Thermal evolution of an early magma ocean in interaction with the atmosphere

By T. Lebrun, H. Massol, E. Chassefière, A. Davaille, E. Marcq, P. Sarda, François Leblanc, G. Brandeis. 2012

231 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/df7831e6ded073c831efa62df5c285dc852eab06

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. M. Gudel
2. H. Lammer
3. L. Noack
4. M. Godolt
5. E. Pilat-Lohinger
6. Athanasia Nikolaou
7. J. Grenfell
8. A. Zerkle

In Geophysics

1. L. Noack
2. M. Godolt
3. E. Pilat-Lohinger
4. M. Gudel
5. Athanasia Nikolaou
6. J. Grenfell
7. H. Lammer
8. A. Zerkle

Citations in the corpus

• Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “…the lifetime of a magma ocean, since the released greenhouse volatiles exert a blanketing effect that can significantly delay solidification (e.g. Abe and Matsui 1985; ZaHnle et al. 1988; Abe 1997; Elkins-Tanton 2008; Lebrun et al 2013; Hamano et al. 2013; Massol et al. 2016; Salvador et al. 2017).”