Research: Squid Evolved 100 Million Years Ago and Experienced Rapid Radiation

Paleontologists have adopted a cutting-edge digital fossil mining technique to examine over 250 fossil beaks from 40 ancient squid species. The findings indicate that there is no prolonged slow-moving change associated with the slower parietal layer, previously linked to the mass extinction event of late white matter around 66 million years ago. Early squid species had already established large populations, surpassing the biomass of both ammonites and fish. They evolved into intelligent and agile swimmers, contributing to modern marine ecosystems.

This lithograph features Loligo Forbesii, a squid species from the order Myopsida. Image credit: Comingio Mercuriano.

Squid are recognized as the most diverse and widely distributed group of marine cephalopods in today’s oceans, serving a crucial role in marine ecosystems as both predators and prey.

Their evolutionary success is generally attributed to the loss of a rigid external shell, a significant characteristic of their parietal ancestors.

Yet, their evolutionary beginnings remain unclear due to the scarcity of fossils from soft-bodied organisms.

The fossil record for squid dates back around 45 million years, with most specimens discovered consisting of fossilized statoris, or small calcium carbonites that assist in balance.

The early absence of such fossils has led to hypotheses that squid diversified following the mass extinctions during the Cretaceous period, approximately 66 million years ago.

Molecular studies of living squid species provide estimates regarding their divergence times; however, these estimates have become increasingly uncertain because of the dearth of prior fossil evidence.

In this recent study, Shin Ikegami, a paleontologist from Hokkaido University, and colleagues addressed these deficiencies using high-resolution grinding tomography and advanced image processing to digitally scan rocks as layered cross-sectional images, effectively revealing hidden 3D models.

This method was applied to Cretaceous carbonate rocks in Japan, resulting in the discovery of 263 fossilized squid beaks from 40 species across 23 genera and five families.

Results indicate that squid emerged around the boundaries of the early and late Cretaceous, roughly 100 million years ago, followed by a rapid diversification.

The authors assert that this newly uncovered fossil record significantly extends the documented origins of the two main squid groups: oegopsida extending back about 15 million years and myopsida extending as far back as 55 million years.

Early oegopsids showcased unique anatomical features that later species lacked, hinting at rapid morphological evolution, whereas Myopsids already displayed modern characteristics.

This study further indicates that late Cretaceous squids were more populous and often larger than their contemporaneous ammonite and bony fish counterparts. This ecological dominance might have triggered the radiation of bony fish and marine mammals roughly 30 million years ago, establishing squid as the first intelligent and agile swimmers that shaped modern marine ecosystems.

“In terms of population and size, these ancient squids were evidently proliferating across the oceans,” stated Dr. Ikenakamoto.

“Their body size rivaled that of fish, often even surpassing the ammonites found alongside them.”

“This demonstrates that squid thrived as the most abundant swimmers in the ancient seas.”

“These discoveries revolutionize our understanding of marine ecosystems in the past,” remarked Dr. Yasuhiro Iba from Hokkaido University.

“Squids were likely the pioneers of fast, intelligent swimmers that dominated the modern ocean.”

Study published in the journal Science.

____

Shin Ikegami et al. 2025. The origin and radiation of squid revealed by digital fossil mining. Science E 388 (6754): 1406-1409; doi: 10.1126/science.adu6248

Source: www.sci.news

This Magnetic Safe Offers Rapid Storage for the World’s Most Dangerous Substances

Antimatter particles are fundamentally similar to their normal matter counterparts, differing primarily in their opposite charges and momentum.

Although extremely rare, physicists routinely generate antiparticles using particle accelerators. Additionally, anti-Dutters occur naturally in high-energy processes near the event horizons of black holes.

The question of how and why the universe is predominantly made up of normal matter remains unresolved.

Creating antimatter is a complex and costly endeavor. The European Institute of Particle Physics (CERN) plays a crucial role in this process. Using an anti-proton decelerator, a proton beam strikes a metal target, resulting in the generation of anti-protons.

However, this process only yields tens of thousands of particles.

One of the significant challenges with antimatter is that when it interacts with normal matter, it vanishes instantly, releasing energy. Therefore, the task of preventing its annihilation and storing it long-term poses a substantial technical hurdle.

Nonetheless, CERN engineers are working on methods to store and transport small amounts of anti-protons.

The challenge with antimatter is that it completely disappears upon contact with normal matter, releasing energy. – Image credits: Getty Images

To achieve this, researchers cool anti-protons to approximately -269ºC (-452.2°F) to nearly halt their motion. They then contain them in a high-vacuum enclosure to avoid contact with normal matter, using superconducting magnets to trap them.

This process must be managed while maintaining the capability to extract particles and introduce new ones into the enclosure.

Despite these challenges, CERN aims to develop “traps” capable of storing billions of anti-protons simultaneously. Recent techniques have been validated by transporting regular matter across the Swiss CERN facility.

With advancements in vacuum systems, antimatter storage and transport may soon become routine activities in the upcoming year.


This article addresses the question posed by Leighton Haas of Hamburg: “How is antimatter preserved?”

We welcome your inquiries! You can email us at Question @sciencefocus.com or reach us on Facebook, Twitter, or Instagram. Please include your name and location.

Explore our ultimate Fun Facts for more amazing science content!


Read more:

Source: www.sciencefocus.com

BYD, a Chinese EV manufacturer, claims their new rapid charging system could rival the speed of filling up a gas tank

BYD, a Chinese electric vehicle (EV) maker, has announced plans to construct a charging network across China. This network aims to enable EVs to charge as quickly as refilling with gasoline.

Founder Wang Chuanfu revealed the “supere platform” at a home event in Shenzhen on Monday. This platform will support a peak charging speed of 1,000 kW, allowing cars to travel 400 km on a five-minute charge.

BYD’s 1,000 kW charging speed is double that of Tesla superchargers, offering faster charging speeds than before in the industry. Fast charging technology is crucial for increasing EV adoption.

Tesla, already struggling, saw its shares drop 15% on March 10, prompting concerns for owner Elon Musk. The company faces challenges in meeting sales targets and producing self-driving cars, with increasing competition from more affordable EV models from Chinese companies like BYD.

Tesla stocks dropped 4.8% on Wall Street, marking an eighth consecutive weekly decline. Baron.

Wang emphasized the goal of reducing EV charging times to match gasoline vehicle refueling times. The new charging architecture will debut with the Han L Sedan and Tang L SUV, priced from 270,000 yuan ($37,330).

BYD plans to build over 4,000 ultra-fast charging stations to support the new platform, but no specific timeline for construction was provided. Previously, BYD owners relied on public charging poles from other manufacturers or third-party operators.

While Tesla has been offering superchargers in China since 2014, other Chinese EV companies like NIO, Li Auto, Xpeng, and Zeekr have also established charging facilities.

BYD’s sales primarily come from plug-in hybrids, with aims to sell 5-6 million units this year.

Reuters and

Source: www.theguardian.com

Monitoring recurring rapid radio bursts at the edge of a stationary elliptical galaxy

The source of the newly detected fast radio burst, FRB 20240209A, is located 2 billion light-years from Earth, on the remote outskirts of an ancient elliptical galaxy with a mass of more than 100 billion solar masses. The remnants of young stars that theorists believe would generate such bursts of radio waves should have long died out in this 11.3 billion-year-old galaxy are detailed in two supplementary studies. Astrophysics Journal Letter this discovery shatters the assumption that fast radio bursts emanate only from regions of active star formation.



Gemini image showing the host galaxy (cyan crosshair) and local ellipse of FRB 20240209A. Image credit: Shah others., doi: 10.3847/2041-8213/ad9ddc.

“The conventional wisdom is that fast radio bursts (FRBs) originate from magnetars formed by collapsing supernovae,” said Taraneh Eftekari, an astronomer at Northwestern University.

“That doesn’t seem to be the case here. Young, massive stars die out as core-collapse supernovae, but we see no evidence of young stars in this galaxy.”

“Thanks to this new discovery, it is becoming clear that not all Feds are born from young stars.”

“Perhaps there is a subpopulation of FRBs associated with older systems.”

“This new FRB shows that just when we think we understand an astrophysical phenomenon, the universe can turn around and surprise us,” added Wen-Fai Feng, an astronomer at Northwestern University. Ta.

“This ‘dialogue’ with the universe is what makes our field of time-domain astronomy so incredibly thrilling.”

FRB 20240209A was discovered by the Canadian Hydrogen Intensity Mapping Experiment (CHIME) in February 2024.

FRBs are short, powerful bursts of radio waves that flare up and disappear within milliseconds, producing more energy in one quick burst than the sun emits in a year.

However, FRB 20240209A flared up multiple times. During the first burst from February to July 2024, the same source produced 21 additional pulses.

After the research team located the FRB, astronomers quickly used telescopes at W.M. Keck and Gemini Observatories to study the environment surrounding the event.

Surprisingly, rather than discovering young galaxies, these observations revealed that the FRB’s origin lies 2 billion light-years from Earth, at the edge of a neighboring galaxy 11.3 billion years ago.

To learn more about this unusual host galaxy, the researchers used high-performance computers to run simulations.

They discovered that this galaxy is extremely bright and incredibly huge – 100 billion times the mass of our Sun.

“This appears to be the most massive FRB host galaxy ever. It’s one of the most massive galaxies out there,” Dr. Eftekari said.

Although most FRBs occur inside galaxies, the authors tracked FRB 20240209A to the outskirts of its homeworld, 130,000 light-years away from the galaxy’s center, where there are few other stars.

“Of all the FRB populations, this FRB is the furthest from the center of its host galaxy,” said Vishwangi Shah, a graduate student at McGill University.

“This is both surprising and interesting because FRBs are expected to occur inside galaxies, often in star-forming regions.”

“The location of this FRB so far outside its host galaxy raises the question of how such an energetic event could occur in a region where new stars are not forming.”

According to the research team, FRB 20240209A likely originated within a dense globular cluster.

Such clusters are promising sites for magnetars that may have formed through other mechanisms, such as the merger of two neutron stars or the collapse of a white dwarf star under its own gravity, or in conjunction with older stars.

“The globular cluster origin of this repeating FRB is the most likely scenario explaining why this FRB is located outside of its host galaxy,” Shah said.

“Although we do not know for a fact whether there is a globular cluster at the FRB’s location, we have submitted a proposal to use NASA/ESA/CSA’s James Webb Space Telescope for follow-up observations of the FRB’s location.”

“If so, this FRB would be only the second FRB known to exist within a globular cluster. If not, consider other exotic scenarios for the origin of FRBs. You will need to.”

“It’s clear that there is still a lot of interesting discovery to be made about the Fed, and that its environment may hold the key to unlocking its secrets,” Dr. Eftekari said.

_____

T. Eftekari others. 2025. A huge, stationary elliptical main galaxy that repeats high-speed radio bursts FRB 20240209A. APJL in press. arXiv: 2410.23336

Vishwangi Shah others. 2025. A source of high-speed radio bursts that repeat on the outskirts of a quiet galaxy. APJL 979, L21; doi: 10.3847/2041-8213/ad9ddc

Source: www.sci.news

The rapid intensification of Hurricane Milton is indicative of a climate trend

The Milton, which is expected to make landfall along the Florida Gulf Coast Wednesday evening, is sailing through unusually warm waters in the Gulf of Mexico. Temperatures in much of the ocean basin were well above 80 degrees Fahrenheit, with some parts of the bay up to 4 degrees warmer than normal. Data from NASA’s Jet Propulsion Laboratory.

Rising temperatures in the Gulf also strengthened Hurricane Helen, which made landfall in Florida’s Big Bend region less than two weeks later.

2023 study published in journal scientific report We find that Atlantic tropical cyclones are about 29% more likely to develop rapidly from 2001 to 2020 compared to 1971 to 1990.

Scientists have documented many recent examples of rapid intensification, including Hurricane Harvey in 2017, Hurricane Laura in 2020, Hurricane Ida in 2021, and Hurricane Idalia last year. 2019 Hurricane Dorian’s peak wind speed increased from 150 mph to 185 mph in nine hours, and 2022 Hurricane Ian experienced two rapid intensifications before making landfall in Florida.

Although this process is well documented, rapid intensification is difficult to predict. Although scientists know the ingredients needed to activate this phenomenon, it remains difficult to predict exactly how and when it will occur, and its exact triggers.

Milton is expected to weaken slightly before making landfall, but the storm’s impacts will be severe. A storm surge watch is in effect for the Florida Gulf Coast, including the Tampa Bay area, with potentially life-threatening storm surges of up to 12 feet expected. As many as 15 million people are under flood watches across the state.

Source: www.nbcnews.com