| タイトル | SAM-Like Evolved Gas Analyses of Phyllosilicate Minerals and Applications to SAM Analyses of the Sheepbed Mudstone, Gale Crater, Mars |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140012601 |
| 著者（英） | Atreya, S. K.; Bish, D. L.; Brunner, B.; Mahaffy, P. R.; Archer, P. D.; Franz, H. B.; Morris, R. V.; McAdam, A. C.; Sutter, B.; Stern, J. C.; Eigenbrode, J. L.; Ming , D. W. |
| 発行日 | 2014-03-17 |
| 言語 | eng |
| 内容記述 | While in Yellowknife Bay, the Mars Science Laboratory Curiosity rover collected two drilled samples, John Klein (hereafter "JK") and Cumberland ("CB"), from the Sheepbed mudstone, as well as a scooped sample from the Rocknest aeolian bedform ("RN"). These samples were sieved by Curiosity's sample processing system and then several subsamples of these materials were delivered to the Sample Analysis at Mars (SAM) instrument suite and the CheMin X-ray diffraction/X-ray fluorescence instrument. CheMin provided the first in situ X-ray diffraction-based evidence of clay minerals on Mars, which are likely trioctahedral smectites (e.g., Fe-saponite) and comprise ~20 wt% of the mudstone samples [1]. SAM's evolved gas analysis (EGA) mass spectrometry analyses of JK and CB subsamples, as well as RN subsamples, detected H2O, CO2, O2, H2, SO2, H2S, HCl, NO, OCS, CS2 and other trace gases evolved during pyrolysis. The identity of evolved gases and temperature( s) of evolution can augment mineral detection by CheMin and place constraints on trace volatile-bearing phases present below the CheMin detection limit or those phases difficult to characterize with XRD (e.g., X-ray amorphous phases). Here we will focus on the SAM H2O data, in the context of CheMin analyses, and comparisons to laboratory SAM-like analyses of several phyllosilicate minerals including smectites. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | JSC-CN-30380 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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