1. Fundamental Properties of Light
For you to see anything, light must travel from an object to your eye. Objects that produce their own light, like the Sun or a light bulb, are called luminous. Most objects, like a book or the Moon, are non-luminous; we see them by the light they reflect from a luminous source. Light is a form of energy that travels in straight lines, which we represent using straight lines with arrows called rays. It is a transverse wave and, uniquely, can travel through a vacuum (empty space). In a vacuum, light travels at the fastest possible speed in the universe: 300,000,000 metres per second (3 x 10^8 m/s).
speed = distance / time
Key term
Examiner insight
Fun fact
Worked example 13 marks
The Sun is approximately 150,000,000 km from Earth. The speed of light is 300,000 km/s. Calculate the time it takes for light from the Sun to reach Earth.
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Step 1: Identify the known values. Distance = 150,000,000 km, Speed = 300,000 km/s.
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Step 2: State the formula: time = distance / speed.
- 3
Step 3: Substitute the values into the formula: time = 150,000,000 km / 300,000 km/s.
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Step 4: Calculate the result: time = 500 s.
Recap
- Luminous objects produce their own light; non-luminous objects reflect light.
- Light travels in straight lines, represented by rays.
- Light is a transverse wave that transfers energy and can travel through a vacuum.
- The speed of light in a vacuum is the universal speed limit, approximately 3 x 10^8 m/s.
Quick check
- Give one example of a luminous object and one example of a non-luminous object.2 marks
- What is the approximate speed of light in a vacuum?1 mark