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  5. Ceres: ice stability and water emission
 

Ceres: ice stability and water emission

Date Issued
2015
Author(s)
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.
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].
Coverage
European Planetary Science Congress 2015 (EPCS)
Start page
EPSC2015-490
Conferenece
European Planetary Science Congress 2015 (EPCS)
Conferenece place
La Cité des Congrès, Nantes, France
Conferenece date
27 September-2 October, 2015
Uri
http://hdl.handle.net/20.500.12386/25100
Url
https://www.epsc2015.eu/
Ads BibCode
2015EPSC...10..490F
Rights
open.access
File(s)
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EPSC2015-490-1.pdf

Description
Abstract
Size

343.41 KB

Format

Adobe PDF

Checksum (MD5)

4d1869611e6895683860e9cf96618f15

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