Speaking of epochs, the first half-billion eon of Earth is called the Hadean (from Hades, Greek god of the underworld). This eon witnessed giant impacts as well as the layered formation of the crust, the mantle, and the core.
Among the objects that impacted Earth was a hypothesized proto-planet called Theia, which hit proto-Earth at around 4.5 billion years ago as Earth was forming. It is believed that the Theia-Earth collision ejected materials into Earth’s orbit, and this debris later coalesced to form the moon.
What’s new: Recently, an article in Nature linked the Theia hypothesis to a totally different observation about the core-mantle boundary—the low-shear velocity provinces.
What are the low-shear velocity provinces?
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These are two continent-size blobs of denser materials in the lowermost mantle surrounding the core.
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We have no sample of them, but they do exist because they are characterized by their lower-than-average seismic wave velocities.
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They are denser than the adjacent rock materials in the lower mantle because seismic waves travel faster in these mysterious blobs.
Their hypothesis: The new research uses giant-impact simulations to suggest that the low-velocity provinces are relics of Theia’s mantle material incorporated into Earth’s body.
Why it matters: If true, the new study suggests after Theia met and hit Earth, it did not simply vanish and vaporize, but some part of it has been within Earth for billions of years. This is an alternative to the “subducted slab graveyard” hypothesis, which suggests these deep blobs are subducted and sunken ocean crust materials.
But wait, there’s more: In a different study with Caltech, the same author and colleagues suggest that about 200 million years after the Theia-Earth collision, strong mantle plumes from the super-hot core-mantle boundary rose and induced the first subduction process in the Earth’s crust. This scenario is investigated by computer simulations of whole mantle convection in early Earth.
A potentially big impact:
Dive deeper:
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Read the full study by Qian Yuan and colleagues here.
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Here is a helpful animation clip for the first study.
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You can also read the second study, published in Geophysical Research Letters, here.