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...

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Bibliographic Details
Main Authors: Sergey Ershkov, Dmytro Leshchenko
Format: Article
Language:English
Published: MDPI AG 2023-03-01
Series:Mathematics
Subjects:
Online Access:https://www.mdpi.com/2227-7390/11/6/1491