UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b
UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b
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London: Nature Publishing Group UK
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Language
English
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London: Nature Publishing Group UK
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Contents
Aerosols have been found to be nearly ubiquitous in substellar atmospheres
1
–
3
. The precise temperature at which these aerosols begin to form in exoplanets has yet to be observationally constrained. Theoretical models and observations of muted spectral features indicate that silicate clouds play an important role in exoplanets betwee...
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UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b
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TN_cdi_hal_primary_oai_HAL_hal_03848956v1
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_03848956v1
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-022-04453-2