What you DO need to know:
- What goes on in the core of a sun-like star when on the MS, sub-giant branch, red giant branch, horizontal branch, 2nd red giant branch, and when becomes a white dwarf.
- This includes what element is present and if fusion is going on or if the core is inert
- Given a sun-like star and a very massive star, pick out what its life-path (evolutionary track) will be and how it will end up.
- For variable stars, the general process that makes these stars pulsate and how the outward pressure and inward pull of gravity are involved.
- Answers to all of the learning objectives for lectures
- Material in the tutorials and exercises
- You should review the review questions emphasized in the text
(see http://www.astro.washington.edu/larson/Astro101/comins_eoc_questions.html)
- Previous exams have included tables of magnitudes, parallaxes, and B-V values. Expect similar things this exam.
What NOT to worry about for Exam 2, Astronomy 101, Autumn 2008 that's in the textbook:
Ch. 11
Binary stars providing information about stellar masses
Kepler's Third Law
Orbital motion of binary stars
(Doppler effect of light)
Ch. 12
Exoplanets and brown dwarfs
Estimating distances using variable stars
Mass transfer in close binary stars
Ch. 13
White dwarfs in close binary systems
Type Ia supernovae
Details about supernova 1987A
Binary neutron stars
X-ray bursts
More exotic end products of stars, like magnetars and quarks stars
Ch. 14
Special relativity
Different types of black holes
Supermassive black holes (comes later)
Binary systems of black holes and neutron stars
Gamma-ray bursts
Evaporation of black holes
In general:
We will have nothing about galaxies, nor anything about distance measurements using variable stars.
From a class member on Monday: "What is the answer to the question of life, the universe, and everything?" 42