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Contamination Knowledge Strategy for the Mars 2020 Sample-Collecting RoverThe Mars 2020 rover will collect carefully selected samples of rock and regolith as it explores a potentially habitable ancient environment on Mars. Using the drill, rock cores and regolith will be collected directly into ultraclean sample tubes that are hermetically sealed and, later, deposited on the surface of Mars for potential return to Earth by a subsequent mission. Thorough characterization of any contamination of the samples at the time of their analysis will be essential for achieving the objectives of Mars returned sample science (RSS). We refer to this characterization as contamination knowledge (CK), which is distinct from contamination control (CC). CC is the set of activities that limits the input of contaminating species into a sample, and is specified by requirement thresholds. CK consists of identifying and characterizing both potential and realized contamination to better inform scientific investigations of the returned samples. Based on lessons learned by other sample return missions with contamination-sensitive scientific objectives, CC needs to be "owned" by engineering, but CK needs to be "owned" by science. Contamination present at the time of sample analysis will reflect the sum of contributions from all contamination vectors up to that point in time. For this reason, understanding the integrated history of contamination may be crucial for deciphering potentially confusing contaminant-sensitive observations. Thus, CK collected during the Mars sample return (MSR) campaign must cover the time period from the initiation of hardware construction through analysis of returned samples in labs on Earth. Because of the disciplinary breadth of the scientific objectives of MSR, CK must include a broad spectrum of contaminants covering inorganic (i.e., major, minor, and trace elements), organic, and biological molecules and materials.
Document ID
20170001707
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Farley, K. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Williford, K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Beaty, D W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
McSween, H. Y.
(Tennessee Univ. Knoxville, TN, United States)
Czaja, A. D.
(Cincinnati Univ. OH, United States)
Goreva, Y. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Hausrath, E.
(Nevada Univ. Las Vegas, NV, United States)
Herd, C. D. K.
(Alberta Univ. Edmonton, Alberta, Canada)
Humayun, M.
(Florida State Univ. Tallahassee, FL, United States)
McCubbin, F. M.
(NASA Johnson Space Center Houston, TX, United States)
McLennan, S. M.
(Stony Brook Univ. Stony Brook, NY, United States)
Pratt, L. M.
(Indiana Univ. Bloomington, IN, United States)
Sephton, M. A.
(Imperial Coll. of London London, United Kingdom)
Steele, A.
(Carnegie Institution of Washington Washington, DC, United States)
Weiss, B. P.
(Massachusetts Inst. of Tech. Boston, MA, United States)
Hays, L. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
February 22, 2017
Publication Date
March 20, 2017
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-38652
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 20, 2017
End Date: March 24, 2017
Sponsors: Universities Space Research Association, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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