dc.contributor.author |
Schenk, Paul M. |
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dc.contributor.author |
Scully, J. E. C. |
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dc.contributor.author |
Buczkowski, Debra L. |
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dc.contributor.author |
Sizemore, Hanna G. |
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dc.contributor.author |
Schmidt, B. |
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dc.contributor.author |
Pieters, Carlé M. |
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dc.contributor.author |
Neesemann, A. |
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dc.contributor.author |
O'Brien, D. P. |
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dc.contributor.author |
Marchi, Simone |
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dc.contributor.author |
Williams, David A. (Planetary geologist) |
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dc.contributor.author |
Nathues, A. |
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dc.contributor.author |
De Sanctis, M. Cristina |
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dc.contributor.author |
Tosi, F. |
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dc.contributor.author |
Russell, C. T. (Christopher T.) |
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dc.contributor.author |
Castillo-Rogez, Julie |
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dc.contributor.author |
Raymond, Carol A. |
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dc.coverage.spatial |
Ceres (Dwarf planet) |
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dc.date.accessioned |
2021-03-25T19:50:20Z |
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dc.date.available |
2021-03-25T19:50:20Z |
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dc.date.issued |
2020-08-10 |
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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 |
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dc.identifier.other |
PMID: 32778649 |
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dc.identifier.other |
PMCID: PMC7417549 |
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dc.identifier.uri |
https://hdl.handle.net/20.500.11753/1748 |
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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 |
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dc.format.extent |
11 pages |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Nature |
en |
dc.relation.ispartofseries |
LPI contribution ; no. 2345 |
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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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