Moroccan Hominin Fossils: Potential Close Ancestors of Modern Humans

Ancient Human Jawbone Discovered in Morocco’s Man Cave

Hamza Mehimdate, Casablanca Pre-History Program

Approximately 550,000-year-old fossils discovered in North Africa potentially belong to a shared ancestor of Neanderthals, Denisovans, and modern humans, existing right before these three significant hominin lineages diverged.

Neanderthals and Denisovans, the final common ancestors of modern humans, are believed to have thrived between 765,000 and 550,000 years ago. However, key questions about their existence and habitats still challenge our understanding of human evolution.

Recent fossil discoveries suggest that researchers, including Jean-Jacques Hublin from the Max Planck Institute for Evolutionary Anthropology in Leipzig, Germany, are nearing the pivotal moment of divergence in ancient human lineages.

Hublin and his team examined various fossils, including two adult jawbones, one juvenile jawbone, and several vertebrae unearthed from a cave referred to as the Cave of Mankind near Casablanca, Morocco. One of the adult jawbones had been detailed in a 1969 study, while the remaining specimens are presented for the first time.

The fossilized molars share similarities with early Homo sapiens and Neanderthals, yet their jaw structures resemble ancient African Homo erectus.

Fortunately, these Moroccan hominids existed around the same period as changes in Earth’s magnetic field, recorded within the geological formations containing the fossils, allowing for precise dating to approximately 773,000 years ago.

Hublin described the find as filling a “significant gap” in the African human fossil record dating back to between one million and 600,000 years ago. Paleogenetic studies reveal that the ancestors of Neanderthals and Denisovans diverged around this time, while H. sapiens evolved independently in Africa.

The newly identified fossils are contemporaneous with a hominid population in Spain, previously hypothesized to serve as a common ancestor between Homo sapiens and Neanderthals.

Excavation Team at Moroccan Fossil Site

R. Gallotti, Casablanca Pre-History Program

Both Homo ancestors and Moroccan hominins exhibit “a mosaic of primitive and derived features,” Hublin notes, suggesting possible genetic exchanges across the Strait of Gibraltar. However, notable distinctions exist between the fossils from both areas, with Spanish specimens appearing more Neanderthal-like.

“The last common ancestor likely inhabited both sides of the Mediterranean during that era, indicating a deep African lineage for Homo sapiens opposed to the Eurasian origin theories proposed by some,” Hublin states.

Julian Lewis, a professor at Griffith University in Brisbane, Australia, expresses intrigue over the physical differences in early Pleistocene hominids closely related to our species.

“The key takeaway is that these differences have been developing for a substantial period,” Lewis concluded, alluding to the arrival of the Homo ancestor in Spain, indicating it may represent one of several species across North Africa that eventually crossed over to Europe.

Chris Stringer from the Natural History Museum in London has also contributed to this discussion. His research, including findings from human fossils in China published last year, suggests that the last common ancestor of Homo sapiens, Neanderthals, and Denisovans could date back over a million years.

“The specific continent for that common ancestor’s existence remains unknown,” Stringer remarked. “Yet even if it lived outside Africa, our analysis indicates that the evolution of Homo sapiens predominantly took place in Africa, suggesting a potential early migration back into Africa for continued evolution.”

These newly identified Moroccan fossils may even represent early specimens of Homo sapiens, though sufficient skeletal fragments are lacking for definitive classification.

Ongoing comparisons with previously studied fossils will help ascertain their evolutionary positioning.

Topics:

  • Human Evolution/
  • Ancient Hominins

Source: www.newscientist.com

Astronomers Identify Three Earth-Sized Exoplanets in a Close Binary Star System

A researcher suggests that the binary star system TOI-2267 is likely home to two warm Earth-sized exoplanets and an additional candidate. A new paper published in the journal Astronomy and Astrophysics discusses these findings.



Artist’s impression of the binary star system TOI-2267. Image credit: Mario Sucerquia, Grenoble-Alpes University.

The system, known as G 222-3 or TIC 459837008, consists of the M5 type star TOI-2267A and the M6 type star TOI-2267B, which are separated by approximately 8 astronomical units.

Located about 22 parsecs (73.5 light-years) from the Sun in the constellation Cepheus, TOI-2267 presents a fascinating planetary arrangement.

Dr. Sebastian Zuniga Fernández, an astronomer at the University of Liege, stated, “Our analysis shows a distinct planetary configuration: two planets orbiting one star and a third planet orbiting its companion star.”

This discovery makes TOI-2267 the first known binary star system to host planets that transit around both stars.

Dr. Francisco Pozuelos from the Andalucía Astronomical Institute remarked, “Our findings set several records, making this star system the most compact and coolest known planet-planet pair, and it is the first observed instance of a planet transiting both components.”

Astronomers utilized the SPECULOOS and TRAPPIST telescopes along with their proprietary detection software, SHERLOCK, to identify the three planetary signals.

“Uncovering three Earth-sized planets within such a compact binary star system is an exceptional opportunity,” Dr. Zuniga-Fernández noted.

“This will enable us to scrutinize the limits of planet formation models in complex environments and deepen our understanding of the variety of planetary structures in our galaxy.”

The two confirmed planets, TOI-2267b and TOI-2267c, have orbital periods of 2.28 days and 3.49 days, respectively.

The authors currently cannot determine which star in the binary system the planets orbit.

When orbiting TOI-2267A, TOI-2267b and TOI-2267c exhibit radii of 1 and 1.14 Earth sizes, while their radii become 1.22 and 1.36 Earth radii when orbiting TOI-2267B.

Furthermore, researchers detected a third strong signal with a period of 2.03 days, which is still classified as a planetary candidate, having sizes of 0.95 or 1.13 Earth radii depending on whether it orbits TOI-2267A or TOI-2267B.

Dr. Pozuelos added, “This system serves as a genuine natural laboratory for exploring how rocky planets can form and persist under extreme mechanical conditions that were previously thought to endanger their stability.”

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S. Zuniga-Fernandez et al. 2025. Two warm Earth-sized exoplanets and an Earth-sized candidate planet in the M5V-M6V binary star system TOI-2267. A&A 702, A85; doi: 10.1051/0004-6361/202554419

Source: www.sci.news

Do Digital Board Games Match the Fun of the Real Deal? Spoiler: Not Even Close

I don’t engage with video game adaptations of traditional board games. Why is this the case? The appeal of video games lies in their speed, visual appeal, and reduced reliance on other players compared to classic games that use dice or cards. However, after my recent family board game night was hindered by scheduling conflicts and familial tensions, I chose to test out some board games on my iPhone that Saturday evening.

I began with Uno, a cherished family favorite. We still play with the Simpsons Uno set we purchased years ago—a simple, comforting card game. The iOS version differs significantly, introducing a three-minute time limit per round, which adds a layer of urgency beyond just strategy. While I appreciate this twist, I find myself missing the lively family interactions (and the fierce shifts in loyalty) of the in-person version. It just doesn’t compare to sending silly faces to MoshOnion933. Believe me, I tried.

Next, I jumped into Yahtzee With Buddies. It’s one of the few games I enjoy that my family doesn’t share my enthusiasm for. I appreciated the fresh spin that highlighted multipliers for specific scoring categories, and I enjoyed unlocking the various dice and treasures. Yet, I soon realized these were merely gateways to microtransactions, complete with a pop-up urging me to buy more rolls just as I was 16 seconds away from achieving Yahtzee. The final straw was when scratch cards started appearing, a sneaky form of gambling reminiscent of the old FIFA packs.


Fever Dream…Monopoly GO. Photo: Scopely/Hasbro

Monopoly Go is even more frustrating. The overwhelming number of beeps and chaotic graphics gave me a headache. Land on a space, and you’ll find yourself assaulting other players’ properties with wrecking balls, only for them to defend with characters like Baby Yoda. It’s like a surreal Monopoly experience, resembling the kind of game you might be forced to endure by a malevolent antagonist.

Opting for the “Triple” option allows you to roll three dice, with the reward being tripled. This, however, leads to faster depletion and microtransaction traps, akin to a slot machine experience. You can even set it to autoplay and passively observe the distracting graphics, much like being trapped inside a retro washing machine. It hardly feels like a game; rather, you’re a landmark in a colorful reset where you spend real money to watch an artificial score fluctuate. Only someone who thinks Mrs. Brown’s Boys is hilarious would consider this fun.

I expected The Game of Life to be similar, but I was pleasantly surprised!

The familiar choices are back: Career or college? Married or single? One child or four? Costs have increased, and you now need to pay $20,000 upon marriage. We just acquired a pasta maker! Tax is only assessed if you land on certain squares, meaning you’ll only pay if you have bad luck. Ah, the life of a billionaire! I wish I could find the original game’s spinner, the second-best piece of equipment in board gaming history (nothing can top the Pop-O-Matic, akin to bubble wrap).


Des re…The Game of Life. Photo: Anadolu/Getty Images

In my subsequent game, I prioritized my career over having children and ended up significantly wealthier. This isn’t merely a game; it’s a highly detailed simulation of life. I’ve avoided playing games because it feels disheartening to see how simple success can be in their version of life. And being in my 50s, I crave something with more complexity.

Then, I remembered chess—the board game where computers excel. I downloaded Zach Gage’s Really Bad Chess to explore if someone could really reinvent this classic by 2025.

I loved his “Pocket Run Pool,” which brilliantly combines ball-hitting with exciting new features. His chess adapts the classic game with a clever premise: random piece placements and numbers. This results in matches where, at times, you may have four queens facing off against three knights and a pawn, liberating chess from its conventional openings and predictability.

We achieve the extraordinary with a version of chess that demands deeper thought. More. As you progress, the difficulty ramps up with AI opponents controlling prime pieces. It’s a delightful experience.

Perhaps the less social facets of board games make computers more beneficial to us. The only individuals who converse while playing chess are the villains from films. I wonder if a microtransaction Chess Go! will surface—there’s likely some entity trying to ruin everything out there.

Source: www.theguardian.com

Elon Musk Invests Close to $1 Billion in Tesla Shares to Increase Control | US News

Elon Musk, the CEO of Tesla, has acquired nearly $1 billion worth of shares in the electric vehicle maker.

Following this announcement, Tesla’s stock surged by over 8% in pre-market trading on Monday.

As Tesla shifts its focus from solely electric vehicle production to becoming a technology powerhouse, the company is racing to achieve ambitious goals in Robotaxis, Artificial Intelligence, and Robotics. By December, Musk held approximately 13% of the company, according to data from LSEG.

On Friday, Musk purchased 2.57 million shares in open market transactions, with prices ranging from $372.37 to $396.54 per share.

Tesla’s shares increased by over 7% on Friday, building on strong gains from the previous session. Despite a year-to-date decline of around 2%, the stock is poised to achieve profits for the third consecutive session if pre-market trends hold steady.

Musk has persistently sought greater ownership interests, enhanced voting power at Tesla, and has threatened to develop AI and robotics ventures outside of Tesla unless he secures 25% voting power.

Earlier this month, Tesla’s board proposed a trillion-dollar compensation package for Musk, even amidst challenges posed by intense competition and declining electric vehicle demand.

On Friday, Robin Denholm, the board chair, downplayed concerns that Musk’s political engagements were negatively impacting sales, asserting that the billionaire had returned to being “front and center” within the company following his time in the White House.

Musk’s political involvement and public disagreements with Donald Trump have placed pressure on the company’s stock this year, raising investor concerns about potential distractions and declines in sales.

Source: www.theguardian.com

Dozens of US Beaches to Close by July 4th Due to Fecal Bacteria Contamination

Right before the extended Independence Day weekend, numerous beaches nationwide were closed due to high levels of harmful bacteria, accompanied by health advisories. The issue stems from fecal waste, a prevalent summer concern in both freshwater and ocean areas, which can lead to gastrointestinal illnesses and skin infections.

At least six states have enacted beach or lake closures and advisories. Testing revealed unsafe levels of fecal bacteria in various waterways. In Massachusetts, nearly 20 beaches are closed due to elevated bacterial counts. In New York, four beaches have been shut down. Illinois has issued at least eight advisories over recent weeks. Los Angeles County announced 8 ocean water quality advisories as of Tuesday. Three beaches in Michigan have been closed.

The bacteria posing threats to summer swimmers include E. coli and enterococcus. Contamination may result from sewage, fertilizers, or stormwater runoff. E. coli is often found in freshwater environments, while enterococcus can develop in both oceans and freshwater.

Edward Dudley, the director of Penn State’s E. coli reference center, noted that testing for swimming waters is a standard practice, as are the subsequent closures.

Antalpreet Jutla, an associate professor of environmental engineering science at the University of Florida, mentioned that beach closures tend to occur during the summer months when surface temperatures rise and bacteria can proliferate more easily. However, he emphasized that various factors — including human activities, temperature, and water movement — can influence bacterial growth.

Jutla also reiterated that closures due to fecal bacteria are quite common.

In North Carolina, authorities cautioned about a cyanobacteria algae bloom in Lake Norman, advising people to keep children and pets away from water that appears bright green, blue, or scummy. Unlike fecal bacteria, cyanobacteria are one of the primary causes of algae in freshwater environments, as noted by the Centers for Disease Control and Prevention. Research indicates that climate change may cause more frequent cyanobacteria blooms.

The Environmental Protection Agency has established guidelines for safe levels of fecal bacteria and recommends water quality and monitoring standards. Some Illinois beaches undergo testing every two weeks.

“Generally, the higher the level, the greater the risk,” Dudley stated.

Fecal waste can result in numerous harmful diseases, but experts are increasingly concerned about the recent rise in another dangerous bacterium, Vibrio.

Vibrio is a potentially lethal bacterium responsible for similar beach closures in the recent past. These carnivorous bacteria flourish in warm coastal waters. Jutla noted that he has observed Vibrio gradually migrating northward across the US. Testing for this bacterium varies based on specific conditions and concentration thresholds.

“While trends nationwide seem unusual at the moment, it’s something we’re particularly worried about: its presence in coastal waters,” Jutla remarked regarding Vibrio.

The deadly V. vulnificus is a rare type of bacterium, yet infections have surged in recent years due to warmer seawater along the US East Coast.

Source: www.nbcnews.com

Astronomers Discover Massive Molecular Hydrogen Clouds Close to the Solar System

Recently identified by astronomers, this newly discovered molecular cloud is one of the largest structures in the sky and is among the closest to the Sun and Earth ever detected.

The EOS Cloud is situated at the boundary of your local bubble—a region populated by large gases within the solar system. Image credits: Thomas Müller, HDA & MPIA/Thavisha Dharmawardena, NYU.

Molecular clouds consist of gas and dust, primarily composed of hydrogen, the most prevalent molecule in the universe and essential for the formation of all known stars and planets.

Additionally, these structures harbor other molecules, including carbon monoxide.

Traditional detection methods for molecular clouds often involve wireless and infrared observations, which readily capture the chemical signatures of carbon monoxide.

However, Blakely Burkhart, an astrophysicist from Rutgers University in New Brunswick, and his team took a different approach.

“This is the first molecular cloud discovered by directly seeking out the distant ultraviolet radiation of molecular hydrogen,” Dr. Burkhart stated.

“Our data revealed glowing hydrogen molecules detected through fluorescence in distant ultraviolet light. This cloud truly shines in the dark.”

The new molecular cloud, named EOS, was located approximately 300 light-years from Earth and can be viewed here.

It resides at the periphery of a local bubble, a region filled with gases surrounding the solar system.

Astronomers estimate that these crescent clouds are immense, spanning about 40 months across the sky and having a mass approximately 3,400 times that of the Sun.

They are projected to dissipate within 6 million years.

According to the research team, the EOS cloud poses no threat to Earth or the solar system.

Its proximity offers a unique opportunity to explore the properties of structures within the interstellar medium.

The interstellar medium, composed of gas and dust, fills the space between stars in the galaxy and is a key source for new star formation.

“When you look through a telescope, you observe the solar system in its formative phase, but the exact process remains unclear,” Dr. Burkhart explained.

“The discovery of EOS is thrilling because it allows us to directly measure how molecular clouds form and dissolve, as well as how galaxies transform interstellar gas and dust into stars and planets.”

The EOS Cloud was identified using data from the FIMS-Spear Far-ultraviolet spectrograph aboard the Korean satellite STSAT-1.

“Utilizing distant UV fluorescence technology could redefine our understanding of the interstellar medium, uncover hidden clouds across the galaxy, and even push our exploration further back to the very edge of the universe’s inception.”

The findings are reported in a study published today in the journal Nature Astronomy.

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B. Burke Hart et al. Dark molecular clouds near local bubbles revealed via H2 fluorescence. Nature Astronomy. Published online on April 28, 2025. doi:10.1038/s41550-025-02541-7

Source: www.sci.news

Lucy shares breathtaking images from close encounter with asteroid Donald Johansson

The asteroid called Donald Johansson was captured by NASA’s Lucy spacecraft during a flyby on April 20, 2025. On the closest approach, the spacecraft was at a distance of 960 km (600 miles).

https://www.youtube.com/watch?v=nyoezs04rhc

Donald Johansson is a carbonaceous asteroid located in the inner region of the main asteroid belt.

It was discovered by American astronomer Shertebas at the Siding Spring Observatory on March 2, 1981.

Donald Johansson had previously observed a large brightness variation over a 10-day period, so some of the expectations of members of the Lucy team were confirmed when the first image showed what appeared to be an elongated contact binary.

However, researchers were surprised by the strange shape of the narrow neck that connects the two leaves.

“The asteroid Donald Johansson has an incredibly complex geology,” says Dr. Hallevison, principal investigator at Lucy, a researcher at the Southwest Research Institute.

“A detailed study of complex structures reveals important information about the building blocks and collision processes that formed planets in the solar system.”

This image of the asteroid Donald Johansson was taken by Lucy Long Range Reconnaissance Imager (l’lorri) by the closest approach from a 1,100 km (660 miles) range. Image credits: NASA/GODDARD/SWRI/JOHNS HOPKINS APL/NOIRLAB.

From a preliminary analysis of the first available images collected by the spacecraft L’Lorri Imager, Donaldjohanson appears to be larger than originally estimated.

“In this first set of high-resolution images returned from the spacecraft, we cannot see a perfect asteroid because the asteroid is larger than the imager’s field of view,” the scientists explained.

“It takes up to a week for the team to downlink the rest of the encounter data from the spacecraft. This dataset provides a more complete image of the overall shape of the asteroid.”

“The NASA Headquarters researcher, Dr. Tom Staller, a scientist with the Lucy Program,” said:

“When Lucy reaches the Trojan asteroid, the chances that she may truly open a new window into the history of our solar system are immeasurable.”

Lucy’s first asteroid flyby target, Dinkinesch and Donald Johansson, are not the main science targets of the mission.

As planned, Dinkinesh Flyby was testing the mission’s system, but the encounter was a full dress rehearsal, with the team conducting a series of close observations to maximize data collection.

Data collected by Lucy’s other scientific instruments, the L’Ralph Color Imager and infrared spectrometers and L’TES thermal infrared spectrometers, will be acquired and analyzed over the next few weeks.

Lucy spacecraft will spend most of the rest of 2025 traveling through the main asteroid belt.

Lucy will encounter the mission’s first major target, the Jupiter Trojan Novel, in August 2027.

Source: www.sci.news

Strange events occurring in close proximity to a neighboring galaxy

The little Magellan Clouds (SMCs), a dwarf galaxy that is orbiting near our own Milky Way, appear to satisfy a rather dramatic ending.

That is the conclusion of a new study published in Astrophysical Journal Supplement Series astronomers have tracked over 7,000 large stars in SMC. Each one is more than eight times the size of our sun.

These star heavyweights burn a short life that lives bright and fast, providing clues about their own movements as well as their turbulent gas clouds.

And what researchers found was impressive. This former codbone universe’s neighbor is torn apart quite badly by the gravity of the large Magellan Cloud (LMC).

The milky stripes of this star-filled sky are two d-star galaxies visible only from the southern hemisphere – here is a small Magellan cloud photographed above the Delusional Observatory of Eso in Chile. -ESO/j. Corosimo

“SMCs are interacting galaxies that are coupled to the LMC by gravity.” Satoya Nakano the first author of the study said BBC Science Focus. “The stars on the side of the SMC near the LMC experience stronger gravity and are moving towards the LMC, but the stars experience even weaker pulls.”

This gravitational tug of war slowly pulls the SMC apart with possible nudges from our own Milky Way approaching about 200,000 light years away.

So why is this important?

For one, the team discovered that the SMC was not rotating the way astronomers had assumed. Spiral galaxies like our own usually rotate with stars and gas processing around the central axis. But not all galaxies are – and SMC may be one of them.

“The question of when rotational motion appears in galaxies is a very interesting topic among researchers,” Nakano said.

“SMC was considered a rotating galaxy, but this study shows that it is not actually rotating. It suggests that if even a nearby galaxy like SMC is misinterpreted, it requires much more attention when assessing galaxy rotations further away.”

The colours of the arrows represent the direction of the movement of the giant stars in the SMC. Compared to the LMC at the bottom left of the image, most red arrows show movement towards the LMC, while most light blue arrows show movement away from the LMC, suggesting that they are being pulled apart. – Satoya Nakano

And SMC is very close by space standards. Just 200,000 light years away, it is more than ten times closer to Andromeda, the nearest largest galaxy.

The lack of rotation not only changes our understanding of SMC’s structure, but also allows us to discard estimates of mass.

“The SMC is not rotating, so historical estimates of its mass may be incorrect.” Professor Tahara the author of another study said BBC Science Focus.

“The estimates of mass were born from previously estimated rotational motions. However, if these are not reliable, the estimates need to be revised. Without this, we cannot predict the future existence of SMC.”

Nakano and Tahara hope that detailed simulation observations to model the fate of the galaxy open the door. But for now, the future appears to be far from bright.

About our experts

Satoya Nakano is a doctoral candidate from the Faculty of Physics, Graduate School of Science, Nagoya University, Japan.

Tahara Sword He is an associate professor at Nagoya University Graduate School of Science, Japan. His research is Publications of the Japanese Astronomical Association, Astrophysical Journal and Astronomy and Astrophysics.

read more:

  • How do you know that the Milky Way is a spiral galaxy?
  • How many galaxies are there in the universe?
  • How Alien Galaxies Will Quickly Collide Ours

Source: www.sciencefocus.com

Binary star system found in close proximity to the central black hole of the Milky Way galaxy

Using data from ESO’s Very Large Telescope (VLT) and the Keck Telescope, astronomers detected a binary star system in the S star cluster near Sagittarius A*, the supermassive black hole at the center of the Milky Way. I discovered it. This is the first time that a binary star has been discovered near a supermassive black hole.

This image shows the location of binary star D9 orbiting Sagittarius A*, the supermassive black hole at the center of the Milky Way. Image credit: ESO / Peißker et al. / S. Guizard.

Sagittarius A* is orbited by fast stars and dusty objects collectively known as the S cluster.

Binary star systems (two stars gravitationally bound to each other around a common center of mass) are predicted to exist within the S cluster, but have not been detected so far.

Previous studies have suggested that such stars are unlikely to be stabilized by their interactions with Sagittarius A*.

“Black holes are not as destructive as we think,” says Florian Peisker, an astronomer at the University of Cologne.

“Our findings show that some binaries can temporarily thrive even under disruptive conditions.”

The newly discovered binary star, named D9, is estimated to be just 2.7 million years old.

Due to the strong gravity of the nearby black hole, it will probably merge into a single star within just a million years, a very short time for such a young system.

“This only provides a short window on the cosmic timescale for observing such binary star systems, but we succeeded,” said Dr. Emma Bordier, also from the University of Cologne. Ta.

“The D9 system shows clear signs of gas and dust surrounding the star, suggesting it may be a very young system that must have formed near a supermassive black hole. ” said Dr. Michal Zajacek. Astronomer at Masaryk University and the University of Cologne.

The most mysterious of the S clusters are the G objects, which behave like stars but look like clouds of gas and dust.

It was while observing these mysterious objects that the research team discovered a surprising pattern in D9.

“This result sheds new light on what the mysterious G-objects are,” the authors said.

“They may actually be a combination of binaries that have not yet merged and leftover material from stars that have already merged.”

“Planets often form around young stars, so this discovery allows us to speculate about their existence,” Dr. Pisker said.

“It seems like it’s only a matter of time before planets are detected at the center of the galaxy.”

a paper This discovery was published in today’s magazine nature communications.

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F. Peisker others. 2024. A binary star system in the S star cluster near the supermassive black hole Sagittarius A*. Nat Commune 15, 10608; doi: 10.1038/s41467-024-54748-3

Source: www.sci.news

Astronomers find scorching-hot Neptune close to TOI-3261

Orbit of newly discovered exoplanet TOI-3261 (also known as TIC 358070912) is an inactive main sequence star located 300 parsecs (978.5 light years) away in the constellation Hydra.

Artist's concept of the super-hot Neptunian exoplanet TOI-3261b. Image credit: NASA/JPL-Caltech/K. Miller, Caltech & IPAC.

The radius of this newly discovered exoplanet, named TOI-3261b (TIC 358070912b), is 3.82 Earth's radius.

Its mass is 30.3 times that of Earth, more than twice the median mass of Neptune-sized planets in longer orbits.

To determine these properties, astronomer Emma Nabby from the University of Southern Queensland and her colleagues used data from NASA's Exoplanet Survey Satellite (TESS), the Las Cumbres Observatory's Global Telescope, and the ESPRESSO and HARPS instruments. I used

“In our measurements, TOI-3261b is exactly hot neptune desert “The planets are so rare that their rarity evokes images of desolate landscapes,” the astronomers said in a statement.

“This type of exoplanet is similar in size and composition to our own Neptune, but it orbits very close to its star.”

The planet orbits its parent star, TOI-3261, every 21 hours.

Such a narrow orbit has so far allowed the planet to belong to the same group as only three other ultrashort-period, high-temperature Neptunes: LTT-9779b, TOI-849b, and TOI-332b.

“TOI-3261b has proven to be an ideal candidate for testing new computer models of planet formation,” the researchers said.

“One reason hot Neptunes are so rare is that it's difficult to maintain a thick gaseous atmosphere in the immediate vicinity of the star.”

“Because stars are massive, they exert a large gravitational force on surrounding objects and can strip away layers of gas surrounding nearby planets.”

“It also releases a lot of energy and blows away the gas layer.”

“Both of these factors mean that a hot Neptune like TOI-3261b may have started out as a much larger Jupiter-sized planet and then lost most of its mass.”

The TOI-3261 system is about 6.5 billion years old, and the planet began as a much larger gas giant, the researchers said.

“But it likely lost mass in two ways: by photoevaporation, where energy from the star causes gas particles to dissipate, and by gravity from the star, which strips layers of gas from the planet. tidal separation,” the scientists said.

“It's also possible that the planet formed further away from the star, where both of these effects would be less strong and it would be able to maintain an atmosphere.”

“The planet's remaining atmosphere is one of its most interesting features and will likely invite further atmospheric analysis, perhaps helping to elucidate the formation history of this hot Neptunian desert dweller.”

“TOI-3261b's density is about twice that of Neptune, indicating that the lighter parts of the atmosphere have been removed over time, leaving only the heavier components,” the researchers added.

“This suggests that the planet must have started out with a variety of elements in its atmosphere, but at this stage it's difficult to know exactly what they are.”

This finding is reported in the following article: paper Published in astronomy magazine.

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Emma Naby others. 2024. Survival in the Hot Neptunian Desert: Discovery of the ultrahot Neptune TOI-3261b. A.J. 168, 132; doi: 10.3847/1538-3881/ad60be

Source: www.sci.news

Next week, the JUICE spacecraft might be visible during a close flyby of Earth.

JUICE spacecraft may be visible from Southeast Asia during unprecedented operation

European Space Agency

The Jupiter Icy Moons Explorer (JUICE) will land on Earth in what the European Space Agency (ESA) calls a “double world first.” It is scheduled to fly past Earth and the Moon on August 19 and 20, the first of several complex maneuvers along a looping path to Jupiter. You may be able to see the spacecraft in the sky as it speeds past.

JUICE was launched on April 14, 2023, and has been orbiting the Sun almost parallel to Earth ever since. But on August 19, its journey will start to get interesting: it will pass within 700 km of the Moon's surface, slowing down slightly using a method called gravity assist. The next day, it will drop to less than 7,000 km above Earth's surface, curving its orbit even further. That's when eagle-eyed astronomy fans in Southeast Asia may get a glimpse of the spacecraft.

All of this is necessary because if JUICE were to fly in a straight line to Jupiter, it would need more than 60,000 kilograms of fuel to get there, and even more to slow down and enter orbit once there. With the entire spacecraft's mass unfueled at 2,420 kilograms, this just isn't feasible. Instead, upcoming Earth-Moon flybys will send the spacecraft to Venus, where it will begin to accelerate, then fly past Earth twice to get it just fast enough to reach Jupiter in 2031.

The first maneuver may be the most complex of the entire mission, as JUICE must pass precise points relative to both the Earth and the Moon to en route to Venus. “It's like going through a very narrow corridor very fast, with the accelerator at full speed with only millimeters of clearance on the side of the road,” said ESA's Ignacio Tanco in statementA dual Earth-Moon flyby has never been attempted before, nor has a dual gravity assist been performed.

If all goes well, JUICE will not only head to Venus and then Jupiter, but it will also perform the first major tests of its scientific instruments. For some of the probes, this will be their only chance to observe the planet's surface and iron out any kinks before they reach orbit around Jupiter and begin their mission to search for hints of possible life on the planet's giant moons.

topic:

Source: www.newscientist.com

Academics now pay close attention to details in the workplace

Paying attention to small details

“Academics are often accused of ‘obsessing over the details,'” David Taylor told Feedback magazine. “This year my team and I have managed to do just that. We have built a machine that can literally split a single hair from end to end. This is the first time that anyone has been able to split a hair in a lab in a controlled environment and quantify the phenomenon. Were you planning any exciting beauty treatments like coloring or curling your hair? You’ll have to wait and see if this will cause split ends.”

He and his team called the adventure “Hair-splitting biomechanics“, published in Interface Focus.

This is based on research done in the 1980s by Y. K. Kamath and H.-D. Weigman, who sought to take a closer look at what happens when a hair splits.

in Journal of Applied Polymer ScienceFractographic analysis of human hairKamath and Weigman calmed their excitement and stated, “Electron microscopic evidence suggests that fracture propagation occurs via secondary cracks generated as a result of stress concentrations that build up around the primary crack.”

Water from the wreckage

Brazilian researchers have been searching outside the cemetery for the remains of people buried there. Their main question is whether the decaying bodies are sending a foul stench into the area’s deep groundwater. Elias Saba and his colleagues have summed it all up in a book with a macabre, geeky title: “The Deadly Sinisters: The Secrets of the Dead.”Assessing the impact of cemeteries on groundwater using multivariate analysis” “.

The team collected data from three “monitoring wells” dug at the cemetery and compared it with data from the local sewer company about water in nearby household cisterns. Multivariate analysis provided both good and not-so-good news.

The researchers explain that the soil, both inside and outside the cemetery, absorbs most of the problematic waste from the bodies, “preventing surface contaminants from reaching the aquifer.” That’s a good thing. But the problem is that water samples taken in areas outside the cemetery do not meet Brazil’s drinking water standards.

Grandma drinking alcohol

Ancestral water resources are not a new issue. Perhaps the most attention on this issue came in 2008. Journal of Environmental Health.

Reader Russ Hodge responded to the feedback with:Drinking Grandma: The Problem with Embalming” ,” by attorney Jeremiah Chiapelli and Ted Chiapelli, a health sciences professor at Western Carolina University in North Carolina.

The Chiappellis explain: “Modern embalming involves replacing organic blood with a variety of toxic and carcinogenic chemicals, particularly formaldehyde. The embalmed body is then buried underground, but even when placed in a coffin, bodily fluids inevitably leak into groundwater. The reasons embalming was first undertaken, and the rationale for the continued practice, do not justify the potential public health and environmental risks posed by embalming.”

The Chiappellis also talk about research done by others about why so many people in the U.S. choose embalming: “In states that require funeral directors to be embalming technicians or have embalming facilities, cremation rates have decreased due to funeral director solicitation.”

settlement

Nothing livens up the social atmosphere at a strange pub like axe throwing, but the sport can pose dangers for some of those who approach it in a obliging, professional manner.

According to researchers Kusha Dabar, Arthur Jeng, and Suzanne Donovan, one such risk factor is blastomycosis, a fungal disease that “manifests as a pulmonary disease” but can also affect the skin, bones, and genitourinary tract.

For more details, please see the three people’s study “Criticism of endemic diagnosis: disseminated blastomycosis due to a new occupational exposure” “.

The patient “worked at an axe-throwing factory after moving to Los Angeles,” and “his work involved cutting wood for customers.”

Dabber, Jenn and Donovan claim that the disease is “not routinely diagnosed” in Southern California. They say: Blastomyces The fungus was present in the wood before entering the patient’s body.

Telltale Title

Below are two titles recently added to our collection of feedback, “The Title Says All You Need to Know.”

The effect of wet underwear on thermoregulatory responses and thermal comfort in cold weather“”teeth, Ergonomics 1994.

and “The pain one may experience when executed in various ways“This probably surprised magazine readers. Sensing 1993.

If you’ve come across similarly impressive examples, please submit them along with citation details to Telltale titles, c/o Feedback.

Marc Abrahams is the founder of the Ig Nobel Prize ceremony and co-founder of the journal Annals of Improbable Research. He previously worked on unusual uses of computers. His website is Impossible.

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Source: www.newscientist.com

Spotting a harmless asteroid passing close to Earth this Saturday: What you need to know.

This weekend, there will be a passing asteroid near Earth, which poses no threat. With the right equipment and timing, you may be able to catch a glimpse of it.

The asteroid, known as 2024 MK, will be at its closest point to Earth on Saturday morning, passing at a distance about three-quarters of the way from Earth to the moon. It was first spotted two weeks ago by an observatory in South Africa and measures approximately 393 to 853 feet (120 to 260 meters) wide.

According to Davide Farnocchia, an asteroid expert at NASA’s Center for Near Earth Object Studies, smaller objects pass by Earth regularly. Asteroids of this size come close to Earth roughly every 25 years.

“We may witness this event a few times in our lifetime, but it’s not a common occurrence,” he noted.

The 7,579-foot (2,310-meter) asteroid made a safe pass near Earth on Thursday, but it was too distant to be visible without specialized telescopes.

To see the asteroid on Saturday, skywatchers will need small telescopes as it won’t be bright enough to be seen with the naked eye. It will move swiftly across the southern sky, making it challenging to spot.

Nick Moskovitz, an astronomer at Lowell Observatory, mentioned, “The asteroid will move rapidly through the star field.”

For the best chance of seeing the asteroid, observers in the Southern Hemisphere should look high overhead. People in the US may have better luck spotting it on Saturday night when it might be less bright, but easier to see without the sun’s glare.

If you miss this event, mark your calendars for April 13, 2029, when the asteroid Apophis will pass close to Earth and be visible to the naked eye from parts of Europe, Africa, and Asia.

Source: www.nbcnews.com

Unexpectedly large stellar-mass black hole spotted in close binary star system

Using data from ESA’s Gaia mission, astronomers discovered a nearby binary system of massive stars orbiting a dormant star-derived black hole over a period of 11.6 years. The black hole’s estimated mass (33 solar masses) is significantly larger than all known stellar-mass black holes in the Milky Way and within the mass range of extragalactic black holes detected by gravitational waves.

Locations of the first three black holes discovered in the Milky Way by ESA’s Gaia mission. Image credit: ESA/Gaia/DPAC.

The binary star system in question is named Gaia BH3 and is located 1,926 light-years from Earth in the constellation Aquila.

Also known as Gaia DR3 4318465066420528000, LS II +14 13, and 2MASS J19391872+1455542, it consists of an old, very metal-poor giant star and a dormant stellar-mass black hole.

Gaia BH3 is the third dormant black hole discovered by ESA’s interstellar mapping satellite Gaia.

“This is the kind of discovery that only happens once in a research career,” said Dr. Pasquale Panuzzo, an astronomer at the CNRS and the Paris Observatory.

“So far, black holes this large have only been detected in distant galaxies by the LIGO-Virgo-KAGRA collaboration, thanks to observations of gravitational waves.”

The average mass of the known stellar-origin black holes in our galaxy is about 10 times the mass of the Sun.

Astronomers face the pressing problem of explaining the origin of black holes as large as Gaia BH3.

Our current understanding of how massive stars evolve and die does not immediately explain how this type of black hole could be born.

Most theories predict that as massive stars age, a significant portion of their material is shed by powerful winds. Eventually, it will be partially blown into space when it explodes as a supernova.

The remainder of the core shrinks further, becoming either a neutron star or a black hole, depending on its mass.

It is extremely difficult to explain a core large enough to eventually become a black hole 30 times the mass of the Sun. But the clues to solving this mystery may lie very close to Gaia BH3.

The star, which orbits Gaia BH3 at about 16 times the distance between the Sun and Earth, is quite unusual and is an ancient giant that formed during the first two billion years after the Big Bang, when our galaxy began to form. It’s a star.

It belongs to the family of galactic stellar halos, which move in the opposite direction to the stars in the galactic disk.

Its orbit indicates that the star was probably part of a small galaxy, or globular cluster, that was swallowed up by the Milky Way more than 8 billion years ago.

This companion star contains almost no elements heavier than hydrogen or helium, indicating that the massive star that became Gaia BH3 may also have been extremely poor in heavy elements.

For the first time, the theory that the massive black holes observed in gravitational wave experiments were created by the collapse of primordial massive stars lacking heavy elements has been confirmed.

These early stars may have evolved differently from the massive stars we see in our galaxy today.

The composition of the companion star can also reveal the formation mechanism of this surprising binary system.

“We were surprised that the chemical composition of the companion star is similar to that seen in older, metal-poor stars in the Milky Way,” said Dr. Elisabetta Cuffo, an astronomer at the CNRS and the Paris Observatory.

“There is no evidence that this star was contaminated by material ejected from the supernova explosion of the massive star that became BH3.”

“This may suggest that the black hole acquired a mate from another star system for the first time after its birth.”

of the team paper be published in a magazine astronomy and astrophysics.

_____

P. Panuzzo other. (Gaia collaboration). 2024. Gaia astronomical measurements prior to release discovered a dormant black hole with the mass of 33 solar masses. A&A, in press. doi: 10.1051/0004-6361/202449763

Source: www.sci.news

Hubble photographs star-forming galaxies in close proximity

This stunning view of a pair of spiral galaxies called Arp 72 is a violent collision occurring in slow motion, according to the Hubble team.

This image shows Arp 72, a galaxy pair that includes NGC 5996 (a large spiral galaxy) and NGC 5994 (a small companion star in the lower left of the image). The color images were taken in the visible and infrared regions of the spectrum using Hubble's Altitude Survey Camera (ACS) and the Dark Energy Camera (DECam) mounted on NSF's Victor M. Blanco 4-meter Telescope. created from separate exposures. Cerro Toloro Interamerican Observatory in Chile. Four filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: NASA / ESA / Hubble / L. Galvany / J. Dalcanton / Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA.

of alp 72 system It is located approximately 160 million light years away in the constellation Serpens.

Arp 72 is made up of a strangely shaped spiral galaxy NGC 5996 and smaller, less deformed spiral galaxies NGC5994.

NGC 5996 was first discovered on March 21, 1784 by German-British astronomer William Herschel.

NGC 5994 is discovered Written by Irish engineer and astronomer Bindon Stoney on March 9, 1851.

“The centers of these galaxies are approximately 67,000 light-years apart from each other,” the Hubble astronomers said.

“Furthermore, the distance between galaxies at their closest points is even smaller, close to 40,000 light-years.”

“This may still sound vast, but from a galactic separation perspective, it's really, really cozy!”

“For comparison, the distance between the Milky Way and its closest independent galactic neighbor Andromeda is about 2.5 million light-years.”

“Alternatively, the distance between the Milky Way and its largest and brightest satellite galaxy, the Large Magellanic Cloud, is about 162,000 light-years.”

“Given this and the fact that NGC 5996 is roughly comparable in size to the Milky Way, it is not surprising that NGC 5996 and NGC 5994 are interacting,” the researchers said.

“In fact, this interaction may be responsible for distorting the helical shape of NGC 5996 and apparently pulling it toward NGC 5994.”

“That's also… Formation of very long and faint tails of stars and gas It curves away from NGC 5996 to the upper right of the image. ”

“This tidal tail is a common phenomenon that appears when galaxies approach each other, as seen in some Hubble images.”

Source: www.sci.news

‘Devil’s Comet’ makes close approach to the sun, possibly visible during solar eclipse

The Devil’s Comet, known for its occasional explosions, is currently visible in the night sky, and fortunate observers may catch a glimpse of it during the eagerly awaited solar eclipse next month.

Comet 12P/Ponsbrooks earned the nickname “Devil’s Comet” after an eruption last year left behind two distinctive trails of gas and ice resembling devil’s horns.

From the Northern Hemisphere, the comet is currently visible with binoculars or telescopes. As it moves through the inner solar system and approaches its closest point to the sun in mid-April, it may become visible to the naked eye by the end of the month.

Comets typically consist of a core of dust, gas, and ice surrounded by a bright gas cloud called a coma. These objects are remnants from the formation of the solar system and can be several miles wide, according to NASA.

The core of a comet can heat up due to sunlight and solar radiation, sometimes leading to explosive events, as seen with Comet 12P/Ponsbrooks. Observers in the Northern Hemisphere can currently see the comet in the western-northwestern sky in the evening.

The comet is expected to brighten towards the end of the month and, under clear and dark conditions, may remain visible until early May. If the comet experiences significant flares in the coming weeks, it could be visible during the total solar eclipse on April 8 along the path stretching from northeast Texas to Maine.

Despite uncertainties surrounding rare synchronistic events, there is a good chance of spotting the comet on its own in the evening sky. Comet 12P/Pons-Brookes was first discovered in 1812 by French astronomer Jean-Louis Pons and later observed in 1883 by British-American astronomer William Brooks. Due to its 71-year orbit around the sun, sightings of this comet are infrequent.

Source: www.nbcnews.com

Capitol Hill raises concerns over Microsoft’s close AI partnership with China

US lawmakers are calling on Microsoft to foster a positive relationship with China in the development of AI technology, despite recent efforts by Microsoft’s president, Brad Smith, to increase cooperation with the US adversary. During a meeting with Chinese Minister of Commerce Wang Wentao, Smith expressed the company’s eagerness to contribute to the digital transformation of China’s economy, with China looking forward to Microsoft’s potential collaboration in AI development.

However, this has raised concerns among US lawmakers and commentators, who fear that Microsoft’s extensive presence in China could pose a national security risk. Senator Josh Hawley has pushed back against Microsoft’s partnership with China, emphasizing the Chinese government’s desire for AI supremacy and the potential risks associated with such collaboration.

Rep. Mike Gallagher also expressed similar concerns, calling for stronger export controls for AI and other critical technologies due to the Chinese government’s intentions for sinister use of advanced AI tools.

The US-China relationship has recently deteriorated, and concerns over national security risks associated with Microsoft’s collaboration have been heightened. Microsoft CEO Satya Nadella emphasized the company’s primary focus on global markets excluding China, distancing the company from doing business with the Chinese government. However, the company has stressed its commitment to responsibly and ethically developing AI technology in China.

Despite heightened scrutiny and concerns, Microsoft continues to expand its operations in China, facing criticism from US lawmakers over potential exploitation of its technology by the Chinese government. Other US tech companies, such as Google and Meta, have pulled back from the region due to disputes with the Chinese government and increased US scrutiny.

Microsoft’s cooperation with China has raised concerns of technology transfers and potential security risks, as China has gained access to sensitive information about AI products and has been accused of misusing advanced technologies for human rights abuses.

Overall, Microsoft’s presence in China and its efforts to collaborate in AI development have sparked concern among US lawmakers and commentators, who fear the potential national security risks associated with such partnerships.

Source: nypost.com

Solar Activity Brings NASA’s NEOWISE 10-Year Mission to a Close



NEOWISE Mission

This artist’s concept shows the Wide Field Infrared Surveyor (WISE) spacecraft orbiting the Earth. The NEOWISE mission will find and characterize asteroids.
Credit: NASA/JPL-California Institute of Technology

Infrared space telescopes searching for asteroids and comets have collected vast amounts of observations, but are now at the mercy of the sun, which is accelerating their demise.

NASA’s Neowise It’s been a busy 10 years. Since its resumed mission began on December 13, 2013, the space telescope has discovered once-in-a-lifetime comets, observed more than 3,000 near-Earth objects, strengthened international planetary defense strategies, and It has helped other NASA missions rendezvous with distant space. asteroid. This is just a partial list of achievements.

But all good things must come to an end. Solar activity is pushing NEOWISE (short for Near-Earth Object Wide-field Infrared Survey Explorer) out of orbit. By early 2025, the spacecraft is expected to have fallen far enough into Earth’s atmosphere that it will become unusable. Eventually it will re-enter the atmosphere and burn up completely.

Approximately every 11 years, the Sun goes through a cycle of increasing activity, peaking during a period called solar maximum. Explosive events such as solar flares and coronal mass ejections will become more frequent, heating the Earth’s atmosphere and causing it to expand. Atmospheric gases increase the drag on satellites as they orbit the Earth, slowing them down. Now, as the Sun approaches its next maximum, NEOWISE will no longer be able to maintain its orbit above the atmosphere.

Comet C/2020 F3 NEOWISE is a composite of several heat-sensitive infrared images taken by NASA’s Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) mission on March 27, 2020. Appears as a blurry red dot.
Credit: NASA/JPL-California Institute of Technology

“The mission has been planning for this day for a long time. After several years of lull, the sun is waking up again,” said NEOWISE co-principal investigator and researcher at the California Institute of Technology in Pasadena, California. said Joseph Masiello, a scientist with the organization IPAC. “With us at the mercy of solar activity and no means of staying in orbit, NEOWISE is now slowly spiraling back to Earth.”

wise beginnings

The past decade has meant a second life for the spacecraft. Managed by NASA’s Jet Propulsion Laboratory in Southern California, NEOWISE is part of another mission launched in 2009, the Wide-Field Infrared Surveyor (wise). Data from WISE and NEOWISE is used to study distant galaxies, cold stars, and explosions. white dwarf Stars, gas-emitting comets, near-Earth asteroids, etc.

In 2010, WISE achieved its scientific goal of conducting an all-sky infrared survey with far greater sensitivity than previous surveys. WISE mission also discovered tens of millions of actively feeding supermassive black holes across the sky.through disc detective In this project, citizen scientists used WISE data to find circumstellar disks, which are clouds of gas, dust, and debris that rotate around stars.

Infrared wavelengths, which are invisible to the naked eye, are emitted by warm objects. To ensure that the heat generated by WISE itself does not interfere with observations in infrared wavelengths, the spacecraft relied on cryogenic coolant. NASA put the spacecraft into hibernation in February 2011 after it ran out of coolant and WISE mapped the sky twice.

Without the coolant, space telescopes could no longer observe the coldest objects in the universe, but they could still see near-Earth asteroids and comets heated by the sun. So NASA restarted the spacecraft in 2013 with a more specialized role in mind. The goal is to support planetary defense efforts by investigating and studying objects that may wander into Earth’s orbit and pose a potential collision hazard.

In addition to relying on missions to explore these objects, astronomers use that data to understand the object’s size, albedo, or how much sunlight its surface reflects, and the composition of its structure. You can also collect clues about the minerals and rocks you find.

“NEOWISE demonstrates the importance of deploying infrared space exploration telescopes as part of NASA’s planetary defense strategy while also monitoring objects in our solar system and beyond,” said lead researcher Amy, from the University of Arizona in Tucson. Mainzer said. .

Mainzer also leads NASA’s future plans. NEO surveyor, built on the NEOWISE tradition. The next generation of infrared space telescopes will search for celestial objects close to the Earth, such as dark asteroids and comets that do not reflect much visible light, or objects that approach the Earth from the direction of the sun. Sun. The launch is scheduled for 2027. JPL-Managed missions will also explore objects known as Earth Trojans – asteroids that lead or follow our planet’s orbit. The first one is wise discovery In 2011.

Comet NEOWISE and beyond

Since becoming NEOWISE, the mission has scanned the entire sky more than 20 times and made 1.45 million infrared measurements on more than 44,000 Solar System objects. This includes over 3,000 near-Earth objects, 215 of which were discovered by his NEOWISE. Data from the mission helped refine the orbits of these objects, while also measuring their sizes.

Its strength is in revealing the characteristics of asteroids near the Earth. In 2021, NEOWISE became a key component of an international planetary defense exercise focused on the dangerous asteroid Apophis.

The mission also discovered 25 comets, including long-period comet C/2020 F3 (NEOWISE). The comet was a dazzling object visible in the Northern Hemisphere for several weeks in 2020, making it the first comet to be visible to the naked eye since 2007, when Comet McNaught was primarily visible in the Southern Hemisphere.

Future researchers will use WISE in 2010, long after observations were made to characterize the asteroid Dinkinesh, in support of NASA’s Lucy mission before the October 2023 encounter. Just as we used the data, we will continue to rely on the vast archive of NEOWISE observations to make new discoveries.

“This is a bittersweet moment. We are sad to see this pioneering mission come to an end, but we know there are even more treasures hidden in the survey data,” Masiello said. “NEOWISE has a vast archive that covers a very long period of time and will inevitably advance the science of the infrared universe long after the spacecraft leaves.”

Mission details
NEOWISE and NEO Surveyor are part of NASA’s Planetary Defense Coordination Office (PDCO) at NASA Headquarters in Washington. The NASA Authorization Act of 2005 directs NASA to discover and characterize at least 90% of near-Earth objects larger than 140 meters (460 feet) in diameter that come within 30 million miles (48 million kilometers) of Earth’s orbit. did. An object of this size could cause significant damage to the region, and it would be even worse if it crashed into Earth.
JPL manages and operates PDCO’s NEOWISE mission within the Science Mission Directorate. The Astrodynamics Laboratory in Logan, Utah, built the scientific instrument. Ball Aerospace & Technologies of Boulder, Colorado, built the spacecraft. Scientific data processing will take place at IPAC at the California Institute of Technology. Caltech manages JPL for NASA.



Source: scitechdaily.com