Photochemical Hazes Can Trace the C/O Ratio in Exoplanet Atmospheres

Photochemical hazes are suspected to obscure molecular features, such as water, from detection in the transmission spectra of exoplanets with atmospheric temperatures

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Bibliographic Details
Published in:Astrophysical journal. Letters 2023-02, Vol.943 (2), p.L26
Main Authors: Corrales, Lía, Gavilan, Lisseth, Teal, D. J., Kempton, Eliza M.-R.
Format: Article
Language:English
Subjects:
Abundance
Astrochemistry
Atmosphere
Atmospheric composition
Atmospheric models
Atmospheric temperature
Exoplanet atmospheric composition
Extrasolar planets
Haze
Helium
Laboratories
Laboratory astrophysics
Metallicity
Modelling
Organic compounds
Oxygen
Photochemicals
Planetary atmospheres
Refractivity
Spectra
Titan
Wavelengths
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Description
Summary:Photochemical hazes are suspected to obscure molecular features, such as water, from detection in the transmission spectra of exoplanets with atmospheric temperatures
ISSN:2041-8205
2041-8213
DOI:10.3847/2041-8213/acaf86