Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
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2024
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| author | Pinto, Marcelo Tala Jordán, Andrés Acuña, Lorena Jones, Matías Brahm, Rafael Reinarz, Yared Eberhardt, Jan Espinoza, Néstor Henning, Thomas Hobson, Melissa Rojas, Felipe Schlecker, Martin Trifonov, Trifon Bakos, Gaspar Boyle, Gavin Csubry, Zoltan Hartmann, Joel Knepper, Benjamin Kreidberg, Laura Suc, Vincent Teske, Johanna Butler, R. Paul Crane, Jeffrey Schectman, Steve Thompson, Ian Osip, Dave Ricker, George Collins, Karen A. Watkins, Cristilyn N. Bieryla, Allyson Stockdale, Chris Wang, Gavin Zambelli, Roberto Seager, Sara Winn, Joshua Rose, Mark E. Rice, Malena Essack, Zahra |
| author_facet | Pinto, Marcelo Tala Jordán, Andrés Acuña, Lorena Jones, Matías Brahm, Rafael Reinarz, Yared Eberhardt, Jan Espinoza, Néstor Henning, Thomas Hobson, Melissa Rojas, Felipe Schlecker, Martin Trifonov, Trifon Bakos, Gaspar Boyle, Gavin Csubry, Zoltan Hartmann, Joel Knepper, Benjamin Kreidberg, Laura Suc, Vincent Teske, Johanna Butler, R. Paul Crane, Jeffrey Schectman, Steve Thompson, Ian Osip, Dave Ricker, George Collins, Karen A. Watkins, Cristilyn N. Bieryla, Allyson Stockdale, Chris Wang, Gavin Zambelli, Roberto Seager, Sara Winn, Joshua Rose, Mark E. Rice, Malena Essack, Zahra |
| contents | We report the discovery and characterization of three new transiting giant planets orbiting TOI-6628, TOI-3837 and TOI-5027, and one new warm sub-Saturn orbiting TOI-2328, whose transits events were detected in the lightcurves of the Transiting Exoplanet Survey Satellite \textbf{(TESS)} space mission. By combining TESS lightcurves with ground-based photometric and spectroscopic follow-up observations we confirm the planetary nature of the observed transits and radial velocity variations. TOI-6628~$b$ has a mass of 0.75$\pm$0.06~$M_\mathrm{J}$, a radius of 0.98$\pm$0.05~$R_J$ and is orbiting a metal-rich star with a period of 18.18424$\pm{0.00001}$ days and an eccentricity of 0.667$\pm0.016$, making it one of the most eccentric orbits of all known warm giants. TOI-3837~$b$ has a mass of 0.59$\pm$0.06~$M_\mathrm{J}$, a radius of 0.96$\pm$0.05~$R_J$ and orbits its host star every 11.88865$\pm$0.00003~days, with a moderate eccentricity of 0.198$^{+0.046}_{-0.058}$. With a mass of 2.01$\pm$0.13~$M_\mathrm{J}$ and a radius of 0.99$^{+0.07}_{-0.12}$ $R_J$, TOI-5027~$b$ orbits its host star in an eccentric orbit with $e$~=~0.395$^{+0.032}_{-0.029}$ every 10.24368$\pm{0.00001}$~days. TOI-2328~$b$ is a Saturn-like planet with a mass of 0.16$\pm$0.02~$M_\mathrm{J}$ and a radius of 0.89$\pm$0.04~$R_J$, orbiting its host star in a nearly circular orbit with $e$~=~0.057$^{+0.046}_{-0.029}$ at an orbital period of 17.10197$\pm{0.00001}$ days.
All four planets have orbital periods above 10 days, and our planet interior structure models are consistsent a rocky-icy core with a H/He envelope, providing evidence supporting the core accretion model of planet formation for this kind of planets. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_02069 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328 Pinto, Marcelo Tala Jordán, Andrés Acuña, Lorena Jones, Matías Brahm, Rafael Reinarz, Yared Eberhardt, Jan Espinoza, Néstor Henning, Thomas Hobson, Melissa Rojas, Felipe Schlecker, Martin Trifonov, Trifon Bakos, Gaspar Boyle, Gavin Csubry, Zoltan Hartmann, Joel Knepper, Benjamin Kreidberg, Laura Suc, Vincent Teske, Johanna Butler, R. Paul Crane, Jeffrey Schectman, Steve Thompson, Ian Osip, Dave Ricker, George Collins, Karen A. Watkins, Cristilyn N. Bieryla, Allyson Stockdale, Chris Wang, Gavin Zambelli, Roberto Seager, Sara Winn, Joshua Rose, Mark E. Rice, Malena Essack, Zahra Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics We report the discovery and characterization of three new transiting giant planets orbiting TOI-6628, TOI-3837 and TOI-5027, and one new warm sub-Saturn orbiting TOI-2328, whose transits events were detected in the lightcurves of the Transiting Exoplanet Survey Satellite \textbf{(TESS)} space mission. By combining TESS lightcurves with ground-based photometric and spectroscopic follow-up observations we confirm the planetary nature of the observed transits and radial velocity variations. TOI-6628~$b$ has a mass of 0.75$\pm$0.06~$M_\mathrm{J}$, a radius of 0.98$\pm$0.05~$R_J$ and is orbiting a metal-rich star with a period of 18.18424$\pm{0.00001}$ days and an eccentricity of 0.667$\pm0.016$, making it one of the most eccentric orbits of all known warm giants. TOI-3837~$b$ has a mass of 0.59$\pm$0.06~$M_\mathrm{J}$, a radius of 0.96$\pm$0.05~$R_J$ and orbits its host star every 11.88865$\pm$0.00003~days, with a moderate eccentricity of 0.198$^{+0.046}_{-0.058}$. With a mass of 2.01$\pm$0.13~$M_\mathrm{J}$ and a radius of 0.99$^{+0.07}_{-0.12}$ $R_J$, TOI-5027~$b$ orbits its host star in an eccentric orbit with $e$~=~0.395$^{+0.032}_{-0.029}$ every 10.24368$\pm{0.00001}$~days. TOI-2328~$b$ is a Saturn-like planet with a mass of 0.16$\pm$0.02~$M_\mathrm{J}$ and a radius of 0.89$\pm$0.04~$R_J$, orbiting its host star in a nearly circular orbit with $e$~=~0.057$^{+0.046}_{-0.029}$ at an orbital period of 17.10197$\pm{0.00001}$ days. All four planets have orbital periods above 10 days, and our planet interior structure models are consistsent a rocky-icy core with a H/He envelope, providing evidence supporting the core accretion model of planet formation for this kind of planets. |
| title | Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328 |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2412.02069 |