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Subsurface Volatile Deposition on Mars

Patel, N.; Hagermann, A.; Lewis, S. R.; Kaufmann, E. and Balme, M. (2018). Subsurface Volatile Deposition on Mars. In: European Planetary Science Congress 2018, 16-21 Sep 2018, Berlin, Germany.

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Abstract

We have modelled the transport of heat in the martian regolith, taking into account the change in thermal properties caused by an increase in water ice content. Under these conditions we have found that the addition of water ice allows for increased ice formation at depth, rather than under the assumption that thermal properties are unchanged. This is important because it will affect estimates of global subsurface volatile deposition.

Item Type: Conference or Workshop Item
Copyright Holders: 2018 The Authors
ISSN: 0019-1035
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
Item ID: 58676
Depositing User: Narissa Patel
Date Deposited: 21 Jan 2019 16:34
Last Modified: 03 May 2019 04:14
URI: http://oro.open.ac.uk/id/eprint/58676
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