Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t...

144
Quizbank/Astronomy Quiz From Wikiversity Contents 1 Cover page 1.1 AstroSizeWhitdwrfNeutstarQSOv1s1 1.1.1 Key to AstroSizeWhitdwrfNeutstarQSOv1s1 1.2 AstroSizeWhitdwrfNeutstarQSOv2s1 1.2.1 Key to AstroSizeWhitdwrfNeutstarQSOv2s1 1.3 AstroSizeWhitdwrfNeutstarQSOv1s2 1.3.1 Key to AstroSizeWhitdwrfNeutstarQSOv1s2 1.4 AstroSizeWhitdwrfNeutstarQSOv2s2 1.4.1 Key to AstroSizeWhitdwrfNeutstarQSOv2s2 1.5 AstroSizeWhitdwrfNeutstarQSOv1s3 1.5.1 Key to AstroSizeWhitdwrfNeutstarQSOv1s3 1.6 AstroSizeWhitdwrfNeutstarQSOv2s3 1.6.1 Key to AstroSizeWhitdwrfNeutstarQSOv2s3 1.7 AstroSizeWhitdwrfNeutstarQSOv1s4 1.7.1 Key to AstroSizeWhitdwrfNeutstarQSOv1s4 1.8 AstroSizeWhitdwrfNeutstarQSOv2s4 1.8.1 Key to AstroSizeWhitdwrfNeutstarQSOv2s4 1.9 AstroSizeWhitdwrfNeutstarQSOv1s5 1.9.1 Key to AstroSizeWhitdwrfNeutstarQSOv1s5 1.10 AstroSizeWhitdwrfNeutstarQSOv2s5 1.10.1 Key to AstroSizeWhitdwrfNeutstarQSOv2s5 Cover page This document contains 10 identical exams, paired into versions v1 and v2. If two exams have the same snumber, then v1 and v2 have the same questions, but full randomized (order and answers) Different snumbers have different questions, chosen randomly from the same bank. While permalinks are immune to capricious editing and vandalism, this pdf file can be replaced at any time. Therefore, one of the following two precautions should be taken: 1. Verify the identity the last known editor before downloading this pdf file to your personal computer. 2. An alternative is to download this not from Wikiversity but from a trusted mirror source. At the end of this document Attribution for the quizzes identifies where the questions were obtained Study guide' links reading materials and/or relevant equations.

Transcript of Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t...

Page 1: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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Quizbank/Astronomy QuizFrom Wikiversity

Contents

1 Cover page1.1 AstroSizeWhitdwrfNeutstarQSO­v1s1

1.1.1 Key to AstroSizeWhitdwrfNeutstarQSO­v1s11.2 AstroSizeWhitdwrfNeutstarQSO­v2s1

1.2.1 Key to AstroSizeWhitdwrfNeutstarQSO­v2s11.3 AstroSizeWhitdwrfNeutstarQSO­v1s2

1.3.1 Key to AstroSizeWhitdwrfNeutstarQSO­v1s21.4 AstroSizeWhitdwrfNeutstarQSO­v2s2

1.4.1 Key to AstroSizeWhitdwrfNeutstarQSO­v2s21.5 AstroSizeWhitdwrfNeutstarQSO­v1s3

1.5.1 Key to AstroSizeWhitdwrfNeutstarQSO­v1s31.6 AstroSizeWhitdwrfNeutstarQSO­v2s3

1.6.1 Key to AstroSizeWhitdwrfNeutstarQSO­v2s31.7 AstroSizeWhitdwrfNeutstarQSO­v1s4

1.7.1 Key to AstroSizeWhitdwrfNeutstarQSO­v1s41.8 AstroSizeWhitdwrfNeutstarQSO­v2s4

1.8.1 Key to AstroSizeWhitdwrfNeutstarQSO­v2s41.9 AstroSizeWhitdwrfNeutstarQSO­v1s5

1.9.1 Key to AstroSizeWhitdwrfNeutstarQSO­v1s51.10 AstroSizeWhitdwrfNeutstarQSO­v2s5

1.10.1 Key to AstroSizeWhitdwrfNeutstarQSO­v2s5

Cover page

This document contains 10 identical exams, paired into versions v1 and v2. If two exams have the same s­number,then v1 and v2 have the same questions, but full randomized (order and answers) Different s­numbers havedifferent questions, chosen randomly from the same bank.

While permalinks are immune to capricious editing and vandalism, this pdf file can be replaced at any time.Therefore, one of the following two precautions should be taken:

1. Verify the identity the last known editor before downloading this pdf file to your personal computer.2. An alternative is to download this not from Wikiversity but from a trusted mirror source.

At the end of this documentAttribution for the quizzes identifies where the questions were obtainedStudy guide' links reading materials and/or relevant equations.

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AstroSizeWhitdwrfNeutstarQSO­v1s1

1. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting to count asteroids

___ b) Attempting one of the first star charts

___ c) Looking for a comet that he knew would be appearing in that part of the sky.

___ d) Trying to measure the orbital radius of a planet

___ e) Looking for lobsters

2. What causes the blue glow of the Crab nebula?

___ a) the same emission found in a Lava lamp (ultra­violet)

___ b) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ c) the Gravitational blue shift

___ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ e) the Doppler blue shift

3. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) temperature­luminosity...redshift...quantum­theory­of­solids

___ b) doppler­shift...period­of­pulsation...temperature­luminosity

___ c) HR­diagram­location...X­ray­emmision...spectral­lines

___ d) all of these are true

___ e) x­ray­emmission...doppler­shift...rotation­rate

Page 3: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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4. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

5. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 4 cm (just like yours).

___ b) expansion from 1 cm to 2 cm (half of yours)

___ c) expansion from 1 cm to 3 cm (since 3­1=2)

___ d) expansion from 1 cm to 8 cm (twice yours).

___ e) expansion from 1 cm to 9 cm (since 5­1=4)

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6. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 25%

___ b) 10%

___ c) 100%

___ d) 0.1%

___ e) 1%

7. This light clock is associated with

___ a) general relativity

___ b) doppler shift

___ c) special relativity

___ d) all of these are true

___ e) gravitational shift

8. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 2

___ b) 8

___ c) 4

___ d) 3

___ e) 6

9. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) Cepheid variables

___ b) entire galaxies

___ c) red giants

___ d) novae

___ e) supernovae

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10. At the center of the Crab nebula is

___ a)d) a neutron star

___ b)e) the remnants of a supernova

___ c)b) a pulsar

___ d)c) none of these is correct

___ e)a) all of these is correct

11. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

___ a) 10,000

___ b) 10

___ c) 1000

___ d) 100

___ e) 100,000

12.

What best explains this figure?

___ a) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ b) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ d) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ e) The photon loses energy, not speed. By E=hf, it loses frequency, and by c=fλ it increases wavelengthand turns red.

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13. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the temperature

___ b) the mass as measured by Kepler's third law (modified by Newton)

___ c) the gravitational redshift

___ d) the expansion of the universe

___ e) the doppler shift

14. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 3

___ b) 8

___ c) 4

___ d) 6

___ e) 2

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster A, because it exhibits greater angular expansion

___ b) cluster A, because it exhibits a blue Doppler shift

___ c) cluster B, because it exhibits less angular expansion

___ d) cluster B, because it exhibits a red Doppler shift

___ e) either cluster might be more distant

Page 7: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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16. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) chimps typing Shakespeare

___ b) recalibration of supernovae luminosity

___ c) cosmic redshift

___ d) recalibration of supernovae relative magnitude

___ e) cosmic expansion

17. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the width the trainto be greater.

___ b) The observer on the ground would perceive the width the trainto be smaller.

___ c) Special relativity is valid only for objects travelling in a vacuum.

___ d) The observer on the ground would perceive the ball to be travelling more slowly.

___ e) The observer on the ground would perceive the ball to be travelling faster.

18. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) novae

___ b) entire galaxies

___ c) supernovae

___ d) Cepheid variables

___ e) red giants

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19. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ b) electrons striking oxygen molecules, like a lava lamp

___ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ d) cyclotron motion, causing the electrons to strike oxygen molecules

___ e) electrons striking hydrogen molecules, like a lava lamp

20. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the distance to Sirius A

___ b) all of these are true

___ c) the relative magnitude of Sirius B

___ d) the wobble of Sirius A

___ e) the "color" (spectral class) of Sirius B

21.

This spectrum of the star Vega suggests that

___ a) all of these are true

___ b) it is an approximate black body

___ c) if is not really a black body

___ d) it can be associated with an "effective" temperature

___ e) it's surface can be associated with a range of temperatures

Page 9: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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Key to AstroSizeWhitdwrfNeutstarQSO­v1s1

1. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting to count asteroids

­ b) Attempting one of the first star charts

+ c) Looking for a comet that he knew would be appearing in that part of the sky.

­ d) Trying to measure the orbital radius of a planet

­ e) Looking for lobsters

2. What causes the blue glow of the Crab nebula?

­ a) the same emission found in a Lava lamp (ultra­violet)

­ b) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ c) the Gravitational blue shift

+ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ e) the Doppler blue shift

3. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

+ a) temperature­luminosity...redshift...quantum­theory­of­solids

­ b) doppler­shift...period­of­pulsation...temperature­luminosity

­ c) HR­diagram­location...X­ray­emmision...spectral­lines

­ d) all of these are true

­ e) x­ray­emmission...doppler­shift...rotation­rate

Page 10: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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4. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

+ a)

­ b)

­ c)

­ d)

­ e)

5. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

+ a) expansion from 1 cm to 4 cm (just like yours).

­ b) expansion from 1 cm to 2 cm (half of yours)

­ c) expansion from 1 cm to 3 cm (since 3­1=2)

­ d) expansion from 1 cm to 8 cm (twice yours).

­ e) expansion from 1 cm to 9 cm (since 5­1=4)

Page 11: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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6. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

+ a) 25%

­ b) 10%

­ c) 100%

­ d) 0.1%

­ e) 1%

7. This light clock is associated with

­ a) general relativity

­ b) doppler shift

+ c) special relativity

­ d) all of these are true

­ e) gravitational shift

8. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

­ a) 2

­ b) 8

­ c) 4

­ d) 3

+ e) 6

9. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) Cepheid variables

+ b) entire galaxies

­ c) red giants

­ d) novae

­ e) supernovae

Page 12: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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10. At the center of the Crab nebula is

­ a)d) a neutron star

­ b)e) the remnants of a supernova

­ c)b) a pulsar

­ d)c) none of these is correct

+ e)a) all of these is correct

11. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

­ a) 10,000

+ b) 10

­ c) 1000

­ d) 100

­ e) 100,000

12.

What best explains this figure?

­ a) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

­ b) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

­ d) The photon slows down, by the Doppler shift, c=fλ, andtherefore by E=hf it turns red.

+ e) The photon loses energy, not speed. By E=hf, it loses frequency, and by c=fλ it increaseswavelength and turns red.

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13. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the temperature

­ b) the mass as measured by Kepler's third law (modified by Newton)

+ c) the gravitational redshift

­ d) the expansion of the universe

­ e) the doppler shift

14. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

­ a) 3

+ b) 8

­ c) 4

­ d) 6

­ e) 2

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

+ a) cluster A, because it exhibits greater angular expansion

­ b) cluster A, because it exhibits a blue Doppler shift

­ c) cluster B, because it exhibits less angular expansion

­ d) cluster B, because it exhibits a red Doppler shift

­ e) either cluster might be more distant

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16. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

+ a) chimps typing Shakespeare

­ b) recalibration of supernovae luminosity

­ c) cosmic redshift

­ d) recalibration of supernovae relative magnitude

­ e) cosmic expansion

17. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the width thetrain to be greater.

­ b) The observer on the ground would perceive the width thetrain to be smaller.

­ c) Special relativity is valid only for objects travelling in a vacuum.

­ d) The observer on the ground would perceive the ball to be travelling more slowly.

+ e) The observer on the ground would perceive the ball to be travelling faster.

18. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) novae

­ b) entire galaxies

+ c) supernovae

­ d) Cepheid variables

­ e) red giants

Page 15: Quizbank/Astronomy Quiz - Wikimedia Commons · 5 / 3 0 2 1 Q u i z b a n k A s t r o m y W v e h t p s: / e n. w i k v r y o g Q u z b a A m _ 3 1 4 4. is the kinetic energy of a

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19. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ b) electrons striking oxygen molecules, like a lava lamp

+ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ d) cyclotron motion, causing the electrons to strike oxygen molecules

­ e) electrons striking hydrogen molecules, like a lava lamp

20. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the distance to Sirius A

+ b) all of these are true

­ c) the relative magnitude of Sirius B

­ d) the wobble of Sirius A

­ e) the "color" (spectral class) of Sirius B

21.

This spectrum of the star Vega suggests that

+ a) all of these are true

­ b) it is an approximate black body

­ c) if is not really a black body

­ d) it can be associated with an "effective" temperature

­ e) it's surface can be associated with a range of temperatures

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AstroSizeWhitdwrfNeutstarQSO­v2s1

1.

What best explains this figure?

___ a) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ c) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ d) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ e) The photon slows down, by the Doppler shift, E=hf, and therefore by c=f&;lambda it turns red.

2. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 2 cm (half of yours)

___ b) expansion from 1 cm to 8 cm (twice yours).

___ c) expansion from 1 cm to 4 cm (just like yours).

___ d) expansion from 1 cm to 3 cm (since 3­1=2)

___ e) expansion from 1 cm to 9 cm (since 5­1=4)

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster B, because it exhibits less angular expansion

___ b) cluster B, because it exhibits a red Doppler shift

___ c) cluster A, because it exhibits a blue Doppler shift

___ d) either cluster might be more distant

___ e) cluster A, because it exhibits greater angular expansion

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4. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

5. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

___ a) 10

___ b) 10,000

___ c) 100,000

___ d) 100

___ e) 1000

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6. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

___ a) 4

___ b) 6

___ c) 8

___ d) 2

___ e) 3

7. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the ball to betravelling faster.

___ b) Special relativity is valid only for objects travelling in avacuum.

___ c) The observer on the ground would perceive the width the train to be greater.

___ d) The observer on the ground would perceive the width the train to be smaller.

___ e) The observer on the ground would perceive the ball to be travelling more slowly.

8. This light clock is associated with

___ a) all of these are true

___ b) doppler shift

___ c) special relativity

___ d) gravitational shift

___ e) general relativity

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9. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 4

___ b) 8

___ c) 2

___ d) 6

___ e) 3

10. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the gravitational redshift

___ b) the expansion of the universe

___ c) the mass as measured by Kepler's third law (modified by Newton)

___ d) the temperature

___ e) the doppler shift

11. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 100%

___ b) 0.1%

___ c) 1%

___ d) 25%

___ e) 10%

12. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) entire galaxies

___ b) novae

___ c) supernovae

___ d) Cepheid variables

___ e) red giants

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13. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ b) electrons striking hydrogen molecules, like a lava lamp

___ c) electrons striking oxygen molecules, like a lava lamp

___ d) cyclotron motion, causing the electrons to strike oxygen molecules

___ e) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

14. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ b) the same emission found in a Lava lamp (ultra­violet)

___ c) the Gravitational blue shift

___ d) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ e) the Doppler blue shift

15. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the relative magnitude of Sirius B

___ b) the "color" (spectral class) of Sirius B

___ c) the distance to Sirius A

___ d) the wobble of Sirius A

___ e) all of these are true

16. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) cosmic redshift

___ b) chimps typing Shakespeare

___ c) cosmic expansion

___ d) recalibration of supernovae relative magnitude

___ e) recalibration of supernovae luminosity

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17. At the center of the Crab nebula is

___ a)d) a neutron star

___ b)a) all of these is correct

___ c)e) the remnants of a supernova

___ d)c) none of these is correct

___ e)b) a pulsar

18.

This spectrum of the star Vega suggests that

___ a) it can be associated with an "effective" temperature

___ b) all of these are true

___ c) it is an approximate black body

___ d) it's surface can be associated with a range of temperatures

___ e) if is not really a black body

19. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Trying to measure the orbital radius of a planet

___ b) Looking for a comet that he knew would be appearing in that part of the sky.

___ c) Looking for lobsters

___ d) Attempting to count asteroids

___ e) Attempting one of the first star charts

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20. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) temperature­luminosity...redshift...quantum­theory­of­solids

___ b) x­ray­emmission...doppler­shift...rotation­rate

___ c) doppler­shift...period­of­pulsation...temperature­luminosity

___ d) all of these are true

___ e) HR­diagram­location...X­ray­emmision...spectral­lines

21. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) novae

___ b) red giants

___ c) entire galaxies

___ d) Cepheid variables

___ e) supernovae

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Key to AstroSizeWhitdwrfNeutstarQSO­v2s1

1.

What best explains this figure?

­ a) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

+ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ c) The photon slows down, by the Doppler shift, c=fλ, and thereforeby E=hf it turns red.

­ d) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

­ e) The photon slows down, by the Doppler shift, E=hf, and therefore by c=f&;lambda it turns red.

2. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 2 cm (half of yours)

­ b) expansion from 1 cm to 8 cm (twice yours).

+ c) expansion from 1 cm to 4 cm (just like yours).

­ d) expansion from 1 cm to 3 cm (since 3­1=2)

­ e) expansion from 1 cm to 9 cm (since 5­1=4)

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) cluster B, because it exhibits less angular expansion

­ b) cluster B, because it exhibits a red Doppler shift

­ c) cluster A, because it exhibits a blue Doppler shift

­ d) either cluster might be more distant

+ e) cluster A, because it exhibits greater angular expansion

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4. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

­ c)

+ d)

­ e)

5. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

+ a) 10

­ b) 10,000

­ c) 100,000

­ d) 100

­ e) 1000

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6. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

­ a) 4

­ b) 6

+ c) 8

­ d) 2

­ e) 3

7. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

+ a) The observer on the ground would perceive the ball to betravelling faster.

­ b) Special relativity is valid only for objects travelling in avacuum.

­ c) The observer on the ground would perceive the width the train to be greater.

­ d) The observer on the ground would perceive the width the train to be smaller.

­ e) The observer on the ground would perceive the ball to be travelling more slowly.

8. This light clock is associated with

­ a) all of these are true

­ b) doppler shift

+ c) special relativity

­ d) gravitational shift

­ e) general relativity

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9. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

­ a) 4

­ b) 8

­ c) 2

+ d) 6

­ e) 3

10. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

+ a) the gravitational redshift

­ b) the expansion of the universe

­ c) the mass as measured by Kepler's third law (modified by Newton)

­ d) the temperature

­ e) the doppler shift

11. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 100%

­ b) 0.1%

­ c) 1%

+ d) 25%

­ e) 10%

12. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

+ a) entire galaxies

­ b) novae

­ c) supernovae

­ d) Cepheid variables

­ e) red giants

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13. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ b) electrons striking hydrogen molecules, like a lava lamp

­ c) electrons striking oxygen molecules, like a lava lamp

­ d) cyclotron motion, causing the electrons to strike oxygen molecules

+ e) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

14. What causes the blue glow of the Crab nebula?

+ a) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ b) the same emission found in a Lava lamp (ultra­violet)

­ c) the Gravitational blue shift

­ d) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ e) the Doppler blue shift

15. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the relative magnitude of Sirius B

­ b) the "color" (spectral class) of Sirius B

­ c) the distance to Sirius A

­ d) the wobble of Sirius A

+ e) all of these are true

16. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) cosmic redshift

+ b) chimps typing Shakespeare

­ c) cosmic expansion

­ d) recalibration of supernovae relative magnitude

­ e) recalibration of supernovae luminosity

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17. At the center of the Crab nebula is

­ a)d) a neutron star

+ b)a) all of these is correct

­ c)e) the remnants of a supernova

­ d)c) none of these is correct

­ e)b) a pulsar

18.

This spectrum of the star Vega suggests that

­ a) it can be associated with an "effective" temperature

+ b) all of these are true

­ c) it is an approximate black body

­ d) it's surface can be associated with a range of temperatures

­ e) if is not really a black body

19. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Trying to measure the orbital radius of a planet

+ b) Looking for a comet that he knew would be appearing in that part of the sky.

­ c) Looking for lobsters

­ d) Attempting to count asteroids

­ e) Attempting one of the first star charts

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20. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

+ a) temperature­luminosity...redshift...quantum­theory­of­solids

­ b) x­ray­emmission...doppler­shift...rotation­rate

­ c) doppler­shift...period­of­pulsation...temperature­luminosity

­ d) all of these are true

­ e) HR­diagram­location...X­ray­emmision...spectral­lines

21. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) novae

­ b) red giants

­ c) entire galaxies

­ d) Cepheid variables

+ e) supernovae

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AstroSizeWhitdwrfNeutstarQSO­v1s2

1. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

2. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) Special relativity is valid only for objects travelling in avacuum.

___ b) The observer on the ground would perceive the width the trainto be greater.

___ c) The observer on the ground would perceive the width the train to be smaller.

___ d) The observer on the ground would perceive the ball to be travelling more slowly.

___ e) The observer on the ground would perceive the ball to be travelling faster.

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3. What causes the blue glow of the Crab nebula?

___ a) the Doppler blue shift

___ b) the same emission found in a Lava lamp (ultra­violet)

___ c) the Gravitational blue shift

___ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ e) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) entire galaxies

___ b) Cepheid variables

___ c) red giants

___ d) novae

___ e) supernovae

5.

This spectrum of the star Vega suggests that

___ a) it is an approximate black body

___ b) it can be associated with an "effective" temperature

___ c) all of these are true

___ d) it's surface can be associated with a range of temperatures

___ e) if is not really a black body

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6.

What best explains this figure?

___ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ c) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ d) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increases wavelengthand turns red.

7. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

___ a) 10,000

___ b) 1000

___ c) 10

___ d) 100,000

___ e) 100

8. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) cyclotron motion, causing the electrons to strike oxygen molecules

___ b) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ d) electrons striking hydrogen molecules, like a lava lamp

___ e) electrons striking oxygen molecules, like a lava lamp

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9. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 2

___ b) 8

___ c) 6

___ d) 4

___ e) 3

10. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting to count asteroids

___ b) Attempting one of the first star charts

___ c) Looking for a comet that he knew would be appearing in that part of the sky.

___ d) Looking for lobsters

___ e) Trying to measure the orbital radius of a planet

11. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the relative magnitude of Sirius B

___ b) the distance to Sirius A

___ c) all of these are true

___ d) the "color" (spectral class) of Sirius B

___ e) the wobble of Sirius A

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) supernovae

___ b) entire galaxies

___ c) novae

___ d) Cepheid variables

___ e) red giants

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13. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) recalibration of supernovae relative magnitude

___ b) chimps typing Shakespeare

___ c) cosmic expansion

___ d) cosmic redshift

___ e) recalibration of supernovae luminosity

14. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 2 cm (half of yours)

___ b) expansion from 1 cm to 9 cm (since 5­1=4)

___ c) expansion from 1 cm to 8 cm (twice yours).

___ d) expansion from 1 cm to 4 cm (just like yours).

___ e) expansion from 1 cm to 3 cm (since 3­1=2)

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster B, because it exhibits less angular expansion

___ b) either cluster might be more distant

___ c) cluster A, because it exhibits greater angular expansion

___ d) cluster A, because it exhibits a blue Doppler shift

___ e) cluster B, because it exhibits a red Doppler shift

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16. At the center of the Crab nebula is

___ a)c) none of these is correct

___ b)a) all of these is correct

___ c)e) the remnants of a supernova

___ d)b) a pulsar

___ e)d) a neutron star

17. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the mass as measured by Kepler's third law (modified by Newton)

___ b) the temperature

___ c) the doppler shift

___ d) the gravitational redshift

___ e) the expansion of the universe

18. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 0.1%

___ b) 25%

___ c) 10%

___ d) 100%

___ e) 1%

19. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 8

___ b) 3

___ c) 4

___ d) 2

___ e) 6

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20. This light clock is associated with

___ a) doppler shift

___ b) general relativity

___ c) special relativity

___ d) gravitational shift

___ e) all of these are true

21. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) all of these are true

___ b) doppler­shift...period­of­pulsation...temperature­luminosity

___ c) x­ray­emmission...doppler­shift...rotation­rate

___ d) HR­diagram­location...X­ray­emmision...spectral­lines

___ e) temperature­luminosity...redshift...quantum­theory­of­solids

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Key to AstroSizeWhitdwrfNeutstarQSO­v1s2

1. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

+ b)

­ c)

­ d)

­ e)

2. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) Special relativity is valid only for objects travelling in avacuum.

­ b) The observer on the ground would perceive the width thetrain to be greater.

­ c) The observer on the ground would perceive the width the train to be smaller.

­ d) The observer on the ground would perceive the ball to be travelling more slowly.

+ e) The observer on the ground would perceive the ball to be travelling faster.

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3. What causes the blue glow of the Crab nebula?

­ a) the Doppler blue shift

­ b) the same emission found in a Lava lamp (ultra­violet)

­ c) the Gravitational blue shift

+ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ e) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

+ a) entire galaxies

­ b) Cepheid variables

­ c) red giants

­ d) novae

­ e) supernovae

5.

This spectrum of the star Vega suggests that

­ a) it is an approximate black body

­ b) it can be associated with an "effective" temperature

+ c) all of these are true

­ d) it's surface can be associated with a range of temperatures

­ e) if is not really a black body

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6.

What best explains this figure?

­ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

+ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ c) The photon slows down, by the Doppler shift, c=fλ, and thereforeby E=hf it turns red.

­ d) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increaseswavelength and turns red.

7. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

­ a) 10,000

­ b) 1000

+ c) 10

­ d) 100,000

­ e) 100

8. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) cyclotron motion, causing the electrons to strike oxygen molecules

­ b) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

+ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ d) electrons striking hydrogen molecules, like a lava lamp

­ e) electrons striking oxygen molecules, like a lava lamp

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9. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

­ a) 2

­ b) 8

+ c) 6

­ d) 4

­ e) 3

10. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting to count asteroids

­ b) Attempting one of the first star charts

+ c) Looking for a comet that he knew would be appearing in that part of the sky.

­ d) Looking for lobsters

­ e) Trying to measure the orbital radius of a planet

11. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the relative magnitude of Sirius B

­ b) the distance to Sirius A

+ c) all of these are true

­ d) the "color" (spectral class) of Sirius B

­ e) the wobble of Sirius A

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

+ a) supernovae

­ b) entire galaxies

­ c) novae

­ d) Cepheid variables

­ e) red giants

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13. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) recalibration of supernovae relative magnitude

+ b) chimps typing Shakespeare

­ c) cosmic expansion

­ d) cosmic redshift

­ e) recalibration of supernovae luminosity

14. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 2 cm (half of yours)

­ b) expansion from 1 cm to 9 cm (since 5­1=4)

­ c) expansion from 1 cm to 8 cm (twice yours).

+ d) expansion from 1 cm to 4 cm (just like yours).

­ e) expansion from 1 cm to 3 cm (since 3­1=2)

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) cluster B, because it exhibits less angular expansion

­ b) either cluster might be more distant

+ c) cluster A, because it exhibits greater angular expansion

­ d) cluster A, because it exhibits a blue Doppler shift

­ e) cluster B, because it exhibits a red Doppler shift

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16. At the center of the Crab nebula is

­ a)c) none of these is correct

+ b)a) all of these is correct

­ c)e) the remnants of a supernova

­ d)b) a pulsar

­ e)d) a neutron star

17. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the mass as measured by Kepler's third law (modified by Newton)

­ b) the temperature

­ c) the doppler shift

+ d) the gravitational redshift

­ e) the expansion of the universe

18. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 0.1%

+ b) 25%

­ c) 10%

­ d) 100%

­ e) 1%

19. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

+ a) 8

­ b) 3

­ c) 4

­ d) 2

­ e) 6

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20. This light clock is associated with

­ a) doppler shift

­ b) general relativity

+ c) special relativity

­ d) gravitational shift

­ e) all of these are true

21. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) all of these are true

­ b) doppler­shift...period­of­pulsation...temperature­luminosity

­ c) x­ray­emmission...doppler­shift...rotation­rate

­ d) HR­diagram­location...X­ray­emmision...spectral­lines

+ e) temperature­luminosity...redshift...quantum­theory­of­solids

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AstroSizeWhitdwrfNeutstarQSO­v2s2

1. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 3 cm (since 3­1=2)

___ b) expansion from 1 cm to 4 cm (just like yours).

___ c) expansion from 1 cm to 9 cm (since 5­1=4)

___ d) expansion from 1 cm to 8 cm (twice yours).

___ e) expansion from 1 cm to 2 cm (half of yours)

2. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) novae

___ b) red giants

___ c) entire galaxies

___ d) Cepheid variables

___ e) supernovae

3. This light clock is associated with

___ a) all of these are true

___ b) doppler shift

___ c) general relativity

___ d) gravitational shift

___ e) special relativity

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4. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 3

___ b) 6

___ c) 2

___ d) 4

___ e) 8

5.

What best explains this figure?

___ a) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ d) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ e) The photon slows down, by the Doppler shift, c=fλ, and therefore by E=hf it turns red.

6. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the distance to Sirius A

___ b) the wobble of Sirius A

___ c) all of these are true

___ d) the "color" (spectral class) of Sirius B

___ e) the relative magnitude of Sirius B

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7. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

___ a) 100,000

___ b) 10

___ c) 10,000

___ d) 100

___ e) 1000

8. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting to count asteroids

___ b) Looking for lobsters

___ c) Looking for a comet that he knew would be appearing in that part of the sky.

___ d) Trying to measure the orbital radius of a planet

___ e) Attempting one of the first star charts

9. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the width the trainto be smaller.

___ b) The observer on the ground would perceive the width the trainto be greater.

___ c) Special relativity is valid only for objects travelling in a vacuum.

___ d) The observer on the ground would perceive the ball to be travelling faster.

___ e) The observer on the ground would perceive the ball to be travelling more slowly.

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10. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) cosmic redshift

___ b) recalibration of supernovae luminosity

___ c) chimps typing Shakespeare

___ d) cosmic expansion

___ e) recalibration of supernovae relative magnitude

11. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 25%

___ b) 0.1%

___ c) 10%

___ d) 100%

___ e) 1%

12. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

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13.

This spectrum of the star Vega suggests that

___ a) if is not really a black body

___ b) it is an approximate black body

___ c) it's surface can be associated with a range of temperatures

___ d) all of these are true

___ e) it can be associated with an "effective" temperature

14. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) novae

___ b) red giants

___ c) entire galaxies

___ d) supernovae

___ e) Cepheid variables

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster A, because it exhibits greater angular expansion

___ b) cluster B, because it exhibits less angular expansion

___ c) cluster A, because it exhibits a blue Doppler shift

___ d) cluster B, because it exhibits a red Doppler shift

___ e) either cluster might be more distant

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16. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) cyclotron motion, causing the electrons to strike oxygen molecules

___ b) electrons striking oxygen molecules, like a lava lamp

___ c) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ d) electrons striking hydrogen molecules, like a lava lamp

___ e) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

17. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the same emission found in a Lava lamp (ultra­violet)

___ c) the Gravitational blue shift

___ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ e) the Doppler blue shift

18. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) x­ray­emmission...doppler­shift...rotation­rate

___ b) doppler­shift...period­of­pulsation...temperature­luminosity

___ c) all of these are true

___ d) temperature­luminosity...redshift...quantum­theory­of­solids

___ e) HR­diagram­location...X­ray­emmision...spectral­lines

19. At the center of the Crab nebula is

___ a)d) a neutron star

___ b)c) none of these is correct

___ c)e) the remnants of a supernova

___ d)a) all of these is correct

___ e)b) a pulsar

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20. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 6

___ b) 3

___ c) 8

___ d) 2

___ e) 4

21. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the gravitational redshift

___ b) the temperature

___ c) the expansion of the universe

___ d) the doppler shift

___ e) the mass as measured by Kepler's third law (modified by Newton)

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Key to AstroSizeWhitdwrfNeutstarQSO­v2s2

1. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 3 cm (since 3­1=2)

+ b) expansion from 1 cm to 4 cm (just like yours).

­ c) expansion from 1 cm to 9 cm (since 5­1=4)

­ d) expansion from 1 cm to 8 cm (twice yours).

­ e) expansion from 1 cm to 2 cm (half of yours)

2. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) novae

­ b) red giants

­ c) entire galaxies

­ d) Cepheid variables

+ e) supernovae

3. This light clock is associated with

­ a) all of these are true

­ b) doppler shift

­ c) general relativity

­ d) gravitational shift

+ e) special relativity

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4. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

­ a) 3

+ b) 6

­ c) 2

­ d) 4

­ e) 8

5.

What best explains this figure?

­ a) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

­ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

+ d) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ e) The photon slows down, by the Doppler shift, c=fλ, and therefore by E=hf it turns red.

6. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the distance to Sirius A

­ b) the wobble of Sirius A

+ c) all of these are true

­ d) the "color" (spectral class) of Sirius B

­ e) the relative magnitude of Sirius B

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7. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

­ a) 100,000

+ b) 10

­ c) 10,000

­ d) 100

­ e) 1000

8. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting to count asteroids

­ b) Looking for lobsters

+ c) Looking for a comet that he knew would be appearing in that part of the sky.

­ d) Trying to measure the orbital radius of a planet

­ e) Attempting one of the first star charts

9. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the width thetrain to be smaller.

­ b) The observer on the ground would perceive the width thetrain to be greater.

­ c) Special relativity is valid only for objects travelling in a vacuum.

+ d) The observer on the ground would perceive the ball to be travelling faster.

­ e) The observer on the ground would perceive the ball to be travelling more slowly.

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10. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) cosmic redshift

­ b) recalibration of supernovae luminosity

+ c) chimps typing Shakespeare

­ d) cosmic expansion

­ e) recalibration of supernovae relative magnitude

11. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

+ a) 25%

­ b) 0.1%

­ c) 10%

­ d) 100%

­ e) 1%

12. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

+ c)

­ d)

­ e)

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13.

This spectrum of the star Vega suggests that

­ a) if is not really a black body

­ b) it is an approximate black body

­ c) it's surface can be associated with a range oftemperatures

+ d) all of these are true

­ e) it can be associated with an "effective" temperature

14. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) novae

­ b) red giants

+ c) entire galaxies

­ d) supernovae

­ e) Cepheid variables

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

+ a) cluster A, because it exhibits greater angular expansion

­ b) cluster B, because it exhibits less angular expansion

­ c) cluster A, because it exhibits a blue Doppler shift

­ d) cluster B, because it exhibits a red Doppler shift

­ e) either cluster might be more distant

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16. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) cyclotron motion, causing the electrons to strike oxygen molecules

­ b) electrons striking oxygen molecules, like a lava lamp

­ c) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ d) electrons striking hydrogen molecules, like a lava lamp

+ e) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

17. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ b) the same emission found in a Lava lamp (ultra­violet)

­ c) the Gravitational blue shift

+ d) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ e) the Doppler blue shift

18. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) x­ray­emmission...doppler­shift...rotation­rate

­ b) doppler­shift...period­of­pulsation...temperature­luminosity

­ c) all of these are true

+ d) temperature­luminosity...redshift...quantum­theory­of­solids

­ e) HR­diagram­location...X­ray­emmision...spectral­lines

19. At the center of the Crab nebula is

­ a)d) a neutron star

­ b)c) none of these is correct

­ c)e) the remnants of a supernova

+ d)a) all of these is correct

­ e)b) a pulsar

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20. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

­ a) 6

­ b) 3

+ c) 8

­ d) 2

­ e) 4

21. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

+ a) the gravitational redshift

­ b) the temperature

­ c) the expansion of the universe

­ d) the doppler shift

­ e) the mass as measured by Kepler's third law (modified by Newton)

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AstroSizeWhitdwrfNeutstarQSO­v1s3

1. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the width the trainto be greater.

___ b) The observer on the ground would perceive the width the trainto be smaller.

___ c) The observer on the ground would perceive the ball to be travelling more slowly.

___ d) The observer on the ground would perceive the ball to be travelling faster.

___ e) Special relativity is valid only for objects travelling in a vacuum.

2. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting one of the first star charts

___ b) Looking for lobsters

___ c) Looking for a comet that he knew would be appearing in that part of the sky.

___ d) Trying to measure the orbital radius of a planet

___ e) Attempting to count asteroids

3. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 10%

___ b) 0.1%

___ c) 25%

___ d) 1%

___ e) 100%

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4. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 4 cm (just like yours).

___ b) expansion from 1 cm to 9 cm (since 5­1=4)

___ c) expansion from 1 cm to 2 cm (half of yours)

___ d) expansion from 1 cm to 3 cm (since 3­1=2)

___ e) expansion from 1 cm to 8 cm (twice yours).

5. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) supernovae

___ b) novae

___ c) entire galaxies

___ d) red giants

___ e) Cepheid variables

6. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) cosmic redshift

___ b) cosmic expansion

___ c) recalibration of supernovae relative magnitude

___ d) recalibration of supernovae luminosity

___ e) chimps typing Shakespeare

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7. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) doppler­shift...period­of­pulsation...temperature­luminosity

___ b) x­ray­emmission...doppler­shift...rotation­rate

___ c) temperature­luminosity...redshift...quantum­theory­of­solids

___ d) HR­diagram­location...X­ray­emmision...spectral­lines

___ e) all of these are true

8. This light clock is associated with

___ a) all of these are true

___ b) gravitational shift

___ c) special relativity

___ d) general relativity

___ e) doppler shift

9. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

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10. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 3

___ b) 2

___ c) 6

___ d) 8

___ e) 4

11. What causes the blue glow of the Crab nebula?

___ a) the Doppler blue shift

___ b) the same emission found in a Lava lamp (ultra­violet)

___ c) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ d) the Gravitational blue shift

___ e) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

12. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

___ a) 3

___ b) 6

___ c) 8

___ d) 4

___ e) 2

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13. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

___ a) 100

___ b) 100,000

___ c) 10

___ d) 10,000

___ e) 1000

14.

What best explains this figure?

___ a) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ c) The photon loses energy, not speed. By E=hf, it loses frequency, andby c=fλ it increases wavelength and turns red.

___ d) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster A, because it exhibits a blue Doppler shift

___ b) cluster B, because it exhibits a red Doppler shift

___ c) cluster A, because it exhibits greater angular expansion

___ d) cluster B, because it exhibits less angular expansion

___ e) either cluster might be more distant

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16. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the relative magnitude of Sirius B

___ b) all of these are true

___ c) the wobble of Sirius A

___ d) the "color" (spectral class) of Sirius B

___ e) the distance to Sirius A

17. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the gravitational redshift

___ b) the temperature

___ c) the doppler shift

___ d) the mass as measured by Kepler's third law (modified by Newton)

___ e) the expansion of the universe

18. At the center of the Crab nebula is

___ a)a) all of these is correct

___ b)d) a neutron star

___ c)e) the remnants of a supernova

___ d)c) none of these is correct

___ e)b) a pulsar

19.

This spectrum of the star Vega suggests that

___ a) all of these are true

___ b) it is an approximate black body

___ c) it's surface can be associated with a range of temperatures

___ d) if is not really a black body

___ e) it can be associated with an "effective" temperature

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20. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) cyclotron motion, causing the electrons to strike oxygen molecules

___ b) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ c) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ d) electrons striking hydrogen molecules, like a lava lamp

___ e) electrons striking oxygen molecules, like a lava lamp

21. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) Cepheid variables

___ b) supernovae

___ c) red giants

___ d) novae

___ e) entire galaxies

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Key to AstroSizeWhitdwrfNeutstarQSO­v1s3

1. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the width thetrain to be greater.

­ b) The observer on the ground would perceive the width thetrain to be smaller.

­ c) The observer on the ground would perceive the ball to be travelling more slowly.

+ d) The observer on the ground would perceive the ball to be travelling faster.

­ e) Special relativity is valid only for objects travelling in a vacuum.

2. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting one of the first star charts

­ b) Looking for lobsters

+ c) Looking for a comet that he knew would be appearing in that part of the sky.

­ d) Trying to measure the orbital radius of a planet

­ e) Attempting to count asteroids

3. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 10%

­ b) 0.1%

+ c) 25%

­ d) 1%

­ e) 100%

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4. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

+ a) expansion from 1 cm to 4 cm (just like yours).

­ b) expansion from 1 cm to 9 cm (since 5­1=4)

­ c) expansion from 1 cm to 2 cm (half of yours)

­ d) expansion from 1 cm to 3 cm (since 3­1=2)

­ e) expansion from 1 cm to 8 cm (twice yours).

5. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) supernovae

­ b) novae

+ c) entire galaxies

­ d) red giants

­ e) Cepheid variables

6. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) cosmic redshift

­ b) cosmic expansion

­ c) recalibration of supernovae relative magnitude

­ d) recalibration of supernovae luminosity

+ e) chimps typing Shakespeare

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7. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) doppler­shift...period­of­pulsation...temperature­luminosity

­ b) x­ray­emmission...doppler­shift...rotation­rate

+ c) temperature­luminosity...redshift...quantum­theory­of­solids

­ d) HR­diagram­location...X­ray­emmision...spectral­lines

­ e) all of these are true

8. This light clock is associated with

­ a) all of these are true

­ b) gravitational shift

+ c) special relativity

­ d) general relativity

­ e) doppler shift

9. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

­ c)

­ d)

+ e)

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10. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

­ a) 3

­ b) 2

­ c) 6

+ d) 8

­ e) 4

11. What causes the blue glow of the Crab nebula?

­ a) the Doppler blue shift

­ b) the same emission found in a Lava lamp (ultra­violet)

­ c) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ d) the Gravitational blue shift

+ e) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

12. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

­ a) 3

+ b) 6

­ c) 8

­ d) 4

­ e) 2

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13. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

­ a) 100

­ b) 100,000

+ c) 10

­ d) 10,000

­ e) 1000

14.

What best explains this figure?

­ a) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

+ c) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ d) The photon slows down, by the Doppler shift, c=fλ, andtherefore by E=hf it turns red.

­ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

15. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) cluster A, because it exhibits a blue Doppler shift

­ b) cluster B, because it exhibits a red Doppler shift

+ c) cluster A, because it exhibits greater angular expansion

­ d) cluster B, because it exhibits less angular expansion

­ e) either cluster might be more distant

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16. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the relative magnitude of Sirius B

+ b) all of these are true

­ c) the wobble of Sirius A

­ d) the "color" (spectral class) of Sirius B

­ e) the distance to Sirius A

17. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

+ a) the gravitational redshift

­ b) the temperature

­ c) the doppler shift

­ d) the mass as measured by Kepler's third law (modified by Newton)

­ e) the expansion of the universe

18. At the center of the Crab nebula is

+ a)a) all of these is correct

­ b)d) a neutron star

­ c)e) the remnants of a supernova

­ d)c) none of these is correct

­ e)b) a pulsar

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19.

This spectrum of the star Vega suggests that

+ a) all of these are true

­ b) it is an approximate black body

­ c) it's surface can be associated with a range oftemperatures

­ d) if is not really a black body

­ e) it can be associated with an "effective" temperature

20. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) cyclotron motion, causing the electrons to strike oxygen molecules

+ b) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ c) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ d) electrons striking hydrogen molecules, like a lava lamp

­ e) electrons striking oxygen molecules, like a lava lamp

21. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) Cepheid variables

+ b) supernovae

­ c) red giants

­ d) novae

­ e) entire galaxies

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AstroSizeWhitdwrfNeutstarQSO­v2s3

1. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) electrons striking hydrogen molecules, like a lava lamp

___ b) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ d) cyclotron motion, causing the electrons to strike oxygen molecules

___ e) electrons striking oxygen molecules, like a lava lamp

2. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the width the trainto be smaller.

___ b) Special relativity is valid only for objects travelling in avacuum.

___ c) The observer on the ground would perceive the ball to be travelling more slowly.

___ d) The observer on the ground would perceive the width the train to be greater.

___ e) The observer on the ground would perceive the ball to be travelling faster.

3. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

___ a) 10,000

___ b) 10

___ c) 1000

___ d) 100,000

___ e) 100

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4. At the center of the Crab nebula is

___ a)c) none of these is correct

___ b)a) all of these is correct

___ c)e) the remnants of a supernova

___ d)d) a neutron star

___ e)b) a pulsar

5.

This spectrum of the star Vega suggests that

___ a) it's surface can be associated with a range of temperatures

___ b) if is not really a black body

___ c) it is an approximate black body

___ d) it can be associated with an "effective" temperature

___ e) all of these are true

6. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ c) the Doppler blue shift

___ d) the Gravitational blue shift

___ e) the same emission found in a Lava lamp (ultra­violet)

7. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 6

___ b) 4

___ c) 2

___ d) 3

___ e) 8

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8. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) doppler­shift...period­of­pulsation...temperature­luminosity

___ b) HR­diagram­location...X­ray­emmision...spectral­lines

___ c) x­ray­emmission...doppler­shift...rotation­rate

___ d) temperature­luminosity...redshift...quantum­theory­of­solids

___ e) all of these are true

9. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) novae

___ b) supernovae

___ c) Cepheid variables

___ d) red giants

___ e) entire galaxies

10.

What best explains this figure?

___ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ c) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ d) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increases wavelengthand turns red.

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11. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 2

___ b) 4

___ c) 3

___ d) 8

___ e) 6

12. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the wobble of Sirius A

___ b) the distance to Sirius A

___ c) the "color" (spectral class) of Sirius B

___ d) the relative magnitude of Sirius B

___ e) all of these are true

13. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Looking for a comet that he knew would be appearing in that part of the sky.

___ b) Trying to measure the orbital radius of a planet

___ c) Attempting to count asteroids

___ d) Looking for lobsters

___ e) Attempting one of the first star charts

14. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the doppler shift

___ b) the temperature

___ c) the gravitational redshift

___ d) the expansion of the universe

___ e) the mass as measured by Kepler's third law (modified by Newton)

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15. This light clock is associated with

___ a) doppler shift

___ b) all of these are true

___ c) special relativity

___ d) general relativity

___ e) gravitational shift

16. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 2 cm (half of yours)

___ b) expansion from 1 cm to 9 cm (since 5­1=4)

___ c) expansion from 1 cm to 3 cm (since 3­1=2)

___ d) expansion from 1 cm to 4 cm (just like yours).

___ e) expansion from 1 cm to 8 cm (twice yours).

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17. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

18. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) recalibration of supernovae relative magnitude

___ b) chimps typing Shakespeare

___ c) cosmic redshift

___ d) cosmic expansion

___ e) recalibration of supernovae luminosity

19. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) entire galaxies

___ b) novae

___ c) red giants

___ d) supernovae

___ e) Cepheid variables

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20. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) either cluster might be more distant

___ b) cluster A, because it exhibits a blue Doppler shift

___ c) cluster B, because it exhibits less angular expansion

___ d) cluster B, because it exhibits a red Doppler shift

___ e) cluster A, because it exhibits greater angular expansion

21. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 25%

___ b) 0.1%

___ c) 1%

___ d) 10%

___ e) 100%

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Key to AstroSizeWhitdwrfNeutstarQSO­v2s3

1. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) electrons striking hydrogen molecules, like a lava lamp

­ b) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

+ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ d) cyclotron motion, causing the electrons to strike oxygen molecules

­ e) electrons striking oxygen molecules, like a lava lamp

2. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the width thetrain to be smaller.

­ b) Special relativity is valid only for objects travelling in avacuum.

­ c) The observer on the ground would perceive the ball to be travelling more slowly.

­ d) The observer on the ground would perceive the width the train to be greater.

+ e) The observer on the ground would perceive the ball to be travelling faster.

3. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

­ a) 10,000

+ b) 10

­ c) 1000

­ d) 100,000

­ e) 100

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4. At the center of the Crab nebula is

­ a)c) none of these is correct

+ b)a) all of these is correct

­ c)e) the remnants of a supernova

­ d)d) a neutron star

­ e)b) a pulsar

5.

This spectrum of the star Vega suggests that

­ a) it's surface can be associated with a range oftemperatures

­ b) if is not really a black body

­ c) it is an approximate black body

­ d) it can be associated with an "effective" temperature

+ e) all of these are true

6. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

+ b) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ c) the Doppler blue shift

­ d) the Gravitational blue shift

­ e) the same emission found in a Lava lamp (ultra­violet)

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7. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

+ a) 6

­ b) 4

­ c) 2

­ d) 3

­ e) 8

8. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) doppler­shift...period­of­pulsation...temperature­luminosity

­ b) HR­diagram­location...X­ray­emmision...spectral­lines

­ c) x­ray­emmission...doppler­shift...rotation­rate

+ d) temperature­luminosity...redshift...quantum­theory­of­solids

­ e) all of these are true

9. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) novae

­ b) supernovae

­ c) Cepheid variables

­ d) red giants

+ e) entire galaxies

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10.

What best explains this figure?

­ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

+ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ c) The photon slows down, by the Doppler shift, c=fλ, and thereforeby E=hf it turns red.

­ d) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increaseswavelength and turns red.

11. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

­ a) 2

­ b) 4

­ c) 3

+ d) 8

­ e) 6

12. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the wobble of Sirius A

­ b) the distance to Sirius A

­ c) the "color" (spectral class) of Sirius B

­ d) the relative magnitude of Sirius B

+ e) all of these are true

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13. What was Messier doing when he independently rediscovered the Crab in 1758?

+ a) Looking for a comet that he knew would be appearing in that part of the sky.

­ b) Trying to measure the orbital radius of a planet

­ c) Attempting to count asteroids

­ d) Looking for lobsters

­ e) Attempting one of the first star charts

14. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the doppler shift

­ b) the temperature

+ c) the gravitational redshift

­ d) the expansion of the universe

­ e) the mass as measured by Kepler's third law (modified by Newton)

15. This light clock is associated with

­ a) doppler shift

­ b) all of these are true

+ c) special relativity

­ d) general relativity

­ e) gravitational shift

16. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 2 cm (half of yours)

­ b) expansion from 1 cm to 9 cm (since 5­1=4)

­ c) expansion from 1 cm to 3 cm (since 3­1=2)

+ d) expansion from 1 cm to 4 cm (just like yours).

­ e) expansion from 1 cm to 8 cm (twice yours).

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17. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

­ c)

­ d)

+ e)

18. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) recalibration of supernovae relative magnitude

+ b) chimps typing Shakespeare

­ c) cosmic redshift

­ d) cosmic expansion

­ e) recalibration of supernovae luminosity

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19. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) entire galaxies

­ b) novae

­ c) red giants

+ d) supernovae

­ e) Cepheid variables

20. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) either cluster might be more distant

­ b) cluster A, because it exhibits a blue Doppler shift

­ c) cluster B, because it exhibits less angular expansion

­ d) cluster B, because it exhibits a red Doppler shift

+ e) cluster A, because it exhibits greater angular expansion

21. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

+ a) 25%

­ b) 0.1%

­ c) 1%

­ d) 10%

­ e) 100%

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AstroSizeWhitdwrfNeutstarQSO­v1s4

1. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 100%

___ b) 25%

___ c) 1%

___ d) 10%

___ e) 0.1%

2. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the distance to Sirius A

___ b) the "color" (spectral class) of Sirius B

___ c) the relative magnitude of Sirius B

___ d) all of these are true

___ e) the wobble of Sirius A

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) either cluster might be more distant

___ b) cluster B, because it exhibits a red Doppler shift

___ c) cluster A, because it exhibits greater angular expansion

___ d) cluster A, because it exhibits a blue Doppler shift

___ e) cluster B, because it exhibits less angular expansion

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4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) Cepheid variables

___ b) supernovae

___ c) entire galaxies

___ d) red giants

___ e) novae

5. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) electrons striking oxygen molecules, like a lava lamp

___ b) electrons striking hydrogen molecules, like a lava lamp

___ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ e) cyclotron motion, causing the electrons to strike oxygen molecules

6. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) doppler­shift...period­of­pulsation...temperature­luminosity

___ b) HR­diagram­location...X­ray­emmision...spectral­lines

___ c) x­ray­emmission...doppler­shift...rotation­rate

___ d) temperature­luminosity...redshift...quantum­theory­of­solids

___ e) all of these are true

7. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the Doppler blue shift

___ c) the Gravitational blue shift

___ d) the same emission found in a Lava lamp (ultra­violet)

___ e) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

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8. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

9. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

___ a) 10

___ b) 1000

___ c) 100

___ d) 10,000

___ e) 100,000

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10. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

___ a) 2

___ b) 8

___ c) 4

___ d) 6

___ e) 3

11.

What best explains this figure?

___ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ b) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ c) The photon loses energy, not speed. By E=hf, it loses frequency, andby c=fλ it increases wavelength and turns red.

___ d) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increases wavelengthand turns red.

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) entire galaxies

___ b) red giants

___ c) novae

___ d) Cepheid variables

___ e) supernovae

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13. This light clock is associated with

___ a) special relativity

___ b) doppler shift

___ c) gravitational shift

___ d) general relativity

___ e) all of these are true

14. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) Special relativity is valid only for objects travelling in avacuum.

___ b) The observer on the ground would perceive the width the trainto be smaller.

___ c) The observer on the ground would perceive the ball to be travelling faster.

___ d) The observer on the ground would perceive the ball to be travelling more slowly.

___ e) The observer on the ground would perceive the width the train to be greater.

15. At the center of the Crab nebula is

___ a)d) a neutron star

___ b)c) none of these is correct

___ c)e) the remnants of a supernova

___ d)b) a pulsar

___ e)a) all of these is correct

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16. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the expansion of the universe

___ b) the gravitational redshift

___ c) the doppler shift

___ d) the mass as measured by Kepler's third law (modified by Newton)

___ e) the temperature

17. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting one of the first star charts

___ b) Looking for lobsters

___ c) Attempting to count asteroids

___ d) Looking for a comet that he knew would be appearing in that part of the sky.

___ e) Trying to measure the orbital radius of a planet

18. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) chimps typing Shakespeare

___ b) recalibration of supernovae luminosity

___ c) recalibration of supernovae relative magnitude

___ d) cosmic redshift

___ e) cosmic expansion

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19. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 2 cm (half of yours)

___ b) expansion from 1 cm to 8 cm (twice yours).

___ c) expansion from 1 cm to 3 cm (since 3­1=2)

___ d) expansion from 1 cm to 9 cm (since 5­1=4)

___ e) expansion from 1 cm to 4 cm (just like yours).

20.

This spectrum of the star Vega suggests that

___ a) it is an approximate black body

___ b) all of these are true

___ c) it's surface can be associated with a range of temperatures

___ d) it can be associated with an "effective" temperature

___ e) if is not really a black body

21. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 8

___ b) 2

___ c) 6

___ d) 4

___ e) 3

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Key to AstroSizeWhitdwrfNeutstarQSO­v1s4

1. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 100%

+ b) 25%

­ c) 1%

­ d) 10%

­ e) 0.1%

2. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the distance to Sirius A

­ b) the "color" (spectral class) of Sirius B

­ c) the relative magnitude of Sirius B

+ d) all of these are true

­ e) the wobble of Sirius A

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) either cluster might be more distant

­ b) cluster B, because it exhibits a red Doppler shift

+ c) cluster A, because it exhibits greater angular expansion

­ d) cluster A, because it exhibits a blue Doppler shift

­ e) cluster B, because it exhibits less angular expansion

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4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) Cepheid variables

­ b) supernovae

+ c) entire galaxies

­ d) red giants

­ e) novae

5. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) electrons striking oxygen molecules, like a lava lamp

­ b) electrons striking hydrogen molecules, like a lava lamp

+ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ e) cyclotron motion, causing the electrons to strike oxygen molecules

6. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) doppler­shift...period­of­pulsation...temperature­luminosity

­ b) HR­diagram­location...X­ray­emmision...spectral­lines

­ c) x­ray­emmission...doppler­shift...rotation­rate

+ d) temperature­luminosity...redshift...quantum­theory­of­solids

­ e) all of these are true

7. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ b) the Doppler blue shift

­ c) the Gravitational blue shift

­ d) the same emission found in a Lava lamp (ultra­violet)

+ e) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

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8. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

+ a)

­ b)

­ c)

­ d)

­ e)

9. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extendsfarther into space by a factor of

+ a) 10

­ b) 1000

­ c) 100

­ d) 10,000

­ e) 100,000

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10. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

­ a) 2

­ b) 8

­ c) 4

+ d) 6

­ e) 3

11.

What best explains this figure?

­ a) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

­ b) The photon slows down, by the Doppler shift, c=fλ, andtherefore by E=hf it turns red.

+ c) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ d) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increaseswavelength and turns red.

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) entire galaxies

­ b) red giants

­ c) novae

­ d) Cepheid variables

+ e) supernovae

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13. This light clock is associated with

+ a) special relativity

­ b) doppler shift

­ c) gravitational shift

­ d) general relativity

­ e) all of these are true

14. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) Special relativity is valid only for objects travelling in avacuum.

­ b) The observer on the ground would perceive the width thetrain to be smaller.

+ c) The observer on the ground would perceive the ball to be travelling faster.

­ d) The observer on the ground would perceive the ball to be travelling more slowly.

­ e) The observer on the ground would perceive the width the train to be greater.

15. At the center of the Crab nebula is

­ a)d) a neutron star

­ b)c) none of these is correct

­ c)e) the remnants of a supernova

­ d)b) a pulsar

+ e)a) all of these is correct

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16. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the expansion of the universe

+ b) the gravitational redshift

­ c) the doppler shift

­ d) the mass as measured by Kepler's third law (modified by Newton)

­ e) the temperature

17. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting one of the first star charts

­ b) Looking for lobsters

­ c) Attempting to count asteroids

+ d) Looking for a comet that he knew would be appearing in that part of the sky.

­ e) Trying to measure the orbital radius of a planet

18. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

+ a) chimps typing Shakespeare

­ b) recalibration of supernovae luminosity

­ c) recalibration of supernovae relative magnitude

­ d) cosmic redshift

­ e) cosmic expansion

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19. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 2 cm (half of yours)

­ b) expansion from 1 cm to 8 cm (twice yours).

­ c) expansion from 1 cm to 3 cm (since 3­1=2)

­ d) expansion from 1 cm to 9 cm (since 5­1=4)

+ e) expansion from 1 cm to 4 cm (just like yours).

20.

This spectrum of the star Vega suggests that

­ a) it is an approximate black body

+ b) all of these are true

­ c) it's surface can be associated with a range oftemperatures

­ d) it can be associated with an "effective" temperature

­ e) if is not really a black body

21. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

+ a) 8

­ b) 2

­ c) 6

­ d) 4

­ e) 3

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AstroSizeWhitdwrfNeutstarQSO­v2s4

1. At the center of the Crab nebula is

___ a)c) none of these is correct

___ b)b) a pulsar

___ c)d) a neutron star

___ d)e) the remnants of a supernova

___ e)a) all of these is correct

2.

This spectrum of the star Vega suggests that

___ a) all of these are true

___ b) it is an approximate black body

___ c) if is not really a black body

___ d) it can be associated with an "effective" temperature

___ e) it's surface can be associated with a range of temperatures

3. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 25%

___ b) 1%

___ c) 100%

___ d) 0.1%

___ e) 10%

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4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) supernovae

___ b) novae

___ c) entire galaxies

___ d) Cepheid variables

___ e) red giants

5. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the relative magnitude of Sirius B

___ b) the distance to Sirius A

___ c) the wobble of Sirius A

___ d) all of these are true

___ e) the "color" (spectral class) of Sirius B

6. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

___ a) 3

___ b) 8

___ c) 2

___ d) 6

___ e) 4

7. This light clock is associated with

___ a) special relativity

___ b) all of these are true

___ c) general relativity

___ d) doppler shift

___ e) gravitational shift

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8. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) recalibration of supernovae relative magnitude

___ b) cosmic redshift

___ c) recalibration of supernovae luminosity

___ d) chimps typing Shakespeare

___ e) cosmic expansion

9. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) either cluster might be more distant

___ b) cluster B, because it exhibits less angular expansion

___ c) cluster A, because it exhibits greater angular expansion

___ d) cluster B, because it exhibits a red Doppler shift

___ e) cluster A, because it exhibits a blue Doppler shift

10. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Trying to measure the orbital radius of a planet

___ b) Attempting to count asteroids

___ c) Looking for a comet that he knew would be appearing in that part of the sky.

___ d) Attempting one of the first star charts

___ e) Looking for lobsters

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11. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) supernovae

___ b) red giants

___ c) entire galaxies

___ d) Cepheid variables

___ e) novae

12. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

___ a) 1000

___ b) 100

___ c) 100,000

___ d) 10

___ e) 10,000

13. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

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14. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the doppler shift

___ b) the gravitational redshift

___ c) the mass as measured by Kepler's third law (modified by Newton)

___ d) the temperature

___ e) the expansion of the universe

15. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ c) the Doppler blue shift

___ d) the same emission found in a Lava lamp (ultra­violet)

___ e) the Gravitational blue shift

16.

What best explains this figure?

___ a) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

___ d) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increases wavelengthand turns red.

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17. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) HR­diagram­location...X­ray­emmision...spectral­lines

___ b) doppler­shift...period­of­pulsation...temperature­luminosity

___ c) temperature­luminosity...redshift...quantum­theory­of­solids

___ d) all of these are true

___ e) x­ray­emmission...doppler­shift...rotation­rate

18. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 8 cm (twice yours).

___ b) expansion from 1 cm to 4 cm (just like yours).

___ c) expansion from 1 cm to 9 cm (since 5­1=4)

___ d) expansion from 1 cm to 2 cm (half of yours)

___ e) expansion from 1 cm to 3 cm (since 3­1=2)

19. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) cyclotron motion, causing the electrons to strike oxygen molecules

___ b) electrons striking hydrogen molecules, like a lava lamp

___ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ e) electrons striking oxygen molecules, like a lava lamp

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20. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

___ a) 3

___ b) 6

___ c) 8

___ d) 4

___ e) 2

21. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the ball to betravelling more slowly.

___ b) The observer on the ground would perceive the width the trainto be greater.

___ c) Special relativity is valid only for objects travelling in a vacuum.

___ d) The observer on the ground would perceive the width the train to be smaller.

___ e) The observer on the ground would perceive the ball to be travelling faster.

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Key to AstroSizeWhitdwrfNeutstarQSO­v2s4

1. At the center of the Crab nebula is

­ a)c) none of these is correct

­ b)b) a pulsar

­ c)d) a neutron star

­ d)e) the remnants of a supernova

+ e)a) all of these is correct

2.

This spectrum of the star Vega suggests that

+ a) all of these are true

­ b) it is an approximate black body

­ c) if is not really a black body

­ d) it can be associated with an "effective" temperature

­ e) it's surface can be associated with a range of temperatures

3. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

+ a) 25%

­ b) 1%

­ c) 100%

­ d) 0.1%

­ e) 10%

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4. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) supernovae

­ b) novae

+ c) entire galaxies

­ d) Cepheid variables

­ e) red giants

5. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the relative magnitude of Sirius B

­ b) the distance to Sirius A

­ c) the wobble of Sirius A

+ d) all of these are true

­ e) the "color" (spectral class) of Sirius B

6. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

­ a) 3

+ b) 8

­ c) 2

­ d) 6

­ e) 4

7. This light clock is associated with

+ a) special relativity

­ b) all of these are true

­ c) general relativity

­ d) doppler shift

­ e) gravitational shift

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8. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) recalibration of supernovae relative magnitude

­ b) cosmic redshift

­ c) recalibration of supernovae luminosity

+ d) chimps typing Shakespeare

­ e) cosmic expansion

9. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) either cluster might be more distant

­ b) cluster B, because it exhibits less angular expansion

+ c) cluster A, because it exhibits greater angular expansion

­ d) cluster B, because it exhibits a red Doppler shift

­ e) cluster A, because it exhibits a blue Doppler shift

10. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Trying to measure the orbital radius of a planet

­ b) Attempting to count asteroids

+ c) Looking for a comet that he knew would be appearing in that part of the sky.

­ d) Attempting one of the first star charts

­ e) Looking for lobsters

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11. The course materials present two cosmic expansion plots. The more recent (2007) plot used

+ a) supernovae

­ b) red giants

­ c) entire galaxies

­ d) Cepheid variables

­ e) novae

12. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

­ a) 1000

­ b) 100

­ c) 100,000

+ d) 10

­ e) 10,000

13. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

­ c)

­ d)

+ e)

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14. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the doppler shift

+ b) the gravitational redshift

­ c) the mass as measured by Kepler's third law (modified by Newton)

­ d) the temperature

­ e) the expansion of the universe

15. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

+ b) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ c) the Doppler blue shift

­ d) the same emission found in a Lava lamp (ultra­violet)

­ e) the Gravitational blue shift

16.

What best explains this figure?

­ a) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

+ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ c) The photon slows down as it goes uphill, and by c=fλ it increaseswavelength therefore by E=hf, it turns red.

­ d) The photon slows down, by the Doppler shift, c=fλ, andtherefore by E=hf it turns red.

­ e) The photon loses energy, not speed. By c=fλ , it loses frequency, and by E=hf it increaseswavelength and turns red.

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17. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) HR­diagram­location...X­ray­emmision...spectral­lines

­ b) doppler­shift...period­of­pulsation...temperature­luminosity

+ c) temperature­luminosity...redshift...quantum­theory­of­solids

­ d) all of these are true

­ e) x­ray­emmission...doppler­shift...rotation­rate

18. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 8 cm (twice yours).

+ b) expansion from 1 cm to 4 cm (just like yours).

­ c) expansion from 1 cm to 9 cm (since 5­1=4)

­ d) expansion from 1 cm to 2 cm (half of yours)

­ e) expansion from 1 cm to 3 cm (since 3­1=2)

19. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) cyclotron motion, causing the electrons to strike oxygen molecules

­ b) electrons striking hydrogen molecules, like a lava lamp

+ c) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ e) electrons striking oxygen molecules, like a lava lamp

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20. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

­ a) 3

+ b) 6

­ c) 8

­ d) 4

­ e) 2

21. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the ball to betravelling more slowly.

­ b) The observer on the ground would perceive the width thetrain to be greater.

­ c) Special relativity is valid only for objects travelling in a vacuum.

­ d) The observer on the ground would perceive the width the train to be smaller.

+ e) The observer on the ground would perceive the ball to be travelling faster.

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AstroSizeWhitdwrfNeutstarQSO­v1s5

1. This light clock is associated with

___ a) general relativity

___ b) all of these are true

___ c) doppler shift

___ d) gravitational shift

___ e) special relativity

2. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

___ a) 2

___ b) 4

___ c) 8

___ d) 3

___ e) 6

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster B, because it exhibits a red Doppler shift

___ b) cluster A, because it exhibits greater angular expansion

___ c) cluster B, because it exhibits less angular expansion

___ d) either cluster might be more distant

___ e) cluster A, because it exhibits a blue Doppler shift

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4. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

___ a) 8

___ b) 4

___ c) 3

___ d) 2

___ e) 6

5. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 10%

___ b) 1%

___ c) 0.1%

___ d) 100%

___ e) 25%

6. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Looking for a comet that he knew would be appearing in that part of the sky.

___ b) Attempting one of the first star charts

___ c) Looking for lobsters

___ d) Trying to measure the orbital radius of a planet

___ e) Attempting to count asteroids

7. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) entire galaxies

___ b) Cepheid variables

___ c) red giants

___ d) supernovae

___ e) novae

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8. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

9. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 3 cm (since 3­1=2)

___ b) expansion from 1 cm to 2 cm (half of yours)

___ c) expansion from 1 cm to 4 cm (just like yours).

___ d) expansion from 1 cm to 8 cm (twice yours).

___ e) expansion from 1 cm to 9 cm (since 5­1=4)

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10. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) temperature­luminosity...redshift...quantum­theory­of­solids

___ b) x­ray­emmission...doppler­shift...rotation­rate

___ c) all of these are true

___ d) doppler­shift...period­of­pulsation...temperature­luminosity

___ e) HR­diagram­location...X­ray­emmision...spectral­lines

11. At the center of the Crab nebula is

___ a)c) none of these is correct

___ b)d) a neutron star

___ c)e) the remnants of a supernova

___ d)a) all of these is correct

___ e)b) a pulsar

12. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) cosmic expansion

___ b) recalibration of supernovae relative magnitude

___ c) cosmic redshift

___ d) chimps typing Shakespeare

___ e) recalibration of supernovae luminosity

13. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

___ a) 10,000

___ b) 100,000

___ c) 100

___ d) 10

___ e) 1000

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14. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) red giants

___ b) Cepheid variables

___ c) novae

___ d) entire galaxies

___ e) supernovae

15. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the doppler shift

___ b) the expansion of the universe

___ c) the temperature

___ d) the gravitational redshift

___ e) the mass as measured by Kepler's third law (modified by Newton)

16.

This spectrum of the star Vega suggests that

___ a) it can be associated with an "effective" temperature

___ b) it's surface can be associated with a range of temperatures

___ c) if is not really a black body

___ d) it is an approximate black body

___ e) all of these are true

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17.

What best explains this figure?

___ a) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ c) The photon loses energy, not speed. By E=hf, it loses frequency, andby c=fλ it increases wavelength and turns red.

___ d) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

18. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ b) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ c) cyclotron motion, causing the electrons to strike oxygen molecules

___ d) electrons striking oxygen molecules, like a lava lamp

___ e) electrons striking hydrogen molecules, like a lava lamp

19. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) the wobble of Sirius A

___ b) the relative magnitude of Sirius B

___ c) the "color" (spectral class) of Sirius B

___ d) all of these are true

___ e) the distance to Sirius A

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20. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the width the trainto be smaller.

___ b) Special relativity is valid only for objects travelling in avacuum.

___ c) The observer on the ground would perceive the ball to be travelling faster.

___ d) The observer on the ground would perceive the ball to be travelling more slowly.

___ e) The observer on the ground would perceive the width the train to be greater.

21. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the same emission found in a Lava lamp (ultra­violet)

___ c) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ d) the Gravitational blue shift

___ e) the Doppler blue shift

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Key to AstroSizeWhitdwrfNeutstarQSO­v1s5

1. This light clock is associated with

­ a) general relativity

­ b) all of these are true

­ c) doppler shift

­ d) gravitational shift

+ e) special relativity

2. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?

­ a) 2

­ b) 4

+ c) 8

­ d) 3

­ e) 6

3. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) cluster B, because it exhibits a red Doppler shift

+ b) cluster A, because it exhibits greater angular expansion

­ c) cluster B, because it exhibits less angular expansion

­ d) either cluster might be more distant

­ e) cluster A, because it exhibits a blue Doppler shift

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4. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distanceof 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?

­ a) 8

­ b) 4

­ c) 3

­ d) 2

+ e) 6

5. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 10%

­ b) 1%

­ c) 0.1%

­ d) 100%

+ e) 25%

6. What was Messier doing when he independently rediscovered the Crab in 1758?

+ a) Looking for a comet that he knew would be appearing in that part of the sky.

­ b) Attempting one of the first star charts

­ c) Looking for lobsters

­ d) Trying to measure the orbital radius of a planet

­ e) Attempting to count asteroids

7. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) entire galaxies

­ b) Cepheid variables

­ c) red giants

+ d) supernovae

­ e) novae

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8. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period.

And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

+ b)

­ c)

­ d)

­ e)

9. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisinoriginally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life issituated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisinview an expansion of a raisin 1 cm away?

­ a) expansion from 1 cm to 3 cm (since 3­1=2)

­ b) expansion from 1 cm to 2 cm (half of yours)

+ c) expansion from 1 cm to 4 cm (just like yours).

­ d) expansion from 1 cm to 8 cm (twice yours).

­ e) expansion from 1 cm to 9 cm (since 5­1=4)

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10. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

+ a) temperature­luminosity...redshift...quantum­theory­of­solids

­ b) x­ray­emmission...doppler­shift...rotation­rate

­ c) all of these are true

­ d) doppler­shift...period­of­pulsation...temperature­luminosity

­ e) HR­diagram­location...X­ray­emmision...spectral­lines

11. At the center of the Crab nebula is

­ a)c) none of these is correct

­ b)d) a neutron star

­ c)e) the remnants of a supernova

+ d)a) all of these is correct

­ e)b) a pulsar

12. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) cosmic expansion

­ b) recalibration of supernovae relative magnitude

­ c) cosmic redshift

+ d) chimps typing Shakespeare

­ e) recalibration of supernovae luminosity

13. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

­ a) 10,000

­ b) 100,000

­ c) 100

+ d) 10

­ e) 1000

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14. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) red giants

­ b) Cepheid variables

­ c) novae

+ d) entire galaxies

­ e) supernovae

15. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the doppler shift

­ b) the expansion of the universe

­ c) the temperature

+ d) the gravitational redshift

­ e) the mass as measured by Kepler's third law (modified by Newton)

16.

This spectrum of the star Vega suggests that

­ a) it can be associated with an "effective" temperature

­ b) it's surface can be associated with a range oftemperatures

­ c) if is not really a black body

­ d) it is an approximate black body

+ e) all of these are true

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17.

What best explains this figure?

­ a) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

­ b) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

+ c) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ d) The photon slows down, by the Doppler shift, c=fλ, andtherefore by E=hf it turns red.

­ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

18. What causes the "finger­like" filamentary structure in the Crab nebula?

­ a) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

+ b) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ c) cyclotron motion, causing the electrons to strike oxygen molecules

­ d) electrons striking oxygen molecules, like a lava lamp

­ e) electrons striking hydrogen molecules, like a lava lamp

19. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

­ a) the wobble of Sirius A

­ b) the relative magnitude of Sirius B

­ c) the "color" (spectral class) of Sirius B

+ d) all of these are true

­ e) the distance to Sirius A

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20. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the width thetrain to be smaller.

­ b) Special relativity is valid only for objects travelling in avacuum.

+ c) The observer on the ground would perceive the ball to be travelling faster.

­ d) The observer on the ground would perceive the ball to be travelling more slowly.

­ e) The observer on the ground would perceive the width the train to be greater.

21. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ b) the same emission found in a Lava lamp (ultra­violet)

+ c) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ d) the Gravitational blue shift

­ e) the Doppler blue shift

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AstroSizeWhitdwrfNeutstarQSO­v2s5

1.

This spectrum of the star Vega suggests that

___ a) if is not really a black body

___ b) it is an approximate black body

___ c) it can be associated with an "effective" temperature

___ d) it's surface can be associated with a range of temperatures

___ e) all of these are true

2. This light clock is associated with

___ a) doppler shift

___ b) special relativity

___ c) gravitational shift

___ d) general relativity

___ e) all of these are true

3. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

___ a) cosmic redshift

___ b) chimps typing Shakespeare

___ c) cosmic expansion

___ d) recalibration of supernovae luminosity

___ e) recalibration of supernovae relative magnitude

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4. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

___ a) the doppler shift

___ b) the expansion of the universe

___ c) the mass as measured by Kepler's third law (modified by Newton)

___ d) the gravitational redshift

___ e) the temperature

5. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

___ a) 100%

___ b) 0.1%

___ c) 25%

___ d) 10%

___ e) 1%

6. What was Messier doing when he independently rediscovered the Crab in 1758?

___ a) Attempting one of the first star charts

___ b) Trying to measure the orbital radius of a planet

___ c) Looking for lobsters

___ d) Attempting to count asteroids

___ e) Looking for a comet that he knew would be appearing in that part of the sky.

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7.

What best explains this figure?

___ a) The photon slows down, by the Doppler shift, E=hf, and thereforeby c=f&;lambda it turns red.

___ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

___ c) The photon slows down, by the Doppler shift, c=fλ, and therefore byE=hf it turns red.

___ d) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

___ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

8. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

___ a) The observer on the ground would perceive the ball to betravelling more slowly.

___ b) The observer on the ground would perceive the width the trainto be greater.

___ c) Special relativity is valid only for objects travelling in a vacuum.

___ d) The observer on the ground would perceive the width the train to be smaller.

___ e) The observer on the ground would perceive the ball to be travelling faster.

9. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

___ a) all of these are true

___ b) the distance to Sirius A

___ c) the wobble of Sirius A

___ d) the relative magnitude of Sirius B

___ e) the "color" (spectral class) of Sirius B

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10. At the center of the Crab nebula is

___ a)c) none of these is correct

___ b)d) a neutron star

___ c)a) all of these is correct

___ d)e) the remnants of a supernova

___ e)b) a pulsar

11. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

___ a) 1000

___ b) 10,000

___ c) 10

___ d) 100,000

___ e) 100

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

___ a) novae

___ b) Cepheid variables

___ c) red giants

___ d) supernovae

___ e) entire galaxies

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13. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

___ a)

___ b)

___ c)

___ d)

___ e)

14. What causes the "finger­like" filamentary structure in the Crab nebula?

___ a) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

___ b) electrons striking hydrogen molecules, like a lava lamp

___ c) electrons striking oxygen molecules, like a lava lamp

___ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

___ e) cyclotron motion, causing the electrons to strike oxygen molecules

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15. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

___ a) 8

___ b) 4

___ c) 6

___ d) 3

___ e) 2

16. What causes the blue glow of the Crab nebula?

___ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

___ b) the Doppler blue shift

___ c) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

___ d) the Gravitational blue shift

___ e) the same emission found in a Lava lamp (ultra­violet)

17. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

___ a) cluster B, because it exhibits less angular expansion

___ b) cluster A, because it exhibits greater angular expansion

___ c) cluster B, because it exhibits a red Doppler shift

___ d) cluster A, because it exhibits a blue Doppler shift

___ e) either cluster might be more distant

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18. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

___ a) 4

___ b) 3

___ c) 8

___ d) 6

___ e) 2

19. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

___ a) x­ray­emmission...doppler­shift...rotation­rate

___ b) HR­diagram­location...X­ray­emmision...spectral­lines

___ c) temperature­luminosity...redshift...quantum­theory­of­solids

___ d) all of these are true

___ e) doppler­shift...period­of­pulsation...temperature­luminosity

20. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

___ a) red giants

___ b) supernovae

___ c) entire galaxies

___ d) Cepheid variables

___ e) novae

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21. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

___ a) expansion from 1 cm to 4 cm (just like yours).

___ b) expansion from 1 cm to 3 cm (since 3­1=2)

___ c) expansion from 1 cm to 9 cm (since 5­1=4)

___ d) expansion from 1 cm to 8 cm (twice yours).

___ e) expansion from 1 cm to 2 cm (half of yours)

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Key to AstroSizeWhitdwrfNeutstarQSO­v2s5

1.

This spectrum of the star Vega suggests that

­ a) if is not really a black body

­ b) it is an approximate black body

­ c) it can be associated with an "effective" temperature

­ d) it's surface can be associated with a range of temperatures

+ e) all of these are true

2. This light clock is associated with

­ a) doppler shift

+ b) special relativity

­ c) gravitational shift

­ d) general relativity

­ e) all of these are true

3. In one respect, the universie is arguably "young", considering how much complexity it contains. This is oftenillustrated by a calculation of

­ a) cosmic redshift

+ b) chimps typing Shakespeare

­ c) cosmic expansion

­ d) recalibration of supernovae luminosity

­ e) recalibration of supernovae relative magnitude

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4. Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found from

­ a) the doppler shift

­ b) the expansion of the universe

­ c) the mass as measured by Kepler's third law (modified by Newton)

+ d) the gravitational redshift

­ e) the temperature

5. As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately,

­ a) 100%

­ b) 0.1%

+ c) 25%

­ d) 10%

­ e) 1%

6. What was Messier doing when he independently rediscovered the Crab in 1758?

­ a) Attempting one of the first star charts

­ b) Trying to measure the orbital radius of a planet

­ c) Looking for lobsters

­ d) Attempting to count asteroids

+ e) Looking for a comet that he knew would be appearing in that part of the sky.

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7.

What best explains this figure?

­ a) The photon slows down, by the Doppler shift, E=hf, andtherefore by c=f&;lambda it turns red.

+ b) The photon loses energy, not speed. By E=hf, it loses frequency,and by c=fλ it increases wavelength and turns red.

­ c) The photon slows down, by the Doppler shift, c=fλ, and thereforeby E=hf it turns red.

­ d) The photon loses energy, not speed. By c=fλ , it loses frequency,and by E=hf it increases wavelength and turns red.

­ e) The photon slows down as it goes uphill, and by c=fλ it increases wavelength therefore by E=hf, itturns red.

8. Suppose the light clock involved a ball being tossed back and forth on atrain going just under the speed of sound. In contrast to the situation forlight reflecting back and forth on a train going just under the speed of light,there is virtually no time dilation. Why?

­ a) The observer on the ground would perceive the ball to betravelling more slowly.

­ b) The observer on the ground would perceive the width thetrain to be greater.

­ c) Special relativity is valid only for objects travelling in a vacuum.

­ d) The observer on the ground would perceive the width the train to be smaller.

+ e) The observer on the ground would perceive the ball to be travelling faster.

9. Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the sizeof the earth, but typically has the same mass as the Sun.

+ a) all of these are true

­ b) the distance to Sirius A

­ c) the wobble of Sirius A

­ d) the relative magnitude of Sirius B

­ e) the "color" (spectral class) of Sirius B

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10. At the center of the Crab nebula is

­ a)c) none of these is correct

­ b)d) a neutron star

+ c)a) all of these is correct

­ d)e) the remnants of a supernova

­ e)b) a pulsar

11. Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latterextends farther into space by a factor of

­ a) 1000

­ b) 10,000

+ c) 10

­ d) 100,000

­ e) 100

12. The course materials present two cosmic expansion plots. The more recent (2007) plot used

­ a) novae

­ b) Cepheid variables

­ c) red giants

+ d) supernovae

­ e) entire galaxies

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13. is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is

period. And, .

You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnantthat closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of thenebula might be. You know both the period of the pulsar, as well as , which represents the amount of time youthink the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you writeon your napkin?

­ a)

­ b)

+ c)

­ d)

­ e)

14. What causes the "finger­like" filamentary structure in the Crab nebula?

+ a) a light(low density) fluid underneath a heavy(high density) fluid, like a lava lamp

­ b) electrons striking hydrogen molecules, like a lava lamp

­ c) electrons striking oxygen molecules, like a lava lamp

­ d) a heavy (high density) fluid underneath a light (low density) fluid, like a lava lamp

­ e) cyclotron motion, causing the electrons to strike oxygen molecules

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15. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cmexpand?

­ a) 8

­ b) 4

+ c) 6

­ d) 3

­ e) 2

16. What causes the blue glow of the Crab nebula?

­ a) the curving motion of electrons in a magnetic field; such motion traps ultra­violet and blue light

­ b) the Doppler blue shift

+ c) the curving motion of electrons in a magnetic field; such motion resembles a radio antenna

­ d) the Gravitational blue shift

­ e) the same emission found in a Lava lamp (ultra­violet)

17. One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion tothe spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity.Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer?

­ a) cluster B, because it exhibits less angular expansion

+ b) cluster A, because it exhibits greater angular expansion

­ c) cluster B, because it exhibits a red Doppler shift

­ d) cluster A, because it exhibits a blue Doppler shift

­ e) either cluster might be more distant

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18. Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at adistance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cmexpand?

­ a) 4

­ b) 3

+ c) 8

­ d) 6

­ e) 2

19. The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth.Which best summarizes them?

­ a) x­ray­emmission...doppler­shift...rotation­rate

­ b) HR­diagram­location...X­ray­emmision...spectral­lines

+ c) temperature­luminosity...redshift...quantum­theory­of­solids

­ d) all of these are true

­ e) doppler­shift...period­of­pulsation...temperature­luminosity

20. The course materials present two cosmic expansion plots. Hubble's original (1929) plot used

­ a) red giants

­ b) supernovae

+ c) entire galaxies

­ d) Cepheid variables

­ e) novae

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21. You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location araisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligentlife is situated exactly halfway between your (central) location and the edge. How would this second "intelligent"raisin view an expansion of a raisin 1 cm away?

+ a) expansion from 1 cm to 4 cm (just like yours).

­ b) expansion from 1 cm to 3 cm (since 3­1=2)

­ c) expansion from 1 cm to 9 cm (since 5­1=4)

­ d) expansion from 1 cm to 8 cm (twice yours).

­ e) expansion from 1 cm to 2 cm (half of yours)

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Attribution (for quiz questions) under CC­by­SA license

http://en.wikiversity.org/w/index.php?title=Astronomy_college_course/Sizes_of_white_dwarfs,_neutron_stars,_quasars/questions&oldid=1389043

Study guide

https://en.wikiversity.org/w/index.php?title=Astronomy_college_course/Sizes_of_white_dwarfs,_neutron_stars,_quasars&oldid=1286949

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