DISCOVERY and VALIDATION of Kepler-452B: a 1.6-R⊕ SUPER EARTH EXOPLANET in the HABITABLE ZONE of a G2 STAR Jon M
Received 2015 March 3; accepted 2015 May 23; published 2015 July 23 by the Astronomical Journal Preprint typeset using LATEX style emulateapj v. 12/16/11 DISCOVERY AND VALIDATION OF Kepler-452b: A 1:6-R⊕ SUPER EARTH EXOPLANET IN THE HABITABLE ZONE OF A G2 STAR Jon M. Jenkins1, Joseph D. Twicken1,2, Natalie M. Batalha1, Douglas A. Caldwell1,2, William D. Cochran3, Michael Endl3, David W. Latham4, Gilbert A. Esquerdo4, Shawn Seader1,2, Allyson Bieryla4, Erik Petigura5, David R. Ciardi6, Geoffrey W. Marcy5, Howard Isaacson5, Daniel Huber7,2,8, Jason F. Rowe1,2, Guillermo Torres4, Stephen T. Bryson1, Lars Buchhave4,9, Ivan Ramirez3, Angie Wolfgang10, Jie Li1,2, Jennifer R. Campbell11, Peter Tenenbaum1,2, Dwight Sanderfer1 Christopher E. Henze1, Joseph H. Catanzarite1,2, Ronald L. Gilliland12, and William J. Borucki1 Received 2015 March 3; accepted 2015 May 23; published 2015 July 23 by the Astronomical Journal ABSTRACT We report on the discovery and validation of Kepler-452b, a transiting planet identified by a search +0:23 through the 4 years of data collected by NASA's Kepler Mission. This possibly rocky 1:63−0:20-R⊕ +0:007 planet orbits its G2 host star every 384:843−0:012 days, the longest orbital period for a small (RP < 2 R⊕) transiting exoplanet to date. The likelihood that this planet has a rocky composition lies between 49% and 62%. The star has an effective temperature of 5757 ± 85 K and a log g of 4:32 ± 0:09. At +0:019 a mean orbital separation of 1:046−0:015 AU, this small planet is well within the optimistic habitable zone of its star (recent Venus/early Mars), experiencing only 10% more flux than Earth receives from the Sun today, and slightly outside the conservative habitable zone (runaway greenhouse/maximum +0:15 greenhouse).
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