Solar-System Dynamics Triggered Earth’s Plate Tectonics

Asteroid Impact


“It is remarkable to think that our oldest animal ancestors—and therefore all of us—may owe our existence, in part, to an unusual episode of plate tectonics over half a billion years ago” said Tim Lenton, professor of Climate Change and Earth System Science with the University of Exeter’s Global Systems Institute in June, 2019 about the most dramatic moment in the history of evolution when the spectacular supernova of biology, the Cambrian Explosion, was detonated and the world of animal life was born with the rise in oxygen levels during the formation of the supercontinent Gondwana and a major increase in continental arc volcanism—chains of volcanoes often thousands of miles long formed where continental and oceanic tectonic plates collided.

Earth’s plate tectonics, unique in the solar system, are critical for maintaining a surface climate where life can thrive –without the cycling of material between its surface and interior, the convection that drives the Earth’s magnetic field would not be possible and without a magnetic field, we would be bombarded by cosmic radiation.

“We tend to think of the Earth as an isolated system, where only internal processes matter. Increasingly, though, we’re seeing the effect of solar system dynamics on how the Earth behaves,” says Craig O’Neill, director of Macquarie University’s Planetary Research Center about a new study, published in Geology, suggesting that this earthly transition may in fact have been triggered by extra-terrestrial impacts.

When—and how—the Earth’s surface evolved from a hot, primordial mush into a rocky planet continually resurfaced by plate tectonics remain some of the biggest unanswered questions in earth science research.

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Lunar Impacts Yield Clues

Modelling simulations and comparisons with lunar impact studies have revealed that following Earth’s accretion about 4.6 billion years ago, Earth-shattering impacts continued to shape the planet for hundreds of millions of years. Although these events appear to have tapered off over time, spherule beds—distinctive layers of round particles condensed from rock vaporized during an extra-terrestrial impact—found in South Africa and Australia suggest the Earth experienced a period of intense bombardment about 3.2 billion years ago, roughly the same time the first indications of plate tectonics appear in the rock record.

This coincidence caused O’Neill and co-authors Simone Marchi, William Bottke , and Roger Fu to wonder whether these circumstances could be related. “Modelling studies of the earliest Earth suggest that very large impacts—more than 300 km in diameter—could generate a significant thermal anomaly in the mantle,” says O’Neill. This appears to have altered the mantle’s buoyancy enough to create upwellings that, according to O’Neill, “could directly drive tectonics.”

But the sparse evidence found to date from the Archaean—the period of time spanning 4.0 to 2.5 billion years ago—suggests that mostly smaller impacts less than 100 km in diameter occurred during this interval. To determine whether these more modest collisions were still large and frequent enough to initiate global tectonics, the researchers used existing techniques to expand the Middle Archaean impact record and then developed numerical simulations to model the thermal effects of these impacts on Earth’s mantle.

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“Primed  for Subduction”

The results indicate that during the Middle Archaean, 100-kilometer-wide impacts (about 30 km wider than the much younger Chixculub crater) were capable of weakening Earth’s rigid, outermost layer. This, says O’Neill, could have acted as a trigger for tectonic processes, especially if Earth’s exterior was already “primed” for subduction.

“If the lithosphere were the same thickness everywhere, such impacts would have little effect,” states O’Neill. But during the Middle Archean, he says, the planet had cooled enough for the mantle to thicken in some spots and thin in others. The modeling showed that if an impact were to happen in an area where these differences existed, it would create a point of weakness in a system that already had a large contrast in buoyancy—and ultimately trigger modern tectonic processes.

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“Our work shows there is a physical link between impact history and tectonic response at around the time when plate tectonics was suggested to have started,” says O’Neill. “Processes that are fairly marginal today—such as impacting, or, to a lesser extent, volcanism, actively drove tectonic systems on the early Earth,” he says. “By examining the implications of these processes, we can start exploring how the modern habitable Earth came to be.”

More information: C. O’Neill et al. The role of impacts on Archaean tectonics, Geology (2019). DOI: 10.1130/G46533.1
Journal information: Geology

The Daily Galaxy, Andy Hennig,   Geological Society of America 

Image credit top of page: BBC “Day the Dinosaurs Died”

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