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X-Ray Computed Tomography: The First Step in Mars Sample Return ProcessingThe Mars 2020 rover mission will collect and cache samples from the martian surface for possible retrieval and subsequent return to Earth. If the samples are returned, that mission would likely present an opportunity to analyze returned Mars samples within a geologic context on Mars. In addition, it may provide definitive information about the existence of past or present life on Mars. Mars sample return presents unique challenges for the collection, containment, transport, curation and processing of samples [1] Foremost in the processing of returned samples are the closely paired considerations of life detection and Planetary Protection. In order to achieve Mars Sample Return (MSR) science goals, reliable analyses will depend on overcoming some challenging signal/noise-related issues where sparse martian organic compounds must be reliably analyzed against the contamination background. While reliable analyses will depend on initial clean acquisition and robust documentation of all aspects of developing and managing the cache [2], there needs to be a reliable sample handling and analysis procedure that accounts for a variety of materials which may or may not contain evidence of past or present martian life. A recent report [3] suggests that a defined set of measurements should be made to effectively inform both science and Planetary Protection, when applied in the context of the two competing null hypotheses: 1) that there is no detectable life in the samples; or 2) that there is martian life in the samples. The defined measurements would include a phased approach that would be accepted by the community to preserve the bulk of the material, but provide unambiguous science data that can be used and interpreted by various disciplines. Fore-most is the concern that the initial steps would ensure the pristine nature of the samples. Preliminary, non-invasive techniques such as computed X-ray tomography (XCT) have been suggested as the first method to interrogate and characterize the cached samples without altering the materials [1,2]. A recent report [4] indicates that XCT may minimally alter samples for some techniques, and work is needed to quantify these effects, maximizing science return from XCT initial analysis while minimizing effects.
Document ID
20170001336
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Welzenbach, L. C.
(Open Univ. Milton Keynes, United Kingdom)
Fries, M. D.
(NASA Johnson Space Center Houston, TX, United States)
Grady, M. M.
(Open Univ. Milton Keynes, United Kingdom)
Greenwood, R. C.
(Open Univ. Milton Keynes, United Kingdom)
McCubbin, F. M.
(NASA Johnson Space Center Houston, TX, United States)
Zeigler, R. A.
(NASA Johnson Space Center Houston, TX, United States)
Smith, C. L.
(Natural History Museum London, United Kingdom)
Steele, A.
(Carnegie Institution of Washington Washington, DC, United States)
Date Acquired
February 7, 2017
Publication Date
March 20, 2017
Subject Category
Instrumentation And Photography
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-38659
Report Number: JSC-CN-38659
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: Lunar and Planetary Inst., Universities Space Research Association
Distribution Limits
Public
Copyright
Public Use Permitted.
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