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A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
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(2022) A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N. Astronomy & Astrophysics, 666 . A183. doi:10.1051/0004-6361/202143002 ISSN 0004-6361.
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Official URL: https://doi.org/10.1051/0004-6361/202143002
Abstract
We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. A joint MCMC analysis of the TESS light curve and the radial-velocity evolution allows us to determine the planetary system properties. From our analysis, TOI-1710 b is found to be a massive warm super-Neptune (Mp = 28.3 ± 4.7 M⊕ and Rp = 5.34 ± 0.11 R⊕) orbiting a G5V dwarf star (Teff = 5665 ± 55 K) on a nearly circular 24.3-day orbit (e = 0.16 ± 0.08). The orbital period of this planet is close to the estimated rotation period of its host star Prot = 22.5 ± 2.0 days and it has a low Keplerian semi-amplitude K = 6.4 ± 1.0 m s−1; we thus performed additional analyses to show the robustness of the retrieved planetary parameters. With a low bulk density of 1.03 ± 0.23 g cm−3 and orbiting a bright host star (J = 8.3, V = 9.6), TOI-1710 b is one of the best targets in this mass-radius range (near the Neptunian desert) for atmospheric characterization via transmission spectroscopy, a key measurement in constraining planet formation and evolutionary models of sub-Jovian planets.
Item Type: | Journal Article | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Subjects: | Q Science > QB Astronomy | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Divisions: | Faculty of Science, Engineering and Medicine > Science > Physics | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Library of Congress Subject Headings (LCSH): | Extrasolar planets, Extrasolar planets -- Detection, Astronomical spectroscopy, Astronomical photometry | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Journal or Publication Title: | Astronomy & Astrophysics | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Publisher: | EDP Sciences | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
ISSN: | 0004-6361 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Official Date: | October 2022 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Dates: |
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Volume: | 666 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Number of Pages: | 17 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Article Number: | A183 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
DOI: | 10.1051/0004-6361/202143002 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Status: | Peer Reviewed | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Publication Status: | Published | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Access rights to Published version: | Open Access (Creative Commons) | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Date of first compliant deposit: | 12 December 2022 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Date of first compliant Open Access: | 14 December 2022 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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