Publication:
Regional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images

cris.virtualsource.author-orcid459711a1-233c-42c7-a62b-2250db4c2e70
cris.virtualsource.author-orcid3de2f4d6-f169-4c8c-9a2d-37a45466fc1f
cris.virtualsource.author-orciddb48bfb1-bfe1-4d45-bd7e-4e8d5eac2e72
cris.virtualsource.author-orcid03bf3cc6-3031-4a7d-83cd-74309eaa64be
cris.virtualsource.author-orcid1e8c45b8-fc96-490b-9882-789289549d45
dc.contributor.authorElmaarry, Mohamed Ramy
dc.contributor.authorThomas, Nicolas
dc.contributor.authorGiacomini, L.
dc.contributor.authorMassironi, M.
dc.contributor.authorPajola, M.
dc.contributor.authorMarschall, Raphael
dc.contributor.authorGracia Berná, Antonio
dc.contributor.authorSierks, H.
dc.contributor.authorBarbieri, C.
dc.contributor.authorLamy, P. L.
dc.contributor.authorRodrigo, R.
dc.contributor.authorRickman, H.
dc.contributor.authorKoschny, D.
dc.contributor.authorKeller, H. U.
dc.contributor.authorAgarwal, J.
dc.contributor.authorA'Hearn, M. F.
dc.contributor.authorAuger, A. T.
dc.contributor.authorBarucci, M. A.
dc.contributor.authorBertaux, J. L.
dc.contributor.authorBertini, I.
dc.contributor.authorBesse, S.
dc.contributor.authorBodewits, D.
dc.contributor.authorCremonese, G.
dc.contributor.authorDa Deppo, V.
dc.contributor.authorDavidsson, B.
dc.contributor.authorDe Cecco, M.
dc.contributor.authorDebei, S.
dc.contributor.authorGuettler, C.
dc.contributor.authorFornasier, S.
dc.contributor.authorFulle, M.
dc.contributor.authorGroussin, O.
dc.contributor.authorGutierrez, P. J.
dc.contributor.authorHviid, S. F.
dc.contributor.authorIp, W. H.
dc.contributor.authorJorda, L.
dc.contributor.authorKnollenberg, J.
dc.contributor.authorKovacs, G.
dc.contributor.authorKramm, J. R.
dc.contributor.authorKuehrt, E.
dc.contributor.authorKueppers, M.
dc.contributor.authorLa Forgia, F.
dc.contributor.authorLara, L. M.
dc.contributor.authorLazzarin, M.
dc.contributor.authorLopez Moreno, J. J.
dc.contributor.authorMarchi, S.
dc.contributor.authorMarzari, F.
dc.contributor.authorMichalik, H.
dc.contributor.authorNaletto, G.
dc.contributor.authorOklay, N.
dc.contributor.authorPommerol, Antoine
dc.contributor.authorPreusker, F.
dc.contributor.authorScholten, F.
dc.contributor.authorTubiana, C.
dc.contributor.authorVincent, J. B.
dc.date.accessioned2024-10-24T17:17:19Z
dc.date.available2024-10-24T17:17:19Z
dc.date.issued2015
dc.description.abstractAims. The OSIRIS camera onboard the Rosetta spacecraft has been acquiring images of the comet 67P/Churyumov-Gerasimenko (67P)'s nucleus at spatial resolutions down to similar to 0.17 m/px ever since Aug. 2014. These images have yielded unprecedented insight into the morphological diversity of the comet's surface. This paper presents an overview of the regional morphology of comet 67P. Methods. We used the images that were acquired at orbits similar to 20-30 km from the center of the comet to distinguish different regions on the surface and introduce the basic regional nomenclature adopted by all papers in this Rosetta special feature that address the comet's morphology and surface processes. We used anaglyphs to detect subtle regional and topographical boundaries and images from close orbit (similar to 10 km from the comet's center) to investigate the fine texture of the surface. Results. Nineteen regions have currently been defined on the nucleus based on morphological and/or structural boundaries, and they can be grouped into distinctive region types. Consolidated, fractured regions are the most common region type. Some of these regions enclose smooth units that appear to settle in gravitational sinks or topographically low areas. Both comet lobes have a significant portion of their surface covered by a dusty coating that appears to be recently placed and shows signs of mobilization by aeolian-like processes. The dusty coatings cover most of the regions on the surface but are notably absent from a couple of irregular large depressions that show sharp contacts with their surroundings and talus-like deposits in their interiors, which suggests that short-term explosive activity may play a significant role in shaping the comet's surface in addition to long-term sublimation loss. Finally, the presence of layered brittle units showing signs of mechanical failure predominantly in one of the comet's lobes can indicate a compositional heterogeneity between the two lobes.
dc.description.numberOfPages28
dc.description.sponsorshipNCCR PlanetS
dc.description.sponsorshipPhysikalisches Institut, Weltraumforschung und Planetologie (WP)
dc.identifier.doi10.7892/boris.81654
dc.identifier.isi000365072200024
dc.identifier.publisherDOI10.1051/0004-6361/201525723
dc.identifier.urihttps://boris-portal.unibe.ch/handle/20.500.12422/141680
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy and astrophysics
dc.relation.issn0004-6361
dc.relation.organizationDCD5A442BE9BE17DE0405C82790C4DE2
dc.relation.organizationF741DD9E19B03C32E043960C5C82F84E
dc.subject.ddc500 - Science::530 - Physics
dc.titleRegional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images
dc.typearticle
dspace.entity.typePublication
dspace.file.typetext
dspace.file.typetext
oaire.citation.issueA26
oaire.citation.startPageA26
oaire.citation.volume583
oairecerif.author.affiliationPhysikalisches Institut, Weltraumforschung und Planetologie (WP)
oairecerif.author.affiliationPhysikalisches Institut, Weltraumforschung und Planetologie (WP)
oairecerif.author.affiliationPhysikalisches Institut, Weltraumforschung und Planetologie (WP)
oairecerif.author.affiliationNCCR PlanetS
oairecerif.author.affiliationPhysikalisches Institut, Weltraumforschung und Planetologie (WP)
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unibe.description.ispublishedpub
unibe.eprints.legacyId81654
unibe.journal.abbrevTitleASTRON ASTROPHYS
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unibe.subtype.articlejournal

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