The 1997 spring regression of the Martian south polar cap: Mars Orbiter camera observations

被引:21
|
作者
James, PB [1 ]
Cantor, BA
Malin, MC
Edgett, K
Carr, MH
Danielson, GE
Ingersoll, AP
Davies, ME
Hartmann, WK
McEwen, AS
Soderblom, LA
Thomas, PC
Veverka, J
机构
[1] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA
[2] Malin Space Sci Syst, San Diego, CA 92191 USA
[3] US Geol Survey, Menlo Park, CA 91125 USA
[4] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[5] RAND Corp, Santa Monica, CA 90406 USA
[6] Planetary Sci Inst, Tucson, AZ 85719 USA
[7] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[8] US Geol Survey, Flagstaff, AZ 86001 USA
[9] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA
关键词
Mars atmosphere; Mars climate; Mars surface;
D O I
10.1006/icar.1999.6289
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Mars Orbiter cameras (MOC) on Mars Global. Surveyor observed the south polar cap of Mars during its spring recession in 1997. The images acquired by the wide angle cameras reveal a pattern of recession that is qualitatively similar to that observed by Viking in 1977 but that does differ in at least two respects. The 1977 recession in the 0 degrees to 120 degrees longitude sector was accelerated relative to the 1997 observations after L-S = 240 degrees; the Mountains of Mitchel also detached from the main cap earlier in 1997. Comparison of the MOC images with Mars Orbiter Laser Altimeter data shows that the Mountains of Mitchel feature is controlled by local topography. Relatively dark, low albedo regions well within the boundaries of the seasonal cap were observed to have red-to-violet ratios that characterize them as frost units rather than unfrosted or partially frosted ground; this suggests the possibility of regions covered by CO2 frost having different grain sizes. (C) 2000 Academic Press.
引用
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页码:410 / 418
页数:9
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