Classical Physics

    

On the Effect of the Central Body Small Deformation on Its Satellite Trajectory in the Problem of the Two-body Gravitational Interaction

Authors: Dmitry G. Kiryan, George V. Kiryan

The problem of the two-body gravitational interaction has been solved numerically based on the classical mechanics principles. One of the bodies is a deformable three-axis ellipsoid (central body) and the other is a material point (satellite). The relationship of the angular discrepancy between the calculated and actual positions of the satellite pericenter with central body’s gravity anomaly has been established.

Comments: 14 Pages. 6 Figures, 1 Table

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Submission history

[v1] 2020-07-26 11:47:49 (removed)
[v2] 2020-08-05 18:52:38

Unique-IP document downloads: 157 times

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