2010/01/02 by Edward W. Dunham, William J. Borucki, W. J. Borucki +31 · 6 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Exoplanet #Hot Jupiter #Jupiter (rocket family) #Jupiter mass #Metallicity #Orbital period #Physics #Planet #Planetary mass #RADIUS #Space exploration #Star (game theory) #Stars #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.1088/2041-8205/713/2/l136
12 pages, 2 figures, submitted to the Astrophysical Journal Letters
arxiv created 2010/01/02 · openalex publication_date 2010/03/30 · arxiv updated 2015/05/14 · openalex created_date 2021/02/01 · openalex updated_date 2026/08/05
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 ρ P = 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 ☉ .