Alessandra Celletti s proposed book presents classical celestial
mechanics and its interplay with dynamical systems in a way that
would be suitable for advance level undergraduate students as well
as postgraduate students and researchers. First she uses
paradigmatic models, such as the logistic map or the standard map,
to introduce the reader to the concepts of order, chaos, invariant
curves, cantori, etc. The main numerical methods to investigate a
dynamical system are presented: Poincare' maps, Lyapunov exponents,
frequency analysis, Fast Lyapunov Indicators, etc. Then she reviews
the classical two-body problem and proceeds to explore the
three-body model in order to investigate orbital resonances and
Lagrange solutions. As far as rotational dynamics are concerned,
she details the derivation of the rigid body motion, and continues
by discussing related topics, from spin-orbit resonances to
dumbbell satellite dynamics.
Perturbation theory is then explored in full detail, both in
classical, resonant and degenerate cases; practical examples of the
application of perturbation theory are presented in connection to
the precession of the perihelion or to the precession of the
equinoxes. The main ideas of KAM theory are provided, and also a
dissipative version of the theorem is discussed; furthermore
long-term stability and converse KAM results are presented. She
then explains the implementation of computer-assisted techniques,
which allow the user to obtain rigorous results in good agreement
with the astronomical expectations.
A perturbative approach to find periodic orbits is presented
together with an application to the computation of the libration in
longitude of the Moon. The study of collisions in the solar system
is approached through regularization theory."
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