Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy

Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy

Exoplanets that orbit close to their host stars are much more highly irradiated than their solar system counterparts. Understanding the thermal structures and appearances of these planets requires investigating how their atmospheres respond to such extreme stellar forcing. We present spectroscopic t...

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Bibliographic Details
Main Authors: Stevenson, K. B., Desert, J.-M., Line, Michael R., Bean, J. L., Fortney, Jonathan J., Showman, A. P., Kataria, T., Kreidberg, Laura, McCullough, Peter R., Henry, Gregory W., Charbonneau, D., Burrows, A., Madhusudhan, Nikku, Williamson, M. H., Homeier, Derek, Seager, Sara
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: American Association for the Advancement of Science (AAAS) 2015
Online Access:http://hdl.handle.net/1721.1/97911
https://orcid.org/0000-0002-6892-6948

Internet

http://hdl.handle.net/1721.1/97911
https://orcid.org/0000-0002-6892-6948

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