Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2011-09-13
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Accepted in ApJ Letters, 17 pages, 3 figures
Scientific paper
The Kepler mission has made an important observation, the first detection of photons from a terrestrial planet by observing its phase curve (Kepler-10b). This opens a new field in exoplanet science: the possibility to get information about the atmosphere and surface of rocky planets, objects of prime interest. In this letter, we apply the Lava-ocean model to interpret the observed phase curve. The model, a planet with no atmosphere and a surface partially made of molten rocks, has been proposed for planets of the class of CoRoT-7b, i.e. rocky planets very close to their star (at few stellar radii). Kepler-10b is a typical member of this family. It predicts that the light from the planet has an important emission component in addition to the reflected one, even in the Kepler spectral band. Assuming an isotropical reflection of light by the planetary surface (Lambertian-like approximation), we find that a Bond albedo of \sim50% can account for the observed amplitude of the phase curve, as opposed to a first attempt where an unusually high value was found. We propose a physical process to explain this still large value of the albedo. The overall interpretation can be tested in the future with instruments as JWST or EChO. Our model predicts a spectral dependence that is clearly distinguishable from that of purely reflected light, and from that of a planet at a uniform temperature.
Cavarroc Céline
Deeg Hans-Joerg
Demangeon Olivier
Fegley Bruce
Leger Alain
No associations
LandOfFree
The orbital phases and secondary transit of Kepler-10b - A physical interpretation based on the Lava-ocean planet model - does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The orbital phases and secondary transit of Kepler-10b - A physical interpretation based on the Lava-ocean planet model -, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The orbital phases and secondary transit of Kepler-10b - A physical interpretation based on the Lava-ocean planet model - will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-333680