Abstract
The varied surfaces and atmospheres of planets make them interesting places to live, explore, and study from afar. Unfortunately, the great distance to exoplanets makes it impossible to resolve their disk with current or near-term technology. It is still possible, however, to deduce spatial inhomogeneities in exoplanets provided that different regions are visible at different times—this can be due to rotation, orbital motion, and occultations by a star, planet, or moon. Astronomers have so far constructed maps of thermal emission and albedo for short-period giant planets. These maps constrain atmospheric dynamics and cloud patterns in exotic atmospheres. In the future, exo-cartography could yield surface maps of terrestrial planets, hinting at the geophysical and geochemical processes that shape them.
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Acknowledgements
The authors are grateful to the International Space Science Institute for hosting the exo-cartography workshops. N.B. Cowan acknowledges support from the McGill Space Institute and l’Institut de recherche sur les exoplanètes. Y. Fujii was supported by the NASA Postdoctoral Program at the NASA Goddard Institute for Space Studies, administered by Universities Space Research Association, as well as by the NASA Astrobiology Program through the Nexus for Exoplanet System Science. The authors thank J.C. Schwartz for creating many of the figures, as well as T. Bell, D. Keating, E. Rauscher, and T. Robinson for providing useful feedback on an earlier draft of this review.
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Cowan, N.B., Fujii, Y. (2021). Mapping Exoplanets. In: Deeg, H.J., Belmonte, J.A. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_147-2
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DOI: https://doi.org/10.1007/978-3-319-30648-3_147-2
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Latest
Mapping Exoplanets- Published:
- 19 January 2021
DOI: https://doi.org/10.1007/978-3-319-30648-3_147-2
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Original
Mapping Exoplanets- Published:
- 20 September 2017
DOI: https://doi.org/10.1007/978-3-319-30648-3_147-1