The Solar System

(Marvins-Underground-K-12) #1
74 PART 1^ |^ EXPLORING THE SKY


  1. Galileo’s telescopes were not of high quality by modern standards. He
    was able to see the moons of Jupiter, but he never reported seeing
    features on Mars. Use the small-angle formula to fi nd the angular
    diameter of Mars when it is closest to Earth. How does that compare
    with the maximum angular diameter of Jupiter?


Learning to Look



  1. Study Figure 4-11 and describe the phases that Venus would have
    displayed to Galileo’s telescope if the Tychonic universe had been
    correct.

  2. What three astronomical objects are represented here? What are the
    two rings?

  3. Use the fi gure below to explain how the Ptolemaic model treated some
    planets differently from the rest. How did the Copernican model treat all
    of the planets the same?


Discussion Questions



  1. Historian of science Thomas Kuhn has said that De Revolutionibus was
    a revolution-making book but not a revolutionary book. How was it an
    old-fashioned, classical book?

  2. Why might Tycho Brahe have hesitated to hire Kepler? Why do you
    suppose he appointed Kepler his scientifi c heir?

  3. How does the modern controversy over creationism and evolution
    refl ect two ways of knowing about the physical world?


Problems



  1. Draw and label a diagram of the eastern horizon from northeast to
    southeast and label the rising point of the sun at the solstices and
    equinoxes. (See page 19 and Figure 4-1.)

  2. If you lived on Mars, which planets would exhibit retrograde motion?
    Which would never be visible as crescent phases?

  3. If a planet has an average distance from the sun of 4 AU, what is its
    orbital period?

  4. If a space probe is sent into an orbit around the sun that brings it
    as close as 0.5 AU and as far away as 5.5 AU, what will be its orbital
    period?

  5. Neptune orbits the sun with a period of 164.8 years. What is its
    average distance from the sun?

  6. Galileo’s telescope showed him that Venus has a large angular
    diameter (61 arc seconds) when it is a crescent and a small angular
    diameter (10 arc seconds) when it is nearly full. Use the small-angle
    formula to fi nd the ratio of its maximum distance to its minimum
    distance. Is this ratio compatible with the Ptolemaic universe shown
    on page 57?

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