Exam 10: Characterizing Stars

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If you compare two stars,the one with the _____ must have the greater luminosity.

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The star Alphard has an apparent magnitude of 2.0,and the star Megrez has an apparent magnitude of 3.3.The only thing that can be said with certainty about Alphard is that it is _____ than Megrez.

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What is parallax?

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Which atom or ion produces strong absorption lines in the spectra of stars with relatively cool surface temperatures?

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Using the Hertzsprung-Russell diagram and the mass-luminosity relationship for main-sequence stars (Figure 10-14 of Comins,Discovering the Essential Universe,6th ed.),determine which type of main-sequence stars would have the highest mass.

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The difference in the brightness of a star as seen through two different colored filters,for example,blue and yellow,is directly related to which stellar property?

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Two stars in our sky have the same apparent brightness.If neither of them is hidden behind gas or dust clouds,then we know that they:

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The first accurate measurement of stellar parallax was made in:

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How are white dwarfs treated in the luminosity class definitions?

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A star of apparent magnitude +2.1 appears _____ than a star of apparent magnitude -1.2.

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Star A has luminosity LA = 100 L⊙ and it is 1000 pc away.Star B has the same luminosity as the Sun,L⊙,and it is 100 pc away.What can you say about the brightnesses of these two stars?

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A particular star appears approximately equally bright when viewed through a blue filter and through a yellow filter.What is the approximate surface temperature of this star? (See Figure 10-4,Comins,Discovering the Essential Universe,6th ed.)

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Which is NOT needed to determine individual masses in a binary star system?

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Two stars in a binary system orbit around a common point that is:

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A star that is 100 pc distant from Earth has an apparent magnitude of m +2.5.According to the equation in Discovery 10-2 in Comins,Discovering the Essential Universe,6th ed.,what is its absolute magnitude?

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What proportion of visible stars in our nighttime sky are members of multiple-star systems,such as binary stars?

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The technique called photometry in stellar astronomy is the measurement of the:

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Measurements indicate that a certain star has a very high intrinsic brightness (100,000 times as bright as the Sun)and yet is relatively cool (3500 K).How can this be?

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The star ɛ Canis Majoris has an absolute magnitude of -4.1 and a spectral luminosity class of B2 V.The star ϒ Crucis has a spectral class of M4 and the same absolute magnitude as ɛ Canis Majoris.Using Figure 10-10 of Comins,Discovering the Essential Universe,6th ed.,the spectral luminosity class ofϒ Crucis is probably:

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What is the difference between an optical double star and a visual binary star?

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