HiRISE observations of gas sublimation-driven activity in Mars' southern polar regions: III. Models of processes involving translucent ice

被引:48
|
作者
Portyankina, Ganna [1 ]
Markiewicz, Wojciech J. [2 ]
Thomas, Nicolas [1 ]
Hansen, Candice J. [3 ]
Milazzo, Moses [4 ]
机构
[1] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
[2] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] US Geol Survey, Flagstaff, AZ 86001 USA
基金
瑞士国家科学基金会;
关键词
Mars; Polar caps; Ices; Surface; LABORATORY SIMULATION; CO2; ICE; BEHAVIOR; SPIDERS; IMAGER; WATER; DUST; CAP; TES;
D O I
10.1016/j.icarus.2009.08.029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Enigmatic surface features, known as 'spiders', found at high southern martian latitudes, are probably caused by sublimation-driven erosion under the seasonal carbon dioxide ice cap. The Mars Reconnaissance Orbiter (MRO) High Resolution Imaging Science Experiment (HiRISE) has imaged this terrain in unprecedented details throughout Southern spring. It has been postulated [Kieffer, H.H., Titus, T.N., Mullins, K.F., Christensen, P.R., 2000. J. Geophys. Res. 105, 9653-9700] that translucent CO2 slab ice traps gas sublimating at the ice surface boundary. Wherever the pressure is released the escaping gas jet entrains loose Surface material and carries it to the top of the ice where it is carried downslope and/or downwind and deposited in a fan shape. Here we model two stages of this scenario: first, the cleaning Of CO2 slab ice from dust, and then, the breaking of the slab ice plate under the pressure built below it by subliming ice. Our modeling results and analysis of HiRISE images support the gas jet hypothesis and show that Outbursts happen very early in spring. (C) 2009 Elsevier Inc. All rights reserved.
引用
收藏
页码:311 / 320
页数:10
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  • [3] HiRISE observations of gas sublimation-driven activity in Mars' southern polar regions: IV. Fluid dynamics models of CO2 jets
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