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A method for choosing the best samples for Mars sample return
File | Description | Size | Format | |
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ast.2017.1744.pdf | Published version | 806.48 kB | Adobe PDF | View/Open |
Title: | A method for choosing the best samples for Mars sample return |
Authors: | Gordon, PR Sephton, MA |
Item Type: | Journal Article |
Abstract: | Success of a future Mars Sample Return mission will depend on the correct choice of samples. Pyrolysis-FTIR can be employed as a triage instrument for Mars Sample Return. The technique can thermally dissociate minerals and organic matter for detection. Identification of certain mineral types can determine the habitability of the depositional environment, past or present, while detection of organic matter may suggest past or present habitation. In Mars history, the Theiikian Era represents an attractive target for life search missions and the acquisition of samples. The acidic and increasingly dry Theiikian may have been habitable and followed a lengthy neutral and wet period in Mars history during which life could have originated and proliferated to achieve relatively abundant levels of biomass with a wide distribution. Moreover, the sulfate minerals produced in the Theiikian are also known to be good preservers of organic matter. We have used pyrolysis-FTIR and samples from a Mars analogue ferrous acid stream with a thriving ecosystem to test the triage concept. Pyrolysis-FTIR identifies those samples with the greatest probability of habitability and habitation. A three tier scoring system was developed based on the detection of i) organic signals, ii) carbon dioxide and water and iii) sulfur dioxide. The presence of each component is given a score of A, B or C depending on whether the substance has been detected, tentatively detected or not detected respectively. Single-step (for greatest possible sensitivity) or multi-step (for more diagnostic data) pyrolysis-FTIR methods can inform the assignments. The system allows the highest priority samples to be categorised as AAA (or A*AA if the organic signal is complex) while the lowest priority samples can be categorised as CCC. Our methods provide a mechanism to rank samples and identify those that should take the highest priority for return to Earth during a Mars Sample Return mission. |
Issue Date: | 1-May-2018 |
Date of Acceptance: | 29-Nov-2017 |
URI: | http://hdl.handle.net/10044/1/54414 |
DOI: | https://dx.doi.org/10.1089/ast.2017.1744 |
ISSN: | 1531-1074 |
Publisher: | Mary Ann Liebert |
Start Page: | 556 |
End Page: | 570 |
Journal / Book Title: | Astrobiology |
Volume: | 18 |
Issue: | 5 |
Copyright Statement: | © Peter R. Gordon and Mark A. Sephton, 2018; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited. |
Sponsor/Funder: | Science and Technology Facilities Council (STFC) |
Funder's Grant Number: | ST/N000560/1 |
Keywords: | Science & Technology Physical Sciences Life Sciences & Biomedicine Astronomy & Astrophysics Biology Geosciences, Multidisciplinary Life Sciences & Biomedicine - Other Topics Geology RECURRING SLOPE LINEAE PYROLYSIS-FTIR LIFE ANALOGS SEARCH RECORD ROCKS 0201 Astronomical And Space Sciences 0402 Geochemistry 0403 Geology |
Publication Status: | Published |
Online Publication Date: | 2018-02-14 |
Appears in Collections: | Earth Science and Engineering Faculty of Engineering |