Earth, Moon, and the Sun

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CLASS VII Science ~6 marks/year Ch 12 of 12
Earth, Moon, and the Sun

Class 7 · Science · NCERT chapter notes · Akanksha Classes

Snapshot
  • The Sun is the nearest star and the centre of our solar system; it gives light and heat to the Earth and is luminous.
  • The Earth spins on its own axis (rotation) once in about 24 hours, causing day and night.
  • The Earth’s axis is tilted at about 23.5°; this tilt plus the Earth’s journey around the Sun (revolution, about 365¼ days) causes the seasons.
  • The Moon is the Earth’s only natural satellite; it is non-luminous and shines by reflecting sunlight.
  • The changing shapes of the bright Moon seen from Earth are the phases of the Moon (new moon to full moon and back), repeating in about 29.5 days.
  • A solar eclipse occurs when the Moon comes between the Sun and the Earth; a lunar eclipse occurs when the Earth comes between the Sun and the Moon.
  • People have always observed the sky — stars, constellations and planets — using the eye and the telescope.
  • Board weightage: ~6 marks/year — 1-mark definitions, 2-mark cause/difference questions, 3-mark phases or eclipse answers.
Detailed Notes

1. The Sun — Our Nearest Star

The Sun is a huge, glowing ball of hot gases at the centre of our solar system. It is the nearest star to the Earth. The Sun is luminous — it gives out its own light and heat. Without the Sun there would be no light, no warmth, no food (plants need sunlight) and no life on Earth.

The Sun is the nearest star and the source of almost all the energy on Earth. It is so large that more than a million Earths could fit inside it, yet it appears small because it is very far away.

Light from the Sun takes about 8 minutes to reach the Earth, even though light is the fastest thing known. We must never look directly at the Sun, especially through a telescope or binoculars, as it can permanently damage the eyes.

2. The Earth’s Rotation and Day and Night

The Earth is shaped like a slightly flattened ball (a sphere). It is always spinning around an imaginary line passing through its centre, called the axis. This spinning is called rotation.

Rotation is the spinning of the Earth on its own axis. The Earth completes one rotation in about 24 hours (one day). It rotates from west to east.

2.1 How Day and Night Are Caused

The Earth is a non-luminous body. The Sun can light up only one half of the Earth at a time — the half facing the Sun has day, while the half facing away is in darkness and has night. As the Earth rotates, different parts come into the sunlight and then move into the shadow, so day and night follow each other continuously.

Because the Earth rotates from west to east, the Sun appears to rise in the east and set in the west. This apparent daily movement of the Sun and stars across the sky is actually caused by the Earth’s own rotation, not by the Sun moving.

NCERT Activity — Day and night with a globe and torch

In a dark room, shine a torch (representing the Sun) on a globe (representing the Earth). Only the half of the globe facing the torch is lit — this is day; the other half is dark — this is night. Slowly rotate the globe from west to east and watch how a marked spot (say India) moves from the lit side into the dark side and back. This shows how the Earth’s rotation causes day and night.

3. The Earth’s Revolution and the Seasons

Besides spinning on its axis, the Earth also moves around the Sun in a fixed path called an orbit. This movement around the Sun is called revolution.

Revolution is the movement of the Earth around the Sun in its orbit. The Earth completes one revolution in about 365¼ days (one year). The extra quarter day is adjusted by adding one day to February every fourth year — a leap year of 366 days.

3.1 The Tilt of the Earth’s Axis

The Earth’s axis is not straight up and down; it is tilted at an angle of about 23.5° from the vertical. This tilt stays in the same direction as the Earth revolves around the Sun. Because of the tilt, the two halves of the Earth (the Northern and Southern hemispheres) receive different amounts of sunlight at different times of the year.

3.2 How Seasons Are Caused

When the Northern Hemisphere is tilted towards the Sun, it receives more direct sunlight and has summer, while the Southern Hemisphere has winter. Six months later, when the Northern Hemisphere is tilted away from the Sun, it gets slanting, weaker sunlight and has winter, while the Southern Hemisphere has summer. This is why the seasons are opposite in the two hemispheres.

Seasons are caused by the tilt of the Earth’s axis together with its revolution around the Sun — NOT by the Earth being nearer to or farther from the Sun.
NCERT Activity — Slanting vs direct light

Shine a torch straight down onto a sheet of paper, then tilt the torch so the light falls at a slant. When the light is straight, the bright patch is small and intense; when slanting, the patch is larger and dimmer, spreading the same light over a bigger area. In the same way, when the Sun’s rays fall more directly on a region it gets hotter (summer), and when they fall at a slant the region gets less heat (winter).

4. The Moon — Earth’s Natural Satellite

The Moon is the natural satellite of the Earth — a body that revolves around the Earth. It is the brightest object in the night sky, but it is non-luminous: it has no light of its own and shines only because it reflects the light of the Sun.

The Moon is the Earth’s only natural satellite. It revolves around the Earth in about 27–29 days and shines by reflecting sunlight. It has no air, no water and no life.

The surface of the Moon has plains, mountains and many bowl-shaped pits called craters, formed by the impact of meteorites long ago. Because the Moon has almost no atmosphere, its sky always looks black and there is no sound on it. The first humans landed on the Moon in 1969 (the Apollo 11 mission). India’s Chandrayaan missions have also explored the Moon, with Chandrayaan-3 landing near the lunar south pole in 2023.

5. Phases of the Moon

Every night the Moon seems to change its shape — sometimes a thin crescent, sometimes a half disc, sometimes a full bright circle, and sometimes not visible at all. These different shapes of the bright part of the Moon are called the phases of the Moon.

5.1 Why the Phases Happen

The Moon does not really change shape. Exactly half of the Moon is always lit by the Sun. As the Moon revolves around the Earth, we see different amounts of its lit half. When the lit side faces away from us, we cannot see the Moon — this is the new moon. As the Moon moves on, more and more of the lit part becomes visible (the Moon is said to be waxing) until the whole lit face is seen — the full moon. After that the bright part shrinks (the Moon is waning) back to a new moon.

The complete cycle from one new moon to the next takes about 29.5 days (roughly a month). The phases occur because we see varying portions of the sunlit half of the Moon as it revolves around the Earth.
NCERT Activity — Modelling the phases with a ball and lamp

In a dark room, place a bright lamp (the Sun) on one side. Hold a ball (the Moon) at arm’s length and slowly turn yourself (the Earth) around in a full circle while keeping the ball up. As you turn, you see different amounts of the lit side of the ball — sometimes none (new moon), sometimes a crescent, sometimes half, and sometimes the full lit side (full moon). This models how the phases of the Moon are produced.

6. Eclipses

Sometimes the Sun, the Earth and the Moon come in a straight line, and the shadow of one falls on another. Such an event is called an eclipse. There are two kinds.

6.1 Solar Eclipse

A solar eclipse occurs when the Moon comes between the Sun and the Earth, and the Moon’s shadow falls on the Earth. The Sun gets partly or fully hidden. It happens on a new moon day.

During a total solar eclipse, the Moon completely covers the Sun for a short while and it becomes dark like night in the daytime. A solar eclipse must never be viewed with the naked eye or through binoculars — only with special safe solar filters, or by using a pinhole projection.

6.2 Lunar Eclipse

A lunar eclipse occurs when the Earth comes between the Sun and the Moon, and the Earth’s shadow falls on the Moon. The Moon becomes dark or coppery red. It happens on a full moon day.

A lunar eclipse is completely safe to watch with the naked eye. It can be seen from the whole night-side of the Earth, so it lasts longer and is visible to more people than a solar eclipse.

Feature Solar eclipse Lunar eclipse
In the middleMoon (between Sun and Earth)Earth (between Sun and Moon)
Shadow falls onThe EarthThe Moon
Day it occursNew moonFull moon
Safe to view?No (needs filters)Yes

7. Exploring the Sky

On a clear, dark night away from city lights, we can see thousands of stars. Stars are huge, hot, glowing balls of gas like our Sun, but they look like tiny points because they are extremely far away. Stars appear to twinkle because their light is disturbed as it passes through the moving layers of the Earth’s atmosphere.

People long ago imagined patterns among groups of stars and named them constellations, such as the Great Bear (Saptarshi or Ursa Major) and Orion (the Hunter). The bright Pole Star appears fixed in the north and was used by travellers and sailors to find direction.

Planets (like Venus, Mars, Jupiter and Saturn) also appear in the sky but, unlike stars, they do not have their own light — they shine by reflecting sunlight and do not twinkle. To study the sky in detail, scientists use telescopes, which make distant objects look bigger and clearer.

Stars are luminous (give their own light) and twinkle; planets are non-luminous, shine by reflecting sunlight, and do not twinkle. A constellation is a recognisable pattern of stars in the sky.
NCERT Activity — Spotting a constellation

On a clear, moonless night, go to an open place away from bright lights. Look towards the northern sky for seven bright stars arranged like a big ladle or question mark — this is the Saptarshi (Great Bear / Ursa Major). The two stars at the end of its "bowl" point towards the Pole Star, which always marks the north. Sketch what you see and note how the pattern slowly shifts position through the night.

Practice MCQs
1. The nearest star to the Earth is:
  1. The Moon
  2. The Pole Star
  3. The Sun
  4. Venus
Answer: (C) The Sun is the nearest star to the Earth and the centre of our solar system. It is luminous and gives us light and heat.
2. Day and night are caused by the:
  1. Revolution of the Earth
  2. Rotation of the Earth on its axis
  3. Tilt of the Earth
  4. Movement of the Moon
Answer: (B) As the Earth rotates on its axis once in about 24 hours, the half facing the Sun has day and the half facing away has night.
3. The Earth completes one rotation in about:
  1. 1 hour
  2. 24 hours
  3. 365 days
  4. 29.5 days
Answer: (B) One rotation (spin on its axis) takes about 24 hours, which is one day.
4. The movement of the Earth around the Sun is called:
  1. Rotation
  2. Revolution
  3. Reflection
  4. Vibration
Answer: (B) Revolution is the movement of the Earth around the Sun in its orbit, completed in about 365¼ days.
5. The seasons on the Earth are mainly caused by:
  1. The Earth being closer to the Sun in summer
  2. The tilt of the Earth’s axis along with its revolution
  3. The rotation of the Earth
  4. The phases of the Moon
Answer: (B) The tilt of the Earth’s axis (about 23.5°) combined with its revolution makes the hemispheres receive different amounts of sunlight, causing the seasons.
6. Why does the Moon shine?
  1. It produces its own light
  2. It reflects sunlight
  3. It is on fire
  4. It reflects starlight
Answer: (B) The Moon is non-luminous; it has no light of its own and shines only by reflecting the light of the Sun.
7. The Earth’s only natural satellite is the:
  1. Sun
  2. Pole Star
  3. Moon
  4. Mars
Answer: (C) The Moon is the Earth’s only natural satellite, revolving around the Earth.
8. The changing shapes of the bright part of the Moon are called its:
  1. Craters
  2. Phases
  3. Eclipses
  4. Orbits
Answer: (B) The phases of the Moon are the different shapes we see as the Moon revolves and we view varying portions of its sunlit half.
9. One complete cycle of the Moon’s phases takes about:
  1. 24 hours
  2. 7 days
  3. 29.5 days
  4. 365 days
Answer: (C) The cycle from one new moon to the next is about 29.5 days, roughly one month.
10. A solar eclipse occurs when:
  1. The Earth comes between the Sun and the Moon
  2. The Moon comes between the Sun and the Earth
  3. The Sun comes between the Earth and the Moon
  4. The Moon is full
Answer: (B) In a solar eclipse the Moon comes between the Sun and the Earth and its shadow falls on the Earth. It happens on a new moon day.
11. A lunar eclipse occurs on a:
  1. New moon day
  2. Full moon day
  3. Half moon day
  4. Crescent moon day
Answer: (B) A lunar eclipse happens on a full moon day, when the Earth comes between the Sun and the Moon and its shadow falls on the Moon.
12. Which eclipse is safe to watch with the naked eye?
  1. Solar eclipse
  2. Lunar eclipse
  3. Both
  4. Neither
Answer: (B) A lunar eclipse is safe to view with the naked eye. A solar eclipse must never be viewed directly — it can damage the eyes.
13. Stars twinkle but planets usually do not, because:
  1. Stars are bigger than planets
  2. Star light is disturbed by the Earth’s atmosphere
  3. Planets give out their own light
  4. Stars are closer than planets
Answer: (B) Stars twinkle because their light is disturbed while passing through the moving layers of the Earth’s atmosphere. Planets shine more steadily by reflected light.
14. The group of seven bright stars seen in the northern sky like a big ladle is the:
  1. Orion
  2. Saptarshi (Great Bear)
  3. Pole Star
  4. Milky Way
Answer: (B) The Saptarshi (Great Bear / Ursa Major) is a well-known constellation of seven bright stars; its end stars point to the Pole Star.
15. The Sun appears to rise in the east and set in the west because the Earth rotates:
  1. From east to west
  2. From west to east
  3. From north to south
  4. It does not rotate
Answer: (B) The Earth rotates from west to east, which makes the Sun appear to move across the sky from east to west.
Important Questions
Q1. Define rotation and revolution of the Earth and give the time taken for each. (3 marks)
Answer: Rotation is the spinning of the Earth on its own axis; it takes about 24 hours (one day) and causes day and night. Revolution is the movement of the Earth around the Sun in its orbit; it takes about 365¼ days (one year) and, together with the axial tilt, causes the seasons.
Q2. Why is the Moon called a non-luminous object even though it shines at night? (2 marks)
Answer: A luminous object gives out its own light, but the Moon does not. The Moon shines only because it reflects the light of the Sun that falls on it. Since it has no light of its own, it is called a non-luminous object.
Q3. Explain how the phases of the Moon are caused. (3 marks)
Answer: Exactly one half of the Moon is always lit by the Sun, but the Moon does not really change shape. As the Moon revolves around the Earth, we see different amounts of its sunlit half. When the lit side faces away from us we see no Moon (new moon); as it moves on we see more of the lit part (crescent, half, gibbous) until the whole lit face is visible (full moon); then the bright part shrinks back. These changing shapes are the phases of the Moon, and the cycle repeats in about 29.5 days.
Q4. Differentiate between a solar eclipse and a lunar eclipse (any two points). (2 marks)
Answer: (1) In a solar eclipse the Moon comes between the Sun and the Earth and the Moon’s shadow falls on the Earth; in a lunar eclipse the Earth comes between the Sun and the Moon and the Earth’s shadow falls on the Moon. (2) A solar eclipse occurs on a new moon day and is unsafe to view directly, whereas a lunar eclipse occurs on a full moon day and is safe to watch with the naked eye.
Q5. Why are seasons opposite in the Northern and Southern hemispheres? (2 marks)
Answer: The Earth’s axis is tilted, so at any time one hemisphere is tilted towards the Sun and the other away from it. When the Northern Hemisphere is tilted towards the Sun it gets more direct sunlight and has summer, while the Southern Hemisphere, tilted away, gets slanting rays and has winter — and vice versa. So the seasons in the two hemispheres are always opposite.
Q6. State two differences between stars and planets. (2 marks)
Answer: (1) Stars are luminous and give out their own light, whereas planets are non-luminous and shine by reflecting sunlight. (2) Stars twinkle because their light is disturbed by the Earth’s atmosphere, while planets usually shine with a steady light and do not twinkle.
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