The Astrophysical Journal Letters (Jan 2023)

TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

  • Jack Lubin,
  • Xian-Yu Wang,
  • Malena Rice,
  • Jiayin Dong,
  • Songhu Wang,
  • Brandon T. Radzom,
  • Paul Robertson,
  • Gudmundur Stefansson,
  • Jaime A. Alvarado-Montes,
  • Corey Beard,
  • Chad F. Bender,
  • Arvind F. Gupta,
  • Samuel Halverson,
  • Shubham Kanodia,
  • Dan Li,
  • Andrea S. J. Lin,
  • Sarah E. Logsdon,
  • Emily Lubar,
  • Suvrath Mahadevan,
  • Joe P. Ninan,
  • Jayadev Rajagopal,
  • Arpita Roy,
  • Christian Schwab,
  • Jason T. Wright

DOI
https://doi.org/10.3847/2041-8213/ad0fea
Journal volume & issue
Vol. 959, no. 1
p. L5

Abstract

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We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter–McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN Telescope at Kitt Peak National Observatory. TOI-1670 hosts a sub-Neptune ( P ∼ 11 days; planet b) interior to the warm Jovian ( P ∼ 40 days; planet c), which presents an opportunity to investigate the dynamics of a warm Jupiter with an inner companion. Additionally, TOI-1670 c is now among the longest-period planets to date to have its sky-projected obliquity angle measured. We find planet c is well aligned to the host star, with λ = − 0.°3 ± 2.°2. TOI-1670 c joins a growing census of aligned warm Jupiters around single stars and aligned planets in multiplanet systems.

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