|Appears in Collections:||Biological and Environmental Sciences Journal Articles|
|Peer Review Status:||Refereed|
|Title:||Comet 67P/Churyumov-Gerasimenko: Hardening of the sub-surface layer|
|Author(s):||Kossacki, Konrad J|
|Citation:||Kossacki KJ, Spohn T, Hagermann A, Kaufmann E & Kührt E (2015) Comet 67P/Churyumov-Gerasimenko: Hardening of the sub-surface layer, Icarus, 260, pp. 464-474. https://doi.org/10.1016/j.icarus.2015.07.024.|
|Abstract:||From the operation of the MUPUS thermal probe Spohn et al. (2015) concluded that the material of the nucleus of 67P/Churyumov-Gerasimenko is likely to have a high strength, at least locally at the Philae landing site. In this work we consider the derived strength of the material in order to constrain its granulation. For this purpose we performed numerical simulations of the long-term sintering of ice-dust granular mixtures of different granulation, covered by a dust mantle. The dust mantle has a thickness of 0-16. cm, and a (pore size and temperature-dependent) thermal conductivity. According to our simulations a hardened layer at least a meter thick forms beneath the dust only when the grains are tens of microns in radius, or smaller. © 2015 Elsevier Inc.|
|Rights:||This article is available under the terms of the Creative Commons Attribution License (CC BY). You may copy and distribute the article, create extracts, abstracts and new works from the article, alter and revise the article, text or data mine the article and otherwise reuse the article commercially (including reuse and/or resale of the article) without permission from Elsevier. You must give appropriate credit to the original work, together with a link to the formal publication through the relevant DOI and a link to the Creative Commons user license above. You must indicate if any changes are made but not in any way that suggests the licensor endorses you or your use of the work.|
|Kossacki et al 2015.pdf||Fulltext - Published Version||658.12 kB||Adobe PDF||View/Open|
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