The Astronomical Journal (Jan 2023)

TESS Spots a Super-puff: The Remarkably Low Density of TOI-1420b

  • Stephanie Yoshida,
  • Shreyas Vissapragada,
  • David W. Latham,
  • Allyson Bieryla,
  • Daniel P. Thorngren,
  • Jason D. Eastman,
  • Mercedes López-Morales,
  • Khalid Barkaoui,
  • Charles Beichman,
  • Perry Berlind,
  • Lars A. Buchave,
  • Michael L. Calkins,
  • David R. Ciardi,
  • Karen A. Collins,
  • Rosario Cosentino,
  • Ian J. M. Crossfield,
  • Fei Dai,
  • Victoria DiTomasso,
  • Nicholas Dowling,
  • Gilbert A. Esquerdo,
  • Raquel Forés-Toribio,
  • Adriano Ghedina,
  • Maria V. Goliguzova,
  • Eli Golub,
  • Erica J. Gonzales,
  • Ferran Grau Horta,
  • Jesus Higuera,
  • Nora Hoch,
  • Keith Horne,
  • Steve B. Howell,
  • Jon M. Jenkins,
  • Jessica Klusmeyer,
  • Didier Laloum,
  • Jack J. Lissauer,
  • Sarah E. Logsdon,
  • Luca Malavolta,
  • Rachel A. Matson,
  • Elisabeth C. Matthews,
  • Kim K. McLeod,
  • Jennifer V. Medina,
  • Jose A. Muñoz,
  • Hugh P. Osborn,
  • Boris Safonov,
  • Joshua Schlieder,
  • Michael Schmidt,
  • Heidi Schweiker,
  • Sara Seager,
  • Alessandro Sozzetti,
  • Gregor Srdoc,
  • Guđmundur Stefánsson,
  • Ivan A. Strakhov,
  • Stephanie Striegel,
  • Joel Villaseñor,
  • Joshua N. Winn

DOI
https://doi.org/10.3847/1538-3881/acf858
Journal volume & issue
Vol. 166, no. 5
p. 181

Abstract

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We present the discovery of TOI-1420b, an exceptionally low-density ( ρ = 0.08 ± 0.02 g cm ^−3 ) transiting planet in a P = 6.96 days orbit around a late G-dwarf star. Using transit observations from TESS, LCOGT, Observatoire Privé du Mont, Whitin, Wendelstein, OAUV, Ca l’Ou, and KeplerCam, along with radial velocity observations from HARPS-N and NEID, we find that the planet has a radius of R _p = 11.9 ± 0.3 R _⊕ and a mass of M _p = 25.1 ± 3.8 M _⊕ . TOI-1420b is the largest known planet with a mass less than 50 M _⊕ , indicating that it contains a sizeable envelope of hydrogen and helium. We determine TOI-1420b’s envelope mass fraction to be ${f}_{\mathrm{env}}={82}_{-6}^{+7} \% $ , suggesting that runaway gas accretion occurred when its core was at most four to five times the mass of the Earth. TOI-1420b is similar to the planet WASP-107b in mass, radius, density, and orbital period, so a comparison of these two systems may help reveal the origins of close-in low-density planets. With an atmospheric scale height of 1950 km, a transmission spectroscopy metric of 580, and a predicted Rossiter–McLaughlin amplitude of about 17 m s ^−1 , TOI-1420b is an excellent target for future atmospheric and dynamical characterization.

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