The Moon formed from debris after a Mars-sized body collided with Earth.The leading explanation for the Moon's origin is the giant-impact hypothesis: a Mars-sized body, sometimes called Theia, struck the young Earth about 4.5 billion years ago. The collision vaporized part of Earth's mantle and the impactor, forming a disk of debris around Earth that eventually coalesced into the Moon. This idea elegantly explains the Moon's large size relative to Earth, its lack of a substantial iron core, and the similar isotopic composition of lunar and terrestrial rocks — a geochemical puzzle that older capture or fission models struggled with.
The hypothesis was proposed in the mid-1970s by William Hartmann and Donald Davis, and independently by Alastair Cameron and William Ward, following the Apollo missions that revealed the Moon's geochemical similarity to Earth.
The impactor's iron core merged with Earth's core, while the lighter rocky material from both bodies was ejected into orbit. This debris formed a hot, partially molten ring around Earth. Over thousands of years, gravitational clumping assembled the debris into the Moon. Because the material came mostly from the mantles of both bodies, the Moon is depleted in iron and has a composition close to Earth's outer layers, matching observations.
It guides planetary formation models and helps interpret the early history of the Earth-Moon system, including the timing of Earth's core formation and the onset of plate tectonics.
The Moon is actually older than its oldest surface rocks — the lunar crust crystallized about 150 million years before the oldest samples brought back by Apollo astronauts.

















