Course Identification

The course will consist of a general overview of some main fields in astrophysics, with particular emphasis on the application of physics to astronomical systems.

The main subjects covered will include:

1. Stellar structure and evolution
2. Planetary systems
3. Galaxy structure and dynamics
4. Cosmology

For example, the study of stellar structure and evolution is used as a virtual laboratory for learning about equations of state of classical and quantum gas, about heat transfer, about hydrostatic equilibrium, nuclear reactions, etc. Black Holes are used to touch on general relativity. Galaxy structure and dynamics is used to learn about gravity (classical and a touch of relativity), gravitational light bending, virial relations, etc. Astrophysical measurements of velocities is used to demonstrate the (relativistic) Doppler effect, and a little special relativity.

Upon successful completion of the course students will be able to:

1. Master the the basics of stellar structure and evolution, galaxy structure and dynamics, astrophysical measurements of velocities, and understand some of the main methods that are used in astrophysical research.
2. Describe the application of physics to astronomical systems
3. Infer from astrophysical systems to various physical processes.