6.1.1Space Physics
The Solar System — Cambridge IGCSE Co-ordinated Sciences 0654 - Physics Revision Notes & Topical Questions
5 min read 10 parts Lesson 2 of 10
Part 1 of 8Members of the Solar System
Members of the Solar System
Sun
- Sun the one star at the centre of the Solar System.
Planets
- Planets eight planets orbit the Sun.
Dwarf planets
- Dwarf planets smaller planet-like bodies.
Satellites
- Satellites natural moons and artificial satellites.
Small bodies
- Small bodies asteroids and comets also orbit the Sun.
Part 2 of 8The eight planets
Order
- Order in increasing distance from the Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune.
- Memory aidMy Very Excellent Mother Just Served Us Noodles.
Inner planets
- Mercury, Venus, Earth and Mars are small and rocky.
Outer planets
- Jupiter, Saturn, Uranus and Neptune are large gas giants.
Part 3 of 8Dwarf planets
Description
- Description an object similar to a planet but much smaller.
Gravity
- Gravity its gravitational field is not strong enough to pull in or clear the nearby objects.
- (apart from its own natural satellites)
Example
- Pluto is classed as a dwarf planet.
Part 4 of 8Satellites
Natural satellite
- Natural satellite an object that orbits a planet, and a moon is one type.
- The Moon is the natural satellite of the Earth.
Artificial satellite
- Artificial satellite a man-made object that orbits another object in space.
- The International Space Station is an artificial satellite that orbits the Earth.
Part 5 of 8Asteroids and comets
Asteroid
- Asteroid a small rocky object that orbits the Sun.
- Most lie in the asteroid belt between Mars and Jupiter.
Comet
- Comet a body of dust and ice that orbits the Sun on a highly elliptical path.
- Comets are usually found in the outer reaches of the Solar System.
- Ice melts as a comet approaches the Sun and forms the comet's tail.
Part 6 of 8What orbits what
| Orbiting body | Body it orbits |
|---|---|
| Planet | The Sun |
| Moon | Planet |
| Asteroid | The Sun |
| Comet | The Sun |
| Artificial satellite | The Earth |
- Rule
- smaller bodies orbit larger ones.
Part 7 of 8Analysing planet data (Extended)
Comparing
- Comparing values can be compared between planets.
- Neptune is about 30 times further from the Sun than the Earth.
- Jupiter has about 320 times the mass of the Earth.
Trend
- Trend as the distance from the Sun increases, the orbital period increases.
- Mercury takes 0.24 Earth years and Neptune takes 160 years.
Trend
- Trend surface temperature generally falls with distance, from about 460 °C on Venus to −220 °C on Neptune.
Anomaly
- Venus is hotter than Mercury although it is further from the Sun.
Prediction
- Prediction a value for an unknown body can be estimated by interpolating between known planets.
Surface gravity
- Surface gravity g depends on the mass and radius of a planet: Mercury 3.7, Venus 8.9, Earth 9.8, Mars 3.7, Jupiter 23.1, Saturn 9.0, Uranus 8.7 and Neptune 11.0 N/kg.
Part 8 of 8More from the specification
1Central gravitational orbital force
- Central gravitational orbital force mutual gravitational attraction from the massive Sun exerts the centripetal force holding all planets in stable elliptical orbits.
2Rotation of Earth
- Earth spins once in about 24 hours, causing day and night as each side faces the Sun or turns away.
3Seasons
- Earth's axis is tilted,
- so the northern hemisphere gets summer when it is tilted toward the Sun, with longer daylight and stronger solar radiation per area.
4Orbit
- Earth orbits the Sun in about 365 days, so the southern hemisphere has opposite seasons to the north.
5Light travel
- Light from the Sun takes about 8 minutes to reach Earth, travelling at 3.0 × 108 m/s.
6Orbital speed
- Speed of an orbiting planet = circumference of orbit divided by orbital period, v = 2πr/T.
7Rotation of Earth
- Earth spins once in about 24 hours, causing day and night as each side faces the Sun or turns away.
8Seasons
- Earth's axis is tilted,
- so the northern hemisphere gets summer when it is tilted toward the Sun, with longer daylight and stronger solar radiation per area.
9Orbit
- Earth orbits the Sun in about 365 days, so the southern hemisphere has opposite seasons to the north.
10Light travel
- Light from the Sun takes about 8 minutes to reach Earth, travelling at 3.0 × 108 m/s.
11Orbital speed
- Speed of an orbiting planet = circumference of orbit divided by orbital period, v = 2πr/T.
12Orbital speed
- Speed of an orbiting object, √(GM/r).
13Field strength
- G = Fg/m.
14Kinetic energy
- K = ½mv2, energy of motion.
15Gravitational potential
- Work done per unit mass in bringing a test mass from infinity to the point.
16Potential energy
- Energy stored by the configuration of a system.
17Hemisphere
- Half of the Earth, northern or southern.
18Nebula
- Cloud of gas and dust in which stars form.
Key terms
| Term | Meaning |
|---|---|
| Solar System | The Sun and all the bodies that orbit it. |
| Planet | A large body that orbits the Sun and whose gravity clears its orbit. |
| Dwarf planet | A small planet-like body that has not cleared its orbit, such as Pluto. |
| Asteroid | A small rocky body orbiting the Sun, mostly in the asteroid belt. |
| Comet | An icy body on a highly elliptical orbit around the Sun. |
| Natural satellite | A moon orbiting a planet. |
| Artificial satellite | A man-made object orbiting a body in space. |
Avoid these mistakes
1
Pluto is the ninth planet — it is classed as a dwarf planet.
2
Comets orbit in circles — they have highly elliptical orbits.
3
The asteroid belt lies beyond Neptune — it lies between Mars and Jupiter.
4
A moon orbits the Sun directly — a moon orbits its planet.
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