Deck 9: Measuring the Stars
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Deck 9: Measuring the Stars
1
Which of the following best describes the size and distance relationship of our Sun and the nearest 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 golf balls 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 golf balls separated by 300 kilometers
E) Two baseballs separated by 100 yards
Two golf balls separated by 300 kilometers
2
The nearest naked- eye star to our Sun, Alpha Centauri, is still over a parsec distant.
True
3
Hydrogen lines are weaker in both very hot and very cool stars.
True
4
For luminosity classification, fat stars have skinny spectral lines.
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5
On the main sequence, almost all stars have radii between about 0.1 and 10 times the Sun.
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6
Eclipsing binaries are the most useful, giving us sizes as well as masses of the pair.
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7
The proper motion of a star, its distance, and Doppler shift can give us its space velocity.
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8
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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9
The vast majority of stars near us would fall to the bottom right on the H-R diagram.
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10
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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11
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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12
A type B9 star is hotter than a type A0.
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13
The proper motion of a star is its true velocity through space.
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14
A star of the Sun's diameter, but twice as hot, must be 16X more luminous than the Sun.
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15
First magnitude Spica appears 2.5 times brighter than second magnitude Polaris.
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16
If a star were moved 10 times farther away, its absolute magnitude would drop five magnitudes.
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17
A nearby star has a parallax of 0.2 arc seconds. What is its distance?
A) 0.1 parsec
B) 0.2 parsec
C) 0.5 parsec
D) 5 parsecs
E) 50 parsecs
A) 0.1 parsec
B) 0.2 parsec
C) 0.5 parsec
D) 5 parsecs
E) 50 parsecs
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18
In a spectroscopic binary, the star whose lines shift the most weighs the most.
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19
If a star were moved 10 times farther away, its apparent magnitude would drop by five magnitudes.
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20
In a binary system, the more massive stars always stay closer to the center of mass and move slower.
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21
Star A has an absolute magnitude of 2.5 and star B has an apparent magnitude of 2.5, but star A 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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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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22
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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23
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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24
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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25
Star A and star B both have an absolute magnitude of 2.0, but star A has an apparent magnitude 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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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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26
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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27
Star A and star B both have an apparent magnitude of 4.0, but star A has an absolute magnitude 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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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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28
If a star is found by spectroscopic observations to be about 500 parsecs distant, its parallax is
A) 0.2".
B) 0.5".
C) 0.02".
D) 0.002".
E) 0.005".
A) 0.2".
B) 0.5".
C) 0.02".
D) 0.002".
E) 0.005".
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29
At the distance of Jupiter (6 times further away from the Sun than Earth) the amount of sunlight received per square centimeter 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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30
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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31
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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32
If a star appears to move back and forth relative to other stars over a six-month period, this motion 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
Roughly how many stars are within 4 parsecs of the solar system?
A) 3
B) 30
C) 3000
D) 300,000
E) 200 billion
A) 3
B) 30
C) 3000
D) 300,000
E) 200 billion
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34
If a star appears to move relative to other stars over a one-year period, this motion 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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35
Star A is a main sequence star of spectral type G5 and star B is a red giant of spectral type K2. 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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36
Star A and star B both have an apparent magnitude of 7.0, but star A is at a distance of 15 pc and star B is at a distance of 30 pc. Which statement below is correct?
A) Star A appears brighter than star B, but star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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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37
Star A is a main sequence star of spectral type F2 and star B is a white dwarf of spectral type B4. 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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38
Star A and star B both have an absolute magnitude of 2.0, but star A is at a distance of 50 pc and star B is at a distance of 20 pc. Which statement below is correct?
A) Star A appears brighter than star B, but star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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 star B and star A have the same intrinsic brightness.
B) Star B appears brighter than star A, but star B and star A have the same intrinsic brightness.
C) Star A and star B appear to have the same brightness, but star B is intrinsically brighter than star A.
D) Star A and star B appear to have the same brightness, but star A is intrinsically brighter than star B.
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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39
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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40
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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41
Compared to the size of the Sun, in what range of sizes are nearly all stars found?
A) 0.5 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) 0.5 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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42
How might the most common occurring stars be described, based on our stellar neighborhood?
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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43
In a spectroscopic binary system, the star showing the larger blue shift 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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44
On the H-R diagram, red supergiants like Betelgeuse 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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45
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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46
Two red stars have surface temperatures of 3000 K, but Star A's luminosity is about 5% of the Sun's and Star B's luminosity is about 32,000 times the luminosity of the Sun. How much bigger 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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47
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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48
A star with a parallax of 1 second of arc is at a distance of ________ by definition.
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49
On the H-R diagram, white dwarfs lie 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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50
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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51
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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52
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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53
In a spectroscopic binary, if a pair shows a combined set of lines tonight, but a maximum split 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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54
In what range of masses are most stars found?
A) 0.1 to 2 solar masses
B) 1 to 3 solar masses
C) 0.1 to 100 solar masses
D) 0.01 to 100 solar masses
E) Stars can have any mass.
A) 0.1 to 2 solar masses
B) 1 to 3 solar masses
C) 0.1 to 100 solar masses
D) 0.01 to 100 solar masses
E) Stars can have any mass.
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55
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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56
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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57
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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58
In a visual binary system with circular orbits, if in 20 years the two stars' position angles have 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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59
Having nothing to do with trigonometry, ________ parallaxes use the width of absorption lines 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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60
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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61
Knowledge of a star's temperature and ________ enables us to calculate its radius, surface area, and volume from the appropriate radiation law.
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62
Why must both parallax and proper motion be known to give transverse velocity?
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63
How is distance determined to the nearest stars? How far out can this technique be applied? How many stars can be measured in this way?
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64
On the main sequence on an H-R diagram, our Sun lies at about ________.
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65
All classes of binary stars yield the basic information on stellar ________.
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66
The apparent magnitude of the Sun is -26, while Sirius has an apparent magnitude of -1; how much brighter does the Sun appear than Sirius?
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67
What types of observations are necessary to determine the motion of a star through space?
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68
In an eclipsing binary, the longer the stages of the eclipse take, the ________ the star.
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69
How is proper motion measured?
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70
On the H-R diagram, most bright naked eye stars would lie at the ________.
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71
From hottest to coolest, the seven letters for the star types are ________.
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72
The ________ magnitude of a star depends directly upon its luminosity and distance.
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73
How can a white dwarf be hotter than our Sun, yet much less luminous?
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74
Capella is the same temperature as our Sun, but about ten times the Sun's diameter; it must be about ________ times as luminous as our star.
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75
Contrast main sequence stars of type B and G.
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76
What is proper motion? How is it related to transverse velocity?
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77
Why is the main sequence main? Why are these stars so common?
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78
If two stars are the same size and one is twice the temperature of the other, how much more luminous is the hotter one?
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79
What role does hydrogen play in spectral classification?
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80
A star's motion across the sky is its ________ motion.
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