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10-1 Measuring the distances to nearby stars utilizes an effect called parallax
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10-2 A starâs brightness can be described in terms of luminosity or magnitude
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10-3 A starâs distance can be determined by comparing its luminosity and brightness
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10-4 A starâs color depends on its surface temperature
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10-5 The spectra of stars reveal their chemical compositions as well as surface temperatures and sizes
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10-6 Stars come in a wide variety of sizes and masses
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10-7 Hertzsprung-Russell (H-R) diagrams reveal the different kinds of stars
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