Evolution of the rotational motion of a viscoelastic planet with a core on an elliptical orbit

The work is devoted to the study of the evolution of the rotational motion of a planet in the central Newtonian field of forces. The planet is modeled by a body consisting of a solid core and a viscoelastic shell rigidly attached to it. A limited formulation of the problem is considered, when the ce...

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Hlavní autoři:	A. A. Shatina, A. V. Starostina
Médium:	Artigo
Jazyk:	Russo
Vydáno:	MIREA - Russian Technological University 2021-10-01
Edice:	Российский технологический журнал
Témata:	viscoelastic body keplerian elliptic orbit andoyer variables averaging method dissipative evolution of motion
On-line přístup:	https://www.rtj-mirea.ru/jour/article/view/370
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