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Thresholds of Temperature and Time for Mars Sample Return: Final Report of The Mars Sample Return Temperature-Time Tiger TeamThe time-temperature tiger team (T4) was chartered by NASA and ESA to evaluate the risks to the scientific return of the MSR samples if they are exposed to temperatures between +30 and +60 ⁰C for different amounts of time. This team consists of 13 scientists, who were selected based on their scientific background to represent the scientific disciplines that are expected to be the ones that will be the most affected if such heating were to happen. The expertise of the team will help to understand whether exposing the MSR samples to temperatures between +30 and +60 ⁰C will pose any risk to the sample integrity and therefore, to future scientific investigations.
Key processes identified by the T4 were: the release of volatiles by desorption and sublimation and release from condensed phases (interiors, decomposition, dehydration); chemical reactions including gas-gas and gas-solid; deliquescence of hygroscopic salts; acid/base interactions (potential for extreme pH conditions); aqueous redox reactions, isotopic exchange (aqueous phases, minerals, gasses, organic phases); condensation and freezing (in the after-heating cooling phase) and interactions with the sample tube materials. There is potential for multiple interactions and overlapping effects.
For inorganic materials and the records they represent, over both long time scales (hours to days) and short time scales (minutes to hours) no temperature excursion above +30 °C could be accommodated without loss of science (Figure 1.1). While there will be some robust constituents (feldspars, quartz, pyroxenes, etc.) that are unaffected, there will also be some less robust constituents (salts, phyllosilicates, radicals, etc.) that are affected across all temperature ranges ≤60 °C.
For organic materials, in particular organic biosignatures, the risks reflect that preservation is reliant on a number of processes, and a change in one component within a sample tube can affect another. For organic materials, over long timescales of hours to days no temperature excursion above +30 °C could be accommodated without loss of science, but over shorter time scales (minutes to hours), raising the temperature to 40 °C could be manageable without major disruption to science, whereas temperatures above 40 °C would lead to significant losses. The consideration of these findings by the MSR team will help to maintain the fidelity of samples returned from Mars in the future and maximize scientific return when analyzed in Earth laboratories.
Document ID
20220010268
Acquisition Source
Goddard Space Flight Center
Document Type
White Paper
Authors
Mark A Sephton
(Imperial College London London, United Kingdom)
Kate Freeman
(Pennsylvania State University State College, United States)
Lindsay Hays
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
Fiona Thiessen
(European Space Research and Technology Centre Noordwijk-Binnen, Netherlands)
Kathleen Benison
(West Virginia University Morgantown, West Virginia, United States)
Brandi Carrier
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Jason Dworkin
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Mihaela Glamoclija ORCID
(Rutgers, The State University of New Jersey New Brunswick, United States)
Raina Gough
(University of Colorado Boulder Boulder, United States)
Silvano Onofri
(Tuscia University Viterbo, Italy)
Ron Peterson
(Queen's University Kingston, Ontario, Canada)
Richard Quinn
(Ames Research Center Mountain View, California, United States)
Sara Russell ORCID
(Natural History Museum London, Westminster, United Kingdom)
Eva E Stüeken ORCID
(University of St Andrews St Andrews, United Kingdom)
Michael Velbel
(Michigan State University East Lansing, United States)
Mikhail Zolotov
(Arizona State University Tempe, United States)
Date Acquired
July 6, 2022
Publication Date
March 6, 2022
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
WBS: 527813.02.01.01.31
CONTRACT_GRANT: J-090011
CONTRACT_GRANT: J-090007
CONTRACT_GRANT: 1549140
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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NASA Peer Committee
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