Lecture 27 – Binary Systems and Star Clusters
Summary / Checklist of the Main Concepts to Understand and Remember
Binary Stars | ||
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How common are binary stars? Polaris, Mizar and Sirius as examples of binary stars. (Where are those stars?) | |
• | What is a visual binary system? | |
• | What is a spectroscopic binary? How should the orbits of the stars be oriented for them to be seen as a spectroscopic binary? | |
• | What is an eclipsing binary? How should the orbits of the stars be oriented for them to be seen as an eclipsing binary? | |
• | Can a binary star be of more than one type? (Visual / Spectroscopic / Eclipsing.) | |
Star Masses | ||
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How can we find out the mass of a star? | |
• | Why are binary stars the only ones for which we can directly find the mass? (As opposed to guessing it based on the type of star.) | |
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Approximately where is the Sun, in the range of possible star masses? Are most stars more massive or less massive than the Sun? | |
Star Clusters | ||
• | Star clusters are common, in particular where young stars are found (stars are born in large interstellar clouds that break into fragments). | |
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What are open clusters? (Approximately how many stars do they contain, in what part of the galaxy are they, are they young or old?) | |
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What are globular clusters? (Approximately how many stars, in what part of the galaxy, are they young or old?) | |
• | How can we find out how old a star cluster is? Name one example of open cluster and one example of globular cluster. |
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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