Rotating planets in Newtonian gravity
Christian Fronsdal

TL;DR
This paper develops and applies a variational action principle to model rotating planets, successfully predicting shapes, velocity fields, and rings with minimal parameters, and demonstrating its potential for planetary physics.
Contribution
It introduces a new, general action principle for modeling rotating fluid bodies, unifying potential and solid-body flows, and applies it to real planets with promising results.
Findings
Model fits planetary shapes with only 2 parameters.
Predicts natural formation of planetary rings.
Accurately describes velocity fields near planetary surfaces.
Abstract
Variational techniques have been used in applications of hydrodynamics in special cases but an action that is general enough to deal with both potential flows and solid-body flows, such as cylindrical Couette flow and rotating planets, has been proposed only recently. This paper is one of a series that aims to test and develop the new Action Principle. We study a model of rotating planets, a compressible fluid in a stationary state of motion, under the influence of a fixed or mutual gravitational field. The main problem is to account for the shape and the velocity fields, given the size of the equatorial bulges, the angular velocity at equator and the density profiles. The theory is applied to the principal objects in the solar system, from Earth and Mars to Saturn with fine details of its hexagonal flow and to Haumea with its odd shape. With only 2 parameters the model gives a fair fit…
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Taxonomy
TopicsAstro and Planetary Science · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
