Primary General Studies: The Solar System and the Movement of the Earth (Paper 3 (challenge))
- 2026-11-13
Primary General Studies: The Solar System and the Movement of the Earth (Paper 3 (challenge))
Paper three chains the steps: hours to degrees, longitude to time zones, light speed to seconds, then shadows and daylight explain the seasons.
Direct answers On any two-step question write the middle number first, then substitute, and only put the units at the end.
01 Paper details (check answers afterwards)
| Item | Detail |
|---|---|
| Questions | 10 |
| Suggested time | 20 |
| Difficulty mix | Foundation 3 · Intermediate 3 · Challenge 3 · Error redo 1 |
| Chapter | Chapter: Primary General Studies: The Solar System and the Movement of the Earth |
| Level | parts of a closed circuit, conductors against insulators, series against parallel, adding up battery voltage, and electrical safety |
02 Questions (10 items)
- FoundationThrough how many degrees does the Earth turn in three hours?
- FoundationTwo places differ by 90 degrees of longitude. How many hours apart are they?
- FoundationHong Kong is 8 hours ahead of London. When it is 8 pm in Hong Kong, what time is it in London?
- IntermediateThe Moon is about 384,400 km away and light travels 300,000 km a second. How long does moonlight take to arrive?
- IntermediateA year has 365 days and one cycle of moon phases lasts 29.5 days. How many whole cycles fit in a year?
- IntermediateThe equator is about 40,000 km round and the Earth turns once a day. How fast does the ground at the equator move each hour?
- ChallengeAn orbit takes 365 days. How long is half a year?
- ChallengeOn a sunny day, when is a shadow shortest?
- ChallengeWhy are summer days so long in the northern hemisphere?
- Error redoError clinic: “Seasons happen because the Earth is sometimes nearer the Sun.” Why is that inaccurate?
03 Answers and one-line notes
| # | Answer | One-line note |
|---|---|---|
| 1 | 45 degrees. | At 15 degrees an hour, 15 × 3 = 45. |
| 2 | Six hours. | Every 15 degrees is one hour, so 90 ÷ 15 = 6 hours. |
| 3 | Noon, 12 pm. | 20 minus 8 is 12, so London is still at midday. |
| 4 | About 1.28 seconds. | 384,400 ÷ 300,000 is about 1.28, so we see the Moon as it was 1.28 seconds ago. |
| 5 | About 12. | 365 ÷ 29.5 is about 12.37, so 12 whole cycles fit, which is why a year has twelve months. |
| 6 | About 1,666.7 km per hour. | 40,000 ÷ 24 is about 1,666.7, faster than any airliner. |
| 7 | 182.5 days. | 365 ÷ 2 = 182.5, half of the yearly circuit and half of the seasons. |
| 8 | Around noon, when the Sun is highest. | The higher the Sun, the closer the light is to vertical and the shorter the shadow. |
| 9 | The tilt of the axis combined with the Earth going round the Sun. | In summer the northern half leans towards the Sun, so it stays in sunlight longer. |
| 10 | The main cause is the tilted axis, not the small change in distance. | If distance were the cause, both hemispheres would have summer together, but their seasons are opposite. |
04 What to do after marking
- After marking, redo only the wrong items and write down which step went wrong (formula, unit, or misread number).
- Repeat the same item two days later; move to the next paper only when both attempts are correct.
- Parents only need the answer and note columns; there is no need to explain every item.
Paper four clears the conductor, insulator and battery direction misconceptions.Tutor Registration →
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