Kan een afbeelding zijn van één of meer mensen en monument

Kan een afbeelding zijn van drank

Health, happiness, and hope

in the New Year.

Carl Sagan Space GIF by Feliks Tomasz Konczakowski

X Files Ufo GIF by SeeRoswell.com

1990: Petit-Rechain, Belgium triangle UFO photograph - Think AboutIts

Ufo Pentagon GIF

ufo abduction GIF by Ski Mask The Slump God

Flying Sci-Fi GIF by Feliks Tomasz Konczakowski

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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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    Rondvraag / Poll
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    In 2011 startte ik deze blog, omdat ik niet mocht stoppen met mijn UFO-onderzoek.

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    Een interessant adres?
    UFO'S of UAP'S, ASTRONOMIE, RUIMTEVAART, ARCHEOLOGIE, OUDHEIDKUNDE, SF-SNUFJES EN ANDERE ESOTERISCHE WETENSCHAPPEN - DE ALLERLAATSTE NIEUWTJES
    UFO's of UAP'S in België en de rest van de wereld
    Ontdek de Fascinerende Wereld van UFO's en UAP's: Jouw Bron voor Onthullende Informatie! Ben jij ook gefascineerd door het onbekende? Wil je meer weten over UFO's en UAP's, niet alleen in België, maar over de hele wereld? Dan ben je op de juiste plek! België: Het Kloppend Hart van UFO-onderzoek In België is BUFON (Belgisch UFO-Netwerk) dé autoriteit op het gebied van UFO-onderzoek. Voor betrouwbare en objectieve informatie over deze intrigerende fenomenen, bezoek je zeker onze Facebook-pagina en deze blog. Maar dat is nog niet alles! Ontdek ook het Belgisch UFO-meldpunt en Caelestia, twee organisaties die diepgaand onderzoek verrichten, al zijn ze soms kritisch of sceptisch. Nederland: Een Schat aan Informatie Voor onze Nederlandse buren is er de schitterende website www.ufowijzer.nl, beheerd door Paul Harmans. Deze site biedt een schat aan informatie en artikelen die je niet wilt missen! Internationaal: MUFON - De Wereldwijde Autoriteit Neem ook een kijkje bij MUFON (Mutual UFO Network Inc.), een gerenommeerde Amerikaanse UFO-vereniging met afdelingen in de VS en wereldwijd. MUFON is toegewijd aan de wetenschappelijke en analytische studie van het UFO-fenomeen, en hun maandelijkse tijdschrift, The MUFON UFO-Journal, is een must-read voor elke UFO-enthousiasteling. Bezoek hun website op www.mufon.com voor meer informatie. Samenwerking en Toekomstvisie Sinds 1 februari 2020 is Pieter niet alleen ex-president van BUFON, maar ook de voormalige nationale directeur van MUFON in Vlaanderen en Nederland. Dit creëert een sterke samenwerking met de Franse MUFON Reseau MUFON/EUROP, wat ons in staat stelt om nog meer waardevolle inzichten te delen. Let op: Nepprofielen en Nieuwe Groeperingen Pas op voor een nieuwe groepering die zich ook BUFON noemt, maar geen enkele connectie heeft met onze gevestigde organisatie. Hoewel zij de naam geregistreerd hebben, kunnen ze het rijke verleden en de expertise van onze groep niet evenaren. We wensen hen veel succes, maar we blijven de autoriteit in UFO-onderzoek! Blijf Op De Hoogte! Wil jij de laatste nieuwtjes over UFO's, ruimtevaart, archeologie, en meer? Volg ons dan en duik samen met ons in de fascinerende wereld van het onbekende! Sluit je aan bij de gemeenschap van nieuwsgierige geesten die net als jij verlangen naar antwoorden en avonturen in de sterren! Heb je vragen of wil je meer weten? Aarzel dan niet om contact met ons op te nemen! Samen ontrafelen we het mysterie van de lucht en daarbuiten.
    22-11-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.AI Cracks Galaxy Simulation

    AI Cracks Galaxy Simulation

    Image of the night sky above Paranal, Chile on 21 July 2007, taken by ESO astronomer Yuri Beletsky. The Milky Way can be seen clearly in the skies overhead
    (Credit : ESO/Y. Beletsky)

    The Milky Way contains more than 100 billion stars, each following its own evolutionary path through birth, life, and sometimes violent death. For decades, astrophysicists have dreamed of creating a complete simulation of our Galaxy, a digital twin that could test theories about how galaxies form and evolve. That dream has always crashed against an impossible computational wall.

    Until now.

    Researchers led by Keiya Hirashima at RIKEN's Center for Interdisciplinary Theoretical and Mathematical Sciences have achieved what seemed beyond reach, a simulation representing every single one of those 100 billion stars over 10,000 years of galactic time. The breakthrough came from an unexpected marriage of artificial intelligence and traditional physics simulations, presented at this year's Supercomputing Conference.

    The problem wasn't merely one of scale, though the numbers are staggering. Previous state of the art galaxy simulations could handle roughly one billion solar masses, meaning their smallest "particle" represented a cluster of about 100 stars. Individual stellar events got averaged away, lost in the noise. To capture what happens to single stars requires taking tiny time steps through the simulation, short enough to catch rapid changes like supernova explosions.

    Barred spiral galaxy known as NGC 1300 viewed nearly face-on. Its thought the Milky Way is a barred spiral like this (Credit : NASA, ESA, and The Hubble Heritage)

    Barred spiral galaxy known as NGC 1300 viewed nearly face-on. Its thought the Milky Way is a barred spiral like this

    (Credit : NASA, ESA, and The Hubble Heritage)

    But smaller time steps demand exponentially more computing power. Using conventional methods to simulate the Milky Way at individual star resolution would require 315 hours of supercomputer time for every million years of galactic evolution. Modelling even one billion years would consume 36 years of real time. Adding more processor cores doesn't solve the problem either since beyond a certain point, efficiency plummets while energy consumption skyrockets.

    Hirashima's team found their solution in a deep learning surrogate model. They trained an AI on high resolution simulations of supernovae, teaching it to predict how gas expands during the 100,000 years following an explosion. This AI shortcut handles the rapid small scale physics without dragging down the rest of the model, allowing the simulation to simultaneously track both galaxy wide dynamics and individual stellar catastrophes.

    The AI simulation has modelled all the stars in our Galaxy. The stars of the Milky Way are pictured here above a dark site with little light pollution (Credit : Steve Jurvetson)

    The AI simulation has modelled all the stars in our Galaxy. The stars of the Milky Way are pictured here above a dark site with little light pollution

    (Credit : Steve Jurvetson)

    The performance gains are remarkable. What would have taken 36 years now requires just 115 days. The team verified their results against large scale tests on RIKEN's Fugaku supercomputer and The University of Tokyo's Miyabi system, confirming the AI enhanced simulation produces accurate results at unprecedented scale.

    This approach could transform how we model any system involving vastly different scales of space and time. Climate science, weather prediction, and ocean dynamics all face similar challenges, needing to link processes that range from molecular to planetary scales.

    Source : 

    RELATED VIDEOS

    https://www.universetoday.com/ }

    22-11-2025 om 20:54 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.Ancient Underground Water Suggests Mars May Have Been Habitable Longer than Previously Thought

    Ancient Underground Water Suggests Mars May Have Been Habitable Longer than Previously Thought

    NASA's Curiosity rover on Mars. Credit: NASA/JPL-Caltech
    NASA's Curiosity rover on Mars.
    Credit: NASA/JPL-Caltech

    It is a scientific consensus that water once flowed on Mars, that it had a denser atmosphere, meaning that it was once habitable. Unfortunately, roughly 4.2 to 3.7 billion years ago, Mars' rivers, lake, and global ocean began to disappear as solar wind slowly stripped its atmosphere away. For scientists, the question of how long it remained habitable has been the subject of ongoing inquiry. Whereas some scientists maintain that Mars ceased being habitable billions of years ago, recent research suggests that it experienced periods of habitability that lasted for eons.

    This includes recent findings by NASA's Curiosity rover, which has been exploring the Gale Crater on Mars to learn more about the planet's past. According to new research by scientists at New York University Abu Dhabi (NYUAD), there is evidence that billions of years ago, ancient sand dunes within the crater gradually turned into rock by interacting with underground water. Their findings, which were published in the Journal of Geophysical Research – Planets, indicate that Mars may have been habitable much longer than expected.

    The research was led by Dimitra Atri, the Principal Investigator of NYUAD’s Center for Astrophysics and Space Science (CASS) with assistance by fellow CASS researcher Vignesh Krishnamoorthy. They were joined by Research Instrumentation Scientist James Weston of NYUAD's Core Technology Platforms, Postdoctoral Associate Marieh B. Al-Handawi of NYUAD's Smart Materials Lab, and Professor Panče Naumov of NYUAD's Center for Smart Engineering Materials, the Research Center for Environment and Materials, and NYU's Molecular Design Institute.

    Mastcam mosaic of the Stimson Formation, which formed through interaction with underground water. Credit: MSL/NASA/JPL-Caltech

    *Mastcam mosaic of the Stimson Formation, which formed through interaction with underground water.

    Credit: MSL/NASA/JPL-Caltech*

    For their study, the team examined dunes in the Stimson Formation (SF), a system of wind-blown (aeolian) sand and sedimentary rock in the Gale Crater. The Curiosity rover has observed evidence of these "lithified" formations (i.e. sediments that hardened into stone) at this location on several occasions. Given the pervasive dry conditions in the Gale Crater, these formations likely formed during the Noachian Period (ca. 4.1 to 3.7 billion years ago) when extensive flooding is believed to have taken place, which included rivers that flowed into the Gale Crater.

    The team accessed this data through the Mars Science Laboratory's (MSL) Curiosity Notebook, which provides access to information gathered by Curiosity's instruments. They then compared this data to field studies of rock formations in the desert environment of the United Arab Emirates (UAE), which are also known to have formed in the presence of water. They determined that the SF was the product of late-stage aqueous activity, meaning they formed from interaction with groundwater from the nearby mountain.

    They further found that this interaction left behind minerals such as gypsum, soft sulfate mineral composed of calcium sulfate dihydrate (CaSO4) that is also found in Earth's deserts. This latest research echoes similar findings presented by Krishnamoorthi and Atri last year at the Tenth International Conference on Mars, which took place from July 22nd to 25th at Caltech in Pasadena, California. In that study, they examined data collected on the Greenheugh Pediments (GP), a nearby dune formation with similarly lithified rock deposits.

    In both cases, the researchers believe that these dunes and their systems of underground water led to the creation of these curious formations, which could have significant implications in the search for past (and present) life on Mars. On Earth, sandstone deposits contain some of the oldest evidence of life on Earth, including communities of microorganisms that bind sediment and cause minerals to precipitate. Based on these terrestrial analogues, Atri and Krishnamoorthi's team believe that lithified deposits in the Gale Crater could contain the preserved remains of ancient bacteria.

    This latest research not only provides new insight into how Mars evolved and transitioned to the extremely cold and dry environment we see there today. It also suggests that these sites would be good candidates for future missions that will continue the search for life on Mars.

    Further Reading: 

    RELATED VIDEOS

    https://www.universetoday.com/ }

    22-11-2025 om 20:44 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.Where Was the Big Bang?

    Where Was the Big Bang?

    None
    None

    Let’s start out with something that we can say for certain: we live in an expanding universe. Every single day, the universe gets a little bit bigger than it was the day before. But right away, when we say something like “we live in an expanding universe” certain questions start to pop up, and they’re far and away the most common kinds of questions that I get asked. If the universe is expanding, then what is it expanding into? And what is it expanding from? Where’s the edge of the universe, and where is it’s center?

    I’m going to be honest with you. I dread this kind of question, especially when I give public talks. Not because I know what the answer is, but because I know how totally unsatisfying that answer feels. It’s like sneaking into your kid’s candy bag the night after Halloween and eating half their chocolates (don’t judge me, I know you’ve done it too): it feels good in the moment, but you instantly have regrets.

    Here's the answer: the big bang has no center, and it has no edge. That’s it. That’s the answer. No more, no less.

    And that doesn’t really feel good because it doesn’t make a lot of sense.

    It’s easy to imagine an expanding universe, and there are plenty of analogies out there to help guide our thinking. We can imagine drawing little galaxies on the surface of a balloon, and inflating that balloon to see the galaxies getting farther apart. We can imagine baking a load of bread with raisins in it (why it’s always raisins, and not chocolate chips, is an enduring mystery) and seeing how as the bread rises the raisins get farther apart.

    Yay, expanding universe! But the balloon has a center, and it has an edge. And the bread has a center, and a crust. So…where’s the center of the universe, and where is its edge?

    This is why we can’t rely on analogies too much when dealing with many concepts in fundamental physics and cosmology. In both the subatomic and cosmological realms, we’re grappling with structures and concepts and physics that is far and above what our puny human brains can imagine. That’s why we have mathematics. Mathematics is a tool that we can use to understanding the universe around us, even when we can’t envision what’s going on. That’s right kids: imagination is important, but mathematics can be even more powerful.

    Let’s start with the center. Where did the big bang start? Right here. And right there. And right over there. And in the next room over. The big bang happened everywhere, all at once. The big bang was an event that the entire universe participated in. The big bang was NOT an explosion that happened somewhere in space, it was an explosion OF space – it was when the expansion of the universe first got started. It was not a place we can point to, it was a TIME that we can point to.

    The big bang was a singular event that happened in the past of every single object in the universe. If you take any particle, any bit of energy, and trace its path backwards through time, you’ll end up at the big bang, where that particle, that bit of energy, gets all mushed together with every other particle and bit of energy in a singularity.

    Think about it. Let’s say the big bang happened over there, say, in the Andromeda galaxy. Well then, where were we, in the Milky Way, when that happened? If we traveled back in time 13 and change billion years, would we be watching the big bang unfold? But…aren’t we a part of the universe? How can we be a part of the universe but somehow outside of the event the created it?

    The big bang had to happen everywhere, because everywhere is by definition part of the universe. You can’t have a universe, especially an expanding one, without a big bang. So no matter where you are, your point in space had, at one time, to participate in the big bang.

    Now what about the other side of the coin? If the universe is expanding, what is it expanding into? Where’s the crust in our expanding loaf of bread, and what’s the oven that we’re sitting in?

    Go ahead, have another piece of chocolate, because this is going to get weird. There is no edge. The universe has no edge. I don’t even want to say something like “the universe isn’t expanding into anything” because that still conjures up the wrong mental image. It’s too tempting to imagine a wall, or boundary, with galaxies and stuff on one side and nothingness on the other, with the universe expanding to fill up that nothingness with somethingness.

    But that’s wrong. Even the vacuum of space is something. There are still point, locations, and existence. There’s no “outside” to the universe because “outside” implies existence, even an empty one. But the universe is, by definition, all there is. There is nothing to physical reality except the universe. Walls separate one region from another, but the universe is all the regions simultaneously.

    If there were an edge, you could imagine working hard enough to get outside that edge. But that’s not possible. There is no outside. There is no…side. There just is, us, the universe. All there is.

    Like I said, it feels a little thrilling at first, but then the stomach aches kick in.

    RELATED VIDEOS

    https://www.universetoday.com/ }

    22-11-2025 om 20:36 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 12th Anomaly of 3I/ATLAS: Orientation of the Jets is Not Smeared by Rotation

    Avi Loeb Avi Loeb

    Stacked images of 3I/ATLAS on November 8, 2025. The sunward direction (opposite to the arrow) is pointing towards the bottom left corner. (Credit: M. Jäger, G. Rhemann, E. Prosperi)
    Press enter or click to view image in full size

    A stacked deep image of 3I/ATLAS, taken on November 9, 2025, through a combination of 5 exposures, each lasting 3 minutes, with two telescopes. The sunward direction is towards the lower left corner.
    (Credit: Frank Niebling and Michael Buechner, posted here)

    Back in July and August of 2025, the interstellar object 3I/ATLAS was inferred to rotate with a period of 16.16 (+/-0.01) hours (as derived here).

    Last week, preliminary images revealed a network of jets around 3I/ATLAS (as discussed here and here). These observed jets from 3I/ATLAS should have been smeared by the rotation. Instead, the image taken by F. Niebling and M. Buechner on November 9, 2025, shows tightly-collimated jets extending to distances larger than a million kilometers. At the expected thermal speed of sublimated volatiles from a natural comet,  400 meters per second, it takes about a month for the material to traverse a million kilometers.

    How could these jets maintain their orientation if 3I/ATLAS is rotating every 16.16 hours?

    The possibility that outflows slowed down the rotation since July is unlikely because asymmetries in outgassing typically enhance rotation (as discussed here). There is no recent measurement of the rotation period of 3I/ATLAS, but we expect related data in the coming weeks.

    Another possibility is that illumination by the Sun induces outgassing only at specific angles relative to the Sun, which are dictated by the orientation of the pockets of ice and the surface topography of the nucleus. For example, ice pockets in deep valleys surrounded by mountains that shadow them will be exposed to direct sunlight and sublimate only when the Sun is at the right angle. This would lead to pulsating outflows from that spot with a period of 16.16 hours, resulting in a jet which looks like peas in a pod separated by a spatial scale of 400 meters per second times 16.16 hours which is 23,270 kilometers. There should be 43 peas on a pod of a million kilometers length and these puffs of gas should all be in the general direction of the Sun as the ice quickly cools when it is not illuminated by sunlight. This sunward orientation effect could not account for jets pointing away from the Sun, as evident in the image of 3I/ATLAS taken by M. Jäger, G. Rhemann and E. Prosperi on November 8, 2025.

    Alternatively, the apparent features might represent the evaporated trail of fragments that were ejected from the main nucleus. This would imply that the nucleus exploded near the Sun, in contrast to the single object inference from the image obtained by D. Jewitt and J. Luu on November 11, 2025.

    A more speculative possibility is that the jets maintain their directionality because they are produced by technological thrusters which preserve global orientation for navigation purposes.

    At any event, the post-perihelion images add a new anomaly to the list, which by now includes 12 mysteries concerning 3I/ATLAS:

    1. Its retrograde trajectory is aligned to within 5 degrees with the ecliptic plane of the planets around the Sun, with a likelihood of 0.2% (see here).

    2. During July and August as well as in early November of 2025, it displayed a sunward jet (anti-tail) that is not an optical illusion from geometric perspective, unlike familiar comets (see here).

    3. Its nucleus is about a million times more massive than 1I/`Oumuamua and a thousand times more massive than 2I/Borisov, while moving faster than both, altogether with a likelihood of less than 0.1% (see here and here).

    4. Its arrival time was fine-tuned to bring it within tens of millions of kilometers from Mars, Venus and Jupiter and be unobservable from Earth at perihelion, with a likelihood of 0.005% (see here).

    5. Its gas plume contains much more nickel than iron (as found in industrially-produced nickel alloys) and a nickel to cyanide ratio that is orders of magnitude larger than that of all known comets, including 2I/Borisov, with a likelihood below 1% (see here).

    6. Its gas plume contains only 4% water by mass, a primary constituent of familiar comets (see here).

    7. It shows extreme negative polarization, unprecedented for all known comets, including 2I/Borisov, with a likelihood below 1% (see here).

    8. It arrived from a direction coincident with the radio “Wow! Signal” to within 9 degrees, with a likelihood of 0.6% (see here).

    9. Near perihelion, it brightened fter than any known comet and was bluer than the Sun (see here).

    10. It exhibits sunward and anti-solar jets which require an unreasonably large surface area in order to absorb enough sunlight needed to sublimate enough ice to feed the mass flux of these jets (as calculated here).

    11. Near perihelion it exhibits non-gravitational acceleration which requires massive evaporation of at least 13% of its mass (as calculated here), whereas preliminary images indicate that the object maintained its integrity and did not break up (as discussed here).

    12. Its tightly-collimated jets maintain orientation across a million kilometers in multiple directions relative to the Sun despite its measured rotation.

    So far, I have not updated my rank for 3I/ATLAS on the (defined here and quantified Loeb Scale  here), since we expect a flood of new data in the coming weeks. If the measured speed, composition and mass flux of the jets are consistent with sublimation of volatiles from pockets of ice on the surface of a natural comet, I will reduce my Loeb Scale rank. On the other hand, if the speed and mass flux are inconsistent with warming by sunlight of a natural comet, then I will raise the Loeb Scale rank to a higher value than 4. The rank will reach a value of 10 if there is evidence for new objects near Earth or Mars that are related to 3I/ATLAS.

    RELATED


    https://medium.com/ }

    22-11-2025 om 15:27 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Is NASA hiding the truth nature of 3I/ATLAS by showing blurry images?

    Is NASA hiding the truth nature of 3I/ATLAS by showing blurry images?

    Is NASA hiding the true nature of interstellar visitor 3I/ATLAS? Low-resolution images and vague explanations are raising serious questions. 
    NASA has finally released its long-awaited images of 3I/ATLAS and for many, the results were a major disappointment. The space agency once again repeated its narrative that the object is a “normal” comet, all while presenting extremely low-grade, fuzzy images that raised more questions than answers. 

    NASA's Mars Reconnaissance Orbiter (MRO) captured an image of the comet on October 2, 2025. Later, on November 19, 2025, amateur astronomers Michael Jäger and Gerald Rhemann obtained an even deeper color filtered image from Earth. 
    The newest photos of the interstellar visitor, taken by a variety of spacecraft, satellites, and telescopes, were unveiled on November 19, 2025, during a NASA press conference,  the first since the U.S. government shutdown. NASA highlighted that eight different observatories contributed to the dataset. 
    Among the most anticipated images were those from the HiRISE camera aboard the Mars Reconnaissance Orbiter, (see image above) which had a rare vantage point only 19 million miles from 3I/ATLAS. Yet the final product shown to the public was a blurry black-and-white smudge devoid of meaningful detail. NASA insisted the object is simply a large space rock and pushed back on claims that 3I/ATLAS is performing any maneuvers or showing any behavior inconsistent with a typical comet. 
    Online, NASA’s “big reveal” was mocked as a joke. Many argued the agency was withholding clearer images and downplaying the object’s anomalies. Photos now circulating from amateur astronomers, taken with $5,000 to $10,000 telescopes, appear far sharper and more informative than anything shown by NASA, despite the agency’s billions-of-dollars worth of equipment, spacecraft, staff, and infrastructure. 
    As geophysicist Stefan Burns noted in a comparison review, the agency’s best image of 3I/ATLAS looks like a street lamp on a foggy day. 
    Meanwhile, Harvard astrophysicist Avi Loeb has identified at least 12 unexplained anomalies linked to 3I/ATLAS, further fueling speculation. NASA’s quick dismissal of all alternative interpretations only intensified online theories that the agency is trying to bury any discussion of extraterrestrial possibilities. 
    In the end, NASA’s long-delayed reveal of 3I/ATLAS left many observers unimpressed and, honestly, what else did we expect? The low-resolution images only fuel the growing sense that something about this interstellar visitor isn’t being fully explained or fully shown. In other words, it feels like NASA is once again keeping the object’s true nature out of view. 
    Anyway, we don’t need NASA for answers. By the time 3I/ATLAS makes its closest approach to Earth on December 19, 2025, there will be far more reliable sources ready to confirm whether it’s just a bizarre interstellar comet or something of extraterrestrial origin on a true renaissance mission.
      

    http://ufosightingshotspot.blogspot.com/ }

    22-11-2025 om 14:55 geschreven door peter  

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    21-11-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Polenverschuiving: Wat zegt de wetenschap en wat is de invloed op de samenleving?

    Polenverschuiving: Wat zegt de wetenschap en wat is de invloed op de samenleving?

    JP: Pole Shift

    Inleiding

    De afgelopen weken is er opnieuw een golf van online discussies ontstaan over een vermeende “pole shift”. Deze term wordt in diverse contexten gebruikt, variërend van een natuurverschijnsel dat in de geologische geschiedenis voorkomt tot spectulatieve theorieën over snelle en catastrofale verschuivingen van de aardrotatie. In sommige online kringen richt men zich op het idee dat de Noord- en Zuidpool op korte termijn zullen veranderen, wat zou kunnen leiden tot enorme natuurrampen en maatschappelijke chaos. Aan de andere kant worden berichten vaak versterkt door angstzaaiende verhalen die niet wetenschappelijk onderbouwd zijn. Het is daarom belangrijk om deze claims kritisch en wetenschappelijk te analyseren. In dit artikel bespreken we de wetenschappelijke feiten rond pole shifts, de historische context, de verbanden met bepaalde alternatieve theorieën en de maatschappelijke impact.

    Wetenschappelijke context: Wat zegt de geofysica?

    Magnetische poolomkeringen

    Een veel besproken verschijnsel in de geofysica is de zogenaamde magnetische pole reversal, of te wel het omkeren van het aardmagnetisch veld. Dit natuurlijke proces vindt plaats over zeer lange tijdschalen, meestal elke enkele honderdduizenden tot miljoenen jaren. Tijdens een reversie ontrafeld het aardmagnetisch veld niet plotseling, maar verloopt het langzaam en geleidelijk. Wetenschappers hebben dat bijvoorbeeld kunnen vaststellen aan de hand van ijsboringen, gesteenten en fossielen die aanwijzingen bevatten over het magnetisch veld van de aarde in het verleden.

    De meest recente reversie, de Brunhes-Matuyama overgang, vond ongeveer 780.000 jaar geleden plaats. Tijdens zo’n reversie kunnen de magnetische noord- en zuidpolen even wegvallen of verwisselen, maar het aardmagnetisch veld wordt nooit compleet uitgeschakeld of plotseling omgekeerd in een korte periode. Volgens Dr. Lena Ortiz, professoraal geofysica aan de Universiteit van Melbourne, “wordt het veld zwakker en kan het wanordelijk worden voor enkele duizenden jaren, maar het proces verloopt vooral geleidelijk. Er is geen bewijs dat er een snel, wereldwijde flip kan plaatsvinden die het dagelijks leven onmiddellijk beïnvloedt.”

    Werkelijke polaire verschuiving

    Naast de magnetische reversies bestaat er ook het fenomeen van “true polar wander” (TPW). Bij TPW verschuift de aardrotatieas relatief ten opzichte van de aardkorst en de mantel, wat zich over miljoenen jaren voltrekt. Dit verschijnsel is een natuurlijk onderdeel van de aardontwikkeling en heeft geen directe impact op kortetermijngebeurtenissen. Dit verschijnsel leidt niet tot snelle veranderingen in het klimaat of natuurrampen, maar moet begrepen worden als onderdeel van langetermijnprocessen.

    Betrouwbaarheid en waarschuwingssystemen

    Tot op heden zijn er geen aanwijzingen dat een plotselinge, snelle pole shift op korte termijn zal plaatsvinden. Geofysische instellingen zoals Geoscience Australia, het European Space Agency en de US Geological Survey houden de aardmagnetische velden nauwlettend in de gaten en zullen pas waarschuwen bij concrete anomalieën. Het ontbreken van betrouwbare bewijzen betekent dat de angst voor een onmiddellijke catastrofe niet op wetenschappelijke grounds staat.

    Verbanden met UFO's en paranormale theorieën

    Historische en culturele aansluiting

    De pole-shiftmythe koppelt zich vaak aan verhalen over buitenaardse wezens en geheime regeringsprojecten. In dat kader wordt gesuggereerd dat bepaalde overheden of aliens kennis zouden hebben van een naderend wereldomvattend verschuivingsproces dat niet aan het zicht van het publiek wordt onttrokken. Proponenten beweren dat zo’n event grote evacuaties zou uitlokken of dat geheime technologieën zouden onthuld worden.

    Waarom ontstaan deze theorieën?

    Deze verhalen zijn vooral populair omdat ze inspelen op de menselijke behoefte aanbetrouwbare verklaringen voor grote onzekerheden en onbegrijpelijke natuurrampen. Daarnaast spelen geheime overheidsprojecten, complottheorieën en het fenomeen van de ‘angst voor de onbekende’ een grote rol. In de context van UFO's en paranormale theorieën wordt de pole shift vaak gekoppeld aan ideeën over ‘extraterrestriële interventie’ of het bestaan van geheime bases waar zich technologieën bevinden die ons kunnen beschermen of juist doen falen. Deze verhalen worden versterkt door populaire media, films en fictie, waardoor ze aantrekkelijk zijn voor een breed publiek dat op zoek is naar antwoorden op onbekende fenomenen.

    Wetenschappelijk gezien ontbreken echter bewijs en solide gegevens om deze theorieën te ondersteunen. Er is geen concreet bewijs dat buitenaardse wezens betrokken zijn bij de aardmagnetische eigenschappen van onze planeet, noch dat geheime regeringsprojecten werkzaam zijn die een wereldwijde pole shift zouden kunnen triggeren. Het koppelen van dergelijke verhalen aan “pole shifts” dient vooral om angst en verwarring te zaaien, maar mist een wetenschappelijke onderbouwing.

    Poolverschuiving

    Door de mens veroorzaakte klimaatveranderingen zullen de geografische polen van de aarde significant verplaatsen.

    © Shutterstock

    Maatschappelijke impact en maatschappelijke reacties

    De angst voor een pole shift of soortgelijke catastrofes kan grote maatschappelijke gevolgen hebben. In het verleden zagen we dat dergelijke angsten leidde tot de opkomst van ‘doomsday-bewegingen’ en groepen die geloven dat de wereld op korte termijn ondergaat. Dit kan leiden tot onrust, paniek en zelfs gedragsveranderingen, zoals het verzamelen van voedselvoorraden, het bouwen van bunkers of het verspreiden van desinformatie via sociale media.

    Zaken als massahysterie en paniekreacties zijn niet nieuw. Anno 2024 is de digitale samenleving bijzonder gevoelig voor dergelijke berichten, waardoor desinformatie snel verspreid wordt en difficult te corrigeren is. Overheden en wetenschappers proberen vaak via officiële kanalen duidelijkheid te scheppen en feiten te communiceren, maar de virale aard van de media maakt het moeilijk om achterhaalde theorieën terug te dringen.

    Daarnaast kunnen deze angsten ook leiden tot sociale vervreemding en wantrouwen jegens wetenschappelijke instellingen en overheden. Er ontstaat een ‘alternatieve waarheid’ waarin feit en fictie door elkaar lopen, wat de maatschappelijke cohesie onder druk zet. Het is daarom belangrijk dat er kritische mediawijsheid wordt bevorderd en dat er transparantie is over de wetenschappelijke stand van zaken.

    lavatunels

    Het aardmagneetveld in kaart gebracht met satelliet data, ESA SWAM missie. De kleuren geven de sterkte van het veld aan, waarbij rood het sterkst en blauw het zwakst.

    Historische context: Hoe vaak en hoe lang duren pole shifts?

    Een groot misverstand is dat mensen denken dat pole shifts frequent en abrupt plaatsvinden. In de geschiedenis van de aarde zijn er wel degelijk veranderingen geweest in de positie van magnetische polen, maar dit gebeuren gebeurt over gigantische tijdsintervallen. De geologische gegevens wijzen uit dat reversies in het magnetisch veld duizenden tot honderdduizenden jaren duren, en dat er geen bewijs is voor een snelle of onmiddellijke omkering.

    De meest recente magnetische reversie, Brunhes-Matuyama genoemd, vond ongeveer 780.000 jaar geleden plaats. Tijdens dat proces viel het magnetische veld tijdelijk uit, voordat het weer terugkeerde in de tegengestelde richting. Voor de mensen van toen was het ongemakkelijk, maar er was geen sprake van natuurrampen of wereldwijde chaos.

    Het idee van een snelle pole shift is vooral populair in populaire cultuur en complottheorieën, maar de wetenschap wijst duidelijk uit dat zulke gebeurtenissen niet op korte termijn plaatsvinden. Wat wel mogelijk is, en dat onderzoek bevestigt, is dat het aardmagnetisch veld in de loop van miljoenen jaren kan veranderen en dat dit inderdaad gevolgen kan hebben voor bijvoorbeeld communicatie- en navigatiesystemen.

    Kansen en risico’s van natuurrijke fenomenen

    Hoewel de meeste wetenschappers elimineren dat een snelle pole shift zich op korte termijn zal voordoen, is het belangrijk om te realiseren dat de aarde wel degelijk onderhevig is aan natuurlijke fenomenen die het functioneren van onze planeet beïnvloeden. Zo hebben we te maken met perioden van vulkanische activiteit, aardbevingen en klimaatveranderingen. Al deze factoren kunnen, indien ze zich op grote schaal voordoen, invloed hebben op de samenleving en het ecosysteem.

    De klimaatverandering bijvoorbeeld, die intense weersomstandigheden en zeespiegelstijgingen veroorzaakt, heeft nu al ingrijpende effecten op menselijke samenlevingen wereldwijd. Het is essentieel dat we deze risico’s serieus nemen en ons aanpassen aan de veranderende omstandigheden. Dit betekent investeren in preventie, duurzaamheid en het versterken van onze infrastructuur.

    Daarnaast is het van belang dat we leren omgaan met onzekerheden. Dat kan door het ontwikkelen van waarschuwings- en monitoringsystemen, zoals het Europees Samenwerkingsprogramma voor aardbevingswaarneming en de NASA Magnetische Velden Tracker. Deze systemen kunnen echter geen voorspellingen doen over langetermijngebeurtenissen zoals pole shifts, maar kunnen wel helpen bij het anticiperen op andere natuurfenomenen waaraan we wel risico’s lopen.

    Artistieke impressie van het magnetisch veld rond de noordpool en zuidpool van de aarde

    De rol van media en wetenschap in het bestrijden van paniek

    De media spelen een cruciale rol in de manier waarop informatie wordt gedeeld en geconsumeerd door het grote publiek. Bij onderwerpen die gevoelig liggen, zoals de vermeende pole shift, is het belangrijk dat journalisten hun verantwoordelijkheid nemen door feitelijke, wetenschappelijk onderbouwde informatie te presenteren. Te snelle of sensationele berichtgeving kan leiden tot onnodige paniek en verwarring.

    Wetenschappers en overheidsinstellingen moeten proactief communiceren over de feiten en duidelijk aangeven wat de beperkingen van onze kennis zijn. Duidelijkheid en transparantie helpen om vertrouwen te behouden en het juiste begrip te stimuleren. Het is tevens belangrijk dat er educatie wordt ingezet om mensen mediawijs te maken en te leren onderscheid te maken tussen wetenschappelijke feiten en fictie.

    Educatieve campagn campagnes en informatievoorziening kunnen ook een rol spelen in het voorkomen van hysterische reacties. Door jongeren en volwassenen te informeren over de natuurlijke processen van de aarde, de tijdschalen waarin veranderingen plaatsvinden en de huidige monitoringtechnologieën, worden paniek en desinformatie moeilijker te laten wortelen.


    Pole Shift Theory EXPLAINED: The Science Behind Earth’s Great Reset

    Conclusie: Wat kunnen we leren uit de wetenschap en hoe vermijden we paniek?

    De angst voor een plotselinge pole shift die de wereld in korte tijd verandert, wordt door de wetenschap volledig ontkracht. Het bestuderen van aardmagnetische reversies en andere geologische processen tonen aan dat dergelijke veranderingen zeer langzaam en over lange tijdschalen plaatsvinden. Geologen, geofysici en klimaatwetenschappers werken sinds decennia aan het monitoren van de planeet, en er is geen wetenschappelijk bewijs voor een snelle of catastrofale pole shift op korte termijn.

    Het is belangrijk dat we kritisch blijven nadenken over de informatie die we ontvangen en dat we vertrouwen op wetenschappelijke bronnen. Complotdenken en sensationele verhalen zorgen voor angst en verwarring, terwijl de realiteit anders is: onze aarde is dynamisch, maar haar veranderingen verlopen geleidelijk en voorspelbaar. De beste manier om onze samenleving te beschermen, is investeren in kennis, infrastructuur en preventie, en de communicatie over natuurlijke risico’s te baseren op feiten.

    Tot slot moeten we begrijpen dat angst vooral ontstaat bij onwetendheid en onzekerheid. Door education, transparantie en het delen van wetenschappelijke inzichten kunnen we die angsten verminderen en een samenleving creëren die beter voorbereid is op de uitdagingen die de toekomst biedt. Het zich bewust zijn van de natuurlijke processen waarvoor de aarde staat, geeft niet alleen rust, maar ook kracht om op een verantwoorde en geïnformeerde manier met de wereld om te gaan.

    Aanbevelingen en toekomstige onderzoekslijnen

    Hoewel de huidige wetenschappelijke kennis duidelijk aangeeft dat een snelle pole shift in de nabije toekomst onwaarschijnlijk is, blijft het noodzakelijk om de aarde en haar magnetische velden nauwlettend te monitoren. Nieuwe technologieën en methoden ontwikkelen zich voortdurend, waardoor we beter inzicht kunnen krijgen in de langetermijntrends en potentiële gevaren.

    Het stimuleren van internationale samenwerking is essentieel. Door gegevensdeling en gezamenlijke onderzoeksinitiatieven kunnen we een beter beeld krijgen van de wereldwijde veranderingen binnen onze planeet en onze atmosfeer. Daarnaast moet er meer geïnvesteerd worden in het verbeteren van de voorlichtingscampagnes, om desinformatie en paniek te voorkomen.

    Ook is het van belang om het bewustzijn over natuurlijke processen te vergroten. Educatieprogramma's op scholen en in de media kunnen helpen om families en gemeenschappen voor te bereiden op verschillende scenario’s, zonder daarbij angst aan te jagen. Het verkennen van andere planeten en het ontwikkelen van technologische innovatie kunnen op lange termijn ook bijdragen aan het vergroten van onze veerkracht.

    Tot slot moeten beleidsmakers en w wetenschappers samenwerken om de belangrijkste risico’s te identificeren en proactief maatregelen te nemen. Het versterken van ons maatschappelijke verdedigingssysteem tegen natuurlijke rampen en het stimuleren van duurzame ontwikkeling zijn belangrijke stappen in het voorbereiden op een onvoorspelbare en complexe wereld.

    Samenvatting

    In dit artikel hebben we besproken dat de angst voor een plotselinge, wereldwijde pole shift niet gebaseerd is op wetenschappelijke feiten. Magnetische pole reversals en andere natuurlijke processen vinden plaats over enorme tijdschalen en verlopen meestal geleidelijk. Hoewel het menselijk verstand geneigd is om snel te reageren op onbegrepen fenomenen, is het cruciaal om kritisch te blijven en te vertrouwen op wetenschappelijke inzichten. De maatschappelijke reactie op deze angsten moet vooral gericht zijn op educatie, wetenschap en transparantie. Alleen door kennis te vergroten en desinformatie tegen te gaan, kunnen we voorkomen dat angst ons gaat beheersen en een ongefundeerd gevoel van onveiligheid ontstaat. De aarde is niet immuun voor veranderingen, maar haar natuurlijke dynamiek vereist vooral dat wij voorbereid en geïnformeerd zijn, zodat we adequaat kunnen reageren op de uitdagingen die de toekomst brengt.

    { PETER2011 }

    21-11-2025 om 22:15 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Scientists put moss on the outside of the International Space Station for 9 months — then kept it growing back on Earth

    Scientists put moss on the outside of the International Space Station for 9 months — then kept it growing back on Earth

    a photo of the ISS with an inset box showing a close-up of moss
    The International Space Station's exposure facility (pictured) hosted a species of moss for 9 months. A majority of the samples survived, and then kept growing back on Earth. 
    (Image credit: NASA / Tomomichi Fujita)

    Moss spores have survived a prolonged trip to space, scientists reveal. The spores spent nine months on the outside of the International Space Station (ISS) before returning to our planet, and over 80% of the spores were still able to reproduce when they arrived back on Earth.

    The discovery improves our understanding of how plant species survive in extreme conditions, the researchers wrote in their findings, published Thursday (Nov. 20) in the journal iScience.

    Previous experiments have explored how plants might cope in space, but so far, they have focused on larger organisms such as bacteria or plant crops. Now, researchers have shown that samples of the moss Physcomitrium patens (PPatens) can not only survive but thrive in space.

    a microscope image of moss spores

    Roughly 80% of the moss spores continued germinating after returning to Earth. 
    (Image credit: Dr. Chang-hyun Maeng and Maika Kobayashi)

    First, the researchers tested three cell types of P. patens from various stages in the moss's reproductive cycle. They found that sporophytes — cell structures that encase spores — showed the greatest stress tolerance when exposed to ultraviolet (UV) light, freezing and heat.

    Sporophyte samples were then placed outside of the ISS in a special exposure facility attached to Japan’s Kibo module, where the samples lived for around nine months in 2022. After this time, the samples were returned to Earth.

    "Surprisingly, over 80% of the spores survived and many germinated normally," study lead author Tomomichi Fujita, a professor of plant biology at Hokkaido University in Japan, told Live Science in an email. From this study, Fujita and his team developed a model that suggests the moss spores could actually survive for up to 5,600 days in space, or around 15 years.

    Back on Earth, the team found that most of the conditions — including the vacuum of space, microgravity and extreme temperature fluctuations — had a limited impact on the moss spores. However, samples that were exposed to light, particularly high-energy wavelengths of UV light, fared less well. Levels of pigments used by the moss for photosynthesis, such as chlorophyll a, were significantly reduced as a result of light damage, which affected later moss growth.

    Even though some moss samples faced damage from the conditions of outer space, P. patens still fared much better than other plant species that have been previously tested under similar conditions. Fujita thinks the protective, spongy casing surrounding the spores may help defend against UV light and dehydration.

    "This protective role may have evolved early in land plant history to help mosses colonize terrestrial habitats," he said.

    While this may seem like an exercise in testing the limits of a single species, the "spores' success in space could offer a biological stepping stone for building ecosystems beyond our planet," Fujita said. In the future, he hopes to test other species and better understand how these resilient cells survive such stressful conditions.

    RELATED VIDEOS



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

    21-11-2025 om 17:39 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Tracking Mars' Ice Ages From Space

    Tracking Mars' Ice Ages From Space

    Image generated from data acquired by the ESA Mars Express’s High Resolution Stereo Camera (HRSC) on Oct. 19th, 2024. Credit: ESA/DLR/FU Berlin
    Image generated from data acquired by the ESA Mars Express’s High Resolution Stereo Camera (HRSC) on Oct. 19th, 2024.
    Credit: ESA/DLR/FU Berlin

    Human beings are pretty familiar with the concept of "ice ages." Not only is their ample physical evidence to suggest that glacial periods occurred during the Pleistocene epoch - which lasted from ca. 2.58 million to 11,700 years ago, there are even Indigenous oral traditions that speak of lake formation and dramatic climate shifts in the distant past. Far from being mere myths, these traditions are considered preserved accounts that are corroborated by scientific findings. However, the cycles of glacial and interglacial periods that characterize the Pleistocene were merely the latest in a long line of historical shifts in Earth's climate.

    According to the geological record, Earth has experienced multiple ice ages during the past 2.5 billion years, which peaked around 20,000 years ago with average temperatures being 8 °C (14.5 °F) cooler than they are today. Today, scientists are making similar finds on Mars, which also bears the marks of repeated ice ages that shaped the landscape. Like Earth, these climatic shifts were the result of long-term variations in Mars' axial tilt (obliquity), leading to fluctuating temperatures that caused ice flows to advance and retreat across the planet.

    Evidence of these flows has been captured in a new series of images taken by the High Resolution Stereo Camera on the ESA’s Mars Express orbit. The images show a prominent feature known as Coloe Fossae, system of intersecting canyons located in the Ismenius Lacus quadrangle between the Northern Lowlands and the Southern Highlands. On the floors of these canyons (and the many craters that mark the region), there are visible patterns of swirling lines that indicate where material flowed during a previous ice age.

    View generated from the digital terrain model and the nadir and colour channels of the High Resolution Stereo Camera on ESA’s Mars Express. Credit: ESA/DLR/FU Berlin

    *View generated from the digital terrain model and the nadir and colour channels of the High Resolution Stereo Camera on ESA’s Mars Express.

    Credit: ESA/DLR/FU Berlin*

    The technical term for these patterns is lineated valley fill (LVF) or concentric crater fill (CCF), which is composed of rocky material deposited by ice flows as they advanced or retreated from an area. Scientists see these patterns on Earth with glaciers, which have left behind what is known as "till" (a combination of clay, silt, sand, and gravel) that form ridges and elongated mounds. However, these features are located in a region that sits far from the ice cap in Mars' northern polar region, indicating that glaciers once covered the region.

    Similar to glacial periods on Earth, these glaciers are believed to have advanced from the Martian poles towards the mid-latitudes before retreating again during interglacial periods. Furthermore, scientists have viewed LVF and CCF features all across the mid-latitudes of Mars, suggesting that the entire planet experienced glacial activity in the past. Lastly, there's the fundamental takeaway from these and other observations, which have revealed that Mars experience multiple glacial periods as its atmosphere was slowly being stripped away, causing most of the water on its surface to disappear.

    Tracking how ice flowed across the Red Planet is key to reconstructing the geological and environmental history of Mars, from which scientists can deduce how and when it made the transition from a warmer, wetter planet to the extremely cold and dry world we see today.

    Click here to see the annotated version of the top image, and click on the circled regions to see the LVF features more closely.

    Further Reading: 

    https://www.universetoday.com/ }

    21-11-2025 om 17:12 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.NASA's long–awaited images of the mysterious object zipping through our solar system confirm 3I/ATLAS is a comet – and NOT an alien spacecraft

    NASA's long–awaited images of the mysterious object zipping through our solar system confirm 3I/ATLAS is a comet – and NOT an alien spacecraft

    NASA has shared its long–awaited images of the mysterious object zipping through our solar system – finally confirming its true identity. 

    Since it was first spotted in July, the object – dubbed 3I/ATLAS – has captivated scientists and internet users alike, even prompting Kim Kardashian to ask NASA for answers.

    Many scientists maintained it was merely a comet visiting us from a different solar system. 

    However, others – including a member of US Congress and a Harvard researcher – were convinced that the object was an alien spacecraft. 

    Now, NASA has released photos snapped by three of its Mars spacecraft as they passed just 18 million miles away from the object. 

    These pictures can finally put any speculation to rest, as they confirm the object's identity.

    And unfortunately for alien hunters, the US space agency says that 3I/ATLAS is a comet.  

    'We want very much to find signs of life in the universe... but 3I/ATLAS is a comet,' said Amit Kshatriya, a senior NASA official, at a press conference on Wednesday. 

    NASA has shared its long–awaited images of the mysterious object zipping through our solar system – finally confirming its true identity. Pictured: a photo taken on October 2 by the HiRISE camera on NASA's Mars Reconnaissance Orbiter

    NASA has shared its long–awaited images of the mysterious object zipping through our solar system – finally confirming its true identity. Pictured: a photo taken on October 2 by the HiRISE camera on NASA's Mars Reconnaissance Orbiter

    These pictures can finally put any speculation to rest, as they confirm the object's true identity as a comet. Pictured: a photo taken on October 9 by NASA's MAVEN spacecraft

    These pictures can finally put any speculation to rest, as they confirm the object's true identity as a comet. Pictured: a photo taken on October 9 by NASA's MAVEN spacecraft

    NASA's Mars spacecraft zoomed in on the comet as it passed just 18 million miles (29 million kilometers) away. 

    In the first image, snapped by HiRISE, the comet looks like a fuzzy white ball. 

    'Captured at a scale of roughly 19 miles (30 kilometers) per pixel, 3I/ATLAS looks like a pixelated white ball on the HiRISE imagery,' NASA explained. 

    'That ball is a cloud of dust and ice called the coma, which the comet shed as it continued its trajectory past Mars.'

    Further analysis of these pictures should allow NASA to estimate the size of the comet's nucleus – its central core of ice and dust. 

    NASA's MAVEN spacecraft, meanwhile, snapped the comet in two unique ways using its UV camera. 

    'First, IUVS took multiple images of the comet in several wavelengths, much like using various filters on a camera,' NASA explained. 

    'Then it snapped high–resolution UV images to identify the hydrogen coming from 3I/ATLAS.'

    Captured at a scale of roughly 19 miles (30 kilometers) per pixel, 3I/ATLAS looks like a pixelated white ball on the HiRISE imagery. That ball is a cloud of dust and ice called the coma, which the comet shed as it continued its trajectory past Mars

    Captured at a scale of roughly 19 miles (30 kilometers) per pixel, 3I/ATLAS looks like a pixelated white ball on the HiRISE imagery. That ball is a cloud of dust and ice called the coma, which the comet shed as it continued its trajectory past Mars

    Down on the surface of Mars, NASA's Perseverance rover even caught a snap of the comet, using its Mastcam-Z camera

    Down on the surface of Mars, NASA's Perseverance rover even caught a snap of the comet, using its Mastcam–Z camera

    What is 3I/ATLAS?

    Comet 3I/ATLAS is the third known object from outside our solar system to be discovered passing through our celestial neighborhood. 

    NASA reassures it 'poses no threat to Earth and will remain far away'. 

    The closest it will approach our planet is about 1.8 astronomical units (about 170 million miles).

    The comet's size and physical properties are being investigated by astronomers around the world.

    Scientists now hope to be able to study a combination of these images to identify a variety of molecules and better understand the comet's composition.

    Down on the surface of Mars, NASA's Perseverance rover even caught a snap of the comet, using its Mastcam–Z camera. 

    'The exposure had to be exceptionally long to detect such a faint object. Unlike telescopes that track objects as they move, Mastcam–Z is fixed in place during long exposures,' the space agency added. 

    NASA has also recently shared photos of the comet taken by its STEREO observatory, and its SOHO spacecraft.  

    Speaking to AFP, Thomas Puzia, an astrophysicist who led the team at the Chilean observatory that made the discovery, described the widespread discussion surrounding the comet as 'amazing'. 

    However, he said: 'It's very dangerous and to a certain degree misleading to put speculations ahead of scientific process.

    'The facts, all of them without exception, point to a normal object that is coming from the interstellar space to us.'

    He added the comet was 'very exceptional in its nature, but it's nothing that we cannot explain with physics.'

    NASA's STEREO (Solar Terrestrial Relations Observatory) spotted the comet from September 11 - to October 2The European Space Agenc  and NASA Solar and Heliospheric Observatory (SOHO) spacecraft captured a glimpse of interstellar comet 3I/ATLAS on Oct. 15–26

    NASA has also recently shared photos of the comet taken by its STEREO observatory, and its SOHO spacecraft

    article image

    The idea that the comet could have been an alien spacecraft were driven by Harvard Professor Avi Loeb – who remains unconvinced by NASA's explanation. 

    'Obviously, it could be natural,' he told AFP. 

    'But I said: we have to consider the possibility that it's technological because if it is then the implications for humanity will be huge.'

    Explained: The difference between an asteroid, meteorite and other space rocks

    An asteroid is a large chunk of rock left over from collisions or the early solar system. Most are located between Mars and Jupiter in the Main Belt.

    comet is a rock covered in ice, methane and other compounds. Their orbits take them much further out of the solar system.

    meteor is what astronomers call a flash of light in the atmosphere when debris burns up.

    This debris itself is known as a meteoroid. Most are so small they are vapourised in the atmosphere.

    If any of this meteoroid makes it to Earth, it is called a meteorite.

    Meteors, meteoroids and meteorites normally originate from asteroids and comets.

    For example, if Earth passes through the tail of a comet, much of the debris burns up in the atmosphere, forming a meteor shower.

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

    21-11-2025 om 16:48 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Why is the constellation of Scorpius so weird?

    Why is the constellation of Scorpius so weird?

    Scorpius is the most amazing of the zodiac constellations. Although astrology divides the year into 12 almost equal parts, astronomers know that in reality the Sun is only in it for 8 days. However, it also has numerous attractions.

    Constellation Scorpius

    Scorpius, who dislikes the Sun

    On November 22, the Sun will enter the constellation Scorpius. As is almost always the case in such situations, astrologers strongly disagree with astronomers, claiming that our star entered the constellation on October 23 and left it on November 21.

    The main reason for this is the shift in the vernal equinox due to the precession of the Earth’s axis of rotation. You can read more about this in this article. In fact, there is at least one more reason why astrologers disagree with astronomers about the time the sun is in different zodiac constellations, but for most of them, it is secondary.

    But not for Scorpius. We are referring to the clarification of constellation boundaries, which occurred at the beginning of the 20th century. And in the case of this constellation, they were drawn in such a way that the Sun actually crosses it only along a narrow strip through its “head” and “claws.”

    The constellation Scorpius. The blue line is the ecliptic.
    Source: Wikipedia

    As a result, of all the constellations, it is in Scorpius that the Sun actually spends the least amount of time – only 8 days. On November 29, it will leave the poisonous multi-legged celestial being and move on to its neighbor, Ophiuchus, where it will stay longer than in Scorpius, but which is not considered a zodiacal constellation.

    In general, November is the worst month for observing Scorpius. The reason for this is the same as for other zodiac constellations: it rises and sets with the Sun at this time of year and hides behind the horizon at night. The best time to observe it is in May and June, when it rises above the southern horizon.

    The mythical monster

    There are several myths about how Scorpius appeared in the sky. But in all of them, he appears as the embodiment of evil, whose actions lead to extremely bad consequences. The most common of these myths links Scorpius with Orion.

    Scorpius in May.
    Source: stellarium-web.org

    Orion was supposedly the most outstanding of human hunters, but his thirst for prey led him astray. According to one version of the myth, he began to pursue the Pleiades and chased them for seven years until the Scorpion, sent by Gaia or Poseidon, stung him, causing him to die in terrible agony.

    According to another version, Orion demanded the goddess of the hunt, Artemis, herself. But she did not reciprocate his feelings, yet he continued to pursue her until she sent a poisonous messenger to kill him. Be that as it may, Orion and Scorpius are indeed located far apart in the sky, as if the former were hiding from the latter.

    Another myth says that the celestial Scorpius is actually the one that frightened the horses pulling the golden chariot of Helios, the sun god. It was driven by his inexperienced son Phaethon, and the horses carried it too close to Earth, causing a worldwide fire. To stop this, Zeus had to kill the boy and the horses with a thunderbolt, and Phaethon fell into the river Eridanus.

    The myth of Phaethon.
    Source: globalpowerelite.com

    Antares and other bright stars

    Although the Sun is in Scorpius for only a short time, there are more interesting objects in it than scary myths about it. The most notable of these is Alpha Scorpii, known as Antares. Among all the stars that make up the zodiacal constellations, it is second only to Alpha Tauri, Aldebaran.

    At the same time, Antares is very noticeable due to its red color. Thanks to this, it got its name “anti-Ares,” meaning the enemy of Mars. In reality, it is much farther away from us than the Red Planet and incomparably larger than it.

    It is a red supergiant located 550 light-years away from us. In fact, it is a binary system. Its main component, which we can actually see, has a mass of 12.4 solar masses, but has already used up almost all of its hydrogen and swelled to a size 400 times larger than our sun. It emits 75,900 times more energy than the Sun. However, all these measurements are actually quite approximate, because the giant star pulsates, changing its radius by 19%.

    Antares compared to other stars.
    Source: www.statesman.com

    The main component of the system is orbited by its companion, which is also a fairly large star. Despite having a mass 7.2 times that of the Sun, it has not yet exhausted its thermonuclear fuel and therefore has a blue color. Its diameter is 5.2 times that of the Sun.

    There is still no consensus among scientists regarding the distance between the two components and, accordingly, their orbital period. The most accurate measurements to date indicate a distance of about 220 AU and an orbital period of approximately 1,218 years.

    In any case, the Antares system is very young. Its age ranges from 11.8 to 17.3 million years. After some time, the larger of the stars will finally exhaust its thermonuclear fuel and turn into a supernova, and then into a black hole. Then, after a few million years, the same fate will befall the second star.

    Lambda Scorpii.
    Source: www.star-facts.com

    The second brightest star in Scorpius is its Lambda, which is called Shaula, derived from the Arabic word for “raised tail.” It is indeed located on the tail of the celestial arthropod and has an apparent magnitude of 1.62.

    In fact, it is a triple system located 570 light-years away from us. The main component is a variable star of the Beta Cephei type. Explosive processes occur inside these hot and heavy blue stars, inflating their outer shells. In the case of Shaula, the mass of the main component exceeds that of the Sun by 10.4 times, and its luminosity by 36,000 times.

    Around it, at a distance of 7,500 AU, there’s a smaller blue star. It’s about twice as heavy as our Sun. And around this pair, at a distance of 17,000 AU, there’s a third star that’s eight times heavier than our Sun.

    The third brightest star in Scorpius is its Theta, Sargas. It is a double system located 329 AU away from us. What the smaller component of the system is and whether it exists at all remains unclear. But here is the main object of interest.

    It is a star of spectral class F, which means it is slightly hotter than the Sun. Its mass is about three times greater than that of our star, its polar radius is 26 times greater than that of the Sun, and its equatorial radius is 36 times greater. In other words, it is flattened, and there is only one explanation for this: it was once a pair of stars that merged.

    Theta Scorpii.
    Source: www.flickr.com

    Nearby stars

    The closest star to us in the constellation of Scorpius is Gliese 682. It is a rather dull red dwarf located 16.3 light-years away from us. Its mass is 27% and its radius is 30% of the Sun’s. In 2016, it was reported that two planets had been discovered around it, but their existence has now been disproved.

    Next is the Gliese 667 system, located 23 light-years away from us. It consists of two orange dwarfs and one red dwarf. The first two have masses of 69% and 73% of the Sun and revolve around a common center of mass in a highly elongated orbit with a semi-major axis of 12.6 AU, completing one revolution every 42 Earth years.

    And around them orbits a third star – a red dwarf with a mass of 31% of the Sun’s. And it is this object that is the most interesting in the entire system. At one time, scientists reported that Gliese 667 C had as many as six planets, but now the existence of two of them is recognized.

    Planet Gliese 667 Cc.
    Source: Wikipedia

    The first is Gliese 667 Cb. With a mass of 5.6 Earths and an orbital period of 7.2 days, it is most likely a large hot super-Earth or an equally hot mini-Neptune. This world must have a powerful hydrosphere and a dense atmosphere, the boundary between which is quite arbitrary.

    But the second planet, Gliese 667 Cc, is much more interesting. Its mass is 4.1 times that of Earth, and it orbits its star once every 28 Earth days. Calculations show that the star can heat it to 4.3 °C, which is slightly higher than on Earth. Most likely, Gliese 667 Cc is significantly warmer than our planet due to a powerful greenhouse effect. However, it may still be the case that the temperature on it is not high enough for life to exist. But there is another problem: like many red dwarfs, Gliese 667 C experiences powerful flares. Whether they rule out the possibility of life on the planet is still an open question.

    Other interesting stars

    There are plenty of other interesting objects in the constellation of Scorpius. For example, the star U Scorpii is located here. It is a repeating nova with one of the shortest periods. The flares repeat every 12 years.

    Like all similar objects, U Scorpii is a binary system consisting of a normal star and a white dwarf, which orbit each other in a very close orbit around a common center of mass. Matter flows from the first component to the second, and when a large amount accumulates on the latter, a thermonuclear explosion occurs, after which the process repeats itself.

    U Scorpii.
    Source: Wikipedia

    Another interesting object is the dawn of AH Scorpii. It is barely visible in our sky, but that is only because it is 7,400 light-years away from us. In fact, it is a red supergiant, compared to which even Antares looks small. This monster is 20 times more massive than the Sun, 1,411 times larger in diameter, and 329,000 times more luminous.

    Also in the constellation of Scorpius is the object Scorpius X-1, which is the second brightest object in the sky when viewed in the X-ray range. The first is the black hole Sagittarius A* in the center of the Milky Way. As for this mysterious source of radiation, in the visible range, there is a hot blue star in its place. Scientists believe that it forms a pair with a neutron star, onto which matter falls from it, serving as a source of energy for such a powerful emitter.

    There is also an object called a microquasar in the constellation Scorpius. Ordinary quasars are supermassive black holes at the centers of galaxies that intensively absorb matter, part of which is converted into relativistic jets emanating from their poles. This makes them visible across the entire universe.

    Microquasar.
    Source: Wikipedia

    So, something like this, only on a much smaller scale, exists right here in our galaxy. The object GRO J1655−40 is a binary system containing a stellar-mass black hole. The second component is a normal star, and it is its material that is used to form a microquasar with jets shooting out from the poles of the black hole.

    Globular clusters and galaxies

    In addition to all of the above, the constellation of Scorpius is rich in objects that are neither stars nor black holes. First and foremost are the Butterfly Cluster, or Messier 6, and Ptolemy’s Cluster, or Messier 7. Both belong to open clusters. The first contains about 120 stars and is located at a distance of 1,590 light-years, while the second contains about 80 stars. The distance to it is 735 light-years.

    There are also two noticeable globular clusters in Scorpius: Messier 4 and Messier 80. The first is the closest object of its kind to us. It is located about 6,000 light-years away. It is a region of space with a diameter of 35 light-years, containing stars with a total mass 84,000 times greater than that of the Sun.

    Messier 4.
    Source: Wikipedia

    In addition to star clusters, Scorpius also contains several nebulae. For example, NGC 6302, or the Bug Nebula. It really does resemble an insect with its antennae spread out on either side. In reality, it is a bipolar planetary nebula formed as a result of a red giant star shedding its outer layers.

    Or NGC 6334, known as the Cat’s Paw Nebula or Bear’s Paw Nebula. It is a huge cloud of interstellar hydrogen illuminated by nearby bright stars. Intense star formation processes are taking place within it.

    And, of course, there are plenty of galaxies in the constellation Scorpius. One example is NGC 6000, a barred spiral galaxy. It is about 112 million light-years away, but it appears relatively bright due to its active core.

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

    21-11-2025 om 16:27 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Earth and Theia were neighbors

    Earth and Theia were neighbors

    Scientists have reproduced the chemical composition and size of Theia. It is believed that at the beginning of the Solar System’s existence, it collided with Earth. Research shows that, like our planet, it formed not too far from the Sun.

    How were Earth and Theia formed?
    Source: phys.org

    Theia

    In a study published in the journal Science, researchers led by the Max Planck Institute for Solar System Research (MPS) and the University of Chicago have discovered where the planet Theia might have come from. It is believed that this small body collided with Earth only a few tens of millions of years after it was formed.

    This theory was put forward to explain where the Moon came from. And in principle, it is consistent. However, to this day, no one has been able to definitively say where this mysterious body came from. Did it follow the same orbit as Earth? Or did it follow a different orbit within the inner Solar System? Could it have come from beyond Jupiter’s orbit?

    The answers to these questions could be found in the isotopic composition of the Earth and the Moon. Atoms of the same element can have different weights. And they were already separated in the protoplanetary disk around the Sun. The inner parts had one set, while the outer parts had another.

    Chemical analysis

    Theoretically, the origin of Theia can be determined by the differences in the isotopic composition of its material from that of Earth. To this end, researchers analyzed 15 samples of Earth rocks and six more brought back from the Moon. It is believed that most of Theia’s material may remain on our moon.

    Scientists were interested in the ratio of iron isotopes, as well as chromium, molybdenum, and zirconium. And they found no particular differences. It seems that Theia did not come to us from the vicinity of the Solar System, but formed somewhere nearby?

    But how close? Simple isotopic analysis cannot answer this question. Scientists resorted to modeling how Earth and Theia could have formed. It turns out that the chemical composition of our planet can easily be reproduced as a combination of different types of meteorites.

    However, Theia should have contained a small but noticeable impurity of unknown origin. Scientists believe that this can be explained by assuming that this body formed closer to the Sun than Earth.

    According to phys.org

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

    21-11-2025 om 16:03 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Moss spores survive for nine months in the vacuum of space

    Moss spores survive for nine months in the vacuum of space

    Recently, scientists have confirmed the incredible resilience of living organisms to space conditions. Moss spores, which spent nine months outside the International Space Station in a vacuum and under intense radiation, were successfully grown into full-fledged plants.

    Moss. Source: Tomomichi Fujita

    Moss survival ability

    Mosses thrive in the most extreme conditions on Earth: from the peaks of the Himalayas to the sands of Death Valley, from the Antarctic tundra to the lava fields of active volcanoes. Inspired by the resilience of moss, researchers sent moss sporophytes—reproductive structures containing spores—to the most extreme environment: space.

    The results of the study, published on November 20 in the journal iScience, show that more than 80% of the spores survived for nine months outside the International Space Station (ISS) and returned to Earth while retaining their ability to reproduce. This is the first time that early terrestrial plants can survive after prolonged exposure by space elements.

    “Most living organisms, including humans, cannot survive even briefly in the vacuum of space,” says lead author Tomomichi Fujita of Hokkaido University. “However, the moss spores retained their vitality after nine months of direct exposure. This provides striking evidence that the life that has evolved on Earth possesses, at the cellular level, intrinsic mechanisms to endure the conditions of space.”

    Simulation of space conditions

    To find out whether a plant such as moss could survive in space, Fujita’s team subjected Physcomitrium patens, a well-studied moss known as spreading earth moss, to simulated space conditions, including high levels of ultraviolet radiation and extremely high and low temperatures.

    They tested three different moss structures—protenemata, or young moss; brood cells, or specialized stem cells that appear under stressful conditions; and sporophytes, or encapsulated spores—to find out which ones had the best chance of surviving in space.

    Researchers found that ultraviolet radiation was the most challenging element for survival, and sporophytes were the most resilient of the three parts of moss. None of the young mosses survived under high levels of ultraviolet radiation or extreme temperatures. The brood cells had a higher survival rate, but the spores in the shell showed approximately 1,000 times greater resistance to ultraviolet radiation. The spores were also able to survive and germinate after exposure to a temperature of -196°C for more than a week, as well as after being kept at a temperature of 55°C for a month.

    The team suggested that the structure surrounding the spore serves as a protective barrier, absorbing ultraviolet radiation and physically and chemically protecting the inner spore from damage. Researchers note that this is likely an evolutionary adaptation that allowed bryophytes—a group of plants that includes mosses—to transition from aquatic to terrestrial plants 500 million years ago and survive several mass extinctions since then.

    “Space Travel” by moss

    To test whether this adaptation could make sporophytes viable in real space conditions, the team sent spores beyond the stratosphere.

    In March 2022, researchers sent hundreds of sporophytes to the ISS aboard the Cygnus NG-17 spacecraft. Upon arrival, astronauts attached the sporophyte samples to the exterior of the ISS, where they remained in open space for a total of 283 days. The moss then returned to Earth aboard SpaceX CRS-16 in January 2023 and was brought back to the lab for testing.

    More than 80% of the spores survived the space journey, and all but 11% of the remaining spores were able to germinate in the laboratory. The team also checked the chlorophyll levels in the spores and found normal levels for all types, except for a 20% reduction in chlorophyll a, a compound that is particularly sensitive to changes in visible light, but this change did not appear to affect the health of the spores.

    “This study demonstrates the astonishing resilience of life that originated on Earth,” says Fujita.

    Mathematical model of moss survival in space

    Interested in how long spores could survive in space, Fujita’s team used data from before and after the moss expedition to create a mathematical model. They estimated that spores in their shells could survive up to 5,600 days — approximately 15 years — in space. However, they emphasize that this figure is only an estimate and that a larger data set is needed for more realistic predictions of how long moss could survive in space.

    Researchers hope that their work will contribute to the development of research into the potential of extraterrestrial soils to promote plant growth and inspire the use of moss to develop agricultural systems in space.

    “Finally, we hope that this work will open up new horizons for building ecosystems in extraterrestrial environments such as the Moon and Mars,” says Fujita. “I hope that our research on moss will serve as a starting point.”

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

    21-11-2025 om 15:44 geschreven door peter  

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    19-11-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Interstellaire komeet 3I/ATLAS onthult zijn geheimen

    Interstellaire komeet 3I/ATLAS onthult zijn geheimen

    Sinds zijn ontdekking in juli 2025 raast de interstellaire komeet 3I/ATLAS door ons zonnestelsel. Een armada van telescopen en ruimtesondes heeft de mysterieuze bezoeker vastgelegd, wat leidt tot een verrassende ontdekking over zijn samenstelling.

    Het is een zeldzaam kosmisch spektakel: een bezoeker van ver buiten ons zonnestelsel. Na Oumuamua en Borisov is komeet 3I/ATLAS pas het derde bevestigde interstellaire object dat door onze kosmische achtertuin suist. Sinds wij in juli al schreven over zijn ontdekking, heeft een hele batterij aan observatoria de komeet bestudeerd. De nieuwste beelden en eerste onderzoeksgegevens schetsen een fascinerend portret van deze kosmische reiziger…

    Een visuele reis langs de komeet

    De eerste aanwijzing dat er iets bijzonders aan de hand was, kwam van het ATLAS-systeem in Chili op 1 juli 2025. De waarneming toonde een vaag, bewegend object dat niet in een gebonden baan om de zon bleek te draaien.

    De ontdekkingsopname van 3I/ATLAS, gemaakt door het Asteroid Terrestrial-impact Last Alert System (ATLAS) in Chili op 1 juli 2025. Het zwakke, bewegende object (aangegeven met pijlen) was de eerste hint van een nieuwe interstellaire bezoeker.
    Foto-animatie: ATLAS/University of Hawaii/NASA

    Nog geen maand later, op 21 juli, bevestigde de Hubble ruimtetelescoop de komeetachtige aard van het object. Een animatie van de waarnemingen toonde een heldere, traanvormige coma van stof en gas die van de kern afkomstig was.

    Animatie van meerdere foto’s genomen door de Hubble ruimtetelescoop op 21 juli 2025, waarop de beweging en de stofcoma van 3I/ATLAS duidelijk zichtbaar zijn. De komeet bevond zich op dat moment op 446 miljoen kilometer van de Aarde.
    Foto-animatie: NASA, ESA, David Jewitt (UCLA); bewerking: Joseph DePasquale (STScI)

    De James Webb ruimtetelescoop bracht op 6 augustus de samenstelling in kaart. Een drieluik in verschillende infrarood golflengten onthulde de aanwezigheid van koolstofdioxide (CO₂) en water (H₂O) in de coma van de komeet.

    Drieluik van 3I/ATLAS, vastgelegd door NIRCam van de James Webb ruimtetelescoop. De beelden tonen de totale helderheid (links), emissie van koolstofdioxide (midden) en emissie van water (rechts) op 6 augustus 2025.
    Foto’s: NASA/James Webb Space Telescope

    Eind augustus legde de Gemini South-telescoop in Chili een prachtig overzichtsbeeld in kleur vast, waarop de coma te zien was die zich duizenden kilometers het heelal in uitstrekte.

    Diepteopname van 3I/ATLAS door de Gemini South-telescoop op 27 augustus 2025. De afbeelding toont de brede coma met een lengte van ongeveer 1/120e graad aan de hemel. Foto: International Gemini Observatory/NOIRLab/NSF/AURA/Shadow the Scientist.
    Beeldbewerking: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)

    Marssondes grijpen hun kans

    Toen 3I/ATLAS op 3 oktober 2025 dicht langs Mars scheerde, veel dichter dan deze ooit bij Aarde kwam, grepen twee orbiters rond de rode planeet hun unieke kans. ESA’s ExoMars Trace Gas Orbiter (TGO) legde vanaf zo’n 30 miljoen kilometer afstand de komeet vast als een heldere, wazige vlek. Bijna gelijktijdig deed ook China’s Tianwen 1 orbiter waarnemingen, waarbij de kern en coma duidelijk van elkaar te onderscheiden waren.

    Gestapelde opnames van 3I/ATLAS (de bewegende wazige vlek), vastgelegd door de CaSSIS-camera aan boord van ESA’s ExoMars Trace Gas Orbiter op 3 oktober 2025, vanuit een baan om Mars.
    Foto/animatie: ESA/TGO/CaSSIS
    3I/ATLAS gefotografeerd door de High-Resolution Imaging Camera (HiRIC) van China’s Tianwen 1 orbiter, eveneens op 3 oktober 2025, vanuit een baan rond Mars. De afstand bedroeg alhier circa 29 miljoen kilometer.
    Foto/animatie: CNSA

    Een komeet met een kosmisch litteken

    Wat kunnen we uit al deze data afleiden? Een opvallende bevinding is dat de kleur van de komeet niet mysterieus veranderde, zoals soms werd vermoed. Volgens wetenschapper Qicheng Zhang is er geen bewijs voor kleurveranderingen van de gassen in de coma. “Onze analyses tonen aan dat de coma sinds de eerste detectie van een coma nog altijd aanwezig is, substantieel bijdraagt aan de waargenomen helderheid van het object, maar kleurveranderingen of een veranderende samenstelling van de uitgestoten gassen werd niet geobserveerd”, zo stelde hij. De karakteristieke blauwgroene tint werd al in september door observatoria maar ook amateurastronomen waargenomen.

    Qicheng Zhang, postdoctoraal astronoom aan de Lowell Observatory in Arizona fotografeerde ook zelf het interstellaire object met een 6-inch (152-mm) Ritchey–Chrétien reflector door dunne bewolking heen in de ochtend van 1 november vanuit Arizona, V.S.
    Foto: Qicheng Zhang

    De meest revolutionaire inzichten komen van de eerste onderzoeksgegevens. Metingen van de James Webb ruimtetelescoop onthullen een extreem hoge verhouding koolstofdioxide ten opzichte van water. Dit unieke kenmerk wijst erop dat de buitenste laag van de komeetkern miljarden jaren lang is blootgesteld aan galactische kosmische straling. Deze intense straling heeft de oorspronkelijke materialen omgezet in een soort verweerd, aan organisch materiaal rijke korst. We kijken dus niet naar een ongerepte tijdcapsule uit een ver gelegen zonnestelsel, maar naar een object dat de littekens draagt van een lange, eenzame reis door de Melkweg.

    Schematische weergave van de naar verwachting gelaagde structuur van de kern van 3I/ATLAS, waaruit het effect van galactische kosmische straling blijkt. De buitenste ~15-20 meter is verrijkt met koolstofdioxide (CO₂) en organisch materiaal, terwijl de ongerepte, oorspronkelijke samenstelling zich eronder bevindt.
    Afbeelding: Romain Maggiolo et al., Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Science Systems and Application Inc. Hampton, Nasa Langley Research Center, Hampton, Centre for mathematical Plasma Astrophysics, Heverlee, Belgium. arXiv:2510.26308
    De geplotte banen van 3I/ATLAS en ons zonnestelsel in ons sterrenstelsel (van bovenaf bezien). De baan van onze zon is weergegeven in gele stippellijn, die van de komeet in rood. Begrepen kan worden dat de komeet een excentrischer baan volgt om het centrum van de Melkweg dan ons zonnestelsel zelf. Afbeelding: M. Hopkins/Ōtautahi-Oxford team.
    Base map: ESA/Gaia/DPAC, Stefan Payne-Wardenaar

    Slot

    3I/ATLAS blijft zich, zoals gepland, haastig van ons verwijderen. De komende weken zal hij echter nog zichtbaar blijven voor telescopen, waarbij zijn reis perfect te volgen is in bijvoorbeeld NASA’s ‘Eyes on the Solar System’ app. Elke nieuwe waarneming biedt een zeldzame kans om de geschiedenis van deze kosmische zwerver verder te ontcijferen.

    Animatie van de hyperbolische baan van 3I/ATLAS door ons zonnestelsel. De baan bevestigt dat het object niet door de zwaartekracht van de Zon is gebonden en ons stelsel weer zal verlaten.
    Afbeelding: NASA/JPL
    De komende weken staan nog observaties met ESA’s sonde JUICE gepland, momenteel onderweg naar Jupiter.
    Afbeelding: ESA/ATG Europe

    Bronmateriaal

    https://scientias.nl/nieuws/astronomie-ruimtevaart/ }

     

    19-11-2025 om 23:38 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.NASA scientists are baffled to discover a rock on Mars that 'doesn't belong there'

    NASA scientists are baffled to discover a rock on Mars that 'doesn't belong there'

    NASA's scientists have been baffled after discovering a mysterious rock on Mars that 'doesn't belong there'.

    The Perseverance rover found the strange boulder near the rim of the 28-mile-wide (45 kilometres) Jezero crater, which experts think could have once hosted life.

    The rock measures 31 inches (80 centimetres) across and initially stood out due to its 'sculpted' appearance.

    Now, experts say that it likely originated from somewhere else in the solar system.

    Perseverance used its SuperCam instrument to measure the rock's composition by heating a small section of the surface with a powerful laser.

    This revealed that the object, which has been named Phippsaksla, has an exceptionally high iron and nickel content.

    This is unusual since Perseverance has not found a single rock with such high metal content anywhere else in Jezero crater.

    Dr Candice Bedford, a geologist from Purdue University and Perseverance operator, wrote in a NASA blog: 'This element combination is usually associated with iron-nickel meteorites formed in the core of large asteroids, suggesting that this rock formed elsewhere in the solar system.'

    NASA scientists have spotted a mysterious rock on Mars which 'shouldn't be there' due to its unusual metallic composition and 'sculpted' appearance. This image of the rock was taken using the Perseverance rover's Mastcam-Z camera

    NASA scientists have spotted a mysterious rock on Mars which 'shouldn't be there' due to its unusual metallic composition and 'sculpted' appearance. This image of the rock was taken using the Perseverance rover's Mastcam-Z camera

    Phippsaksla rock on Mars

    NASA has discovered an interesting rock it's called Phippsaksla. 

    (NASA/JPL-Caltech/ASU)

    Since landing on Mars in February 2021, Perseverance has been exploring the geology of Mars' northern Jezero crater.

    This is an area of particular interest to scientists, who believe the crater may have once been filled with water, making it one of the best places to search for signs of life.

    Recently, Perseverance climbed into a region known as the Vernodden, high on the crater's rim, where it spotted Phippsaksla.

    Finding a meteor on Mars' cratered surface isn't unexpected, but the high metal content is much rarer.

    Professor Gareth Collins, an expert on meteor impacts from Imperial College London, told the Daily Mail that Mars is hit by meteors 'all the time'.

    'At some point in time, the entire Martian surface has been shaped by impacts,' he explained.

    'Meteors are expected on Mars on a daily basis; we don’t know the number precisely, but there should be lots each day'.

    The vast majority of the meteorites falling on Mars are rocky, while only about one in 20 are rich in iron and nickel.

    The rock, which has been named Phippsaksla, measures 31 inches (80 centimetres across) and has an unusually high iron and nickel content. Experts say this means it could be a meteorite which formed elsewhere in the solar system

    The rock, which has been named Phippsaksla, measures 31 inches (80 centimetres across) and has an unusually high iron and nickel content. Experts say this means it could be a meteorite which formed elsewhere in the solar system 

    The different types of space rock

    Asteroid: A chunk of rock left over from collisions in the early solar system.

    Comet: A ball of ice, rock, methane, and other compounds.

    Meteoroid: A piece of rock which burns up in the atmosphere.

    Meteor: What astronomers call a flash of light in the atmosphere when debris burns up 

    Meteorite: Rock that makes it through the atmosphere to the planet's surface.  

    These metallic meteorites are typically forged in the hearts of large asteroids, as the heavy minerals sank to the centre of heated rocks during the solar system's formation.

    Phippsaksla's composition suggests that it might have had a similar origin elsewhere in the solar system, rather than forming on Mars.

    Dr Gareth Dorrian, of the University of Birmingham, told the Daily Mail: 'It is quite likely this one on Mars came from the asteroid belt.

    'These particular meteorites are quite resistant to chemical weathering and are more likely to survive the fiery fall through a planetary atmosphere.'

    However, despite being rarer than rocky meteorites, the sheer volume of meteorites hitting Mars means that all other Mars rovers have found iron-nickel rocks.

    The Curiosity rover has found many iron-nickel meteorites in the Gale crater, including a massive 39-inch (one metre) metallic meteorite dubbed 'Lebanon'.

    Likewise, both the Curiosity and Spirit rovers found similar iron-nickel meteorites during their own missions.

    Dr Bedford writes: 'As such, it has been somewhat unexpected that Perseverance had not seen iron-nickel meteorites within Jezero crater, particularly given its similar age to Gale crater and number of smaller impact craters suggesting that meteorites did fall on the crater floor, delta, and crater rim throughout time.'

    The Mars rover Perseverance (pictured) spotted the strange rock while exploring a region known as Vernodden, high on the rim of the Jezero Crater. This is a particular area of interest, since scientists think the crater may once have been filled with water

    The Mars rover Perseverance (pictured) spotted the strange rock while exploring a region known as Vernodden, high on the rim of the Jezero Crater. This is a particular area of interest, since scientists think the crater may once have been filled with water

    This is not the first time rovers have found iron and nickel meteorites. In 2014, the Curiosity rover found a massive 39-inch (one metre) metallic meteorite dubbed 'Lebanon' (pictured)

    This is not the first time rovers have found iron and nickel meteorites. In 2014, the Curiosity rover found a massive 39-inch (one metre) metallic meteorite dubbed 'Lebanon' (pictured)

    This comes after Perseverance spotted an unusual 'helmet' rock in the Jezero crater, which may have been formed by volcanic activity

    This comes after Perseverance spotted an unusual 'helmet' rock in the Jezero crater, which may have been formed by volcanic activity  

    Due to Phippsaksla's exotic nature, NASA's scientists say they will need more time to analyse it to confirm whether it is a meteorite.

    If it is proven that the rock fell from space, then Perseverance can finally be ranked among the rovers to have investigated these rare and fascinating Martian visitors.

    However, this is not the first unusual discovery that Perseverance has made on its journey through the Jezero crater.

    article image

    In August, Perseverance snapped a picture of a bizarre 'helmet' on the Martian surface.

    A closer look reveals it was covered from top to bottom with small bobbles, which are known by geologists as 'spherules'.

    On Earth, spherules are formed by the rapid cooling of molten rock droplets during a volcanic eruption, or by the condensation of rock vaporised by a meteorite impact.

    This suggests it might have been formed some time in the distant past when Mars' surface was dotted with active volcanoes.

    MARS: THE BASICS

    Mars is the fourth planet from the sun, with a 'near-dead' dusty, cold, desert world with a very thin atmosphere. 

    Mars is also a dynamic planet with seasons, polar ice caps, canyons, extinct volcanoes, and evidence that it was even more active in the past. 

    It is one of the most explored planets in the solar system and the only planet humans have sent rovers to explore.

    One day on Mars takes a little over 24 hours and a year is 687 Earth days.

    Facts and Figures 

    Orbital period: 687 days

    Surface area: 55.91 million mi²

    Distance from Sun: 145 million miles

    Gravity: 3.721 m/s²

    Radius: 2,106 miles

    Moons: Phobos, Deimos

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

    19-11-2025 om 23:07 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.'From another world': 3I/ATLAS photobombs a galaxy and shows off its multiple tails in stunning new image
    'From another world': 3I/ATLAS photobombs a galaxy and shows off its multiple tails in stunning new image

    Overview

    The interstellar visitor 3I/ATLAS—the third confirmed object of its kind—has once again captured the attention of astronomers and the public alike. First spotted in early July 2025 as it barreled toward the Sun at more than 130,000 mph, the object is thought to have originated from the distant “frontier” region of the Milky Way and could be as old as seven billion years. After passing perihelion on 29 October, 3I/ATLAS emerged from behind the Sun and, on 16 November, was photographed by amateur astrophotographer Satoru Murata with a modest 0.2‑meter telescope. The resulting image not only showcases the comet’s striking green coma and twin tails but also inadvertently “photobombs” the barred spiral galaxy NGC 4691, which appears in the top‑left corner of the frame.

    The Photographic Capture

    Murata’s long‑exposure shot reveals a bright green coma—a hallmark of ionized carbon monoxide and cyanogen gases fluorescing under solar ultraviolet radiation. Extending from the nucleus is a long ion tail that points directly away from the Sun, indicating the influence of the solar wind. A shorter, broader anti‑tail trails behind the comet, a feature created by excess dust particles that lag in the comet’s orbital path and become illuminated from Earth’s perspective. The image also shows smaller jets erupting from the nucleus, suggesting localized outgassing regions.

    “The moment I realized the galaxy was in the frame, I knew we had something special,” Murata told Live Science. “It’s rare to have an interstellar comet and a distant galaxy share the same field of view—like a cosmic coincidence.” The photograph, posted to the astronomy community’s forums, quickly garnered over 12,000 likes and sparked discussion about the object’s unusual morphology.

    Scientific Context and Anomalies

    Since its discovery, 3I/ATLAS has exhibited a series of anomalous behaviors that set it apart from typical solar‑system comets. After perihelion, the comet brightened more rapidly than models predicted, prompting speculation about a volatile‑rich interior. Spectroscopic observations recorded a temporary color shift from green to a faint blue hue, hinting at changes in the composition of the coma as different ices sublimated. Moreover, the comet’s surface appears highly irradiated, with an overabundance of carbon‑bearing molecules such as C₂ and CN, which are rarely seen in such quantities in other comets.

    These characteristics have led a small contingent of researchers to propose more exotic explanations, including the provocative—but widely contested—hypothesis that 3I/ATLAS could be an artificial probe or “alien spaceship.” Dr. Elena Mendoza of the Institute for Interstellar Studies remarked, “While the data are intriguing, the bulk of evidence aligns with natural cometary processes. Extraordinary claims require extraordinary evidence, and we have yet to see any definitive signs of technology.” The majority of planetary scientists concur, emphasizing that the observed phenomena can be explained by thermal stressesheterogeneous composition, and solar‑wind interactions typical of icy bodies entering the inner solar system at high speed.

    Trajectory and Upcoming Close Approach

    3I/ATLAS will make its closest approach to Earth on 19 December 2025, passing within roughly 0.23 AU (about 34 million kilometers). At that distance, the comet’s apparent magnitude is expected to reach +6, making it visible to the naked eye under dark skies for observers in the northern hemisphere. Astronomers worldwide are coordinating a series of observations—including high‑resolution spectroscopy, polarimetry, and radio measurements—to capture the comet’s activity as it recedes from the Sun.

    The object’s hyperbolic orbit confirms its interstellar origin; calculations indicate an incoming velocity of ~30 km s⁻¹ relative to the Sun, far exceeding the escape velocity of the solar system. Its trajectory suggests it entered from a direction roughly aligned with the galactic anti‑center, supporting the hypothesis that it originated in the sparsely populated outer regions of the Milky Way.

    Significance for Interstellar Research

    The third confirmed interstellar visitor offers a rare laboratory for studying material that formed around another star. The multiple tails captured in Murata’s image provide clues about the distribution of volatile ices and dust, while the spectral signatures of unusual chemicals may reflect a different chemical pathway in its natal system. Comparative analysis with the first two interstellar objects—‘Oumuamua (2017) and 2I/Borisov (2019)—will help refine models of planetary system formation across the galaxy.

    As Dr. Ravi Kumar, a cometary physicist at the University of Arizona, noted, “Each interstellar object is a messenger from a distant world. 3I/ATLAS, with its vivid tails and unexpected chemistry, expands our understanding of the diversity of planetary building blocks beyond our own solar system.” The upcoming observations, combined with the striking visual record of its encounter with NGC 4691, ensure that 3I/ATLAS will remain a focal point of scientific inquiry and public fascination well into the next year.

     https://usubjects.com/  }

    19-11-2025 om 22:23 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.NASA Releases Long-Delayed Image of 3I/ATLAS

    NASA Releases Long-Delayed Image of 3I/ATLAS

    Finally.
    NASA finally released an early "peek" at the observations of its spacecraft of interstellar object 3I/ATLAS during a livestream today.
    NASA

    Mysterious interstellar object 3I/ATLAS made an astonishingly close pass of Mars last month, allowing scientific instruments in the planet’s orbit to get a tantalizing glimpse.

    Yet thanks to the US federal government shutdown that ended earlier this month, NASA was forced to delay the release of images taken by the HiRISE camera attached to its Mars Reconnaissance Orbiter, prompting outrage from lawmakers and astronomers alike.

    Fortunately, NASA finally released some of the observations during a livestream today.

    One image, taken by HiRISE on October 2, shows a “fuzzy white ball,” as NASA associate administrator Amit Kshatriya described it. At the time, 3I/ATLAS was just 19 million miles away from the instrument.

    “That ball is a cloud of dust and ice called the coma, which is shed by the comet,” Kshatriya said.

    Image of 3I/ATLAS taken by NASA's HiRISE instrument on the Mars Reconnaissance Orbiter.

    NASA also released images of the comet taken by the Mastcam-Z instrument attached to its Perseverance Mars rover, taken on October 4, showing the object whipping by at around 137,000 mph.

    Image of 3I/ATLAS taken by NASA's HiRISE Perseverance Mars rover.

    Separate ultraviolet spectrograph observations by NASA’s MAVEN spacecraft show the comet emitting hydrogen gas as it approached Mars in late September.

    Before getting to the latest observations during today’s livestream, Kshatriya chose to “address the rumors right at the beginning,” publicly denouncing a prevalent theory — prominently championed by Harvard astronomer Avi Loeb in the media — that 3I/ATLAS could be an alien spacecraft that came to visit.

    “This object is a comet,” Kshatriya said. “It looks and behaves like a comet, and all evidence points towards it being a comet.”

    Fortunately, 3I/ATAS is expected to make its closest pass of the Earth on December 19, giving NASA spacecraft yet another chance to observe it.

    More on 3I/ATLAS:

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    {  https://futurism.com/category/science-energy }

    19-11-2025 om 22:13 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.NASA’s Perseverance Has Seen a Lot of Rocks—But Not One Like This

    NASA’s Perseverance Has Seen a Lot of Rocks—But Not One Like This

    In a first for the Perseverance rover, it appears to have found an iron-nickel meteorite near the Jezero Crater.

    This exotic rock was discovered near the rim of the Jezero Crater by NASA's Perseverance rover. Named "Phippsaksla," preliminary analysis suggests it could be an iron-nickel meteorite

    NASA’s Perseverance rover has seen its fair share of rocks, and most are unremarkable. Once in a while, however, Perseverance stumbles upon something exotic. That’s precisely what happened during the rover’s recent investigation of the bedrock at “Vernodden.”

    While exploring this site along the rim of the Jezero Crater, Perseverance encountered an oddly shaped rock about 31 inches (80 centimeters) wide, according to NASA. Now named “Phippsaksla,” it caught the attention of Perseverance’s handlers due to its sculpted, high-standing appearance, rising sharply above the flat, fragmented rocks surrounding it.

    Further investigations are required to determine the true nature of Phippsaksla, but a preliminary analysis of its composition suggests it may be a meteorite rich in iron and nickel. This type of meteorite is less commonly found on Earth but dominates the small number of meteorites that rovers have found on Mars. Still, finding one near the Jezero Crater is a first for Perseverance.

    A possible sample from an ancient asteroid

    Perseverance used its SuperCam instrument to reveal Phippsaksla’s composition. This tool examines rocks and soils with a camera, laser, and spectrometers to identify their chemical and mineral components.

    The combination of elements Perseverance found is typically associated with iron-nickel meteorites, suggesting Phippsaksla hails from somewhere else in the solar system.

    A zoomed-out image of an exotic rock found on Mars

    This image of Phippsaksla (upper left), captured by Perseverance from farther away, showcases its distinct shape
    © NASA/JPL-Caltech/ASU

    These meteorites are samples from the cores of ancient worlds. Asteroids that melted early on in their history formed iron and nickel cores as these dense elements sank to the center. Iron-nickel meteorites are fragments of those cores, freed by collisions between their parent asteroid and other celestial bodies.

    Other Mars rovers have found several while exploring the Red Planet. Curiosity has identified many in the Gale Crater, including the one-foot-wide “Cacao” meteorite found in 2023. Both of the twin Mars Exploration Rovers, Spirit and Opportunity, also found iron-nickel meteorites during their missions.

    A surprising first for Perseverance

    It’s somewhat surprising that it took Perseverance this long to find an iron-nickel meteorite, especially considering that its primary exploration area, the Jezero Crater, is roughly the same age as the Gale Crater. What’s more, a number of smaller impact craters within Jezero suggest meteorites did impact the crater floor, delta, and rim throughout its history.

    But again, additional analysis will need to confirm that Phippsaksla is actually an iron-nickel meteorite. In addition to SuperCam, Perseverance is equipped with other instruments capable of analyzing rock samples in situ, such as PIXL (Planetary Instrument for X-Ray Lithochemistry). This tool could provide a more refined picture of Phippsaksla’s chemistry.

    Perseverance is also the first Mars rover capable of collecting and caching rock samples for a potential return to Earth, and it’s possible that it could add a chunk of Phippsaksla to its collection. NASA has tentative plans to retrieve Perseverance’s samples, but the future of the Mars Sample Return mission is currently uncertain.

    Phippsaksla has certainly caught NASA’s attention, and we should learn more about this specimen as the Perseverance team continues to probe its exotic chemistry.  With no end in sight to the rover’s mission, there’s no telling what this intrepid explorer will find next.

    RELATED VIDEOS

    https://gizmodo.com/science }

    19-11-2025 om 21:50 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.Webb Captures a Stunning Cosmic Structure We’ve Never Seen Before

    Webb Captures a Stunning Cosmic Structure We’ve Never Seen Before

    The aging pair of stars swing by one another once every 190 years, producing four spirals of dust.
    Webb’s mid-infrared image shows four coiled shells of dust around a pair of Wolf-Rayet stars.

    Webb’s mid-infrared image shows four coiled shells of dust around a pair of Wolf-Rayet stars.
    NASA, ESA, CSA, STScI; Science: Yinuo Han (Caltech), Ryan White (Macquarie University); Image Processing: Alyssa Pagan (STScI)
    The Webb telescope has unlocked a mystery in an exotic star system located approximately 8,000 light-years from Earth. Using its mid-infrared observation capabilities, the space telescope captured the first image of four swirling spirals of dust encircling two aging stars locked together in an orbital dance.
    NASA released the image on Wednesday, confirming the existence of the layered shells of dust surrounding two Wolf-Rayet stars in the Apep system. Previous observations had only detected one dust spiral, while Webb was not only able to see all four, but it also narrowed down how long the binary stars take to orbit one another.
    “Looking at Webb’s new observations was like walking into a dark room and switching on the light—everything came into view,” Yinuo Han, a researcher at Caltech in Pasadena, California, and lead author of a new study published in the Astrophysical Journal, said in a statement. “There is dust everywhere in Webb’s image, and the telescope shows that most of it was cast off in repetitive, predictable structures.”

    One of a kind

    Wolf-Rayet stars are extremely rare, with only about a thousand of them believed to exist in the Milky Way galaxy. They are massive, bright stars in late stages of their stellar evolution. Stars that big don’t last very long; Wolf-Rayets burn through their fuel rather quickly, expelling their mass into space through high-pressure winds.

    The pair of stars in Apep, named after the Egyptian god of chaos, have been shedding their outer layers over the past 700 years. The two Wolf-Rayet stars are gravitationally bound to one another, along with a third companion, a massive supergiant star that carves a hole into the clouds of dust from its wider orbit.

    Most Wolf-Rayet stars orbit one another within two to 10 years, with the longest recorded orbital period being 30 years. The Apep stars, however, swing by one another every 190 years. The team of researchers behind the new study was able to figure out the orbits of the stars by combining measurements of the location of the rings from Webb’s image with the speed of the shells’ expansion from observations taken by the European Southern Observatory’s Very Large Telescope in Chile over a period of eight years.

    With each long orbit, the two stars remain close for 25 years, forming the expanding dust shells. As the stars approach and pass one another, their stellar winds collide and mix, forming the spirals of dust for a period that lasts a quarter of a century. The dust of other star systems lasts for a few months at a time.

    Although the Webb image may inspire tranquility, there is nothing chill about the Apep stars. The two stars are emitting dust at 1,200 to 2,000 miles per second (2,000 to 3,000 kilometers per second) while speeding through the cosmos.

    The Wolf-Rayet stars were initially more massive than their third companion but have shed most of their mass over the years. Scientists estimate that the two stars are between 10 and 20 times the mass of the Sun, while the supergiant is 40 or 50 times as massive as our host star.

    Although scientists have known about the third star in the Apep system, Webb’s observations confirmed that it is gravitationally bound to the system by revealing it slicing through the dust shells. “Webb gave us the ‘smoking gun’ to prove the third star is gravitationally bound to this system,” Ryan White, a PhD student at Macquarie University in Sydney, Australia, and author of another paper published in the Astrophysical Journal, said in a statement.

    The two massive stars are on a path to destruction and will eventually explode as supernovas. It’s possible that either of the stars may emit a gamma ray burst before becoming a black hole.

    RELATED VIDEOS

    19-11-2025 om 21:28 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    18-11-2025
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Space fashion face-off! While NASA's astronauts wear spacesuits designed by Prada, European Space Agency's travellers will have to settle for... Decathlon

    Space fashion face-off! While NASA's astronauts wear spacesuits designed by Prada, European Space Agency's travellers will have to settle for... Decathlon

    For decades, the USA and Europe have been battling it out in the space race.

    But when it comes to high fashion, there's now a clear winner.

    While NASA's spacesuits are being developed, in part, by Prada, astronauts at the European Space Agency (ESA) will have to settle for a more humble designer – Decathlon.

    The high street brand, best known for selling affordable sportswear, has announced it is behind a new intra-vehicular activity (IVA) space suit prototype.

    Its dark grey 'EuroSuit' is designed to be worn during 'critical' phases of a mission, such as launch and landing, and can be donned or removed without assistance in under two minutes.

    It will be tested by ESA astronaut Sophie Adenot during a mission to the International Space Station (ISS) next year.

    The mainstream sports shop couldn't be further from the iconic Italian fashion powerhouse behind NASA's suits.

    But Decathlon says the opportunity demonstrates its ability to 'transfer its sports innovation expertise into the extreme environment of human spaceflight'.

    High street store Decathlon has announced it is behind a new intra-vehicular activity (IVA) space suit prototype

    High street store Decathlon has announced it is behind a new intra-vehicular activity (IVA) space suit prototype

    Its dark grey ‘EuroSuit’ is designed to be worn during ‘critical’ phases of a mission, such as launch and landing, and can be donned or removed without assistance in under two minutes

    Its dark grey 'EuroSuit' is designed to be worn during 'critical' phases of a mission, such as launch and landing, and can be donned or removed without assistance in under two minutes

    Meanwhile Prada, founded in Milan in 1913, has teamed up with Axiom Space to advise on NASA's suit design and materialsIts creation, called the Axiom Extravehicular Mobility Unit (AxEMU) spacesuit, has been described as 'evolvable, scalable and adaptable' for missions on the lunar surface and in low-Earth orbit

    Prada - known for its luxury handbags, accessories and footwear - has turned to designing a spacesuit to be worn on the next mission to the moon

    The prototype features a range of 'groundbreaking' advancements, including a lattice-structured helmet design that allows for perfectly tailored fits.

    Expanding 'bellows' at the shoulders, elbows and knees ensure maximum mobility in confined environments.

    Air-tight zippers with 'ergonomic pullers' make it easy to open and close the suit, while the suit's length can be adjusted to compensate for the natural elongation of astronauts' bodies in microgravity.

    The ability to don or remove the suit in under two minutes unaided is a first for IVA suits and could significantly improve response times during spacecraft emergencies.

    Aboard the ISS, Ms Adenot will perform a series of test sequences including putting the suit on, manipulating small objects, using the onboard touchscreen tablet and taking the suit off.

    Her feedback will fuel the development of a fully operational version of the EuroSuit, complete with key systems such as air-tight sealing, fire resistance, breathable atmosphere control, built-in communications and head-up display interfaces.

    'The EuroSuit embodies our ability to push the boundaries of innovation beyond our traditional fields of expertise,' Sébastien Haquet, Head of Advanced Innovation at Decathlon, said.

    'It is a remarkable opportunity to explore new applications for our textile and product design know-how in an environment as demanding as space.'

    Prada's suit has been designed to accommodate both male and female astronauts with enhanced flexibility and mobility to allow them to move around for at least eight hoursDecathlon's prototype features a range of ‘groundbreaking’ advancements, including a lattice-structured helmet design that allows for perfectly tailored fits

    Decathlon's prototype (left) features a range of 'groundbreaking' advancements, including a lattice-structured helmet design that allows for perfectly tailored fits. Meanwhile Prada's suit (right) has been designed to accommodate both male and female astronauts with enhanced flexibility and mobility to allow them to move around for at least eight hours

    Decathlon is a French retailer with stores all over the UK and is best known for its affordable sportwear (file image)

    Decathlon is a French retailer with stores all over the UK and is best known for its affordable sportwear (file image)

    EuroSuit: Key specs 

    Custom-fit ergonomics: a lattice-structured helmet design allows for perfectly tailored fits to each astronaut's morphology.

    Freedom of movement: bellows integrated at the shoulders, elbows, and knees ensure maximum mobility in confined environments.

    Sealed, user-friendly zippers: air-tight zippers with ergonomic pullers facilitate easy opening and closing of the suit.

    Dimensional adaptability: the suit's length can be adjusted to compensate for the natural elongation of astronauts' bodies in microgravity

    Decathlon has worked in conjunction with French national space agency CNES, start-up Spartan Space and The Institute of Space Medicine and Physiology in the design of the suit.

    'In line with Europe's ambition to achieve greater autonomy in human spaceflight, CNES has decided to focus on intra-vehicular suits,' Sébastien Barde, Deputy Director for Exploration and Human Spaceflight, said.

    'By relying on the exceptional expertise of our partners, we are prepared to deliver this type of suit when the time comes.

    'In doing so, we are fully playing our role of supporting and guiding our industry.'

    Last year, Prada announced it was teaming up with Axiom Space to advise on the design and materials for a spacesuit to be worn on the next mission to the moon.

    The renowned fashion company said its team were able to assist with recommending customised materials and features for the spacesuit, as well as sewing methods that could improve its performance.

    The suit, which will be worn by the next humans to walk on the surface of the moon, will be capable of withstanding extreme temperatures at the lunar south pole and the coldest temperatures in permanently-shadowed regions.

    It has been designed to accommodate both male and female astronauts with enhanced flexibility and mobility to allow them to move around for at least eight hours.

    ESA astronaut Sophie Adenot (far right) will test the prototype suit during a mission to the ISS next year

    ESA astronaut Sophie Adenot (far right) will test the prototype suit during a mission to the ISS next year

    Features also include variable suit pressure, a carbon dioxide 'scrubbing' system, a portable life support system backpack and a bright white outer layer to reflect heat.

    The entire design also includes advanced coatings on the helmet and visor to enhance the astronauts' view of their surroundings, as well as custom gloves.

    READ MORE

    article image

    The suit will be used for NASA's Artemis III mission, a crewed lunar landing that will take place in September 2026 at the earliest.

    It will be the first time humans have returned to the moon since Apollo 17 in 1972 and will involve a week-long exploration of the lunar surface while conducting scientific studies.

    HOW DO ASTRONAUTS GO TO THE TOILET?

    On board the ISS there is a toilet which has several attachments.

    As there is no gravity in space, liquids do not flow but accumulate in floating globules.

    To counter this problem, there are hoses which are used and provide pressure to suck the fluid from the body.

    Each astronaut has their own personal attachment.

    When a toilet is not available or the astronaut is on a space-walk, the astronauts use MAGs (maximum absorbency garments) which are diapers that soak up all the waste.

    They are effective for short missions but have been known to leak occasionally.  

    Nasa is aiming to develop a suit which allows for long-term spacesuit usage and complete independent disposal of human waste. 

    On the moon missions there was no toilet and the all-male crew had 'condom catheter's that attached to the penis and the fluid was fed to a bag that resided outside of the suit.  

    According to an 1976 interview with astronaut Rusty Schweickart, the condom catheters came in three sizes: small, medium and large. 

    Despite the practical advantages of having the right size, the astronauts often ordered the large ones and this resulted in a leakage of urine in the suit.

    To combat this, Nasa renamed the sizes as large, gigantic, and humongous to appease the male ego. 

    There has yet to be an effective female equivalent developed, something Nasa aims to change for the Orion missions. 

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

    18-11-2025 om 23:08 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.Mapping the Milky Way: Incredible simulation charts more than 100 BILLION stars over the course of 10,000 years

    Mapping the Milky Way: Incredible simulation charts more than 100 BILLION stars over the course of 10,000 years

    Scientists from Japan's RIKEN research centre have created the most detailed simulation of the Milky Way ever made.

    The incredible galactic map charts more than 100 billion individual stars over the course of 10,000 years.

    Researchers use simulations like these to test theories about how the galaxy formed and changed over time.

    However, this is the very first 'star-by-star' simulation of our home galaxy to chart the evolution of the cosmos with such stunning detail.

    Even the best cutting-edge computer models struggle to accurately simulate complex movements of 100 billion stars in the Milky Way.

    This is because the galaxy is shaped by forces on both the enormously large and extremely small scales of distance and time.

    Galaxy simulations must consider gravity, fluid dynamics, supernova explosions, and the creation of elements in the hearts of dying stars.

    Now, by using AI, the researchers say they can make simulations that track 100 times as many stars.

    Scientists have created the most detailed simulation of the Milky Way ever created, charting the movements of 100 billion stars over 10,000 years. Pictured: A top-down view of the simulation showing areas of gases in red

    Scientists have created the most detailed simulation of the Milky Way ever created, charting the movements of 100 billion stars over 10,000 years. Pictured: A top-down view of the simulation showing areas of gases in red 

    Most simulations struggle to render more than a billion stars at a time, forcing them to group hundreds of suns. However, this is the very first true star-by-star simulation, plotting the movement of every individual star. Pictured: A side-on view of the simulation

    Most simulations struggle to render more than a billion stars at a time, forcing them to group hundreds of suns. However, this is the very first true star-by-star simulation, plotting the movement of every individual star. Pictured: A side-on view of the simulation 

    Because changes in the galaxy take place over such a long time, scientists can't just sit back and watch to learn about galactic evolution.

    By looking at galaxies that are very far away from Earth, astronomers can get an idea of what galaxies might have looked like at an earlier point in the universe's history.

    However, this data only provides a snapshot and doesn't tell us anything about our own galaxy.

    For that, astronomers are now trying to create powerful computer simulations that work out how stars would move and evolve based on what we know about the laws of physics.

    By changing the rules of the simulation and comparing the results to the universe around us, scientists can learn more about how our galaxy came to be.

    The problem is that the Milky Way is enormously vast and incredibly complex, making it far too difficult for any normal computer to simulate.

    In the past, scientists had tried to build bigger and more powerful supercomputers to run more complex simulations.

    However, if the best conventional simulation to date tried to model the Milky Way down to the individual star, it would take 315 hours for every million years of simulated time.

    Simulations of the galaxy are used to test our theories about how stars and supernovae form over time. But these processes are so complex (illustrated) that most simulations would take 315 years to model a billion years of history

    Simulations of the galaxy are used to test our theories about how stars and supernovae form over time. But these processes are so complex (illustrated) that most simulations would take 315 years to model a billion years of history 

    HOW MUCH DOES THE MILKY WAY WEIGH? 

    One solar mass is equivalent to  2 times 10 to the 30th of a single kilogram. 

    The entire galaxy is 1.5 trillion times greater (1.5 multiplied by ten to the power of 12) than this. 

    That means the the sun weighs 3 x 10^42 kg.  

    This equates to 3 x 10^39 tonnes. 

    In non-mathematics, this means the Milky Way's weight is therefore equal to 3,000 trillion trillion trillion tonnes. 

    At this rate, simulating just one billion years of the Milky Way's 13.61-billion-year history would take more than 36 years.

    To solve this problem, lead researcher Dr Hirashima, of the RIKEN Center for Interdisciplinary Theoretical and Mathematical Sciences (iTHEMS), alongside colleagues from the University of Tokyo and Universitat de Barcelona in Spain, tried a new approach.

    Instead of simulating the physics of every single process, the researchers let an AI fill in some of the gaps.

    The 'surrogate' AI was trained on thousands of highly detailed simulations of supernova explosions and learned to predict how the gases would expand over the next 100,000 years.

    By allowing the AI to do much of the heavy lifting, the researchers were able to make their simulation 100 times larger and complete it 100 times faster.

    When they compared their results to simulations painstakingly created on some of the world's largest supercomputers, the researchers found that they matched.

    The researchers charted the movements of 100 billion stars over one million years in just two hours and 47 minutes.

    This means that one billion years of the galaxy's history could be simulated in a mere 115 days, not 36 years.

    By using AI, the researchers' new model could simulate the movements of 100 billion stars over a billion years in just 115 days. This makes it 100 times more detailed and 100 times faster (stock image)

    By using AI, the researchers' new model could simulate the movements of 100 billion stars over a billion years in just 115 days. This makes it 100 times more detailed and 100 times faster (stock image)

    article image

    Dr Hirashima says this new method could mark a 'fundamental shift' in how scientists simulate the galaxy.

    He says: 'This achievement also shows that AI-accelerated simulations can move beyond pattern recognition to become a genuine tool for scientific discovery - helping us trace how the elements that formed life itself emerged within our galaxy.'

    In the future, these same techniques could be used to improve other areas where highly detailed simulations are used.

    That could lead to a better understanding of ocean currents, more accurate models of climate change, and even better weather forecasts.

    HOW DO STARS FORM?

    Stars form from dense molecular clouds - of dust and gas - in regions of interstellar space known as stellar nurseries. 

    A single molecular cloud, which primarily contains hydrogen atoms, can be thousands of times the mass of the sun. 

    They undergo turbulent motion with the gas and dust moving over time, disturbing the atoms and molecules causing some regions to have more matter than other parts. 

    If enough gas and dust come together in one area then it begins to collapse under the weight of its own gravity. 

    As it begins to collapse it slowly gets hotter and expands outwards, taking in more of the surrounding gas and dust.

    At this point, when the region is about 900 billion miles across, it becomes a pre-stellar core and the starting process of becoming a star. 

    Then, over the next 50,000 years this will contract 92 billion miles across to become the inner core of a star. 

    The excess material is ejected out towards the poles of the star and a disc of gas and dust is formed around the star, forming a proto-star. 

    This matter is then either incorporated into the star or expelled out into a wider disc that will lead to the formation of planets, moons, comets and asteroids.

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

    18-11-2025 om 22:29 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART


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