8.1.1Astrophysics
Objects in Space — Edexcel International GCSE Science Double Award 4SD0 - Physics Revision Notes & Topical Questions
5 min read 9 parts Lesson 2 of 8
Part 1 of 7The Solar System
The Solar System is made up of the Sun, eight planets, and the many smaller objects that orbit the Sun. The Sun is a star, an enormous ball of hot gas that releases energy by nuclear fusion; it contains over 99% of the mass of the whole Solar System. Its gravity keeps everything else in orbit.
- In order from the SunMercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.
- The four inner planets are small and rocky; the four outer planets are large gas or ice giants.
Part 2 of 7Smaller bodies: asteroids and comets
Asteroids are rocky or metallic lumps, from a few metres to hundreds of kilometres across. Most are found in the asteroid belt between the orbits of Mars and Jupiter and orbit the Sun in roughly circular paths.
Comets are balls of ice and dust, often called "dirty snowballs", that follow very elongated (elliptical) orbits taking them from the outer Solar System close to the Sun and back out again.
Part 3 of 7Stars, galaxies and the Universe
Stars like our Sun are not evenly scattered in space.
The Universe is everything that exists: all of space, matter and energy, including billions of galaxies. In order of increasing size: moon, planet, star, solar system, galaxy, cluster of galaxies, Universe.
Part 4 of 7The light-year
Distances beyond the Solar System are so large that metres and kilometres become awkward. Astronomers use the light-year: the distance that light travels through space in one year. Because light travels at 3.0 × 108 m s−1 and a year has about 3.15 × 107 s:
1 light-year = 3.0 × 108 × 3.15 × 107 ≈ 9.5 × 1015 m.
A light-year is a unit of distance, not of time. The nearest star after the Sun, Proxima Centauri, is about 4.2 light-years away. Within the Solar System, distances are often compared with the average distance from the Earth to the Sun, 1.5 × 1011 m, which light covers in about 500 s (8.3 minutes).
Part 5 of 7Scale and observations
The scale of the Universe is astonishing: the Moon is about 1.3 light-seconds from Earth, the Sun about 8 light-minutes, the outer planet Neptune about 4 light-hours, the nearest star 4 light-years, the centre of our galaxy about 26 000 light-years and the nearest large galaxy 2.5 million light-years.
- so we see it as it was then.
Part 6 of 7Putting the sizes in order
It helps to build a mental ladder of sizes.
Part 7 of 7Worked examples
Calculate the distance in metres of 1 light-year, using a speed of light of 3.0 × 108 m s−1 and 1 year = 3.15 × 107 s.
distance = speed × time = 3.0 × 108 × 3.15 × 107
= 9.5 × 1015 m.
Proxima Centauri is 4.2 light-years from Earth. Calculate this distance in metres, and the time in years that light takes to reach us.
Distance = 4.2 × 9.5 × 1015 = 4.0 × 1016 m.
Light takes 4.2 years to arrive, because one light-year is the distance light travels in a year.
The Sun is 1.5 × 1011 m from the Earth. How long does sunlight take to reach us?
time = distance ÷ speed = 1.5 × 1011 ÷ 3.0 × 108
= 500 s = 8.3 minutes.
Key terms
| Term | Meaning |
|---|---|
| Solar System | The Sun and all the objects bound to it by gravity. |
| Galaxy | A very large collection of stars, gas and dust held together by gravity. |
| Light-year | Distance travelled by light in one year, about 9.5 × 1015 m. |
| Asteroid | Rocky or metallic body orbiting the Sun, mostly in the belt between Mars and Jupiter. |
| Comet | Body of ice and dust in a highly elliptical orbit around the Sun. |
| Dwarf planet | Roughly spherical body orbiting the Sun that has not cleared its orbit. |
| Moon | Natural satellite orbiting a planet. |
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