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The slow revolution of the Earth and Moon around their barycentrum does notinduce Coriolis accelerations. On the other hand, the motion of Sun and Earthis a rotation with Coriolis forces which appear not to have been calculatedyet, nor have the inertial accelerations within the system of motion of allthree celestial bodies. It is the purpose of this contribution to evaluate therelated Coriolis and centrifugal terms and to compare them to the availableatmospheric standard terms. It is a main result that the revolution is ofcentral importance in the combined dynamics of Earth, Moon and Sun. Covariantflow equations are well known tools for dealing with such complicated flowsettings. They are used here to quantify the effects of the Earth's revolutionaround the Earth-Moon barycenter and its rotation around the Sun on theatmospheric circulation. It is found that the motion around the Sun adds timedependent terms to the standard Coriolis forces. The related centrifugalaccelerations are presented. A major part of these accelerations is balanced bythe gravitational attraction by Moon and Sun, but important unbalancedcontributions remain. New light on the consequences of the Earth's revolutionis shed by repeating the calculations for a rotating Earth-Moon pair. It isfound that the revolution complicates the atmospheric dynamics.

Overlooked centrifugal and Coriolis forces in the Atmosphere due to the Earth's motion in the solar system