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Kepler-47: A Transiting Circumbinary Multiplanet System
Ist Teil von
Science (American Association for the Advancement of Science), 2012-09, Vol.337 (6101), p.1511-1514
Ort / Verlag
Washington, DC: American Association for the Advancement of Science
Erscheinungsjahr
2012
Quelle
Science Online_科学在线
Beschreibungen/Notizen
We report the detection of Kepler-47, a system consisting of two planets orbiting around an eclipsing pair of stars. The inner and outer planets have radii 3.0 and 4.6 times that of Earth, respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, 18 transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars. The outer planet's orbital period is 303.2 days, and although the planet is not Earth-like, it resides within the classical "habitable zone," where liquid water could exist on an Earth-like planet. With its two known planets, Kepler-47 establishes that close binary stars can host complete planetary systems.