Exam 9: Measuring the Stars
Exam 1: The Night Sky88 Questions
Exam 2: Light and Telescopes111 Questions
Exam 3: The Solar System109 Questions
Exam 4: Earth and Its Moon108 Questions
Exam 5: The Eight Planets112 Questions
Exam 6: Small Bodies in the Solar System108 Questions
Exam 7: Formation of Planetary Systems84 Questions
Exam 8: The Sun95 Questions
Exam 9: Measuring the Stars86 Questions
Exam 10: Star Formation and Evolution85 Questions
Exam 11: Stellar Explosions101 Questions
Exam 12: Black Holes77 Questions
Exam 13: The Milky Way Galaxy82 Questions
Exam 14: Galaxies98 Questions
Exam 15: Cosmology and the Universe98 Questions
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In a spectroscopic binary, if a pair shows a combined set of lines tonight, but a maximum split two nights later, its orbital period must be
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From hottest to coolest, the seven letters for the star types are ________.
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Explain how the shifting spectral lines of spectroscopic binaries let us find their periods.
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If two stars are the same size and one is twice the temperature of the other, how much more luminous is the hotter one?
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What types of observations are necessary to determine the motion of a star through space?
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In a spectroscopic binary system, the star showing the larger blue shift is
(Multiple Choice)
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Having nothing to do with trigonometry, ________ parallaxes use the width of absorption lines to estimate the star's luminosity and size and distance.
(Multiple Choice)
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Star A is a main sequence star of spectral type F2 and star B is a white dwarf of spectral type B4. Which statement below is correct?
(Multiple Choice)
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Capella is the same temperature as our Sun, but about ten times the Sun's diameter; it must be about ________ times as luminous as our star.
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Star A has an absolute magnitude of 2.5 and star B has an apparent magnitude of 2.5, but star A is a main sequence star and star B is a red giant. Which statement below is correct?
(Multiple Choice)
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A star with a parallax of 1 second of arc is at a distance of ________ by definition.
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On the H-R diagram, white dwarfs lie Sirius B and Procyon B lie
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In comparing first magnitude Deneb with second magnitude Polaris, we find that
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