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

Hubble Reveals Stunningly Detailed Image of Interstellar Comet 3i/Atlas

Recent analysis of new images from the NASA/ESA Hubble Space Telescope reveals that the nucleus of 3i/Atlas measures between 320 m (1,000 ft) and 5.6 km (3.5 miles).



Hubble captured this image of 3i/Atlas, which was located 446 million km (277 million miles) from Earth on July 21, 2025. Image credits: NASA/ESA/David Jewitt, UCLA/Joseph Depasquale, Stsci.

3i/Atlas was discovered on July 1, 2025, by the Asteroid Land Impact Trastor Alt System (ATLAS) funded by NASA.

Its orbit is the most dynamically extreme among recorded solar system objects.

New observations from Hubble have provided astronomers with a more precise estimation of the comet’s solid icy nucleus size.

“The maximum diameter of the nucleus is 5.6 km, but it averages around 320 m,” stated David Jewitt, an astronomer from UCLA, along with his colleagues.

“Hubble’s images offer tighter constraints on the nucleus’s size compared to earlier ground-based measurements, although the solid core of the comet is not currently visible directly even with Hubble.”

“Data from other NASA missions, like Webb, TESS, Neil Gehrels Swift Observatory, and WM Keck Observatory, will further enhance our understanding of comets, including their chemical composition.”

Hubble also detected indications of dust plumes ejected from the sun-warmed side of the comet, along with dust tails drifting away from the nucleus.

The new findings indicate a dust loss velocity that aligns with the first comet observed at roughly 480 million km (300 million miles) from the Sun.

This behavior closely resembles the characteristics of a previously seen sun-bound comet observed within our solar system.

A notable difference is that this interstellar visitor originates from planetary systems beyond our Milky Way galaxy.

3i/Atlas speeds through the solar system at an astonishing rate of 209,000 km (130,000 miles) per hour, marking the highest speed ever recorded for visitors to our solar system.

This remarkable velocity indicates that comets have been traversing interstellar space for billions of years.

The gravitational pull from countless stars and nebulae has contributed to its increased speed.

The longer 3i/Atlas journeys through space, the faster it moves.

“No one knows the origin of this comet; it’s like catching a glimpse of a bullet for a thousandth of a second,” Dr. Jewitt observed.

“You can’t accurately trace that back to determine where you commenced your path.”

“This latest interstellar traveler represents a previously undetected group of objects, enriching the narrative that has gradually unfolded.”

“This achievement is now possible due to the powerful Sky Survey capability we previously lacked. We’ve reached a new milestone.”

The team’s paper will be published in the Astrophysical Journal Letters.

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David Jewitt et al. 2025. Observations of the Hubble Space Telescope of Interstellar Interloper 3i/Atlas. apjl in press; Arxiv: 2508.02934

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

408 Tentacles: A Detailed Analysis

Dr. Clifford attempted to explain the challenges of owning an octopus in his post. He faced high costs, sleep deprivation, and significant water damage to his home, which necessitated extensive renovations. He mentioned, “I didn’t want to form a permanent or romantic attachment to my baby while still caring for it.”

Despite his efforts, he was inundated with requests to adopt the hatching octopuses.

Vincent Nyman, a wildlife trade expert at Oxford Brooks University, who researched the impact of social media on the exotic pet trade, stated, “If you showcase it, people will want it. And if you advise against getting it, it’s like saying ‘Don’t do this,’ right?”

Nevertheless, Dr. Clifford ultimately decided that he could not send the baby octopuses to private homes. Instead, he arranged for them to be placed in a reputable aquarium or university once they were healthy enough. On April 21st, he made an announcement that he had found homes for all the hatching.

The following day, one of the hatching octopuses, Terrance, passed away and was buried in the backyard beside trees whose trunks resembled octopus tentacles.

Now, the priority was to keep the baby octopuses alive until they could be relocated to their new homes. The odds were stacked against them, as only a small percentage typically survives in the wild.

Dr. Clifford shared that approximately 20 hatching octopuses died within the first month alone, due to factors like cannibalism and power outages.

The pressure to ensure the survival of the baby octopuses weighed heavily on Dr. Clifford, especially with a large and invested audience following his journey.

A local reptile expert and breeder who had become a friend to Dr. Clifford stepped in to help care for and house a baby octopus while Dr. Clifford’s home underwent renovations. Despite their collaborative efforts, the hatching octopuses continued to perish.

Source: www.nytimes.com

Researchers create detailed map of neural connections in mouse brain

The human brain is so complex that the scientific brain has a hard time understanding it. Nerve tissue, the size of a grain of sand, could be packed with hundreds of thousands of cells connected by miles of wiring. In 1979, Nobel Prize-winning scientist Francis Crick concluded that the anatomy and activity of only a cubic millimeter of brain material would forever surpass our understanding.

“It’s useless to seek the impossible,” says Dr. Crick. I wrote it.

46 years later, a team of over 100 scientists achieved that impossible by recording cell activity and mapping the structure of cubic millimeters of the mouse brain. In achieving this feat, they accumulated 1.6 petabytes of data. This is equivalent to 22 years of non-stop high-resolution video.

“This is a milestone,” said Davi Bock, a neuroscientist at the University of Vermont. the studywas published in the journal Nature on Wednesday. Dr. Bock said that it enabled advances that allowed it to cover the cubic bones of the cubic brain to map the entire brain wiring of a mouse.

“It’s completely doable and I think it’s worth doing,” he said.

Over 130 years It has passed since Spanish neuroscientist Santiago Ramon y Kajal first spies on individual neurons under a microscope, creating a unique branching shape. Scientists from subsequent generations have resolved many of the details about how neurons send voltage spikes into long arms called axons. Each axon makes contact with small branches or dendrites of adjacent neurons. Some neurons excite their neighbors and fire their own voltage spikes. Some quiet other neurons.

Human thinking emerges in some way from this combination of excitation and inhibition. But how this happens remains a ridiculous mystery as scientists could only study a small number of neurons at a time.

Over the past few decades, technological advances have allowed scientists to begin mapping the whole brain. 1986, British researcher Published A small worm circuit made up of 302 neurons. The researchers then charted larger brains, including 140,000 neurons in the fly’s brain.

After all, is Dr. Crick’s impossible dream possible? The US government began in 2016 100 million dollar effort Scan cubic millimeters of mouse brain. The project was called Cortical Network (or Mechanical Intelligence from Microns) and was led by scientists from the Allen Institute of Brain Science, Princeton University, and Baylor School of Medicine.

Researchers have zeroed into part of the mouse’s brain, which receives signals from the eyes and reconstructs what the animal is seeing. In the first phase of the study, the team recorded the neuronal activity in that area as they showed mouse videos of different landscapes.

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Source: www.nytimes.com

Unraveling the Mystery of Space Mediation Particles: Exploring the Most Detailed Survey

International Space Station AMS particle detector

NASA

The 11 -year survey of particles near our sun and anti -particles has emerged the history of our solar system and causes a new mystery about the particles itself.

“It seems like I stepped into a dark room and saw a lot of new things.” Samuel Tin At Massachusetts Institute of Technology.

Energy particles are filled in the space, which is moved by burst called cosmic rays. When the cosmic ray enters the Alpha Magnetic Difference (AMS) detector of the International Space Station (ISS), the magnetic field separates particles based on the charge, and the detector measures mass and energy. This separation is important because it helps to identify the differences between particles and their anti -particles.

AMS collaboration, and his colleagues, analyzed more than 11 years of AMS data, and found that we didn’t know much about the particle behavior as we thought. For example, this survey reveals how the number of particles tends to be over time and how different types of particles interact with each other. Ting says that there are more than 600 theoretical models that can explain each of these trends, but there is nothing to explain both surveys at the same time.

And the results of the survey may be important for more than a single particle. Researchers say that the changing characteristics may be useful as a record of the history of the solar system, so they are shooting cosmic rays with different detectors for more than a century. Jamie Lankin At Princeton University. However, she says that we have never understood how the solar cycle affects the light rays.

This is because 11 years is the length of one solar cycle, so collecting data during that period captures all repeated fluctuations in the sun magnetic field, and the behavior of cosmic rays changes. She says that such a detailed investigation can be a key to solving a method of using cosmic rays in “solar system archeology”.

However, he says that the cosmic ray itself is still mysterious. Gavin Lowell At Adelaide University in Australia. “The measured value of the particle AMS is essentially from outside the solar system,” he says. Detailed amounts of new analysis, including how different particle nuclei on the cosmic ray acts, may help researchers focus on more decisive theories of cosmic rays.

There is also a question of other unexplored universe. “It’s a big mystery for me that AMS can observe antiproton because we don’t see antimatters in our world.” Ian Low At Northwestern University, Illinois. He says that the origin of these anti -particles is connected to a mysterious dark substance, and otherwise it may be better than our current universe.

Ting and his colleagues are currently working on upgrading the AMS detector, can detect more particles, and are adjusted as astronauts who support the installation.

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Source: www.newscientist.com

Review of Civilization VII – Your civilization will rise to new heights in this detailed and captivating game

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Many years ago, during the progress of Civilization II, I began my career as a writer for the video game magazine Edge. As an enthusiast of the original Civilization game, I was eager to review its sequel and impressed the editor enough with my comprehensive analysis of the complex turn-based strategy game that I nearly lost my job due to my addiction to playing it non-stop for two weeks instead of writing my assigned articles. This led to a stern warning about my performance and ultimately ended my tenure as a game writer. Consequently, I did not review the next four installments of the series. Now, Civilization VII is making a comeback, and I find myself facing this captivating nemesis once again.

This game has always been a favorite among me and many other fans, offering a compelling simulation of building an empire from ancient tribes to modern superpowers. As a player, you have the opportunity to establish cities, gather resources, research new technologies, send out settlers, merchants, and armies, and expand your influence through peaceful relations or conquest. Victory can be achieved through military prowess, cultural dominance, or economic power, depending on your chosen playstyle. Each campaign offers a unique experience, making it a game that has withstood the test of time.




Extra nuances … civilization VII. Photo: 2K game

In this latest installment, Firaxis has made some significant changes, deviating from guiding a single civilization through the entire campaign. Instead, players now choose different leaders with unique attributes and guide them through three distinct historical ages, each time selecting a new country to control. Each country brings its own units and buildings, adding depth to the gameplay. The game structure encourages continuity and strategic decision-making, enhancing the overall experience.

Civilization VII will be released on PC (version tested), PS4/5, switch, Xbox One, Xbox series S/X on February 11th.

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

NOIRLab unveils detailed images of 88 constellations and expansive night sky photo

NSF’s NOIRLab, in collaboration with ESA/Hubble, released A collection of free high-resolution images of all 88 zodiac signs. The largest open source and free available all-sky photography night sky.

This all-sky photo of the night sky was compiled by astrophotographer Eckhart Slavik using images taken from the best and darkest locations around the world. Image credit: NOIRLab / NSF / AURA / E. Slawik / M. Zamani.

“This complete collection of free, high-resolution, downloadable images of all 88 Western IAU-recognized constellations serves as an educational archive for personal and academic use,” NOIRLab astronomers said in a statement.

“This project also includes the release of the largest open-source and freely available all-sky photography of the night sky.”

The photographer behind these amazing high-quality images is German astrophotographer Eckhard Slavik.

“The images were taken on film and each panel consists of two separate exposures, one with a diffuser filter and one without, allowing the colors of the stars to shine through. visible,” the astronomers said.

“All products include a comprehensive description of the constellation and its historical origins, as well as corresponding standardized stick figures, outline drawings, finder charts, and descriptions of the constellation's most prominent deep-sky objects. Included.

“Existing astronomical images of these deep-sky objects taken with various NSF NOIRLab telescopes are also included.”

“Downloadable flashcards and other audio-visual aids and materials make it easy to bring constellations into the classroom.”

NOIRLab astronomers have also released the largest open-source, freely available all-sky photo of the night sky.

“With 40,000 pixels, this is probably one of the best images of its kind ever made,” they wrote.

“This giant skyscape was compiled using images taken by Slavik from the highest and darkest places around the world: Tenerife, La Palma, Spain; Namibia; and Chile.”

“The 88 constellation images can be viewed by all ages and are particularly suitable for use in planetariums and museums.”

“Please visit” Project webpage Learn about all 88 constellations and see how many you can spot in the night sky. ”

Source: www.sci.news

First Detailed Map of Solar Coronal Magnetic Field Created by Inouye Solar Telescope

This groundbreaking achievement will improve our understanding of the Sun’s atmosphere and shed light on how its changing conditions affect our technology-dependent society.



The Inouye Solar Telescope has released the first map of the magnetic field signal in the solar corona measured using the Zeeman effect. Image courtesy of NSF/NSO/AURA/NASA’s Solar Dynamics Observatory.

The Earth’s magnetic field protects us from the solar wind, protects our atmosphere and makes life possible.

But electromagnetic fields and high-energy particles from extreme solar activity could disrupt satellites, power grids, and other systems necessary for an increasingly technological society.

Understanding these dynamic interactions, which change on timescales ranging from days to centuries, is crucial to safeguarding our infrastructure and current ways of life.

Measuring the magnetic properties of the Sun’s corona, or outer atmosphere, has long challenged astronomers and the limits of technology.

today, Daniel K. Inouye Solar TelescopeLocated near the summit of Haleakala on the Hawaiian island of Maui, the facility is a state-of-the-art facility designed to study coronas.

The satellite has produced the first and most detailed map of the coronal magnetic field to date, taking an important first step in solving these mysteries.

“Inoue’s achievements in mapping the Sun’s coronal magnetic field are a testament to the innovative design and capabilities of this pioneering and unique observatory,” said Dr. Tom Shad, NSF National Solar Observatory investigator.

“This groundbreaking discovery is expected to greatly improve our understanding of the Sun’s atmosphere and its impact on the solar system.”

The researchers used the Zeeman effect, which measures magnetic properties by observing the splitting of spectral lines, to create a detailed map of the magnetic field of the solar corona.

“Spectral lines are distinct lines that appear at particular wavelengths in the electromagnetic spectrum and represent light absorbed or emitted by atoms and molecules,” they explained.

“These lines are unique to each atom and molecule and act like a fingerprint. By looking at the spectrum, scientists can determine the chemical composition and physical properties of an object.”

“When exposed to a magnetic field like the Sun’s, these lines split apart, giving us insight into the magnetic properties of the object.”

Previous attempts to detect such signals, last reported 20 years ago, have lacked the detail and regularity needed for widespread scientific investigation.

Now, Inouye’s unparalleled capabilities make it possible to study these important signals in detail and on a regular basis.

The solar corona can usually only be seen during a total solar eclipse, when most of the Sun’s light is blocked and Earth’s sky becomes dark.

But the Inouye Telescope uses a technique called coronagraphy to create an artificial eclipse that allows it to detect extremely faint polarized signals, highlighting its unparalleled sensitivity and cementing its status as a unique window into viewing our home star.

This telescope is Cryogenic near-infrared spectropolarimeter (Cryo-NIRSP) is one of the telescope’s main instruments used to study the corona and map its magnetic field.

“Just as detailed maps of the Earth’s surface and atmosphere have improved the accuracy of weather forecasts, this remarkably complete map of the magnetic field of the Sun’s corona will help us more accurately predict solar storms and space weather,” said Dr. Carrie Black, program director for NSF’s National Solar Observatory.

“The invisible yet incredibly powerful forces captured in this map will continue to drive solar physics for the next century and beyond.”

“Mapping the strength of the corona’s magnetic field is a fundamental scientific advance not only for solar research but for astronomy in general,” said Dr. Christoph Keller, director of the National Solar Observatory.

“This marks the beginning of a new era in understanding how stars’ magnetic fields affect planets in our solar system and the thousands of exoplanetary systems currently known.”

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This article has been edited from an original release by the National Solar Observatory.

Source: www.sci.news

The mystery of Cretaceous shark hunting techniques revealed through detailed fossil analysis

Petitcodus shark fossil discovered in Mexico

Roman Vullo

A fossil shark that thrived during the Cretaceous period has been found and has shed light on how sharks hunted and their place on the evolutionary tree.

Fossil shark teeth Ptychodus have been in museums for over 200 years. While some members of this group grew to be enormous, the anatomy of others was largely unknown.

This lack of information left researchers uncertain about the shark’s overall appearance and feeding habits, but the wide, flat teeth suggest it was capable of eating hard-shelled prey.

Recently, Professor Roman Vullo at the University of Rennes in France discovered six well-preserved full-body fossils of Ptychodus in Mexico, placing the shark in the order Lamniformes alongside modern shark species like great whites and basking sharks.

What makes this discovery interesting is that while modern white sharks are known for hunting in open waters, Ptychodus were fast swimmers and voracious eaters in the open ocean, preying on armored pelagic fish like large ammonites and sea turtles.

Despite the small size of the studied specimens, estimated to be less than 3 meters long, researchers believe some members of the genus reached lengths of about 9.7 meters – twice the size of a great white shark. Females tended to be larger, measuring between 4.6 and 4.9 meters in length.

During the Cretaceous period, Ptychodus sharks played a significant role in the marine food chain. They likely competed with large marine reptiles with crushing dentition, which may have led to their extinction before the end-Cretaceous extinction event.

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Source: www.newscientist.com

Researchers Develop Detailed Geological Map of Oxia Plain

Using data from ESA’s ExoMars Trace Gas Orbiter and NASA’s Mars Reconnaissance Orbiter, planetary scientists created a 1:30,000-scale geological map of the Oxian Plain, the landing site for ESA’s ExoMars Rosalind Franklin rover mission. Created.



Faudon other. Created the most detailed geological map of Oxia Planitia, the Mars landing site for ESA’s Rosalind Franklin rover. Image credit: Faudon other., doi: 10.1080/17445647.2024.2302361.

Oxia Planum Located on the northern edge of Arabian Terra, it preserves a record of the diverse geological processes that shaped the region.

It is a transitional region between the cratered Arabian Terra and the young lowland plain of the Chryse Planitia.

“Oxia Planum is located near the Martian equator and contains deposits that are nearly 4 billion years old,” said Open University researcher Peter Faudon and colleagues.

“On a geological scale, this would be the oldest landing site ever visited by a spacecraft on Mars.”

“This region is rich in clay minerals that form due to the presence of water. These rocks are ideal for preserving evidence of the earliest forms of life. This makes it possible to predict that life once existed on Mars. It’s a great place to look for clues as to whether this is the case.”

To map the Oxian Plains, the authors used several instruments, including the Color and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter and the HiRISE camera on NASA’s Mars Reconnaissance Orbiter (MRO). We used data from.

This map details 15 rock units classified into 6 groups and 7 textural and surface units.

“This map includes the main types of rock and structures with unique shapes, such as ridges and craters,” the researchers said.

“It also features materials that are placed on top, blown by the wind or blown long distances when a meteorite hits the Earth’s surface, for example.”

The result is the highest-resolution map of the Oxian plains to date at a scale of 1:25000, where 1 centimeter corresponds to 250 meters on the surface of Mars.

Average daily driving time is 25-50 minutes. rosalind franklin rover On the map it is 1-2 mm.

“This map is really interesting because it’s a guide to where the answers are,” Dr. Faudon said.

“This serves as a visual hypothesis for what we currently know about the different rocks at the landing site.”

“With the instruments on board the Rosalind Franklin rover, you can test your knowledge on the fly when the time comes.”

of result Published in map journal.

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peter faudon other. 2024. High-resolution map of the Oxian Plains on Mars. Landing site for the ExoMars Rosalind Franklin rover mission. map journal 20(1); doi: 10.1080/17445647.2024.2302361

Source: www.sci.news

Detailed Image of Black Hole Unveiled in New Fiery Donut Visualization

The image on the right is the latest and best image of a black hole.

EHT collaboration

Thanks to an update to the world’s first black hole image taken a year later, we now have the most detailed observation of a black hole to date.

In 2019, researchers released an image of the supermassive black hole known as M87*, located 55 million light-years away at the center of galaxy M87. The image, the world’s first glimpse of a black hole, was taken during the first observations in 2017 by a network of radio astronomical observatories around the world called the Event Horizon Telescope (EHT).

Now, the EHT collaboration has released tracking images of M87* taken during 2018 observations using additional telescopes in Greenland.

As the name suggests, these objects do not emit light, so the light in the image does not come out of the black hole. What we see instead is the silhouette of a black hole at the center of a mass of hot material, pulled inward by its powerful gravity.

“This image tells us that the black hole’s shadow is permanent and still exists,” says the EHT scientist. Eduardo Ross. “You can see that the ring is a beautiful circle. It’s very circular, not an oval or anything. We also see an enhancement on the south side in this ring, which is what we expected.”

This enhancement, visible as a slightly bright glow under the slightly displaced shadow of M87*, is due to the distortion of space-time associated with the black hole’s rotation (as explained by Albert Einstein’s theory of general relativity). This is due to

The additional telescopes have slightly increased the resolution of the images, greatly increasing the amount of data that can be cross-referenced with observations from other telescopes. However, less than ideal weather made viewing conditions difficult. This means the resolution is not as high as theoretically expected, Ross says.

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Source: www.newscientist.com

Juno spacecraft captures incredibly detailed image of Jupiter’s moon Io

This image of Io was taken by the Juno spacecraft.

NASA/SwRI/MSSS

Thanks to NASA's Juno spacecraft, which passed the moon on December 30, we had the closest look at Jupiter's volcanic moon Io in decades.

Juno, which has been orbiting Jupiter since 2016, has increasingly taken images of Io's vicinity in recent months as its orbit around Jupiter changes.

This latest image was taken just 1500 kilometers above the moon's surface. In it, you can see some of Io's hundreds of towering mountains, some of which can exceed 10 kilometers in height, and their long, sharp shadows.

Io is thought to be the most volcanically active body in the solar system, with hundreds of active volcanoes. These volcanoes tend to be smaller than the largest mountains, averaging only 1 to 2 kilometers in height, and are difficult to see in images.

But by comparing the data with images from Juno's previous 56 lunar passes, astronomers are starting to understand how these volcanoes have changed over time and why they are so active. You can know.

Juno has also been exploring Jupiter's other moons, including Europa and Ganymede, collecting data and taking the closest images. NASA's Galileo spacecraft In February, Juno will again fly very close, about 1,500 kilometers above Io's surface.

Juno will fly close to Io seven more times before leaving orbit for Jupiter at the end of 2025, but that won't be the end of learning about Jupiter's moons. NASA's Europa Clipper spacecraft, scheduled to launch in October this year, is designed to fly just 25 kilometers above the surface of Europa, considered one of the most promising sites for life on Earth. This will provide important information about the mysterious inland sea. Solar system. The spacecraft is scheduled to arrive at Europa in 2030.

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Source: www.newscientist.com