ASTR 498N      Stellar Structure and Evolution     Spring 2002

 

Class meetings:          Tuesday and Thursday, 9:30–10:45 in CSS 0201

 

Required Text:           D. A. Ostlie and B. W. Carroll, An Introduction to Modern Stellar Astrophysics (Addison-Wesley 1996). 

                              [An Introduction to Modern Astrophysics, by the same authors, is a superset of the above text.]

 

Instructor:               Doug Rabin, Goddard Space Flight Center

                              Douglas.Rabin@gsfc.nasa.gov 

                              301-286-5682

                              Office hours after class, CSS 1247

 

Outline

 

Dates

Topic

Text

 

 

 

Jan

 

 

29

31

Preliminaries.  Why?  Review.

Ch 3, 5, 8

Feb

 

 

5

7

Tour of the stellar menagerie.

8

12

14

Hydrostatic and thermal equilibrium.  Equation of state.

10.1, 10.2

19

21

Stellar energy sources.

10.3

26

28

Energy transport. 

10.4

Mar

 

 

5

7

Equations of equilibrium stellar structure. 

10.5

12

14

Simplified stellar models.

 

19

21

Building and calculating models (Dr. A. Sweigart).

10.5

 

 

Spring break

 

Apr

 

 

2

4

Overview of stellar life cycles.

 

9

11

Main sequence stars.

10.6

16

18

The Sun.  Asteroseismology.

11

23

25

Pre-main sequence evolution (Dr. C. Grady).

12

30

 

Post-main sequence evolution.

13

May

 

 

 

2

Post-main sequence evolution.

 

7

9

Endpoints of stellar evolution.

13, 15

14

 

Close binary systems.

17

21

 

Final   1:30 pm in class

 

 

 

 

 

Grading

 

Homework              30%

Midterm                  20%

Individual project          20%

Final                       30%

 

Normally I’ll assign homework on Thursdays, collect it the next Thursday, and return it to you the following Tuesday.  I’ll use a four-point scale for grading problems:  one point for demonstrating an understanding of the physical ingredients, one point for using the correct equations, two points for the correct solution.   Homework more than four days late (without prior approval) will be graded in the same way but for a maximum of half credit.  We can discuss the individual project, probably a 4–5 page paper (Word or LaTeX); the aim will be to get you into the research literature in a limited area.  The final will cover material from the full semester.

 

Letter Grades:          80–100% A, 65–80% B, 50–65% C.