Study of the Formation of Duricrusts on the Martian Surface and Their Effect on Sampling Equipment
Kömle, N, Pitcher, Craig, Gao, Yang and Richter, L (2017) Study of the Formation of Duricrusts on the Martian Surface and Their Effect on Sampling Equipment Icarus, 281. pp. 220-227.
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Abstract
The Powdered Sample Dosing and Distribution System (PSDDS) of the ExoMars rover will be required to handle and contain samples of Mars regolith for long periods of time. Cementation of the regolith, caused by water and salts in the soil, results in clumpy material and a duricrust layer forming on the surface. It is therefore possible that material residing in the sampling system may cement, and could potentially hinder its operation. There has yet to be an investigation into the formation of duricrusts under simulated Martian conditions, or how this may affect the performance of sample handling mechanisms. Therefore experiments have been performed to create a duricrust and to explore the cementation of Mars analogues, before performing a series of tests on a qualification model of the PSDDS under simulated Martian conditions.It was possible to create a consolidated crust of cemented material several millimetres deep, with the material below remaining powder-like. It was seen that due to the very low permeability of the Montmorillonite component material, diffusion of water through the material was quickly blocked, resulting in a sample with an inhomogeneous water content. Additionally, samples with a water mass content of 10% or higher would cement into a single solid piece. Finally, tests with the PSDDS revealed that samples with a water mass content of just 5% created small clumps with significant internal cohesion, blocking the sample funnels and preventing transportation of the material. These experiments have highlighted that the cementation of regolith in Martian conditions must be taken into consideration in the design of sample handling instruments.
Item Type: | Article | |||||||||||||||
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Subjects : | Electronic Engineering | |||||||||||||||
Divisions : | Faculty of Engineering and Physical Sciences > Electronic Engineering > Surrey Space Centre | |||||||||||||||
Authors : |
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Date : | 1 January 2017 | |||||||||||||||
DOI : | 10.1016/j.icarus.2016.08.019. | |||||||||||||||
Copyright Disclaimer : | © 2016. This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/ | |||||||||||||||
Uncontrolled Keywords : | Mars, Surface, Instrumentation, Regoliths | |||||||||||||||
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Additional Information : | Full text not available from this repository. | |||||||||||||||
Depositing User : | Symplectic Elements | |||||||||||||||
Date Deposited : | 02 Nov 2016 15:41 | |||||||||||||||
Last Modified : | 06 Sep 2019 11:28 | |||||||||||||||
URI: | http://epubs.surrey.ac.uk/id/eprint/812711 |
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