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Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process

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dc.contributor.author Schenk, Paul M.
dc.contributor.author Scully, J. E. C.
dc.contributor.author Buczkowski, Debra L.
dc.contributor.author Sizemore, Hanna G.
dc.contributor.author Schmidt, B.
dc.contributor.author Pieters, Carlé M.
dc.contributor.author Neesemann, A.
dc.contributor.author O’Brien, D. P.
dc.contributor.author Marchi, Simone
dc.contributor.author Williams, David A. (Planetary geologist)
dc.contributor.author Nathues, A.
dc.contributor.author De Sanctis, M. Cristina
dc.contributor.author Tosi, F.
dc.contributor.author Russell, C. T. (Christopher T.)
dc.contributor.author Castillo-Rogez, Julie
dc.contributor.author Raymond, Carol A.
dc.coverage.spatial Ceres
dc.date.accessioned 2021-03-25T19:50:20Z
dc.date.available 2021-03-25T19:50:20Z
dc.date.issued 2020-08-10
dc.identifier.citation Schenk, P., Scully, J., Buczkowski, D. et al. Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process. Nat Commun 11, 3679 (2020). https://doi.org/10.1038/s41467-020-17184-7 en
dc.identifier.other DOI:10.1038/s41467-020-17184-7
dc.identifier.other PMID: 32778649
dc.identifier.other PMCID: PMC7417549
dc.identifier.uri https://hdl.handle.net/20.500.11753/1748
dc.description.abstract Here we show using Dawn high-resolution stereo imaging and topography that Ceres’ unique composition has resulted in widespread mantling by solidified water- and salt-rich mud-like impact melts with scattered endogenic pits, troughs, and bright mounds indicative of outgassing of volatiles and periglacial-style activity during solidification. en
dc.description.statementofresponsibility P. Schenk, J. Scully, D. Buczkowski, H. Sizemore, B. Schmidt, C. Pieters, A. Neesemann, D. O’Brien, S. Marchi, D. Williams, A. Nathues, M. De Sanctis, F. Tosi, C. T. Russell, J. Castillo-Rogez & C. Raymond
dc.format.extent 11 pages
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Nature en
dc.relation.ispartofseries LPI contribution ; no. 2345
dc.subject Ceres (Dwarf planet) en
dc.subject Cratering en
dc.title Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process en
dc.type Article en
dc.rights.license This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format


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