23.1 - The Solar System
The Sun, our star
- The Sun is a medium-sized star, made up mostly of hydrogen and helium.
- It radiates energy across the electromagnetic spectrum, mostly as infrared, visible light, and ultraviolet.
- The Sun contains most of the mass of the Solar System, so its gravitational pull dominates, keeping the planets and other bodies in orbit around it.
Light-travel time across the Solar System
- Distances in the Solar System are so large that it's useful to measure them by how long light takes to cross them.
- Light travels at a speed of about 3 × 108 m/s.
Formula for light-travel time
Where:
- = Time, in seconds (s)
- = Distance, in metres (m)
- = Speed of light, about 3 × 108 m/s
Worked example - Light from the Sun to the Earth
The Earth is about 1.5 × 1011 m from the Sun. How long does light take to travel from the Sun to the Earth?
Step 1 - Formula
Step 2 - Substitution and calculation
Step 3 - Interpretation
Light from the Sun reaches the Earth in about 500 seconds, which is roughly 8 minutes.