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Compared with the spectral lines in the solar spectrum,lines in a supergiant spectrum are


A) sharper.
B) broader.
C) weaker.
D) stronger.
E) b and c

F) A) and B)
G) All of the above

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To observe a spectroscopic binary,we must be able to see both stars individually.

A) True
B) False

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The correct sequence of spectral type letters from hot on the left to cool on the right is


A) M,K,G,F,A,B,O
B) O,B,A,F,G,K,M
C) G,K,M,F,O,B,A
D) A,B,O,F,G,K,M

E) A) and C)
F) All of the above

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The most accurate way to determine the surface temperature of a star is to study


A) the pattern of absorption lines from various atoms.
B) the relative intensities of light measured through different photometric filters.
C) the peak wavelength of the star's continuum blackbody spectrum.
D) pattern of emission lines that are on the star's spectrum.

E) A) and D)
F) A) and C)

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Giant stars are Giant stars are   A)  I & II B)  II & IV C)  I,II,& IV D)  II,III,& IV E)  I,II,III,& IV


A) I & II
B) II & IV
C) I,II,& IV
D) II,III,& IV
E) I,II,III,& IV

F) A) and D)
G) A) and B)

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How is a luminosity class assigned to a star?


A) By combining the apparent magnitude with the star's parallax.
B) By measuring the period of variability in the star's apparent magnitude.
C) By studying the absorption lines in the spectrum of the star.
D) By observing the angular size of the star's image in a photograph or digital image.

E) B) and D)
F) A) and D)

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Absolute visual magnitude is


A) the apparent magnitude of a star observed from Earth.
B) the luminosity of a star observed from a distance of 1000 pc.
C) the apparent magnitude of a star observed from a distance of 10 pc.
D) the luminosity of a star observed from Earth.
E) c and d

F) None of the above
G) A) and E)

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The location of a star in the HR diagram indicates its temperature and intrinsic brightness.

A) True
B) False

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In the H-R diagram,90 percent of all stars are


A) in the giant region.
B) in the supergiant region.
C) among the B stars.
D) among the G stars.
E) on the main sequence.

F) C) and D)
G) B) and D)

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A star's absolute magnitude depends only on the star's


A) distance and diameter.
B) temperature and distance.
C) distance.
D) temperature and diameter.
E) apparent magnitude.

F) A) and B)
G) A) and E)

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We know that giant stars are larger in diameter than the sun because


A) they are more luminous but have about the same temperature.
B) they are less luminous but have about the same temperature.
C) they are hotter but have about the same luminosity.
D) they are cooler but have about the same luminosity.
E) they have a larger absolute magnitude than the sun.

F) None of the above
G) C) and D)

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The mass of a visual binary pair of stars can be obtained from


A) the time in years for them to orbit one another.
B) the size of their orbit.
C) their apparent magnitudes.
D) both a and b

E) A) and C)
F) B) and D)

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Use the following chart to answer the questions below: Use the following chart to answer the questions below:     -Refer to Table 9-1.The star HR 4621 is A)  closer than 10 pc. B)  farther than 10 pc. C)  No way to tell. -Refer to Table 9-1.The star HR 4621 is


A) closer than 10 pc.
B) farther than 10 pc.
C) No way to tell.

D) A) and B)
E) All of the above

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Luminosity class IV objects are known as ____________________.

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Doppler shift observations of a spectroscopic binary star can enable astronomers to calculate ____ of its individual stars.


A) the masses
B) the sizes
C) both a and b
D) neither a nor b

E) A) and B)
F) B) and C)

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The distance to Rigel is 250 pc.Which of the following statements is true based on this information?


A) The distance to Rigel can be determined by measuring its parallax.
B) Rigel's apparent visual magnitude has a smaller value than its absolute visual magnitude.
C) The absolute bolometric magnitude of Rigel is nearly equal to its absolute visual magnitude.
D) Rigel is located in the upper right corner of the HR diagram.
E) none of the above

F) A) and E)
G) D) and E)

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A star's apparent magnitude is a measure of ...


A) how bright it appears to us if it is at its actual distance.
B) how bright it appears to us at a standard distance of 10 pc.
C) its energy output per second compared to the sun.
D) its mass in solar masses.
E) its surface temperature in degrees Kelvin.

F) D) and E)
G) A) and B)

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If a star has a parallax of 0.02 seconds of arc,then its distance will be


A) 20 pc
B) 50 pc
C) 2 pc
D) 5 pc
E) 500 pc

F) A) and B)
G) A) and C)

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Use the following chart to answer the questions below:  Use the following chart to answer the questions below:    NARREND -Which star in Table 9-2 would appear the faintest in the night sky? A)  65 Tau B)  HR 4621 C)  ( \alpha  Pic)  D)  58 Ori E)  HR 2491 NARREND -Which star in Table 9-2 would appear the faintest in the night sky?


A) 65 Tau
B) HR 4621
C) ( Ξ±\alpha Pic)
D) 58 Ori
E) HR 2491

F) C) and E)
G) None of the above

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How can we tell that some stars are relatively close to us in the sky?


A) Some stars are occasionally eclipsed by the Moon,so they must be nearby.
B) Some stars vary in brightness caused by sunspots we can see because they are so close.
C) Some stars appear to be extremely bright and must therefore be very close to us.
D) Some stars appear to move periodically back and forth against the background stars because of the Earth's movement around the Sun

E) C) and D)
F) B) and C)

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