Exploring how Jupiter shapes Mars: a rigorous look at secular perturbations in celestial motion.
This scholarly study explains how the gravitational influence of Jupiter affects Mars, using classical methods from celestial mechanics. It presents foundational formalisms—Lagrange’s generalized equations, Hamilton’s canonical forms, and Jacobi’s method—and shows how they transform complex multi-body motion into solvable equations. The text includes practical computations and an application to the Jupiter–Mars system, illustrating how perturbations are analyzed and quantified.
Perfect for readers with an interest in the history and methods of celestial mechanics, this edition clarifies the steps researchers use to reduce, transform, and solve the equations governing orbital motion. It blends theory with a concrete, worked example to demonstrate how perturbations are modeled and calculated.
- Foundational methods for analyzing perturbations in multi-body systems
- Derivation and interpretation of canonical forms and Jacobi’s equation
- Worked computations applying Hill’s method to Jupiter and Mars
- A historical view of how these techniques evolved to study orbital dynamics
Ideal for students and readers of astronomy, physics, and the history of science who seek a clear, methodical treatment of orbital perturbations.