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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 4.

Solutions of the five selected TNOs (see Table 1) for (ac) as a function of the mass silicate ratio σ. The line with circles represents the heterogeneous solutions computed from Clairaut’s equations and the line with squares are plotted for the MacLaurin solutions. The two sets of solutions are close at σ = 0 and 1 as expected (see Figure 1(a) for an estimation of the differences). The figure shows that the difference between the homogenous and stratified solutions can be larger than the observation uncertainties, at least for Makemake and Salacia.

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