Information content of exoplanetary transit spectra: An initial look

Michael R. Line, Xi Zhang, Gautam Vasisht, Vijay Natraj, Pin Chen, Yuk L. Yung

Research output: Contribution to journalArticlepeer-review

110 Scopus citations

Abstract

It has been shown that spectroscopy of transiting extrasolar planets can potentially provide a wealth of information about their atmospheres. Herein, we set up the inverse problem in spectroscopic retrieval. We use nonlinear optimal estimation to retrieve the atmospheric state (pioneered for Earth sounding by Rodgers). The formulation quantifies the degrees of freedom and information content of the spectrum with respect to geophysical parameters; herein, we focus specifically on temperature and composition. First, we apply the technique to synthetic near-infrared spectra and explore the influence of spectral signal-to-noise ratio and resolution (the two important parameters when designing a future instrument) on the information content of the data. As expected, we find that the number of retrievable parameters increases with increasing signal-to-noise ratio and resolution, although the gains quickly level off for large values. Second, we apply the methods to the previously studied dayside near-infrared emission spectrum of HD 189733b and compare the results of our retrieval with those obtained by others.

Original languageEnglish (US)
Article number93
JournalAstrophysical Journal
Volume749
Issue number1
DOIs
StatePublished - Apr 10 2012

Keywords

  • methods: data analysis
  • planets and satellites: atmospheres
  • planets and satellites: individual(HD189733b)
  • radiative transfer

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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