Analytical modeling of the gravitational potential of irregularly shaped celestial bodies considering three distinct internal structures: application to (21) Lutetia
Marcelo L. Mota, Safwan A., Antonio F. B. A. Prado

TL;DR
This paper develops an analytical model for the gravitational potential of irregularly shaped celestial bodies with layered internal structures, applied specifically to asteroid (21) Lutetia, improving understanding of its internal composition.
Contribution
It introduces a three-layered internal structure model using the Potential Series Expansion Method, providing a computationally efficient alternative to classical polyhedral models.
Findings
The model captures the effects of internal layering on gravitational potential.
It reduces computational time compared to traditional methods.
The approach offers a balance between accuracy and analytical simplicity.
Abstract
The classical polyhedral model is one of the most accurate methods currently used to represent the gravitational field of irregularly shaped bodies. However, it assumes a homogeneous density distribution, which may not accurately reflect the internal composition of real objects. This study aims to analyze the effects of the internal structure of asteroid (21) Lutetia on gravitational potential modeling by considering a three-layered composition with distinct densities. The gravitational approach adopted in this study is the Potential Series Expansion Method (PSEM), represents models the body as a polyhedron and decomposes it into tetrahedral elements to estimate of the total potential around the asteroid. This estimation involves summing the contributions of each tetrahedron using a direct triple integral over its volume. Although this method does not achieve the same level of accuracy…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Geomagnetism and Paleomagnetism Studies
