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Beyond Point Masses. VI. Spin–Orbit Evolution of the Centaur Binary Typhon–Echidna

  • Authors: Benjamin Proudfoot, Will Grundy, Darin Ragozzine

Benjamin Proudfoot et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

A corner plot showing the posterior distribution from our non-Keplerian orbit fit. At the top of each column, marginal (one-dimensional) posterior distributions for each parameter are shown. Beneath, two-dimensional joint posterior distributions are shown for every pair of parameters. Contours on the joint distributions show the 0.5σ, 1σ, 1.5σ, and 2σ confidence intervals. Horizontal and vertical lines show the location of the best-fit parameter set.

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