PHYSICS · Stage 7 · Chapter 5: The Earth in Space
Physics 5.10 Chapter 5 Review: The Earth in Space
5 min read 5 parts Lesson 10 of 11
Lesson summary
Physics 5.10 Chapter 5 Review: The Earth in Space — Alhussan International Academy — Physics (Stages 7–9) notes: Summarise the Earth's spin and orbit, distances in the Solar System, models of the Universe and the use of planetary data.Spin — The Earth spins on its axis once every…
- Objects seen from Earth
- Large distances
- Astronomy and experiments
- Heliocentric model
- Telescope evidence
- Atmospheres
Part 1 of 5Spin, orbit and the seasons
- Spin — The Earth spins on its axis once every 24 hours, causing day and night.
- The Sun does not orbit the Earth once a day.
- Orbit — The Earth orbits the Sun once in about 365 days, which is one year.
- Seasons — The tilt of the Earth's axis (23.5 degrees) causes the seasons.
Part 2 of 5Objects and distances in the Solar System
- Objects seen from Earth — With the naked eye or a telescope we see the Sun, the Moon, planets, stars, comets, meteors and artificial satellites.
- Large distances — Mercury is about 60 million km from the Sun and the Earth is about 150 million km from the Sun.
- The Earth is 150 ÷ 602.5 times further from the Sun than Mercury.
- The Earth is 150 − 6090 million km further away.
- Pattern — Planets nearer the Sun are generally hotter and have shorter orbit times.
Part 3 of 5Geocentric and heliocentric models
- Astronomy and experiments — Astronomers cannot do experiments on the Universe, so they make observations and develop explanations to account for them.
- Heliocentric model — The Sun is at the centre and the planets orbit it.
- It explains the apparent backward motion of planets more simply than the geocentric model.
- It also explains the phases of Venus.
- Telescope evidence — Galileo's observations of Jupiter's moons and sunspots helped the heliocentric model replace the geocentric model.
Part 4 of 5Using data about planets
- SourcesData from a science book is secondary data and should be checked against other sources.
- ComparingCompare planets' mass, distance from the Sun and temperature to look for patterns.
- AtmospheresThe atmospheres of the outer planets differ from those of the inner planets.
- TestingExplanations should be tested against more evidence.
Part 5 of 5Key facts in a table
| Topic | Key fact |
|---|---|
| Day and night | The Earth spins once every 24 hours |
| Seasons | Axis tilted by 23.5 degrees; the Earth orbits the Sun in 365 days |
| Moon | Reflects sunlight; its phases and eclipses result from its orbit |
| Solar System | Eight planets, dwarf planets, asteroids and comets held by gravity |
| Models | The heliocentric model explains planet motion more simply than the geocentric model |
Last updated: