Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon
Michael Efroimsky, Michaela Walterova, Yeva Gevorgyan, Amirhossein Bagheri, Valeri V. Makarov, Amir Khan

TL;DR
This paper explores how the Pluto-Charon system could have achieved mutual synchronization through tidal approach rather than recession, analyzing the conditions, scenarios, and geophysical implications of such evolution.
Contribution
It introduces a detailed analysis of tidal approach synchronization, compares it with tidal recession, and applies it to the Pluto-Charon system considering capture and spin-reversal scenarios.
Findings
Capture scenario is more consistent with geophysical evidence.
Temporary spin-orbit resonances can occur during early evolution.
Lower tidal stress and dissipation explain lack of fracture patterns.
Abstract
It is usually taken for granted that mutual synchronisation of a tidal two-body system is attained through tidal recession, assuming the reduced Hill sphere is not reached. However, synchronisation can be achieved also via tidal approach, provided the Roche limit is not crossed. For each of the two scenarios, we derive the condition under which the evolving synchronicity radius catches up with the tidally evolving orbit. We consider the two scenarios for the Pluto-Charon system and examine the impact-origin hypothesis of Charon's formation against capture. Based on geophysical evidence, we propose that capture appears more likely. Motivated by this conclusion, we investigate the capture scenario, wherein the orbital evolution of Charon starts at a larger distance than present and undergoes tidal descent, both analytically and numerically. We also consider the possibility that Pluto's…
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