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...
Asıl Yazarlar: | Mousis, O, Aguichine, A, Helled, R, Irwin, PGJ, Lunine, JI |
---|---|
Materyal Türü: | Journal article |
Dil: | English |
Baskı/Yayın Bilgisi: |
Royal Society, The
2020
|
Benzer Materyaller
-
Neptune and Uranus: ice or rock giants?
Yazar:: Teanby, NA, ve diğerleri
Baskı/Yayın Bilgisi: (2020) -
Insights on the Formation Conditions of Uranus and Neptune from Their Deep Elemental Compositions
Yazar:: Olivier Mousis, ve diğerleri
Baskı/Yayın Bilgisi: (2024-01-01) -
Modelling the seasonal cycle of Uranus’s colour and magnitude, and comparison with Neptune
Yazar:: Irwin, PGJ, ve diğerleri
Baskı/Yayın Bilgisi: (2024) -
Scientific rationale for Uranus and Neptune in situ explorations
Yazar:: Mousis, O, ve diğerleri
Baskı/Yayın Bilgisi: (2017) -
Variations of brightness temperatures of Uranus and Neptune
Yazar:: V. M. Krushevs’ka, ve diğerleri
Baskı/Yayın Bilgisi: (2003-12-01)