A) period of brightness variation and spectral color.
B) variation of spectral color and distance to the star.
C) period of brightness variation and luminosity.
D) amplitude of brightness variation and luminosity.
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Multiple Choice
A) spiral (a regular pattern of spiral arms)
B) elliptical (a smooth star distribution lacking spiral arms)
C) The Milky Way is not a galaxy at all but a large cluster of stars.
D) irregular (possible clumps of stars but no overall pattern)
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Multiple Choice
A) synchrotron (nonthermal) radiation produced by electrons spiraling in a powerful magnetic field
B) huge filaments of gas similar in structure to solar prominences
C) rapidly fluctuating emissions from a gigantic millisecond pulsar
D) halo of lobes of hot, ionized X-ray-emitting gas
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Multiple Choice
A) whether all stars were like the Sun or fundamentally different
B) whether the spiral "nebulae" were part of the Milky Way Galaxy or more distant, separate entities
C) whether the universe was expanding outward in all directions
D) whether the Sun was at the center of the Milky Way Galaxy
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Multiple Choice
A) distance measurements to galaxies
B) determination of stellar luminosities
C) determination of speeds of stars in galactic arms from the Doppler shift of their spectra
D) keeping of accurate time
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Multiple Choice
A) Edwin Hubble in 1923.
B) Immanuel Kant in 1755.
C) William Parsons, Earl of Rosse, in 1845.
D) Sir Isaac Newton in 1690.
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Multiple Choice
A) nowhere
B) only in the galactic center
C) in the galactic center and within some globular clusters
D) in the galactic center, within some globular clusters, and in several locations between the spiral arms
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Multiple Choice
A) stars at the same orbital distance as the Sun
B) stars in directions 45° from the Sun's direction of motion
C) All the companion stars are moving along with the Sun and have no relative velocity with respect to it.
D) stars directly between the Sun and the galactic center
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Multiple Choice
A) isolated field stars
B) globular clusters
C) small dwarf galaxies
D) large spiral galaxies
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Multiple Choice
A) visible and infrared
B) visible and ultraviolet
C) radio
D) microwave
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Multiple Choice
A) an X-ray flare that faded over a few hours
B) synchrotron radiation from the surrounding magnetic fields
C) the Doppler shifts of stars orbiting the black hole
D) the rate gas falls onto the black hole
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Multiple Choice
A) The Balmer lines are associated with neutral hydrogen, and most of the hydrogen astronomers need to observe is molecular hydrogen.
B) The Balmer lines are associated with molecular hydrogen, and most of the hydrogen astronomers need to observe is neutral hydrogen.
C) The Balmer lines are in the visible and ultraviolet regions of the spectrum, and these do not penetrate the gas and dust clouds easily.
D) Photons released in the spin-flip transition have much more energy than those that come from the Balmer transitions.
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Multiple Choice
A) The neutral hydrogen in this region is not moving relative to Earth.
B) The neutral hydrogen in this region is moving perpendicularly across the line of sight.
C) The neutral hydrogen in this region is in a circular orbit around the galactic center at the same radius as the solar system.
D) The neutral hydrogen in this region is moving away from Earth instead of toward Earth.
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Multiple Choice
A) locations of globular clusters around the Galaxy.
B) density of stars in different directions along the Milky Way.
C) distances to open star clusters and H II regions in the disk of the Galaxy.
D) structure of the Andromeda Galaxy and a comparison of it with the structure of the Milky Way.
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Multiple Choice
A) The two shells are virtually identical except for their distance from the galactic nucleus.
B) The stars of the outer shell are much younger than those of the shell layer.
C) The stars of the outer shell are relatively metal-rich.
D) The stars of the outer shell orbit in the opposite sense from those of the inner shell.
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Multiple Choice
A) globular clusters in the halo of the Galaxy.
B) Balmer emission lines of visible radiation from hydrogen.
C) 21-cm radiation from interstellar hydrogen and the distribution of young stars.
D) Lyman UV radiation from hot hydrogen gas.
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Multiple Choice
A) Sagittarius
B) Lyra
C) Hercules
D) Ursa Major
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Multiple Choice
A) The curve is a straight line, slanted upward, suggesting that the velocity increases linearly with radius.
B) The curve rises steeply, levels off, and then experiences the "Keplerian falloff" expected from Kepler's third law.
C) The curve rises steeply and then oscillates up and down showing the effect of the spiral arms.
D) The curve rises steeply, and then levels off or rises gradually until well beyond the edge of the visible galaxy.
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Multiple Choice
A) No. The distances were still correct.
B) Yes. For a given Cepheid period, the new distances were smaller than those originally calculated.
C) Yes. For a given Cepheid period, the new distances were larger than those originally calculated.
D) Yes. New distances had to be calculated, which could be larger or smaller than the original calculation.
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Multiple Choice
A) Cepheid variable stars appeared to be very faint in the "nebula."
B) the "nebula" appeared to be rotating night by night around a center that was not the center of the Milky Way.
C) stars with characteristics similar to those of the Sun appeared to be absent in the "nebula."
D) globular clusters appeared to be distributed in a halo around the "nebula," a sure sign of a separate galaxy.
Correct Answer
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