Antarctic Ice Sheet Computer Animations and Paper Model by Tau Rho Alpha, and Alan K

Total Page:16

File Type:pdf, Size:1020Kb

Antarctic Ice Sheet Computer Animations and Paper Model by Tau Rho Alpha, and Alan K Go Home U.S. DEPARTMENT OF THE INTERIOR U.S. GEOLOGICAL SURVEY Antarctic Ice Sheet Computer animations and paper model By Tau Rho Alpha, and Alan K. Cooper Open-file Report 98-353 fl This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government. Although this program has been used by the U.S. Geological Survey, no warranty, expressed or implied, is made by the USGS as to the accuracy and functioning of the program and related program material, nor shall the fact of distribution constitute any such warranty, and no responsibility is assumed by the USGS in connection therewith. U.S. Geological Survey Menlo Park, CA 94025 Comments encouraged [email protected] [email protected] 1998 (go backward) <T"1 L^ (go forward) Description of Report This report illustrates, through computer animation and a paper model, why there are changes on the ice sheet that covers the Antarctica continent. By studying the animations and the paper model, students will better understand the evolution of the Antarctic ice sheet. Included in the paper and diskette versions of this report are templates for making a papetfttiodel, instructions for its assembly, and a discussion of development of the Antarctic ice sheet. In addition, the diskette version includes a animation of how Antarctica and its ice cover changes through time. Many people provided help and encouragement in the development of this HyperCard stack, particularly Page Mosier, Sue Priest and Art Ford. This report was enhanced by reviews from Bonnie Murchey, Peter Stauffer and Stephen Eittreim. Table of Contents for paper version of this report. Title page page 1 Description of report page 2 Teachers guide page 4 Paper model of Antarctica page 35 (go backward) <J (go forward) Description of Report Requirements for using the diskette version are: Apple Computer, Inc., HyperCard 2.2 software and an Apple Macintosh computer with an internal disk drive. If you are using System 7, we recommend having at least 8 MB of physical RAM with 4.5MB of memory available for HyperCard. The animation is accompanied by sound. If no sound is heard, change the memory of HyperCard to 4500K and ensure that the control panel "Sound," which is in the "Control Panels" folder under the "Apple" menu, has the volume set to at least 2. To change the memory available to HyperCard, quit this stack. Highlight the HyperCard program icon and choose "Get Info" from the File Menu. Change the "memory requirements" to 4500K and start this stack again. Purchasers of the diskette version of this report, which includes all of the text and graphics, can use HyperCard 2.2 software (not supplied) to change the model (by adding patterns, symbols, colors, etc.) or to transfer the model to other graphics software packages. To see the entire page (card size: MacPaint), select "Scroll" from the "Go" menu and move the hand pointer in the scroll window. If you are experiencing trouble with user-level buttons, select "message" from the "Go" menu. Type "magic" in the message box and press return. Three more user-level buttons should appear. The date of this Open File Report is 6/30/1998. OF 98-353-A, paper copy, 49p.; OF 98-353-B, 3.5-in. Macintosh 1.4-MB high-density diskette. To order this report, contact: USGS ESIC Open-File Report Section, Box 25286, MS 517, Denver Federal Center, Denver, CO 80225-0046 or call (303) 236-4476. These stacks (reports) can be down loaded from self-extracting archives, that are on the U.S. Geological Survey's Learning Web site. The address is: < http://ww^^^gs.gov^ducation/animations/ > [ Back to table of contents ) Teachers Guide: Page 1 of 31 Learn about Antarctica Antarctica lies at the "bottom of the world" and is the highest (in elevation), driest, and coldest continent on earth. It is nearly one and a half times larger than the continental United States, and its coastlines are longer than those that surround North America. The continent is surrounded by the largest of all the oceans - the Southern Ocean - that includes parts of the Atlantic, Pacific, and Indian Oceans. Yet, Antarctica has not always been this way, and at one time it was a more hospitable place. In the following descriptions, you will discover how Antarctica evolved from a giant land mass called Gondwanaland to a continent surrounded by water and covered by ice. And, you will learn how the massive ice sheet that now covers Antarctica evolved, and how the ice sheet acts as the "Earth's refrigerator" to strongly control our global climate and sea level. Antarctica is a remote continent of great beauty and is a challenge to adventurous explorers and scientists who want to know more about "The Last Place on Earth". The Great Southern Continent Antarctica is a vast continent that lies below an even larger "slab" of ice called the Antarctic Ice Sheet. When we look at maps, we see mostly the outline of the edges of the Ice Sheet. But, when we lift up the ice sheet (as you can do with the paper model that comes with this report), we see that there is water and land beneath the ice. There are large seaways and bays that go far into the continent and lie below sea level. And, there are large isolated lakes. Mountain ranges also lie under the ice. They are as long and high as those that cross the western United States. All that we know about what lies under the ice comes from remote sensing "radar" surveys that have been done by scientists from many countries. These surveys cover only a very small part of Antarctica, and there are many surprises yet to be discovered under areas of the ice sheet that have not been studied. But, in general, the continent under the ice is much like any other land areas without ice. [ Back to table of contents j 4 Teachers Guide: O Page 2 of 31 Index map of Antarctica 30° W. 30° E. South America 60° E. L 90° W. 90° E. Australia 120° E. 120° W. 150°W. 150° E. 180C Figure 1. A view of the South Pole and an Index map of Antarctica, showing the relationship of South America, New Zealand and Australia. Teachers Guide: \^] Page 3 of 31 Relative size of Antarctica and the Continental United States 0 1,000 2,000 Km 1,000 2,000 Statute Miles Figure 2. Relative size of Antarctica and the continental United States. Antarctica is estimated to have a surface area of 5,500,000 square miles and the continental United States 3,022,387 square miles. The lines of longitude and latitude that make up the graticule locate only Antarctica. Teachers Guide: Page 4 of 31 Atlantic Ocean Antarctica Weddell Indian Ocean ^V Gambursev . subglacial (under the ice) ^ - Mountains East .«^ ^° Antarctica Antarctica Pacific Ocean Boundary between East and West Antarctica Arrovs indicate ice-flov directions Figure 3. Index map of Antarctica today showing features and ice-flow directions for the Antarctic Ice Sheet. Teachers Guide: Page 5 of 31 Deep oceans surround Antarctica today, but 180 million years ago, the Antarctic land mass was at the center of a super-continent called Gondwanaland. The super-continent was pulled apart into many pieces by the processes of sea-floor spreading. Over the last 175 million years, Antarctica has remained near the south pole while the other pieces of Gondwanaland moved north to become the continents and land masses that we now know of as Africa, India, Madagascar, Australia, New Zealand, and South America. The areas between the land masses became great ocean basins. Antarctica has been in its position at the "bottom of the world" for about the last 100 million years. See Figure 1. The Great Ice Sheets Antarctica has not always been covered by ice. In fact, until 45-50 million years ago, there was little, if any, glacier ice in Antarctica. The climate was temperate and warm, and there were lush forests. We know this from examining rocks from some of the few areas on Antarctica that are not covered by ice in Antarctica. Today, only 2% of Antarctica's land mass is exposed, with the rest under ice. We also have sedimentary rock samples from drilling operations done by ships in the oceans around Antarctica. The rocks.contain information such as fossils, oxygen isotopes, clay minerals, and ice-rafted debris that we can use to piece together what the climates were like and how much of Antarctica was covered by glaciers. The evidence indicates that the first of many large ice sheets of the Cenozoic glacial era began to grow between 36-45 million years ago. Teachers Guide: Page 6 of 31 Ice sheets are composed of snow from frozen fresh water. In fact, the Antarctic Ice Sheet currently holds 68% of the world's fresh water. Where does all this water come from? The answer lies in how ice sheets grow. Many times in the past,however, enormous ice sheets have covered large parts of the Northern Hemisphere, including Greenland, Scandinavia, northern Russia, and North America, as well as Antarctica. Today the ice sheets are smaller, and only exist on Greenland and Antarctica. Before describing the history of the Antarctic Ice Sheet, let us learn a bit more about other great ice sheets and how and why they get thicker or "grow". The last glacial period was at its maximum about 20,000 years ago.
Recommended publications
  • T Antarctic Ce Sheet Itiative
    race Publication 3115, Vol. 1 t Antarctic ce Sheet itiative :_,.me.-1: Science and ;mentation Plan iv-_J_ E -- --__o • E _-- rz " _ • _ _v_-- . "2-. .... E _ ____ __ _k - -- - ...... --rr r_--_.-- .... m-- _ £3._= --- - • ,r- ..... _ k • -- ..... __= ---- = ............ --_ m -- -- ..... Z Im .... r .... _,... ___ "--. 11 1"1 I' I i ¸ NASA Conference Publication 3115, Vol. 1 West Antarctic Ice Sheet Initiative Volume 1: Science and Implementation Plan Edited by Robert A. Bindschadler NASA Goddard Space Flight Center Greenbelt, Maryland Proceedings of a workshop cosponsored by the National Aeronautics and Space Administration, Washington, D.C., and the National Science Foundation, Washington, D.C., and held at Goddard Space Flight Center Greenbelt, Maryland October 16-18, 1990 IXl/_/X National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1991 CONTENTS Page Preface v Workshop Participants vi Acknowledgements vii Map viii 1. Executive Summary 1 2. Climatic Importance of Ice Sheets 4 3. Marine Ice Sheet Instability 5 4. The West Antarctic Ice Sheet Initiative 6 4.1 Goal and Objectives 6 4.2 A Multidisciplinary Project 7 4.3 Scientific Focus: A Single Goal 7 4.4 Geographic Focus: West Antarctica 7 4.5 Duration: A Phased Approach 8 5. Science Plan 10 5.1 Glaciology 10 5.1.1 Ice Dynamics 10 5.1.2 Ice Cores 16 5.2 Meteorology 19 5.3 Oceanography 23 5.4 Geology and Geophysics 27 5.4.1 Terrestrial Geology 27 5.4.2 Marine Geology and Geophysics 28 5.4.3 Subglacial Geology and Geophysics 30 6.
    [Show full text]
  • Lecture 21: Glaciers and Paleoclimate Read: Chapter 15 Homework Due Thursday Nov
    Learning Objectives (LO) Lecture 21: Glaciers and Paleoclimate Read: Chapter 15 Homework due Thursday Nov. 12 What we’ll learn today:! 1. 1. Glaciers and where they occur! 2. 2. Compare depositional and erosional features of glaciers! 3. 3. Earth-Sun orbital parameters, relevance to interglacial periods ! A glacier is a river of ice. Glaciers can range in size from: 100s of m (mountain glaciers) to 100s of km (continental ice sheets) Most glaciers are 1000s to 100,000s of years old! The Snowline is the lowest elevation of a perennial (2 yrs) snow field. Glaciers can only form above the snowline, where snow does not completely melt in the summer. Requirements: Cold temperatures Polar latitudes or high elevations Sufficient snow Flat area for snow to accumulate Permafrost is permanently frozen soil beneath a seasonal active layer that supports plant life Glaciers are made of compressed, recrystallized snow. Snow buildup in the zone of accumulation flows downhill into the zone of wastage. Glacier-Covered Areas Glacier Coverage (km2) No glaciers in Australia! 160,000 glaciers total 47 countries have glaciers 94% of Earth’s ice is in Greenland and Antarctica Mountain Glaciers are Retreating Worldwide The Antarctic Ice Sheet The Greenland Ice Sheet Glaciers flow downhill through ductile (plastic) deformation & by basal sliding. Brittle deformation near the surface makes cracks, or crevasses. Antarctic ice sheet: ductile flow extends into the ocean to form an ice shelf. Wilkins Ice shelf Breakup http://www.youtube.com/watch?v=XUltAHerfpk The Greenland Ice Sheet has fewer and smaller ice shelves. Erosional Features Unique erosional landforms remain after glaciers melt.
    [Show full text]
  • Rapid Cenozoic Glaciation of Antarctica Induced by Declining
    letters to nature 17. Huang, Y. et al. Logic gates and computation from assembled nanowire building blocks. Science 294, Early Cretaceous6, yet is thought to have remained mostly ice-free, 1313–1317 (2001). 18. Chen, C.-L. Elements of Optoelectronics and Fiber Optics (Irwin, Chicago, 1996). vegetated, and with mean annual temperatures well above freezing 4,7 19. Wang, J., Gudiksen, M. S., Duan, X., Cui, Y. & Lieber, C. M. Highly polarized photoluminescence and until the Eocene/Oligocene boundary . Evidence for cooling and polarization sensitive photodetectors from single indium phosphide nanowires. Science 293, the sudden growth of an East Antarctic Ice Sheet (EAIS) comes 1455–1457 (2001). from marine records (refs 1–3), in which the gradual cooling from 20. Bagnall, D. M., Ullrich, B., Sakai, H. & Segawa, Y. Micro-cavity lasing of optically excited CdS thin films at room temperature. J. Cryst. Growth. 214/215, 1015–1018 (2000). the presumably ice-free warmth of the Early Tertiary to the cold 21. Bagnell, D. M., Ullrich, B., Qiu, X. G., Segawa, Y. & Sakai, H. Microcavity lasing of optically excited ‘icehouse’ of the Late Cenozoic is punctuated by a sudden .1.0‰ cadmium sulphide thin films at room temperature. Opt. Lett. 24, 1278–1280 (1999). rise in benthic d18O values at ,34 million years (Myr). More direct 22. Huang, Y., Duan, X., Cui, Y. & Lieber, C. M. GaN nanowire nanodevices. Nano Lett. 2, 101–104 (2002). evidence of cooling and glaciation near the Eocene/Oligocene 8 23. Gudiksen, G. S., Lauhon, L. J., Wang, J., Smith, D. & Lieber, C. M. Growth of nanowire superlattice boundary is provided by drilling on the East Antarctic margin , structures for nanoscale photonics and electronics.
    [Show full text]
  • 2. Disc Resources
    An early map of the world Resource D1 A map of the world drawn in 1570 shows ‘Terra Australis Nondum Cognita’ (the unknown south land). National Library of Australia Expeditions to Antarctica 1770 –1830 and 1910 –1913 Resource D2 Voyages to Antarctica 1770–1830 1772–75 1819–20 1820–21 Cook (Britain) Bransfield (Britain) Palmer (United States) ▼ ▼ ▼ ▼ ▼ Resolution and Adventure Williams Hero 1819 1819–21 1820–21 Smith (Britain) ▼ Bellingshausen (Russia) Davis (United States) ▼ ▼ ▼ Williams Vostok and Mirnyi Cecilia 1822–24 Weddell (Britain) ▼ Jane and Beaufoy 1830–32 Biscoe (Britain) ★ ▼ Tula and Lively South Pole expeditions 1910–13 1910–12 1910–13 Amundsen (Norway) Scott (Britain) sledge ▼ ▼ ship ▼ Source: Both maps American Geographical Society Source: Major voyages to Antarctica during the 19th century Resource D3 Voyage leader Date Nationality Ships Most southerly Achievements latitude reached Bellingshausen 1819–21 Russian Vostok and Mirnyi 69˚53’S Circumnavigated Antarctica. Discovered Peter Iøy and Alexander Island. Charted the coast round South Georgia, the South Shetland Islands and the South Sandwich Islands. Made the earliest sighting of the Antarctic continent. Dumont d’Urville 1837–40 French Astrolabe and Zeelée 66°S Discovered Terre Adélie in 1840. The expedition made extensive natural history collections. Wilkes 1838–42 United States Vincennes and Followed the edge of the East Antarctic pack ice for 2400 km, 6 other vessels confirming the existence of the Antarctic continent. Ross 1839–43 British Erebus and Terror 78°17’S Discovered the Transantarctic Mountains, Ross Ice Shelf, Ross Island and the volcanoes Erebus and Terror. The expedition made comprehensive magnetic measurements and natural history collections.
    [Show full text]
  • Asynchronous Antarctic and Greenland Ice-Volume Contributions to the Last Interglacial Sea-Level Highstand
    ARTICLE https://doi.org/10.1038/s41467-019-12874-3 OPEN Asynchronous Antarctic and Greenland ice-volume contributions to the last interglacial sea-level highstand Eelco J. Rohling 1,2,7*, Fiona D. Hibbert 1,7*, Katharine M. Grant1, Eirik V. Galaasen 3, Nil Irvalı 3, Helga F. Kleiven 3, Gianluca Marino1,4, Ulysses Ninnemann3, Andrew P. Roberts1, Yair Rosenthal5, Hartmut Schulz6, Felicity H. Williams 1 & Jimin Yu 1 1234567890():,; The last interglacial (LIG; ~130 to ~118 thousand years ago, ka) was the last time global sea level rose well above the present level. Greenland Ice Sheet (GrIS) contributions were insufficient to explain the highstand, so that substantial Antarctic Ice Sheet (AIS) reduction is implied. However, the nature and drivers of GrIS and AIS reductions remain enigmatic, even though they may be critical for understanding future sea-level rise. Here we complement existing records with new data, and reveal that the LIG contained an AIS-derived highstand from ~129.5 to ~125 ka, a lowstand centred on 125–124 ka, and joint AIS + GrIS contributions from ~123.5 to ~118 ka. Moreover, a dual substructure within the first highstand suggests temporal variability in the AIS contributions. Implied rates of sea-level rise are high (up to several meters per century; m c−1), and lend credibility to high rates inferred by ice modelling under certain ice-shelf instability parameterisations. 1 Research School of Earth Sciences, The Australian National University, Canberra, ACT 2601, Australia. 2 Ocean and Earth Science, University of Southampton, National Oceanography Centre, Southampton SO14 3ZH, UK. 3 Department of Earth Science and Bjerknes Centre for Climate Research, University of Bergen, Allegaten 41, 5007 Bergen, Norway.
    [Show full text]
  • The Evolution of the Antarctic Ice Sheet at the Eocene-Oligocene Transition
    Geophysical Research Abstracts Vol. 19, EGU2017-8151, 2017 EGU General Assembly 2017 © Author(s) 2017. CC Attribution 3.0 License. The evolution of the Antarctic ice sheet at the Eocene-Oligocene Transition. Jean-Baptiste Ladant (1), Yannick Donnadieu (1,2), and Christophe Dumas (1) (1) LSCE, CNRS-CEA, Paris, France ([email protected]), (2) CEREGE, CNRS, Aix-en-Provence, France An increasing number of studies suggest that the Middle to Late Eocene has witnessed the waxing and waning of relatively small ephemeral ice sheets. These alternating episodes culminated in the Eocene-Oligocene transition (34 – 33.5 Ma) during which a sudden and massive glaciation occurred over Antarctica. Data studies have demonstrated that this glacial event is constituted of two 50 kyr-long steps, the first of modest (10 – 30 m of equivalent sea level) and the second of major (50 – 90 m esl) glacial amplitude, and separated by ∼ 200 kyrs. Since a decade, modeling studies have put forward the primary role of CO2 in the initiation of this glaciation, in doing so marginalizing the original “gateway hypothesis”. Here, we investigate the impacts of CO2 and orbital parameters on the evolution of the ice sheet during the 500 kyrs of the EO transition using a tri-dimensional interpolation method. The latter allows precise orbital variations, CO2 evolution and ice sheet feedbacks (including the albedo) to be accounted for. Our results show that orbital variations are instrumental in initiating the first step of the EO glaciation but that the primary driver of the major second step is the atmospheric pCO2 crossing a modelled glacial threshold of ∼ 900 ppm.
    [Show full text]
  • Sea Level and Climate Introduction
    Sea Level and Climate Introduction Global sea level and the Earth’s climate are closely linked. The Earth’s climate has warmed about 1°C (1.8°F) during the last 100 years. As the climate has warmed following the end of a recent cold period known as the “Little Ice Age” in the 19th century, sea level has been rising about 1 to 2 millimeters per year due to the reduction in volume of ice caps, ice fields, and mountain glaciers in addition to the thermal expansion of ocean water. If present trends continue, including an increase in global temperatures caused by increased greenhouse-gas emissions, many of the world’s mountain glaciers will disap- pear. For example, at the current rate of melting, most glaciers will be gone from Glacier National Park, Montana, by the middle of the next century (fig. 1). In Iceland, about 11 percent of the island is covered by glaciers (mostly ice caps). If warm- ing continues, Iceland’s glaciers will decrease by 40 percent by 2100 and virtually disappear by 2200. Most of the current global land ice mass is located in the Antarctic and Greenland ice sheets (table 1). Complete melt- ing of these ice sheets could lead to a sea-level rise of about 80 meters, whereas melting of all other glaciers could lead to a Figure 1. Grinnell Glacier in Glacier National Park, Montana; sea-level rise of only one-half meter. photograph by Carl H. Key, USGS, in 1981. The glacier has been retreating rapidly since the early 1900’s.
    [Show full text]
  • West Antarctic Ice Sheet Divide Ice Core Climate, Ice Sheet History, Cryobiology
    QUARTERLY UPDATE August 2009 West Antarctic Ice Sheet Divide Ice Core Climate, Ice Sheet History, Cryobiology 2009/2010 Field Operations Our main objectives for the coming field season are: 1) To ship ice from 680 to ~2,100 m to NICL 2) Recover core to a depth of 2,600 to 2,900 m The U.S. Antarctic Program will be establishing a multi year field camp at Byrd this season to support field operations around Pine Island Bay and elsewhere in West Antarctica. The camp at Byrd will complicate our logistics because the heavy equipment that will prepare the Byrd skiway will be flown to WAIS Divide and driven to Byrd, and a camp at Byrd will make for more competition for flights. But this is a much better plan than supporting those operations out of WAIS Divide, which would have increased the WAIS Divide population to 100 people. Other science activities at WAIS Divide this season include the following: CReSIS ground traverse to Pine Island Bay Flow dynamics of two Amundsen Sea glaciers: Thwaites and Pine Island. PI: Anandakrishnan Ocean-Ice Interaction in the Amundsen Sea sector of West Antarctica. PI: Joughin Space physics magnetometer. PI: Zesta Antarctic Automatic Weather Station Program. PI: Weidner Polar Experiment Network for Geospace Upper atmosphere Investigations. PI: Lessard Artist, paintings of ice and glacial features. PI: McKee IDDO is making several modifications to the drill that should increase the amount of core that can be recovered each time the drill is lowered into the hole, which will increase the amount of ice we can recover this season.
    [Show full text]
  • A Review of Ice-Sheet Dynamics in the Pine Island Glacier Basin, West Antarctica: Hypotheses of Instability Vs
    Pine Island Glacier Review 5 July 1999 N:\PIGars-13.wp6 A review of ice-sheet dynamics in the Pine Island Glacier basin, West Antarctica: hypotheses of instability vs. observations of change. David G. Vaughan, Hugh F. J. Corr, Andrew M. Smith, Adrian Jenkins British Antarctic Survey, Natural Environment Research Council Charles R. Bentley, Mark D. Stenoien University of Wisconsin Stanley S. Jacobs Lamont-Doherty Earth Observatory of Columbia University Thomas B. Kellogg University of Maine Eric Rignot Jet Propulsion Laboratories, National Aeronautical and Space Administration Baerbel K. Lucchitta U.S. Geological Survey 1 Pine Island Glacier Review 5 July 1999 N:\PIGars-13.wp6 Abstract The Pine Island Glacier ice-drainage basin has often been cited as the part of the West Antarctic ice sheet most prone to substantial retreat on human time-scales. Here we review the literature and present new analyses showing that this ice-drainage basin is glaciologically unusual, in particular; due to high precipitation rates near the coast Pine Island Glacier basin has the second highest balance flux of any extant ice stream or glacier; tributary ice streams flow at intermediate velocities through the interior of the basin and have no clear onset regions; the tributaries coalesce to form Pine Island Glacier which has characteristics of outlet glaciers (e.g. high driving stress) and of ice streams (e.g. shear margins bordering slow-moving ice); the glacier flows across a complex grounding zone into an ice shelf coming into contact with warm Circumpolar Deep Water which fuels the highest basal melt-rates yet measured beneath an ice shelf; the ice front position may have retreated within the past few millennia but during the last few decades it appears to have shifted around a mean position.
    [Show full text]
  • GSA TODAY • Southeastern Section Meeting, P
    Vol. 5, No. 1 January 1995 INSIDE • 1995 GeoVentures, p. 4 • Environmental Education, p. 9 GSA TODAY • Southeastern Section Meeting, p. 15 A Publication of the Geological Society of America • North-Central–South-Central Section Meeting, p. 18 Stability or Instability of Antarctic Ice Sheets During Warm Climates of the Pliocene? James P. Kennett Marine Science Institute and Department of Geological Sciences, University of California Santa Barbara, CA 93106 David A. Hodell Department of Geology, University of Florida, Gainesville, FL 32611 ABSTRACT to the south from warmer, less nutrient- rich Subantarctic surface water. Up- During the Pliocene between welling of deep water in the circum- ~5 and 3 Ma, polar ice sheets were Antarctic links the mean chemical restricted to Antarctica, and climate composition of ocean deep water with was at times significantly warmer the atmosphere through gas exchange than now. Debate on whether the (Toggweiler and Sarmiento, 1985). Antarctic ice sheets and climate sys- The evolution of the Antarctic cryo- tem withstood this warmth with sphere-ocean system has profoundly relatively little change (stability influenced global climate, sea-level his- hypothesis) or whether much of the tory, Earth’s heat budget, atmospheric ice sheet disappeared (deglaciation composition and circulation, thermo- hypothesis) is ongoing. Paleoclimatic haline circulation, and the develop- data from high-latitude deep-sea sed- ment of Antarctic biota. iments strongly support the stability Given current concern about possi- hypothesis. Oxygen isotopic data ble global greenhouse warming, under- indicate that average sea-surface standing the history of the Antarctic temperatures in the Southern Ocean ocean-cryosphere system is important could not have increased by more for assessing future response of the Figure 1.
    [Show full text]
  • Antarctic Primer
    Antarctic Primer By Nigel Sitwell, Tom Ritchie & Gary Miller By Nigel Sitwell, Tom Ritchie & Gary Miller Designed by: Olivia Young, Aurora Expeditions October 2018 Cover image © I.Tortosa Morgan Suite 12, Level 2 35 Buckingham Street Surry Hills, Sydney NSW 2010, Australia To anyone who goes to the Antarctic, there is a tremendous appeal, an unparalleled combination of grandeur, beauty, vastness, loneliness, and malevolence —all of which sound terribly melodramatic — but which truly convey the actual feeling of Antarctica. Where else in the world are all of these descriptions really true? —Captain T.L.M. Sunter, ‘The Antarctic Century Newsletter ANTARCTIC PRIMER 2018 | 3 CONTENTS I. CONSERVING ANTARCTICA Guidance for Visitors to the Antarctic Antarctica’s Historic Heritage South Georgia Biosecurity II. THE PHYSICAL ENVIRONMENT Antarctica The Southern Ocean The Continent Climate Atmospheric Phenomena The Ozone Hole Climate Change Sea Ice The Antarctic Ice Cap Icebergs A Short Glossary of Ice Terms III. THE BIOLOGICAL ENVIRONMENT Life in Antarctica Adapting to the Cold The Kingdom of Krill IV. THE WILDLIFE Antarctic Squids Antarctic Fishes Antarctic Birds Antarctic Seals Antarctic Whales 4 AURORA EXPEDITIONS | Pioneering expedition travel to the heart of nature. CONTENTS V. EXPLORERS AND SCIENTISTS The Exploration of Antarctica The Antarctic Treaty VI. PLACES YOU MAY VISIT South Shetland Islands Antarctic Peninsula Weddell Sea South Orkney Islands South Georgia The Falkland Islands South Sandwich Islands The Historic Ross Sea Sector Commonwealth Bay VII. FURTHER READING VIII. WILDLIFE CHECKLISTS ANTARCTIC PRIMER 2018 | 5 Adélie penguins in the Antarctic Peninsula I. CONSERVING ANTARCTICA Antarctica is the largest wilderness area on earth, a place that must be preserved in its present, virtually pristine state.
    [Show full text]
  • The Antarctic Contribution to Holocene Global Sea Level Rise
    The Antarctic contribution to Holocene global sea level rise Olafur Ing6lfsson & Christian Hjort The Holocene glacial and climatic development in Antarctica differed considerably from that in the Northern Hemisphere. Initial deglaciation of inner shelf and adjacent land areas in Antarctica dates back to between 10-8 Kya, when most Northern Hemisphere ice sheets had already disappeared or diminished considerably. The continued deglaciation of currently ice-free land in Antarctica occurred gradually between ca. 8-5 Kya. A large southern portion of the marine-based Ross Ice Sheet disintegrated during this late deglaciation phase. Some currently ice-free areas were deglaciated as late as 3 Kya. Between 8-5 Kya, global glacio-eustatically driven sea level rose by 10-17 m, with 4-8 m of this increase occurring after 7 Kya. Since the Northern Hemisphere ice sheets had practically disappeared by 8-7 Kya, we suggest that Antarctic deglaciation caused a considerable part of the global sea level rise between 8-7 Kya, and most of it between 7-5 Kya. The global mid-Holocene sea level high stand, broadly dated to between 84Kya, and the Littorina-Tapes transgressions in Scandinavia and simultaneous transgressions recorded from sites e.g. in Svalbard and Greenland, dated to 7-5 Kya, probably reflect input of meltwater from the Antarctic deglaciation. 0. Ingcilfsson, Gotlienburg Universiw, Earth Sciences Centre. Box 460, SE-405 30 Goteborg, Sweden; C. Hjort, Dept. of Quaternary Geology, Lund University, Sdvegatan 13, SE-223 62 Lund, Sweden. Introduction dated to 20-17 Kya (thousands of years before present) in the western Ross Sea area (Stuiver et al.
    [Show full text]