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

The Dawn mission found that the dominant colour variation on the surface of dwarf planet Ceres is a change of the visible spectral slope, where fresh impact craters are surrounded by blue (negative spectral-sloped) ejecta. The origin of this colour variation is still a mystery. Here we investigate a...

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Detalles Bibliográficos
Autores principales: Schröder, Stefan E., Poch, Olivier, Ferrari, Marco, Angelis, Simone De, Sultana, Robin, Potin, Sandra M., Beck, Pierre, De Sanctis, Maria Cristina, Schmitt, Bernard
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2021
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7804090/
https://www.ncbi.nlm.nih.gov/pubmed/33436561
http://dx.doi.org/10.1038/s41467-020-20494-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7804090/
https://www.ncbi.nlm.nih.gov/pubmed/33436561
http://dx.doi.org/10.1038/s41467-020-20494-5

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