| These questions are about the Hertzsprung–Russell (HR) diagram, and the measurements needed to create it. | |||||||||||||||||
| Q1-2. To find distances to nearby stars, the method of stellar parallax is used, measuring the shift in position as shown in the diagram below: 
 The distance to the star (in parsecs) is given by: $ \text{d (parsecs)} = {1 \over{\text{parallax angle p (seconds of arc)}}} $ | |||||||||||||||||
| 1. Which angle A to D in the diagram above is the required parallax angle p? | |||||||||||||||||
| 2. The star is being observed from 2 positions, shown as X and Y in the diagram. These points are... 
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| 3. Once the distance to a star is known, the luminosity can be calculated by measuring the... 
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| 4. A star of radius R has a luminosity L and surface temperature T. Another star has half the surface temperature but a luminosity of ¼L. This means the radius of the second star is: 
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| 5+6: The diagram below shows the Hertzsprung-Russell diagram, with three regions of stars indicated: 
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| 5. What type of stars are in region 1? A). red giants | |||||||||||||||||
| 6. What type of stars are in region 2 and 3? 
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| 7 Which of these HR diagrams shows the correct location of supergiants? 
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| 8. Which of these diagrams correctly shows lines of equal radius? 
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| 9. Which of these diagrams shows the approximate location of the 'instability strip' - with unstable variable stars? 
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| 10. The HR diagram here shows two stars, X and Y. From information given in the diagram, which statement below is correct? |  | ||||||||||||||||
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