Pre-lab PowerPoint Lesson for S.W.A.T. E-lab PowerPoint PPT Presentation

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Title: Pre-lab PowerPoint Lesson for S.W.A.T. E-lab


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  • Pre-lab PowerPoint Lesson for S.W.A.T. E-lab

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It all starts with vibrations!
  • Vibrations are waves of energy that move from one
    place to another.
  • These vibrations can occur in.
  • Water waves on the ocean shore
  • Electricity running through a wire
  • Light from the Sun or light bulbs
  • Air vibrating string in a piano

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Electromagnetic Spectrum
  • Whenever you watch TV, send a text message, or
    heat food in a microwave, you are using waves.
    Some waves, like sound waves, need molecules to
    travel through. This is why you can hear sound
    in our atmosphere but not in space.
  • Some waves, however, do not need molecules to
    travel. These waves are called electromagnetic
    waves. These waves can travel through solid
    materials - but they can also travel through
    empty space.

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Electromagnetic Waves
  • The word electromagnetic comes from the two words
    electricity and magnetism. When an electric
    field and magnetic field move together, they make
    waves - electromagnetic waves!

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Parts of Waves
  • Waves go up and down, and they move forward -
    like a shaken rope.

(How Long)
(How Tall)
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Wavelength
  • The length of a wave from crest to crest is
    called WAVELENGTH. The different waves of the
    spectrum can be as small as the nucleus of an
    atom, or as big as a planet!

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Frequency
  • How many waves move pass a point in one second is
    called FREQUENCY. The more wiggles the higher
    the energy.

Different colors of light are due to waves of
different length and frequency
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Amplitude
  • The height of a wave is referred to as AMPLITUDE.

With sound waves, the higher the amplitude, the
louder the noise.
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Types of Waves
  • There are many types of waves along the
    electromagnetic spectrum, from very long radio
    waves to very short gamma rays. We are only able
    to see a small portion of this spectrum called
    visible light. However, scientific instruments
    use the full range of the electromagnetic
    spectrum to study and learn about both Earth and
    space.

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Radio Waves
  • Radio waves have the longest wavelengths in the
    electromagnetic spectrum. They can be as large as
    a football field to larger than our planet! They
    have the lowest frequency of all the
    electromagnetic waves. Since radio waves can
    carry energy, we use them to transmit information
    by changing either the frequency or the amplitude
    of the radio wave to encode a message.
  • Radio waves are useful because they can travel
    through many different materials, like clouds,
    without being absorbed.
  • Radio telescopes are used to view planets,
    comets, giant clouds of gas and dust, stars, and
    galaxies.

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Microwaves
  • Microwaves are higher frequency than radio waves.
    They range in size from about 1 millimeter to 1
    foot long. You are probably most familiar with
    them when you heat your food up in a microwave,
    but they have a lot more uses including weather
    forecasting and cell phones! Microwaves can even
    pass through clouds, which make them an excellent
    wavelength for transmitting satellite
    communications.
  • In 1965, two scientists at Bell Labs, Arno
    Penzias and Robert Wilson, detected a strange
    background noise. The scientists soon realized
    that they had discovered noise left over from the
    Big Bang that began the universe billions of
    years ago!

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Infrared
  • Infrared waves are about the length of a grain of
    sand. While we cannot see infrared, we can sense
    some of the energy as heat.
  • Infrared light is used in television remote
    controls and even in video games. We can use
    infrared cameras to study heat loss patterns,
    such as from a house. This can help us to better
    insulate openings such as doors and windows to
    keep thermal energy in and reduce the cost to
    heat the house.
  • Infrared energy can reveal objects in the
    universe that cannot be seen in visible light
    using optical telescopes. Infrared light is
    helpful in studying new stars because often dense
    gas clouds block their visible light.

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Visible Light
  • All electromagnetic radiation is light, but we
    can only see a small portion of this radiation.
    This is the part of the spectrum we call visible
    light.
  • Each color of the visible light spectrum has a
    different wavelength. This is why when white
    light travels through a prism, the wavelengths
    separate into the colors of the rainbow.
  • Your color TV has only red, green and blue dots
    but these make all the other colors on your
    screen. Objects appear to be different colors
    because they absorb different amounts of the red,
    green and blue light. They reflect the rest of
    the wavelengths in visible light and this is the
    color we see.

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Radiation from Sun
  • About 43 of the total radiant energy from the
    sun is in the visible parts of the spectrum.
  • Most of the remainder is in the near-infrared
    (49) and ultraviolet section (7).
  • Less than 1 of solar radiation is emitted as
    x-rays, gamma waves, and radio waves.

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Ultraviolet
  • Ultraviolet (UV) light has shorter wavelengths
    than visible light. Although UV waves are
    invisible to the human eye, some animals can see
    them.
  • The Sun is a source of the full spectrum of
    ultraviolet radiation, UV-A, UV-B, and UV-C
    waves. UV-C rays are the most harmful but are
    almost completely absorbed by our atmosphere.
    UV-B rays are the harmful rays that can cause our
    skin to burn. About 95 percent of UV-B rays are
    absorbed by ozone in the Earth's atmosphere.
  • Young stars shine most of their light in the
    ultraviolet wavelength, so scientists are able to
    study the formation of new stars using
    ultraviolet telescopes.

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X-Rays
  • X-rays have much higher energy and much shorter
    wavelengths than ultraviolet light.
  • X-rays were first studied in 1895 by a German
    scientist named Wilhelm Conrad Roentgen. He
    discovered that aiming x-rays through the human
    body created detailed images of the bones inside.
    Because bones are so dense, they absorb more
    x-rays than skin does creating shadows on the
    x-ray film.
  • Some things in space naturally emit x-rays. The
    hotter the object is, the shorter the wavelengths
    that are emitted.
  • Earth's atmosphere blocks x-ray radiation. This
    is beneficial for us here on Earth, because
    x-rays are so energetic that they would harm
    almost every living thing on earth!

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Gamma Rays
  • Gamma rays have the smallest wavelengths and the
    most energy of all the waves. They are produced
    by the hottest and most energetic objects in the
    universe.
  • On Earth, gamma waves are created by nuclear
    explosions, lightning, and radioactive decay.
  • Exposure to these high-energy waves can cause
    damage to cells in living things. Sometimes,
    though, these changes to cells can be helpful.
    Gamma radiation is used to kill cancer cells.
  • Gamma-ray bursts are the most energetic and
    luminous electromagnetic events and can release
    more energy in 10 seconds than our Sun will emit
    in its entire 10-billion-year expected lifetime!
    Scientists can also use gamma rays to determine
    the elements on other planets.

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Dangers of the Spectrum
  • Some waves can be harmful if you are exposed to
    them for too long. The side of the spectrum with
    wavelengths shorter than visible light tend to be
    more dangerous to humans because they can have
    effects on the cellular level.
  • The Sun bombards our Earth constantly with
    electromagnetic energy. However, the Earth's
    atmosphere protects us from higher energy waves
    that can be harmful to life.
  • Some waves, such as visible light and microwaves,
    pass through the atmosphere. While the atmosphere
    is essential to protecting life on Earth, it is
    not helpful when it comes to studying waves in
    space. Because it blocks much of the radiation,
    instruments have to be positioned above the
    atmosphere in order to study higher energy and
    even some lower energy sources.

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Now lets see you create your own electromagnetic
spectrum in the Spectrum Scramble Activity!
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