Geochemistry and Petrology of Basaltic Rocks from the Marshall Islands
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Field Geology and Petrologic Investigation of the Strawberry Volcanics, Northeast Oregon
Portland State University PDXScholar Dissertations and Theses Dissertations and Theses Winter 2-24-2016 Field Geology and Petrologic Investigation of the Strawberry Volcanics, Northeast Oregon Arron Richard Steiner Portland State University Follow this and additional works at: https://pdxscholar.library.pdx.edu/open_access_etds Part of the Geology Commons, and the Volcanology Commons Let us know how access to this document benefits ou.y Recommended Citation Steiner, Arron Richard, "Field Geology and Petrologic Investigation of the Strawberry Volcanics, Northeast Oregon" (2016). Dissertations and Theses. Paper 2712. https://doi.org/10.15760/etd.2708 This Dissertation is brought to you for free and open access. It has been accepted for inclusion in Dissertations and Theses by an authorized administrator of PDXScholar. Please contact us if we can make this document more accessible: [email protected]. Field Geology and Petrologic Investigation of the Strawberry Volcanics, Northeast Oregon by Arron Richard Steiner A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Environmental Sciences and Resources: Geology Dissertation Committee: Martin J. Streck, Chair Michael L. Cummings Jonathan Fink John A.Wolff Dirk Iwata-Reuyl Portland State University 2016 © 2015 Arron Richard Steiner i ABSTRACT The Strawberry Volcanics of Northeast Oregon are a group of geochemically related lavas with a diverse chemical range (basalt to rhyolite) that erupted between 16.2 and 12.5 Ma and co-erupted with the large, (~200,000 km3) Middle Miocene tholeiitic lavas of the Columbia River Basalt Group (CRBG), which erupted near and geographically surround the Strawberry Volcanics. The rhyolitic lavas of the Strawberry Volcanics produced the oldest 40Ar/39Ar ages measured in this study with ages ranging from 16.2 Ma to 14.6 Ma, and have an estimated total erupted volume of 100 km3. -
Geochemistry of Sideromelane and Felsic Glass Shards in Pleistocene Ash Layers at Sites 953, 954, and 9561
Weaver, P.P.E., Schmincke, H.-U., Firth, J.V., and Duffield, W. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 157 25. GEOCHEMISTRY OF SIDEROMELANE AND FELSIC GLASS SHARDS IN PLEISTOCENE ASH LAYERS AT SITES 953, 954, AND 9561 Andrey A. Gurenko2 and Hans-Ulrich Schmincke2 ABSTRACT Sideromelane and felsic glass shards from unconsolidated Pleistocene volcaniclastic sediments drilled at Sites 953, 954, and 956 are thought to have derived from submarine and subaerial volcanic eruptions on Gran Canaria (Sites 953 and 954) and Tenerife (Sites 954 and 956). We analyzed these glasses by electron microprobe for major elements and sulfur, chlorine, and fluorine. Sideromelane glasses represent a spectrum from alkali basalt through basanite, hawaiite, mugearite, and tephrite to nephelinite. Felsic glasses have compositions similar to benmoreite, trachyte, and phonolite. Vesiculated mafic and felsic glass shards, which are characterized by low S and Cl concentrations (0.01−0.06 wt% S and 0.01–0.04 wt% Cl), are interpreted to have formed by pyroclastic activity on land or in shallow water and appeared to have been strongly degassed. Vesicle-free blocky glass shards having 0.05−0.13 wt% S are likely to have resulted from submarine eruptions at moderate water depths and represent undegassed or slightly degassed magmas. Cl concentrations range from 0.01 to 0.33 wt% and increase with increasing MgO, suggesting that Cl behaves as an incompatible element during magma crystallization. Concentrations of fluorine (0.04− 0.34 wt% F) are likely to represent undegassed values, and the variations in F/K ratios between 0.02 and 0.24 are believed to reflect those of parental magmas and of the mantle source. -
Nonexplosive and Explosive Magma/Wet-Sediment Interaction
Journal of Volcanology and Geothermal Research 181 (2009) 155–172 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Nonexplosive and explosive magma/wet-sediment interaction during emplacement of Eocene intrusions into Cretaceous to Eocene strata, Trans-Pecos igneous province, West Texas Kenneth S. Befus a,⁎, Richard E. Hanson a, Daniel P. Miggins b, John A. Breyer a, Arthur B. Busbey a a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b U.S. Geological Survey, Denver Federal Center, Box 25046, Denver, CO 80225, USA article info abstract Article history: Eocene intrusion of alkaline basaltic to trachyandesitic magmas into unlithified, Upper Cretaceous Received 16 June 2008 (Maastrichtian) to Eocene fluvial strata in part of the Trans-Pecos igneous province in West Texas produced Accepted 22 December 2008 an array of features recording both nonexplosive and explosive magma/wet-sediment interaction. Intrusive Available online 13 January 2009 complexes with 40Ar/39Ar dates of ~47–46 Ma consist of coherent basalt, peperite, and disrupted sediment. Two of the complexes cutting Cretaceous strata contain masses of conglomerate derived from Eocene fluvial Keywords: deposits that, at the onset of intrusive activity, would have been N400–500 m above the present level of phreatomagmatism peperite exposure. These intrusive complexes are inferred to be remnants of diatremes that fed maar volcanoes during diatreme an early stage of magmatism in this part of the Trans-Pecos province. Disrupted Cretaceous strata along Trans-Pecos Texas diatreme margins record collapse of conduit walls during and after subsurface phreatomagmatic explosions. -
Alkalic-Type Epithermal Gold Deposit Model
Alkalic-Type Epithermal Gold Deposit Model Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. Department of the Interior U.S. Geological Survey Cover. Photographs of alkalic-type epithermal gold deposits and ores. Upper left: Cripple Creek, Colorado—One of the largest alkalic-type epithermal gold deposits in the world showing the Cresson open pit looking southwest. Note the green funnel-shaped area along the pit wall is lamprophyre of the Cresson Pipe, a common alkaline rock type in these deposits. The Cresson Pipe was mined by historic underground methods and produced some of the richest ores in the district. The holes that are visible along several benches in the pit (bottom portion of photograph) are historic underground mine levels. (Photograph by Karen Kelley, USGS, April, 2002). Upper right: High-grade gold ore from the Porgera deposit in Papua New Guinea showing native gold intergrown with gold-silver telluride minerals (silvery) and pyrite. (Photograph by Jeremy Richards, University of Alberta, Canada, 2013, used with permission). Lower left: Mayflower Mine, Montana—High-grade hessite, petzite, benleonardite, and coloradoite in limestone. (Photograph by Paul Spry, Iowa State University, 1995, used with permission). Lower right: View of north rim of Navilawa Caldera, which hosts the Banana Creek prospect, Fiji, from the portal of the Tuvatu prospect. (Photograph by Paul Spry, Iowa State University, 2007, used with permission). Alkalic-Type Epithermal Gold Deposit Model By Karen D. Kelley, Paul G. Spry, Virginia T. McLemore, David L. Fey, and Eric D. Anderson Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. -
Analogues for Radioactive Waste For~1S •
PNL-2776 UC-70 3 3679 00049 3611 ,. NATURALLY OCCURRING GLASSES: ANALOGUES FOR RADIOACTIVE WASTE FOR~1S • Rodney C. Ewing Richard F. Haaker Department of Geology University of New Mexico Albuquerque, ~ew Mexico 87131 April 1979 Prepared for the U.S. Department of Energy under Contract EY-76-C-06-1830 Pacifi c i'lorthwest Laboratory Richland, Washington 99352 TABLE OF CONTENTS List of Tables. i i List of Figures iii Acknowledgements. Introduction. 3 Natural Glasses 5 Volcanic Glasses 9 Physical Properties 10 Compos i ti on . 10 Age Distributions 10 Alteration. 27 Devitrification 29 Hydration 32 Tekti tes. 37 Physical Properties 38 Composition . 38 Age Distributions . 38 Alteration, Hydration 44 and Devitrification Lunar Glasses 44 Summary . 49 Applications to Radioactive Waste Disposal. 51 Recommenda ti ons 59 References 61 Glossary 65 i LIST OF TABLES 1. Petrographic Properties of Natural Glasses 6 2. Average Densities of Natural Glasses 11 3. Density of Crystalline Rock and Corresponding Glass 11 4. Glass and Glassy Rocks: Compressibility 12 5. Glass and Glassy Rocks: Elastic Constants 13 6. Glass: Effect of Temperature on Elastic Constants 13 7. Strength of Hollow Cylinders of Glass Under External 14 Hydrostatic Pressure 8. Shearing Strength Under High Confining Pressure 14 9. Conductivity of Glass 15 10. Viscosity of Miscellaneous Glasses 16 11. Typical Compositions for Volcanic Glasses 18 12. Selected Physical Properties of Tektites 39 13. Elastic Constants 40 14. Average Composition of Tektites 41 15. K-Ar and Fission-Track Ages of Tektite Strewn Fields 42 16. Microprobe Analyses of Various Apollo 11 Glasses 46 17. -
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 ICELAND GEOSURVEY Reykjavík: Orkugardur, Grensásvegur 9, 108 Reykjavík, Iceland - Tel.: 528 1500 - Fax: 528 1699 Akureyri: Rangárvellir, P.O. Box 30, 602 Akureyri, Iceland - Tel.: 528 1500 - Fax: 528 1599 [email protected] - www.isor.is Report Project no.: 540105 Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 December 2011 Key page Report no. Date Distribution ÍSOR-2011/064 December 2011 Open Closed Report name / Main and subheadings Number of copies Icelandic Hyaloclastite Tuffs. Petrophysical Properties, Alteration 7 and Geochemical Mobility Number of pages 103 Authors Project manager Hjalti Franzson, Gudmundur H. Gudfinnsson, Julia Frolova, Hjalti Franzson Helga M. Helgadóttir, Bruce Pauly, Anette K. Mortensen and Sveinn P. Jakobsson Classification of report Project no. 540105 Prepared for National Energy Authority and Reykjavík Energy Cooperators Moscow University, University of California in Davis, Natural History Museum in Iceland Abstract This study attempts to define the properties of hyaloclastite formations which control their petrophysical characteristics during their progressive alteration. It is based on 140 tuffaceous cores from last glaciation to 2–3 m y. The water content shows a progressive increase with alteration to about 12%, which mainly is bound in the smectite and zeolite alteration minerals. -
Basalt-Trachybasalt Samples in Gale Crater, Mars
Open Research Online The Open University’s repository of research publications and other research outputs Basalt-trachybasalt samples in Gale Crater, Mars Journal Item How to cite: Edwards, Peter H.; Bridges, John C.; Wiens, Roger; Anderson, Ryan; Dyar, Darby; Fisk, Martin; Thompson, Lucy; Gasda, Patrick; Filiberto, Justin; Schwenzer, Susanne P.; Blaney, Diana and Hutchinson, Ian (2017). Basalt- trachybasalt samples in Gale Crater, Mars. Meteoritics & Planetary Science, 52(11) pp. 2391–2410. For guidance on citations see FAQs. c 2017 The Authors Meteoritics Planetary Science https://creativecommons.org/licenses/by-nc-nd/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1111/maps.12953 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Meteoritics & Planetary Science 52, Nr 11, 2391–2410 (2017) doi: 10.1111/maps.12953 Basalt–trachybasalt samples in Gale Crater, Mars Peter H. EDWARDS1, John C. BRIDGES 1*, Roger WIENS2, Ryan ANDERSON3, Darby DYAR4, Martin FISK5, Lucy THOMPSON 6, Patrick GASDA2, Justin FILIBERTO7, Susanne P. SCHWENZER8, Diana BLANEY9, and Ian HUTCHINSON1 1Department of Physics and Astronomy, Leicester Institute for Space and Earth Observation, University of Leicester, Leicester LE1 7RH, UK 2Los Alamos National Lab, Los Alamos, New Mexico 87545, USA 3USGS Astrogeology Science -
THE PETROCHEMISTRY of JAKE M: a MARTIAN MUGEARITE. Stolper
44th Lunar and Planetary Science Conference (2013) 1685.pdf THE PETROCHEMISTRY OF JAKE_M: A MARTIAN MUGEARITE. Stolper, E.M.1, Baker, M.B.1, Fisk, M.2, Gellert, R.3, King, P.L.4, McLennan, S.M.5, Minitti, M.6, Newcombe, M.1, Schmidt, M.E. 7, Treiman, A.H.8, and the MSL Science Team. 1Caltech, Pasadena, CA 91125, 2Oregon State Univ., 3Univ. Guelph, 4Res. School Earth Sci., ANU, 5SUNY, Stony Brook, 6Applied Phys. Lab., Johns Hopkins Univ., 7Brock Univ., 8Lunar & Planet. Inst. Introduction: Rock “Jake_M” (JM; named for JPL The surface of JM was not brushed or abraded prior engineer Jake Matijevic) was the first sample analyzed to analysis, so the APXS analyses probably include by the Alpha Particle X-ray Spectrometer (APXS) in- contributions from surface coatings, including adhering strument on MSL [1]. Although it is an isolated frag- dust, and these are the probable source of the S and Cl ment lacking field context, its dark color and apparently in JM. Experience with MER, however, indicates that fine-grained texture suggested it was a relatively homo- the characteristics of rock compositions are typically geneous igneous rock and thus an appropriate sample to not obscured by surface components, and the levels of S initiate the APXS analytical program. We report here and Cl in JM are lower than virtually all unbrushed the preliminary APXS analyses of JM and a plausible analyses from the Spirit rover and lower than many of interpretation of their significance for petrogenesis. the brushed analyses, so the level of surface contamina- Results: Three spots on JM were analyzed with the tion and alteration are likely relatively minor [5]. -
Deep Sea Drilling Project Initial Reports Volume 59
37. THE GEOCHEMISTRY, MINERALOGY, AND PETROLOGY OF BASALTS FROM THE WEST PHILIPPINE AND PARECE VELA BASINS AND FROM THE PALAU-KYUSHU AND WEST MARIANA RIDGES, DEEP SEA DRILLING PROJECT LEG 59 David P. Mattey, Nicholas G. Marsh, and John Tarney,1 Department of Geological Sciences, University of Birmingham, Birmingham B15 2TT, England INTRODUCTION netic fabric of the Parece Vela Basin suggest a similar origin—the sundering of the Palau-Kyushu Ridge in the Legs 59 and 60 of the International Phase of Oceanic late Oligocene (Karig, 1975). The origin of the West Drilling (IPOD) were designed to study the nature and Philippine Basin is less clear, however, and the age and history of volcanism of the active Mariana arc, its cur- magnetic fabric of this basin remain controversial. Re- rently spreading inter-arc basin (the Mariana Trough), cent studies of rocks dredged from the Mariana Trough and the series of inactive basins and intervening ridges (Hart et al., 1972), the Lau Basin (Hawkins, 1976), and that lie to the west (Fig. 1). The older basins and ridges the Scotia Sea (Saunders and Tarney, 1979) all reveal were drilled during Leg 59 as the first part of a transect that these basins are floored by basalts geochemically of single-bit holes drilled in each major basin and ridge. similar to basalts erupted at mid-ocean ridges. The for- The eastern part of the transect—the technically active mation of active back-arc basins (e.g., the East Scotia region—was drilled during Leg 60. Sea, Barker 1970) in the Mariana Trough (Karig et al., The evolution of island-arc volcanos and magma 1978) is considered by many authors to be the result of genesis associated with lithospheric subduction remain seafloor spreading broadly similar to that associated some of the most complex petrologic problems con- with a mid-ocean ridge (e.g., Karig, 1971). -
29. Sulfur Isotope Ratios of Leg 126 Igneous Rocks1
Taylor, B., Fujioka, K., et al., 1992 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 126 29. SULFUR ISOTOPE RATIOS OF LEG 126 IGNEOUS ROCKS1 Peter Torssander2 ABSTRACT Sulfur isotope ratios have been determined in 19 selected igneous rocks from Leg 126. The δ34S of the analyzed rocks ranges from -0.1 o/00 to +19.60 o/oo. The overall variation in sulfur isotope composition of the rocks is caused by varying degrees of seawater alteration. Most of the samples are altered by seawater and only five of them are considered to have maintained their magmatic sulfur isotope composition. These samples are all from the backarc sites and have δ34S values varying from +0.2 o/oo to +1.6 o/oo , of which the high δ34S values suggest that the earliest magmas in the rift are more arc-like in their sulfur isotope composition than the later magmas. The δ34S values from the forearc sites are similar to or heavier than the sulfur isotope composition of the present arc. INTRODUCTION from 0 o/oo to +9 o/00 (Ueda and Sakai, 1984), which could arise from inhomogeneities in the mantle but are more likely a result of contami- Sulfur is a volatile element that can be degassed during the ascent nation from the subducting slab (A. Ueda, pers. comm., 1988). of basaltic magma. Degassing causes sulfur isotope fractionation; the Leg 126 of the Ocean Drilling Program (ODP) drilled seven sites isotopic composition of sulfur in rocks can vary with the concentra- in the backarc and forearc of the Izu-Bonin Arc (Fig. -
Cretaceous Basaltic Phreatomagmatic Volcanism in West Texas: Maar Complex at Peña Mountain, Big Bend National Park ⁎ K.S
Available online at www.sciencedirect.com Journal of Volcanology and Geothermal Research 173 (2008) 245–264 www.elsevier.com/locate/jvolgeores Cretaceous basaltic phreatomagmatic volcanism in West Texas: Maar complex at Peña Mountain, Big Bend National Park ⁎ K.S. Befus a, , R.E. Hanson a, T.M. Lehman b, W.R. Griffin c a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b Department of Geosciences, Texas Tech University, Box 41053, Lubbock, TX 79409, USA c Department of Geosciences, University of Texas at Dallas, Box 830688, Richardson, Texas 75083, USA Received 23 March 2007; accepted 25 January 2008 Available online 10 March 2008 Abstract A structurally complex succession of basaltic pyroclastic deposits produced from overlapping phreatomagmatic volcanoes occurs within Upper Cretaceous floodplain deposits in the Aguja Formation in Big Bend National Park, West Texas. Together with similar basaltic deposits recently documented elsewhere in the Aguja Formation, these rocks provide evidence for an episode of phreatomagmatic volcanism that predates onset of arc magmatism in the region in the Paleogene. At Peña Mountain, the pyroclastic deposits are ≥70 m thick and consist dominantly of tabular beds of lapillistone and lapilli tuff containing angular to fluidal pyroclasts of altered sideromelane intermixed with abundant accidental terrigenous detritus derived from underlying Aguja sediments. Tephra characteristics indicate derivation from phreatomagmatic explosions involving fine- scale interaction between magma and sediment in the shallow subsurface. Deposition occurred by pyroclastic fall and base-surge processes in near-vent settings; most base-surge deposits lack tractional sedimentary structures and are inferred to have formed by suspension sedimentation from rapidly decelerating surges. -
TERTIARY MAGMATISM in NORTHERN SARDINIA by Michael
TERTIARY MAGMATISM IN NORTHERN SARDINIA by Michael John Rutter A Thesis submitted for the Degree of Doctor of Philosophy, University of London Department of Geology, Imperial College of Science & Technology, Prince Consort Road, LONDON SW7. ABSTRACT Tertiary magmatism in northern Sardinia is dominated by a temporal transition from subduction-related (29.9-13 Ma) to extensional (5-0.12 Ma) volcanism. Geochemical parameters of lavas, independent of any differentiation processes, have been used to constrain the changing chemical characteristics of magma-producing source mantle beneath Sardinia, during and after active subduction. Late Oligocene and Miocene (29.9-13 Ma) basalt-andesite- dacite-rhyolite lavas were associated with active subduction, to the east of the Sardinia continental block. They are associated with contemporaneous extension, possibly in a back-arc environment, which facilitated passage of magmas to the surface, and high-T low-P fractionation of an anhydrous gabbroic mineral assemblage. Low K/Cs and high Ba/La ratios in Sardinian subduction-related magmas, may reflect the influx of fluids or melts, derived from the subducted slab, into their mantle source. Low Nb and Ta abundances can be explained by the retention of these elements in some residual phase, stable under the hydrous conditions which may exist in the mantle wedge, although this phase is probably not titaniferous. High LILE-HFSE ratios may represent the addition of LILE-enriched fluids or melts from the subducted oceanic lithosphere to MORB-source mantle, or to magma generation in OIB-source mantle. Following a gap in magmatic activitiy, volcanism resumed in the Pliocene with the eruption of high-Al basalt, dacite and rhyolite lavas, which require the persistence of subduction-related source mantle beneath Sardinia at least 8 Ma after the cessation of active subduction.