Formation of the Moon
Although most scientists would agree that the Moon is critical for the formation of life on Earth, there is no consensus about the way that the Moon formed. Although there are several additional theories to explain the way that the Moon came into being, three hypotheses are commonly debated among lunar scientists.
The fission theory maintains that the Moon was once part of the Earth and became separated early in the formation of the solar system, probably while the Earth was spinning rapidly. The large piece of the Earth's surface that formed the Moon is believed to have broken off from the Pacific Ocean basin.
The co-accretion theory, also called the condensation theory, contends that the Moon was formed at the same time as the Earth from the original nebula of interstellar dust and gas that comprised the young solar system. In other words, the Moon was a sister planet that formed, like the Earth, by the aggregation of small particles into a single, much larger body. This event probably took place shortly after the Big Bang, about 13 billion years ago.
The giant impact theory states that the Moon was formed from the debris of an indirect collision between the Earth and a planetary body about the size of Mars. It is estimated that the collision occurred about 4.5 billion years ago. Initially, there would have been a number of pieces from both Earth and the collision planet that would have orbited Earth, but eventually, they would have coalesced to form a ball of molten rock about the size of today's Moon.