Question # | Letter Answer | Comments |
---|---|---|
1 | (a) | heat energy transport |
2 | (e) | highest energy is shortest wavelength |
3 | (d) | 'nuff said |
4 | (c) | due to continuous scatterings |
5 | (e) | "peri" = closest, "helion" = Sun |
6 | (e) | as per the definition |
7 | (d) | charge not conserved |
8 | (d) | Moon is in free fall around Earth |
9 | (a) | due to high opacity |
10 | (b) | size = radius, L/Lsun = (R/Rsun)^2 (T/Tsun)^4 |
11 | (b) | p-p in low mass stars, CNO in high mass stars |
12 | (c) | trailing zeros not necessarily significant |
13 | (b) | page II-3 of the course notes |
14 | (d) | named after physicist who discovered the relation |
15 | (e) | page II-7 of the course notes |
16 | (e) | page II-3 of the course notes |
17 | (b) | Stefan-Boltzmann's & Wien's Law |
18 | (e) | page I-1 of the course notes |
19 | (a) | textbook readings |
20 | (a) | the scientific method |
21 | (c) | page I-7 of the course notes |
22 | (c) | page I-1 of the notes |
23 | (e) | page II-2 of the course notes |
24 | (c) | Galileo did that |
25 | (d) | page II-1 of the course notes |
26 | (d) | page I-13 of the course notes |
27 | (d) | a particle of light has both characteristics |
28 | (c) | from the definition of temperature |
29 | (c) | page I-8 of the course notes |
30 | (b) | textbook readings |
31 | (b) | page I-2 of the course notes |
32 | (a) | page I-10 of the course notes |