Lunar Geology

The lunar highlands are predominantly composed of anorthosite, a rock type rich in the mineral plagioclase feldspar.

Craters are impact basins formed by the collision of asteroids or comets with the lunar surface.

Oceanus Procellarum is the largest mare on the Moon, covering an area of approximately 2.5 million square kilometers.

Rilles are believed to be formed by the collapse of lava tubes or by tectonic activity.

Dorsa are wrinkle ridges formed due to compressional forces in the lunar crust.

Rupes Recta is a prominent cliff-like feature on the Moon, stretching for approximately 120 kilometers.

Catenae are chains of craters formed by the impact of secondary ejecta from a larger crater.

Mons Huygens is the tallest mountain on the Moon, with a height of approximately 4,700 meters.

Crater Tycho is a prominent crater on the Moon, known for its bright ejecta rays and central peak.

Crater Copernicus is a prominent crater on the Moon, known for its well-preserved ejecta blanket and central peak.

Crater Aristarchus is a prominent crater on the Moon, known for its bright ejecta rays and central peak.

Crater Tranquillitatis is the landing site of the Apollo 11 mission, where Neil Armstrong and Buzz Aldrin became the first humans to walk on the Moon.

Mare Imbrium is a large, dark-floored crater on the Moon, formed by a massive impact event.

Crater Shackleton is a prominent crater located near the Moon's south pole, known for its unique lighting conditions.

Crater Kepler is a prominent crater on the Moon, known for its concentric ridges and grooves.