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Properties of Light

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Title: Properties of Light


1
  • Properties of Light

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3
Speed of E.M. Spectrum Waves in a Vacuum
  • 299,792,458 m/s (3 x 108 m/s), or 186,000 miles
    per second.
  • It takes about two and a half seconds, for
    instance, for a radio communication traveling at
    the speed of light to get to the moon and back.
  • Speed decreases as density of medium increases
  • Change in medium causes refraction (bending)
  • At this speed it can go around the world 7.5
    times in one second

c f?
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Electromagnetic Waves
  • Electromagnetic Waves - energy-carrying waves
    emitted by vibrating electrons
  • Light, Radiation, or Photons

http//cse.ssl.berkeley.edu/img/em_wave.gif
6
Electromagnetic Spectrum

Cosmic rays Background radiation particles of enormous energy given off by stars.
Gamma radiation Deadly high energy given out by the sun and other stars.
X rays High energy used in X ray equipment.
Ultraviolet rays Invisible energy waves in sunlight, which cause skin to tan.
Visible light Basic colors of light, emitted by the sun and visible to the human eye.  ROYGBIV.
Infrared rays Rays of heat energy sensed by our nervous system.
Radio waves Microwaves TV radio energy

7
Radio Waves
  • Longest wavelength, lowest frequency (smallest
    amount of energy)
  • Used for radio, television, cellular phones,
    cordless phones, radio astronomy, microwaves, and
    RADAR
  • Types
  • Shortwave (for very long ranges)
  • AM (can bend around large objects such as
    mountains)
  • FM (strong signals in range of about 50-70 miles)
  • Television broadcast waves (FM for sound and AM
    for picture)

8
Infrared Radiation
  • Heat
  • Thermograms show how much infrared radiation is
    being given off by a living thing
  • Used to view objects in the dark
  • night vision goggles
  • Heat lamps use infrared radiation to heat food

9
Visible Light
  • Only part of the EM spectrum humans can see
  • 4 x 1014 Hz to 7.9 x 1014 Hz
  • Visible spectrum of color (from longest
    wavelength to shortest)
  • Red (650 nanometers)
  • Orange
  • Yellow (580 nanometers)
  • Green (530 nanometers)
  • Blue (470 nanometers)
  • (Indigo)
  • Violet (400 nanometers)

10
Visible Light
  • What we call light depends on the overall
    sensitivity of the eye, ranging in wavelength
    from 380 nm to 760 nm.

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Ultraviolet Radiation
  • Causes us to make vitamin D in our skin
  • Can be harmful
  • can cause skin cancer
  • Used to kill germs and sterilize medical
    equipment
  • Nail shops
  • Safety goggles

13
X rays
  • Their high energy makes then pass through many
    materials
  • Various exposure times allows for numerous views

14
Gamma Rays
  • Most energetic
  • Used in radiation therapy to kill cancer cells

15
Important Properties of Light
  • Amplitude determines brightness
  • The greater the amplitude, the greater the
    brightness
  • Wavelength determines color

16
Light Intensity
  • Intensity or brightness of the light changes
    along with the colors

http//fuse.pha.jhu.edu/wpb/spectroscopy/basics.h
tml
17
Inverse Square Law
http//www.anees.com/6.html
http//www.astrosociety.org/education/publications
/tnl/32/starscience2.html
18
Additive Primary Colors of Light
  • By overlapping or adding various colors of
    light together almost any color can be made.

Additive PrimariesRGBRed, Green, and BlueLight
19
Secondary Colors of Light
  • Colors made by mixing 2 primary colors.
  • G R yellow
  • R B magenta
  • B G cyan

http//www.colorado.edu/physics/2000/tv/colortv.ht
ml
20
Light Mixing (Additive)
  • White light is formed where red, blue and green
    light overlap

http//sol.sci.uop.edu/jfalward/reflection/reflec
tion55.html
21
Photons
  • Light and EM radiation are composed of small
    particles called photons.
  • Photons are thought to be carriers of EM force.
  • Have either particle or wavelike behavior. This
    duality in the nature of photons is a key aspect
    of Quantum theory.

22
Different Wavelengths
  • Medium dictates speed
  • Since the photon's energy does not change, its
    frequency cannot change therefore its wavelength
    changes.
  • Wavelength decreases as the speed decreases.

23
Particle or Wave?
  • Particles are discrete
  • energy is concentrated into what appears to be
    finite space is homogeneous with definite
    boundaries
  • Waves, not considered a finite entity.
  • Light energy does not exist in a single location,
    as a wave varies in both place and time.

http//www.savagechickens.com/tag/particle
24
Wave Theory VS Particle Theory Photon-massless
bundle of concentrated electromagnetic energy
  • Particle Theory
  • Light acts like particles that stream from the
    source (creating shadows)
  • Wave Theory
  • Light acts like wavesripples in space

http//www.thespectroscopynet.com/Educational/wave
_particle_duality.htm
25
Dual Nature of Light
Proof that Light is a wave Proof of Nothing Proof that light is a Particle
Diffraction (particles dont change direction as they pass BY a barrier) Interference (two or more particles can NOT exist in the same place at the same time) Polarization (polarized filters allow light which is vibrating in one direction through only transverse waves can be polarized Reflection Refraction Photoelectric effect (When light hits a photoemissive metal, electrons are knocked off) Proves light is a particle since each photon knocks loose one electron Compton Effect (light can collide with small particles change their momentum)
26
Duality of Light
  • Wave-Particle Duality not strictly one or the
    other
  • Quantum electrodynamics (QED) combines the
    wave-particle nature of light into a single
    theory.
  • Light behaves as a wave
  • When light travels through an opening
  • Light behaves as particles
  • when light bounces off of metal

http//nobelprize.org/nobel_prizes/physics/article
s/ekspong/index.html
http//www.crcs.k12.ny.us/physics/notes/modern/mod
ern_note.htm
27
Photoelectric effect
  • The photoelectric effect refers to the emission,
    or ejection, of electrons from the surface of,
    generally, a metal in response to incident light.
  • Discovered by Einstein in the early 20th century
  • electrons are ejected from a solid when impinged
    upon by electromagnetic radiation
  • excitation
  • led to the understanding of light as particles,
    or photons

http//www.physics.uiowa.edu/adventure/fall_2005/o
ct_15-05.html
http//www.uwsp.edu/geo/faculty/ritter/geog101/tex
tbook/energy/nature_of_electromagnetic_radiation_p
_2.htm
28
Light as a Particle
http//www-inst.eecs.berkeley.edu/cs39j/sp02/sess
ion07.html
29
Polarization
  • The process of transforming non-polarized light
    into polarized light is known as polarization.
  • Polarized light waves are light waves in which
    the vibrations occur in a single plane.

http//www.glenbrook.k12.il.us/gbssci/phys/Class/l
ight/u12l1e.html
30
Light reflected from a horizontal surface is
partially polarized in the horizontal plane.
31
http//www.olympusmicro.com/primer/lightandcolor/p
articleorwave.html
Polarized Light wave not particle
  • Light consists of transverse waves having
    components that are perpendicular to the
    direction of propagation.

32
Polarized Lenses Really Make a Difference!
  • Light reflected from surfaces like a flat road or
    smooth water is generally horizontally polarized.
  • Vertically oriented polarized lenses result in a
    reduction in glare.
  • Eliminate reflected glare
  • Enhance contrast
  • Great for use during snow or water sports

http//www.chicagopearle.com/eyeglasses/lenses/pol
arized/index.asp
http//www.spyoptic.com/img/4219_tridentPolarized
.jpg
33
Are your lenses polarized?
http//www.agape1.com/polarized.htm
34
3-D Glasses
  • Two projectors project two respective views onto
    the screen
  • each with a different polarization.
  • The glasses are polarized oppositely
  • allowing only one image into each eye

http//www.3dglassesonline.com/how-do-3d-glasses-w
ork/index.html
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Law of Reflection
Angle of incidence is equal to angle of
reflection I incoming light N Normal R
Reflected light
37
Reflected Light
  • SPECULAR REFLECTION light is reflected in the
    same forward direction only
  • DIFFUCE REFLECTION light is reflected in many
    directions

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Total Internal Reflection
  • Occurs when light travels from a medium of larger
    to smaller index of refraction
  • the light ray can actually bend so much that it
    never goes beyond the boundary between the two
    media

40
Total Internal Reflection
  • If the fish looks upwards it sees the sky, but if
    it looks at too large an angle to the vertical it
    sees the bottom of the pond reflected on the
    surface of the water.
  • The critical angle to the vertical is equal to
    the critical angle for total internal reflection
    at an air-water interface which is approximately
    49.

41
Total Internal Reflection
Refracted ray
http//www.glenbrook.k12.il.us/gbssci/phys/CLass/r
efrn/u14l3b.html
42
Fiber Optics
  • Fiber-optic lines are strands of optically pure
    glass as thin as a human hair
  • The light in a fiber-optic cable travels through
    the core (hallway) by constantly bouncing from
    the cladding (mirror-lined walls)
  • total internal reflection

43
Refraction
http//fr.wikipedia.org/wiki/RC3A9fraction
44
The Law of Refraction
  • The law of refraction is used to predict the
    amount of bend, or refraction.
  • The law of refraction is also known as Snell's
    Law, named for Willobrord Snell, who discovered
    the law in 1621.

45
More on Refraction
  • Assuming that the air on both sides of a window
    have the same refractive indices
  • Then the incoming and outgoing light beams are
    actually parallel

46
Snells Law
http//www.iop.org/activity/education/Teaching_Res
ources/Teaching20Advanced20Physics/Vibrations20
and20Waves/Reflection20and20refraction/page_447
7.html
The relationship between the angles of incidence
and refraction and the indices of refraction of
the two media involved.
47
Bending Towards the Normal
  • ex light passing from air into water
  • lower to higher density
  • the angle of refraction is smaller than the angle
    of incidence

http//id.mind.net/zona/mstm/physics/light/rayOpt
ics/refraction/refraction1.html
48
Bending Away From the Normal
  • ex light passing from water into air
  • higher to lower density
  • the angle of refraction is larger than the angle
    of incidence.

http//id.mind.net/zona/mstm/physics/light/rayOpt
ics/refraction/refraction1.html
49
Examples of objects that create a Spectrum
  • Prism
  • Raindrops
  • CDs
  • Diffraction Grating
  • The tracks of a compact disc act as a diffraction
    grating, producing a separation of the colors of
    white light

50
  • The color of light emitted by a hot object
    changes with its temperature.
  • Glowing object colors
  • Reddish ? coolest glowing object
  • Orangeish
  • Yellowish
  • White
  • Bluish ? hottest glowing object

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Transparent Materials
  • object through which light can pass in straight
    lines

http//www.gcsescience.com/pwav21.htm
53
Clear glass is transparent to visible light but
not to infrared light therefore trapped heat!
http//www.ucolick.org/bolte/AY4_00/week2/light_s
idetripsC.html
54
Visible Light to Infrared
  • Clear glass is transparent to Visible light.
  • Absorbed, converted, emitted as Infrared.
  • Clear glass is not transparent to Infrared Light.
  • Trapped infrared light increases interior
    temperature.

55
Opaque Materials
  • Opaque - the term applied to materials that
    absorb light

http//www.ronbigelow.com/articles/color-perceptio
n-2/perception-2.htm
56
Translucent Material
  • Allows some light to pass through
  • ex a filter or tinted glass

http//www.ronbigelow.com/articles/color-perceptio
n-2/perception-2-6.jpg
57
Shadows
  • Umbra - the darker part of a shadow where all the
    light is blocked
  • Penumbra - a partial shadow

58
Solar Eclipse
Umbra
Sun
Full Shadow
Earth
Moon
Partial Shadow
Penumbra
  • A solar eclipse occurs when the Moon passes in
    front of the Sun.

59
Lunar Eclipse
Sun
Earth
Moon
  • A lunar eclipse occurs when the Moon passes into
    the Earth's shadow.

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