About the various contributions in Venus rotation rate and LOD
L.Cottereau, N.Rambaux, S.Lebonnois, J.Souchay

TL;DR
This paper analyzes the physical processes affecting Venus's rotation rate, finding that tidal torque from the Sun dominates, with variations of about 2 minutes, which are larger than atmospheric or core effects.
Contribution
It provides a comparative analysis of the major physical influences on Venus's rotation, applying models similar to Earth's to evaluate their relative impacts.
Findings
Tidal torque causes ~2 minutes of rotation variation.
Atmospheric effects induce 25-50 seconds of variation.
Core effects contribute 3-20 seconds of variation.
Abstract
% context heading (optional) {Thanks to the Venus Express Mission, new data on the properties of Venus could be obtained in particular concerning its rotation.} % aims heading (mandatory) {In view of these upcoming results, the purpose of this paper is to determine and compare the major physical processes influencing the rotation of Venus, and more particularly the angular rotation rate.} % methods heading (mandatory) {Applying models already used for the Earth, the effect of the triaxiality of a rigid Venus on its period of rotation are computed. Then the variations of Venus rotation caused by the elasticity, the atmosphere and the core of the planet are evaluated.} % results heading (mandatory) {Although the largest irregularities of the rotation rate of the Earth at short time scales are caused by its atmosphere and elastic deformations, we show that the Venus ones are dominated by…
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