Spectroscopic characterisation of close orbiting extrasolar giant planets

J. R. Barnes, Travis S. Barman, H. R.A. Jones, C. J. Leigh, A. Collier Cameron, Lisa Prato, R. Barber

Research output: Contribution to journalConference articlepeer-review

1 Scopus citations


A number of successful mid-infrared detections and studies of close orbiting extrasolar giant planetary atmospheres have been responsible for both driving and informing modelling efforts. Recent models have indicated that these planets may be subdivided into two groups, one with cooler atmospheres exhibiting solely absorption features, and a second comprising the most highly irradiated atmospheres which possess a temperature inversion leading to emission features. To date, no firm detection of the direct spectrum of a close orbiting extrasolar giant planet or "Hot Jupiter" has been made at near infrared wavelengths. We present the current status of such ground based studies of the bright systems, HD 189733b, HD 179949b.

Original languageEnglish (US)
Pages (from-to)417-420
Number of pages4
JournalAIP Conference Proceedings
StatePublished - 2009
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom
Duration: Jul 21 2008Jul 25 2008


  • (Stars:) planetary systems Stars
  • Formation
  • HD 179949
  • HD 189733
  • Individual
  • Infrared
  • Line
  • Profiles
  • Spectroscopic
  • Stars
  • Techniques

ASJC Scopus subject areas

  • Physics and Astronomy(all)


Dive into the research topics of 'Spectroscopic characterisation of close orbiting extrasolar giant planets'. Together they form a unique fingerprint.

Cite this