Kepler-7B: A Transiting Planet With Unusually Low Density

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Date

2010-04

Authors

Latham, David W.
Borucki, William J.
Koch, David G.
Brown, Timothy M.
Buchhave, Lars A.
Basri, Gibor
Batalha, Natalie M.
Caldwell, Douglas A.
Cochran, William D.
Dunham, Edward W.

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Abstract

We report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M(P) = 0.43 M(J), but the radius is 50% larger, R(P) = 1.48 R(J). The resulting density, rho(P) = 0.17 g cm(-3), is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T(eff) = 6000 K. However, it is more massive and considerably larger than the Sun, M(star) = 1.35 M(circle dot) and R(star) = 1.84R(circle dot), and must be near the end of its life on the main sequence.

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Latham, David W., William J. Borucki, David G. Koch, Timothy M. Brown, Lars A. Buchhave, Gibor Basri, Natalie M. Batalha et al. "Kepler-7b: a transiting planet with unusually low density." The Astrophysical Journal Letters, Vol. 713, No. 2 (Apr., 2010): L140.