Astrophysical Dynamics

Lecture, three hours. Orbital dynamics: two-body problem, three-body problem, resonances, tides, migration. Galactic potentials. Milky Way structure and observed properties of galaxies. Collisionless Boltzmann equation and relaxation processes. Stability of stellar systems. Spiral structure. Letter grading.

Review Summary

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Enrollment Progress

Jul 13, 4 PM PDT
LEC 1: 0/0 seats taken (Canceled)
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Section List

  • LEC 1

    Canceled

    TR 10am-11:50am

    Physics and Astronomy Building

    Review

Course

Instructor
No instructors
Previously taught
24F

Previous Grades

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