Exam 17: The Nature of the Stars

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The triple star system α Centauri has the largest known stellar parallax angle, namely 0.75 arcsec. How far is this star system from the Sun in parsecs? (Careful with units!)

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Where are brown dwarfs located on the H-R diagram?

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Sirius has a brightness through a blue filter of bB = 9.4 × 10-8 W/m2. What does this tell you about Sirius?

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On the basis of the Hertzsprung-Russell diagram (Figure 17-15a) and the mass-luminosity relationship for main-sequence stars (Figure 17-22), which of the following main-sequence stars have the greatest mass?

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The spectrum of a particular star shows absorption lines due to calcium, iron, carbon, and titanium oxide. Which of these substances is classified as a "metal" by astronomers?

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When the spectrum of a particular star is photographed and analyzed, it is found that the spectrum contains absorption bands of the metal hydrides methane (CH4) and ammonia (NH3). Based on this information, the star is:

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A star with an apparent magnitude of m = +2.5 is at 100 pc from Earth. What is its absolute magnitude, M?

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A particular star has an absolute magnitude of 0 and a spectral class similar to that of the Sun. Using Figure 17-18, how would this star be classified?

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A star with a ratio of brightness bV/bB of 1.00 has a surface temperature of about: (See Figure 17-9.(in the text))

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How do the characteristics of a K5V star compare to those of a K5II star? The K5II star:

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The star γ Phoenecis has an apparent magnitude of 3.4 and an absolute magnitude of -4.6. The North Star (Polaris) has an apparent magnitude of 2.0 and an absolute magnitude of -4.6. Assuming that no light has been absorbed or scattered by interstellar dust, we can say for sure that:

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The most straightforward way to measure the distance to a nearby star uses:

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If a nearby star shows a parallax of 0.5 arcsec, what is its distance from Earth in light-years?

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The ratio of the brightness of a star at two different colors, blue and visual-bV/bB-is a direct measure of what property of the star?

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Suppose a star lying on the celestial equator has a proper motion, directed along the equator, equal to the rather large value of Barnard's star, namely 10 arcsec/yr. How long would it take this star to change its right ascension by 1 hour?

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Using the Hertzsprung-Russell diagram in Figure 17-15a, determine which type of star has the following characteristics: surface temperature of 40,000 K and luminosity 100,000 times that of the Sun.

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Vega is an A0 V star with a surface temperature of about 10,000 K. Use Figures 17-15a and 17-22 to estimate the mass of Vega.

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Suppose we observe the light curve of a totally eclipsing binary like that in Figure 17-24b. The brightness falls gradually from magnitude 5 to magnitude 9 and remains there for 12 hours before increasing gradually to magnitude 5. Then, after a while, it drops gradually to magnitude 6, remains there for 8 hours, and returns to magnitude 5. What conclusion can be drawn from this light curve?

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Which of the following statements is TRUE of the population of stars in our neighborhood?

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The absolute magnitude of the Sun is +4.8 and its luminosity is 3.9 × 1026 watts. The luminosity of a star whose absolute magnitude is +3.8 is:

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