Syllabus for Astronomy
Professor: Ken Koehler
Office: Muntz 372
Office Hours: MWF 10:30-11, MW 2:30-3, M 5:30-6 and by appt.
Telephone: 745-5782
E-mail: koehlekr@ucrwcu.rwc.uc.edu
Course Goals
This is a year-long course in Astronomy. Our goals are:
- To understand how we know what we know about the universe.
- To comprehend astronomical distances.
- To understand how the appearance of the universe is related to its 3 dimensional structure.
- To understand modern observational technologies across the electromagnetic spectrum.
- To interpret visual cues in terms of planetary structure and history.
- To use Kepler's and Newton's Laws to compute orbital and planetary characteristics.
- To use spectra to determine stellar characteristics.
- To understand absolute and apparent magnitude, and be able to assign spectral and luminosity classes to stars based on their spectra.
- To understand the life cycles of stars in terms of the nuclear processes that power them.
- To understand the end results of stellar evolution.
- To understand statistical populations of stars.
- To recognize and be able to assign galaxies to morphological classes.
- To understand the Hubble relation and its use in computing astronomical distances.
- To understand galactic rotation curves and the dark matter hypothesis.
- To understand how cosmological parameters are reflected in observations of the Cosmic Microwave Background Radiation.
This course fulfills the General Education Breadth of Knowledge (BoK) area of Natural Science.
Prerequisites
Intermediate Algebra (or its equivalent)
You must have access to a web browser with Java capability. If you do not have it, you may
obtain the Java Runtime Environment (JRE) from java.sun.com (page down to find the button on the
right side labeled "Get Java Software").
You must also have a browser that can display the Greek letters that we use in astronomy to denote some variables.
If the following letter:
l
looks like the letter "l", you may need to install a newer version of your browser, or use a different browser.
Text
One of the following texts is required reading for this course:
In addition, the following course notes will be used heavily in class and for portfolio assignments:
The notes and supporting material are available in three folders stored in
this zip file (6/27/08, 70 MB). The tidal time lapse animated slide show files,
which are very large and largely redundant, have been omitted to save space.
Electronic Communications Policy
Because of e-mail instabilities, all assignments must be turned in on paper.
Attendance Policy
Failure to attend class will result in the following:
- 0 to 10% of class meetings missed: no grade reduction
- 11 to 20% of class meetings missed: final grade is reduced by one letter grade
- 21 to 30% of class meetings missed: final grade is reduced by two letter grades
- more than 30% of class meetings missed: final grade is an F
Attendance will be taken at the start of each class period. If you are not present when it is taken, it counts as a missed class.
Schedule
Autumn
- Principles of Remote Sensing: The Photon and Radiometric Quantities
- Electromagnetic Spectrum: Distribution of Radiant Energies
Astronomy Today, Chapters 1-4
- The Hubble Space Telescope
Astronomy Today, Chapter 5
- Remote Sensing Techniques applied to Planetary bodies
- Intoduction to Planetary Bodies;
Solar System Parameters; History of Planetary Exploration; Meteorites
Astronomy Today, Chapter 6
- Earth as a Planet
Astronomy Today, Chapter 7
- Mercury and Venus
Astronomy Today, Chapters 8-9
- Mars, The Red Planet
- Stratigraphy and Physiography of Mars; The Martian Atmosphere; Ice at the Poles
- Martian Landscapes: Linear Features, Volcanoes, Impact Craters, Channels; Exotic Terrains
Astronomy Today, Chapter 10
- Overview of the Outer Planets
- Jupiter
- The Galilean Satellites
Astronomy Today, Chapter 11
- Saturn and its Moons
Astronomy Today, Chapter 12
- Uranus and Neptune, and their Satellites; the Pluto dwarfs
Astronomy Today, Chapter 13
- Asteroids and Comets / Comet Shoemaker-Levy
Astronomy Today, Chapter 14
- Models for the Origin of Planetary Systems
Astronomy Today, Chapter 15
Winter
- The Birth, Life and Death of Stars
- Spectral Analysis of Star Composition; Element Synthesis in Stars
Astronomy Today, Chapters 16-20
- Novae,
Supernovae; Neutron Stars and Pulsars; Quasars and Black Holes; Gamma Ray Bursts; and Star Collisions
Astronomy Today, Chapters 21-22
Spring
- The Nature and Evolution of Galaxies
- Continuation of Galaxies Page
- Images of Galaxies and Stars outside the Visible Light Range
- Some Special Features of Galaxies
Astronomy Today, Chapters 23-25
- Space-Time and Expansion of the Universe
- Evidence for the Big Bang:
The Redshift; Stellar/Galactic Distances; Age of the Universe; Cosmic Background Radiation; Expansion Models; Dark Matter/Energy
Astronomy Today, Chapters 26-27
- Nature and Origin of Life on Planetary Bodies
- Nature and Origin of Life on Planetary Bodies (Continued)
Astronomy Today, Chapter 28
There are 6 portfolio exercises each quarter (described in the course notes),
tentatively due in weeks 4 through 9. Your final portfolio submission will be due at the beginning of exam week.
It will include corrected versions of all six portfolio assignments, and a 1-2 page paper discussing the relationships between
the results of the exercises in the context of the material covered thus far.
All references must be from texts or .gov web sites; .edu and .org sites must be approved in advance. WIKIs are not allowed.
Grades
Each portfolio exercise will be evaluated when it is turned in, and you will be able to correct it before submitting the final
portfolio. The final portfolio will consist of the 6 corrected exercises, and the paper, and each of the seven portfolio
constituents will be evaluated on the following scale:
-
2 - correct and complete
-
1 - incomplete or contains minor errors
-
0 - incorrect, irrelevant or missing
Course grades will be assigned on the following scale:
12 to 14 points = an A
10 to 11 points = a B
8 to 9 points = a C
6 to 7 points = A D
0 to 5 points = an F
Plus or minus grades will not be given.
©2008, Kenneth R. Koehler. All Rights Reserved.