ASTR 112: Physics of Stars
University of California, Santa Cruz
The leading observational facts about stars as interpreted by current theories of stellar structure and evolution. Spectroscopy, abundances of the elements, nucleosynthesis, stellar atmospheres, stellar populations. Final stages of evolution, including white dwarfs, neutron stars, supernovae.
Average GPA: 2.89
Grade distribution records: 195 students across 6 terms.
Grade distribution
| Grade | Students | Percent |
|---|---|---|
| A+ | 14 | 7.2% |
| A | 28 | 14.4% |
| A- | 20 | 10.3% |
| B+ | 28 | 14.4% |
| B | 27 | 13.8% |
| B- | 10 | 5.1% |
| C+ | 10 | 5.1% |
| C | 20 | 10.3% |
| C- | 2 | 1.0% |
| D | 2 | 1.0% |
| D- | 1 | 0.5% |
| F | 15 | 7.7% |
| P | 3 | 1.5% |
| NP | 6 | 3.1% |
| W | 9 | 4.6% |
Based on 195 student grade records across 6 terms and 3 professors.
Instructors
- Natalie Batalha 111 students, Average GPA 2.79
- Ryan Joseph Foley 84 students, Average GPA 3.04
- Kendall Sullivan 39 students, Average GPA 2.92