Deck 1: Astronomy and the Universe
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Deck 1: Astronomy and the Universe
1
Which unique quality distinguishes human beings from other living things?
A)the continuing need to test the ability and strength of their leaders
B)curiosity, the need to explore and understand our surroundings
C)social behavior, the desire to protect the young, the old, and the weak
D)the will to fight to resolve conflicts
A)the continuing need to test the ability and strength of their leaders
B)curiosity, the need to explore and understand our surroundings
C)social behavior, the desire to protect the young, the old, and the weak
D)the will to fight to resolve conflicts
B
2
Which scientific discipline can be considered as truly universal?
A)astronomy
B)social studies
C)geology
D)biological science
A)astronomy
B)social studies
C)geology
D)biological science
A
3
Astronomy:
A)has not yet influenced our lives significantly, although future developments like mining on the Moon may become important.
B)studies only far-away places and has no application to our lives here on Earth.
C)allows us to predict our individual destinies from the movements of the planets, but has never had any other useful application.
D)has had important practical applications including the development of Newtonian mechanics, on which much of modern technology is based.
A)has not yet influenced our lives significantly, although future developments like mining on the Moon may become important.
B)studies only far-away places and has no application to our lives here on Earth.
C)allows us to predict our individual destinies from the movements of the planets, but has never had any other useful application.
D)has had important practical applications including the development of Newtonian mechanics, on which much of modern technology is based.
D
4
The scientific method is a major force in science and has been developed to ensure that:
A)theories about physical phenomena are so good and our faith in them is so strong that we never need to test them against observations.
B)theories about physical phenomena agree with the wisdom of the ancients.
C)results from experiments can be adjusted to agree with our carefully developed theories about physical phenomena.
D)theories about physical phenomena agree with what we find in experiments and observations.
A)theories about physical phenomena are so good and our faith in them is so strong that we never need to test them against observations.
B)theories about physical phenomena agree with the wisdom of the ancients.
C)results from experiments can be adjusted to agree with our carefully developed theories about physical phenomena.
D)theories about physical phenomena agree with what we find in experiments and observations.
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5
The rules that govern the behavior of matter and have inspired major advances in engineering are known as:
A)Murphy's laws.
B)the laws of physics.
C)the laws of social behavior.
D)the laws of chance.
A)Murphy's laws.
B)the laws of physics.
C)the laws of social behavior.
D)the laws of chance.
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6
The laws of physics developed in laboratories on Earth are generally assumed to be valid:
A)only on Earth.
B)only in our solar system.
C)only in our galaxy.
D)everywhere in the universe.
A)only on Earth.
B)only in our solar system.
C)only in our galaxy.
D)everywhere in the universe.
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7
The most important reason for exploring other planets is that:
A)the study of the solar system is our greatest source of information on the formation of the universe.
B)it allows us to understand our own planet more thoroughly.
C)it extends human's thoughts onto a plane that is totally removed from our limited existence here on Earth.
D)it has become vital for us to develop these planets as sources of raw materials.
A)the study of the solar system is our greatest source of information on the formation of the universe.
B)it allows us to understand our own planet more thoroughly.
C)it extends human's thoughts onto a plane that is totally removed from our limited existence here on Earth.
D)it has become vital for us to develop these planets as sources of raw materials.
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8
Based on dating of meteorites, the oldest rocks found on Earth, we have concluded that our solar system formed about 4.56 __________ years ago.
A)thousand
B)million
C)billion
D)trillion
A)thousand
B)million
C)billion
D)trillion
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9
Which of the following space exploits has not yet been accomplished by humans?
A)walking on the surface of the Moon
B)landing a spacecraft on Saturn's surface
C)studying the surface of Venus under its thick, permanent cloud cover
D)discovering active volcanoes on other worlds
A)walking on the surface of the Moon
B)landing a spacecraft on Saturn's surface
C)studying the surface of Venus under its thick, permanent cloud cover
D)discovering active volcanoes on other worlds
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10
In our exploration of the solar system, we have sent spacecraft intended to land on or fly past:
A)only the closer planets: Venus, Mars, Jupiter, and Saturn.
B)all the planets, but not Pluto.
C)only the nearest planets to Earth, Venus, and Mars.
D)all planets from Mercury to Neptune as well as Pluto.
A)only the closer planets: Venus, Mars, Jupiter, and Saturn.
B)all the planets, but not Pluto.
C)only the nearest planets to Earth, Venus, and Mars.
D)all planets from Mercury to Neptune as well as Pluto.
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11
The oldest objects in the solar system whose age has been measured are:
A)the Moon rocks brought back by the Apollo astronauts.
B)rocks from the Canadian shield of North America.
C)the large satellites of the jovian planets.
D)meteorites.
A)the Moon rocks brought back by the Apollo astronauts.
B)rocks from the Canadian shield of North America.
C)the large satellites of the jovian planets.
D)meteorites.
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12
So far, our study of the other bodies in our solar system is based on:
A)Earth-based telescopic observations only.
B)telescopic observations from Earth and from spacecraft only.
C)telescopic observations from Earth and spacecraft plus geologic samples brought back from the Moon.
D)telescopic observations from Earth and spacecraft plus information from crewed landings on about half the planets.
A)Earth-based telescopic observations only.
B)telescopic observations from Earth and from spacecraft only.
C)telescopic observations from Earth and spacecraft plus geologic samples brought back from the Moon.
D)telescopic observations from Earth and spacecraft plus information from crewed landings on about half the planets.
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13
Which of the following is not considered to be part of our solar system?
A)the Sun
B)the Moon
C)Pluto
D)the Orion Nebula
A)the Sun
B)the Moon
C)Pluto
D)the Orion Nebula
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14
Which of the following is not considered to be part of our solar system?
A)meteors
B)comets
C)exoplanets
D)asteroids
A)meteors
B)comets
C)exoplanets
D)asteroids
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15
The idea of thermonuclear fusion, the release of energy following the conversion of hydrogen nuclei into a helium nucleus, was first suggested as the source of energy in:
A)the interior of Earth.
B)the central core of the Sun.
C)a weapon of mass destruction.
D)a controllable nuclear power station.
A)the interior of Earth.
B)the central core of the Sun.
C)a weapon of mass destruction.
D)a controllable nuclear power station.
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16
Larger stars have more thermonuclear "fuel":
A)and, since all nuclear reactions proceed at the same rate, they live longer than smaller stars which have less fuel.
B)but they also consume their fuel at a larger rate and thus live the same length of time as smaller stars, which have less fuel but consume it more slowly.
C)but they also consume their fuel at a larger rate and thus live the a shorter time than smaller stars, which have less fuel but consume it more slowly.
D)but there is no correlation between the size of a star and its lifetime.
A)and, since all nuclear reactions proceed at the same rate, they live longer than smaller stars which have less fuel.
B)but they also consume their fuel at a larger rate and thus live the same length of time as smaller stars, which have less fuel but consume it more slowly.
C)but they also consume their fuel at a larger rate and thus live the a shorter time than smaller stars, which have less fuel but consume it more slowly.
D)but there is no correlation between the size of a star and its lifetime.
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17
The lifetime of a typical star (like our Sun) appears to be:
A)a few thousands of years.
B)a few millions of years.
C)a few billions of years.
D)essentially infinite because we know of no mechanism that can terminate the nuclear processes in a star's interior.
A)a few thousands of years.
B)a few millions of years.
C)a few billions of years.
D)essentially infinite because we know of no mechanism that can terminate the nuclear processes in a star's interior.
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18
Heavy elements, such as those throughout Earth and within our bodies, appear to have been formed:
A)only during the initial Big Bang formation of the universe.
B)by radioactive decay here on Earth.
C)inside the Sun.
D)deep inside some now-vanished star.
A)only during the initial Big Bang formation of the universe.
B)by radioactive decay here on Earth.
C)inside the Sun.
D)deep inside some now-vanished star.
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19
Now about halfway through its life cycle, our Sun is expected to last another __________ billion years.
A)1
B)5
C)10
D)20
A)1
B)5
C)10
D)20
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20
The lifetime of our Sun is estimated to be about:
A)125 million years.
B)4.56 billion years.
C)12.5 billion years.
D)110 billion years.
A)125 million years.
B)4.56 billion years.
C)12.5 billion years.
D)110 billion years.
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21
The study of galaxies gives astronomers important clues about the:
A)origin of intellect.
B)existence of life in the universe beyond Earth.
C)formation of planets.
D)beginning of the universe.
A)origin of intellect.
B)existence of life in the universe beyond Earth.
C)formation of planets.
D)beginning of the universe.
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22
In galaxies, where are the sites of star formation?
A)in the spiral arms
B)in the center
C)in black holes
D)nowhere; stars appear to be formed in the space between galaxies.
A)in the spiral arms
B)in the center
C)in black holes
D)nowhere; stars appear to be formed in the space between galaxies.
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23
What do we mean by the Big Bang?
A)the cosmic explosion at the beginning of the universe and the origin of the cosmic expansion that we now observe
B)the projected end of the universe, the result of the cosmic collapse that will inevitably follow the cosmic expansion we now observe
C)the cataclysmic event that produced our solar system about 13.7 billion years ago
D)the tremendous explosion that occurs when a quasar becomes a black hole, sending gravitational waves and cosmic rays throughout the universe
A)the cosmic explosion at the beginning of the universe and the origin of the cosmic expansion that we now observe
B)the projected end of the universe, the result of the cosmic collapse that will inevitably follow the cosmic expansion we now observe
C)the cataclysmic event that produced our solar system about 13.7 billion years ago
D)the tremendous explosion that occurs when a quasar becomes a black hole, sending gravitational waves and cosmic rays throughout the universe
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24
If we could view each of the following objects from the same distance, which would be the brightest?
A)a star
B)a quasar
C)a normal galaxy
D)a solar system
A)a star
B)a quasar
C)a normal galaxy
D)a solar system
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25
Each of the following is a possible stage in the late evolution of a massive star except one. Which is the exception?
A)quasar
B)supernova
C)pulsar
D)black hole
A)quasar
B)supernova
C)pulsar
D)black hole
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26
In angular measurements used in astronomy, how many right angles are there in a full circle?
A)two
B)six
C)one
D)four
A)two
B)six
C)one
D)four
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27
The angle of 60° between the line from the Sun to Jupiter and the line from the Sun to the Trojan group of asteroids (See Figure 15-14a of Universe, 11th ed.) is what fraction of a full circle?
A)1/2
B)1/3
C)1/5
D)1/6

A)1/2
B)1/3
C)1/5
D)1/6
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28
The angle subtended by the Moon (diameter 3500 km) to an observer on Earth (Moon-Earth distance is about 400,000 km) is approximately:
A)1/2 degree.
B)1700 degrees.
C)1/1700 degree.
D)1/2 arcminute.
A)1/2 degree.
B)1700 degrees.
C)1/1700 degree.
D)1/2 arcminute.
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29
The Saturn 5 rocket, used to send astronauts to the Moon, stood about 110 m high. At what distance would you have to stand in order to have the rocket subtend an angle of about 2.5 degrees? (This angle is the field of view of a 600-mm focal length telephoto lens on a 35-mm camera.)
A)275 km
B)0.25 km
C)2700 km
D)2.5 km
A)275 km
B)0.25 km
C)2700 km
D)2.5 km
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30
At what distance would a friend have to hold a dime (about 1 cm diameter) for it to subtend an angle of 2 arcseconds?
A)at the distance of the Moon
B)1 km
C)10 cm
D)105 km
A)at the distance of the Moon
B)1 km
C)10 cm
D)105 km
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31
Suppose a star rises due east, passes directly overhead, and then sets 12 hours after it rose. What is its average angular speed (in arcseconds per second)?
A)7.5
B)15
C)30
D)180
A)7.5
B)15
C)30
D)180
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32
Using a technique known as very long baseline interferometry (VLBI), in which the signals received by two radio telescopes located on different continents are combined as if they were a single radio telescope, astronomers can resolve two objects separated by only 0.00001 second of arc. What is the smallest detail we can see in a quasar 15 billion light-years away using this kind of interferometer?
A)0.7 ly
B)44 ly
C)2400 ly
D)150,000 ly
A)0.7 ly
B)44 ly
C)2400 ly
D)150,000 ly
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33
A globular cluster of stars is measured to have an angular diameter of 20.6 arcseconds, and its distance from Earth is measured to be 200,000 light-years. What is its approximate physical diameter in light-years?
A)200,000
B)1/20
C)20
D)2
A)200,000
B)1/20
C)20
D)2
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34
What is the approximate angular diameter of the Sun in arcseconds?
A)186
B)930
C)1.86
D)1860
A)186
B)930
C)1.86
D)1860
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35
On May 9, 2018, the planet Jupiter had an angular diameter of 43.8 arcseconds as viewed from Earth. Which of the following is a correct statement about this angular diameter?
A)This value is constant. Jupiter always has that angular diameter when viewed from Earth.
B)This value changes. The angular diameter gets larger as the distance to Jupiter becomes larger, and smaller as the distance to Jupiter becomes smaller.
C)This value changes. The angular diameter gets larger as the distance to Jupiter becomes smaller, and smaller as the distance to Jupiter becomes larger.
D)This value changes. It is always larger during that part of Saturn's orbit when Jupiter is closer to the Sun, and it is smaller when Jupiter is farther from the Sun.
A)This value is constant. Jupiter always has that angular diameter when viewed from Earth.
B)This value changes. The angular diameter gets larger as the distance to Jupiter becomes larger, and smaller as the distance to Jupiter becomes smaller.
C)This value changes. The angular diameter gets larger as the distance to Jupiter becomes smaller, and smaller as the distance to Jupiter becomes larger.
D)This value changes. It is always larger during that part of Saturn's orbit when Jupiter is closer to the Sun, and it is smaller when Jupiter is farther from the Sun.
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36
If a stick of length 5.18 m is placed so that the ends just touch a circle of radius 10 m, the stick will subtend a 30° angle when viewed from the center of the circle. What does the formula derived in Box 1-1 give you as the length of this stick?
A)1.26 m
B)5.18 m
C)5.24 m
D)11.8 m
A)1.26 m
B)5.18 m
C)5.24 m
D)11.8 m
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37
A circle of radius 10m has a circumference C = 2πR = 62.83 m. A 30° angle would intercept an arc that is 30/360 or 1/12 of this, namely 5.24 m. What does this result (along with the result in the previous problem) suggest about the validity of the formula derived in Box 1-1? [Note to instructors: This question and the previous one are intended to reinforce concept that the small angle formula computes subtended arc length, which is slightly greater than D in Box 1-1 for large angles, but a reasonably good approximation for small angles.]
A)The formula is valid even for angles as large as 30°.
B)The formula actually calculates the length subtended by a given angle at a given distance. Thus the formula computes a length that is longer than length D in Box 1-1.
C)The formula actually calculates the length subtended by a given angle at a given distance. Thus the formula computes a length that is shorter than length D in Box 1-1.
D)The formula is valid for angles larger than 30° but not for angles smaller than 30°.
A)The formula is valid even for angles as large as 30°.
B)The formula actually calculates the length subtended by a given angle at a given distance. Thus the formula computes a length that is longer than length D in Box 1-1.
C)The formula actually calculates the length subtended by a given angle at a given distance. Thus the formula computes a length that is shorter than length D in Box 1-1.
D)The formula is valid for angles larger than 30° but not for angles smaller than 30°.
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38
The average distance from Earth to the Sun, 149,600,000 km, can be written in shorthand notation as:
A)1.496 × 109 km.
B)1.496 × 106 km.
C)1.496 × 108 km.
D)1.496 × 107 km.
A)1.496 × 109 km.
B)1.496 × 106 km.
C)1.496 × 108 km.
D)1.496 × 107 km.
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39
The mean distance of Jupiter from the Sun, 778,300,000 km, can be written in shorthand notation as:
A)7.783 × 108 km.
B)7.783 × 109 km.
C)7.783 × 107 km.
D)7.783 × 106 km.
A)7.783 × 108 km.
B)7.783 × 109 km.
C)7.783 × 107 km.
D)7.783 × 106 km.
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40
There are 1000 mm in 1 m. This means that a distance of 5 mm is:
A)5 × 103 m.
B)5 × 10-3 m.
C)2 × 10-4 m.
D)5 × 10-2 m.
A)5 × 103 m.
B)5 × 10-3 m.
C)2 × 10-4 m.
D)5 × 10-2 m.
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41
0.0064 m is:
A)0.64 mm.
B)640 mm.
C)6.4 mm.
D)64 mm.
A)0.64 mm.
B)640 mm.
C)6.4 mm.
D)64 mm.
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42
10 × 105 =
A)1 billion
B)10 million
C)1 million
D)10,000
A)1 billion
B)10 million
C)1 million
D)10,000
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43
25 =
A)100,000
B)32
C)25
D)200,000
A)100,000
B)32
C)25
D)200,000
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44
(1/2)3 =
A)8
B)1.25 × 10-1
C)0.5
D)0.167
A)8
B)1.25 × 10-1
C)0.5
D)0.167
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45
(0.5)2 =
A)2.5 × 10-2
B)0.25
C)2.5
D)1.0
A)2.5 × 10-2
B)0.25
C)2.5
D)1.0
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46
10-2 × 102 =
A)0
B)1/100
C)1
D)10,000
A)0
B)1/100
C)1
D)10,000
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47
(2 × 102)3 =
A)6 × 106
B)8 × 106
C)8 × 105
D)6 × 105
A)6 × 106
B)8 × 106
C)8 × 105
D)6 × 105
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48
105 × 108 =
A)1040
B)103
C)1013
D)1020
A)1040
B)103
C)1013
D)1020
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49
106/109 =
A)1054
B)1015
C)10-3
D)103
A)1054
B)1015
C)10-3
D)103
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50
106/106 =
A)1
B)10
C)0
D)1012
A)1
B)10
C)0
D)1012
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51
(9.0 × 105)/(1.5 × 103) =
A)13.5 × 1015
B)3 × 10-2
C)600
D)7.5 × 10-2
A)13.5 × 1015
B)3 × 10-2
C)600
D)7.5 × 10-2
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52
2.5 × 104 × 2.5 × 10-4 =
A)5.0 × 10-8
B)5.0
C)6.25
D)1.0 × 106
A)5.0 × 10-8
B)5.0
C)6.25
D)1.0 × 106
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53
A particular molecule has a diameter of 12 billionths of a meter. This distance is equal to:
A)1.2 nanometers (1.2 nm).
B)1.2 micrometers (1.2 μm).
C)12 nanometers (12 nm).
D)12 micrometers (12 μm).
A)1.2 nanometers (1.2 nm).
B)1.2 micrometers (1.2 μm).
C)12 nanometers (12 nm).
D)12 micrometers (12 μm).
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54
An astronomer is measuring the brightness of a star using infrared light of wavelength 7.8 μm. This corresponds to a wavelength of:
A)7.8 millionths of a meter.
B)7.8 billionths of a meter.
C)7.8 trillionths of a meter (where 1 trillion = 1 million million)
D)780 millionths of a meter.
A)7.8 millionths of a meter.
B)7.8 billionths of a meter.
C)7.8 trillionths of a meter (where 1 trillion = 1 million million)
D)780 millionths of a meter.
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55
The distance from Earth to the star Betelgeuse (in the constellation Orion) has been measured as 520 light-years. Expressed in parsecs, this is approximately:
A)160 pc.
B)350 pc.
C)520 Mpc (megaparsecs).
D)1700 pc.
A)160 pc.
B)350 pc.
C)520 Mpc (megaparsecs).
D)1700 pc.
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56
The distance to the star τ Scorpii has been measured as 230 pc. Expressed in light-years, this is approximately:
A)230 Mly (million light-years).
B)340 ly.
C)750 ly.
D)70 ly.
A)230 Mly (million light-years).
B)340 ly.
C)750 ly.
D)70 ly.
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57
The star Aquilii is 340 ly from Earth. Expressed in parsecs, this is approximately:
A)1100 pc.
B)105 pc.
C)750 pc.
D)0.340 kpc (kiloparsecs).
A)1100 pc.
B)105 pc.
C)750 pc.
D)0.340 kpc (kiloparsecs).
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58
The star ? Puppis is about 750 pc from Earth. Expressed in light-years, this is approximately:
A)230 ly.
B)1500 ly.
C)2445 ly.
D)7.5 × 105 ly.
A)230 ly.
B)1500 ly.
C)2445 ly.
D)7.5 × 105 ly.
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59
What is the distance between Earth and the nearest star? (Think carefully about your answer!) (Check the list of stars in the Appendix 4 of Universe, 11th ed.)
A)5.2 au
B)4.3 pc
C)1 au
D)4.3 ly

A)5.2 au
B)4.3 pc
C)1 au
D)4.3 ly
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60
The Orion Nebula is shown in Figure 1-7 of Universe, 11th ed. How long has the light been traveling from this object before it arrives on Earth?
A)750 years
B)4890 years
C)460 years
D)1500 years

A)750 years
B)4890 years
C)460 years
D)1500 years
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61
The time taken for light to travel from Jupiter to Earth when they are closest to each other is (you need to think carefully about this, and draw a diagram):
A)12 years.
B)34 minutes.
C)8 minutes.
D)a few seconds.
A)12 years.
B)34 minutes.
C)8 minutes.
D)a few seconds.
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62
The Crab Nebula (See Figure 1-8 of Universe, 11th ed.) is the result of a supernova explosion of a star that occurred at a distance of about 1.99 kpc from Earth. If people on Earth saw the explosion in the year 1054 C.E., when did the explosion actually occur? 
A) 936 C.E.
B) about 1048 C.E.
C) about 5446 B.C.E.
D) 936 B.C.E.

A) 936 C.E.
B) about 1048 C.E.
C) about 5446 B.C.E.
D) 936 B.C.E.
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63
If a supernova was first seen in 1572 C.E. and its distance from Earth is measured to be 2 kpc, approximately when did the supernova actually explode?
A) 1572 B.C.E.
B) 4968 B.C.E.
C) 428 B.C.E.
D) 4968 C.E.
A) 1572 B.C.E.
B) 4968 B.C.E.
C) 428 B.C.E.
D) 4968 C.E.
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64
If a fire burned a large part of a medieval city 1000 years ago, approximately how far out in space has some of that light now reached? (Note to instructors: This question must be modified yearly.)
A)1000 × (3 × 108) m = 6.04 × 1011 m
B)1000 au
C)1000 ly
D)1000 pc
A)1000 × (3 × 108) m = 6.04 × 1011 m
B)1000 au
C)1000 ly
D)1000 pc
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65
Light from a campfire lit by Roman centurions in the year 100 B.C.E. travels out into space at the speed of light. Which is the farthest of the 20 brightest stars (See Appendix 5, Universe, 11th ed.) beyond which this light will now have traveled? 
A)Sirius
B)Rigel
C)Betelgeuse
D)Deneb

A)Sirius
B)Rigel
C)Betelgeuse
D)Deneb
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66
In 2018, an inhabitant of a planet orbiting a distant star observes the flash of the first nuclear explosion on Earth, which occurred in July 1945. Approximately how far away is his solar system from Earth?
A)73 pc
B)2.24 pc
C)224 pc
D)22.4 pc
A)73 pc
B)2.24 pc
C)224 pc
D)22.4 pc
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67
If an extraterrestrial being were to send a signal to Earth immediately to confirm the sighting in 2018 of a nuclear explosion on Earth in July 1945, and we were ready to receive such a message, when would we expect it? (Note to instructors: This question is linked to the previous question.)
A) 2032 C.E.
B) 2127 C.E.
C) 2016 C.E.
D) 2077 C.E.
A) 2032 C.E.
B) 2127 C.E.
C) 2016 C.E.
D) 2077 C.E.
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68
One yard is the same distance as:
A)0.9144 m.
B)1.0936 m.
C)100 cm
D)10-3 km.
A)0.9144 m.
B)1.0936 m.
C)100 cm
D)10-3 km.
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69
The following distance units, arranged in size from smallest to largest, are:
A)km, ly, au, pc.
B)ly, au, pc, km.
C)km, au, ly, pc.
D)au, pc, km, ly.
A)km, ly, au, pc.
B)ly, au, pc, km.
C)km, au, ly, pc.
D)au, pc, km, ly.
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70
The speed of light is approximately 3 × 108 m/sec. This is the same as:
A)1.34 × 108 mi/hr.
B)3.35 × 108 mi/hr.
C)4.41 × 108 mi/hr.
D)6.71 × 108 mi/hr.
A)1.34 × 108 mi/hr.
B)3.35 × 108 mi/hr.
C)4.41 × 108 mi/hr.
D)6.71 × 108 mi/hr.
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71
How long does it take light to travel from the Sun to Earth? (There are 3.15 x 107 seconds in 1 year.)
A)0.007 seconds
B)9 minutes
C)4 and a half days
D)11 weeks
A)0.007 seconds
B)9 minutes
C)4 and a half days
D)11 weeks
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72
How great a distance is 1 light second, the distance light travels in 1 second?
A)186,000 m
B)300 million m
C)1 au
D)1.76 pc
A)186,000 m
B)300 million m
C)1 au
D)1.76 pc
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73
An object on the surface of Earth has a mass of 40 kg. This is the same as:
A)4 × 104 g.
B)3.92 × 105 gs.
C)40 lb.
D)392 lb.
A)4 × 104 g.
B)3.92 × 105 gs.
C)40 lb.
D)392 lb.
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74
If the 40-kg object in the previous problem were taken to the surface of the Moon its mass would be:
A)4 × 104 g.
B)6.53 × 104 g.
C)40 lb.
D)65.3 lb.
A)4 × 104 g.
B)6.53 × 104 g.
C)40 lb.
D)65.3 lb.
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75
One foot is the same distance as:
A)3.048 × 10-7 μm.
B)3.048 × 108 nm.
C)0.621 km.
D)5.28 × 10-3 mi.
A)3.048 × 10-7 μm.
B)3.048 × 108 nm.
C)0.621 km.
D)5.28 × 10-3 mi.
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76
An underlying theme of astronomy is that the:
A)fundamental physical laws differ randomly from galaxy to galaxy, but they can be learned for a given galaxy by detailed observation.
B)fundamental physical laws governing the universe change in a predictable way with increasing distance from Earth.
C)universe is a hodgepodge of unrelated things behaving in arbitrary and unexplainable ways.
D)entire universe is governed by a single set of fundamental physical laws.
A)fundamental physical laws differ randomly from galaxy to galaxy, but they can be learned for a given galaxy by detailed observation.
B)fundamental physical laws governing the universe change in a predictable way with increasing distance from Earth.
C)universe is a hodgepodge of unrelated things behaving in arbitrary and unexplainable ways.
D)entire universe is governed by a single set of fundamental physical laws.
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77
We know the properties of hydrogen atoms well from studying them in laboratories on Earth. A fundamental idea in astronomy is that:
A)a hydrogen atom anywhere else in the universe is the same as it is here.
B)hydrogen atoms change in regular and predictable ways as they get farther from Earth.
C)the characteristics of hydrogen atoms follow different rules in different galaxies, but these can be predicted by studying the properties of each galaxy as a whole.
D)hydrogen atoms are unique to our solar system and the manner in which it was formed.
A)a hydrogen atom anywhere else in the universe is the same as it is here.
B)hydrogen atoms change in regular and predictable ways as they get farther from Earth.
C)the characteristics of hydrogen atoms follow different rules in different galaxies, but these can be predicted by studying the properties of each galaxy as a whole.
D)hydrogen atoms are unique to our solar system and the manner in which it was formed.
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78
The element helium was discovered (through spectroscopy) in the atmosphere of the Sun before it was discovered in trace amounts on Earth. This was possible because:
A)helium is the simplest element in its atomic structure.
B)the helium on Earth ultimately came from the Sun; thus we know the structure of solar helium must be the same as that of terrestrial helium.
C)all helium atoms in the universe are believed to be fundamentally the same.
D)both Earth and the Sun sweep up helium in their motion through space, so it is not surprising that the helium discovered on the Sun was the same as terrestrial helium.
A)helium is the simplest element in its atomic structure.
B)the helium on Earth ultimately came from the Sun; thus we know the structure of solar helium must be the same as that of terrestrial helium.
C)all helium atoms in the universe are believed to be fundamentally the same.
D)both Earth and the Sun sweep up helium in their motion through space, so it is not surprising that the helium discovered on the Sun was the same as terrestrial helium.
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