The Pan-African Nappe Tectonics in the Shackleton Range W
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Friedrich-Alexander Universität Erlangen-Nürnberg
Petrologische und Geochemische Untersuchungen an ultramafischen und mafischen Gesteinen der Shackleton Range, Ost-Antarktis Zeugen des Zusammenschlusses Gondwanas und letzte Relikte eines einstigen Ozeans? Der Naturwissenschaftlichen Fakultät/ Dem Fachbereich Geographie und Geowissenschaften der Friedrich-Alexander-Universität Erlangen-Nürnberg zur Erlangung des Doktorgrades Dr. rer. Nat. vorgelegt von Tanja Romer aus Illertissen i Als Dissertation genehmigt von der Naturwissenschaftlichen Fakultät/ vom Fachbereich Geographie und Geowissenschaften der Friedrich-Alexander-Universität Erlangen-Nürnberg Tag der mündlichen Prüfung: 01.06.2017 Vorsitzende/r des Promotionsorgans: Prof. Dr. Georg Kreimer Gutachter/in: Prof. Dr. Esther Schmädicke Prof. Dr. Reiner Klemd ii Zusammenfassung Im östlichen Teil der Antarktis liegt die Shackleton Range. Es handelt sich hierbei um ein Kollisionsorogen, das nach heutigen Erkenntnissen der panafrikanischen Orogenese zugeordnet wird. Hinweise darauf finden sich im nördlichen Bereich (z.B. Haskard Highlands) der Shackleton Range. Hier treten granatführende, ultramafische Gesteine als Linsen, eingeschlossen in hochgradig metamorphen Gneisen auf. Die Linsen setzen sich hauptsächlich aus granat- und/oder spinell-führenden Pyroxeniten und untergeordnet auch Peridotiten zusammen. Die nähere Umgebung der Linsen wird vor allem durch Amphibolite dominiert. Die Pyroxenite enthalten teilweise eine Verwachsung von Granat und Olivin und sind damit ein eindeutiger Indikator für eine eklogitfazielle Metamorphose in diesem Bereich. Weiterhin zeugen sie als ultramafische Gesteine von einer möglichen Suturzone. In dieser Forschungsarbeit konnte mittels Mikrosondenanalytik an Granat, Ortho- und Klinopyroxen, Spinell, Olivin und Amphibol für die ultramafischen Gesteine ein Teil des im Uhrzeigersinn verlaufenden P-T-Pfads rekonstruiert werden. Thermobarometrische Berechnungen ergaben maximale Metamorphosetemperaturen von 800 bis 850 °C. Die maximal erreichten Drücke dürften zwischen 20 bis 23 kbar gelegen haben. -
Petrogenesis of the Metasediments from the Pioneers Escarpment, Shackleton Range, Antarctica
Polarforschung 63 (2/3): 165-182,1993 (erschienen 1995) Petrogenesis of the Metasediments from the Pioneers Escarpment, Shackleton Range, Antarctica By Norbcrt W. Roland', Martin Olcsch2 and Wolfgang Schubert' Summary: During the GEISHA expedition (Geologische Expedition in die during apre-Ross metarnorphic event or orogeny. The Ross Orogeny at about Shackleton Range 1987/88), the Pioneers Escarpment was visited and sampled 500 Ma probably just led to the weak greensehrst facies overprint that is evi extensively for the first time. Most of the rock types eneountered represent dent in the rocks of the Pioneers Group. amphibolite faeies metamorphics, but evidence for granulite facies conditions was found in cores of garnet. These conelitions must have been at least partly Finally, sedimentation resumed in the area of the present Shacklcton Range, or reached during the peak of metamorphism. at least in the eastern part of the Pioneers Escarpment, probably when detritus from erosion of the basement (Read Group and Pioneers Group) was deposi For the Pioneers Escarpment a varicolored succession of sedimentary anel bi ted, forming sandstones and greywackes of possibly Jurassie age. There is no modal volcanic origin is typical. It comprises: indication that these sediments belong to the former Turnpike Bluff Group. quartzites muscovite quartzite, sericite quartzite, fuchsite quartzite, garnet quartz schists etc.; Zusammenfassung: Während GEISHA (Geologische Expedition in die Shack pelites: mica schists and plagiocJase 01' plagioclase-microcline gneisses, alu leton Range 1987/88) wurde erstmals das Pioneers Escarpment der Shackleton minous schists; Range intensiver beprobt. Es treten Überwiegend Metamorphire der Amphibo marls and carbonates: grey meta-limestones, carbonaceous guartzites, but also litfazies auf. -
The Stratigraphy of the Ohio Range, Antarctica
This dissertation has been 65—1200 microfilmed exactly as received LONG, William Ellis, 1930- THE STRATIGRAPHY OF THE OHIO RANGE, ANTARCTICA. The Ohio State University, Ph.D., 1964 G eology University Microfilms, Inc., Ann Arbor, Michigan THE STRATIGRAPHY OF THE OHIO RANGE, ANTARCTICA DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By William Ellis Long, B.S., Rl.S. The Ohio State University 1964 Approved by A (Miser Department of Geology PLEASE NOTE: Figure pages are not original copy* ' They tend tc "curl11. Filled in the best way possible. University Microfilms, Inc. Frontispiece. The Ohio Range, Antarctica as seen from the summit of ITIt. Glossopteris. The cliffs of the northern escarpment include Schulthess Buttress and Darling Ridge. The flat area above the cliffs is the Buckeye Table. ACKNOWLEDGMENTS The preparation of this paper is aided by the supervision and advice of Dr. R. P. Goldthwait and Dr. J. M. Schopf. Dr. 5. B. Treves provided petrographic advice and Dir. G. A. Doumani provided information con cerning the invertebrate fossils. Invaluable assistance in the fiBld was provided by Mr. L. L. Lackey, Mr. M. D. Higgins, Mr. J. Ricker, and Mr. C. Skinner. Funds for this study were made available by the Office of Antarctic Programs of the National Science Foundation (NSF grants G-13590 and G-17216). The Ohio State Univer sity Research Foundation and Institute of Polar Studies administered the project (OSURF Projects 1132 and 1258). Logistic support in Antarctica was provided by the United States Navy, especially Air Development Squadron VX6. -
The Shackleton Range of East Antarctica
General Information Project Title: The Shackleton Range of East Antarctica: unravelling a complex geological history via an integrated geochronological, geochemical and geophysical approach Lead Institution: BAS Department / School / Institute Geology & Geophysics CASE Partner Organisations CASP, West Building, Madingley Road, [OPTIONAL] Cambridge, CB3 0UD. Leave blank if not applicable End-user Collaborations [OPTIONAL] Leave blank if not applicable Project Team The first supervisor should be from the lead institution. The Second Supervisor should be from a second IAPETUS2 organisation Supervisor 1 Name Dr Teal Riley Organisation BAS Email [email protected] Biography URL https://WWW.bas.ac.uk/profile/trr/ Supervisor 2 Name Dr Nick Gardiner Organisation University of St Andrews Email [email protected] Biography URL https://WWW.st-andrews.ac.uk/earth- sciences/people/njg7 Supervisor 3 (if applicable) Name Dr Fausto Ferraccioli Organisation BAS Email [email protected] Biography URL https://WWW.bas.ac.uk/profile/ffe/ Supervisor 4 (if applicable) Name Organisation Choose an item. Email Biography URL Supervisor 5 (if applicable) Name Organisation Choose an item. Email Biography URL CASE Partners If applicable, add any CASE Partners here Name [optional] Dr Michael FlowerdeW Organisation CASP Email [email protected] Biography URL https://casp.org.uk/people/michael-floWerdeW End-user Collaborations If applicable, add any End-user Collaborations here Name [optional] Organisation Email Biography URL In Collaboration with Add any non-IAPETUS University collaboration partners here. [OPTIONAL] Leave blank if not applicable Name Organisation Email Biography URL Project Details The information provided here will be used to create the project advertisement online and in pdf format. -
Depositional History of Pre-Devonian Strata and Timing of Ross Orogenic Tectonism in the Central Transantarctic Mountains, Antarctica
Depositional history of pre-Devonian strata and timing of Ross orogenic tectonism in the central Transantarctic Mountains, Antarctica Paul M. Myrow* Department of Geology, Colorado College, Colorado Springs, Colorado 80903, USA Michael C. Pope Department of Geology, Washington State University, Pullman, Washington 99164, USA John W. Goodge Department of Geological Sciences, Southern Methodist University, Dallas, Texas 75275, USA Woodward Fischer Department of Geology, Colorado College, Colorado Springs, Colorado 80903, USA Alison R. Palmer Institute for Cambrian Studies, 445 North Cedarbrook Road, Boulder, Colorado 80304-0417, USA ABSTRACT small fraction of its previous extent. The into trilobite- and hyolithid-bearing calcar- basal unit of the Byrd GroupÐthe predom- eous siltstone of the Starshot Formation A combination of ®eld mapping, detailed inantly carbonate ramp deposits of the and alluvial-fan deposits of the Douglas sedimentology, carbon isotope chemostra- Shackleton LimestoneÐrest with presumed Conglomerate. Trilobite fauna from the tigraphy, and new paleontological ®nds unconformity on the restricted Goldie For- lowermost siltstone deposits of the Starshot provides a signi®cantly improved under- mation. Paleontological data and carbon Formation date the onset of this transition standing of the depositional and tectonic isotope stratigraphy indicate that the Low- as being late Botomian. history of uppermost Neoproterozoic and er Cambrian Shackleton Limestone ranges The abrupt transition from the Shackle- lower Paleozoic strata of the central Trans- from lower Atdabanian through upper ton Limestone to a large-scale, upward- antarctic Mountains. On the basis of these Botomian. coarsening siliciclastic succession records data, we suggest revision of the existing This study presents the ®rst description deepening of the outer platform and then stratigraphy, including introduction of new of a depositional contact between the deposition of an eastward-prograding mo- formations, as follows. -
CURRICULUM VITAE 10 August 2015
IAN W. D. DALZIEL B.SC., PH.D., D.SC. (Hon), FRSE CURRICULUM VITAE 10 August 2015 PERSONAL ..................................................................................................................................................... 1 EDUCATION ................................................................................................................................................... 1 AWARDS AND DISTINCTIONS ........................................................................................................................ 1 ACADEMIC POSITIONS ................................................................................................................................... 1 ADMINISTRATIVE POSITIONS ........................................................................................................................ 2 MAIN FIELDS OF RESEARCH INTEREST ......................................................................................................... 2 ELECTIONS TO FELLOWSHIP .......................................................................................................................... 2 EDITORIAL RESPONSIBILITIES ....................................................................................................................... 2 LEADERSHIP OF MAJOR INTERNATIONAL RESEARCH PROJECTS .................................................................. 2 CONVENER, INTERNATIONAL WORKSHOPS AND CONFERENCES ................................................................. 2 PROFESSORSHIPS, LECTURESHIPS, AND -
Clastos Con Calcimicrobios Y Arqueociatos Procedentes De
Estudios Geológicos julio-diciembre 2019, 75(2), e112 ISSN-L: 0367-0449 https://doi.org/10.3989/egeol.43586.567 Calcimicrobial-archaeocyath-bearing clasts from marine slope deposits of the Cambrian Mount Wegener Formation, Coats Land, Shackleton Range, Antarctica Clastos con calcimicrobios y arqueociatos procedentes de depósitos marinos del talud de la Formación cámbrica del Monte Wegener, Coats Land, Cordillera de Shackleton Antártida M. Rodríguez-Martínez1, A. Perejón1, E. Moreno-Eiris1, S. Menéndez2, W. Buggisch3 1Universidad Complutense de Madrid, Departamento de Geodinámica, Estratigrafía y Paleontología, Madrid, Spain. Email: [email protected], [email protected], [email protected]; ORCID ID: http://orcid.org/0000-0002-4363-5562, http://orcid.org/0000-0002-6552-0416, http://orcid.org/0000-0003-2250-4093 2Museo Geominero, Instituto Geológico y Minero de España (IGME), Ríos Rosas, 23, 28003 Madrid, Spain. Email: [email protected]; ORCID ID: Silvia Menéndez: http://orcid.org/0000-0001-6074-9601 3GeoZentrum Nordbayern. Friedrich-Alexander-University of Erlangen-Nürnberg (FAU). Schlossgarten 5, 91054 Erlangen, Germany. ABSTRACT The carbonate clasts from the Mount Wegener Formation provide sedimentological, diagenetic and palaeonto- logical evidences of the destruction and resedimentation of a hidden/unknown Cambrian carbonate shallow-water record at the Coats Land region of Antarctica. This incomplete mosaic could play a key role in comparisons and biostratigraphic correlations between the Cambrian record of the Transantarctic Mountains, Ellsworth-Whitmore block and Antarctic Peninsula at the Antarctica continent. Moreover, it represents a key record in future palaeobio- geographic reconstructions of South Gondwana based on archaeocyathan assemblages. Keywords: Calcimicrobes; Archaeocyaths; Shackleton Range; Antarctica; Gondwana. -
Emergence of the Shackleton Range from Beneath the Antarctic
Edinburgh Research Explorer Emergence of the Shackleton Range from beneath the Antarctic Ice Sheet due to glacial erosion Citation for published version: Sugden, D, Fogwill, CJ, Hein, AS, Stuart, FM, Kerr, AR & Kubik, PW 2014, 'Emergence of the Shackleton Range from beneath the Antarctic Ice Sheet due to glacial erosion', Geomorphology, pp. 1-22. https://doi.org/10.1016/j.geomorph.2013.12.004 Digital Object Identifier (DOI): 10.1016/j.geomorph.2013.12.004 Link: Link to publication record in Edinburgh Research Explorer Document Version: Peer reviewed version Published In: Geomorphology General rights Copyright for the publications made accessible via the Edinburgh Research Explorer is retained by the author(s) and / or other copyright owners and it is a condition of accessing these publications that users recognise and abide by the legal requirements associated with these rights. Take down policy The University of Edinburgh has made every reasonable effort to ensure that Edinburgh Research Explorer content complies with UK legislation. If you believe that the public display of this file breaches copyright please contact [email protected] providing details, and we will remove access to the work immediately and investigate your claim. Download date: 01. Oct. 2021 NOTICE: this is the author's final version of a work that was accepted for publication in Geomorphology. Changes resulting from the publishing process, such as editing, corrections and structural formatting may not be reflected in this document. A definitive version of this document is due to be published in Geomorphology by Elsevier (2014). Emergence of the Shackleton Range from beneath the Antarctic Ice Sheet due to glacial erosion a b a c a d D.E. -
Shackleton Range Traverse Lock Back for This Work
Shackleton Range Traverse lock back for this work. Along with another surveyor, Tony True, he flew via Washington, D.C. and Christ- church to McMurdo Sound, where they awaited fa- SIR VIVIAN FUCHS vorable weather for the flight across the continent. On November 23, their LC-130 landed at Halley Bay, British Antarctic Survey where two geologists, two assistants, and 27 dogs, to- gether with 10,000 lbs of supplies and equipment, The Shackleton Range was discovered by the Com- were loaded and the plane refuelled. monwealth Trans-Antarctic Expedition in February When the aircraft reached the Shackletons, only a 1956. The mountains extend for about 100 miles few peaks were visible through low cloud cover, which along an east-west axis between latitudes 80°S. and made it impossible to locate the Stratton Glacier 81°S. The highest peak is just 6,000 feet. In 1957, where it was intended to land the party. After circling surveyors David Stratton and Kenneth Blaikiock the mountains for an hour, the pilot saw a small gap made a &osed traverse by dog sledge, tied to astro- in the clouds to the south of the range and was able to fixes, through the western part of the range. make a skillful but very bumpy landing on the sastru- In recent years, the British Antarctic Survey has gi-cut surface of the great, 40-mile wide Recovery succeeded in reaching these mountains on the ground Glacier. At this time, the precise position was un- from Halley Bay, although it entailed a round trip of known, but the plane was quickly unloaded and took over 1,000 miles for the tractors and (log teams, which off for McMurclo in thick clouds. -
Constraints on Early Paleozoic Magmatic Processes and Tectonic Setting of Inexpressible Island, Northern Victoria Land, Antarctica
• Article • Advances in Polar Science doi: 10.13679/j.advps.2019.1.00052 March 2019 Vol. 30 No. 1: 52-69 Constraints on early Paleozoic magmatic processes and tectonic setting of Inexpressible Island, Northern Victoria Land, Antarctica CHEN Hong1,2*, WANG Wei1,2 & ZHAO Yue1,2 1 Institute of Geomechanics, Chinese Academy of Geological Sciences, Beijing 100081, China; 2 Key Laboratory of Paleomagnetism and Tectonic Reconstruction of Ministry of Natural Resources, Beijing 100081, China Received 2 May 2018; accepted 12 February 2019 Abstract During the Cambrian and Ordovician, widespread magmatic activity occurred in the Ross Orogen of central Antarctica, forming the Granite Harbor Intrusives and Terra Nova Intrusive Complex. In the Terra Nova Intrusive Complex, the latest magmatic activity comprised the emplacement of the Abbott Unit (508 Ma) and the Vegetation Unit (~475 Ma), which were formed in different tectonic settings. Owing to their similar lithological features, the tectonic transformation that occurred between the formation of these two units has not been well studied. Through a detailed geological field investigation and geochemical and geochronological analyses, four types of magmatic rock—basalt, syenite, mafic veins, and granite veins—were identified on Inexpressible Island, Northern Victoria Land. Our SHRIMP (Sensitive High Resolution Ion Micro Probe) zircon U–Pb ages of the basalt and the granite veins are 504.7 ± 3.1 and 495.5 ± 4.9 Ma, respectively. Major- and trace-element data indicate a continental-margin island-arc setting for the formation of these two rock types. The zircon U–Pb ages of the syenite and the monzodiorite veins are 485.8 ± 5.7 and 478.5 ± 4.0 Ma, respectively. -
Tectonic Model for Development of the Byrd Glacier Discontinuity and Surrounding Regions of the Transantarctic Mountains During the Neoproterozoic – Early Paleozoic
Published in: Fütterer, D K, Damaske, D, Kleinschmidt, G, Miller, H & Tessensohn, F (eds.), Antarctica: contributions to global earth sciences, Springer, Berlin, Heidelberg, New York, 45-54 http://dx.doi.org/10.1007/3-540-32934-X The original publication is available at http://www.springerlink.com see http://dx.doi.org/10.1007/3-540-32934-X_22 Data are available at: http://dx.doi.org/10.1594/PANGAEA.611703 Tectonic Model for Development of the Byrd Glacier Discontinuity and Surrounding Regions of the Transantarctic Mountains during the Neoproterozoic – Early Paleozoic Edmund Stump1 · Brian Gootee1 · Franco Talarico2 1 Department of Geological Sciences, Arizona State University, Tempe, Arizona AZ 85287-1404, USA 2 Dipartimento di Scienze della Terra, Università di Siena, Via del Laterino 8, 53100 Siena, Italy Abstract. The Byrd Glacier discontinuity is a major tectonic boundary crossing the Ross Orogen, with crystalline rocks to the north and primarily sedimentary rocks to the south. Most models for the tectonic development of the Ross Orogen in the central Transantarctic Mountains consist of two-dimensional transects across the belt, but do not address the major longitudinal contrast at Byrd Glacier. This paper presents a tectonic model centering on the Byrd Glacier discontinuity. Rifting in the Neoproterozoic produced a crustal promontory in the craton margin to the north of Byrd Glacier. Oblique convergence of a terrane (Beardmore microcontinent) during the latest Neoproterozoic and Early Cambrian was accompanied by subduction along the craton margin of East Antarctica. New data presented herein in support of this hypothesis are U-Pb dates of 545.7 ±6.8 Ma and 531.0 ±7.5 Ma on plutonic rocks from the Britannia Range, directly north of Byrd Glacier. -
ARCHIVED-CARN Vol 24, Nov 2007 [PDF-2.77
Vol 24, November 2007 NEWSLETTER FOR THE Canadian Antarctic Research Network Inside Measuring Crustal Motion in Antarctica: Measuring Crustal Motion GPS, Tectonics, and Glacio-isostatic Adjustment in Antarctica: Thomas James GPS, Tectonics, and Glacio-isostatic Adjustment 1 For five weeks in early 2006, I joined the U.S. National Science Foundation’s (NSF) field team of the Transantarctic Mountain Deformation (TAMDEF) pro- RUGBY ject (www.geology.ohio-state.edu/tamdef/) measuring crustal motion in the (Research on Ultraviolet and Global warming effects Transantarctic Mountains near McMurdo Station (Fig. 1). My initial involvement on Biological pump Yields) 8 in this was as a modeller of the crustal motions expected from past and present changes in the Antarctic ice sheet. By observing and modelling these motions, Canadians in Antarctic known as glacio-isostatic adjustment (GIA), we learn about the structure and Place-Names: properties of the Earth beneath the TAMDEF region, and may possibly discern Supplement 13 new features of the ice-sheet history. In turn, well-constrained GIA models allow better interpretation of remote-sensing data to determine the mass balance of Protocol for Canada–Argentina ice sheets and the contribution that ice sheets make to sea-level change. Collaboration 16 The Transantarctic Mountains are adjacent to the West Antarctic Rift Sys- tem, a broad zone which has experienced significant extension in the past. When Canadian Involvement TAMDEF started, an issue in global tectonics was whether West Antarctica and in Antarctic Tourism Research: East Antarctica were moving relative to one another, or whether the continent an update on some moves as a relatively rigid block.