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EARLY EARTH
Collisions After Moon Formation Remodeled Early Earth
by Staff Writers
San Antonio TX (SPX) Dec 05, 2017


SwRI scientists modeled the protracted period of bombardment after the Moon formed, determining that impactor metals may have descended into Earth's core. This artistic rendering illustrates a large impactor crashing into the young Earth. Light brown and gray particles indicate the projectile's mantle (silicate) and core (metal) material, respectively.

Southwest Research Institute scientists recently modeled the protracted period of bombardment following the Moon's formation, when leftover planetesimals pounded the Earth. Based on these simulations, scientists theorize that Moon-sized objects delivered more mass to the Earth than previously thought.

Early in its evolution, Earth sustained an impact with another large object, and the Moon formed from the resulting debris ejected into an Earth-orbiting disk. A long period of bombardment followed, the so-called "late accretion," when large bodies impacted the Earth delivering materials that were accreted or integrated into the young planet.

"We modeled the massive collisions and how metals and silicates were integrated into Earth during this 'late accretion stage,' which lasted for hundreds of millions of years after the Moon formed," said SwRI's Dr. Simone Marchi, lead author of a Nature Geoscience paper outlining these results.

"Based on our simulations, the late accretion mass delivered to Earth may be significantly greater than previously thought, with important consequences for the earliest evolution of our planet."

Previously, scientists estimated that materials from planetesimals integrated during the final stage of terrestrial planet formation made up about half a percent of the Earth's present mass. This is based on the concentration of highly "siderophile" elements - metals such as gold, platinum and iridium, which have an affinity for iron - in the Earth's mantle.

The relative abundance of these elements in the mantle points to late accretion, after Earth's core had formed. But the estimate assumes that all highly siderophile elements delivered by the later impacts were retained in the mantle.

Late accretion may have involved large differentiated projectiles. These impactors may have concentrated the highly siderophile elements primarily in their metallic cores. New high-resolution impact simulations by researchers at SwRI and the University of Maryland show that substantial portions of a large planetesimal's core could descend to, and be assimilated into, the Earth's core - or ricochet back into space and escape the planet entirely.

Both outcomes reduce the amount of highly siderophile elements added to Earth's mantle, which implies that two to five times as much material may have been delivered than previously thought.

"These simulations also may help explain the presence of isotopic anomalies in ancient terrestrial rock samples such as komatiite, a volcanic rock," said SwRI co-author Dr. Robin Canup.

"These anomalies were problematic for lunar origin models that imply a well-mixed mantle following the giant impact. We propose that at least some of these rocks may have been produced long after the Moon-forming impact, during late accretion."

Research Report: "Heterogeneous Delivery of Silicate and Metal to the Earth by Large Planetesimals," Simone Marchi et al., 2017 Dec. 4, Nature Geoscience

EARLY EARTH
Feathered dinosaurs were extra fluffy, new research shows
Washington (UPI) Nov 30, 2017
New analysis of the remains of a bird-like dinosaur called Anchiornis suggests feathered dinosaurs were fluffier than researchers thought. Modern birds are the evolutionary offspring of a group of feathered theropod dinosaurs. Together they comprise the group known as paravians - a group that included the famed Velociraptor. The fossilized remains of an Anchiornis specimen offer ... read more

Related Links
Southwest Research Institute
Explore The Early Earth at TerraDaily.com


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