An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269*

, , , , , , and

© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation John Asher Johnson et al 2006 ApJ 652 1724 DOI 10.1086/508255

0004-637X/652/2/1724

Abstract

We report the detection of a Jupiter-mass planet in a 6.838 day orbit around the 1.28 M subgiant HD 185269. The eccentricity of HD 185269b (e = 0.30) is unusually large compared to other planets within 0.1 AU of their stars. Photometric observations demonstrate that the star is constant to ±0.0001 mag on the radial velocity period, strengthening our interpretation of a planetary companion. This planet was detected as part of our radial velocity survey of evolved stars located on the subgiant branch of the H-R diagram—also known as the Hertzsprung gap. These stars, which have masses between 1.2 and 2.5 M, play an important role in the investigation of the frequency of extrasolar planets as a function of stellar mass.

Export citation and abstract BibTeX RIS

Footnotes

  • Based on observations obtained at the Lick Observatory, which is operated by the University of California.

Please wait… references are loading.
10.1086/508255