The Astronomical Journal (Jan 2024)

TESS Hunt for Young and Maturing Exoplanets (THYME). X. A Two-planet System in the 210 Myr MELANGE-5 Association

  • Pa Chia Thao,
  • Andrew W. Mann,
  • Madyson G. Barber,
  • Adam L. Kraus,
  • Benjamin M. Tofflemire,
  • Jonathan L. Bush,
  • Mackenna L. Wood,
  • Karen A. Collins,
  • Andrew Vanderburg,
  • Samuel N. Quinn,
  • George Zhou,
  • Elisabeth R. Newton,
  • Carl Ziegler,
  • Nicholas Law,
  • Khalid Barkaoui,
  • Francisco J. Pozuelos,
  • Mathilde Timmermans,
  • Michaël Gillon,
  • Emmanuël Jehin,
  • Richard P. Schwarz,
  • Tianjun Gan,
  • Avi Shporer,
  • Keith Horne,
  • Ramotholo Sefako,
  • Olga Suarez,
  • Djamel Mekarnia,
  • Tristan Guillot,
  • Lyu Abe,
  • Amaury H. M. J. Triaud,
  • Don J. Radford,
  • Ana Isabel Lopez Murillo,
  • George R. Ricker,
  • Joshua N. Winn,
  • Jon M. Jenkins,
  • Luke G. Bouma,
  • Michael Fausnaugh,
  • Natalia M. Guerrero,
  • Michelle Kunimoto

DOI
https://doi.org/10.3847/1538-3881/ad4993
Journal volume & issue
Vol. 168, no. 1
p. 41

Abstract

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Young (<500 Myr) planets are critical to studying how planets form and evolve. Among these young planetary systems, multiplanet configurations are particularly useful, as they provide a means to control for variables within a system. Here, we report the discovery and characterization of a young planetary system, TOI-1224. We show that the planet host resides within a young population we denote as MELANGE-5. By employing a range of age-dating methods—isochrone fitting, lithium abundance analysis, gyrochronology, and Gaia excess variability—we estimate the age of MELANGE-5 to be 210 ± 27 Myr. MELANGE-5 is situated in close proximity to previously identified younger (80–110 Myr) associations, Crius 221 and Theia 424/Volans-Carina, motivating further work to map out the group boundaries. In addition to a planet candidate detected by the TESS pipeline and alerted as a TESS object of interest, TOI-1224 b, we identify a second planet, TOI-1224 c, using custom search tools optimized for young stars ( Notch and LOCoR ). We find that the planets are 2.10 ± 0.09 R _⊕ and 2.88 ± 0.10 R _⊕ and orbit their host star every 4.18 and 17.95 days, respectively. With their bright ( K = 9.1 mag), small ( R _* = 0.44 R _⊙ ), and cool ( T _eff = 3326 K) host star, these planets represent excellent candidates for atmospheric characterization with JWST.

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