LIGHT
Chapter 14
What is Light?
1. Is both a wave and a particle
 Acts like a wave:
 Carries energy (heat)
 Has color
 Different l and f
 Can be reflected and refracted
 Shows interference (destructive & constructive)
 Acts like a particle:
 Travels without a medium (space)
2. Considered a photon (a packet or unit of light)
3.Transverse wave on 2 planes of motion
 electric field (on vertical plane)
 magnetic field (on horizontal plane)
How is light made?
 Atoms
 Electrons orbiting around nucleus
 Farther e- are from the nucleus, the more energy they
have
 Move towards nucleus, they lose/give off energy
Light Examples
 Light bulbs
1. Incandescence - makes light with heat
 Filament inside is heated
 e- in filament gain and lose energy, which gives
off light
 Give off A LOT of heat, wastes energy
2. Fluorescent - add energy to e- inside a gas
 Little heat created, so little is lost
3. LED – e- constantly moving in semiconductor
 ‘Light emitting diode’
Light Examples
4. Photoluminescence – process of creating light
 Objects contain Phosphorus
 Glow in the dark objects
 Exposed to any light, e- gain energy
 Lose energy very slowly
 Once energy is gone, it can be “recharged” by
putting it back in the light
The Speed of Light (“c”)
 The “universal speed limit” – nothing in universe
can go faster than light
 Unaffected by any medium
 Is 3 x 108 m/s (300,000,000 m/s)
 Can circle the Earth 7.5 times in 1 sec
 Light from the sun is 8 minutes old
 We use light to determine distance in space:
 1 light year = the distance light travels in one year
What can we see?
 We see white light
 Separate white light with a prism through refraction
 Get different colors (ROY G BIV)
 Also called visible light
 Colors have different energies (f & l)
 Think about fire –
 red flames are coolest (outside of flame)
 blue are hottest (middle of fire)
 As you move from red to blue:
 light GAINS energy, so shorter l
 White light is hottest since made up of all colors
 Color can also tell us other things:
 We can determine their chemical make-up based on
the colors we see (i.e. stars)
Visible and Invisible Light
 The amount of energy given off by e- varies
greatly
 Leads to different l
 Small l are measured in nanometers (nm)
 1 nm = 1 x 10-9 m (0.0000000001 m)
 Whole range of energy is known as the
Electromagnetic radiation (EMR)
 All light in this spectrum travels at (c)
 EMR
 Organized longest l to shortest l
 Longer l = low energy, low frequency
 Shorter l = high energy, high frequency
 DANGEROUS STUFF!
1. Radio waves: very high l, low energy waves
 Used to transmit radio andTV signals
 Radio towers are so tall – to make long radio waves
2. Microwaves:
 Used to cook food (by vibrating water molecules)
 Cell phones transmissions
3. Infrared:
 Shows heat signatures of objects
4.Visible Light:
 What we see – colors
5. Ultraviolet Light (UV):
 Causes sunburns and skin cancer
 Much of this is absorbed by the ozone layer
6. X-Rays:
 Small enough l to penetrate materials and tissues
 Medical use: see bones or teeth
7. Gamma Rays:
 most powerful & most dangerous
 Lowest l & highest energy
 Emitted from nuclear reactions
 Can break cellular bonds and cause mutations (cancer)
 Medical use: used to help treat cancer

Light Notes

  • 1.
  • 2.
    What is Light? 1.Is both a wave and a particle  Acts like a wave:  Carries energy (heat)  Has color  Different l and f  Can be reflected and refracted  Shows interference (destructive & constructive)  Acts like a particle:  Travels without a medium (space) 2. Considered a photon (a packet or unit of light)
  • 3.
    3.Transverse wave on2 planes of motion  electric field (on vertical plane)  magnetic field (on horizontal plane)
  • 4.
    How is lightmade?  Atoms  Electrons orbiting around nucleus  Farther e- are from the nucleus, the more energy they have  Move towards nucleus, they lose/give off energy
  • 5.
    Light Examples  Lightbulbs 1. Incandescence - makes light with heat  Filament inside is heated  e- in filament gain and lose energy, which gives off light  Give off A LOT of heat, wastes energy 2. Fluorescent - add energy to e- inside a gas  Little heat created, so little is lost 3. LED – e- constantly moving in semiconductor  ‘Light emitting diode’
  • 6.
    Light Examples 4. Photoluminescence– process of creating light  Objects contain Phosphorus  Glow in the dark objects  Exposed to any light, e- gain energy  Lose energy very slowly  Once energy is gone, it can be “recharged” by putting it back in the light
  • 8.
    The Speed ofLight (“c”)  The “universal speed limit” – nothing in universe can go faster than light  Unaffected by any medium  Is 3 x 108 m/s (300,000,000 m/s)  Can circle the Earth 7.5 times in 1 sec  Light from the sun is 8 minutes old  We use light to determine distance in space:  1 light year = the distance light travels in one year
  • 9.
    What can wesee?  We see white light  Separate white light with a prism through refraction  Get different colors (ROY G BIV)  Also called visible light
  • 10.
     Colors havedifferent energies (f & l)  Think about fire –  red flames are coolest (outside of flame)  blue are hottest (middle of fire)  As you move from red to blue:  light GAINS energy, so shorter l  White light is hottest since made up of all colors  Color can also tell us other things:  We can determine their chemical make-up based on the colors we see (i.e. stars)
  • 11.
    Visible and InvisibleLight  The amount of energy given off by e- varies greatly  Leads to different l  Small l are measured in nanometers (nm)  1 nm = 1 x 10-9 m (0.0000000001 m)  Whole range of energy is known as the Electromagnetic radiation (EMR)  All light in this spectrum travels at (c)
  • 12.
     EMR  Organizedlongest l to shortest l  Longer l = low energy, low frequency  Shorter l = high energy, high frequency  DANGEROUS STUFF!
  • 13.
    1. Radio waves:very high l, low energy waves  Used to transmit radio andTV signals  Radio towers are so tall – to make long radio waves 2. Microwaves:  Used to cook food (by vibrating water molecules)  Cell phones transmissions
  • 14.
    3. Infrared:  Showsheat signatures of objects 4.Visible Light:  What we see – colors
  • 15.
    5. Ultraviolet Light(UV):  Causes sunburns and skin cancer  Much of this is absorbed by the ozone layer 6. X-Rays:  Small enough l to penetrate materials and tissues  Medical use: see bones or teeth
  • 16.
    7. Gamma Rays: most powerful & most dangerous  Lowest l & highest energy  Emitted from nuclear reactions  Can break cellular bonds and cause mutations (cancer)  Medical use: used to help treat cancer