The effects of tidal evolution on the motion of planets and satellites
are examined, treating planets as elastic solid bodies in which energ
y dissipation occurs through deformations. The elastic medium is assum
ed to obey linear viscosity-elasticity theory. The investigation metho
d combines modal analysis and small-parameter methods. The tidal evolu
tion for the rotational motions of a viscous, elastic, axisymmetric pl
anet is analyzed in detail. The spatial evolution of a deformable plan
et-satellite system in the field of a gravitating center is examined.
This article is dedicated to the memory of Evgenii Petrovich Aksenov.