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Groombridge 34 : ウィキペディア英語版 | Groombridge 34
Groombridge 34 is a binary star system located about 11.7 light-years from the Sun. It consists of two red dwarfs in a nearly circular orbit with a separation of about 147 AU. Both stars in this pair exhibit variability due to random flares and they have been given variable star designations. (The brighter member Groombridge 34 A is designated ''GX And'', and the other member is designated ''GQ And''). ==Planetary system== In August 2014, a planet orbiting around Groombridge 34 A was reported.〔 The planet's existence was deduced from analysis of the radial velocities of the parent Star by the Eta-Earth Survey using HIRES at Keck Observatory. The planet is thought to have a minimum mass of 5.35 ± 0.75 Earth masses,〔Andrew Howard, Geoffrey Marcy, Debra A. Fischer, Howard Isaacson, Philip S. Muirhead, Gregory W. Henry, Tabetha S. Boyajian, Kaspar von Braun, Juliette C. Becker, Jason T. Wright, John Asher Johnson, (Astrophysics Earth and Planetary Astrophysics : The NASA-UC-UH Eta-Earth Program: IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth ).〕 and at its discovery was the sixth nearest known exoplanet.
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