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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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Hovedforfatter: Roberto Tejada Arevalo
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2025-01-01
Serier:The Astrophysical Journal Letters
Fag:
Solar system gas giant planets
Uranus
Neptune
Planetary interior
Planetary structure
Atmospheric evolution
Online adgang:https://doi.org/10.3847/2041-8213/adf3a5
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