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About the application of angle–action variables to the rotation of deformable celestial bodies

Published online by Cambridge University Press:  25 May 2016

Yuri V. Barkin ,
Jose M. Ferrandiz  and
Juan Getino
Yuri V. Barkin
Affiliation:
Depto. Matemática Aplicada Universidad de Alicante, 03080 Alicante. Spain
Jose M. Ferrandiz
Affiliation:
Depto. Matemática Aplicada Universidad de Alicante, 03080 Alicante. Spain
Juan Getino
Affiliation:
Grupo de Mecánica Celeste Facultad de Ciencias, 47005 Valladolid. Spain e-mail: getino@hp9000.uva.es

Abstract

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We begin with the development of a new analytical theory for the rotational motion of deformable celestial bodies. In this work we present a new unperturbed Hamiltonian which includes the main term affecting the Chandler period.

Type
Part VI - Earth and Deformable Celestial Bodies
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 243 - 244
Copyright
Copyright © Kluwer 1996 

References

Getino, J. and Ferrándiz, J.M.: 1991, Celes. Mech., 51, 35–65.Google Scholar
Getino, J. and Ferrándiz, J.M.: 1995, Celes. Mech., 61, 117–180.Google Scholar