5.7Chapter 5: The Earth in Space
Changing ideas 2: geocentric model — Alhussan Physics - Stage 7 Revision Notes & Topical Questions
5 min read 7 parts Lesson 7 of 11 1 quiz
Lesson summary
Physics 5.7 Changing ideas 2: geocentric model — Ptolemy vs Copernicus — Alhussan International Academy — Physics (Stages 7–9) notes: Describe the geocentric model, the evidence for it, the observation it could not simply explain, and why the heliocentric model replaced it.Geocen…
- Plato and Aristotle
- Seven planets
- Crystalline spheres
- Everyday experience
- Falling objects
- Stars above and below the horizon
Part 1 of 5The Greek geocentric model
Geocentric
Earth-centred, since "geo" means Earth in Greek.
Plato and Aristotle
- Greek astronomers who lived about 2400 years ago and developed the model.
- The Earth did not move; the stars and planets moved around it.
- All objects, including the Earth, were spherical and moved at a steady speed.
Seven planets
- Mercury, Venus, Mars, Jupiter, Saturn, the Sun and the Moon, with the stars beyond them.
Crystalline spheres
- Objects were carried round on invisible spheres that light could travel through.
- The Moon was on the sphere closest to the Earth.
- The stars were on the sphere furthest from the Earth.
Part 2 of 5Why the geocentric model was believed
Why the geocentric model was believed
Everyday experience
- The ground does not feel as if it is moving, which supported a stationary Earth at the centre.
Falling objects
- Greek philosophers thought all objects fall towards the centre of the Universe, and dropped objects fall to the Earth.
Stars above and below the horizon
- Ptolemy saw that half the stars are above the horizon and half below at any time.
- This fits an Earth at the centre; if it were not central the numbers would differ.
No apparent shift of the stars
- If the Earth moved round the Sun, stars would seem to change position between January and July.
- No shift could be seen without a telescope.
- Stars are so far away that the shift is too small for ancient astronomers to detect.
Success
- The model explained many observations and made predictions, and it fitted what people could see and feel.
Part 3 of 5The observation that was a problem
Retrograde motion
- Planets seem to wander across the sky and sometimes move backwards against the stars before resuming their normal direction.
Ptolemy
- A Greek astronomer who lived about 1800 years ago and changed the model to explain this motion.
- He added small circles (epicycles) on top of the larger circles that were the planets' paths.
- He worked out the size needed to explain the backward motion and predicted future planet positions.
- His book describing the model was used for hundreds of years.
Drawback
- The epicycles worked for predictions but made the model more and more complicated.
Part 4 of 5Copernicus and the heliocentric model
Copernicus and the heliocentric model
Heliocentric
Sun-centred, since "helio" means Sun.
Copernicus
- In his model the planets orbit the Sun.
- The backward motion is a natural result of the Earth overtaking an outer planet, like a faster car passing a slower one.
- This explains the planets' motion more simply than epicycles.
Why scientific explanations change
- They change when there is new evidence, often from things people cannot immediately see.
Part 5 of 5Geocentric and heliocentric models compared
| Feature | Geocentric (Ptolemy) | Heliocentric (Copernicus) |
|---|---|---|
| Centre | Earth | Sun |
| Planets' backward motion | Needs epicycles | Natural result of orbits |
| Apparent shift of stars over a year | No shift expected | Shift expected but too small to see |
| Simplicity | Complicated | Simpler |
Key terms
| Term | Meaning |
|---|---|
| Geocentric model | A model of the Universe with the Earth at the centre. |
| Heliocentric model | A model with the Sun at the centre of the Solar System. |
| Crystalline sphere | An invisible sphere thought to carry the Moon, Sun, a planet or the stars. |
| Retrograde motion | The apparent backward movement of a planet against the stars. |
| Epicycle | A small circle added to the geocentric model so that planets could move backwards. |
Avoid these mistakes
1
Thinking people were foolish to believe the geocentric model — it fitted observations and made good predictions.
2
Thinking Copernicus proved the Earth moves — his model was simpler, but more evidence was needed.
3
Mixing up the prefixes — geo means Earth and helio means Sun.
4
Thinking stars do not shift because the Earth is still — they shift too little to see because they are very far away.
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