Kepler-7B: A Transiting Planet With Unusually Low Density
Access full-text files
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.
Journal Title
Journal ISSN
Volume Title
Publisher
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.
Department
Description
LCSH Subject Headings
Citation
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.