Webb Telescope Unveils Most Detailed Dark Matter Map to Date

Utilizing the ultra-sharp images from the NASA/ESA/CSA James Webb Space Telescope, astronomers have successfully crafted a highly detailed, wide-area mass map of the Universe. This groundbreaking map reveals the intricate interweaving of dark matter and ordinary matter, stretching from the filaments of galaxies to the dense clusters. Developed as part of the COSMOS-Web survey, this new map boasts more than double the resolution of previous efforts and delves deeper into the early universe’s evolution.



This web image shows about 800,000 galaxies, overlaid with a dark matter map in blue. Image credit: NASA / STScI / J. DePasquale / A. Pagan.

Dark matter constitutes roughly 85% of the universe’s total matter, yet it’s challenging to detect since it neither emits nor absorbs light, rendering it invisible to standard telescopes.

However, its gravitational influence alters the trajectory of light from far-off galaxies.

By examining subtle distortions in the shapes of numerous distant galaxies, scientists can ascertain how this unseen mass is distributed, irrespective of its nature.

When compared with known luminous structures, researchers can pinpoint the locations of dark matter.

Previous mass maps generated using the NASA/ESA Hubble Space Telescope and other observatories suffered from limited resolution, sensitivity, and area coverage, restricting their views to only the largest cosmic structures.

Dr. Diana Scognamiglio from NASA’s Jet Propulsion Laboratory and her team harnessed Webb’s imaging capabilities to analyze the shapes of approximately 250,000 galaxies, reconstructing the most detailed mass map of a contiguous universe region to date.

“This is the most extensive dark matter map produced in conjunction with Webb, boasting clarity unmatched by any prior dark matter maps from other observatories,” stated Dr. Scognamiglio.

“Previously, we only glimpsed blurred images of dark matter.”

“With Webb’s extraordinary resolution, we can now observe the universe’s invisible framework in unprecedented detail.”

This new map uncovers substantial galaxy clusters along with intricate networks of dark filamentary bridges and low-mass galaxies, too faint or too distant to be spotted by conventional telescopes.

These formations align with major cosmological models, suggesting that galaxies emerge at dense points between the dark matter filaments spreading throughout the universe.

Dr. Gavin Leroy, an astronomer at Durham University, remarked: “By illustrating dark matter with unparalleled precision, our map demonstrates how the unseen elements of the universe shaped visible matter, facilitating the creation of galaxies, stars, and ultimately, life itself.”

“This map highlights the crucial role of dark matter, the universe’s true architect, which gradually organizes the structures we observe through our telescopes.”

Professor Richard Massey of Durham University added, “Wherever normal matter exists in the universe today, dark matter is also present.”

“Every second, billions of dark matter particles pass through your body. They are harmless and continue on their paths unnoticed.”

“However, the entire cloud of dark matter surrounding the Milky Way possesses enough gravity to keep our galaxy intact. Without dark matter, the Milky Way would disintegrate.”

For more information, refer to the published results in this week’s edition of Nature Astronomy.

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D. Scognamiglio et al. Ultra-high resolution map of (dark) matter. Nat Astron published online on January 26, 2026. doi: 10.1038/s41550-025-02763-9

Source: www.sci.news

DNA Cassette Tapes: A Storage Solution for All Recorded Songs to Date

SEI 265469254

DNA cassettes resemble music cassette tapes

Jiankai Li et al. 2025

With a modern twist, the nostalgic cassette tape may be resurging in the form of DNA. Previously used solely as a medium for information storage, researchers have now fused the concept with the style of 1980s cassette tapes, leading to the innovation termed DNA cassettes.

Xingyu Jiang and his colleagues at the Southern University of Science and Technology in Guangdong, China, crafted these cassettes by printing synthetic DNA molecules onto plastic tapes. “The sequences can be designed in such a manner that the order of DNA bases (A, T, C, G) conveys digital information just like binary code (0 or 1) in a computer,” he remarks. This allows for the storage of all forms of digital files, from text and images to audio and video.

A significant challenge of earlier DNA storage methods was accessing the data. To remedy this, the team implemented a series of barcodes on the tape to simplify searching. “It’s akin to locating a book in a library,” explains Jiang. “You first identify the shelf corresponding to the book and then locate the specific book on that shelf.”

The tape is also treated with a protective coating dubbed “crystal armor,” made from zeolite imidazolate, which ensures the integrity of the DNA. This allows the cassettes to retain data for centuries without degradation.

While classic cassette tapes can hold around 12 songs per side, the new 100-meter DNA cassette can house over 3 billion pieces of music comprising 10 megabytes of songs. This results in an astounding total data storage capacity of 36 petabytes, comparable to a 36,000 terabyte hard drive.

However, Jiankai Li warns that if one were to place the new tape into an old-school Walkman, it wouldn’t produce sound. “Our tapes contain DNA molecules,” he notes. “It’s similar to trying to play a photograph on a record player—the formats simply don’t align.”

Topic:

Source: www.newscientist.com

Discovered the Largest Black Hole in the Universe to Date

Astronomers have been monitoring the largest black holes observed in space thus far.

Through a combination of two distinct measurement techniques, researchers have recently identified that these colossal black holes possess nearly 10,000 times the mass of the ultra-massive black holes at the center of our galaxy.

This colossal black hole is situated five billion light-years from Earth, at the core of the Cosmic Horseshoe, one of the largest known galaxies. This massive galaxy seems to gather all the galaxies in its vicinity, meaning both it and its black hole have reached their ultimate sizes.

The black hole itself weighs an astonishing 36 billion times the mass of our sun.

The discovery is particularly remarkable given that these black holes are inactive, lacking the typical surrounding luminous dusty disc.

Instead, a recent study published in the Monthly Notices of the Royal Astronomical Society utilized a combination of two established methods to ascertain the size of this mega black hole.

“The ‘golden’ method generally depends on the kinematics of stars, meaning we measure how the stars move within the galaxy,” noted Carlos Mello in an interview with BBC Science Focus. He is a PhD student at a federal university in Brazil that led the research.

The speed of stars situated at the center of a galaxy correlates closely with the mass of its supermassive black hole. Scientists report that these stars are moving at astonishing velocities, around 400 kilometers (249 miles) per second, indicating an extraordinarily large black hole.

“However, this technique is most efficient for nearby galaxies where telescopes can better resolve the area surrounding the black hole,” Mello explained.

Given that the Cosmic Horseshoe is five billion light-years away, astronomers also employed a second method that utilizes the gravitational lensing effect of galaxies.

The Cosmic Horseshoe is known for the nearly perfect ring of light formed by a gravitational lens that bends light from a background galaxy – Credit: NASA/ESA

Gravitational lenses occur when light from a distant galaxy passes by a massive “lens” object, in this case, the black hole within the Cosmic Horseshoe. The gravity from this “lens” distorts the incoming light much like a magnifying glass, amplifying the light from the background galaxy while altering its appearance.

Astronomers can utilize this distortion to gauge the mass of the lensing object.

“The Cosmic Horseshoe is exceptional because it enables us to leverage both of these powerful methods simultaneously. This gives me greater confidence in the measurements of the black hole and its mass,” Mello remarked.

Both the galaxy and its black hole have achieved immense scales by merging with neighboring galaxies. This is the typical growth process for galaxies over time; ultimately, no surrounding galaxies can merge without reaching significant mass increases.

The Cosmic Horseshoe has reached this advanced stage, existing within a bubble of relatively few bright galaxies nearby.

“This discovery provides a unique insight into the culmination of galaxy and black hole formation,” Mello stated. “By examining this system, we can enhance our understanding of how other galaxies and their ultra-massive black holes evolve over cosmic time.”

About Our Experts

Carlos Mello is a doctoral student at a Federal University in Brazil.

Read more:

Source: www.sciencefocus.com

Astrophysicists Identify Gravitational Waves from the Largest Black Hole Mergers Recorded to Date

The twin detectors of the NSF’s Laser Interferometer Gravitational-Wave Observatory (LIGO) have made a groundbreaking discovery by detecting the highest composite mass recorded to date and the merger of two black holes. This event, identified as GW231123 and discovered on November 23, 2023, produced a final black hole with a mass over 225 times that of the Sun.



GW231123 An infographic detailing the merger of black holes. Image credits: Simona J. Miller/Caltech.

LIGO made history in 2015 with the first direct detection of gravitational waves, the ripples in spacetime.

In that instance, the waves were generated by the merger of black holes, culminating in a black hole with a mass 62 times that of our Sun.

The signal was simultaneously detected by LIGO’s twin detectors located in Livingston, Louisiana, and Hanford, Washington.

Since then, the LIGO team has collaborated with partners from Italy’s Virgo detectors and Japan’s KAGRA to create the LVK collaboration.

These detectors have collectively observed over 200 black hole mergers during their fourth observational run since starting in 2015.

Previously, the largest black hole merger recorded was in 2021 during the event GW190521, which had a total mass of 140 times that of the Sun.

During the GW231123 event, a black hole with a mass of 225 was formed by merging two black holes, one approximately 100 times and the other 140 times the mass of the Sun.

This discovery places it in a rare category known as intermediate mass black holes, which are heavier than those resulting from star collapses but significantly lighter than the supermassive black holes found at the centers of galaxies.

In addition to their substantial mass, these merged black holes exhibited rapid rotation.

“This is the largest black hole binary we’ve observed in gravitational waves and poses a significant challenge to our understanding of black hole formation,” stated Dr. Mark Hannam, an astrophysicist at Cardiff University and a member of the LVK collaboration.

“The existence of such a large black hole defies standard stellar evolution models.”

“One potential explanation is that the two black holes in this binary could have formed from the merger of smaller black holes.”

“This observation highlights how gravitational waves uniquely uncover the fundamental and exotic properties of black holes throughout the universe,” remarked Dr. Dave Reitze, executive director of LIGO at Caltech.

Researchers announced this week the discovery of GW231123, which will be discussed at the 24th International Conference on General Relativity and Gravity (GR24) and the 16th Edoardo Amaldi Meeting on Gravitational Waves, held jointly at the Gr-Amaldi Meeting in Glasgow, Scotland.

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LIGO-Virgo-KAGRA Collaboration. GW231123: The largest black hole binary detected by gravitational waves. Gr-Amaldi 2025

Source: www.sci.news

VLT Unveils the Most Detailed Image of NGC 253 to Date

Astronomers utilizing the Multi-unit Spectroscopic Explorer (Muse) on ESO’s Very Large Telescope (VLT) captured an active starburst galaxy, NGC 253, in thousands of colors simultaneously.



This VLT/Muse image displays a detailed multi-colored view of NGC 253. Image credit: ESO/Congiu et al.

NGC 253 lies approximately 11.5 million light-years away in the Sculptor constellation.

Commonly referred to as the Silver Coin, Silver Dollar Galaxy, or Sculptor Galaxy, this galaxy was discovered on September 23, 1783, by Caroline Herschel, the sister of William Herschel.

It is one of the brightest members of the Sculptor group of galaxies.

Characterized as a starburst galaxy, it experiences unusually rapid star formation and stellar explosions.

“NGC 253 is one of the largest star-forming galaxies near the Milky Way,” noted ESO astronomer Enrico Kong and his team.

“It also ranks among the largest galaxies in the sky, with apparent dimensions of 42 x 12 arcminutes2.

“With its distinct stellar bars, well-defined spiral arms, and widespread star formation, NGC 253 exemplifies a classic spiral galaxy near the main sequence.”

To create a new image of the galaxy, astronomers dedicated over 50 hours observing it with the VLT’s Muse Instrument.

They needed to stitch together more than 100 exposures to encapsulate an area of approximately 65,000 light-years.

“You can focus on individual regions where stars form at a scale of individual stars, or you can zoom out to view the entire galaxy,” explained Dr. Kathryn Kreckel, an astronomer at the University of Heidelberg.

In their initial data analysis, researchers identified 500 planetary nebulae and regions of gas and dust within NGC 253.

“In areas outside our galaxy, we typically find fewer than 100 detections per galaxy,” remarked Fabian Schuerman, a doctoral student at Heidelberg University.

“Due to the properties of planetary nebulae, they serve as distance markers for host galaxies.”

“By locating the planetary nebulae, we can confirm the distance to the galaxy, which is crucial for other galaxy research.”

“Future projects utilizing maps will investigate gas flows and how their composition influences star formation across this galaxy.”

“It remains a mystery why such a minor process can significantly influence galaxies that are thousands of times larger,” stated Dr. Kong.

The results will be published in the journal Astronomy and Astrophysics.

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E. Congiu et al. 2025. Sculptor’s Muse View of the Galaxy: Overview of the Survey and the Planetary Nebula Luminosity Function. A&A in print;

Source: www.sci.news

Remember the tip and boost your chances with Driver Res Taxi for work or a date

name: Waymo.

year: It was founded in 2009 as a Google Autonomous Car Project.

exterior: Unmanned taxis and recruitment services.

What a futuristic – And have they been working on this since 2009? In fact, it is a prototype self-driving car built by Stanford University, dating back to 2004. The Google Project became known as Waymo in 2016.

Have you been thinking about it for so many years before you first saw the self-driving taxi? They already have them in San Francisco, LA, and Phoenix.

Does that mean they are testing technology on real roads? No, I mean you can get a Waymo to take you somewhere in San Francisco now…

That’s a miracle! … and perhaps provide you with work while you’re there.

That’s the service now. How does the technology behind adoption work at the end of this whole end? That’s amazing. That’s amazing. Those on Waymo left handwritten notes promoting senior software engineers “to tackle AI/Music Project.”

Do you think people who enter unmanned taxis are exactly like the devil’s May care nerd they were looking for? that’s right.

Did it work? The person who left the note, flu CEO Alessandra Angelini, says he received around 60 CVs as a result.

I’m amazed that 60 qualified applicants had entered the same Waymo that day. That’s statistically unlikely, but the taxi hire took photos of the notes and posted them on social media, where they saw them 300,000 times.

That’s how it works. It’s not just the advantages of driverless technology. Another rider left a note to Waymo looking for the date, listing his age (26), his height (5 feet 10 inches on a good day), other details (“run marathon”), and phone number.

did that work? He got 200 replies, but again, because someone else posted a photo on social media.

This new recruiting system appears to be quite dependent on third parties. X account. Also, taxis are cleaned quite regularly, so ads don’t last long.

Will the novelty of this approach be exhausted when driverless taxis become commonplace? probably. This means that it won’t respond to ads for dates someone left with Uber.

say: “Enjoy your ride and thank you for your application!”

Don’t say: “I wanted a driver.”

Source: www.theguardian.com

Gaia Announces Most Detailed Map of Milky Way to Date, Achieves Skyscan Milestone in Mission

Released on December 19, 2013, ESA's star mapping satellite “Gaia” We are now nearing the sky, but this does not mean the mission is complete. Technical tests are scheduled in the weeks before Gaia moves into its “retirement” orbit, with two major data releases scheduled for around 2026 and the end of the century, respectively.

An artist's impression of the Milky Way galaxy based on data from ESA's Gaia Space Telescope. Image credit: ESA / Gaia / DPAC / Stefan Payne-Wardenaar.

ESA Director of Science Carol Mandel said: “Today, as the science observations conclude, we celebrate this amazing mission that has exceeded all our expectations, extending almost twice its original predicted lifetime.” said.

“The treasure trove of data collected by Gaia has given us unique insight into the origin and evolution of the Milky Way galaxy, and has also provided insight into astrophysics and the solar system in ways we still don't fully understand. It transformed science.”

“Gaia is built on Europe’s unique excellence in astronomical measurements and will leave a lasting legacy for future generations.”

“After 11 years in space, surviving micrometeorite impacts and solar storms along the way, Gaia has completed collecting scientific data,” said Gaia project scientist Johannes Sahlmann.

“All eyes are now on preparing for the next data release.”

“We are excited to carry out this incredible mission and are excited about the discoveries that await us.”

An annotated artist's impression of the Milky Way galaxy, based on data from ESA's Gaia Space Telescope. Image credit: ESA / Gaia / DPAC / Stefan Payne-Wardenaar.

Gaia has used the three instruments many times over the course of its mission to observe and chart the stars' positions, distances, movements, changes in brightness, compositions, and numerous other characteristics.

This will allow Gaia to achieve its primary goal of building the largest and most accurate map of the Milky Way, displaying our home galaxy like no other mission has been able to achieve to date. is completed.

“Gaia has changed our impression of the Milky Way, so it contains major changes from previous models,” said Stefan Payne Waldenaar, a science visualizer at the House of Astronomy and the IAU Directorate of Astronomy Education. said.

“Even basic ideas such as the rotation of the galaxy's central bar, the distortion of the disk, the detailed structure of the spiral arms, and the interstellar dust near the sun have been revised.”

“Still, we are still speculating about the distant parts of the Milky Way based on incomplete data.”

“As more Gaia data is released, our view of the Milky Way will become even more accurate.”

Gaia's science and engineering teams are already hard at work preparing for Gaia Data Release 4 (DR4), scheduled for 2026.

The amount and quality of data is increasing with each release, and Gaia DR4, with an expected 500 TB data product, is no exception.

Additionally, it will cover the first 5.5 years of the mission, which is the length of the mission as originally planned.

“This is the release of Gaia that the community has been waiting for, but it's exciting considering it only covers half of the data collected,” said Dr. Antonella Valenari, an astronomer at the National Institute of Astronomical Sciences. Ta.

“Although the mission is currently suspending data collection, it will be business as usual for many years to come as we continue to make these impressive datasets available.”

Over the past decade, Gaia has accumulated more than 3 trillion observations of nearly 2 billion stars and other astronomical objects, revolutionizing the way we see our home galaxy and neighboring universe, and advancing its mission. You have completed the empty scan stage. Image credit: ESA / Gaia / DPAC / Stefan Payne-Wardenaar.

After several weeks of testing, Gaia will leave its current orbit around Lagrangian Point 2, 1.5 million km from Earth, away from the Sun and be placed into a final heliocentric orbit far from Earth's sphere of influence. .

The spacecraft is scheduled to be passivated on March 27, 2025 to avoid harm or interference with other spacecraft.

During the technical test, Gaia's orientation is changed, temporarily making it several orders of magnitude brighter and making it much easier to observe with small telescopes.

Gaia mission manager Uwe Lammers said: “Gaia will shine among the stars before her sad retirement and will treat us with this final gift to bid her farewell.”

“This is a moment to celebrate this transformative mission and to thank all the teams who have worked hard for more than a decade to operate Gaia, plan observations, and ensure the smooth return of valuable data to Earth.”

Source: www.sci.news

Exciting Upcoming Games of 2025: Mark Your Calendars for Date Everything!

LLots of great stuff, date them all! It started as a joke. Envisioning a game in which a lonely remote worker starts chatting to furniture, Final Fantasy voice actors Ray Chase and Robbie Daymond immediately fell in love with the concept. What would happen if it really happened? It was A game where you can date literally anything?

A bizarre game of banging home appliances that boasts over 70,000 lines of dialogue and 100 dateable inanimate objects has become a reality. Working with Team 17 and fellow voice actress and producer Amanda Hufford, they brought their ridiculous concept to life, resulting in a game they describe as wholesome, frivolous, and fun.

You may be wondering how this works. Now, when players don Dateviators (VR glasses that turn inanimate household objects into talkable, dateable beings), inanimate furniture and appliances suddenly become very chatty, and within seconds I'm talking about a dishwasher and Start flirting.

“We knew we wanted to make sure it felt wholesome, that it was sexy, but in no way vulgar,” says Robbie Daymond. “Our mantra is that we want to create something that people won't feel embarrassed about if they come in. We're playing around with that.”

From tables and microwaves to fireplaces and televisions, there are “characters” you can write dates on, and each potential lover is brought to life by a different voice actor. Every appliance is decidedly and endearingly weird, from a surprisingly liberating microwave that makes you think you're fighting an interdimensional war to a gushing frat-boy fireplace dubbed “The Art of the Pick-Up Line.” is.




No need to be shy…date everything! Photo: Sassy Chap Games

They're also taking a different approach to paying actors fairly. “One of the superpowers we have is that we know a lot of people in the industry,” Daymond says. “We have a good relationship with [actors union] SAG and we were able to work out a deal that would give back the balance to the actors who worked on it. Thanks to a combination of clever scripting by TV writer Logan Burdick and great voice acting throughout, even my short demo gives me the following endearing freedom to see what happens next. I felt I had to meet a new appliance.

Although it sounds like a product of the pandemic, the premise of Date Everything was actually born in 2018 when Draymond wondered if anyone could empathize with the boredom and social deprivation of remote work. . “I’m really excited that something so surreal exists,” Burdick reflects. “I think it’s unbelievable that everyone got a chance.”

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“I was a little skeptical when I started working with the team,” exclaims Jack, the game's quiet programmer. “But I was really impressed when I actually played it and saw how much care and attention was put into each character. A lot of games do primarily the same thing in slightly different ways. It's not a typical game, and that's very important today.”

Date Everything will be released on PC, Nintendo Switch, PlayStation 5, and Xbox on February 14th

Source: www.theguardian.com

Scientists create the tiniest walking robot to date

A team of researchers at Cornell University has created a new class of magnetically controlled microscopic robots (microbots) that operate at the diffraction limit of visible light. These microbots, called diffractive robots, can interact with visible light waves and yet move independently, allowing them to move to specific locations, take images, and measure forces at the scale of the body’s smallest structures. You can.

Diffraction robot. Image credit: Smart others., doi: 10.1126/science.adr2177.

Diffractive robotics connects untethered robots with imaging techniques that rely on visible light diffraction (the bending of light waves as they pass through an aperture or around something).

Imaging techniques require an aperture with a size comparable to the wavelength of light.

For the optics to work, the robot must be at that scale, and for the robot to reach the target it is imaging, it must be able to move on its own.

The robot is controlled by a magnet that performs a pinching motion, allowing it to move inchworm-like across solid surfaces. The same motion can also be used to “swim” through a fluid.

The combination of maneuverability, flexibility, and sub-diffractive optical technology represents a major advance in the field of robotics.

“A walking robot that is small enough to interact with light and effectively shape it would place a microscope lens directly into the microworld,” said Paul McEwen, a professor at Cornell University.

“We can perform close-up imaging in a way that would never be possible with a regular microscope.”

“These robots are 2 to 5 microns in size. They're tiny. And by controlling the magnetic fields that drive their movement, we can make them do whatever we want them to do.”

“I'm really excited about the fusion of microrobotics and micro-optics,” said Dr. Francesco Monticone of Cornell University.

“The miniaturization of robotics has finally reached a stage where these actuated mechanical systems can interact with and actively shape light on the scale of just a few wavelengths (one millionth of a meter). I did.”

To magnetically drive a robot at this scale, the research team used hundreds of nanometer-scale magnets with two different shapes, long and thin or short and stubby, with the same volume of material to drive the robot. I made it into a pattern.

Professor Itai Cohen of Cornell University says, “Long, thin objects require a larger magnetic field to switch from pointing in one direction to pointing in another direction, whereas short, stubby objects require a larger magnetic field to switch from pointing in one direction to pointing in another direction.'' “Things require smaller magnetic fields.”

“So if you apply a large magnetic field, you can align them all, but if you apply a smaller field, only the short and thick ones will flip.”

To create the robot, the authors combined this principle with a very thin film.

“One of the main challenges for optical engineering was to find the best approach for the three tasks (light conditioning, focusing, and super-resolution imaging) for this particular platform, because “different approaches “There are different performance trade-offs depending on how the microrobots behave,” said Dr. Monticone. “They can move and change shape.”

“There are advantages to being able to mechanically move the diffractive elements to enhance imaging,” Professor Cohen says.

The robot itself can be used as a diffractive grader or a diffractive lens can be added. In this way, the robot can act as a local extension of the microscope lens looking down from above.

The robot measures force using the same magnet-driven pinching motions used to push structures while walking.

“These robots are very compliant springs, so if something pushes on them, it can squeeze them,” Professor Cohen said.

“That changes the diffraction pattern and allows us to measure it very well.”

Force measurements and optical capabilities can be applied to basic research such as exploring the structure of DNA. Or it may be introduced into clinical practice.

“Looking to the future, we can imagine swarms of diffractive microbots walking along the surface of samples to perform super-resolution microscopy and other sensing tasks,” Professor Monticone said.

“I think we have just scratched the surface of what is possible with this new paradigm of combining robotics and optics at the microscale.”

of study Published in a magazine science.

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Conrad L. Smart others. 2024. Magnetically programmed diffractive robotics. science 386 (6725): 1031-1037;doi: 10.1126/science.adr2177

Source: www.sci.news

The South American lungfish has the largest genome ever sequenced to date.

Researchers from the University of Konstanz and other institutions Africa(Protopterus annectens) and South American lungfish (Lepidosiren paradoxa)The genome of the South American lungfish (approximately 91 gigabases, about 30 times the size of the human genome) is the largest animal genome sequenced to date. Australia(Neoceratodus forsteri) African lungfish.

South American lungfish (Lepidosiren paradoxaImage courtesy of Katherine Seghers, Louisiana State University.

Lungfish are freshwater vertebrates belonging to the order Dipnoi (Pulmonaceae) and have existed for 400 million years, from the Devonian to the present day.

Some people consider lungfish to be “living fossils” because their morphology has changed very little over the years.

They, like all terrestrial vertebrates, have the ability to breathe air through lungs similar to our own.

Only six species of lungfish remain today: four live in Africa, one in South America, and one in Australia.

“These ancient 'living fossils' still resemble their ancestors so closely that they seem to have been forgotten during evolution,” said biologist Axel Meyer of the University of Konstanz and his colleagues.

“Since our genetic material, DNA, is made up of nucleobases and the sequence of these nucleobases contains the actual genetic information, a comparative analysis of the lungfish genome will only be possible if we know its complete sequence.”

“We already knew that the lungfish genome was large, but until now it was unclear how large it really was and what we could learn from it,” the researchers added.

“Sequencing the lungfish genome has therefore been very labor-intensive and complex, both from a technical and bioinformatics point of view.”

In a new study, scientists have sequenced the genome of African and South American lungfish.

“The South American species' DNA is 91 gigabases (or 91 billion bases), the largest of any animal genome and more than twice the size of the genome of the previous record holder, the Australian lungfish,” Dr Meyer said.

“Eighteen of the South American lungfish's 19 chromosomes are each larger than the entire human genome, about 3 billion base pairs in length.”

The largest genome sequence to date, that of the Australian lungfish, was also sequenced by the same team.

“Autonomous transposons are responsible for the large size of the lungfish genome over time,” the authors write.

“These are DNA sequences that are 'replicated' and change position in the genome, which causes the genome to grow.”

“Although similar phenomena have occurred in other organisms, our analysis shows that the South American lungfish has by far the fastest rate of genome expansion ever recorded; every 10 million years, its genome has expanded to a size equivalent to the entire human genome.”

“And it continues to grow. We now have evidence that the transposon responsible is still active.”

“We have identified a mechanism for this enormous genome growth. This extreme expansion is due, at least in part, to the very low presence of piRNAs.”

“This type of RNA is normally part of the molecular mechanism that silences transposons.”

Team paper Published in the journal Nature.

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M. Chartres othersAll lungfish genomes provide information on genome expansion and tetrapod evolution. NaturePublished online August 14, 2024, doi: 10.1038/s41586-024-07830-1

Source: www.sci.news

Physicists may have discovered a method to create element 120, the most massive element to date.

Jacqueline Gates of Lawrence Berkeley National Laboratory isolating livermorium atoms.

Marilyn Sargent/Berkeley Lab 2024 Regents of the University of California

The third heaviest element in the universe has been created in a way that points the way to synthesizing the elusive element 120, the heaviest element in the periodic table.

“We were very shocked, very surprised and very relieved that we had not made the wrong choice in installing the equipment,” he said. Jacqueline Gates At the Lawrence Berkeley National Laboratory (LBNL), California.

She and her colleagues created the element, livermorium, by bombarding pieces of plutonium with beams of charged titanium atoms. Titanium has never been used in such experiments before because it’s hard to turn into a well-controlled beam and it takes millions or trillions of collisions to create just a few new atoms. But physicists think that the titanium beam is essential to making a hypothetical element 120, also known as unbinylium, which has 120 protons in its nucleus.

The researchers first evaporated a rare isotope of titanium in a special oven at 1,650°C (about 3,000°F). They then used microwaves to turn the hot titanium vapor into a charged beam, which they sent into a particle accelerator. When the beam reached about 10% of the speed of light and smashed into a plutonium target, a fragment of it hit a detector, where it detected a trace of two livermorium atoms.

As expected, each atom rapidly decayed into other elements. The stability of an atomic nucleus decreases as an atom’s mass increases. But the measurements were so precise that there’s only about a one in a trillion chance that the discovery was a statistical fluke, Gates says. The researchers announced their findings on July 23. Nuclear Structure 2024 Meeting at Argonne National Laboratory, Illinois.

Michael Thornessen The Michigan State University researcher says the experiment supports the feasibility of creating element 120. “We have to do the basic research and we have to go in the dark, so this is a really important and necessary experiment in that sense,” he says.

Toennesen says the creation of unbinylium will have profound implications for our understanding of the strong force, which determines whether heavy elements are stable. Studying unbinylium may also help us understand how exotic elements formed in the early universe.

The heaviest artificial element to date, element 118 (also known as oganesson), has two more protons than livermorium and was first synthesized in 2002. Since then, researchers have struggled to make atoms even heavier, because that requires colliding already-heavy elements with each other, which themselves tend to be unstable. “It’s really, really difficult work,” Thornesen says.

But the new experiment has LBNL researchers feeling optimistic: They plan to launch experiments aimed at creating element 120 in 2025 after replacing the plutonium target with the heavier element californium.

“I think we’re pretty close to knowing what to do,” Gates says, “and we have an opportunity to add new elements to the periodic table.” [is exciting]”…Very few people get that opportunity.”

topic:

  • Chemical /
  • Nuclear Physics

Source: www.newscientist.com

What is the date of the summer solstice in 2024 and what leads to the longest day of the year?

As we welcome summer, the Northern Hemisphere is now experiencing longer daylight hours due to the 2024 summer solstice. This day has been celebrated for millennia, whether for religious reasons or simple festivities like barbecues. If you’re curious about the significance of this day, particularly at sites like Stonehenge, we have information to share.

When is the summer solstice in 2024?

The summer solstice in 2024 will occur on Thursday, June 20th at 9:51pm BST (4:50pm EDT New York time, 1:50pm PDT Los Angeles time). This precise astronomical moment marks the start of summer in the Northern Hemisphere when it faces the sun directly, resulting in the longest day of the year with the most hours of sunshine.


When are sunrise and sunset on the summer solstice?

On Thursday, June 20th, sunrise in London is at 4:43am BST, and sunset is at 9:21pm BST. Timings vary slightly depending on the location within the UK and the US.

  • Summer solstice sunrise times in New York City: 5:25 a.m. EDT.
  • Summer solstice sunset times in New York City: 8:31pm EDT.
  • Summer solstice sunrise times in Austin, Texas: 6:30 a.m. CDT.
  • Summer solstice sunset times in Austin, Texas: 8:36pm CDT.
  • Summer solstice sunrise times in Los Angeles: 5:42 a.m. PDT.
  • Summer solstice sunset times in Los Angeles: 8:08pm PDT.

Although the summer solstice is the longest day, it does not always have the earliest sunrise or latest sunset, which vary based on the latitude.

What is the Summer Solstice?

The summer solstice represents the moment when the Northern Hemisphere is most tilted towards the sun, resulting in the longest day of the year. This tilt of the Earth’s axis causes different seasons in the hemispheres, with the summer solstice marking peak summer in the Northern Hemisphere and peak winter in the Southern Hemisphere.

Due to the Earth’s tilt, sunlight falls directly on the Northern Hemisphere during the summer solstice. In the Southern Hemisphere, this marks the shortest day of the year, or winter solstice. – Image credit: Getty

Various celebrations of the summer solstice take place globally, with Stonehenge being a famous site for observing this phenomenon. People have gathered at this ancient stone circle to witness the sunrise aligning with the central altar stone, marking the arrival of summer.

Starting in the late Middle Ages, Swedes began the tradition of erecting a Midsummer pole and dancing around it. The custom of decorating the pole with flowers and greenery was called a “maja”, which also came to be called a Maypole. – Image credit: Getty

What is the difference between the equinox and the summer solstice?

While equinoxes mark the change of seasons when day and night are approximately equal, solstices like the summer solstice focus on sunlight. The summer solstice in the Northern Hemisphere is the longest day of the year, contrasting with the winter solstice, which is the shortest day.

Do other planets have solstices?

Every planet in the solar system experiences solstices due to its axial tilt, with Earth’s tilt being more noticeable than other planets like Venus or Jupiter. The tilt of a planet’s axis affects its seasons, with Uranus being particularly tilted and experiencing extreme variations in sunlight.

Upcoming Summer Solstice Dates and Times, BST

  • 2025: June 21, 3:42 AM
  • 2026: June 21, 9:24 AM
  • 2027: June 21, 3:10 p.m.
  • 2028: June 20, 9:01 p.m.
  • 2029: June 21, 2:48 AM
  • 2030: June 21, 8:31 AM

About our experts

Darren Baskill is an Outreach Officer and Lecturer in the School of Physics and Astronomy at the University of Sussex. She has a background in astrophotography and astronomy, bringing expertise to the study of celestial events like the summer solstice.


Source: www.sciencefocus.com

Tomorrow’s SpaceX Live Stream: Starship Launch 4 Date, Time, and Viewing Information

SpaceX’s giant Starship rocket was deployed on the launch pad at StarBase, the company’s facility in South Texas, in June 2024 ahead of a planned test flight.

SpaceX is getting ready Starship. The most powerful rocket ever built is gearing up for its next test launch. Here’s everything you need to know.

What time is the launch scheduled?

The launch is expected to take place in the next week or so, but SpaceX has said it could take place as soon as June 5, pending regulatory approval. Each flight must be approved by the US Federal Aviation Administration.

Other signs point to the same day. Judge Eddie Trevino of Cameron County, Texas, home to SpaceX’s Starbase launch site, said: Nearby roads are closed. It will be carried out at the beginning of June. This precautionary measure is usually taken during launches, but it may also be relevant for some of the ground tests.

However, Treviño explicitly states in official documents that these closures are for “flight testing,” and establishes a 14-hour closure period from midnight to 2 p.m. local time on June 5. The documents also state that alternative closures of the same duration could be scheduled on June 6 and 7, if the company so desires.

How can I watch the Starship launch?

SpaceX has announced that a live webcast will begin approximately 30 minutes before launch.

Where is Starship going?

The fourth test flight will focus on returning Starship from orbit and conducting a mock landing of both the Starship and the Super Heavy first stage booster. Because landings on ground are currently deemed too risky, both vehicles will make a “soft splashdown” in the ocean, using their engines to slow their descent and line up, as if they were landing on a base, to gently touch down on the water. The first stage booster is scheduled to splash down in the Gulf of Mexico, not far from the launch site, about seven minutes after liftoff, while Starship aims to splash down in the Indian Ocean about an hour later.

What has happened in Starship launches so far?

All three Starship launches have ended in explosions, which was expected as part of SpaceX’s “fail fast, learn fast” strategy.

During the first launch on April 20 last year, three of the first stage’s three engines (out of a total of 33) failed to ignite. Several more subsequently failed during the flight. The rocket then spun out of control and its self-destruct safety mechanism was activated. The entire flight lasted about three minutes, reaching a maximum altitude of 39 kilometers.

Starship’s second launch was on November 18. This time, all 33 engines were working, and the rocket flew far enough for the first and second stages to separate. But as the first stage rotated to begin its deceleration and landing procedure, it exploded. The second stage continued on smoothly to an altitude of about 90 miles, passing the Kármán line, which marks the beginning of the universe. But it was destroyed by a safety device after it stopped transmitting data before completing an orbit or returning to Earth.

SpaceX’s third Starship test flight, on March 14, was at least partially successful, as it reached space, performed a fuel transfer test, and flew farther and faster than ever before. However, it lost attitude control during the flight and failed to make the planned soft landing. Nevertheless, it achieved several important milestones, including Starship’s first atmospheric reentry from space, the first opening and closing of Starship’s payload door in space, and a successful demonstration of fuel transfer, which is key for future NASA Artemis missions to the Moon.

What would happen if this launch were to fail?

The chances of Starship completing its mission perfectly are slim, so it’s likely to fail in some way. But failure will provide data and experience that can be used to improve the design and process for the fifth launch. SpaceX has shown it can iterate quickly and make great strides with each launch.

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Source: www.newscientist.com

Top 17 Mind-Blowing Science Experiments of the Year (To Date)

The Swiss National Science Foundation (SNSF) has announced the winners of this year’s Scientific Image Competition, which celebrates the hidden beauty of scientific research.

The contest is divided into four categories: “Subjects of Research,” “Locations and Equipment,” “Women and Men Scientists,” and “Video Loops.”

The winning entries include an image of the transparent abdomen of a glass frog taken by Francesca Angiolani-Larrea, a doctoral student at the University of Bern, who won first place in the “Research Subject” category.

Check out the winners and standout images from this year’s contest.

Distinguishing between locations and instrument categories – organized chaos

This operating room image was taken before pig surgery began. The purpose of this surgery was to evaluate the in vivo performance of a new vascular graft for aortic replacement. This treatment has the potential to improve patients’ life expectancy and quality of life after intervention. Photo credit: Georgios Lovas

Distinguishing research target categories – maize root microbiome

This image visualizes the corn root microbiome (the collection of microorganisms that live in or on the roots) and how they process the plant’s secondary metabolites. Photo credit: Lisa Tennen

Winners in the Research Subject Category – In Search of a Good Father

This image shows Hyalinobtrachium valerioi, a type of glass frog with a transparent stomach. Although child rearing in the animal kingdom has traditionally been seen as the job of the mother, it takes on a more diverse form in amphibians. This species is a good example. The female’s role is to select the best mate and lay eggs. Males stay close to their children and take care of them. Sometimes they hold up to seven animals at once. Photo credit: Francesca Angiolani-Larrea

Differentiating between video loop categories – Smapshot

“Smapshot” is a crowdsourcing project that allows citizens to localize historical photos using a virtual globe. Participants can georeference the image by clicking on points that appear within the image and on the virtual globe. Georeferenced images are of interest to researchers and the general public because they help visualize phenomena such as climate change and urbanization. Video stills by Jens Ingensand

Video Loop Categories Distinction – Tumor Cells…

A still image from a video showing how tumor cells extracted from patient tissue grow within a three-dimensional matrix. Video stills by Michele Gallioni

Male and female science winners – more than just wearing lab coats

In this photo, a veterinarian is auscultating a mini pig’s heart to make sure it’s healthy. Photo credit: Mariafrancesca Petrucci

Winner of the Video Loop Category – Wingtip vortex…

This shows the flow pattern in a wind tunnel test section that occurs downstream of an aircraft arched wing located near a solid surface. In classic flight conditions, high above the ground, a single vortex develops at the wing tip. In this case, a complex spiral system is seen. Video stills by Cyprien de Sepibus

Distinguishing research subject categories – Cerebrospinal fluid…

This supercomputing simulation shows how cerebrospinal fluid flows around the optic nerve. Cerebrospinal fluid flows from the brain to the optic nerve, nourishing it and removing toxic metabolites. Photos by Diego Rossinelli, Jatta Berberat, Jill Forsti

Location and Equipment Winner – Bees and Chips

This photo shows a close-up of a robotic device inhabited by bees, developed within the Mobile Robot Systems Group at the Swiss Federal Institute of Technology Lausanne (EPFL). Trials were being carried out in Austria in collaboration with biologists from the University of Graz as part of the EU-funded Hiveopolis project. Photo credit: Raphael Balmak

Scientists Women and Men by Category – Wheat Harvest

Hundreds of research wheat fields must be threshed to study crop growth using sensors and high-tech equipment. This includes manual labor such as bagging and collecting seed samples for drying and further processing. Photo credit: Andreas Hund

Distinguishing between locations and equipment categories – UV reactors…

The photo shows the UV reactor used for photopolymerization. Photopolymerization is a process in which light induces the chemical assembly of short monomer molecules to form long polymer chains. The reactor is built with a 5-meter strip containing 300 LEDs wrapped inside an aluminum cylinder. Photo credit: Deborah Toney

Distinguishing women from men in science – the big stakes in the history of medicine

This photo was taken at the historic library and museum of the Saint-Louis Hospital in Paris, France. It has a collection of books on the history of medicine and dermatology, many of which are out of print and extremely rare. Photo by Alexandre Wenger and Radu Suciu

Video loop category differentiation – tumor growth simulation

This computer simulation shows how a malignant tumor grows from a single cell to a million cells. Each cell is colored according to its relative age, from red (young) to blue (old). Video stills by Roman Vetter

Classification of research subject categories – My voice in the video…

My Voice in Images is a photo-based participatory research method that gives children and young people the opportunity to express their views on social issues and public policies that interest them. The children who created this photo emphasized the need for a solid roof over their heads. Photo by Sylvia Garcia Delahaye and Lavinia Johnson.

Distinguishing between locations and instrument categories – Wandering eye

An ophthalmic microsurgeon practices surgical techniques for artificial eyes. The development of educational materials aims to create realistic conditions for surgical training workshops before it is possible to safely operate on live patients. Photo credit: Julien Boussette

Distinguishing research object categories – thin layer chromatography plates…

Thin layer chromatography plates in fluorescent dye synthesis. Chromatography is a technique for spatially separating the components of a mixture. This example image was generated during the purification of a complex fluorochrome, or fluorescent compound. Photo credit: Salome Puntenar

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Source: www.sciencefocus.com

Microsoft and Quantinuum’s quantum computer could be the most dependable to date

Quantinuum H2 chip

Quantinum

Microsoft and quantum computing company Quantinuum claim to have developed a quantum computer with unprecedented levels of reliability. The ability to correct its own errors could be a step toward more practical quantum computers in the near future.

“What we did here gave me goosebumps. We showed that error correction is reproducible, works, and is reliable.” Krista Svoir At Microsoft.

Experts have long expected the arrival of practical quantum computers that can complete calculations too complex for traditional computers. Although quantum computers have steadily grown larger and more complex, this prediction has not yet been fully realized. One big reason for this is that all modern quantum computers are subject to errors, and researchers have found that it is technically difficult to implement algorithms to detect and correct errors during calculations. That’s it.

The new experiment could be an important step toward overcoming this error problem. The researchers say that on his H2 quantum processor at Quantinuum, he ran more than 14,000 individual calculation routines without making a single error.

Errors occur even in classical computers, but error correction can be coded into programs by creating backup copies of the information being processed. This approach is not possible with quantum computing because quantum information cannot be copied. Instead, researchers distributed it across a group of connected qubits, or qubits, creating what are known as logical qubits. Microsoft and the Quantinuum team created four of these logical qubits using 30 qubits.

Svore said a process developed by Microsoft was used to generate these logical qubits, allowing them to run error-free, or fault-tolerant, experiments repeatedly. Typically, individual qubits are easily disturbed, but at the level of logical qubits, researchers were able to repeatedly detect and correct errors.

The approach was so successful, they say, that four logical qubits produced only 0.125 percent of the errors that would occur if 30 qubits were left ungrouped. This means that ungrouped qubits generate as many as 800 errors for every one error generated by a logical qubit.

“Having a logical error rate that is 800 times lower than that of physical qubits is a huge advance in the field and brings us one step closer to fault-tolerant quantum computing,” he said. says. mark suffman from the University of Wisconsin was not involved in the experiment.

jennifer strobley Quantinuum said the team’s hardware is well-suited for new experiments because it provides advanced control over qubits and quantum computers have already achieved some of the lowest error rates ever. .

In 2023, a team of Harvard University researchers and their colleagues, including members of the quantum computing startup QuEra, broke the record for the largest number of logical qubits at once, 48. This is much more than his four logical qubits in the new device. But Strabley said the new device requires fewer physical qubits for each logical qubit, and the logical qubits have fewer errors than the one built by the Harvard team. “We used significantly fewer physical qubits and got better results,” she says.

However, some experts new scientist Without details about the experiment, researchers were not yet ready to qualify this new research as a breakthrough in quantum error correction.

It is generally believed that only quantum computers with more than 100 logical qubits can actually tackle scientifically and socially relevant problems in fields such as chemistry and materials science. The next challenge is to make everything bigger. Strabley and Svore say they are confident that the long-standing collaboration between Microsoft and Quantinuum will soon come to fruition.

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Source: www.newscientist.com

The Bitcoin Halving: Date and Significance Explained

Bitcoin price volatility appears to be decreasing

Pedrošek/Shutterstock

What is Bitcoin halving?

Bitcoin is a digital currency that operates freely from central control. Rather than an authority like a bank or government tracking who owns what, Bitcoin relies on encryption.

So-called miners collect information about transactions and record them on a ledger called a blockchain. These miners perform a huge number of calculations with the aim of completing cryptographic problems, 0.69% of the world's electricity in the process. The first miner to solve this problem adds a collection (block) of transaction data to the blockchain.

You will also be rewarded with a certain amount of newly created Bitcoins. Bitcoin is built into the source code that writes and runs the network. Every 210,000 blocks, an event called a halving occurs where the size of the reward is reduced by 50%. This is intended to avoid inflation due to too many coins being created.

The first block ever mined gave a reward of 50 coins, which is now down to 6.25 coins after three halvings. The last halving was in May 2020.

When is the next Bitcoin halving?

The next Bitcoin halving is expected to occur around April 19th, reducing miners' rewards to 3.125 coins. The reward continues to decrease and disappears completely around 2140 after 21 million coins have been created. At that point, there are no new coins.

Why is it important?

For those who use Bitcoin to purchase goods and services or hold Bitcoin as an investment, nothing changes. The current Bitcoin pool will remain. However, for miners, the value of the rewards they receive will be significantly reduced.

This could lead some miners to close up shop if they decide the effort isn't worth the reward. But the reality is that mining economics are constantly changing, and the industry is likely to adapt and continue as it has always done.

More powerful computers are being created all the time that can perform mining calculations faster, making it easier to mine blocks. However, the feedback mechanism within Bitcoin's code constantly adapts to this by increasing or decreasing the difficulty of calculations depending on the total computer power currently allocated to mining. The purpose of Bitcoin's source code is that a new block is created approximately every 10 minutes, and the network adjusts to speed up or slow down as needed.

When Bitcoin was first launched in 2009, it was possible to mine coins almost instantly with even a basic computer. Nowadays, you need a room filled with powerful equipment, often high-end graphics cards and computationally proficient custom hardware.

What will happen to the price of Bitcoin?

The recent emergence of exchange-traded funds (ETFs), regulated financial products offered by large banks that offer an easier way to invest in Bitcoin, has been long anticipated and was expected to drive up prices. .Some analysts are now estimate Approximately 704,400 coins are already in the hands of the ETF.

There are currently two schools of thought regarding the effect of half-life. Some think the halving will give Bitcoin more impetus, causing the price to rise further, while others think the impact is already priced in. Regulatory approval for Bitcoin ETFs is by no means certain, but the halving is a certainty, so its impact may already be reflected in the price. But it's almost certain that halving won't double the price.

The wild price fluctuations that Bitcoin has experienced over the past few years have become less frequent, and metrics that track volatility seems to be on a downward trend. But at the end of the day, any discussion about Bitcoin's price is just speculation.

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Source: www.newscientist.com

Ancient bone beads discovered in Wyoming date back 12,940 years

Archaeologists have discovered ancient tubular beads made from hare bone at the La Prele mammoth site in Wyoming, USA. This is the oldest bead discovered in the Western Hemisphere.

La Prele bone beads. Polished end (top) and side view with notch (bottom). Image credit: Surovell other., doi: 10.1038/s41598-024-53390-9.

“The manufacture and use of personal ornaments, most commonly beads, is an important indicator of the increasing cultural and social complexity of humans during the Paleolithic period, first appearing in the Middle Stone Age of Africa. It then appeared in the Early Upper Paleolithic of Eurasia,” says the University of Wisconsin. Wyoming Professor Todd Surovell and his colleagues.

“Beads are not well documented from early archaeological contexts in the Americas, but some examples have been reported from Paleoindian regions, where the first immigrants to the Western Hemisphere used beads on their bodies and clothing. It shows that he created and used personal ornaments to decorate his home.”

Archaeologists examined ancient tubular beads from an active area centered around a hearth at the La Prele Mammoth ruins in Converse County, Wyoming, USA.

“The La Prele Mammoth Site is an early Paleoindian site located along La Prele Creek near its confluence with the North Platte River in Converse County, Wyoming,” they said.

“Test excavations in 1987 revealed an association between the chipped stone remains and the partial remains of a subadult.” Colombian mammoth (mammoth colombi)Subsequent excavations revealed that a nearby campsite preserved active areas centered around multiple hearths. ”

“The occupied surface was filled with low-energy dyke deposits, and based on an average of five radiocarbon dates of the bones, occupation occurred 12,941 years ago.”

The length of the beads is small, about 7mm. The inner diameter averages 1.6 mm and the outer diameter averages 2.9 mm.

“Two deep parallel grooves with a U-shaped cross section develop on the surface of the bead aligned perpendicular to the long axis,” the researchers said.

“Similar grooves also occur on Paleolithic and Archaic tubular bone beads, although it is unclear whether these notches are a byproduct of manufacturing, skinning, abrasion, or perhaps decoration. It's very smooth and polished.”

“The beads are lightly coated with red ocher, but the presence of ocher on the surface may be coincidental since they were recovered from a sediment contaminated with powdered hematite.”

To determine the origin of the beads, scientists extracted collagen for zooarchaeology by mass spectrometry, also known as ZooMS. This allowed us to gain insight into the chemical composition of bone.

Researchers believe that the beads are attached to either the metatarsals (the bones that connect the phalanges of the fingers to the more proximal bones of the limbs) or the proximal phalanges (the bones found in the fingers and toes of humans and other vertebrates). I concluded that it was made from either. rabbit.

The discovery provides the first solid evidence of the use of hares in BC. Clovis periodspecifically refers to the prehistoric period of North America, about 12,000 years ago.

“We also considered the possibility that the beads were the result of consumption and digestion by carnivores and were not produced by humans,” the authors said.

“However, carnivores are not common at this site, and the artifacts were recovered one meter away from a densely scattered area of ​​other cultural materials.”

“Additionally, the grooves on the outside of the beads are consistent with those made by humans with stones and teeth.”

“Such beads may have been used to decorate their bodies or clothing.”

of findings It was published in the magazine scientific report.

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TA Slovel other. 2024. Rabbit bones are used to make Clovis beads. science officer 14/2937. doi: 10.1038/s41598-024-53390-9

Source: www.sci.news