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GROW · Science · Week 8A · Explore

Day and Night: Sky Shift

Learning objective

I can explain that Earth's rotation causes day and night and makes the Sun appear to move across our sky.

Success looks like

  • Identify the lit side of Earth as day and the unlit side as night.
  • Sequence one place on Earth through a full rotation.
  • Use rotate and apparent to explain what an observer sees.

We will observe, work together, then use the evidence ourselves.

Arrival task

Arrival task

Choose a route. Think first, then check the answers together.

1. Light and viewpoint

The Moon stays spherical. Why can the lit part we see look different?

The Sun lights about half the Moon. As it orbits Earth, our viewpoint changes which part of that lit half we see.

2. Rotation and orbit

What does it mean to say Earth orbits the Sun?

Orbit = travel around another body. Rotation = turn on an axis.

3. A useful model

Why keep a model Sun lamp fixed while testing what happens as a globe turns?

The lamp represents the Sun. The investigation changes the globe’s rotation only.

4. A place in light

A marked place on the globe turns from the lit half into the unlit half. What would this model for someone there?

Lit = receiving sunlight. Unlit = facing away. Track the same place.

Starter

Starter

“It is night here. Has the Sun switched off?”

Make a prediction. Use a ball and a fixed light, or your hands, to show what could change.

We will test the explanation with a model.

I do

I do · turn Earth, track one place

Earth turns; the model Sun stays to the leftView from above the North Pole. The left half of Earth is lit. A marked place turns anticlockwise from top to left to bottom to right.SunDAYNIGHTNorth-pole viewOne daily turn ≈ 24 hRed dot:one place

Sunrise: our place is entering the lit half.

Simplified view from above the North Pole. The dot represents a place away from the poles. Size, distance and time are not to scale; equal stages do not mean equal daylight everywhere. Keep the Sun fixed for this short daily model.

Rotate means turn on an axis: an imaginary line through Earth. A quarter turn is one of four equal turns making a full turn. Lit means receiving light. A daily cycle is about 24 hours.

We do

We do · organise one daily cycle

Use the arrows to organise the steps. Read the sequence aloud before checking.

  1. Sunset · our place leaves the light
  2. Sunrise · our place enters the light
  3. Night · our place faces away
  4. Middle of the day · our place faces the Sun

Use Up and Down to organise the steps.

I do

I do · change the viewpoint

Stand in for the marked observer. Turn slowly while keeping a fixed object in view.

As you turn, the fixed object appears to move across your view.

Use a finger or paper arrow if you prefer to stay still.

The observer sees the Sun appear to cross the sky from east to westEastWestObserver’s simplified view

Morning: the Sun appears in the eastern sky.

A sketch of apparent daily movement, not a precise path for every date or location.

Apparent means how something seems from a viewpoint. Rotation is Earth turning on its axis; orbit is travelling around another body.

We do

We do · sketch and orientate

Sketch an Earth circle. Put the Sun on the left. Shade Earth’s right half.

Mark a place at the top, then predict where it goes next. Add a rotation arrow.

From this north-pole view, where does the top marker go next?

You do

You do · explain day and night

Use the supplied evidence. Write, draw, point, explain or direct an adult.

Open evidence and reference diagrams

Model evidence: fixed Sun on the LEFT; RIGHT half unlit; view from above the North Pole. Follow the same marked place TOP → LEFT → BOTTOM → RIGHT → TOP.

C · Sunrise

SunDAYNIGHTNorth-pole view

Entering light. Sun appears low in the east.

D · Middle of day

SunDAYNIGHTNorth-pole view

Facing light. Sun appears higher across the sky.

B · Sunset

SunDAYNIGHTNorth-pole view

Leaving light. Sun appears low in the west.

A · Night

SunDAYNIGHTNorth-pole view

Facing away. Sun appears below the local horizon.

Rotation = turning on an axis (an imaginary line through Earth). Apparent = how something seems from the observer’s viewpoint. Cycle = a sequence that returns to its start.

Earth rotates west to east, anticlockwise in this view. A daily cycle is about 24 hours. The observer turns with Earth, so the Sun appears to move east to west. The lamp stays on; no clouds are needed.

Supplied model observations, not pupil measurements. Size, distance and time are not to scale. Equal quarter turns simplify season and latitude; they do not establish 12 hours of daylight everywhere.

Standard

1. Draw four Earth circles. In EVERY picture put the Sun on the LEFT; shade the RIGHT half of Earth. View the circles from above the North Pole.

Help with this question

Before adding a marker, check that the light comes from the same side in all four frames.

2. Mark the same place at the TOP in picture 1, LEFT in picture 2, BOTTOM in picture 3 and RIGHT in picture 4. Add anticlockwise rotation arrows.

Help with this question

Keep one marker identity throughout. Check the viewing direction before drawing an arrow.

3. Label the four moments: sunrise, middle of the day, sunset, night. Use the evidence: entering light; facing the Sun; leaving light; facing away.

Help with this question

Use the marker’s movement into or out of the lit half to distinguish sunrise from sunset.

4. Explain day and night using 'Earth rotates'. Then finish: 'The Sun appears to move across the sky because…'.

Help with this question

Link an Earth movement to a change in illumination. For the second sentence, imagine looking out from the marker.

5. State about how long one full daily turn takes. Give one thing the model simplifies.

Help with this question

Give an approximate duration, then name a feature your small, quickly turned diagram cannot reproduce exactly.

Exit

Exit ticket

Use your book OR one ticket. Show your explanation with the supplied evidence. Say it, write it, draw it, sign it, choose it or show it; an adult can scribe it.

Model view: above the North Pole. The Sun is on the LEFT; Earth’s RIGHT half is unlit. X marks a place on the RIGHT, away from the poles. The lamp stays on. Size, distance and equal stages are simplified.

1. Explain why X has night and how it will reach daylight. Include Earth’s movement.

Help with this question

Link the direction of the light to what happens to one place as Earth turns.

2. Why does the Sun appear to cross our sky? About how long is one daily cycle?

Help with this question

Imagine standing at X and turning with Earth. Separate what you see from what causes it.

Pause

Take a quiet pause.

You can look away from the screen. Come back when you are ready.

The lesson and your work are still here. Close this box to return.

Cold Call

Give thinking time. Invite a response by voice, pointing or showing work. A pupil can pass; check in privately when useful.

Lesson tools

W8B · Day and Night: 24-Hour Control Room

Choose a slide or a print route.

Knowledge organiser

Teacher Print Tools

Print a complete pupil pack here, or print just the selected arrival questions from the Arrival task slide. Each pack includes the organiser, supported questions and the selected exit route. Teacher answers are separate in TA Brief.

Knowledge organiser

One A4 reference sheet for your book.

GROW Knowledge Organiser A4 printable science reference or exit task. All text and diagrams are included in this file. GROW SCIENCE | KNOWLEDGE ORGANISER Day and night Made by Matt LEARNING OBJECTIVE I can explain that Earth's rotation causes day and night and makes the Sun appear to move across our sky. SUCCESS CRITERIA 1. Identify the lit side of Earth as day and the unlit side as night. 2. Sequence one place on Earth through a full rotation. 3. Use rotate and apparent to explain what an observer sees. One place moves through light and dark Sun DAY NIGHT 1 2 3 4 North-pole view 1 Sunrise: entering light 2 Middle of day: facing Sun 3 Sunset: leaving light 4 Night: facing away Turn anticlockwise: 1 → 2 → 3 → 4. Words that explain the model Rotation Turning on an axis. Axis Imaginary pole-to-pole line. Orbit A path around another body. Apparent How it seems from a viewpoint. Cause and what we observe Earth rotates west to east. We turn with Earth, so the Sun appears to move east to west across the sky. One daily cycle ≈ 24 hours Earth’s yearly orbit is a different movement. A complete explanation Earth rotates, carrying our place into sunlight and then away into the unlit half. The Sun stays lit. The changing direction of our view makes its daily movement apparent. Use the model carefully Size, distance and tilt are simplified. Equal quarter turns do not prove 12 hours of daylight everywhere; day length varies with place and season.

Word help

rotation

Turning on an axis.

axis

An imaginary line through Earth from pole to pole.

apparent

How something seems from a particular viewpoint.

orbit

The path of one body around another.

TA Brief

Current stage

Preparation

Use the supplied diagrams, cards and booklet. An optional cool LED lamp, globe and removable marker can represent the same model. Keep cables secure and sufficient room light for safe movement. Never look at the real Sun or into a bright lamp. Pointing and pupil-directed drawing are equivalent routes.

Real-world link

Choose a route at each task, using what the pupil shows. Switching takes no extra task, record or label.

Teacher answers

Shared activities

C → D → B → A: TOP sunrise, LEFT middle of day, BOTTOM sunset, RIGHT night. Anticlockwise from above the North Pole; west-to-east Earth rotation. Sun appears to move east to west. A daily cycle is about 24 hours. The fixed lamp stays on. Equal stages do not establish equal daylight everywhere.

Supported arrival

  • 1. The Sun lights the Moon. We see reflected sunlight.
  • 2. Earth orbits the Sun.
  • 3. Keep the lamp still and track the marked place as the globe turns.
  • 4. The lit side. This models daytime at that place.

Supported independent task

  • 1. C, D, B, A: sunrise, middle of the day, sunset, night.
  • 2. Keep the Sun LEFT. Move TOP → LEFT → BOTTOM → RIGHT → TOP; anticlockwise from above the North Pole.
  • 3. TOP C/sunrise; LEFT D/middle of day; BOTTOM B/sunset; RIGHT A/night.
  • 4. Facing the Sun gives day. Facing away gives night. Earth rotates.
  • 5. Our place turns away from the Sun. The model lamp stays on.

Supported exit

  • 1. X is in night. Earth rotates, carrying X around into the lit half. Accept a clear demonstration with explanation, signing or exact scribing.
  • 2. About 24 hours. The Sun continues shining during our night; our place faces away from it.

Standard arrival

  • 1. The Sun lights about half the Moon. As the Moon orbits Earth, our viewpoint shows different amounts of that lit half.
  • 2. Earth travels around the Sun. One orbit takes about a year.
  • 3. It lets us see the effect of the globe turning without also changing the light's position.
  • 4. A transition towards night: sunset as the place leaves the lit half. This is a prediction to test with the model.

Standard independent task

  • 1. Four circles, each with the Sun LEFT and the RIGHT half shaded.
  • 2. Same marker: TOP, LEFT, BOTTOM, RIGHT. Anticlockwise arrows in this north-pole view.
  • 3. Sunrise/entering light; middle of day/facing Sun; sunset/leaving light; night/facing away.
  • 4. Earth rotates, carrying a place into and out of sunlight. We turn with Earth, so the Sun appears to move across our sky.
  • 5. About 24 hours. A valid limit is scale, compressed time, simplified tilt, season or latitude. Equal model stages do not prove 12 hours of daylight everywhere.

Standard exit

  • 1. X faces away from the Sun, so it has night. Earth rotates, carrying X into the sunlit half and daylight. Anticlockwise in this north-pole view is correct.
  • 2. We turn with Earth, so the Sun appears to move across our view. Earth rotates west to east and the apparent daily Sun movement is east to west. One daily cycle is about 24 hours; compass directions may extend a correct causal explanation.

Stretch arrival

  • 1. No. About half is sunlit, but from Earth we see only a thin part of the lit half. A crescent is not Earth's shadow covering most of the Moon.
  • 2. Rotation is turning on an axis; orbit is travelling around another body.
  • 3. Valid examples: sizes and distances are not to scale; the nearby lamp's rays spread more than sunlight at Earth; a quick turn compresses time; Earth's tilt may be simplified.
  • 4. Earth rotates, carrying the observer with it, so the direction they face changes relative to the Sun. Test this with the fixed-lamp model.

Stretch independent task

  • 1. Keep the Sun fixed left. Four frames explain the daily pattern with Earth rotating; do not infer a daily Sun orbit from an apparent path.
  • 2. TOP sunrise; LEFT middle of day; BOTTOM sunset; RIGHT night. Right half shaded; anticlockwise rotation.
  • 3. Observer: “The Sun appears to cross my sky.” Actual motion: Earth rotates west to east, carrying us with it; the daily apparent Sun movement is east to west.
  • 4. Moving the lamp can reproduce changing light but gives the wrong moving object for the accepted explanation of the real daily cycle. The classroom model alone does not establish every astronomical claim.
  • 5. The marker shows one place entering and leaving sunlight. Size, distance, time, latitude and seasons are simplified; equal quarter-turn stages do not establish 12 hours of daylight everywhere.

Stretch exit

  • 1. X is on the unlit half. Earth rotates west to east, anticlockwise in this view, carrying X into sunlight. An observer turns with Earth and sees the Sun appear to move east to west.
  • 2. About 24 hours. No: equal stages are a model simplification; daylight length varies with latitude and season. The diagram does not establish equal daylight everywhere.

NASA: Earth facts · NASA: a daily cycle

Next teaching after W8B: w/c 2 November, after half term.

Made by Matt