Inelastic Collision Influencing the Rotational Dynamics of a Non-Rigid Asteroid (of Rubble Pile Type)
We have considered here a novel particular model for dynamics of a <i>non-rigid</i> asteroid rotation, assuming the added mass model instead of the concept of <i>Viscoelastic Oblate Rotators</i> to describe the physically reasonable response of a ‘rubble pile’ volumetric mate...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2023-03-01
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Series: | Mathematics |
Subjects: | |
Online Access: | https://www.mdpi.com/2227-7390/11/6/1491 |