We announce the discovery of Kepler-6b, a transiting hot Jupiter orbiting a star with unusually high metallicity, . The planet's mass is about 2/3 that of Jupiter, M P = 0.67 M J, and the radius is 30% larger than that of Jupiter, R P = 1.32 R J, resulting in a density of ρP = 0.35 g cm-3, a fairly typical value for such a planet. The orbital period is P = 3.235 days. The host star is both more massive than the Sun, M = 1.21 M ⊙, and larger than the Sun, R * = 1.39 R ⊙. © 2010. The American Astronomical Society.
CITATION STYLE
Dunham, E. W., Borucki, W. J., Koch, D. G., Batalha, N. M., Buchhave, L. A., Brown, T. M., … Sasselov, D. D. (2010). Kepler-6b: A transiting hot jupiter orbiting a metal-rich star. Astrophysical Journal Letters, 713(2 PART 2). https://doi.org/10.1088/2041-8205/713/2/L136
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