Movements of the Earth: Rotation and Its Effects

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Vocabulary flashcards created from lecture material detailing the rotation of the Earth, its speeds, scientific proofs, and environmental effects.

Last updated 9:06 AM on 9/15/26
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21 Terms

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Rotation of the Earth

The spinning of the Earth on its imaginary axis (661266\frac{1}{2}^\circ inclined to its orbital plane) from west to east once in every 24hour24\,\text{hour} (actually 23hour56minute4second23\,\text{hour}\,56\,\text{minute}\,4\,\text{second}).

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Diurnal Motion

The rotation of the Earth on its axis, also known as 'the daily movement of the earth', which causes the formation of day and night.

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Rotation (A.N. Strahler)

According to A.N. Strahler, "The spinning of the earth in its polar axis is termed rotation".

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Direction of Earth's Rotation

The spinning of the Earth from west to east or in an anticlockwise direction when looking down upon the Earth from outside.

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Earth's Rotation and Revolution Movement Diagram

A diagram showing the Earth rotating on its axis while revolving around the Sun at a distance of 14crores90lakhkm14\,\text{crores}\,90\,\text{lakh}\,\text{km}, alongside the Moon.

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Rotational Speed at the Equator (00^\circ)

The speed of the Earth's rotation at the equator, which measures 1670km/hour1670\,\text{km/hour}.

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Rotational Speed at Kolkata (2234N22^\circ34'\,\text{N})

The speed of the Earth's rotation at Kolkata, which is 1536km/hour1536\,\text{km/hour}.

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Rotational Speed at London (5112N51\frac{1}{2}^\circ\,\text{N})

The speed of the Earth's rotation at London, which is 1050km/hour1050\,\text{km/hour}.

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Rotational Speed at the Poles (90 N & S90^\circ\text{ N \& S})

The speed of the Earth's rotation at the North and South Poles, which is approximately 0km/hour0\,\text{km/hour}.

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Equatorial Bulge

The shape effect of Earth's rotation resulting in a flattening at the two poles and bulging at the equator, making the equatorial diameter 43km43\,\text{km} longer than the polar diameter.

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Rotational Deflection of Air and Ocean Currents

The effect of Earth's rotation that deflects moving air, ocean water, cyclones, and anti-cyclones to the right in the Northern Hemisphere and to the left in the Southern Hemisphere.

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Drop of Stone from High Tower Proof

A proof of Earth's rotation where a stone dropped from a high tower in still air falls slightly to the east of vertical due to the Earth's west-to-east rotational speed.

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Foucault's Pendulum Experiment

An experiment where Foucault suspended a cannon ball to swing in a north-south direction, demonstrating that the Earth slowly turns beneath it from west to east as the path traced by the pendulum gradually shifts.

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Photograph of the Pole Star Proof

A proof of rotation where a long-exposure photograph focused on the Pole Star captures light trails as curved lines instead of points due to the camera turning with the Earth.

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Circle of Illumination

The imaginary line (also called the Shadow Circle) that separates the lit-up half of the Earth from the darkened half.

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Formation of Day and Night Diagram

A diagram depicting how the Earth's rotation relative to the Sun creates day (0Noon0^\circ\,\text{Noon}), night (0Midnight0^\circ\,\text{Midnight}), dawn (0Dawn0^\circ\,\text{Dawn}), and evening (180Evening180^\circ\,\text{Evening}).

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Buys Ballot's Law

The rule governing the relation of wind to pressure in the Northern Hemisphere, where air flow at high altitudes generally parallels the isobars.

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Inclination of the Earth's Axis

The tilt of the Earth's axis, which makes an angle of 231223\frac{1}{2}^\circ with the vertical or 661266\frac{1}{2}^\circ with the plane of the Earth's orbit.

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Formation of Dawn and Twilight Diagram

A diagram illustrating the inclination of the Earth's axis (231223\frac{1}{2}^\circ to the vertical, 661266\frac{1}{2}^\circ to the axis plane), the equatorial circle, and alignment relative to the Pole Star.

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Hours of Daylight at the Equator

The equator experiences 12hours12\,\text{hours} of daylight and 12hours12\,\text{hours} of night throughout the year because the circle of illumination always bisects the equator into two equal halves.

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Transition Period

The gradual and continuous process of changing between sun-lit day and night darkness, encompassing stages such as dawn, sunrise, noon, evening, twilight (dusk), and midnight.