TOI-132 b: A short-period planet in the Neptune desert transiting a G-type star
arXiv:1911.02012 · doi:10.1093/mnras/staa277
Abstract
The Neptune desert is a feature seen in the radius-mass-period plane, whereby a notable dearth of short period, Neptune-like planets is found. Here we report the {\it TESS} discovery of a new short-period planet in the Neptune desert, orbiting the G-type dwarf TYC\,8003-1117-1 (TOI-132). {\it TESS} photometry shows transit-like dips at the level of 1400 ppm occurring every 2.11 days. High-precision radial velocity follow-up with HARPS confirmed the planetary nature of the transit signal and provided a semi-amplitude radial velocity variation of 11.5 m s, which, when combined with the stellar mass of , provides a planetary mass of 22.83 . Modeling the {\it TESS} high-quality light curve returns a planet radius of 3.43 , and therefore the planet bulk density is found to be 3.11 g cm. Planet structure models suggest that the bulk of the planet mass is in the form of a rocky core, with an atmospheric mass fraction of 4.3\%. TOI-132 b is a {\it TESS} Level 1 Science Requirement candidate, and therefore priority follow-up will allow the search for additional planets in the system, whilst helping to constrain low-mass planet formation and evolution models, particularly valuable for better understanding the Neptune desert.
arXiv comment12 pages, 10 figures, 4 tables. Submitted to MNRAS. Comments welcome. Missing labels, Typos fixed
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