Deck 17: The Stars: Giants, Dwarfs, and the Main Sequence
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ملء الشاشة (f)
Deck 17: The Stars: Giants, Dwarfs, and the Main Sequence
1
The Hipparcos mission's data on parallaxes is useful for stellar distances out to about 200 pc.
True
2
On the main sequence, almost all stars have radii between about 0.1 and 10 times the Sun.
True
3
First magnitude Spica appears 2.5 times brighter than second magnitude Polaris.
True
4
The proper motion of a star, its distance, and Doppler shift can give us its space velocity.
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5
About 500 stars can be seen by the naked eye from somewhere on Earth.
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6
Like the Sun, main sequence stars are converting hydrogen into helium in their cores.
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7
In a binary system, the more massive stars always stay closer to the center of mass and moveslower.
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8
For luminosity classification, fat stars have skinny spectral lines.
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9
The vast majority of stars near us would fall to the bottom right on the H-R diagram.
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10
The proper motion of a star is its true velocity through space.
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11
If a star were moved 10 times farther away, its apparent magnitude would drop by fivemagnitudes.
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12
The nearest naked-eye star to our Sun, Alpha Centauri, is still over a parsec distant.
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13
The Sun's complete classification is
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14
If a star were moved 10 times farther away, its absolute magnitude would drop fivemagnitudes.
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15
A star of the Sun's diameter, but twice as hot, must be 16X more luminous than the Sun.
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16
In a spectroscopic binary, the star whose lines shift the most weighs the most.
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17
Hydrogen lines are weaker in both very hot and very cool stars.
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18
Star A and star B have the same apparent magnitude. Star A is twice as distant as star B.Therefore, star A has twice the luminosity as star B.
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19
A type B9 star is hotter than a type A0.
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20
Eclipsing binaries are the most useful, giving us sizes as well as masses of the pair.
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21
If a star is found by spectroscopic observations to be about 500 parsecs distant, its parallax is:
A).2".
B).5".
C).02".
D).002".
E).005".
A).2".
B).5".
C).02".
D).002".
E).005".
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22
If a star has a parallax of 0.05", then its distance in light-years is about:
A)6.4 light-years.
B)12.7 light-years.
C)20 light-years.
D)65 light-years.
E)100 light-years.
A)6.4 light-years.
B)12.7 light-years.
C)20 light-years.
D)65 light-years.
E)100 light-years.
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23
Which statement about stellar motion is incorrect?
A)In general, the closer a star is, the more its proper motion.
B)The radial velocity is measured by the Doppler shift.
C)The transverse velocity is measured by the proper motion and the distance.
D)Like parallax, proper motion is measured over intervals of exactly six months.
E)The Pythagorean theorem relates space, transverse, and radial velocities.
A)In general, the closer a star is, the more its proper motion.
B)The radial velocity is measured by the Doppler shift.
C)The transverse velocity is measured by the proper motion and the distance.
D)Like parallax, proper motion is measured over intervals of exactly six months.
E)The Pythagorean theorem relates space, transverse, and radial velocities.
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24
About how many stars has the Hipparcos mission given us accurate distance data on?
A)about 3,000, about half of what you can see with the naked eye alone
B)over 6000, the visible naked eye stars and some seen in binoculars
C)60,000, those within about 100 light-years of us
D)a million, those with parallaxes of .005" or larger
E)over 100 billion, almost every star in the galaxy
A)about 3,000, about half of what you can see with the naked eye alone
B)over 6000, the visible naked eye stars and some seen in binoculars
C)60,000, those within about 100 light-years of us
D)a million, those with parallaxes of .005" or larger
E)over 100 billion, almost every star in the galaxy
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25
The ESA's GAIA project will be able to measure parallax and stellar properties of about howmany stars?
A)one million
B)ten thousand
C)one billion
D)one hundred billion
E)None; it has a different purpose.
A)one million
B)ten thousand
C)one billion
D)one hundred billion
E)None; it has a different purpose.
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26
Procyon lies about 13 light-years distant, thus its parallax is about:
A)0.01".
B)0.25".
C)0.40".
D)0.65".
E)1.3".
A)0.01".
B)0.25".
C)0.40".
D)0.65".
E)1.3".
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27
A nearby star has a parallax of 0.2 arc seconds. What is its distance?
A).1 parsec
B).2 parsec
C).5 parsec
D)5 parsecs
E)50 parsecs
A).1 parsec
B).2 parsec
C).5 parsec
D)5 parsecs
E)50 parsecs
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28
Which of the following best describes the size and distance relationship of our Sun and thenearest star?
A)a tennis ball here, another on the Moon
B)two beach balls separated by 100 city blocks
C)two grains of sand separated by 100 light-years
D)two marbles separated by 300 kilometers
E)two baseballs separated by 100 yards
A)a tennis ball here, another on the Moon
B)two beach balls separated by 100 city blocks
C)two grains of sand separated by 100 light-years
D)two marbles separated by 300 kilometers
E)two baseballs separated by 100 yards
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29
About how many stars can be seen from somewhere on Earth with the naked eye?
A)600
B)6,000
C)600,000
D)6,000,000
E)uncountably many
A)600
B)6,000
C)600,000
D)6,000,000
E)uncountably many
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30
If a star appears to move relative to other stars over a one-year period, this motion is due tothe star's
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
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31
The absolute magnitude of a star is its brightness as seen from a distance of:
A)one million kilometers.
B)one astronomical unit.
C)one light-year.
D)ten parsecs.
E)10 light-years.
A)one million kilometers.
B)one astronomical unit.
C)one light-year.
D)ten parsecs.
E)10 light-years.
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32
If a star appears to move back and forth relative to other stars over a six-month period, thismotion is due to the star's:
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
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33
High mass stars provide most of the mass and most of the light in galaxies.
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34
The Hipparcos mission's observations have given us good data on stars out to about:
A)100 light-years.
B)200 light-years.
C)200 parsecs.
D)1000 light-years.
E)1000 parsecs.
A)100 light-years.
B)200 light-years.
C)200 parsecs.
D)1000 light-years.
E)1000 parsecs.
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35
What is the absolute magnitude of our Sun?
A)-23.0
B)-4.6
C)-1.4
D)+4.8
E)+9.4
A)-23.0
B)-4.6
C)-1.4
D)+4.8
E)+9.4
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36
In order to turn a star's proper motion into its space velocity, we must also know:
A)its mass and spectral type.
B)its temperature and age.
C)its distance and radial velocity.
D)its distance and mass.
E)its spectral type and period of rotation.
A)its mass and spectral type.
B)its temperature and age.
C)its distance and radial velocity.
D)its distance and mass.
E)its spectral type and period of rotation.
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37
A star of ten solar masses would probably stay stable on the main sequence only about1/1000th as long as our Sun.
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38
The motion of a star towards or away from us is called its:
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
A)transverse motion.
B)radial motion.
C)parallax shift.
D)Doppler shift.
E)true space motion.
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39
Gaia will be able to measure which two apparent motions of stars?
A)transverse and radial
B)parallax and transverse
C)radial and parallax
D)parallax and orbital
E)orbital and radial
A)transverse and radial
B)parallax and transverse
C)radial and parallax
D)parallax and orbital
E)orbital and radial
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40
What is proper motion?
A)It is the true, not apparent, motion of a star in space.
B)It is the apparent shift as we go to opposite sides of our orbit every six months.
C)It is the annual apparent motion of a star across the sky.
D)It is the motion of a star towards or away from us, revealed by Doppler shifts.
E)It is the orbital motion of a star around the Galaxy.
A)It is the true, not apparent, motion of a star in space.
B)It is the apparent shift as we go to opposite sides of our orbit every six months.
C)It is the annual apparent motion of a star across the sky.
D)It is the motion of a star towards or away from us, revealed by Doppler shifts.
E)It is the orbital motion of a star around the Galaxy.
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41
On the H-R diagram, the Sun lies:
A)at the top left.
B)at the bottom left.
C)at the bottom right.
D)about the middle of the main sequence.
E)at the top right.
A)at the top left.
B)at the bottom left.
C)at the bottom right.
D)about the middle of the main sequence.
E)at the top right.
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42
Star A and star B both have an absolute magnitude of 2.0, but star A has an apparentmagnitude of 5.0 and star B has an apparent magnitude of 7.0. Which statement below is correct?
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
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43
At the distance of Jupiter (6 times further away from the Sun than Earth)the amount ofsunlight received per square centimeter is different by what factor?
A)6 times less
B)12 times less
C)36 times less
D)6 times more
E)12 times more
A)6 times less
B)12 times less
C)36 times less
D)6 times more
E)12 times more
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44
What physical property of a star does the spectral type measure?
A)density
B)luminosity
C)temperature
D)mass
E)composition
A)density
B)luminosity
C)temperature
D)mass
E)composition
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45
Star A is a main sequence star of spectral type ad star B is a white dwarf of spectral typeB4. Which statement below is correct?
A)Star A appears brighter than star B.
B)Star B appears brighter than star A.
C)Star A is hotter than star B.
D)Star B is hotter than star A.
E)None of the above can be said about these two stars.
A)Star A appears brighter than star B.
B)Star B appears brighter than star A.
C)Star A is hotter than star B.
D)Star B is hotter than star A.
E)None of the above can be said about these two stars.
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46
The Hertzsprung-Russell Diagram plots ________ against the spectral type or temperature.
A)distance
B)luminosity or absolute magnitude
C)brightness or apparent magnitude
D)size or density
E)mass
A)distance
B)luminosity or absolute magnitude
C)brightness or apparent magnitude
D)size or density
E)mass
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47
The most famous G type star is:
A)Polaris.
B)Betelguese.
C)Sirius.
D)the Sun.
E)Pollux.
A)Polaris.
B)Betelguese.
C)Sirius.
D)the Sun.
E)Pollux.
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48
Star A is a main sequence star of spectral type G5 and star B is a red giant of spectral typeK2. Which statement below is correct?
A)Star A appears brighter than star B.
B)Star B appears brighter than star A.
C)Star A is hotter than star B.
D)Star B is hotter than star A.
E)None of the above can be said about these two stars.
A)Star A appears brighter than star B.
B)Star B appears brighter than star A.
C)Star A is hotter than star B.
D)Star B is hotter than star A.
E)None of the above can be said about these two stars.
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49
Perhaps the greatest of the Greek astronomers, ________ compiled the first catalog of stars,accurately measured their positions, and defined the basic system of stellar brightnesses.
A)Erastothenes
B)Aristotle
C)Ptolemy
D)Hipparchus
E)Aristarchus
A)Erastothenes
B)Aristotle
C)Ptolemy
D)Hipparchus
E)Aristarchus
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50
Two red stars have surface temperatures of 3000 K, but Star A's luminosity is about 5% ofthe Sun's and Star B's luminosity is about 32,000 times the luminosity of the Sun. How muchbigger is star B than star A?
A)They are the same size.
B)Star B's radius is about 16 times larger than star A's radius.
C)Star B's radius is about 800 times larger than star A's radius.
D)Star B's radius is about 640,000 times larger than star A's radius.
E)This cannot be determined from the information given.
A)They are the same size.
B)Star B's radius is about 16 times larger than star A's radius.
C)Star B's radius is about 800 times larger than star A's radius.
D)Star B's radius is about 640,000 times larger than star A's radius.
E)This cannot be determined from the information given.
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51
Star A and star B both have an apparent magnitude of 4.0, but star A has an absolutemagnitude of 1.0 and star B has an absolute magnitude of 7.0. Which statement below is correct?
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
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52
Which of the following is the most common type of star?
A)high mass main sequence
B)low mass main sequence
C)white dwarfs
D)red giants
E)blue supergiants
A)high mass main sequence
B)low mass main sequence
C)white dwarfs
D)red giants
E)blue supergiants
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53
Star A has an absolute magnitude of 2.5 and star B has an apparent magnitude of 2.5, but starA is a main sequence star and star B is a red giant. Which statement below is correct?
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
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54
Star A and star B both have an absolute magnitude of 2.0, but star A is at a distance of 50 pcand star B is at a distance of 20 pc. Which statement below is correct?
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
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55
Compared to the size of the Sun, in what range of sizes are nearly all stars found?
A).5 to 2 solar radii
B)0.1 to 1.0 solar radii
C)0.5 to 50 solar radii
D)1 to 100 solar radii
E)0.01 to 100 solar radii
A).5 to 2 solar radii
B)0.1 to 1.0 solar radii
C)0.5 to 50 solar radii
D)1 to 100 solar radii
E)0.01 to 100 solar radii
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56
Star A and star B both have an apparent magnitude of 7.0, but star A is at a distance of 15 pcand star B is at a distance of 30 pc. Which statement below is correct?
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
A)Star A appears brighter than star B, but actually star B and star A are the same brightness.
B)Star B appears brighter than star A, but actually star B and star A are the same brightness.
C)Star A and star B appear to have the same brightness, but actually star B is brighter than starA.
D)Star A and star B appear to have the same brightness, but actually star A is brighter than starB.
E)It is impossible to determine how bright these stars are or appear to be relative to one another,given the information above.
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57
In comparing first magnitude Deneb with second magnitude Polaris, we find that:
A)Polaris is in reality much more luminous.
B)Deneb must be much hotter than Polaris.
C)Deneb appears 2.5 times brighter to us than does Polaris.
D)Polaris is really 100 times brighter than nearby Deneb.
E)Deneb is really much closer than Polaris.
A)Polaris is in reality much more luminous.
B)Deneb must be much hotter than Polaris.
C)Deneb appears 2.5 times brighter to us than does Polaris.
D)Polaris is really 100 times brighter than nearby Deneb.
E)Deneb is really much closer than Polaris.
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58
Stars that have masses similar to the Sun's, and sizes similar to the Earth are:
A)main sequence stars.
B)white dwarfs.
C)red giants.
D)red dwarfs.
E)brown dwarfs.
A)main sequence stars.
B)white dwarfs.
C)red giants.
D)red dwarfs.
E)brown dwarfs.
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59
What are the two most important intrinsic properties used to classify stars?
A)mass and age
B)luminosity and surface temperature
C)distance and luminosity
D)distance and surface temperature
E)distance and color
A)mass and age
B)luminosity and surface temperature
C)distance and luminosity
D)distance and surface temperature
E)distance and color
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60
The star's color index is a quick way of determining its:
A)density.
B)luminosity.
C)mass.
D)temperature.
E)composition.
A)density.
B)luminosity.
C)mass.
D)temperature.
E)composition.
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61
In what range of masses are most stars found?
A).1 to 2 solar masses
B)1 to 3 solar masses
C).1 to 100 solar masses
D).01 to 100 solar masses
E)Stars can have any mass.
A).1 to 2 solar masses
B)1 to 3 solar masses
C).1 to 100 solar masses
D).01 to 100 solar masses
E)Stars can have any mass.
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62
In a visual binary system with circular orbits, if in 20 years the two stars' position angleshave shifted by 30 degrees, the pair's period must be:
A)60 years.
B)90 years.
C)120 years.
D)240 years.
E)360 years.
A)60 years.
B)90 years.
C)120 years.
D)240 years.
E)360 years.
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63
In eclipsing binaries, in contrast to spectroscopic binaries, we can also determine a star's:
A)temperature.
B)color.
C)speed.
D)shape.
E)radius.
A)temperature.
B)color.
C)speed.
D)shape.
E)radius.
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64
In the H-R diagram, the bright blue-white stars that dominate the naked eye sky lie to the:
A)top left.
B)top right.
C)middle of the main sequence.
D)top center.
E)bottom left.
A)top left.
B)top right.
C)middle of the main sequence.
D)top center.
E)bottom left.
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65
Eclipsing binaries are less common than spectroscopic binaries because:
A)their orbital planes must be nearly edge on from our perspective.
B)their orbital planes must be nearly face on from our perspective.
C)both stars must have the same mass.
D)both stars must have the same diameter.
E)both stars must be spectral type O or B.
A)their orbital planes must be nearly edge on from our perspective.
B)their orbital planes must be nearly face on from our perspective.
C)both stars must have the same mass.
D)both stars must have the same diameter.
E)both stars must be spectral type O or B.
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66
On the H-R diagram, red supergiants like Betelguese lie:
A)at the bottom left.
B)at the bottom right.
C)at the top left.
D)at the top right.
E)They can't be plotted, for they are not main sequence.
A)at the bottom left.
B)at the bottom right.
C)at the top left.
D)at the top right.
E)They can't be plotted, for they are not main sequence.
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67
In a spectroscopic binary system, the star showing the larger blueshift is:
A)cooler and receding the fastest.
B)less massive of the pair and receding slower.
C)more massive and approaching us.
D)less massive and approaching us at this moment.
E)hotter and receding faster.
A)cooler and receding the fastest.
B)less massive of the pair and receding slower.
C)more massive and approaching us.
D)less massive and approaching us at this moment.
E)hotter and receding faster.
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68
On the H-R diagram, white dwarfs like Sirius B and Procyon B lie:
A)at the top left.
B)at the top right.
C)close to the Sun, near the center.
D)at the lower left.
E)at the lower right.
A)at the top left.
B)at the top right.
C)close to the Sun, near the center.
D)at the lower left.
E)at the lower right.
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69
For a star of 10 solar masses, its main sequence life span will be:
A)ten times longer than our Sun's.
B)about the same as the Sun's.
C)only a tenth of the Sun's.
D)about a hundred times less than the Sun's.
E)only 1/1000th of the Sun.
A)ten times longer than our Sun's.
B)about the same as the Sun's.
C)only a tenth of the Sun's.
D)about a hundred times less than the Sun's.
E)only 1/1000th of the Sun.
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70
Having nothing to do with trigonometry, ________ parallaxes use the width of absorptionlines to estimate the star's luminosity and size and distance.
A)bolometric
B)photometric
C)spectroscopic
D)holographic
E)videometric
A)bolometric
B)photometric
C)spectroscopic
D)holographic
E)videometric
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71
In a spectroscopic binary, if a pair shows a combined set of lines tonight, but a maximumsplit two nights later, its orbital period must be:
A)one day.
B)two days.
C)four days.
D)eight days.
E)twelve days.
A)one day.
B)two days.
C)four days.
D)eight days.
E)twelve days.
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72
What is the typical main sequence lifetime of a G-type star?
A)10 million years
B)100 million years
C)1 billion years
D)10 billion years
E)100 billion years
A)10 million years
B)100 million years
C)1 billion years
D)10 billion years
E)100 billion years
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73
High mass stars account for most of the ________ in large regions of star formation, such asgalaxies.
A)mass
B)stars
C)planetary nebulae
D)light
A)mass
B)stars
C)planetary nebulae
D)light
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74
In general, the narrower the spectral line of a star:
A)the hotter the star is.
B)the bigger the star is.
C)the denser the star is.
D)the smaller the star is.
E)the cooler the star is.
A)the hotter the star is.
B)the bigger the star is.
C)the denser the star is.
D)the smaller the star is.
E)the cooler the star is.
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75
How might the most common occurring stars be described, based on our stellarneighborhood?
A)white dwarfs
B)K giants
C)G main sequence
D)A main sequence
E)M main sequence
A)white dwarfs
B)K giants
C)G main sequence
D)A main sequence
E)M main sequence
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76
What is the typical main sequence lifetime of an M-type star?
A)one million years
B)ten million years
C)one billion years
D)ten billion years
E)a trillion years
A)one million years
B)ten million years
C)one billion years
D)ten billion years
E)a trillion years
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77
Which type of binary can have their sizes measured directly by photometry?
A)virtual
B)visual
C)eclipsing
D)spectroscopic
E)astrometric
A)virtual
B)visual
C)eclipsing
D)spectroscopic
E)astrometric
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78
What is the typical main sequence lifetime of a B-type star?
A)less than a million years
B)20 million years
C)100 million years
D)1 billion years
E)10 billion years
A)less than a million years
B)20 million years
C)100 million years
D)1 billion years
E)10 billion years
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79
Upon what data do measurements of sizes of eclipsing binaries depend?
A)their orbital periods and separations
B)their masses and luminosities
C)their Doppler shifts and durations of stages of their eclipses
D)their temperatures and speeds
E)their temperatures and masses
A)their orbital periods and separations
B)their masses and luminosities
C)their Doppler shifts and durations of stages of their eclipses
D)their temperatures and speeds
E)their temperatures and masses
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80
What is the single most important characteristic in determining the course of a star'sevolution?
A)density
B)absolute brightness
C)distance
D)surface temperature
E)mass
A)density
B)absolute brightness
C)distance
D)surface temperature
E)mass
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