Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation

The origin of blue ejecta around the fresh craters of dwarf planet Ceres is unknown. Here, the authors show that the blue color results from high porosity of the surface, induced by sublimation of ice-phyllosilicate mixture produced by impacts.

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Autores principales:	Stefan E. Schröder, Olivier Poch, Marco Ferrari, Simone De Angelis, Robin Sultana, Sandra M. Potin, Pierre Beck, Maria Cristina De Sanctis, Bernard Schmitt
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2021
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/4b2db4ce986b48a99005da7f15e656de
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spelling	oai:doaj.org-article:4b2db4ce986b48a99005da7f15e656de2021-12-02T14:01:26ZDwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation10.1038/s41467-020-20494-52041-1723https://doaj.org/article/4b2db4ce986b48a99005da7f15e656de2021-01-01T00:00:00Zhttps://doi.org/10.1038/s41467-020-20494-5https://doaj.org/toc/2041-1723The origin of blue ejecta around the fresh craters of dwarf planet Ceres is unknown. Here, the authors show that the blue color results from high porosity of the surface, induced by sublimation of ice-phyllosilicate mixture produced by impacts.Stefan E. SchröderOlivier PochMarco FerrariSimone De AngelisRobin SultanaSandra M. PotinPierre BeckMaria Cristina De SanctisBernard SchmittNature PortfolioarticleScienceQENNature Communications, Vol 12, Iss 1, Pp 1-9 (2021)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Stefan E. Schröder Olivier Poch Marco Ferrari Simone De Angelis Robin Sultana Sandra M. Potin Pierre Beck Maria Cristina De Sanctis Bernard Schmitt Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
description	The origin of blue ejecta around the fresh craters of dwarf planet Ceres is unknown. Here, the authors show that the blue color results from high porosity of the surface, induced by sublimation of ice-phyllosilicate mixture produced by impacts.
format	article
author	Stefan E. Schröder Olivier Poch Marco Ferrari Simone De Angelis Robin Sultana Sandra M. Potin Pierre Beck Maria Cristina De Sanctis Bernard Schmitt
author_facet	Stefan E. Schröder Olivier Poch Marco Ferrari Simone De Angelis Robin Sultana Sandra M. Potin Pierre Beck Maria Cristina De Sanctis Bernard Schmitt
author_sort	Stefan E. Schröder
title	Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
title_short	Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
title_full	Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
title_fullStr	Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
title_full_unstemmed	Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
title_sort	dwarf planet (1) ceres surface bluing due to high porosity resulting from sublimation
publisher	Nature Portfolio
publishDate	2021
url	https://doaj.org/article/4b2db4ce986b48a99005da7f15e656de
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Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation

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