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haldemann_2024.md

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Option Possible values Description
models_haldemann2024 C0, C1, R0, R1, R2, E0, etc1. Iso-composition curve
T_out_haldemann2024 50, 300, 800, 1500, or 2000 Outer boundary temperature (K)
colors_haldemann2024 Any color Colors of each model

Notes: The pressure at which the integration of the internal structure was started was always set to 1 mbar. It is possible that for some combinations no transit radius is provided. This is the case if the radius of the planet is so big that the outermost layers would not be bound to the planet, for example, in the case of very small masses, high equilibrium temperatures and volatile rich compositions.

1 Below you can find all the iso-composition curves from Haldemann et al. (2024) available now (v1+) in mr-plotter. Just try and choose the one that better fits with the properties of your planet! This table was obtained from https://github.com/mnijh/BICEPS_mass_radius.

Model wCore wRock wH2O wH/He xFe,Core xS,Core xMgO,Mantle xSiO2,Mantle xFeO,Mantle
C0 1 0 0 0 1 0 N/A N/A N/A
C1 1 0 0 0 0.87 0.13 N/A N/A N/A
R0 0 1 0 0 N/A N/A 1 0 0
R1 0 1 0 0 N/A N/A 0.5 0.5 0
R2 0 1 0 0 N/A N/A 0.519 0.423 0.058
E0 0.32 0.68 0 0 0.87 0.13 0.519 0.423 0.058
W0 0 0 1 0 N/A N/A N/A N/A N/A
W1 0.3168 0.6732 0.01 0 1 0 0.5 0.5 0
W2 0.304 0.646 0.05 0 1 0 0.5 0.5 0
W3 0.288 0.612 0.1 0 1 0 0.5 0.5 0
W4 0.16 0.34 0.5 0 1 0 0.5 0.5 0
D0 0.319968 0.679932 0 0.0001 1 0 0.5 0.5 0
D1 0.31968 0.67932 0 0.001 1 0 0.5 0.5 0
D2 0.3168 0.6732 0 0.01 1 0 0.5 0.5 0
D3 0.288 0.612 0 0.1 1 0 0.5 0.5 0
D4 0.256 0.544 0 0.2 1 0 0.5 0.5 0
N0 0.316768 0.673132 0.01 0.0001 1 0 0.5 0.5 0
N1 0.31648 0.67252 0.01 0.001 1 0 0.5 0.5 0
N2 0.3136 0.6664 0.01 0.01 1 0 0.5 0.5 0
N3 0.2848 0.6052 0.01 0.1 1 0 0.5 0.5 0
N4 0.2528 0.5372 0.01 0.2 1 0 0.5 0.5 0
N5 0.287968 0.611932 0.1 0.0001 1 0 0.5 0.5 0
N6 0.28768 0.61132 0.1 0.001 1 0 0.5 0.5 0
N7 0.2848 0.6052 0.1 0.01 1 0 0.5 0.5 0
N8 0.256 0.544 0.1 0.1 1 0 0.5 0.5 0
N9 0.224 0.476 0.1 0.2 1 0 0.5 0.5 0