EdusalsaDiscover Your Stanford

MATH 138

Celestial Mechanics

  • Not Offered

3 units

Letter or Credit/No Credit

Mathematically rigorous introduction to the classical N-body problem: the motion of N particles evolving according to Newton's law. Topics include: the Kepler problem and its symmetries; other central force problems; conservation theorems; variational methods; Hamilton-Jacobi theory; the role of equilibrium points and stability; and symplectic methods. Prerequisites: 53, and 115 or 171.

Fulfills

  • GER:DB-Math

Course Prequisites

Sign Up

To save MATH 138 to your course bucketlist

Already Have An Account? Log In