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

Dawn mission’s second extended phase provided high resolution observations of Occator crater of the dwarf planet Ceres. Here, the authors show stereo imaging and topographic maps of this crater revealing the influence of crustal composition on impact related melt and hydrothermal processes, and comp...

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Autores principales:	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
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2020
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/044c971ba7d34351b217f63896b98c6a
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spelling	oai:doaj.org-article:044c971ba7d34351b217f63896b98c6a2021-12-02T15:07:56ZImpact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process10.1038/s41467-020-17184-72041-1723https://doaj.org/article/044c971ba7d34351b217f63896b98c6a2020-08-01T00:00:00Zhttps://doi.org/10.1038/s41467-020-17184-7https://doaj.org/toc/2041-1723Dawn mission’s second extended phase provided high resolution observations of Occator crater of the dwarf planet Ceres. Here, the authors show stereo imaging and topographic maps of this crater revealing the influence of crustal composition on impact related melt and hydrothermal processes, and compare features to those on Mars, Earth and the Moon.P. SchenkJ. ScullyD. BuczkowskiH. SizemoreB. SchmidtC. PietersA. NeesemannD. O’BrienS. MarchiD. WilliamsA. NathuesM. De SanctisF. TosiC. T. RussellJ. Castillo-RogezC. RaymondNature PortfolioarticleScienceQENNature Communications, Vol 11, Iss 1, Pp 1-11 (2020)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q 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 Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
description	Dawn mission’s second extended phase provided high resolution observations of Occator crater of the dwarf planet Ceres. Here, the authors show stereo imaging and topographic maps of this crater revealing the influence of crustal composition on impact related melt and hydrothermal processes, and compare features to those on Mars, Earth and the Moon.
format	article
author	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
author_facet	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
author_sort	P. Schenk
title	Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
title_short	Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
title_full	Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
title_fullStr	Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
title_full_unstemmed	Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
title_sort	impact heat driven volatile redistribution at occator crater on ceres as a comparative planetary process
publisher	Nature Portfolio
publishDate	2020
url	https://doaj.org/article/044c971ba7d34351b217f63896b98c6a
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Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process

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