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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Detalles Bibliográficos
Autores principales: 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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2017
Materias:
Research Letters
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5606497/
https://www.ncbi.nlm.nih.gov/pubmed/28989206
http://dx.doi.org/10.1002/2017GL073970

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5606497/
https://www.ncbi.nlm.nih.gov/pubmed/28989206
http://dx.doi.org/10.1002/2017GL073970

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