Fall 2010 not offered
|Course Cluster: Planetary Science|
Most of the visible matter in the galaxy is in the form of stars. It is important, therefore, to understand their structure and their evolution. Fortunately, we have a fairly well-developed and tested theory of stellar structure covering both their interiors and atmospheres. In this course, we will provide an introduction to that theory and examine its key results, including a basic description of how stars evolve.
||Gen Ed Area Dept:
|Course Format: Lecture||Grading Mode: Graded|
||Prerequisites: PHYS213 AND PHYS214 AND ASTR155 AND ASTR211
||Fulfills a Major Requirement for: (ASTR)(CIS)(PSCI-MN)(SISP)
One book. Several papers.
|Examinations and Assignments: |
Weekly or bi-weekly problem sets, 2 hour exams, 1 final exam.
|Additional Requirements and/or Comments: |
ASTR231 is for undergraduates only.
ASTR531 is for graduate students only.
|Drop/Add Enrollment Requests|
|Total Submitted Requests: 0||1st Ranked: 0||2nd Ranked: 0||3rd Ranked: 0||4th Ranked: 0||Unranked: 0|