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

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