Home
Schedule
Classes
Professional
Previous Page |
Fall
Quarter, 2012
- Welcome to the Web page for PHY 424 - Astrophysics.
- Course Description
Physics 424, Astrophysics is a general survey of modern astrophysics. The course starts with the fundamental physical concepts underlying much of astrophysics, including gravitation and orbital mechanics, and radiative processes (including blackbody radiation, line emission and rudiments of radiative transfer). We then move on to discuss the stellar structure, evolution and death, the physics of compact stars, the interstellar medium and star-formation, and the structure and evolution of the galaxies, galaxy clusters and the universe. (4 credits).
- CURRENT ANNOUNCEMENTS
- I will communicate with you frequently via your Cal Poly e-mail address, so read your e-mail regularly (at least once per day!)
|
- Powerpoint slides (added after class)
- Reading Assignments
All reading should be done before the date indicated (i.e., before the class in which we will discuss the topic). You will almost certainly want to reread the chapter when you go to work on the related homework assignment. This is difficult technical material, and you will need to read it more than once to fully understand it. Reading the same material multiple times is the norm in Physics and Astronomy!
Assn.# Due Date Reading Assignment
| 1 |
M, 9/24 |
Chapter 1.1, 1.2, 1.4, The Celestial Sphere
Chapter 2.1-2.3, Celestial Mechanics |
2 |
W, 9/26 |
Chapter 3, The Continuous Spectrum of Light |
3 |
F, 9/28 |
Chapter 5, The Interaction of Light and Matter |
4 |
W, 10/3 |
Chapter 7, Binary Systems and Stellar Parameters |
5 |
M, 10/8 |
Chapter 8, The Classification of Stellar Spectra |
6 |
M, 10/15 |
Chapter 10.1-10.3, 10.4 (p. 315), 10.5 (pp. 329-334), 10.6, The Interiors of Stars |
7 |
M, 10/22 |
Chapter 12, The Interstellar Medium and Star Formation |
8 |
W, 10/31 |
Chapter 13, Main Sequence and Post-Main-Sequence Stellar Evolution
Chapter 15.1-15.3, The Fate of Massive Stars |
9 |
F, 11/2 |
Chapter 16, The Degenerate Remnants of Stars |
10 |
M, 11/5 |
Chapter 17, General Relativity and Black Holes |
11 |
W, 11/7 |
Chapter 24.1-24.2, The Milky Way Galaxy |
12 |
F, 11/9 |
Chapter 24.3, The Milky Way Galaxy |
13 |
W, 11/14 |
Chapter 25.1, The Nature of Galaxies
Chapter 26.1, Galactic Evolution |
14 |
F, 11/16 |
Chapter 27.1 (pp. 1038-1042, 1051), 27.2, The Structure of the Universe |
15 |
M, 11/19 |
Chapter 29.1, Cosmology |
16 |
M, 11/26 |
Chapter 29.3, Cosmology |
| 17 |
W, 11/28 |
Chapter 29.2, Cosmology |
| 18 |
F, 11/30 |
Chapter 30.1, The Early Universe |
All of the problems come from the textbook, except those with names, which will be handed out in class. Assignments will be due at the beginning of the class period on the due date. I may not collect the homework until the end of class, in case there are questions about the problems. Unless you speak to me ahead of the due date, late homework depreciates in point value (not necessarily in pedagogic value) at the rate of 20% per day. You should begin homework several days in advance of the due date.
Assn.# Due Date Homework Problems
| 1 |
M, 10/1 |
2.6, 2.7, 2.8, 2.14 |
2 |
M, 10/8 |
3.3, 3.4, 3.12, 3.14 |
3 |
M, 10/15 |
5.8, 5.11, 5.16, 7.4, 7.6, 7.10 |
4 |
M, 10/22 |
8.4, 8.6, 8.10, 8.13 |
5 |
M, 10/29 |
10.3, 10.4, 10.12 + What is the total energy released in the PPI chain?, 10.21 |
6 |
M, 11/5 |
12.1, 12.2, Stromgen Sphere, HII Region Emission, Molecular Hydrogen Formation |
7 |
W, 11/14 |
13.5, 13.8, 15.11, 15.12, 15.13 |
8 |
M, 11/19 |
16.1, 16.19, 17.5, 17.21 |
9 |
M, 11/26 |
24.1, 24.18, 24.22, 26.1 |
10 |
M, 12/3 |
27.2, 29.3, 29.4, 29.17, 29.30 |
- Homework solutions (added after HW is due)
|