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A new study of the chemical components of rocks led by researchers at Penn State and Columbia University provides the clearest evidence yet for how Earth's continents became and remained so stable — and the key ingredient is heat. Photo Credit: Jaydyn Isiminger / Penn State (CC BY-NC-ND 4.0) |
The new discovery has implications beyond geologic history, such as the search for critical minerals and habitable planets beyond Earth
For billions of years, Earth’s continents have remained remarkably stable, forming the foundation for mountains, ecosystems and civilizations. But the secret to their stability has mystified scientists for more than a century. Now, a new study by researchers at Penn State and Columbia University provides the clearest evidence yet for how the landforms became and remained so stable — and the key ingredient is heat.
In a paper published today (Oct. 13) in the journal Nature Geoscience, the researchers demonstrated that the formation of stable continental crust — the kind that lasts billions of years — required temperatures exceeding 900 degrees Celsius in the planet’s lower continental crust. Such high temperatures, they said, were essential for redistributing radioactive elements like uranium and thorium. The elements generate heat as they decay, so as they moved from the bottom to the top of the crust, they carried heat out with them and allowed the deep crust to cool and strengthen.