Lecture 24 – General Properties of Stars, Part 1/3
Summary / Checklist of the Main Concepts to Understand and Remember
| General Idea | ||
| • | In what main ways does our understanding of the stars' location and nature differ from that in antiquity and up to the 1600s? | |
| • | When is an astronomical object called a star? How do we know that the Sun is a star like the others? | |
| Distance and Motion | ||
| How do we find the distances to the nearest stars (other than the Sun)? Out to what distances does it work? | ||
| What is a parsec? Which star is closest to us (other than the Sun), and how far is it, in pc and in ly? | ||
| • | What types of stars are most common in our neighborhood? | |
| • | What does one have to do to observe the sideways motion of stars? | |
| • | What does one have to do to observe the stars' radial motion (towards or away from us)? | |
| Brightness | ||
| What is the apparent magnitude of a star, and what are its values for naked-eye stars? What is the absolute magnitude of a star? | ||
| • | What information do we get about a star if we compare its apparent and absolute magnitudes? | |
| Which star is the brightest, as seen from Earth? | ||
Topics from the lecture page and textbook not listed above [or between square brackets]
were not covered in class;
Underlined words indicate that I will expect students to remember a number or a name related to that topic.
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