Astronomy 200 Final Study Guide
|
|
Exam Format
- Saturday, April 25, 1:00 pm
- 2 hours
- 60 multiple choice questions
- From the following topics:
|
Topic One: Stars and Motion in the Heavens
Things to know:
- terminology (asterism, magnitude, altitude, etc)
- how to read a magnitude-brightness graph
- how magnitudes work
- celestial sphere, celestial poles and celestial equator
- motion of Sun, Moon and planets in the sky
- precession
- how to find latitude and longitude from astronomical data
|
Topic Two: Lunar and Solar Eclipses
Things to know:
- condition necessary for Lunar and Solar eclipses
- kinds of eclipses
- the Saros
- how to predict eclipses using the Saros
|
Topic Three: Historical Ideas in Astronomy
Things to know:
- early ideas in Greek astronomy.
- astronomical ideas and motifs in other cultures
- Copernicus, Brahe, Kepler - their contributions
- Galileo and the "Galileo Affair" including arguments for and against Copernicanism
- how Newton changed Astronomy and our view of the universe
|
Topic Four: Gravity, Light and Matter
Things to know:
- the inverse square nature of gravity
- orbits - how they work including concepts of circular and escape velocity
- tides
- Einstein's ideas on light, matter and energy
- Einstein's idea of gravity as bending of space
- telescopes (all diff rent kinds)
- the electromagnetic spectrum and how concepts of photon, wavelength, frequency and energy are related
- how atoms emit and absorb energy
- bright line, absorption and continuous spectra
|
Topic Five : Atoms, Spectra and Stellar Classification
- the blackbody spectrum
- understand what continuous, brightline and absorption line spectra are and how to use them
- know how to use Wien's and Stefan's Laws
- know what colour-indices are and how they tell us temperature
- how spectral lines tell us about temperature, density, composition and motion
- what the Doppler Effect is and how to use the Doppler Shift formula
- the spectral classification sequence and how to identify spectral types by major features in the spectrum
|
Topic Six : The Sun
- be able to identify the major parts of the sun
- explain sunspots, flares, coronal mass ejections, spicules etc
- understand what the solar cycle is
- know what the Babcock cycle refers to
- understand why aurora happen and how they are related to the sunspot cycle
- understand how the sun generates energy via fusion of hydrogen to helium
|
Topic Seven : The Stars
- know how to use parallax
- distinguish between apparent and absolute magnitudes
- explain how star sizes can be estimated from spectral type and absolute and apparent magnitude
- explain what the HR diagram is and how it tells us about the birth and evolution of stars
- describe how stars form
|
Topic Eight : Stellar Evolution
- how stars generate energy via pp and CNO cycles
- how stars change as they age
- how a star's "age" shows up on the HR diagram
- the evolution and death of low mass stars (similar to Sol)
- the evolution and death of high mass stars
- the role of mass in determining the fate of a star
- how stellar mass determines absolute magnitude and main sequence lifetime
- neutron stars
- black holes
|
Mathematical Considerations:
You should be able to do simple brightness-magnitude , parallax, distance -modulus, and use Kepler's Third Law. Otherwise do not
worry about lot's of math - The focus of the exam is conceptual.
Formulae will be provided! |