Well Posed Origin Anywhere Consistent Systems in Celestial Mechanics
Harry Gingold, Jocelyn Quaintance

TL;DR
This paper addresses mathematical issues in celestial mechanics when the coordinate origin coincides with a point mass, proposing a translation-invariant relative system and deriving a new constant of motion.
Contribution
It introduces a translation-invariant relative system for celestial mechanics and derives a new constant of motion, resolving inadequacies in Newton's equations.
Findings
Identifies inadequacies in Newton's equations when origin coincides with a mass.
Proposes a system of relative differences free of these inadequacies.
Derives a new constant of motion indicating the 'restless' nature of the universe of relative differences.
Abstract
Certain measurements in celestial mechanics necessitate having the origin O of a Cartesian coordinate system (CCS) coincide with a point mass. For the two and three body problems we show mathematical inadequacies in Newton's celestial mechanics equations (NCME) when the origin of a coordinate system coincides with a point mass. A certain system of equations of relative differences implied by NCME is free of these inadequacies and is invariant with respect to any CCS translation. A new constant of motion is derived for the relative system. It shows that the universe of relative differences of the -body problem is ``restless''.
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Taxonomy
TopicsAstro and Planetary Science
