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Light and the Electromagnetic Spectrum

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Title: Light and the Electromagnetic Spectrum


1
Light and the Electromagnetic Spectrum
2
How We See the Universe
  • We see the Universe in visible light
  • Visible light between 700nm (red) and 400 nm
    (violet)
  • The spectrum of all EM radiation
  • gamma rays
  • X-rays
  • Ultraviolet (UV)
  • Visible light
  • Infrared (IR)
  • Microwaves
  • Radio

3
Electromagnetic Waves
  • EM Waves are a response to changes in electrical
    and/or magnetic fields elsewhere. (accelerated
    charges)
  • EM Waves are transverse waves (like ripples on a
    pond)
  • EM waves do NOT need a medium to travel through
  • ALL EM Waves travel at the speed of light
  • (c 3 x 108 m/s)

4
The Electromagnetic Spectrum
  • High Energy Low energy
  • High Frequency Low frequency
  • Short wavelengths Long wavelengths

What we see (visible light) VIB G YOR
5
(No Transcript)
6
Visible light Spectrum
  • Isaac Newton showed that ordinary sunlight could
    be split into many colors with a prism
    (dispersion)
  • ROY G BIV
  • (red, orange, yellow, green, blue, indigo,
    violet)
  • Each color corresponds to light of a specific
    wavelength with a specific frequency

7
Example EM Wave
Wavelength, ?, is length from crest to
crest Frequency, f is the number of wave crests
per second that pass a given point speed
v f ? ALL emag. Waves travel at the speed of
light ( 3 x 108 m/s)
8
Example
  • A yellow light wave has a frequency of 5 x
    1014 Hz. What is the wavelength of this yellow
    light?
  • (all emag waves travel at speed of light)
  • v f ?
  • 3x108 m/s (5x1014 Hz) ?
  • (divide by 5x1014 Hz)
  • ? 6 x 10-7 m

9
(No Transcript)
10
Wave-Particle duality
  • Light behaves like a wave (proof double slit
    interference pattern)
  • Light behaves like a particle (proof
    photoelectric effect)
  • Light is BOTH a particle and a wave!

11
Photoelectric effect
  • Light shines on a metal and kicks out electrons.
  • We get more energetic electrons byshining a
    higher frequency light on it (blue?violet)
  • Brighter light ejects more electrons but not with
    higher energies.
  • Uses???? (solar powered calculatorsor solar
    powered anything)
  • E hf (h 6.63 x 10-34 J-s )
  • electron

12
Brightness
  • Flux (rate of energy per area) falls off
    according to the inverse square law
  • example
  • Two light bulbs (AB) are equally as bright. Bulb
    B is placed 3 times further away. How does its
    brightness compare?
  • Brightness ? 1/d2
  • Brightness ? 1/32 1/9 as bright

13
Color
  • Additive primary colors for LIGHT
  • (NOT like mixing paints---thats subtractive)
  • Primary colors red, green, blue
  • For light
  • Red green yellow
  • Red blue magenta
  • Blue green cyan
  • All colors white light

14
Why does a green shirt appear green?
ROY G BIV
  • White light on a green shirt will reflect green
    and absorb all the other colors
  • What if a red light shines on a green shirt?
  • There are no green wavelengths to reflect, so it
    absorbs the red and appears black

Red
15
Colorreflection and absorption
  • A color will appear a particular color because it
    reflects that wavelength of light (and absorbs
    all others)

16
Colorsubtractive color mixing (like paints)
  • More complex
  • Think about which wavelengths can be reflected.
  • M Y R
  • C Y G
  • C M B

17
Polarizationtransmission of light such that
electric field waves are oriented in one direction
18
Tyndall Effect
  • Scattering of light through particles
  • Higher frequency light scatters more (Why our
    sky appears blue)
  • Lower frequency light scatters less (why sunsets
    appear red)

19
Doppler Effect
  • Motion of an object that emits or absorbs light
    causes a shift in the observed spectrum
  • Receding objects spectrum red-shifts, so
    observed wavelength longer than normal
  • Approaching objects spectrum blue-shifts, so
    observed wavelength is shorter than normal

20
How Light is Emitted Black Body Radiation
  • Ideal object that gives off radiation
  • Perfectly absorbs all radiation, then re-emits
    radiation depending on temperature
  • Hot object appears bluer, cold object appears
    redder

21
Planck Curve Brightness of a black body
spectrum
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