Deck 9: The Family of Stars
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Deck 9: The Family of Stars
1
Absolute visual magnitude is
A) the apparent magnitude of a star observed from Earth.
B) the luminosity of a star observed from a distance of 1000 pc.
C) the apparent magnitude of a star observed from a distance of 10 pc.
D) the luminosity of a star observed from Earth.
E) c and d
A) the apparent magnitude of a star observed from Earth.
B) the luminosity of a star observed from a distance of 1000 pc.
C) the apparent magnitude of a star observed from a distance of 10 pc.
D) the luminosity of a star observed from Earth.
E) c and d
the apparent magnitude of a star observed from a distance of 10 pc.
2
A star's absolute magnitude depends only on the star's
A) distance and diameter.
B) temperature and distance.
C) distance.
D) temperature and diameter.
E) apparent magnitude.
A) distance and diameter.
B) temperature and distance.
C) distance.
D) temperature and diameter.
E) apparent magnitude.
temperature and diameter.
3
Use the following chart to answer the questions below:
-Which star in Table 9-1 is most distant from Earth? Note that the distance may be calculated if it is not given explicitly.
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-1 is most distant from Earth? Note that the distance may be calculated if it is not given explicitly.
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
58 Ori
4
The distance to Rigel is 250 pc.Which of the following statements is true based on this information?
A) The distance to Rigel can be determined by measuring its parallax.
B) Rigel's apparent visual magnitude has a smaller value than its absolute visual magnitude.
C) The absolute bolometric magnitude of Rigel is nearly equal to its absolute visual magnitude.
D) Rigel is located in the upper right corner of the HR diagram.
E) none of the above
A) The distance to Rigel can be determined by measuring its parallax.
B) Rigel's apparent visual magnitude has a smaller value than its absolute visual magnitude.
C) The absolute bolometric magnitude of Rigel is nearly equal to its absolute visual magnitude.
D) Rigel is located in the upper right corner of the HR diagram.
E) none of the above
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5
If a star has a parallax of 0.02 seconds of arc,then its distance will be
A) 20 pc
B) 50 pc
C) 2 pc
D) 5 pc
E) 500 pc
A) 20 pc
B) 50 pc
C) 2 pc
D) 5 pc
E) 500 pc
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6
Use the following chart to answer the questions below:
-Which star in Table 9-1 is the closest to Earth? Note that the distance may be calculated if it is not given explicitly.
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-1 is the closest to Earth? Note that the distance may be calculated if it is not given explicitly.
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
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7
We can determine the surface temperature of a star
A) only by studying its continuous spectrum (color).
B) only by studying its line absorption spectrum.
C) Either "a" or 'b" will work but "b" is more precise
A) only by studying its continuous spectrum (color).
B) only by studying its line absorption spectrum.
C) Either "a" or 'b" will work but "b" is more precise
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8
If a star with an absolute magnitude of -5 has an apparent magnitude of +5,then its distance is
A) 1 pc.
B) 10 pc.
C) 100 pc.
D) 1000 pc.
E) 10,000 pc.
A) 1 pc.
B) 10 pc.
C) 100 pc.
D) 1000 pc.
E) 10,000 pc.
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9
Parallax would be easier to measure if
A) Earth's orbit was larger.
B) the stars were farther away.
C) Earth moved slower along its orbit.
D) all of these
E) none of these
A) Earth's orbit was larger.
B) the stars were farther away.
C) Earth moved slower along its orbit.
D) all of these
E) none of these
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10
Use the following chart to answer the questions below:
NARREND
-Which star in Table 9-2 would appear the faintest in the night sky?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-2 would appear the faintest in the night sky?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
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11
The ____ of a star is a measure of the total energy radiated by the star in one second.
A) absolute visual magnitude
B) apparent visual magnitude
C) luminosity class
D) spectral type
E) luminosity
A) absolute visual magnitude
B) apparent visual magnitude
C) luminosity class
D) spectral type
E) luminosity
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12
The absorption lines in the ultraviolet portion of the spectrum of a star that are produced by hydrogen are from the
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
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13
The absorption lines in the visible portion of the spectrum of a star that are produced by hydrogen are from the
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
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14
Use the following chart to answer the questions below:
Refer to Table 9-1.The star HR 4621 is
A) closer than 10 pc.
B) farther than 10 pc.
C) No way to tell.

Refer to Table 9-1.The star HR 4621 is
A) closer than 10 pc.
B) farther than 10 pc.
C) No way to tell.
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15
We know that giant stars are larger in diameter than the sun because
A) they are more luminous but have about the same temperature.
B) they are less luminous but have about the same temperature.
C) they are hotter but have about the same luminosity.
D) they are cooler but have about the same luminosity.
E) they have a larger absolute magnitude than the sun.
A) they are more luminous but have about the same temperature.
B) they are less luminous but have about the same temperature.
C) they are hotter but have about the same luminosity.
D) they are cooler but have about the same luminosity.
E) they have a larger absolute magnitude than the sun.
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16
Use the following chart to answer the questions below:
NARREND
-Which star in Table 9-2 has the greatest luminosity?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-2 has the greatest luminosity?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
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17
The absorption lines in the infrared portion of the spectrum of a star that are produced by hydrogen are from the
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
A) Lyman series.
B) Balmer series.
C) Paschen series.
D) isotopes of hydrogen.
E) ions of hydrogen.
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18
The correct sequence of spectral type letters from hot on the left to cool on the right is
A) M,K,G,F,A,B,O
B) O,B,A,F,G,K,M
C) G,K,M,F,O,B,A
D) A,B,O,F,G,K,M
A) M,K,G,F,A,B,O
B) O,B,A,F,G,K,M
C) G,K,M,F,O,B,A
D) A,B,O,F,G,K,M
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19
The star Sadir has an absolute magnitude of -5.3,and the absolute bolometric magnitude of the sun is +4.7.Based on this information,which of the following statements is true?
A) Sadir has a greater surface temperature than the sun.
B) Sadir has a larger diameter than the sun.
C) Sadir is 10,000 times more luminous than the sun.
D) Sadir is 100 parsecs from Earth.
E) all of the above
A) Sadir has a greater surface temperature than the sun.
B) Sadir has a larger diameter than the sun.
C) Sadir is 10,000 times more luminous than the sun.
D) Sadir is 100 parsecs from Earth.
E) all of the above
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20
The spectra of the coolest stars contain strong absorption features (or lines)of
A) TiO molecules
B) ionized helium
C) helium
D) hydrogen.
E) All of the above
A) TiO molecules
B) ionized helium
C) helium
D) hydrogen.
E) All of the above
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21
Sheat is an M2 II star.Based on this information,which of the following are true? 
A) I & II
B) II & IV
C) II,III,& IV
D) I,II,& III
E) I,II,III,& IV

A) I & II
B) II & IV
C) II,III,& IV
D) I,II,& III
E) I,II,III,& IV
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22
Binary (double)stars can be detected by
A) being seen as two separate stars with a telescope.
B) one star traveling a wiggly proper motion path across the sky.
C) one star dimming abruptly as another passes in front of it.
D) pairs of absorption lines seen in the spectrum of what appears to be one star.
E) all of the above
A) being seen as two separate stars with a telescope.
B) one star traveling a wiggly proper motion path across the sky.
C) one star dimming abruptly as another passes in front of it.
D) pairs of absorption lines seen in the spectrum of what appears to be one star.
E) all of the above
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23
Vega is an A0 V star.Based on this information which of the following are true? 
A) I & II
B) II & III
C) II,III,& IV
D) I,II,& III
E) I,II,III,& IV

A) I & II
B) II & III
C) II,III,& IV
D) I,II,& III
E) I,II,III,& IV
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24
NARRBEGIN: Diagram 09-01
Diagram 9-1
Use the following HR diagram to answer the questions below:
NARREND
Which star in Diagram 9-1 has the greatest surface temperature?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
Diagram 9-1
Use the following HR diagram to answer the questions below:

Which star in Diagram 9-1 has the greatest surface temperature?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
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25
In the H-R diagram,90 percent of all stars are
A) in the giant region.
B) in the supergiant region.
C) among the B stars.
D) among the G stars.
E) on the main sequence.
A) in the giant region.
B) in the supergiant region.
C) among the B stars.
D) among the G stars.
E) on the main sequence.
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26
The mass of a visual binary pair of stars can be obtained from
A) the time in years for them to orbit one another.
B) the size of their orbit.
C) their apparent magnitudes.
D) both a and b
A) the time in years for them to orbit one another.
B) the size of their orbit.
C) their apparent magnitudes.
D) both a and b
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27
Spectroscopic and eclipse duration observations of an eclipsing binary star can enable astronomers to calculate____ of its individual stars.
A) the masses
B) the sizes
C) both a and b
D) neither a nor b
A) the masses
B) the sizes
C) both a and b
D) neither a nor b
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28
Giant stars are 
A) I & II
B) II & IV
C) I,II,& IV
D) II,III,& IV
E) I,II,III,& IV

A) I & II
B) II & IV
C) I,II,& IV
D) II,III,& IV
E) I,II,III,& IV
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29
Compared with the spectral lines in the solar spectrum,lines in a supergiant spectrum are
A) sharper.
B) broader.
C) weaker.
D) stronger.
E) b and c
A) sharper.
B) broader.
C) weaker.
D) stronger.
E) b and c
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30
The best true sample of the true members of different stars consists of
A) stars that appear brightest in the sky to an observer on the Earth.
B) all of the stars within our solar system.
C) all the stars within a given distance from Earth.
A) stars that appear brightest in the sky to an observer on the Earth.
B) all of the stars within our solar system.
C) all the stars within a given distance from Earth.
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31
Doppler shift observations of a spectroscopic binary star can enable astronomers to calculate ____ of its individual stars.
A) the masses
B) the sizes
C) both a and b
D) neither a nor b
A) the masses
B) the sizes
C) both a and b
D) neither a nor b
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32
The hydrogen lines in spectral type A stars
A) are most narrow for supergiants.
B) are most narrow for main sequence stars.
C) cannot be used to estimate the luminosity of the star.
D) are very weak and difficult to see.
E) are useful in determining the apparent magnitude of the star.
A) are most narrow for supergiants.
B) are most narrow for main sequence stars.
C) cannot be used to estimate the luminosity of the star.
D) are very weak and difficult to see.
E) are useful in determining the apparent magnitude of the star.
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33
Use the following chart to answer the questions below:
-Which star in Table 9-3 has the greatest diameter?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-3 has the greatest diameter?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
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34
NARRBEGIN: Diagram 09-01
Diagram 9-1
Use the following HR diagram to answer the questions below:
NARREND
Which of the stars in Diagram 9-1 has the brightest absolute visual magnitude?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
Diagram 9-1
Use the following HR diagram to answer the questions below:

Which of the stars in Diagram 9-1 has the brightest absolute visual magnitude?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
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35
A pair of stars orbit around one another in an elliptical orbit with a semimajor axis,"a",of 1 AU with an orbital period,"P",of 1 year.What is the mass of the pair of stars?
A) m1 + m2 = a3 / P2 = 1 solar masses
B) m1 + m2 = a3 / P2 = 2 solar masses
C) m1 + m2 = a3 / P2 = 4 solar masses
D) m1 + m2 = a3 / P2 = 8 solar masses
E) m1 + m2 = a3 / P2 = 16 solar masses
A) m1 + m2 = a3 / P2 = 1 solar masses
B) m1 + m2 = a3 / P2 = 2 solar masses
C) m1 + m2 = a3 / P2 = 4 solar masses
D) m1 + m2 = a3 / P2 = 8 solar masses
E) m1 + m2 = a3 / P2 = 16 solar masses
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36
NARRBEGIN: Diagram 09-01
Diagram 9-1
Use the following HR diagram to answer the questions below:
NARREND
Which star in Diagram 9-1 above is most like the sun?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
Diagram 9-1
Use the following HR diagram to answer the questions below:

Which star in Diagram 9-1 above is most like the sun?
A) Alnilam
B) Antares
C) Arcturus
D) HR 5337
E) Sirius B
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37
Groombridge 34 is an M1 V star.Based on this information,which of the following are true? 
A) I & II
B) II & IV
C) I & IV
D) I & III
E) II & III

A) I & II
B) II & IV
C) I & IV
D) I & III
E) II & III
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38
In an H-R Diagram,stars with the smallest radius are found in the ____ of the diagram.
A) center
B) upper left corner
C) upper right corner
D) lower left corner
E) lower right corner
A) center
B) upper left corner
C) upper right corner
D) lower left corner
E) lower right corner
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39
Use the following chart to answer the questions below:
-Which star in Table 9-3 has the greatest surface temperature?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491

-Which star in Table 9-3 has the greatest surface temperature?
A) 65 Tau
B) HR 4621
C) ( Pic)
D) 58 Ori
E) HR 2491
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40
We know the white dwarf star Sirius B has a mass comparable to the Sun because of
A) its measured color
B) its measured temperature compared to Sirius A
C) it is part of binary star system with Sirius A.
A) its measured color
B) its measured temperature compared to Sirius A
C) it is part of binary star system with Sirius A.
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41
How can we tell that some stars are relatively close to us in the sky?
A) Some stars are occasionally eclipsed by the Moon,so they must be nearby.
B) Some stars vary in brightness caused by sunspots we can see because they are so close.
C) Some stars appear to be extremely bright and must therefore be very close to us.
D) Some stars appear to move periodically back and forth against the background stars because of the Earth's movement around the Sun
A) Some stars are occasionally eclipsed by the Moon,so they must be nearby.
B) Some stars vary in brightness caused by sunspots we can see because they are so close.
C) Some stars appear to be extremely bright and must therefore be very close to us.
D) Some stars appear to move periodically back and forth against the background stars because of the Earth's movement around the Sun
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42
Stars in the upper right part of the Hertzsprung-Russell diagram are always ____ when compared to stars near the middle of the diagram.
A) cooler
B) brighter as seen from Earth.
C) larger.
D) smaller.
E) more massive.
A) cooler
B) brighter as seen from Earth.
C) larger.
D) smaller.
E) more massive.
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43
If two stars are emitting the same amount of light,the star that is farther will appear
A) brighter.
B) dimmer.
C) redder.
D) bluer.
E) They will have the same brightness as seen from Earth.
A) brighter.
B) dimmer.
C) redder.
D) bluer.
E) They will have the same brightness as seen from Earth.
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44
Giant stars are members of luminosity class III.
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45
The most common stars are
A) supergiants.
B) giants.
C) upper main sequence stars.
D) white dwarfs.
E) lower main sequence stars.
A) supergiants.
B) giants.
C) upper main sequence stars.
D) white dwarfs.
E) lower main sequence stars.
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46
The most accurate way to determine the surface temperature of a star is to study
A) the pattern of absorption lines from various atoms.
B) the relative intensities of light measured through different photometric filters.
C) the peak wavelength of the star's continuum blackbody spectrum.
D) pattern of emission lines that are on the star's spectrum.
A) the pattern of absorption lines from various atoms.
B) the relative intensities of light measured through different photometric filters.
C) the peak wavelength of the star's continuum blackbody spectrum.
D) pattern of emission lines that are on the star's spectrum.
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47
Which stars always have large positive absolute magnitude?
A) Stars of high luminosity.
B) Stars of low luminosity.
C) Nearby stars.
D) Distant stars.
E) Not enough information given.
A) Stars of high luminosity.
B) Stars of low luminosity.
C) Nearby stars.
D) Distant stars.
E) Not enough information given.
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48
The two stars near one another on the sky,MizarA,are shown.Positions of one member areshown relative to the other star at different times.From plots like this one,astronomers concude that ... 
A) the stars are in an elliptical orbit around one another
B) the mass of the pair can be estimated
C) one star is passing by the other never to return
D) both A and B

A) the stars are in an elliptical orbit around one another
B) the mass of the pair can be estimated
C) one star is passing by the other never to return
D) both A and B
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49
In the list below,the least common stars are
A) upper main sequence stars.
B) white dwarfs.
C) lower main sequence stars.
A) upper main sequence stars.
B) white dwarfs.
C) lower main sequence stars.
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50
If you compare two stars,
A) the one with the larger radius will always have the greater luminosity.
B) the one with the higher surface temperature will always have the greater luminosity.
C) the one with the smaller absolute magnitude will always have the greater luminosity.
D) the one with the larger surface area has the greater energy flux from its surface.
A) the one with the larger radius will always have the greater luminosity.
B) the one with the higher surface temperature will always have the greater luminosity.
C) the one with the smaller absolute magnitude will always have the greater luminosity.
D) the one with the larger surface area has the greater energy flux from its surface.
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51
How is a luminosity class assigned to a star?
A) By combining the apparent magnitude with the star's parallax.
B) By measuring the period of variability in the star's apparent magnitude.
C) By studying the absorption lines in the spectrum of the star.
D) By observing the angular size of the star's image in a photograph or digital image.
A) By combining the apparent magnitude with the star's parallax.
B) By measuring the period of variability in the star's apparent magnitude.
C) By studying the absorption lines in the spectrum of the star.
D) By observing the angular size of the star's image in a photograph or digital image.
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52
The method of spectroscopic parallax cannot be applied to stars beyond about 100 pc.
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53
If a star is twice as hot as the sun and only half the sun's diameter,it will be less luminous than the sun.
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54
A star whose parallax is 0.01 seconds of arc is at a distance of 1,000 pc.
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55
The location of a star in the HR diagram indicates its temperature and intrinsic brightness.
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56
The absolute magnitude of a star is the apparent magnitude it would have if it were 10 pc from Earth.
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57
A star's apparent magnitude is a measure of ...
A) how bright it appears to us if it is at its actual distance.
B) how bright it appears to us at a standard distance of 10 pc.
C) its energy output per second compared to the sun.
D) its mass in solar masses.
E) its surface temperature in degrees Kelvin.
A) how bright it appears to us if it is at its actual distance.
B) how bright it appears to us at a standard distance of 10 pc.
C) its energy output per second compared to the sun.
D) its mass in solar masses.
E) its surface temperature in degrees Kelvin.
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58
Lines in the spectra of supergiant stars are broader than the same spectral lines in main sequence stars of the same spectral type.
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59
Which one of the methods below enables astronomers to measure the distance of a star near the sun in our galaxy?
A) sound echoes knowing the speed of sound and time
B) parallax using the earth's orbit
C) human binocular vision
D) Balmer series
E) none of the above
A) sound echoes knowing the speed of sound and time
B) parallax using the earth's orbit
C) human binocular vision
D) Balmer series
E) none of the above
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60
How do humans use their eyes to measure relative distance by parallax?
A) By continuously focusing our eyes on distant objects we can determine distance.
B) Since our eyes are separated the brain interprets the relative look angles of these eyes in terms of distance to the object viewed.
C) Our eyes can measure the time it takes light to travel from an object and from this we get distance.
D) By moving our heads from side to side our brain compares look angles from each of these positions to obtain the distance to the object viewed.
A) By continuously focusing our eyes on distant objects we can determine distance.
B) Since our eyes are separated the brain interprets the relative look angles of these eyes in terms of distance to the object viewed.
C) Our eyes can measure the time it takes light to travel from an object and from this we get distance.
D) By moving our heads from side to side our brain compares look angles from each of these positions to obtain the distance to the object viewed.
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61
The most common kinds of stars are low-luminosity stars.
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62
Stars of spectra type K have strong Balmer lines.
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63
The largest of the red stars are the ____________________ stars.
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64
Most stars on the H-R diagram are on the ____________________.
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65
An M star is hotter than an O star.
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66
Supergiants are about as common as the sun.
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67
____________________ can be used to determine the distance to a star when the spectrum of the star can be used to determine its spectral type and luminosity class.
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68
Hydrogen lines are weak in the spectra of hot stars because many of the hydrogen atoms have their electrons in levels above the second level.
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69
Luminosity class IV objects are known as ____________________.
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70
A G2 I star is ____________________ in diameter and ____________________ luminous than the sun.
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71
White dwarfs have such a low luminosity that even the nearest white dwarfs are not visible to the naked eye.
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72
On the HR diagram below,indicate the location of the white dwarf stars. 

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73
On the H-R diagram,lines of constant radius slants down from left to right.
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74
The Lyman series lines of hydrogen all lie in the infrared.
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75
The luminosity of a star is the total amount of energy it radiates each second.
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76
To observe a spectroscopic binary,we must be able to see both stars individually.
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