The instability of a south polar cap on Mars composed of carbon dioxide

被引:54
作者
Nye, JF
Durham, WB
Schenk, PM
Moore, JM
机构
[1] Univ Bristol, HH Wills Phys Lab, Bristol BS8 1TL, Avon, England
[2] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[3] Lunar & Planetary Inst, Houston, TX 77058 USA
[4] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
基金
美国国家航空航天局;
关键词
Mars; surface; ices; geophysics;
D O I
10.1006/icar.1999.6306
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
If the martian south polar cap were composed of solid carbon dioxide, would it be sufficiently stable against collapse under its own weight? This question is examined in the light of new experiments on the creep of solid carbon dioxide and new high-resolution topographic mapping of the south polar cap. The conclusion from a simple model is that, with the strongest of three flow laws compatible with the measurements, CO2 is strong enough to support a cap of this material with thickness about 1800 m for 10(7) years or more, which is the age suggested by the cratering record. However, none of the three possible flow laws will allow a 3000-m cap, the thickness suggested by stereogrammetry, to survive for 10(7) years, indicating that the south polar ice cap is probably not composed of pure CO2 ice. (C) 2000 Academic Press.
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页码:449 / 455
页数:7
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