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Lesson pack · IGCSE Physics 0625 · 6.1.1 · Core

The Earth, day, night and seasons

Spin and tilt. Two motions shape our calendar.

Student lesson Lab, full screen
At a glance

The shape of the lesson

Topic
The Earth and the Solar System
Syllabus reference
Cambridge IGCSE Physics 0625, 6.1.1
Level
Core
Duration
45 minutes, lab-led; stretches to a 60 minute block (see the contingency notes)
Position in topic
Lesson 1 of 5 in The Earth and the Solar System; leads into Orbital speed
Central model
The Earth rotates on its tilted axis once every 24 hours, giving day and night, and orbits the Sun once a year.
Cooperative structure
Assessment
Stage 1 check and the exam-style plenary from the student lesson, plus the worksheet as the exit task
Learning objectives

By the end of the lesson, learners can

Section by section
  • Turn the Earth: Spin the Earth and orbit it round the Sun, and watch day, night and the seasons appear.
  • Three effects, two motions: Rotation gives day and night, the orbit gives the year, and the tilt gives the seasons.
Key points to leave on the board
  • Rotation: once in about 24 hours, giving day and night.
  • Orbit: once in about 365 days (a year); the Moon orbits the Earth in about a month.
  • Seasons: caused by the tilt of the axis, not by distance from the Sun.
The core visual model

One picture every idea returns to

The Earth rotates on its tilted axis once every 24 hours, giving day and night, and orbits the Sun once a year. The tilt of the axis causes the seasons, as each hemisphere leans toward or away from the Sun.

Lesson sequence

Forty-five minutes, phase by phase

TimePhaseWhat happens in the roomGrouping
0 to 5 minHook: predictOpen with the question in the title, Spin and tilt.. Two motions shape our calendar.Whole class, then pairs
5 to 17 minTeach and check: Turn the EarthSpin the Earth and orbit it round the Sun, and watch day, night and the seasons appear. Project tab 2 of the lab (Earth, day and night, the Moon) and let a student drive it while the class predicts.Whole class, then pairs
17 to 30 minTeach and check: Three effects, two motionsRotation gives day and night, the orbit gives the year, and the tilt gives the seasons.Frayer Model
30 to 36 minCheckThe four Stage 1 questions from the student lesson, answered on mini whiteboards or by show of fingers. Re-teach the one most get wrong.Individual, then whole class
36 to 43 minPlenaryThe exam-style questions from Stage 2, one at a time: thirty seconds alone, then a random call. The feedback lines in the key give the examiner's wording.Individual, random call
43 to 45 minExit and homeworkSet the worksheet below (6 questions, 13 marks). Learners self-assess against the objectives before they leave.Individual
Timing and contingency

Protect the parts that carry the learning

The sequence carries about fifty minutes of material, so the lab is driven by one student while the class predicts rather than explored freely. Times are a guide.

Protected: the check at 30 minutes. It is the only individual read on whether the key idea landed, and it is not cut.

Cut first if the build overruns: the last check in Three effects, two motions, never the check or the plenary.

In a 60 minute block: run worksheet questions 1 to 3 in class as a Rally Coach set and model both the hardest worked example and its check live.

Running the cooperative task

Frayer Model

Pairs fill a four-box grid for the key term: definition, characteristics, examples and non-examples. The non-examples box is where the misconceptions surface, so give it the most time.

The full structure, with its variations and the other twelve, is on the cooperative-learning page.

Examiner traps to pre-empt

What to head off, and how

Trap learners fall intoTeaching move that pre-empts it
The seasons are caused by the tilt of the Earth’s axis, not by the Earth being nearer to or further from the Sun.Day and night come from the Earth’s rotation, not from its orbit.
Worksheet

The Earth, day, night and seasons: worksheet

6 questions, 13 marks. Written in the style of the papers; no past paper question is reproduced.

NameClassDate
Q1 · analysis[2 marks]

Explain what causes day and night on the Earth.

Q2 · analysis[2 marks]

State how long the Earth takes to orbit the Sun, and how long the Moon takes to orbit the Earth.

Q3 · analysis[2 marks]

The Sun appears to move across the sky during the day. Explain why, and state the direction it appears to move.

Q4 · analysis[3 marks]

Explain why the northern hemisphere has summer in June. Refer to the tilt of the Earth's axis.

Q5 · analysis[2 marks]

A student says the seasons happen because the Earth is closer to the Sun in summer. Use the two hemispheres to explain why this cannot be the reason.

Q6 · analysis[2 marks]

It is midday for a person standing on the Earth. Describe where they are in relation to the Sun, and state what they will see about 12 hours later.

Answer key and marking notes
Q1 · 2 marks
  • The Earth spins on its axis once in about 24 hours. ✓
  • The half facing the Sun has day; the half facing away has night. ✓
Q2 · 2 marks
  • The Earth orbits the Sun in about 365 days (one year). ✓
  • The Moon orbits the Earth in about one month. ✓
Q3 · 2 marks
  • The Earth is rotating, which makes the Sun appear to move (the Sun itself is not going round us). ✓
  • It appears to rise in the east and set in the west. ✓
Q4 · 3 marks
  • In June the northern hemisphere is tilted toward the Sun. ✓
  • It receives more direct sunlight. ✓
  • The days are longer, so it is warmer: summer. ✓
Q5 · 2 marks
  • When the north has summer, the south has winter at the same time. ✓
  • Both hemispheres are the same distance from the Sun, so distance cannot be the cause; the tilt is. ✓
Q6 · 2 marks
  • At midday they are on the side of the Earth facing the Sun. ✓
  • About 12 hours later the Earth has turned halfway, so they face away from the Sun: it is night (midnight). ✓
Quiz

3 multiple-choice questions on this lesson

From the topic question bank. Assign them in the app for a marked score in your gradebook, or run the topic as a class game.

Q11 mark

What causes day and night on the Earth?

sunlight day night
  • Athe Earth rotating once on its axis each day
  • Bthe Sun orbiting the Earth once a day
  • Cthe Earth orbiting the Sun once a day
  • Dthe Moon passing in front of the Sun
Q21 mark

The Sun appears to rise in the east and set in the west. Why?

  • AThe Earth spins from west to east, so the Sun appears to move the opposite way.
  • BThe Sun really travels around the Earth from east to west each day.
  • CThe Earth orbits the Sun once each day.
  • DThe Earth wobbles back and forth on its axis.
Q31 mark

What is the main cause of the seasons on Earth?

  • Athe tilt of the Earth's axis as it orbits the Sun
  • Bthe changing distance between the Earth and the Sun
  • Cthe Sun giving out more heat in summer
  • Dthe phases of the Moon
Quiz key
Q1: A

The Earth spins on its axis about once every 24 hours; the half facing the Sun has day and the half facing away has night. The Sun does not orbit the Earth, and one orbit of the Sun takes a year, not a day.

Q2: A

Because the Earth rotates from west to east, the Sun appears to move across the sky in the opposite direction, rising in the east and setting in the west. The Sun is not actually orbiting the Earth.

Q3: A

The Earth's axis is tilted, so as it orbits the Sun each hemisphere is angled toward the Sun for part of the year (summer) and away for another part (winter). The small change in Earth-Sun distance is not the cause.

Lab and demo

What to project

The student lesson embeds these tabs. Open them full screen on the projector; every slider has a drag handle on the stage.

Slides

Slides for this lesson

A projectable deck for every pack is on the way. Until then, present the student lesson full screen: its sections, figure and lab tabs follow the same order as the plan above.

Also for this topic

Everything else you can use

Original work by the TheLucidSTEM team. The worksheet items are written in the style of the papers; no past paper question is reproduced.