The Moon Is Formed by Tiny Moons Amassing Together: Study

The moon, our planet's constant companion for some 4.5 billion years, may have been forged by a rash of smaller bodies smashing into an embryonic Earth, researchers said Monday.

RELATED:
2017 Will See the Solar 'Eclipse of the Century'

Such a theory would explain a major inconsistency in the prevailing hypothesis that the moon splintered off in a single, giant impact between Earth and a Mars-sized celestial body.

In such a scenario, scientists expect that about a fifth of the moon's material would have come from Earth and the rest from the impacting body. Yet, the makeup of the Earth and the moon are nearly identical, an improbability that has long perplexed backers of the single-impact hypothesis.

"The multiple impact scenario is a more 'natural' way of explaining the formation of the Moon," said Raluca Rufu of the Weizmann Institute of Science in Rehovot, who co-authored the new study published in the journal Nature Geoscience.

Such multiple hits would have excavated more Earth material than a single one, which means the moonlets would more closely resemble our planet's composition, said the study authors, concluding that about 20 such crashes would have been required to build the moon.

Rufu and a team created nearly a thousand computer simulations of collisions between a proto-Earth and embryonic planets called planetesimals, smaller than Mars.

RELATED:
The Best and Worst in Science and Technology in 2016

Every collision would have formed a disk of debris around the proto-Earth which would, in turn, amass together to form a "moonlet," the researchers found. Moonlets would eventually come together to form the moon.

"In the early stages of the Solar System, impacts were very abundant, therefore it is more natural that several common impactors formed the moon rather than one special one," Rufu told AFP. Our solar system is thought to have formed 4,567 billion years ago, followed by the moon about 100 million years later.

The giant-impact hypothesis was first proposed in the mid-1970s, followed in the 1980s with the first suggestions that several collisions may have given the Earth its tide-creating satellite.