Astronomy 102 - Summer
2008
Introductory Astronomy:
Stars, Galaxies, and the Universe
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Instructor |
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Dr. Jimmy Irwin |
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Office |
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905 Dennison |
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Phone |
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936-7904 |
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Office Hours |
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10:00 AM – 11:00 AM Tuesday, Thursday, or by appointment |
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Web page |
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http://www.astro.lsa.umich.edu/~jairwin/ASTR02/ASTR102.html |
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Time and Room |
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Lecture: MTWRF 11:00 AM - 12:00 PM in 807 Dennison Discussion: T or W 1:00 PM - 3:00 PM in Angell Hall 5179 |
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Textbook |
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The Cosmic Perspective: Stars, Galaxies, & Cosmology, by Bennett, Donahue, Schneider, and Voit (5th Edition) |
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GSI
Eva-Marie Proszkow
Office: 3241 Randall Lab
Email: emdavid@umich.edu
Office
Hours: Wednesdays 10:00 AM -11:00 AM, in Den. 1053
Discussion
Sections: Angell Hall 5179, T/W 1:00 PM – 3:00 PM
Description
This course provides an overview of astronomy outside the solar system. Lectures topics include
· an inventory of the different types of stars
· the relationships between red giants, white dwarfs, black holes, and supernovae
· our Milky Way galaxy
· less hospitable exploding galaxies
· enigmatic quasars
· the present state of knowledge or speculation regarding the origin and ultimate fate of our universe
It all came from somewhere, but where... and why?
This course is intended primarily for non-science concentrators, who wish to understand the phenomena and properties of the universe beyond our solar system.
Guidelines
This course is an introduction to a large part of modern astronomy: stars – their temperatures and evolution; galaxies; cosmology. The course is not highly mathematical, although values for lengths, masses, luminosities, etc., will be widely used, and simple equations will be introduced from time to time. A command of high school mathematics (algebra, geometry, and the application of logarithms) is necessary for this course.
No extra credit will be offered in this course, with the possible exception of extra credit problems on a quiz or exam. Due to the rapid nature of a 7-week course, it is imperative to keep up with the reading and attend the lectures and the discussion sessions. While there will be no formal homework assignments, problem sets (particularly those involving mathematical concepts) will be suggested for you to work on, and these problems will be discussed in your discussion session. As these types of problems will appear on quizzes and tests, failure to learn these concepts will have a negative impact on your grade.
The timetable for the quizzes and exams are not negotiable, and it will not be possible to make them up, except in the case of a doctor-certified illness.
If you ever have questions about any of the material covered in
lecture, please don't hesitate to talk to me. This course is very
short and moves very quickly, so it is vital to keep up with the
material.
Grading
Your final course grade will be
determined based on the following point structure:
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Midterm |
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20% |
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Quizzes |
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12% |
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2 quizzes, 6% each |
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Final Exam |
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30% |
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Discussion |
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30% |
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You will complete 5 labs during the discussion session, each worth 6% of your final grade |
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Project |
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8% |
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Options for the project may be found on the course web page, and help in choosing one will be given in the discussion session. |
Timetable
Time spent on a given subject is indicative only; as the term advances, you may find we are a little ahead or behind this plan.
Date Topic Chapter Suggested Problems
W 25 - Introduction/Overview CH 1 1.44, 1.52
(read CH 2 (Celestial Sphere) Before First Discussion Session)
R 26 - Length Scales, Time Scales, Our Location in the Universe 2.51, 2.55
F 27 - History of the Heliocentric Theory and Kepler's Laws CH 3 3.49, 3.54
M 30 - Distinguishing Science From Pseudoscience
T 1 - Newton's Laws and Gravity CH 4 4.56, 4.57, 4.58, 4.60
W 2 - Gravity (cont.)
R 3 - Light and Matter CH 5 5.49, 5.52, 5.54, 5.570, 5.60
F 4 - 4th of July - no class
M 7 - Light and Matter (cont.)
T 8 - Telescopes CH 6 6.45, 6.46, 6.48, 6.49
W 9 - Telescopes (cont.)
R 10 - Our Sun: Energy Source and Structure - Quiz 1 CH 14 14.53, 14.54
F 11 - Our Sun: Fusion and Sunspots/Solar Activity
M 14 - Stars: Properties and the Magnitude System/Parallax CH 15 15.40(e thru l), 15.48, 15.49
T 15 - Stars: The HR-Diagram
W 16 - Binary Stars/Masses of Stars/Star Clusters
R 17 - Star Birth CH 16 16.47, 16.50
F 18 - Star Birth (cont.)
M 21 - Life of Low-Mass Stars: Planetary Nebula CH 17 17.50, 17.54, 17.55, 17.56
T 22 - Life of High-Mass Stars: Supernova
W 23 - Supernova Remnants/Review for Midterm
R 24 - Midterm
F 25 - Stellar Remnants - White Dwarfs and Neutron Stars CH 18 18.47, 18.50, 18.51
M 28 - Stellar Remnants - Black Holes
T 29 - Finish Black Holes and Review Stellar Evolution
W 30 - Our Galaxy - The Milky Way CH 19
R 31 - Our Galaxy - The Milky Way (cont.)
F 1 - Galaxies: Types and Distances CH 20
M 4 - Galaxies: Types and Distances (cont.) - Quiz 2
T 5 - Galaxy Evolution and Active Galactic Nuclei CH 21
W 6 - Clusters of Galaxies and Dark Matter
R 7 - The Big Bang: Observational Evidence and Implications CH 22+23
F 8 - The Big Bang: The Role of Dark Matter and Dark Energy
M 11 - The Big Bang: Inflation and the Age and Fate of The Universe
T 12 - Finish Big Bang; Review for Final
R 14 - FINAL EXAM 4:00 PM - 6:00 PM 807 Dennison