Transiting exoplanets from the CoRoT space mission

P. Bordé, F. Bouchy, M. Deleuil, J. Cabrera, L. Jordá, C. Lovis, Szilárd Csizmadia, S. Aigrain, J. M. Almenara, R. Alonso,

Astronomy and Astrophysics · 2010 · 63 citations · 36 references

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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 R J , a mass of 0.22 0.03 M J , 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.

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