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arXiv · 0709.0944

An m sin i = 24 Earth Mass Planetary Companion To The Nearby M Dwarf GJ 176

Michael Endl·William D. Cochran·Robert A. Wittenmyer·Alan P. Boss
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Abstract

We report the detection of a planetary companion with a minimum mass of m sin i = 0.0771 M_Jup = 24.5 M_Earth to the nearby (d = 9.4 pc) M2.5V star GJ 176. The star was observed as part of our M dwarf planet search at the Hobby-Eberly Telescope (HET). The detection is based on 5 years of high-precision differential radial velocity (RV) measurements using the High-Resolution-Spectrograph (HRS). The orbital period of the planet is 10.24 d. GJ 176 thus joins the small (but increasing) sample of M dwarfs hosting short-periodic planets with minimum masses in the Neptune-mass range. Low mass planets could be relatively common around M dwarfs and the current detections might represent the tip of a rocky planet population.

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Michael Endl, William D. Cochran, Robert A. Wittenmyer, Alan P. Boss. 2007-09-06. An m sin i = 24 Earth Mass Planetary Companion To The Nearby M Dwarf GJ 176. https://doi.org/10.1086/524703

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