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Constraining the parameter space of comet simulation experiments

Kaufmann, Erika and Hagermann, Axel (2018). Constraining the parameter space of comet simulation experiments. Icarus, 311 pp. 105–112.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1016/j.icarus.2018.03.025
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Abstract

Our interpretation of the data returned by Rosetta and other cometary missions is based on the predictions of theoretical models and the results of laboratory experiments. For example, Kossacki et al. (2015) showed that 67P's surface hardness reported by Spohn et al. (2015) can be explained by sintering. The present work supports Rosetta's observations by investigating the hardening process of the near-surface layers and the change in surface morphology during insolation. In order to create as simple an analogue as possible our sample consists of pure, porous H2O ice and carbon black particles. The observations suggest that translucence of the near-surface ice is important for enabling subsurface hardening. As an end product of our experiments we also obtained carbon agglomerates with some residual strength.

Item Type: Journal Item
Copyright Holders: 2018 The Authors
ISSN: 0019-1035
Project Funding Details:
Funded Project NameProject IDFunding Body
Consolidated Grant - Solar Studies and Planetary Studies (SS & PL 2016)ST/P000657/1STFC (Science & Technology Facilities Council)
Keywords: Comet analogues; Comet simulation experiments; Dusty ice; Laboratory; Surfaces; Hardness; Porous ices
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 56389
Depositing User: ORO Import
Date Deposited: 30 Aug 2018 11:15
Last Modified: 02 May 2019 09:39
URI: http://oro.open.ac.uk/id/eprint/56389
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