The Lick-Carnegie Exoplanet Survey: A Saturn-Mass Planet in the Habitable Zone of the Nearby M4V Star HIP 57050
Nader Haghighipour, Steven S. Vogt, R. Paul Butler, Eugenio J. Rivera,, Greg Laughlin, Stefano Meschiari, Gregory W. Henry

TL;DR
This paper reports the discovery of a Saturn-mass exoplanet in the habitable zone of a nearby M4V star using radial velocity measurements, highlighting its potential for atmospheric study despite low transit probability.
Contribution
First detection of a Saturn-mass planet in the habitable zone around a high-metallicity M dwarf using precision radial velocities.
Findings
Planet has a 41.4-day orbit in the habitable zone.
Host star's high metallicity supports planet-metallicity correlation.
Transit probability is about 1%, with a potential 7% eclipse depth.
Abstract
Precision radial velocities from Keck/HIRES reveal a Saturn-mass planet orbiting the nearby M4V star HIP 57050. The planet has a minimum mass of 0.3 Jupiter-mass, an orbital period of 41.4 days, and an orbital eccentricity of 0.31. V-band photometry reveals a clear stellar rotation signature of the host star with a period of 98 days, well separated from the period of the radial velocity variations and reinforcing a Keplerian origin for the observed velocity variations. The orbital period of this planet corresponds to an orbit in the habitable zone of HIP 57050, with an expected planetary temperature of approximately 230 K. The star has a metallicity of [Fe/H] = 0.32+/-0.06 dex, of order twice solar and among the highest metallicity stars in the immediate solar neighborhood. This newly discovered planet provides further support that the well-known planet-metallicity correlation for F, G,…
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