The Three-Body Problem and the Equations of Dynamics

Henri Poincare

Springer International Publishing AG, 2017

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In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations of planetary motion and studied these differential equations in the limited case of three bodies to arrive at properties of the equations’ solutions, such as orbital resonances and horseshoe orbits.

ISBN-13
9783319528984
ISBN-10
331952898X
Publisher
Springer International Publishing AG
Year
2017
Publication date
2017-05-22
Pages
248
Dimensions
160x241x22
Weight
562