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M2K: I. A Jovian mass planet around the M3V star HIP79431

Doppler observations from Keck Observatory reveal the presence of a planet with Msini of 2.1 Mjup orbiting the M3V star HIP79431. This is the sixth giant planet to be detected in Doppler surveys of M dwarfs and it is one of the most massive planets discovered around an M dwarf star. The planet has an orbital period of 111.7 days and an orbital eccentricity of 0.29. The host star is metal rich, with an estimated [Fe/H] = +0.4. This is the first planet to emerge from our new survey of 1600 M-to-K dwarf stars.

preprint2010arXivOpen access
Kevin AppsKelsey I. ClubbDebra A. FischerEric GaidosAndrew W. HowardJohn A. JohnsonGeoffrey W. MarcyHoward IsaacsonMatthew J. GiguereJeff A. ValentiVictor RodriguezCarley ChubakSebastian Lepine
astro-ph.EP
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Kevin AppsKelsey I. ClubbDebra A. FischerEric GaidosAndrew W. HowardJohn A. JohnsonGeoffrey W. MarcyHoward IsaacsonMatthew J. GiguereJeff A. ValentiVictor RodriguezCarley ChubakSebastian Lepine

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