Abstract
Aims. We report the discovery of CoRoT-8b, a dense small Saturn-class exoplanet that orbits a K1 dwarf in 6.2 days, and we derive its orbital parameters, mass, and radius. Methods. We analyzed two complementary data sets: the photometric transit curve of CoRoT-8b as measured by CoRoT and the radial velocity curve of CoRoT-8 as measured by the HARPS spectrometer. Results. We find that CoRoT-8b is on a circular orbit with a semi-major axis of 0.063 ± 0.001 AU. It has a radius of 0.57 ± 0.02 RJ, a mass of 0.22 ± 0.03 MJ, and therefore a mean density of 1.6 ± 0.1 g cm-3. Conclusions. With 67% of the size of Saturn and 72% of its mass, CoRoT-8b has a density comparable to that of Neptune (1.76 g cm-3). We estimate its content in heavy elements to be 47-63 M, and the mass of its hydrogen-helium envelope to be 7-23 M. At 0.063 AU, the thermal loss of hydrogen of CoRoT-8b should be no more than ∼0.1% over an assumed integrated lifetime of 3 Ga.
Original language | English |
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Article number | A66 |
Journal | Astronomy and Astrophysics |
Volume | 520 |
Issue number | 10 |
DOIs | |
State | Published - 2010 |
Keywords
- planets and satellites: detection
- planets and satellites: fundamental parameters
- stars: fundamental parameters
- techniques: photometric
- techniques: radial velocities
- techniques: spectroscopic