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Synchronization of a Tidal Binary by Inward Orbital Migration. The Case of Pluto and Charon

  • Authors: Michael Efroimsky, Michaela Walterová, Yeva Gevorgyan, Amirhossein Bagheri, Valeri V. Makarov, Amir Khan

Michael Efroimsky et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Tidal evolution of the Pluto–Charon system. Initially prograde Pluto and Charon with various initial ratios of rotation rates Ωm00 and the initial eccentricity e0 = 0.4. Panel (a): semimajor axis ratio a/ap (where ap is the present semimajor axis value); panel (b): eccentricity e; panel (c): spin rates Ω/n (shades of blue) and Ωm/n (shades of red); panel (d): tidally dissipated power, ﹩\dot{E}﹩ and ﹩{\dot{E}}_{{\rm{m}}}﹩.

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