Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/25100
Title: | Ceres: ice stability and water emission | Authors: | FORMISANO, Michelangelo DE SANCTIS, MARIA CRISTINA Magni, G. CAPRIA, MARIA TERESA CAPACCIONI, FABRIZIO Marchi, S. Ammannito, E. Bockelee-Morvan, D. Raymond, C. A. Russell, C. T. |
Issue Date: | 2015 | Volume: | European Planetary Science Congress 2015 (EPCS) | First Page: | EPSC2015-490 | Abstract: | Recent observations of H2O vapor plumes in localized regions [1] suggest the presence of ice on surface and/or on sub-surface regions of asteroid Ceres. In the hypothesis of a cometary-like emission mechanism (as already suggested by [2]), we performed several simulations in order to establish what are the likely physical conditions (in particular ice depth and thermal conductivity of crust) to fit Herschel observations [1]. | Conference Name: | European Planetary Science Congress 2015 (EPCS) | Conference Place: | La Cité des Congrès, Nantes, France | Conference Date: | 27 September-2 October, 2015 | URI: | http://hdl.handle.net/20.500.12386/25100 | URL: | https://www.epsc2015.eu/ | Bibcode ADS: | 2015EPSC...10..490F | Fulltext: | open |
Appears in Collections: | 3.02 Abstract in Atti di convegno |
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EPSC2015-490-1.pdf | Abstract | 343.41 kB | Adobe PDF | View/Open |
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