Ancient Rocks Reveal the First Signs of Earth’s Structural Activity

The Pilbara Craton in Western Australia features rocks that date back 3.5 billion years.

Elizabeth Czitronyi / Alamy

Rocks from Australia reveal that tectonic plates were shifting as far back as 3.5 billion years ago, a breakthrough that alters our understanding of the onset of plate tectonics over subsequent hundreds of millions of years.

Currently, along with roughly eight major hard rock plates on Earth’s surface, several smaller plates are interacting with the softer rock layer beneath. When these plates’ edges grind against one another, it can lead to sudden geological upheavals, such as earthquakes, and gradual processes like mountain range formation.

However, there is disagreement among geologists regarding the configurations of these ancient plates and their movements. Some researchers claim to have found indications of tectonic activity as far back as 4 billion years ago when the planet was significantly hotter; others argue that more compelling evidence is noted after 3.2 billion years ago.

Much of this data derives from the chemical compositions of rocks, which suggest past movements. Despite this, records detailing the interactions of early plates remain scarce, which is regarded as critical evidence supporting plate tectonics.

Recently, Alec Brenner and his team from Yale University claim to have uncovered substantial evidence of relative plate movement dating back 3.5 billion years in the eastern Pilbara Craton of Western Australia. They traced the magnetic orientation of rocks aligned with Earth’s magnetic field, observing shifts similar to how a compass needle changes direction when the ground moves.

Brenner and colleagues initially dated the rock using radioisotope analysis, establishing that at certain times, the rock’s magnetism remained unchanged. By observing this magnetization shift, they demonstrated that the rock mass progressively moved at a rate of several centimeters each year. They compared these findings to similarly examined rocks in the Barberton Greenstone Belt in South Africa, which exhibited no such movement.

“This suggests that some type of plate boundary must exist between these two regions to accommodate that relative movement,” remarked Brenner during his presentation at the Goldschmidt Geochemical Conference in Prague, Czech Republic, on July 9.

“Approximately 3.8 billion years ago, the Pilbara plate transitioned from medium to high latitudes, eventually reaching proximity to Earth’s magnetic poles and, possibly millions of years later, to the latitude of Svalbard.”

“If two plates are moving relative to one another, there must be various dynamic interactions happening between them,” noted Robert Hazen from the Carnegie Institute of Science in Washington, DC. “It cannot be an isolated event.”

Nonetheless, multiple interpretations exist regarding the underlying causes of this movement, according to Hazen. The variability in plate movement rates adds to the confusion, and existing data could align with various theories regarding Earth’s interior structure at that time.

At the very least, this discovery indicates the presence of structural boundaries, according to Michael Brown from the University of Maryland. However, he argues that the nature of rock movement appears dissimilar to contemporary understanding of plate tectonics. “Essentially, the Pilbara plate moved to higher latitudes to prevent stagnation, which is atypical within any current plate structural model.”

Brown posits that this aligns with the theory suggesting the Earth’s crust consisted of numerous smaller plates propelled by a thermal mantle plume during that period. He believes the remnants of these small plates examined by Brenner and his team provide evidence of movement; however, due to their limited representation of the crust, they may not accurately reflect broader Earth movements.

Brenner’s team also discovered indications that the Earth’s magnetic field underwent reversals around 3.46 billion years ago. Unlike today’s magnetic field reversals, which occur every million years, these ancient magnetic shifts seemed to happen much more frequently, over spans of tens of millions of years. This could imply a fundamentally different set of energies and mechanisms at play, as noted by Brenner.

Hazen emphasized that the scarcity of magnetic data leads to ongoing debates about the state of Earth’s magnetic field during that era of its evolution. “I believe this discovery raises the bar significantly,” he asserts. “It represents a vital breakthrough in understanding early magnetic reversals, shedding light on the core’s geomechanics in ways previously unexplored.”

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Source: www.newscientist.com

Webb Sheds New Light on the Structural Evolution of Disk Galaxies

Modern disk galaxies frequently display distinct thin and thick disks. The mechanisms driving the formation of these two discs and the timeline of their emergence are still unanswered questions. To investigate these issues, astronomers examined various epochs (statistical samples of 111 edge-on disk galaxies dating back up to 11 billion years, or approximately 2.8 billion years post-Big Bang) utilizing archived data from the NASA/ESA/CSA James Webb Space Telescope.

Webb/nircam composite images of a quarter of the team’s samples were sorted by increasing redshift. Image credit: Tsukui et al., doi: 10.1093/mnras/staf604.

Present-day disk galaxies often comprise extensive, star-rich outer disks alongside thin, star-like disks.

For instance, the thick discs of the Milky Way reach approximately 3,000 light-years in height, while the thin discs are roughly 1,000 light-years thick.

But what mechanisms lead to the formation of this dual disk structure?

“The thickness of high redshift discs, or unique measurements from the early universe, serve as benchmarks for theoretical research that can only be conducted using Webb,” states Takagi, an astronomer at the Australian National University.

“Typically, older, thicker disk stars are dim, while the younger, thinner disk stars dominate the galaxy.”

“However, Webb’s exceptional resolution allows us to observe and highlight faint older stars, enabling us to distinguish between two disk structures in a galaxy and measure their thickness separately.”

Through an analysis of 111 edge-on targets over cosmological time, astronomers studied both single-disc and double-disc galaxies.

The findings indicate that galaxies initially form a thick disk, which is followed by the formation of a thin disk.

The timing of this process is contingent on the galaxy’s mass: high-mass, single-disk galaxies transitioned to two-disk structures around 8 billion years ago.

In contrast, a thin disk emerged about 4 billion years ago within low-mass, single-disk galaxies.

“This is the first time we’ve resolved a thin star disk at such a high redshift,” remarked Dr. Emily Wysnioski from the Australian National University.

“The novelty becomes evident when observing the onset of thin star disks.”

“It was astonishing to witness a thin star disk from 8 billion years ago, and even further back.”

To elucidate the transition from a single thick disk to a dual-disk structure, as well as the timing differences between high-mass and low-mass galaxies, researchers expanded their investigation beyond the initial edge-on-galaxy samples. They examined data showing the movement of gases from large millimeter/sub-millimeter arrays (ALMAs) in Atacama and ground surveys.

By considering the movement of the galaxy’s gas disks, they found their results aligned with the “turbulent gas disk” scenario.

In this framework, the turbulent gas disks of the early universe catalyze intense star formation, leading to the creation of thick star disks.

As stars form, they stabilize the gas disks, diminishing turbulence and consequently resulting in thinner disks.

Larger galaxies can convert gas into stars more efficiently and thus calm down more quickly than their lower-mass counterparts, leading to the formation of the earlier thin disk.

“This study delineates structural differences between thin and thick discs, but we aim to explore further,” Dr. Tsukui mentioned.

“We look to incorporate the types of information typically acquired from nearby galaxies, such as stellar movement, age, and metallicity.”

“By doing so, we can bridge insights from both nearby and distant galaxies, enhancing our understanding of disk formation.”

Survey results were published in Monthly Notices of the Royal Astronomical Society.

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Takagi Tsukui et al. 2025. The emergence of thin and thick discs of galaxies across the history of the universe. mnras 540(4): 3493-3522; doi: 10.1093/mnras/staf604

Source: www.sci.news