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A new study has found that a single mysterious event about 19 million years ago wiped nearly the entire population of sharks. Scientists behind the new research say that studying the shark teeth buried in deep-sea sediment, revealed that the current diversity among sharks is only a tiny remnant of a much larger variety that existed back then. They say this unidentified major ocean extinction caused the reduction in the shark diversity by over 70 percent and nearly a complete loss in total abundance. The cause of this event remains a mystery, scientists said.

Researchers say that this single event led to the virtual disappearance of sharks from open-ocean sediments, declining in abundance by almost 90 percent. They added that the abrupt extinction was independent of any known global climate event.

According to the research report published in the journal Science, modern shark forms began to diversify within two to five million years after the near extinction, but they represent only a sliver of what sharks once were.

A report in Life Science quoted Elizabeth Sibert, a postdoctoral fellow at Yale University’s Institute for Biospheric Studies and co-author of the study, as saying, “Sharks have been around for 400 million years; they’ve weathered a lot of mass extinctions.”

The study into the ichthyolites, microscopic fossils of shark scales, found in most types of sediments but are tiny and relatively rare when compared to other microfossils, led to the discovery, Sibert told Live Science.

While scientists in the 1970s and ’80s studied ichthyolites, only a few researchers examined them before Sibert, who investigated them for her doctorate, which she completed in 2016. “A lot of what I’ve done in my early career as a scientist was figuring out how to work with these fossils, what kinds of questions we can ask about them,” Sibert said.

For their new study, Sibert and Leah Rubin, a co-author who was an undergraduate student at the College of the Atlantic in Bar Harbor, Maine at the time of the research, studied sediment cores extracted many years ago by deep-sea drilling projects from two different sites: one in the middle of the North Pacific, and the other in the middle of the South Pacific.

“We picked those sites particularly because they are far away from land and they’re far away from any influences of changing ocean circulation or ocean currents,” Sibert said.

Rubin, who is now going to be a doctoral student at the State University of New York College of Environmental Science and Forestry, said that the extreme nature of this decline in the diversity of sharks was the most surprising aspect of the study to them as well. The million-dollar question, Rubin says, is what caused it?

The paper is just the beginning, Sibert says, and hopes it’s going to be a really interesting next decade to figure out more about what happened at the time that caused the extinction among sharks.


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NASA’s EZIE Satellites Begin Mission to Study Auroral Electrojets and Space Weather

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NASA’s EZIE Satellites Begin Mission to Study Auroral Electrojets and Space Weather

Under the night sky in California, NASA’s Electrojet Zeeman Imaging Explorer (EZIE) mission was launched aboard a SpaceX Falcon 9 rocket at 11:43 p.m. PDT on March 14 from Vandenberg Space Force Base. Three small satellites, designed to study Earth’s auroral electrojets, were carried into orbit. The deployment of these satellites was confirmed at approximately 2 a.m. PDT on March 15. Over the next ten days, signals will be transmitted to ensure they are functioning properly before commencing their 18-month mission.

Mission Objectives and Scientific Significance

According to the mission details shared by NASA, EZIE’s satellites will operate in a formation known as “pearls-on-a-string,” flying between 260 and 370 miles above Earth. These satellites will map the intense electrical currents that flow through the upper atmosphere in polar regions. These currents, linked to solar storms, influence auroras and Earth’s magnetic field. The study aims to improve understanding of space weather and its effects on technology, including satellite operations and communication systems.

Speaking to NASA, Jared Leisner, Program Executive for EZIE, stated that small-scale missions like EZIE are being prioritised for their scientific value despite their inherent risks. The data collected will contribute to research not only about Earth but also about magnetic interactions on other planets.

Unique Approach to Orbit Control

Instead of traditional propulsion methods, EZIE satellites will utilise atmospheric drag to adjust their positions. As reported by NASA’s Goddard Space Flight Center, Larry Kepko, EZIE’s mission scientist, explained that previous studies have focused on either large or small-scale observations of these currents. EZIE’s approach will provide new insights into their formation and evolution.

Public Engagement and Educational Outreach

To expand public participation, magnetometer kits known as EZIE-Mag are being distributed to students and science enthusiasts. Data collected from these kits will be integrated with EZIE’s space-based measurements to provide a more detailed understanding of Earth’s electrical currents.
The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center and funded by NASA’s Heliophysics Division. The Johns Hopkins Applied Physics Laboratory leads the project, with CubeSats developed by Blue Canyon Technologies and magnetometers built by NASA’s Jet Propulsion Laboratory.

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Antarctic Ice Melt Weakens Strongest Ocean Current, Disrupting Global Circulation

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Antarctic Ice Melt Weakens Strongest Ocean Current, Disrupting Global Circulation

Earth’s most powerful ocean current is losing strength, with potential consequences for global ocean circulation. Scientists have projected that the Antarctic Circumpolar Current (ACC) could slow down by as much as 20 percent by 2050. The weakening of this current, which connects multiple oceans and regulates heat exchange, is being attributed to the increasing influx of cold meltwater from Antarctica. This shift in ocean dynamics could have far-reaching effects on sea levels, temperatures, and marine ecosystems worldwide.

Findings from Climate Modelling

According to a study published in Environmental Research Letters, a team led by Bishakhdatta Gayen, a fluid mechanist at the University of Melbourne, has analysed how Antarctic ice melt is affecting the ACC. Using one of Australia’s most advanced climate simulators, researchers modelled interactions between the ice sheet and ocean waters. The study indicates that the introduction of fresh, cold meltwater weakens the current by altering ocean density and reducing convection between surface and deep waters.

Consequences of a Slower Current

The slowdown of the ACC is expected to disrupt global ocean circulation. As convection weakens, warm water may travel further into Antarctic waters, accelerating ice melt and contributing to rising sea levels. The weakening current could also allow invasive species to reach the Antarctic coastline, affecting the region’s ecosystem.

Speaking to Live Science, Gayen compared the process to a “merry-go-round,” explaining that a slower current could lead to faster migration of marine organisms toward Antarctica. Long-term monitoring will be necessary to fully understand these changes, as scientists have only recently begun studying the ACC’s behaviour in detail. The impact of these shifts will not remain confined to Antarctica but will influence ocean circulation patterns across the planet.

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Wolf-Rayet 104’s Orbit Tilt Reduces Gamma-Ray Burst Threat, Study Finds

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Wolf-Rayet 104's Orbit Tilt Reduces Gamma-Ray Burst Threat, Study Finds

A new study has shed light on the orbital alignment of the well-known Wolf-Rayet 104 (WR 104) system, long considered a potential threat due to its speculated gamma-ray burst (GRB) risk. Observations conducted using multiple instruments at the W. M. Keck Observatory in Hawaiʻi have confirmed that the star system‘s orbit is tilted 30 to 40 degrees away from Earth. This discovery significantly reduces concerns that a supernova from WR 104 could direct a GRB toward the planet.

Study Confirms Orbital Tilt

According to research published in the Monthly Notices of the Royal Astronomical Society, WR 104 comprises two massive stars locked in an eight-month orbital cycle. The system features a Wolf-Rayet star emitting a strong carbon-rich wind and an OB star producing a hydrogen-dominated stellar wind. Their collision generates a distinctive dust spiral that glows in infrared light.

The structure was first observed in 1999 at the Keck Observatory, and early models suggested that the pinwheel-like dust formation was face-on from Earth’s perspective. This led to speculation that the rotational axis of the stars—and potentially a GRB—could be aimed directly at Earth. However, new spectroscopic data contradicts this assumption.

Unexpected Findings Challenge Previous Models

Reportedly, Grant Hill, Instrument Scientist and astronomer, stated, that their view of the pinwheel dust spiral from Earth absolutely looked face-on and it seemed like a pretty safe assumption that the two stars are orbiting the same way. However, his analysis revealed a surprising discrepancy, with the stellar orbit misaligned from the dust structure.

This unexpected finding raises new questions about how the dust plume forms and whether additional factors influence its shape. While the discovery brings relief regarding potential GRB risks, it also suggests there is still much to understand about WR 104’s unique characteristics

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