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images, left to right:  Research ship near Palmer Station, field camp near Dufek Massif, 10-meter telescope under construction at the South Pole
Table of Contents
I. Some reasons to perform scientific research in the Antarctic
II. Season project highlights, 2007-2008
III. Construction highlights, 2007-2008
IV. Environmental protection; waste management
V. Personnel, Stations, and Camps
VI. Support Operations, 2007-2008
VII. United States Antarctic Policy and Achievements
VIII. National Science Foundation
XI. U.S. Antarctic Program aircraft and supply ship operations, 2007-2008 season
U.S. Antarctic Program research project list, 2007-2008
 
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OPP 08-001 December 2007

Some reasons to perform scientific research in the Antarctic

  1. Largest ocean current.  The Antarctic Circumpolar Current transports 130 million cubic meters of water per second towards the east, making it the mightiest of the ocean’s currents.  It influences formation of cold, dense, and nutrient-rich bottom water that extends throughout much of the world ocean and is a key to understanding change in world ocean circulation and its influence on global climate.1 Recent research has shown that understanding the carbon cycle in the Southern Ocean is critically important to understanding the global carbon cycle.

  2. Marine ecosystem.  Research on the marine ecosystem around Antarctica is providing an understanding of the strong coupling in the Southern Ocean between climate processes and ecosystem dynamics2  and helps to understand levels at which harvesting can take place without damaging the ecosystem.

  3. Sea ice.  The annual eightfold growth and decay of sea ice around Antarctica has been termed the greatest seasonal event on Earth.3 It affects regional climate and the global heat budget. Particularly near the edges, it nurtures some of the world’s most productive ecosystems.4

  4. Ozone hole.  One of the best examples of basic research about Earth’s environment that led to important public policy decisions is the story surrounding the Antarctic ozone hole. The discovery of the annual Antarctic ozone depletion, the research that uncovered the cause of the ozone depleting reactions, and the subsequent decisions about phasing out ozone depleting CFC’s is a compelling illustration of the value of science to society. Starting in 1979, ozone in the stratosphere over Antarctica has been observed almost to disappear every austral spring. In the 1990’s seasonal ozone depletion in the Arctic was first observed. Elsewhere, stratospheric ozone depletions are only incremental. Stratospheric ozone keeps much of the Sun’s harmful ultraviolet radiation from reaching the Earth’s surface and therefore, the ozone hole has received widespread attention.

    1. Finding the cause.  Research in Antarctica, particularly at McMurdo, was key to explaining how Antarctic natural phenomena conspire with the global buildup of manmade chemicals to cause the ozone hole.5
    2. Removing the cause.   The research led to an international decision (the Montreal Protocol) to reduce production of the destructive chemicals.  Annual consumption of CFCs dropped from 1,100,000 tons in 1986 to 150,000 tons in 1999.  Without the protocol, consumption would have reached 3,000,000 tons by 2010.6
    3. Monitoring the recovery.  While atmospheric concentrations of the harmful manmade chemicals are in decline, it might take another 10 years of observation before we can be sure the Antarctic ozone hole is shrinking. The best estimates are that annual depletion will occur for another 50 years. Current Antarctic research continues to provide further understanding of the ozone hole.7
    4. Effect on life.  The ozone hole lets abnormally high levels of the Sun's ultraviolet-B radiation penetrate to the Earth's surface and oceans. Scientists have documented how UV-B affects bacteria, phytoplankton, and the embryos of Antarctic invertebrates and fish.8
    5. Effect on climate.  Research indicates that the ozone hole has increased the winds around Antarctica and reduced rainfall in Australia and elsewhere.9 Some research indicates that the annual ozone depletion allows additional heat loss from the earth resulting in the minor cooling observed in the Antarctic interior.

    6. Awards.

      1. The 1995 Nobel Prize in Chemistry was awarded to three professors who explained that the ozone layer is sensitive to anthropogenic emissions.10
      2. The 1999 National Medal of Science (the Nation's highest scientific honor) was awarded to Dr. Susan Solomon, who led U.S. Antarctic Program expeditions in 1986 and 1987 giving the first direct evidence that anthropogenic chlorine depletes stratospheric ozone.
      3. The 2002 National Medal of Technology (the Nation's highest honor for technological innovation) was awarded to the Dupont Company for leadership in the phase-out and replacement of chlorofluorocarbons (CFCs).11

  5. Polar adaptations of biota.  Antarctica’s cold, desert conditions, and annual light cycles have led to molecular, biochemical, and physiological adaptations that enable biota to survive, reproduce, and indeed thrive under environmental extremes not experienced elsewhere.  Studies provide basic understanding of these unique adaptations and help understand how changes in populations may be linked to changing climate.12

  6. Atmospheric background levels.  Antarctica is the planet’s farthest region from human population centers and records the world’s background levels of atmospheric constituents.  Measurements since 1956 at the geographic South Pole have documented changes in world levels of greenhouse gases such as carbon dioxide and methane. Measure­ments in the data-sparse Southern Hemisphere are important to understanding and predicting global levels of these gases and their impact on (or forerunner to) climate change.13

  7. Weather and climate.  The unbroken collection of weather data from manned and unmanned stations in Antarctica, now exceeding 40 years for some locations, provides a data base and real-time information from which to make operational forecasts, study the dynamics of the Antarctic atmosphere, and chart the progress of human-induced global warming.14

  8. Ice sheets and ice shelves.  Antarctica’s ice sheets contain 90 percent of the world’s ice and 70 percent of the world’s fresh water.  Melted, it would raise sea level 65 meters (200 feet).

    1. Global process.  Antarctica’s ice—the world’s largest area of cold (the Arctic is 35oF warmer)—affects and responds to world climate change.  Just 20,000 years ago, the ice sheet was far larger, and correspondingly, sea level was 11 meters (36 feet) lower, as the water was locked into the Antarctic ice.15
    2. Climate history.  The ice, deposited annually as snow over millions of years, traps past atmospheric constituents that reveal climate history with a precision not equaled by other proxies such as ocean sediments and tree rings. The world's deepest ice core (3,650 meters) and another core containing the world’s oldest ice then sampled (possibly 1 million years old) both were drilled in Antarctica.16
    3. West Antarctic Ice Sheet. The West Antarctic Ice Sheet if melted would raise sea level 5 meters.  It is less stable than the East Antarctic ice because its base is below sea level.  Its low-probability/high-impact collapse has stimulated vigorous research over the last 30 years indicating that it has largely or completely disappeared after it formed, but at an unknown rate. Portions of it are changing rapidly now, while averages over the whole ice sheet show little change.  Some models project stability, while others suggest the possibility of rapid change.17
    4. Ice shelf dynamics.  Ice shelves—extensions of continental ice sheets that are afloat on the ocean—can control the rate at which their parent ice sheets or glaciers move into the sea and can respond more quickly than ice sheets to environmental change.  The Larsen Ice Shelf on the east coast of the Antarctic Peninsula lost massive sections in 1995 and 2002, possibly in response to atmospheric and oceanic warming over the last several decades.  Some scientists call it a model for what could happen to larger ice shelves farther south.18
    5. Subglacial lakes.  More than 70 lakes lie beneath the ice sheet, most of them several kilometers long.  One, Vostok Subglacial Lake, is an order of magnitude larger and represents the closest analog to both Europa (a moon of Jupiter) and a Neoproterozoic (“Snowball Earth”) subglacial environment. Lake Vostok is likely oligotrophic—an environment with low nutrient levels and low standing stocks of organisms. Life there may depend on alternative energy sources and survival strategies.19
    6. Monitoring Ice Mass Change and Sea Level Rise.  The Gravity Recovery and Climate Experiment (GRACE) satellite mission offers important observations about changes in mass in the Antarctic region. This mass change is predominantly due to two interwoven processes; 1) changes in ice mass and 2) the response of the lithosphere beneath the ice sheet to change in ice loading. However, GRACE observations alone cannot separate these processes. Consequently, the ground observations of crustal response to changes in ice loading that will be provided by the Polar Earth Observing Network (PoleNet) are essential to fully understanding how total ice mass is changing.

  9. Polar landmass.  Almost 10 percent of the Earth's continental crust resides in Antarctica.  The continent is old and stable and has been in a near-polar position for over 100 million years.  It thus contains unique high latitude environmental records of a time when Earth changed from greenhouse to icehouse conditions. The landmass is different from the other continents in that Antarctica's crustal structure—or its underlying mantle—has allowed the continent to remain essentially fixed on Earth's surface for a long time.

  10. Astronomy by high-altitude balloons.  Antarctica's summer weather provides a stable ride for instruments suspended from a balloon, which floats around Antarctica at a steady height above most of the atmosphere, providing an inexpensive way to get scientific experiments into near-space. 20

    1. The 2006 Balzan Prize for Astrophysics (one of four 1-million-Swiss-Franks awards made annually with the stipulation that half of each award must be used to support research of young investigators) was awarded to Dr. Andrew Lange of CalTech and his co-investigator Dr. Paolo de Bernardis of Italy in recognition of their contributions to cosmology, in particular the BOOMERANG Antarctic Long Duration Balloon experiment that produced the first images of structure in the Cosmic Microwave Background.21

  11. Astrophysics and astronomy from the surface.  The cold, clean, dry atmosphere over the South Pole provides viewing conditions that in some wavelengths are equal to those in space.  Amundsen-Scott South Pole Station has become a major astronomy and astrophysics center.22 

    1. Cosmic Microwave Background Radiation (CMBR) has been studied at the South Pole with unprecedented accuracy. Predicted in 1980s, the CMBR polarization was revealed for the first time in experimental data obtained by the University of Chicago Degree Angular Scale Interferometer (DASI)23 in 2002. Current studies are trying to detect the B-mode polarization with the Caltech small telescope BICEP24. The 10-m South Pole Telescope25 received its first light in February 2007, and now focuses on determining the nature of dark energy and dark matter and tests cosmological models aimed at explaining the origin of the Universe.
    2. Neutrino detection. The ice sheet beneath the South Pole is 2,900 meters deep and is homogeneous and clear.  Investigators buried downward-looking detectors to observe light produced by neutrinos (ultra-high-energy particles created by cataclysmic collisions in deep space) when they on rare occasions collide with ice molecules after they pass through the Earth.  The data help in descriptions of galactic centers, dark matter, and supernovae. The observatory became the first in the world to detect neutrinos in March 2001.26

  12. Meteorites.  Meteorites offer important information about the origin of our solar system and Antarctica is the principal source of meteorites for science. Since 1969, teams from the United States, Japan, and Europe have collected more than 30,000 meteorite specimens from the surface of the ice sheet and represent many meteorite classes (including some from the Moon and Mars), extending our knowledge of the solar system. Antarctica has yielded four-fifths of the meteorites known to science.27 Martian and lunar meteorites provide information about processes that helped form the crust of these bodies. The large numbers of meteorites available from the Antarctic collections have allowed unprecedented discoveries because more material has been available for both destructive analysis that was not previously possible. For example, common chondrites have yielded diamonds and other highly refractory grains that are remnants of the dust clouds that coalesced to form our solar system.

  13. Mount Erebus — one of Earth’s few long-lived lava lakes.  The world’s southern-most active volcano, Mount Erebus is one of the few volcanoes in the world with a long-lived (decades or more) convecting lava lake.  Although the volcano was discovered by James Ross in 1841, scientists still know relatively little about its geology because of extensive snow and ice cover, its remoteness, the extreme environment, and the short field season.28


End notes
[1] “The Southern Ocean,” by Arnold L. Gordon, Current 15(3): 4-6, 1999. The bountiful recent literature on the topic includes “What drove past teleconnections?” by Frank Sirocko, p. 1336-1337, Science, 5 September 2003.
[2] http://www.ccpo.odu.edu/Research/globec_menu.html
[3] The area of sea ice around Antarctica varies between 1 and 8 million square miles annually.  See images 4 and 5 in http://www.nsf.gov/od/opp/antarct/imageset/start.jsp
[4] http://www.antcrc.utas.edu.au/aspect/
[5]  “Overview of the polar ozone issue,” by Solomon, S.; Schoeberl, M.R.(ed), Geophysical Research Letters, 15(8), p.845-846 (August 1988), introduces a special issue on polar ozone.
[6]  “Montreal Protocol Benefits Cited,” page 395, 30 September 2003 EOS.
[7] http://www.cmdl.noaa.gov/ozwv/ozsondes/spo/ozhole.html (historical significance of the ozone hole)
[8] Scroll down to “Ozone Hole Consequences” in http://www.theozonehole.com/
[9] “Ozone and climate change,” p. 236-237, and “Simulation of recent Southern Hemisphere climate change,” p. 273-275, Science, 10 October 2003.   www.sciencemag.org.
[10] http://www.nobel.se/chemistry/laureates/1995/
[11] http://www.technology.gov/Medal/p_Recipients.htm#2002
[12] See, for example, The Adélie Penguin: Bellwether of Climate Change,” Columbia University Press, October 2002 http://www.columbia.edu/cu/cup/catalog/data/023112/023112306X.HTM
[13] The Climate Monitoring and Diagnostics Laboratory, National Oceanic and Atmospheric Administration, operates four baseline observatories worldwide, including the one at the South Pole in cooperation with NSF.  See http://www.cmdl.noaa.gov/
[14] The automatic weather station project, University of Wisconsin, is described at  http://amrc.ssec.wisc.edu/aws.html
[15] http://neptune.gsfc.nasa.gov/wais/articles/perspective.html
[16] Russian, French, and U.S. investigators drilled and analyzed the world's deepest ice core (3,650 meters). The core spans four glacial-interglacial cycles, furnishing an unparalleled archive. “Climate and atmospheric history of the past 420,000 years from the Vostok ice core, Antarctica,” by J.R. Petit and others, Nature (London), 399(6735), 429-436, 1999.  European coring at Dome C, East Antarctica, in 2003 reached 3,200 meters, yielding some of the world’s oldest ice, possibly 1 million years old.
[17] http://neptune.gsfc.nasa.gov/wais/
[18] “Warmer ocean could threaten antarctic ice shelves” (p. 759) and “Larsen Ice Shelf has progressively thinned” (p. 856-859), Science, 31 October 2003, www.sciencemag.org.  See also http://nsidc.org/sotc/iceshelves.html.
[19] http://www.ldeo.columbia.edu/~mstuding/vostok.html
[20] A microwave telescope borne for 10½ days 120,000 feet over Antarctica provided detailed evidence that the large-scale geometry of the universe is flat (Nature, 27 April 2000). Following the Big Bang 12-15 billion years ago, the universe was smooth, dense, and hot. The intense heat still is detectable as a faint glow called cosmic microwave background radiation.  Scientists had sought high-resolution images of the radiation since 1965, when a ground-based radio telescope discovered it. http://www.nsf.gov/od/lpa/news/press/00/pr0025.htm
[21] See http://www.balzan.com/index_en.cfm
[22] The University of Chicago (Yerkes Observatory) and 15 institutions from four nations installed telescopes at South Pole Station emphasizing infrared and submillimeter wavelengths.  This large project, one of NSF's 24 Science & Technology Centers, in 2001 provided science with the strongest evidence to date for the theory of inflation, the leading model for the formation of the universe.  http://www.nsf.gov/od/lpa/news/press/01/pr0138.htm
[23]  http://astro.uchicago.edu/dasi
[24] http://www.astro.caltech.edu/~lgg/bicep_front.htm
[25]http://spt.uchicago.edu/
[26]http://amanda.berkeley.edu/
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27 http://geology.cwru.edu/~ansmet/
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28 http://www.ees.nmt.edu/Geop/mevo/mevo.html
 
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