The role of ice lines in the formation of Uranus and Neptune.

The role of ice lines in the formation of Uranus and Neptune.

<p>We aim at investigating whether the chemical composition of the outer region of the protosolar nebula can be consistent with current estimates of the elemental abundances in the ice giants. To do so, we use a self-consistent evolutionary disc and transport model to investigate the time and...

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Bibliografische gegevens
Hoofdauteurs:	Mousis, O, Aguichine, A, Helled, R, Irwin, PGJ, Lunine, JI
Formaat:	Journal article
Taal:	English
Gepubliceerd in:	Royal Society, The 2020

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