Exoplanets synchronization in the habitable zone: Learning from Venus' retrograde rotation
Sylvio Ferraz-Mello

TL;DR
This paper explores how exoplanets in the habitable zone can naturally reverse their rotation due to atmospheric and tidal torques, using Venus as a case study and mathematical modeling.
Contribution
It demonstrates that planetary rotation reversal is a common, non-catastrophic process driven by atmospheric and tidal interactions, challenging previous assumptions about planetary spin stability.
Findings
Retrograde rotation can occur without collisions or perturbations.
Tidal and atmospheric torques can cause bifurcations leading to retrograde spin.
Venus's retrograde rotation exemplifies this natural process.
Abstract
The rotation of a planet located in the habitable zone of a solar-type star can be reversed by a smooth process associated with the formation of its atmosphere and the increase of stronger torques, opposite to normal tidal torques. Our understanding of the rotational dynamics of Venus is revisited to analyze what might happen to exoplanets in the habitable zone of a solar-type star. The creep tide theory is used to calculate the gravitational tidal torque. Mathematical analysis is used to study the differential equation resulting from the combined effects of tidal torque and atmospheric torque. It shows that no collision with other bodies or critical planetary perturbations is necessary to convert the rotation of an Earth or super-Earth with a significant atmosphere formed during its evolution into a retrograde rotation. The reversal of a planet's rotation is not an exceptional event…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Scientific Research and Discoveries · Spacecraft Dynamics and Control
