A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere

Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot Jupiters (relative to their host stars) provide insight into their formation location and subsequent orbital migration 1 , 2 . Hot Jupiters that form beyond the major volatile (H 2 O/CO/CO 2 ) ice lines and sub...

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Veröffentlicht in:	Nature (London) 2021-10, Vol.598 (7882), p.580-584
Hauptverfasser:	Line, Michael R., Brogi, Matteo, Bean, Jacob L., Gandhi, Siddharth, Zalesky, Joseph, Parmentier, Vivien, Smith, Peter, Mace, Gregory N., Mansfield, Megan, Kempton, Eliza M.-R., Fortney, Jonathan J., Shkolnik, Evgenya, Patience, Jennifer, Rauscher, Emily, Désert, Jean-Michel, Wardenier, Joost P.
Format:	Artikel
Sprache:	eng
Schlagworte:	639/33/445/824 639/33/445/862 Atmosphere Atmospheric gases Carbon Carbon dioxide Extrasolar planets Gas giant planets Humanities and Social Sciences Hydrogen Jupiter Jupiter (Planet) Jupiter atmosphere Measurement Metallicity Mixing ratio multidisciplinary Natural history Oxygen Planet formation Planets Science Science (multidisciplinary) Solar system Spectroscopic observation Velocity
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