Moons · Space Codex

The Moon

A dry, airless world about a quarter of Earth's width, probably assembled from debris after a Mars-sized body struck the young Earth.

Earth's only natural satellite

  • Last reviewed 10 Oct 2026
  • 6 sources

At a glance

The Moon at a glance, with sources
MeasureValueSource
Mean radius1,737.4 km (0.273 Earth)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mass7.35 × 10²² kgDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Surface gravity1.62 m/s² (0.17 g)Derived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Escape velocity2.38 km/sDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mean density3.344 g/cm³JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mean distance from Earth384,400 kmJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Distance range363,300 km (perigee) to 405,500 km (apogee)NASA NSSDC Moon Fact Sheet (opens in a new tab)NASA NSSDC Moon Fact Sheet (opens in a new tab)
Light travel time from EarthAbout 1.3 seconds384,400 km divided by the speed of light.JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Orbital period (sidereal)27.32 daysJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Phase cycle (synodic month)29.53 daysNASA NSSDC Moon Fact Sheet (opens in a new tab)NASA NSSDC Moon Fact Sheet (opens in a new tab)
Orbital inclination5.16° to the eclipticJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
RotationSynchronous: the same face always points at EarthNASA Science: Moon facts (opens in a new tab)NASA Science: Moon facts (opens in a new tab)
Geometric albedo0.12, about as dark as worn asphaltNASA NSSDC Moon Fact Sheet (opens in a new tab)NASA NSSDC Moon Fact Sheet (opens in a new tab)
Surface temperature (equator)About 95 K (−178 °C) at night to 390 K (117 °C) at noonNASA NSSDC Moon Fact Sheet (opens in a new tab)NASA NSSDC Moon Fact Sheet (opens in a new tab)
AtmosphereExosphere only: a few atoms per cubic centimetreNASA NSSDC Moon Fact Sheet (opens in a new tab)NASA NSSDC Moon Fact Sheet (opens in a new tab)

Key points

Its gravity drives our tides and steadies Earth's axial tilt.

  • Artemis II carried humans 406,770 km from Earth in April 2026, a new record
  • Reflects only about 12% of the sunlight that hits it
  • Surface swings from −178 °C to 117 °C between night and day

Interior

Seismometers left by Apollo crews recorded moonquakes for eight years. Together with orbital gravity maps they show a crust about 30–50 km thick, a thick rocky mantle and a small iron-rich core only about a fifth of the Moon's radius. The Moon's low density, 3.34 g/cm³, matches Earth's mantle far better than Earth as a whole, one of the clues behind the giant-impact origin.

Surface

The bright highlands are ancient crust of anorthosite, saturated with craters. The dark maria are basalt lava that flooded giant impact basins more than three billion years ago, mostly on the near side. On the far side lies the South Pole–Aitken basin, roughly 2,500 km across, one of the largest impact structures in the Solar System. Inside permanently shadowed craters near the poles, temperatures stay low enough for water ice to survive.

Exploration

Twelve Apollo astronauts walked on the Moon between 1969 and 1972 and returned 382 kg of samples. In April 2026 Artemis II flew four astronauts around the far side and set a human distance record of 406,770 km. NASA has since re-scoped Artemis III into a crewed docking test in Earth orbit targeted for mid-2027; the next landing is planned for Artemis IV in 2028. China's Chang'e-7 south-pole mission was postponed out of its 2026 window.

What we still don't know

How much water ice the polar craters hold and in what form, why the near and far sides are so different, and whether the Moon formed from mostly impactor material or mostly Earth material.

Missions

  1. 1969–1972

    Apollo 11–17

    NASACompleted

    Six crewed landings; 12 astronauts walked on the Moon.

  2. 2009–

    Lunar Reconnaissance Orbiter

    NASAActive

    High-resolution mapping of the whole Moon, including permanently shadowed craters.

  3. 1–10 Apr 2026

    Artemis II

    NASA / CSACompleted

    First crewed lunar flyby since 1972; set a human distance record of 406,770 km (252,756 mi).

    Mission page (opens in a new tab)

  4. Target mid-2027

    Artemis III

    NASAPlanned

    Re-scoped in Feb 2026 to a crewed low-Earth-orbit rendezvous and docking test with the commercial landers. Crew named 9 Jun 2026.

    Mission page (opens in a new tab)

  5. Target 2028

    Artemis IV

    NASAPlanned

    Planned first Artemis crewed landing, near the lunar south pole.

  6. Postponed

    Chang'e-7

    CNSAPlanned

    South-pole water-ice mission (orbiter, lander, rover, hopper); postponed out of its Aug 2026 window with no new date announced.

First-hand · our 3D model

How we render it

The Moon starts with a light colour map from NASA's Lunar Reconnaissance Orbiter camera (LROC). When you select it, a 4K LROC map and LOLA laser-altimeter elevation data load, so craters and maria gain real relief.

Its size and distance are art-directed rather than scaled, so it stays in frame beside Earth, but its orbit is real in direction: prograde, inclined 5.16° to the ecliptic, with the near side always facing Earth.

Moon sizes and orbits are compressed so a whole system fits on screen, but never reordered: each moon is drawn at 0.72 × (true size ratio)^0.6 of its planet, capped so no large moon is drawn bigger than it really is, and orbit distances are log-compressed into a band that clears the planet's rings. Orbital periods keep their true ratios, every moon is tidally locked, and on lighter devices only the two largest moons of each planet are drawn.

Sources

  1. NASA: Artemis II milestones (opens in a new tab)
  2. NASA: Artemis III (opens in a new tab)
  3. JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
  4. JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
  5. NASA NSSDC Moon Fact Sheet (opens in a new tab)
  6. NASA Science: Moon facts (opens in a new tab)

Last reviewed against these sources. Built from public NASA, ESA and JPL data; not affiliated with or endorsed by any agency.