ASTR 100 (Hamilton)
FINAL EXAM (200 points)
Wednesday, May 19
Details of the Exam
The exam will be given on Wednesday May 19 in PHYS 1412 from 8:00am -
10:00am. I will ask you to wait outside in the hall until the TAs and
I have the exams laid out on the seats in the classroom. Please be
patient; the exam should take less than 2 hours to complete, so you
should have plenty of time. Bring a #2 pencil to the exam - notes,
books, and calculators are not allowed!
There will be 50 multiple choice question worth 2 points each. For
each one, choose the best answer from the available choices. In
addition, there will be a short answer section with eight to ten
questions worth a total of 100 points. A few of these may involve
interpreting mathematical equations, however, any equations that you
need will be given to you so you don't need to memorize them. Written
responses to short answer questions will be graded on completeness. It
is always a good idea to go back and re-read the questions after you
have finished to make sure that you have answered them as completely as
possible!
The exam is cumulative and will cover all lecture material and
chapters 1-17 in the book. The material since the second midterm will
be more heavily weighted. If you have been keeping up in the class by
attending lecture and section, reading and studying the book,
reviewing your notes, doing your homework, and going over your
corrected homeworks and exams, you should be in good shape to take the
final. It is a good idea to review this material again during the week
before the final so that it will be fresh in your mind. Don't just
cram the night before the exam!
Review Session
There will be a review session in PHYS 1412 on Tuesday, May 18 from
6:00pm-7:30pm held by the ASTR100 TAs. Please bring lots of questions
to the review session; this is your chance get last minute help from
experts!
Extended Office Hours
Dr. Hamilton will hold extra office hours Monday and Tuesday from noon
to 5:00pm. Drop by with questions!
Some Important Topics We've Studied
- The Cause of the Seasons
- Motions of the Stars, Sun, Moon, and Planets in the Sky
- Scientific Method
- Contributions of the Ancient Greeks to Astronomy
- Contributions of the Renaissance Europeans to Astronomy
- Phases of the Moon
- Lunar and Solar Eclipses
- Geocentric and Heliocentric Theories
- Kepler's Laws
- Newton's Laws
- Law of Gravity
- The Electromagnetic Spectrum
- Atoms and the Formation of Spectra
- Doppler Shift
- Physical Properties of the Earth
- Interior and Atmosphere of the Earth
- Telescopes
- Physical Properties of the Moon
- Components of the Solar System
- Origin of the Solar System
- Mercury
- Atmospheres of Venus and Mars
- Surfaces of Venus and Mars
- Formation of Moons in the Solar System
- Atmosphere of Jupiter
- Interior of Jupiter and Saturn
- Satellites of Jupiter
- Satellites of Saturn
- Ring Systems
- Comet Shoemaker-Levy 9
- Uranus and Neptune
- Pluto and Charon
- Asteroids
- Meteorites
- The Interior of the Sun
- Energy Production in the Sun
- Stellar Flux & Luminosity
- The Hertzsprung-Russel (HR) diagram
- The Life of the Sun
- The Life of Massive Stars
- White Dwarfs, Neutron Stars, Black Holes
- The Milky Way Galaxy
- Spiral, Irregular, and Elliptical Galaxies
- Active Galaxies: Radio Galaxies, Seyferts, Quasars
- Large Scale Structure of the Universe
- Fate of our Universe
- Birth of our Universe
Click "Reload" to get the most up to date version of this page.
Back
to ASTR100 Home Page
Last modified: Thu May 6 19:03:33 1999