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UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b

UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_03848956v1

UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b

About this item

Full title

UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2022-04, Vol.604 (7904), p.49-52

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

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...

Alternative Titles

Full title

UV absorption by silicate cloud precursors in ultra-hot Jupiter WASP-178b

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_hal_primary_oai_HAL_hal_03848956v1

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_03848956v1

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/s41586-022-04453-2

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