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Galaxies

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Some quasars are among the most distant objects in the known universe. Which of the following statements about them must be correct? 17-6. – PowerPoint PPT presentation

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Title: Galaxies


1
Galaxies Review Questions!
2
  • 16-1.The stars in which type of galaxy can be
    uniformly distributed in a sphere?
  • a) elliptical
  • b) normal spiral
  • c) barred spiral
  • d) irregular

3
  • 16-1.The stars in which type of galaxy can be
    uniformly distributed in a sphere?
  • a) elliptical
  • b) normal spiral
  • c) barred spiral
  • d) irregular

4
  • 16-2. Which type of galaxy is presently the most
    commonly observed type?
  • a) normal spiral
  • b) barred spiral
  • c) elliptical
  • d) irregular

5
  • 16-2. Which type of galaxy is presently the most
    commonly observed type?
  • a) normal spiral
  • b) barred spiral
  • c) elliptical
  • d) irregular

6
  • 16-3. The smallest known galaxies are of which
    kind?
  • a) elliptical
  • b) barred spiral
  • c) normal spiral
  • d) irregular

7
  • 16-3. The smallest known galaxies are of which
    kind?
  • a) elliptical
  • b) barred spiral
  • c) normal spiral
  • d) irregular

8
16-12. Which type of galaxy has very little gas
or dust?
  • a) Elliptical
  • b) Spiral
  • c) Irregular
  • d) All of the above

9
16-12. Which type of galaxy has very little gas
or dust?
  • a) Elliptical
  • b) Spiral
  • c) Irregular
  • d) All of the above

10
  • 16-4. The largest known galaxies are of which
    kind?
  • a) elliptical
  • b) normal Spiral
  • c) barred Spiral
  • d) irregular

11
  • 16-4. The largest known galaxies are of which
    kind?
  • a) elliptical
  • b) normal Spiral
  • c) barred Spiral
  • d) irregular

12
  • 16-5. If a galaxy is moving away from us, its
    absorption lines will
  • a) change towards higher or lower wavelengths
    depending on the speed of the galaxy.
  • b) remain at the same wavelengths as lines from
    galaxies not moving away from us.
  • c) all change towards shorter wavelengths.
  • d) all change towards longer wavelengths.

13
  • 16-5. If a galaxy is moving away from us, its
    absorption lines will
  • a) change towards higher or lower wavelengths
    depending on the speed of the galaxy.
  • b) remain at the same wavelengths as lines from
    galaxies not moving away from us.
  • c) all change towards shorter wavelengths.
  • d) all change towards longer wavelengths.

14
  • 16-6. What is located between a disk galaxys
    spiral arms?
  • a) nothing
  • b) only interstellar gas and dust
  • c) almost as many stars as in the arms
  • d) more stars than are in the arms

15
  • 16-6. What is located between a disk galaxys
    spiral arms?
  • a) nothing
  • b) only interstellar gas and dust
  • c) almost as many stars as in the arms
  • d) more stars than are in the arms

16
16-7. Which observation correctly applies to
galaxies in other superclusters?
  • a) they are all moving towards us
  • b) they are all moving away from us
  • c) they are all larger than the Milky Way
  • d) they are all smaller than the Milky Way

17
16-7. Which observation correctly applies to
galaxies in other superclusters?
  • a) they are all moving towards us
  • b) they are all moving away from us
  • c) they are all larger than the Milky Way
  • d) they are all smaller than the Milky Way

18
16-8. Spiral density waves describe which of the
following?
  • a) the ripples seen in comet tails
  • b) the pulses of a pulsar
  • c) the belts and zones in Jupiters upper
    layers
  • d) ripples in the gas of our Galaxy

19
16-8. Spiral density waves describe which of the
following?
  • a) the ripples seen in comet tails
  • b) the pulses of a pulsar
  • c) the belts and zones in Jupiters upper
    layers
  • d) ripples in the gas of our Galaxy

20
16-9. The Andromeda galaxy, in our local
cluster, is
  • a) a spiral galaxy smaller than the Milky Way.
  • b) a spiral galaxy larger than the Milky Way.
  • c) an elliptical galaxy smaller than the Milky
    Way.
  • d) an elliptical galaxy larger than the Milky
    Way.

21
16-9. The Andromeda galaxy, in our local
cluster, is
  • a) a spiral galaxy smaller than the Milky Way.
  • b) a spiral galaxy larger than the Milky Way.
  • c) an elliptical galaxy smaller than the Milky
    Way.
  • d) an elliptical galaxy larger than the Milky
    Way.

22
16-10. Edwin Hubble first showed that Andromeda
was a distant galaxy by
  • a) measuring the distance to it using Cepheid
    variables.
  • b) measuring the distance to it using RR Lyrae
    variables.
  • c) precisely measuring its parallax angle.
  • d) observing nova in the galaxy.

23
16-10. Edwin Hubble first showed that Andromeda
was a distant galaxy by
  • a) measuring the distance to it using Cepheid
    variables.
  • b) measuring the distance to it using RR Lyrae
    variables.
  • c) precisely measuring its parallax angle.
  • d) observing nova in the galaxy.

24
Chapter 16 Thought/Writing Questions
  • 1. List three methods of determining distances
    in the universe.
  • 2. Why do spiral galaxies have spiral arms?

25
17-1. Some quasars are among the most distant
objects in the known universe. Which of the
following statements about them must be correct?
  • a) they have the highest blue shifts of any
    objects in the universe
  • b) they have the smallest blue shifts of any
    objects in the universe
  • c) they have the highest red shifts of any
    objects in the universe
  • d) they have the smallest red shifts of any
    objects in the universe

26
17-1. Some quasars are among the most distant
objects in the known universe. Which of the
following statements about them must be correct?
  • a) they have the highest blue shifts of any
    objects in the universe
  • b) they have the smallest blue shifts of any
    objects in the universe
  • c) they have the highest red shifts of any
    objects in the universe
  • d) they have the smallest red shifts of any
    objects in the universe

27
17-6. The time for a fluctuation in brightness
of a quasar allows astronomers to place an upper
limit on its
  • a) luminosity.
  • b) size.
  • c) age.
  • d) distance.

28
17-6. The time for a fluctuation in brightness
of a quasar allows astronomers to place an upper
limit on its
  • a) luminosity.
  • b) size.
  • c) age.
  • d) distance.
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