The Astronomical Journal (Jan 2024)

Two Earth-size Planets and an Earth-size Candidate Transiting the nearby Star HD 101581

  • Michelle Kunimoto,
  • Zifan Lin,
  • Sarah Millholland,
  • Alexander Venner,
  • Natalie R. Hinkel,
  • Avi Shporer,
  • Andrew Vanderburg,
  • Jeremy Bailey,
  • Rafael Brahm,
  • Jennifer A. Burt,
  • R. Paul Butler,
  • Brad Carter,
  • David R. Ciardi,
  • Karen A. Collins,
  • Kevin I. Collins,
  • Knicole D. Colón,
  • Jeffrey D. Crane,
  • Tansu Daylan,
  • Matías R. Díaz,
  • John P. Doty,
  • Fabo Feng,
  • Eike W. Guenther,
  • Jonathan Horner,
  • Steve B. Howell,
  • Jan Janik,
  • Hugh R. A. Jones,
  • Petr Kabáth,
  • Shubham Kanodia,
  • Colin Littlefield,
  • Hugh P. Osborn,
  • Simon O’Toole,
  • Martin Paegert,
  • Pavel Pintr,
  • Richard P. Schwarz,
  • Steve Shectman,
  • Gregor Srdoc,
  • Keivan G. Stassun,
  • Johanna K. Teske,
  • Joseph D. Twicken,
  • Leonardo Vanzi,
  • Sharon X. Wang,
  • Robert A. Wittenmyer,
  • Jon M. Jenkins,
  • George R. Ricker,
  • Sara Seager,
  • Joshua Winn

DOI
https://doi.org/10.3847/1538-3881/ad9266
Journal volume & issue
Vol. 169, no. 1
p. 47

Abstract

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We report the validation of multiple planets transiting the nearby ( d = 12.8 pc) K5V dwarf HD 101581 (GJ 435, TOI–6276, TIC 397362481). This system consists of at least two Earth-size planets whose orbits are near a mutual 4:3 mean-motion resonance, HD 101581 b ( ${R}_{p}={0.956}_{-0.061}^{+0.063}\,{R}_{\oplus }$ , P = 4.47 days) and HD 101581c ( ${R}_{p}={0.990}_{-0.070}^{+0.070}\,{R}_{\oplus }$ , P = 6.21 days). Both planets were discovered in Sectors 63 and 64 TESS observations and statistically validated with supporting ground-based follow-up. We also identify a signal that probably originates from a third transiting planet, TOI-6276.03 ( ${R}_{p}={0.982}_{-0.098}^{+0.114}\,{R}_{\oplus }$ , P = 7.87 days). These planets are remarkably uniform in size and their orbits are evenly spaced, representing a prime example of the “peas-in-a-pod” architecture seen in other compact multiplanet systems. At V = 7.77, HD 101581 is the brightest star known to host multiple transiting planets smaller than 1.5 R _⊕ . HD 101581 is a promising system for atmospheric characterization and comparative planetology of small planets.

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