The purpose of this blog is the creation of an open, international, independent and free forum, where every UFO-researcher can publish the results of his/her research. The languagues, used for this blog, are Dutch, English and French.You can find the articles of a collegue by selecting his category. Each author stays resposable for the continue of his articles. As blogmaster I have the right to refuse an addition or an article, when it attacks other collegues or UFO-groupes.
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Deze blog is opgedragen aan mijn overleden echtgenote Lucienne.
In 2012 verloor ze haar moedige strijd tegen kanker!
In 2011 startte ik deze blog, omdat ik niet mocht stoppen met mijn UFO-onderzoek.
BEDANKT!!!
Een interessant adres?
UFO'S of UAP'S, ASTRONOMIE, RUIMTEVAART, ARCHEOLOGIE, OUDHEIDKUNDE, SF-SNUFJES EN ANDERE ESOTERISCHE WETENSCHAPPEN - DE ALLERLAATSTE NIEUWTJES
UFO's of UAP'S in België en de rest van de wereld Ontdek de Fascinerende Wereld van UFO's en UAP's: Jouw Bron voor Onthullende Informatie!
Ben jij ook gefascineerd door het onbekende? Wil je meer weten over UFO's en UAP's, niet alleen in België, maar over de hele wereld? Dan ben je op de juiste plek!
België: Het Kloppend Hart van UFO-onderzoek
In België is BUFON (Belgisch UFO-Netwerk) dé autoriteit op het gebied van UFO-onderzoek. Voor betrouwbare en objectieve informatie over deze intrigerende fenomenen, bezoek je zeker onze Facebook-pagina en deze blog. Maar dat is nog niet alles! Ontdek ook het Belgisch UFO-meldpunt en Caelestia, twee organisaties die diepgaand onderzoek verrichten, al zijn ze soms kritisch of sceptisch.
Nederland: Een Schat aan Informatie
Voor onze Nederlandse buren is er de schitterende website www.ufowijzer.nl, beheerd door Paul Harmans. Deze site biedt een schat aan informatie en artikelen die je niet wilt missen!
Internationaal: MUFON - De Wereldwijde Autoriteit
Neem ook een kijkje bij MUFON (Mutual UFO Network Inc.), een gerenommeerde Amerikaanse UFO-vereniging met afdelingen in de VS en wereldwijd. MUFON is toegewijd aan de wetenschappelijke en analytische studie van het UFO-fenomeen, en hun maandelijkse tijdschrift, The MUFON UFO-Journal, is een must-read voor elke UFO-enthousiasteling. Bezoek hun website op www.mufon.com voor meer informatie.
Samenwerking en Toekomstvisie
Sinds 1 februari 2020 is Pieter niet alleen ex-president van BUFON, maar ook de voormalige nationale directeur van MUFON in Vlaanderen en Nederland. Dit creëert een sterke samenwerking met de Franse MUFON Reseau MUFON/EUROP, wat ons in staat stelt om nog meer waardevolle inzichten te delen.
Let op: Nepprofielen en Nieuwe Groeperingen
Pas op voor een nieuwe groepering die zich ook BUFON noemt, maar geen enkele connectie heeft met onze gevestigde organisatie. Hoewel zij de naam geregistreerd hebben, kunnen ze het rijke verleden en de expertise van onze groep niet evenaren. We wensen hen veel succes, maar we blijven de autoriteit in UFO-onderzoek!
Blijf Op De Hoogte!
Wil jij de laatste nieuwtjes over UFO's, ruimtevaart, archeologie, en meer? Volg ons dan en duik samen met ons in de fascinerende wereld van het onbekende! Sluit je aan bij de gemeenschap van nieuwsgierige geesten die net als jij verlangen naar antwoorden en avonturen in de sterren!
Heb je vragen of wil je meer weten? Aarzel dan niet om contact met ons op te nemen! Samen ontrafelen we het mysterie van de lucht en daarbuiten.
09-01-2026
Vera C. Rubin Observatory discovers enormous, record-breaking asteroid in first 7 nights of observations
Vera C. Rubin Observatory discovers enormous, record-breaking asteroid in first 7 nights of observations
In its preliminary data release, taken from just seven nights of observations, the powerful Vera C. Rubin Observatory has discovered an enormous, fast-spinning asteroid that sets a new record.
An artist’s illustration of the massive, fast-spinning asteroid 2025 MN45, discovered in the first data from the Vera C. Rubin Observatory.
(Image credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA/P. Marenfeld)
Scientists analyzing the first images from the Vera C. Rubin Observatory have discovered the fastest-spinning asteroid in its size class yet.
The record-breaking space rock, called 2025 MN45, is larger than most skyscrapers on Earth at about 2,300 feet (710 meters) wide. The massive rock completes a rotation in about 113 seconds — making it the fastest-spinning known asteroid over 1,640 feet (500 meters) in diameter.
The research, published in The Astrophysical Journal Letters Wednesday (Jan. 7), is part of an asteroid survey aimed at improving our understanding of how these small bodies formed and evolved.
The study is the first peer-reviewed paper from the Rubin Observatory's LSST Camera — the largest digital camera in the world — which will repeatedly scan the Southern Hemisphere's night sky over 10 years to create an unprecedented time-lapse movie of the universe.
Rocks that roll
Asteroids are essentially large space rocks, and many are remnants of how our solar system appeared early in its 4.5 billion-year-old history, before the evolution of planets and moons. Therefore, by studying asteroids, scientists can figure out how our solar system changed over the eons.
Scientists found 2025 MN45 using the preliminary data release from the Rubin Observatory, which has already revealed thousands of previously unknown asteroids around the solar system after just seven nights of observations. (The 10-year LSST survey has yet to formally begin, but is expected to start in the next few months.)
The asteroid's remarkably fast spin excited the team, as it provides clues about the ancient rock’s composition.
"Clearly, this asteroid must be made of material that has very high strength in order to keep it in one piece," Sarah Greenstreet, an assistant astronomer at the National Science Foundation's National Optical-Infrared Astronomy Research Laboratory, said in a statement. "It would need a cohesive strength similar to that of solid rock."
"This is somewhat surprising," added Greenstreet, who also leads a Rubin working group about near-Earth objects and interstellar objects, "since most asteroids are believed to be what we call 'rubble pile' asteroids, which means they are made of many, many small pieces of rock and debris that coalesced under gravity during solar system formation or subsequent collisions."
This lightcurve shows how the asteroid’s brightness (x-axis) changes as it rotates (y-axis). Analyzing the curve allowed the team to calculate the asteroid's rotation speed, which sets a new record among asteroids of its size. (Image credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA/J. Pollard. Acknowledgement: PI: Sarah Greenstreet (NSF NOIRLab/Rubin Observatory))
Thousands more to come
In general, fast-spinning asteroids could have reached that state after a collision with another space rock, the study team said. It is also possible that 2025 MN45 is a remnant of a much larger asteroid that was shattered by a cosmic crash.
Most asteroids in the solar system are in the main asteroid belt between Mars and Jupiter. But most fast-spinning asteroids that astronomers have observed are much closer to Earth, simply because they are easier to see, the study authors noted. 2025 MN45 is a main-belt object, where most asteroids (as they are loose piles of rubble) must take at least 2.2 hours to rotate in order to avoid fragmentation. Anything that rotates faster than that "must be structurally strong," they wrote.
That said, 2025 MN45 is not the only fast spinner in the main asteroid belt. In addition to 2025 MN45, Rubin's first dataset includes 16 "super-fast" rotators, each of which has a rotational period of between 13 minutes and 2.2 hours, as well as two "ultra-fast" rotators with spins of less than two minutes each. All of these asteroids are also longer than 100 yards (90 m), and all but one of the newfound asteroids lives in the main belt.
The commissioning data from Rubin, which was released last June, underwent a deeper look in the new paper, which was also discussed Wednesday at a news conference at the 247th meeting of the American Astronomical Society in Phoenix.
The huge set of observations has about 1,900 never-before-seen asteroids, according to the statement. There will be many more to come when Rubin formally begins its 10-year survey of the sky in the coming months.
In particular, the initial results suggest that crashes may not be the only way asteroids reach extreme speeds, perhaps pressing astronomers to develop new explanations.
Europa, een van de vele manen van Jupiter, is een van de meest veelbelovende plekken om buitenaards leven te vinden in ons zonnestelsel. Onder een kilometers dikke ijslaag bevindt zich wellicht een oceaan van vloeibaar water. Maar uit een nieuwe studie blijkt dat de zeebodem mogelijk geologisch dood is en dat zet een flinke domper op de hoop dat Europa leven kan herbergen.
Op aarde wemelt het van het leven rond hydrothermale bronnen op de oceaanbodem. Dat zijn plekken waar scheuren in de aardkorst zeewater in contact brengen met vers gesteente. Bij die interactie komen allerlei chemische stoffen vrij die micro-organismen als energiebron kunnen gebruiken. Geen zonlicht nodig.
Wetenschappers koesteren al decennialang de hoop dat er zich onder de oppervlakte van Europa iets gelijkaardigs voordoet. De Jupitermaan heeft een oceaan die zo’n 97 kilometer diep is. Als er op de bodem breuken zouden ontstaan door tektonische activiteit, zou dat de perfecte omgeving kunnen zijn voor primitief leven.
Te weinig kracht om de bodem te breken
Maar daar zit nu het probleem. Amerikaanse onderzoekers hebben berekend hoeveel spanning er nodig is om breuken te laten bewegen op Europa’s zeebodem. Daarna keken ze naar alle bekende krachten die zulke spanning zouden kunnen veroorzaken.
De resultaten zijn ontmoedigend. De getijdenkracht van Jupiter, die Europa elke 84 uur een beetje uitrekt en samenperst, levert slechts ongeveer 3 procent van de benodigde spanning op. Zelfs als je aanneemt dat het gesteente al verzwakt is door miljarden jaren aan slijtage, blijft de getijdenkracht een factor tien tot twaalf te zwak.
Ook andere mechanismen schieten tekort. De stroming in Europa’s mantel (de laag onder de korst) zou in theorie breuken kunnen veroorzaken, maar zelfs in het meest optimistische scenario is die kracht honderden keren te zwak. En het krimpen van Europa’s binnenste door afkoeling? Daarvoor zou de rotsige kern met een hele kilometer moeten slinken voordat er iets zou breken.
Chemisch evenwicht: einde verhaal?
Zonder actieve breuken kan zeewater niet diep in de rotsbodem doordringen. Reacties tussen water en gesteente blijven dan beperkt tot hooguit de bovenste paar honderd meter. Na verloop van tijd bereikt die zone een chemisch evenwicht met de oceaan erboven en dan stopt de aanvoer van chemische energie.
Voor leven dat afhankelijk is van zulke chemische reacties is dat een probleem. Organismen die energie halen uit het mengen van vloeistoffen met verschillende chemische samenstellingen zouden op den duur zonder brandstof komen te zitten.
Is alle hoop verloren?
Niet helemaal. De onderzoekers wijzen op alternatieve energiebronnen die niet afhankelijk zijn van tektonische activiteit. Radioactief verval van uranium, thorium en kalium in het gesteente kan waterstof produceren, een proces dat radiolyse heet. Op aarde leven er micro-organismen in oude rotsformaties die precies dat doen, kilometers onder het aardoppervlak.
Of dit voldoende energie kan leveren voor een heel ecosysteem op Europa is nog onduidelijk. Maar het betekent wel dat de zoektocht naar leven niet per se ophoudt bij een geologisch stille zeebodem.
Europa Clipper gaat het uitzoeken
De NASA-missie Europa Clipper, die in 2024 is gelanceerd en in 2030 bij Jupiter aankomt, zal helpen om deze vragen te beantwoorden. Het ruimtevaartuig gaat onder andere meten hoe dik de ijslaag is, hoeveel warmte er vrijkomt door getijdenwerking en of er misschien waterpluimen uit de ijskorst spuiten die iets kunnen onthullen over de chemische samenstelling van de oceaan.
Toch zal zelfs deze missie wellicht geen definitief antwoord geven. Uiteindelijk zullen we de oceaan en misschien ooit de zeebodem rechtstreeks moeten onderzoeken om te weten of er leven is op Europa.
The smell of space has been described as similar to the smell of something cooking on a charcoal grill.
Rbkomar/Getty Images
Key Takeaways
Astronauts report that space has a distinct smell, often described as metallic or sweet.
These descriptions come from astronauts' experiences after returning from spacewalks and noticing the smell in the airlock, which suggests the scent clings to their suits and equipment.
The smell of space is thought to be due to the presence of polycyclic aromatic hydrocarbons, compounds that form in the dust and debris of space.
We all know space is empty, right? Most of space is completely absent of anything – not dust, not planets nor sun, not even air. So, why do many of the people who've been to space and spent time in it report that space has a smell?
It turns out that space does smell, and our solar system has a very particular smell. This is likely the result of several factors, but all are clear: Our corner of the universe is kind of stinky. If you're curious to learn what space smells like and why it smells that way, the explanation might surprise you.
While no astronaut has been unwise enough to unclasp and remove their helmet in the vacuum of space (which is very bad for longevity), astronauts have reported a smell upon returning from space. Specifically, many astronauts report different smells in the airlock after participating in spacewalks.
"The best description I can come up with is metallic; a rather pleasant sweet metallic sensation," wrote astronaut Don Pettit, according to Space.com. "It reminded me of my college summers where I labored for many hours with an arc welding torch repairing heavy equipment for a small logging outfit. It reminded me of pleasant sweet-smelling welding fumes. That is the smell of space." Pettit participated in several EVAs (extravehicular activities or spacewalks) during his NASA career, accumulating repeated experience with the smell.
Other astronauts have described it in similar yet varying ways: "burning metal," "a distinct odor of ozone, an acrid smell," "walnuts and brake pads," "gunpowder" and even "burnt almond cookie." Much like all wine connoisseurs smell something a bit different in the bottle, astronaut reports differ slightly in their "smelling notes" but have one thing in common: a burnt smell.
What might explain why space smells burnt? There are two possible explanations.
The Oxidation Explanation
One theory to explain the smell of space relates to the process that occurs in the airlock as astronauts return from space to the International Space Station or spacecraft they call home while orbiting Earth. During re-pressurization, the chemical reaction of oxidation occurs; atoms of oxygen in space attach to the astronaut's suit and float in during the de-pressurized time when the airlock is open and combine to form atmospheric oxygen (O2).
This process is similar to combustion without the flame and smoke – and smells similar too, which might explain the smoky, charred odor astronauts report.
The Stellar Explosion Explanation
A second hypothesis about what might explain the smell of space that astronauts report upon returning through the airlock relates to stellar explosions — that is, dying stars.
Though we've only been studying the night sky for a few centuries, the universe dates some 13.7 billion years old, and our solar system is estimated to be about 4.5 billion years old. This means that for literally billions of years before our solar system even formed, stars were being born and dying across the universe.
When stars die, it tends to be a dramatic affair, and this bombastic process creates a compound called polycyclic aromatic hydrocarbons (PAHs). PAHs are present throughout the solar system, including here on Earth; they can be found in some foods, coal and oil, among other materials. They also occur when coal, tobacco, wood, meat and other substances are burned. Perhaps part of the reason space has a distinctly burnt and charcoal smell is because it — like a grill on a summer evening — is emitting smelly PAHs.
Now That's Interesting
Outside our solar system, it's not as stinky! Other parts of the universe have other compounds and elements, which create different smells — though no human is likely to ever take a big whiff to confirm. For example, the dust cloud Sagittarius B2 has a high concentration of ethyl formate, which is the organic compound that gives both raspberries and rum their distinctive odors. If you love a good raspberry daiquiri, that's the corner of the universe for you!
A shocking admission by the CIA has just reopened the mystery surrounding 3I/ATLAS, the interstellar object speeding through our solar system.
Although NASA has claimed the object is an ordinary comet, an icy rock with a long tail of gas and dust, intelligence officials have refused to answer whether they investigated the possibility that 3I/ATLAS is an extraterrestrial craft.
In response to a November 2025 Freedom of Information Act (FOIA) request regarding the supposed comet, the CIA said it could 'neither deny nor confirm the existence or nonexistence of records' regarding 3I/ATLAS.
The federal government had maintained that the object showed no signs of harboring alien life or that it was an artificially constructed spacecraft since it was detected in July 2025.
However, the CIA still decided to provide what is known as a 'Glomar response.' It's a way for the government to say, 'We're not going to tell you if we have information or not, because even admitting that could reveal sensitive secrets.'
Harvard professor Avi Loeb has continued to challenge NASA's claims, highlighting that 3I/ATLAS has exhibited at least 12 strange behaviors that scientists have not been able to explain as natural occurrences.
Those anomalies include the object having a bright 'anti-tail' pointing in the opposite direction of a normal comet, course changes that defy the laws of gravity, and a nickel shell, which is a metal typically used by spacecraft to deflect heat.
'That this information is treated as sensitive enough to be classified by the CIA is surprising, given that NASA officials stated decisively at a press conference on November 19, 2025, that 3I/ATLAS is definitely a comet of natural origin,' Loeb said.
Amateur stargazers have taken clear images of the interstellar object 3I/ATLAS (Pictured) using common telescopes during its journey through the solar system
The CIA has released a statement neither confirming nor denying any investigations into 3I/ATLAS, complying with a November 2025 FOIA request
As 3I/ATLAS nears Jupiter on March 16, the Harvard physicist said the new revelations by the US intelligence community suggest the government has secretly investigated the possibility that the object is a hostile threat, as he theorized last year.
The Daily Mail has requested comment from both the CIA and NASA and is awaiting a response.
The FOIA request was submitted by UFO and government conspiracy researcher John Greenewald Jr, who noted in a post on X that he was filing an appeal to get a clearer answer from the CIA.
Greenewald Jr added that he has filed the same request for information regarding 3I/ATLAS with NASA and other US agencies and is still waiting for them to reply.
FOIA requests are part of US law that lets anyone, including citizens, journalists, and researchers, ask government agencies for documents or records on a specific topic.
The agency must give a response, but it can withhold revealing details if the information is classified for national security reasons or falls under certain exemptions.
'Very interesting, apparently CIA [director John] Ratcliffe knows something,' one person on social media alleged.
The new revelations have come months after NASA completely dismissed the possibility of 3I/ATLAS being extraterrestrial in origin, with space agency administrator Nicky Fox saying they've found nothing 'that would lead us to believe it was anything other than a comet.'
3I/ATLAS is projected to reach its closest point to Jupiter in March 2026 before leaving the solar system for good
However, NASA's November announcement created more doubt about the object's origins than it solved, as the agency was widely mocked for the blurry images it released of 3I/ATLAS.
Many critics quickly pointed out that amateur astronomers with common telescopes had been taking much clearer photographs of the alleged comet as it approached Earth in December, despite being over 200million miles from the object.
In comparison, NASA Mars orbiters were less than 20million miles away from 3I/ATLAS in early October 2025, but still only returned heavily pixelated images of the visitor, which caused some to claim it was a cover-up.
'NASA officials were encouraged to deliver the likely scientific interpretation, while at the same time, the serious consideration of a black swan event by the CIA was hidden from public view to prevent panic from taking hold for no good reason,' Loeb speculated in a statement published Monday.
A black swan event is a rare, totally unexpected happening that's highly unlikely but could have huge, world-changing consequences for the Earth.
In the case of the interstellar comet 3I/ATLAS, Loeb said if the tiny chance that the object was artificial alien technology turned out to be true, it would be a massive shock with enormous implications for humanity, including proving aliens exist.
The cryptic response from the CIA adds another layer to the eight-decade conspiracy theory UFO believers have had, claiming that the US government has been concealing what it knows about extraterrestrial life.
Just days after Greenewald Jr's FOIA request was submitted in November, the hit documentary 'The Age of Disclosure' was released, interviewing 34 US government, military, and intelligence officials about their knowledge of an alleged UFO cover-up.
Despite the speculation, the US military and federal government have said there has never been any physical proof that UFOs or beings from other planets exist.
Out in the depths of space, somewhere in between Mars and Jupiter, is a newly discovered asteroid that’s breaking records.
Astronomers have spotted a celestial rock the size of seven football pitches that is spinning faster than they’ve ever seen before.
The asteroid, named 2025 MN45, is 710 metres in diameter and completes a full rotation every 1.88 minutes.
The fact that it spins so rapidly has baffled experts, who say it must consist of solid rock in order to maintain its shape.
‘Clearly, this asteroid must be made of material that has very high strength in order to keep it in one piece as it spins so rapidly,’ Sarah Greenstreet, who leads the Rubin Observatory’s Solar System Science Collaboration’s Near-Earth Objects and Interstellar Objects working group, said.
‘We calculate that it would need a cohesive strength similar to that of solid rock.
‘This is somewhat surprising since most asteroids are believed to be what we call “rubble pile” asteroids, which means they are made of many, many small pieces of rock and debris that coalesced under gravity during Solar System formation or subsequent collisions.’
While it is currently out in the asteroid belt, hundreds of millions of kilometres away, asteroids and comets have previously been ‘nudged’ into Earth’s neighbourhood by the gravity of nearby planets.
This artist’s illustration depicts 2025 MN45 — the fastest-rotating asteroid with a diameter over 500 meters that scientists have ever found
The lightcurve of the asteroid - the y-axis shows the asteroid’s brightness, and the x-axis shows its phase, or where it is in its rotation
The sighting forms part of a much larger discovery, as scientists have detected 1,900 new asteroids cruising about our Solar System that have never been seen before.
Within this flurry are 19 super and ultra-fast rotating asteroids – with 2025 MN45 taking the new record for the fastest-spinning asteroid with a diameter over 500 meters that astronomers have found.
For their study, researchers collected data over the course of about 10 hours across seven nights in April and May of last year.
They used the Rubin Observatory’s LSST Camera – the largest digital camera in the world – to capture the night sky.
‘Discoveries like this exceptionally fast-rotating asteroid are a direct result of the observatory's unique capability to provide high-resolution, time-domain astronomical data, pushing the boundaries of what was previously observable,’ Regina Rameika, from the US Department of Energy, said.
As asteroids orbit the Sun, they also rotate at a wide range of speeds, the researchers explained.
These spin rates not only offer clues about the conditions of their formation billions of years ago but also tell us about their internal composition and evolution over their lifetimes.
In particular, an asteroid spinning quickly may have been sped up by a past collision with another asteroid, suggesting that it could be a fragment of an originally larger object.
Most asteroids can be found orbiting our Sun between Mars and Jupiter within the main asteroid belt
An illustration of the main asteroid belt, orbiting the Sun between Mars and Jupiter, where asteroid 2025 MN45 can be found
This image, one of the first released by Rubin Observatory, exposes a Universe teeming with stars and galaxies — transforming seemingly empty, inky-black pockets of space into glittering tapestries for the first time
‘Fast rotation also requires an asteroid to have enough internal strength to not fly apart into many smaller pieces, called fragmentation,’ the team said in a release.
‘Most asteroids are ‘rubble piles’, which means they are made of many smaller pieces of rock held together by gravity, and thus have limits based on their densities as to how fast they can spin without breaking apart.
‘For objects in the main asteroid belt, the fast-rotation limit to avoid being fragmented is 2.2 hours; asteroids spinning faster than this must be structurally strong to remain intact.
‘The faster an asteroid spins above this limit, and the larger its size, the stronger the material it must be made from.’
Within the main asteroid belt are space rocks ranging in size from 530km (329 miles) to just 10 metres (33 feet) in diameter.
‘Sometimes, asteroids and comets are nudged into Earth’s neighbourhood by the gravity of nearby planets,’ NASA says.
However, they explained that it is ‘highly unlikely’ an asteroid large enough to cause widespread damage will impact Earth for the next 100 years or more.
Currently, NASA would not be able to deflect an asteroid if it were heading for Earth but it could mitigate the impact and take measures that would protect lives and property.
This would include evacuating the impact area and moving key infrastructure.
Finding out about the orbit trajectory, size, shape, mass, composition and rotational dynamics would help experts determine the severity of a potential impact.
However, the key to mitigating damage is to find any potential threat as early as possible.
NASA and the European Space Agency completed a test which slammed a refrigerator-sized spacecraft into the asteroid Dimorphos.
The test is to see whether small satellites are capable of preventing asteroids from colliding with Earth.
The Double Asteroid Redirection Test (DART) used what is known as a kinetic impactor technique—striking the asteroid to shift its orbit.
The impact could change the speed of a threatening asteroid by a small fraction of its total velocity, but by doing so well before the predicted impact, this small nudge will add up over time to a big shift of the asteroid's path away from Earth.
This was the first-ever mission to demonstrate an asteroid deflection technique for planetary defence.
The results of the trial are expected to be confirmed by the Hera mission in December 2026.
NASA has just revealed that the crew of the International Space Stationwas being evacuated for the first time in history after one of the astronauts suffered a medical emergency.
NASA administrator Jared Isaacman said in a press conference Thursday that Crew-11 would not continue its missionuntil its scheduled return date in February, and that the steps for their safe return would be worked out over the next 48 hours.
'I've come to the decision that it's in the best interest of our astronauts to return Crew-11 ahead of their planned departure,' Isaacman revealed.
The announcement came less than a day after NASA cancelled a Thursday spacewalk due to the medical issue, with officials saying they were 'erring on the side of caution for the crew member'.
Crew-11 includes four astronauts: NASA's Zena Cardman and Mike Fincke, Japanese astronaut Kimiya Yui, and Russian cosmonaut Oleg Platonov.
The group was recently joined by Japanese astronaut Koichi Wakata and NASA astronaut Chris Williams, who arrived at the station aboard a Russian Soyuz spacecraft in November 2025.
Isaacman said that Williams will remain on the station with the Soyuz crew to maintain America's presence in space.
While the astronaut who suffered the medical issue was not revealed, NASA's chief medical officer Dr James Polk said the astronaut was not in any immediate danger and they were being cared for by their fellow crewmates until their return.
Crew-11 before launching to the ISS. Pictured (L to R): Roscosmos cosmonaut Oleg Platonov, NASA astronaut Mike Fincke, JAXA astronaut Kimiya Yui, and NASA's Zena Cardman
NASA cancelled a planned spacewalk on Thursday involving the crew of the International Space Station (Pictured) over an unspecified medical issue involving one of the astronauts
Dr Polk added that the medical issue the astronaut suffered had nothing to do with the upcoming spacewalk or any other operations on board the station.
'It's mostly having a medical issue in the difficult areas of microgravity,' Polk explained without going into specific medical details.
NASA officials noted that no special precautions would need to be taken to keep the ailing astronaut safe until their return and called their condition 'stable' until the evacuation plan is finalized.
NASA has never had to bring an astronaut home for medical reasons, but an evacuation plan has been built into every ISS mission, with crew return vehicles kept on standby.
'We are looking for the correct opportunity to use our existing landing sites,' Isaacman said when asked if NASA would be making an emergency landing to get Crew-11 home faster.
'I´m proud of the swift effort across the agency thus far to ensure the safety of our astronauts,' the NASA chief added.
The NASA administrator did note that the space agency did consider this a 'serious medical condition' which forced officials to conclude that the first ever evacuation was necessary.
However, Dr Polk stressed that the astronaut was not in immediate danger which would force NASA to consider rushing the evacuation into an unsafe flight window.
NASA administrator Jared Isaacman (Left) and NASA chief medical officer Dr James Polk (Center) revealed on Thursday that Crew-11 would be returning as soon as possible
JAXA astronaut Kimiya Yui (center) was helping NASA astronaut Zena Cardman (left) and Mike Fincke prepare for the spacewalk before it was postponed
'The crew member is absolutely stable, so I don't foresee massive changes to the timeline or their activities,' Polk said.
Crew-11 arrived at the ISS on August 1, 2025, meaning their return date had been scheduled for late February.
The four astronauts were supposed to leave after Crew-12 arrived on a SpaceX Dragon capsule no earlier than February 15.
Isaacman said that any decision to potentially move up the launch of Crew-12 would not impact the upcoming Artemis II mission planned for February 2026.
He called the two launches 'totally separate campaigns,' meaning there should be no issue in launching Artemis on time. Artemis II will be the first manned spaceflight to orbit the moon since 1972.
Meanwhile, the ISS is required to have astronauts aboard at all times, as they are essential to carry out maintenance, repairs, operate complex experiments, manage life support and perform spacewalks, tasks that automation cannot fully handle, ensuring constant human oversight for safety and scientific output.
Until now, there had never been a crew evacuated ahead of their scheduled departure time from the ISS, however, two spacewalks were recently cancelled because of various health issues among the astronauts.
A mission was cancelled in 2021 when Mark Vande Hei experienced a pinched nerve and was unable to travel outside the ISS.
Another spacewalk in 2024 was called off at the last minute because an astronaut experienced 'spacesuit discomfort'.
Scientists have discovered a mysterious hole on the surface of Mars, and they have no idea what lies inside it.
This pit, located in the Arsia Mons region — one of Mars’ giant volcanoes — could potentially be a skylight leading to a vast network of lava tubes.
Lava tubes are natural caverns formed by flowing lava. Here on Earth, they provide shelter for many life forms, and on Mars, they could offer human explorers much-needed protection from the harsh Martian environment.
So, is this hole the key to unlocking a potential Martian habitat?
A Mysterious Martian Pit — Leading to Where?
There’s no shortage of environmental hazards out to kill any astronaut bold enough to dare set foot on Mars. With Mars having only 0.7% of Earth’s sea-level pressure, humans would have to don a full pressure suit or live inside a specialized chamber. Without these precautions, oxygen wouldn’t circulate in the bloodstream, with potentially fatal consequences.
Radiation, however, remains the primary concern. Although Mars is farther from the Sun than Earth, the absence of a magnetic field and its thin atmosphere mean it’s exposed to much higher radiation levels than Earth. The Mars Odyssey probe has shown radiation levels on Mars are at least 2.5 times higher than what astronauts face on the International Space Station. Furthermore, besides regular exposure to cosmic rays and solar wind, it receives occasional, lethal radiation blasts due to solar flares.
The Photos NASA Sent To Aliens
Any attempt to colonize the Red Planet will require measures to ensure radiation exposure is kept to a minimum. Some of the proposed ideas thus far involve habitats built directly into the ground or even above-ground habitats using inflatable modules encased in ceramics.
However, a promising alternative lies in Mars’ natural landscape. The planet is scattered with deep pits, caves, and lava tube structures that can act as a shield against radiation.
Collapsed sections of these tubes, called skylights, could provide access to these subterranean refuges. This is what scientists believe this newly identified pit could be. It was recently imaged by the High-Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter (MRO).
The Nature of Martian Pits
Two images of the pit in Arsia Mons. The one on the left was taken a couple of years ago. The one on the right is more recent and shows a side wall, which may mean the hole is not an entrance to a lava tube or cave.
The newly examined pit measures only a few meters across and resides in the Tharsis region — a vast volcanic plain, thousands of kilometers across and elevated about 10 km above the planet’s mean elevation. This area was once very volcanically active, so scientists’ best guess is that the pit is a skylight to a lava tube.
However, that’s not the only option. In another image, you can see an illuminated sidewall, indicating it might just be a cylindrical pit. This raises the possibility that the hole may simply be a pit crater, similar to those found in Hawaii.
These craters form when cracks in volcanic rock widen and collapse, offering no access to underground chambers. In Hawaii, pit craters range from 6 to 186 meters deep and 8 to 1140 meters wide. The Arsia Mons pit is about 178 meters deep, Universe Today reports.
Lessons from the Moon
So, the big question now is: does this hole on Mars lead to a larger underground cavern? We don’t have a straight answer yet. But with time, scientists might be able to study and understand Martian pits as well as they do those on the Moon.
We understand lunar lava pits and tubes much better than those on Mars. Some lunar tubes are thermally stable and have boulder-covered floors. There are even plans for robots to explore these lunar caves, potentially housing astronauts in inflatable habitats.
Mars, with its weaker gravity, should support even larger lava tubes. This would provide extremely valuable shelter on a very unforgiving planet. Perhaps this is not all that different from how the first human explorers made bases in caves as they traveled across uncharted territory, colonizing the world.
However, unlike the Moon, we lack conclusive evidence of their existence on Mars. This intriguing pit on Arsia Mons is part of an ongoing search for Martian lava tubes. Future robotic missions designed to explore these potential underground worlds will be crucial in unlocking the secrets they hold.
Renewed Interest and New Discoveries
In November 2024, a breakthrough study on Earth provided some supporting evidence that Martian caves could act as time capsules. Researchers exploring lava tubes in Lanzarote, Spain, found that the tubes shielded minerals and organic compounds from weathering, effectively preserving “biosignatures” of past microbial life. This confirms that if life ever existed on Mars, a lava tube would be the most likely place to find its fossilized remains, protected from the harsh radiation on the surface.
Meanwhile, the region hosting the pit, Arsia Mons, received a stunning visual update in May 2025.
Arsia Mons, an ancient Martian volcano, was captured before dawn on May 2, 2025, by NASA’s 2001 Mars Odyssey orbiter while the spacecraft was studying the Red Planet’s atmosphere, which appears here as a greenish haze.
NASA’s Mars Odyssey orbiter captured a rare panorama showing the volcano’s summit poking through a vast blanket of morning clouds. This image highlighted the extreme altitude of the Tharsis region (where the pit is located), reminding us that any habitat here would need to contend with not just radiation, but unique atmospheric weather patterns distinct from the rest of the planet.
But there could be other, even more interesting caves.
In late 2025, when scientists identified a potential new class of caves in the Hebrus Valles region. Unlike the volcanic tubes of Arsia Mons, these new candidates appear to be “karstic”—caves formed by the dissolution of bedrock by water. If confirmed, these wouldn’t just be shelters; they would be remnants of ancient aquifers, making them the ultimate “holy grail” for both human habitation and the search for alien life.
This article was originally published in 31 May, 2024, and has been reedited to include additional information.
The giant planet Jupiter has nearly 100 known moons, yet none have captured the interest and imagination of astronomers and space scientists quite like Europa, an ice-shrouded world that is thought to possess a vast ocean of liquid salt water. For decades, scientists have wondered whether that ocean could harbor the right conditions for life, placing Europa near the top of the list of solar system bodies to explore.
A new study led by Paul Byrne, an associate professor of Earth, environmental, and planetary sciences, throws cold water on the idea that Europa could support life at the seafloor. The study was published in Nature Communications.
Co-authors from the Department of Earth, Environmental, and Planetary Sciences include Professor Philip Skemer, associate chair of the department; Professor Jeffrey Catalano; Douglas Wiens, the Robert S. Brookings Distinguished Professor; and graduate student Henry Dawson. Byrne, Skemer, Catalano, Wiens, and Dawson are also members of the McDonnell Center for the Space Sciences.
Study findings challenge life potential
Using calculations that consider the moon's size, the makeup of its rocky core, and the gravitational forces from Jupiter, Byrne and a team of scientists conclude that Europa likely lacks the tectonic motion, warm hydrothermal vents, or any other sort of underwater geologic activity that would presumably be a prerequisite for life.
"If we could explore that ocean with a remote-control submarine, we predict we wouldn't see any new fractures, active volcanoes, or plumes of hot water on the seafloor," Byrne said.
"Geologically, there's not a lot happening down there. Everything would be quiet." And on an icy world like Europa, a quiet seafloor might well mean a lifeless ocean, he added.
Europa's geology and tidal forces explained
For Byrne, a planetary scientist, Europa's appeal extends well beyond the question of life. "I'm really interested to know what that seafloor looks like," he said. "For all of the talk about the ocean itself, there has been little discussion about the seafloor."
Without a submarine, Byrne and co-authors had to combine known facts about Europa with inferences drawn from the geology of Earth and other bodies, including our own moon.
The ice shell on Europa is thought to be 15 to 25 km thick, and the ocean covers the entire moon to a depth of up to 100 km. Even though Europa is slightly smaller than our own moon, it likely holds much more water than Earth.
Beneath that ice and water lies a rocky core analogous to Earth's. While Earth's core still burns hot, Byrne and co-authors calculated that any heat from Europa's core would have escaped billions of years ago.
The team also calculated the gravitational forces from Jupiter, a pull that can be strong enough to keep a moon geologically alive. On its innermost large moon, Io, Jupiter's gravity roils tides and heats the rocks beneath the icy surface. Io, in fact, is the most volcanically active body in the solar system.
The tides on Io are especially violent because the moon has an erratic orbit that periodically takes it closer to Jupiter, but Europa's orbit is relatively stable and distant, lessening the chance for substantial tidal forces, Byrne explained.
"Europa likely has some tidal heating, which is why it's not completely frozen," Byrne said. "And it may have had a lot more heating in the distant past. But we don't see any volcanoes shooting out of the ice today like we see on Io, and our calculations suggest that the tides aren't strong enough to drive any sort of significant geologic activity at the seafloor."
Future missions and scientific curiosity
Europa's quiet seafloor geology doesn't provide much support for any contemporary life beneath the ice, Byrne said. "The energy just doesn't seem to be there to support life, at least today."
Byrne is still excited about future chances to explore Europa, especially the Europa Clipper spacecraft that will fly by the moon in the spring of 2031. That mission—conceived and championed in part by Bill McKinnon, the Clark Way Harrison Distinguished Professor in Arts & Sciences and interim director of the McDonnell Center for the Space Sciences—will take close-up pictures of Europa's surface and provide more precise measurements of its ice cap and ocean.
"Those measurements should answer a lot of questions and give us more certainty," Byrne said.
Even if, eventually, modern Europa is found to be lifeless, Byrne won't be disappointed.
"I'm not upset if we don't find life on this particular moon," he said. "I'm confident that there is life out there somewhere, even if it's 100 light-years away. That's why we explore—to see what's out there."
Scientists spot a massive object quietly shadowing Earth’s orbit
Scientists spot a massive object quietly shadowing Earth’s orbit
Story byCassian Holt
Scientists spot a massive object quietly shadowing Earth’s orbit
Far from the bright glare of the Moon, a much smaller companion has been quietly keeping pace with Earth, looping around the Sun in a complex dance that only looks like a shared orbit from our vantage point. Astronomers now recognize this object, designated 2025 PN7, as a quasi-moon, a tiny asteroid that appears to shadow our planet without being truly captured by its gravity. The discovery turns a routine scan of the sky into a reminder that even in our own celestial backyard, there are still neighbors we are only just meeting.
Despite the headline-friendly idea of a “massive” new world, the reality is more subtle and scientifically richer: 2025 PN7 is physically small but dynamically significant, a compact body whose path reveals how Earth interacts with the swarm of rocks that share its orbital neighborhood. In practical terms, this is a miniature object with outsized importance for understanding near-Earth space, planetary defense, and even the long-term story of how material moves through the inner Solar System.
Meet 2025 PN7, Earth’s tiny quasi-moon
The object at the center of this story is not a second Moon in any familiar sense, but a modest asteroid that happens to move in step with Earth around the Sun. Cataloged as 2025 PN7, it follows a path that keeps it relatively close to our planet over long stretches of time, so from certain perspectives it seems to hover near us like a faint, offbeat satellite. Astronomers classify such bodies as quasi-moons or quasi-satellites, a label that reflects their gravitational independence from Earth even as they trace a similar yearly journe
What makes 2025 PN7 stand out is not its bulk but its delicacy: observations indicate it measures just 19 units across, a scale that places it firmly in the “tiny companion” category rather than anything approaching a true second Moon. That compact size, combined with its subtle motion against the background stars, explains why it could orbit in this configuration for a long time before anyone noticed, and why its discovery has prompted a fresh look at how many other small neighbors might be sharing Earth’s path around the Sun.
How a “surprise sidekick” was finally spotted
Finding something as small as 2025 PN7 requires both patient sky coverage and sensitive detectors, and in this case the breakthrough came from a survey instrument built precisely for that task. The asteroid was discovered on July 30, 2025 by the Pan-STARRS1 telescope at Haleakalā Observatory in Hawaii, a facility designed to sweep large swaths of the sky for moving points of light that betray the presence of near-Earth objects. That combination of wide-field imaging and repeated exposures allowed astronomers to pick out the faint track of this new body against the static star field.
In social media posts describing the find, researchers likened the object to a “surprise sidekick,” emphasizing that such a small body, only 19 units across, had been quietly accompanying Earth without drawing attention to itself. The discovery at Pan on the summit of Haleakalā Observatory in Hawaii underscores how modern survey programs can reveal companions that would have been invisible to earlier generations of telescopes, even though they share our planet’s orbital neighborhood.
What makes a quasi-moon different from a real Moon
Although 2025 PN7 is already being described as a quasi-moon, that label can be misleading if it is taken to mean Earth has acquired a second natural satellite in the same sense as the familiar Moon. A true moon is gravitationally bound to its planet and orbits that planet directly, tracing a closed path around it while both bodies circle the Sun. In contrast, a quasi-moon like 2025 PN7 orbits the Sun, not Earth, and only appears to loop around our planet because its orbital period and shape are closely matched to ours.
The distinction becomes clearer when compared with other known quasi-satellites, such as (469219) Kamoʻoalewa (2016 HO3), which is described as a quasi-satellite of Earth that, in certain frames of reference, appears to orbit our planet even though it is really circling the Sun. Studies of Kamo have even suggested it may be a fragment of the Moon blasted into space, highlighting how quasi-moons can be both dynamically intriguing and compositionally revealing. By placing 2025 PN7 in this context, astronomers can use its motion to probe the subtle gravitational interplay between Earth, the Moon, and the swarm of near-Earth asteroids.
A companion hiding in plain sight for decades
Orbital reconstructions indicate that 2025 PN7 has likely been accompanying Earth for a long time, its path shaped by the same solar gravity that governs our own orbit. Astronomers analyzing its trajectory have concluded that this asteroid has been shadowing Earth for decades, maintaining a configuration that keeps it relatively close to our planet without ever becoming a conventional satellite. That long-term stability is part of what makes the object so scientifically valuable, since it offers a natural experiment in how small bodies can share a planet’s orbital space over extended periods.
Reports on the discovery emphasize that Astronomers now see 2025 PN7 as an asteroid that has been moving with Earth for decades, effectively hiding in plain sight because of its tiny size and the complexity of its apparent motion in the sky. The fact that such a long-standing companion could go unnoticed until now underscores both the limitations of past surveys and the growing power of new instruments to map the near-Earth environment in far greater detail.
Earth’s “New Cosmic Companion” and what it tells us
Beyond the orbital mechanics, 2025 PN7 has quickly taken on a more evocative identity as Earth’s New Cosmic Companion, a phrase that captures both its proximity and its novelty. Descriptions of the find frame it as The Story of Quasi Moon 2025 PN7, a narrative that situates this small body within a broader effort to catalog the subtle, often surprising structures that share our planet’s path around the Sun. By treating it as a character in that story, scientists and communicators alike are highlighting how even a 19-unit-wide rock can reshape our sense of the Solar System’s architecture.
Analyses of Earth and its New Cosmic Companion emphasize that quasi-moons like 2025 PN7 remind us that space is full of surprises, particularly in the near-Earth region where gravitational resonances can trap small bodies in unusual configurations. The Story of Quasi Moon 2025 PN7 is therefore not just about a single asteroid, but about the dynamic processes that populate our orbital neighborhood with temporary companions, some of which may eventually escape or collide with other objects as their paths evolve.
How surveys and interstellar visitors sharpen our view
The detection of 2025 PN7 is part of a larger revolution in how astronomers scan the sky, driven by systematic survey programs that repeatedly image wide fields to catch anything that moves. One example is the ATLAS project, which has already demonstrated its power by identifying Comet 3I/ATLAS, an interstellar object discovered by a NASA-funded survey telescope in Rio Hurtado, Chile. That discovery relied on a survey strategy that flags unusual trajectories, and the same philosophy underpins the work of facilities like Pan-STARRS1 that are now revealing quasi-moons and other subtle companions.
According to Comet 3I/ATLAS facts, the object was identified through a survey approach that can pick out faint, fast-moving bodies, including those on paths that indicate an origin outside the Solar System. That same survey mindset has also led astronomers to spot other strange visitors, such as the interstellar object discussed in a Jul video that describes something unusual moving through our Solar System and heading our way. By refining these techniques, researchers are better equipped to notice both dramatic interstellar interlopers and quiet, long-term companions like 2025 PN7.
From Oumuamua to 3I/ATLAS: context for small, strange objects
The excitement around 2025 PN7 also reflects a broader fascination with small, hard-to-classify objects that challenge our expectations about what orbits the Sun. Earlier interstellar visitors such as ʻOumuamua showed that not every passing body fits neatly into the categories of comet or asteroid, and subsequent detections have reinforced that lesson. In one widely discussed case, NASA confirmed that a mysterious object shooting through the Solar System was an interstellar visitor and even assigned it a new name, underscoring how quickly such discoveries can reshape scientific debates.
Reports on that event note that NASA experts concluded the object was not bound to the Sun in the long term, marking it as a traveler from beyond our planetary system. A similar story has unfolded with Interstellar object 3I/ATLAS, which passed Earth and is now leaving the Solar System, headed out again after its brief visit. Coverage of Interstellar 3I/ATLAS highlights how even a relatively small body can carry crucial information about conditions in distant star systems, just as a quasi-moon like 2025 PN7 can illuminate the fine structure of our own orbital environment.
Why a tiny quasi-moon matters for planetary defense
On a practical level, the discovery of 2025 PN7 feeds directly into the growing field of planetary defense, which depends on a detailed inventory of near-Earth objects and their trajectories. Even though this particular asteroid is only 19 units across and poses no known threat, its detection proves that such small bodies can share Earth’s orbit for decades without being cataloged, a gap that matters when assessing impact risks. By refining the techniques that revealed this quasi-moon, astronomers improve their chances of spotting more hazardous objects of similar size or slightly larger before they come too close.
The broader survey ecosystem that caught 2025 PN7 is also responsible for identifying other unusual bodies, including the interstellar object highlighted in a An interstellar object video that describes something strange moving through our Solar System. Each of these detections, whether a fleeting visitor like 3I/ATLAS or a long-term companion like 2025 PN7, adds to a statistical picture of how many small objects cross Earth’s path and how their orbits evolve. In that sense, a tiny quasi-moon is not just a curiosity, but a data point that helps refine models used to protect the planet from future impacts.
The quiet revolution in mapping Earth’s orbital neighborhood
Stepping back, 2025 PN7 is part of a quiet revolution in how thoroughly we map the space around Earth, a process driven by better detectors, smarter software, and coordinated survey strategies. Where earlier generations of astronomers might have focused on bright planets and comets, today’s instruments are tuned to pick out faint, fast-moving specks that reveal a rich population of near-Earth asteroids, quasi-moons, and other transient companions. Each new detection, from Kamoʻoalewa to 3I/ATLAS to 2025 PN7, fills in another piece of a complex gravitational puzzle.
As I see it, the real story behind Earth’s so-called “second moon” is not about size or spectacle, but about the precision with which we can now track even a 19-unit-wide rock as it quietly shadows our orbit. The work that identified 2025 PN7, building on survey methods refined in projects like ATLAS and on analyses that recognized quasi-satellites such as Kamoʻoalewa, shows how far observational astronomy has come in just a few decades. It also hints at how many more subtle companions may still be waiting in the data, small in scale but large in what they can teach us about the constantly shifting architecture of our Solar System.
Scientists have discovered a new type of astronomical object, calling the strange entity a 'window into the dark universe'.
The object known as Cloud-9 is a completely starless, gas-rich cloud of dark matter located 14 million light-years from Earth.
The cloud's core is a vast, compact sphere of neutral hydrogen, about 4,900 light-years across.
That is more than 1,000 times greater than the distance between Earth and the nearest star, Proxima Centauri.
However, despite containing abundant stellar fuel, astronomers have now used the Hubble Space Telescope to confirm that Cloud-9 contains no stars whatsoever.
Scientists say that makes the cloud a building block of a galaxy that never quite formed, left over as a relic from the early universe.
Co-author Dr Andrew Fox, of the European Space Agency and the Space Telescope Science Institute, told the Daily Mail: 'You can think of it as a failed galaxy.
'A ghostly object that didn’t quite have enough mass to become self-gravitating and cross the threshold into star formation.'
Scientists have discovered a new type of astronomical object, a cloud of dark matter and hydrogen gas that contains no stars. Pictured: Magenta shows radio data from the gas cloud, and the dotted circle shows the peak of radio emissions
Cloud-9 is a previously theoretical type of object known as a Reionization-Limited H I Cloud, or 'RELHIC'.
'The main piece of evidence for dark matter in this cloud is its size,' says Dr Fox,
'A cloud this size needs a source of gravity to hold it together. There are no stars to provide this gravity, and the neutral hydrogen gas does not contain enough mass, so dark matter must be the culprit. Without it, the cloud would simply fall apart.'
By looking at the radiation emitted by gases in the cloud, scientists estimate that the mass of hydrogen within is about one million times that of the sun.
However, for the cloud not to drift apart, Dr Fox and his colleagues estimate that it must contain around five billion solar masses of dark matter.
This discovery is extremely exciting for astronomers because RELHICs like Cloud-9 offer a snapshot into an exceptionally early moment in the universe's history.
Scientists say that the strange object (pictured), dubbed Cloud-9 and located 14 million light-years from Earth, is a failed galaxy that didn't have enough mass to produce stars
Dr Fox says: 'Theories of galaxy formation predicted that there is a minimum threshold of dark matter required to ignite star formation and turn a dark cloud into a luminous galaxy.
'With Cloud-9, we have an example of an object just below this threshold, containing no stars.'
Although some scientists had thought that RELHICs might exist, they have proven exceptionally hard to find.
If the cloud were much larger, the gases would collapse into stars and form a galaxy; much smaller, and it would have fallen apart and blown away.
Co-author Dr Alejandro Benitez Llambay, of the Milano-Bicocca University in Milan, told Daily Mail: 'Cloud-9 is a rare "middle ground" survivor.'
'According to our models, fewer than 10 per cent of halos in this mass range remain in such a pristine state, making Cloud-9 a "missing link" in our understanding of how galaxies are born.'
Likewise, since these objects don't contain any stars, RELHICs barely give off any of their own radiation and are exceptionally difficult to detect.
Cloud-9 was first spotted three years ago by the Five-hundred-meter Aperture Spherical Telescope (FAST) in Guizhou, China.
If the cloud had more mass, the gases would have collapsed into stars and formed a galaxy like its neighbour, the M94 spiral galaxy (pictured). Cloud-9 had just enough mass to stay together, but not so much that it formed stars
However, it is only now that researchers have been able to use the Hubble Telescope to confirm that it contains no stars, making it very likely to be a RELHIC.
Lead author Dr Gagandeep Anand, of the Space Telescope Science Institute, says: 'Before we used Hubble, you could argue that this is a faint dwarf galaxy that we could not see with ground-based telescopes. They just didn't go deep enough in sensitivity to uncover stars.
'In science, we usually learn more from the failures than from the successes. In this case, seeing no stars is what proves the theory right. It tells us that we have found in the local universe a primordial building block of a galaxy that hasn't formed.'
The discovery of Cloud-9, published in The Astrophysical Journal Letters, also makes it likely that there are more RELHICs out there, even in our local neighbourhood.
China's FAST telescope is particularly good at spotting these kinds of dark gas clouds, so researchers hope to discover more in the future.
Dr Fox adds: 'There absolutely should be more RELHICs out there, and we are looking for more candidates. We need more cases to know whether Cloud-9 is an oddball with unusual properties, or alternatively, is fairly typical.'
Dark matter is a hypothetical substance said to make up roughly 85 per cent of the universe.
The enigmatic material is invisible because it does not reflect light, and has never been directly observed by scientists.
Astronomers know it to be out there because of its gravitational effects on known matter.
The European Space Agency says: 'Shine a torch in a completely dark room, and you will see only what the torch illuminates.
Dark matter is a hypothetical substance said to make up roughly 27 per cent of the universe. It is thought to be the gravitational 'glue' that holds the galaxies together
(artist's impression)
'That does not mean that the room around you does not exist.
'Similarly we know dark matter exists but have never observed it directly.'
The material is thought to be the gravitational 'glue' that holds the galaxies together.
Calculations show that many galaxies would be torn apart instead of rotating if they weren't held together by a large amount of dark matter.
Just five per cent the observable universe consists of known matter such as atoms and subatomic particles.
'Artificial intelligence' myths have existed for centuries — from the ancient Greeks to a pope's chatbot
Prometheus – Heinrich Füger (c.1817)
(Image credit: Heinrich Füger, Public domain, via Wikimedia Commons)
It seems the AIhype has turned into an AI bubble. There have been many bubbles before, from the Tulip mania of the 17th century to the derivatives bubbleof the 21st century. For many commentators, the most relevant precedent today is the dotcom bubble of the 1990s. Back then, a new technology (the World Wide Web) unleashed a wave of "irrational exuberance." Investors poured billions into any company with ".com" in the name.
Three decades later, another new technology has unleashed another wave of exuberance. Investors are pouring billions into any company with "AI" in its name. But there is a crucial difference between these two bubbles, which isn't always recognised. The World Wide Web existed. It was real. General Artificial Intelligence does not exist, and no one knows if or when it ever will.
In February, the CEO of OpenAI, Sam Altman, wrote on his blog that the very latest systems have only just started to "point towards" AI in its "general" sense. OpenAI may market its products as "AIs," but they are merely statistical data-crunchers, rather than "intelligences" in the sense that human beings are intelligent.
So why are investors so keen to give money to the people selling AI systems? One reason might be that AI is a mythical technology. I don't mean it is a lie. I mean it evokes a powerful, foundational story of Western culture about human powers of creation.
Perhaps investors are willing to believe AI is just around the corner because it taps into myths that are deeply ingrained in their imaginations?
The myth of Prometheus
The most relevant myth for AI is the Ancient Greek myth of Prometheus.
Prometheus was a Titan, a god in the Ancient Greek pantheon. He was also a criminal who stole fire from Hephaestus, the blacksmith god. Hiding the fire in a stalk of fennel, Prometheus came to earth and gave it to humankind. As punishment, he was chained to a mountain, where an eagle visited every day to eat his liver.
Prometheus' gift was not simply the gift of fire; it was the gift of intelligence. In Prometheus Bound, he declares that before his gift humans saw without seeing and heard without hearing. After his gift, humans could write, build houses, read the stars, perform mathematics, domesticate animals, construct ships, invent medicines, interpret dreams and give proper offerings to the gods.
The myth of Prometheus is a creation story with a difference. In the Hebrew Bible, God does not give Adam the power to create life. But Prometheus gives (some of) the gods' creative power to humankind.Hesiod indicates this aspect of the myth in Theogony. In that poem, Zeus not only punishes Prometheus for the theft of fire; he punishes humankind as well. He orders Hephaestus to fire up his forge and construct the first woman, Pandora, who unleashes evil on the world.
The fire that Hephaestus uses to make Pandora is the same fire that Prometheus has given humankind.
In this 18th-century engraving, Prometheus constructs the first man.
The Greeks proposed the idea that humans are a form of artificial intelligence. Prometheus and Hephaestus use technology to manufacture men and women. As historian Adrienne Mayor reveals in her book Gods and Robots, the ancients often depicted Prometheus as a craftsman, using ordinary tools to create human beings in an ordinary workshop.
If Prometheus gave us the fire of the gods, it would seem to follow that we can use this fire to make our own intelligent beings. Such stories abound in Ancient Greek literature, from the inventor Daedalus, who created statues that came to life, to the witch Medea, who could restore youth and potency with her cunning drugs. Greek inventors also constructed mechanical computers for astronomy and remarkable moving figures powered by gravity, water and air.
The Pope and the chatbot
2,700 years have passed since Hesiod first wrote down the story of Prometheus. In the ensuing centuries, the myth has been endlessly retold, especially since the publication of Mary Shelley's Frankenstein; or the Modern Prometheus in 1818.
But the myth is not always told as fiction. Here are two historical examples where the myth of Prometheus seemed to come true.
Gerbert of Aurillac was the Prometheus of the 10th century. He was born in the early 940s CE, went to school at Aurillac Abbey, and became a monk himself. He proceeded to master every known branch of learning. In the year 999, he was elected Pope. He died in 1003 under his pontifical name, Sylvester II.
Rumours about Gerbert spread wildly across Europe. Within a century of his death, his life had already become legend. One of the most famous legends, and the most pertinent in our age of AI hype, is that of Gerbert's "brazen head." The legend was told in the 1120s by the English historian William of Malmesbury, in his well researched and highly regarded book, Deeds of the English Kings.
Gerbert was deeply learned in astronomy, a science of prediction. Astronomers could use the astrolabe to predict the position of the stars and foresee cosmological events such as eclipses. According to William, Gerbert used his knowledge of astronomy to construct a talking head. After inspecting the movements of the stars and planets, he cast a head in bronze that could answer yes-or-no questions.
First Gerbert asked the head:
"Will I become Pope?"
"Yes," answered the head.
Then Gerbert asked: "Will I die before I sing mass in Jerusalem?"
"No," the head replied.
In both cases, the head was correct, though not as Gerbert anticipated. He did become Pope, and he sensibly avoided going on pilgrimage to Jerusalem. One day, however, he sang mass at Santa Croce in Gerusalemme in Rome. Unfortunately for Gerbert, Santa Croce in Gerusalemme was known in those days simply as "Jerusalem."
Gerbert sickened and died. On his deathbed, he asked his attendants to cut up his body and cast away the pieces, so he could go to his true master, Satan. In this way, he was, like Prometheus, punished for his theft of fire.
It is a thrilling story. It is not clear whether William of Malmesbury actually believed it. But he does try to persuade his readers that it is plausible. Why did this great historian with a devotion to the truth insert some fanciful legends about a French pope into his history of England? Good question!
Is it so fanciful to believe that an advanced astronomer might build a general-purpose prediction machine? In those days, astronomy was the most powerful science of prediction. The sober and scholarly William was at least willing to entertain the idea that brilliant advances in astronomy might make it possible for a Pope to build an intelligent chatbot.
Today, that same possibility is credited to machine-learning algorithms, which can predict which ad you will click, which movie you will watch, which word you will type next. We can be forgiven for falling under the same spell.
The anatomist and the automaton
The Prometheus of the 18th century was Jacques de Vaucanson, at least according to Voltaire:
Bold Vaucanson, rival of Prometheus,Seems, imitating the springs of nature,To steal the fire of heaven to animate the body.
Jacques de Vaucanson – Joseph Boze (1784)
(Image credit: Joseph Boze, Public domain, via Wikimedia Commons)
Vaucanson was a great machinist, famous for his automata. These were clockwork devices that realistically simulated human or animal anatomy. Philosophers of the time believed that the body was a machine — so why couldn't a machinist build one?
Sometimes Vaucanson's automata were scientifically significant. He constructed a piper, for example, that had lips and lungs and fingers, and blew the pipe in much the same way a human would. Historian Jessica Riskin explains in her book The Restless Clock that Vaucanson had to make significant discoveries in acoustics in order to make his piper play in tune.
Sometimes his automata were less scientific. His digesting duck was hugely famous, but turned out to be fraudulent. It appeared to eat and digest food, but its poos were in fact prefabricated pellets hidden inside the mechanism.
Vaucanson spent decades working on what he called a "moving anatomy." In 1741, he presented a plan to the Lyons Academy to build an "imitation of all animal operations." Twenty years later, he was at it again. He secured support from King Louis XV to build a simulation of the circulatory system. He claimed he could build a complete, living artificial body.
Three of Vaucanson’s famous automata: the Flute Player, the Digesting Duck, and the Provençal Farmer, who played the pipe and tambourine. (Image credit: See page for author,Public domain, via Wikimedia Commons)
There is no evidence that Vaucanson ever completed a whole body. In the end, he couldn't live up to the hype. But many of his contemporaries believed he could do it. They wanted to believe in his magical mechanisms. They wished he would seize the fire of life.
If Vaucanson could manufacture a new human body, couldn't he also repair an existing one? This is the promise of some AI companies today. According to Dario Amodei, CEO of Anthropic, AI will soon allow people "to live as long as they want." Immortality seems like an attractive investment.
Sylvester II and Vaucanson were great technologists, but neither was a Prometheus. They stole no fire from the gods. Will the aspiring Prometheans of Silicon Valley succeed where their predecessors have failed? If only we had Sylvester II's brazen head, we could ask it.
Chang’e 4 is a Chinese space probe that landed on the far side of the Moon on January 3, 2019. It not only studied the chemical composition of the rocks in this location, but also conducted the first experiment in history to grow plants on another celestial body.
The Chang’e 4 spacecraft
Chinese space program
January 3, 2019, was a triumph for the Chinese space program. The rest of humanity also had reason to rejoice. For the first time in history, the Chang’e 4 spacecraft landed on the far side of the Moon, which we never see from Earth.
The road to this landing was quite long. China was late to the lunar race between the US and the USSR. The PRC had to implement its lunar program in the 21st century. It began with two spacecraft that operated in lunar orbit, photographing and remotely sensing the Moon. Both were named after Chang’e, the Chinese goddess of the Moon.
Initially, the Chang’e 1 spacecraft operated in lunar orbit from 2007 to 2009. It made general observations, which were hardly surprising at the time, since the US had already found water on our satellite.
However, in 2010, Chang’e 2 was launched to the Moon. It photographed the surface of our satellite from an altitude of only 100 km. In 2012, based on the data it collected, the Chinese government presented the most detailed map of the Moon at that time, and it was confirmed that all this time, the Chinese had been looking for a landing site for Chang’e 3.
Around that time, the first discussions about China’s lunar ambitions began, but no one knew how seriously to take them, since only two countries – the US and the USSR – had successfully landed on the Moon at that point.
However, on December 14, 2013, Chang’e 3 landed in the Sinus Iridum of the Mare Imbrium. It was not only the first spacecraft in 37 years to remain intact after reaching the surface of our satellite. It also carried the Yutu rover, named after the jade rabbit, a character from Chinese legends who is said to have prepared the powder of immortality on the Moon. At that time, China was able to explore the material of our satellite for the first time and confirm that it was exactly as American and Soviet scientists had determined.
The Chang’e 3 landing site. Source: Wikipedia
The Chang’e 4
However, all this was a repeat of achievements made many years ago. In order to challenge the US, which had already announced plans to return to the Moon, it was necessary to show that Chinese missions could provide the global scientific community with data that no one had previously had access to.
This was the goal of the Chang’e 4 probe. In terms of design, it was a copy of the previous mission, with the same cameras and spectrographs, and even carried the Yutu-2 rover on board. However, this device was to land on the far side of the Moon, which humans first saw only in 1959 and, before the Chinese attempt, had only seen from orbit.
Moreover, Chang’e 4 was supposed to land in the Von Kármán lunar crater, which covers the much older and largest basin on our satellite, the South Pole-Aitken basin. Once, at the dawn of the solar system’s existence, a body much larger than the asteroid that ended the dinosaurs crashed into the Moon, which, scientists believe, led to the asymmetry of its two hemispheres: the visible and the reverse.
South Pole-Aitken basin. Source: Wikipedia
Almost all experimental data confirming this was obtained thanks to the Chinese missions Chang’e 4 and Chang’e 5, which followed it. But for them to be possible, it was first necessary to ensure their connection with Earth. This mission was entrusted to the Queqiao-1 relay satellite, which was launched to the Lagrange 2 point of the Earth-Moon system, i.e., directly behind our natural satellite.
Queqiao-1 began operating in May 2018, and in December of the same year, Chang’e 4 was launched to the Moon. It remained in orbit around our satellite for some time, and on January 3, 2019, it landed at the planned location. On the same day, it began scientific research and took photographs.
Yutu-2 rolled off the platform and began performing spectroscopic analysis of the rocks. After a few days, scientists had to interrupt their work because night fell on the Moon and the temperature dropped to extreme levels. However, two weeks later, when dawn finally broke, the mission resumed its work.
Yutu-2 . Source: news.cgtn.com
In total, Chang’e 4 lasted more than a year and a half. Technically, the mission is not yet complete. It is currently in sleep mode. Ultimately, it accomplished its main task: it examined the mantle rock emissions and noted how they are similar to and different from those found on the visible side of the Moon.
Growing plants on the Moon
The biggest difference in the design of Chang’e 4 from previous spacecraft was the addition of a module for biological experiments. It consisted of germinating seeds. This had been done repeatedly in space before, but it was all in Earth orbit.
It was Chang’e 4 that became the first spacecraft to successfully grow cotton, potato, and rapeseed seeds on another celestial body. This happened a few days after landing, and photos of the tiny sprouts went viral around the world. The experiment was supposed to last 100 days. During this time, the capsule with the samples had to be heated and humidified.
Plants on the Moon. Source: nextshark.com
Incidentally, it also contained yeast spores and Drosophila fly eggs. So, theoretically, an entire ecosystem could have developed on board in later stages. However, with the onset of the lunar night, the temperature outside dropped too sharply, and too much electricity was needed for heating. Therefore, the experiment had to be interrupted.
Nevertheless, it is considered successful and was extremely important for global science. It proved the fundamental ability of plants to overcome the most difficult stage of their development in space conditions. In the future, humans will inevitably live in space, and we will need oxygen and nutrients that plants can provide. To achieve this, large modules with artificial biospheres will need to be created on planets. Similar to the one that was on board Chang’e 4.
A newly discovered galaxy cluster could rewrite our understanding of the cosmos, as scientists spot 'something the universe wasn’t supposed to have’.
Researchers found that the cluster was burning five times hotter than expected just 1.4 billion years after the Big Bang.
Astronomers had thought that such extreme temperatures would only be possible in more mature, stable galaxy clusters that formed later in the universe's life.
This hot 'baby cluster' could suggest that the earliest moments of the universe were far more explosive than previously thought.
Scientists believe that the unexpected heat might be the product of three supermassive black holes hidden in the depths of the cluster.
Co-author Dazhi Zhou, a PhD candidate at the University of British Columbia, says: 'We didn’t expect to see such a hot cluster atmosphere so early in cosmic history.
'In fact, at first I was sceptical about the signal as it was too strong to be real.
'But after months of verification, we’ve confirmed this gas is at least five times hotter than predicted, and even hotter and more energetic than what we find in many present-day clusters.'
Scientists have discovered 'something the universe wasn’t supposed to have' as they find a galaxy cluster burning five times hotter than expected just 1.4 billion years after the Big Bang
They are enormous collections of individual galaxies, invisible dark matter, and superheated clouds of gas.
In the spaces between the galaxies, gas is heated into plasma that can reach hundreds of millions of degrees and shines brightly in the X-ray spectrum.
Scientists had thought this 'intracluster medium' was heated by gravitational interactions between galaxies as an immature, unstable cluster matures and collapses inward to a stable state.
However, the researchers' new discovery, published in Nature, suggests that this model of evolution might not be correct.
Using a group of telescopes known as the Atacama Large Millimeter/submillimeter Array (ALMA), the researchers looked 12 billion years into the past.
At this time, the galaxy cluster dubbed SPT2349-56 was extremely immature, but already extraordinarily large for its age.
Its core extends more than 500,000 light-years across, roughly the size of the vast halo of matter and dark matter surrounding the Milky Way.
Galaxy clusters are some of the largest objects in the universe, sometimes containing thousands of individual galaxies connected by clouds of superheated gas known as the intracluster medium. Pictured: A separate globular cluster known as NGC 2210
Using the ALMA (Atacama Large Millimeter/submillimeter Array) observatory, scientists measure the temperature of the intracluster medium in a galaxy cluster over 12 billion light-years from Earth. They discovered that this was far hotter than the best theories predicted
The cluster also contains more than 30 extremely active galaxies which produce stars over 5,000 times faster than our own galaxy.
However, when researchers used ALMA to measure the temperature of the intracluster medium, they found that it was far hotter than the models predicted for this time in the universe.
Scientists aren't entirely sure how the cluster came to be so much hotter than expected.
However, the researchers suggest that it could be related to the three recently discovered supermassive black holes in the cluster.
Supermassive black holes are the largest class of black holes, with masses at least 100,000 times greater than that of our sun.
Supermassive black holes are typically found in the hearts of galaxies, where they feed on gases and release huge quantities of X-ray radiation.
Co-author Professor Scott Chapman, of Dalhousie University who conducted the research while at the National Research Council of Canada, says that these black holes were 'already pumping huge amounts of energy into the surroundings and shaping the young cluster, much earlier and more strongly than we thought.'
Scientists say the heat was likely generated by three supermassive black holes. These are the largest class of black holes (artist's impression), and typically form in the cores of galaxies
This comes after researchers found a supermassive black hole actively growing inside a galaxy just 570 million years after the Big Bang (pictured), suggesting that black holes might have grown faster in the early universe than expected
Last year, researchers using the James Webb Space Telescope spotted a 'little red dot' supermassive black hole that was actively growing inside a galaxy just 570 million years after the Big Bang.
Importantly, this black hole was much bigger than the size of the host galaxy would suggest.
This implies that black holes may have grown faster than the galaxies that hosted them in the early universe, even in relatively small galaxies.
Professor Chapman says that studying how these dynamics unfold is critical to explaining the universe around us today.
He says: 'Understanding galaxy clusters is the key to understanding the biggest galaxies in the universe.
'These massive galaxies mostly reside in clusters, and their evolution is heavily shaped by the very strong environment of the clusters as they form, including the intracluster medium.'
Black holes are so dense and their gravitational pull is so strong that no form of radiation can escape them - not even light.
They act as intense sources of gravity which hoover up dust and gas around them. Their intense gravitational pull is thought to be what stars in galaxies orbit around.
How they are formed is still poorly understood. Astronomers believe they may form when a large cloud of gas up to 100,000 times bigger than the sun, collapses into a black hole.
Many of these black hole seeds then merge to form much larger supermassive black holes, which are found at the centre of every known massive galaxy.
Alternatively, a supermassive black hole seed could come from a giant star, about 100 times the sun's mass, that ultimately forms into a black hole after it runs out of fuel and collapses.
When these giant stars die, they also go 'supernova', a huge explosion that expels the matter from the outer layers of the star into deep space.
Chang’e 4 is a Chinese space probe that landed on the far side of the Moon on January 3, 2019. It not only studied the chemical composition of the rocks in this location, but also conducted the first experiment in history to grow plants on another celestial body.
The Chang’e 4 spacecraft
Chinese space program
January 3, 2019, was a triumph for the Chinese space program. The rest of humanity also had reason to rejoice. For the first time in history, the Chang’e 4 spacecraft landed on the far side of the Moon, which we never see from Earth.
The road to this landing was quite long. China was late to the lunar race between the US and the USSR. The PRC had to implement its lunar program in the 21st century. It began with two spacecraft that operated in lunar orbit, photographing and remotely sensing the Moon. Both were named after Chang’e, the Chinese goddess of the Moon.
Initially, the Chang’e 1 spacecraft operated in lunar orbit from 2007 to 2009. It made general observations, which were hardly surprising at the time, since the US had already found water on our satellite.
However, in 2010, Chang’e 2 was launched to the Moon. It photographed the surface of our satellite from an altitude of only 100 km. In 2012, based on the data it collected, the Chinese government presented the most detailed map of the Moon at that time, and it was confirmed that all this time, the Chinese had been looking for a landing site for Chang’e 3.
Around that time, the first discussions about China’s lunar ambitions began, but no one knew how seriously to take them, since only two countries – the US and the USSR – had successfully landed on the Moon at that point.
However, on December 14, 2013, Chang’e 3 landed in the Sinus Iridum of the Mare Imbrium. It was not only the first spacecraft in 37 years to remain intact after reaching the surface of our satellite. It also carried the Yutu rover, named after the jade rabbit, a character from Chinese legends who is said to have prepared the powder of immortality on the Moon. At that time, China was able to explore the material of our satellite for the first time and confirm that it was exactly as American and Soviet scientists had determined.
The Chang’e 3 landing site. Source: Wikipedia
The Chang’e 4
However, all this was a repeat of achievements made many years ago. In order to challenge the US, which had already announced plans to return to the Moon, it was necessary to show that Chinese missions could provide the global scientific community with data that no one had previously had access to.
This was the goal of the Chang’e 4 probe. In terms of design, it was a copy of the previous mission, with the same cameras and spectrographs, and even carried the Yutu-2 rover on board. However, this device was to land on the far side of the Moon, which humans first saw only in 1959 and, before the Chinese attempt, had only seen from orbit.
Moreover, Chang’e 4 was supposed to land in the Von Kármán lunar crater, which covers the much older and largest basin on our satellite, the South Pole-Aitken basin. Once, at the dawn of the solar system’s existence, a body much larger than the asteroid that ended the dinosaurs crashed into the Moon, which, scientists believe, led to the asymmetry of its two hemispheres: the visible and the reverse.
South Pole-Aitken basin. Source: Wikipedia
Almost all experimental data confirming this was obtained thanks to the Chinese missions Chang’e 4 and Chang’e 5, which followed it. But for them to be possible, it was first necessary to ensure their connection with Earth. This mission was entrusted to the Queqiao-1 relay satellite, which was launched to the Lagrange 2 point of the Earth-Moon system, i.e., directly behind our natural satellite.
Queqiao-1 began operating in May 2018, and in December of the same year, Chang’e 4 was launched to the Moon. It remained in orbit around our satellite for some time, and on January 3, 2019, it landed at the planned location. On the same day, it began scientific research and took photographs.
Yutu-2 rolled off the platform and began performing spectroscopic analysis of the rocks. After a few days, scientists had to interrupt their work because night fell on the Moon and the temperature dropped to extreme levels. However, two weeks later, when dawn finally broke, the mission resumed its work.
Yutu-2 . Source: news.cgtn.com
In total, Chang’e 4 lasted more than a year and a half. Technically, the mission is not yet complete. It is currently in sleep mode. Ultimately, it accomplished its main task: it examined the mantle rock emissions and noted how they are similar to and different from those found on the visible side of the Moon.
Growing plants on the Moon
The biggest difference in the design of Chang’e 4 from previous spacecraft was the addition of a module for biological experiments. It consisted of germinating seeds. This had been done repeatedly in space before, but it was all in Earth orbit.
It was Chang’e 4 that became the first spacecraft to successfully grow cotton, potato, and rapeseed seeds on another celestial body. This happened a few days after landing, and photos of the tiny sprouts went viral around the world. The experiment was supposed to last 100 days. During this time, the capsule with the samples had to be heated and humidified.
Plants on the Moon. Source: nextshark.com
Incidentally, it also contained yeast spores and Drosophila fly eggs. So, theoretically, an entire ecosystem could have developed on board in later stages. However, with the onset of the lunar night, the temperature outside dropped too sharply, and too much electricity was needed for heating. Therefore, the experiment had to be interrupted.
Nevertheless, it is considered successful and was extremely important for global science. It proved the fundamental ability of plants to overcome the most difficult stage of their development in space conditions. In the future, humans will inevitably live in space, and we will need oxygen and nutrients that plants can provide. To achieve this, large modules with artificial biospheres will need to be created on planets. Similar to the one that was on board Chang’e 4.
The US Space Agency has announced a search for an innovative system to detect and neutralize potential airborne threats in the form of drones. The goal is to protect personnel, rockets, and critical infrastructure in the area of the Kennedy Space Center at Cape Canaveral.
Any outside interference in the Kennedy Space Center area at Cape Canaveral, even accidental, could have catastrophic consequences. Illustration generated by Copilot AI
The Kennedy Space Center is the heart of the Artemis lunar program, from where powerful Space Launch System rockets will be launched. Any outside interference, even accidental, could have catastrophic consequences.
How the “smart shield” will work
Space Launch System rocket. Source: JOE SKIPPER | REUTERS
According to the agency’s request, the system should include a network of stationary and mobile sensors (radar, radio frequency, optical). Its key tasks are:
Detect and identify unknown drones at a distance of up to 64 km.
Analyze risk in real time.
Provide data for quick decision-making by the security service.
The system is scheduled to be implemented in April 2026. From now on, all drone flights in the central area will be strictly limited and will require special permission.
Balancing security and innovation
Interestingly, NASA itself periodically uses drones for festive events – for example, the visitor center hosts a show featuring 600 autonomous devices. The new system is designed to distinguish authorized flights from potentially dangerous ones, protecting the future of lunar missions.
This move demonstrates how space agencies are adapting to the challenges of a new era, where advanced technologies can bring both benefits and risks.
The idea of humans living beyond Earth was once only possible in science fiction, but now space agencies are making plans to bring space colonization closer to reality. NASA and SpaceXare exploring long-term missions to the moon and Mars, while astronomers continue to discover potentially habitable exoplanets orbiting distant stars beyond our solar system.
Supporters of planetary colonization argue that becoming a multi-planet species could safeguard us from potentially Earth-ending events. However, it will require an enormous effort to colonize another planet or moon. And if we look beyond Mars, potentially habitable planets may take thousands of years to reach.
But as technology advances and space agencies consider long-term human settlements on other planets, a more fundamental issue now beckons — not whether we can expand to other worlds, but whether we should.
What's your take? Answer our poll below and share the reasoning behind your choice in the comments.
Tractor beams inspired by sci-fi are real, and could solve the looming space junk problem
Tractor beams inspired by sci-fi are real, and could solve the looming space junk problem
Researchers are developing a real-life tractor beam, with the goal of pulling defunct satellites out of geostationary orbit to alleviate the space junk problem.
An artist's illustration shows how an electrostatic tractor beam could be used to pull defunct satellites out of geostationary orbit around Earth. In reality, the beam would be invisible.
In science fiction films, nothing raises tension quite like the good guys' spaceship getting caught in an invisible tractor beam that allows the baddies to slowly reel them in. But what was once only a sci-fi staple could soon become a reality.
Scientists are developing a real-life tractor beam, dubbed an electrostatic tractor. This tractor beam wouldn't suck in helpless starship pilots, however. Instead, it would use electrostatic attraction to nudge hazardous space junk safely out of Earth orbit.
The science is pretty much there, but the funding is not.
The electrostatic tractor beam could potentially alleviate that problem by safely moving dead satellites far out of Earth orbit, where they would drift harmlessly for eternity.
While the tractor beam wouldn't completely solve the space junk problem, the concept has several advantages over other proposed space debris removal methods, which could make it a valuable tool for tackling the issue, experts told Live Science.
A prototype could cost millions, and an operational, full-scale version even more. But if the financial hurdles can be overcome, the tractor beam could be operational within a decade, its builders say.
"The science is pretty much there, but the funding is not," project researcher Kaylee Champion, a doctoral student in the Department of Aerospace Engineering Sciences at the University of Colorado Boulder (CU Boulder), told Live Science.
Avoiding Disaster
Tractor beams are a staple of sci-fi films and TV shows, such as Star Trek.
(Image credit: Star Trek)
The tractor beams depicted in "Star Wars" and "Star Trek" suck up spacecraft via artificial gravity or an ambiguous "energy field." Such technology is likely beyond anything humans will ever achieve. But the concept inspired Hanspeter Schaub, an aerospace engineering professor at CU Boulder, to conceptualize a more realistic version.
In the wake of this disaster, Schaub wanted to be able to prevent this from happening again. To do this, he realized you could pull spacecraft out of harm's way by using the attraction between positively and negatively charged objects to make them "stick" together.
Over the next decade, Schaub and colleagues refined the concept. Now, they hope it can someday be used to move dead satellites out of geostationary orbit (GEO) — an orbit around Earth's equator where an object's speed matches the planet's rotation, making it seem like the object is fixed in place above a certain point on Earth. This would then free up space for other objects in GEO, which is considered "prime real estate" for satellites, Schaub said.
How does it work?
The researchers have been testing the electron gun on pieces of metal in the lab.
(Image credit: Nico Goda/CU Boulder)
The electrostatic tractor would use a servicer spacecraft equipped with an electron gun that would fire negatively charged electrons at a dead target satellite, Champion told Live Science. The electrons would give the target a negative charge while leaving the servicer with a positive charge. The electrostatic attraction between the two would keep them locked together despite being separated by 65 to 100 feet (20 to 30 meters) of empty space, she said.
Once the servicer and target are "stuck together," the servicer would be able to pull the target out of orbit without touching it. Ideally, the defunct satellite would be pulled into a "graveyard orbit" more distant from Earth, where it could safely drift forever, Champion said.
The electrostatic attraction between the two spacecraft would be extremely weak, due to limitations in electron gun technology and the distance by which the two would need to be separated to prevent collisions, project researcher Julian Hammerl, a doctoral student at CU Boulder, told Live Science. So the servicer would have to move very slowly, and it could take more than a month to fully move a single satellite out of GEO, he added.
That's a far cry from movie tractor beams, which are inescapable and rapidly reel in their prey. This is the "main difference between sci-fi and reality," Hammerl said.
Advantages and limitations
The amount of space junk surrounding Earth has greatly increased in recent years. Here is a comparison of space junk in 1965 (left) and 2010 (right).
(Image credit: NASA)
The electrostatic tractor would have one big advantage over other proposed space junk removal methods, such as harpoons, giant nets and physical docking systems: It would be completely touchless.
"You have these large, dead spacecraft about the size of a school bus rotating really fast," Hammerl said. "If you shoot a harpoon, use a big net or try to dock with them, then the physical contact can damage the spacecraft and then you are only making the [space junk] problem worse."
Scientists have proposed other touchless methods, such as using powerful magnets, but enormous magnets are both expensive to produce and would likely interfere with a servicer's controls, Champion said.
The main limitation of the electrostatic tractor is how slowly it would work. More than 550 satellites currently orbit Earth in GEO, but that number is expected to rise sharply in the coming decades.
If satellites were moved one at a time, then a single electrostatic tractor wouldn't keep pace with the number of satellites winking out of operation. Another limitation of the electrostatic tractor is that it would work too slowly to be practical for clearing smaller pieces of space junk, so it wouldn't be able to keep GEO completely free of debris.
Cost is the other big obstacle. The team has not yet done a full cost analysis for the electrostatic tractor, Schaub said, but it would likely cost tens of millions of dollars. However, once the servicer were in space, it would be relatively cost-effective to operate it, he added.
Next steps
Researcher Julian Hammerl photographed next to the ECLIPS machine at CU Boulder.
(Image credit: Nico Goda/CU Boulder)
The researchers are currently working on a series of experiments in their Electrostatic Charging Laboratory for Interactions between Plasma and Spacecraft (ECLIPS) machine at CU Boulder. The bathtub-sized, metallic vacuum chamber, which is equipped with an electron gun, allows the team to "do unique experiments that almost no one else can currently do" in order to simulate the effects of an electrostatic tractor on a smaller scale, Hammerl said.
Once the team is ready, the final and most challenging hurdle will be to secure funding for the first mission, which is a process they have not yet started.
Most of the mission cost would come from building and launching the servicer. However, the researchers would ideally like to launch two satellites for the first tests, a servicer and a target that they can maneuver, which would give them more control over their experiments but also double the cost.
If they can somehow wrangle that funding, a prototype tractor beam could be operational in around 10 years, the team previously estimated.
Is it viable?
Space junk is becoming a major problem for the space exploration industry.
(Image credit: CU Boulder)
While tractor beams may sound like a pipe dream, experts are optimistic about the technology.
"Their technology is still in the infancy stage," John Crassidis, an aerospace scientist at the University at Buffalo in New York, who is not involved in the research, told Live Science in an email. "But I am fairly confident it will work."
If you shoot a harpoon, use a big net or try to dock with them, then the physical contact can damage the spacecraft and then you are only making the [space junk] problem worse.
Removing space junk without touching it would also be much safer than any current alternative method, Crassidis added.
The electrostatic tractor "should be able to produce the forces necessary to move a defunct satellite" and "certainly has a high potential to work in practice," Carolin Frueh, an associate professor of aeronautics and astronautics at Purdue University in Indiana, told Live Science in an email. "But there are still several engineering challenges to be solved along the way to make it real-world-ready."
Scientists should continue to research other possible solutions, Crassidis said. Even if the CU Boulder team doesn't create a "final product" to remove nonfunctional satellites, their research will provide a stepping stone for other scientists, he added.
The interstellar comet 3I/ATLAS has been the subject of a flurry of sensational reports claiming that it is an alien spacecraft. However, recent studies show that no technosignatures, i.e., radio signals or emissions of substances indicating that extraterrestrial technology is operating on its surface, have been detected.
Comet 3I/ATLAS turned out not to be an alien spacecraft after all. Source: starwalk.space
New observations
Since the interstellar object (ISO) 3I/ATLAS was first discovered on July 1, 2025, it has garnered much attention, including speculation, hopes, and fears that it may somehow contain evidence of technologically advanced civilizations outside of our solar system.
Now, a new paper published on the arXiv preprint server details the findings from radio observations made at the 100-meter Green Bank Telescope as a part of the Breakthrough Listen program, designed to look for signs of alien life. The data were taken on December 18, 2025 — the day before the object’s closest approach to Earth, and those hoping for evidence of advanced alien civilizations may not like the results.
3I/ATLAS — natural or artificial object?
Only two other ISOs have ever been observed to enter our solar system. The first ISO, 1I/Oumuamua, was initially classified as an asteroid, then a comet; while the second, 2I/Borisov, was deemed to be a comet. 3I/ATLAS exhibits typical cometary characteristics, like a coma and an unelongated nucleus.
Yet, these objects often initially spark a lot of speculation. After its discovery, many rumors spread online about odd features of 3I/ATLAS indicating alien technology. However, scientists have also been actively studying the object, albeit with a bit more skepticism.
Now that six months have passed since its discovery, multiple telescopes have taken data in various wavelength bands, including radio, infrared, X-ray, and optical, and these data have been analyzed by many researchers. According to SETI, none of these observations have resulted in evidence of technosignatures.
Green Bank observations
The researchers involved in the new study say that interstellar probes are most likely to communicate using narrowband radio signals, due to their transmission efficiency and because of the low extinction associated with these signals across interstellar space. And so, the team conducted their signal search at four different radio bands covering 1-12 GHz right around the time of the comet’s closest approach.
The search picked up over 471,000 candidate signals initially, but after applying a sky localization filter, they were left with nine “events.” Further analysis showed that these were due to radio frequency interference, as they also appeared in off-target scans or were known contaminants. Even with its higher levels of sensitivity, the analysis found no candidate technosignature signals from 3I/ATLAS, which is in line with the results of other studies.
The study authors write, “Our survey concludes that there are no isotropic continuous-wave transmitters above 0.1W at the location of 3I/ATLAS. For comparison, a cell phone is an approximately isotropic continuous-wave transmitter at a level of ∼1W.”
The search continues
The data used in this study and other studies from the Breakthrough Listen program are publicly available, and data collection will continue on certain telescopes, such as Hubble. Those interested in 3I/ATLAS can expect more information to come, although it is unlikely at this point that technosignatures will be found.
Still, Earth’s many telescopes will continue to be on the lookout for future ISOs entering our solar system and potential technosignatures.
Een tijdlijn die steeds sneller gaat De kolonisatie van Mars komt steeds dichterbij. Elon Musk, de CEO van SpaceX, heeft een nieuwe streefdatum aangekondigd voor de eerste Starship-missie naar de Rode Planeet. Volgens Musk zou deze missie tegen eind 2026 kunnen plaatsvinden. Dit ambitieuze tijdschema onderstreept de vooruitstrevende interplanetaire ambities van het bedrijf.
Mars vóór mensen Zoals de BBC meldt, zal de missie die voor 2026 gepland staat geen mensen aan boord hebben. Het plan is om een onbemande Starship te sturen, bedoeld als een grootschalige generale repetitie om cruciale systemen te testen voordat een menselijke landing wordt overwogen.
Een erkende kansberekening Musk schat de kans op ongeveer 50% dat SpaceX erin slaagt om binnen dit tijdsvenster een onbemande Starship naar Mars te sturen. Dat percentage weerspiegelt zowel technologisch optimisme als een opvallende erkenning van de omvang van de resterende uitdagingen.
Waarom 2026 cruciaal is Het jaar is geen toeval. In 2026 staan de aarde en Mars gunstig ten opzichte van elkaar, wat de reistijd en het brandstofverbruik aanzienlijk vermindert. Zo’n lanceervenster doet zich slechts ongeveer eens in de twee jaar voor.
Starship als spil van de strategie Starship vormt het hart van het hele plan. Met een hoogte van 123 meter is het het grootste raketsysteem ooit gebouwd en volledig ontworpen voor hergebruik. Voor Musk is het het onmisbare voertuig om Mars van idee tot daadwerkelijke bestemming te maken.
Tests getekend door explosies De weg naar Mars is allesbehalve probleemloos geweest. Starship kende meerdere mislukkingen tijdens testvluchten, waaronder twee explosies in de lucht in 2025. SpaceX analyseert momenteel gegevens om het verlies van meerdere motoren te begrijpen.
De rol van de toezichthouder Na het laatste incident eiste de Amerikaanse Federal Aviation Administration een formeel onderzoek voordat nieuwe vluchten worden toegestaan. Dat toezicht voegt extra onzekerheid toe aan een toch al kwetsbare planning.
Een eerste stap, geen nederzetting Ondanks het woord kolonisatie zal 2026 niet het jaar zijn waarin mensen op Mars wonen. In het beste geval markeert dit het begin van een reeks technische missies die het pad effenen, niet het eindpunt ervan, zoals ook de BBC benadrukt.
Mensen vanaf 2029 – of later Musk heeft aangegeven dat, als de eerste missies succesvol zijn, de eerste menselijke landingen rond 2029 zouden kunnen plaatsvinden. Tegelijkertijd erkent hij, zoals Al Jazeera opmerkt, dat 2031 waarschijnlijk realistischer is.
Een multiplanetaire visie Het uiteindelijke doel blijft om van de mensheid een multiplanetaire soort te maken. Mars neemt daarin een centrale plaats in, voorgesteld als een tweede thuis dat de overleving van de mens op lange termijn kan waarborgen.
Optimus als symbolische passagiert De eerste Marsmissie zou mogelijk de humanoïde robot Optimus van Tesla vervoeren. Zijn aanwezigheid zou vooral symbolisch zijn en technologische ambitie uitstralen, meer dan wetenschappelijke noodzaak.
Een robot voor de aarde – en verder Optimus werd in 2024 publiekelijk gepresenteerd en is ontworpen om alledaagse taken uit te voeren. Musk heeft gezegd dat de robot uiteindelijk tussen de 20.000 en 30.000 dollar zou kunnen kosten, wat het experimentele karakter onderstreept.
Mars en de maan, parallelle routes Mars is niet het enige doel op korte termijn. SpaceX speelt ook een sleutelrol in de maanplannen van NASA, waarbij een aangepaste versie van Starship moet dienen als menselijke lander voor het Artemis-programma.
Een lange geschiedenis van beloftes Musk heeft zijn tijdlijnen vaker moeten bijstellen. In 2016 sprak hij over een Marsmissie in 2018, in 2020 voorspelde hij menselijke aankomst zes jaar later, en in 2024 stelde hij opnieuw 2026 als mijlpaal.
Ambitie versus realiteit Deze geschiedenis verklaart waarom experts nieuwe aankondigingen met voorzichtigheid benaderen. Technische complexiteit, mislukte tests en regelgeving maken elke deadline voorlopig.
Verkenning als iteratief proces Binnen deze aanpak dient elke onbemande missie om systemen te valideren, fouten te corrigeren en risico’s te verkleinen voordat mensenlevens op het spel staan. Zelfs een mislukte poging in 2026 zou al een historisch moment betekenen.
Meer dan symboliek De impact zou verder reiken dan technologie alleen. Een interplanetaire lancering van deze schaal zou wetenschappelijke, economische en culturele gevolgen hebben op wereldniveau.
Voorzichtige verwachtingen Opmerkelijk genoeg temperde Musk zelf de verwachtingen. Zijn nadruk op een kans van 50% is ongebruikelijk in zijn retoriek en onderstreept de echte onzekerheid rond de missie.
Het begin van een verhaal Zo zal 2026 waarschijnlijk niet het jaar zijn waarin Mars daadwerkelijk wordt gekoloniseerd, maar het zou wel het jaar kunnen zijn waarin dat verhaal echt begint: een onzekere eerste stap, maar mogelijk een beslissen
2026 is shaping up to be a stellar year for space exploration with the return of crewed Moon missions, preparations for futureMarsmissions, planetary defense initiatives, and a final slingshot to determine if Jupiter’s moonEuropa could be habitable.
Just days into the New Year, on January 6, NASA will begin spacewalks outside the International Space Station to prepare for installing a new solar array. As 2026 continues, international missions will proliferate, heralding a promising year for scientific discoveries and space exploration.
NASA Returns to the Moon in 2026
NASA’s Artemis II mission will get the year off to an early start with current plans for an early-February launch for the first crewed lunar flyby since the Apollo program ended in 1972. Over the course of 10 days, it will bring astronauts around the Moon and back. During that time, Artemis II will test essential systems ahead of future moon landings under the Artemis program. These include the Orion life support system and optical communications between Earth and the Moon. Additionally, the mission will deploy cubesats from several countries, including Argentina, Saudi Arabia, and South Korea.
NASA Artemis II astronauts (left to right) Christina Koch, Victor Glover, Reid Wiseman, and Canadian Space Agency Astronaut Jeremy Hansen. Credit: NASA/Josh Valcarcel
Through NASA’s Commercial Lunar Payload Services (CLPS) initiative, the space agency will send essential materials to the lunar surface this year through two missions with private commercial partners. These missions will serve as important steps toward a crewed Artemis III Moon landing and, eventually, a permanent lunar base.
Intuitive Machines IM-3
The Intuitive Machines IM-3 mission builds on the IM-2 mission, which was cut short in 2025 due to touchdown errors, leaving the Athena lander unable to generate sufficient power. IM-3 will include multiple landers, a rover, robotic explorers, and an environmental monitor, with a particular focus on investigating the Reiner Gamma lunar swirl. The strange spiraling features known as lunar swirls are linked to magnetic anomalies that have long been observed on the Moon. IM-3 will investigate their nature and, ideally, provide scientists with new insights into how they form.
Meanwhile, Firefly Aerospace’s Blue Ghost Mission 2, set for late 2026, and its Elytra Dark orbital vehicle will deploy both Blue Ghost and the ESA’s Lunar Pathfinder satellite. After Blue Ghost sets down on the far side of the moon, Elyta will stay in orbit to provide communications relay and radio frequency calibration support for five years. The mission will lay the groundwork for permanent habitation by identifying helpful resources, testing lunar power network technologies, and improving lunar communications.
This year, SpaceX hopes to make Starship’s first orbital flight
(Credit: SpaceX)
From the Moon to Mars with SpaceX
SpaceX plans to continue operations with its twelfth Starship launch, which is expected to reach suborbital altitude. The booster stack for the launch has already been assembled, keeping the mission on track for February or March. Following that, flight thirteen may achieve Starship’s first orbital flight, proving the vehicle’s spaceworthiness.
Later in the year, SpaceX has even more ambitious plans for Starship, including testing and demonstrating its Human Landing System for a crewed Artemis III mission and possibly launching uncrewed upper stages to Mars. From October to December, the 2026 Mars launch window will be open, a period when the two planets are optimally positioned for the shortest, most fuel-efficient journey between them every 26 months.
In 2024, SpaceX CEO Elon Musk outlined a plan to send five Starships loaded with Optimus robots to scout resources and prepare infrastructure for crewed missions scheduled for later windows. By May 2025, Musk estimated a 50% chance of meeting this goal. Later in the year, he admitted it was looking increasingly unlikely, but there was still a chance. Notably, the SpaceX website still states that the next launch window is in 2026, with no clear indication whether this goal will be met.
Another American aerospace company, Vast, is targeting a 2026 launch for the first-ever commercial space station. They will turn to SpaceX to launch the Haven-1 space station in May with a Falcon 9 rocket, followed by a 14-day crewed mission in June, arriving via a SpaceX Crew Dragon. Haven-1 will host a 10-slot microgravity research and manufacturing platform, along with amenities for a crew of four, available to paying customers
Blue Origin’s New Glenn rocket carrying NASA’s twin ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) spacecraft launched in November 2025 from Cape Canaveral Space Force Station in Florida. Credit: Blue Origin
NASA Launches in 2026
Musk isn’t the only one taking advantage of the 2026 Mars window. In November, NASA launched the ESCAPADE mission into Earth orbit. Once the launch window opens, ESCAPADE, using Earth’s gravity, will slingshot to the red planet, where its two identical satellites will study how space weather affects the strange Martian magnetosphere.
To establish long-term habitability, the mission will explore how space weather, the planet’s thin atmosphere, and its magnetic crust interact. Scientists hope this new data will conclusively reveal how Mars lost its thick atmosphere. Data from the project will be essential to long-term safe habitation on the Red Planet, as it will enable mission planners to mitigate the effects of dangerous space weather in an environment that depends on artificial life support systems.
Several other NASA missions will make progress this year. The Discovery Program’s Psyche spacecraft will use a Mars gravity assist this summer to catapult it on its journey to the metallic asteroid 16 Psyche. The Europa Clipper Mission will use another gravity assist from Earth in December to fling it on its way to its final destination. In 2030, once it arrives at Europa, one of Jupiter’s moons, it will assess whether the moon is habitable.
Over the summer, NASA will launch a group of small cubesats about the size of toasters as part of its SunRISE (Sun Radio Interferometer Space Experiment) mission. Focused on space weather, the mission will monitor solar radio bursts and map the Sun’s magnetic field. As NASA extends human missions to the Moon and beyond to Mars, a better understanding of how the Sun’s charged particles can affect spacecraft will be essential to mission safety.
China’s previous lunar mission, Chang’e-6, returned samples from the far side of the Moon.
Credit: CNSA
Chinese Space Exploration in 2026
America is not the only country with grand space ambitions for 2026. China’s Chang’e 7 is anticipated to launch toward the end of the year. Named for the Chinese moon goddess, the Chang’e series has focused on investigating the lunar surface, which will continue with Chang’e 7’s exploration of the lunar south pole.
This area is particularly interesting for its cold traps: the shadowy craters that never receive enough direct sunlight to become illuminated. Their perpetual darkness leaves them with stores of frozen water and other minerals that could make them an essential supply for future permanent bases. The mission includes an orbiter, a relay satellite, a lander, a rover, and a mini-flying probe. While NASA has already sent missions such as LRCROSS to the area, future missions, including Artemis III, will revisit it.
To investigate another rocky body in space, the Chinese Tianwen-2 sample-return mission will rendezvous with the asteroid 469219 Kamo’oalewa in July for exploration and sample collection.
China’s Space Telescope
In addition to another lunar mission, China will add a new companion to its Tiangong space station, which launched in three sections between 2021 and 2022. Tiangong is China’s first long-term space station and has been used to host numerous experiments in low Earth orbit. The new addition is a space telescope named Xuntian, expected to capture 40% of the sky during its mission, with a field of view approaching 350 times that of the Hubble Space Telescope.
Initially, the telescope was to be part of the Tiangong itself, but concerns about light pollution, vibration, and the space station obstructing the view led China to decide to launch Xuntian as a free-standing object in the same orbit as the space station. The mission is planned to last 10 years. It will utilize five onboard instruments: a survey camera, a terahertz receiver, a multichannel imager, an integral-field spectrograph, and a cool-planet imaging coronagraph.
These images will allow researchers to measure the positions, shapes, and brightnesses of nearly one billion galaxies, providing new context for their growth and evolution. To capture them, Xuntian features a two-meter-wide aperture, which enables a field of view 350 times that of NASA’s Hubble Space Telescope.
JAXA’s Hayabusa-2 will continue its mission to investigate asteroids in 2026.
Credit: ESO/M. Kornmesser. Asteroid: T. Santana-Ros et al. Hayabusa2 model: SuperTKG (CC-BY-SA).
International Missions in 2026
The European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA) also have major plans for the year. Working together, the ESA-JAXA BepiColombo mission will enter Mercury orbit in November 2026, after which it will split into the Mercury Planetary Orbiter and the Mercury Magnetic Orbiter.
As the closest planet to the Sun, the mission will provide new insights into how hot planets near their stars evolve, with particular attention to their magnetic fields and magnetospheres. Additionally, mission measurements of Mercury’s motion will provide essential new data to evaluate Einstein’s general theory of relativity within the post-Newtonian formalism.
On its own, JAXA has two notable events planned. In July, Japan’s Haybusa-2 will conduct a flyby of the asteroid 98943 Torifune as part of its extended mission. More importantly, the Martian Moons eXploration (MMX) will launch in 2026 to perform a sample-return mission on the Martian moon Phobos and a flyby of the Martian moon Deimos. The return sample should reach Earth for study sometime in 2031.
Planetary defense will receive some significant attention in 2026 with the ESA HERA mission’s arrival at the asteroid Didymos in November. HERA will follow up on the 2022 NASA DART mission. DART was a practical planetary defense test that used a kinetic impactor to alter the course of an asteroid. With its two cubists, HERA will rendezvous with the binary asteroid Didymos to observe the aftermath of DART’s impact up close.
2026 will not just be a year of beginnings but also of endings. The ESA’s Solar Orbiter mission is scheduled to conclude in 2026, with a possible 2030 extension under consideration.
With a plethora of launches, gravity slingshots, tests, landings, flybys, and sample return missions slated for the upcoming year, don’t expect the space news to slow down in 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
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