Geography Atlas
Antarctic Desert
Image: MODIS Land Rapid Response Team, NASA GSFC · Public domain
Continental Polar Desert

Antarctic Desert

The Antarctic Desert, also called the Antarctic polar desert, is the cold, precipitation-poor land environment of Antarctica around the South Pole. Its surface is chiefly the Antarctic Ice Sheet: a high interior plateau divided by ice-flow divides and the Transantarctic Mountains, then drained outward to the Southern Ocean through ice streams, outlet glaciers, and floating ice shelves.

Why This Record Matters

Arid climate, immense frozen store

“Desert” describes the low moisture supply, not bare sand or an absence of ice. The continent-wide snowfall estimate is only about 150 millimetres of water equivalent per year, yet snowfall retained over long periods has built an ice sheet containing an estimated 27.17 million cubic kilometres of ice.[3][2]

Feature TypePolar desert region

A descriptive climatic region; Köppen–Geiger maps classify most of its climate as EF, or ice cap.[4]

Geographic ScopeAntarctic land

This record uses the continental land frame rather than claiming one surveyed climatic perimeter; it excludes the Southern Ocean and seasonal sea ice.

Mean Surface ElevationAbout 2,500 m

A continental mean reported by the Australian Antarctic Program; local bed and ice surfaces differ greatly.[1]

Snow Accumulation~150 mm w.e. yearly

Estimated continent-wide mean; the elevated plateau receives less than 50 mm water equivalent.[3]

Definition

What the name covers

Antarctic Desert is a regional climate-and-landscape name rather than a single basin or bounded landform with one set of coordinates. This page uses it for the very dry terrestrial environment of Antarctica: grounded ice, the small areas of exposed rock and sediment within the continental frame, and the processes linking that land to its margins. “Antarctic polar desert” and “polar ice desert” are descriptive variants. The Antarctic Ice Sheet is the dominant surface system inside the region, but the two terms are not exact synonyms.

The South Pole at 90° S supplies a geographic reference point, but longitude converges there and no single coordinate represents a continent-scale region. Likewise, 60° S—the northern edge of many Antarctic datasets and of the Antarctic Treaty area—is not the desert's physical boundary. Floating shelves are included here only where they explain how grounded ice drains; drifting sea ice is frozen ocean and lies outside the terrestrial desert.

Formal climate terminology needs care. In the widely used Köppen–Geiger scheme, Antarctica was mapped mainly as EF (ice-cap climate), with small low coastal areas assigned ET (tundra); the authors also noted that Antarctic station coverage was sparse.[4] Calling Antarctica a desert therefore expresses its exceptionally small precipitation supply, not a Köppen BWh or BWk desert classification.

Extent

Land, grounded ice, and floating margins

Antarctica surrounds the South Pole and is encircled by the Southern Ocean. East Antarctica is the larger, more continuous continental block, chiefly south of the Indian and Atlantic sectors of that ocean. West Antarctica lies between the Ross and Weddell seas and includes Marie Byrd Land, the Ellsworth Mountains, and the Antarctic Peninsula, which projects north toward South America. The Transantarctic Mountains extend from the Ross Sea side toward the Weddell Sea side and form the conventional physical divide between East and West Antarctica.[5]

The Australian Antarctic Program reports 13,661,000 square kilometres for Antarctica including its islands and ice shelves.[1] That value is a useful continental-scale frame, not a measured desert area: it incorporates floating ice and does not follow a climatic isohyet. Bedmap3 treats grounded ice, transiently grounded ice, floating shelf, and exposed rock as separate mask classes. Its outer shelf front comes from January–March 2022 Landsat imagery, while most observations informing its grounding-zone mask span about 2015–2020; both boundaries can migrate.[2]

The Ross and Filchner–Ronne ice shelves fill large embayments on opposite sides of the continent. They are floating extensions of land ice rather than additions to the land desert. Farther north, sea ice grows and retreats seasonally across the ocean surface; including it in a desert-area total would mix a terrestrial climate region with a changing marine cover.

Relief

Two landscapes: ice surface and buried bed

The visible relief is dominated by a broad ice plateau. Ice domes and divides stand highest in the East Antarctic interior, and long surface slopes descend toward coastal escarpments. Antarctica's mean elevation is reported as about 2,500 metres, a figure for the ice-covered continental surface rather than the average height of its bedrock.[1] Nunataks—rock peaks projecting through ice—and ranges such as the Transantarctic and Ellsworth mountains interrupt the otherwise smooth ice surface.

The underlying relief is much rougher. East Antarctica includes an old continental shield, highlands, subglacial mountain blocks, and deep basins. Much of West Antarctica is a set of lower crustal blocks and basins whose bed lies below sea level beneath one continuous ice surface. Bed troughs steer fast flow, while ridges and mountain flanks divide catchments and can pin floating shelves. This is why “elevation” must specify whether it means ice surface or rock bed.

Bedmap3 (2025) models surface elevation, ice thickness, bed elevation, and shelf cavities on a 500-m polar-stereographic grid; elevations are tied to the g104c geoid. It estimates 27.17 million cubic kilometres of Antarctic ice and 58 metres of potential global-mean sea-level equivalent from the grounded component.[2] These are inventory/model results, not direct measurements at every grid cell: 93% of its ice-thickness cells are interpolated, and the product's inputs represent different observation periods, approximately 2007–2022 overall. Bed detail is therefore most dependable near survey lines and should not be read as uniformly measured to 500-m resolution.

East Antarctica

High continental interior

A larger shield-and-plateau sector carries most of the ice and contains both buried highlands and deep basins.

West Antarctica

Marine-based basins

Large areas of bed lie below sea level between the Antarctic Peninsula, Ross Sea, and Weddell Sea margins.

Margin

Grounding zone

The grounding line marks the transition from ice supported by rock to shelf ice floating in seawater; it is not the same as the calving front.

Geology & History

Ancient crust beneath a young ice landscape

Only about one percent of Antarctica's rock base is exposed, so its geology is reconstructed from coastal and mountain outcrops, airborne radar, gravity and magnetic surveys, seismic measurements, and drilling. East Antarctica contains an ancient shield with rocks up to about four billion years old. West Antarctica is geologically younger and more fragmented, with multiple crustal blocks and a history that includes rifting and volcanism. The Transantarctic Mountains stand along the boundary between these contrasting provinces.[5]

Antarctica was once part of Gondwana. Its separation from Australia began around 85 million years ago and was complete by about 30 million years ago according to the Australian Antarctic Program.[5] Continental-scale ice growth was not a single instantaneous event: the major expansion across the Eocene–Oligocene transition occurred about 34 million years ago. Modelling and geological evidence identify falling atmospheric carbon dioxide as a principal driver, while changing ocean gateways and the emerging ice sheet altered Southern Ocean circulation.[6]

Since then, repeated advances and retreats have eroded troughs, overdeepened basins, deposited sediment on the continental shelf, and left older landscapes preserved beneath cold-based interior ice. The present desert surface is therefore the product of both inherited tectonic relief and long-running glacial erosion and deposition.

Drainage

Ice catchments instead of river basins

Antarctica has no continent-spanning surface-river network. Its principal drainage is the movement of solid ice. Snow accumulates, compacts first into firn—old granular snow—and then into glacier ice. Gravity carries ice away from high domes and divides. Motion is slow near broad summits, commonly centimetres to metres per year, but narrows into ice streams and outlet glaciers that can move hundreds of metres or kilometres per year near the coast.[7]

The direction is broadly radial but bed relief organizes distinct catchments. Ice crosses the Transantarctic Mountains through major outlets to the Ross Ice Shelf; the West Antarctic interior drains toward the Ross, Weddell, Amundsen, and Bellingshausen seas. Pine Island and Thwaites glaciers are two major West Antarctic pathways to the Amundsen Sea.[8] At a grounding line the ice begins to float; farther seaward it may spread through an ice shelf before basal melting or calving transfers ice and freshwater to the ocean.

Ice shelves do not themselves raise sea level when floating ice melts, but they exert back stress that slows grounded tributary ice. Weakening or loss of a shelf can therefore accelerate upstream discharge.[9] Shelf-front position, grounding-zone position, glacier speed, snow accumulation, and basal melt all vary, so no one coastline or ice-area figure should be presented as timeless.

Liquid Water

Surface melt and hidden drainage

Surface liquid water is strongly seasonal and concentrated toward lower, milder margins, especially the Antarctic Peninsula and some coastal and shelf surfaces. Melt ponds and streams can refreeze, drain through fractures, or contribute to shelf break-up. Across the high interior, annual mean temperatures remain far below freezing and surface melting is rare.

Liquid water is more widespread beneath the ice than the surface suggests. Geothermal heat, friction, and pressure allow basal melting; water then follows hydraulic gradients set jointly by bed elevation and the weight of the overlying ice. A 2016 scientific review catalogued 402 published subglacial lakes and documented active lakes that fill and drain, sometimes transferring water hundreds of kilometres and altering ice motion.[10] Lake Vostok is the best-known deep-interior example, but active drainage is also found nearer ice-stream onset zones.

These systems are not ordinary exposed rivers or lakes. Their locations and volumes are inferred from radio-echo sounding, seismic data, and small changes in ice-surface height measured by satellites. The mapped extent of an “active lake” can therefore be less certain than the existence of a drainage event.

Climate

A steep coast-to-plateau moisture gradient

Antarctic aridity comes from several reinforcing controls. Very cold air carries little water vapour; the high interior is remote from open-ocean moisture; and subsiding air over the plateau suppresses cloud. The surrounding Southern Ocean storm belt supplies much more moisture to coastal slopes, where uplift produces snowfall, than to the interior. Elevation also helps keep the plateau cold: the Australian Antarctic Program reports average annual temperatures of roughly −10°C at the coast and −60°C over the highest interior.[3]

The best interpretable precipitation figures are water-equivalent estimates, not snow depth. The same source estimates an Antarctic mean near 150 mm water equivalent per year, less than 50 mm on the elevated plateau, generally more than 200 mm near the coast, and more than 1,000 mm in the wettest area near the Bellingshausen Sea.[3] Snow depth can be several times larger and varies with density, so “millimetres of snow” and “millimetres water equivalent” are not interchangeable.

Radiative cooling creates dense air that drains downslope as katabatic wind. Valleys and coastal slopes can accelerate and converge that flow; coastal low-pressure systems can strengthen it further. Wind then redistributes or sublimates snow, leaving scoured blue-ice and exposed-rock surfaces beside deep drifts. This transport makes gauge-based snowfall particularly difficult to measure and helps explain why accumulation is not simply equal to precipitation at a point.[3]

Connections

From polar plateau to ocean margin

The Antarctic Desert belongs in the Desert Hub because precipitation scarcity and limited available liquid water define the terrestrial environment even where frozen water storage is immense. Compare the Arctic Desert, a discontinuous dryland around an ocean, and the Gobi Desert, a cold-winter continental dryland with exposed rock, gravel, and sediment rather than a continent-scale ice sheet.

Its defining physical sequence is snowfall on high divides, compaction into ice, flow through bed-controlled catchments, transition at the grounding line, and loss through shelf-bottom melting or calving. That sequence links atmosphere, rock relief, ice, subglacial water, and the Southern Ocean; it is more informative than treating the region as a uniform white surface.

References

Sources and measurement notes

  1. Australian Antarctic Program, “Antarctic geography and geology” (continental area and mean elevation; page updated 27 October 2020; accessed 29 August 2026).
  2. Pritchard, H. D. et al., “Bedmap3 updated ice bed, surface and thickness gridded datasets for Antarctica”, Scientific Data 12, 414 (2025). The paper documents the 500-m grid, g104c geoid, mask dates, ice volume, sea-level equivalent, interpolation, and uncertainty.
  3. Australian Antarctic Program, “Antarctic weather” (temperature, katabatic winds, and estimated snow accumulation in millimetres water equivalent; page updated 18 February 2019; accessed 29 August 2026).
  4. Peel, M. C., Finlayson, B. L. & McMahon, T. A., “Updated world map of the Köppen–Geiger climate classification”, Hydrology and Earth System Sciences 11, 1633–1644 (2007). Antarctic coverage limitations are stated in the paper.
  5. Australian Antarctic Program, “Antarctic geology” (East–West geological contrast, exposed rock, Transantarctic Mountains, and Gondwana separation; updated 27 October 2020; accessed 29 August 2026).
  6. Goldner, A., Herold, N. & Huber, M., “Antarctic glaciation caused ocean circulation changes at the Eocene–Oligocene transition”, Nature 511, 574–577 (2014).
  7. National Snow and Ice Data Center, “Ice Sheet Science” (ice-flow controls, speed ranges, outlet glaciers, and shelf transition; accessed 29 August 2026).
  8. NASA Earth Observatory, “The Wide View of a Shrinking Glacier: Retreat at Pine Island” (Pine Island and Thwaites drainage to the Amundsen Sea; published 9 April 2019, updated 10 February 2026; accessed 29 August 2026).
  9. National Snow and Ice Data Center, “Quick Facts About Ice Shelves” (floating-shelf definition, buttressing, calving, and glacier response; accessed 29 August 2026).
  10. Siegert, M. J. et al., “Recent advances in understanding Antarctic subglacial lakes and hydrology”, Philosophical Transactions of the Royal Society A 374 (2016).