Cited by 1,346Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchAstro and Planetary Science

Detection of an Extrasolar Planet Atmosphere

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Charbonneau, David, Brown, Timothy M., Noyes, Robert W., Gilliland, Ronald L.·2002·The Astrophysical Journal

Abstract

We report high-precision spectrophotometric observations of four planetary transits of HD 209458, in the region of the sodium resonance doublet at 589.3 nm. We find that the photometric dimming during transit in a bandpass centered on the sodium feature is deeper by (2.32 ± 0.57) × 10 -4 relative to simultaneous observations of the transit in adjacent bands. We interpret this additional dimming as absorption from sodium in the planetary atmosphere, as recently predicted from several theoretical modeling efforts. Our model for a cloudless planetary atmosphere with a solar abundance of sodium in atomic form predicts more sodium absorption than we observe. There are several possibilities that may account for this reduced amplitude, including reaction of atomic sodium into molecular gases and/or condensates, photoionization of sodium by the stellar flux, a low primordial abundance of sodium, and the presence of clouds high in the atmosphere.

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Crossref · 10.1086/338770

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  • Transit spectroscopy has been used to identify sodium and water in the atmosphere of extrasolar gas giants.

    “This technique has been used to identify sodium and water in the atmosphere of extrasolar gas giants (Charbonneau et al., 2002; Kreidberg et al., 2014b).”

    From The Astrobiology Primer v2.0 (2016) · cites this paper as Charbonneau et al., 2002

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Authors
Charbonneau, D., Brown, T. M., Noyes, R. W., & Gilliland, R. L.
Affiliations
  • California Institute of Technology (US)
  • NSF National Center for Atmospheric Research (US)
  • Center for Astrophysics Harvard & Smithsonian (US)
  • Space Telescope Science Institute (US)
Venue
The Astrophysical Journal
Published
2002-03-20
Volume
568
Issue
1
Pages
377-384
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2096390283
Cited by
1,346
References
1
Citations by year
2026: 27 · 2025: 31 · 2024: 57 · 2023: 61 · 2022: 55 · 2021: 55 · 2020: 100 · 2019: 57 · 2018: 76 · 2017: 70 · 2016: 65 · 2015: 64 · 2014: 60 · 2013: 57 · 2012: 54
FWCI
29.17
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (NAS 5-26555)
  • National Aeronautics and Space Administration (NAG510854, NAS 526555, 526555)
  • Space Telescope Science Institute (NAS5- 26555, 5-26555, 26555)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
Keywords
HD 209458, exoplanet atmospheres, sodium uptake, planetary transits, transit photometry, photoionization

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