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    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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    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.
    12-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Physicists capture rare illusion of an object moving at 99.9% the speed of light

    Physicists capture rare illusion of an object moving at 99.9% the speed of light

    An image of two shapes made out of red light. On the left, a rectangular prism. On the right, a series of vertical lines that form the shape of a circle.
    The Vienna team stitched together slices of light to create snapshots. At rest (left), the cube looks normal. But when simulated at 99.9% of light speed (right), a sphere still looks round but reveals parts of its far side. 
    (Image credit: Hornof et al., 2025CC BY 4.0)

    Using ultra-fast laser pulses and special cameras, scientists have simulated an optical illusion that appears to defy Einstein's theory of special relativity.

    One consequence of special relativity is that fast-moving objects should appear shortened in the direction of motion — a phenomenon known as Lorentz contraction. This effect has been confirmed indirectly in particle accelerator experiments.

    Although previous models have worked with this illusion, now called the Terrell-Penrose effect, this is the first time it has been done in a lab setting. The team described their results in the journal Communications Physics.

    "What I like most is the simplicity," Dominik Hornof, a quantum physicist at the Vienna University of Technology and first author of the study, told Live Science. "With the right idea, you can recreate relativistic effects in a small lab. It shows that even century-old predictions can be brought to life in a really intuitive way."

    Re-creating the illusion

    In the new study, physicists used ultra-fast laser pulses and gated cameras to produce snapshots of a cube and a sphere "moving" at nearly the speed of light. The results showed snapshots of rotated objects. This proved the Terrell-Penrose effect to be true.

    A diagram of an experimental set-up

    The researchers fired ultra-short laser pulses at their test object and then used a delay generator to tell the camera exactly when to open its shutter (for just billionths of a second). This camera captured single slices of light bouncing off the object. They repeated the process and shifted the object between shots. The team built up the illusion of an object racing at near light speed. (Image credit: Hornof et al., 2025CC BY 4.0)

    But like every study, this one also had its difficulties. Moving any object at or near the speed of light is currently impossible. "In Einstein's theory, the faster something moves, the more its effective mass increases. As you get closer to the speed of light, the energy you need grows by a lot," Hornof said. We cannot generate enough energy to accelerate something like a cube, and "that's why we need huge particle accelerators, even just to move electrons close to that speed. It would take a huge amount of energy."

    So the team used a clever substitute. "What we can do is mimic the visual effect," Hornof said. They started with a cube of about 3 feet (1 meter) on each side. Then, they fired ultra-short laser pulses — each just 300 picoseconds long, or about a tenth of a billionth of a second — at the object. They captured the reflected light with a gated camera that opened only for that instant and produced a thin "slice" each time.

    After each slice, they moved the cube forward about 1.9 inches (4.8 cm). That is the distance it would have traveled if it were moving at 80% the speed of light during the delay between pulses. Then, the scientists put all of these slices together into a snapshot of the cube in motion.

    "When you combine all the slices, the object looks like it's racing incredibly fast, even though it never moved at all," Hornof said. "At the end of the day, it's just geometry."

    They repeated the process with a sphere, shifting it by 2.4 inches (6 cm) per step to mimic 99.9% light speed. When the slices were combined, the cube appeared rotated and the sphere looked as if you could peek around its sides.

    "The rotation is not physical," Hornof said. "It's an optical illusion. The geometry of how light arrives at the same time tricks our eyes."

    That is why the Terrell-Penrose effect does not contradict Einstein's special relativity. A fast-moving object is physically shortened along its direction of travel, but a camera doesn't capture that directly. Because light from the back takes longer to arrive than light from the front, the snapshot shifts in a way that makes the object appear rotated.

    "When we did the calculations, we were surprised how beautifully the geometry worked out," Hornof said. "Seeing it appear in the images was really exciting."

    https://www.livescience.com/physics-mathematics }

    12-10-2025 om 18:41 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.10 Dark Matter Facts That Will Surprise You

    10 Dark Matter Facts That Will Surprise You

    The following 10 facts are a summary of what scientists have learned about this invisible stuff.

    Dark matter is one of the biggest mysteries of modern science, because we can’t see it, touch it or feel it with our current instruments, and yet, we know it’s there because we can see how it affects galaxies, and its presence is felt through its gravity. Light bends around it as it travels across the universe, and the distribution of dark matter is known because of the way galaxies and galaxy clusters move, and the universe itself evolved differently than it would have if dark matter weren’t present.

    The following 10 facts are a summary of what scientists have learned about this invisible stuff.

    1. It outweighs the stuff we can see, because scientists have taken data from a number of missions, including the European Space Agency’s Planck mission, to show that regular atoms make up only about 5 percent of the universe, while dark matter makes up about 26 percent, and dark energy about 69 percent, which means that everything we can see and touch is only a small fraction of the universe’s mass-energy budget.

    2. It’s invisible to light, because dark matter doesn’t emit, absorb or reflect any electromagnetic radiation, so our telescopes can’t spot it directly, but we know it’s there from the gravitational pull it exerts on stars, planets and galaxies, and stars in the outer regions of galaxies move faster than the stars closer to the center, which wouldn’t be possible if all we could see was the total amount of mass in the universe.

    3. It’s not a new idea, since in the 1930s, Swiss astrophysicist Fritz Zwicky noticed that galaxies were moving so fast within galaxy clusters that the clusters should be flying apart, unless there was some invisible mass holding them together, which he called “dunkle Materie” — dark matter, and in the 1970s, Vera Rubin and Kent Ford made the same discovery in the rotation curves of spiral galaxies, thus turning it from a hunch to a fact of modern cosmology.

    4. The Big Bang afterglow agrees, because dark matter affects the cosmic microwave background, the afterglow of the Big Bang, and satellites like WMAP and Planck have mapped the tiny ripples of heat in the CMB in exquisite detail, which agree with models that include dark matter, and without it, galaxies would not have formed so quickly.

    5. It’s not made of normal atoms, because if dark matter were made of protons, neutrons or electrons, we would see clear signatures of that in the cosmic microwave background and in the abundance of light elements created in the first few minutes after the Big Bang, but we don’t, so that means dark matter is some other kind of particle.

    6. Top candidates for dark matter are WIMPs and axions, because weakly interacting massive particles (WIMPs) and axions are two of the top contenders, where WIMPs would be heavy and interact via gravity and the weak force, while axions would be extremely light, and several experiments, such as XENONnT, LUX-ZEPLIN and ADMX, are currently hunting for signs of WIMPs and axions.

    7. It molds galaxies and clusters, because dark matter provides the gravitational scaffolding that keeps galaxies and galaxy clusters together, while it also warps light across the universe, according to Einstein, where mass warps space and bends light, an effect called gravitational lensing, which has been observed by the Hubble Space Telescope, the Atacama Cosmology Telescope and other observatories, that have seen distant galaxies that are stretched and warped by massive, invisible structures, and those distortions create maps of where dark matter is.

    8. It might only feel gravity, because no lab has yet detected dark matter interacting with anything except gravity, and the lack of signals at the Large Hadron Collider and other facilities has led some researchers to explore other ideas, such as self-interacting dark matter and sterile neutrinos.

    9. It draws the cosmic web, because on the largest scales, galaxies are arranged into a web of filaments and galaxy clusters, which matches the distribution of dark matter in both simulations and maps of gravitational lensing, and dark matter’s gravity drew normal matter into those structures, giving the universe its large-scale architecture.

    10. The existence of dark matter is supported by a wide range of observations, from the rotation curves of galaxies to the cosmic microwave background, therefore, whether it turns out to be a new particle, a tweak to gravity, or something we haven’t yet imagined, solving this mystery is key to understanding the universe and what it’s really made of.

    Related Posts

    https://curiosmos.com/category/unsolved-mysteries/ }

    12-10-2025 om 17:59 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen. The cosmos is changing before our eyes — and astronomers can barely keep up. A never-before-seen supernova is rewriting ...

    The cosmos is changing before our eyes — and astronomers can barely keep up. A never-before-seen supernova is rewriting ...

    The cosmos is changing before our eyes — and astronomers can barely keep up. A never-before-seen supernova is rewriting ...

    {https://www.youtube.com/ }

    12-10-2025 om 17:25 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.A Mysterious Warp at the Edge of the Solar System May Point to the Existence of a Hidden “Planet Y”

    Planet Y

    (Image Credit: Kevin Gill/Elizabeth Gill/CC 2.0)

    A Mysterious Warp at the Edge of the Solar System May Point to the Existence of a Hidden “Planet Y”

    A strange tilt in the outer reaches of the Kuiper Belt has scientists wondering if the solar system is hiding another planet—a potential “Planet Y” that could soon join the family of known worlds.

    The Kuiper Belt is an enormous ring of icy bodies that extends from the orbit of Neptune to a distance of close to 30 astronomical units (AU), or approximately 30 times the distance from Earth to the Sun. During recent investigations of this mysterious outer solar system region, a team of Princeton researchers uncovered a strange warp in its plane, which could mean that something is pulling on some of the icy objects beyond Neptune—possibly even an undiscovered planet.

    Eying the Kuiper Belt

    The Princeton team’s work began with a simple question: “Is the Kuiper Belt flat?” Despite some slight deviations, the planets in our solar system all lie on roughly the same plane, which should be reflected in the belt. However, the Kuiper Belt unexpectedly changes this orientation with a tilt of about 15 degrees. Despite the team’s best efforts, most potential explanations failed to account for the unusual warpage, save for one: the potential existence of an unknown body the researchers dub “Planet Y.”

    While there has been no direct observation of this currently theoretical planet, the team believes that current data suggests the planet would be between the sizes of Earth and Mercury, positioned deep in the outer reaches of our solar system. 

    “This paper is not a discovery of a planet, but it’s certainly the discovery of a puzzle for which a planet is a likely solution,”  the authors said when presenting their work in the Monthly Notices of the Royal Astronomical Society: Letters.

    A New Addition to the Solar System?

    This isn’t the first time a theoretical planet has been suspected to lurk in the Kuiper Belt, which once held a recognized planet until one of its largest residents, Pluto, was reclassified as a dwarf planet in 2006. The region remains mysterious due to difficulties in observing it at such great distances.

    Earlier work sought what astronomer Percival Lowell dubbed “Planet X,” an attempt to explain away other anomalies by proposing a mysterious hidden planet. Those anomalies were in the orbits of the planets Neptune and Uranus, and even the 1930 discovery of Pluto didn’t prove to be enough to account for them. 

    However, the mystery resolved itself in a less dramatic way than expected when Voyager 2 probe data revealed Neptune’s mass to be less than speculated in the 1990s. The recognition of a less massive Neptune seemingly resolved the question of the irregularities without requiring the pull of an unknown body.

    Planet Y and the Search for Planet Nine

    However, the search for a mysterious planet reignited with a 2016 paper speculating on what was now being called “Planet Nine” instead of “Planet X.” However, this long-suspected outer-solar system planetary body differs considerably from what the recent Princeton University research proposes, as this planet would be much larger and farther out beyond Pluto.

    There is a great deal of debate over what an undiscovered planet in our solar system might look like, but the Princeton team says that they are not mutually exclusive. In theory, a pair of undiscovered planets could coexist beyond the range of our present observations.

    Pentetrating the mysteries of the Kuiper Belt may soon be on the horizon, though, as the Vera C. Rubin Observatory in Chile is about to launch its decade-long survey, which the researchers believe will likely detect any such planet in the Kuiper Belt within two to three years.

    Hence, the Vera C. Rubin Observatory may soon be able to finally resolve the question of whether other worlds might exist in our planetary neighborhood, as well as which planetary category the Princeton team’s suspected “Planet Y” belongs to.

    The paper, “Measuring the Mean Plane of the Distant Kuiper Belt,” appeared in Monthly Notices of the Royal Astronomical Society: Letters on August 21, 2025.

    • Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

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    https://thedebrief.org/category/astronomy/ }

    12-10-2025 om 17:12 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    11-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Precise date interstellar visitor will reveal itself as 'alien mothership' or comet confirmed

    Precise date interstellar visitor will reveal itself as 'alien mothership' or comet confirmed

    The mysterious interstellar visitor streaking through our Solar System is just days away from revealing its true origins.

    Harvard professor Avi Loeb told DailyMail.com that if the object, dubbed 3I/ATLAS, is a comet, it should 'disintegrate into fragments' as it swings closest to the sun on October 29, 2025. 

    The European Space Agency's Jupiter probe will have a front-row seat, capturing the moment it either breaks apart or, as Loeb speculated, 'releases mini-probes as a technological mothership.'

    'When a comet gets close to the sun, solar radiation heats its icy nucleus,' Loeb explained. 

    'Volatile ices like carbon dioxide, carbon monoxide, or water sublimate directly into gas, carrying away dust and small rocks. 

    'This process can cause the comet to break apart if the mix of ice and dust cannot withstand the thermal stress.'

    But if it does not, Loeb said, it could release 'a fleet of mini-probes to study multiple targets simultaneously.'

    Loeb noted there is a 30 to 40 percent chance the object 'does not have a fully natural origin,' noting the possibility it is a 'Trojan Horse,' where a technological object masquerades as a comet.

    Harvard professor Avi Loeb told DailyMail.com that if the object, dubbed 3I/ATLAS, is a comet, it should 'disintegrate into fragments' as it swings closest to the sun on October 29, 2025

    Harvard professor Avi Loeb told DailyMail.com that if the object, dubbed 3I/ATLAS, is a comet, it should 'disintegrate into fragments' as it swings closest to the sun on October 29, 2025

    The ESA's Jupiter Icy Moons Explorer (Juice) craft will have a view of the object when it comes 125 million miles from the planet and monitor it through November.

    'During November and December, terrestrial observatories will also be able to monitor 3I/ATLAS and check whether it disintegrated like a natural comet or released mini-probes as a technological mothership,' Loeb explained.

    While the professor believes there is a possibility it is of alien origin, NASA has long said the object is a natural comet.

    The American space agency released images of 3I/ATLAS as it soared past Mars on October 3, showing it as cylindrical-shaped. 

    Stargazers on social media shared color-enhanced images of the object, which showed the interstellar visitor having a green glow. 

    Loeb and many other scientists are anticipating the visitor's journey to the sun as it will finally put the mystery to rest

    3I/ATLAS will appear as a fuzzy ball of light in the blackness of space, and if it does disintegrate, the professor said it will break into independent, smaller dots of light. 

    'Comets disintegrate primarily as a result of heating by the sun, but sometimes also by gravitational tides and rotational stress from outgassing,' Loeb explained.

    NASA released images of 3I/ATLAS as it soared past Mars on October 3, showing it as cylindrical-shaped. Stargazers on social media shared color-enhanced images of the object, which showed the interstellar visitor having a green glow

    NASA released images of 3I/ATLAS as it soared past Mars on October 3, showing it as cylindrical-shaped. Stargazers on social media shared color-enhanced images of the object, which showed the interstellar visitor having a green glow

    'The catastrophic breakup of a comet into multiple fragments is difficult to forecast without knowing its detailed composition and material strength.' 

    So far, ESA’s Mars orbiters have not spotted any verified fragments, only faint artifacts and noise, as 3I/ATLAS moves closer to the sun.

    Some reports have claimed that mysterious objects have been spotted with 3I/ATLAS, but Loeb told Daily Mail that these are false.

    'There are unrelated contemporary comets, background stars and images of the moons of Mars, Phobos and Deimos, which appear in some images. But so far, no verified object branched off 3I/ATLAS,' the professor explained.

    The object was first identified in July 2025 by the ATLAS telescope network, which looks for objects that might hit Earth.

    Earlier images taken by the Vera C Rubin Observatory in Chile this summer had unknowingly photographed the object as well, but no one realized it was there at the time.

    https://www.dailymail.co.uk/sciencetech/index.html }

    11-10-2025 om 14:50 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    10-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Celestial standoff! Scientists capture an image of two black holes circling each other for the first time

    Celestial standoff! Scientists capture an image of two black holes circling each other for the first time

    An image of two black holes circling each other has been captured for the very first time.

    Astronomers spotted the celestial standoff in the heart of the galaxy OJ287, around five billion light-years from Earth.

    Previously, scientists have only been able to produce images of individual supermassive black holes, such as the one at the centre of our own Galaxy.

    However, scientists from the University of Turku, Finland, have now produced the first direct proof that black holes can come in pairs.

    For years, scientists have suspected that OJ287 might be hiding two black holes, but there hasn't been a telescope powerful enough to tell them apart.

    By combining antennas on Earth with a satellite located halfway to the moon, the astronomers created a radio telescope effectively 15 times larger than Earth.

    That allowed them to take an image with a resolution 100,000 times higher than anything that had been used to observe OJ287 in the past.

    Lead researcher Professor Mauri Valtonen says: 'For the first time, we managed to get an image of two black holes circling each other.'

    Scientists have captured an image of two black holes circling one another for the very first time, proving that black holes come in pairs

    Scientists have captured an image of two black holes circling one another for the very first time, proving that black holes come in pairs 

    The pair of black holes is located at the centre of the quasar OJ287, an extremely bright galactic core around five billion light-years from Earth. Pictured: An artist's impression of OJ287

    The pair of black holes is located at the centre of the quasar OJ287, an extremely bright galactic core around five billion light-years from Earth.

    Pictured: An artist's impression of OJ287

    OJ287 is a type of object known as a quasar, which is an extremely bright galactic core holding a supermassive black hole.

    The black hole itself doesn't give out any light, but the gas and dust falling into the singularity become so hot that they produce massive amounts of radiation.

    Quasar OJ287 is actually so bright that, despite being five billion light-years away, even an amateur astronomer with a decent telescope should be able to see it.

    However, in the 1980s, scientists realised that the quasar's light was fluctuating in a reliable 12-year pattern.

    Professor Valtonen says: 'What is special about OJ287 is that it has been thought to harbour not one but two black holes circling each other in a twelve-year orbit, which produces an easily recognisable pattern of light variations in the same period.'

    Even though scientists were pretty sure that there were two supermassive black holes hiding within the quasar, it still took decades to prove this.

    Even when NASA's TESS satellite was able to detect light from both black holes in 2021, the resulting image still only showed a single object.

    The problem was that normal light-based telescopes simply can't produce a high enough resolution to peel apart the signals from these extremely distant objects.

    Until now, scientists have only ever been able to take images of single black holes such as the black hole at the centre of our own galaxy, Sagittarius A* (pictured)

    Until now, scientists have only ever been able to take images of single black holes such as the black hole at the centre of our own galaxy, Sagittarius A* (pictured)

    Using a very large radio telescope, the scientists revealed that there are two black holes. A very large one at the centre, and a smaller one that orbits its neighbour once every 12 years

    Using a very large radio telescope, the scientists revealed that there are two black holes. A very large one at the centre, and a smaller one that orbits its neighbour once every 12 years 

    What are black holes?

    Black holes are areas where matter has become so dense that it forms a 'singularity'.

    Their gravitational pull is so strong that not even light can escape, which is why they appear black.

    Inside the singularity, the laws of physics as we understand them appear to break down and behave in unusual ways. 

    Scientists think most black holes are formed when stars collapse in supernovae.

    However, some supermassive black holes might have been formed right after the Big Bang, before the first stars had even formed.  

    To see more, the scientists used a technique called 'Very Long Baseline Interferometry'.

    This essentially involves combining radio telescopes scattered across Earth and throughout space into a single enormous 'virtual' telescope.

    By adding the RadioAstron satellite, which was halfway to the moon when the images were taken, researchers were finally able to take a radio image of the quasar.

    In their new paper, published in the Astrophysical Journal, Professor Valtonen compared their images to theoretical calculations and found that the black holes were exactly where they were expected to be.

    Professor Valtonen says: 'In the image, the black holes are identified by the intense particle jets they emit.

    'The black holes themselves are perfectly black, but they can be detected by these particle jets or by the glowing gas surrounding the hole.'

    These images revealed that one of the black holes was significantly larger than the other.

    The bigger has a mass about 18.35 billion times that of the sun, while the smaller is around 150 million solar masses. 

    By comparing these radio images (pictured) to the theoretical models (shown as stars), the researchers showed that the jets produced by the black holes followed the exact path scientists had predicted

    By comparing these radio images (pictured) to the theoretical models (shown as stars), the researchers showed that the jets produced by the black holes followed the exact path scientists had predicted 

    That means the smaller is constantly spun around by the intense gravity, slamming through the larger black hole's accretion disk with each pass.

    Every time the black hole passes through this cloud of dust and gas, the researchers estimate that it pulls away about 16 solar masses of material.

    However, the larger black hole's accretion disc is so large that this barely makes a difference to the overall system.

    In addition to proving that black hole pairs exist, the researchers also made an interesting discovery about these particle jets.

    They found that the jet emanating from the smaller black hole was twisted, much like the stream of water emerging from a spinning, out-of-control firehose.

    Because this smaller black hole is moving so fast around its larger neighbour, its particle jet is diverted depending on where it is currently moving.

    The researchers call this a 'wagging tail' jet and predict that it should be seen twisting in different directions in the coming years when the smaller black hole changes its speed and direction.

    EINSTEIN'S GENERAL THEORY OF RELATIVITY

    Albert Einstein

    Albert Einstein

    In 1905, Albert Einstein determined that the laws of physics are the same for all non-accelerating observers, and that the speed of light in a vacuum was independent of the motion of all observers - known as the theory of special relativity.

    This groundbreaking work introduced a new framework for all of physics, and proposed new concepts of space and time.

    He then spent 10 years trying to include acceleration in the theory, finally publishing his theory of general relativity in 1915.

    This determined that massive objects cause a distortion in space-time, which is felt as gravity.

    At its simplest, it can be thought of as a giant rubber sheet with a bowling ball in the centre.

    Pictured is the original historical documents related to Einstein's prediction of the existence of gravitational waves, shown at the Hebrew university in Jerusalem

    Pictured is the original historical documents related to Einstein's prediction of the existence of gravitational waves, shown at the Hebrew university in Jerusalem

    As the ball warps the sheet, a planet bends the fabric of space-time, creating the force that we feel as gravity.

    Any object that comes near to the body falls towards it because of the effect.

    Einstein predicted that if two massive bodies came together it would create such a huge ripple in space time that it should be detectable on Earth.

    It was most recently demonstrated in the hit film film Interstellar.

    In a segment that saw the crew visit a planet which fell within the gravitational grasp of a huge black hole, the event caused time to slow down massively.

    Crew members on the planet barely aged while those on the ship were decades older on their return.

    https://www.dailymail.co.uk/sciencetech/index.html }

    10-10-2025 om 18:17 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.3I/ATLAS is Displaying Surprising New Activity That Scientists Liken to “a Note from Another Planetary System”

    3I/ATLAS

    3I/ATLAS, as seen by the Gemini South observatory in August 2025

    (Credit: International Gemini Observatory/NOIRLab/NSF/AURA/Shadow the Scientist).

    3I/ATLAS is Displaying Surprising New Activity That Scientists Liken to “a Note from Another Planetary System”

    Physicists have detected water activity during observations of the mysterious comet 3I/ATLAS, marking the first time hydroxyl gas, a chemical signature of water, has been detected from the interstellar visitor

    Using NASA’s Neil Gehrels Swift Observatory, the Auburn University team determined 3I/ATLAS is releasing water at a rate of roughly 40 kilograms per second, comparable to a fire hose running at full blast, while positioned nearly three times farther from the Sun than Earth.

    What makes this finding particularly remarkable is the distance at which this activity was observed: 2.90 astronomical units, well beyond the region where most solar system comets show any significant signs of such activity.

    “When we detect water—or even its faint ultraviolet echo, OH—from an interstellar comet, we’re reading a note from another planetary system,” explained Dennis Bodewits, professor of physics at Auburn University and principal investigator of the study, in a press release. “It tells us that the ingredients for life’s chemistry are not unique to our own.”

    3I/ATLAS
    NASA’s Swift Ultraviolet/Optical Telescope (UVOT) observed interstellar comet 3I/ATLAS during two visits in July and August 2025. The panels show visible-light (left) and ultraviolet (right) images, where the faint glow of water vapor escaping from the comet.
    (Image: Dennis Bodewits, Auburn University)

    According to their paper, the scientists used ultraviolet light to detect water molecules coming off the comet. The team found that there is a specific signal water gives off as it breaks apart in space, and the water the comet was releasing grew significantly between late July and mid-August 2025.

    To make this discovery, they relied on NASA’s Swift telescope, which orbits high above Earth. Even though Swift only has a 12-inch mirror, it can see ultraviolet light much better than telescopes on the ground because it’s beyond our atmosphere, which normally blocks most ultraviolet light from reaching telescopes on the surface. From its location in space, Swift has the same power as a much larger 13-foot telescope would have on Earth for this type of observation.

    Since its discovery on July 1, 2025, by the NASA-funded ATLAS survey telescope in Chile, 3I/ATLAS has consistently defied expectations. Previous research reported by The Debrief has revealed that this interstellar visitor is “anomalously massive” compared to its predecessors, with recent studies suggesting a minimum nucleus diameter of roughly five kilometers and a mass of at least 33 billion tons.

    This extraordinary size places 3I/ATLAS several orders of magnitude more massive than the first two known interstellar objects, 1I/’Oumuamua and 2I/Borisov. As Harvard astronomer Avi Loeb noted in previous correspondence with The Debrief, “We should have detected an order of 100,000 ‘Oumuamuas before discovering an object as big as 3I/ATLAS”.

    3I/ATLAS
    Hubble Telescope image of the mysterious interstellar comet 3I/ATLAS
    (Image Credit: ESA/Hubble).

    The comet’s massive nature helps explain its ability to maintain course despite significant outgassing activity. Unlike smaller objects that would be deflected by gas jets from their sun-facing surfaces, 3I/ATLAS has shown remarkable orbital stability, with non-gravitational acceleration measured at less than 15 meters per day squared.

    The discovery of water emanating from the comet only adds to its complexity and mystique.

    Rather than simple nuclear sublimation, the research suggests water production originates from extended sources, most likely large icy grains in the comet’s coma that sublimate as they’re heated by sunlight. This mechanism, observed in only a handful of distant comets, points to complex, layered ice structures that preserve their ancient formation clues.

    The water detection adds another chapter to the evolving story of interstellar objects in our solar system. As lead researcher Zexi Xing noted, “Every interstellar comet so far has been a surprise. ‘Oumuamua was dry, Borisov was rich in carbon monoxide, and now ATLAS is giving up water at a distance where we didn’t expect it.”

    “Each one is rewriting what we thought we knew about how planets and comets form around stars,” Xing said. 

    Moreover, recent observations by ESA’s ExoMars Trace Gas Orbiter during 3I/ATLAS’s close approach to Mars provided additional imaging opportunities. While the challenging observation conditions highlighted the technical difficulties of studying these rare visitors, it was still considered a unique opportunity to use the orbiter for something outside of its mission parameters.

    “Though our Mars orbiters continue to make impressive contributions to Mars science,” ESA project scientist Colin Wilson said at the time. “It’s always extra exciting to see them responding to unexpected situations like this one.”

    3I/ATLAS will become observable again after mid-November 2025, offering additional opportunities to track its evolution as it approaches perihelion on October 30. The comet’s trajectory will take it within 1.4 astronomical units of the Sun, just inside Mars’s orbit, before it exits our solar system forever, traveling at a speedy 130,000 miles per hour.

    The discovery has profound implications for our understanding of planetary system formation across the galaxy. The presence of water activity in an interstellar comet demonstrates that the basic chemical ingredients for life are not unique to our solar system. Moreover, the complex ice structures indicated by extended water sources preserve information about formation conditions in distant stellar environments billions of years ago.

    As 3I/ATLAS continues on its journey through our solar system, astronomers worldwide are seizing this rare opportunity to study material that has drifted through interstellar space for potentially billions of years. Each observation brings new insights into the diversity of planetary systems and the cosmic processes that shape the building blocks of life throughout our galaxy.

    • MJ Banias covers space, security, and technology with The Debrief. You can email him at mj@thedebrief.org or follow him on Twitter @mjbanias.

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    https://thedebrief.org/category/space/ }

    10-10-2025 om 17:11 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    09-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Soar through a 1,000-mile-long maze on Mars in this mesmerizing new satellite video

    Soar through a 1,000-mile-long maze on Mars in this mesmerizing new satellite video

    Fly over Xanthe Terra with Mars Express - YouTube
    Watch OIf you've ever wanted to get lost on Mars, now's your chance: You can fly over a maze-like canyon on the Red Planet in a stunning new video from the European Space Agency (ESA).

    "Central to the tour is a 1300 km [808-mile]-long outflow channel called Shalbatana Vallis," they explained. "It cascades down from the highland region of Xanthe Terra to the smoother lowlands of Chryse Planitia. Billions of years ago, water surged through this channel, creating many of the features we see today. The tour culminates in a spectacular view of a 100 km [62-mile]-wide impact crater, smashed out of Mars's surface when it collided with a space rock."

    Xanthe Terra was the name the International Astronomical Union gave to this region in 1979, following high-resolution mapping of Mars by spacecraft of that era. The name means something like "golden-yellow land," according to DLR, the German space agency, which funded the camera equipment.

    Keen-eyed video viewers will see the flight cross the "Martian dichotomy boundary," where the craters of the southern highlands gradually smooth into flatter plains in the northern lowlands, DLR stated in a separate statement. Researchers are still not sure why this dichotomy exists.

    The video also features outflow channels that "are wide, deeply incised valley structures that likely formed in Mars' geological past during catastrophic flood events involving enormous quantities of water," DLR officials said. This carving may have happened as volcanoes melted underground ice deposits.

    The Mars Express camera scours Mars' geology as part of the larger mission's search for life, DLR officials added the statement.

    Mars Express has been at the Red Planet since 2003, for what was supposed to be a two-year mission. The spacecraft is still healthy after more than 20 years of service, and it has received multiple mission extensions based on its scientific return.

    "While it may be feeling its age, it continues to lift the lid on the Red Planet, with implications for our understanding of our own home," ESA officials wrote of the long-running mission in 2023.

    RELATED 

    James Webb Space Telescope: Stunning images that show the beauty of space – from galaxies to nebulae

    Everything Discovered By The James Webb Space Telescope (since launch)

    https://www.livescience.com/space }

    09-10-2025 om 22:20 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.An Asteroid Flew Closer Than The ISS Recently

    An Asteroid Flew Closer Than The ISS Recently

    Image of Asteroid 2025 TF, which made a close approach over Antarctica on October 1st. Credit - ESA / Las Cumbres Observatory
    Image of Asteroid 2025 TF, which made a close approach over Antarctica on October 1st.
    Credit - ESA / Las Cumbres Observatory

    An asteroid recently made the second closest pass to Earth ever observed on October 1st. And astronomers only found it after it had already completed its closest approach. That offers another lesson in how difficult it is to find small objects coming close to our planet in the vast dark ocean of space.

    To be clear, the asteroid, now known as Asteroid 2025 TF, didn’t pose any sort of danger. It is likely only 1-3m across, and would have created a pretty spectacular fireball if it had entered Earth’s atmosphere - but most likely no one would have been there to see it as it flew over Antarctica in the beginning of their spring. There was a possibility it would have burnt down to a meteorite that could have one day been discovered though.

    Alas, that didn’t happen as the asteroid made a pass around 428 km above the southern continent at around 1 AM UTC on October 1st. For comparison, that’s around the same height as the international space station’s orbit, which can vary from between 370 and 460 km. It would have been a very bad day if those two had found each other, but luckily the orbital space that far above the planet is vast, and even something as large as the ISS is easy to miss in that vastness.

    Fraser discusses the difficulty in finding asteroids that could impact Earth

    Astronomers from the Kitt Peak National Observatory in Arizona first detected the asteroid only a few hours after its closest approach using the Bott Telescope. Additional observations came from the Catalina Sky Survey and the European Space Agency’s Planetary Defense Office, who utilized the Las Cumbres Observatory in Siding Spring, Australia.

    2025 TF marks the second closest approach of any known asteroid, behind only 2020 VT4, a slightly larger asteroid estimated to be about 5-10 m across that passed about 386 km above the Pacific Ocean in November 2020. It, too, was found after its closest approach - about 15 hours later compared to the 6 hours that it took astronomers to discover 2025 TF.

    While these relatively small asteroids don’t pose any danger to the planet themselves, they do pose a threat to the increasing constellation of orbital infrastructure present, especially in low Earth orbit. An impact of one of these rocks, which likely occurs relatively frequently, could be the start of a chain reaction that leads to Kessler Syndrome or a similar dismal fate for our orbital infrastructure.

    The fireball video Fraser describes in this video is similar to what might have happend if Asteroid 2025 TF hit the atmosphere.

    Unfortunately, we still don’t have the means to protect against these kinds of incursions into our planet’s personal space. To do so would require a massive effort with a combination of more ground-based telescopes linked up with space-based observatories specifically designed to track these small, dark, fast-moving objects. Given the current state of international cooperation and funding in space, that seems unlikely for now.

    Until we get to that point, we just have to hope that, when we see a fireball in the sky, its not one of these asteroids taking out a piece of valuable orbital infrastructure. Or, if it is, then maybe that would provide enough impetus to the powers that be to do something about what could be an impending disaster that locks us on our world for decades.

    Learn More:

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    https://www.universetoday.com/ }

    09-10-2025 om 20:29 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Longstanding “Ice Giant” Classification of Uranus and Neptune Might Be Conflicted

    Longstanding “Ice Giant” Classification of Uranus and Neptune Might Be Conflicted

    Uranus and Neptune. Credit: NASA
    Uranus and Neptune.
    Credit: NASA

    What if our understanding of Uranus and Neptune’s compositions have been wrong, specifically regarding their classifications as “ice giants”? This is what a recent study accepted for publication in *Astronomy & Astrophysics* hopes to address as a team of researchers from the University of Zurich investigated the interior structures of Uranus and Neptune. This study has the potential to help scientists not only better understand the formation and evolution of Uranus and Neptune but could also provide key insights into Jupiter and Saturn, and gaseous exoplanets, too.

    For the study, the researchers analyzed a series of computer models designed to simulate the interiors of Uranus and Neptune based on current planetary data for each, including mass, equatorial radius, pressure, reference radius, rotation period, and gravitational moments. Combining this with new algorithms, the researchers wanted to ascertain a better understanding of the interiors of both Uranus and Neptune and planetary interiors, overall. While a planet’s equatorial radius is measured from the center of the planet to its equator, this works best for solid surfaces. Since Uranus and Neptune are gas planets, their equatorial radii are measured from the center to the edge of their gaseous atmospheres. Therefore, reference radii are used for gas planets like Uranus and Neptune for modeling purposes.

    In the end, the researchers found interiors compositions of Uranus and Neptune are dominated by rock and water. Specifically, their rock-to-water ratios list Uranus having a larger ratio than Neptune by almost 10 times. As a result, the researchers allude to changing the longstanding classification of Uranus and Neptune being “ice giants” as being “rock giants”.

    The study concludes by stating, “With the potential for future dedicated missions to Uranus and Neptune, our method also provides a flexible and unbiased tool for interpreting forthcoming data. Ultimately, the interiors of Uranus and Neptune remain enigmatic, not because they are beyond reach, but because the data required to resolve their secrets are still out of grasp. Until then, only a plurality of models, not a singular one, can capture the full extent of possibilities for their hidden depths.”

    The only human-made spacecraft to have visited Uranus and Neptune is NASA’s Voyager 2, which occurred in January 1986 and August 1989, respectively. Despite these two brief flybys, Voyager 2 obtained a wealth of knowledge about both gas giants, including data regarding their atmospheres, interiors compositions, moons, and rotational properties. For Uranus, Voyager 2 discovered two new rings and 10 moons, which provided scientists with new insights into rocky planetary body formation and evolution. Voyager 2 was the first to discover that Uranus rotated on its side but still exhibited a magnetic field like Earth’s. The planet’s sunlit pole was found to emit ultraviolet radiation and even emit a peculiar glow. For Neptune, Voyager 2 measured the planet’s mass while also observing auroras that were weaker than on Earth since Neptune’s magnetic field was offset from the center of the planet.

    Future planned missions to Uranus have either only been proposed or are still in the planning stages, the latter of which is China’s Tianwen-4 spacecraft, and with NASA considering the Uranus Orbiter and Probe mission. For Neptune, more than a half-dozen missions have been proposed, most notably NASA’s Neptune Odyssey mission. One of the primary reasons for not sending another spacecraft to Uranus or Neptune is the enormous distance and time it would take to reach them. Voyager 2 circumvented this by taking advantage of a planetary alignment that only happens every 175 years, enabling Voyager 2 and its twin spacecraft, Voyager 1, to visit all the outer planets in a fraction of the time.

    Uranus and Neptune have long been designated as “ice giants” due to their higher water-to-rock ratio than Jupiter and Saturn, which are primarily comprised of hydrogen and helium and are appropriately designated as “gas giants”. Therefore, studies like this not only help scientists understand the formation and evolution of gas giants within our solar system but also shed light on the formation and evolution of gas giant exoplanets, too. What new discoveries about the interiors of Uranus and Neptune will researchers make in the coming years and decades? Only time will tell, and this is why we science!

    • As always, keep doing science & keep looking up!

    https://www.universetoday.com/ }

    09-10-2025 om 20:19 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Yes, Mars Once Had an Ocean, says New Research

    Yes, Mars Once Had an Ocean, says New Research

    The ESA's Mars Express captured this image of an ancient, dried-up river system that spans nearly 700 km (435 mi) across the surface of Mars. Credit: ESA/Björn Schreiner/FU Berlin
    The ESA's Mars Express captured this image of an ancient, dried-up river system that spans nearly 700 km (435 mi) across the surface of Mars.
    Credit: ESA/Björn Schreiner/FU Berlin

    Today, it's a scientific consensus that Mars was once a very different place, with a warmer, denser atmosphere and liquid water on its surface. This is evidenced by flow channels, delta fans, lakebeds, and many other features that form in the presence of flowing water here on Earth. Based on the way many of these channels feed into the Northern Lowlands on Mars, scientists speculate that this region was once home to an ocean that covered the northern hemisphere. According to new research from the University of Arkansas, there is a strong case for the existence of this ancient ocean.

    This was the conclusion reached by geosciences PhD candidate Cory Hughes, who studies the geology of the Earth to the geological history of Mars. For years, researchers have studied sandstone formations in northwestern Arkansas, which were created by rivers that flowed across the area 300 million years ago. By analyzing images taken by NASA's Mars Reconnaissance Orbiter (MRO), Hughes and his colleagues identified key features in delta fans located in Aeolis Dorsa, a northern region within Utopia Planitia. On Earth, these features are known as "backwaters," which form where rivers narrow before emptying into oceans.

    Hugh was joined by John B. Shaw, an associate professor of geosciences and the Vice Chair of the Department of Geosciences at the University of Arkansas, as well as Anjali M. Fernandes and Travis E. Swanson. Fernandes is an Associate Professor of Earth and Environmental Sciences at Denison University, while Swanson is a geoscientist with the Water Institute (a Louisiana-based applied research organization dedicated to supporting coastal and river delta regions). The results of their analysis were published in the journal Geophysical Research Letters.

    Image of the Edington Sandstone formation, located in northwestern Arkansas. Credit: Office of the State Geologist

    Image of the Edington Sandstone formation, located in northwestern Arkansas.

    Credit: Office of the State Geologist

    On Earth, rivers that have no system of levees or human-built barriers shift constantly as they snake across the landscape. The sediment they carry erodes one side, causing the river to bend in that direction while depositing sand and fine dirt on the opposite side, also known as a "channel belt." As a river approaches an open body of water (like an ocean), its velocity will slow down, causing it to carry less sediment. This leads to sediment being deposited, forming river deltas, and causes the channel belt to narrow before it reaches the ocean. This section is known as the "backwater zone," which can extend for hundreds of kilometers.

    Over time, gravity will pull the coarsest grains to the bottom of the river, which will become buried if the river dries up. This is believed to have been what happened on Mars billions of years ago after the planet's atmosphere was slowly stripped away by solar wind (owing to the disappearance of its magnetic field). When rivers dry up, heat and pressure will turn the sediment in the riverbeds into sandstone deposits. On Earth, tectonic activity pushes this stone to the surface, where wind and rain erosion eventually leave behind a ridge known as "inverted channel" (or "inverted ridge").

    This is what took place in northwestern Arkansas roughly 300 million years ago, when a river that ran from modern-day Indiana flowed into a sea that covered central Arkansas. When the ancient river dried up, what resulted was the Wedington Sandstone formation, the only known example of an inverted river delta on Earth. The presence of similar ridges and channel belts on Mars provides direct evidence that rivers once flowed there that emptied into an ocean that covered the northern hemisphere. However, since Mars lacks plate tectonics, its inverted ridges likely formed when finer deposits around the sandstone were eroded.

    "This is a large-scale process taking place, which is why we're able to see it from space on Mars," said Hughes. "These are very mature deltas. This is a strong point in favor of an ancient ocean, or at the very least a large sea." Back in January, Hughes, Shaw, and the Department of Geosciences at the University of Arkansas hosted a conference attended by 12 planetary scientists from NASA's Jet Propulsion Laboratory, the Planetary Science Institute (PSI), the University of Texas, and Stanford University. As part of the conference, attendees visited the Edington Sandstone formation to observe its similarities to the Aeolis Dorsa region.

    As Shaw noted, this latest piece of evidence of Mars' warmer, watery past also bolsters the case for the existence of life on Mars at one time. "We don't know of any lifeforms on Earth, or anywhere in the universe, that don't require liquid water, he said. "So the more liquid water we have on Mars, a simple argument could be made that you have a higher chance of life."

    Further Reading: 

    RELATED VIDEOS

    https://www.universetoday.com/ }

    09-10-2025 om 20:12 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Mysterious interstellar visitor heading towards Earth dubbed a 'Trojan Horse' for alien tech

    Mysterious interstellar visitor heading towards Earth dubbed a 'Trojan Horse' for alien tech

    A scientist has warned that the interstellar visitor moving closer to Earth could be a 'Trojan Horse,' where a technological object masquerades as a comet.

    The Harvard professor, who has been monitoring 3I/ATLAS since its discovery in July, said Wednesday that there is a 30 to 40 percent chance the object 'does not have a fully natural origin.'

    Avi Loeb admitted that his ranking could change after new data comes in over the next few months, including observations next month from a spacecraft en route to Jupiter and when 3I/ATLAS comes 167 miles within Earth in December.

    'We have no idea of the amount of traffic of extraterrestrial probes in the vicinity of the Solar system,' he said in a blog post.

    'Given the uncertainty, it would be prudent to collect as much data as possible on interstellar objects from all directions and assess the level of risk based on that data.'

    The object, a rare visitor from beyond the solar system, is unusually large and closely aligned with the plane of the planets, making it visible to orbiters around Mars over the weekend.

    NASA's rover on the Martian planet snapped images of 3I/ATLAS, which captured it as a massive cylindrical object, sparking fresh theories about alien technology.

    Stargazers on social media shared color-enhanced images of the object, which showed the interstellar visitor having a green glow

    A Harvard scientists said there is a possibility that the interstellar visitor moving closer to Earth could be a 'Trojan Horse,' where a technological object masquerades as a comet

    A Harvard scientists said there is a possibility that the interstellar visitor moving closer to Earth could be a 'Trojan Horse,' where a technological object masquerades as a comet

    Loeb analyzed the Perseverance rover's photos by calculating its distance, speed, and camera settings.

    According to his initial study, Loeb was not convinced that 3I/ATLAS is actually a massive cylindrical object, noting that the strange shape might have been a trick of the rover's camera stretching the object out.

    He explained that the apparent cylinder from the rover's 'Navcam' was likely caused by the camera stacking hundreds of images of 3I/ATLAS over a period of about 10 minutes, making it look more like a log than a ball.

    The professor added that 3I/ATLAS is likely smaller and rounder, but still massive, with a potential diameter of more than 28 miles across.

    Dr Horace Drew, a retired senior researcher at Australia's Commonwealth Scientific and Industrial Research Organization (CSIRO), noted that the mysterious green glow seen in some images could be a result of the object being an interstellar spacecraft coated in nickel.

    He explained that humans use the same practice on Earth-made space technology on a much smaller scale.

    'It is not a "comet,"' Drew shared in a post on X.

    Drew disagreed with Loeb's conclusion that the cylindrical shape was a result of the Mars rover sending back a stretched image over several minutes, claiming that an amateur astronomer on Earth captured a similar shape with their telescope.

    The Perseverance rover on Mars captured new images of the interstellar object 3I/ATLAS as it passed by the planet this weekend
    +1
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    The Perseverance rover on Mars captured new images of the interstellar object 3I/ATLAS as it passed by the planet this weekend

    'We can see an extended white shape, with a green coma outside. Not a small white ball,' Drew explained in a post about the astronomer's photograph.

    However, Loeb recently cited the findings from the Very Large Telescope, highlighting how it detected an unusual nickel plume from the object.

    Unlike natural comets, which always emit nickel alongside iron, 3I/ATLAS shows the metallic element without any detectable iron.

    Loeb explained that this nickel signature is a hallmark of industrial production of nickel alloys.

    'Is this anomaly another clue for a possible technological origin of 3I/ATLAS?' Loeb wrote in a blog post.

    'The paper suggests that chemical formation occurs through the nickel carbonyl channel, an extremely rare process in comets, but a standard technique in industrial nickel refining,' he added.

    The new study, published by astrophysicists in Chile in late August, found that 3I/ATLAS is shedding nickel at roughly five grams per second and cyanide at 20 grams per second, with both rising sharply as the object moves closer to the sun.

    Researchers noted that the mechanisms driving these emissions are not typical of natural cometary processes.

    They hypothesized that nickel might be released from dust through gentle processes, such as sunlight, causing it to evaporate or breaking down small nickel-containing compounds.

    RELATED VIDEOS

    https://www.dailymail.co.uk/sciencetech/index.html }

    09-10-2025 om 16:50 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.“Dust devils” race at the speed of a sports car

    “Dust devils” race at the speed of a sports car

    Even the smallest details of the Martian landscape can hide incredible phenomena. It turns out that dust whirlwinds, also known as “dust devils” on the Red Planet, move at incredible speeds that significantly exceed scientists’ previous estimates.

    A camera aboard ESA’s ExoMars Trace Gas Orbiter captured three dust devils moving across the surface of Mars.
    Image: ESA/TGO/CaSSIS

    Researchers from the University of Bern in Switzerland analyzed archives of images from the European Space Agency’s Mars Express and Trace Gas Orbiter spacecraft. Using artificial intelligence models, they were able to track more than a thousand dust devils recorded over the past two decades. 

    The result is impressive: these whirlwinds can reach speeds of up to 158 km/h, making them much more powerful than previously thought. This discovery radically changes our understanding of the dynamics of the Martian atmosphere.

    Turning artifacts into scientific data

    The most ingenious aspect of this study was the method. None of the orbital vehicles were specifically designed to measure wind. However, the team found a way. They noticed slight color shifts in the images caused by split-second delays between the camera channels. These shifts are usually considered technical noise. But everything that moves across the surface of Mars — clouds or dust whirlwinds — leaves its mark in these shifts. By analyzing these tiny shifts between frames, scientists were able to calculate the speed and direction of each whirlwind.

    Dust devil on the surface of Mars.
    Photo: ESA

    As research leader Valentin Bickel noted, they literally “turned image artifacts into valuable scientific measurements.” 

    This fundamental discovery has direct practical significance for the exploration of Mars. A dust devil is a kind of visualizer of invisible wind. By measuring it, we obtain a map of winds across the entire surface of the planet.

    Animation of the movement of the “dust devil” on Mars

    This information will be invaluable for planning future landings. Scientists will be able to more accurately assess wind conditions at the landing site, predict how much dust will settle on the rovers’ solar panels, and determine the optimal frequency of self-cleaning to maintain viability. 

    Rhythms of Martian weather

    The new catalog also confirms that dust devils have their “favorite” places and times. They most often occur on dust plains such as Amazonis Planitia during the warm seasons of spring and summer. Their activity peaks between late morning and early afternoon, which is very similar to patterns on Earth.

    Map showing 1,039 dust devils detected on Mars, recorded over a period of 20 years by ESA’s Mars Express and ExoMars Trace Gas Orbiter.
    Image: ESA/TGO/CaSSIS

    However, there is a key difference on Mars. Since no rain falls there, dust can remain in the atmosphere for months. Understanding how and when it enters the atmosphere is key to unraveling the planet’s long-term climate cycles and accurately predicting Martian weather. As ESA scientist Colin Wilson noted: “Dust on Mars affects absolutely everything.” 

    Earlier, we reported on how robots on Mars would quickly turn into scrap metal.

    • According to ESA

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    https://universemagazine.com/en/articles-en/ }

    09-10-2025 om 14:27 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    08-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.“Exotic” Discovery Revealed in New Analysis of Apollo-Era Moon Samples is “Different from Anything We Find on Earth”

    apollo 17

    Credit: NASA

    “Exotic” Discovery Revealed in New Analysis of Apollo-Era Moon Samples is “Different from Anything We Find on Earth”

    After half a century, samples collected during NASA’s 1972 Apollo 17 Moon mission are still revealing new secrets about the lunar surface.

    Fortunately for today’s scientists, the Apollo Moon missions had the foresight to store samples for exploitation by technologies and methodologies not yet known at the time. Because of that, a new study in JGR: Planets brings to light a surprising sulfur isotope hiding in the lunar regolith that may also provide clues to the origin of our solar system.

    Apollo Sample Preservation

    Apollo 17 astronauts Gene Cernan and Harrison Schmitt collected these samples of volcanic material from the Taurus Littrow region, after pushing a hollow metal cylinder 60 centimeters into the regolith. Upon their return, the NASA Apollo Next Generation Sample Analysis (ANGSA) program preserved the entire tube full of material in a helium chamber for future scientists to study.

    After fifty years on the shelf, NASA has finally begun allowing researchers to apply modern scientific tools to ANGSA samples. Gaining access to the precious samples is no easy feat, though. A rigorous and competitive application process is in place to ensure that ANGSA releases materials only to the most deserving projects.

    One of the recipients of the lunar samples was James Dottin of Brown University, whose work proposed using ion mass spectrometry on the lunar soil for the first time, in an effort to explore the sulfur in what resembled mantle-derived volcanic rock.

    “I was targeting sulfur that had a texture that would suggest it was erupted with the rock and not added through a different process,” Dottin explained.

    Sulfur-33

    The unexpected sulfur compounds found in the samples were strange for their high depletion of sulfur-33, which is among the four most radioactively stable sulfur isotopes. Compared to sulfur-33 samples recovered on Earth, the lunar samples are far different, as terrestrial sulfur-33 is typically far less depleted.

    “Before this, it was thought that the lunar mantle had the same sulfur isotope composition as Earth,” Dottin said. “That’s what I expected to see when analyzing these samples, but instead we saw values that are very different from anything we find on Earth.”

    Isotope ratios form a sort of “fingerprint” from which rocks can be identified as originating from the same source. Existing research has shown similarities between oxygen on the Moon and Earth, leaving scientists to expect a resemblance between sulfur isotopes as well. 

    “My first thought was, ‘Holy shmolies, that can’t be right,’” Dottin exclaimed. “So we went back to make sure we had done everything properly, and we had. These are just very surprising results.”

    Exploring Lunar Origins

    Dottin suggests two possibilities behind the unexpected sulfur. One is that the early moon briefly held a thin atmosphere, just enough to allow for reactions between ultraviolet light and sulfur. This could have depleted the isotope early on, carrying significant implications for lunar evolution.

    “That would be evidence of ancient exchange of materials from the lunar surface to the mantle,” Dottin said. “On Earth, we have plate tectonics that does that, but the Moon doesn’t have plate tectonics. So this idea of some kind of exchange mechanism on the early Moon is exciting.”

    Another possibility is that the depleted isotope arrived from the Moon’s initial formation. The most commonly accepted lunar origin story is that Theia, an object roughly the size of Mars, impacted the ancient Earth, sending off debris that eventually formed the Moon. If this were the case, the anomalous sulfur isotope may be remnants of Theia, which could have had a far different sulfur signature than the Earth.

    While both theories are possible, no clear evidence from the isotopes themselves currently supports one over the other. Dottin hopes that continued analysis of sulfur isotopes from different bodies in our solar system, such as Mars, will help identify the correct explanation and provide a better understanding of how our solar system formed as a whole.

    The paper, “Endogenous, yet Exotic, Sulfur in the Lunar Mantle,” appeared in JGR Planets on September 10, 2025.

    • 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.

    https://thedebrief.org/category/space/ }

    08-10-2025 om 21:19 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Water on interstellar comet 3I/ATLAS glows in ultraviolet light

    Water on interstellar comet 3I/ATLAS glows in ultraviolet light

    Scientists observed the interstellar comet 3I/ATLAS using the Swift ultraviolet space telescope. With the help of this instrument, they found hydroxyl ions, indicating the presence of water on the comet. This allows us to compare it to the “cosmic icebergs” that are constantly present in our Solar System.

    Comet 3I/ATLAS.
    Source: starwalk.space

    Water on comet 3I/ATLAS

    Scientists have published a study of the interstellar comet 3I/ATLAS using NASA’s Swift space telescope. This orbital observatory operates in ultraviolet light and is capable of performing spectral analysis for this wavelength range. As a result, scientists learned something interesting about its chemical composition.

    In particular, water was found on it. More precisely, the telescope captured ultraviolet light from the hydroxyl ion OH, but it cannot be anything other than the decay product of a water molecule. Thus, a safe assumption is that it is present there.

    But the really important thing was that this discovery was made when 3I/ATLAS was three times farther from the Sun than Earth. At this distance, comets in the Solar System do not show any activity. But for some reason, up to 40 kg of water evaporated from the interstellar space every second.

    Origin of comets

    Nevertheless, scientists believe that ultraviolet research has enabled them to compare 3I/ATLAS with comets in the Solar System. Its abnormal activity can be easily explained by the existence of complex layers of ice on the surface of its core. Similar ones were observed in several objects that formed far from the Sun.

    3I/ATLAS is only the third interstellar object that scientists have been able to study in detail. And they are all completely different. Oumuamua was completely dry, while Borisov’s comet was rich in carbon monoxide. And now 3I/ATLAS shows a large amount of water.

    All this indicates their formation under different conditions. This means that the systems from which they originate have to be really different from each other. Although this conclusion is based on a small sample size, future interstellar visitors will be able to provide more information.

    RELATED VIDEOS


    https://universemagazine.com/en/news-en/science-en/ }

    08-10-2025 om 21:02 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Scientists cast doubt on the reasons for the anomalous behavior of the asteroid Dimorphos

    Scientists cast doubt on the reasons for the anomalous behavior of the asteroid Dimorphos

    A new study has refuted the popular theory about the unexpected shortening of Dimorphos’ orbital period. Scientists have discovered that the proposed mechanism would actually have the opposite effect. 

    Asteroid Dimorphos.
    Source: NASA/Johns Hopkins APL

    In 2022, NASA’s Double Asteroid Redirection Test (DART) vehicle deliberately collided with Dimorphos, a small satellite of the near-Earth asteroid Didymos. The mission was dedicated to protecting our planet. Scientists wanted to test whether the space ram technique could be used to change the orbit of a celestial body threatening Earth.

    The demonstration was quite impressive. The period of Dimorphos’s orbit around Didymos after the impact was reduced by as much as 33 minutes, which far exceeded the scientists’ expectations. However, in the following weeks, something unusual happened: observations revealed an additional reduction in the orbital period of another 30 seconds. This situation has left researchers perplexed as to its causes.

    The initial hypothesis suggested a scenario known as binary system hardening. It involves debris ejected as a result of the collision interacting with Dimorphos’ gravity and ultimately being ejected from the system, causing it to lose angular momentum and acquire a tighter orbit. 

    Illustration of debris ejected after the collision of the DART spacecraft with the asteroid Dimorphos.
    Source: ESO

    However, the results of a recent study conducted by scientists from Université Côte d’Azur have cast doubt on this scenario. Simulation showed that Dimorphos was too weak a “scatterer” to affect the angular momentum of the system. 

    If the ejected particles do not disperse, the most likely consequence will be re-accretion, in which the debris falls back onto one of the components of the binary system. Since the collision between DART and Dimorphos was head-on, most of the ejected material entered prograde orbits. This means that they are moving in the same direction as Dimorphos and Didymos in their mutual motion around the Sun. In turn, when material moving in the prograde direction re-accretes, it increases the angular momentum of the binary system. This leads not to a decrease, but to an increase in the orbital period, which contradicts the observed pattern.

    All this suggests the existence of an additional mechanism that can counteract this effect and cause the observed decrease in the orbital period. Researchers suggested that the most likely alternative explanation is a change in the shape of Dimorphos after the impact. At the same time, they admitted that further research would be needed to reach a final conclusion.

    Perhaps the European Hera mission will provide the answer to this question. It will reach Didymos and Dimorphos at the end of 2026.

    https://universemagazine.com/en/news-en/science-en/ }

    08-10-2025 om 20:52 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Space agency breaks silence on 'foreign' interstellar object soaring past Mars: 'A rare visitor'

    Space agency breaks silence on 'foreign' interstellar object soaring past Mars: 'A rare visitor'

    The European Space Agency (ESA) has finally shared new details about the mysterious interstellar visitor days after its closest approach to Mars.

    The object, dubbed 3I/ATLAS, came within 18.6 million miles of the Red Planet on October 3, and while NASA quickly uploaded images captured by its Perseverance rover on the Martian surface, ESA had remained quiet until now. 

    The ESA's ExoMars Trace Gas Orbiter (TGO) captured images of the object, appearing as a tiny, blurry white dot in a series of images.

    The object's icy nucleus and its surrounding halo of gas and dust, called a coma, could not be distinguished separately, but the faint glow was clearly visible against the blackness of space. 

    Scientists were initially unsure whether either orbiter's cameras would detect the comet at all. Both are designed to photograph Mars' bright, rocky surface from just a few hundred to a few thousand miles away, not to capture a dim object tens of millions of miles distant.

    'This was a very challenging observation for the instrument,' said Nick Thomas, principal investigator of the CaSSIS camera. 

    'The comet is around 10,000 to 100,000 times fainter than our usual targets.'

    The visible coma suggested that 3I/ATLAS is beginning to heat up as sunlight reaches its surface, causing ice to vaporize and release dust, which gives comets their ghostly appearance. 

    The European Space Agency finally released images 3I/ATLAS, captured by a Mars orbiter

    The European Space Agency finally released images 3I/ATLAS, captured by a Mars orbiter 

    Originating from outside our Solar System, 3I/ATLAS is only the third interstellar comet ever seen, following 1I/ʻOumuamua in 2017 and 2I/Borisov in 2019.

    'These comets are absolutely foreign,' the ESA shared on Tuesday, referring to 3I/ATLAS as a 'rare visitor.'

    'Every planet, moon, asteroid, comet and lifeform in our Solar System shares a common origin. 

    'But interstellar comets are true outsiders, carrying clues about the formation of worlds far beyond our own.'

    ExoMars TGO captured the series of images with its Color and Stereo Surface Imaging System (CaSSIS), which was unable to distinguish the nucleus from the coma due to 3I/ATLAS being too far away.

    However, the device was able to image the coma that spanned thousands of miles across. 

    'The full size of the coma could not be measured by CaSSIS because the brightness of the dust decreases quickly with distance from the nucleus,' the ESA report shared.

    'This means that the coma fades into the noise in the image.'

    3I/ATLAS made its closest approach to Mars on October 3 and is set to continue through our Solar System

    3I/ATLAS made its closest approach to Mars on October 3 and is set to continue through our Solar System

    NASA was quick to release images of the object snapped by its Perseverance rover on Mars. The agency uploaded them over the weekend

    NASA was quick to release images of the object snapped by its Perseverance rover on Mars. The agency uploaded them over the weekend 

    Typically, material from the coma is swept into a long tail that can stretch for millions of miles as the comet moves closer to the sun. 

    'The tail is much dimmer than the coma. We can’t see the tail in the CaSSIS images, but it may become more visible in future observations as the comet continues to heat up and release more ice,' shared the ESA. 

    The images have flooded X, where one user posted: 'ESA Finally Releases Images of 3I/ATLAS. After days of silence, ESA finally broke the blackout.'

    The ESA's report comes days after NASA released its view of the visitor.

    Harvard astrophysicist Avi Loeb, who has been convinced that the object could be an alien craft or probe, analyzed the Perseverance rover's photos by calculating its distance, speed, and camera settings.

    According to his initial study, Loeb was not convinced 3I/ATLAS is actually a massive cylindrical object, noting that the strange shape might have been a trick of the rover's camera stretching out its shape.

    He explained that the apparent cylinder from the rover's 'Navcam' was likely caused by the camera stacking hundreds of images of 3I/ATLAS over a period of about 10 minutes, making it look more like a log than a ball.

    The professor added that 3I/ATLAS is likely smaller and rounder, but still massive, with a potential diameter of more than 28 miles across.

    Dr Horace Drew, a retired senior researcher at Australia's Commonwealth Scientific and Industrial Research Organization (CSIRO), noted that the mysterious green glow seen in some images could be a result of the object being an interstellar spacecraft coated in nickel.

    Color-enhanced images shared by multiple social media users revealed a strange green glow around 3I/ATLAS

    Color-enhanced images shared by multiple social media users revealed a strange green glow around 3I/ATLAS

    Drew explained that humans use the same practice on Earth-made space technology on a much smaller scale.

    'It is not a 'comet,'' Drew declared on a post on X Monday morning.

    Drew disagreed with Loeb's conclusion that the cylindrical shape was a result of the Mars rover sending back a stretched image over several minutes, claiming that an amateur astronomer on Earth captured a similar shape with their telescope.

    'We can see an extended white shape, with a green coma outside. Not a small white ball,' Drew explained in a post about the astronomer's photograph.

    Drew, who earned his PhD in chemistry from the California Institute of Technology, added that previous images of the interstellar object were allegedly from a 'head-on view' and didn't capture its shape from the side, like the new photos from Mars.

    Loeb said he's excited about another image taken by a different Mars camera, called HiRISE, which has better resolution and could show 3I/ATLAS more clearly.

    That image is being sent back to Earth by the Mars Reconnaissance Orbiter (MRO) and has yet to be released by NASA.


    https://www.dailymail.co.uk/sciencetech/index.html }

    08-10-2025 om 18:27 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.'Meteor' streaks through Britain's skies overnight - leaving lucky gazers in awe

    Brits have been left in awe after spotting what is believed to be a 'meteor' glowing through the night sky. 

    Lucky stargazers in Northfields and Ealing, west London, have reported seeing a blue-ish green blob race through the city's sky on Tuesday. 

    One onlooker described seeing the 'streak' of light dash through the clouds at around 8.10pm to 8.30pm, and initially believed it was fireworks.  

    'I'm used to seeing planes coming and going to Heathrow, and also helicopters coming and going; this was not that,' they wrote on Reddit

    'My next thought was fireworks but I'm 90% sure it wasn't that, and there was no explosion.

    'For reference it was about the same size as the full-ish moon tonight, visible through the clouds, but as a much brighter blue-green color and, again, moving quite fast.

    'It was a very odd combination of speed, size and brightness and didn't look like anything I've ever seen in the sky here before.'

    Others claimed to have seen the unusual sighting from Wimbledon and Hampstead Heath, with some even catching a glimpse as far afield as Brighton and Grantham.

    Lucky stargazers in Northfields and West Ealing, west London, and further afield, have reported seeing a blue-ish green blob race through the city's sky on Tuesday night

    Lucky stargazers in Northfields and West Ealing, west London, and further afield, have reported seeing a blue-ish green blob race through the city's sky on Tuesday night

    It has not yet been confirmed what the colourful 'streak' in Tuesday's sky was, however, the Daily Mail has approached the Met Office for comment. 

    It comes as earlier this week Jessica Lee, an astronomer at the Royal Observatory Greenwich also said sky gazers could expect the Draconid meteor shower today. 

    But, the meteor shower, which is expected to peak Wednesday night may be difficult to see due to the moonlight, Ms Lee warned. 

    'The Draconids meteor shower is named after the constellation of Draco the dragon,' Ms Lee said.

    'This is because, although meteors appear all over the sky, they all appear to emerge or radiate from a single point that lies within this constellation.

    'The meteor shower is visible from the 6th until the 10th of October this year.

    'The best time will be from around 8pm on the 8th of October.

    'At this time, that radiant point within Draco will be in the north-west of the sky, slowly getting lower in the sky until sunrise.

    'The moon will be almost full on this night, however, so it could make the meteors tricky to see.'

    The Draconids are caused when debris from the comet 21P/Giacobini-Zinner burns up in the Earth's atmosphere, Ms Lee added.

    article image

    'Most of this debris will burn up at a height of around 80km above the ground, so this is not a dangerous event,' she said.

    'For the best chances to spot them, find a dark area of clear sky and allow around 20 minutes to let your eyes adapt to the dark.

    'It may also be advisable to lie down as you may be looking up for a long time.'

    In September, walkers were urged to keep an eye out for meteorite fragments scattered over Scotland after a shooting star was spotted in the early hours of July 3. 

    The meteor is believed to have exploded over northern Scotland, with the 'fall zone' straddling Loch Treig in Lochaber, Highland. 

    The aerial event was captured on some cameras and shared on social media, showing a big yellow spark soaring through the dark sky.

    Members of the public have since been tasked to look for the fragments, which should appear 'black, glassy and shiny'.

    Meteorites – rocks from outer space and have fallen to the surface of a planet – may have delivered essential compounds facilitating the evolution of life as we know it.

    Professor Luke Daly, a planetary geoscientist and space rock hunter at the University of Glasgow, called them 'time capsules of the early solar system'.

    'They hold a wealth of information about how our solar system formed and developed,' he said.

    'This is a very exciting opportunity to learn more about where this rock came from and where it has been and fill in a bit more of the jigsaw of our solar system's history.' 

    RELATED

    https://www.dailymail.co.uk/sciencetech/index.html }

    08-10-2025 om 18:14 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    07-10-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Sneaky asteroid zooms past Antarctica closer than a satellite — and astronomers didn't catch it until hours after

    Sneaky asteroid zooms past Antarctica closer than a satellite — and astronomers didn't catch it until hours after

    A grainy black-and-white image with a black dot in red crosshairs in the center

    The near-Earth asteroid 2025 TF (red crosshairs) came about as close to Earth as the International Space Station on Wednesday (Oct. 1), evading detection until hours later. 
    (Image credit: ESA / Las Cumbres Observatory)

    A small asteroid zoomed past Earth closer than most satellites last week — and astronomers didn't notice it until hours later.

    Measuring an estimated 3.3 to 9.8 feet wide (1 to 3 meters), the asteroid posed no serious threat to Earth, ESA added, and likely would have burned up as a bright fireball had it reached Earth's atmosphere. However, even small asteroids can cause big problems for spacecraft — and this one happened to whip by at around the same altitude where the International Space Station usually orbits. Fortunately, no spacecraft were in the space rock's path.

    Space agencies like NASA and ESA track thousands of known near-Earth objects, carefully monitoring which ones pose the greatest risk of colliding with Earth. (Currently, no known objects pose a significant threat to our planet for at least 100 years). For an asteroid to be considered "potentially hazardous," it must measure at least 460 feet (140 m) in diameter, and follow an orbit that comes within 4.65 million miles (7.48 million km) of Earth — or roughly 20 times the average distance between Earth and the moon. Asteroid 2025 TF falls far short of that size threshold, which may also explain why it evaded detection until after it had passed.


    25 Most Terrifying Things in Space You Never Knew – Everything You Missed | Astronomy Facts

    Astronomers at ESA's Planetary Defence Office observed the asteroid shortly after it was discovered, ESA officials reported. NASA, which has paused all public communications during the ongoing U.S. government shutdown, did not make any announcements about the asteroid — however, an entry for the asteroid has been updated on NASA's Center for Near-Earth Object Studies website. The tiny space rock is not expected to fly by our planet again until April of 2087, according to NASA.

    Earth may have dodged a "fireball" with this near-miss asteroid encounter, but skywatchers can expect more fiery lights this week. The Draconid meteor shower peaks on Wednesday (Oct. 8) — and while the display of shooting stars will be somewhat dampened by the light of the full Harvest Moon, the appearance of bright fireball meteors is possible. No asteroids play a part in this annual sky show; the Draconids come from icy debris left by the comet 21P/Giacobini-Zinner, which blazes through the inner solar system every 6.5 years.

    https://www.livescience.com/space }

    07-10-2025 om 20:14 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.That was close! Huge asteroid comes within 300 miles of hitting Earth – and NASA only noticed AFTER the close encounter

    That was close! Huge asteroid comes within 300 miles of hitting Earth – and NASA only noticed AFTER the close encounter

    A huge asteroid came within 300 miles of hitting Earth, and scientists only noticed after it had already skimmed past the planet.

    The 9.8-foot (three metre) space rock, dubbed 2025 TF, flew over Antarctica in the early hours of October 1.

    Passing at an altitude of just 265 miles (428 kilometres), the rock came closer to the Earth's surface than the orbit of the International Space Station.

    However, space agencies only realised the near-miss had occurred when the asteroid was detected by the Catalina Sky Survey a few hours later.

    While a miss this close might sound alarming, the European Space Agency (ESA) claims there was never any serious danger.

    Based on its estimated size, 2025 TF would have most likely burned up or exploded in the atmosphere rather than slamming into the surface.

    ESA said in a statement: 'Objects of this size pose no significant danger.

    'They can produce fireballs if they strike Earth’s atmosphere, and may result in the discovery of small meteorites on the ground.'

    A huge asteroid passed within 300 miles of Earth, but astronomers only realised the close encounter had happened when telescopes picked up the asteroid hours later. Pictured: Image of the asteroid taken by the Las Cumbres Observatory

    A huge asteroid passed within 300 miles of Earth, but astronomers only realised the close encounter had happened when telescopes picked up the asteroid hours later. Pictured: Image of the asteroid taken by the Las Cumbres Observatory

    After the asteroid passed, astronomers at the ESA's Planetary Defence Office observed it using the Las Cumbres Observatory in Australia.

    This allowed for a more accurate estimate of the object's size and worked out that it had reached its closest point to Earth at exactly 01:47:26 BST.

    ESA says: 'Tracking down a metre-scale object in the vast darkness of space at a time when its location is still uncertain is an impressive feat.

    'This observation helped astronomers determine the close approach distance and time given above to such high precision.'

    While it might not have done much damage to the planet, even a small space rock could have caused serious damage to a spacecraft.

    This is particularly concerning since 2025 TF passed within the orbit of the ISS.

    However, there were thankfully no spacecraft or satellites in the way as this asteroid passed.

    Although NASA has paused all public communication during the government shutdown, the space agency has created an entry for 2025 TF on its Center for Near-Earth Object Studies website.

    The asteroid, dubbed 2025 TF, passed 265 miles (428 kilometres) above Antarctica in the early hours of October 1. This put it at roughly the same altitude as the International Space Station (stock image)

    The asteroid, dubbed 2025 TF, passed 265 miles (428 kilometres) above Antarctica in the early hours of October 1. This put it at roughly the same altitude as the International Space Station (stock image) 

    How many Near Earth Asteroids have been detected?

    Total: 39,585

    Over 140 metres: 11,453

    Over 1 kilometre: 877 

    Figures as of October 4, 2025 

    According to this entry, the asteroid will next return to Earth in 2087 when it will pass within 3,710,795 miles (5,971,946 km) of the planet.

    However, to be classed as a 'potentially hazardous' asteroid, a space rock must have a diameter of at least 460 feet (140 metres) and follow an orbit that will take it within 4.65 million miles (7.48 million km) of Earth.

    Although 2025 TF's orbit takes it well within this distance, it is simply too small to be considered a hazard.

    This small size also makes it extremely difficult to spot, which likely explains why it wasn't noticed until it had already passed Earth.

    Each year, space agencies around the world discover thousands of so-called near-earth asteroids (NEAs).

    These range from relatively harmless space rocks like 2025 TF to enormous 'city-killers' like the asteroid 99942 Apophis.

    As of October 4, there were 39,585 known NEAs, including 11,453 asteroids larger than 460 feet (140 metres) in diameter.

    Of these, about 2,500 are considered potentially hazardous, according to the International Astronomical Union's (IAU) Minor Planet Center.

    2025 TF measures up to 9.8 feet (three metres) in diameter. Even though its orbit (illustrated) took it close to Earth, it is too small to be considered a potentially hazardous object

    2025 TF measures up to 9.8 feet (three metres) in diameter. Even though its orbit (illustrated) took it close to Earth, it is too small to be considered a potentially hazardous object 

    Each year, astronomers find thousands of Near Earth Asteroids (NEAs), many of which are over 460 feet (140 metres) in diameter. However, there are currently no objects that pose a risk to Earth in the next 100 years 

    These hazardous space rocks are subject to a much higher level of scrutiny, and their orbital paths are carefully calculated to see if they will hit Earth.

    But, as this near miss demonstrates, even the world's most sophisticated planetary defence systems can't capture anything.

    While scientists expect that almost all city or planet-killer asteroids will be detected long before they arrive, small but dangerous asteroids can still slip through.

    In January last year, NASA's Scout impact hazard assessment system alerted authorities to a six-foot (two metre) asteroid heading towards Berlin just 95 minutes before it impacted.

    article image

    Most famously, in 2013, residents of the Russian town of Chelyabinsk witnessed a 66-foot (20 metre) asteroid explode less than 19 miles (30 km) above the surface.

    Scientists hadn't seen the asteroid at all since it was approaching from the direction of the sun and couldn't be seen during the day.

    However, the blast released 30 times more energy than the atomic bomb dropped on Hiroshima, destroying 7,200 buildings and sending 1,500 people to the hospital.

    Since this time, planetary defence systems have greatly improved, but many scientists still think more work needs to be done to ensure similar asteroids aren't missed in the future.

    WHAT COULD WE DO TO STOP AN ASTEROID COLLIDING WITH EARTH?

    Currently, NASA would not be able to deflect an asteroid if it were heading for Earth but it could mitigate the impact and take measures that would protect lives and property.

    This would include evacuating the impact area and moving key infrastructure.

    Finding out about the orbit trajectory, size, shape, mass, composition and rotational dynamics would help experts determine the severity of a potential impact.

    However, the key to mitigating damage is to find any potential threat as early as possible.

    NASA and the European Space Agency completed a test which slammed a refrigerator-sized spacecraft into the asteroid Dimorphos.

    The test is to see whether small satellites are capable of preventing asteroids from colliding with Earth.

    The Double Asteroid Redirection Test (DART) used what is known as a kinetic impactor technique—striking the asteroid to shift its orbit.

    The impact could change the speed of a threatening asteroid by a small fraction of its total velocity, but by doing so well before the predicted impact, this small nudge will add up over time to a big shift of the asteroid's path away from Earth.

    This was the first-ever mission to demonstrate an asteroid deflection technique for planetary defence.

    The results of the trial are expected to be confirmed by the Hera mission in December 2026.

    RELATED VIDEOS

    https://www.dailymail.co.uk/sciencetech/index.html }

    07-10-2025 om 17:51 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART


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