ASTRONOMY 4
Fall, 2000 Midterm #1
Study Topics
H-R Diagrams
know what the axis are
luminosity or energy output and temperature or spectral type
what type of stars are where
protostar, main sequence, red giant, white dwarfs, neutron stars, black holes
evolution of a solar mass star on the diagram
evolution of a large mass star on the diagram
stellar classification
OBAFGKM, & I-V
Fundamental Particles and Forces
Particles: know their mass, charge, where it is found
|
Particle |
Charge |
Mass |
|---|---|---|
|
Electron |
-1 |
Light (0.5 MeV/c2) |
|
Proton |
1 |
Heavy (936 MeV/c2) |
|
Neutron |
none |
Heavy (938MeV/c2) |
|
Neutrino |
none |
Very Light (?) |
|
Photons |
none |
No Mass |
Forces: know what force is responsible for stellar processes
|
Force |
Strength |
Mediate |
Range |
|---|---|---|---|
|
Strong |
4 |
Fusion |
Within nucleus |
|
E&M |
3 |
Radiation |
infinite |
|
Weak |
2 |
Radioactive Decay |
Within nucleus |
|
Gravity |
1 |
Collapse |
infinite |
Pressure
know what pressure is, and what affects pressure
motion of atoms and molecules; density, temperature
know what quantum pressure is
know the Pauli Exclusion Principle
two particles of same state cannot be at the same place
how do you get quantum pressure
which particles can have quantum pressure
electrons and neutrons
know how pressure affects a star
holds up a star (like it's skeleton)
Stellar Structure
know the internal structure of each type of star listed above
e.g. MS stars fuse H, may have a small core, large H envelope
know especially well the Red Giant
the mirror effect
onion shell structure
steps of successive nuclear fusion
(H --> He --> C,O,N -->Fe)
Feedback mechanism and the stability of stars
negative and positive feedback
Special Relativity
know the caveats of special relativity
speed of light is constant
all observers equal
know what an inertial frame is
know the results of special relativity
time dilation (moving clocks run slower)
length contraction (moving yardsticks are shorter)
Neutron Stars and Black Holes
know how a white dwarf turns into a Neutron star
know why there is a limit to White Dwarf mass
know what an event horizon is
Binary Stars
know the characteristics defining a binary star
primary mass, secondary mass, orbital separation/period
know what a Roche Lobe is
know how mass transfer between binary stars occur
know what tidal forces are
Answers to the study questions:
week #1
|
1 |
c |
|
2 |
d |
|
3 |
a |
|
4 |
b |
week #2
|
1 |
c |
|
2 |
d |
|
3 |
a |
|
4 |
a |