Rotation and Revolution
ICSE Class 9 · Geography · Chapter 3
What this chapter covers
- The two motions of the earth
- Direction of rotation
- Speed of rotation
- Occurrence of day and night
- The sun rising in the east and setting in the west
- Coriolis effect
- Revolution of the earth
- The inclined axis of the earth
- Variation in the length of day and night
- Seasonal changes
- Equinoxes
- Solstices
Key definitions
Rotation is the spinning of the earth on its own axis from west to east, one complete turn taking about 24 hours.
Revolution is the movement of the earth around the sun in a fixed path, one complete round taking about 365¼ days.
Angular speed of rotation is the angle through which the earth turns in a given time, equal to 15° every hour, or 1° every 4 minutes, at every place on the earth.
Linear speed of rotation is the actual distance a point on the earth's surface travels in a given time because of the spin, and it is greatest at the equator and zero at the poles.
Day is the period during which a place lies in the half of the earth facing the sun and receives sunlight.
Night is the period during which a place lies in the half of the earth turned away from the sun and receives no direct sunlight.
Apparent motion of the sun is the movement of the sun across the sky from east to west that an observer on the earth sees, which is not a real movement of the sun but the result of the earth rotating from west to east.
Coriolis force is the apparent force, arising from the earth's rotation, that is used to describe this deflection of moving winds and currents.
Perihelion is the position of the earth in its orbit when it is nearest to the sun, at about 147 million km, which occurs around 3 January.
Aphelion is the position of the earth in its orbit when it is farthest from the sun, at about 152 million km, which occurs around 4 July.
Parallelism of the axis is the property by which the earth's axis remains inclined in the same direction at every position of the earth in its orbit, so that the axis at any one position is parallel to the axis at any other position.
Key points
- The earth has two motions: rotation on its axis in about 24 hours and revolution round the sun in about 365¼ days.
- The earth rotates from west to east, anticlockwise when seen from above the North Pole.
- The angular speed of rotation is 15° per hour (1° in 4 minutes) everywhere; the linear speed is about 1,670 km per hour at the equator and zero at the poles.
- Rotation of the spherical earth causes day and night; the circle of illumination separates the lit and dark halves.
- The sun's rising in the east and setting in the west is an apparent motion caused by the earth's west-to-east rotation.
- The Coriolis effect deflects winds and ocean currents to the right in the Northern Hemisphere and to the left in the Southern Hemisphere (Ferrel's law); it is zero at the equator and greatest at the poles.
- The Coriolis effect produces the North-East and South-East Trade Winds, the anticlockwise spin of northern cyclones and the circulation of ocean currents.
- The earth revolves at about 30 km per second; it is nearest the sun at perihelion (about 3 January) and farthest at aphelion (about 4 July). A leap year of 366 days corrects for the extra quarter-day.
- The axis is inclined at 23(1)/(2)° to the perpendicular (66(1)/(2)° to the orbital plane) and stays parallel to itself throughout the orbit.
- Revolution with an inclined axis causes the variation in the length of day and night, which is nil at the equator and greatest at the poles.
- Seasons result from the changing angle of the sun's rays and the changing length of day; the seasons of the two hemispheres are opposite.
- The equinoxes (21 March and 23 September) bring vertical rays at the equator and equal day and night everywhere.
- The solstices (21 June and 22 December) bring vertical rays at the Tropic of Cancer and the Tropic of Capricorn, and the longest and shortest days.
Questions answered
Define rotation and revolution, and state the time each takes.
In which direction does the earth rotate, and how would the rotation appear from above the North Pole?
Why is the linear speed of rotation greatest at the equator and zero at the poles, although the angular speed is the same everywhere?
Calculate the linear speed of rotation of a place on the 30° parallel, which is about 34,700 km long.
Explain how day and night occur. What is the circle of illumination?
Give a reason: the sun appears to rise in the east and set in the west.
Define the Coriolis effect and state Ferrel's law.
Why do cyclones over the Bay of Bengal spin anticlockwise, and why do cyclones rarely form at the equator?
Past board exam questions
ICSE 2019 sample paper · 2 marks
(i) What is meant by the inclination of the Earth’s axis? (ii) At what angle is the Earth’s axis inclined?
Show answer
ICSE 2019 sample paper · 2 marks
State two effects of the rotation of the earth.