Thermal evolution of Uranus and Neptune - I. Adiabatic models

Free Access

Table 1

Model parameters for the Uranus and Neptune structure models, as well as EOS data used for H, He, and water (cf. Sect. 2.2 for details).

	H,He-EOS	H₂ O-EOS	Z₁	Z₂	M₁₂	M_core	M_H,He
					[M_E]	[M_E]	[M_E]
Uranus 1	REOS.3	Sesame	0.261	0.941	12.5	0.25	2.2
Uranus 2	REOS.3	Mazevet	0.273	0.96	12.44	0.79	2.0
Neptune 1	REOS.3	Sesame	0.42	0.91	15.0	1.06	2.4
Neptune 2	REOS.3	Mazevet	0.42	0.929	15.17	1.04	2.2
Neptune 3	Chabrier	Mazevet	0.424	0.92	15.17	1.05	2.3

Notes. The quantities are outer envelope metallicity Z₁, inner envelope metallicity Z₂, transition mass between outer and inner fluid envelope M₁₂, core mass M_core, and total mass of combined hydrogen and helium M_H,He.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.