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ChemCam Investigation of the Last Four MSL Drill Sites in the Murray Formation, Gale Crater, MarsThis study utilizes ChemCam data for outcrop surfaces, drill hole walls, tailings, and dump piles in the Middle Murray Formation to investigate chemical variations with depth in the drill holes and pos-sible effects of the drilling and sample processing. This work is a continuation of similar work on drill sites at Yellowknife Bay [1], the Pahrump Hills [2], and the Stimson Formation [3].
Document ID
20180006500
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Jackson, R. S. (New Mexico Univ. Albuquerque, NM, United States)
Wiens, R. C. (Los Alamos National Laboratory Los Alamos, NM, United States)
Beegle, L. W. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rampe, E. B. (NASA Johnson Space Center Houston, TX, United States)
Johnson, J. R. (Johns Hopkins Univ. Laurel, MD, United States)
Forni, O. (Institut de Recherche en Astrophysique et Planetologie (UMR) Toulouse, France)
Newsom, H. E. (New Mexico Univ. Albuquerque, NM, United States)
Date Acquired
October 18, 2018
Publication Date
March 19, 2018
Subject Category
General
Report/Patent Number
JSC-E-DAA-TN53595
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.

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