Cuesta College :: Astronomy 10 :: Fall 2007
Calendar Policies Goals Grades
    Quiz 1
    Quiz 2
    Quiz 3
    Midterm 1
    Quiz 4
    Quiz 5
    Quiz 6
    Midterm 2
    Quiz 7
    Quiz 8
    Quiz 9
    Midterm 3
    Quiz 10
    Quiz 11
    Quiz 12
    Final Exam


Supplemental materials for these learning goals will be added frequently.


Quiz 11 Learning Goals and Supplemental Resources
[Fix, Astronomy: Journey to the Cosmic Frontier, 4/e, Chapter 22]
[Reading guide (*.pdf)
[CPS inquiry questions (*.pdf)]
[CPS review questions (*.pdf)]
  1. Provide and explain the evidence for interstellar gas and dust, and understand the processes that produce its observed features.
  2. Provide and explain the evidence for the spiral arm structure of the Milky Way, and "dark matter."
    • In-class activity 26, The Milky Way--How Big/How Distant? (*.pdf)
      Discuss what features in/outside of the Milky Way can be seen, whether in the disk itself, or lying above/below the plane of the disk.
    • Fig. 22.28 from Fix, Astronomy, Journey to the Cosmic Frontier, 4/e (*.gif)
      The overall structure of the Milky Way.   Note that the size of the galaxy here is given as 40 kiloparsecs, or 130,400 light years; which is only approximately known (compare to the Lecture-Tutorials value of 100,000 light years!).
    • Fig. 22.23, ibid (*.gif)
      Evidence for the flattened disk shape of the Milky Way, from star distributions in different directions.
    • Fig. 22.26, ibid (*.gif)
      Evidence for the overall size of the Milky Way, from globular cluster positions.
    • Fig. 22.33, ibid (*.gif)
      Local spiral arm tracer evidence.
    • Fig. 22.35, ibid (*.gif)
      Evidence from radio waves emitted by CO molecules (using a technique similar to the detection of 21 cm radio waves emitted by hydrogen atoms).
    • Fig. 22.29, ibid (*.gif)
      Comparing rotation curves of two extreme cases.
    • Fig. 22.30, ibid (*.gif)
      Graph of the rotation curve of the Milky Way Galaxy.
    • Dark matter as plot device, Futurama, "Love's Labours Lost in Space" (*.jpeg)
      Tongue-in-cheek interpretation of dark matter as extremely dense alien feces.
    • NASA Astronomy Picture of the Day:
    • Websites:
      • Dark Matter Interactive (*.swf)
        Use this simulation to produce various rotation curves given the presence or absence of dark matter (McGraw-Hill Publishers).
      • PlanetQuest 3D Guide to the Galaxy (*.js)
        Interactive model of the Milky Way.   Note that their estimate of its diameter is 100,000 light years, and that the nucleus has a barred structure (Jet Propulsion Laboratory, NASA).
      • Multi-ending MAD Magazine flexidisc
        Eight nested spirals in this record allows for different versions of the same song on the same record.

  3. Understand the processes that produce the spiral arms of the Milky Way.
  4. Provide and describe evidence for a massive black hole at the center of the Milky Way.
  5. Provide and explain the evidence for the processes that formed the Milky Way (halo clusters versus disk stars, metal-poor versus metal-rich, spherical versus flat/thin).

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