Enormous ‘mega-blob’ under Hawaii is solid rock and iron, not gooey — and it may fuel a hotspot

Enormous ‘mega-blob’ under Hawaii is solid rock and iron, not gooey — and it may fuel a hotspot

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A “mega-blob” deep below Hawaii might be sustaining a volcanic hotspot, according to a brand-new research study.
(Image credit: Warren Ishii/ 500px through Getty Images)

An enormous blob deep under Hawaii appears to be strong and iron-rich, brand-new research study discovers.

This blob– clinically referred to as a mega-ultralow speed zone– might anchor the Hawaii hotspot, a location where hot product increases through the mantle and drives the volcanic activity that developed the Hawaiian Islands.

“Because it’s iron-rich material, it is going to be electrically more conductive, and that will actually promote thermal conduction — so it will actually help localize the plume to last longer,” stated Doyeon Kima seismologist at Imperial College London and the very first author of the brand-new research study, released Jan. 28 in the journal Science AdvancesUltralow speed zones (ULVZs) are huge hunks of the world that sit near the border of the mantle and the core, at about 1,800 miles (2,900 kilometers) listed below the Earth’s surface area. They get their name from the truth that seismic waves from earthquakes decrease considerably in these areas. Mega-ultralow speed zones are the biggest of these areas, which frequently cover numerous kilometers. They’re frequently discovered near volcanic hotspots, such as Hawaii, Iceland and the Marquesas Islands of the South Pacific.

“It actually makes them one of our few direct windows into deep-Earth composition and dynamics,” Kim informed Live Science.

Since these blobs are so deep, researchers generally study them utilizing compressional waves produced by earthquakes. These pressure waves, or P waves, supply restricted details. Kim and his coworkers utilized an approach they established in 2020 that might likewise include S waves, or shear waves, which produce vertical movement. By integrating information from both kinds of waves and after that modeling rocks and minerals that might match those information, the scientists might get a clearer image of why the waves decrease in those zones.

They discovered that the mega-ULVZ under Hawaii is most likely abundant in iron and strong rock. That mainly eliminate a contending hypothesis that recommended the location may be extra-melty

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With this info, “we can think about where it is coming from,” Kim stated. “It could be coming from the relics of Earth’s earliest evolution, particularly from the crystallization of a basal magma ocean or recrystallized melt from past mantle melting.”

Not every mega-ULVZ might be developed similarly, Kim included. Some may form from the subduction of water-rich oceanic crust deep into the mantle. Maybe others include product from the core itself. The method in the brand-new paper can assist distinguish these kinds of ULVZs worldwide, he stated, in addition to clarifying how worlds form in the very first location.

“We have to first clearly understand what’s happening on Earth to understand fully what’s happening on other planets,” he stated.

Kim, D., Song, J.-H., Dobrosavljevic, V. V., & & Lekić, V. (2026 ). Seismic and mineralogical proof for an iron-rich mega– ultralow-velocity zone underneath Hawai’i. Science Advances12( 5 ). https://doi.org/10.1126/sciadv.adz1962

Stephanie Pappas is a contributing author for Live Science, covering subjects varying from geoscience to archaeology to the human brain and habits. She was formerly a senior author for Live Science however is now a freelancer based in Denver, Colorado, and routinely adds to Scientific American and The Monitor, the regular monthly publication of the American Psychological Association. Stephanie got a bachelor’s degree in psychology from the University of South Carolina and a graduate certificate in science interaction from the University of California, Santa Cruz.

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