Physical Properties of Shallow Ice Cores from Antarctic and Sub-Antarctic Islands
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Late Quaternary Volcanic Activity in Marie Byrd Land: Potential 40Ar/39Ar-Dated Time Horizons in West Antarctic Ice and Marine Cores
Late Quaternary volcanic activity in Marie Byrd Land: Potential 40Ar/39Ar-dated time horizons in West Antarctic ice and marine cores T. I. Wilch* Department of Geological Sciences, Albion College, Albion, Michigan 49224 W. C. McIntosh Department of Earth and Environmental Science, New Mexico Institute of Mining and Technology, and New Mexico Bureau of Mines and Mineral Resources, Socorro, New Mexico 87801 N. W. Dunbar New Mexico Bureau of Mines and Mineral Resources, Socorro, New Mexico 87801 ABSTRACT More than 12 40Ar/39Ar-dated tephra lay- ies is to determine the basal age of the ice sheet. ers, exposed in bare ice on the summit ice cap The 1968 Byrd Station ice core in the West Late Quaternary volcanic activity at three of Mount Moulton, 30 km from their inferred Antarctic Ice Sheet has an inferred basal age of major alkaline composite volcanoes in Marie source at Mount Berlin, range in age from 492 only 74 ka (Hammer et al., 1994). The exten- Byrd Land, West Antarctica, is dominated by to 15 ka. These englacial tephra layers provide sive lateral flow of ice from the ice divide area explosive eruptions, many capable of deposit- a minimum age of 492 ka for the oldest iso- to Byrd Station may have removed or disturbed ing ash layers as regional time-stratigraphic topically dated ice in West Antarctica. This much of the basal ice record. Consequently, the horizons in the West Antarctic Ice Sheet and well-dated section of locally derived glacial ice 74 ka date of the Byrd core provides only a in Southern Ocean marine sediments. -
Volcanoes at Antarctica
ClimateChangeTheFacts.org.au FACT SHEET #4 FIRE AND ICE: VOLCANOES AT ANTARCTICA HOT TAKES Figure 1: Volcanoes of West Antarctica3 1 At West Antarctica, 91 newly discovered volcanoes lie buried kilometres beneath a thick ice sheet. Ronne-Filchner Ice Shelf 2 The ice sheet has co-existed with volcanism for millions 0 of years. 90 W Ellsworth Whitmore South Pole 3 Future volcanism is inevitable but fears it would Land Mountains destabilise the ice sheet and accelerate sea-level rise Mount Takahe are unfounded. Transantarctic Mount Sidley Mountains 135 Mount Cumming 0 E Marie Many people are concerned the (slight) global warming Amundsen Sea Byrd observed over the past 100 years is unnatural and caused Land 80 0 Mount Siple S Ross Ice Shelf by human activity. Some also believe this will accelerate melting of ice sheets and glaciers and cause rapid 0 W Mount Erebus catastrophic sea level rise. However this conclusion is 135 Ross Sea dependent on complex computer models containing many W 0 untested assumptions. A great many of the assumptions the 70 0 1000 km S models need to get right before they are of any use are only 180 very poorly understood. Visible volcanoes Volcanoes hidden beneath ice Some environmentalists believe volcanoes associated with the Not even the large inland volcanoes protruding through the West Antarctic Ice Sheet (WAIS) could magnify the ‘climate WAIS were known to exist before 1940 when first seen from change’ risk to the ice sheet. However close examination of the air. Mount Takahe is so remote it was not visited until the relationship between the volcanoes and the ice shows this 1957. -
Mineral Resources of Antarctica
GEOLOGICAL SURVEY CIRCULAR 705 Mineral Resources of Antarctica Mineral Resources of Antarctica Compiled ancl eclitecl &y N. A. Wright ancl P. L. Williams GEOLOGICAL SURVEY CIRCULAR 705 1974 United States Department of the Interior ROGERS C. B. MORTON, Secretary Geological Survey V. E. McKelvey, Director Free on application to the U.S. Geological Survey, National Center, Reston, Va. 22092 CONTENTS Page )Lbstract ---------------------------------------------------------------- 1 Introduction ------------------------------------------------------------ 1 ldineral occurrences ------------------------------------------------------ 3 Sand and gravel ---------------------------------------------------- 3 Other nonmetals ---------------------------------------------------- 3 Iron ---------------------------------------------------------------- 10 Copper --------_____ -.- ____ - __ - _________ - ___ - ___ - --__ ----------------- 11 Gold and silver ------------------------------------------------------ 11 ldolybdenum ___________________________________ ---_ -~- --------------- 11 Other metals -------------------------------------------------------- 11 Potential resources _--- _-_________ - ________ - ____ ---_----__ ---------------- 11 ldanganese nodules _____________________________ ---____ --------------- 11 Geothermal energy --------------------------------------------------- 12 VVater (as ice) ------------------------------------------------------ 15 Coal ---------------------------------------------------------------- 15 Oil and natural gas -
US Geological Survey Scientific Activities in the Exploration of Antarctica: 1946–2006 Record of Personnel in Antarctica and Their Postal Cachets: US Navy (1946–48, 1954–60), International
Prepared in cooperation with United States Antarctic Program, National Science Foundation U.S. Geological Survey Scientific Activities in the Exploration of Antarctica: 1946–2006 Record of Personnel in Antarctica and their Postal Cachets: U.S. Navy (1946–48, 1954–60), International Geophysical Year (1957–58), and USGS (1960–2006) By Tony K. Meunier Richard S. Williams, Jr., and Jane G. Ferrigno, Editors Open-File Report 2006–1116 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior DIRK KEMPTHORNE, Secretary U.S. Geological Survey Mark D. Myers, Director U.S. Geological Survey, Reston, Virginia 2007 For product and ordering information: World Wide Web: http://www.usgs.gov/pubprod Telephone: 1-888-ASK-USGS For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment: World Wide Web: http://www.usgs.gov Telephone: 1-888-ASK-USGS Although this report is in the public domain, permission must be secured from the individual copyright owners to reproduce any copyrighted material contained within this report. Cover: 2006 postal cachet commemorating sixty years of USGS scientific innovation in Antarctica (designed by Kenneth W. Murphy and Tony K. Meunier, art work by Kenneth W. Murphy). ii Table of Contents Introduction......................................................................................................................................................................1 Selected.References.........................................................................................................................................................2 -
Mount Siple Volcano, Marie Byrd Land (<\C:)
assessment of Gondwana reconstructions. Earth and Planetary Science Cambrian volcanics of the Bowers Supergroup and implications for Letters, 57, 152-158. the Early Paleozoic tectonic evolution of northern Victoria Land, Weaver, S.D., J.D. Bradshaw, and M.G. Laird. 1984. Geochemistry of Antarctica. Earth and Planetary Science Letters, 68, 128-140. Mount Siple volcano, Marie Byrd Land USCGC Polar Sea. The initial landing was made at Lovill Bluff (figure 1) by helicopter, piloted by LCDR Rick McLean and crewed by AM2 Robert OConner. The scientific party included Pamela Ellerman (on her birthday), David Johnson, William W. E. LEMASURIER McIntosh, and me. We spent a full day visiting Lovill Bluff and two other western flank localities before steaming north to the Geology Department vicinity of Maher Island (figure 1). Because of poor weather University of Colorado at Denver conditions, we were forced to examine the northern flank ex- Denver, Colorado 80202 posures with binoculars over the next 4 days and finally left the area on the morning of 27 February to maintain the ships Mount Siple, one of the largest volcanoes in Antarctica, was schedule. A very useful series of close-up photographs along visited for the first time on 22 February 1984 during cruise II of the north flank of the volcano was taken by Seaman A.R. Sul- Limit of fast ice - Maher (February 1965) Island - 125000W 126° 1280 (<\c:) 73°00S -1-- Lauff I Island Burtis C_; C^l \ 0 Island I ri?- 0 Cape Dart Recely Bluff MOUNT SIPLE 3110 I KEY Possible source Trachyte Lovill of felsic beach U° C— — .- cobbles ¼ Bluff ._® c. -
The Antarctican Society 905 North Jacksonville Street Arlington, Virginia 22205
THE ANTARCTICAN SOCIETY 905 NORTH JACKSONVILLE STREET ARLINGTON, VIRGINIA 22205 HONORARY PRESIDENT — AMBASSADOR PAUL C. DANIELS __________________________________________________________ Presidents: Dr. Carl R. Eklund, 1959-61 Vol. 83-84 March No. 5 Dr. Paul A. Siple, 1961-2 Mr. Gordon D. Cartwright. 1962-3 RADM David M. Tyree (Ret.), 1963-4 Mr. George R. Toney, 1964-5 WELCOME SPRING Mr. Morton J. Rubin, 1965-6 with Dr. Albert P. Crary, 1966-8 Dr. Henry M. Dater, 1968-70 Mr. George A. Doumani, 1970-1 WHALE WATCHING IN THE ANTARCTIC Dr. William J. L Sladen, 1971-3 by Mr. Peter F. Bermel, 1973-5 Dr. Kenneth J. Bertrand, 1975-7 Dr. William E. Evans Mrs. Paul A. Siple, 1977-8 Director Dr. Paul C Dalrymple, 1978-80 Dr. Meredith F. Burrill, 1980-82 Hubbs-Sea World Research Institute Dr. Mort D. Turner, 1982-84 San Diego, California on Honorary Members: Tuesday, 20 March 1984 Ambassador Paul C. Daniels Dr. Laurence McKinley Gould Count Emilio Pucci 8 PM Sir Charles S. Wright Mr. Hugh Blackwell Evans National Science Foundation Dr. Henry M. Dater Mr. August Howard 18th and G Streets NW Room 543 - Light Refreshments - Memorial Lecturers: Dr. William J. L Sladen, 1964 RADM David M. Tyree (Ret.), 1965 Dr. Roger Tory Peterson, 1966 Dr. J. Campbell Craddock, 1967 Mr. James Pranke, 1968 Dr. Henry M. Dater, 1970 Dr. William Evans is dedicated to understanding the interaction of man Sir Peter M. Scott, 1971 Dr. Frank T. Davies, 1972 and the marine environment. The White House announced on 15 November Mr. Scott McVay, 1973 1983 the intention of the President to nominate Dr. -
Print Cruise Information
The Ross Sea From 2/16/2022 From Ushuaia Ship: LE COMMANDANT CHARCOT to 3/12/2022 to Ushuaia Sailing the Ross Sea means discovering one of the most extreme and conserved universes in the Antarctic. Partially occupied by the Ross Ice Shelf, the largest ice platform in Antarctica , this immense bay located several hundred kilometres from theSouth Pole, is considered as the“ last ocean”, the last intact marine ecosystem and the largest marine sanctuary since 2016. Here, the cold is more intense, the wind more powerful, the ice more impressive, and the scenery more spectacular… In the heart of this polar Garden of Eden, where the ice shelf turns into icebergs, you will encounter prodigious fauna, as well assurrealist landscapes, with infinite shades of blue and stunning reliefs. Antarctic petrels, Minke whales, orcas and seals are at home here, as are very large Overnight in Santiago + flight Santiago/Ushuaia + transfers + flight Ushuaia/Santiago colonies of Adelie and emperor penguins. We are privileged guests in these extreme lands where we are at the mercy of weather and ice conditions. Our navigation will be determined by the type of ice we come across; as the coastal ice must be preserved, we will take this factor into account from day to day in our itineraries. The sailing schedule and any landings, activities and wildlife encounters are subject to weather and ice conditions. These experiences are unique and vary with each departure. The Captain and the Expedition Leader will make every effort to ensure that your experience is as rich as possible, while respecting safety instructions and regulations imposed by the IAATO. -
Discovery of the First Emperor Penguin Aptenodytes Forsteri Colony in Marie Byrd Land, Antarctica
Short Communications 59 DISCOVERY OF THE FIRST EMPEROR PENGUIN APTENODYTES FORSTERI COLONY IN MARIE BYRD LAND, ANTARCTICA MARY-ANNE LEA1 & TIM SOPER2 1 Antarctic Wildlife Research Unit, School of Zoology, University of Tasmania, PO Box 252-05, Hobart, Tasmania, 7001, Australia ([email protected]) 2 Gerston Point, Kingsbridge, Devon, TQ7 3BA, UK Received 22 August 2005, accepted 31 October 2005 Emperor Penguins Aptenodytes forsteri have been reported to area marks the eastern extent of the Wrigley Shelf Polynya (Arrigo breed at a total of 45 colonies surrounding the Antarctic Continent & van Dijken 2003), a region characterized by maximum annual (Woehler 1993, Mellick & Bremers 1995, Coria & Montalti 2000, primary production in December/January, coinciding with fledging Todd et al. 2004). Their known breeding distribution extends from of Emperor Penguin chicks. The habitat is similar to that found the Antarctic Peninsula at Snow Hill Island (64°31′S, 57°27′W) Emperor Penguin colonies in the Ross Sea, characterized by stable eastwards along the coasts of Dronning Maud Land, Enderby fast ice, nearby open water, access to fresh snow and shelter from Land, Mac. Robertson Land and Wilkes Land to Cape Crozier on wind (Kooyman 1990). Fast ice extent is variable from year to year Ross Island (77°31′S, 169°23′E). Sightings of Emperor Penguins in this region (Swithinbank et al. 2003) and may have influenced in rarely-visited Marie Byrd Land have been reported, although previous locations of the colony. Approximately 100 adult Emperor no colonies have ever been recorded in the sector between the Penguins, in groups of 10–25 individuals, were also sighted Dion Islands (67°52′S, 68°43′W) in Marguerite Bay on the west travelling northwards to the ice edge. -
Graduate Course in Antarctic Studies 2004-2005 Student
Graduate Course in Antarctic Studies 2004-2005 Student: Lucia Sala Simian Christchurch , January 1Oth, 2005 LITERATURE REVIEW (Anta 502) The volcanoes of Marie Byrd Land and their importance in understanding the tectonics of West Antarctica as well as the reconstruction of the West Antarctic ice sheet (WAfS) in the last interglacial. Marie Byrd Land (MBL, longitude 100-150° W) is one of the least accessible and least frequently visited regions in Antarctica (Fig. 1, 2). It was discovered from the air and claimed for the United States by Richard E. Byrd in 1929, and named for his wife. Much of this region was then explored during the second Byrd expedition (1934-35) by two tractor parties, one sled party led by Paul Siple and four exploratory flights. The US Antarctic Service Expedition explored the region in 1939-41, as well as the Executive Committee Range Traverse in 1959, with oversnow tracked vehicles from Byrd Station. More recently, US scientists mapped, sampled and collected GPS data, as well as drilled snow and ice cores on the summit of some of the volcanoes. Marie Byrd Land contains the largest volcanic region of Antarctica and one of the largest in the world, covering a lenght of almost 960 Km along the Pacific coast. The West Antarctic Ice Sheet (WAIS) covers most of the region, with a thickness exceeding 4.000 m in some areas. Protruding up through the vast expanse of ice are 18 large central volcanoes, including Mount Sidley (4.181 m, the highest volcano in Antarctica, Fig. 3) and more than 30 small satellitic volcanic centers. -
Clay Mineral Assemblage Evidence WERNER EHRMANN1, CLAUS-DIETER HILLENBRAND2, JAMES A
Antarctic Science 23(5), 471–486 (2011) & Antarctic Science Ltd 2011 doi:10.1017/S0954102011000320 Provenance changes between recent and glacial-time sediments in the Amundsen Sea embayment, West Antarctica: clay mineral assemblage evidence WERNER EHRMANN1, CLAUS-DIETER HILLENBRAND2, JAMES A. SMITH2, ALASTAIR G.C. GRAHAM2, GERHARD KUHN3 and ROBERT D. LARTER2 1University of Leipzig, Institute of Geophysics and Geology, Talstraße 35, D-04103 Leipzig, Germany 2British Antarctic Survey, NERC, High Cross, Madingley Road, Cambridge CB3 0ET, UK 3Alfred Wegener Institute for Polar and Marine Research, Am Alten Hafen 26, D-27568 Bremerhaven, Germany [email protected] Abstract: The Amundsen Sea embayment is a probable site for the initiation of a future collapse of the West Antarctic Ice Sheet. This paper contributes to a better understanding of the transport pathways of subglacial sediments into this embayment at present and during the last glacial period. It discusses the clay mineral composition of sediment samples taken from the seafloor surface and marine cores in order to decipher spatial and temporal changes in the sediment provenance. The most striking feature in the present- day clay mineral distribution is the high concentration of kaolinite, which is mainly supplied by the Thwaites Glacier system and indicates the presence of hitherto unknown kaolinite-bearing sedimentary strata in the hinterland, probably in the Byrd Subglacial Basin. The main illite input is via the Pine Island Glacier. Smectite originates from the erosion of volcanic rocks in Ellsworth Land and western Marie Byrd Land. The clay mineral assemblages in diamictons deposited during the last glacial period are distinctly different from those in corresponding surface sediments. -
Important Bird Areas in Antarctica 2015. Birdlife International and Environmental Research & Assessment Ltd., Cambridge
Important Bird Areas in Antarctica 2015 Important Bird Areas in Antarctica 2015 Harris, C.M., Lorenz, K., Fishpool, L.D.C., Lascelles, B., Cooper, J., Coria, N.R., Croxall, J.P., Emmerson, L.M., Fraser, W.R., Fijn, R.C., Jouventin, P., LaRue, M.A., Le Maho, Y., Lynch, H.J., Naveen, R., Patterson-Fraser, D.L., Peter, H.-U., Poncet, S., Phillips, R.A., Southwell, C.J., van Franeker, J.A., Weimerskirch, H., Wienecke, B., & Woehler, E.J. June 2015 Important Bird Areas in Antarctica 2015 Citation Harris, C.M., Lorenz, K., Fishpool, L.D.C., Lascelles, B., Cooper, J., Coria, N.R., Croxall, J.P., Emmerson, L.M., Fijn, R.C., Fraser, W.L., Jouventin, P., LaRue, M.A., Le Maho, Y., Lynch, H.J., Naveen, R., Patterson-Fraser, D.L., Peter, H.-U., Poncet, S., Phillips, R.A., Southwell, C.J., van Franeker, J.A., Weimerskirch, H., Wienecke, B., & Woehler, E.J. 2015. Important Bird Areas in Antarctica 2015. BirdLife International and Environmental Research & Assessment Ltd., Cambridge. Cover photograph Adélie Penguin colony at Seabee Hook, Cape Hallett, Important Bird Area (IBA) ANT170 and Antarctic Specially Protected Area (ASPA) No.106. © era-images C. Harris 2010. Acknowledgements BirdLife International and Environmental Research & Assessment Ltd. gratefully acknowledge generous support for this study from the Governments of Australia (Australian Antarctic Division), New Zealand (Antarctica New Zealand and Department of Conservation), Norway (Norsk Polarinstitutt and Ministry of Foreign Affairs), the United Kingdom (Foreign & Commonwealth Office), and the United States (National Science Foundation Division of Polar Programs), from the Scientific Committee on Antarctic Research in supporting the workshops, and from the Pew Charitable Trusts and the British Birdwatching Fair 2014, which has been vital to undertake the Antarctic IBA assessment and for the preparation of this report. -
Physical Properties of Shallow Ice Cores from Antarctic and Sub-Antarctic Islands
https://doi.org/10.5194/tc-2020-110 Preprint. Discussion started: 24 June 2020 c Author(s) 2020. CC BY 4.0 License. Physical properties of shallow ice cores from Antarctic and sub-Antarctic islands Elizabeth R. Thomas1, Guisella Gacitúa2, Joel B.Pedro3,4, Amy C.F. King1, Bradley Markle5, 6,7 1,8 5 Mariusz Potocki , Dorothea E. Moser 1British Antarctic Survey, Cambridge, CB3 0ET, UK 2Centro de Investigación Gaia Antártica, Universidad de Magallanes, Punta Arenas, Chile 3Australian Antarctic Division, Kingston, 7050, Australia 10 4Australian Antarctic Programme Partnership, Hobart, Tasmania 7001 Australia 5California Institute of Technology, Pasadena, CA, USA, 91125 6Climate Change Institute, University of Maine, Orono, ME 04469, USA 7School of Earth and Climate Sciences, University of Maine, Orono, ME 04469, USA 8Institut für Geologie und Paläontologie, University of Münster, 48149 Münster, Germany 15 Abstract. The sub-Antarctic is one of the most data sparse regions on earth. A number of glaciated Antarctic and sub- Antarctic islands have the potential to provide unique ice core records of past climate, atmospheric circulation 20 and sea ice. However, very little is known about the glaciology of these remote islands or their vulnerability to warming atmospheric temperatures. Here we present ground penetrating radar (GPR), melt histories and density profiles from shallow ice cores (14 to 24 m) drilled on three sub-Antarctic islands and two Antarctic coastal domes. This includes the first ever ice cores from Bouvet Island (54o26’0 S, 3o25’0 E) in the South Atlantic, from Peter 1st Island (68o50’0 S, 90o35’0 W) in the Bellingshausen Sea and from Young Island (66°17′S, 25 162°25′E) in the Ross Sea sector’s Balleny Islands chain.