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











