Figure 3 from Equilibrium Shapes of Large Trans-Neptunian Objects

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Equilibrium Shapes of Large Trans-Neptunian Objects

Authors: Nicolas Rambaux, Daniel Baguet, Frederic Chambat, and Julie C. Castillo-Rogez

2017 The Astrophysical Journal Letters 850 L9.

Provider: AAS Journals

Caption: Figure 3.

Solution of ν₃ = (a − c)₃/R computed for the two-layer model, developed to the order of 3, for the parametric space covered in this study and for specific bodies. σ = 0 corresponds to a homogeneous body of density equal to 920 kg m⁻³, whereas σ = 1 corresponds to a homogeneous body of density 3000 kg m⁻³.

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