Use these questions to test your understanding. If you get them wrong, you will be linked back to the relevant part of the notes.
Be sure you study them thoroughly (don't just get a quick fix for your mistake) so your overall understanding is improved.
1. The current status of a star is determined by its
a. age, mass, initial composition b. temperature, distance, color
c. spectral type, composition, temperature d. distance, magnitude, color
2. A star will become a red giant when
a. it begins to convert H to He b. when its composition changes
c. when it can no longer convert H to He in its core d. when it gains mass
3. A star may be a variable star because
a. it alternately expands and contracts b. planets fall into it and block the light
c. it makes more or less dust d. its mass changes
4. The oldest stars are most likely to be
a. the brightest stars b. the most massive stars c. the hottest stars
d. the least massive stars e. the stars with largest percentage of hydrogen
5. The lower limit on the size of a star is set by
a. the size of cloud fragment that can form b. the gravitational field of a cloud
c. the amount of H that can coalesce d. the mass require to get the core hot enough for conversion of H to He
6. Two stars both have spectral type A. One has a luminosity that is 1000 times larger than the other. What parameter differs the most between these two stars?
a. temperature b. color c. radius d. composition e. distance
7. The upper limit on the size of a star is set by
a. the size of cloud fragment that can form b. the gravitational field of a cloud
c. the stability against photon pressure d. the mass require to get the core hot enough for conversion of Si to Fe
Here are the properties of three main sequence stars: 1.)Barnard's Star T= 3370° K L=0.005 LSun ; 2.) Sun T= 5800° K L = 1 LSun
3.) Spica T=26,000° K L = 23,000 LSun
8. List these stars in order of increasing mass.
9. Under what circumstances can a star convert oxygen to silicon?
a. when it makes dust in its outer layers
b. when it reaches the main sequence
c. when it becomes a white dwarf