Plateau Collapse Model for the Transantarctic Mountains–West Antarctic Rift System: Insights from Numerical Experiments Robert W

Total Page:16

File Type:pdf, Size:1020Kb

Plateau Collapse Model for the Transantarctic Mountains–West Antarctic Rift System: Insights from Numerical Experiments Robert W Plateau collapse model for the Transantarctic Mountains–West Antarctic Rift System: Insights from numerical experiments Robert W. Bialas W. Roger Buck Department of Earth and Environmental Science, Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964, USA Michael Studinger Lamont-Doherty Observatory of Columbia University, Palisades, New York 10964, USA Paul G. Fitzgerald Department of Earth Sciences, Syracuse University, Syracuse, New York 13244, USA ABSTRACT The high elevation and considerable length of the Transantarctic Mountains have led to speculation about their origin. To date, no model has been able to adequately reconcile the jux- taposition of the high, curvilinear Transantarctic Mountains with the adjacent West Antarctic Rift System, a broad region of thin extended continental crust exhibiting wide rift character- istics. We present a fi rst-order investigation into the idea that the West Antarctic Rift System– Transantarctic Mountains region was a high-elevation plateau with thicker than normal crust before the onset of continental extension. With major Cretaceous extension, the rift underwent a topographic reversal, and a plateau edge with thickened crust, representing the ancestral Transantarctic Mountains, remained. In the Cenozoic, minor extension and major denuda- tion reduce the crustal root while simultaneously uplifting peak heights in the mountains. The Cretaceous stage of this concept is investigated using two-dimensional numerical models to determine under what conditions plateau collapse is plausible. Model results indicate that elevation of a remnant plateau edge decreases with increasing initial Moho temperature. Very cold initial Moho temperatures, <675 °C, under the plateau leave a thick plateau edge but do not exhibit wide rifting. A cold to moderate initial thermal structure, Moho temperatures of 675–850 °C, is needed to retain the plateau edge and still exhibit wide rifting in the middle of the plateau. We conclude that this plateau collapse concept is possible using these numerical experiments, and that application of this idea to the West Antarctic Rift System–Transantarctic Mountains system is also supported by geological and geophysical evidence. Keywords: Transantarctic Mountains, West Antarctic Rift System, rifting, numerical modeling, plateau collapse, Antarctica. INTRODUCTION While the spatial relationship between the The Transantarctic Mountains are one of the mountains and rift system is obvious, many dominant features of the Antarctic continent aspects of their formation remain unclear. Large- and defi ne the boundary between cratonic East magnitude extension in the West Antarctic Rift Antarctica and the West Antarctic Rift System System during the Cretaceous accompanied (Fig. 1). The Transantarctic Mountains are more relatively little denudation in the Transantarctic than 3000 km long and have local peak eleva- Mountains at that time. Conversely, minor Ceno- tions in excess of 4 km, making them the larg- zoic extension adjacent to the mountains accom- est and longest rift-related mountain belt in the panied or is younger than most of the denudation world. The West Antarctic Rift System is adja- (Fitzgerald, 2002; Karner et al., 2005; Huerta and cent to the mountains, and is a broad region of Harry, 2007). Geological and geophysical evi- thin, extended continental crust 750–1000 km dence arguing against the often-cited broken plate wide, comparable to the Basin and Range Prov- model for Transantarctic Mountains uplift (ten ince of North America (Fitzgerald et al., 1986). Brink et al., 1997) is mounting (e.g., Studinger Previous quantitative models for the Trans- et al., 2004, 2006; Lawrence et al., 2006), most antarctic Mountains have mostly been kine- notably, the absence of a laterally continuous matic and include mainly thermal uplift of the crustally penetrating fault at the mountain–rift mountains (e.g., Smith and Drewry, 1984), a system interface required by such a model. Figure 1. Topographic and bathymetry map of combination of thermal and mechanical uplift Distributed extension in the West Antarctic Transantarctic Mountains and Ross Embay- related to rifting (e.g., Fitzgerald et al., 1986; Rift System may require hot, thin lithosphere ment; reference location map is in upper ten Brink et al., 1997), and mechanical effects (e.g., Buck, 1991), while rift shoulder uplift of the right. Ross Sea is characterized by a series of basins and basement highs and elevated of rifting thick lithosphere (van der Beek et al., Transantarctic Mountains may require a region of heat fl ow. Ross Embayment—Ross Sea plus 1994; Busetti et al., 1999). Stern et al. (2005) uniformly cold, thick lithosphere (Fig. 2). Distrib- Ross Ice Shelf. WARS—Ross Embayment attributed as much as 50% of peak height to the uted wide rifting in the Cretaceous would leave a plus extended parts of West Antarctica. effects of glacial erosion. broad area of hot, thinned lithosphere, similar to © 2007 The Geological Society of America. For permission to copy, contact Copyright Permissions, GSA, or [email protected]. GEOLOGYGeology, August, August 2007; 2007 v. 35; no. 8; p. 687–690; doi: 10.1130/G23825A.1; 4 fi gures; Data Repository item 2007177. 687 West Antarctic Rift System and to determine the Zealand to the Pacifi c plate, and marking the conditions for which retention of a plateau edge onset of major extension in the West Antarctic with thick crust is plausible. Rift System (Lawver and Gahagan, 1995). Wide rifting (~400 km) ended with the 84–79 Ma sepa- TECTONIC SETTING ration of New Zealand and the Campbell Plateau The Transantarctic Mountains and West Ant- from Antarctica (Stock and Cande, 2002). Denu- arctica have been the site of repeated orogenies, dation (1–2 km magnitude) during the Creta- including Rodinian assembly, Rodinian breakup, ceous synchronous with this major extension and a transition from a passive to an active mar- is recorded along the Transantarctic Mountains Figure 2. Two classes of models of Trans- gin during Gondwana assembly (e.g., Goodge, (e.g., Fitzgerald, 2002, and references therein). antarctic Mountain uplift and Ross Embay- 2002). During the Cambrian–Ordovician Ross The major phase of denudation, 4−9 km along ment subsidence. Dashed lines approximate orogeny the region was part of the active mar- the Transantarctic front, began in the Eocene, brittle-ductile transition. Top panel shows pre-rift confi guration; bottom panels show gin of Gondwana (Goodge, 2002, and refer- spatially correlative with but temporally preced- post-rift confi guration. Class A demonstrates ences therein). Subduction moved outboard to ing minor extension localized in the Ross Sea extension of cold, thick lithosphere. Rift fl ank the Pacifi c margin of Gondwana from at least adjacent to the mountains (e.g., Fitzgerald, 2002, uplift raises the edges of the rift due to ther- 320 Ma to ca. 110 Ma (Mukasa and Dalziel, and references therein). The nature and extent of mal effects. Extension is characterized by narrow rifting, and isotherms are shallowed 2000). Reconstructions (e.g., Foster and Gray, Cenozoic rifting as well as its relationship to the locally. Class B, proposed in this paper, dem- 2000) indicate that the along-strike equiva- thermochronology data are still uncertain. Nar- onstrates extension of a high plateau under- lent to the region between Marie Byrd Land row rifting in the Terror Rift, transtension in Vic- lain by hot thick crust. Extension occurs over and the Transantarctic Mountains, what would toria Land (Wilson, 1995; Rossetti et al. 2006), a broad region in the former plateau, and rift have been the majority of the unextended Ross Adare Trough spreading projected into the Ross fl anks retain much of their elevation through retention of thick crustal roots. Isotherms are Embayment, from the Cambrian to the Middle Sea (Davey et al., 2006, and references therein), shallowed over a wide region. Devonian was the Lachlan Fold Belt (orogen) of and minimal extension with mostly climate- southeastern Australia, then adjacent to Antarc- controlled denudation (Karner et al., 2005) have tica. This correlation implies high paleotopog- all been proposed as key mechanisms active in the the Basin and Range. The time between the end raphy and thickened crust in the West Antarctic Cenozoic. Cenozoic alkaline magmatism associ- of Cretaceous and beginning of Cenozoic rifting Rift System into the Devonian. ated with Cenozoic rifting (e.g., LeMasurier and is insuffi cient to cool and thicken the lithosphere Paleocurrent orientations, lithofacies, and Thomson, 1990) has a much smaller volume and under the mountain–rift system interface to the stratigraphic relationships of the Devonian– limited extent compared to Jurassic magmatism, level required for rift shoulder uplift. Triassic Beacon Supergroup in the central and is not a viable mechanism for thickening the As a way to reconcile the structures, distri- Transantarctic Mountains suggest that deposi- Transantarctic crust. bution of rifting, and the great elevation of the tion began within two intermontane or succes- Studinger et al., (2004, 2006) demonstrated mountains, we explore the possibility that the sor basins after postorogenic uplift of the Ross that gravity anomalies across southern Victoria West Antarctic Rift System was a high-elevation terrain (e.g., Isbell, 1999). These data and the Land and the Scott and Reedy Glacier region plateau with thicker than normal crust before presence of sub-Beacon relief in the central are
Recommended publications
  • The Undiscovered Oil and Gas of Antarctica
    DEPARTMENT OF THE INTERIOR U.S. Geological Survey The Undiscovered Oil and Gas of Antarctica by John Kingston^ OPEN-FILE REPORT 91-597 This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards or with the North American Stratigraphic Code. Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Government. ^Santa Barbara, California CONTENTS Page Abstract ....................................................... 1 Introduction ................................................... 2 Size of area .............................................. 2 Premise and problems of petroleum recoverability .......... 2 Previous investigations and petroleum assessments ......... 2 Methods of assessment ..................................... 4 Regional geology and petroleum occurrence ...................... 6 Assessment by play analysis .................................... 13 Rifted continental margin provinces ....................... 13 General; the south Australia rifted margin analog .... 13 Antarctica-Australia rift province ................... 17 Antarctica-India rift province ....................... 20 Antarctica-Africa rift province ...................... 24 Antarctica-Falkland rift province .................... 24 Interior rift provinces ................................... 30 General .............................................. 30 Ross sea interior rift province ...................... 30 Weddell sea interior rift province ..................
    [Show full text]
  • Geological Studies in Western Muhlig-Hofmann Mountains, Central Dronning Maud Land, East Antarctica
    Twenty Second Indian Expedition to Antarctica, Scientific Report, 2008 Ministry of Earth Sciences, Technical Publication No. 20, pp 177-189 Geological Studies in Western Muhlig-Hofmann Mountains, Central Dronning Maud Land, East Antarctica A. Dharwaclkar, R. Asthana, K. Kachroo, L.K. Oberoi and Aran Chaturvedi Geological Survey of India INTRODUCTION In pursuance of its long term program of mapping the entire Wohlthat ranges in cDML, East Antarctica, geological mapping was carried out in the western parts of Muhlig-Hofmann Mountains during the 22nd Indian Antarctic Expedition. About 1000 sq km area bounded by Longitudes 5°00' and 5°45' East and Latitudes 71°45' and 72° 10' South was covered during the austral summer of 2002-03. The study area lies more than 170NM WSW of Maitri station and the fieldwork was carried out using helicopters by taking drop- points in the area. GEOLOGICAL SETTING The East Antarctic shield is mostly composed of Precambrian crystalline rocks and has undergone a complex tectono-metamorphic history (Ravich & Kamenev, 1975; Sengupta, 1988; Tingey, 1991; D'Souza et al., 1997). The cDML basically consists of polymetamorphosed metasedimentary rocks represented by garnet-biotite schists, hornblende gneisses, metapelites, calc- silicates etc. These are intruded by various inagmatic units like anorthosite, granodiorite, granite, monzonite, charnockite and other minor instrusives. The deformational record of the region indicates a granulite facies metamorphism (Grenvillian) superimposed by later Pan-African (amphibolite to granulite) event. Record of the earlier Grenvillian event is preserved in the pelitic/ semipelitic schists and mafic granulites. (Jacobs et al., 2003). The Muhlig-Hofmann Mountains occurring in the western part of cDML are dominated by magmatic phase with large plutons of charnockite, granite and syenite forming the intrusive phase.
    [Show full text]
  • 4: Potential Mineral Resources in Antarctica
    Chapter 4 Potential Mineral Resources in Antarctica Photo credit: U.S. Geological Survey Byrd Glacier CONTENTS Page SUMMARY . 93 INTRODUCTION . 93 GEOLOGICAL ASSOCIATIONS . 96 Relationship to Adjacent Continents . 99 Offshore Shelf Areas . 102 ANTARCTICA IN THE CONTEXT OF FUTURE MINERALS SUPPLY . 103 Prospecting and Exploration in Antarctica . 105 Probabilities of Discovering Antarctic Mineral Deposits . 110 SELECTED MINERAL RESOURCES ● . 111 Oil and Gas . .. 111 coal . .114 Uranium . 114 Chromium . .115 Copper . 116 Gold . 117 Iron . .118 Molybdenum . .119 Platinum-Group Metals . .119 Rare-Earth Metals . .120 Diamonds . .. 122 Boxes Box Page 4-A. Mineral Resources and Reserves . 95 4-B. Geologic Time Scale . 98 4-C. Icebergs . 121 Figures Figure Page 4-1. Antarctic Mineral Occurrences . 97 4-2. Geologic Provinces of Antarctica and Their Relationship to Adjacent Gondwana Continents . 100 4-3. Reconstruction of Gondwana in Early Cretaceus Time . 103 4-4. Exposed Rock Outcrop in Antarctica . .. 106 4-5. What Antarctica Would Look Like If the Ice Were Removed . 107 4-6. Multichannel Seismic Data . .. 108 4-7. Sedimentary Basins in Antarctica . ,.. , 112 Tables Table Page 4-1. Desirable Research for Evaluating Resource Potential of Antarctica . 110 4-2. Research Required To Ensure That Petroleum Resources Are Safely and Efficiently Recovered With Minimum Environmental Impact . 110 4-3. Estimated Number of Major Mineral Deposits in Antarctica . 112 Chapter 4 Potential Mineral Resources in Antarctica SUMMARY The offshore sedimentary basins surrounding Antarctica offer the best prospects for petroleum Scientists have discovered occurrences (small exploration. The Weddell and Ross embayments in amounts) of several minerals in Antarctica, but West Antarctica, and Prydz Bay and the Wilkes there are no known mineral deposits of commer- Basin in East Antarctica are among the basins most cial interest.
    [Show full text]
  • Geology of Antarctica
    GEOLOGY OF ANTARCTICA 1. Global context of Antarctica Compared with other continents, the geological evolution of Antarctica is relatively little known, since less than 2% of the land emerges from beneath the thick cover of glacier ice. Yet where rocks are exposed, their pristine nature and lack of vegetation has enabled geologists to unravel many key components of the region’s history. In addition, the use of geophysical and remote sensing techniques, together with drilling on the Continental Shelf, has helped resolve many of the geological questions posed by the limited outcrop. Antarctica is the remotest of the world’s continents, with its nearest neighbour being South America, some 100 km (560 miles) distant. Yet, relatively early on in the geological exploration of Antarctica it was recognized that Antarctica shared a common history with other southern hemisphere continents, such as South America, Africa, Arabia, India and Australasia. However, these early ideas of movement of continents by joining together, followed by splitting apart, were ridiculed by many geologists and geophysicists, until the revolution in geological thinking in the late 1960s that led to the ‘theory of plate tectonics’. This collection of photographs is assembled to capture the spirit of Antarctica’s geological evolution, grouped according to the key events that have shaped the continent. A limited knowledge of geological processes and terms is required to fully appreciate this set. Conditions of use of images 1 Contributors (who retain copyright), to whom requests for reproduction should be sent, are listed after the caption by their initials. In general, reproduction of these relatively low-resolution images is permitted for educational purposes without prior permission, e.g.
    [Show full text]
  • Studies of the Geology and Mineral Resources of the Southern Antarctic Peninsula and Eastern Ellsworth Land, Antarctica
    Studies of the Geology and Mineral Resources of the Southern Antarctic Peninsula and Eastern Ellsworth Land, Antarctica U.S. GEOLOGICAL SURVEY PROFESSIONAL PAPER 1351 Work done in cooperation with the National Science Foundation ,«/*' Studies of the Geology and Mineral Resources of the Southern Antarctic Peninsula and Eastern Ellsworth Land, Antarctica PETER D. ROWLEY and WALTER R. VENNUM, Editors A. Geology of the Southern Black Coast, Antarctic Peninsula By PETER D. ROWLEY, KARL S. KELLOGG, WALTER R. VENNUM, RICHARD B. WAITT, and STEPHEN J. BOYER B. Igneous Petrology of the Merrick Mountains, Eastern Ellsworth Land, Antarctica By WALTER R. VENNUM and THOMAS S. LAUDON C. Porphyry-type Copper Deposits and Potassium-Argon Ages of Plutonic Rocks of the Orville Coast and Eastern Ellsworth Land, Antarctica By PETER D. ROWLEY, EDWARD FARRAR, PAUL E. CARRARA, WALTER R. VENNUM, and KARL S. KELLOGG U.S. GEOLOGICAL SURVEY PROFESSIONAL PAPER 1351 Work done in cooperation with the National Science Foundation UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON: 1988 DEPARTMENT OF THE INTERIOR DONALD PAUL HODEL, Secretary U.S. GEOLOGICAL SURVEY Dallas L. Peck, Director Library of Congress Cataloging-in-Publication Data Studies of the geology and mineral resources of the southern Antarctic Penninsula and eastern Ellsworth Land, Antarctica. (U.S. Geological Survey professional paper ; 1351) "Work done in cooperation with the National Science Foundation." Contents: Geology of the southern Black Coast, Antarctic Peninsula/by Peter D. Rowley .. .[et al.] Igneous petrology of the Merrick Mountains, eastern Ellsworth Land, Antarctica/by Walter R. Vennum and Thomas S. Laudon Porphyry-type copper deposits and potassium-argon ages of plutonic rocks of the Orville Coast and eastern Ellsworth Land, Antarctica/by Peter D.
    [Show full text]
  • USGS Open-File Report 2007-1047, Keynote Paper 05
    Cooper, A. K., P. J. Barrett, H. Stagg, B. Storey, E. Stump, W. Wise, and the 10th ISAES editorial team, eds. (2008). Antarctica: A Keystone in a Changing World. Proceedings of the 10th International Symposium on Antarctic Earth Sciences. Washington, DC: The National Academies Press. doi:10.3133/of2007-1047.kp05 Landscape Evolution of Antarctica S. S. R. Jamieson and D. E. Sugden1 ABSTRACT shelf before retreating to its present dimensions at ~13.5 Ma. Subsequent changes in ice extent have been forced mainly by The relative roles of fluvial versus glacial processes in shap- sea-level change. Weathering rates of exposed bedrock have ing the landscape of Antarctica have been debated since the been remarkably slow at high elevations around the margin of expeditions of Robert Scott and Ernest Shackleton in the East Antarctica under the hyperarid polar climate of the last early years of the 20th century. Here we build a synthesis of ~13.5 Ma, offering potential for a long quantitative record Antarctic landscape evolution based on the geomorphology of of ice-sheet evolution with techniques such as cosmogenic passive continental margins and former northern mid-latitude isotope analysis. Pleistocene ice sheets. What makes Antarctica so interesting is that the terrestrial landscape retains elements of a record of change that extends back to the Oligocene. Thus there is the INTRODUCTION potential to link conditions on land with those in the oceans Our aim is to synthesize ideas about the evolution of the and atmosphere as the world switched from a greenhouse terrestrial landscapes of Antarctica. There are advantages to to a glacial world and the Antarctic ice sheet evolved to its such a study.
    [Show full text]
  • Licht and Hemming 2017.Pdf
    Quaternary Science Reviews 164 (2017) 1e24 Contents lists available at ScienceDirect Quaternary Science Reviews journal homepage: www.elsevier.com/locate/quascirev Invited review Analysis of Antarctic glacigenic sediment provenance through geochemical and petrologic applications * Kathy J. Licht a, , Sidney R. Hemming b a Department of Earth Sciences, Indiana University Purdue University Indianapolis, Indianapolis, IN, USA b Department of Earth and Environmental Sciences, Columbia University, Lamont-Doherty Earth Observatory, Palisades, NY, USA article info abstract Article history: The number of provenance studies of glacigenic sediments in Antarctica has increased dramatically over Received 2 October 2016 the past decade, providing an enhanced understanding of ice sheet history and dynamics, along with the Received in revised form broader geologic history. Such data have been used to assess glacial erosion patterns at the catchment 10 February 2017 scale, flow path reconstructions over a wide range of scales, and ice sheet fluctuations indicated by Accepted 6 March 2017 iceberg rafted debris in circumantarctic glacial marine sediments. It is notable that even though most of the bedrock of the continent is ice covered and inaccessible, provenance data can provide such valuable information about Antarctic ice and can even be used to infer buried rock types along with their geo- and Keywords: Glacial geology thermochronologic history. Glacigenic sediments provide a broader array of provenance analysis op- Bedrock geology portunities than any other sediment type because of their wide range of grain sizes, and in this paper we Till review methods and examples from all size fractions that have been applied to the Antarctic glacigenic Ice-rafted debris sedimentary record.
    [Show full text]
  • Cenozoic Antarctic Climate Evolution Based on Molecular and Isotopic Biomarker Reconstructions from Geological Archives in the Ross Sea Region
    Cenozoic Antarctic climate evolution based on molecular and isotopic biomarker reconstructions from geological archives in the Ross Sea region by Bella Jane Duncan A thesis submitted to the Victoria University of Wellington in fulfilment of the requirements for the degree of Doctor of Philosophy In Geology Victoria University of Wellington 2017 Geology! the helicopter rises, the scientists crowd around, and Emily’s drill goes down through a thousand years of ice: ghost of a dog, ghost of a pony Oates going deeper and deeper Below the surface * still perfectly himself still gone for some time, lost in whatever Emily might find of sediments and algae, the movement and retreat of seasons, time passing in samples and traces -beech and conifer- stuff from the core to take home and question and even then perhaps not quite be sure… * May the years of her life look after her Emily’s gone to Antarctica From Hoosh by Bill Manhire i ii Abstract During the Cenozoic Era (the last 65 Ma), Antarctica’s climate has evolved from ice free conditions of the ‘Greenhouse world’, which at its peak (~ 55 Ma) supported near-tropical forests, to the ‘Icehouse’ climate of today with permanent ice sheets, and a very sparse macroflora. This long-term cooling trend is punctuated by a number of major, abrupt, and in some cases, irreversible climate transitions. Reconstructing past changes in vegetation, sea surface temperature, hydroclimate and the carbon cycle require robust geological proxies that in turn can provide insights into climatic thresholds and feedbacks that drove major transitions in the evolution of Antarctica’s ice sheets.
    [Show full text]
  • Heavy Mineral Composition of Surface Sediments Around the Ross Sea, Antarctica Christopher M. Agyingi*, Shuichi Tokuhashi**
    17 堆 積 学 研 究, 41号, 17-25, 1995 J.Sed. Soc. Japan, No.41, 17-25, 1995 Heavy mineral composition of surface sediments around the Ross Sea, Antarctica ChristopherM. Agyingi*, Shuichi Tokuhashi** and Akira Nishimura In this paper are shown the results of the heavy mineral analysis of ice-rafted sand fractions of undisturbed surface sediments collected from several gravity cores in and around the Ross Sea shelf area during the TH91 and TH92 Antarctic research cruises by Technology Research Center, Japan National Oil Corporation, using R/V Hakurei-maru. The areal distribution pattern of the fre- quency of each heavy mineral suggests the existence of at least two petrographic provinces, i.e. western and central-eastern areas. Especially, olivine and clinopyroxene with titanaugite, which were probably supplied from the late Quaternary McMurdo alkaline basaltic rocks fringing the eastern margin of the Victoria Land, are exclusively or dominantly distributed in the western area of the Ross Sea. This results support the northward movement of icebergs nearly parallel to the east coast of the Victoria Land at least in the western part of the Ross Sea shelf area. key words : Antarctica, Ross Sea, glacial marine sediments, heavy mineral analysis. depth (approximately 800m) and the greatest depths Introduction on the shelf occur in its landward rather than sea- Sediments and sedimentary process on the shelves ward (Chriss and Frakes ,1972) . According to around Antarctica are very different from those Anderson et al. (1984) , the deeper (greater than around other continents and are characterized more approximately 300m) portions or basin floors of the or less by the actions of ice sheets, glaciers and Ross Sea continental shelf are covered by muddy icebergs.
    [Show full text]
  • 6. Geology Resources
    Continental plate margins Resource G1 Block diagram showing FORE-ARC MAGMATIC ARC BACK ARC spreading at a mid-ocean MID-OCEAN RIDGE ridge and subduction at (spreading centre) Mainly marine sediments Lavas, volcanoes Marine & non marine a boundary between an sediments oceanic and a continental plate Plutons Continental crust Oceanic crust Subduction zone (about 40 km thick) (about 5 km thick) Mantle Mantle BAS The break-up of Gondwana Resource G2 At about 180 million years ago the Gondwana super- Map of Gondwana showing break-up dates continent began to rift apart. As the continental fragments parted, ocean crust was generated in the intervening rifts, and the new southern oceans KEY were born. 130 ages of continent-continent separation in millions of years Ocean crust is formed of basalt lava erupted at mid-ocean before present spreading centres. By successive eruptions the ocean floors Arabia spread at the rate of a few centimetres per year. This was Africa fast enough to create the present day southern oceans over a period of 150 million years or so. Africa and South America split to form the South Atlantic, and India moved India north as the Indian Ocean opened, eventually colliding with Asia. The result of this collision was massive buckling of the crust which produced the Himalayas. Different parts of Gondwana separated at different Australia South 122 times. The first rift was between Africa and Antarctica, 178-132 America where the continental rifting lasted many tens of millions East Antarctic of years. The earliest signs of the developing rift were the Shield eruption of voluminous lavas in southern Africa and Antarctica at about 180 million years ago.
    [Show full text]
  • The Evolution of the Sub-Glacial Landscape of Antarctica Stewart S.R
    Durham Research Online Deposited in DRO: 19 September 2013 Version of attached le: Accepted Version Peer-review status of attached le: Peer-reviewed Citation for published item: Jamieson, S.S.R. and Sugden, D.E. and Hulton, N.R.J. (2010) 'The evolution of the subglacial landscape of Antarctica.', Earth and planetary science letters., 293 (1-2). pp. 1-27. Further information on publisher's website: http://dx.doi.org/10.1016/j.epsl.2010.02.012 Publisher's copyright statement: NOTICE: this is the author's version of a work that was accepted for publication in Earth and planetary science letters. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reected in this document. Changes may have been made to this work since it was submitted for publication. A denitive version was subsequently published in Earth and planetary science letters, 293, 1-2, 2010,10.1016/j.epsl.2010.02.012 Additional information: Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in DRO • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full DRO policy for further details.
    [Show full text]
  • Geologie Signifieanee of Regional Magnetie Anomalies in Coats Land
    Polarforschung 67 (3): 91 - 99, 1997 (erschienen 2000) Geologie Signifieanee ofRegional Magnetie Anomalies in Coats Land and Western Dronning Maud Land By Alexander V Golynsky', Garrik E. Grikurov' and Eugene N. Kamenev' Summary: Some aspects of the Late-Proterozoic-Early Mesozoic tectonic INTRODUCTION development of western Dronning Maud Land and Coats Land are examined in this study by using aeromagnetic data. Results of our study neither contra­ dict nor support a postulated connection ofthe Kaapvaal-Zimbabwe Province Coats Land (CL) and western Dronning Maud Land (WDML) into western Droning Maud Land but certainly indicate that the Coats Land are situated in the pivotal region which lay between East crustal block has never been part of the African craton; it appears rather to be Gondwana and West Gondwana during the transition from typical of the East Antarctic Shield. Our interpretation contradicts the sug­ gestion that the Coast Land area is a continuation of the Mazatal-Yavapai­ amalgamation to Gondwana fragmentation. In the geodynamic Grenville provinces of North America. Structural relationship of magnetic context, this area has significant interest due to the recent anomalies in the neighboring terranes (Maudheim Province, Shackleton proposal of the SWEAT hypothesis (Southwest United States­ Range and Coats Land) strongly indicate the existence of an ancient cratonic fragment in Coats Land. Magnetic anomalies related to the Ross orogenie East Antarctica) which suggests that East Antarctica and event are very limited in western Dronning Maud Land and not discernible in Laurentia may have been connected in an Early Neopro­ the Shackleton Range area. This observation together with the geologie data terozoic supercontinent (MOORES 1991, DALZIEL 1991).
    [Show full text]