CaltechAUTHORS
  A Caltech Library Service

A Spitzer Spectrum of the Exoplanet HD 189733b

Grillmair, C. J. and Charbonneau, D. and Burrows, A. S. and Armus, L. and Stauffer, J. R. and Meadows, V. and Van Cleve, J. and Levine, D. (2007) A Spitzer Spectrum of the Exoplanet HD 189733b. Astrophysical Journal Letters, 658 (2). L115-L118. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:20100506-122421966

[img]
Preview
PDF - Published Version
See Usage Policy.

94Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20100506-122421966

Abstract

We report on the measurement of the 7.5-14.7 μm spectrum for the transiting extrasolar giant planet HD 189733b using the Infrared Spectrograph on the Spitzer Space Telescope. Although the observations comprise only 12 hr of telescope time, the continuum is well measured and has a flux ranging from 0.6 to 1.8 mJy over the wavelength range, or 0.49% ± 0.02% of the flux of the parent star. The variation in the measured fractional flux is very nearly flat over the entire wavelength range and shows no indication of significant absorption by water or methane, in contrast with the predictions of most atmospheric models. Models with strong day/night differences appear to be disfavored by the data, suggesting that heat redistribution to the night side of the planet is highly efficient.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/513741DOIArticle
http://iopscience.iop.org/1538-4357/658/2/L115PublisherArticle
ORCID:
AuthorORCID
Grillmair, C. J.0000-0003-4072-169X
Charbonneau, D.0000-0002-9003-484X
Burrows, A. S.0000-0002-3099-5024
Armus, L.0000-0003-3498-2973
Stauffer, J. R.0000-0003-3595-7382
Additional Information:© 2007 American Astronomical Society. Received 2007 January 19; accepted 2007 February 12; published 2007 February 23. We are grateful to an anonymous referee for several suggestions that significantly improved the analysis and presentation of this work. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. This study was supported in part by NASA grant NNGO4GL22G and through the NASA Astrobiology Institute under Cooperative Agreement CAN-02-OSS-02 issued through the Office of Space Science.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASANNGO4GL22G
NASACAN-02-OSS-02
Subject Keywords:binaries: eclipsing; planetary systems; stars: individual (HD 189733, HD 189733)
Issue or Number:2
Record Number:CaltechAUTHORS:20100506-122421966
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100506-122421966
Official Citation:C. J. Grillmair et al 2007 ApJ 658 L115 doi: 10.1086/513741
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:18168
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:06 May 2010 21:16
Last Modified:09 Mar 2020 13:18

Repository Staff Only: item control page