The Astrophysical Journal Letters (Jan 2023)

TOI-1859b: A 64 Day Warm Jupiter on an Eccentric and Misaligned Orbit

  • Jiayin Dong,
  • Songhu Wang,
  • Malena Rice,
  • George Zhou,
  • Chelsea X. Huang,
  • Rebekah I. Dawson,
  • Gudmundur K. Stefánsson,
  • Samuel Halverson,
  • Shubham Kanodia,
  • Suvrath Mahadevan,
  • Michael W. McElwain,
  • Jaime A. Alvarado-Montes,
  • Joe P. Ninan,
  • Paul Robertson,
  • Arpita Roy,
  • Christian Schwab,
  • Sarah E. Logsdon,
  • Ryan C. Terrien,
  • Karen A. Collins,
  • Gregor Srdoc,
  • Ramotholo Sefako,
  • Didier Laloum,
  • David W. Latham,
  • Allyson Bieryla,
  • Paul A. Dalba,
  • Diana Dragomir,
  • Steven Villanueva Jr.,
  • Steve B. Howell,
  • George R. Ricker,
  • S. Seager,
  • Joshua N. Winn,
  • Jon M. Jenkins,
  • Avi Shporer,
  • David Rapetti

DOI
https://doi.org/10.3847/2041-8213/acd93d
Journal volume & issue
Vol. 951, no. 2
p. L29

Abstract

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Warm Jupiters are close-in giant planets with relatively large planet–star separations (i.e., 10 < a / R _⋆ < 100). Given their weak tidal interactions with their host stars, measurements of stellar obliquity may be used to probe the initial obliquity distribution and dynamical history for close-in gas giants. Using spectroscopic observations, we confirm the planetary nature of TOI-1859b and determine the stellar obliquity of TOI-1859 to be λ = 38.9 ${}_{-2.7}^{+2.8}$ ° relative to its planetary companion using the Rossiter–McLaughlin effect. TOI-1859b is a 64 day warm Jupiter orbiting around a late F dwarf and has an orbital eccentricity of 0.57 ${}_{-0.16}^{+0.12}$ inferred purely from transit light curves. The eccentric and misaligned orbit of TOI-1859b is likely an outcome of dynamical interactions, such as planet–planet scattering and planet–disk resonance crossing.

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