Taking both a theoretical and observational perspective, this
book is an introduction to recent developments in the field of
celestial mechanics. It emphasizes the application to extended
celestial bodies and devotes much attention to rotational aspects.
In particular, it explains the state of art for accurate modelling
of the rotation of celestial bodies such as the Earth, the Moon,
and Mercury, which involves principles related to hydrodynamics and
geodesy. Comparisons between the light curves of the asteroids and
their rotational state are made and spatial techniques leading to
the determination of the Earth's gravitational field are explained.
Also, the book provides a general overview of the collisional
processes in the solar system and of the dynamics of the rings. It
is addressed to graduate students and researchers in space sciences
and celestial dynamics.
General
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