Thermal evolution of an early magma ocean in interaction with the atmosphere: conditions for the condensation of a water ocean
The thermal evolution of magma oceans produced by collision with giant impactors late in accretion is xpected to depend on the composition and structure of the atmosphere through the greenhouse effect of CO2 and H2O released from the magma during its crystallization. We developed a 1D parameterize...
Main Authors: | Lebrun T., Massol H., Chassefière E., Davaille A., Marcq E., Sarda P., Leblanc F., Brandeis G. |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2014-02-01
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Series: | BIO Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/bioconf/20140201006 |
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