English

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

Earth and Planetary Astrophysics 2015-06-03 v1 Solar and Stellar Astrophysics

Abstract

We report 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 0.89Msun late G-dwarf, with solar metallicity, and a radius of 0.92Rsun. The planetary companion has a mass of 0.27MJ, and radius of 0.82RJ. HAT-P-38b is one of the closest planets in mass and radius to Saturn ever discovered.

Keywords

Cite

@article{arxiv.1201.5075,
  title  = {HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star},
  author = {B. Sato and J. D. Hartman and G. Á. Bakos and B. Béky and G. Torres and D. W. Latham and G. Kovács and Z. Csubry and K. Penev and R. W. Noyes and L. A. Buchhave and S. N. Quinn and M. Everett and G. A. Esquerdo and D. A. Fischer and A. W. Howard and J. A. Johnson and G. W. Marcy and D. D. Sasselov and T. Szklenár and J. Lázár and I. Papp and P. Sári},
  journal= {arXiv preprint arXiv:1201.5075},
  year   = {2015}
}

Comments

9 pages, 5 figures, 6 tables, submitted to PASJ