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Integrated Coordinated Science for the 21st Century

Active Physics
+ Chapter 6
Is Anyone Out There?
Answers
Physics To Go
  1. The speed of light is too large for Galileo to have measured. If the hilltops were a few hundred meters apart, the travel-time for light is only about one millionth of a second. Human reaction time is at least a half a second. The only delay Galileo was able to observe was due to the reaction time of his assistant.
  2. a) The estimate for the wavelength is 1.0 X 10-6 m. In fact, wavelengths of visible light range from about .40 X 10-6 m to .75 X 10-6 m.
    b) From c = λ f, the frequency is 3 X 1014 Hz.
  3. a-b) See chart below.

    AM radio:
    FM radio/commercial TV:
    radar:
    microwaves:
    infrared radiation:
    light:
    ultraviolet radiation:
    x-rays:
    gamma rays:
    3 x 102 m
    3 m
    0.3 m
    0.03 m
    3 x 10-4 m
    5 x 10-7 m
    3 x 10-8 m
    3 x 10-10m
    3 x 10-13 m

  4. See chart below.

    From—To
    Earth to Moon
    Earth to Sun
    Sun to Pluto
    Sun to nearest star
    light travel-time
    1.2 s
    500s = 8.3 min
    2.0 x104 s = 5.6 hr
    1.4 x 108 s = 4.3 light-years

    Note: The number of seconds in a year is 60 X 60 X 24 X 365 = 3.2 X 107 s. To find the travel-time to the nearest star in light-years, divide 1.4 X 108 s by 3.2 X 107 s.
  5. a) 1.6 X 10-5 s
    b) No. The travel time was much too short.
  6. Not necessarily. If extraterrestrials could see microwaves, their eyes would be much larger than ours.
  7. We can choose a frequency that penetrates space well, like microwaves. We can choose a frequency that is near (or perhaps a multiple of) 1420 MHz, which is the frequency of microwave radiation given off by the hydrogen atom.