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Detailed Reference Information |
Zimbelman, J.R. (2000). Non-active dunes in the Acheron Fossae Region of Mars between the Viking and Mars Global Surveyor eras. Geophysical Research Letters 27: doi: 10.1029/1999GL008399. issn: 0094-8276. |
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Comparison of a high resolution Viking image (422B10; 8 m/pixel) with a Mars Orbiter Camera image (SP2-502/06; 5.6 m/pixel) of dunes in the Acheron Fossae region of Mars (38 ¿N, 135 ¿W) reveals that the dunes moved <1 pixel during a span of almost 21 Earth years. Very shallow illumination in the MOC image indicates the dunes are <1.5 m high. The images indicate that any movement of these Martian dunes is <0.4 m/yr, a rate that is less than the documented movement of comparable dunes on Earth by a factor of up to 200. The Acheron Fossae dunes occur within a region of low thermal inertia, indicating that the dunes may be stabilized by a pervasive dust cover. Alternatively, the saltation threshold was not exceeded significantly at this location in more than 20 years. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Hydrology, Geomorphology, Planetology, Solid Surface Planets, Erosion and weathering, Planetology, Solid Surface Planets, Surface materials and properties, Planetology, Solar System Objects, Mars |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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