Groundbreaking research led by a York University professor offers new insights into the Earth's earliest development and may challenge long-standing assumptions in planetary science about how rocky planets evolve. By linking Earth's internal dynamics during its first 100 million years to its current structure, the study is among the first to blend fluid mechanics with chemistry to better understand the young Earth.
“This is the first time a physical model has shown that key features of the Earth’s lower mantle structure were already in place four billion years ago, just after the planet formed,” said Charles-Édouard Boukaré, assistant professor in the Department of Physics and Astronomy at York’s Faculty of Science and lead author of the study.
The mantle is the thick, rocky layer surrounding Earth's iron core, and its structure and behavior have played a critical role in the planet's evolution—particularly in how it cools and how the magnetic field is generated through the core. Understanding the mantle’s early solidification has remained a mystery, despite progress in fields such as seismology, geodynamics, and petrology.
Boukaré, who hails from France, collaborated with researchers in Paris on the paper, Solidification of Earth's mantle led inevitably to a basal magma ocean, published in Nature.
One key question the study addresses is how old the structures in Earth's interior are and how they came to be. Boukaré likens this to comparing the behavior of a child with that of an adult—early activity levels and conditions are vastly different, but the effects of those early years can persist throughout life.
“Kids do wild things because they have so much energy—planets are similar when they’re young,” he said. “Later in life, activity slows down, but some things that happen early can shape the entire future. It's the same for planets. Some features from the very beginning are still imprinted in their structure.”
Most existing mantle models focus on present-day conditions, assuming a solid-state mantle. To look further back in time, Boukaré developed a new model that simulates a much hotter, partially molten early mantle. This work, which he began during his PhD, uses a multiphase flow approach to simulate how magma solidified on a planetary scale.
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His simulations revealed a surprising result: most crystals formed under low-pressure conditions near the surface, rather than deep within the Earth under high pressure. This creates a different chemical signature than previously thought and may overturn long-held ideas about how rocky planets, including Earth, transitioned from molten bodies to solid worlds.
The findings not only provide a new perspective on Earth's formation but may also reshape our understanding of how other rocky planets develop across the solar system and beyond. To fully grasp the nature of ancient planets, the study suggests, we must begin by understanding the dynamics of their youth.
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