Earth's Rotation and Revolution Facts

Discover why a day is 24 hours long, why the seasons change, and other science facts about Earth.

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Rotation and the Length of a Day

Earth completes one rotation roughly every 24 hours

Explanation

The exact time it takes Earth to complete one full rotation (360°) on its axis is about 23 hours 56 minutes (a sidereal day), but a solar day — measured relative to the Sun — comes out to about 24 hours because of Earth’s orbital motion.

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Revolution and the Length of a Year

Earth orbits the Sun once roughly every 365.25 days

Explanation

The time it takes Earth to complete one orbit around the Sun isn’t exactly 365 days, but about 365.2422 days. Those extra roughly six hours accumulate every four years into February 29 — a leap day.

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How Leap Years Work

An extra day is added to February every four years

Explanation

To correct for the leftover time in Earth’s orbital period, a leap year is added every four years — but years divisible by 100 are common years, while those also divisible by 400 are leap years, a refined rule (for example, 2000 was a leap year, but 1900 was not).

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Earth’s Axial Tilt

Earth is tilted about 23.5 degrees

Explanation

Earth’s rotational axis is tilted about 23.5 degrees relative to its orbital plane, and this tilt is the fundamental reason the seasons exist.

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Why the Seasons Happen

The tilt — not the distance — causes the seasons

Explanation

Many people assume otherwise, but the seasons are caused not by a change in the distance between Earth and the Sun, but by the tilt of Earth’s axis. When the Northern Hemisphere tilts toward the Sun it’s summer there, and winter when it tilts away.

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Summer and Winter Solstice

The longest and shortest days of the year

Explanation

The summer solstice (around June 21) is the longest day of the year in the Northern Hemisphere, and the winter solstice (around December 21) is the shortest. The Southern Hemisphere is the exact opposite.

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Spring and Autumn Equinox

The days when daytime and nighttime are nearly equal

Explanation

At the spring equinox (around March 20) and autumn equinox (around September 22), the Sun passes directly over the equator, making day and night nearly equal in length almost everywhere in the world.

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Reversed Seasons Between Hemispheres

The Northern and Southern Hemispheres have opposite seasons

Explanation

Because of the direction of Earth’s axial tilt, the Southern Hemisphere has winter while the Northern Hemisphere has summer, and vice versa. That’s why Christmas falls in the middle of summer in Australia.

Why is it useful to understand Earth's motion?

Concepts we use every day — a day, a year, the seasons, leap years — all come from the astronomical motions of Earth's rotation and revolution. Understanding these principles answers questions like why February 29 shows up every four years, or why Christmas falls in summer in Australia.

A Note

The figures on this page are rounded approximations, and Earth's actual rotation and revolution speeds keep changing by tiny amounts. For precise values, please refer to official data from astronomical research institutions.

Frequently Asked Questions

Is Earth actually closer to the Sun in winter than in summer?

Yes — in the Northern Hemisphere, Earth is actually closest to the Sun around January (winter) and farthest around July (summer). In other words, the distance difference works opposite to the seasons, and the real cause of the seasons is the tilt of Earth's axis.

Do you have information about space exploration too?

Yes, check out our Space Exploration History page for milestones from Sputnik to the James Webb Space Telescope.