Exoplanet atmospheremeasurements from transmission spectroscopy and other planet star combined light observations
Handbook of Exoplanets, Page: 2083-2105
2018
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- 117Captures
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Book Chapter Description
It is possible to learn a great deal about exoplanet atmospheres even when we cannot spatially resolve the planets from their host stars. In this chapter, we overview the basic techniques used to characterize transiting exoplanets-transmission spectroscopy, emission and reflection spectroscopy, and full-orbit phase curve observations. We discuss practical considerations, including current and future observing facilities and best practices for measuring precise spectra. We also highlight major observational results on the chemistry, climate, and cloud properties of exoplanets.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85086424798&origin=inward; http://dx.doi.org/10.1007/978-3-319-55333-7_100; http://link.springer.com/10.1007/978-3-319-55333-7_100; http://link.springer.com/content/pdf/10.1007/978-3-319-55333-7_100; https://dx.doi.org/10.1007/978-3-319-55333-7_100; https://link.springer.com/referenceworkentry/10.1007/978-3-319-55333-7_100
Springer Nature America, Inc
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