3.6 and 4.5 Micron Phase Curves and Evidence for Non-Equilibrium Chemistry in the Atmosphere of Extrasolar Planet HD 189733b
We present new, full-orbit observations of the infrared phase variations of the canonical hot Jupiter HD 189733b obtained in the 3.6 and 4.5 micron bands using the Spitzer Space Telescope. When combined with previous phase curve observations at 8.0 and 24 micron, these data allow us to characterize...
Main Authors: | Knutson, H, Lewis, N, Fortney, J, Burrows, A, Showman, A, Cowan, N, Agol, E, Aigrain, S, Charbonneau, D, Deming, D, Desert, J, Henry, G, Langton, J, Laughlin, G |
---|---|
Format: | Journal article |
Language: | English |
Published: |
Institute of Physics Publishing
2012
|
Similar Items
-
The 4.5 mm full-orbit phase curve of the hot Jupiter HD 209458b
by: Zellem, Robert T., et al.
Published: (2015) -
Probing the haze in the atmosphere of HD 189733b with HST/WFC3
transmission spectroscopy
by: Gibson, N, et al.
Published: (2012) -
Tight constraints on the existence of additional planets around HD 189733
by: Hrudková, M, et al.
Published: (2010) -
Probing the haze in the atmosphere of HD 189733b with Hubble Space Telescope/WFC3 transmission spectroscopy
by: Gibson, N, et al.
Published: (2012) -
Hubble Space Telescope Transmission Spectroscopy of the Exoplanet HD
189733b: High-altitude atmospheric haze in the optical and near-UV with STIS
by: Sing, D, et al.
Published: (2011)