TESS Giants Transiting Giants. VII. A Hot Saturn Orbiting an Oscillating Red Giant Star
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2024
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| author | Saunders, Nicholas Grunblatt, Samuel K. Huber, Daniel Ong, J. M. Joel Schlaufman, Kevin C. Hey, Daniel Li, Yaguang Butler, R. P. Crane, Jeffrey D. Shectman, Steve Teske, Johanna K. Quinn, Samuel N. Yee, Samuel W. Brahm, Rafael Trifonov, Trifon Jordán, Andrés Henning, Thomas Sing, David K. MacGregor, Meredith Page, Emma Rapetti, David Falk, Ben Levine, Alan M. Huang, Chelsea X. Lund, Michael B. Ricker, George R. Seager, S. Winn, Joshua N. Jenkins, Jon M. |
| author_facet | Saunders, Nicholas Grunblatt, Samuel K. Huber, Daniel Ong, J. M. Joel Schlaufman, Kevin C. Hey, Daniel Li, Yaguang Butler, R. P. Crane, Jeffrey D. Shectman, Steve Teske, Johanna K. Quinn, Samuel N. Yee, Samuel W. Brahm, Rafael Trifonov, Trifon Jordán, Andrés Henning, Thomas Sing, David K. MacGregor, Meredith Page, Emma Rapetti, David Falk, Ben Levine, Alan M. Huang, Chelsea X. Lund, Michael B. Ricker, George R. Seager, S. Winn, Joshua N. Jenkins, Jon M. |
| contents | We present the discovery of TOI-7041 b (TIC 201175570 b), a hot Saturn transiting a red giant star with measurable stellar oscillations. We observe solar-like oscillations in TOI-7041 with a frequency of maximum power of $ν_{\rm max} = 218.50\pm2.23$ $μ$Hz and a large frequency separation of $Δν= 16.5282\pm0.0186$ $μ$Hz. Our asteroseismic analysis indicates that TOI-7041 has a radius of $4.10 \pm 0.06$(stat) $\pm$ 0.05(sys) $R_\odot$, making it one of the largest stars around which a transiting planet has been discovered with the Transiting Exoplanet Survey Satellite (TESS), and the mission's first oscillating red giant with a transiting planet. TOI-7041 b has an orbital period of $9.691 \pm 0.006$ days and a low eccentricity of $e = 0.04 \pm 0.04$. We measure a planet radius of $1.02 \pm 0.03$ $R_J$ with photometry from TESS, and a planet mass of $0.36 \pm 0.16$ $M_J$ ($114 \pm 51$ $M_\oplus$) with ground-based radial velocity measurements. TOI-7041 b appears less inflated than similar systems receiving equivalent incident flux, and its circular orbit indicates that it is not undergoing tidal heating due to circularization. The asteroseismic analysis of the host star provides some of the tightest constraints on stellar properties for a TESS planet host and enables precise characterization of the hot Saturn. This system joins a small number of TESS-discovered exoplanets orbiting stars that exhibit clear stellar oscillations and indicates that extended TESS observations of evolved stars will similarly provide a path to improved exoplanet characterization. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_11037 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | TESS Giants Transiting Giants. VII. A Hot Saturn Orbiting an Oscillating Red Giant Star Saunders, Nicholas Grunblatt, Samuel K. Huber, Daniel Ong, J. M. Joel Schlaufman, Kevin C. Hey, Daniel Li, Yaguang Butler, R. P. Crane, Jeffrey D. Shectman, Steve Teske, Johanna K. Quinn, Samuel N. Yee, Samuel W. Brahm, Rafael Trifonov, Trifon Jordán, Andrés Henning, Thomas Sing, David K. MacGregor, Meredith Page, Emma Rapetti, David Falk, Ben Levine, Alan M. Huang, Chelsea X. Lund, Michael B. Ricker, George R. Seager, S. Winn, Joshua N. Jenkins, Jon M. Earth and Planetary Astrophysics Solar and Stellar Astrophysics We present the discovery of TOI-7041 b (TIC 201175570 b), a hot Saturn transiting a red giant star with measurable stellar oscillations. We observe solar-like oscillations in TOI-7041 with a frequency of maximum power of $ν_{\rm max} = 218.50\pm2.23$ $μ$Hz and a large frequency separation of $Δν= 16.5282\pm0.0186$ $μ$Hz. Our asteroseismic analysis indicates that TOI-7041 has a radius of $4.10 \pm 0.06$(stat) $\pm$ 0.05(sys) $R_\odot$, making it one of the largest stars around which a transiting planet has been discovered with the Transiting Exoplanet Survey Satellite (TESS), and the mission's first oscillating red giant with a transiting planet. TOI-7041 b has an orbital period of $9.691 \pm 0.006$ days and a low eccentricity of $e = 0.04 \pm 0.04$. We measure a planet radius of $1.02 \pm 0.03$ $R_J$ with photometry from TESS, and a planet mass of $0.36 \pm 0.16$ $M_J$ ($114 \pm 51$ $M_\oplus$) with ground-based radial velocity measurements. TOI-7041 b appears less inflated than similar systems receiving equivalent incident flux, and its circular orbit indicates that it is not undergoing tidal heating due to circularization. The asteroseismic analysis of the host star provides some of the tightest constraints on stellar properties for a TESS planet host and enables precise characterization of the hot Saturn. This system joins a small number of TESS-discovered exoplanets orbiting stars that exhibit clear stellar oscillations and indicates that extended TESS observations of evolved stars will similarly provide a path to improved exoplanet characterization. |
| title | TESS Giants Transiting Giants. VII. A Hot Saturn Orbiting an Oscillating Red Giant Star |
| topic | Earth and Planetary Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2410.11037 |