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

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

  • 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.
OriginalsprogEngelsk
Artikelnummer97
TidsskriftPublications of the Astronomical Society of Japan
Vol/bind64
Udgave nummer5
Antal sider8
ISSN0004-6264
DOI
StatusUdgivet - 2012

Bibliografisk note

HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star

ID: 49413135