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Related papers: Kepler-68: Three Planets, One With a Density Betwe…

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We present 44 days of high duty cycle, ultra precise photometry of the 13th magnitude star Kepler-5 (KIC 8191672, Teff=6300 K, logg=4.1), which exhibits periodic transits with a depth of 0.7%. Detailed modeling of the transit is consistent…

Kepler-78 (KIC 8435766) was identified by Sanchis-Ojeda et al. (2013) as harbouring a transiting planet of 1.16 times the size of the Earth and an orbital period of only 8.5 hours. While the exquisite Kepler photometry was able to determine…

Early time-series photometry from NASA's Kepler spacecraft has revealed a planet transiting the star we term Kepler-4, at RA = 19h02m27.68s, Dec = +50:08:08.7. The planet has an orbital period of 3.213 days and shows transits with a…

We report the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, Mp = 0.43 Mj, but the radius is fifty percent larger, Rp = 1.48 Rj. The resulting density,…

We discuss the discovery and characterization of the circumbinary planet Kepler-38b. The stellar binary is single-lined, with a period of 18.8 days, and consists of a moderately evolved main-sequence star (M_A = 0.949 +/- 0.059 solar masses…

Kepler-33 hosts five validated transiting planets ranging in period from 5 to 41 days. The planets are in nearly co-planar orbits and exhibit remarkably similar (appropriately scaled) transit durations indicative of similar impact…

Earth and Planetary Astrophysics · Physics 2022-11-16 James Sikora , Jason Rowe , Daniel Jontof-Hutter , Jack J. Lissauer

Kepler-78b is a transiting planet that is 1.2 times the radius of Earth and orbits a young, active K dwarf every 8 hours. The mass of Kepler-78b has been independently reported by two teams based on radial velocity measurements using the…

Earth and Planetary Astrophysics · Physics 2015-08-10 Samuel K. Grunblatt , Andrew W. Howard , Raphaëlle D. Haywood

The Kepler-11 planetary system contains six transiting planets ranging in size from 1.8 to 4.2 times the radius of Earth. Five of these planets orbit in a tightly-packed configuration with periods between 10 and 47 days. We perform a…

We present the discovery of a super-earth-sized planet in or near the habitable zone of a sun-like star. The host is Kepler-69, a 13.7 mag G4V-type star. We detect two periodic sets of transit signals in the three-year flux time series of…

We announce the discovery of Kepler-6b, a transiting hot Jupiter orbiting a star with unusually high metallicity, [Fe/H] = +0.34 +/- 0.04. The planet's mass is about 2/3 that of Jupiter, Mp = 0.67 Mj, and the radius is thirty percent larger…

We present the characterization of the Kepler-93 exoplanetary system, based on three years of photometry gathered by the Kepler spacecraft. The duration and cadence of the Kepler observations, in tandem with the brightness of the star,…

A search of the time-series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days. The characteristics of the host star are well…

Earth and Planetary Astrophysics · Physics 2015-06-03 William J. Borucki , David G. Koch , Natalie Batalha , Stephen T. Bryson , Douglas A. Caldwell , Jørgen Christensen-Dalsgaard , William D. Cochran , Edna DeVore , Thomas N. Gautier , John C. Geary , Ronald Gilliland , Alan Gould , Steve B. Howell , Jon M. Jenkins , David W. Latham , Jack J. Lissauer , Geoffrey W. Marcy , Jason Rowe , Dimitar Sasselov , Alan Boss , David Charbonneau , David Ciardi , Guillermo Torres , Francois Fressin , Lisa Kaltenegger , Laurance Doyle , Andrea K. Dupree , Eric B. Ford , Jonathan Fortney , Matthew J. Holman , Jason A. Steffen , Fergal Mullally , Martin Still , Jill Tarter , Sarah Ballard , Lars A. Buchhave , Josh Carter , Jessie L. Christiansen , Brice-Olivier Demory , Jean-Michel Désert , Courtney Dressing , Michael Endl , Daniel Fabrycky , Debra Fischer , Michael R. Haas , Christopher Henze , Elliott Horch , Andrew W. Howard , Howard Isaacson , Hans Kjeldsen , John Asher Johnson , Todd Klaus , Jeffery Kolodziejczak , Thomas Barclay , Jie Li , Søren Meibom , Andrej Prsa , Samuel N. Quinn , Elisa V. Quintana , Paul Robertson , William Sherry , Avi Shporer , Peter Tenenbaum , Susan E. Thompson , Joseph D. Twicken , Jeffrey Van Cleve , William F. Welsh , Sarbani Basu , Bill Chaplin , Andrea Miglio , Steve Kawaler , Torben Arentoft , Dennis Stello , Travis S. Metcalfe , Graham Verner , Christoffer Karoff , Mia Lundkvist , Mikkel Lund , Rasmus Handberg , Yvonne Elsworth , Saskia Hekker , Daniel Huber , Timothy R. Bedding

Fewer than 20 transiting Kepler planets have periods longer than one year. Our early search of the Kepler light curves revealed one such system, Kepler-1654 b (originally KIC~8410697b), which shows exactly two transit events and whose…

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