Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution

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...

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Udgivet i:Geophys Res Lett
Main Authors: Sizemore, H. G., 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.
Format: Artigo
Sprog:Inglês
Udgivet: John Wiley and Sons Inc. 2017
Fag:
Research Letters
Online adgang:https://ncbi.nlm.nih.gov/pmc/articles/PMC5606497/
https://ncbi.nlm.nih.gov/pubmed/28989206
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1002/2017GL073970
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