A) sharper.
B) broader.
C) weaker.
D) stronger.
E) b and c
Correct Answer
verified
True/False
Correct Answer
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Multiple Choice
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
Correct Answer
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Multiple Choice
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.
Correct Answer
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Multiple Choice
A) I & II
B) II & IV
C) I,II,& IV
D) II,III,& IV
E) I,II,III,& IV
Correct Answer
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Multiple Choice
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.
Correct Answer
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Multiple Choice
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
Correct Answer
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True/False
Correct Answer
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Multiple Choice
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.
Correct Answer
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Multiple Choice
A) distance and diameter.
B) temperature and distance.
C) distance.
D) temperature and diameter.
E) apparent magnitude.
Correct Answer
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Multiple Choice
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.
Correct Answer
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Multiple Choice
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
Correct Answer
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Multiple Choice
A) closer than 10 pc.
B) farther than 10 pc.
C) No way to tell.
Correct Answer
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Short Answer
Correct Answer
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Multiple Choice
A) the masses
B) the sizes
C) both a and b
D) neither a nor b
Correct Answer
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Multiple Choice
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
Correct Answer
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Multiple Choice
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.
Correct Answer
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Multiple Choice
A) 20 pc
B) 50 pc
C) 2 pc
D) 5 pc
E) 500 pc
Correct Answer
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Multiple Choice
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
Correct Answer
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Multiple Choice
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
Correct Answer
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