Evidence of three mechanisms explaining the radius anomaly of hot Jupiters

Context. The anomalously large radii of hot Jupiters are still not fully understood, and all of the proposed explanations are based on the idea that these close-in giant planets possess hot interiors. Most of the mechanisms proposed have been tested on a handful of exoplanets. Aims. We approach the...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021, Vol.645, p.A79
Hauptverfasser:	Sarkis, P., Mordasini, C., Henning, Th, Marleau, G. D., Mollière, P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Context Cooling rate Efficiency Extrasolar planets Gas giant planets Heating Irradiation Jupiter Luminosity Ohmic dissipation Planetary interiors
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