Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?

ABSTRACT The origin of Uranus and Neptune has long been challenging to explain, due to the large orbital distances from the Sun. After a planetary embryo has been formed, the main accretion processes are likely pebble, gas, and planetesimal accretion. Previous studies of Uranus and Neptune formation...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-10, Vol.526 (4), p.4860-4876
Hauptverfasser:	Eriksson, Linn E J, Mol Lous, Marit A S, Shibata, Sho, Helled, Ravit
Format:	Artikel
Sprache:	eng
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