Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs

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Hauptverfasser: O'Brien, Shane, Wong, Amber, Han, Te, Robertson, Paul, Kanodia, Shubham, Cañas, Caleb I., Gupta, Arvind F., Swaby, Tera, Kobulnicky, Henry A., Morrell, Nidia, Rodruck, Michael, Lin, Andrea S. J., Monson, Andrew, Cochran, William D., Bender, Chad F., Diddams, Scott A., Halverson, Samuel, Krolikowski, Daniel M., Libby-Roberts, Jessica E., Ninan, Joe P., Roy, Arpita, Schwab, Christian, Stefansson, Gudmundur
Format: Preprint
Veröffentlicht: 2025
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author O'Brien, Shane
Wong, Amber
Han, Te
Robertson, Paul
Kanodia, Shubham
Cañas, Caleb I.
Gupta, Arvind F.
Swaby, Tera
Kobulnicky, Henry A.
Morrell, Nidia
Rodruck, Michael
Lin, Andrea S. J.
Monson, Andrew
Cochran, William D.
Bender, Chad F.
Diddams, Scott A.
Halverson, Samuel
Krolikowski, Daniel M.
Libby-Roberts, Jessica E.
Ninan, Joe P.
Roy, Arpita
Schwab, Christian
Stefansson, Gudmundur
author_facet O'Brien, Shane
Wong, Amber
Han, Te
Robertson, Paul
Kanodia, Shubham
Cañas, Caleb I.
Gupta, Arvind F.
Swaby, Tera
Kobulnicky, Henry A.
Morrell, Nidia
Rodruck, Michael
Lin, Andrea S. J.
Monson, Andrew
Cochran, William D.
Bender, Chad F.
Diddams, Scott A.
Halverson, Samuel
Krolikowski, Daniel M.
Libby-Roberts, Jessica E.
Ninan, Joe P.
Roy, Arpita
Schwab, Christian
Stefansson, Gudmundur
contents We confirm the planetary nature of (1) TOI-5916 b and (2) TOI-6158 b, two Exoplanets Transiting M-dwarf Stars (GEMS), both discovered by the Transiting Exoplanet Survey Satellite (TESS). Both systems were confirmed with ground-based photometry (Red Buttes Observatory and Swope, respectively) and radial velocity data from the Habitable-zone Planet Finder. Their radii are $R_{1}=11.8^{+0.52}_{-0.51}\text{ }R_{\oplus}$ and $R_{2}=10.4^{+2.70}_{-1.11}\text{ }R_{\oplus}$ and masses are $M_{1}=219\pm28\text{ }M_{\oplus}$ and $M_{2}=135^{+19}_{-18}\text{ }M_{\oplus}$. Both planets have Saturn-like densities ($ρ_{1} = 0.73^{+0.14}_{-0.13}\,\text{g cm}^{-3}$, $ρ_{2} = 0.66^{+0.41}_{-0.23}\,\text{g cm}^{-3}$), which appears to be a growing trend among GEMS systems and, more generally, warm Jupiters. In confirming both of these exoplanets, we add to the growing evidence for a population of Saturn-density planets among the GEMS systems. We also find evidence for a preliminary trend in which GEMS exhibit systematically closer orbits compared to FGK giants.
format Preprint
id arxiv_https___arxiv_org_abs_2510_11798
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs
O'Brien, Shane
Wong, Amber
Han, Te
Robertson, Paul
Kanodia, Shubham
Cañas, Caleb I.
Gupta, Arvind F.
Swaby, Tera
Kobulnicky, Henry A.
Morrell, Nidia
Rodruck, Michael
Lin, Andrea S. J.
Monson, Andrew
Cochran, William D.
Bender, Chad F.
Diddams, Scott A.
Halverson, Samuel
Krolikowski, Daniel M.
Libby-Roberts, Jessica E.
Ninan, Joe P.
Roy, Arpita
Schwab, Christian
Stefansson, Gudmundur
Earth and Planetary Astrophysics
We confirm the planetary nature of (1) TOI-5916 b and (2) TOI-6158 b, two Exoplanets Transiting M-dwarf Stars (GEMS), both discovered by the Transiting Exoplanet Survey Satellite (TESS). Both systems were confirmed with ground-based photometry (Red Buttes Observatory and Swope, respectively) and radial velocity data from the Habitable-zone Planet Finder. Their radii are $R_{1}=11.8^{+0.52}_{-0.51}\text{ }R_{\oplus}$ and $R_{2}=10.4^{+2.70}_{-1.11}\text{ }R_{\oplus}$ and masses are $M_{1}=219\pm28\text{ }M_{\oplus}$ and $M_{2}=135^{+19}_{-18}\text{ }M_{\oplus}$. Both planets have Saturn-like densities ($ρ_{1} = 0.73^{+0.14}_{-0.13}\,\text{g cm}^{-3}$, $ρ_{2} = 0.66^{+0.41}_{-0.23}\,\text{g cm}^{-3}$), which appears to be a growing trend among GEMS systems and, more generally, warm Jupiters. In confirming both of these exoplanets, we add to the growing evidence for a population of Saturn-density planets among the GEMS systems. We also find evidence for a preliminary trend in which GEMS exhibit systematically closer orbits compared to FGK giants.
title Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2510.11798