Exometeorology
Exometeorology is the study of atmospheric conditions of exoplanets and other celestial bodies outside the Solar System, such as brown dwarfs.[1][2] The diversity of possible sizes, compositions, and temperatures for exoplanets (and brown dwarfs) leads to a similar diversity of theorized atmospheric conditions. For example, a gas giant's orbital period can determine whether its wind patterns are primarily advective (heat and air flowing from the top of the star-heated atmosphere to the bottom) or convective (heat and air flowing from down near the gradually contracting planet's core up through the atmosphere).[3]
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In 2012, an international team of astronomers from the Institut d'Astrophysique de Paris and the Institut de Planétologie et d'Astrophysique de Grenoble detected meteorological variations in the atmosphere of the exoplanet HD 189733 b using the Hubble Space Telescope. [2] In 2017, astronomers using a telescope at the European Southern Observatory (ESO) in Chile found an atmosphere on earth-sized exoplanet Gliese 1132 b.[4]
See Also
- Atmosphere and Extraterrestrial Atmosphere
- Atmospheric circulation of exoplanets; the mathematical models governing exoplanetary air circulation
- Atmospheric physics
References
- Allers, Katelyn (2019-10-10). "Exometeorology: Determining atmospheric ..., Dr. K. Allers". Western Events Calendar. The University of Western Ontario. Retrieved 2023-03-14.
- "Exoplanets subject to meteorological variations". ScienceDaily. Délégation Paris Michel-Ange. 2012-07-10. Retrieved 2023-03-14.
- Stevenson, David S. (2016). The Exo-Weather Report : Exploring Diverse Atmospheric Phenomena Around the Universe. Switzerland: Springer Cham. pp. 370–371. ISBN 978-3-319-25679-5. OCLC 957655924.
- Lewin, Sarah (2017-04-06). "Discovery! Atmosphere Spotted on Nearly Earth-Size Exoplanet in First". Space.com. Retrieved 2023-03-14.