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  Pinnacles on the 67P comet nucleus: Evidence for large scale erosion and hierarchical agglomeration of the nucleus

Basilevsky, A. T., Krasilnikov, S. S., Mall, U., Hviid, S., Skorov, Y. V., & Keller, H. (2017). Pinnacles on the 67P comet nucleus: Evidence for large scale erosion and hierarchical agglomeration of the nucleus. Planetary and Space Science, 140, 80-85. doi:10.1016/j.pss.2016.11.005.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0003-2F2C-9 Version Permalink: http://hdl.handle.net/21.11116/0000-0003-2F2D-8
Genre: Journal Article

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 Creators:
Basilevsky, A. T.1, Author              
Krasilnikov, S. S.1, Author              
Mall, Urs1, Author              
Hviid, S.F.S., Author
Skorov, Yuri V.1, Author              
Keller, H.U., Author
Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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Free keywords: Comets General - comets Individual Comet 67P/Churyumov-Gerasimenko – Space vehicles Rosetta
 Abstract: Context Pinnacles, local promontories of varied shapes including spires with pointed tops, are observed on the surface of the 67P's cometary nucleus in the OSIRIS and NavCam images. Their presence and characteristics allow to infer the magnitude of the surface erosion and the degree of heterogeneity of the consolidated nucleus material. Aims To identify these pinnacles and consider implications, which follow from their presence and characteristics. Methods Identification of pinnacles in the available OSIRIS and NavCam images, as well as in the model images of the nucleus built from the digital terrain model, and an investigation of their morphology. Results We identified and measured 49 pinnacles in 13 regions of the studied part of the nucleus. The pinnacles are typically asymmetric with somewhat different slope angles at different slopes whose maximum values range from 40 to 90°, sometimes with small overhangs. Their heights vary from 10 to 20 to 100–200 m and the foot diameters from 30 to 300 m. Our analysis of the OSIRIS images of the pinnacles showed that they have surface texture similar to that of consolidated nucleus material and are probably composed of it. Conclusions The observed characteristics of pinnacles found on 67P agree with the suggestion that they are erosion remnants formed due to a slowdown of erosion in places where nucleus material is more resistant to sublimational erosion than the material around it. In this case the maximum heights of pinnacles (100–200 m) gives a lower boundary for the amount of surface material lost and their diameters (typically tens of meters) are a measure of the size of the erosion-resistant parts.

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Language(s): eng - English
 Dates: 2017
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1016/j.pss.2016.11.005
 Degree: -

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Title: Planetary and Space Science
Source Genre: Journal
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Publ. Info: Amsterdam : Elsevier B.V.
Pages: - Volume / Issue: 140 Sequence Number: - Start / End Page: 80 - 85 Identifier: ISSN: 0032-0633
CoNE: https://pure.mpg.de/cone/journals/resource/954925434422