CLASS 7 SCIENCE · CHAPTER 12 · STUDY NOTES
Earth, Moon, and the Sun
Explain daily sky changes, seasons and eclipses by following positions and light.
01 / EXPLORE & UNDERSTAND
The sky seems to move because we move
A moving observer can see a still object appear to move.
1. Imagine a turning ride
On a slowly turning merry-go-round, a nearby tree seems to move around you. The tree has not run around the ride: your direction of view is changing.
2. Apply this to sunrise
Earth turns while we stand on it. This makes the Sun appear to travel across the sky each day. The daily rising and setting do not mean that the Sun circles Earth once a day.
Your turn
Question
A tree appears to pass behind you on a turning ride. Must the tree be moving?
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02 / EXPLORE & UNDERSTAND
Earth spins from west to east
Rotation is a spin, not a journey around the Sun.
Find the axis and the direction of spin
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1. Choose the viewpoint
Looking down from above the North Pole, Earth rotates anticlockwise. We call this west-to-east rotation. Viewed from above the South Pole, the same spin looks clockwise; Earth has not reversed direction.
2. Use the approximate time carefully
For the day–night cycle we use about 24 hours. Earth’s turn relative to distant stars takes about 23 hours 56 minutes. Its movement around the Sun accounts for the small difference.
A little deeper: A historical explanation
Aryabhata compared the apparent motion of stars with still objects seeming to move backwards from a moving boat. Later, a Foucault pendulum provided a physical demonstration of Earth’s rotation. These examples connect an explanation with evidence.
Your turn
Question
Does rotation mean moving around the Sun?
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03 / EXPLORE & UNDERSTAND
Your location turns into and out of daylight
At any moment, roughly half of Earth faces the Sun.
Day and night exist at the same time
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1. Follow one sticker on a globe
Keep a lamp still and slowly rotate a globe west to east. A sticker on the lit side represents daytime. When the sticker turns to the unlit side, it represents night. Sunrise is entry into sunlight; sunset is departure from it.
2. Connect location with time
Different places face the Sun at different times. Broadly, places farther east reach their daylight cycle earlier. Exact sunrise times also depend on latitude, season and terrain. Earth’s revolution is not the cause of the daily cycle.
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Question
A place turns away from the Sun. What happens there?
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04 / EXPLORE & UNDERSTAND
Star trails reveal a turning viewpoint
A long-exposure photograph records the changing apparent positions of stars.
The arcs record apparent movement
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1. Look for the centre of the arcs
In a north-facing star-trail photograph, stars trace arcs around the north celestial pole. Earth’s axis points close to the Pole Star, so its apparent movement is small. This does not mean it sits directly above every observer.
2. Compare observations fairly
Record the place, date, time and a fixed landmark. Compare the same star pattern later that night. Clouds may hide it; a different viewing direction can also confuse the comparison. Some stars stay above the horizon rather than rising and setting.
Your turn
Question
Do star trails prove that all stars circle Earth once every day?
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05 / EXPLORE & UNDERSTAND
One orbit takes about a year
Earth rotates and revolves at the same time.
1. Separate the two motions
Earth spins on its axis and travels around the Sun. One revolution takes about 365 days and 6 hours. The orbit is an ellipse that is close to a circle, not the very stretched oval many drawings suggest.
2. Read diagrams with care
A slanted view makes a nearly circular path look flattened. Earth and Sun are usually drawn much too large compared with their separation. Use these diagrams to understand positions, not to measure actual distances.
A little deeper: Why calendars need adjustments
A year is not exactly 365 whole days. The extra fraction accumulates, so calendars use leap-year rules. “Add a day every four years” is a useful first idea, but the Gregorian calendar also has century exceptions.
Your turn
Question
Which motion gives the approximate length of a year?
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06 / EXPLORE & UNDERSTAND
Our night-facing direction changes during the year
Earth’s orbit changes which distant stars lie beyond its night side.
The night-facing direction changes
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1. Face away from the Sun
At midnight, your side of Earth faces broadly away from the Sun. Six months later Earth is on the opposite side of its orbit, so that night-facing direction points towards a different part of space.
2. Distinguish nightly and yearly changes
Changes across one night mainly show rotation. Changes at the same clock time across months reflect revolution as well. A given star pattern typically reaches a similar position about four minutes earlier each following night.
Your turn
Question
Why compare the sky at the same clock time across months?
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07 / EXPLORE & UNDERSTAND
A tilted axis sets up the seasons
During one orbit, the axis keeps pointing in nearly the same direction in space.
The axes keep nearly the same direction
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1. Compare June and December
Around June, the Northern Hemisphere leans towards the Sun. Around December it leans away. The Southern Hemisphere has the opposite arrangement. The axis does not turn to keep leaning towards the Sun all year.
2. Explain two heating effects
A hemisphere tilted towards the Sun receives more direct sunlight and generally longer days. Light spread over a smaller surface area heats it more strongly. Longer daylight gives more time for heating. Together these produce the seasonal pattern.
Your turn
Question
Name two reasons a hemisphere is warmer in its summer.
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08 / EXPLORE & UNDERSTAND
Opposite hemispheres have opposite seasons
Distance from the Sun cannot explain opposite seasons at the same time.
The same light spreads over different areas
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1. Use a counterexample
In December, the Northern Hemisphere has winter while the Southern Hemisphere has summer. Both belong to the same Earth at almost the same distance from the Sun. Tilt and daylight explain this contrast.
2. Allow local differences
Seasons do not give every place the same weather. Latitude, height, winds and nearby seas matter. Near the Equator, day length changes relatively little; rain patterns may be more noticeable than temperature changes.
Your turn
Question
Would “Earth is farther from the Sun” explain northern winter and southern summer together?
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09 / EXPLORE & UNDERSTAND
The year has turning points in day length
Solstices and equinoxes describe Earth’s seasonal geometry.
Compare the lit and dark parts of a latitude
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1. Locate the four milestones
The Northern Hemisphere’s longest day is near the June solstice and its shortest is near the December solstice. The March and September equinoxes lie between them. Exact calendar dates vary slightly from year to year.
2. Compare equator and poles
Near the Equator, daylight stays close to 12 hours. At the poles, long periods of continuous daylight alternate with continuous darkness. The textbook’s six-month description is approximate; sunrise and sunset are not instantaneous switches.
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Question
When the north has its longest day, which kind of day does the south have?
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10 / EXPLORE & UNDERSTAND
A nearby small object can hide a faraway large one
What fills your view depends on size and distance together.
Near and small can hide far and large
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1. Try an ordinary-object comparison
A thumb held near your eye can hide a distant building. The thumb is not physically larger. It covers a similar angle in your view because it is much closer. Use ordinary objects for this comparison, never the Sun.
2. Apply this to the Moon
The Moon is much smaller than the Sun but much closer to Earth. Their apparent sizes are similar, so the Moon can sometimes cover the Sun’s bright disc. Their changing distances mean the match is not always exact.
Your turn
Question
If the same object moves farther away, how does its apparent size change?
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11 / EXPLORE & UNDERSTAND
Solar eclipse: the Moon’s shadow reaches Earth
Order along the alignment: Sun → Moon → Earth.
The Moon is in the middle
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1. Find who blocks whom
The Moon lies between Sun and Earth. Within the small central shadow, observers may see the Sun’s bright disc completely covered: a total eclipse. Nearby observers may see only part covered: a partial eclipse.
2. Keep the effect local
The entire Earth does not become dark. The shadow covers a limited region and moves across Earth. Totality at one place is brief. If the Moon appears too small to cover the whole disc, a bright ring remains: an annular eclipse.
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Question
Which body casts the shadow in a solar eclipse?
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12 / EXPLORE & UNDERSTAND
Enjoy an eclipse without risking your eyes
A dim-looking Sun can still harm the eyes.
1. Choose supervised viewing
Join a teacher-led or planetarium session. For an indirect pinhole projection, look at the image on the screen, not through the hole at the Sun. A photograph or live stream is another way to observe safely.
2. Know what does not protect you
Ordinary sunglasses are not solar viewers. Never look through binoculars, telescopes or camera optics towards the Sun without specialist solar equipment and expert supervision. This chapter does not ask you to observe the Sun directly.
A little deeper: An eclipse is a predictable alignment
The Moon’s motion and the shadow geometry explain an eclipse. There is no scientific reason to avoid ordinary food because of an eclipse. The real observation risk is exposing the eyes to unsafe sunlight.
Your turn
Question
In an indirect projector, where should you look?
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13 / EXPLORE & UNDERSTAND
Lunar eclipse: Earth’s shadow reaches the Moon
Order along the alignment: Sun → Earth → Moon.
Earth is in the middle
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1. Find the shadowed body
Earth comes between the Sun and Moon. A total lunar eclipse occurs when the whole Moon is inside Earth’s dark central shadow; a partial one covers only part. Many people on Earth’s night side can see it if the Moon is above their horizon.
2. Explain the reddish colour
During a total eclipse, some sunlight passes through Earth’s atmosphere and bends towards the Moon. Much of the blue light is scattered away, leaving reddish light. A lunar eclipse can be watched with the unaided eye; it is not the same eye hazard as viewing the Sun.
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Question
Which eclipse places Earth in the middle?
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14 / EXPLORE & UNDERSTAND
Why eclipses do not happen every month
Being between two bodies is not enough: the alignment must also be close.
1. Allow for the Moon’s tilted orbit
The Moon’s orbital plane is tilted relative to Earth’s orbital plane. Most new and full moons pass above or below the exact alignment needed for an eclipse. This supporting idea explains why eclipses are special events.
2. Distinguish phases from eclipses
Ordinary Moon phases show changing views of its sunlit half. They are not caused by Earth’s shadow. Earth’s shadow explains a lunar eclipse only when the alignment is right.
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Question
Is an ordinary crescent Moon partly hidden by Earth’s shadow?
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Sign inNew here? Sign up freeCHAPTER RECAP
Take these ideas with you
- Rotation causes the daily day–night cycle.
- Revolution takes about one year.
- Tilt changes sunlight angle and day length, producing seasons.
- Opposite hemispheres have opposite seasons.
- Solar eclipse: Moon in the middle. Lunar eclipse: Earth in the middle.
- Moon phases are not Earth’s shadow.
Use your understanding in a new situation
Question
A student says the whole Earth has winter because it moves farther from the Sun. Give a counterexample.
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Which motion best explains the Sun crossing the sky during one day?
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