Deck 19: The Universe Galaxies
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Deck 19: The Universe Galaxies
1
The stars in globular clusters
A) are relatively close together.
B) have an average spacing like that of stars in the galactic disk.
C) are relatively far apart.
D) form spiral arms.
A) are relatively close together.
B) have an average spacing like that of stars in the galactic disk.
C) are relatively far apart.
D) form spiral arms.
are relatively close together.
2
The individual stars we can see with the unaided eyes
A) are all members of our galaxy.
B) include members of other galaxies.
C) are all giant stars.
D) are all members of the main sequence.
A) are all members of our galaxy.
B) include members of other galaxies.
C) are all giant stars.
D) are all members of the main sequence.
are all members of our galaxy.
3
Our galaxy is
A) one of the smallest known.
B) average in size.
C) one of the largest known.
D) impossible to compare with others because they are so far away.
A) one of the smallest known.
B) average in size.
C) one of the largest known.
D) impossible to compare with others because they are so far away.
one of the largest known.
4
A source of radio waves from space is
A) cosmic rays.
B) dark matter.
C) fast electrons that move through magnetic fields.
D) white dwarfs.
A) cosmic rays.
B) dark matter.
C) fast electrons that move through magnetic fields.
D) white dwarfs.
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5
All spiral galaxies apparently
A) are rotating.
B) are contracting.
C) are expanding.
D) consist entirely of Population II stars.
A) are rotating.
B) are contracting.
C) are expanding.
D) consist entirely of Population II stars.
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6
Emissions of various kinds from near the center of the Milky Way galaxy suggests the presence of a
A) quasar.
B) globular cluster.
C) black hole.
D) galactic nebula.
A) quasar.
B) globular cluster.
C) black hole.
D) galactic nebula.
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7
Compared with the Population I stars in the disk of our galaxy, the Population II stars in globular clusters
A) are generally younger.
B) have about the same age distribution.
C) are generally older.
D) Any of these choices may be correct in a particular cluster.
A) are generally younger.
B) have about the same age distribution.
C) are generally older.
D) Any of these choices may be correct in a particular cluster.
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8
The ratio of dark matter to ordinary matter in our galaxy is about
A) 1:1.
B) 2:1.
C) 6:1.
D) 25:1.
A) 1:1.
B) 2:1.
C) 6:1.
D) 25:1.
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9
The number of galaxies in the universe seems to be about
A) 200.
B) 200,000.
C) 200 million.
D) 200 billion.
A) 200.
B) 200,000.
C) 200 million.
D) 200 billion.
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10
Dark matter
A) apparently occurs only in our galaxy.
B) apparently occurs in all galaxies.
C) consists of antimatter.
D) consists of cosmic rays.
A) apparently occurs only in our galaxy.
B) apparently occurs in all galaxies.
C) consists of antimatter.
D) consists of cosmic rays.
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11
Interstellar space in our galaxy
A) is completely empty.
B) is completely empty except for clouds of gas and dust.
C) contains about 1 atom or molecule per cm3.
D) contains about 1 atom or molecule per cm3between denser clouds of gas and dust.
A) is completely empty.
B) is completely empty except for clouds of gas and dust.
C) contains about 1 atom or molecule per cm3.
D) contains about 1 atom or molecule per cm3between denser clouds of gas and dust.
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12
Globular clusters of stars
A) are uniformly distributed throughout the universe.
B) are uniformly distributed throughout our galaxy.
C) are located above and below the central disk of our galaxy.
D) are located in the central disk of our galaxy.
A) are uniformly distributed throughout the universe.
B) are uniformly distributed throughout our galaxy.
C) are located above and below the central disk of our galaxy.
D) are located in the central disk of our galaxy.
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13
The Milky Way is a
A) globular duster.
B) nearby galaxy.
C) galaxy with the sun at its center.
D) galaxy with the sun some distance from its center.
A) globular duster.
B) nearby galaxy.
C) galaxy with the sun at its center.
D) galaxy with the sun some distance from its center.
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14
Galaxies
A) have a variety of shapes.
B) are evenly distributed in space.
C) are moving closer to one another.
D) rarely contain more than one or two million stars.
A) have a variety of shapes.
B) are evenly distributed in space.
C) are moving closer to one another.
D) rarely contain more than one or two million stars.
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15
Magnetic fields in our galaxy trap
A) cosmic rays.
B) radio waves.
C) spectral lines.
D) meteoroids.
A) cosmic rays.
B) radio waves.
C) spectral lines.
D) meteoroids.
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16
Our galaxy is shaped roughly like a
A) bunch of grapes.
B) football.
C) fried egg.
D) salami.
A) bunch of grapes.
B) football.
C) fried egg.
D) salami.
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17
The stars in the universe are
A) approximately evenly spaced.
B) concentrated near its center.
C) grouped in widely separated galaxies.
D) irregularly distributed.
A) approximately evenly spaced.
B) concentrated near its center.
C) grouped in widely separated galaxies.
D) irregularly distributed.
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18
The stars in our galaxy
A) move entirely at random.
B) move toward its center.
C) move away from its center.
D) revolve around its center.
A) move entirely at random.
B) move toward its center.
C) move away from its center.
D) revolve around its center.
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19
Molecules in space can be identified from their emissions of
A) light waves.
B) radio waves.
C) cosmic waves.
D) X-rays.
A) light waves.
B) radio waves.
C) cosmic waves.
D) X-rays.
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20
The sun is
A) a Population I star.
B) a Population II star.
C) different from Population I and II stars.
D) a member of a globular cluster.
A) a Population I star.
B) a Population II star.
C) different from Population I and II stars.
D) a member of a globular cluster.
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21
Some, and perhaps all, spiral galaxies have at their centers
A) quasars.
B) pulsars.
C) black holes.
D) globular star clusters.
A) quasars.
B) pulsars.
C) black holes.
D) globular star clusters.
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22
Considering matter and energy together, the largest component of the universe seems to be
A) electromagnetic radiation of various kinds.
B) ordinary matter.
C) dark matter.
D) dark energy.
A) electromagnetic radiation of various kinds.
B) ordinary matter.
C) dark matter.
D) dark energy.
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23
The most distant galaxies are receding at speeds that are
A) much less than the speed of light.
B) not far from the speed of light.
C) equal to the speed of light.
D) greater than the speed of light.
A) much less than the speed of light.
B) not far from the speed of light.
C) equal to the speed of light.
D) greater than the speed of light.
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24
The energy that reaches the earth in cosmic rays is comparable to the energy that reaches the earth in
A) sunlight.
B) moonlight.
C) starlight.
D) radio waves.
A) sunlight.
B) moonlight.
C) starlight.
D) radio waves.
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25
Present evidence suggests that the universe
A) will expand forever.
B) will eventually stop expanding and then remain a fixed size.
C) will eventually stop expanding and then contract.
D) has just begun to contract.
A) will expand forever.
B) will eventually stop expanding and then remain a fixed size.
C) will eventually stop expanding and then contract.
D) has just begun to contract.
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26
The Doppler shifting of radiation from the early universe has resulted in today's universe being bathed in a sea of
A) cosmic rays.
B) X-rays.
C) radio waves.
D) infrared waves.
A) cosmic rays.
B) X-rays.
C) radio waves.
D) infrared waves.
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27
In the past several billion years the rate of expansion of the universe has
A) been constant.
B) decreased.
C) increased.
D) varied irregularly.
A) been constant.
B) decreased.
C) increased.
D) varied irregularly.
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28
Information about the origin of the universe does not come from the
A) fact that spiral galaxies rotate.
B) red shifts in galactic spectra.
C) relative abundances of hydrogen and helium.
D) cosmic background radiation.
A) fact that spiral galaxies rotate.
B) red shifts in galactic spectra.
C) relative abundances of hydrogen and helium.
D) cosmic background radiation.
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29
The proportionality between the recession speeds of the galaxies and their distances from the earth is known as
A) Hess's Law.
B) Herschel's Law.
C) Hubble's Law.
D) Hersey's Law.
A) Hess's Law.
B) Herschel's Law.
C) Hubble's Law.
D) Hersey's Law.
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30
In a "closed" universe
A) expansion of the universe will continue forever.
B) no additional new stars will form.
C) the universe will neither expand nor collapse.
D) expansion will stop and the universe will ultimately collapse.
A) expansion of the universe will continue forever.
B) no additional new stars will form.
C) the universe will neither expand nor collapse.
D) expansion will stop and the universe will ultimately collapse.
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31
Considering matter and energy together, the smallest component of the universe seems to be
A) electromagnetic radiation of various kinds.
B) ordinary matter.
C) dark matter.
D) dark energy.
A) electromagnetic radiation of various kinds.
B) ordinary matter.
C) dark matter.
D) dark energy.
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32
The "big bang" refers to the origin of
A) the sun.
B) the solar system.
C) our galaxy.
D) the universe.
A) the sun.
B) the solar system.
C) our galaxy.
D) the universe.
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33
Quasars
A) are weak sources of light and radio waves.
B) are large in view of the energy they emit.
C) show relatively small red shifts, which suggests they are not far away.
D) seem to have massive black holes at their centers.
A) are weak sources of light and radio waves.
B) are large in view of the energy they emit.
C) show relatively small red shifts, which suggests they are not far away.
D) seem to have massive black holes at their centers.
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34
Galactic spectra show
A) red and blue shifts.
B) red shifts of the same magnitude.
C) red shifts that decrease with distance.
D) red shifts that increase with distance.
A) red and blue shifts.
B) red shifts of the same magnitude.
C) red shifts that decrease with distance.
D) red shifts that increase with distance.
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35
In the light of current evidence, a reasonable figure for the age of the universe is
A) 13.7 million years.
B) 13.7 billion years.
C) 100 billion years.
D) 15 trillion years.
A) 13.7 million years.
B) 13.7 billion years.
C) 100 billion years.
D) 15 trillion years.
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36
The galaxies in the universe are distributed
A) uniformly.
B) randomly.
C) in groups, groups of groups, and so on.
D) in spiral arms.
A) uniformly.
B) randomly.
C) in groups, groups of groups, and so on.
D) in spiral arms.
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37
Primary cosmic rays are produced
A) in the solar system.
B) in galaxies.
C) in the regions between galaxies.
D) everywhere in the universe.
A) in the solar system.
B) in galaxies.
C) in the regions between galaxies.
D) everywhere in the universe.
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38
In the universe today there
A) seems to be little or no antimatter.
B) is much antimatter but less than the amount of matter.
C) are equal amounts of antimatter and matter.
D) is more antimatter than matter.
A) seems to be little or no antimatter.
B) is much antimatter but less than the amount of matter.
C) are equal amounts of antimatter and matter.
D) is more antimatter than matter.
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39
Primary cosmic rays consist of
A) atomic nuclei, mainly protons.
B) neutral atoms, mainly of hydrogen.
C) molecules.
D) electrons.
A) atomic nuclei, mainly protons.
B) neutral atoms, mainly of hydrogen.
C) molecules.
D) electrons.
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40
Dark energy
A) is the energy equivalent of dark matter.
B) is the energy of black holes.
C) is the energy of neutrinos.
D) has an unknown nature as yet.
A) is the energy equivalent of dark matter.
B) is the energy of black holes.
C) is the energy of neutrinos.
D) has an unknown nature as yet.
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41
The number of planets outside the solar system thus far detected is
A) about 20.
B) about 100.
C) several thousand.
D) several million.
A) about 20.
B) about 100.
C) several thousand.
D) several million.
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42
The heavy elements in the earth were formed in
A) the sun.
B) the big bang.
C) supernova explosions.
D) white dwarfs.
A) the sun.
B) the big bang.
C) supernova explosions.
D) white dwarfs.
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43
Communications with planets outside the solar system are most likely to be achieved using
A) spacecraft of the kind that went to the moon.
B) spacecraft that travel with the speed of light.
C) spacecraft that travel faster than light.
D) radio waves.
A) spacecraft of the kind that went to the moon.
B) spacecraft that travel with the speed of light.
C) spacecraft that travel faster than light.
D) radio waves.
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44
Nearly all the helium in the universe was formed in
A) the first few minutes after the big bang.
B) the interior of stars.
C) supernova explosions.
D) black holes.
A) the first few minutes after the big bang.
B) the interior of stars.
C) supernova explosions.
D) black holes.
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45
Planetary systems are probably
A) very rare in the universe.
B) present around many stars.
C) present around all stars.
D) present only around stars that rotate rapidly.
A) very rare in the universe.
B) present around many stars.
C) present around all stars.
D) present only around stars that rotate rapidly.
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46
Studies of the cosmic background radiation suggest that matter in the early universe
A) was uniformly distributed.
B) had small irregularities that grew into today's galaxies.
C) had large irregularities that grew into today's galaxies.
D) formed spiral arms like those in today's galaxies.
A) was uniformly distributed.
B) had small irregularities that grew into today's galaxies.
C) had large irregularities that grew into today's galaxies.
D) formed spiral arms like those in today's galaxies.
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47
The members of the solar system
A) came from space and were captured by the sun.
B) came into being at the same time as the sun did.
C) were formed from material ejected by the sun after it came into being.
D) were formed from dark matter.
A) came from space and were captured by the sun.
B) came into being at the same time as the sun did.
C) were formed from material ejected by the sun after it came into being.
D) were formed from dark matter.
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48
The cosmic background radiation today
A) is present only in galaxies.
B) is present everywhere in the universe.
C) accounts for less of the radiation in the universe than starlight.
D) is visible as a faint glow in the sky on dark nights.
A) is present only in galaxies.
B) is present everywhere in the universe.
C) accounts for less of the radiation in the universe than starlight.
D) is visible as a faint glow in the sky on dark nights.
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49
Immediately after the big bang, the universe contained
A) only matter.
B) equal amounts of matter and antimatter.
C) slightly more matter than antimatter.
D) slightly more antimatter than matter.
A) only matter.
B) equal amounts of matter and antimatter.
C) slightly more matter than antimatter.
D) slightly more antimatter than matter.
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50
As they came into being, the planets were primarily heated by
A) gravitational compression.
B) solar radiation.
C) cosmic rays.
D) cosmic background radiation.
A) gravitational compression.
B) solar radiation.
C) cosmic rays.
D) cosmic background radiation.
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