Science 9: Unit E: Space Exploration - PowerPoint PPT Presentation

1 / 6
About This Presentation
Title:

Science 9: Unit E: Space Exploration

Description:

Science 9: Unit E: Space Exploration Topic 5: What Channel is That? Electromagnetic Radiation Light is one kind of electromagnetic radiation (EMR). – PowerPoint PPT presentation

Number of Views:40
Avg rating:3.0/5.0
Slides: 7
Provided by: Nelso140
Category:

less

Transcript and Presenter's Notes

Title: Science 9: Unit E: Space Exploration


1
Science 9 Unit E Space Exploration
  • Topic 5 What Channel is That?

2
Electromagnetic Radiation
  • Light is one kind of electromagnetic radiation
    (EMR). Stars and other celestial objects give off
    all kinds of EMR the Sun sends out infrared
    radiation which warms the Earth, UV radiation
    which tans/burns our skin, and radio waves which
    we detect as static on our radios.

3
History of Radio Astronomy
  • Radio astronomy is the studying of radio waves
    given off by these celestial objects in order to
    learn more about them.
  • In the 1930s telephone engineers noticed that
    there was a constant source of background radio
    radiation which interfered with their equipment.
    Karl Jansky built a radio antenna to study these
    signals and concluded that the signals came from
    outer space.
  • Grote Reber, using a radio dish, discovered that
    certain areas in the sky gave off especially
    strong radio signals. Reber noted that the
    strongest radio signal came from the Sun,
    followed by Jupiter. He also noticed that outside
    the solar system, the strongest signal came from
    the center of the Milky Way Galaxy, full of
    stars. Objects that gave off especially strong
    signals were called Radio Objects.

4
Radio Astronomy Contd
  • Using radio waves to study celestial objects has
    one major disadvantage They dont produce as
    much detail as light. Our eyes cannot see radio
    waves so we lose information. A major advantage
    is that radio waves can travel farther because
    theyre larger and pass through dust clouds while
    light waves cannot.
  • Computers now produce images showing the strength
    of radio signals weak signals are bluish while
    stronger signals get redder and finally white.

5
Interferometry and the VLA
  • Interferometry The use of many telescopes
    combined together so that the many radio signals
    could be combined by computer to produce a much
    more detailed single signal. The biggest example
    of radio interferometry is the Very Large Array
    (VLA) in New Mexico. This array has been used to
    study radio signals from alien sources. So far no
    luck.

6
Very Long Baseline Interferometry (VLBI)
  • Very Long Baseline Interferometry (VLBI) A much
    larger and newer example of interferometry that
    relies on radio telescopes connected wirelessly
    over a much larger distance, even the entire
    planet.
Write a Comment
User Comments (0)
About PowerShow.com