Planetary collisions are at the core of our solar system's formation, according to the study supported by NASA's Solar System Exploration Research Virtual Institute (SSERVI).
Scientists have long believed that after the Moon's formation, the early Earth experienced a long period of bombardment that diminished about 3.8 billion years ago.
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It is estimated that about 0.5 per cent of Earth's present mass was delivered during this stage of planetary evolution.
Researchers at the Southwest Research Institute (SwRI) and University of Maryland in the US created high-resolution impact simulations that show significant portions of a large planetesimal's core could penetrate all the way down to merge with Earth's core - or ricochet back into space and escape the planet entirely.
In the research published in the journal Nature Geoscience, Simone Marchi and his colleagues found evidence of more massive accretion onto the Earth than previously thought after the Moon's formation.
The mantle abundances of certain trace elements such as platinum, iridium and gold, which tend to bond chemically with metallic iron, are much higher than what would be expected to result from core formation, the researchers said.
This discrepancy can most easily be explained by late accretion after core formation was complete, they said.
The team determined the total amount of material delivered to Earth may have been 2-5 times greater than previously thought, and the impacts altered Earth in a profound way while depositing familiar elements like gold.
"These results have far-reaching implications for Moon- forming theories and beyond," said Marchi.
"Interestingly, our findings elucidate the role of large collisions in delivering precious metals like gold and platinum found here on Earth," Marchi added.
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