Seasonal erosion and restoration of Mars' northern polar dunes
Science
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Abstract
Despite radically different environmental conditions, terrestrial and martian dunes bear a strong resemblance, indicating that the basic processes of saltation and grainfall (sand avalanching down the dune slipface) operate on both worlds. Here, we show that martian dunes are subject to an additional modification process not found on Earth: springtime sublimation of Mars' CO 2 seasonal polar caps. Numerous dunes in Mars' north polar region have experienced morphological changes within a Mars year, detected in images acquired by the High-Resolution Imaging Science Experiment on the Mars Reconnaissance Orbiter. Dunes show new alcoves, gullies, and dune apron extension. This is followed by remobilization of the fresh deposits by the wind, forming ripples and erasing gullies. The widespread nature of these rapid changes, and the pristine appearance of most dunes in the area, implicates active sand transport in the vast polar erg in Mars' current climate.
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Seasonal erosion and restoration of Mars' northern polar dunes |
| Series title | Science |
| DOI | 10.1126/science.1197636 |
| Volume | 331 |
| Issue | 6017 |
| Year Published | 2011 |
| Language | English |
| Publisher | American Association for the Advancement of Science |
| Contributing office(s) | Astrogeology Science Center |
| Description | 4 p. |
| Larger Work Type | Article |
| Larger Work Subtype | Journal Article |
| Larger Work Title | Science |
| First page | 575 |
| Last page | 578 |
| Other Geospatial | Mars |
| Google Analytic Metrics | Metrics page |