Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..399e&link_type=abstract
SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.
Astronomy and Astrophysics
Astrophysics
Scientific paper
Microlensing technique used to detect extrasolar planets is sensible to low-mass planets orbiting a few AU away from their stars. The detection of OGLE-2005-BLG-390Lb (hereafter, OGLE-390Lb) around an M star from the Galactic bulge (Beaulieu et al. 2006) unveil the existence of few-Earth-masses and cold (˜40 K) planets. These frozen planets might nonetheless host liquid water underneath an ice shell, due to a strong radiogenic heating at the bottom of the ice layer. Heating and cooling are depending upon the mass ratio ice/rock and the age of the planet. OGLE-390Lb seems too old to have a subsurface ocean for any value of the ratio ice/rock; however, liquid water below an ice shell was certainly present in the past for several billion years. See Ehrenreich et al. (2006b) for details.
Beaulieu J.-Ph.
Ehrenreich David
Grasset Olivier
Lecavelier Des Etangs Alain
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