Different Inhomogeneous Evolutionary Histories for Uranus and Neptune
We present updated nonadiabatic and inhomogeneous evolution models for Uranus and Neptune, employing an interior composition of methane, ammonia, water, and rocks. Following the formation trends of the gas giants, Uranus and Neptune formation models are applied, where both planets begin with layers...
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| Glavni autor: | |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2025-01-01
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| Serija: | The Astrophysical Journal Letters |
| Teme: | |
| Online pristup: | https://doi.org/10.3847/2041-8213/adf3a5 |
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