Physics 427 INTRODUCTION TO aSTROPHYSICS Course Outline
V. SEMESTER SCHEDULE
Class meets at 12:00-12:50 pm in C261 ESC
|
WK# |
DATE |
TOPIC |
Figures, Tables, Images |
SUPPL RDG (pp.) | HW ASSGN DUE* | |||||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | W Sep 3 |
Nomenclature, Data Sources, Catalogs, Astronomical Literature, Simbad |
0-7 |
- |
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| F Sep 5 |
Simbad, Astronomical Literature, Coordinate Systems |
8-12 |
3-21 |
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| 2 | M Sep 8 |
Spherical Trigonometry |
13 | |||||||
| W Sep 10 |
No Class |
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| F Sep 12 | Stellar Positions |
Time Systems and Seasons |
14-23 | |||||||
| 3 | M Sep 15 |
Coordinate Precession:
Exact Method and |
24-29 |
15-16 |
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| W Sep 17 | ||||||||||
| F Sep 19 | ||||||||||
| 4 | M Sep 22 |
Chandler Wobble, Refraction |
30-35 | |||||||
| W Sep 24 |
Stellar Aberration |
36 | ||||||||
| F Sep 26 |
Trigonometric Parallaxes, Parallactic and Proper Motion |
37-43 |
63-65 |
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| 5 | M Sep 29 | Stellar Motions: Radial, Transverse & Space Velocities, Moving-Cluster π |
39-44 |
18-21, 126-130, 960-964 |
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| W Oct 1 | Statistical Parallaxes, Luminosities: Apparent & Absolute Magnitudes |
45-51 |
65-69 |
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| F Oct 3 | Magnitudes, Flux Densities, Luminosities, Color Indices |
52-53 |
82-87 |
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| 6 | M Oct 6 | Effects of Interstellar Absorption: Extinction and Reddening |
54-55 |
265-268, 437-442 |
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| W Oct 8 | Stellar Spectral Classification |
56-65 |
223-240 |
|
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| F Oct 10 | The H-R Diagram, Measures of Stellar Temperature |
66-75 |
223-250 |
|||||||
| 7 | M Oct 13 |
|
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| W Oct 15 |
The Stellar Luminosity Function |
76-81 |
1044-1046 |
|||||||
| F Oct 17 | ||||||||||
| 8 | M Oct 20 |
|
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| W Oct 22 |
Telescopes |
Primary Functions, Light-Gathering Power |
82-84 |
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| Θ Oct 23 |
M I D T E R M E X A M I N A T I O N ( in Testing Center) |
Midterm |
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| F Oct 24 |
Telescopes |
Image and Apparent Surface Brightness, Plate Scale | 159-197 | |||||||
| 9 | M Oct 27 |
Angular Resolution, Seeing |
85-86 |
|||||||
| W Oct 29 |
Magnification, Refractors, Aberrations |
87-91 |
||||||||
| F Oct 31 | Reflector Designs, Aberrations, Observatory Sites |
92-108 |
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| 10 | M Nov 3 | Schmidt Telescopes, Radio Telescopes |
109-117 |
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| W Nov 5 | Spectrographs | Basic Designs, Performance Characteristics |
118-121 |
129 |
|
|||||
| F Nov 7 | Speed |
122-124 |
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| 11 | M Nov 10 | Diffraction Gratings |
125-128 |
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| W Nov 12 | ||||||||||
| F Nov 14 | ||||||||||
| 12 | M Nov 17 |
Detectors |
The Eye, Photographic Emulsions |
129-135 |
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| W Nov 19 | Photon-Counting Statistics |
136-138 |
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| F Nov 21 | CCDs |
139 |
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| 13 | M Nov 24 |
Basic Equations of |
Introduction, Black-body Radiation |
140 |
223-240 |
|
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| T Nov 25 | The Boltzmann Equation |
141-142 |
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| W Nov 26 - F Nov 28 |
T H A N K S G I V I N G H O L I D A Y |
|
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| 14 | M Dec 1 |
Basic
Equations of Astrophysics |
The Boltzmann Equation |
141-142 |
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| W Dec 3 | The Maxwellian Kinematic Distributions | 143-145 | 13 | |||||||
| F Dec 5 |
The Saha Equation Applications of the Boltzmann & Saha Equations |
146 | ||||||||
| 15 | M Dec 8 | |||||||||
| W Dec 10 | Calculations of Pe(Pg,T ) | 147-148 | 14 | |||||||
| F Dec 12 - S Dec 13 |
E X A M P R E P A R A T I O N D A Y S |
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| 16 | W Dec 17 | F I N A L E X A M I N A T I O N (2:30 pm - 5:30 pm) | Final | |||||||
*Additional problem assignments may be added to this schedule as the semester progresses.