Near side & far side
The Moon is tidally locked, so the same hemisphere always faces Earth. The near side is dominated by dark, smooth maria; the far side — first photographed in 1959 — is rugged, heavily cratered highland with very few seas.
Our only natural satellite — 4.5 billion years of history, written in craters and seas of basalt.
37.9M km²
Surface area — about the size of Asia
384,400 km
Average distance from Earth
1,737 km
Mean radius
1/6 g
Surface gravity (1.62 m/s²)
27.3 days
One rotation = one orbit (tidal lock)
−173 / +127 °C
Night and day temperature
The Moon is tidally locked, so the same hemisphere always faces Earth. The near side is dominated by dark, smooth maria; the far side — first photographed in 1959 — is rugged, heavily cratered highland with very few seas.
The dark patches are ancient lava plains that filled giant impact basins 3–3.8 billion years ago. Early astronomers mistook them for oceans, which is why we still call them Mare Imbrium, Mare Tranquillitatis and so on.
The bright highlands are older crust covered by countless impact craters. Young craters like Tycho and Copernicus have bright rays of ejecta visible from Earth with binoculars.
Craters near the south pole, such as Shackleton, contain regions of permanent shadow that may hold water ice — the most sought-after destination for future bases.
Twelve astronauts walked on the Moon between 1969 and 1972 during six Apollo missions. In 2019 China's Chang'e 4 made the first soft landing on the far side.