| Abstract |
Using both ground-based transit photometry and high-precision radial velocity (RV) spectroscopy, we confirm the planetary nature of TOI-3785 b. This transiting Neptune orbits an M2-Dwarf star with a period of ~4.67 days, a planetary radius of 5.14 +/- 0.16 Earth Radii, a mass of 14.95 +4.10, -3.92 Earth Masses, and a density of 0.61 +0.18, -0.17 g/cm^3. TOI-3785 b belongs to a rare population of Neptunes (4 Earth Radii < Rp < 7 Earth Radii) orbiting cooler, smaller M-dwarf host stars, of which only ~10 have been confirmed. By increasing the number of confirmed planets, TOI-3785 b offers an opportunity to compare similar planets across varying planetary and stellar parameter spaces. Moreover, with a high transmission spectroscopy metric (TSM) of ~150 combined with a relatively cool equilibrium temperature of 582 +/- 16 K and an inactive host star, TOI-3785 b is one of the more promising low-density M-dwarf Neptune targets for atmospheric follow-up. Future investigation into atmospheric mass loss rates of TOI-3785 b may yield new insights into the atmospheric evolution of these low-mass gas planets around M-dwarfs. |
| Authors |
Luke Powers  , Jessica E. Libby-Roberts , Andrea S. J. Lin , Caleb I. Cañas , Shubham Kanodia , Suvrath Mahadevan , Joe P. Ninan , Guðmundur Stefánsson , Arvind F. Gupta , Sinclaire Jones , Henry A. Kobulnicky  , Andrew Monson , Brock A. Parker , Tera N. Swaby , Chad F. Bender , William D. Cochran , Leslie Hebb , Andrew J. Metcalf , Paul Robertson , Christian Schwab , John P. Wisniewski , Jason T. Wright
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