Published October 29, 2015
| Version public
Book Section - Chapter
Photochemistry of Terrestrial Exoplanet Atmospheres
Contributors
Abstract
Terrestrial exoplanets are exciting objects to study because they could be potential habitats for extraterrestrial life. Both the search and the characterization of terrestrial exoplanets are flourishing. Particularly, NASA's Kepler spacecraft has discovered Earth-sized planets receiving similar amount of radiative heat as Earth. Central in the studies of terrestrial exoplanets is to characterize their atmospheres and to search for potential biosignature gases (the atmospheric components that indicate biogenic surface emissions). To achieve this goal, a deep understanding of the key physical and chemical processes that control the atmospheric composition and the atmosphere-surface interaction is pivotal.
Additional Information
© 2015 Springer.Additional details
Identifiers
- Eprint ID
- 78236
- DOI
- 10.1007/978-3-662-45052-9_12
- Resolver ID
- CaltechAUTHORS:20170615-082032083
Dates
- Created
-
2017-06-15Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
Caltech Custom Metadata
- Series Name
- Springer Geophysics