HAT-P-38h: a Saturn-mass planet transiting a late G star

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  • Bun'ei Sato
  • Joel D. Hartman
  • Gaspar Á. Bakos
  • Bence Béky
  • Guillermo Torres
  • David W. Latham
  • Geza Kovacs
  • Zoltán Csubry
  • Kaloyan Penev
  • Robert W. Noyes
  • Samuel N. Quinn
  • Mark Everett
  • Gilbert A. Esquerdo
  • Debra A. Fischer
  • Andrew W. Howard
  • John A. Johnson
  • Geoff W. Marcy
  • Dimitar D. Sasselov
  • Tamás Szklenár
  • József Lázár
  • István Papp
  • Pál Sári
We report on the discovery of HAT-P-38b, a Saturn-mass exoplanet, transiting the V = 12.56 dwarf star GSC 2314-00559 on a P = 4.6404 d circular orbit. The host star is a 0.89 M-circle dot late G dwarf, with solar metallicity and a radius of 0.92 R-circle dot. The planetary companion has a mass of 0.27 M-J and a radius of 0.82 R-J. HAT-P-38b is one of the planets the mass and radius of which have ever been discovered to be the closest to those of Saturn.
Original languageEnglish
Article number97
JournalPublications of the Astronomical Society of Japan
Volume64
Issue number5
Number of pages8
ISSN0004-6264
DOIs
Publication statusPublished - 2012

ID: 49413135