Motion of the Earth
Rotation
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- The Earth spins on its axis from west to east.
- It takes 24 hours to complete one full rotation.
- Causes day and night.
- The speed of rotation is fastest at the equator (~1,600 km/h) and decreases towards the poles.

Revolution
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- The Earth moves around the Sun in an elliptical orbit.
- It takes 365¼ days (~one year) to complete one revolution.
- Causes seasons due to the tilt of the Earth’s axis.
Orbital Plane
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- The imaginary plane in which the Earth orbits around the Sun.
- The Earth’s axis is tilted at 66.5° to the orbital plane.
- This tilt is responsible for seasonal changes.
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Circle of Illumination
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- The imaginary line separating the day and night sides of the Earth.
- Due to the Earth’s spherical shape, only one-half of the planet receives sunlight at any given time.
- The tilt of the Earth affects the length of daylight hours.
Earth Day
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- The time taken by Earth to complete one full rotation.
- It is approximately 24 hours (23 hours, 56 minutes, and 4 seconds).
- Divided into daytime and nighttime depending on location.
Leap Year
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- The Earth takes 365¼ days to revolve around the Sun.
- To adjust for the extra ¼ day, an extra day (February 29) is added every four years.
- The last leap year was 2020, and the next one is 2024.
Elliptical Orbit
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- The Earth’s orbit around the Sun is not a perfect circle but an ellipse.
- Due to this, the distance between the Earth and the Sun varies throughout the year.
- Closest to Sun (Perihelion): January 3 (~147 million km).
- Farthest from Sun (Aphelion): July 4 (~152 million km).
Summer Solstice
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- Occurs on June 21.
- Sun shines directly over the Tropic of Cancer (23.5°N).
- Northern Hemisphere: Longest day & shortest night (Summer).
- Southern Hemisphere: Shortest day & longest night (Winter).
Winter Solstice
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- Occurs on December 22.
- Sun shines directly over the Tropic of Capricorn (23.5°S).
- Northern Hemisphere: Shortest day & longest night (Winter).
- Southern Hemisphere: Longest day & shortest night (Summer).
Equinox
- Occurs on March 21 (Spring Equinox) and September 23 (Autumn Equinox).
- The Sun is directly overhead at the Equator.
- Day and night are of equal length worldwide.
- Marks the transition between seasons.

