Global Gravity Inversion of Bodies with Arbitrary Shape
Pasquale Tricarico

TL;DR
This paper introduces a novel gravity inversion method for bodies of arbitrary shape, combining matrix inversion and Monte Carlo techniques to explore interior mass distributions constrained by shape, rotation, and gravity data.
Contribution
It develops a linear, polynomial-based approach for exact interior solutions and integrates Monte Carlo methods to handle degeneracy and assumptions, applicable to arbitrary-shaped planetary bodies.
Findings
Range of solutions converges with correct assumptions
Method effectively handles moderate noise
Applicable to arbitrary shape bodies
Abstract
Gravity inversion allows us to constrain the interior mass distribution of a planetary body using the observed shape, rotation, and gravity. Traditionally, techniques developed for gravity inversion can be divided into Monte Carlo methods, matrix inversion methods, and spectral methods. Here we employ both matrix inversion and Monte Carlo in order to explore the space of exact solutions, in a method which is particularly suited for arbitrary shape bodies. We expand the mass density function using orthogonal polynomials, and map the contribution of each term to the global gravitational field generated. This map is linear in the density terms, and can be pseudo-inverted in the under-determined regime using QR decomposition, to obtain a basis of the affine space of exact interior structure solutions. As the interior structure solutions are degenerate, assumptions have to be made in order…
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