Mineralogy of an ancient lacustrine mudstone succession from the Murray formation, Gale crater, Mars

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Date
2017-05-12
Authors
Rampe, Elizabeth
Craig, Patricia I.
https://orcid.org/0000-0003-4080-4997
Treiman, Allan H.
https://orcid.org/0000-0002-8073-2839
Journal Title
Journal ISSN
Volume Title
Publisher
Elsevier
Abstract
The Mars Science Laboratory Curiosity rover has been traversing strata at the base of Aeolis Mons (informally known as Mount Sharp) since September 2014. The Murray formation makes up the lowest exposed strata of the Mount Sharp group and is composed primarily of finely laminated lacustrine mudstone intercalated with rare crossbedded sandstone that is prodeltaic or fluvial in origin. We report on the first three drilled samples from the Murray formation, measured in the Pahrump Hills section. Rietveld refinements and FULLPAT full pattern fitting analyses of X-ray diffraction patterns measured by the MSL CheMin instrument provide mineral abundances, refined unit-cell parameters for major phases giving crystal chemistry, and abundances of X-ray amorphous materials.
Description
Keywords
Mars (Planet), X-ray diffraction imaging, Diagenesis
Citation
Rampe, E.B., D.W. Ming, D.F. Blake, T.F. Bristow, S.J. Chipera, J.P. Grotzinger, R.V. Morris, et al. 2017. "Mineralogy of an ancient lacustrine mudstone succession from the Murray formation, Gale crater, Mars". Earth and Planetary Science Letters. 471: 172-185.