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Light - Overview of light - Properties of light

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Presentation on theme: "Light - Overview of light - Properties of light"— Presentation transcript:

1 Light - Overview of light - Properties of light
- Luminous and non-luminous objects - The strangeness of light - The electromagnetic spectrum - Wavelength of frequency - color & color Blindness - The production of light - The speed of light

2 Where does light come from?
The SUN!! The sun is a star located 1.50 x 108 km, or 1 Astronomical Unit, away from Earth. It provides energy in the form of light through a process called nuclear fusion. Nuclear fusion occurs when two atoms that naturally repelled each other are pulled together by a superior force and the atoms fuse together. Nuclear fusion produces energy that reaches us as heat and light.

3 The sun provides the energy that enables life on Earth.

4 What The Heck Is Light

5 Light travels in straight lines:
Properties of Light Light travels in straight lines: Laser

6 Light travels VERY FAST – 3.0X108m/s = 300,000 kilometres per second.
At this speed it can go around the world 7.5 times in one second.

7 Light travels much faster than sound.
For example: Thunder and lightning start at the same time, but we will see the lightning first.

8 We see things because they reflect light into our eyes:
Homework

9 Luminous and non-luminous objects
A luminous object is one that produces light. A non-luminous object is one that reflects light.

10 Properties of Light summary
Light travels in straight lines Light travels much faster than sound We see things because they reflect light into our eyes

11 The Strangeness of Light
Nothing moves faster than the speed of light 3.0 x 108 m/s Anything with mass cannot travel at the speed of light Light is defined as a collection of one or more photons (particles) propagating through space as electromagnetic waves therefore, it’s a particle and a wave Unlike heat and sound energy which requires a medium (a physical substance) to move, light does not Light is transferred through radiation (via electromagnetic waves) in a vacuum

12 Fun Science Light Video

13 Modern electromagnetic waves
Today we have identified many types of electromagnetic waves which makes up our electromagnetic spectrum The Electromagnetic Spectrum video

14 The Electromagnetic Spectrum
Your eyes can only see the visible part of the EM spectrum, but your hands can feel the infrared part.

15 The Electromagnetic Spectrum
Machines can detect other parts of the EM spectrum, but the information needs to be converted into colours for us to see it.

16 Example – The Sun visible x-ray UVA UVB

17

18 As we decrease wavelength, we increase frequency and energy
Modern View Continued Longer Wavelength (Low Energy) Shorter Wavelength (High Energy) As we decrease wavelength, we increase frequency and energy

19 Wavelength and Frequency
Wavelength – the distance between successive crests on a wave. Frequency – the number of cycles a wave goes through in one second.

20 The Visible Light Spectrum
Different colours have different wavelengths!

21 color White light is not a single color; it is made up of a mixture of the seven colours of the rainbow. We can demonstrate this by splitting white light with a prism: This is how rainbows are formed: sunlight is “split up” by raindrops.

22 The colours of the rainbow:
Red Orange Yellow Green Blue Indigo Violet ROY-G-BIV

23 Adding colours White light can be split up to make separate colours. These colours can be added together again. The primary colours of light are red, blue and green: Adding blue and red makes magenta (purple) Adding blue and green makes cyan (light blue) Adding red and green makes yellow Adding all three makes white again

24 Only red light is reflected
Seeing color The color an object appears depends on the colours of light it reflects. For example, a red book only reflects red light : Homework White light Only red light is reflected

25 A white hat would reflect all seven colours:
A pair of purple pants would reflect purple light (and red and blue, as purple is made up of red and blue): Purple light A white hat would reflect all seven colours: White light

26 color Blindness The tricky thing about color blindness is that many people don’t know they are color blind until they get tested 40% of color blind pupils currently leaving secondary school are unaware that they are color blind There are of course advantages

27 How many animals are there?

28 6!

29 Red Green color Blindness is caused by a gene on the X chromosome therefore, since males have 1 X and 1 Y while females carry 2 X’s, this issue is predominately found in males (7-10% of the overall population) and is very rarely seen in females.   For these people, they cannot see red and green light.

30 Blue color Blindness is equally unlikely for both males and females as the deficient gene is found on chromosome 7. These people can’t see blue color light In both these cases the problem isn't as straight forward as not seeing blue, red or green light.  If what they are looking at contains these colours, they will not be seen.

31

32 What Colorblind People See

33 What is color Blindness

34 The Production of Light
Light is produced by three main ways: Incandescence Hot things glow

35 The Production of Light
Luminescence Electrons jump around

36 The Production of Light
Chemoluminescence Chemical reactions Bioluminescence is a chemical reaction inside a living organism

37 The speed of light The speed of light in a vacuum is a universal constant. 300,000,000 m/s The speed of light in a medium is always slower than the speed of light in a vacuum.

38 How long will it take? Earth Moon 384,000,000 m How long does light take to reach the Earth from the Sun? 8.3 minutes

39 Looking Into The Past By looking at objects in the universe (stars and galaxies), you are looking into the past. Why?

40 Looking Into The Past Time for the light to reach us Object The Moon
1.3 seconds The Sun 8.3 minutes Jupiter 35 to 52 minutes Pluto 5.5 hours Alpha Centauri (nearest star) 4.3 years Sirius (Brightest star in our sky) 9 years Betelgeuse (Another bright star) 430 years Orion Nebula 1500 years Andromeda Galaxy 2.5 million years


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