Detailed Record
TOI-5344 b: A Saturn-like Planet Orbiting a Super-solar Metallicity M0 Dwarf
| Abstract | We confirm the planetary nature of TOI-5344 b as a transiting giant exoplanet around an M0-dwarf star. TOI-5344 b was discovered with the Transiting Exoplanet Survey Satellite photometry and confirmed with ground-based photometry (the Red Buttes Observatory 0.6 m telescope), radial velocity (the Habitable-zone Planet Finder), and speckle imaging (the NN-Explore Exoplanet Stellar Speckle Imager). TOI-5344 b is a Saturn-like giant planet ( ρ = 0.80 {-0.15}^{+0.17} g cm −3 ) with a planetary radius of 9.7 ± 0.5 R ⊕ (0.87 ± 0.04 R Jup ) and a planetary mass of{135}_{-18}^{+17} M⊕} (0.42 {-0.06}^{+0.05} {M}_{Jup}). It has an orbital period of {3.792622}_{-0.000010}^{+0.000010} days and an orbital eccentricity of {0.06}_{-0.04}^{+0.07}. We measure a high metallicity for TOI-5344 of [Fe/H] = 0.48 ± 0.12, where the high metallicity is consistent with expectations from formation through core accretion. We compare the metallicity of the M-dwarf hosts of giant exoplanets to that of M-dwarf hosts of nongiants (≲8 R ⊕ ). While the two populations appear to show different metallicity distributions, quantitative tests are prohibited by various sample caveats. |
|---|---|
| Authors |
Te Han |
| Journal Info | Institute of Physics | The Astronomical Journal , vol: 167 , iss: 1 , pages: 4 - 4 |
| Publication Date | 12/4/2023 |
| ISSN | 0004-6256 |
| Type |
article |
| Open Access |
gold
|
| DOI | https://doi.org/10.3847/1538-3881/ad09c2 |
| Keywords |
Extraterrestrial Organic Matter (Score: 0.441327) |