GSTDTAP  > 气候变化
DOI10.1029/2018GL079073
Sand Mineralogy Within the Bagnold Dunes, Gale Crater, as Observed In Situ and From Orbit
Rampe, E. B.1; Lapotre, M. G. A.2; Bristow, T. F.3; Arvidson, R. E.4; Morris, R. V.1; Achilles, C. N.5; Weitz, C.6; Blake, D. F.3; Ming, D. W.1; Morrison, S. M.7; Vaniman, D. T.6; Chipera, S. J.8; Downs, R. T.5; Grotzinger, J. P.9; Hazen, R. M.7; Peretyazhko, T. S.10; Sutter, B.10; Tu, V.10; Yen, A. S.11; Horgan, B.12; Castle, N.13; Craig, P. I.6; Des Marais, D. J.3; Farmer, J.14; Gellert, R.15; McAdam, A. C.16; Morookian, J. M.11; Sarrazin, P. C.17; Treiman, A. H.13
2018-09-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:18页码:9488-9497
文章类型Article
语种英语
国家USA; Canada
英文摘要

Curiosity investigated active eolian sands near linear dunes during Phase 2 of the Bagnold Dunes campaign in Gale crater, Mars. Ogunquit Beach, a sample scooped from a large-ripple trough within the Mount Desert Island ripple field and delivered to the Chemistry and Mineralogy (CheMin) X-ray diffraction instrument, is dominated by basaltic igneous minerals and X-ray amorphous materials. CheMin mineralogy of the Gobabeb sample acquired at a large-ripple crest on the Namib barchan dune during Phase 1 is similar to Ogunquit Beach. Ogunquit Beach, however, contains more plagioclase and Gobabeb contains more olivine. Compact Reconnaissance Imaging Spectrometer for Mars (CRISM)-based estimates of mineralogy at the optical surface of Namib Dune and Mount Desert Island demonstrate that surface sands are enriched in olivine and depleted in plagioclase over Mount Desert Island relative to Namib Dune. Differences between CheMin-derived and CRISM-derived mineralogies suggest sorting by grain size on bedform to dune field scales. Crystal chemistry from CheMin suggests contributions from multiple igneous sources and the local bedrock.


Plain Language Summary Remote sensing data from orbit indicate that wind-blown sands in the Bagnold Dune Field in Gale crater, Mars, are sorted by their composition. The Mars Science Laboratory Curiosity rover studied the Bagnold Dune Field at two locations to investigate the chemical and mineral composition of the sands and why they are sorted across the dune field. Data from Curiosity show distinct differences between the minerals in the upwind portion of the dune field compared to the downwind portion, but these differences are not the same as those observed from orbit. The scale and location of the sampling by Curiosity compared to orbiters explains the discrepancy between the two techniques. Results from both techniques suggest subtle differences in mineralogy within a single dune and across the dune field that can be explained by sorting from wind and contribution from the erosion of local bedrock.


英文关键词Mars eolian mineralogy X-ray diffraction CheMin CRISM
领域气候变化
收录类别SCI-E
WOS记录号WOS:000447761300018
WOS关键词MARS ; SURFACE
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
被引频次:50[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/28610
专题气候变化
作者单位1.NASA, Astromat Res & Explorat Sci Div, Johnson Space Ctr, Houston, TX 77058 USA;
2.Harvard Univ, Dept Earth & Planetary Sci, 20 Oxford St, Cambridge, MA 02138 USA;
3.NASA, Ames Res Ctr, Moffett Field, CA 94035 USA;
4.Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA;
5.Univ Arizona, Dept Geosci, Tucson, AZ 85721 USA;
6.Planetary Sci Inst, Tucson, AZ USA;
7.Carnegie Inst Sci, Geophys Lab, Washington, DC 20005 USA;
8.Chesapeake Energy, Oklahoma City, OK USA;
9.CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA;
10.NASA, Jacobs, Johnson Space Ctr, Houston, TX USA;
11.CALTECH, Jet Prop Lab, Pasadena, CA USA;
12.Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA;
13.Lunar & Planetary Inst, Houston, TX USA;
14.Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA;
15.Univ Guelph, Dept Phys, Guelph, ON, Canada;
16.Goddard Space Flight Ctr, Greenbelt, MD USA;
17.SETI Inst, Mountain View, CA USA
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Rampe, E. B.,Lapotre, M. G. A.,Bristow, T. F.,et al. Sand Mineralogy Within the Bagnold Dunes, Gale Crater, as Observed In Situ and From Orbit[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(18):9488-9497.
APA Rampe, E. B..,Lapotre, M. G. A..,Bristow, T. F..,Arvidson, R. E..,Morris, R. V..,...&Treiman, A. H..(2018).Sand Mineralogy Within the Bagnold Dunes, Gale Crater, as Observed In Situ and From Orbit.GEOPHYSICAL RESEARCH LETTERS,45(18),9488-9497.
MLA Rampe, E. B.,et al."Sand Mineralogy Within the Bagnold Dunes, Gale Crater, as Observed In Situ and From Orbit".GEOPHYSICAL RESEARCH LETTERS 45.18(2018):9488-9497.
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