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TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf

Authors: Shubham Kanodia, Jessica Libby-Roberts, Caleb I. Cañas, Joe P. Ninan, Suvrath Mahadevan, Gudmundur Stefansson, Andrea S. J. Lin, Sinclaire Jones, Andrew Monson, Brock A. Parker, Henry A. Kobulnicky, Tera N. Swaby, Luke Powers, Corey Beard, Chad F. Bender, Cullen H. Blake, William D. Cochran, Jiayin Dong, Scott A. Diddams, Connor Fredrick, Arvind F. Gupta, Samuel Halverson, Fred Hearty, Sarah E. Logsdon, Andrew J. Metcalf, Michael W. McElwain, Caroline Morley, Jayadev Rajagopal, Lawrence W. Ramsey, Paul Robertson, Arpita Roy, Christian Schwab, Ryan C. Terrien, John Wisniewski, Jason T. Wright

Shubham Kanodia et al 2022 The Astronomical Journal 164 .

Provider: AAS Journals

Caption: Figure 9.

TOI-3757 b (circled in green) in a mass–radius plane alongside other M dwarf planets (colored by the T _eff). We also include planets around FGK stars in the background, along with density contours for 0.3, 1, 3 g cm⁻³. TOI-3757 b is the lowest-density planet orbiting an M dwarf with precise mass and radius measurements.

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