Prior to the arrival of the Dawn spacecraft at Ceres, the dwarf planet was anticipated to be ice-rich. Searches for morphological features related to ice have been ongoing during Dawn's mission at Ceres. Here we report the identification of pitted terrains associated with fresh Cerean impact cr...
Détails bibliographiques
| Publié dans: | Geophysical research letters. - 1984. - 44(2017), 13 vom: 16. Juli, Seite 6570-6578
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| Auteur principal: |
Sizemore, H G
(Auteur) |
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| Autres auteurs: |
Platz, T,
Schorghofer, N,
Prettyman, T H,
De Sanctis, M C,
Crown, D A,
Schmedemann, N,
Neesemann, A,
Kneissl, T,
Marchi, S,
Schenk, P M,
Bland, M T,
Schmidt, B E,
Hughson, K H G,
Tosi, F,
Zambon, F,
Mest, S C,
Yingst, R A,
Williams, D A,
Russell, C T,
Raymond, C A |
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| Format: | Article en ligne
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| Langue: | English |
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| Publié: |
2017
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| Accès à la collection: | Geophysical research letters
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| Sujets: | Journal Article
Ceres
craters
geomorphology
ground ice
pitted terrain
volatiles |
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