Planet Hunters VII. Discovery of a New Low-Mass, Low-Density Planet (PH3 c) Orbiting Kepler-289 with Mass Measurements of Two Additional Planets (PH3 b and d)
arXiv:1410.8114 · doi:10.1088/0004-637X/795/2/167
Abstract
We report the discovery of one newly confirmed planet ( days, ) and mass determinations of two previously validated Kepler planets, Kepler-289 b ( days, ) and Kepler-289-c ( days, ), through their transit timing variations (TTVs). We also exclude the possibility that these three planets reside in a Laplace resonance. The outer planet has very deep (), high signal-to-noise transits, which puts extremely tight constraints on its host star's stellar properties via Kepler's Third Law. The star PH3 is a young ( Gyr as determined by isochrones and gyrochronology), Sun-like star with , , and K. The middle planet's large TTV amplitude ( hours) resulted either in non-detections or inaccurate detections in previous searches. A strong chopping signal, a shorter period sinusoid in the TTVs, allows us to break the mass-eccentricity degeneracy and uniquely determine the masses of the inner, middle, and outer planets to be , , and , which we designate PH3 b, c, and d, respectively. Furthermore, the middle planet, PH3 c, has a relatively low density, g/cm for a planet of its mass, requiring a substantial H/He atmosphere of by mass, and joins a growing population of low-mass, low-density planets.
arXiv comment21 pages, 10 figures, 5 tables, accepted into ApJ
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