TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system - Archive ouverte HAL
Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2023

TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system

Lizhou Sha
Andrew Vanderburg
Rafael Brahm
Steven Giacalone
Mackenna Wood
Karen Collins
Louise Nielsen
Melissa Hobson
Steve Howell
Pascal Torres-Miranda
  • Fonction : Auteur
Andrew Mann
George Zhou
Elisa Delgado-Mena
Felipe Rojas
Lyu Abe
Trifon Trifonov
Vardan Adibekyan
Sérgio Sousa
Sergio Fajardo-Acosta
Tristan Guillot
Saburo Howard
Colin Littlefield
Faith Hawthorn
François-Xavier Schmider
Jan Eberhardt
Thiam-Guan Tan
Ares Osborn
Richard Schwarz
Paul Strøm
Andrés Jordán
Gavin Wang
Thomas Henning
Bob Massey
Nicholas Law
Chris Stockdale
Elise Furlan
Gregor Srdoc
  • Fonction : Auteur
Peter Wheatley
David Barrado Navascués
Jack Lissauer
Keivan Stassun
George Ricker
Roland Vanderspek
David Latham
Joshua Winn
Sara Seager
Jon Jenkins
Thomas Barclay
Luke Bouma
Jessie Christiansen
Natalia Guerrero
Mark Rose

Résumé

Hot jupiters (P < 10 d, M > 60 M⊕) are almost always found alone around their stars, but four out of hundreds known have inner companion planets. These rare companions allow us to constrain the hot jupiter’s formation history by ruling out high-eccentricity tidal migration. Less is known about inner companions to hot Saturn-mass planets. We report here the discovery of the TOI-2000 system, which features a hot Saturn-mass planet with a smaller inner companion. The mini-neptune TOI-2000 b (2.70 ± 0.15 R⊕, 11.0 ± 2.4 M⊕) is in a 3.10-d orbit, and the hot saturn TOI-2000 c ($8.14_{-0.30}^{+0.31}$ R⊕ , $81.7_{-4.6}^{+4.7}$ M⊕) is in a 9.13-d orbit. Both planets transit their host star TOI-2000 (TIC 371188886, V = 10.98, TESS magnitude = 10.36), a metal-rich ([Fe/H] = 0.439 $_{-0.043}^{+0.041}$) G dwarf 173 pc away. TESS observed the two planets in sectors 9–11 and 36–38, and we followed up with ground-based photometry, spectroscopy, and speckle imaging. Radial velocities from CHIRON, FEROS, and HARPS allowed us to confirm both planets by direct mass measurement. In addition, we demonstrate constraining planetary and stellar parameters with MIST stellar evolutionary tracks through Hamiltonian Monte Carlo under the PyMC framework, achieving higher sampling efficiency and shorter run time compared to traditional Markov chain Monte Carlo. Having the brightest host star in the V band among similar systems, TOI-2000 b and c are superb candidates for atmospheric characterization by the JWST, which can potentially distinguish whether they formed together or TOI-2000 c swept along material during migration to form TOI-2000 b.
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hal-04729522 , version 1 (10-10-2024)

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Lizhou Sha, Andrew Vanderburg, Chelsea Huang, David Armstrong, Rafael Brahm, et al.. TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system. Monthly Notices of the Royal Astronomical Society, 2023, 524 (1), pp.1113-1138. ⟨10.1093/mnras/stad1666⟩. ⟨hal-04729522⟩
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