Structure, stratigraphy, and origin of Husband Hill, Columbia Hills, Gusev Crater, Mars

被引:39
|
作者
McCoy, T. J. [1 ]
Sims, M. [2 ]
Schmidt, M. E. [1 ]
Edwards, L. [2 ]
Tornabene, L. L. [3 ]
Crumpler, L. S. [8 ]
Cohen, B. A. [4 ]
Soderblom, L. A. [5 ]
Blaney, D. L. [6 ]
Squyres, S. W. [14 ]
Arvidson, R. E. [7 ]
Rice, J. W., Jr. [13 ]
Treguier, E. [9 ]
d'Uston, C. [9 ]
Grant, J. A. [10 ]
McSween, H. Y., Jr. [12 ]
Golombek, M. P. [6 ]
Haldemann, A. F. C. [11 ]
de Souza, P. A., Jr. [15 ]
机构
[1] Smithsonian Inst, Natl Museum Amer Hist, Dept Mineral Sci, Washington, DC 20560 USA
[2] NASA Ames, Intelligent Syst Div, Moffett Field, CA 94035 USA
[3] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[4] Univ New Mexico, Inst Meteorit, Albuquerque, NM 87131 USA
[5] US Geol Survey, Branch Astrogeol, Flagstaff, AZ 86001 USA
[6] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[7] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[8] New Mexico Museum Nat Hist & Sci, Albuquerque, NM 87104 USA
[9] Ctr Etud Spatiale Rayonnements, OMP, F-31400 Toulouse, France
[10] Smithsonian Inst, Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
[11] European Space Technol Ctr, European Space Agcy, HME ME, NL-2200 AG Noordwijk, Netherlands
[12] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN 37996 USA
[13] Arizona State Univ, Dept Geol Sci, Tempe, AZ 85287 USA
[14] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[15] Vallourec Res Ctr, Aulnoye Aymeries, France
关键词
D O I
10.1029/2007JE003041
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The strike and dip of lithologic units imaged in stereo by the Spirit rover in the Columbia Hills using three-dimensional imaging software shows that measured dips (15-32 degrees) for bedding on the main edifice of the Columbia Hill are steeper than local topography (similar to 8-10 degrees). Outcrops measured on West Spur are conformable in strike with shallower dips (7-15 degrees) than observed on Husband Hill. Dips are consistent with observed strata draping the Columbia Hills. Initial uplift was likely related either to the formation of the Gusev Crater central peak or ring or through mutual interference of overlapping crater rims. Uplift was followed by subsequent draping by a series of impact and volcaniclastic materials that experienced temporally and spatially variable aqueous infiltration, cementation, and alteration episodically during or after deposition. West Spur likely represents a spatially isolated depositional event. Erosion by a variety of processes, including mass wasting, removed tens of meters of materials and formed the Tennessee Valley primarily after deposition. This was followed by eruption of the Adirondack-class plains basalt lava flows which embayed the Columbia Hills. Minor erosion, impact, and aeolian processes have subsequently modified the Columbia Hills.
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页数:14
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