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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...
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. |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2016
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Materias: | |
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 |
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