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Mineralogy of a mudstone at Yellowknife Bay, Gale crater, Mars.

Authors :
Vaniman DT
Bish DL
Ming DW
Bristow TF
Morris RV
Blake DF
Chipera SJ
Morrison SM
Treiman AH
Rampe EB
Rice M
Achilles CN
Grotzinger JP
McLennan SM
Williams J
Bell JF 3rd
Newsom HE
Downs RT
Maurice S
Sarrazin P
Yen AS
Morookian JM
Farmer JD
Stack K
Milliken RE
Ehlmann BL
Sumner DY
Berger G
Crisp JA
Hurowitz JA
Anderson R
Des Marais DJ
Stolper EM
Edgett KS
Gupta S
Spanovich N
Source :
Science (New York, N.Y.) [Science] 2014 Jan 24; Vol. 343 (6169), pp. 1243480. Date of Electronic Publication: 2013 Dec 09.
Publication Year :
2014

Abstract

Sedimentary rocks at Yellowknife Bay (Gale crater) on Mars include mudstone sampled by the Curiosity rover. The samples, John Klein and Cumberland, contain detrital basaltic minerals, calcium sulfates, iron oxide or hydroxides, iron sulfides, amorphous material, and trioctahedral smectites. The John Klein smectite has basal spacing of ~10 angstroms, indicating little interlayer hydration. The Cumberland smectite has basal spacing at both ~13.2 and ~10 angstroms. The larger spacing suggests a partially chloritized interlayer or interlayer magnesium or calcium facilitating H2O retention. Basaltic minerals in the mudstone are similar to those in nearby eolian deposits. However, the mudstone has far less Fe-forsterite, possibly lost with formation of smectite plus magnetite. Late Noachian/Early Hesperian or younger age indicates that clay mineral formation on Mars extended beyond Noachian time.

Details

Language :
English
ISSN :
1095-9203
Volume :
343
Issue :
6169
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
24324271
Full Text :
https://doi.org/10.1126/science.1243480