Lecture: | MW 1:30 -- 2:45 pm Van Allen 358 |
---|---|
Instructor: | Kenneth
G. Gayley 707 Van Allen Hall 335-3282 |
Office Hours: | 3-4:30 pm WF, or by appointment 707 Van Allen Hall |
Textbook: | (No required text) | Suggested texts (on reserve:) | online notes from Onno Pols | Kippenhahn and Weigert (1990) Stellar Structure and Evolution | Bohm-Vitense (1989) Introduction to Stellar Astrophysics II. Stellar Atmospheres |
The purpose of the course is to gain a physical understanding of stars. You can open almost any physics book to any page, and what is being described there happens at some place and time in the structure and evolution of some type of star. We cannot understand in detail how every page of physics pertains to every type of star, so our goal instead will be to understand general trends and behaviors, from as simple a perspective as possible. In so doing, we will find that stars behave in mysterious ways that at first seem surprising and even paradoxical, but ultimately can be made sense of. They also provide a stage for laboratory physics to play out on the grand scale, so not only do we learn physics so we can understand stars, but understanding stars helps us learn physics.
The course grade will come from the three (3) homework assignments, which each count 10% of the grade, the two in-class midterms, which each counts 15%, the take-home final exam (20%), one mock research presentations (10%), and one group proposals (10%). Details about the curve are: