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Motions of the Earth Class 6 Social Science Geography Chapter 3 CBSE Notes - 2025-26

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Social Science Geography Notes for Chapter 3 Motions of the Earth Class 6 - FREE PDF Download

The planet Earth has two types of motions: Rotation and Revolution.

  • Rotation: When the planet earth spins on its axis, it is called rotation. It rotates counterclockwise or west to east when viewed from the North Pole.

  • Revolution: When the planet earth moves around the Sun in a fixed orbit or path, it is called revolution. At this time, the earth is also performing a rotation.

Read in Class 6 Social Science Geography Motions of the Earth Chapter 3 how rotation and revolution affect life on earth. Learn new terms like Solstices, Equinox, orbital plane, axis of the earth, etc.


In these revision notes, a detailed explanation is available on all the important topics. So, students can download the free PDF of Motions of the Earth Class 6 Notes CBSE Geography Chapter 3 to clear all their doubts.


Topics Covered in Chapter 3 Motions of the Earth of Class 6 Geography

Class 6 Social Science Geography Motions of the Earth teaches students the following important topics:

  • Rotation

  • Revolutions

  • Circle of illumination

  • Orbital plane

  • Leap year

  • Elliptical orbit

  • Summer solstice

  • Winter solstice

  • Equinox 


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Access Class 6 Geography Chapter 3 - Motions of the Earth Notes

Some Important Definitions

The Axis of the Earth: An imaginary line makes an angle of 66 1/2° with its orbital plane.

The Orbital Plane: The plane formed by the orbit is known as the orbital plane.

Circle of Illumination: The imaginary circle on the earth which divides the earth into day and night halves is known as the circle of illumination. It is not the same as the axis of the earth and doesn’t coincide with it. The circle of illumination makes a 23 ½ degrees angle from the earth’s axis.


Rotation of Earth

  • The phenomenon of day and night is because of the rotation of the earth. Had there been no rotation, one side of the earth would perpetually have night, and temperatures would have dropped in this half. The other half would forever have a day, and temperatures would have risen in this half. In such cases, it would not be possible to sustain life on earth. 

  • Earth takes 24 hours to complete one rotation, and this is known as earth day. 

  • 23 hr, 56 min, and 4 sec is the actual time taken to complete one rotation, but for convenience purposes, it is taken to be 24 hours.


Revolution of the Earth

  • The movement of the Earth on its own axis around the Sun is termed a revolution. 

  • The Earth moves around the Sun in an elliptical-shaped orbit. 

  • It takes 365.25 days to complete one revolution. This is the time taken by the Earth to go round an elliptical orbit with the Sun as the focus. 

  • We consider 365 days as one year, and the rest one-fourth of a day is added up for every four years to give us one extra day. This day is added up to the fourth year, and the year has 366 days. This year is called a leap year. This day is added up to the month of February.

  • In a leap year, February has 29 days instead of 28 days.


Seasons

  • Seasons change due to changes in the position of the Earth around the Sun. Due to the change in the position of Earth, a year is divided into summer, winter, spring, and autumn.


Summer Solstice

  • Summer Solstice begins on 21st June in the Northern Hemisphere. 

  • On this day, the Northern Hemisphere is tilted towards the Sun.

  • Sunrays fall on the Tropic of Cancer.

  • The North Pole is inclined towards the Sun, and areas beyond the Arctic Circle experience continuous daylight for about six months.

  • The longest day and shortest night occur on 21st June, the Summer Solstice.

The conditions in the Southern Hemisphere are reversed, and it is winter season there.


Winter Solstice

  • The Winter Solstice occurs on the 22nd of December in the Northern Hemisphere.

  • The Southern Hemisphere at this time is tilted towards the Sun. 

  • The Sunrays fall on the Tropic of Capricorn in the Southern Hemisphere.

  • The Southern Hemisphere has longer days during this period and shorter nights. 

The conditions are reversed in the Northern Hemisphere.


Equinox

  • The direct rays of the Sun fall on the equator on 21st March and 23rd September.

  • The whole Earth experiences equal days and equal nights because neither of the poles is tilted towards the Sun.

  • On 23rd September, it is autumn in the Northern Hemisphere and spring in the Southern Hemisphere. 

It is the opposite on 21st March when it is spring in the Northern Hemisphere and autumn in the Southern Hemisphere.


Class 6 Geography Chapter 3 - Motions of the Earth Notes

Important Terms Used to Describe Motions of the Earth

To learn the motions of the earth in detail, it is essential to understand some important terms.

  • The axis of the earth or Earth’s axis is an imaginary pole or line passing through the centre of the earth and makes an angle of 66½° with its orbital plane. It runs from the North Pole to the South Pole.

  • The orbital plane is the plane formed by the orbit.

  • The circle of illumination is the circle that divides day and night on the globe. The Sun gives light to the earth, which is spherical in shape. Due to its shape, only half of the earth gets sunlight at a time, i.e., the portion of the earth facing the Sun experiences day while the other half, which is away from the Sun, experiences night. This circle of illumination does not coincide with the earth’s axis. 

  • Earthday is the daily motion of the earth and the period of rotation that the planet earth takes to make one complete rotation around its axis, which is 24 hours. 


What Will Happen if the Earth Stops Rotating?

In such a case, the portion of the earth facing the Sun would always experience a day, thus bringing continuous warmth to that region. The other half would remain dark and cold all the time. The existence of life would not be possible in such extreme conditions. Thus, the motion of the earth is important for life to exist.


How Long does the Earth Take to Revolve?

The earth takes 365¼ days (one year) to revolve around the Sun. For convenience, we consider only a year of 365 days and ignore six hours. Over a span of four years, these six hours saved every year are added to make one complete day of 24 hours. This surplus day is then added to the month of February of that year. Thus, every fourth year, February has 29 days instead of 28 days and such a year with an additional one day by making it 366 days is called a leap year. 


The earth revolves around the Sun in an elliptical orbit, and the earth is inclined in the same direction throughout its orbit. This revolution gives four seasons in the year: summer, autumn, winter, and spring. Seasons change according to the change in the position of the earth around the Sun.


Positions of the Sun

  • Summer Solstice: On 21st June, the Northern Hemisphere is tilted maximum towards the Sun. The Sun's rays fall directly on the Tropic of Cancer, and as a result, these areas receive more heat. Since the sunrays are slanting, the areas near the poles receive less heat. The area beyond the Arctic Circle experiences continuous daylight for about six months as the North Pole is inclined towards the Sun. 

Since a majority portion of the Northern Hemisphere receives light from the Sun, it is the summer season in the regions north of the equator. On 21st June, there is the longest day and the shortest night at these places. At this time, all conditions are reversed in the Southern Hemisphere. They experience the winter season, and the nights are longer than the days. 

  • Winter Solstice: On 22nd December, the South Pole is tilted maximum towards the Sun, and the Tropic of Capricorn receives direct sunrays. As the rays of the Sun fall vertically at the Tropic of Capricorn at 231/2° S, a major portion of the Southern Hemisphere receives light. Therefore, the Southern Hemisphere experiences summer with longer days and shorter nights. The opposite happens in the Northern Hemisphere at this time. 22nd December experiences the longest night and the shortest day.

  • Equinox: On 21st March and September 23rd, the Sun's rays fall directly on the equator. At this unique position, neither of the poles is tilted towards the Sun; the entire earth experiences equal days and nights. This position is called an equinox. On 23rd September, while the Northern Hemisphere experiences autumn, the Southern Hemisphere has the spring season. The contrary happens on 21st March when the Northern Hemisphere has spring season, and the Southern Hemisphere has autumn.

Thus, based on the earth’s rotation and revolution around the Sun, we see days/nights and changes in the seasons.


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  • These are expert-curated, hence guaranteeing 100% accuracy and factual correctness.

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Conclusion 

Vedantu's free PDF notes on CBSE Class 6 Geography Chapter 3, "Motions of the Earth," are a valuable educational resource for young learners. These notes provide a comprehensive understanding of the Earth's dynamic movements, aligning seamlessly with the CBSE curriculum. Vedantu's commitment to providing accessible educational content empowers students to explore the complexities of our planet's motion with ease. These notes simplify intricate concepts related to the Earth's rotation and revolution, encouraging students to develop a solid foundation in geography. By utilizing these resources, students can enhance their scientific knowledge, critical thinking skills, and overall academic performance, fostering a deeper appreciation for the celestial dance that governs our world.

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FAQs on Motions of the Earth Class 6 Social Science Geography Chapter 3 CBSE Notes - 2025-26

1. What is a quick summary of the two main motions of the Earth?

The two main motions are rotation and revolution. Rotation is the Earth's daily spin on its axis, which causes day and night and takes about 24 hours. Revolution is the Earth's yearly movement around the Sun in a fixed path or orbit, which takes approximately 365¼ days and is responsible for the change of seasons.

2. How is a leap year accounted for in Earth's revolution?

Earth takes approximately 365 and 1/4 days to revolve around the Sun. For convenience, we count 365 days in a normal year. The remaining quarter day (about 6 hours) is saved for four years. Every fourth year, this saved time adds up to one full day (24 hours), which is added to the month of February. This year with 366 days is called a leap year.

3. What is the 'circle of illumination' and what does it separate?

The circle of illumination is the imaginary line that divides the sunlit part of the Earth from the part in darkness. It essentially separates day from night on the globe. This circle does not coincide with the Earth's axis because the axis is tilted, which is why day and night are not always equal in length.

4. Why are seasons in the Northern and Southern Hemispheres opposite?

This happens because of the Earth's axial tilt. When the Northern Hemisphere is tilted towards the Sun, it receives more direct sunlight and experiences summer. At the same time, the Southern Hemisphere is tilted away from the Sun, receiving slanted rays, and thus experiences winter. The situation reverses as the Earth revolves to the other side of its orbit.

5. What is the key difference to remember between a solstice and an equinox?

The key difference lies in the length of day and night. During a solstice, one hemisphere experiences its longest day (summer solstice) while the other has its shortest day (winter solstice). During an equinox, the Sun's direct rays fall on the equator, resulting in nearly equal lengths of day and night across the entire world.

6. How does the tilt of the Earth's axis lead to the change of seasons?

The Earth's axis is tilted at an angle of 23.5°. This constant tilt causes different parts of the Earth to receive more direct or indirect sunlight at different times of the year as it revolves around the Sun.

  • When a hemisphere is tilted towards the Sun, it gets more concentrated sunlight for longer hours, leading to summer.
  • When it is tilted away from the Sun, it receives less concentrated sunlight for shorter hours, resulting in winter.
  • The transition periods between these extremes are spring and autumn.

7. Why do the poles experience about six months of day and six months of night?

Due to the Earth's axial tilt, during its revolution, one pole remains tilted continuously towards the Sun for about six months. For instance, when the North Pole is tilted towards the Sun, it experiences continuous daylight for this period. At the same time, the South Pole is tilted away and remains in darkness. This situation reverses for the next six months of the year.

8. What would be the effect on Earth if its axis were not tilted?

If the Earth's axis were not tilted, there would be no change in seasons. The Sun's rays would always fall directly on the equator. Consequently, every place on Earth would have the same temperature and climate throughout the year, and days and nights would be of equal length everywhere, every day.

9. How does Earth's rotation define an 'earthday'?

The rotation of the Earth on its axis is a daily motion. The time taken for the Earth to complete one full spin is approximately 24 hours. This period of one complete rotation is known as an earthday, and it is the fundamental reason we have a cycle of day and night.