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Use Figure 20.3 to estimate the radius of a 0.9 solar mass white dwarf star. |
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| 2 | |
A white dwarf star has a radius two-thirds as large as the Earth's. Use Figure 20.3 to find the mass of the star. |
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| 3 | |
Use Figure 20.5 to find the mass of the white dwarf star that results from the evolution of a 6 solar mass main sequence star. |
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Use Figure 20.9 to find the brightness (relative to its maximum brightness) of a type II supernova 100 days after the time of maximum light. |
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| 5 | |
Use Figure 20.17 to estimate the radius of a 0.5 solar mass neutron star. |
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