Moon

Earth's Moon is its only natural satellite and the nearest large celestial body to our planet. Its orbit and synchronous rotation shape the phases we see, while its gravity contributes to ocean tides. A surface marked by impact craters, ancient lava plains and bright highlands preserves evidence of the early Solar System; samples and observations from space missions continue to inform research into its origin and evolution.

Last updated
13 October 2026
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High (96%)
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This article was researched and drafted with AI assistance and checked by an automated review pass. It is not guaranteed to be accurate — verify important facts against the references below.

Orbit and appearance

The Moon follows an elliptical orbit around Earth at an average distance of about 384,400 kilometres. It rotates once in roughly the time it takes to orbit Earth, a condition called synchronous rotation, so observers on Earth usually see the same hemisphere. The far side is not permanently dark: sunlight illuminates different portions of the Moon as it moves around Earth. Those changing viewing angles create the phases, from new moon to full moon and back. The Moon's gravity, together with the Sun's, is a major influence on Earth's ocean tides.

Surface and interior

The lunar surface preserves a long record of impacts and volcanic activity. Bright, elevated highlands contrast with broad, darker plains called maria; these plains formed when lava flooded some large impact basins and later cooled. The Moon is a differentiated body with a crust, mantle and core. It has only a very thin, weak atmosphere, so its surface is not shielded from meteoroid impacts or the Sun's radiation as Earth's surface is by its atmosphere.

Origin

The leading family of explanations holds that the Moon formed from debris produced by a massive collision involving the young Earth about 4.5 billion years ago. In NASA's account, the impactor may have been a single body about the size of Mars or several objects; the precise details of the event remain under investigation. Lunar rocks returned by the Apollo missions helped researchers test formation models: their chemistry and other evidence indicate that the early Moon was once molten and that its materials have close similarities to Earth's.

Observation and exploration

People have observed the Moon for millennia, using its recurring phases to track time and mark calendars. Robotic spacecraft and the crewed Apollo missions transformed it from a distant object of observation into a world that can be studied directly. Apollo astronauts returned about 382 kilograms of lunar material, while later orbiters and landers have mapped the surface and examined its environment. These investigations make the Moon an important natural record of the processes that shaped Earth and the early Solar System.

Key facts

Type
Earth's only natural satellite
Average distance from Earth
About 384,400 kilometres
Rotation
Synchronous with its orbit around Earth; the same hemisphere generally faces Earth
Surface features
Impact craters, bright highlands and dark volcanic plains called maria
Interior
Crust, mantle and core

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References

  1. 1.
    Moon Facts

    NASA Science · other · reliability: high · retrieved 13 October 2026

    Supports: Orbital distance, synchronous rotation, phases, age, surface features and the Moon's weak atmosphere.

  2. 2.
    Moon Formation

    NASA Science · other · reliability: high · retrieved 13 October 2026

    Supports: Leading impact-based formation models and evidence from Apollo lunar samples.

  3. 3.
    Moon Composition & Structure

    NASA Science · other · reliability: high · retrieved 13 October 2026

    Supports: The Moon's differentiated interior and the composition and history of its surface.

  4. 4.
    Moon Features, Phases, Surface, Exploration, & Facts

    Encyclopaedia Britannica · encyclopedia · reliability: high · retrieved 13 October 2026

    Supports: Independent overview of the Moon's orbit, appearance, geology, origin and human exploration.

References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.

Article history

  1. Version 113 October 2026 · EditorCreated by Zapia