KOI-2939b: the largest and longest-period Kepler transiting circumbinary planet
Veselin B. Kostov, Jerome A. Orosz, William F. Welsh, Laurance R. Doyle, Daniel C. Fabrycky, Nader Haghighipour, Billy Quarles, Donald R. Short, William D. Cochran, Michael Endl, Eric B. Ford, Joao Gregorio, Tobias C. Hinse, Howard Isaacson, Jon M. Jenkins, Eric L. N. Jensen, Ilya Kull, David W. Latham, Jack J. Lissauer, Geoffrey W. Marcy, Tsevi Mazeh, Tobias W. A.Muller, Joshua Pepper, Samuel N. Quinn, Darin Ragozzine, Avi Shporer, Jason H. Steffen, Guillermo Torres, Gur Windmiller, William J. Borucki
(Submitted on 1 Dec 2015)
We report the discovery of a new Kepler transiting circumbinary planet (CBP). This latest addition to the still-small family of CBPs defies the current trend of known short-period planets orbiting near the stability limit of binary stars. Unlike the previous discoveries, the planet revolving around the eclipsing binary system KOI-2939 has a very long orbital period (~1100 days) and was at conjunction only twice during the Kepler mission lifetime. Due to the singular configuration of the system, KOI-2939b is not only the longest-period transiting CBP at the time of writing, but also one of the longest-period transiting planets. With a radius of 1.06+/-0.01 RJup it is also the largest CBP to date. The planet produced three transits in the light-curve of KOI-2939 (one of them during an eclipse, creating a syzygy) and measurably perturbed the times of the stellar eclipses, allowing us to measure its mass to be 1.52+/-0.65 MJup. The planet revolves around an 11-day period eclipsing binary consisting of two Solar-mass stars on a slightly inclined, mildly eccentric (e_bin = 0.16), spin-synchronized orbit. Despite having an orbital period three times longer than Earth’s, KOI-2939b is in the conservative habitable zone of the binary star throughout its orbit.
Comments: 61 pages, 21 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1512.00189 [astro-ph.EP] (or arXiv:1512.00189v1 [astro-ph.EP] for this version)
Submission history
From: Veselin Kostov B
[v1] Tue, 1 Dec 2015 09:37:34 GMT (6861kb,D)
http://arxiv.org/abs/1512.00189
