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A Carbonaceous Chondrite Based Simulant of Phobos

Rickman, D.; Patel, M.; Pearson, V. K.; Wilson, S. and Edmunson, J. (2017). A Carbonaceous Chondrite Based Simulant of Phobos. In: 15th Biennial ASCE Conference on Engineering, Science, Construction, and Operations in Challenging Environments, 11-15 Apr 2016, Orlando, Florida, American Society of Civil Engineers.

DOI (Digital Object Identifier) Link: https://doi.org/10.1061/9780784479971.054
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Abstract

In support of an ESA-funded concept study considering a sample return mission, a simulant of the Martian moon Phobos was needed. There are no samples of the Phobos regolith, therefore none of the four characteristics normally used to design a simulant are explicitly known for Phobos. Because of this, specifications for a Phobos simulant were based on spectroscopy, other remote measurements, and judgment. A composition based on the Tagish Lake meteorite was assumed. The requirement that sterility be achieved, especially given the required organic content, was unusual and problematic. The final design mixed JSC-1A, antigorite, pseudo-agglutinates and gilsonite. Sterility was achieved by radiation in a commercial facility.

Item Type: Conference or Workshop Item
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 56339
SWORD Depositor: Jisc Publications-Router
Depositing User: Jisc Publications-Router
Date Deposited: 31 Aug 2018 11:41
Last Modified: 17 Jun 2019 10:34
URI: http://oro.open.ac.uk/id/eprint/56339
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