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.
11-09-2025
Scientists reveal what ancient Martians might have looked like - as NASA announces strongest evidence yet for life on the Red Planet
Scientists reveal what ancient Martians might have looked like - as NASA announces strongest evidence yet for life on the Red Planet
Yesterday, NASAmade the startling announcement that its scientists have uncovered the 'clearest evidence' yet for the existence of life on Mars.
Last year, NASA's Perseverance rover discovered that a dry riverbed just north of the Martian equator is dotted with rusty circular markings known as 'leopard spots'.
Now, scientists have revealed what these alien organisms might have looked like.
Any life that evolved on Mars would have had to contend with harsh radiation, weak gravity, and temperatures that can swing between 20°C (70°F) in the day and -153°C (-225°F) at night.
However, the scientists behind this groundbreaking research say that it is still possible for some forms of life to evolve.
In the unlikely case that more complex life did evolve somewhere on the Red Planet, it would need to develop special adaptations to survive this impossibly harsh climate.
NASA has revealed the 'clearest evidence' yet for the existence of life on Mars, as it claims that 'leopard spots' on Martian rocks could have been created by ancient microbes
Scientists say that Mars' Jezero Crater was once filled with water that would have been 'clement' for microbial life to develop. Pictured: AI-generated impression
What did NASA find on Mars?
While investigating a region known as the 'Bright Angel', NASA's Perseverance rover spotted a group of unusual markings that resemble leopard spots.
Scientists call these spots 'reaction fronts', and they are points of contact where chemical and physical reactions have occurred in the past.
Critically, Perseverance's on-board lab found that these spots contained two iron-rich minerals: Vivianite, which is found in decaying organic matter, and greigite, which is produced by microbes on Earth.
Dr Keyron Hickman-Lewis, an Earth scientist from Birkbeck, University of London and co-author of the NASA report, told Daily Mail: 'The kinds of organic–mineral associations observed at Bright Angel that are reported in this paper are known to be generated by microbial life on Earth, and so it is a very promising observation to see something so similar on Mars.
'Certainly, I think that this is the most compelling potential evidence of life on Mars found to date.'
The scientists can't yet rule out that these spots could be caused by non-biological processes, and Dr Hickman-Lewis says that this is not a 'smoking gun'.
However, after spending a year reviewing the evidence and looking for alternative explanations, the researchers are now confident enough to say that this could be a 'biosignature', an elusive sign which proves the existence of life.
These signs of life were found by the Perseverance rover in a region called 'Bright Angel'. Researchers say that chemicals found in the leopard spots are produced by biological processes on Earth
Although Mars is now a barren desert, billions of years ago, it would have been covered with rivers and lakes that could have supported life
Dr Hickman-Lewis adds: 'The Mars 2020 team does not use the term "potential biosignature" lightly.'
What would this life look like?
The potential signs of life were found in a region called Jezero Crater, an impact basin just north of the equator.
Although it is now a barren wasteland, billions of years ago, the Jezero Crater was filled with water that could have been home to life.
If life did exist in these waters, the most plausible explanation is that it was some sort of simple microorganism.
Dr Hickman-Lewis says: 'The environment in which these potential biosignatures were found seems to be a low-temperature water-rich setting and therefore very clement for microbial life.'
In their paper, published in Nature, the researchers suggest that microbes could have fed on the naturally occurring carbon, sulphur, and phosphorus in the rocks.
These microbes would have then 'excreted' the minerals which we now see as leopard spots.
NASA Administrator Sean Duffy (center) revealed that a sample collected by Perseverance is the 'clearest sign of life' on Mars ever found in 30 years
The Jezero Crater, where the potential signs of life were found, was once a river delta. Observations from orbiting spacecraft show patterns of sediment that are similar to those made by rivers on Earth. Pictured: AI-generated impression
As microbes fed on the carbon, sulphur, and phosphorus in the rocks, they might have released iron-rich chemicals which permanently stained the rocks to leave 'leopard spots'. Pictured: AI-generated impression
The conditions on the surface would have been incredibly harsh, but the researchers say that life still could have eked out a simple existence.
Dr Sanjeev Gupta, an Earth scientist from Imperial College London and member of the research team, told Daily Mail: 'There was liquid water present at the surface at the time billions of years ago, so it was a habitable environment.
'This would have been simple microbial life. We can say much more than that.'
Since we can only see the possible traces left behind by these microorganisms, it's difficult to know what they might have looked like or how they behaved.
However, it is possible to make some very general predictions based on parallels from Earth.
Professor Michael Garrett, an astronomer from the University of Manchester and Director of Jodrell Bank Centre for Astrophysics who was not involved in the study, told Daily Mail: 'Think of hardy bacteria, similar to terrestrial extremophiles that thrive in very salty, cold, or low-oxygen conditions here on Earth.
'Good analogues are the microbial mats in very salty lakes or microbes that live kilometres underground in Earth’s crust or in the high desert in Chile.
'These examples show us that life can be tough, minimalistic, and persistent even in places where surface conditions are brutal.'
Scientists say that the best parallels for what life might have looked like are the microbial mats that form in extremely salty lakes on Earth. Pictured: AI-generated impression
It is unlikely that more complex life could have evolved since Mars' climate changed rapidly about a billion years after the first microbes could have appeared. This means complex organisms like animals probably didn't have time to develop. Pictured: AI-generated impression
Could more complex life have evolved?
If these leopard spots really are biosignatures, then the researchers say it's unlikely that they only existed in one place.
Perseverance is currently studying very ancient rocks outside of the Jezero Crater to look for signs of more widespread life.
However, it is extremely unlikely that more complex life evolved anywhere on the Red Planet.
However, after about one billion years, Mars' climate began to change rapidly as solar winds stripped away its atmosphere - leaving the planet very cold and dry.
Professor Garrett says: 'Those harsh conditions on Mars after 1 billion years would put strong limits on body size and complexity of any lifeform.
If complex life had emerged, it would have needed to develop adaptations like thick skin or live underground to avoid the intense radiation of the Martian surface. Pictured: AI-generated impression
On Earth, some of the first animals to evolve were simple filter feeders. Filter feeders also survive in extreme environments such as hydrothermal vents, so complex Martian life might have followed a similar evolutionary trajectory. Pictured: AI-generated impression
In the unlikely case that more complex life did evolve, Mars' harsh conditions would also put strong constraints on what it might look like.
'It would need to be adapted to survive the intense UV radiation from the Sun, extreme cold, and limited liquid water - we don’t really see complicated animal life in such environments,' says Professor Garret.
He adds: 'If they were present, they would need protection from the UV radiation from the sun – maybe a thick skin, for example, or perhaps mostly living under the Martian soil.'
That means complex life might resemble creatures on Earth that live in exceptionally harsh environments, such as desert-dwelling lizards or the simple filter-feeders that survive near hydrothermal vents.
At first thought to hold the pesticide DDT, some mysterious barrels dumped in the deep sea near Los Angeles actually contain caustic alkaline waste that stops most life from living nearby.
The toxic barrels, which came to public attention in 2020, appear to have "halos" around them — and researchers have finally figured out why.
(Image credit: Schmidt Ocean Institute.)
Thousands of barrels of industrial waste litter the ocean floor off Los Angeles and have been there for decades — but scientists still don't fully understand what chemicals this junkyard is leaking into the environment.
Now, research has revealed that some of the chemicals leaking from the barrel graveyard have been identified as strongly alkaline, the chemical opposite of acidic — and they are still concentrated enough to stop most life living nearby.
But to this day, the total number of barrels on the seafloor — and what most of them contain — remains unknown.
Now,Johanna Gutleben, a microbiologist at the Scripps Institution, and her colleagues have revealed the results of sediment samples taken near five barrels using a remotely operated vehicle in 2021. They found that levels of DDT contamination didn't increase closer to the barrels, so they say the drums didn't contain that chemical.
Three of the barrels they checked had white halos around them and all the samples from near these barrels had an extremely high pH (around 12) and very few microbes living there, so the team say the barrels contained caustic alkaline waste, which can damage organic matter and leach out high concentrations of potentially toxic metals.
The team's study was published Tuesday (Sept. 9) in the journalPNAS Nexus.
"Up to this point we have mostly been looking for DDT. Nobody was thinking about alkaline waste before this and we may have to start looking for other things as well," Gutleben said in astatement.
The sampling didn't identify which specific chemicals were in the barrels, but notably, DDT manufacturing produces alkaline waste, as does oil refining.
"One of the main waste streams from DDT production was acid and they didn't put that into barrels," said Gutleben. "It makes you wonder: What was worse than DDT acid waste to deserve being put into barrels?"
As the researchers found very limited levels of microbial DNA near the barrels, they say the alkali waste likely transformed parts of the seafloor into extreme environments where most life can't survive. They did find traces of some specialized bacteria, though — species from families adapted to alkaline environments, like deep-sea hydrothermal vents and alkaline hot springs.
The team also discovered how the weird haloes form. When the alkaline waste leaks from the barrels, it reacts with magnesium in the water and creates a mineral form of magnesium hydroxide, called brucite, forming a concrete-like crust. The brucite then slowly dissolves, keeping the pH in the sediments high while leading to reactions in surrounding seawater. This results in the formation of calcium carbonate, which settles as white dust around the barrels.
Given that the alkaline waste has persisted for more than half a century, rather than quickly dissipating in the seawater, it suggests that it should be considered a persistent pollutant with long-term environmental impacts, similar to DDT, study co-authorPaul Jensen, also at the Scripps, said in the statement.
"It's shocking that 50-plus years later you're still seeing these effects," he said.
The researchers suggest using the white halos to identify which barrels contain alkaline waste so the overall extent of contamination can be assessed. Jensen said roughly one-third of the barrels that have been seen so far have halos, but it's unclear if this ratio will hold as more barrels are uncovered.
NASA's Perseverance rover has photographed a peculiar rock formation that looks eerily like a turtle poking its head out from its protective shell.
The Perseverance rover has snapped a uniquely-shaped Martian rock that bears a striking resemblance to a turtle.
(Image credit: NASA/JPL-Caltech)
NASA's Perseverance rover has snapped an intriguing photo of a "turtle" appearing to poke its head out of its shell on the surface of Mars. The reptile-like structure is the latest in a long list of Martian rocks that look similar to living creatures or other Earth objects.
Perseverance captured the new image on Aug. 31, on what was its 1,610th Sol, or Martian day, on the Red Planet. The wandering, car-sized robot snapped the shot somewhere in the Jezero Crater — a 28-mile-wide (45 kilometers) depression where the rover touched down in 2021, which is thought to have previously contained a large lake.
The photo was taken using the rover's Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC) and Wide Angle Topographic Sensor for Operations and eNgineering (WATSON) instruments, which combined to scan the rock in visible and ultraviolet wavelengths of light, according to Live Science's sister site Space.com. Both instruments are mounted on the rover's robotic-arm turret.
The featured rock has garnered comparisons to a turtle, thanks to a head with two eyes that look as if it has protruded from a protective "shell" with a pair of "front legs" on either side (see image below).
It is currently unclear which geological processes have shaped the rock into this unusual shape.
The turtle-like rock features a protective "shell," a "head" with two "eyes" and a pair of equally sized "front legs."(Image credit: NASA/JPL-Caltech, annotations by Harry Baker)
The Mars rovers have collectively captured tens of thousands of photos of Mars' surface, most of which feature multiple different rocks or other geological features that have been sculpted into unique shapes by ancient water sources or millenia of strong winds. Every once in a while, one of these rocks bears a resemblance to something we can see on Earth, such as blueberries, human-like fingerprints, a mysterious doorway and even a "Star Trek" symbol, to name a few.
These associations are often made due to pareidolia — a psychological phenomenon where the human mind perceives a familiar pattern, such as a face or image, in random objects or structures, such as clouds.
Perseverance has been particularly good at spotting these weird rocks during its five-year mission. Its other recent finds include a bizarre medieval "helmet" that it wheeled past in August and an out-of-place "skull" that is snapped in April.
NASA scientists have found more intriguing details on speckled Martian rocks spotted by the Perseverance rover. But bringing samples back to Earth will be key.
A selfie taken by NASA's Perseverance Rover while on Mars.
(Image credit: NASA)
Strange nodules of unusual minerals found on speckled rocks on Mars have offered more tantalizing clues that ancient life may have once thrived on the now-dead planet, NASA says.
NASA's Perseverance rover found one such arrow-shaped rock, nicknamed Cheyava Falls, in 2024 along the northern bank of Neretva Vallis, the dried-up remnants of an ancient river that once rushed into Mars' Jezero crater.
An initial analysis of the rock, which appeared in a lake bed formation known as Bright Angel, revealed it was crammed with organic compounds, had evidence that water once flowed through it, and contained flecks of leopard-like spots from chemical reactions that ancient microbes could have used for energy.
These features may result from non-biological processes occurring over millions of years. But now, in a new study published Sept. 10 in the journal Nature, NASA scientists have announced intriguing details about additional rock samples found at two nearby sites — and they say these clues bolster the case for past life on Mars.
"After a year of review, they have come back and they said, listen, we can't find another explanation," Acting NASA Administrator Sean Duffy, said during a news briefing following the announcement. "So this very well could be the clearest sign of life that we've ever found on Mars, which is incredibly exciting."
Since arriving on Mars in 2021, Perseverance has been trundling across the 30-mile-wide (50 kilometers) Jezero crater, collecting dozens of rock samples for eventual return to Earth. Upon finding the leopard-spotted rock, scans by the rover's Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) instrument showed that the specimen contained carbon-based molecules, alongside bands of reddish hematite that featured spots of iron and phosphate.
"When the rover entered Bright Angel and started measuring the compositions of the local rocks, the team was immediately struck by how different they were from what we had seen before," study co-author Michael Tice, a geobiologist and astrobiologist at Texas A&M University, said in a statement. "They showed evidence of chemical cycling that organisms on Earth can take advantage of to produce energy. And when we looked even closer, we saw things that are easy to explain with early Martian life but very difficult to explain with only geological processes."
An image of Cheyava Fallas, showing white markings that could be traces of ancient microbial activity. (Image credit: NASA/JPL-Caltech/MSSS)
The additional discoveries announced by NASA today relate to clay-rich rock samples found at two sites, named Sapphire Canyon and Masonic Temple, containing vivianite, an iron-phosphate mineral, and greigite, a mineral containing iron sulfide.
These minerals may have formed from reactions between the mud and organic matter, according to the scientists. The minerals' distribution across the rocks appears to support this hypothesis.
"It's not just the minerals, it's how they are arranged in these structures that suggests that they formed through the redox cycling [in which bacteria are key players on Earth] of iron and sulfur," Tice said. "On Earth, things like these sometimes form in sediments where microbes are eating organic matter and 'breathing' rust and sulfate. Their presence on Mars raises the question: could similar processes have occurred there?"
Nonetheless, a definitive ruling over the biological or non-biological processes that created the patterns can only be made in labs on Earth, and whether Perseverence's precious cargo will be fetched for that analysis remains a contentious political question.
The European Space Agency (ESA) and NASA originally proposed the use of NASA’s Sample Retrieval Lander — a spacecraft carrying a small rocket — to collect the rover's samples by 2033 as a part of their Mars Sample Return mission. The rocket would then launch back into orbit with the samples.
When pressed by reporters during a Q&A session following the announcement, Duffy was unable to confirm if or when the sample-return mission would happen, but he remained optimistic.
"The president loves space — he asked me about it," Duffy said. "I give him updates, how it's going, what we're doing, and he doesn't brush me off."
"If there was an issue with resources, I would go to him and I'm sure he would support us," he added.
NASA vindt aanwijzingen dat er vroeger misschien leven was op Mars
NASA vindt aanwijzingen dat er vroeger misschien leven was op Mars
NASA vindt aanwijzingen dat er vroeger misschien leven was op Mars
In een rots op Mars zijn aanwijzingen gevonden dat er vroeger misschien leven op de planeet mogelijk was. De steen heeft "potentiële tekenen voor oud leven van microbes". De Amerikaanse ruimtevaartorganisatie NASA zegt "niet eerder zo dicht bij het ontdekken van leven op Mars te zijn geweest". De organisatie houdt nog wel een slag om de arm en zegt dat er ook andere verklaringen mogelijk zijn.
De onbemande robotjeep Perseverance ontdekte in juli vorig jaar een rots met luipaardvlekken. Het gaat mogelijk om "overgebleven fossielen, uitgescheiden door microbes", aldus de NASA. De ruimtevaartorganisatie zegt de vondst te hebben voorgelegd aan wetenschappers. Zij zouden hebben geconcludeerd dat oud leven de meest logische verklaring is, blijkt uit een artikel in het wetenschappelijk tijdschrift Nature.
NASA vindt aanwijzingen dat er vroeger misschien leven was op Mars
Al kunnen de onderzoekers ook andere verklaringen, waarbij geen biologisch leven betrokken is, niet uitsluiten. Daarom is het belangrijk om een monster van het materiaal te onderzoeken in een labo op aarde, klinkt het.
De Perseverance landde in 2021 op Mars. De verkenner met zes wielen heeft twintig camera's en een boor aan boord om de planeet te onderzoeken. Het werkgebied van de rover is de krater Jezero. Miljarden jaren geleden, toen op Mars mogelijk water stroomde, mondde daar mogelijk een rivier uit in een meer.
De robotjeep onderzoekt stalen, maar transporteert die niet. Daarvoor zijn andere robotten nodig. Vraag is wel of de NASA daar nog geld voor zal vinden, nadat de Amerikaanse president Donald Trump vraagtekens plaatste bij de plannen om materiaal vanop Mars naar de aarde te brengen.
Astronomers and students working together through a unique educational initiative have obtained a striking new image of the growing tail of interstellar Comet 3I/ATLAS. The observations reveal a prominent tail and glowing coma from this rare celestial visitor, while also providing new scientific measurements of its colors and composition.Image Credit: NOIRLab. http://creativecommons.org/licenses/by/4.0/
Interstellar visitors like Comet 3I/ATLAS grant astronomers a rare opportunity to study something from another solar system. It was first discovered on July 1st when it was entering the inner Solar System and was about 4.5 au from the Sun. It's an active comet with an icy nucleus, meaning it's warming up as it approaches the Sun and releasing gas and dust that form a coma and tail.
It's the third confirmed interstellar object (ISO) after Oumuamua and Comet 2L/Borisov. These objects provoke extreme curiosity among astronomers, driven by the fact that they won't be visible again. As ISOs, their trajectory will take them out of the Solar System completely, never to be seen again.
These new images of Comet 3I/ATLAS are from the Gemini South Telescope in Chile. It's an 8.1 meter optical/infrared telescope that has a twin, the Gemini North Telescope, in Hawaii. The telescopes are operated by the National Science Foundation's NOIRLab.
In a twist, these images aren't part of a dedicated strictly scientific observing program. Instead, they're from a public outreach initiative involving NOIRLab and Shadow the Scientists. Shadow the Scientists is an effort to connect astronomers working with powerful telescopes with interested members of the public.
The images are from 27 August 2025, when astronomers used the Gemini South's Gemini Multi-Object Spectrograph (GMOS) to obtain deep images of Comet 3I/ATLAS, its coma, and its tail. The images show that the coma and tail are growing, when compared to earlier images of the comet.
During the outreach initiative, members of the public and students from Hawaii and Chile joined a Zoom call with astronomers at Gemini South. They were able to ask questions, interact with the scientists, and follow observations in real time. People from around the world, including from Europe, New Zealand, and South America, also joined in.
During the session, time-critical communication among the science team and observatory/telescope staff are given the highest priority. This is necessary for obvious reasons, and it gave public participants an opportunity to be immersed in real-time astronomical observations.
Gemini South's Gemini Multi-Object Spectrograph (GMOS) captured the comet's spectrum, which yields information about the comet's chemical makeup. This lets astronomers understand the changes the comet goes through as it traverses the inner Solar System and the Sun's energy drives changes in the comet.
Comet 3I/ATLAS is only the third confirmed ISO to visit our Solar System, though there must have been many more of them throughout the Solar System's history. The comet provides a rare opportunity to study something from a distant star up close.
Image Credit: International Gemini Observatory/NOIRLab/NSF/AURA/Shadow the Scientist Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector
(University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)
"The primary objectives of the observations were to look at the colors of the comet, which provide clues to the composition and sizes of the dust particles in the coma, and to take spectra for a direct measure of the chemistry,” said Karen Meech, astronomer at the University of Hawai‘i Institute for Astronomy, and leader of the scientific program. “We were excited to see the growth of the tail, suggesting a change in the particles from the previous Gemini images, and we got our first glimpse of the chemistry from the spectrum.”
The new observation and spectrum indicate broad similarity with comets from our own Solar System. This suggests that planetary system formation and evolution is similar in other Solar Systems, or at least in Comet 3I/ATLAS's home system.
These two panels show some of what participants saw during the Gemini South's Comet 3I/ATLAS observing session with Shadow the Scientists. The panel on the left shows a screen displaying different aspects of the telescope's status, and also the weather. The panel on the right is the main software, called the observing tool, that astronomers use in a lot of their interactions with the Gemini South Telescope.
Image Credits: NSF/NOIRLab/Gemini South
“As 3I/ATLAS speeds back into the depths of interstellar space, this image is both a scientific milestone and a source of wonder,” said Meech. “It reminds us that our Solar System is just one part of a vast and dynamic galaxy — and that even the most fleeting visitors can leave a lasting impact.”
“These observations provide both a breathtaking view and critical scientific data,” said Bryce Brolin, a research scientist who was also present. “Every interstellar comet is a messenger from another star system, and by studying their light and color, we can begin to understand the diversity of worlds beyond our own.”
Brolin will lead a follow-up Shadow the Scientists session when Comet 3L/ATLAS reappears from behind the Sun. That session will be held from the Gemini North Telescope on Mauna Kea, Hawaii.
Below is a video of the entire Shadow the Scientists observing session.
Deep exposures on 7 September 2025 show 3I/ATLAS wrapped in a green coma.
(Credit: M. Jäger and Gerald Rhemann)
I have been staring at 3I/ATLAS for weeks, not through an eyepiece, but through the stack of reports and images that keep arriving. At first the object looked reddish. Now its glow reads as green. The gas around it is heavy on carbon dioxide and thin on water, which is not how a regular comet behaves near the Sun. In some images the light seems to extend toward the Sun rather than away from it. That is the kind of detail that makes you sit up, because it refuses to fit neatly into the usual picture.
One anomaly can be a measurement quirk. A handful of them begins to sound like a pattern. With 3I/ATLAS we have color change, unusual chemistry, odd scattering of light, and a path that hugs the plane of the planets more closely than chance would suggest. When you place those facts side by side, you get a portrait that does not match the familiar family of icy bodies in the solar system where we are from.
This is where the culture of science matters. Many researchers are careful, honest, and conservative in how they talk about data. That caution serves the field well. It also means that oddities sometimes get smoothed out by language before they are faced head on. PRofessor Avi Loeb takes a different tack. He keeps pointing at the data and asking simple questions in public. He does not chase applause and he does not hide behind comfortable phrasing. I respect that. Science is not a popularity contest. It is a process for finding out what is true in the world, and that process only works if people are willing to ask the questions that feel awkward.
Let me be direct about one thing. I do not think 3I/ATLAS is an alien spacecraft. I would love it to be, sure. Natural explanations should be worked through first, with patience and rigor. The chemistry could reflect a crust rich in carbon dioxide ice. The color shift could track changes in sunlight and temperature that wake up different molecules at different distances. The odd light pattern could be geometry and timing. I mean, remember the face on Mars? There is work to do before anyone should claim anything extraordinary.
Still, I will take the other path because it is worth thinking clearly about it. If 3I/ATLAS were artificial, it would almost certainly not carry living organisms. Biology does not like deep space. It breaks down under radiation and time. A machine can wait and repair itself. An autonomous probe guided by artificial intelligence makes more engineering sense for an interstellar mission than a cabin full of breath and bone. That is not a romantic picture, but it is a practical one.
Deep exposures on 7 September 2025 show 3I/ATLAS wrapped in a green coma. (Credit: M. Jäger and Gerald Rhemann)
I keep returning to ʻOumuamua. (I also loved Loeb’s book on ʻOumuamua) It was small, fast, and behaviorally odd. It showed no clear signs of venting, yet its motion suggested a small push that gravity alone did not account for. It looked nothing like the textbook comets we teach. It passed. Many argued. It kept its secrets. If you allow a speculative frame for one paragraph, you can imagine ʻOumuamua as a scout, a light vehicle meant to sense, sample, and move on. You can then imagine 3I/ATLAS as a larger platform with a different set of capabilities. If that picture were true, it would point to a civilization far beyond us in age and capacity, one that builds in classes of craft and sends them across star systems as calmly as we send weather satellites across the Atlantic.
I am not claiming that is the case. I am laying out a clean line of reasoning so that readers understand what is at stake when we talk about anomalies. The right response is not to fall in love with the extraordinary answer. The right response is to gather the kind of data that lets the ordinary answer win on evidence, not on habit.
Here is what the data say in plain terms. When 3I/ATLAS was far from the Sun, the light it threw around itself increased very quickly as it moved inward. Once it crossed a certain distance, that increase slowed. That pattern suggests that the material around it changed character. At first the light likely bounced off dust lifted from a dark surface layer. Closer in, fresh, small ice grains likely took over and brightened the glow in a different way. Independent observations show a gas plume dominated by carbon dioxide, with smaller amounts of carbon monoxide and only traces of water. That is unusual when set next to the comets that spend their lives in our system. But thenagain, space is weird, and the universe has so many secrets we are just starting to explore.
You do not need to be a specialist to grasp the next step. If an object from another star looks different from most of our comets, we should not force it into the old mold. We should describe it as it is and ask what that tells us about where it came from, how it formed, and how it is changing now. That is the heart of science. Describe the thing. Test the description. Change your mind when the facts warrant it.
This is also where public conversation can go wrong. People hear “anomaly” and think “mystery solved by a wild claim.” That habit hurts everyone. The better habit is calm curiosity. Loeb often argues for that posture, even when it upsets colleagues. He asks for open data, independent measurements, and patient analysis. He reminds us that history is full of mistakes that felt safe at the time. The Sun did not circle Earth. Diseases did not spring from bad air. Continents did not stand still. Our job is not to protect an old story. Our job is to find the right one.
So what should we do with 3I/ATLAS right now? Keep observing. Compare instruments. Cross-check photometry and spectra. Model the light scattering with more than one set of assumptions. Publish the methods in detail. Invite rival teams to replicate the results. Treat the object as a laboratory for learning about interstellar debris, not as a prop in a culture war between skeptics and believers. If the mundane explanation is correct, it will earn its place by explaining the color, the chemistry, and the geometry without hand-waving. If it fails, we will know exactly where it fails, and that will be valuable.
I will close where I began. The sky is not tidy. It is real and indifferent. It holds dust that glows green and rocks that tumble and gas that tricks the eye. We do not honor it by draping it in stories that flatter us. We honor it by looking closely, asking better questions, and letting evidence lead, even when it drags us somewhere we did not plan to go. If 3I/ATLAS turns out to be a strange but natural traveler, that will be worth knowing. If it is something else, we will need the same tools and the same temperament to face that result. Either way, curiosity and discipline carry us forward.
Chinese scientists have developed a comprehensive mission to study asteroids. One of its targets could be the asteroid Apophis.
Asteroid Apophis in an artist’s impression. Source: ESA Science Office
The asteroid Apophis has a diameter of 375 meters. On April 13, 2029, it will make a close flyby of Earth, passing at a distance of 32,000 km from its surface (i.e., inside the orbits of geostationary satellites). At that moment, the asteroid will be visible to the naked eye across most of Europe and Africa, as well as in some parts of Asia. The encounter with Earth is expected to affect the asteroid and cause landslides and shifts on it.
According to scientists’ estimates, such large objects approach Earth on average once every 5,000 to 10,000 years. It is not surprising that Apophis’ visit has attracted increased attention, and a number of countries and space agencies are considering options for sending missions to it. Currently, ESA and JAXA are working on the Ramses spacecraft, while NASA is focusing on the OSIRIS-APEX mission, which previously studied the asteroid Bennu.
Chinese scientists do not intend to miss such a rare opportunity and are also working on their own mission. It has been named CROWN/Apophis and is part of a larger project called CROWN, which aims to launch six different probes to study near-Earth objects in heliocentric orbits similar to those of Venus.
The main task of CROWN/Apophis will be to measure the fundamental properties of this potentially dangerous asteroid and the consequences of its approach to Earth. The goal of the project is to observe the processes that will occur on the surface of Apophis and how it interacts with Earth’s magnetosphere.
CROWN/Apophis will consist of two spacecraft. The larger one, weighing 44 kg, will use a combined chemical and ion propulsion system and will be equipped with cameras, a microwave rangefinder/Doppler system, and low-frequency radar. The 8 kg CubeSat will be equipped with some of the same systems as the main spacecraft.
The devices are proposed to be launched as accompanying cargo as part of a mission that has not yet been determined. After that, they will fly to the L1 Lagrange point of the Sun-Earth system, where they will wait for Apophis to arrive. They will make a close flyby of the asteroid shortly after it visits the vicinity of our planet. This will happen on April 13, 2029.
NASA specialists conducted a series of key tests on components of the Dragonfly drone. These tests were successful, allowing them to move on to the next stage of mission development.
Dragonfly drone in an artist’s impression. Source: NASA/Johns Hopkins APL/Steve Gribben
Development of the Dragonfly mission began in 2019. As part of this mission, NASA plans to send a rotary-wing aircraft with a total mass of about 450 kg to Titan. It will be equipped with four twin propellers, allowing it to travel at speeds of around 36 km/h and rise to an altitude of up to 8 km. The drone will use a radioisotope generator as its power source.
Dragonfly’s primary mission is to search for complex organic molecules and assess the overall suitability of this celestial body for past and present life. The drone will be able to collect samples from the Titanian surface and conduct chemical analysis on them. Dragonfly will also study the moon’s terrain, atmosphere, and hydrocarbon reservoirs. The spacecraft is designed to operate on Titan for at least three years.
To date, the mission has already gone far beyond computer concepts. In April, its design underwent critical review. This allowed engineers to begin manufacturing and testing the drone’s components. One of the most important tests was conducted in a wind tunnel. For a month, engineers from NASA and the Applied Physics Laboratory (APL) immersed a sensor-equipped drone model in a stream of heavy gas simulating Titan’s dense atmosphere. The collected data helped to understand the kind of loads that the device, its rotary system, and blades would be subjected to. This will enable the preparation of the software necessary for drone flights.
Dragonfly drone blades in a wind tunnel. Source: NASA
APL engineers also completed structural and thermal testing of the foam insulation for the Dragonfly lander, confirming that it will retain its shape and protect the internal components from the environment, which reaches temperatures of approximately -185 °C on Titan. The landing module body will be covered with a 7.6 cm thick layer of solimide-based foam.
In addition, APL engineers have completed the development of onboard radio stations that will serve as receivers and transmitters during Dragonfly’s flight to Titan and its work on the surface. Employees at the Goddard Space Flight Center have completed work on the DraMS mass spectrometer in search of biosignatures. And Lockheed Martin specialists conducted the first series of tests on the aerodynamic fairing that would protect Dragonfly during its re-entry into the moon’s atmosphere.
The DraMS mass spectrometer, which Dragonfly will use to search for signs of life on Titan. Source: NASA
The success of all these tests made it possible to move on to the next stage of mission development. In January, engineers will begin assembling the device components and conducting comprehensive testing. The launch of Dragonfly is scheduled for July 2028, with landing on Titan planned for 2034.
Scientists investigated the source of radiation Sh 2-283-1a SMM1. It is a stream of matter emitted by a newborn star located at the very edge of the Galaxy. Its chemical composition shows that it contains far fewer heavy elements than similar objects observed to date, but the general patterns of physical processes remain the same.
Newborn star Sh 2-283-1a SMM1. Source: Ikeda et al. (Niigata University), background: R. Hurt / NASA / JPL-Caltech / ESO
Jets from a newborn star
Research conducted using the Atacama Large Millimeter/submillimeter Array (ALMA) may help us better understand the processes of star formation. This giant radio telescope observed the radiation source Sh2-283-1a SMM1. It is located 26,000 light-years away from us and 51,000 light-years from the center of the Galaxy.
In fact, it consists of jets of matter emitted by a newborn star. This phenomenon is not new and has been observed more than once. A large amount of matter falls onto the newly formed star, and part of it is ejected back into space due to the large angular momentum.
What makes Sh 2-283-1a SMM1 unusual is the star’s location. Not only is it far away from us, but it is also at the very edge of the Galaxy. Scientists have not yet observed such a phenomenon so far from the center of the Galaxy, and this should be an interesting region, because even compared to the vicinity of the Sun, it is poor in metals, i.e., elements heavier than hydrogen and helium.
Research results
Observations made with ALMA have provided insight into the chemical composition of the jets. It has been confirmed that it is much poorer in heavy elements than similar structures that have been observed previously. In particular, the ratio of silicon oxide to carbon oxide was significantly lower than in jets emanating from young stars near the Sun.
At the same time, this object is a “hot core” — a hot structure rich in chemical elements. They are quite common in star-forming regions closer to the center of the galaxy, but this is only the second time such an object has been observed at its edge.
The luminosity of the core is 6,700 times greater than that of the Sun, which suggests that the star, when fully formed, will be of average or large mass. The jets are not emitted continuously, but at intervals of 900–1400 years.
ALMA also detected increased activity in four other young stars on the outskirts of the Galaxy. This indicates that the processes of star formation here are quite intense and, in general, follow the same patterns as in the center of the Galaxy.
On October 19 2017, Robert Weryk, a Canadian astronomer working at the University of Hawaii, discovered the first-ever known interstellar object in our solar system. If that sounds a bit strange, what with all the relatively regular sightings of asteroids and comets popping up in the news, it’s important to understand the significance of the phrase ‘in our solar system’.
Unlike previous interstellar objects, ‘Oumuamua which means ‘a message from afar arriving first’ in Hawaiian) had entered the zone controlled by the sun’s gravity. What’s potentially more alarming is that ‘Oumuamua had come closer to Earth than any other known interstellar object, and we still don't know much about it.
So what do we know? 'Oumuamua, a shining object that measured approximately 400-800 metres in length, entered our Solar System travelling 57,000 miles per hour (that's 16 miles per second). It sped straight down towards the Sun but curled underneath due to the star's gravitational pull. This sent the object off on a new trajectory, which was once again altered slightly as it passed Mercury. At its closest point, 'Oumuamua was 15 million miles away from the Earth, which may seem like a lot, but can be classed as a near-miss in the grand scheme of things. The whole process lasted forty days.
But no-one knows what 'Oumuamua really was. An asteroid comprised of metal and rocks, a comet made up of rocks, dust and ice, or a spinning, intensely bright, cigar-shaped (or 'prolate ellipsoid' to give it the technical description) alien probe?
The popular conclusion that ‘Oumuamua was most probably a cosmic iceberg, a mass of frozen hydrogen, is based upon observed findings that ‘Oumuamua couldn’t have contained any water, carbon monoxide or carbon dioxide, as found in asteroids and comets, because they would have been visible phenomena.
Perhaps more contentiously, astronomers also discovered that the object was accelerating as it left the solar system, yet it had no antitail as one might expect to find on a comet. The theory was that tails on comets and asteroids (though less common) act like rocket engines, but a frozen lump of hydrogen could have rocket-engine like propulsion, while the tail remained invisible from the gaze of the telescope.
Based on this, the general conclusion is that ‘Oumuamua was a highly luminescent, half-billion old chunk of planet from outside the Solar System., However, the theory is in a perpetual case of dispute. There are also a growing number of high-profile voices, such as Harvard astrophysicist Professor Avi Loeb, that claim ‘Oumuamua might have been an alien spacecraft from the far reaches of space.
His theory that ‘Oumuamua was a fully operational probe sent intentionally to the Earth’s vicinity by an alien civilization, was based on exactly the same observations that deemed it a cosmic iceberg.
In the series finale of Craig Charles: UFO Conspiracies, Craig Charles and astrophysicist Sarah Cruddas investigate ‘Oumuamua in an attempt to get one step closer to the answer. They speak to Professor Loeb who warns that the object could be a ‘message in a bottle telling us we’re not alone’. Sarah and Craig also speak with members of the SETI Institute who offer their hypotheses about the event and ponder the existence of intelligent life outside of Earth.
Is Oumuamua an alien probe sent from another galaxy, as Professor Loeb believes or a cosmic glacier? We’ll probably never know for sure, but let's leave you with this: the Drake Formula. Formulated in 1961 by Dr Frank Drake, this provides the formula for a probabilistic argument to estimate the number of communicative extraterrestrial civilizations in our galaxy. The answer is 12,600, and that’s just in the Milky Way. The Hubble Telescope has revealed an estimated 100 billion galaxies in the universe and the James Webb Telescope will probably double that…
Humanity is advancing into space rather slowly – astronauts landed on the moon 55 years ago, and since then, we have not been able to boast of any achievements of a similar scale. But our journey through the Solar System will continue, and its next destination will obviously be Mars.
While some scientists are trying to figure out how colonists can protect themselves and adapt to Martian conditions, others are proposing to change the planet itself. Is it possible to make the Martian environment more suitable for future colonists, and is it worth doing? Let’s try to figure it out.
The greenhouse effect: enemy of Earth, friend of Mars?
The technology for creating conditions on the surface of a celestial body that are as close as possible to those on Earth is called “terraforming”. The term was first used by American science fiction writer Jack Williamson in his 1942 novel Collision Course.
In 1971, astronomer and science popularizer Carl Sagan became the first scientist to propose terraforming Mars, which currently has a thin atmosphere consisting almost entirely of carbon dioxide with small amounts of nitrogen, oxygen, and other gases. He suggested that by releasing gases from various sources on the Red Planet, it would be possible to artificially thicken its gas envelope and increase the chances of liquid water appearing on the surface due to the greenhouse effect.
NASA took an interest in the concept. Carbon dioxide and water vapor are the only greenhouse gases present in the atmosphere and ice deposits on Mars and beneath the planet’s surface. Carbon dioxide molecules are excellent at trapping the Sun’s infrared rays. So if enough of this substance is released by melting the ice caps and filling the atmosphere with it, it will create a greenhouse effect that will raise the average temperature and thus “warm” the cold planet. This is literally the same effect that is currently causing climate change on our planet.
For its part, increased pressure will contribute to the appearance of water bodies on the surface of Mars. And although it will not be possible to breathe fresh Martian air for a long time, at least it will be possible to do without airtight compression suits there.
However, in 2018, after a series of studies, NASA scientists abandoned the project. It turned out that there was not enough carbon dioxide on the Red Planet. Based on data from the MAVEN, Mars Express, Mars Reconnaissance Orbiter, and Mars Odyssey missions, experts calculated that even if all Martian carbon dioxide were completely evaporated, the atmospheric pressure would only rise to 15 mbar (for comparison: the average pressure at the Earth’s surface is 987 mbar). The project was closed with the conclusion: “Terraforming Mars is impossible with current technology. Any such plans are only possible in the very distant future”.
Regional terraforming
Of course, they decided not to stop there. Researchers from Harvard University, the Jet Propulsion Laboratory (JPL NASA), and the University of Edinburgh came up with the idea that it is not necessary to change the climate of the entire planet – it is enough to influence only certain regions where the colonists will live. The scientists proposed using silica aerogel, one of the best insulating materials that mimics the greenhouse effect in the Earth’s atmosphere. These aerogels are currently used in several engineering projects, including the Mars Exploration Rovers mission probes. Through modeling and experiments, scientists have shown that a two- to three-centimeter-thick aerogel shield without any internal heat source can transmit enough visible light for photosynthesis, block dangerous ultraviolet radiation, and raise and maintain the surface temperature above the melting point of water ice. This material can be used to build dwellings or even autonomous biospheres on Mars.
Artistic illustration of the stages of terraforming Mars.
Source: Daein Ballard
Controlled heating of limited areas would not require large amounts of energy or maintenance of modular settlements to keep the area warm for a long time. The results of studies simulating the Martian surface showed that a thin layer of aerogel generally increased surface temperatures in the mid-latitudes of Mars to those found on Earth. However, further research is needed to build such “greenhouses”. In addition, this miracle material does not solve the problem of the harsh climate of the entire planet, and it is also quite fragile and requires large-scale production.
Nuclear bombing, or Musk’s method
Even the eccentric billionaire Elon Musk has become fascinated with the seductive idea of terraforming Mars, in his own style, through nuclear bombing. Musk is the most famous contemporary proponent of colonizing the fourth planet from the Sun. He has repeatedly shared his plans to populate it by 2050 with more than a million colonists who will live under the glass domes of Martian cities. However, he also has a long-term goal – to make Mars more like Earth.
Source: TechInsider
Musk also proposes to use the greenhouse effect. First, it is necessary to heat the frozen carbon dioxide reserves at the Martian poles, which can be accomplished by detonating nuclear bombs above them. In response to comments about the insufficient amount of carbon dioxide in frozen deposits, the billionaire emphasized that Martian soil may also contain a “huge amount” of this substance. Its release will help warm the planet, melt frozen glaciers, and further thicken the atmosphere, causing warming.
Therefore, scientists point out the shortcomings of this method of transforming Mars into a blooming oasis. Even if there were enough frozen CO2, such a strategy would require the use of an almost unattainable amount of nuclear weapons. According to some estimates, 3,500 half-megaton nuclear warheads would need to be detonated every day for seven weeks straight. And even at that rate, the subsequent terraforming process would take several millennia.
Giant orbital mirrors
Another popular method of terraforming Mars is to build giant mirrors in orbit around the planet, which will reflect and direct more sunlight and heat its surface. Among the most prominent proponents of this method are Christopher McCain, a planetary scientist and researcher at NASA, and Robert Zubrin, an American aerospace engineer, writer, and founder of the Mars Society.
Source: nextbigfuture.com
The idea is to build orbital mirrors with a radius of about 100 km from thin aluminized thermoplastic film (a similar material is used to make solar sails). Such mirrors would weigh about 200,000 tons! If they were manufactured in space using resources from the Moon or asteroids, the production of the necessary aluminum would require a huge amount of energy, not to mention time.
According to Zubrin, we do not have enough data to claim that there are insufficient carbon dioxide deposits on Mars. Until now, experts have relied on data from the MAVEN satellite and several Mars rovers, which have only penetrated a few centimeters into the Martian soil. There may be more deposits of volatile substances deeper underground. Further research involves drilling several hundred meters deep in various locations on the planet.
Asteroid bombardments
Another way to raise the temperature is to direct small asteroids or comets toward the surface of Mars. For decades, humanity has been developing programs to track potentially hazardous objects and creating systems to protect Earth from collisions. Therefore, one or more of these methods could be used to arrange for such objects to collide with Mars. The energy from the crash would then serve as a source of heat.
Source: Science Photo Library
Asteroids can be selected based on their “usefulness” – for example, based on their ammonia content, which, when released into the Martian atmosphere, will further enhance the greenhouse effect, or based on the presence of water, which will turn into water vapor.
However, NASA believes that thousands of such asteroids will be needed, and there is currently no ready-made technology for their targeted transportation to Mars.
The hardest part is still ahead
There are other methods of bringing conditions on Mars closer to those on Earth by importing ammonia, hydrogen, or bacteria capable of living and serving as a nutrient substrate for plants in Martian regolith. However, scientists believe that instead of fighting the consequences, we should look at the root of the problem. More precisely, at the core. After all, any attempts to create an atmosphere on the Red Planet will be futile without a magnetosphere to hold it in place. A terraformed Mars will need a reinforced magnetosphere, similar to the one that protects Earth from the flow of charged particles from the Sun.
It is believed that about 4 billion years ago, Mars lost its magnetic field due to the cessation of core rotation. Without a magnetosphere to serve as a shield, solar winds began to bombard and destroy the atmosphere. Leading NASA scientist James Green, who has worked at the agency for 40 years, proposes creating a huge magnetic shield to prevent our star from destroying the future Martian atmosphere. As a result, the planet will be able to retain heat near the surface, pressure will increase, and the climate will improve and become suitable for life. According to the scientist, this method will entail the least amount of interference and destruction, and then Mars will begin to terraform on its own. However, he does not provide estimates of the cost of the project, the necessary technological capabilities, or the time required for such long-term processes.
Ethical issues and the benefits of concepts and research for the Earth
Although humanity is still quite far from realizing its plans to terraform Mars, we must nevertheless consider the ethical and appropriateness of such projects. Similar to protected wilderness areas on Earth, Mars has extreme, historically important, and aesthetically valuable regions. Any interference with the planet’s natural development will lead to irreversible changes. Mars will forever lose its unique historical and research value for future generations.
Source: DETLEV VAN RAVENSWAAY/SCIENCE PHOTO LIBRARY
Another problem with terraforming Mars is the high cost of such missions. And if, say, humanity had such resources, wouldn’t it be more expedient to use them for the benefit of Earth? Scientists around the world are already sounding the alarm about climate change, the destruction of fertile land, the depletion of fresh water and mineral resources, and the lack of preparedness for possible epidemics.
We should not forget the history of colonization, which has always been accompanied by tragedy. Even today, destructive wars continue over territory, resources, religious beliefs, and so on. So, have we reached the point of moral development where we can become wise guests in the Universe, rather than destructive invaders?
We will have to find answers to these and other questions in the future. However, similar research, such as improving soil quality or developing protection against asteroids, can also be used on our planet. Like many other technologies that are part of our everyday life, thanks to space developments. And in the event of an inevitable catastrophe, Mars would become “plan B” for the salvation of the human race.
Author: Anastasiia Bernatska, journalist
This article was published in issue No. 1 (190) of Universe Space Tech magazine in 2024. You can purchase this issue in print or electronic format from our store.
In a world limited to three dimensions, imagining a fourth is incredibly difficult, especially for an unprepared reader. But one genius scientist found a way to show people the hidden world using an ordinary apple.
Legendary science popularizer Carl Sagan explained what the fourth dimension looked like 45 years ago. Illustration: Copilot
As it happens, the human mind is attuned to perceiving only three dimensions: height, width, and depth. Representing the fourth dimension seems like an impossible task, because our brains are limited by the physical world around us. But what if there is a dimension that we simply cannot see? Legendary science popularizer Carl Sagan comes to the rescue.
Known for his research into space, Sagan possessed a unique gift — the ability to explain complex scientific theories through simple stories and vivid analogies. He could turn the most complex concept into a fascinating adventure for the mind.
In search of the fourth dimension
Time is often referred to as the fourth dimension. This is logical: to determine the position of an object in the Universe, you need three coordinates in space and one in time. But there is another, more theoretical concept — a space where all four dimensions are spatial. It is precisely this concept that is so difficult to understand.
Sagan begins his explanation with a simple analogy. He invites us to imagine a two-dimensional world — a Flat World whose inhabitants have no concept of “up” or “down.” When a three-dimensional object, such as an apple, passes through this flat world, its inhabitants see only a strange phenomenon.
They do not see the apple as a whole. They only observe the point of contact that appears when the apple crosses their world. When an object moves, this point may change shape, split into several parts, or disappear. For a resident of the Flat World, this is an incomprehensible phenomenon, a set of changing forms that cannot be explained in his/her world.
From apple to hypercube
The same logic, Sagan notes, applies to us when we try to imagine the fourth dimension. We are like those inhabitants of the Flat World. Our minds cannot comprehend anything beyond our three dimensions. But we can see its “imprint” in our world.
To demonstrate this, the scientist uses a tesseract — a four-dimensional hypercube. We cannot see a real tesseract, but we can observe its three-dimensional projection, just as the inhabitants of Flat world saw only a two-dimensional trace of an apple. This projection looks like a complex cube, as if nested within itself. It is only a shadow, an attempt by our brain to reproduce something much more complex.
Truth beyond reach
Sagan’s work is not just an interesting scientific trick. Studying measurements that lie beyond our immediate experience is key to understanding the fundamental laws of the Universe. Many phenomena in physics, such as black holes or the curvature of space-time, cannot be adequately described in only three dimensions.
Carl Sagan not only dispelled the myth that complex concepts are inaccessible. He showed that the best way to understand something is through clear explanations, vivid metaphors, and engaging stories. His lesson on the fourth dimension remains a brilliant example of how to talk about the most complex things in a simple way.
Researchers have made a discovery involving how the Earth’s core initially froze and crystallized millions of years ago, suggesting that a previously unexpected amount ofcarbon, as revealed in a new paper published in Nature Communications.
Accounting for 3.8% of the Earth’s interior, such a percentage is far higher than researchers believed was likely to exist in the planet’score, which is primarily believed to be rich in iron. Presently, it continues to grow as more of its molten surroundings cool to join the core’s mass in a process that scientists have debated for decades.
Understanding The Earth’s Inner Core
Forming a solid inner core requires more than just cooling—it depends on the precise chemistry of the molten material. The process can be compared to hail formation: water droplets in clouds must reach temperatures well below water’s normal freezing point before crystallizing into ice. Similarly, molten iron in Earth’s core must become “supercooled,” dropping roughly 800–1000 °C below its normal freezing point to solidify.
However, geological evidence suggests Earth’s core has never cooled this far. Simulations show such extreme cooling would have caused runaway core growth and likely collapsed the planet’s magnetic field—an event that never appears to have happened. Data instead indicate the core cooled by less than 250 °C below its melting point.
Reconciling A Warm Core
To explain how the core could crystallize without extreme supercooling, researchers from the University of Oxford, the University of Leeds, and University College London turned to computer simulations. Lacking direct access to the planet’s center, they modeled how elements like carbon, oxygen, sulfur, and silicon—known to exist in the mantle—would influence crystallization if present in the core.
“Each of these elements exist in the overlying mantle and could therefore have been dissolved into the core during Earth’s history,”said co-author Associate Professor Andrew Walkerof the University of Oxford. “As a result, these could explain why we have a solid inner core with relatively little supercooling at this depth. The presence of one or more of these elements could also rationalise why the core is less dense than pure iron, a key observation from seismology.”
A diagram of the Earth’s inner and molten cores, displaying how convection generates the magnetic field.
Credit: Dr Alfred Wilson
The First Steps Of Freezing
The team simulated atomic-scale interactions, tracking how roughly 100,000 atoms behaved under high pressure and supercooled conditions similar to those in the inner core. They focused on “nucleation,” the moment when small crystal clusters first form, marking the beginning of freezing.
The results were striking. Elements like silicon and sulfur, once thought to be major components of the core, actually slowed freezing and required greater supercooling. Carbon, by contrast, accelerated freezing, bringing models closer to observed conditions. A 2.4% carbon mixture still fell short, but at 3.8% carbon, the simulations aligned perfectly with expectations—producing an inner core temperature requiring just 266 °C of supercooling. No other combination reproduced the core’s observed nucleation and size.
Continuing to Investigate the Core
“It is exciting to see how atomic-scale processes control the fundamental structure and dynamics of our planet,” said lead author Dr Alfred Wilson of the University of Leeds. “By studying how Earth’s inner core formed, we are not just learning about our planet’s past. We’re getting a rare glimpse into the chemistry of a region we can never hope to reach directly and learning about how it could change in the future.”
The study also lends new data to the ongoing debate over the age of Earth’s core. Some scientists argue it began crystallizing more than two billion years ago, while others suggest it solidified less than half a billion years ago. The new evidence, pointing to carbon’s crucial role, may help resolve this long-standing question.
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.
With the recent discovery of the mysterious space object 3I/ATLAS, the third-known interstellar object directly observed by astronomers, debate over its origins—and even the possibility that it might be of technological origin—has captured the public imagination.
Now, an international team of astronomers suggests that the rare appearances of interstellar objects passing through our solar system could provide scientists with an opportunity to search for signs of extraterrestrial technology.
While the available evidence strongly supports the view that 3I/ATLAS is a comet, albeit one bearing some rather unusual qualities, the team behind the recent study nonetheless suggests that there are good reasons to consider interstellar objects passing through our solar system as potential candidates in the search for alien technosignatures.
3I/ATLAS: A Comet, or Alien Technology?
Following the discovery of 3I/ATLAS on July 1, 2025, speculations about the object’s nature and origin have entertained a range of possibilities based on some of its unusual characteristics. Among these is the idea proposed by Harvard astronomer Avi Loeb and colleagues in a preprint paper earlier this year, which examined whether the object’s trajectory and non-gravitational motion through the solar system might suggest that it bears the qualities astronomers could expect from an intelligently controlled spacecraft.
Notably, Loeb and his co-authors stated in the paper that their examination of the potentially technological origins of 3I/ATLAS had been largely pedagogical, although they maintained that such views should not be dismissed outright, even if the likeliest interpretation by far remains that the object is an interstellar comet.
Now, in a new study by an international team of scientists that reviews decades of speculation and outlines concrete strategies for examining interstellar comets and asteroids, the paper’s authors similarly argue that 3I/ATLAS and its predecessors, 1I/‘Oumuamua and 2I/Borisov, bore all the qualities of comets, but that the search for genuine alien technosignatures associated with interstellar objects that make our way to our solar system is not unwarranted.
Cosmic Hitchhikers
“Since humanity has sent many of our own spacecraft on interstellar trajectories, we know that it is possible to send probes to other stars,” the study’s authors write. Equally, they argue that a range of different types of technosignatures could essentially “hitchhike” across interstellar distances and arrive with an interstellar object.
“Technology could either be active throughout an object’s interstellar journey, or wake from a dormant state upon arrival in the Solar System,” the authors write. “Defunct technology may also be found, such as spacecraft whose power supplies have long since become inactive.”
Other possibilities include technology that might be buried beneath the surface of an interstellar object. According to this premise, as the surface material begins to sublimate as the object begins to approach our Sun—the same processes producing the Sun-facing coma or “halo” of cometary material currently surrounding 3I/ATLAS—any alien technologies may be revealed through such natural processes. This would allow for the deployment of a once-buried probe, but only if its interstellar carrier manages to reach the vicinity of a star like our Sun.
Other possibilities include interstellar asteroids that are modified to produce “world ships, objects which may include natural structures and other technological features that would allow any “interstellar nomads” on board to utilize generational habitats that could be carried along with any prospective comets capable of spanning interstellar distances.
“Given the extreme distance between star systems, sending physical objects between stars may be advantageous for an extraterrestrial civilization, compared with direct communication,” the authors note.
Four Avenues for Technosignature Searches
In their paper, the team examines four primary categories of potential searches for technosignatures, which include
1) anomalous trajectories (the presence of unexpected accelerations or maneuvers that can’t be explained by natural outgassing or radiation pressure),
2) spectral or coloration anomalies (including unusual reflectance, coatings, or waste heat detectable in the infrared),
3) objects with unnatural shapes such as cylinders or thin “light-sails,” and
4) any detectable transmissions in the form of narrowband radio or optical signals, including lasers, that could indicate intentional or incidental communication.
Interestingly, such observations were made of ‘Oumuamua and Borisov, although no detectable signatures were discernible. As it continues its journey through our solar system, 3I/ATLAS has already been targeted by the Allen Telescope Array and observed by multiple observatories, including NASA’s Webb and Hubble telescopes. Based on all the available data, everything astronomers have observed thus far suggests that these objects have natural origins.
Nonetheless, the authors of the new paper emphasize that there remains a chance that even a few mundane observations—such as monitoring a comet’s rotation, its color, or how it accelerates—could still provide some critical context that may be helpful in identifying potential outliers that might arrive in the future.
Why Technosignature Searches Matter
Currently, with the Rubin Observatory’s Legacy Survey of Space and Time expected to discover anywhere from six to more than 50 interstellar objects in the next decade, the team behind the new study argues that technosignature investigations should not be overlooked and must be incorporated into routine follow-ups. Coordinated campaigns that scour radio, optical, infrared, and radar frequencies could maximize the chances of spotting anything unusual, in the unlikely event that it existed.
For now, although speculation about alien probes captures public imagination, the real value of taking such studies seriously lies in building a systematic framework for distinguishing natural phenomena from any potential anomalies we might find.
“Any potential detection of technosignatures from an [interstellar space object] will require the most stringent and detailed confirmation possible,” the paper’s authors write, underscoring the need for rigorous protocols and independent verification if—or perhaps when—we spot something truly anomalous.
The team’s paper, “Technosignature Searches of Interstellar Objects,” by James R.A. Davenport, et al, appeared on the preprint arXiv.org server on August 22, 2025.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached atmicah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
CAPE CANAVERAL, Fla. (AP) — Telescope observations reveal a growing tail on the comet that’s visiting from another star.
Released Thursday, the pictures taken by the Gemini South telescope in Chile late last month are the most detailed yet of the recently discovered comet. They show a wide coma of dust and gas around the ice ball as it speeds toward the sun, and also a tail that’s more extended than it was in previous shots.
These new images confirm that the comet is becoming more active as it plows harmlessly through our solar system, according to the National Science Foundation's NoirLab, which operates the telescope. It’s only the third known interstellar object to venture our way.
As of Thursday, the comet known as 3I-Atlas was 238 million miles (384 million kilometers) from Earth and growing ever nearer, according to NASA. It will make its closest approach to the sun at the end of October and then pass closest to Earth in December from 167 million miles (269 million kilometers) away — farther from Earth than the sun.
This story was first published on Sep. 4, 2025. It was updated on Sep. 5, 2025 to correct the name of the agency that operates the telescope. It is the National Science Foundation, not the National Space Foundation.
The Associated Press Health and Science Department receives support from the Howard Hughes Medical Institute’s Department of Science Education and the Robert Wood Johnson Foundation. The AP is solely responsible for all content.
Planeten vinden die lijken op de aarde en waar mogelijk ook leven is: het blijft een ontzettende uitdaging. Wetenschappers hebben echter een methode ontwikkeld waarmee we mogelijk aliens kunnen opsporen.
Tot nu toe hebben wetenschappers nog geen bewijs gevonden voor buitenaards leven. Alle levensvormen die we kennen – van eencellig tot meercellig – komen voor op onze eigen planeet waar vloeibaar water zorgt voor de noodzakelijke chemische reacties. Het opsporen van aarde-achtige exoplaneten is een enorme uitdaging. Een team astrofysici denkt nu een haalbare oplossing te hebben.
Exoplaneten vinden met huidige technologie is moeilijk Exoplaneten met vloeibaar water zenden het meeste licht uit bij golflengtes rond de 10 micrometer, ongeveer de dikte van een dunne mensenhaar en twintig keer de typische golflengte van zichtbaar licht. Om een planeet als de aarde te onderscheiden van een ster op een afstand van 30 lichtjaar, is een telescoop met een spiegeldiameter van minstens 20 meter nodig. Bovendien moet die telescoop in de ruimte worden geplaatst, omdat de aardse atmosfeer het beeld te veel vervaagt. De James Webb Space Telescope (JWST), met een diameter van 6,5 meter, was al een huzarenstukje om te lanceren. Een telescoop van 20 meter is simpelweg niet uitvoerbaar.
Alternatieve opties Daarom zoeken wetenschappers naar alternatieven. Ideeën variëren van zwermen kleinere telescopen die samen één groot geheel vormen, tot het gebruik van kortere golflengtes waarmee kleinere spiegels volstaan. Maar die opties brengen weer andere problemen met zich mee: de precisie die nodig is om meerdere telescopen in de ruimte te laten samenwerken is onhaalbaar en in zichtbaar licht is een zonachtige ster meer dan tien miljard keer helderder dan een planeet als de aarde. Het blokkeren van dat sterlicht ligt nog ver buiten ons technische bereik.
Wel haalbaar Een team onder leiding van Heidi Newberg van het Rensselaer Polytechnic Institute stelt nu een alternatief voor dat dichterbij de huidige mogelijkheden ligt. In Frontiers in Astronomy and Space Sciences presenteren de onderzoekers een ontwerp voor een telescoop met ongeveer hetzelfde formaat als de JWST, maar met een andere vorm: een rechthoekige spiegel van één bij twintig meter, in plaats van een ronde van 6,5 meter.
Die langwerpige spiegel zou het mogelijk maken een ster van een exoplaneet te scheiden. Door de spiegel te draaien kan de lange as telkens worden uitgelijnd met zowel ster als planeet. Volgens berekeningen van het team kan een dergelijke telescoop in minder dan drie jaar tijd de helft van alle aarde-achtige planeten binnen 30 lichtjaar opsporen.
30 veelbelovende planeten vinden Hoewel het ontwerp nog verdere ontwikkeling en optimalisatie vereist, zijn er geen onoverkomelijke technische obstakels. In veel opzichten lijkt de telescoop op de JWST, maar dan met een andere spiegelvorm. Als we veronderstellen dat er sowieso één aarde-achtige planeet draait om de gemiddelde zonachtige ster, dan zouden we ongeveer 30 veelbelovende planeten vinden. Nadat deze ontdekt zijn kunnen we aan de hand van vervolgonderzoek identificeren of er leven aanwezig kan zijn. De onderzoekers dromen er in ieder geval al van om vervolgens een sonde te sturen naar de meest veelbelovende planeet voor verder onderzoek.
Astronomers have obtained a color image of a rare visitor from deep space — comet 3I/ATLAS, which is hurtling through our Solar System at breakneck speed. This scientific photograph reveals the secrets of the formation of celestial bodies in distant star systems.
New images of 3I/ATLAS were obtained by the Gemini South telescope in Chile as part of the Shadow the Scientists program.
In August 2025, the GMOS spectrograph on the Gemini South telescope in Chile took a unique image of comet 3I/ATLAS. This object attracts the attention of scientists around the world because it is an interstellar traveler that has come to us from beyond our planetary system. Its incredible speed — over 200,000 km/h — undeniably confirms its origin in interstellar space.
Scientific value of the photograph
The magnificent color photograph clearly shows the coma — a cloud of gas and dust that surrounds the comet’s nucleus and expands as it approaches the Sun. Astronomers were particularly struck by the comet’s expressive tail, which had grown significantly longer compared to previous observations. Its length in the sky reaches 1/120 of a degree, which is comparable to the width of your pinky finger when you look at it with your arm outstretched.
In addition to its aesthetic appeal, this photograph has enormous scientific value. The main purpose of the observations was to study the colors of the comet and obtain its spectra. By analyzing the wavelengths of light emitted by the comet, scientists can accurately determine the chemical composition of dust particles in its coma and directly measure its chemical composition.
Discovery that brings worlds together
Color photograph 3I/ATLAS without distortion. Photo: noirlab.edu
Despite its exotic origin, spectral analysis of comet 3I/ATLAS revealed something surprising: its composition is very similar to comets that originated in our own Solar System. This discovery leads to a revolutionary assumption: comets in different parts of our galaxy are formed from similar materials and according to the same laws, regardless of their star system.
Karen Meech, an astronomer at the University of Hawaii who led the observations, notes that scientists have for the first time been able to see the chemical composition of such a comet from its spectrum and track changes in its particles.
Space traveler
Comets like 3I/ATLAS are extremely rare. It is only the third confirmed interstellar comet in history, joining the famous comets discovered in 2017 and 2019.
Unlike ordinary comets, which often perish when they approach the Sun, this traveler has a hyperbolic orbit. This means that it has only visited us temporarily and will soon return to the abyss of interstellar space, taking with it new knowledge about the Universe.
"Marsquake" data collected by NASA's InSight lander have revealed dozens of mysterious blobs within the Red Planet's mantle. The structures may have been left by powerful impacts up to 4.5 billion years ago.
Researchers believe they have found several blobs within Mars that were leftover from giant impacts with "protoplanets" up to 4.5 billion years ago.
(Image credit: NASA/JPL-Caltech)
Giant impact structures, including the potential remains of ancient "protoplanets," may be lurking deep beneath the surface of Mars, new research hints. The mysterious lumps, which have been perfectly preserved within the Red Planet's immobile innards for billions of years, may date back to the beginning of the solar system.
In a new study, published Aug. 28 in the journal Science, researchers analyzed "Marsquake" data collected by NASA's InSight lander, which monitored tremors beneath the Martian surface from 2018 until 2022, when it met an untimely demise from dust blocking its solar panels. By looking at how these Marsquakes vibrated through the Red Planet's unmoving mantle, the team discovered several never-before-seen blobs that were much denser than the surrounding material.
The researchers have identified dozens of potential structures, measuring up to 2.5 miles (4 kilometers) across, at various depths within Mars' mantle, which is made of 960 miles (1,550 km) of solid rock that can reach temperatures as high as 2,700 degrees Fahrenheit (1,500 degrees Celsius).
"We've never seen the inside of a planet in such fine detail and clarity before," study lead author Constantinos Charalambous, a planetary scientist at Imperial College London, said in a NASA statement. "What we're seeing is a mantle studded with ancient fragments."
Based on the hidden objects' size and depth, the researchers think the structures were made when objects slammed into Mars up to 4.5 billion years ago, during the early days of the solar system. Some of the objects were likely protoplanets — giant rocks that were capable of growing into full-size planets if they had remained undisturbed, the researchers wrote.
The researchers first noticed the buried structures when they found that some of the Marsquake signals took longer to pass through parts of the mantle than others. By tracing back these signals, they identified regions with higher densities than the surrounding rock, suggesting that those sections did not originate there.
Researchers identified dozens of impact structures in Mars' mantle by analyzing how vibrations from Marsquakes moved through the planet's interior. (Image credit: NASA/JPL-Caltech)
Mars is a single-plate planet, meaning that its crust remains fully intact, unlike Earth's, which is divided into tectonic plates. As pieces of Earth's crust subduct through plate boundaries, they sink into the mantle, which causes the molten rock within our planet to rise and fall via convection. But on Mars, this does not happen, which means its mantle is fixed in place and does not fully melt.
The newly discovered blobs are further proof that Mars' interior is much less active than Earth's.
"Their survival to this day tells us Mars' mantle has evolved sluggishly over billions of years," Charalambous said. "On Earth, features like these may well have been largely erased."
NASA's InSight lander recorded more than 1,300 Marsquakes on the Red Planet between 2018 and 2022. (Image credit: NASA/JPL-Caltech)
Because Mars has no tectonic activity, Marsquakes are instead triggered by landslides, cracking rocks or meteoroid impacts, which frequently pepper the planet's surface. These tremors have also been used to detect other hidden objects beneath the Red Planet's surface, including a giant underground ocean discovered using InSight data last year.
In total, InSight captured data on 1,319 Marsquakes during its roughly four-year-long mission. However, scientists were still surprised that they could map the planet's insides in such great detail.
"We knew Mars was a time capsule bearing records of its early formation, but we didn't anticipate just how clearly we'd be able to see with InSight," study co-author Tom Pike, a space exploration engineer at Imperial College London, said in the statement.
Was ‘Oumuamua an Extraterrestrial Craft and Will It Return?
In the vast expanse of our galaxy, the discovery of interstellar objects passing through our solar system has long fascinated astronomers and the general public alike. Among these, ‘Oumuamua—an enigmatic object detected in October 2017—stands out as one of the most intriguing and debated celestial phenomena in recent history. Its peculiar characteristics have sparked widespread speculation about its nature, with some proposing it could be an extraterrestrial craft. This essay aims to analyze the evidence surrounding ‘Oumuamua, evaluate the plausibility of it being an alien spacecraft, and explore the likelihood of its return to our solar system.
Discovery and Initial Observations
‘Oumuamua was first observed by the Pan-STARRS 1 telescope in Hawaii on October 19, 2017. Its name, derived from Hawaiian, means “scout” or “messenger,” reflecting its status as the first known interstellar object detected passing through our solar system. Unlike typical comets or asteroids, ‘Oumuamua exhibited several unusual features that defied easy classification. Its trajectory was hyperbolic, indicating an origin outside our solar system, and its high velocity suggested it had come from interstellar space, traveling at an impressive speed of approximately 87.3 kilometers per second relative to the Sun.
The initial observations revealed that ‘Oumuamua had an elongated shape, estimated to be about 400 meters long and only 40 meters wide, giving it a striking aspect ratio of approximately 10:1. Its surface reflected sunlight unevenly, leading to a brightness variation as it rotated—indicative of an irregular shape. The object displayed a brightness variation of about 2.5 magnitudes over a rotation period of roughly 8 hours, implying a highly elongated or flattened structure. Moreover, telescopic observations showed that ‘Oumuamua lacked a visible coma or tail, which are typical features of comets when they approach the Sun and begin to outgas.
One of the most intriguing aspects of ‘Oumuamua was its non-gravitational acceleration. As it moved away from the Sun, its velocity increased slightly beyond what would be expected from gravitational influences alone. This subtle acceleration suggested that ‘Oumuamua was experiencing some form of outgassing, releasing material that provided a small push. However, unlike typical comets, no detectable gas or dust emissions were observed, leading to considerable debate among astronomers about the precise nature of this outgassing—or whether it was caused by some other process altogether.
Further observations using various telescopes, including the Hubble Space Telescope and ground-based observatories, confirmed these unusual features. Spectroscopic analysis revealed a featureless, reddish surface, similar to some primitive asteroids and comets. Its lack of detectable activity and peculiar shape made ‘Oumuamua an unprecedented object in our solar system—an interstellar visitor that challenged existing theories about small body formation and behavior in space. This initial discovery sparked a wave of scientific interest, leading to numerous hypotheses about its origin, composition, and the possibility of artificial or extraterrestrial nature, making ‘Oumuamua one of the most fascinating objects ever encountered in our cosmic neighborhood.
Theories on ‘Oumuamua’s Nature
The unusual features of ‘Oumuamua, the first known interstellar object passing through our Solar System, sparked widespread scientific debate and numerous hypotheses about its true nature. The initial consensus among astronomers was that ‘Oumuamua was a natural object, likely a fragment of a larger body that was ejected from its parent star system due to gravitational interactions, such as close encounters with massive planets or other celestial events. Many researchers believed it to be an elongated asteroid, perhaps a remnant of a collision or disruption event in another star system. Its highly elongated shape, with estimates suggesting it was at least five to ten times longer than it was wide, was unusual compared to typical asteroids within our Solar System.
One of the key features that puzzled scientists was the absence of a visible coma or tail. Comets generally develop a glowing envelope of gas and dust—called a coma—when their ices sublimates as they approach the Sun, creating a characteristic tail. ‘Oumuamua, however, showed no such features despite passing relatively close to the Sun at about 0.25 astronomical units. This lack of outgassing was initially interpreted as evidence that it might be a rocky or metallic object, similar to an asteroid, rather than a comet.
Yet, the most intriguing aspect of ‘Oumuamua was its observed non-gravitational acceleration—an unexplained push that slightly altered its trajectory without any corresponding visible outgassing. This phenomenon challenged the traditional understanding that such acceleration is caused solely by the sublimation of volatile ices. The absence of detectable gases or dust in the observational data led some scientists to question whether ‘Oumuamua was a typical comet or asteroid.
Several hypotheses emerged to explain this acceleration. One prominent idea was that ‘Oumuamua could be a comet with outgassing composed of materials that are difficult to detect, such as molecular hydrogen or other volatiles that produce minimal observable gases. Alternatively, some scientists suggested that the acceleration might be caused by radiation pressure—solar photons exerting a force on ‘Oumuamua. This hypothesis would imply that the object has an extremely low mass-to-area ratio, possibly indicating a thin, sheet-like structure or an artificial origin.
The radiation pressure hypothesis gained further attention because it could account for the observed acceleration without the need for detectable outgassing. If ‘Oumuamua were a thin, lightweight object—perhaps a spacecraft or a light sail—solar radiation could effectively push it, influencing its trajectory. Although this idea was met with skepticism and considered speculative, it opened up new discussions about the possibility, however remote, of extraterrestrial technology.
Additional theories proposed that ‘Oumuamua could be a fragment of an interstellar comet or asteroid that had undergone surface processing, such as space weathering, which might suppress outgassing signatures. Others suggested it could be a piece of alien technology, like a probe or a fragment of a larger artificial object, although such hypotheses remain highly controversial and lack concrete evidence.
In conclusion, the true nature of ‘Oumuamua remains an open question. Its unusual shape, lack of visible activity, and unexplained acceleration continue to inspire debate. While the majority of scientists favor a natural origin, the peculiar characteristics of this interstellar visitor have broadened our understanding of the diversity of objects that exist beyond our Solar System and have highlighted the need for further observations and research into such enigmatic objects.
The Alien Craft Hypothesis
A more provocative and controversial theory was proposed by Harvard astrophysicist Avi Loeb, along with his colleague Shmuel Bialy, in 2018. They suggested that ‘Oumuamua, the first known interstellar object passing through our solar system, could potentially be an artificially manufactured artifact—a piece of alien technology rather than a natural cosmic body. This hypothesis garnered significant attention both within the scientific community and the public, as it challenged conventional understanding of such objects.
Loeb and Bialy’s proposition was primarily based on the unusual physical characteristics observed in ‘Oumuamua, particularly its acceleration and shape. Unlike typical asteroids or comets, ‘Oumuamua exhibited a non-gravitational acceleration—that is, it moved faster than could be explained solely by the Sun’s gravitational pull. Interestingly, astronomers did not detect any signs of outgassing, such as cometary jets, which are usually responsible for such acceleration in natural objects. This lack of outgassing was perplexing because the observed acceleration appeared to be consistent with the effect of radiation pressure— the push exerted by sunlight on a small, lightweight object.
Based on these observations, Loeb and Bialy hypothesized that ‘Oumuamua could be a form of artificial structure—a light sail. A light sail is a type of spacecraft propulsion technology that harnesses radiation pressure from sunlight to propel itself through space. Such a design would imply that ‘Oumuamua was not a natural asteroid or comet, but an engineered object, possibly a probe or a piece of alien spacecraft technology. The object’s elongated shape and high velocity further supported this idea, as these features could be consistent with a deliberately crafted artificial object intended for interstellar travel or exploration.
Supporters of the alien craft hypothesis argued that the peculiar features of ‘Oumuamua—its unusual shape, its rapid acceleration without observable outgassing, and its high velocity—could be more straightforwardly explained if the object were an extraterrestrial probe or artifact. They suggested that an advanced civilization might have sent such a probe to explore the galaxy, and that ‘Oumuamua was simply a chance encounter with this technological relic.
While the hypothesis remains speculative and controversial within the scientific community, it has sparked a great deal of debate and further investigation into the nature of interstellar objects. Critics argue that natural explanations, such as a fragment of an extinct comet, could still account for ‘Oumuamua’s properties, citing the lack of direct evidence for alien technology. Nonetheless, the idea that ‘Oumuamua could be an alien spacecraft continues to inspire discussions about the possibility of detecting other extraterrestrial artifacts and the potential for intelligent life beyond Earth.
In summary, the alien craft hypothesis presents a provocative perspective that challenges traditional astrophysics. It emphasizes the importance of open-mindedness in scientific inquiry and encourages further research into the mysterious objects traveling through our solar system, which could hold clues to the existence of advanced extraterrestrial civilizations.
An illustration of bizarre interstellar visitor 'Oumuamua
(Image credit: VICTOR HABBICK VISIONS/SCIENCE PHOTO LIBRARY via Getty Images)
Criticisms and Counterarguments
The alien craft hypothesis has faced significant criticism within the scientific community, with many experts emphasizing the importance of natural explanations over speculative theories. A primary argument against the extraterrestrial origin hypothesis is that the observed properties of ‘Oumuamua can be adequately explained by well-understood natural phenomena. For instance, some astrophysicists propose that ‘Oumuamua is a fragment of a larger parent body, such as an asteroid or comet, that was tidally disrupted during a close passage to its host star. This process can produce elongated, irregular shapes similar to what is observed. Additionally, the object’s unusual acceleration as it moved away from the Sun can be attributed to outgassing—where volatile materials, like hydrogen or other sublimating substances, escape from the surface of the object. Importantly, such outgassing can occur without forming a visible coma or tail, especially if the materials are less volatile or the outgassing is highly anisotropic, which means the gases are released unevenly, providing a recoil effect that alters the trajectory.
This simulation depicts the interstellar object 'Oumuamua as a mass of fragments forced into an elongated shape by stellar tidal forces.
(Image credit: ZHANG Yun/background by ESO/M. Kornmesser)
Furthermore, the lack of direct evidence supporting artificiality remains a core challenge for proponents of the alien hypothesis. No definitive signals or artifacts have been detected that would indicate technological origins. The rarity of interstellar objects passing through our solar system also raises questions; such objects are expected to be extremely uncommon, making it statistically less likely that ‘Oumuamua is an alien probe or spacecraft. Critics argue that extraordinary claims require extraordinary evidence—a principle rooted in scientific rigor. Invoking extraterrestrial technology without concrete proof risks undermining the credibility of scientific inquiry and diverts attention from more plausible natural explanations.
Another important aspect of criticism involves cognitive biases, such as apophenia—the tendency to perceive meaningful patterns or connections where none actually exist. Given the limited data and the enigmatic nature of ‘Oumuamua, it is easy for observers to interpret ambiguous signals as evidence of alien technology. This psychological tendency can lead to overinterpretation of uncertain observations, especially in the face of a mysterious object that defies easy classification. Skeptics caution against jumping to conclusions based on circumstantial evidence, emphasizing the need for caution and rigorous analysis.
In conclusion, while the idea of an alien craft is intriguing and captures popular imagination, the scientific consensus favors natural explanations for ‘Oumuamua’s peculiar properties. Ongoing observations and future interstellar object detections will be crucial in providing more data to settle these debates. Until then, the hypothesis of extraterrestrial origin remains speculative and not sufficiently supported by empirical evidence.
Recent Developments and Ongoing Research
In 2021, the scientific community received a wealth of new data from the Hubble Space Telescope, along with observations from other ground-based and space-based observatories, such as the Pan-STARRS telescope in Hawaii and the European Southern Observatory's Very Large Telescope (VLT). These observations aimed to unravel the mysteries surrounding ‘Oumuamua, the first known interstellar object detected passing through our Solar System. The data collected provided increasingly detailed information about its physical characteristics, trajectory, and possible origins. Despite these advances, conclusive evidence about its true nature remains elusive, fueling ongoing debates among astronomers and astrophysicists.
The collected data reinforced the idea that ‘Oumuamua was an unusual natural object with peculiar features that set it apart from typical comets or asteroids. For instance, its elongated shape, estimated to be about 400 meters long and 40 meters wide, was extraordinary. Additionally, ‘Oumuamua exhibited non-gravitational acceleration—an unexpected change in its trajectory that could not be explained solely by gravitational forces from the Sun and planets. Some scientists theorized that this might be due to outgassing, similar to comets, but no visible tail or coma was observed, leading others to propose more exotic explanations, including the possibility of artificial origin or manufactured components.
Looking ahead, the upcoming Vera C. Rubin Observatory, located in Chile, is set to revolutionize the detection of interstellar objects. Scheduled to begin full operations in the near future, this observatory will survey the entire sky with unprecedented sensitivity and frequency. Its wide-field telescope is expected to discover dozens of interstellar visitors over the coming years, vastly increasing the potential for in-depth study of these enigmatic objects. Such data will be instrumental in providing a broader statistical understanding of their composition, trajectories, and physical properties, helping scientists distinguish between natural and potentially artificial origins.
In addition to observational efforts, plans are underway for more direct exploration of interstellar objects. The European Space Agency’s proposed Comet Interceptor mission aims to visit a pristine, unaltered interstellar object in the near future. Unlike previous missions that targeted known comets or asteroids, the Comet Interceptor will be launched to rendezvous with an object that has recently entered our Solar System, offering a unique opportunity to study its composition and physical properties up close. This mission could yield invaluable insights into the building blocks of planetary systems and the processes involved in their formation.
Furthermore, the recent emergence of the interstellar object 3I/ATLAS has garnered significant attention. Discovered in late 2017, 3I/ATLAS was notable for its hyperbolic trajectory, confirming its interstellar origin. Its passage through the Solar System provided another valuable dataset, especially regarding its brightness variations and spectral properties. Studying objects like 3I/ATLAS helps scientists understand the diversity of interstellar visitors and refine models of their origin and evolution.
The combined data from these observations and upcoming missions will deepen our understanding of interstellar objects. They may also shed light on the possibility that some objects could possess artificial characteristics, potentially originating from extraterrestrial technological civilizations. While such claims remain speculative, the scientific community continues to explore all possibilities with rigorous analysis and open-minded inquiry.
In conclusion, recent advancements—from detailed observations of ‘Oumuamua to the anticipated discoveries by the Vera C. Rubin Observatory and dedicated missions like the Comet Interceptor—are paving the way for a new era of interstellar exploration. These efforts will not only improve our knowledge of these mysterious visitors but also enhance our understanding of the broader cosmos and the potential for extraterrestrial life or technology. The discovery of the interloper 3I/ATLAS serves as a reminder of the richness of interstellar phenomena and the importance of continued vigilance and innovation in astronomical research.
Will ‘Oumuamua Return?
Given its hyperbolic trajectory, ‘Oumuamua is highly unlikely to return to our solar system. Objects on hyperbolic paths are not gravitationally bound to the Sun; instead, they are interstellar travelers passing through our solar neighborhood at high speeds. Once ‘Oumuamua passed perihelion—its closest approach to the Sun—its velocity increased significantly due to gravitational acceleration, and it is now receding from our solar system at an estimated speed of approximately 26 kilometers per second relative to the Sun. This rapid departure means that, barring extraordinary gravitational influences or unforeseen cosmic events, it will not return.
‘Oumuamua’s trajectory through the inner Solar System.
The probability of ‘Oumuamua making a second pass is effectively zero. Its trajectory indicates a one-time visit, highlighting the importance of developing advanced detection and tracking systems to identify interstellar objects early on. Such preparedness would allow scientists to study these visitors more comprehensively and potentially gather valuable data about their composition, origin, and trajectories. Understanding ‘Oumuamua's characteristics—such as its elongated shape, unusual acceleration, and surface properties—has already sparked debates about its nature, with some researchers suggesting it could be an alien probe or artifact, though mainstream science remains cautious.
The discovery of additional interstellar objects, like 2I/Borisov, which was identified in 2019, will provide a broader context for understanding these visitors. Each new object offers crucial insights into the composition, diversity, and frequency of interstellar bodies passing through our solar system. These findings could eventually help scientists piece together the history of material exchange between star systems, shedding light on the formation and evolution of planetary systems across the galaxy.
In conclusion, while ‘Oumuamua itself is unlikely to revisit our solar system, its passage has opened an exciting new chapter in astronomy. Continued efforts to detect and analyze interstellar objects could not only enhance our understanding of the cosmos but also possibly reveal signs of extraterrestrial technology or life, should such evidence exist. The future of interstellar object research promises to be a fascinating and rapidly evolving field, offering much to explore beyond our solar neighborhood.
Conclusion
In sum, ‘Oumuamua remains one of the most perplexing interstellar objects observed to date. While some have proposed that it could be an extraterrestrial craft, the majority of scientific evidence supports a natural origin—most likely as a fragment of a larger body from another star system. Its peculiar shape, acceleration, and lack of typical cometary features have fueled speculation, but no definitive proof has emerged to confirm an artificial origin.
The question of whether ‘Oumuamua is an alien spacecraft ultimately hinges on the quality and interpretation of available data. As our observational capabilities improve and we detect more interstellar visitors, the scientific community will be better equipped to answer these profound questions. For now, ‘Oumuamua remains a fascinating natural enigma, reminding us of the vast unknowns that lie beyond our solar neighborhood. Its passing has underscored the importance of continued exploration and vigilance in the search for extraterrestrial life and technology.
References
Meech, K. J., et al. (2017). "A brief visit from a strange interstellar visitor." Nature, 552(7685), 378–381.
Bialy, S., & Loeb, A. (2018). "Could Solar Radiation Pressure Explain ‘Oumuamua’s Peculiar Acceleration?" Astrophysical Journal Letters, 868(2), L1.
Loeb, A., & Bialy, S. (2018). "Could ‘Oumuamua be a lightsail from an alien civilization?" Astrophysical Journal Letters, 857(2), L3.
Jewitt, D. (2022). "Interstellar objects: A review." The Astrophysical Journal, 927(2), 123.
NASA. (2018). "'Oumuamua: First Interstellar Object Detected Passing Through Our Solar System." NASA Fact Sheet.
In conclusion, while the hypothesis that ‘Oumuamua is an extraterrestrial craft is intriguing and has garnered significant media attention, the prevailing scientific consensus attributes its unusual characteristics to natural phenomena. Its unlikely return underscores the importance of ongoing and future observations to better understand interstellar objects. As our detection capabilities improve, so too will our understanding of these cosmic visitors, possibly revealing more about the universe’s hidden wonders and the potential for extraterrestrial life.
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The asteroid size distribution. Even though there are only a handful of large asteroids, those objects outweigh all of the small ones.
Credit: Marco Colombo, DensityDesign Research Lab via Wikimedia Commons.
A simulation of how a cigar-like shape for ‘Oumuamua would match its large observed brightness oscillations.
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Over mijzelf
Ik ben Pieter, en gebruik soms ook wel de schuilnaam Peter2011.
Ik ben een man en woon in Linter (België) en mijn beroep is Ik ben op rust..
Ik ben geboren op 18/10/1950 en ben nu dus 75 jaar jong.
Mijn hobby's zijn: Ufologie en andere esoterische onderwerpen.
Op deze blog vind je onder artikels, werk van mezelf. Mijn dank gaat ook naar André, Ingrid, Oliver, Paul, Vincent, Georges Filer en MUFON voor de bijdragen voor de verschillende categorieën...
Veel leesplezier en geef je mening over deze blog.