Earth's Movements: Rotation, Revolution, and Seasonal Dynamics, and Seasonal Impacts, and Seasonal Variations (copy)

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Last updated 3:08 PM on 7/27/26
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16 Terms

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Rotation

The spinning of the Earth on its imaginary Polar Axis.

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Sidereal Day

The time required for the Earth to turn through 360o360^{\text{o}}, approximately 23hr,56min,4.09sec23 \text{hr}, 56 \text{min}, 4.09 \text{sec}.

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Coriolis Effect

A force resulting from the Earth's rotation that deflects moving bodies; towards the right in the Northern Hemisphere and left in the Southern Hemisphere.

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Revolution

The movement of the Earth along its elliptical orbit around the Sun, completing one revolution in approximately 36514days365 \frac{1}{4} \text{days}.

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Mean Distance from the Sun

Approximately 150million km150 \text{million km}.

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Perihelion

The point in Earth's orbit closest to the Sun, occurring around January 3rd at a distance of approximately 147million km147 \text{million km}.

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Aphelion

The point in Earth's orbit farthest from the Sun, occurring around July 4th at a distance of approximately 152million km152 \text{million km}.

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Angle of Inclination

The Earth's axis makes an angle of 6612o66 \frac{1}{2}^\text{o} with the plane of the ecliptic.

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Summer Solstice

Occurs on June 21; North Pole is inclined toward the Sun, resulting in the longest day in the Northern Hemisphere.

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Winter Solstice

Occurs on December 22; South Pole is inclined toward the Sun, resulting in the shortest day in the Northern Hemisphere.

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Equinox

Occurs on March 21 and September 23; the Sun is directly overhead at the Equator, resulting in equal day and night.

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Circle of Illumination

An imaginary line that divides the Earth into a sunlit half and a shadowed half.

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Centrifugal Force

The outward force experienced by Earth due to its rotation, causing a bulge at the Equator.

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Variations in Temperature

Caused by the accumulation of heat during the day and the release of heat at night, preventing extreme temperature changes.

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Leap Year

A year added with an extra day on February 29th every 4 years to account for the extra 14\frac{1}{4} day per year in the calendar.

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Day Length Variation

The duration of day and night due to the inclination of the axis and Earth's position in orbit, influencing seasons.