A Theory for the Radius of the Transiting Giant Planet HD 209458B

Adam S. Burrows, D. Sudarsky, W. B. Hubbard

Research output: Contribution to journalArticlepeer-review

120 Scopus citations


Using a full frequency-dependent atmosphere code that can incorporate irradiation by a central primary star, we calculate self-consistent boundary conditions for the evolution of the radius of the transiting planet HD 209458b. Using a well-tested extrasolar giant planet evolutionary code, we then calculate the behavior of this planet's radius with age. The measured radius is in fact a transit radius that resides high in HD 209458b's inflated atmosphere. Using our derived atmospheric and interior structures, we find that irradiation plus the proper interpretation of the transit radius can yield a theoretical radius that is within the measured error bars. We conclude that if HD 209458b's true transit radius is at the lower end of the measured range, an extra source of core heating power is not necessary to explain the transit observations.

Original languageEnglish (US)
Pages (from-to)545-551
Number of pages7
JournalAstrophysical Journal
Issue number1 I
StatePublished - Sep 1 2003

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


  • Planetary systems
  • Planets and satellites: General
  • Stars: Individual (hd 209458)


Dive into the research topics of 'A Theory for the Radius of the Transiting Giant Planet HD 209458B'. Together they form a unique fingerprint.

Cite this