Characterization of the hot Neptune GJ 436 b with Spitzer and ground-based observations

  • B. O. Demory
  • , M. Gillon
  • , T. Barman
  • , X. Bonfils
  • , M. Mayor
  • , T. Mazeh
  • , D. Queloz
  • , S. Udry
  • , F. Bouchy
  • , X. Delfosse
  • , T. Forveille
  • , F. Mallmann
  • , F. Pepe
  • , C. Perrier

Research output: Contribution to journalArticlepeer-review

84 Scopus citations

Abstract

We present Spitzer Space Telescope infrared photometry of a secondary eclipse of the hot Neptune GJ 436 b. The observations were obtained using the 8-μm band of the InfraRed Array Camera (IRAC). The data spanning the predicted time of secondary eclipse show a clear flux decrement with the expected shape and duration. The observed eclipse depth of 0.58 mmag allows us to estimate a blackbody brightness temperature of TP = 717 ± 35 K at 8 μm. We compare this infrared flux measurement to a model of the planetary thermal emission, and show that this model reproduces properly the observed flux decrement. The timing of the secondary eclipse confirms the non-zero orbital eccentricity of the planet, while also increasing its precision (e = 0.14 ± 0.01). Additional new spectroscopic and photometric observations allow us to estimate the rotational period of the star and to assess the potential presence of another planet.

Original languageEnglish (US)
Pages (from-to)1125-1129
Number of pages5
JournalAstronomy and astrophysics
Volume475
Issue number3
DOIs
StatePublished - Dec 2007
Externally publishedYes

Keywords

  • Eclipses
  • Infrared: general
  • Planetary systems
  • Stars: individual: GJ 436
  • Techniques: photometric
  • Techniques: spectroscopic

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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