Lucy provides a comprehensive look at the main belt asteroid Donald Johansson

NASA’s Lucy Mission is actively examining images obtained during its encounter with the carbonaceous asteroid Donald Johansson on April 20, 2025.



Donald Johanson is located on NASA’s Lucy spacecraft, approximately 2,700 km (1,700 miles) away, about 3.2 minutes before closest approach on April 20, 2025. The lighting conditions, which are primarily behind Lucy, significantly diminish the visibility of topographic features. Image credit: NASA/GODDARD/SWRI/JOHNS HOPKINS APL.

Donald Johansson resides in the inner region of the solar system’s major asteroid belt.

The asteroid was initially discovered on March 2, 1981, by American astronomer Sheltebus at the Siding Spring Observatory.

On April 20, 2025, NASA’s Lucy spacecraft executed a flyby near Donald Johansson, approaching within 960 km (600 miles) of its surface.

This encounter confirmed that the asteroid is an elongated contact binary, a structure that forms when two small celestial bodies collide.

Nonetheless, members of the Lucy team were taken aback by the unusual shape of the narrow neck connecting the two lobes.



A pair of stereo images combining the final full approach image (right) with slightly clipped images taken 72 seconds later. For a three-dimensional view of the asteroid’s structure, cross your eyes while focusing on the image. Image credits: NASA/GODDARD/SWRI/JOHNS HOPKINS APL/BRIAN MAY/CLAUDIA MANZONI.

“The newly released image was captured by the L’Lorri Imager on the spacecraft just minutes before the closest approach,” the researchers stated.

“This successful dress rehearsal assures the team that both the spacecraft and our crew are well-prepared for the main event: an encounter with a Jupiter Trojan asteroid.”

“Currently, the spacecraft is in a relatively quiet cruising phase as it journeys through the main asteroid belt.”

“Lucy is traveling at over 50,000 km/h (30,000 mph) away from the Sun.”

“We will continue to monitor the spacecraft as it heads toward the cooler, dimmer regions of the solar system.”

“Upon reaching the Trojan asteroid, the mission plans to conduct four encounters and observe at least six asteroids (including two satellites discovered by our team) over the course of 15 months.”

“The first encounter is scheduled with the asteroid Euribates in August 2027.”

Source: www.sci.news

Possible Main Belt Asteroid Asteroid 2024 YR4 Approaches Earth

Astronomers using Gemini Multi-Object Spectrograph (GMOS) A telescope in southern Gemini determined that the recently discovered nearby asteroid 2024 YR4 is one of the largest objects in recent history that could affect the moon, and is likely to originate from the major asteroid belt in the solar system. Their Survey results It will be published in Astrophysics Journal Letter.

This image from the 2024 YR4 was captured at Gemini Southeres Scope in Chile, half of the International Gemini Observatory run by Noallab. Image credits: International Gemini Observatory / Noirlab / NSF / Aura / M. Zamani.

The 2024 YR4 was discovered on December 27, 2024 by the Asteroid’s Ground Impact Last Altar System (ATLAS).

At the time, the asteroids had a close approach to Earth, passing a distance of just 0.017 Au (astronomy unit).

In January 2025, a month after its discovery, the 2024 YR4 exceeded the International Asteroid Warning Network (IAND) notification threshold, which was predicted on December 22, 2032, with a 1% chance of future impact on Earth.

The asteroid misses Earth during this encounter, but there is still a few percent remaining chance that it could hit the moon instead.

Now interested in characterizing famous asteroids, Eureka scientific Athleton Mar Bryce Borin A colleague used a Gemini Southeres scope to capture images of the 2024 YR4 at several different wavelengths.

A detailed analysis of the asteroid LightCurve allowed the team to determine its composition, orbital properties and 3D shape.

“Our observation with Gemini South provided an important part of the puzzle in determining the characteristics of the 2024 YR4,” Dr. Bolin said.

“Studying this asteroid could be an Earth impactor and was crucial in understanding the poorly understood Earth Cross population.”

Information collected from the light curve indicates that the 2024 YR4 is likely an S-type asteroid. In other words, it has a silicate-rich composition.

The reflective pattern suggests a diameter of approximately 30-65 m (98-213 feet), making it one of the largest objects in recent history and affects the moon.

It is unlikely, but if it affects the moon, the asteroid would provide an unprecedented opportunity to study the relationship between the size of the asteroid and the size of the resulting impact crater – an amount previously unknown.

Analysis also revealed that the asteroid’s rotation period is about once every 20 minutes, and is shaped like a rare hockey puck.

“The discovery was pretty unexpected as most asteroids are thought to be shaped like potatoes and toy tops rather than flat disks,” Dr. Bolin said.

Based on these orbital characteristics, astronomers determined that the 2024 YR4 is most likely to originate from the main asteroid belt, and that gravity interaction with Jupiter is likely to cause it to be disrupted by its current short-range orbit.

Its retrograde spin direction suggests that it may have moved inward from the central main belt region, adding to its understanding of how small asteroids evolve and reach orbits beyond Earth.

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Bryce T. Borin et al. 2025. Discovery and characterization of the Asteroid 2024 YR4, which crosses the Earth. apjlin press; arxiv: 2503.05694v2

Source: www.sci.news

Research lab identifies meteorites linked to specific asteroid with 75 main belts.

Astronomers from SETI Institute, NASA’s Ames Research Center, and Curtin University have tracked the impact orbits of 75 observed metstone waterfalls to previously unidentified source regions of several of the main asteroid belt.

Impressions of an artist on a rocky asteroid. Image credits: Mark A. Garlick, Space-Art.co.uk / Warwick University / Cambridge University.

“This is a 10-year detective story, with each recorded metstone waterfall providing new clues,” said Dr. Peter Jenniskens, an astronomer at Seti Institute and NASA’s Ames Research Center.

“We currently have the first overview of the asteroid belt geological map.”

Ten years ago, Dr. Jenniskens and his colleagues were aiming to build a network of all ski cameras in California and Nevada.

“Others built similar networks that spanned the world, and together formed a fireball observatory around the world,” said Hadrian Devillepova, an astronomer at Curtin University.

“For many years, we have tracked the routes of 17 recovered metstone waterfalls.”

“More fireballs have been tracked by doorbells and dashcam video cameras from citizen scientists and other dedicated networks around the world.”

“Overall, this quest produced 75 laboratory classified metstones with impact trajectories tracked by video cameras and photo cameras,” Dr. Jennis Kens said.

“It has proven sufficient to start seeing some patterns in the direction of metstones approaching the Earth.”

Most metstones come from the asteroid belt, the region between Mars and Jupiter.

These rocks come from a few larger asteroids that have been broken in the collision.

Even today, asteroids collide and create remnant fields within these asteroid families known as clusters.

“We can see that the 12 metstones (h-cartilage) of ordinary chondrites, which are now rich in iron, come from a debris field called low colonies on the pristine main belt,” Dr. Jennis Kens said.

“These metstones arrived from low-coupled orbital periods that match this debris field.”

“By measuring the age of cosmic ray exposure in metstones, we can determine that three of these 12 metstones originate from kalin clasters of dynamic ages of 5.8 million years, and two come from Koronis2 clusters of dynamic ages of 100-15 million years.”

“Another metstone can measure the age of Koronis3 clusters, about 83 million years.”

The authors also discovered a group of H-chondrites on steep orbits that appear to originate from the Nere Asteroididae in the central main belt, with a dynamic age of approximately 6 million years.

The mean motion resonance with nearby 3:1 Jupiter can raise the slope to the observed people.

A third group of H cartilage with an exposure age of approximately 35 million years of age emerged from the medial main belt.

“In our opinion, these H-cartilages came from the low masalia asteroids on the inner main belt, as their families have clusters of that same dynamic era,” Dr. Jennis Kens said.

“Asteroid (20) Masalia, the asteroid that created the cluster, is a parent body of the H-chondrite type.”

Researchers have discovered that low iron (l cartilage) and very low iron (LL chondrite) metstones mainly come from the inner main belt.

“I propose that L cartilage comes from the Hertha Asteroid family, just above the Masalia family,” Dr. Jennis Kens said.

“The asteroid Elsa doesn’t look like its fragments. Hertha is covered in dark rocks of shock black, which exhibits unusually violent collisions. The L-chondrites experienced a very violent origin 468 million years ago, when these metstones bombarded the Earth with numbers found in geological records.”

Knowing from the remains of the asteroid belt, the birth of our metstones is important for our planetary defense efforts against asteroids on the near Earth.

The orbits of approaching asteroids can provide clues to the origin of the asteroid belt, just like the metstone orbit.

“Asteroids near Earth do not arrive in the same orbit as Metstones because it takes time for them to evolve into Earth,” Dr. Jennis Kens said.

“But they come from some of the same Astide family.”

Team’s paper Published in the journal Weather and Planetary Science.

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Peter Jenniskens & Hadrien ar Devillepoix. Asteroids, meteors, and meteor-shaped link reviews. Weather and Planetary SciencePublished online on March 17th, 2025. doi:10.1111/maps.14321

Source: www.sci.news

Lucy Takes First Photo of Donald Johansson on Asteroid in Main Belt

NASA’s Lucy spacecraft flies by the small asteroid Donald Johansson on April 20, 2025.

By flashing between images captured by NASA’s Lucy spacecraft on February 20th and 22nd, 2025, this animation shows Donald Johansson’s perceived movement against the background star as the spacecraft rapidly approaches the asteroid. Image credit: NASA/GODDARD/SWRI/JOHNS HOPKINS APL.

Donald Johansson It is a carbonaceous small intestine about 4 km (2.5 miles) in diameter.

First discovered by American astronomer Sheltebas at the Siding Spring Observatory on March 2, 1981, it orbited within the inner region of the main asteroid belt.

NASA’s Lucy spacecraft will pass within 960 km (596 miles) of Donald Johansson on April 20th.

“This second asteroid encounter for Lucy will serve as a rehearsal for Jupiter’s Trojan asteroid outfit, the spacecraft’s main target,” a member of the Lucy team said in a statement.

“The spacecraft had already successfully observed the main belt asteroid Dinkinesh and its moon, Serum and Serum in November 2023.”

These new images have been captured Lucy Long Range Reconnaissance Imager (L’Lorri) Musical instrument.

This diagram shows NASA’s Lucy spacecraft passing through one of the Trojan asteroids near Jupiter. Image credit: Southwest Research Institute.

“But at a distance of 70 million km (45 million miles), Donald Johansson is still dim, but he stands out clearly in this area of ​​relatively faint stars in the constellations of Sextane,” the researchers said.

“The north of the sky is on the right side of the frame, with a 0.11-degree field of vision corresponding to 85,500 miles (140,000 km) of asteroidal distance.”

“Of the two images, another dimly lit asteroid can see the photobomb in the quadrant at the bottom right of the image.”

“However, as the headlights of approaching cars often remain relatively still, Donald Johansson’s obvious movement between these two images is much smaller than that of this intruder, who has fallen out of sight in the second image.”

According to scientists, Donald Johansson was named after anthropologist Donald Johansson, who discovered “Lucy.” Lucy Mission is named after the fossil.

“Lucy will continue to image Donald Johansson as part of his optical navigation program for the next two months. The optical navigation program will use the apparent position of the asteroid against the star’s background to ensure an accurate flyby,” they said.

Source: www.sci.news

Main Biological Breakthrough: Two Fathers and a Mouse

In a groundbreaking scientific achievement, a mouse with two male parents has successfully reached adulthood.

Researchers utilized embryo stem cell engineering to accomplish this milestone by accurately correcting an important gene involved in reproduction. Double-headed mouse.

This innovative method has allowed scientists to overcome previously insurmountable barriers in reproducing single-identified mammals.

In previous experiments, using two male mice resulted in genetic issues during fertilization, leading to severe congenital defects and early termination of mouse embryo development.

However, the researchers of this new study suspected that these genetic issues were caused by “imprinted” genes, which are inherited from both male and female parents.

“The unique characteristics of imprinted genes have led scientists to believe they are the fundamental barriers to mammal reproduction,” said Research co-author Professor Qi Zhou.

“Even in the artificial creation of a two-cell embryo or double-headed embryo, they were unable to develop properly and stalled at a certain point due to these genes.”

Based on this theory, researchers altered 20 important imprinted genes using various methods before implanting the modified embryos into surrogate mothers.

Their findings revealed that these genetic edits not only allowed for the creation of double-headed mice but also enabled them to survive to adulthood.

“These discoveries offer compelling evidence that imprinted abnormalities are the primary barriers in mammals,” said co-author Professor Guan Zan Ruo from SUN YAT-SEN University.

“This approach greatly advances the manipulation of embryo stem cells and cloned animals, paving the way for progress in regenerative medicine.”

However, researchers noted that only 11.8% of surviving embryos successfully developed to birth, and some did not survive to adulthood due to developmental disorders.

In fact, most of the adult mice displayed abnormal growth and lifespan, and the surviving mice were infertile.

The team is actively working to address these issues by investigating whether altering a specific gene can improve embryo development. They also plan to extend their research to include larger animals like monkeys, though the use of this technology in humans remains uncertain.

Read more:

  • Y chromosome has disappeared. Is this the end of man?
  • Mice display emotions on their faces like humans
  • Male mice transformed into females using previously considered “junk” DNA.

Source: www.sciencefocus.com

Webb finds 138 main belt asteroids measuring 10 meters in diameter

These asteroids are as small as 10 meters in diameter, making them the smallest asteroids ever observed in the major asteroid belt.

Artist Webb's illustration reveals clusters of main-belt decameter asteroids in infrared light. Image credit: Ella Mall/Julian de Wit.

The discovery of asteroids is essential to planetary defense efforts aimed at preventing collisions with Earth, such as the frequent megaton explosions caused by decameter impactors.

Large asteroids (=>100 km) remain in the main belt since their formation, while smaller asteroids are typically transported into the near-Earth object (NEO) population.

“We were able to detect NEOs very close to Earth, up to 10 meters in size,” said MIT researcher Dr. Artem Brudanov.

“We now have a way to discover these small asteroids when they are far away, so we can do more precise trajectory tracking, which is important for planetary defense.”

For this study, astronomers used data from the NASA/ESA/CSA James Webb Space Telescope to search for small asteroids.

Coincidentally, asteroids orbiting the main asteroid belt are much brighter in infrared wavelengths than in visible wavelengths, making them much easier to detect with Webb's infrared capabilities.

Researchers were able to discover eight known asteroids in the main asteroid belt.

Further investigation subsequently discovered 138 new asteroids around the belt, all within a few tens of meters in diameter, making them the smallest main-belt asteroids ever detected. .

They think several asteroids may be on their way to becoming NEOs, and one of them is probably the Trojans, or Jupiter-tracking asteroids.

“We thought we would only detect a few new objects, but we detected far more objects than we expected, especially small ones,” said Professor Julian de Witt of the Massachusetts Institute of Technology.

“This is an indication that we are exploring a new population regime, where many more small objects are formed by a chain of collisions that very efficiently disintegrates asteroids smaller than about 100 meters. It will be done.”

“This is a completely new and unexplored territory that we are entering, thanks to modern technology,” said Dr. Brudanov.

“This is a great example of what we can do as a field when we look at data from a different perspective. Sometimes the benefits can be huge, and this is one of them.”

“The statistics of these very small main-belt asteroids are very important for modeling asteroid populations,” said Dr. Miroslav Broz, a researcher at Charles University in Prague.

In fact, these are debris ejected during the impact of larger, kilometer-sized asteroids, which are observable and often exhibit similar orbits around the sun, placing them in a “family” of asteroids. Can be grouped. ”

“We never expected that we could use state-of-the-art exoplanet observations to achieve such impactful solar system bonus science,” said Dr. Michael Guillon, a researcher at the University of Liège.

ESA researcher Dr Marco Micheli said: “Thanks to the web, we can now discover these small asteroids even when they are located far from Earth, allowing us to make more accurate orbit determinations. “This is extremely important for planetary defense.” Near Earth Object Coordination Center.

of the team paper Published in today's magazine nature.

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AY Brudanov others. JWST sighting of a 10-meter main belt asteroid and views on the meteorite source. naturepublished online on December 9, 2024. doi: 10.1038/s41586-024-08480-z

Source: www.sci.news

Research reveals Stonehenge’s main stone originated in Scotland

summary

  • The “altar stone” at the heart of Stonehenge was likely made in what is now Scotland, a study has found.
  • It’s more than 450 miles away, raising the question of how ancient humans managed to transport the stone that far.
  • The study authors suggest they may have used boats.

Scientists say they have unlocked the secrets of Stonehenge’s six-tonne rock, a discovery that adds even more mystery to the site.

A study published Wednesday in the journal Nature suggests that the ancient site’s central sandstone “altar stone” was likely created in what is now Scotland, meaning it was transported more than 450 miles to southern England — farther than any of Stonehenge’s other stones of known origin.

The discovery raises important questions: Researchers estimate that the altar stone was placed about 4,500 years ago, meaning Neolithic people could have moved it hundreds of miles, long before the invention of the lightweight spoked wheel.

The find also suggests that culture and social structure in the British Isles at this time was more intertwined than previously thought, and that Neolithic people were capable of carrying out complex projects with relatively simple tools.

The discovery was made based on the dating analysis of mineral grains within the sandstone. After profiling the age of the grains, the researchers were able to compare the altar stone’s age “fingerprint” with a database of sandstone samples from across the UK and nearby areas, such as Brittany in France.

“We can link the age spectrum with a fairly high degree of statistical certainty – in fact more than 95% confidence – to a very specific region in northeast Scotland,” said study co-author Chris Kirkland, professor of earth and planetary sciences at Curtin University in Australia.

The area Kirkland refers to, the Orkney Basin, includes the Orkney Islands themselves; Known for its elaborate stone circles.

“We can’t directly answer the question of why this rock was transported,” Kirkland said, “all we know is that this 6.5-ton rock was transported from 750 kilometers away, and that alone tells us an awful lot about Neolithic societies and their connections.”

Stonehenge — UNESCO World Heritage Site One of the best-preserved prehistoric megalithic monuments, the site is surrounded by large sandstone slabs called “sarsens”, which support stone lintels (also horizontal spans of rock, some held together by joints). Inside the outline of the sarsens is an inner circle of “bluestones”, which in turn is a horseshoe shape.

of The sarsens are thought to have originated approximately 15 miles north of Stonehenge.Meanwhile, bluestone comes from Wales, about 140 miles away.

The new study concerns the central Altar Stone, a roughly 16-foot-long slab of stone that shows evidence of being shaped by human tools. Stonehenge’s other slabs currently rest on top of the Altar Stone but have apparently been toppled over time.

“Whatever the reason, this is a special stone,” said David Nash, a professor of physical geography at the University of Brighton who has studied Stonehenge but was not involved in the new study. “It’s totally different to the other stones on the site.”

Kirkland and his colleagues looked at three possible routes the altar stones could have taken from Scotland to Stonehenge: They could have been transported by shifting glacial ice during the Ice Age, but the study authors don’t think that’s a good explanation, or they could have been transported overland by humans, but the team thinks that would be too difficult in the wooded area.

The third possibility, which they consider to be the most likely, is that the stones were transported by ship, and there is evidence of seaborne transport during this period, when England’s coastline was different to what it is today.

Nash said the authors had reached a “sound conclusion” about the altar stone’s origins.

“Their work is really fascinating,” he said, adding that their findings add to the evidence that Neolithic people travelled throughout the British Isles and were part of wider social structures. “There was clearly a social structure, there were connections and there was a very clear transmission of ideas.”

Stonehenge is one of approximately 1,300 surviving ancient stone circles. According to the British MuseumResearchers believe the site’s stones were shaped with hand tools and assembled using a winch and pulley system, with the stones aligned to coincide with the movement of the sun and the summer and winter solstices.

Experts speculate that Neolithic people may have used these sites for rituals and ceremonies, but details have been lost to time — especially what was so special about the altar stones.

“Today’s billionaires decorate their mansions with Italian Carrara marble, but I don’t understand why they do it. It’s a mystery,” said Anthony Clark, lead author of the new study and a doctoral student at Curtin University. “Humans have always been fascinated by finding the perfect stone, and perhaps Neolithic Britons were too, so their motivations have been forgotten over time.”

As a next step, the researchers hope to pinpoint the exact outcrop or region where the rocks originated, but said fundamental mysteries are likely to remain.

“They placed a lot of value in transporting that stone 700, 800, 900 kilometres,” said Nick Pearce, a professor of geography and geosciences at Aberystwyth University in Wales and another co-author of the study. “However they transported it, it meant something to them. What did it mean? Why did it mean so much to them? It gives us all something to think about.”

Source: www.nbcnews.com

454 new asteroids discovered in the main asteroid belt by astronomers

632 main-belt asteroids (178 known objects and 454 unknown objects) have been identified in archival images from the NASA/ESA Hubble Space Telescope. Citizen scientists from around the world contributed to the discovery of this asteroid. Professional astronomers identified the asteroid using a combination of volunteer efforts and machine learning algorithms.

This Hubble image of barred spiral galaxy UGC 12158 looks like someone took it with a white marking pen. In reality, this is a combination of long exposures of a foreground asteroid moving within Hubble's field of view, adding light bombardment to observations of the galaxy. The galaxy was photographed several times. The dashed pattern is proof of this. Due to parallax, the asteroid appears as a curved trajectory. Hubble is not stationary, but orbits around the Earth, giving the illusion of a faint asteroid swimming along a curved trajectory. This unknown asteroid is located inside the solar system's asteroid belt, so it is 10 trillion times closer to Hubble than the background galaxy. Image credits: NASA / ESA / Hubble / Pablo García Martín, UAM / Joseph DePasquale, STScI / Alex Filippenko, University of California, Berkeley.

More than 4 billion years ago, the eight major planets around the sun formed by sweeping up debris from the vast disk of dust and gas surrounding the sun.

This is common in the birth process of planets, and the NASA/ESA Hubble Space Telescope has for the first time optically observed a similar disk surrounding a newborn star, providing a glimpse into the solar system's formative years.

Four billion years later, debris still litters the planet's construction yards.

Most of this ancient space debris, or asteroids, lies between the orbits of Mars and Jupiter within the main asteroid belt.

“We are starting to learn more about the presence of a small number of main-belt asteroids,” said Dr. Pablo García Martín, an astronomer at the Autonomous University of Madrid.

“We were surprised to see so many candidate objects.”

“We've had some hints that this population exists, but we're now confirming it with a random asteroid population sample obtained using the entire Hubble archive.”

“This is important for gaining insight into models of the evolution of the solar system.”

Since Hubble orbits around the Earth at high speed, Hubble exposure allows us to follow its trail and capture a wandering asteroid.

When viewed from a telescope on Earth, the asteroid leaves streaks across the photo.

The asteroid appears as an unmistakable curved trajectory in the photo, making the Hubble exposure a “photobomb.”

Hubble observes the asteroid from different perspectives as it moves around Earth, but the asteroid also moves along its own orbit.

By knowing Hubble's position during observations and measuring the curvature of its stripes, scientists can determine the distance to the asteroid and estimate the shape of its orbit.

Most of the asteroids involved are in the main belt between the orbits of Mars and Jupiter.

Their brightness is measured by Hubble's sensitive camera. Then, by comparing its brightness and distance, we can estimate its size.

The faintest asteroid found in the survey is approximately 40 million times less bright than the faintest star visible to the human eye.

“Because the asteroid's position changes over time, you can't find the asteroid's location just by entering the coordinates, because the asteroid may not be there at a different time,” Melin said.

“As astronomers, we don't have time to study images of every asteroid.”

“So we came up with the idea of ​​collaborating with more than 10,000 citizen science volunteers to browse the massive Hubble archive.”

of result appear in the diary astronomy and astrophysics.

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Pablo Garcia-Martin other. 2024. Hubble Asteroid Hunter III. Physical properties of newly discovered asteroids. A&A 683, A122; doi: 10.1051/0004-6361/202346771

Source: www.sci.news