Iron Oxide Endures Extreme Temperatures and Pressures in the Depths of the Earth

Iron Oxide Endures Extreme Temperatures and Pressures in the Depths of the Earth

The core–mantle boundary⁢ (CMB) is the interface between the Earth’s iron metal core and the thick rocky layer of mantle ⁤just above the core. It is a world of extremes—temperatures thousands of degrees⁢ Fahrenheit ‍and pressures ‍over a million times the pressure⁢ at the surface of ‌the Earth. While it may seem far away from our environment on Earth’s ‌surface, plumes of material⁤ from the CMB can ascend upwards through the‍ planet over tens ‌of millions of ⁣years, influencing the chemistry, geologic structure, and plate tectonics of the surface world‌ where we live.

Though scientists cannot travel to the ‌center of⁤ the Earth to study the ⁤CMB, ​they can get clues ‍about what⁣ lies beneath the planet’s surface by measuring earthquakes. Seismic waves travel ​at different speeds depending on the material they ​are traveling through, ​allowing researchers to infer what lies⁤ deep below the surface using seismic ​signatures.​ This ‍is‌ analogous to how ultrasound uses​ waves of sound to image inside of the human body.

Recent research shows that the ​base of Earth’s‌ mantle is actually complex and heterogeneous—in particular, there are mountain-like regions where seismic waves mysteriously slow down. These blobs, ‍named ultralow velocity zones (ULVZs)⁤ and first discovered by Caltech’s Don Helmberger,​ are‌ dozens of kilometers thick and lie around 3,000 kilometers beneath our feet.

“Because we can’t simply go down to the CMB and take measurements, there ⁣are many open questions ⁣about a region that is‍ so⁣ important to our planet’s evolution,” says Jennifer Jackson, the William E. Leonhard Professor of ‌Mineral Physics. “Why do the ULVZs exist and what are they made ‌of? What do they teach us ‌about how the ⁤Earth evolved and what role the region plays⁢ in the dynamics of the Earth? Are the blobs solid or molten at the ‌extreme conditions at the CMB?”

In 2010,‌ Jackson and her team suggested that the blobs contain a higher iron⁤ oxide content than the mantle surrounding them. Solid iron⁢ oxide⁤ would slow down seismic waves, which could explain the⁤ low⁤ velocities measured passing through⁢ the blobs. But could iron oxide even be solid at the ⁢extreme ‌temperatures and pressures of the CMB?

2023-11-18⁣ 03:41:02
Original from phys.org rnrn

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