An m sin i = 24 M Planetary Companion to the Nearby M Dwarf GJ 176*

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, , Citation Michael Endl et al 2008 ApJ 673 1165 DOI 10.1086/524703

0004-637X/673/2/1165

Abstract

We report the detection of a planetary companion with a minimum mass of m sin i = 0.0771 MJup = 24.5 M to the nearby (d = 9.4 pc) M2.5 V 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 days. GJ 176 thus joins the small (but increasing) sample of M dwarfs hosting short-period 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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Footnotes

  • Based on observations obtained with the Hobby-Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Stanford University, Ludwig-Maximilians-Universität München, and Georg-August-Universität Göttingen.

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10.1086/524703