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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 to Launch First Quantum Sensor for Gravity Monitoring in Space

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NASA to Launch First Quantum Sensor for Gravity Monitoring in Space

NASA’s Jet Propulsion Laboratory, commercial companies, and academic institutions together are developing the first space-based quantum sensors for gravitational measurement. Two groups of very cold rubidium atoms will be used as weights for the Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument, ensuring accurate measurements over long periods. Measuring gravity with a volume of 0.3 cubic yards (0.25 cubic meters) and weighing just over 275 pounds (125 kg), the instrument will be smaller and lighter than conventional space-based gravity instruments.

Quantum sensors offer enormous promise for sensitivity; estimates suggest they could be as much as ten times more sensitive in tracking gravity than conventional sensors. Approved to begin at the end of the decade, the technology validation project aims to test novel atomic-scale atomic manipulation of interactions between light and matter. To progress the sensor head technology and the laser optical system, NASA is working with small companies. The QGGPf instrument could lead to planetary science and fundamental physics applications.

NASA’s Quantum Gravity Sensor to Reveal Earth’s Subsurface

According to a NASA post, the Jet Propulsion Laboratory, private companies, and academic institutions are developing the first space-based quantum sensor for measuring gravity. This mission, supported by NASA’s Earth Science Technology Office (ESTO), will pave the way for groundbreaking observations of everything from petroleum reserves to global supplies of fresh water. Its gravitational field is dynamic and changing every day as geologic processes distribute mass throughout its surface. Sensitive instruments called gravity gradiometers can map the subtleties of Earth’s gravitational field and link them to belowground structures such as mineral deposits and aquifers.

The Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument will use two clouds of ultracold rubidium atoms as test masses. The difference in acceleration between these matter waves will measure the difference in acceleration between these matter waves to locate gravitational anomalies. This system allows for space-based gravity measurements to remain accurate over long periods and is smaller and lighter than traditional space-based gravity instruments.

NASA Tests Atomic-Scale Tech to Advance Space Sensors and Earth Science

The main purpose of this technology validation mission is to test a collection of novel technologies for manipulating interactions between light and matter at the atomic scale. With JPL partnering with AOSense and Infleqtion to enhance sensor head technology and NASA’s Goddard Space Flight Center working with Vector Atomic to advance the laser optical system, the project involves notable partnerships between NASA and a few quantum-focused entrepreneurs.

Ultimately, the findings of this Pathfinder project might increase our capacity to explore Earth, understand far-off worlds, and value the role gravity plays in creating the universe.

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NASA’s Hubble Shares Detailed Mosaic of the Sombrero Galaxy

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NASA’s Hubble Shares Detailed Mosaic of the Sombrero Galaxy

NASA’s Hubble Space Telescope, on its 35th anniversary, reprocessed a detailed image of the Sombrero Galaxy (Messier 104) on April 11, shared by the European Space Agency. This improvised image, generated from numerous Hubble images, signals fine dust structures, the luminous galactic nucleus with a backdrop occupied by stars and various distant galaxies. This mosaic, taken from the updated data and refined processing techniques, makes it a significant upgrade to previous Hubble observations. This release marks a milestone in the so-far legacy of the Hubble Space Telescope, showcasing the evolution of modern techniques and escalation into archival space imagery.

Research and Discovery

Katie Noll and other scientists of the European Space Agency worked in collaboration with NASA using the Hubble Space Telescope. New imaging technology and methods were used to build upon the original Hubble image released in October 2003. On November 25, 2024, the James Webb Space Telescope also offered a fresh image and perspective on the galaxy, further enriching the research.
The Sombrero Galaxy is located about 30 million light years away in the Virgo constellation and is renowned for its unique shape that resembles a sombrero hat. Its sharp and edgy orientation, titled just six degrees, throws a dramatic view with a dust-laced disc and a brightening central bulge.

Structure and Star Formation

In terms of star formation, the Sombrero Galaxy is visually rich but surprisingly calm. Within its dusty disc, less than one solar mass is transformed into stars every year. This galaxy is so silent that even its massive black hole, with a weight of nine billion solar masses, stays inactive or dormant. Looking into the structure of the galaxy, it is baffling as it displays the classic disc of spiral galaxies.
However, it also features a halo and bump similar to those of elliptical galaxies. This uneven combination leaves scientists unsure of whether it should be kept in the category of elliptical or somewhere in between.

Future Exploration

The crucial part is analysing the chemical composition of stars in the galaxy’s halo. In the precise measurements done by Hubble there revealed an astonishing presence of metal-rich stars was revealed in its outer region. Researchers believe that the Sombrero Galaxy could have blended with other large galaxies billions of years ago, resulting in the mysterious hybrid structure observed in the present.

Scientists are looking forward to fusing Hubble’s optical data with infrared imaging from the James Webb Space Telescope for future investigation of the galaxy’s structure. This multi-wavelength research could unleash deeper insights about its formation and clarify how galaxy mergers can shape its evolution.

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Did Domesticated Cats Originate in Tunisia? New Study Sheds Light

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Did Domesticated Cats Originate in Tunisia? New Study Sheds Light

The origin of domestic cats has been a prominent topic amongst researchers. Their emergence has been linked to the Neolithic period, where they accompanied the farmers while spreading across Europe, along with the agricultural adaptation. However, further investigations have been conducted wherein the significance puzzled the archaeologists. Recently, two large-scale investigations were conducted by the University of Rome Tor Vergata and 42 institutions, and another by the University of Exeter and contributors from 37 institutions, pointing out that Tunisia could be the place of the origin of the domestic cat.

The Tor Vergata Study on Cats

The expert team of researchers from the University of Rome Tor Vergata conducted paleo-genomic analyses, where they analyzed the specimens of cats from 97 archaeological sites across Europe and Anatolia. Likewise, they also took samples from North Africa, Bulgaria, and Italy.

According to the study published on bioRxiv titled “The dispersal of domestic cats from Northern Africa and their introduction to Europe over the last two millennia”, the researchers analysed a total of 70 low-coverage ancient genomes, 37 radiocarbon-dated cat remains, and 17 modern and museum genomes.

The Tor Vergata Study Results

The Tor Vergata Team, as a result of the nuclear DNA analyses, identified felines embedded by domestic ancestry that appeared from the first century CE onwards in Europe. The team also identified two introductory waves — one from the second century BCE, where wildcats were brought from Northwest Africa to Sardinia, raising the current island population, whereas the other wave belonged to the Roman Imperial period, where the cats genetically sounded similar to domestic cats in Europe. Here, Tunisia was observed as the base for early domestication.

The University of Exeter Study

According to a reprint titled, “Redefining the timing and circumstances of cat domestication, their dispersal trajectories, and the extirpation of European Wildcats,” the collaborative study by the University of Exeter shed light on a distinct timeline. They analysed 2,416 archeological field bones around 206 sites and cross-referenced morphological data, accompanied by genetic findings.

The key findings of this collaborative study defined that domestic cats first appeared in the early first millennium BCE in Europe. Their existence occurred before Roman expansion.

The Egyptian Connection

According to mythological theories, the emergence of domestication of cats was related to religious and cultural dimensions. In Egypt, the cats were considered holy. Also, in Greek culture, these creatures became religious symbols of Artemis and Diana — a multifaceted divinity.

Although the two studies offer different understandings, the results indicate that cats appeared in Europe after moving from North Africa as a result of cultural practices, religious reverence, and trade networks.

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