The missing large impact craters on Ceres

Asteroids provide fundamental clues to the formation and evolution of planetesimals. Collisional models based on the depletion of the primordial main belt of asteroids predict 10–15 craters >400 km should have formed on Ceres, the largest object between Mars and Jupiter, over the last 4.55 Gyr. L...

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Detalles Bibliográficos
Autores principales: Marchi, S., Ermakov, A. I., Raymond, C. A., Fu, R. R., O'Brien, D. P., Bland, M. T., Ammannito, E., De Sanctis, M. C., Bowling, T., Schenk, P., Scully, J. E. C., Buczkowski, D. L., Williams, D. A., Hiesinger, H., Russell, C. T.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2016
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4963536/
https://www.ncbi.nlm.nih.gov/pubmed/27459197
http://dx.doi.org/10.1038/ncomms12257

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4963536/
https://www.ncbi.nlm.nih.gov/pubmed/27459197
http://dx.doi.org/10.1038/ncomms12257

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