteria are rarely quantitatively definitive, however. The Cretaceous Western Interior Basin has been commonly referred to as an epeiric sea way or a ramp setting, with the connotation that it lacked deep marine environments analogous to a continental slope or deep sea basin. From west to east, strata of the Greenhorn and Niobrara cycles were deposited in environments ranging from nonmarine and deltaic to offshore. The western part of the basin shows predominance of shallow marine and nonmarine deposits and water depths in this region probably remained fairly shallow, possibly no greater than that of a typical shelf environment. For example, Lessard (1973) studied the paleowater depth of the Tununk Shale in Henry Mountains Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 125 region on the basis of microfauna and sediment characteristics. His analysis suggested that the water depths of the seaway extending from central Utah to eastern Colorado were no more than 150 to 200 meters (300-600 feet). Zelt (1985) arrived at the same water depth range for the marine Tropic Shale of southern Utah by using Asquith's (1970) model of depositional topography. Towards the east, the predominantly deltaic deposits become finer and thinner, eventually grading into fully marine shales interbedded with siltstones and limestones. Through detailed subsurface stratigraphic correlation of clinoform geometry exhibited by rocks of the Mesaverde Formation in Wyoming, Asquith (1970) constructed the depositional topography assumed by these rocks at the time of deposition. On the basis of his depositional topography model, Asquith estimated that these rocks were deposited a water depth as high as 600 meters. Unlike the younger, coarse grained rocks in the Mesaverde Formation, however, strata of the Greenhorn and Niobrara cycles display greater lateral constancy in thickness and lithofacies, and therefore more subdued depositional topography. For example, Hattin (1971), Kauffman (1977a, 1985), and Weimer (1983) suggested that maximum depths experienced by the Cretaceous strata in the central and eastern part of the basin were as shallow as 100 to 300 meters. The water depth correction in backstripping analysis is a measure of how much the water depths may have changed at each location since deposition of the Mowry Shale. This variation certainly cannot be greater than the maximum water depth of the seaway, and probably was less. For convenience, 100 meters was used as the upper limit for net changes in local water depth and the actual values assigned to each lithofacies were scaled accordingly. A NOTE ON ERROR SOURCES The potential sources of errors in the backstripping analysis of this study are mainly two types: those arising from the backstripping techniques, such as the decompaction and Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 126 flexural unloading procedures, and those inherited from input stratigraphic data, such as age determination, stratigraphic correlation, water depth estimation, and lithology. A rigorous evaluation of the total error is difficult because the magnitudes of individual types of errors involved are essentially quantitatively unknown. Nevertheless, those errors stemming from the backstripping procedures are systematic rather than random. Such errors have been discussed in several case studies and their results provide a reference. For example, Sawyer et al. (1982) and Steckler et al. (1988) examined the error bars of backstripping techniques in studying the U.S. Atlantic continental margin. By using extreme values for physical parameters and by comparing results of different backstripping calculations, they suggested an error bar of 5% and 10% respectively. In a particular study like this, the specific error could of course differ from this reference because errors inherited from input stratigraphic data vary from case to case. Of such errors, correlation is probably the single most important source. Although many distinct stratigraphic intervals can be correlated accurately over long distances, correlation errors on the order of tens of meters or more are quite possible on some less distinctive and sparsely fossiliferous intervals, particularly in areas where wireline log control is poor. Likewise, errors on the same order of magnitude are also quite possible for water depth correction. In the final analysis, however, results of this study represent a significant quantitative improvement over the earlier ones because of the heavy reliance on biostratigraphic data and the use of two-dimensional backstripping scheme. RESULTS By applying flexural backstripping techniques to the six regional stratigraphic cross sections, six subsidence profiles are obtained (See Chapter 5). These profiles show the amount of tectonic subsidence taking place across the basin at different times since the deposition of the Mowry Shale. These subsidence profiles along with their corresponding subsidence curves will be analyzed in the following two chapters. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 5 FLEXURAL SUBSIDENCE AND BASEMENT TECTONICS INTRODUCTION The Western Interior basin is a retro-arc foreland basin developed in the late Mesozoic on the western North American craton (Dickinson, 1974). It provides a potentially decipherable record of nearly 100 m.y. of interactions between thrust loading, lithospheric flexure, basement block movements, and eustatic sea level changes. Efforts to unravel this record in the past have led to the development of quantitative foreland basin models (Price, 1973; Jordan, 1981; Beaumont, 1981). In recent years, these efforts have been succeeded by those devoted to the isolation of tectonic factors and sea level signals recorded in the stratigraphy of the Western Interior basin, either using backstripping techniques (e.g., Heller et al., 1986; Cross, 1986), through field observations (e.g., Nummedal, 1990; Ryer, 1993; DeCelles, 1986) or relying on numerical simulation techniques (e.g., Jordan and Flemings, 1991; Jervey, 1992). These works have provided valuable insights into evolution of the Cretaceous Western Interior basin. Further progress in understanding the Cretaceous Western Interior basin is now hampered by an inadequate knowledge of its subsidence history. Many site-specific subsidence analyses based on Airy backstripping have been conducted, but no efforts went beyond this limitation to document the variations in flexural subsidence in space and time on a broad basis. As a result, many attributes of the flexural mechanism, such as the role of certain long-lived basement structures, thrust load distribution along the Sevier belt etc., remain poorly known. The flexural backstripping analysis of this study documents the subsidence history on a broad spatial and refined temporal scales. Through a window of 16 m.y., this chapter 127 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 128 intends to show that flexural subsidence in the U.S. Cretaceous Western Interior was characterized by spatial segmentation as well as temporal discordance. These variations in flexural subsidence have not been documented in previous studies. Following this discussion, an elastic flexural model is applied to two backstripped subsidence profiles across the Wyoming foreland to evaluate the role of lithospheric flexure during basin development. This modeling, though limited by its two-dimensional nature, provides a quantitative assessment of the spatial extent of the flexural subsidence and its control on sedimentation. Finally, the observed subsidence patterns are discussed in the context of the structural elements of the basement and the thrust belt. This leads to a qualitative basin subsidence model that reconciles observations from two independent sources: basin stratigraphy and the tectonic record. PREVIOUS WORK In studying the coupled Cordillera fold-thrust belt and foreland basin in the southern Canadian Rockies, Price (1973) intuitively recognized the physical analogy between foreland basins coupled with orogenic highlands and the well-known peripheral flexural depressions caused by ice sheets. He proposed that the North American Western Interior foreland basin resulted from flexural isostatic response to the excess mass in the Cordillera. Viewed from this perspective, he stated, "the record of fluctuating rates of sedimentation and of intermittent erosion in the clastic wedge deposits of the foredeep is a sensitive gauge of variations in the intensity of deformation within the whole of the orogenic belt." (p. 50, Price, 1973). Elaborating further on the stratigraphic implications of this model he went to say that "unconformities in the clastic wedge sequence of the foredeep do not mark the times of most intense deformation within the orogenic belt but instead reflect anorogenic intervals." (p. 50-51, Price, 1973). These unpopular but insightful thoughts went unnoticed until very recently with the publication of a series of Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 129 papers arguing that conglomerates in proximal foreland basins should be vestiges of tectonic quiescence rather than indicators of thrusting events (e.g., Burbank et al., 1988). The foreland basin model proposed by Price (1973) was subsequently tested quantitatively in the North American Western Interior basin by Jordan (1981) and Beaumont (1981). Jordan (1981) applied an elastic flexural model to evaluate the effect of Sevier thrust loading on the Cretaceous stratigraphic architecture observed near the Idaho- Wyoming thrust belt. Beaumont (1981), on the other hand, adopted a viscoelastic flexural model to simulate subsidence and large scale stratigraphic stacking pattern of Mesozoic rocks in the Alberta foreland basin. Figure 46 graphically illustrates the mechanics of the foreland basin model. Curve 1 depicts the lithospheric flexural subsidence profile as a load is applied to an originally undeformed lithosphere. Given an elastic assumption (Jordan, 1981), the basin geometry will be maintained until the load changes. If, however, viscoelastic flexure is dominant (Beaumont, 1981), the basin geometry will evolve through time in accordance with the predictions highlighted by curves 2 and 3. Although supported by stratigraphic data from different parts of the basin, both Jordan's and Beaumont's work demonstrated that lithospheric flexure exerted first order control on the stratigraphic architecture observed within a few hundred kilometers of the thrust belt. This finding not only provided a theoretical framework for understanding the relationships between basin sedimentation and tectonics but also served as a model guiding studies of other foreland basins around the world. Following these early works, many others continued to search for more comprehensive and representative foreland basin models (Schedl and Wiltschko, 1984; Stockmal and Beaumont, 1987; Cant and Stockmal, 1989). Recognizing that many cratonic interior foreland basins developed on the attenuated passive margin crust, Stockmal et al. (1986) and Stockmal and Beaumont (1987) developed a flexural model that takes into account the inherited thermal subsidence of the passive margin as well as effects of pre-existing basement topography on thrust motion. Their model, constrained Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. OJ o Load — 3— r I_i involving viscous relaxationunder aconstant load. FromQuinlan andBeaumont (1984). resulting from initial emplacementof aload, oran elastic response. Curves 2 and 3 dipict flexure Figure46. Qualitative representation ofthe flexural responses to loading. Curve depicts1 flexure Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 131 by the Alberta and the Alpine Molasse foreland basins, enabled them to predict the evolution of thrust wedge topography through time. In an effort to further test this model, Cant and Stockmal (1989) related this model to the sedimentary record of the Alberta foreland basin and to the terrane accretion history in the Canadian Cordillera. Their work suggested that the clastic wedges in the foreland might record the terrane accretion history on the older passive margin. Cross (1986) provided a regional synthesis of the development of the U.S. Cretaceous Western Interior basin in the context of plate tectonics. Drawing on the gross isopach trends, he suggested that lithospheric flexure by thrust loading was most effective in the early phase of basin subsidence history during early Late Cretaceous. With the inferred onset of the low-angle subduction of the Farallon Plate in late Late Cretaceous, he inferred that sublithospheric loading and cooling resulted in a broad downwarping centered in Wyoming and Colorado. This subsidence mechanism therefore complicated the lithospheric flexure by thrust loading. In the past few years, several workers have developed quantitative foreland basin stratigraphic models with particular reference to the North American Western Interior basin (Jordan and Flemings, 1991, Pepper, 1993; Jervey, 1992). The recent model by Jordan and Flemings (1992) is perhaps the most refined and rigorous. In this model, flexural subsidence, sea level changes, and sediment supply were approximated with empirical relationships and treated as independent variables. Given certain initial and boundary conditions, the model can be executed to simulate evolution of basin stratigraphic architecture through time. The works selectively summarized here greatly enhanced our understanding of the Western Interior basin. In particular, the advent of increasingly sophisticated quantitative models has defined a common ground for multidisplinary research to unravel the relationships between the many factors involved in foreland basin development. These models can potentially be a useful analytic tool to predict the amount of flexural Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 132 subsidence in the foreland basin, infer tectonic loading history, and constrain lithospheric rheology from the stratigraphic record. However, as shown in paragraphs below, the subsidence pattern in the Cretaceous Western Interior basin is highly complex. Therefore, development of future foreland basin models should be accompanied by more realistic constraints, particularly accurate documentations of the actual basin subsidence history. SUBSIDENCE PATTERNS IN SPACE AND TIME Subsidence profiles The six subsidence profiles calculated by flexural backstripping across different segments of the U.S. Western Interior basin are shown in Figure 47. Their locations are shown in Figure 20 in chapter 3. These profiles portray the subsidence as it varies spatially both across and along the basin axis. Clearly, the pattern of cumulative subsidence over the 16 m.y. of the Greenhorn and Niobrara cycles reveals two spatially distinct components. On the eastern cratonic platform, basin subsidence is essentially uniform. In areas within a few hundred kilometers of the thrust belt, in contrast, basin subsidence increases westward, although the rate of increase varies significantly from western Montana to southwestern Utah. Because of its spatial proximity to the thrust belt to the west, this subsidence pattern is interpreted as the flexural response to thrust loading, as has been demonstrated by Jordan (1981). This part of the basin is hence considered the foreland basin proper. The geometry of the flexural subsidence pattern, or the shape of the foreland basin, is highly variable both in amplitude and in wavelength along the Sevier belt. In western Montana, flexural subsidence just barely exceeds the platform subsidence (Fig. 47, profiles 1 and 2). Viewed in isolation, this subdued flexural subsidence pattern is hardly consistent with the assertion that the Cretaceous Western Interior basin is a typical foreland basin. This observation suggests that thrust loading near this part of the foreland was rather insignificant, at least during the time interval of this study. Farther south, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. M etres 0 200 400 km k ■ - 1 Figure 47. Flexurally backstripped subsidence profiles across basin. Light shading marks amount of subsidence from 96 (94 on e and f) to 90 Ma, and dark shading marks amount of subsidence from 90 to 80 (83 on c and d) Ma. Vertical scale is tectonic subsidence in metres. Triangles indicate locations of subsidence curves discussed next. DCA is Douglas Creek Arch. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 134 however, in Wyoming and northern Utah, the flexural subsidence pattern is far more distinctive. On both profiles across Wyoming, the amplitude of the flexural subsidence near the thrust front is several times greater than the platform subsidence, and its half wavelength is on the order o f400 km, reaching as far east as the Laramie and Powder River Basins (Fig. 47, profiles 3 and 4). This flexural subsidence pattern here defines a broad and deep foreland basin that requires significant thrust loading coupled with a strong basement foundation. Southward across the Uinta Mountain, the flexural subsidence in central Utah has even greater amplitude, but shorter half wavelength (Fig. 47, profile 5). Towards the east, the flexural subsidence pattern was strongly influenced by the differential subsidence on the Douglas Creek Arch, a persistent structural high throughout the Phanerozoic, particularly during the Tertiary Laramide orogeny (Johnson and Finn, 1986). Notwithstanding this structural complication, this particular flexural subsidence pattern in central Utah implies a relatively weak basement crust. In southern Utah, some 200 kilometers or so farther south, the flexural subsidence is again relatively small, implying that local thrust loading was minor (Fig. 47, profile 6). Subsidence curves To complement this analysis of spatial variations in basin subsidence, a series of site- specific subsidence curves were constructed by plotting flexurally backstripped subsidence against time (Fig. 48). These sites are chosen 100 to 150 kilometers east of the Sevier belt depending on the local flexural wavelength. The six curves show that the temporal changes in subsidence vary with location along the strike of the thrust belt. From the middle Cenomanian to late Turanian (96 to 90 Ma), or the Greenhorn cycle, subsidence rates were high in Utah (Fig. 48, curves 5 and 6) and much lower in Wyoming and Montana (Fig. 48, curves 1,2,3, and 4). In contrast, during the Coniacian and Santonian stages (90 to 85 Ma), or the Niobrara cycle, subsidence accelerated rapidly in Wyoming, increased slightly in Montana, and decreased Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 135 Cen.- L. Tur. i Con.- E. Camp. 100 80 (Ma) •3 1500 Metres Figure 48. Temporal subsidence trends at six locations 100-150 km east of the thrust belt. Hatched areas represent cumulative tectonic subsidence through time. Solid lines below represent total (uncorrected) subsidence. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 136 in Utah. At the end of the Santonian and into the early Campanian, rates of subsidence appear to have slowed everywhere. The temporal trends in subsidence as described above differentiate the Utah province from the rest of the foredeep area. MODELING FLEXURAL SUBSIDENCE Model description Since the pioneering work by Jordan (1981) and Beaumont (1981), there have been substantial improvements in both the quality and quantity of the stratigraphic data in the Western Interior basin. However, no attempts were taken to further test the lithospheric flexural mechanism with this improved stratigraphic database. In view of this, this chapter includes a quantitative test of the lithospheric flexure model on the basis of two subsidence profiles across the Wyoming foreland. The decision to limit the modeling effort to this area was made in part because thrust loading history in the Idaho-Wyoming salient is better understood, and in part because this area depicts the most pronounced flexural depression. By comparison, the remainder of the profiles are either less pronounced or complicated by intrabasinal differential subsidence. Models describing the evolution of foreland basins approximate the flexural deflection with either elastic or viscoelastic thin plate theory (Nadai, 1963; Turcotte, 1979). In most models, flexural deflection is treated in two-dimensions because orogenic belts are large- scale linear features on earth's surface. This study selected a two-dimensional elastic flexural model to evaluate the documented subsidence patterns. In such a model, the half wavelength of flexure is governed by the lithospheric strength and the amplitude by the applied load in addition to lithospheric strength (Fig. 49). In addition to its mathematical simplicity, an elastic flexural model is chosen because it has been applied to approximate flexural deflections in many different tectonic settings with satisfying results. Furthermore, because the duration of the stratigraphic interval to be examined is relatively short, an elastic flexural model is an adequate first order Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 100 km Te=25 km Te=110 km - 0- Figure 49. Flexural halfwave-length as afunction ofthe of loadlithospheric shape, elasticTe controls thickness the Te. flexural Irrespective halfwave-length and, to alesser extent, the depth offlexure. 1000 2000 J m eters Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 138 approximation. In adopting such a model, however, one should remember a potentially more serious problem: the errors introduced by using a two-dimensional approximation of the three-dimensional problem of flexural subsidence. Structural evidence reviewed in Chapter 2 suggests not only a heterogeneous crustal fabric beneath the sedimentary cover of the U.S. Western Interior but also along-strike variations in thrust loads. These complicating factors are ignored in this model, but their implications will be discussed later in this chapter. Method The spatial pattern of cumulative subsidence on the two backstripped subsidence profiles across Wyoming provide observational constraints for flexural modeling. Flexural subsidence in response to a thrust load was calculated by using the same mathematical procedures as described in Chapter 4 for flexural sediment unloading. In the calculations, a trial and error method was used to search for a best-fitting theoretical profile. This consisted of iteratively calculating flexural deflection profiles by systematically varying the applied load and elastic thickness independently. If a particular theoretical profile matched the geometry of the backstripped subsidence profile, and if the applied load and elastic thickness lies within their accepted range, then it can be considered as a best-fitting profile. If, however, the flexural model is unable to generate a subsidence profile that matches the geometry of the backstripped profile, the conclusion would be that either subsidence mechanisms other than flexure played an important role during basin development, or the model itself is an inadequate approximation of the actual flexural subsidence. Model results The best-fitting theoretical flexural profiles and their corresponding backstripped profiles are shown in Figure 50. These two profiles were obtained by using an elastic Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 139 S. BIGHORN POWDER RIVER W. NORTH DAKOTA b. t GREEN RIVER HANNA W. NEBRASKA 5 km meters 100 km Figure 50. Best-fitting flexural profiles for the backstripped subsidence profiles across the Wyoming foreland, a: model match for subsidence profile 3; b: model match for subsidence profile 4. Solid lines are backstripped subsidence profiles and dashed lines are best-fitting model profiles. Flexural rigidity D=4 x 1024 Nm. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 140 thickness of 80 + 10 km and crustal loads 100 km wide and 3 to 5 km high, respectively. The elastic thickness value is considerably greater than previously suggested for the Cretaceous Western Interior basin (Jordan, 1981), but not unusual in cratonic interior foreland basins (McNutt et al. 1988; Watts, 1992). The model thrust loads are comparable to the size of the Meade-Crawford thrust system as reconstructed by Jordan (1981) (see Chapter 2). To a first approximation, the theoretical flexural profiles yield a reasonable match to the westward-deepening trends in the subsidence profiles. The overall agreement between model results and observations, though not quite unexpected, support the conclusion reached in previous studies that the observed asymmetric basin geometry can be generated entirely by lithospheric flexure in response to Sevier thrust loading (Beaumont, 1981; Jordan, 1981). Without such a model, it is not certain how much of the asymmetric subsidence can be attributed to lithospheric flexure or what are the required loads and lithospheric strength. Notwithstanding this general agreement, the details of the flexural mechanisms predicted in this model differ from those in Jordan's model (1981). The flexural half wavelength of the Wyoming foredeep is about 400 km, encompassing the Bighorn Basin, the Green River Basin, and their contiguous areas to the east. This basin width suggests that in the Cretaceous the lithosphere beneath Wyoming was strong, comparable to those in other broad foreland basins such as that in front of the late Paleozoic Appalachian and the Ganges (McNutt et al., 1988; Watts, 1992; Watts et al., 1982). The predicted outer flexural bulge is located slightly east of the Powder River and Hanna basins (Fig 50 a and b), not near the Moxa Arch as previously suggested by several people. Further to the east, basin subsidence was not affected by lithospheric flexure under Sevier thrust loading. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 141 A note on the lithosphere's elastic thickness Because lithospheric elastic thickness is an important determinant of the foreland basin geometry, the value required for the best-fitting flexural subsidence profiles warrants an explanation. Studies of continental lithospheric flexure in a wide variety of tectonic settings demonstrate that continental elastic thickness varies over a range from 10 km to 100 km or more (McNutt et al., 1988; Watts, 1992). According to Watts (1992), the distribution of continental lithospheric elastic thickness is strongly 'bi-modal' (Fig. 51). The mode with small elastic thickness corresponds to narrow and deep foreland basins, such as the Alpine foreland basin. The other mode represented by a large elastic thickness corresponds to wide foreland basins, such as the Appalachian and Ganges foreland basins. Examined with this reference, the elastic thickness from Jordan's (1981) model, which is in the neighborhood of 30-40 km, places the U.S. Western Interior basin into the first mode, whereas results of this study put it in the second mode. Because this study applied a similar flexural model to that of Jordan, the discrepancy in elastic thickness reflects the disparity in the quality of the stratigraphic data between the two. In light of the current understanding of the variations in continental lithospheric elastic thickness, the value obtained in this study is not unreasonable. According to Kamer et al. (1983), one of the most important factors dictating lithospheric strength is the secular cooling of the basement crust since its formation. As shown in Figure 52, continental elastic thickness generally increases with the age of the basement crust, much like oceanic lithosphere. As described in Chapter 2, the Wyoming foreland region is underlain by Archean crusts of the Wyoming Province. If secular cooling has been a dominant factor controlling the lithospheric strength, the Wyoming foreland basement should be cold and strong. In addition to secular cooling, McNutt et al. (1988) suggested that another possible factor controlling lithospheric strength is the state of stress and strain in the lithosphere. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 142 Frequency (%) 20 - Jordan's study (1981) Figure 51. Bi-modal distribution of continental lithospheric elastic thickness (Te). Te is based on foreland basin and glacial rebound studies. Number of estimated Te values N=28. From Watts (1992). Arrows indicate Te for the Wyoming foreland derived from Jordan's (1981) and this study, respectively. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. l_ 3000 __ Wyoming foreland ______2000 ♦ Caucasus + Z a g ro s ♦ U rals + Carpathians ♦ Fennoscandia X G anges ^ Sub-Andean Lake A lgonquin4 X 1000 ♦ ♦Appalachians Lake Agassiz Age of Lithosphere at time of loading (m.y.) S. Tienshan T a r im + E. E. Alps ♦ i • ♦ g W. Alps g Lake Bonneville N xienshan < J - 150 100 y u c (A O S 50 5 H *•*3 ^ 4 Solid circlesestimates are from glacial studies anddiamonds from foreland basin studies. Tefor the Wyoming forelandderived from this study shownis in square (with errorbars). ModifiedfromWatts (1992). Figure 52. Distribution ofcontinental elastic thickness Te versus age oflithosphere atthe timeofloading. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 144 She argued that orogenic belts that appear highly arcuate are associated with low values of elastic thickness, whereas long, linear orogenic belts are supported by strong plates. By the same token, steeply dipping plates, having been bent at a greater angle, appear weaker than shallowly dipping plates because of inelastic yielding. The Western Interior basin was coupled with a linear thrust belt and accompanied by insignificant bending of the continental plate during its development. Therefore, the lithosphere in the Wyoming foreland should be strong. This inference, however, does not exclude the possibility that the lithosphere beneath other parts of the U.S. Western Interior might be weakened by basement faults/lineaments. As discussed next, variations in basement strength with location are quite significant. DISCUSSION Complexities offoreland basin subsidence The six subsidence profiles in Figure 47, supplemented by the above flexural modeling, clearly suggest that lithospheric flexure in response to the Sevier thrust loading played a major role in the basin history. However, rather than a spatially invariant flexural depression coaxial with the thrust belt, as occasionally implied in some stratigraphic studies, the Western Interior foreland was characterized by considerable spatial and temporal variations in the flexural subsidence over the chosen 16 m.y. time interval. Spatially, the magnitude and half wavelength of the flexural subsidence varied with location in the Western Interior foreland. In Wyoming and northern Utah, flexural subsidence resulted in a deep and wide foreland basin. In contrast, flexural subsidence in southern Utah and western Montana was insignificant. These spatial variations imply that the gross crustal shortening over the 16 m.y. was centered in the Idaho-Wyoming salient rather than evenly distributed along the Sevier belt. They also imply that the Western Interior foreland basement was segmented, consisting of the Wyoming, Montana, and Utah blocks. Each block Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 145 responded to thrust loading with flexural subsidence of different magnitude and half wavelength as observed. Temporally, flexural subsidence was rapid in the Utah foreland and slower in Wyoming and Montana foreland during the Greenhorn cycle. During the succeeding Niobrara cycle, in contrast, flexural subsidence accelerated rapidly in Wyoming, increased slightly in Montana, and decreased in Utah. This implies that thrusting was not synchronous along the length of the Sevier belt. Specifically, the thrust load was first emplaced in Utah. Late on, as thrusting decreased there, the Wyoming-Idaho salient experienced rapid thrusting. As shown below, these temporally discordant and spatially non-uniform thrusting activities are not inconsistent with geologic evidence residing in the styles of thrusting and basement structures of the Western Interior. Basement structures and their influences on lithospheric flexure This study proposes that the above described spatial and temporal variations in the flexural subsidence were controlled by zones of crustal weakness oriented at high angles to the Cordillera hingeline. As described in Chapter 2, these zones of crustal weakness were mostly faults and lineaments inherited from Precambrian rifting and early Paleozoic passive margin development. They persistently influenced Phanerozoic sedimentation. During the development of the Western Interior basin, these basement structures influenced the Cretaceous flexural subsidence in the following manners. First, basement irregularities due to these zones of crustal weakness affected spatial distribution of crustal shortening through buttressing. Secondly, the east-west trending normal faults inherited from the Proterozoic Belt Basin and the Uinta aulacogen probably dissected the foreland lithosphere into more or less mechanically independent blocks. Thirdly, each basement block had different mechanical strength depending on the internal zones of crustal weakness. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 146 The thin-skinned Sevier thrusting interacted with coeval basement uplifts in many places in a so called overlap province. The interactions between the two contrasting tectonic styles took place primarily in the form of buttressing (Schmidt and Perry, 1988). Buttressing not only led to local deflections in thrust sheet propagation but also created nonuniform crustal shortening along the thrust belt. Specifically, in response to the buttresses located in the Uinta aulacogen and northwest Wyoming and southwestern Montana, the Sevier thrust sheets preferably moved to the east along the less resistant course between them. Therefore, disaproportionally greater crustal shortening was probably accommodated in the Idaho-Wyoming salient through time. The cartoon in Figure 53 is drawn to illustrate this effect. Coupled with a segmented lithosphere, such a crustal shortening pattern could cause greater cumulative flexural subsidence in the adjacent southwestern Wyoming foreland than in Montana or southern Utah during the Greenhorn and Niobrara cycles, as documented in this study. The east-west trending normal faults in west-central Montana associated with the Proterozoic Belt basin and boundary faults of the Proterozoic Uinta aulacogen represent major zones of crustal weakness. According to Tonnsen (1986), these basement structures partitioned the crust underlying the Rocky Mountain region into three large paleotectonic blocks: the Montana, Wyoming, and Utah-Colorado blocks (Fig. 54). These blocks correlate well with the Cretaceous flexural subsidence pattern. Under thrust loading during the Cretaceous, these blocks probably behaved as more or less mechanically independent regions. It is conceivable that during the Greenhorn cycle, in response to the loading of thrust sheets concentrated in Utah, possibly the Pavant thrusts, the Uinta foreland experienced greater subsidence while the Wyoming foreland remained unaffected. By the same token, once the locus of thrusting activities shifted to the Wyoming-Idaho salient during the succeeding Niobrara cycle, possibly on the Meade and Crowford thrusts, the Wyoming block underwent greater flexural subsidence than the neighboring foreland areas. Lack of pronounced flexural subsidence in Montana was Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 147 buttressing buttressing near Uinta Mt. and in southwestern Montana. Figure 53. Interpretative diagram Figure 53. Interpretative diagram showing differential crustal shortening result as a of Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 4^ 00 Continental crust Colorado 'yoming IMontana Attenuatedcrust Oceaniccrust time. Theunderwent blocks recurrent movements during the Phanerozoic. FromTonnsen (1986). Figure Diagramatic 54. sketch ofthe paleotectonic blocks during the middleProterozoic i Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 149 probably due to insignificant thrusting throughout the Greenhorn and Niobrara cycles. This inferred complex lithospheric flexure mechanism is not unique to the Cretaceous Western Interior Basin; similar observations have been made in the late Paleozoic Antler foreland basin (Dorobek et al., 1991), and elsewhere (Royden, 1988; Waschbusch and Royden, 1992). In addition to foreland basement segmentation, the internal basement strength of each block was also different from each other. The Wyoming block, composed of Archean rocks of the Wyoming Province, was probably the strongest, as evidenced by its large elastic thickness value derived from this study. In contrast, the Utah block was much weaker than the Wyoming block, as indicated by its deep and narrow flexural subsidence pattern. The weak mechanical strength of the Utah block was probably a long-lived feature caused by zones of weakness inherited from the Precambrian rifting. According to Picha and Gibson (1985), the major zones of crustal weakness in the Utah basement block consist of a north-south trending normal fault called the Ancient Ephraim Fault and a series of northeast trending lineaments that offset the thrust belt. It is possible that the observed weak mechanical strength in the Utah foreland was just a consequence of these faults. The contrast in the mechanical strength between the Wyoming and the Utah blocks has persisted today despite the Tertiary Laramide orogeny and the Basin and Range extension. By numerical inversion of modem gravity and topography data, Lowry and Smith (1994) calculated and mapped the lithospheric strength in the middle and southern Rocky Mountain region. Their work documented that the modem elastic thickness in this region varies from as low as 5 km in the Basin and Range to as high as 77 km in Wyoming. This latter value is essentially identical to the one derived from this study on the basis of flexural backstripping of the Cretaceous rocks. More importantly, as shown in Figure 55, the spatial variations in the mechanical strength from Utah to Wyoming correlate well with those inferred from the subsidence profiles derived from this study Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 150 Elastic thickness (km) Uinta Mt. Sevier thrust faults Figure 55. Spatial variations in the present day lithospheric elastic thickness across parts of Idaho, Wyoming, and Utah. The elastic thickness is derived from inversion of gravity and topography data. Modified from Lowry and Smith (1994). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 151 (Fig. 47). North of the Uinta Mountain, the Archean crust in Wyoming has an elastic thickness ranging from 40 km to 77 km, whereas in central Utah, the elastic thickness lies within 15 km to 20 km. The transition from a strong crust in Wyoming to a weak crust in Utah occurs close to and parallel with the Uinta aulacogen. The subsidence profiles derived from this study clearly show a similar pattern in the lithospheric strength as it varied from Wyoming to Utah during the Cretaceous (Fig. 47). One might therefore argue that the correlation between the Cretaceous subsidence pattern and the modem lithospheric strength is not simply a coincident. Rather, it reflects the long-lived nature of the Precambrian basement tectonics, particularly the zones of crustal weakness. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 6 RESIDUAL SUBSIDENCE AND SPECULATIONS ON ITS CAUSES INTRODUCTION The flexural subsidence resulting from thrust loading takes a fairly distinct pattern so that it can be easily identified (Fig. 56). If this component is separated from the composite subsidence profiles and the intrabasinal differential subsidence ignored, the Western Interior basin is left with a residual or "background" subsidence component. This residual component measures about 200 meters over much of the eastern platform of the basin. Extrapolated to the foreland area towards the thrust belt, it is superimposed on the flexural component. Locally, such as in western Montana, the residual subsidence plays a dominant role even close to the thrust belt. Unlike the westward-increasing subsidence pattern, which signifies a tectonic mechanism such as lithospheric flexure, the cause of the observed residual subsidence component cannot be easily determined. In theory, it could be caused by a eustatic sea level rise, an episode of regional tectonic subsidence, or a combination of both. This ambiguity exists because the backstripping techniques as implemented do not allow for differentiation between the two (see Chapter 4). Deposition of marine Cretaceous strata on the eastern platform has long been attributed to eustatic sea level changes and tectonic subsidence was rarely the subject of discussion. For example, many authors considered the cratonic platform part of the Western Interior basin to be tectonically stable and therefore have tried to determine the elevation of the Cretaceous eustatic sea level presumably preserved in these platform strata (Sleep et al., 1980; Haq et al., 1988; Sahagian, 1987; McDonough and Cross, 1991). Likewise, in other studies 152 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Cratonic platform forebulge across southern Wyoming (subsidenceprofile 4). flexural subsidence tothe west andresidual subsidence overdie entire basin. The frontal view is Figure 56. Diagram illustrating the two main subsidence components in theWestern Interiorbasin: ! Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 154 concerned with flexural modeling or its applications, strata deposited beyond the flexural effect were either ignored or simply attributed to a eustatic sea level rise and associated sediment loading (e.g., Jordan, 1981). However, as demonstrated by Bond (1976) almost two decades ago, the development of the Cretaceous Western Interior basin requires regional tectonic subsidence in addition to the eustatic factors. This chapter intends to show that the residual subsidence calculated above can not be explained by eustasy. This is followed by a review of several recent hypotheses that relate subsidence in the Cretaceous Western Interior basin to coeval plate tectonics in the subduction zone between the Farallon and North American plates. This review shows that although the exact cause of the residual subsidence remains elusive, the concept of mantle dynamic topography driven by subduction and mantle convection provides a plausible explanation that deserves special attention in future studies. NATURE OF THE RESIDUAL SUBSIDENCE It is widely believed that sedimentation on the eastern cratonic platform of the Western Interior basin was subjected to domination by eustatic sea level changes (e.g., Kauffman, 1985; Weimer, 1983). Observations that led to this assumption can be summarized as follows. First, unlike tectonically active areas where eustasy, lithospheric deformation, and thermal subsidence are all inscripted into the sedimentary records, this portion of the basin lacked conspicuous tectonic activities throughout the Phanerozoic. The only known structural feature active during the Cretaceous is the Transcontinental Arch, which, according to Weimer (1983) and others, influenced Cretaceous sedimentation by subtle vertical movements in the basement. Secondly, Upper Cretaceous strata deposited in this platform region consist of marine shales and limestones that display remarkable lateral continuity in lithofacies and consistency in thickness. This is in sharp Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 155 contrast to those deposited in the tectonically active foredeep region, where complexly intertongued marine and nonmarine strata dominate. Perhaps more important, the Cretaceous strata are distinguished by regionally correlative transgressive and regressive cycles. The major cycles such as the Greenhorn and Niobrara have generally been interpreted as the result of eustatic sea level fluctuations. Thirdly, it is well documented that the Cretaceous is a period of global transgression when many continental interiors were flooded. Hays and Pitman (1973) first proposed that this transgression resulted from a eustatic sea level rise caused by changes in spreading rates and mid-ocean ridge length, a mechanism subsequently known as tectonoeustasy. Using global spreading rates as a data base, Kominz (1984) demonstrated that the long term eustatic sea level fluctuations driven by tectonoeustasy amounted to 230 m (±100) over the last 80 m.y. In the absence of any direct evidence for a viable tectonic mechanism, it stands to reason that the residual "subsidence" perhaps record the long term Cretaceous eustatic sea level rise. Intuitively appealing as it may be, this view can be discounted simply because the required eustatic sea level rise proves unrealistic, at least according to current understanding of tectonoeustasy (Kominz, 1984; Engebretson et al., 1992). The first important step in this direction was made by Bond (1978), who demonstrated that eustasy alone can not explain the size of the Cretaceous Western Interior basin. He calculated the amount of sea level rise required to accommodate the extensive Cretaceous deposits under the assumption that no tectonic subsidence other than sediment loading occurred. His results indicate that given an unusually large sea level rise of 310 meters during the Cretaceous, sedimentation in nearly half of the Western Interior basin still remains unaccounted for. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 156 Since Bond's work, progress has been made in understanding and documenting Cretaceous eustasy. A widely accepted document marking this progress, though not without controversies, is the detailed eustatic sea level curve by Haq et al. (1988), which is presumably based on a synthesis of seismic, borehole, geochronologic, and biostratigraphic data from around the world. Figure 57 shows the Cretaceous and Tertiary eustatic sea level curve by Haq and others (1988). The curve has been smoothed with a 10 m.y. running window so that short term sea level fluctuations can be filtered out. These short term fluctuations, at time scales of 10 m.y. or less, may be recorded in the Cretaceous strata, but they are irrelevant here because this analysis focuses only on the long term sea level trends. The modified sea level curve by Haq and others (1988) is superimposed on a group of theoretical sea level curves Engebretson et al. (1992) calculated on the basis of global spreading rates. From middle Cenomanian to early Campanian (96 to 80 Ma), the time interval of study in this paper, the long term eustatic sea level trend shows a net lowering instead of a rise. Apparently, if this trend is a true representation of the Cretaceous eustatic sea level history, then the residual subsidence of the Western Interior basin must reflect tectonic mechanisms. In addition to the difficulty presented by the timing of the eustatic sea level changes, the amplitude of the sea level rise required to account for the residual subsidence documented in this study is equally problematic. It can easily be calculated on isostatic grounds that 200 meters of residual subsidence is in effect equivalent to a sea level rise of 150 m. Such a sea level rise almost equals Haq et al's documented rise for the previous 90 m.y. Granted that eustatic sea level fluctuations on time scales of 10 m.y. or less may be an important control on the varied cyclicities in the Cretaceous strata of the Western Interior basin, the net, long term sea level rise enough to account for the residual subsidence seems Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 157 300 ’\ 200 /M / / > o \ Eustatic (:urve I C'\W " - - o ' ; Si * /fj& \ % o 1 / /// \\ V ^ V \, a y H '///// / II \\\\\* « 100 1,11 ’/ii v > \ \ «V u 1,1 1, A \ w \ > tflt/i1,1 if '/! JO ' \W ' * * *iini / Pre x — - II ___ / -100 I i f f 180 150 120 90 60 30 Time (Ma) Figure 57. Eustatic sea level curve (heavy line) of Haq et al. (1988) and predicted sea level curves by Engebreston et al. (1992) using global spreading rate data (dashed lines). Shaded column represents the time span of this study. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. improbable. From this simple test, the inescapable conclusion is that the residual subsidence resulted from mechanism(s) other than eustatic sea level changes. EPEIROGENIC SUBSIDENCE MECHANISMS Many Phanerozoic cratonic platforms are characterized by laterally extensive strata punctuated by unconformities of various durations. These settings have been the preferred areas for measuring eustatic sea level changes (Hancock and Kauffman, 1979; Sleep et al., 1980; McDonough and Cross, 1991; Sahagian et al. 1992). Despite this, there is quite unequivocal evidence from continents around the world for long term epeirogenic movements (Fig. 58. Harrison, 1990). An expanding body of data suggests that such epeirogenic movements, after correction for possible eustatic sea level changes, could occur on time scales of tens or hundreds of millions of years and amount to several hundred meters in amplitude (Sloss, 1974, 1991; Bond, 1978; Harrison, 1988, 1990; Bond and Kominz, 1992). Such movements have been advocated as an alternative to eustasy as a control on platform sedimentation. Sloss (1991) even argued that the synchronous vertical motions observed in some widely separated Paleozoic cratonic basins may not necessarily be indicators of eustatic control. He suggested that such motions can be the product of secular variations in radial heat flow, which result in alternate episodes of inflation and deflation of continental lithosphere. This mechanism is an early form of the concept of mantle-driven dynamic topography. In the following paragraphs, several recent hypotheses proposed with specific reference to the Western Interior basin are briefly reviewed, including sublithospheric loading and cooling, continental tilting, and mantle dynamic topography. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. VO 100 80 Time (Ma) N. America Australia X Asia +■ Africa A S. Am erica ▼ Europe Figure 58. Vertical continental movements during the past Ma. 180 FromHarisson (1990), partlybased on Bond (1978). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Sublithospheric loading and cooling Subduction at convergent margins can be identified as the ultimate cause for many crustal and surface processes. Following this tenet of plate tectonics, attempts have been made to relate the subsidence recorded in the Cretaceous strata to the subduction of the Farallon Plate beneath the North American craton (Cross, 1986; Mitrovica et al. 1989). On the basis of Cretaceous isopach patterns, Cross and Pilger (1978) and Cross (1986) inferred that two modes of subsidence succeeded each other in the Western Interior basin. During early Late Cretaceous time (100-80 Ma), basin subsidence was mostly confined to the thrust front and insignificant on the cratonic interior. Because the foredeep’ outlined on the isopach map is fairly distinct, lithospheric flexure under thrust loading affords a reasonable explanation. During late Late Cretaceous time (80-70 Ma), basin subsidence assumed a different and more complicated mode: flexural subsidence gave way to a broad down warping centered in Wyoming and Colorado. Cross (1986) proposed the sublithospheric loading and cooling occurred in the later period of time and caused the downwarping. Several lines of geologic evidence, including plate convergence rates and Cordilleran magmatism, suggest that subduction of the Farallon Plate changed from "normal" to "low angle" in middle Late Cretaceous (80 Ma) (Dickinson and Snyder, 1978, Cross and Pilger, 1978, Cross, 1986). According to Cross (1986), the timing of the postulated low angle subduction coincided with the transition between the two subsidence modes described above. Inspired by this coincidence, Cross (1986) proposed that as the Farallon Plate was placed in virtual contact with the overlying North American Plate, it acted as a sublithospheric load causing a broad downwarping in Wyoming and Colorado. In addition, because the subducting Farallon Plate was colder than the mantle it Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. replaced, thermal cooling also occurred to further enhance subsidence due to sublithospheric loading mechanism. This hypothesis represents one of the earliest attempts to find a tectonic mechanism for deposition of the widespread Cretaceous strata beyond the influence of thrust loading. However, the physics of sublithospheric loading and cooling as a subsidence mechanism is highly problematic. In fact, many workers have interpreted the formation of widespread Laramide uplifts and intervening basins as the result of the flat subduction (Dickinson and Snyder, 1978; Hamilton, 1988,1989). Also, the broad downwarping cited by Cross (1986) appears to coincide in time with the break-up of the Western Interior basin into isolated Laramide structural basins. Therefore, it is possible that the inferred "downwarping" may be an artifact of the nature of stratigraphic correlations between individual Laramide basins. Continental tilting More recently, Mitrovica et al. (1989) used numerical simulation techniques in a study of the dynamic effects of plate subduction on the surface topography of cratonic platform basins. By comparing the Cretaceous isopach and present day. topography of the U.S. Western Interior, Mitrovica et al. (1989) reconstructed the history of vertical movements western North America was subjected from Cretaceous to Tertiary (Fig. 59, A.). The Cretaceous-Tertiary vertical movements consist of a regional subsidence during the Cretaceous, and a rebound during the Tertiary. They attributed the vertical movements experienced by western North America to "continental tilt". Mitrovica et al. (1989) proposed that the continental tilt resulted from large scale lithospheric deflection dynamically coupled with the subduction of the Farallon Plate. The lithospheric deflections induced by subduction can be a Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Black Hills Thrust / belt edge 2 km 500 km Cretaceous Fold-Thrust Foredeep Platform Active subduction Tertiary Inactive subduction Figure 59. Continental tilt model by Mitrovica et al. (1989). A. Schematic illustration of the net effect of Late Cretaceous subsidence and Tertiary uplift across Wyoming. The base of the Cretaceous series is shown in by a. During subsequent uplift in Tertiary, a moved to b. The surface of the uplift is c. B. The proposed tilting mechanism resulting from subduction and mantle convection. Active subduction during the Cretaceous leads to a continental tilt, or regional subsidence (top of B). Cessation of subduction brings the the tilting mechanism to an end. Therefore the platform rebounds (below). Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. kilometer in amplitude and up to 1000 km in wavelength, depending on the angle of subduction as well as on lithospheric rigidity. Specifically, this mechanism predicts that broad lithospheric deflection or epeirogenic subsidence occurred across much of the Western Interior during Cretaceous time when subduction remained active (Fig. 59 B). During the Tertiary, in contrast, as subduction slowed down and eventually ceased when the East Pacific spreading center reached the Californian coast, the cratonic margin began to rebound, creating much of the present day topography in the Western Interior. Although the observation that led to this model may be an oversimplification of the tectonic evolution of the western North America, the physics underlying the "continental tilt" mechanism is derived from some well established concepts of mantle convection model. In a study of the relationships between active subduction zones and surface topography, Gumis (1993b) documented that many modem coastal plains inland of subduction zones display gently depressed topography after corrections were made for surface processes. This finding lends support to the concept of continental tilt as a mechanism for the vertical movement patterns western North America was subjected to during the Cretaceous and Tertiary. The limitation of this mechanism, however, is that it does entail very shallow subduction and a strong lithosphere for the deflection to reach far enough into the cratonic interior. For example, if "continental tilt" is invoked to explain the residual subsidence documented in this study, one would expect a "tilted" subsidence profile similar to curve a in Fig 59 A. Clearly, this is not the case. Nevertheless, this mechanism deserves further testing in future studies, particularly in the rock record. The ideal settings to test this mechanism would be cratonic interior basins bordering subduction zones. Specifically, the approach taken in this study can be applied to make corrections for tectonic subsidence originating in crustal processes, such as thrust loading. If "continental tilt" is a Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. valid mechanism, then predictably the regional subsidence patterns, once corrected for other subsidence mechanisms, should always increases slowly towards the subduction zones. Mantle dynamic topography Over the years, epeirogenic movements have been hypothesized to be a consequence of secular variations in the mantle thermal regimes (Sloss, 1974). However, it is not until recently, owing to progress in studies of mantle convection, that the relationships between the dynamics of mantle convection and vertical movements of continents has begun to be understood (Gumis, 1990, 1988). Using sophisticated numerical modeling techniques and drawing on the latest findings in tomographic mapping of the mantle, Gumis (1988,1990) and others have demonstrated that significant changes in dynamic topography and the geoid can occur as plates move from regions of upwelling to downwelling (Fig. 60). With respect to individual plates in motion, such changes are reflected in episodic vertical movements that measure up to several hundreds of meters. Although contemporaneous tectonoeustatic fluctuations brought about by ridge volume changes also are important, the epeirogenic movements are continent-specific, depending on the rate and path of plate motion. Gumis (1988) suggested that the epeirogenic movements documented in cratonic basins around the world may be the records of continental vertical movements caused by dynamic topography. Gumis (1990,1993a) interpreted the widespread Cretaceous shallow marine deposits in the Western Interior basin as the result of this mechanism. Specifically, this model can be expanded as follows. As seen in Figure 60, following the break-up of Pangaea in the early Mesozoic, the North American plate became separated from Africa plate. Since then, it has been moving Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Downwelling CRETACEOUS Sea surface Seasurface [Pangaea; Upwelling TRIASSIC 1111! Distance Distance 1 1 1 I I (North Americaduring the Cretaceous) moving towards downwellings has alower topography and reduced free a. Aplate (Pangaeaduring the Triassic) positioned overupwellings has ahigh topography; b. a fragmentof the plate board area. Modified fromGumis (1990). Figure 60. Diagram showing changes in continental topography relative to sea surface during continental breakup, Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. northwestward and away from regions of mantle upwelling (Engebretson et al., 1985). Based on this plate motion history, the model for dynamic topography predicts that the western the North America should experience a decrease in the dynamic topography or a gradual reduction in the freeboard. The changes in the dynamic topography therefore should lead to epeirogenic subsidence in the Western Interior. The "residual" subsidence documented in this study, which has so far been difficult to explain either in terms of eustasy factors or using other known tectonic mechanisms, may be the evidence of changes in the dynamic topography. Until a more refined model arrives, the model for dynamic topography at least provides a plausible explanation for the residual subsidence documented in this study. The concept of dynamic topography is based on recent breakthroughs in solid earth geophysics. To stratigraphers, it provides a powerful conceptual framework within which to investigate epeirogenic movements and their relationships to contemporaneous eustatic sea level changes. However, because much of this model is based on modem plate tectonics data, it remains unclear what stratigraphic signatures it would leave in the rock record. Compelling evidence in support of it has been found in many Phanerozoic cratonic platform basins (Gumis, 1993a), but the challenge of unequivocally documenting its role in sedimentary basins around the world has not been met. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. CHAPTER 7 CONCLUSIONS The abundant litho- and biostratigraphic data in the Cretaceous Western Interior basin are superbly suited to flexural backstripping and foreland basin modeling. To document basin subsidence history, a major effort of this study went into compiling a regional stratigraphic data base by integrating subsurface and outcrop stratigraphic data from various sources. The result is a set of six regional stratigraphic sections showing middle Cenomanian to early Campanian (96 to 80 Ma) stratal thickness, lithofacies, and chronostratigraphic relationships across different segments of the U.S. Western Interior. Application of the two-dimensional flexural backstripping techniques to this stratigraphic data base resulted in six regional subsidence profiles. These profiles document a subsidence pattern that is spatially and temporally much more complex than previously recognized. Analysis of the observed subsidence pattern in terms of foreland basin models and in the context of basement tectonics furnished significant new insights into the Cretaceous subsidence history and its probable causes. The main conclusions follow: 1. The subsidence profiles, supplemented by a flexural model, document that the cumulative subsidence across the Western Interior over the 16 m.y. study interval consists of two distinct components: a westward-increasing flexural subsidence confined within a few hundred kilometers of the thrust belt, and a spatially uniform "residual" subsidence that affected the entire basin. The flexural subsidence generally exceeds the residual subsidence in magnitude along the thrust belt. However, in western Montana the residual subsidence actually exceeded flexural subsidence in this time interval. This observation implies that subsidence trends observed in the foreland of the Western Interior basin can not be all attributed to orogenic loading. 167 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 168 2. The regional flexural subsidence was characterized by spatial segmentation and temporal discordance. Spatially, the westward-increasing flexural subsidence shows great variations along the strike of the thrust belt. In Wyoming, flexural subsidence generated a deep and wide foreland basin. In contrast, flexural subsidence in southern Utah and western Montana was insignificant. In these areas, total subsidence was dominated by the residual subsidence component which extended eastward far beyond the effect of lithospheric flexure due to thrust loading. Temporally, the rates of subsidence also vary with location along the thrust belt. From middle Cenomanian to late Turonian (96 to 90 Ma), subsidence rates were high in Utah and much lower in Wyoming and Montana. In contrast, during the Coniacian and Santonian stages (90 to 85 Ma) subsidence accelerated rapidly in Wyoming, increased slightly in Montana, and decreased in Utah. At the end of the Santonian and into the early Campanian, rates of subsidence appear to have slowed everywhere. 3. The observed variations in flexural subsidence may be manifestations of basement structures, particularly those zones of weakness inherited from Precambrian rifting and early Paleozoic passive margin development. Three different mechanisms are proposed concerning this basement control on the Cretaceous flexural subsidence. First, basement directly affected the emplacement of thrust loads through the formation of buttresses that inhibited the eastward advance of the Sevier thrust sheets. Buttressing by basement structures may have controlled discrete, diachronous thrusting along the thrust belt, causing variations in subsidence trends with location. Moreover, buttresses such as those in southwestern Montana and northwestern Wyoming could lead to differential crustal shortening, creating spatially concentrated crustal loads. Second, basement faults or lineaments at high angle to the Cordilleran hingeline probably partitioned the crust underlying the Rocky Mountain region into tectonic blocks. During loading by the Sevier thrust sheets these separate blocks may have responded more or less independently. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 169 Third, the internal mechanical strength of the tectonic blocks differed from each other, depending on the nature of the Precambrian crust and the distribution of the zones of crustal weakness. Therefore, considerable variations in half flexural wavelength occurred along the basin strike. 4. A two-dimensional flexural model of the two subsidence profiles across the Wyoming foreland suggests that the westward-increasing flexural subsidence can be satisfactorily accounted for by flexure of a lithosphere with an elastic thickness of 80 ± 10 km and under a crustal load measuring 100 km in width and 3 to 5 km in height. These dimensions compare to earlier estimates for the size of the Meade-Crawford thrust system. The flexural half wavelength of the Wyoming foredeep is about 400 km. The predicted flexural forebulge is located slightly east of the Powder River and Hanna basins. 5. The "residual" subsidence documented in this study probably reflects epeirogenic movements specific to the North American Western Interior rather than eustatic sea level changes. Tectonic mechanism(s) to explain the residual subsidence remains controversial. Dynamic topography, driven by mantle convection, provides a plausible explanation. 6. The approach taken in this study of the tectonic subsidence history presents several distinct advantages over site-specific studies or those based on gross lithostratigraphic data. First, the broad stratigraphic data base of this study permits adequate sampling of the temporal and spatial variations in basin subsidence on different scales. Second, the large amount of outcrop biostratigraphy integrated into this data base improves the temporal resolution and precision of the results. Third, compared to Airy backstripping techniques, flexural backstripping techniques provide a superior means of calculating Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. basin subsidence history by accounting for both the flexural effects of sediment loading and the compaction of the Pre-Cretaceous strata. Reproduced with permission of the copyright owner. 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Further reproduction prohibited without permission. 213 Zelt, F. B., 1985, Natural gamma-ray spectrometry, lithofacies, and depositional environments of selected Upper Cretaceous marine mudrocks, western United States, including Tropic Shale and Tununk Member of Mancos Shale (unpublished Ph.D. dissertation): Princeton, N. J., Princeton University, 340 p. Zhou, Shaohua, 1993, A 3-D backstripping method and its application to the Eromanga Basin in central and eastern Australia: Geophysical Journal International, v. 112, p. 225-243. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. APPENDIX Wireline logs used in the stratigraphic cross-sections 1 to 6. Operator Well Name Location State Cross-section #1 (based on USGS Chart OC-71 and 72 by R ice): 1. Montalban 1 Don Wilson 27-36N-9W Montana 2. Johnston Petroleum Co. 1 Humes 21-36N-6W do 3. Grannell Sands 1 Fey 23-37N-2E do 4. Buttes Petroleum Co. Van Dessel 1 17-36N-7E do 5. Webb Resources Inc. 18-16-Lipp 18-32N-11E do 6. Gordon Hurd 1 James W.Davey 23-32N-17E do 7. Honolulu Oil 29-3 Thieltges 29-33N-23E do 8. Champlin Oil 1 Fed.-Kaufman 20-33N-27E do 9. W.A. Moncrief 1 Federal 22-33N-31E do 10. Seaboard & Honolulu Oil 1 Loberg 26-30N-36E do 11. Phillips Petrol. Co. 1-AUnruh 23-31N-45E do 12. J. P. Johnson 1 Blair 6-30N-50E do 13. Maxwell Oil Ostby 1 1-30N-58E N. Dakota 14. H.L. Hunt Marvin Nylander 1 15-156N-95W do 15. Pel-Tex and Conoco Haaland 26-159N-86W do 16. Midwest Gunning 22-159N-82W do 17. Pubco Petrol. Anklam 7-159-72W do 18. Mclaughlin Wolfe Fed. Land Bank 1 33-158-62W do Cross-section #2 (based on USGS Chart OC-71 and 72 by Rice): 1. Composite outcrop section by Roberts (1972). Livingston area Montana 2. Naftzer-Barker 1 Glennie 20-6N-14E do 3. Occidental I Gov't -Hall 2-8N-24E do 4. Sumatra 1 Hougan-Whelan 7-9N-32E do 5. Champlin Oil 1 Treasure County 12-7N-35E do 6. Texaco Texaco 1 State-’F 32-7N-39E do 7. George J. Greer 1 N. P. 15-3N-44E do 8. Gulf Oil Co. 1 State 16-1S-48E do 214 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 215 9. Davis Oil Co. 1 Federal 35-7S-50E do 10. Sinclair Oil and Gas 6-1 Espy 6-8S-55E do 11. Superior Oil Campbell Gov't 14-9 9-8S-60E S. Dakota 12. Mobil Mickelson 1 7-9N-9E do 13. Amerada Meade-Corwin 1 18-6N-13E do 14. F.E. Pohle May 1 21-4N-18E do 15. Gulf Oil C. E. Harry 1 4-3N-23E do 16. Tenneco Herman Estate 1 10-1N-29E do 17. Gulf Oil Hutchinson 1 4-103N-77W do Cross-section #3: 1. Texaco Spread Creek Unit 1 31-44N-112W Wyoming 2. Kingwood Oil Dicke 3 22-45N-101W do 3. R.L. Manning Cottonwood Land company 1 15-45N-97W do 4. Continental Oil Boulder Gulch 27-1 27-45N-95W do 5. The California Company Neiber Unit 3 14-45N-93W do 6. Amoco USA-Dale D Ozman 1 10-45N-91W do 7. Mapco 1-8 Gov't 8-45N-89W do 8. Mapco 1-30 Fed. 30-50N-82W do 9. Davis Oil Co. Healy-Fed. 1 8-51N-80W do 10. Webb Resources Inc. Fed. 12-13 12-51N-78W do 11. R.L. Manning Gov't Hawks 1 22-52N-76W do 12. Davis Oil Co. Smith-Fed. 2 12-53N-74W do 13. Stuarco Oil Co. Herrington Fed. 19-11 19-54N-72W do 14. Jerry Enkich and Ass. Co. Enkich Gov't Norfolk 1 19-54N-71W do 15. C.E Brehm Co. Gov’t 13-2 2-54N-70W do 16. William Ham, Jr., Co. Heald Gov't 1 27-55N-69W do 17. Gulf Oil C. E. Harry 1 4-3N-23E do Cross-section #4: 1. Amoco Dry Muddy Creek unit 1 16-20N-114W Wyoming 2. Carter Oil Co. Opal 1 34-22N-112W do 3. Davis Oil Co. East Storm Shelter 1 6-23N-110W do 4. Wolf Energy Sandy Bend 1 14-23N-108W do 5. Davis Oil Co. Dines Unit 1 7-20N-105W do Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 216 6. Texaco Delaney Rim Unit 1 30-18N-97W do 7. U.S. Natural Gas Co. Cow Creek unit 22-13 13-16N-92W do 8. Tenneco Sugar Creek Unit 3 11-18N-90W do 9. Tesoro Tesoro-Skyline Fed. 1 28-19N-88W do 10. Sinclair Oil and Gas Fed. 12-22-87 1 12-22N-87W do 11. Composite log: upper part: Union 1 Gov't 22-20N-84W do lower part: (Skelly Oil) U.P.R.R-Maden 1 29-21-N-85W do 12. The Texas Company Hill Creek Unit 1 14-20N-81W do 13. R.G. Berry Fed. 1-24 24-21N-78W do 14. True Oil Company Schmale 11-1 1-19N-75W do 15. Phillips Petrol. Co. U. P. A. 6-23 23-16N-73W do 16. Apache Coip. 1 Polo Ranch 14-14N-68W do 17. M.L. Goodston Hutchinson 1 18-17N-62W do 18. Superior Oil Emers 33-5 5-5N-20W Nebraska Cross-section #5: 1. Phillips Petrol. Co. Wasatch Plateau 1 24-2 IS-IE Utah 2. Tennessee Gas Transmission Irons 1 16-15S-3E do 3. Three States Natural Gas Joe's Valley Unit 2 23-16S-5E do 4. Composite log: upper: Pacific Western Oil Gordan Creek Unit 1 24-14S-7E do lower: Three States-Morgan-Walton Mary D Kearns 1 27-16S-6E do 5. Occidental Gordan Creek 1 19-14S-8E do 6. Amerada USA Abbott 1 29-14S-9E do 7. Forest Oil Co. Gov't Arnold 25-1 25-16S-14E do 8. Gulf Oil Co. US Norris Fed. 1 8-18S-16E do 9. Tenneco Butter Canyon USA 33-12 33-19S-17E do 10. Tenneco Rattle Snake Canyon 16-4 16-19S-19E do 11. Pacific Natural Gas Segundo Canyon 23-4 4-17S-21E do 12. Mountain Fuel & Supply Main Canyon 1 28-15S-23E do 13. Raymond Oil Company Government 1 17-13S-25E do 14. Coseka Resources USA Arco Fed. 11-4-5-103 4-5S-103W Colorado 15. Nucorp Energy Inc. Turner 1-27 27-6S-99W do 16. Phillips Petrol. Co. Mannel 1 27-1N-95W do Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. 217 17. Seaboard Oil Co. Kritsas 2 32-2N-93W do 18. California Oil Co. California Gov't 1 7-2N-92W do 19. The Texas Company Knolton 14 6-4N-91W do 20. Miami Oil Producers O'brien 1 14-4N-90W do 21. McCulIoch Oil Corp Skeeter 1 8-5N-89W do 22. Havenstrite Oil Company Pretiss 3 2-3N-86W do 23. Aztec Oil & Gas Company Carter Creek 1 7-3N-80W do 24. Great Lakes Natural Gas Underwood 54-B-’B' 31-2N-76W do 25. National Assoc. Petrol. Martin 1-33 33-2N-69W do 26. Equitable Petroleum Co. Hawkins 1 22-5N-67W do 27. The Ohio Oil Co. Eva S. Nordloh 1 20-5N-63W do 28. GEM Oil Company Redman 1 25-6-61W do 29. National Assoc. Petrol. Bomhart 1 14-4N-58W do 30. M.P. Gilbert Ebsack-State 16-33 16-1N-51W do 31. R.E. Hibbert Vorce 1 28-1S-49W do 32. LION Oil Company Earl 1 1-4N-41W Nebraska 33. Superior Oil Emers 33-5 5-5N-20W do Cross-section #6 1. Phillips Petrol. Co. Hatch 16-37S-6W Utah 2. Tenneco Griffin Point USA 1 22-33S-1W do 3. Sam Gary & West Henry Mt. Co. Fed. Apple 22-7 22-31S-9E do 4. British Petrol. Fed. Cronigan 1 23-30N-16W New Mexico 5. Southland Royalty Comp. Locke 1 3-29N-14W do 6. Union Texas Petrol. Helh's Fed. 1-E 22-30N-10W do 7. Northwest Pipeline Co. San Juan 29-6-62-A 4-29N-6W do 8. Phillips Petrol. Co. Jicarilla 28-3 #1 6-28N-3W do 9, Texota Fed. 1-A 17-26N-1E do 10. Continental Oil Colorado Fuel & Iron 1 13-34S-66W Colorado 11. Coronado Co. Bohart 1 19-15S-62W do 12. Sinclair-Prairie Robbins 1 32-4S-35W Kansas Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. VITA Ming Pang was bom and grew up in Hami, Xinjiang, a province in the northwestern part of the People's Republic of China. In 1978, he was enrolled into the Chengdu College of Geology to study petroleum geology. In 1982, he graduated with a Bachelor’s degree in geology. After graduation from college, he attended graduate school at the China University of Geosciences at Beijing, where he studied sedimentary geology and its applications to petroleum explorations. He graduated in 1985 with a thesis on the diagenesis of the coal-bearing Permian and Carboniferous rocks in north-central China. After the graduate study, he joined the faculty of the Department of Petroleum Geology at the China University of Geosciences at Beijing. In 1988, he came to the Department of Geology and Geophysics of the Louisiana State University to pursue a Ph.D. degree. While at the Louisiana State University, he directed his interest to stratigraphy and geophysics. His Ph.D. dissertation is a regional stratigraphic and tectonic analysis of the U.S. Cretaceous Western Interior basin. 218 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. DOCTORAL EXAMINATION AND DISSERTATION REPORT Candidate: Ming Pang Major Pield: Geology Title of Dissertation: Tectonic Subsidence of the Cretaceous Western Interior Basin, United States EXAMINING COMMITTEE: MM- ■J M Date of Examination: November 30. 1994 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. .*;• .*;•. .*.• .*;• . *.*.•.* * *.*.•.* m c c River Central £ Central ^ South £ EmerySs " *.*• *.*• *.*• *.*• *.*• yy . • * .* . •• •• • / . • . * . \ \ • * % C.R. ■ *S *•’.* *•’.* •.• • f \n• > •> * *. • *. • •, • *. • • • •. • *. • • p i *.• •.* .*.• .*.* .*.• . *«V *•*«• *•*«• . *«V •