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1 Light Mike Maloney Physics, SHS

Light - MR. D PHYSICS

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1

Light Mike Maloney Physics, SHS

© 2003 Mike Maloney 2

Light

• What is LIGHT?

• WHERE DOES IT COME FROM?

© 2003 Mike Maloney 3

What is Light?

• Light is a wave, or rather acts like a wave.

• How do we know since we cannot see it?

• We can detect how it acts through …

– Reflection

– Refraction

– Dispersion

– Diffraction

– Interference

– Polarization

© 2003 Mike Maloney 4

What is Light

• Light is a special type of wave

• What we know as VISIBLE LIGHT is

actually a type of something called

ELECTROMAGNETIC RADIATION.

• So, what is electromagnetic radiation

and what are electromagnetic waves?

Do you know any other types?

© 2003 Mike Maloney 5

Electromagnetic Waves

• Electromagnetic waves are

everywhere.

• Light is only a small part of them

– Radios

– TVs

– Microwaves

– Light (Visible/UV/InfraRed)

– Radiation

– Lasers

– Tanning Huts

– X-Rays

© 2003 Mike Maloney 6

Electromagnetic Waves

• Where do these waves come from?

• When something releases energy it

also emits radiation. Depending on

the amount of energy, the object

will emit different types of

electromagnetic radiation.

• But what is creating the

disturbance? What is emitting this

energy?

• ELECTRONS, oscillating electrons!

© 2003 Mike Maloney 7

Electromagnetic Waves

• Electrons in materials are vibrated and emit energy in the form of photons, which propagate across the universe.

– http://www.colorado.edu/physics/2000/waves_particles/wavpart4.html

• Photons have no mass, but are pure quantized packets of energy.

• Electromagnetic Waves are waves that are made up of these “photons”.

• When these photons come in contact with boundaries, E-M waves interact like other waves would.

© 2003 Mike Maloney 8

Electromagnetic Waves

• When we studied mechanical waves,

they were all transferred through a

medium. What medium is light

transferred through?

• LIGHT DOES NOT NEED ONE!

• Electromagnetic waves are special in

the fact that they do not need a

medium to propagate through.

• Then what is oscillating through space?

– SPACE ITSELF!

© 2003 Mike Maloney 9

Electromagnetic Spectrum

© 2003 Mike Maloney 10

What creates the different types?

• gamma rays are produced by radioactive

decay and nuclear processes.

• X-rays are produced by decelerating

electrons.

• ultraviolet (UV), visible, and infrared (IR)

waves are produced by electron transitions

and by vibrating atoms and molecules.

• Microwaves, radio and TV waves are produced

by charges accelerated in antennas.

• waves with even lower energy are known as

long waves, because of their very long

wavelength

© 2003 Mike Maloney 11

How do they affect us? Electromagnetic waves can have a number of

different interactions with the human body:

• Gamma rays and X-rays are known as ionizing radiation. They can cause chemical changes as well as mutations of DNA. (remember the vest they put on you when you get an XRAY)

• Ultraviolet light is associated with suntans, sunburns, and cataracts and can damage cells.

• Rods and cones in our eyes are sensitive to visible light, which is why we can see.

• Heat sensors in our skin can detect infrared waves which is why we can tell if stuff is hot.

• We're not particularly sensitive to EM waves with longer wavelengths than infrared.

© 2003 Mike Maloney 12

Speed of E/M Waves

• From last chapter, we found that

– V = f * l

• We also said that the speed of a wave in a

certain medium is always constant.

• It has been found that the speed of E-M

waves and light in a vacuum is

– 3 x 108 or 300,000,000 m/s

– 671,000,000 mph

– 186,000 miles per second

– We call this value “c”

© 2003 Mike Maloney 13

c = f * l

• C is constant throughout the universe, as

long as light is in a vacuum.

• When it is in other materials, c can change,

but can never be larger than its value in a

vacuum.

• Since “c” is constant, all of E-M waves will

have a corresponding frequency to go along

with their wavelength.

• Lets find the corresponding frequency

ranges for a few of the groups of E-M waves.

© 2003 Mike Maloney 14

Energy in E-M Waves • Which waves do you think have more energy,

Radio waves or gamma waves?

• Because waves don’t really have a mass, we can’t really talk about their energy like mechanical waves.

• The greater the frequency of an E-M wave, the more crests pass a point in a certain amount of time, therefore the more photons pass that point.

• Which means More energy moves past that point in a certain amount of time or the wave is more energetic.

• We can even find out how much energy each of those wiggling photons has E = h * f, where h is Plank’s constant .. but don’t worry you won’t need to know this until next year, now just knowing that higher frequency light has more energy is good enough.

• HANG ON A SECOND?!

© 2003 Mike Maloney 15

Electromagnetic Spectrum

Let’s Talk about some of these again…

© 2003 Mike Maloney 16

Electromagnetic Waves

• Electromagnetic waves are

everywhere.

• Light is only a small part of them

– Radios

– TVs

– Microwaves

– Light (Visible/UV/InfraRed)

– Radiation

– Lasers

– Tanning Huts

– X-Rays

What makes some of these dangerous?

© 2003 Mike Maloney 17

Back to Light

• There seem to me an

incredible about of light in the

universe that we don’t even

notice.

• So, why can we only see a

small portion of these E-M

waves?

© 2003 Mike Maloney 18

Our Eyes

© 2003 Mike Maloney 19

Visible Light

• We now know what we see is part of

the electromagnetic spectrum. We

know that the light waves enter our

eye, and stimulate parts of it that

cause a electrical impulse to be sent

to the brain which creates this visual

image.

• But everything does not emit EM

radiation. How do we see my shirt?

And why can we barely see a

window?

© 2003 Mike Maloney 20

Seeing things

• We know that when waves run into a boundary they are partially transmitted and partially reflected.

• Light behaves as a wave, so it too is reflected.

• Therefore, an object does not need to emit photons itself to be seen, it just has to reflect light back to our eyes where we can detect it.

• Objects that do not allow light to pass through them are called opaque.

• Objects that allow light to pass through them are considered transparent.

• Objects in between are called translucent.

© 2003 Mike Maloney 21

Polarization

• Another reason we know light is a wave it

because it can be polarized.

• Polarization is a phenomenon of light that

is used in sun-glasses and 3-D movies.

• Play with the two polarizing filters for a

few minutes and note what is happening

and see if you can think of any reasons for

it.

• Think about the following:

– What happens to the strength of the light

when it goes through one polarizer.

– What about two or three?

© 2003 Mike Maloney 22

Polarization Hint

• Light vibrates in all directions.

• A polarizing filter acts like a picket

fence. It only lets certain direction

vibrations pass through it.

• Therefore, if you pass light through

two of them you can completely

block the light from passing through.

• HOW?

© 2003 Mike Maloney 23

Polarization

© 2003 Mike Maloney 24

Color

• Different objects may emit different wavelengths of E-M radiation, so we would see that light as different colors.

• But why do we see colors in objects that reflect light? If you shine a white light on my clothes, and it gets reflected why doesn’t all of my clothes appear white?

• When I shine white light through a colored piece of plastic, why does it change color?

© 2003 Mike Maloney 25

Color

• The light we see is know as visible or

white light – although it is not that

simple.

• The light is not really white, the

white we see is a combination of all

the colors of the rainbow.

• Remember R-O-Y G. B-I-V from art

class.

• When all of these light waves are

combined we see white light.

© 2003 Mike Maloney 26

Color Reflection

• So if we see something as WHITE,

that means …

– It reflected back all the wavelengths of

light to our eyes

• If we see something as RED or BLUE

– It reflected only the RED or only the

BLUE wavelengths

– The others were absorbed.

• And if we see something as black ?

– It did not reflect back any of the light.

© 2003 Mike Maloney 27

Color Transmission

• Filters work in a similar way. They

control what wavelengths of light

leave a material.

– RED filters only let RED light thru.

– BLUE let only BLUE light thru.

• What do you think that UV sticker

means on your sunglasses?

• Why do they sell those orange glasses

that are supposed to reduce glare?

© 2003 Mike Maloney 28

Some Sweet Color Tricks

• Combining color lights

• Combining colors in art class

• How does color printing work?

• What color is your shirt really?

• Why is the sky blue?

• Why are sunsets red?

• Why is water greenish-blue?

• How does a greenhouse work?

• InfraRed, that’s HOT

• How does 3-D work?

• Why does a CD reflect a rainbow?

• How does Phosphorescence (blacklight) work?

• How can you help people who are color blind? --http://colorfilter.wickline.org/

• Doppler Effect / Red shift of stars

• Lasers

© 2003 Mike Maloney 29

Flux

• We now know how light behaves, but we

must measure how strong it is.

• The rate at which a source emits light is

called the LUMINOUS FLUX (P).

(greek or latin for light flow)

• What do you think this is measured in?

What are light bulbs measured in.

• LUMINOUS FLUX (P) is actually measured

in something called a lumen (lm).

• A typical 100-W bulb emits about 1500 lm.

© 2003 Mike Maloney 30

Illuminance

• Flux is the total of all the light that is

emitted from a source.

• This is not very useful, often we

would like to know how much of that

light is hitting a surface at some

point.

• The illumination of a surface is called

illuminance, E. It is measured in

lumens per square meter, lm/m2

© 2003 Mike Maloney 31

Illuminance

• How do you think illuminance is

affected when the object moves

away from the source?

– Right the illuminance decreases

• So what would you expect an

equation to look like for E in terms of

P and the distance away d?

– Close for an expanding sphere of light,

it is

E = P

4pd2

Where did the 4 p d2

come from?

© 2003 Mike Maloney 32

© 2003 Mike Maloney 33

Electromagnetic Spectrum

BACK

© 2003 Mike Maloney 34

Visible Light Spectrum

BACK

Short wavelength

High Frequency

Long wavelength

Low Frequency

© 2003 Mike Maloney 35

Excited Electrons

1. The atom is normal.

2. The electron absorbs a packet of energy.

3. Because of the excess energy, the electron must move to a higher energy level.

4. The atom is now "excited".

5. The electron immediately drops back to its normal energy level.

6. To do this, the electron releases the excess energy in the form of a photon.

7. Light is produced. BACK

© 2003 Mike Maloney 36

Combining Colored Lights • Also known as color addition. • When you combine light colors from

different sources, you add that color to the light that gets reflected to our eyes.

• If you add two complimentary colors, such as blue and yellow, or green and magenta, or red and cyan, you end up with white light.

BACK

© 2003 Mike Maloney 37

Combining Colored Pigments • Also known as color subtraction. • When you combine pigment colors, as you do

when mixing paints, you end up subtracting colors that get reflected to our eyes.

• If you add two complimentary color pigments, such as blue and orange, or green and magenta, you end up with black, because all colors end up absorbed.

• The same is true if you filter colors from a source. If you have a white source, and you first filter with blue then with orange, almost all the light will be blocked.

BACK

© 2003 Mike Maloney 38

Why is the Sky Blue? • As light moves through the atmosphere, most of the

longer wavelengths pass straight through. Little of the red, orange and yellow light is affected by the air.

• However, much of the shorter wavelength light is absorbed by the gas molecules. The absorbed blue light is then radiated in different directions. It gets scattered all around the sky. Whichever direction you look, some of this scattered blue light reaches you. Since you see the blue light from everywhere overhead, the sky looks blue.

BACK

© 2003 Mike Maloney 39

Why is the Sunset Red? • As the sun begins to set, the light must travel farther through the

atmosphere before it gets to you. More of the light is reflected and scattered. As less reaches you directly, the sun appears less bright. The color of the sun itself appears to change, first to orange and then to red. This is because even more of the short wavelength blues and greens are now scattered. Only the longer wavelengths are left in the direct beam that reaches your eyes.

• The sky around the setting sun may take on many colors. The most spectacular shows occur when the air contains many small particles of dust or water. These particles reflect light in all directions. Then, as some of the light heads towards you, different amounts of the shorter wavelength colors are scattered out. You see the longer wavelengths, and the sky appears red, pink or orange.

BACK

© 2003 Mike Maloney 40

What color is your shirt really?

BACK

• You are wearing a white shirt.

• What color is it really? Is it always white?

• The color of something depends on what type of light it is reflecting.

• A “white” shirt in blue light looks blue not white.

• What would a pure RED shirt look like in pure BLUE light?

– BLACK

© 2003 Mike Maloney 41

Why is Water Blue? • It absorbs the reds, yellows and greens

allowing only the blues and purples to pass thru to reach our eyes.

• It IS NOT just a reflection of the sky.

BACK

© 2003 Mike Maloney 42

BACK

© 2003 Mike Maloney 43

3-D

BACK

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Thanks Elizabeth!

© 2003 Mike Maloney 44

Light Amplification by the Stimulated Emission of Radiation • Laser light is very different from normal light.

• The light released is monochromatic. It contains one specific wavelength of light (one specific color). The wavelength of light is determined by the amount of energy released when the electron drops to a lower orbit.

• The light released is coherent. It is “organized” -- each photon moves in step with the others. This means that all of the photons have wave fronts that launch in unison.

• The light is very directional. A laser light has a very tight beam and is very strong and concentrated. A flashlight, on the other hand, releases light in many directions, and the light is very weak and diffuse.

BACK

© 2003 Mike Maloney 46

Doppler Effect and Color Shifts

• The radiation emitted by an object moving

toward an observer is squeezed – its pulses are

pushed closer together; its frequency appears

to increase and is therefore said to be

blueshifted because it moves towards the blue

end of the light spectrum. In contrast, the

radiation emitted by an object moving away is

stretched or redshifted.

• Blueshifts and redshifts exhibited by stars,

galaxies and gas clouds also indicate their

motions with respect to the observer.

See the animation

BACK

© 2003 Mike Maloney 47

BACK

© 2003 Mike Maloney 48

Greenhouses

• Greenhouses work on the same principle that the Mythbusters used to beat the IR camera.

• Think glass allows visible light to pass through, but does not allow IR light to pass through.

• The energy in the sunlight in the form of visible light can get in to feed the plants.

• The plants then radiate IR energy in the form of heat, like all living things.

• This IR radiation gets reflected when it tries to pass through the glass.

• The energy is trapped, and the greenhouse stays warm.

BACK