Geen fotobeschrijving beschikbaar.

Geen fotobeschrijving beschikbaar.

Geen fotobeschrijving beschikbaar.

 Geen fotobeschrijving beschikbaar.

Carl Sagan Space GIF by Feliks Tomasz Konczakowski

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

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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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    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.
    19-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.NASA delivers 11MILLION lbs rocket to launch pad as countdown to historic moon mission begins

    The countdown to the first moon mission in more than 50 years officially started Saturday, as NASA rolled out the massive rocket set to blast off in just weeks.

    The 11million pound Artemis II rocket reached the launch pad at the Kennedy Space Center in Cape Canaveral, Florida after nearly 12-hour crawl from its home in NASA's Vehicle Assembly Building.

    The 10-day manned mission to orbit the moon is set to launch as early as February 6, marking the first manned mission to leave low Earth orbit since Apollo 17 in 1972.

    Artemis II will not land on the moon, with NASA saying that the future Artemis III mission scheduled for 2027 will return humans to the lunar surface.

    The space agency said Artemis, 'will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars.'

    The crawler-transporter 2 vehicle carried Artemis II's Space Launch System (SLS) rocket and Orion spacecraft along a four-mile route from an assembly building to Launch Pad 39B.

    At the launch pad, engineers will spend the next few days preparing SLS and Orion for a 'wet rehearsal' test that includes loading all the propellants that will blast the rocket into space.

    NASA Administrator Jared Isaacman said the mission would fulfill 'a promise to the American people that we will return to the moon.'

    Artemis II (Pictured) arrived at NASA's Launch Pad 39B Saturday evening as the space agency prepares for its first moon mission in 53 years

    Artemis II (Pictured) arrived at NASA's Launch Pad 39B Saturday evening as the space agency prepares for its first moon mission in 53 years

    Pictured: The rocket will propel a four-person team, comprised of three NASA astronauts and an astronaut from the Canadian Space Agency, out of Earth's atmosphere as soon as February 6

    Pictured: The rocket will propel a four-person team, comprised of three NASA astronauts and an astronaut from the Canadian Space Agency, out of Earth's atmosphere as soon as February 6

    From L-R: Canadian Space Agency astronaut Jeremy Hansen stands alongside NASA astronauts Christina Koch, Victor Glover and Reid Wiseman. Wiseman will also serve as the mission's commander. The group of four address reporters with the rocket and spacecraft directly behind them

    From L-R: Canadian Space Agency astronaut Jeremy Hansen stands alongside NASA astronauts Christina Koch, Victor Glover and Reid Wiseman. Wiseman will also serve as the mission's commander. The group of four address reporters with the rocket and spacecraft directly behind them

    NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and Canadian Space Agency astronaut Jeremy Hansen are scheduled to briefly orbit the Earth after detaching the Orion spacecraft from its rockets and then set off on their lunar flyby. 

    With Artemis II now at the launching site, NASA will soon load over 700,000 gallons of super-cold liquid hydrogen and oxygen into the SLS rocket, which are the propellants that ignite and blast the craft into orbit.

    NASA will then run through a fake countdown to launch, practice holds and restarts, and then safely drain the tanks of the fuel until it's time for the real launch.

    These rehearsals of the fueling procedures help check for any problems with the rocket, such as leaks in the rocket tanks or valves.

    If any problems are spotted, NASA will likely need to run multiple rehearsals and possibly delay the launch to one of the many alternate dates already chosen by the space agency.

    February 7, 8, 10, and 11 have been chosen as potential backup launch dates if problems or weather issues postpone the February 6 launch. If something prevents a launch in February, NASA has also picked out dates in early March and April.

    In September 2025, former NASA Administrator Sean Duffy publicly announced that 'about a year and a half' after the Artemis II mission, the Artemis III astronaut mission would 'land and establish a long-term presence of life on the moon led by America'.

    He continued by saying that what astronauts learn from the renewed missions to the moon will help in future efforts to 'put American boots on Mars'. 

    Pictured: Early in the morning on Saturday, January 17, NASA begins to move the Artemis II rocket out of the Vehicle Assembly Building at NASA's Kennedy Space Center. Next month, it will be used for the first manned mission to the moon since 1972

    Pictured: Early in the morning on Saturday, January 17, NASA begins to move the Artemis II rocket out of the Vehicle Assembly Building at NASA's Kennedy Space Center. Next month, it will be used for the first manned mission to the moon since 1972


    Over the first 24 to 48 hours in Earth orbit after blasting off, the four astronauts will conduct extensive tests of the Orion spacecraft's life support systems, guidance and navigation computers, and communications before attempting the moon mission. 

    The journey to the moon is scheduled to take about three to four days, ending with the spacecraft conducting a lunar flyby, looping around the far side of the moon roughly 5,500 miles above the surface.

    Artemis II won't enter orbit around the moon, allowing the crew to test deep-space operations and gather data while traveling farther from Earth than any previous human mission.

    The moon's gravity will help slingshot the spacecraft back toward Earth on the return leg of the trip, which will take another three to four days.

    Pictured: The Artemis II rocket sits in the Vehicle Assembly Building prior to its move

    Pictured: The Artemis II rocket sits in the Vehicle Assembly Building prior to its move

    Pictured: The Orion spacecraft sits atop the Artemis II rocket. The spacecraft will carry the astronauts to the moon and back

    Pictured: The Orion spacecraft sits atop the Artemis II rocket. The spacecraft will carry the astronauts to the moon and back

    Pictured: NASA Administrator Jared Isaacman stands with the four astronauts during a press briefing

    Pictured: NASA Administrator Jared Isaacman stands with the four astronauts during a press briefing

    Koch emphasized how important adaptability is for an astronaut, especially since none of them have been to the moon and it's been decades since a mission like this has been undertaken.

    READ MORE

    article image


    'This idea that, yes, you train and prepare for everything, but the most important thing is that you're ready to take on what you haven't prepared for,' Koch said.

    'The moon is like a witness plate for everything that's actually happened to Earth but has since been erased by our weathering processes and our tectonic processes and our other geologic processes,' the astronaut continued.

    'We can actually learn more about solar system formation, more about how planets form maybe around other stars, more about the likelihood of life out there - starting with studying the moon.'

    At the end of the mission, Artemis II will splash down in the Pacific Ocean, and the spacecraft and crew will be recovered with the help of the US Navy.


    NASA mega-rocket for moon mission could launch in weeks

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

    19-01-2026 om 18:38 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.Hidden portals in Earth's magnetic field

    Hidden portals in Earth's magnetic field

    It turns out that they do, sort of, and a NASA-funded researcher at the University of Iowa has figured out how to find them.

    "We call them X-points or electron diffusion regions," explains plasma physicist Jack Scudder of the University of Iowa.  "They're places where the  of Earth connects to the magnetic field of the Sun, creating an uninterrupted path leading from our own planet to the sun's atmosphere 93 million miles away."

    Observations by NASA's THEMIS spacecraft and Europe's Cluster probes suggest that these magnetic portals open and close dozens of times each day.  They're typically located a few tens of thousands of kilometers from Earth where the geomagnetic field meets the onrushing solar wind.  Most portals are small and short-lived; others are yawning, vast, and sustained.  Tons of energetic particles can flow through the openings, heating Earth's upper atmosphere, sparking geomagnetic storms, and igniting bright polar auroras.

    NASA is planning a mission called "MMS," short for Magnetospheric Multiscale Mission, due to launch in 2014, to study the phenomenon. Bristling with energetic particle detectors and magnetic sensors, the four spacecraft of MMS will spread out in Earth's magnetosphere and surround the portals to observe how they work.

    Just one problem:  Finding them.  Magnetic portals are invisible, unstable, and elusive.  They open and close without warning "and there are no signposts to guide us in," notes Scudder.

    Actually, there are signposts, and Scudder has found them.

    Portals form via the process of magnetic reconnection.  Mingling lines of magnetic force from the sun and Earth criss-cross and join to create the openings. "X-points" are where the criss-cross takes place.  The sudden joining of magnetic fields can propel jets of charged particles from the X-point, creating an "electron diffusion region."

    To learn how to pinpoint these events, Scudder looked at data from a space probe that orbited Earth more than 10 years ago.

    "In the late 1990s, NASA's Polar spacecraft spent years in Earth's magnetosphere," explains Scudder, "and it encountered many X-points during its mission."

    Because Polar carried sensors similar to those of MMS, Scudder decided to see how an X-point looked to Polar. "Using Polar data, we have found five simple combinations of magnetic field and energetic particle measurements that tell us when we've come across an X-point or an electron diffusion region. A single spacecraft, properly instrumented, can make these measurements."

    This means that single member of the MMS constellation using the diagnostics can find a portal and alert other members of the constellation. Mission planners long thought that MMS might have to spend a year or so learning to find portals before it could study them.  Scudder's work short cuts the process, allowing MMS to get to work without delay.

    It's a shortcut worthy of the best portals of fiction, only this time the  are real. And with the new "signposts" we know how to find them. 

    The work of Scudder and colleagues is described in complete detail in the June 1 issue of the Physical Review Letters.

    A new ScienceCast video explains how hidden portals form--and how we can find them.

    RELATED VIDEOS

    https://phys.org/space-news/ }

    19-01-2026 om 16:43 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.Fly over the 'Grand Canyon' of Mars in high-resolution orbiter imagery

    Fly over the 'Grand Canyon' of Mars in high-resolution orbiter imagery

    See the 2,500 mile-long (4000 km) Valles Marineris in imagery captured the Mars Reconnaissance Orbiter. Global topography: NASA/GSFC CTX global mosaic: NASA/MSSS/Caltech/ CTX topography: NASA/MSSS/USGS HiRISE: NASA/U.Arizona/USGS/Amazon

    { https://www.msn.comid=nl_articl/ }

    19-01-2026 om 16:15 geschreven door peter  

    0 1 2 3 4 5 - Gemiddelde waardering: 0/5 - (0 Stemmen)
    Categorie:ASTRONOMIE / RUIMTEVAART
    18-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.What interesting phenomena did the New Horizons spacecraft encounter on its way to Pluto?

    What interesting phenomena did the New Horizons spacecraft encounter on its way to Pluto?

    Tweny years ago, the New Horizons spacecraft launched from Cape Canaveral. Eight and a half years later, the whole world was talking about it when it transmitted the first-ever close-up images of Pluto’s surface back to Earth. However, its adventures actually began much earlier.

    New Horizons spacecraft.
    Source: www.space.com

    Who is interested in Pluto?

    January 19 marks the 20th anniversary of the launch of the Atlas 5 rocket from the US Space Force base, which carried the New Horizons spacecraft beyond Earth’s gravitational sphere. Nowadays, it is mainly talked about in connection with the discoveries it made during its brief flyby of Pluto.

    However, in reality, the interesting adventures of the probe designed to explore Pluto began long before the summer of 2015 and even long before its launch, although these adventures were a little unusual.

    First, it should be noted that the first spacecraft could have reached Pluto several decades earlier. Voyager 1 could well have been that spacecraft. At least in the 1970s, during the mission planning stage, there was an idea to perform a gravitational maneuver during the flyby of Saturn, which would allow the probe to be directed towards the object that was then considered the ninth planet of the Solar System in a few years.

    Voyager-1 could have been the first spacecraft to fly by Pluto.
    Source: www.planetary.org

    However, at that time, Pluto was considered too distant and uninteresting, so preference was given to a trajectory that allowed for better exploration of Saturn’s largest moon, Titan. However, over the next 15 years, everything changed dramatically. In 1978, Pluto’s moon Charon was discovered, unusually large and close to the planet, and in 1985, its atmosphere was discovered. All this was already worth launching a spacecraft to what seemed at the time to be the most distant body in the Solar System.

    In 1989-90, NASA established a working group that developed a project called Pluto 350. It was supposed to be a truly epic mission, designed to last 15 years. Initially, the spacecraft was to head for Venus and Mercury to gain speed, then perform another gravitational maneuver near Jupiter, and only then head for Pluto.

    Such a cunning plan was necessary because the speed that can be achieved by the spacecraft during launch is quite limited, and the entire time it flies to Pluto, the Sun’s gravitational pull will slow it down. It will reach its destination, but it will take several decades.

     of Trajectorythe New Horizons spacecraft

    That is why, without an intermediate point in the form of Jupiter, which, with the right calculations, can be turned into acceleration, it is impossible to do without. But 15 years was still too long, so NASA’s Jet Propulsion Laboratory developed another plan called Pluto Fast Flyby. It involved flying two small spacecraft for a total of seven years and performing a gravitational maneuver near Jupiter. In fact, this plan was later implemented during the New Horizons mission.

    Is the flight to Pluto justified?

    However, at that very moment, in 1993, after the loss of Mars Observer, the number of people willing to pay $1 billion – the estimated cost of the mission to Pluto at the time – dropped sharply. Instead, scientists’ interest only grew. The fact is that in 1987, the planet passed its equinox, and in 1989, it passed its perihelion, i.e., the point in its orbit closest to the Sun.

    In addition, Pluto’s orbit is not only highly elongated but also significantly inclined to the ecliptic. This means that the most favorable moment for launching a spacecraft from Earth was in the second half of the 1980s. This crazy celestial body completes a full revolution around the Sun in 247 years.

    Pluto’s orbit.
    Source: astrobites.org

    This means that with each passing year, the spacecraft’s flight path would become longer and higher above the plane in which the rest of the planets in the Solar System revolve. This would mean higher costs and less equipment that could be delivered to the target.

    In an attempt to save the mission, a desperate option was proposed: it would be launched by a Russian rocket, and Germany would provide funding in exchange for the opportunity to place its own sub-probe on board. The plan was to drop it onto one of Jupiter’s moons as the spacecraft flew through the gas giant’s system.

    So, in discussions about the flight to Pluto, the topic arose that on its way there, the spacecraft should not only “sleep” but also explore something interesting as it flew past. But the plan did not work out, and in the mid-1990s, the project was abandoned.

    Pluto Kuiper Express.
    Source: Wikipedia

    But not for long, because at that very moment, more and more new objects began to be discovered beyond Neptune’s orbit. The flight plan to Pluto was taken out of the drawer again and supplemented with a section in which, after exploring the planet, the probe was to fly further and take a closer look at one of the newly discovered asteroids.

    The mission was renamed Pluto Kuiper Express, and only one of the two previously planned spacecraft remained, but this did not help the project. In 1999, it was rejected again. But this time, the public was on the side of the scientists, and soon NASA had to announce a new competition, which the New Horizons won: the Shedding Light on Frontier Worlds project from the Johns Hopkins University Applied Physics Laboratory. It was this project that was implemented.

    New Horizons design

    Ready for launch, the spacecraft weighed 478 kg, of which 77 kg was fuel, and was about the size of a small car. It was propelled by four main rocket engines and 12 orientation engines. All of them ran on hydrazine as a single fuel.

    The payload consisted of a whole set of scientific instruments. The Alice camera provided observation of objects and spectroscopy in the ultraviolet range, Ralph performed similar studies in the infrared part of the spectrum, and the main LORRI telescope was responsible for the visible range.

    NewHorizons collection.
    Source: Wikipedia

    Also on board were the SWAP solar wind analyzer and PEPSSI. These two instruments captured all the high-energy particles that New Horizons encountered during its flight. They were designed to answer the question of how strongly solar radiation affects objects at such a distance from the sun.

    The VBSDC device was responsible for studying much larger particles that the spacecraft might encounter. Also on board was the REX radio spectrometer, designed to study Pluto’s atmosphere by measuring the signal from Earth as it passed through it.

    All of this was controlled by the onboard computer. Signals were sent to it from Earth via a communication system. Inside New Horizons, the temperature was maintained between 10 and 30°C.

    All this required a lot of energy. Solar batteries could not be used due to Pluto’s considerable distance from the Sun. Therefore, a radioisotope thermoelectric generator with 72 plutonium “pills” was used to power New Horizons. It provided 245 watts of power.4

    New Horizons radioisotope thermoelectric generator.
    Source: Wikipedia

    Flight to Pluto

    When New Horizons finally launched into space on January 19, 2006, it was launched using the most powerful modification of Atlas 5, called 551. It has five solid-fuel boosters. Thanks to this, the spacecraft was able to accelerate to 12.4 km/s. Then the acceleration unit kicked in, bringing the speed up to 16.207 km/s.

    New Horizons headed for Jupiter, but only reached it a year later, in February 2007. A lot happened during that time. Back in February 2006, engineers tested the spacecraft’s cameras and used them to photograph an asteroid that at the time was known only by its number, 132524. The distance to it was then 102,000 km. Thus, at the beginning of its mission, the spacecraft enriched our collection of celestial bodies photographed from close range.

    However, on August 24 of the same year, an event occurred that was significantly less pleasant for the spacecraft team. The 26th General Assembly of the International Astronomical Union adopted a new classification of bodies in the Solar System. The reason for this was the discovery of new bodies beyond Neptune’s orbit, which gave new impetus to the study of Pluto.

    Lava fountain above Io.
    Source: Wikipedia

    Ironically, under the new classification, Pluto was classified not as a large planet but as a dwarf planet. Eris’s discoverer, Michael Brown, was openly delighted about this. However, New Horizons team leader Alan Stern called the new classification complete nonsense.

    This assessment is not surprising. If the new classification had been adopted a few years earlier, it would have been difficult for the New Horizons team to prove the importance of the project. However, the spacecraft was already flying in space and in September 2007 even began observing Jupiter.

    The flyby itself, with its gravitational maneuver, took place in February 2007, and it was an extremely successful moment in terms of raising the mission’s prestige. Some spacecraft had already completed their exploration of the largest planet in the Solar System at that time, while others were still on their way to it. New Horizons turned out to be its main explorer.

    Arrokoth.
    Source: Wikipedia

    The probe took numerous photographs of the planet itself and its moons. The images of the four largest moons were particularly interesting, as it photographed a lava fountain on Io shooting hundreds of kilometers into space. Jupiter’s atmosphere and magnetosphere were also studied.

    The mission continues

    After flying past Jupiter, New Horizons went into “sleep” mode. Every two to three months, engineers would wake it up and check the systems. This continued until it approached Pluto. Then the whole world started talking about the probe, and this lasted for several weeks. And then, like any sensation, it disappeared from the public eye again.

    But the spacecraft’s scientific mission did not end there. It continued to explore trans-Neptunian objects and on January 1, 2019, flew past the asteroid Arrokoth, photographing and studying it. This is the first study of such a body, and it is thanks to it that we know what the outskirts of the Solar System look like.

    And the New Horizons mission continues. The radioisotope generator is expected to operate until at least 2035. We can expect that it will make many more discoveries before then.

    RELATED VIDEOS

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

    18-01-2026 om 23:10 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.The race for reusability and the flight to the Moon: the most anticipated space events of 2026
    The race for reusability and the flight to the Moon: the most anticipated space events of 2026

    The year 2026 should bring us many interesting events that will go down in the annals of world space exploration, from the first manned flight to the Moon in more than half a century to new Starship tests. Here are the main space expectations for the year.

    The Artemis II mission

    The Artemis II mission will likely be the most high-profile event of 2026. And there is hardly any need to explain why. After all, this will be the first manned flight beyond Earth’s orbit in 54 years, during which humanity will once again touch the Moon.

    The Artemis II mission (concept).
    Source: NASA

    The flight plan is as follows. The super-heavy SLS rocket will launch the Orion spacecraft with four astronauts (three representing NASA and one representing the Canadian Space Agency) into Earth orbit. After making sure that all systems are operating normally, the crew will perform a maneuver that will put the spacecraft on a trajectory for a free flyby of the Moon.

    On the sixth day of the flight, Orion will fly around the Moon (the minimum approach distance will be approximately 7,400 km), after which it will turn back toward Earth under the influence of the Moon’s gravity. This will eliminate the need for the expedition to use engines to change course, which should reduce the risks for the expedition. On the tenth day of the flight, the capsule with four astronauts will enter the Earth’s atmosphere and splash down.

    The Artemis II mission flight plan.
    Source: NASA

    Of course, flying around the moon is not the same as landing on it. But still, it is difficult to deny the symbolic significance of this mission. Since the Apollo program, several generations have grown up without seeing humans fly to other celestial bodies. The flight to the Moon will clearly help to raise interest in space exploration and astronautics. Artemis II will also mark the beginning of the next stage in the new lunar race between the US and China. At the moment, the launch of the mission is scheduled for February – March 2026.

    The new Starship

    As in previous years, the attention of all space enthusiasts will be focused on Starship. This year, SpaceX plans to begin testing a new, even more powerful modification of the super-heavy rocket, designated V3. Its first flight is tentatively scheduled for February. It will follow the same pattern as previous tests.

    Transporting Starship to the launch pad.
    Source: SpaceX

    If V3 proves to be a more reliable rocket than its predecessor, SpaceX will begin working on the next key elements needed to transform Starship from an experimental to a working system. These include reaching orbit, landing on land, and orbital refueling.

    The last element is critical for the Artemis program. Without a functioning orbital refueling system, SpaceX will not be able to fulfill its obligations to NASA. As a reminder, as part of the Artemis III mission, the Starship HLS lander, which will be refueled in near-Earth orbit by tanker ships, is to land two astronauts at the south pole of the Moon.

    Given the complexity and ambition of the project, it is extremely difficult to predict how successful the V3 tests will be. But one thing is certain – they will remain one of the main events of the year.

    The race for reusability

    For almost ten years, SpaceX was the only company with a partially reusable orbital rocket. This allowed it to take an unprecedented position in the global launch market and start building the Starlink system, which not so long ago seemed like science fiction.

    The first stage of the New Glenn rocket after landing on a barge.
    Source: Blue Origin

    But in 2025, the situation began to change. Blue Origin became the second company in history to successfully return a rocket stage from space. The Chinese company LandSpace and the China Aerospace Science and Technology Corporation made their first attempts to land the stages of their Zhuque-3 and Long March 12A rockets. They failed – but it is clear that this is only the beginning. In 2026, they will make new attempts to return to the stages.

    New rockets will also join the reusability race. Rocket Lab intends to launch its first medium-class Neutron carrier rocket. It features an interesting “sliding” nose cone design, which allows it to be returned to Earth together with the stage.

    Artist’s impression of the Neutron rocket.
    Source: Rocket Lab

    There are also plans to debut several other rockets with reusable first stages. These include Terran-R, Hyperbola-3, Long March 10A… Yes, the launch dates for most of them may subsequently be postponed until next year. And those rockets that do fly are unlikely to be able to return to Earth on their first attempt. Nevertheless, 2026 will likely bring us new reusable launch vehicles.

    The first private orbiting station

    For many years, discussions about private orbital stations did not go beyond attractive promises and concepts. Bigelow came closest to achieving this goal, even launching an experimental inflatable module that became part of the ISS. However, the company subsequently went bankrupt.

    Artist’s impression of the Haven-1 orbital station.
    Source: Vast

    Nevertheless, in 2026, we may witness the launch of the first private orbital station in history. Vast Space is attempting to accomplish this task.

    Vast Space first announced its plans to build the Haven-1 orbital station in 2023. Its main difference from similar projects, which never made it past the drawing board, is its relative simplicity. While other companies typically announce complex multi-module orbital stations, Haven-1 will consist of just one 14-ton compartment with an internal volume of 80 m³, not designed for permanent human habitation. The station will rely on the Crew Dragon spacecraft’s life support system and will be able to accommodate four astronauts for 30 days.

    Welding of the main body of Haven-1 has been completed. Vast Space is currently actively testing it, as well as various components of the future station, such as solar panels and the docking mechanism.

    Haven-1 orbital station on a test bench.
    Source: Vast

    Vast Space hopes to launch its station sometime in the second half of 2026. Of course, given the ambitious nature of the task, the date may change. It cannot be ruled out that the launch of Haven-1 will ultimately be postponed until 2027. But we hope that the wait will not be too long. The first commercial orbital station will clearly be a powerful stimulus for other similar projects and will accelerate their implementation.

    Events in deep space

    In 2026, we can also expect many interesting events in deep space. Four private missions to the Moon are planned (Blue Moon Pathfinder Mission 1, IM-3, Griffin Mission One, Blue Ghost Mission 2). China will also send its mission to our planet’s satellite. We are talking about Chang’e-7, which has a very complex architecture, including a relay satellite, a lander, a rover, and even a flying drone. It is scheduled to land on the south pole of the Moon at the end of 2026.

    Selfie taken by the Tianwen-2 spacecraft.
    Source: CNSA

    During 2026, we will also see several objects in the Solar System up close for the first time. In June, the Chinese Tianwen-2 mission will enter orbit around the asteroid Kamoʻoalewa. It is a quasi-satellite of Earth and is believed to be a fragment of the Moon that was knocked out as a result of some collision.

    In June, the Japanese spacecraft Hayabusa2 will fly past the asteroid Torifune. And in December, the European spacecraft Hera will reach the double asteroid Didymos. In 2022, the DART probe crashed into its satellite Dimorph. In this way, NASA tested whether such an impact could change the orbit of a celestial body (in the future, this technology could be used to deflect dangerous objects away from Earth). Hera will carefully study Didymos and Dimorph to gather as much information as possible about how the impact affected the pair.

    The Hera mission as imagined by an artist.
    Source: ESA

    The launch of the Japanese MMX mission is also planned for the end of 2026. Its goal will be to deliver a sample of Phobos material to Earth. Along with it, a pair of ESCAPADE probes will travel to Mars, which are currently monitoring space weather at one of the Lagrange points. The European-Japanese BepiColombo mission will finally enter a permanent orbit around Mercury. After that, it will split into two separate spacecraft, which will begin studying the first planet from the Sun.

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

    18-01-2026 om 22:49 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    17-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Astronomers Have Uncovered a “Definitive Clue” to the Origin of Mysterious Fast Radio Bursts Originating from Binary Stars

    sky eye fast radio burst

    Credit: Y. Liu, X. Yang, Y.F. Liang, W.L. Zhang and Y. Li (PMO).

    Astronomers Have Uncovered a “Definitive Clue” to the Origin of Mysterious Fast Radio Bursts Originating from Binary Stars

    For the first time, astronomers have discovered clear evidence that some fast radio bursts (FRBs) are emitted by binary stars, according to an international team of researchers.

    The powerful yet brief bursts of radio waves emanate from distant galaxies and have puzzled scientists for some time, until a general consensus emerged that they are produced by isolated, single stars.

    Now, a recent paper published in Science challenges that idea, based on observations of FRB 220529A made possible by the Five-hundred-meter Aperture Spherical Telescope (FAST), also known as China’s Sky Eye, which demonstrates that binary systems can produce FRBs.

    The China Sky Eye

    Located in southwestern China’s Guizhou province, FAST is also nicknamed “Tianyan,” which translates to “Heaven’s Eye” or “Sky Eye.” The radio telescope features a 1,640-foot-diameter dish, making it the largest single-dish telescope in the world, nestled within a natural depression.

    The bright, millisecond-long flashes known as FRBs travel to us from distant galaxies. Generally, they are singular events, but the rare repeaters offer scientists intriguing opportunities to study the phenomena over longer periods and observe changes. Since 2020, Professor Bing Zhang has co-led a program to study these repeating FRBs. They found something remarkable in FRB 220529A, located 2.5 billion light-years from Earth.

    “FRB 220529A was monitored for months and initially appeared unremarkable,’ said co-author Professor Bing Zhang. ‘Then, after a long-term observation for 17 months, something truly exciting happened.” The researchers used FAST to monitor the FRB for 20 months, eventually revealing that the source had a companion star.

    Fast Radio Burst Polarization

    Analyzing a radio wave’s polarization properties offers important clues about its source’s surroundings. In this FRB, the most notable feature was a sudden and dramatic polarization change known as an RM flare, indicative of a coronal mass ejection from a companion star interfering with the burst source.

    “This finding provides a definitive clue to the origin of at least some repeating FRBs,” said co-author Professor Bing Zhang, Chair Professor of Astrophysics of the Department of Physics and Founding Director of the Hong Kong Institute for Astronomy and Astrophysics at HKU. “The evidence strongly supports a binary system containing a magnetar—a neutron star with an extremely strong magnetic field, and a star like our Sun.”

    An FRB’s linear polarization allows researchers to track its journey through space. Due to the Faraday rotation effect, a radio wave’s polarization angle rotates when it travels through magnetized plasma. That rotation can be precisely measured using a quantity called a rotation measure (RM).

    “Near the end of 2023, we detected an abrupt RM increase by more than a factor of a hundred,” said lead author Dr Ye LI of Purple Mountain Observatory and the University of Science and Technology of China. “The RM then rapidly declined over two weeks, returning to its previous level. We call this an ‘RM flare’.”

    Binary Sourced Fast Radio Bursts

    A brief RM change like this is consistent with the FRB having intercepted a dense magnetized plasma, likely ejected from a companion star.

    “Such a model works well to interpret the observations,” said co-first author Professor Yuanpei Yang, a professor from Yunnan University. “The required plasma clump is consistent with CMEs launched by the Sun and other stars in the Milky Way.”

    Directly observing the companion star over these billions of light-years was not feasible, but FAST and supplemental observations from the Parkes telescope in Australia successfully confirmed its presence.

    “This discovery was made possible by the persevering observations using the world’s best telescopes and the tireless work of our dedicated research team,” said co-lead author Professor Xuefeng Wu of Purple Mountain Observatory and the University of Science and Technology of China.

    The work supports a proposal by Professor Bing Zhang that FRBs are generated by magnetars and that binary systems produce a geometry that allows bursts to occur more frequently, and marks the beginning of ongoing studies required to determine how common binary systems are as sources of FRBs.

    The paper, “A Sudden Change and Recovery in the Magnetic Environment Around a Repeating Fast Radio Burst,” appeared in Science on January 15, 2025.

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

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

    17-01-2026 om 20:05 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    16-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Why Mars is Actively Manufacturing Poison

    Why Mars is Actively Manufacturing Poison

    Model of the chemical cycle on Mars that is driven by the electrostatic discharges of dust storms. Credit - WUSL
    Model of the chemical cycle on Mars that is driven by the electrostatic discharges of dust storms.
    Credit - WUSL

    Chemistry on other worlds varies widely from that on Earth. Much of Earth’s chemistry is driven by well-understood processes, which typically involve water and heat in some form. Mars lacks both of those features, which makes how some of its chemicals formed a point of ongoing debate in the scientific community. A new paper led by Alian Wang and Neil Sturchio of Washington University of St. Louis and the University of Delaware, respectively, and published recently in Earth and Planetary Science Letters offers a new framework for understanding chemical reaction processes on Mars. Despite the differences, Earthlings will still be familiar with the driving force behind Martian chemistry - electricity.

    Various rovers and orbits on and around Mars have noticed a peculiar isotopic imbalance on the surface of the Red Planet. An isotopic imbalance can occur when the ratio of two different isotopes of a particular element is skewed from the natural ratios expected. In particular, “heavy” isotopes of some of the most common elements - chlorine, oxygen, and carbon, seem to be lacking on Mars.

    For example, Chlorine-37, the “heavy” isotope of that particular element, is 51 parts per thousand (ppt) less abundant than would otherwise be expected on the Martian surface. Given that it is a key ingredient in the hazardous “perchlorates” that stand as one of the major challenges to long-term biological systems living on Mars (like humans), understanding why that imbalance has occurred is key to understanding how we might mitigate the threat those chemicals represent.

    Fraser discusses an idea to treat Mars of its toxic perchlorates.

    The heavy isotope imbalance for carbon (11.4 ppt) and oxygen (22.8 ppt) are less pronounced, but no less important. Both are key ingredients for the formation of carbonates, which previous generations of scientists thought were evidence of previous liquid water on the planet’s surface. So what is causing these imbalances? And what does electricity have to do with it?

    Another common feature of Mars’ surface are its famous dust storms. These massive storms take up a significant amount of the planet’s surface in certain seasons. They also form mini-vortices that look like miniaturized tornadoes. Importantly, those storms, and especially those vortices, cause Martian dust they kick up to rub together, eventually building up an electrostatic charge, similar to what happens when you rub a balloon on your head.

    But in Mars’ weaker atmosphere, it’s relatively easy to overcome the dielectric constant of the atmosphere itself, allowing small “arcs” that are familiar to anyone who has played under a blanket in a dry room at night. These arcs, known technically as electrostatic discharges, or ESDs, are the driving force of one of the primary chemical cycles on Mars, according to the new paper.

    Fraser talks about how a realistic mars mission will play out.

    The authors built several test chambers, including the Planetary Environment and Analysis Chamber (PEACh), specifically to test how salts commonly found on Mars would react to the electricity produced during a dust storm. They found the ESDs that happen in dust storms create high-energy electrons that run into the CO2 that comprises the Martian atmosphere. When they do so, they create reactive radicals like CO and O. These free radicals then fall to the chloride salts that exist on the ground, bonding oxygen to them, and changing chlorine to perchlorates, the deadly substance carbon-based lifeforms would rather avoid.

    But it does explain where they came from. The same process happens for carbonates, which were commonly thought to be formed by liquid water. But like their chlorinated cousins, it seems a wide variety of Mars-based chemicals can form with nothing other than static shocks during a dust storm.

    This data matches up much more closely with in-situ and remote observations - in particular the lower density of “heavy” isotopes they’ve found. ESD acts like a “filter”, selecting the lighter atoms to participate in chemical reactions that form the compounds rovers like Curiosity and orbiters like ExoMars have captured. The actual physics behind that process is complicated, but needless to say, this idea that chemical cycles on Mars are driven by dust-derived electrical discharge seems to fit the data very well.

    Video of dust devils captured on Mars by Curiosity. These are the types of storms that create ESDs, which then create perchlorates and carbonates on the Martian surface.

    Such electrical-driven reactions have applications on more than just Mars. Venus, some of the outer Gas Giants, and even our own Moon, could have their own version of ESD-driven chemical reaction chains. While that means there’s plenty more to study, there’s also a cautionary tale for future Martian explorers. ESD is an ongoing, active process that is part of Mars’ natural, cold climate. That means that perchlorates, the deadly chemicals that might very well hinder our tentative efforts at a permanent base on the Red Planet, are constantly being created there.

    While that’s certainly not a deal breaker for exploration, it is something we need to be aware of. But the authors certainly aren’t done with their exploration of the impact that small arcs of electricity have on driving chemical reactions throughout the solar system. Expect more papers about how arcs on Venus affect that planet’s surface chemistry soon.

    Learn More:

    https://www.universetoday.com/ }

    16-01-2026 om 23:24 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.NASA Enters Final Preparations for Artemis II Mission

    NASA Enters Final Preparations for Artemis II Mission

    Inside high bay 3 of NASA’s Vehicle Assembly Building at NASA's Kennedy Space Center, the SLS (Space Launch System) for NASA Artemis II stands fully stacked as the retractable platforms pull away. Credit: NASA
    Inside high bay 3 of NASA’s Vehicle Assembly Building at NASA's Kennedy Space Center, the SLS (Space Launch System) for NASA Artemis II stands fully stacked as the retractable platforms pull away.
    Credit: NASA

    Between February and April of this year, NASA will conduct its first crewed mission beyond Low Earth Orbit (LEO) in over fifty years. At 09:41 p.m. EST (06:41 p.m. PDT), the Artemis II crew will launch aboard their Orion spacecraft atop the Space Launch System (SLS) from Launch Pad-39B at the Kennedy Space Center in Florida. With the launch date rapidly approaching, NASA is entering the final stages of preparation, including the rollout of the SLS and Orion to the launch pad for the first time. This will be followed by the final integration and testing of the rocket and spacecraft, then launch rehearsals.

    The Artemis II crew consists of NASA astronauts Reid Wiseman (commander), Victor Glover (pilot), and Christina Koch (mission specialist), and Canadian Space Agency (CSA) astronaut Jeremy Hansen (mission specialist). Building on the success of the uncrewed Artemis I mission, *Artemis II* will see this crew execute a circumlunar flight, taking them around the Moon without landing and returning them to Earth. The entire mission will take 10 days and will be the curtain-raiser for the first crewed mission to the lunar surface since Apollo 17 landed there in 1972.

    The rollout is targeted for no earlier than this Saturday (Jan. 17th) and will take up to 12 hours for the rocket and crawler-transporter-2 to travel the ~6.5 km (4 mi) that lie between the Vehicle Assembly Building and Launch Pad 39B. "We are moving closer to Artemis II, with rollout just around the corner," said Lori Glaze, acting associate administrator for NASA’s Exploration Systems Development Mission Directorate (ESDMD). "We have important steps remaining on our path to launch, and crew safety will remain our top priority at every turn, as we near humanity’s return to the Moon."

    Teams are currently working around the clock to complete all remaining tasks ahead of the rollout, a process that has been ongoing for months. In December, during a countdown demonstration test, engineers detected a problem with a valve associated with the Orion capsule's hatch pressurization. They replaced the valve on Jan. 5th, which was followed by a successful pressure test. They also resolved a leak with the ground support hardware that is part of the loading system for pressurizing the Orion with oxygen gas. The work will continue for weeks after the SLS and Orion roll out to the launch pad.

    At this point, ground crews will begin connecting electrical lines, fuel-control-system ducts, cryogenic propellant feeds, and other ground-support equipment. They will then power up all of the rocket's integrated systems for the first time to ensure they work properly with each other, the mobile launcher, and the launch pad infrastructure. The final preparation, scheduled for the end of January, will consist of a prelaunch fuel test (aka a "wet dress rehearsal") where NASA will fuel the rocket with about 2.65 million liters (700,000 US gallons) of cryogenic fuel into the rocket, conduct a launch countdown, then safely unload it.

    Several countdowns are scheduled to allow mission controllers to hold, resume, and recycle back to previous times in the final 10 minutes before liftoff (aka terminal count). Several lessons from the previous mission have been integrated into this launch's preparations, including the challenges ground crews experienced while loading liquid hydrogen propellant during Artemis I's wet dress rehearsal. So in addition to carefully watching the propellant loading process, the ground teams will also closely monitor the effectiveness of recently updated procedures that limit how much nitrogen gas accumulates between the Orion crew module and the launch abort system.

    Additional wet dress rehearsals may be required to make sure the vehicle is ready for flight, and NASA may opt to roll the SLS and Orion back into the VAB for additional work (as they did with Artemis I). Following a successful wet dress rehearsal, NASA's mission management team will convene a "flight readiness review" to assess the readiness of all systems before committing to a firm launch date. Once all of this is complete, and in what will be a major media event, the Artemis II astronauts will conduct a final walkdown at the pad.

    While the Artemis II launch window opens as early as Friday, Feb. 6th, the mission management team may push the launch to a date before the window closes (no later than April). These launch opportunities require that the planned trajectory account for the complex orbital mechanics of Earth and the Moon. Basically, the rotation of the Earth and the Moon's orbit result in a pattern of approximately a week of launch opportunities, followed by three weeks without. The opportunities between February and April (subject to change) are available here.

    NASA and its partners have high expectations for the Artemis II test flight. Much like the Apollo 10 mission, which was a dress rehearsal for the first landing on the Moon, this mission will provide the necessary experience and validate the systems that will allow humans to return to the lunar surface after more than 50 years. Currently scheduled for 2028, Artemis III will last for about 30 days and will depend on the development of the Human Landing System (HLS).

    Further Reading: 

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    https://www.universetoday.com/ }

    16-01-2026 om 23:14 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.How DARPA, Star Trek, and UFOs Inspired This Engineer to Unravel the Secrets to Warp Drive Propulsion

    How DARPA, Star Trek, and UFOs Inspired This Engineer to Unravel the Secrets to Warp Drive Propulsion

    Warp drive propulsion, the hypothetical means by which advanced spacecraft of the future may one day explore the universe by way of superluminal travel, has its origins as a concept in science fiction. Best known for its appearances in the famed 1960s TV series Star Trek, it wasn’t until 1994, when a Mexican mathematician named Miguel Alcubierre laid out the mathematics of warp theory, that some scientists–and at least one engineer–began to take the concept seriously.

    Since then, a handful of experts have tried to improve on those theories, including former NASA engineer Dr. Harold G “Sonny” White. Until now, all of those ideas have remained mathematical theories that are particularly difficult–if not impossible–to construct with today’s technology.

    More recently, an international think-tank of over 30 physicists called Applied Physics has inched closer to a working concept by laying out the math behind what they call a physical warp drive. But in order to overcome many of the energy violations that have haunted previous efforts, their concept is unable to go faster than the speed of light.

    Of course, traveling at 90% light speed would make trips to other planets possible. But even this potentially breakthrough design (dubbed the Martire-Bobrick warp drive for the two authors behind the concept Alexey Bobrick and Gianni Martire) is still purely theoretical.

    Now, a new player has entered the fray, and unlike most of the others working in this field, he says he is ready to run an experiment on his theory right now. Ladies and gentlemen, meet the university professor and Provost of the University of Houston-Victoria, and the man who may finally crack the warp drive puzzle, Dr. Chance Glenn.

    The Engineer

    warp drive propulsion

    Dr. Chance Glenn recently won the 2022 Permission to Dream Award at the Space Cowboy Ball in Austin, Texas, an award previously given to Jeff Bezos. The award was presented by SpaceX’s Gwynne Shotwell, who also won an award

    (Credit: Thomas Colvin/University of Houston-Victoria).

    “I’m a huge Star Trek lover,” the impressively calm and cool Glenn told The Debrief when discussing his interest in warp drive. “I was drawn by the future that it projects.”

    Glenn says he is partial to the original series “by far” and has identified with one character in particular.

    “Mr. Spock is my guy,” said Glenn. “I tried to be him.”

    Like Spock, Glenn is undoubtedly left-brained, having earned a number of degrees in electrical engineering, including a Masters and a Ph.D. from Johns Hopkins University. But unlike Mr. Spock, Glenn embraces his creative side as well, including writing and recording music. He says that he actually knows of many engineers like himself that are drawn to the mathematical nature of music and that he often finds unexpected inspiration for his engineering work when creating a tune. Although he didn’t say so, one could almost imagine the theme of Star Trek The Original Series playing in the background when he decided to take a look at warp drive.

    “I took a closer look at (Einstein’s Theory) General Relativity and all of that,” said Glenn, which led him to try to work out exactly how one would go about building a warp drive. Oh yeah, and the massive media coverage around UFOs over the last few years had an impact as well.

    “There was actually some DARPA research a few years ago where they were actually looking at this,” explained Glenn, “and it may even intersect with this seriousness that DOD and NASA have gotten around UFOs, or UAPs, to see how were they doing it? If there are vessels flying around, how are they doing it? So that got my interest”

    The first thing Glenn noticed was the massive amounts of negative energy required in the faster-than-light concepts, including the more popular models of Alcubierre and White, as well as those published by Dr. Eric Lentz.

    “I said, ‘well, if the shaping function was complex, with a larger imaginary part, then it would make all of the energy density requirements positive,’” Glenn told The Debrief. “And I modeled that and got some results that are positive. That’s what’s shown in the paper.”

    Of course, being an engineer at heart and by trade, Glenn knew he would have to go beyond simple theory if, as Captain Picard might say, he was going to “make it so.”

    “Mathematics and all of that is cool,” Glenn said with a sly grin, “but there is nothing like proving it.”

    The Proof

    According to Glenn, he labored for some time to come up with a viable way to test his new theory before landing on a class of material known as dielectrics.

    “I know from my RF (radio frequency) background that dielectrics can be complex,” Glenn told The Debrief. “So if you put an RF signal through a dielectric material, that could be a way to implement this, implement a shaping function, having whatever characteristics you want.”

    He says he found this approach particularly intriguing since it seemed to address the negative energy issue. And he says, he didn’t see anyone else taking this route.

    “The difference (between his model and others) is, I’ve identified a material which I think can take us there, and that mathematically fits what the equations are saying,” Glenn told The Debrief. “A lot of the (warp theories) out there haven’t speculated actually how they would do these things,” he added. “Nobody has looked at it that way that I was able to find.”

    The self-described ‘engineer with a physicist’s heart’ says he looked around for a material that had the exact properties he would need, and “lo and behold,” one of them is something called ethylene glycol. For those of us not trained in chemistry, he explained that ethylene glycol is more commonly known as antifreeze. That’s right, Star Trek fans. Not the fictional dilithium crystals or anti-matter used to power the starship Enterprise, but good old-fashioned, your-grandpa-keeps-a-can-in-the-garage, anti-freeze.

    Glenn says that the realization that such a simple material could unlock the door to warp drive motivated him to begin to design an actual lab experiment, one that could be performed with present-day tools and materials.

    “I am, at the present time, working on conducting that experiment using an interferometer to measure any changes that you may see,” Glenn told The Debrief, “because that’s how they’re measuring gravitational waves now.”

    For reference, gravitational waves were theorized way back in 1916 by Albert Einstein. Still, they were not proven to exist until 2015, when researchers used the Laser Interferometer Gravitational Observatory (LIGO) run by The California Institute of Technology (Cal Tech) and the Massachusetts Institute of Technology (MIT) to actually observe real gravitational waves in space. It was a discovery nearly 100 years in the making and one that won the researchers involved a Nobel Prize.

    As a matter of fact, the group from Applied Physics recently proposed a method for detecting an alien warp drive-enabled spacecraft using LIGO, a story covered by The Debrief.

    “My planned experiment (involves) pumping an RF chamber with a laser beam running through it,” explained Glenn, “and if somehow, even slightly, space/time is distorted in some way, it could be detected.”

    Of course, the observably brilliant yet humble engineer makes it perfectly clear that his first goal is to see that warping of space/time and not the construction of an actual warp spaceship.

    “In the lab, I don’t want to see a warp bubble shooting by at ten times the speed of light,” Glenn told The Debrief. “I can’t detect it anyway.”

    Fortunately, the experiment he does plan to run is something he is almost ready to execute.

    The Experiment

    The actual design of Glenn’s lab experiment is rather straightforward. It involves building a chamber, filling it with anti-freeze, blasting that chamber with RF energy, and measuring the impact with a laser interferometer, just like LIGO.

    “If it can concentrate (the RF energy) into a particular spot, which the chamber I am designing allows us to do, that may be enough, at the atomic level, I’m only speculating, could be the thing that actually bends space/time.”

    Of course, Glenn points out that there are a number of variables he has to take into account, variables that he is currently writing into his experiment.

    “If I’m trying to measure stuff at such a small level, and a small resolution, there are a lot of variables that could affect the results,” he explained. “Like heat, or vibrations on the table could make the laser beam look like it’s being jostled or moved, but it (might not) be what you think.”

    The key to making sure he is actually seeing what he hopes to see is pulsing the RF signal. That’s because pulsing the signal not only allows for the tuning and shaping of the RF to improve performance and reduces the overall energy required (a stalling point for many warp theories) but also gives a method for making sure any perturbance of space/time witnessed is a result of the RF and not some outside force.

    “I want to pulse it so that if I see distortions based on those pulses, I know that I’m doing it,” explained Glenn, “and not the train that is riding down the tracks 20 miles away.”

    The Warp Drive Propulsion

    The first step, Glenn explained, is finishing the design of the chamber to make sure the RF energy is concentrated at a single point. To accomplish this task, he is using a design software tool known as COMSOL. And, he says, he is already about 75% of the way through that work.

    Next, as is the case in pretty much every visionary engineering endeavor, Glenn will need to secure the funding to perform his experiment. Fortunately, his pre-proposal to the National Science Foundation (NSF) for a grant has already been accepted for review. If it is approved, the professor says there should be more than enough funding to build his chamber, pour the concrete for his stable test table, buy the cutting-edge interferometer and other tools, and compensate all of the people he will need to pull it off.

    Of course, in his position as provost at the university, Glenn could just appropriate the resources and people and do it right there on campus. But if he receives the NSF grant, he wants to create a dedicated facility off campus to avoid any conflicts of interest. Towards that end, he has also received some support from other warp theorists who are excited about his idea.

    “Dr. White has opened up his (Eagleworks) lab to us if we need it,” said Glenn, “so there is always that option.”

    The professor also noted that his initial paper outlining his theory has garnered him some rather high-profile allies that are supporting his efforts to test his warp drive concept.

    “The exciting thing is, SpaceX is indirectly involved,” Glenn told The Debrief. “I am actually working with someone who is connected to the Jet Propulsion Laboratory (JPL), so NASA, and also connected to SpaceX. They are centered at Texas A&M’s technology and engineering center.”

    Whichever route he takes, Dr. Glenn says his experiment should be conducted very soon.

    “I’m hoping to run initial experiments in the 1st half of 2023,” said Glenn. “Maybe sometime in March or early spring.”

    The Vision

    Along with being a fan of Star Trek and an engineer who loves a good challenge, Glenn says there is a larger driving force behind his work. It is the idea of access to space for all.

    “We look at all of these ideas, like building colonies on Mars or hotels in space, and we wonder if any of this is going to be accessible to the average person or if it is going to be another case of the haves versus the have-nots,” explained Glenn.

    He calls his idea “space for everyone” and has even chartered an organization whose primary goal is to make sure everyday people can reap the rewards of trillion-dollar asteroids or colonies on the moon.

    “I am representing a group called the Morningbird Foundation,” said Glenn. “Our goal is to make sure everyone benefits from access to space, not just the wealthy.” If this idea sounds familiar, that’s because it is more or less one of the primary factors that motivated Gene Roddenberry to create the original Star Trek series.

    So, although we don’t know if Dr. Glenn will be successful in warping space/time, it sounds like he may have already realized his first dream: to actually become Mr. Spock.

    To that, we say good luck with your experiment, Dr. Glenn. We can’t wait to report the results.

    Until then, live long and prosper.

    RELATED VIDEOS


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

    16-01-2026 om 22:49 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Medicine in orbit: how health problems affected space missions

    Medicine in orbit: how health problems affected space missions

    On January 14, an unprecedented event in NASA history took place. For the first time, the aerospace administration terminated a manned space mission ahead of schedule due to health problems of one of the Crew-11 mission participants. For confidentiality reasons, NASA is not disclosing his name or details of his diagnosis. According to unofficial sources, the astronaut in question is Michael Fincke.

    The Crew-11 mission crew.
    Source: NASA

    But although evacuation to Earth is an unprecedented event for NASA, it is far from the first such case. Yes, cosmonauts and astronauts undergo thorough medical examinations, but they are still human beings. It is no secret that even healthy people can unexpectedly experience health problems under certain circumstances. Moreover, space explorers work in extremely harsh conditions and are exposed to factors such as weightlessness, increased radiation levels, and confinement in a closed space – not to mention significant stress.

    In this article, you will learn about the most famous cases in history when medical problems directly affected the course of space expeditions.

    Cold and disobedience, Apollo 7

    At the dawn of the space age, NASA did not have a preflight quarantine for astronauts. The Apollo 7 mission clearly demonstrated the shortcomings of this practice. Shortly after launch, mission commander Walter Schirra came down with a cold. Later, the rest of the crew also developed symptoms. Colds in zero gravity were much more severe than on Earth. Aspirin from the onboard first aid kit did not help, and it was impossible to clear their noses and ears.

    The Apollo 7 mission crew.
    Source: NASA

    It is worth noting that Apollo 7 was a very difficult mission. It was supposed to demonstrate that NASA had recovered from the loss of three astronauts who died in a fire during Apollo 1 testing, and that after all the changes made, the spacecraft was safe for flight. The crew was under a great deal of pressure. And illness only exacerbated the situation.

    From a technical point of view, the flight itself went brilliantly: the astronauts completed absolutely all of their tasks, paving the way to the Moon. The flip side of the coin was that communication between Mission Control (RKA) and the astronauts was very difficult and accompanied by a number of conflicts. The final straw was the landing. Mission Control (RKA) demanded that the astronauts put on their helmets in case of depressurization of the spacecraft. But the crew refused to do so, citing concerns that the increase in pressure could cause their eardrums to rupture due to their airways still being blocked. The astronauts wanted to be able to perform the Valsalva maneuver to equalize the pressure in their ears. As a result, they refused to obey a direct order and did not put on their helmets.

    This had direct consequences. Even before the flight, Wally Schirra announced that he would soon be leaving NASA, so the aerospace administration was unable to impose any serious sanctions on him. However, for the other two crew members, Donn Eisele and Walter Cunningham, this flight was their last. NASA management decided to no longer allow astronauts who did not follow orders to fly into space.

    Moon allergy

    Scientists and engineers working on projects to create lunar settlements have identified a number of problems that need to be solved before colonization of Earth’s satellite can begin. But actual flights have revealed another problem that no one had thought about before, and that could seriously complicate long-term stays on the Moon. We are talking about allergies to lunar dust.

    Harrison Schmitt inside the lunar module. Note that his spacesuit is covered in moondust.
    Source: NASA

    The fact is that lunar dust is completely different from Earth dust. It consists of very fine and extremely sharp particles – after all, there is no atmosphere or water on the Moon to smooth them out. Lunar dust is extremely sticky. It easily sticks to spacesuits and equipment, which creates a number of problems. It can also cause allergies.

    Harrison Schmitt, a member of the Apollo 17 mission, saw this for himself. When he took off his spacesuit after returning to the lunar module, he developed hay fever – an allergic reaction caused by inhaling dust particles. The next day, the allergy had almost disappeared, allowing the astronaut to continue his work. However, as it soon became clear, Cernan’s case was not unique. Later, the same symptoms appeared in a person who worked with the astronauts’ spacesuits after their return to Earth.

    It is possible that long-term inhalation of dust could have even more serious consequences for humans and cause lung disease. Therefore, designers of modern lunar missions are taking this factor into account and looking for ways to combat dust.

    Skylab strike

    Information about the so-called Skylab “strike” can easily be found on the Internet. It is claimed that on December 28, 1973, in protest against an overly busy work schedule, the station crew (astronauts Gerald Carr, Edward Gibson, and William Pogue) cut off communication with Mission Control (RKA) and spent the entire day relaxing and looking at Earth.

    Skylab orbital station.
    Source: NASA

    What really happened? For all the astronauts at the station, it was their first flight into space. At the same time, NASA had drawn up an overly ambitious work plan for them. This led to the crew falling behind schedule and the psychological atmosphere becoming very tense. It is claimed that this is precisely why the astronauts broke down at some point and went on strike.

    But in reality, everything was much more complicated. Communication was lost not for a day, but for an entire orbit. According to the astronauts, this was due to a mistake – they confused who was responsible for maintaining contact with Earth that day. The available records of the conversations also do not confirm that the crew refused to work. In fact, there was a dialogue between the crew and Mission Control (RKA) about the problems that had arisen – something like the first psychotherapy session in space. At first, the crew reported everything they did not like and what needed to be changed first. Then Mission Control (RKA) openly told the crew about everything that was bothering them.

    The changes introduced after this discussion yielded results. As a result, the second half of the mission turned out to be much more productive than the first. In some respects, the crew even managed to exceed the initial plan. After this flight, NASA began to pay much more attention to the psychological aspects of space travel, realizing that they were just as important as the crew’s physical health.

    The Skylab mission became the starting point for numerous medical studies devoted to human behavior in space. Its results are still actively used in the selection and training of crews for long-term expeditions. The most obvious legacy of this mission was the introduction of the practice that at least one member of a space expedition must have experience flying in orbit.

    The mysterious return of Soyuz-21

    Despite all the problems, the Skylab crew remained at the station until the end of their scheduled stay. The same cannot be said about the crew of Soyuz-21. In July 1976, it docked with the Salyut 5 military orbital station. It was assumed that crew commander Boris Volynov and flight engineer Vitaly Zholobov would spend 60 days aboard the station. In reality, they returned to Earth after only 49 days.

    Boris Volynov and Vitaly Zholobov

    The reason for the early return of Soyuz-21 is still shrouded in rumors. According to Volynov, after an emergency arose at the station, Zholobov began to suffer from severe headaches, and his condition continued to deteriorate. By the time the Mission Control Center decided to terminate the expedition early, he was unable to put on his spacesuit by himself. As for the reasons for his deteriorating health, a strange smell was cited, which was presumably caused by a nitric acid leak. Because of this, the next expedition boarded Salyut-5 wearing respirators. However, the cosmonauts did not detect any smell or leaks.

    However, according to popular opinion, the real reason was the difficult psychological situation and conflict between the crew members, which led to the early termination of the mission. Later, Zholobov denied some of the rumors surrounding the flight, but at the same time stated that he had essentially taken on the problems that had arisen for Volynov, who was in command of the mission.

    Astronaut sickness

    While there are many gray areas in the history of Soyuz-21, there is no doubt about the main reason for the early termination of the Soyuz T-14 expedition: cosmonaut Vladimir Vasyutin fell ill. While on board the Salyut-7 station, he developed symptoms of prostatitis.

    The Salyut 7 orbital station.
    Source: Wikipedia

    The treatment administered on board the space station after consultation with doctors was unsuccessful. The cosmonaut’s health deteriorated rapidly. As a result, on November 21, 1985, Soyuz T-14 returned to Earth. Instead of the planned 200 days, the flight lasted only 64 days.

    According to the widely accepted version, Vasyutin knew about his illness and concealed it, attempting to treat himself, and the responsibility lies solely with him. However, there is also an alternative opinion, according to which, given the thoroughness of medical examinations, regardless of his wishes, the cosmonaut would never have been able to hide a chronic illness from doctors, and that this was an acute illness that suddenly developed during the space flight.

    Regardless of whether Vasyutin knew about his illness or not, it led to the failure of a very ambitious expedition and the cancellation of a number of missions planned for Salyut 7. Subsequently, only one spacecraft visited the station, after which it was mothballed and, a few years later, fell out of orbit. Shortly after returning to Earth, Vasyutin himself was removed from the cosmonaut corps due to health reasons and never flew into space again.

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

    16-01-2026 om 22:09 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Wormholes may not exist—we've found they reveal something deeper about time and the universe

    Wormholes may not exist—we've found they reveal something deeper about time and the universe

    Story by Enrique Gaztanaga

    Credit: Pixabay/CC0 Public Domain

    Credit: Pixabay/CC0 Public Domain

    Wormholes are often imagined as tunnels through space or time—shortcuts across the universe. But this image rests on a misunderstanding of work by physicists Albert Einstein and Nathan Rosen.

    In 1935, while studying the behavior of particles in regions of extreme gravity, Einstein and Rosen introduced what they called a "bridge": a mathematical link between two perfectly symmetrical copies of spacetime. It was not intended as a passage for travel, but as a way to maintain consistency between gravity and quantum physics. Only later did Einstein–Rosen bridges become associated with wormholes, despite having little to do with the original idea.

    Phase space of inverted harmonic oscillator representing doubly degenerate positive and negative energy solutions. Credit: Classical and Quantum Gravity (2026). DOI: 10.1088/1361-6382/ae3044

    Phase space of inverted harmonic oscillator representing doubly degenerate positive and negative energy solutions.
    Credit: Classical and Quantum Gravity (2026). DOI: 10.1088/1361-6382/ae3044

    But in new research published in Classical and Quantum Gravity, my colleagues and I show that the original Einstein–Rosen bridge points to something far stranger—and more fundamental—than a wormhole.

    The puzzle Einstein and Rosen were addressing was never about space travel, but about how quantum fields behave in curved spacetime. Interpreted this way, the Einstein–Rosen bridge acts as a mirror in spacetime: a connection between two microscopic arrows of time.

    Quantum mechanics governs nature at the smallest scales such as particles, while Einstein's theory of general relativity applies to gravity and spacetime. Reconciling the two remains one of physics' deepest challenges. And excitingly, our reinterpretation may offer a path to doing this.

    Einstein–Rosen bridges (ERB): "A particle in the physical Universe must be described by a mathematical bridge between two sheets of spacetime." Credit: Classical and Quantum Gravity (2026). DOI: 10.1088/1361-6382/ae3044

    Einstein–Rosen bridges (ERB): "A particle in the physical Universe must be described by a mathematical bridge between two sheets of spacetime."
    Credit: Classical and Quantum Gravity (2026). DOI: 10.1088/1361-6382/ae3044

    A misunderstood legacy

    The "wormhole" interpretation emerged decades after Einstein and Rosen's work, when physicists speculated about crossing from one side of spacetime to the other, most notably in the late-1980s research.

    But those same analyses also made clear how speculative the idea was: within general relativity, such a journey is forbidden. The bridge pinches off faster than light could traverse it, rendering it non-traversable. Einstein–Rosen bridges are therefore unstable and unobservable—mathematical structures, not portals.

    Nevertheless, the wormhole metaphor flourished in popular culture and speculative theoretical physics. The idea that black holes might connect distant regions of the cosmos—or even act as time machines—inspired countless papers, books and films.

    Yet there is no observational evidence for macroscopic wormholes, nor any compelling theoretical reason to expect them within Einstein's theory. While speculative extensions of physics—such as exotic forms of matter or modifications of general relativity—have been proposed to support such structures, they remain untested and highly conjectural.

    Two arrows of time

    Our recent work revisits the Einstein–Rosen bridge puzzle using a modern quantum interpretation of time, building on ideas developed by Sravan Kumar and João Marto.

    Most fundamental laws of physics do not distinguish between past and future, or between left and right. If time or space is reversed in their equations, the laws remain valid. Taking these symmetries seriously leads to a different interpretation of the Einstein–Rosen bridge.

    Rather than a tunnel through space, it can be understood as two complementary components of a quantum state. In one, time flows forward; in the other, it flows backward from its mirror-reflected position.

    This symmetry is not a philosophical preference. Once infinities are excluded, quantum evolution must remain complete and reversible at the microscopic level—even in the presence of gravity.

    The "bridge" expresses the fact that both time components are needed to describe a complete physical system. In ordinary situations, physicists ignore the time-reversed component by choosing a single arrow of time.

    But near black holes, or in expanding and collapsing universes, both directions must be included for a consistent quantum description. It is here that Einstein–Rosen bridges naturally arise.

    Solving the information paradox

    At the microscopic level, the bridge allows information to pass across what appears to us as an event horizon—a point of no return. Information does not vanish; it continues evolving, but along the opposite, mirror temporal direction.

    This framework offers a natural resolution to the famous black hole information paradox. In 1974, Stephen Hawking showed that black holes radiate heat and can eventually evaporate, apparently erasing all information about what fell into them—contradicting the quantum principle that evolution must preserve information.

    The paradox arises only if we insist on describing horizons using a single, one-sided arrow of time extrapolated to infinity—an assumption quantum mechanics itself does not require.

    If the full quantum description includes both time directions, nothing is truly lost. Information leaves our time direction and re-emerges along the reversed one. Completeness and causality are preserved, without invoking exotic new physics.

    These ideas are difficult to grasp because we are macroscopic beings who experience only one direction of time. On everyday scales, disorder—or entropy—tends to increase. A highly ordered state naturally evolves into a disordered one, never the reverse. This gives us an arrow of time.

    But quantum mechanics allows more subtle behavior. Intriguingly, evidence for this hidden structure may already exist. The cosmic microwave background—the afterglow of the Big Bang—shows a small but persistent asymmetry: a preference for one spatial orientation over its mirror image.

    This anomaly has puzzled cosmologists for two decades. Standard models assign it extremely low probability—unless mirror quantum components are included.

    Echoes of a prior universe?

    This picture connects naturally to a deeper possibility. What we call the "Big Bang" may not have been the absolute beginning, but a bounce—a quantum transition between two time-reversed phases of cosmic evolution.

    In such a scenario, black holes could act as bridges not just between time directions, but between different cosmological epochs. Our universe might be the interior of a black hole formed in another, parent cosmos. This could have formed as a closed region of spacetime collapsed, bounced back and began expanding as the universe we observe today.

    If this picture is correct, it also offers a way for observations to decide. Relics from the pre-bounce phase—such as smaller black holes—could survive the transition and reappear in our expanding universe. Some of the unseen matter we attribute to dark matter could, in fact, be made of such relics.

    In this view, the Big Bang evolved from conditions in a preceding contraction. Wormholes aren't necessary: the bridge is temporal, not spatial—and the Big Bang becomes a gateway, not a beginning.

    This reinterpretation of Einstein–Rosen bridges offers no shortcuts across galaxies, no time travel and no science-fiction wormholes or hyperspace. What it offers is far deeper. It offers a consistent quantum picture of gravity in which spacetime embodies a balance between opposite directions of time—and where our universe may have had a history before the Big Bang.

    It does not overthrow Einstein's relativity or quantum physics—it completes them. The next revolution in physics may not take us faster than light—but it could reveal that time, deep down in the microscopic world and in a bouncing universe, flows both ways.

    More information: Enrique Gaztañaga et al, A new understanding of Einstein–Rosen bridges, Classical and Quantum Gravity (2026). DOI: 10.1088/1361-6382/ae3044

     Phys.org. }

    16-01-2026 om 21:52 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.Is this how the world will end? Earth could be VAPORISED by the sun as it expands, scientists warn

    Is this how the world will end? Earth could be VAPORISED by the sun as it expands, scientists warn

    Scientists have discovered a mysterious 'iron bar' in the heart of a nearby nebula that could offer a glimpse into Earth's grizzly fate.

    The strip of ionised iron atoms was spotted stretching across the Ring Nebula, located 2,283 light-years from Earth.

    Experts are baffled about how it formed, as scientists have never seen anything like it before. 

    But they say it could be the remains of an Earth-like rocky planet that was vaporised by a dying star.

    When stars like our sun run out of nuclear fuel at the end of their lives, the outer layers balloon to enormous size even as the core shrinks and cools.

    Eventually, the core becomes a tiny white dwarf without enough gravity to hold the star together, and the outer layers are shed to leave behind a planetary nebula.

    In about five billion years from now, our sun will undergo the same transformation as it swells into an enormous Red Giant and swallows Earth.

    In a new paper, researchers say this never-before-seen structure in the Ring Nebula could reveal what Earth would look like after being destroyed by the sun.

    Scientists have spotted a mysterious iron 'bar' at the centre of the Ring Nebula, and it could offer a glimpse of Earth's grim future

    Scientists have spotted a mysterious iron 'bar' at the centre of the Ring Nebula, and it could offer a glimpse of Earth's grim future 

    In this new study, scientists looked at the Ring Nebula using a new tool called the Large Integral Field Unit (LIFU), mounted on the William Herschel Telescope.

    This is essentially a bundle containing hundreds of fibre-optic wires that allow scientists to look at the different wavelengths of light, or spectra, across the entire face of the nebula.

    Lead author Dr Roger Wesson, of Cardiff University and University College London, says: 'By obtaining a spectrum continuously across the whole nebula, we can create images of the nebula at any wavelength and determine its chemical composition at any position.

    'When we processed the data and scrolled through the images, one thing popped out as clear as anything – this previously unknown "bar" of ionised iron atoms, in the middle of the familiar and iconic ring.'

    The strip of ionised iron atoms was spotted stretching across the Ring Nebula, located 2,283 light-years from Earth

    The strip of ionised iron atoms was spotted stretching across the Ring Nebula, located 2,283 light-years from Earth

    Astronomers believe that the Ring Nebula formed when a dying star shed its outer layers about 4,000 years ago

    Astronomers believe that the Ring Nebula formed when a dying star shed its outer layers about 4,000 years ago

    A star's life cycle

    Around 90 per cent of stars in the sun are what scientists call 'main sequence' stars.

    These are stars that fuse hydrogen into helium in their cores, and range from about a tenth of the mass of the sun to about 200 times as massive.

    Main sequence stars start as clouds of gas and dust, which collapse under gravity into 'protostars'.

    When a protostar is dense enough, the pressure and heat start nuclear fusion and a star is born.

    Stars keep burning helium until it runs out in around 10 to 20 billion years.

    At this point, stars will enter the post–main sequence phase and become red dwarfs, white dwarfs, red giants, or even explode into neutron stars, depending on their size.  

    The researchers aren't actually sure how this strange bar might have been formed, but there are two likely scenarios.

    Either the bar was made by some unknown process during the ejection of the nebula as the parent star collapsed, or it is an arc of plasma resulting from the vaporisation of a rocky planet caught up in the star’s earlier expansion.

    'We know that there are planets around many stars, and if there were planets around the star that formed the Ring Nebula, they would have vaporised when the star became a red giant,' Dr Wesson told the Daily Mail.

    'And the mass of iron in the bar is about what you'd expect from the vaporisation of a planet: if Mercury or Mars were vaporised, that would give a bit less iron than the bar in the Ring, while if Earth or Venus were vaporised, it would give a bit more.'

    If the latter is true, then this strange structure could be a fascinating look at how our planet might appear to astronomers billions of years in the future.

    Main-sequence stars like our sun are stable because the inward forces of gravity are matched by the outward push of nuclear fusion reactions in the core.

    However, when the star runs out of hydrogen fuel, it can't sustain that reaction and the outer layers start to collapse inwards.

    The pressure from this collapse creates such intense heat that it can fuse helium atoms into carbon, releasing a surge of energy that kickstarts nuclear fusion in the outer layers.

    One possible explanation is that the iron bar is the remains of a rocky planet that was engulfed by its star as the outer layers expanded to form the nebula. Earth is likely to suffer this same fate when the sun starts to run out of fuel in five billion years' time

    One possible explanation is that the iron bar is the remains of a rocky planet that was engulfed by its star as the outer layers expanded to form the nebula. Earth is likely to suffer this same fate when the sun starts to run out of fuel in five billion years' time

    The outer layers then expand and cool into what is known as a Red Giant, becoming anywhere from 100 to 1,000 times larger.

    When this happens to our sun in about five billion years' time, scientists think it is very likely that Earth will be destroyed.

    As the sun expands, Earth will either be vaporised by the intense heat or torn to pieces and pulled in by the powerful gravitational tidal forces.

    In a paper published last year, scientists found that stars which had already expanded into red giants were much less likely to host large, close–orbiting planets like Earth.

    Overall, 0.28 per cent of stars surveyed were home to a giant planet, with the youngest stars in the sequence having planets more frequently.

    However, for stars that had already grown enough to be classed as red giants, just 0.11 per cent were home to planets.

    When this does happen, Earth might be smeared into something very much like the iron bar seen in the Ring Nebula.

    However, the researchers say they still need a lot more evidence before they can say for certain whether the bar was left by a planet.

    In about five billion years, scientists say that the sun will burn the last of its hydrogen fuel. When this happens, it will expand to about 200 times its current size to become a red giant and destroy Earth (artist's impression)

    In about five billion years, scientists say that the sun will burn the last of its hydrogen fuel. When this happens, it will expand to about 200 times its current size to become a red giant and destroy Earth (artist's impression)

    Dr Wesson says: 'A vaporised planet is a possibility. But it's not the only possibility, and we'd have to work out how the iron ended up in a bar shape if it did come from a planet. 

    article image

    'More likely, there are iron "bars" waiting to be found in other nebulae. The more we can find, the more information we will have to determine how they formed, so we're hunting for more of them!'

    In the future, the researchers hope to use the LIFU tool to find more nebulae with similar features, to try to figure out where the bar might have come from. 

    Co-author Professor Janet Drew, of University College London, says: 'We definitely need to know more - particularly whether any other chemical elements co-exist with the newly-detected iron, as this would probably tell us the right class of model to pursue. 

    'Right now, we are missing this important information.'

    WHAT WILL HAPPEN TO EARTH WHEN THE SUN DIES?

    Five billion years from now, it's said the Sun will have grown into a red giant star, more than a hundred times larger than its current size. 

    Eventually, it will eject gas and dust to create an 'envelope' accounting for as much as half its mass.

    The core will become a tiny white dwarf star. This will shine for thousands of years, illuminating the envelope to create a ring-shaped planetary nebula.

    Five billion years from now, it's said the Sun will have grown into a red giant star, more than a hundred times larger than its current size

    Five billion years from now, it's said the Sun will have grown into a red giant star, more than a hundred times larger than its current size

    While this metamorphosis will change the solar system, scientists are unsure what will happen to the third rock from the Sun.

    We already know that our Sun will be bigger and brighter, so that it will probably destroy any form of life on our planet.

    But whether the Earth's rocky core will survive is uncertain. 

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

    16-01-2026 om 20:38 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Black hole awakens after 100 million years of silence – and it's erupting like a cosmic VOLCANO

    Black hole awakens after 100 million years of silence – and it's erupting like a cosmic VOLCANO

    Astronomers have captured the moment a 'reborn' supermassive black hole awakened after 100 million years of silence.

    Incredible images show the black hole erupting like a 'cosmic volcano', with enough force to reshape its entire host galaxy.

    While almost all galaxies host a monstrous supermassive black hole at their heart, few produce such spectacular explosions of superheated plasma.

    Spanning almost one million light–years, these plumes of cosmic lava are nearly 10 times wider than the Milky Way.

    Lead researcher Dr Shobha Kumari, of Midnapore City College in India, says: 'It's like watching a cosmic volcano erupt again after ages of calm.'

    The researchers say their radio images aren't just impressive to look at, but also reveal the hidden violence of the 'messy, chaotic struggle' at the galaxy's core.

    The black hole, dubbed J1007+3540, lives inside an enormous galaxy cluster filled with extremely hot gas.

    This creates a constant battle between the explosive power of the black hole and the crushing pressure of the surrounding galaxy.

    Scientists have captured the moment a supermassive black hole roared back to life after 100 million years of silence, erupting like a 'cosmic volcano'

    Scientists have captured the moment a supermassive black hole roared back to life after 100 million years of silence, erupting like a 'cosmic volcano' 

    Supermassive black holes are the ultra–dense cores of dead stars that collapsed in supernova explosions, with masses up to 10 million times larger than that of the sun.

    Their gravitational pull is so strong that not even light can escape beyond the point of no return known as the 'event horizon'.

    Typically, the supermassive black holes at the centre of most galaxies are relatively stable, with the surrounding matter orbiting at a safe distance.

    However, these monstrous objects can sometimes start to feed on the surrounding clouds of gas that fill the galactic core and become 'active'.

    As matter swirls inwards towards the event horizon like water circling a drain, it starts to move incredibly quickly, and friction heats it to enormous temperatures.

    Eventually, these forces become so powerful that the black hole starts shooting a jet of superheated plasma into space that produces a blast of electromagnetic radiation.

    This ejects a huge amount of the matter falling into the black hole, which is why astronomers sometimes call black holes 'messy eaters'.

    In their new paper, published in Monthly Notices of the Royal Astronomical Society, scientists used the Low Frequency Array (LOFAR) in the Netherlands and India's upgraded Giant Metrewave Radio Telescope (uGMRT) to look for radio emissions from J1007+3540.

    The supermassive black hole, dubbed J1007+3540, has now become active, shooting a jet of plasma almost 10 times wider than the Milky Way out into space (illustrated)

    The supermassive black hole, dubbed J1007+3540, has now become active, shooting a jet of plasma almost 10 times wider than the Milky Way out into space (illustrated)

    Why do black holes 'erupt'?

    Most supermassive black holes are considered 'dormant', which means they aren't actively feeding on matter.

    However, when a black hole starts to feed on matter, it becomes 'active' and begins to produce radiation.

    This is because matter swirling around the black hole is superheated to the point that it is shot out in a jet.

    This plasma produces large amounts of X–rays and radio radiation that can be detected from Earth as an eruption.

    These images showed a compact, bright inner jet of radio–emitting magnetised plasma that is the telltale sign of the black hole's recent awakening.

    The researchers also discovered just how profoundly the intense pressures at the heart of the galaxy cluster were shaping the black hole.

    As the jets are pushed outwards, they are bent, squeezed and distorted by their extreme environment.

    As their radio images show, the topmost 'northern lobe' of the jet has been compressed into a curve that seems to have been shoved sideways by the gases.

    However, the astronomer's observations didn't just reveal the secrets of this black hole's current eruption.

    Just like the volcanoes here on Earth, J1007+3540 has a long and violent history of eruptions.

    Just outside the bright inner jet, astronomers spotted a cocoon of older, faded plasma.

    This is the leftover debris from past eruptions that has been squeezed and distorted by the hostile environment.

    Uniquely, the researchers discovered the remains of previous 'eruptions' surrounding the active black hole (artist's impression). This suggests that this cosmic volcano has erupted multiple times in the past

    Uniquely, the researchers discovered the remains of previous 'eruptions' surrounding the active black hole (artist's impression). This suggests that this cosmic volcano has erupted multiple times in the past 

    Dr Kumari says: 'This dramatic layering of young jets inside older, exhausted lobes is the signature of an episodic AGN [Active Galactic Nucleus] – a galaxy whose central engine keeps turning on and off over cosmic timescales.'

    In our own galaxy, the supermassive black hole at the galactic core is currently dormant.

    article image

    However, scientists do believe that the black hole, known as Sagittarius A*, could make a similar eruption.

    If this were to happen, Sagittarius A* would produce its own jets or plasma that could fundamentally reshape the universe.

    While Earth would likely be protected from any radiation, a direct hit from one of those jets would be strong enough to wipe out life on Earth.

    But there's no need to worry as scientists think this won't happen until the Milky Way collides with our neighbouring galaxy, the Large Magellanic Cloud (LMC), in 2.4 billion years.

    BLACK HOLES HAVE A GRAVITATIONAL PULL SO STRONG NOT EVEN LIGHT CAN ESCAPE

    Black holes are so dense and their gravitational pull is so strong that no form of radiation can escape them - not even light.

    They act as intense sources of gravity which hoover up dust and gas around them. Their intense gravitational pull is thought to be what stars in galaxies orbit around.

    How they are formed is still poorly understood. Astronomers believe they may form when a large cloud of gas up to 100,000 times bigger than the sun, collapses into a black hole.

    Many of these black hole seeds then merge to form much larger supermassive black holes, which are found at the centre of every known massive galaxy.

    Alternatively, a supermassive black hole seed could come from a giant star, about 100 times the sun's mass, that ultimately forms into a black hole after it runs out of fuel and collapses.

    When these giant stars die, they also go 'supernova', a huge explosion that expels the matter from the outer layers of the star into deep space. 

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

    16-01-2026 om 20:00 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    15-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Aresibo Legacy: 100 potential signals from extraterrestrial civilizations detected

    Aresibo Legacy: 100 potential signals from extraterrestrial civilizations detected

    One of the most ambitious hunting expeditions in history — the search for signals from extraterrestrial civilizations — is getting a new lease on life. The SETI@Home project, which has attracted more than 2 million enthusiasts from around the world, is completing its analysis of a colossal array of data collected by the legendary Arecibo telescope. Despite the destruction of the observatory, scientists now have a unique “golden hundred” of candidate signals for detailed verification.

    The Arecibo radio telescope in Puerto Rico. The facility’s famous 300-meter radio antenna collapsed in 2020.
    American Photo Archive

    The idea of searching for extraterrestrial intelligence (SETI) faces a fundamental problem: space is filled with radio noise from stars, gas, and other natural sources. It is incredibly difficult to pick out a possible technological signal from this chaos. In 1999, a team of scientists decided to enlist the help of the entire planet. They asked volunteers to install a special program on their home computers that would analyze real data from Arecibo in the background. They expected 50,000 participants, but ended up with a true global collective mind — millions of people from 100 countries used their home computers to help science.

    The Legacy of Areisibo

    A screenshot of the SETI@home program interface on a desktop computer in 2009. The software ran on millions of home computers around the world, analyzing radio data from space in search of signals from extraterrestrial civilizations.
    Source: berkeley.edu

    Over the course of 21 years, volunteers sifted through the information and identified more than 12 billion “interesting” signals. Now, this list has been narrowed down to the 100 most promising ones. Their detailed verification has been entrusted to a new giant — the Chinese FAST radio telescope, the world’s largest single-dish antenna. This is a symbolic passing of the baton from the late Arecibo, who in 1974 sent the famous message about humanity into space.

    Aresio Telescope’s Message

    So far, none of the candidate signals has provided irrefutable evidence of extraterrestrial intelligence. However, as project co-founder David Anderson notes, this work is of immense value: “If we don’t find aliens, we can say that we have established a new level of sensitivity. We have a long list of things we would do differently.”

    Path to future discoveries

    SETI@Home has concluded as a large-scale experiment in citizen science. It has not only sifted through cosmic noise, but also created an invaluable database of knowledge and methodologies. This experience will serve as a foundation for future, even more accurate searches, proving that the most complex scientific problems can be solved through the combined efforts of all humanity.

    Earlier, we explained the reasons behind humanity’s failure to detect extraterrestrial life to date.

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

    15-01-2026 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.Little red dots in deep space are 'the most violent forces in the universe', study finds - solving a mystery that has baffled scientists for decades

    Little red dots in deep space are 'the most violent forces in the universe', study finds - solving a mystery that has baffled scientists for decades

    Scientists have solved one of the universe's great mysteries as they finally reveal the identity of the 'little red dots' in deep space.

    Ever since the James Webb Space Telescope (JWST) started peering back into the dawn of the universe, experts have been perplexed by the appearance of these tiny red dots.

    Astronomers found hundreds of the faint lights in images from when the universe was only a few hundred million years old, without any clue what they might be.

    Now, scientists from the University of Copenhagen have revealed that the JWST's little red dots are actually 'the most violent forces in nature'.

    According to a new study, published in the journal Nature, the red dots are actually supermassive black holes concealed in 'cocoons of ionised gas'.

    As these young black holes feed on their cocoon, the swirling matter creates a vast amount of heat and radiation that shines out through the cloud of gas.

    Lead author Professor Darach Watson says: 'We have captured the young black holes in the middle of their growth spurt at a stage that we have not observed before.

    'The dense cocoon of gas around them provides the fuel they need to grow very quickly.'

    Scientists say that the mysterious 'little red dots' discovered by the James Webb Space Telescope (pictured) are actually ancient supermassive black holes

    Scientists say that the mysterious 'little red dots' discovered by the James Webb Space Telescope (pictured) are actually ancient supermassive black holes 

    When the first little red dots were discovered, they presented a baffling puzzle for astronomers of the early universe.

    The dots first appear in images from around 13 billion years ago, and simply disappear about a billion years later.

    At first, scientists thought that the dots must be very young galaxies in their earliest stages of formation.

    However, this didn't fit with our understanding of how the universe evolved after the Big Bang, as the first galaxies shouldn't have been visible until much later.

    Others suggested that the dots might be black holes, ultra-dense bodies formed by the collapse of enormous stars, but there was another problem.

    Scientists couldn't explain how any black hole could have become big enough to form a red dot so soon after the Big Bang.

    Professor Watson's solution is that the black holes that form little red dots are actually much smaller than previously thought.

    He says: 'When gas falls towards a black hole, it spirals down into a kind of disk or funnel towards the surface of the black hole.

    Ever since the James Webb Space Telescope (JWST) started peering back into the dawn of the universe, astronomers have been perplexed by the appearance of these tiny red dots

    Ever since the James Webb Space Telescope (JWST) started peering back into the dawn of the universe, astronomers have been perplexed by the appearance of these tiny red dots

    Now scientists say that these dots are actually young black holes wrapped in a cocoon of ionised gases, giving them a distinctive red glow

    Now scientists say that these dots are actually young black holes wrapped in a cocoon of ionised gases, giving them a distinctive red glow 

    'It ends up going so fast and is squeezed so densely that it generates temperatures of millions of degrees and lights up brightly.'

    'The red colour arises because the UV and X-ray radiation from the central black hole is absorbed and reprocessed by the ionised gas around it, which gives it the characteristic red colour and spectra that look reminiscent of a star. 

    Professor Watson and his co-authors looked at the spectral emission lines, the 'fingerprint' of the light being released, from several little red dots.

    Just as they had suspected, these spectral lines were missing much of their UV and X-ray radiation, suggesting that the light was passing through a cloud of gas. 

    More importantly, this data also shows that little red dots are far smaller than previously thought.

     Professor Watson told the Daily Mail: 'They are quite small - only a few light days or weeks at most. 

    'The only mechanism we know in the universe that can dump that much energy in such a small volume is a BH.'

    In fact, their analysis shows that the masses of these objects are about 100 times lower than astronomers had assumed.

    Even though they are up to 10 million times more massive than the sun, these black holes are still around 100 times smaller than previously estimated. This makes them much more consistent with theories about the evolution of the universe (artist's impression)

    Even though they are up to 10 million times more massive than the sun, these black holes are still around 100 times smaller than previously estimated. This makes them much more consistent with theories about the evolution of the universe (artist's impression)

    Even though these would be some of the smallest black holes ever discovered, they are still up to 10 million times more massive than the sun and have diameters of over 6.2 million miles (10 million km).

    However, that is still 'small' enough to be consistent with our understanding of how black holes formed after the Big Bang.

    The researchers say this discovery could shed light on how black holes appeared so quickly in the early universe.

    article image

    These young black holes' feeding frenzies could allow them to grow at speeds close to the maximum theoretical rate, known as the Eddington Limit.

    That could explain why astronomers have started to discover black holes with masses up to a billion times greater than the sun, just 700 million years after the Big Bang.

    'We found that the black hole masses are 10 to 100 times smaller than previously supposed, and that they are accreting gas at the limit, so these facts ease up very much on the problem of how they grow so fast,' says Professor Watson. 

    'These black holes are more like one of the missing links between stellar mass black holes and the real monster black holes that lie in quasars that are 1000 times larger than the Little Red Dots.'

    BLACK HOLES HAVE A GRAVITATIONAL PULL SO STRONG NOT EVEN LIGHT CAN ESCAPE

    Black holes are so dense and their gravitational pull is so strong that no form of radiation can escape them - not even light.

    They act as intense sources of gravity which hoover up dust and gas around them. Their intense gravitational pull is thought to be what stars in galaxies orbit around.

    How they are formed is still poorly understood. Astronomers believe they may form when a large cloud of gas up to 100,000 times bigger than the sun, collapses into a black hole.

    Many of these black hole seeds then merge to form much larger supermassive black holes, which are found at the centre of every known massive galaxy.

    Alternatively, a supermassive black hole seed could come from a giant star, about 100 times the sun's mass, that ultimately forms into a black hole after it runs out of fuel and collapses.

    When these giant stars die, they also go 'supernova', a huge explosion that expels the matter from the outer layers of the star into deep space. 

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

    15-01-2026 om 22:07 geschreven door peter  

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    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.China applies to launch 200,000 satellites into space, sparking concerns they plan to build a 'mega-constellation'

    China applies to launch 200,000 satellites into space, sparking concerns they plan to build a 'mega-constellation'

    China has applied to launch almost 200,000 satellites into space, sparking concerns that the nation seeks to build a 'mega-constellation'.

    On December 29, a newly formed body called the Institute of Radio Spectrum Utilisation and Technological Innovation filed applications for two satellite constellations.

    Each of these enormous collections of spacecraft, dubbed CTC-1 and CTC-2, would contain 96,714 satellites spread over 3,660 different orbits.

    If completed, China's new mega-constellation would dwarf even SpaceX's bold ambition to put 49,000 Starlink satellites in orbit.

    Together, CTC-1 and CTC-2 would be the largest assembly of satellites ever put in orbit, and would effectively lock competitors out of a region of low-Earth orbit.

    With Chinese authorities remaining quiet about the satellites' intended use, experts have raised concerns that the constellation may pose a security or defence threat.

    As reported by China in Space, the Nanjing University of Aeronautics claims that the satellites will focus on: 'Low-altitude electromagnetic space security, integrated security defence systems, electromagnetic space security assessment of airspace, and low-altitude airspace safety supervision services.'

    This suggests the constellations may play a similar role to the SpaceX Starshield satellites used by the US military for secure tracking and communications.

    China has filed an application to launch almost 200,000 satellites into orbit, sparking concerns that the country might be building a mega-constellation (stock image)

    China has filed an application to launch almost 200,000 satellites into orbit, sparking concerns that the country might be building a mega-constellation (stock image) 

    These applications were filed with the International Telecommunications Union (ITU), a UN body that allocates spectrum allowances in space.

    With the applications filed, other operators will need to demonstrate to the ITU that new satellites in this orbit won't interfere with the constellation's operations.

    These satellites may have any number of benign functions, from tracking extreme weather and providing navigation for aircraft to offering Starlink-style communication services.

    However, the applications come at a time of increasing tension between the space ambitions of China and the US.

    Not only are the two nations racing to be the first to establish a permanent presence on the moon, but they are also competing for dominance in the field of low-Earth orbit.

    Military satellites form part of the so-called 'kill mesh', an automated network linking sensors, satellites, communications systems and weapons.

    In the war in Ukraine, satellite communications and the ability to jam the enemy's own satellites have been critical to shaping the conflict.

    Additionally, analysts have recently become concerned that the behaviour of China's satellites is becoming increasingly erratic and dangerous.

    The Chinese People's Liberation Army has increasingly pursued space capacity to provide communications and surveillance. Experts are concerned that this new constellation could form part of that capacity

    The Chinese People's Liberation Army has increasingly pursued space capacity to provide communications and surveillance. Experts are concerned that this new constellation could form part of that capacity 

    The constellation may be similar to Starlink's Starshield system for secure communications, which has been used to great effect by Ukrainian troops fighting Russia's invasion (pictured)

    The constellation may be similar to Starlink's Starshield system for secure communications, which has been used to great effect by Ukrainian troops fighting Russia's invasion (pictured) 

    China appears to be testing several 'fast movers' capable of moving around the geostationary orbit belt (GEO), lifting falling satellites back into orbit or potentially sabotaging US space assets.

    Speaking at an event at Chatham House in March, Chief Master Sergeant Ron Lerch, deputy chief of Space Operations for Intelligence with the U.S. Space Force, said: 'There are a number of what the Chinese refer to as these experimental communication satellites that are out in GEO, and yet these GEO satellites.

    'They’re sliding, or they’re moving very frequently across the GEO belt, which is a behaviour that is very uncharacteristic of a satellite that’s intended to provide satellite communication.'

    Mr Lerch added: 'We [U.S. Space Force] see great risk right now because of the unprecedented growth, as well as the unmanaged competition.'

    For its part, China has been clear that it sees space as a legitimate frontier for competition with the US.

    As early as 2021, President Xi Jinping claimed that space was an 'important strategic asset for the country that must be well managed and utilised and, more importantly, protected.'

    China now has approximately 1,000 satellites in orbit, marking a significant increase from around 40 satellites in 2010.

    While these two new constellations might become part of China's growing military space presence, the more serious worry is that they may be part of a 'land grab'.

    China has been clear that it sees space as a legitimate area for competition, with President Xi Jinping (pictured) calling space 'an important strategic asset for the country'

    China has been clear that it sees space as a legitimate area for competition, with President Xi Jinping (pictured) calling space 'an important strategic asset for the country'

    By staking their claim with the ITU, the Institute of Radio Spectrum Utilisation and Technological Innovation has effectively locked off a huge section of GEO.

    Under the ITU's rules, they must launch at least one satellite within seven years of the initial filing, with another seven years to complete launching all the satellites.

    China might have legitimate aims to build the constellations, but there is nothing preventing China from filing a 'dummy' application to lock off a section of space for later use.

    Victoria Samson, Chief Director of space security and stability for Secure World Foundation, told New Scientist: 'It is possible they’re just trying to create some space for later on.'

    This would not be the first time that a nation has attempted such a manoeuvre.

    In 2021, Rwanda filed an application for a constellation of 327,000 satellites in 27 orbits that it had absolutely no realistic ability complete.

    Similarly, it seems extraordinarily unlikely that China even has the capacity to complete CTC-1 and CTC-2 if it wanted to.

    China's commercial sector can currently produce about 300 spacecraft per year, with plans to expand up to 600, while the state can produce several hundred more.

    China does not have the rocket launch capacity to realistically complete this project, launching only 94 rockets last year. This makes it likely that the application is a form of 'land grab' to secure orbital space for future use. Pictured: A Chinese Long March-2F rocket launches in October 2025

    China does not have the rocket launch capacity to realistically complete this project, launching only 94 rockets last year. This makes it likely that the application is a form of 'land grab' to secure orbital space for future use. Pictured: A Chinese Long March-2F rocket launches in October 2025

    However, China would need to launch 500 satellites per week, every week, for seven years to get 200,000 satellites in orbit.

    In 2025, China launched a record 92 rockets into space but hundreds, if not thousands, would be needed to complete the project.

    Even within China, experts don't seem to seriously believe that this project will ever be completed.

    Yang Feng, General Manager of commercial satellite maker Spacety, told China Daily: 'Leading in terms of filing applications does not mean surpassing in final execution.

    article image

    'Turning these plans into operational constellations faces major challenges in terms of systems engineering, manufacturing and launch capacity.'

    This makes it more likely that China is simply attempting to secure a large section of orbit for later use.

    Perhaps ironically, this move comes just weeks after China lambasted SpaceX for creating 'safety and security' concerns by locking off sections of orbit with its own satellite constellations.

    'With the unchecked proliferation of commercial satellite constellations by a certain country, in the absence of effective regulation, has given rise to pronounced safety and security challenges,' a Chinese representative said at an informal UN Security Council event.

    THE NINE FIRMS WORKING ON NASA'S RETURN TO THE MOON

    Astrobiotics' Peregrine lander is one of the many in the running

    Astrobiotics' Peregrine lander is one of the many in the running

    Astrobotic Technology : The Pittsburgh-based firm was founded in 2008 by Carnegie Mellon professor Red Whittaker. It was among the many teams that participated in Google’s $20 million Lunar XPrize, which shut down this year without a winner.

    Astrobiotic’s lunar lander, dubbed Peregrine, stands on four shock-absorbing legs and attaches to the launch vehicle via a standard clamp.

    'The Peregrine Lander precisely and safely delivers payloads to lunar orbit and the lunar surface on each mission,' the firm says.

    'Payloads can be mounted above or below the decks, and can remain attached or deployed according to their needs.'

    Deep Space Systems: The systems engineering company from Colorado is long been a subcontractor to NASA and other aerospace giants, including Lockheed Martin. 

    The firm develops everything from plans and interface control documents to ground software tools for missions. Deep Space Systems says it focuses on the ‘the design, development, integration, testing and operations of science and exploration spacecraft.’

     Their lunar lander concept is a rover that appears to feature smaller scouting robots that can be deployed.

    Draper: The Cambridge, Massachusetts-based laboratory is a not-for-profit research and development organization. Draper develops everything from autonomous systems and biomedical solutions to systems. 

    Notably, Drapers accomplishments include a device that measures cabin air on the International Space Station to check for volatile organic compounds.

    The firm’s concept lander, dubbed Artemis-7, will sit on four mechanical legs to carry out sample collection and return.

    Firefly Aerospace: Firefly showed off a concept for a commercial launch vehicle and a lunar lander. 

    While the firm hasn’t released much detail just yet, it appears to be a three-stage system upon which the lander sits at the very top.

    Intuitive Machines: The Houston-based firm also unveiled a concept lander that looks much like R2D2. 

    The Nova-C lander is the key component of its Lunar Payload and Data Service plan. It’s capable of 24/7 data coverage, and can hold a payload of at least 85 kg.

    The firm says it can land anywhere on the moon.

    The Houston-based firm also unveiled a concept lander that looks much like R2D2 (left). Firefly showed off a concept for a commercial launch vehicle and a lunar lander (right)

    Lockheed Martin: The aerospace giant unveiled its McCandless Lunar Lander, named after late NASA astronaut Bruce McCandless.

    Lockheed Martin named its lunar lander after late NASA astronaut, Bruce McCandless

    Lockheed Martin named its lunar lander after late NASA astronaut, Bruce McCandless

    It’s ‘capable of transporting large payloads weighing hundreds of kilograms – including stationary scientific instruments, deployable rovers, or even sample return vehicles – to the surface of the Moon,’ the firm says.

    ‘The lander uses a proven propulsive landing approach that relies upon on-board radars and a set of rocket thrusters firing 10 times a second to slow to just five mph before touching down. 

    'Once on the lunar surface, the lander can provide power, communications and thermal management for sophisticated payloads.’

    Masten Space Systems: Masten’s XL-1 is a ‘small, single use lander’ that can carry 100-kg payload.

    ‘The XL-1 is designed to offer a mission duration that is minimally sufficient to land on the lunar surface, transmit payload activation commands, and activate the payload release/deployment mechanism,’ the firm says.

    Masten’s XL-1 is a ‘small, single use lander’ that can carry 100-kg payload

    Masten’s XL-1 is a ‘small, single use lander’ that can carry 100-kg payload

    Moon Express: Cape Canaveral-based Moon Express was previously pegged to develop a fleet of low-cost robotic spacecraft that can be assembled like Legos.

    The initial spacecraft, known as MX-1E,is a similar size and shape to the R2D2 droid from Star Wars. It will hop across the lunar surface on its legs.

    Last year, the firm said it hoped its ‘Harvest Moon’ expedition will take place by 2020, including the first commercial sample return mission, which also begins the business phase of lunar resource prospecting.

    Orbit Beyond: The New Jersey firm unveiled a four-legged concept lander that could soon be used to deliver payloads to the moon. The firm has yet to reveal more details on the project.

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

    15-01-2026 om 21:43 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 carries out first-ever medical evacuation from ISS as astronauts return to Earth from space

    NASA has carried out the first-ever medical evacuation of astronauts from the International Space Station (ISS), rushing a four-person crew back to Earth after an in-orbit health emergency.

    The Crew-11 capsule splashed down in the Pacific Ocean off the coast of San Diego, California at approximately 3:41am ET on Thursday, ending a roughly 10-hour return flight after leaving the ISS the day prior.

    The return was prompted by a medical issue that NASA flight surgeons determined could not be fully treated in microgravity.

    On board were NASA astronauts Zena Cardman and Mike Fincke, Japanese astronaut Kimiya Yui and Russian cosmonaut Oleg Platonov. 

    The spacecraft fired its engines to deorbit at 2:50am before enduring a fiery re-entry through Earth's atmosphere, deploying four parachutes to slow its descent into the ocean moments before splashdown.

    A recovery vessel with medical personnel retrieved the capsule at sea, conducted immediate health assessments, and transported the astronauts by helicopter and jet to NASA's Johnson Space Center in Houston for further evaluation.

    The American space agency has declined to identify the affected crew member or disclose the nature of the condition, citing medical privacy.

    NASA administrator Jared Isaacman decided to bring the crew home early out of an abundance of caution, noting that the astronaut's medical episode was considered 'serious' and would require additional medical care on Earth. 

    The spacecraft fired its engines to deorbit at 2:50am before enduring a fiery re-entry through Earth’s atmosphere, deploying four parachutes to slow its descent into the ocean

    The spacecraft fired its engines to deorbit at 2:50am before enduring a fiery re-entry through Earth's atmosphere, deploying four parachutes to slow its descent into the ocean

    Crew-11 before leaving the ISS. Roscosmos cosmonaut Oleg Platonov (Back left), NASA astronaut Mike Fincke (Front left), JAXA astronaut Kimiya Yui (Front right), and NASA's Zena Cardman (Back right)

    Crew-11 before leaving the ISS. Roscosmos cosmonaut Oleg Platonov (Back left), NASA astronaut Mike Fincke (Front left), JAXA astronaut Kimiya Yui (Front right), and NASA's Zena Cardman (Back right)

    A live press briefing was held about one hour after the crew returned to Earth, where Isaacman said the crew member of concern is doing fine, and NASA will release more when possible.

    NASA's chief medical officer, Dr James Polk, said last week they were in stable condition and were not in any immediate danger. 

    He noted that the astronaut's medical condition had nothing to do with an upcoming spacewalk on January 8, which was cancelled, or any other operations on board the station. 

    Boats swarmed the capsule as it bobbed on top of the water, which pulled the craft towards a recovery vessel in the distance, following splashdown.

    The capsule was then hoisted onto the vessel, and the SpaceX ground team quickly went to work cooling it down and removing any debris that may have attached to the hatch door during the descent. 

    The hatch was opened at 3:19am, giving the astronauts their first breath of fresh air since launching to the ISS on August 1.

    Medical doctors were the first to meet the crew for a quick routine health check. 

    Fincke was the first to emerge from the capsule, followed by Cardman, Platonov and Yui. 

    The SpaceX Dragon capsule hit the water at 3:41am, brining the four-person Crew-11 home

    The SpaceX Dragon capsule hit the water at 3:41am, brining the four-person Crew-11 home

    The return capsule was hoisted onto a recover vessel that was waiting nearby in the Pacific Ocean

    The return capsule was hoisted onto a recover vessel that was waiting nearby in the Pacific Ocean

    The crew spent 10 hours soaring through space before splashing down in the Pacific Ocean. Pictured is Crew-11 inside the capsule

    'It's so good to be home,' said Cardman, the capsule commander. This was her first space mission.

    Each astronaut was put on a stretcher, as they had been in zero-gravity for more than 100 days, and then carried off for more medical tests.

    The four astronauts who were evacuated had been trained to handle unexpected medical situations, said Amit Kshatriya, a senior NASA official, praising how they have dealt with the situation. 

    Crew-11 is set to stay overnight at a medical facility outside of San Diego. 

    Michael Fincke was the first to emerge from the capsule (PICTURED)

    Michael Fincke was the first to emerge from the capsule (PICTURED)

    Pictured is cosmonaut Oleg Platonov after emerging from the capsule

    Pictured is cosmonaut Oleg Platonov after emerging from the capsule

    The four astronauts were scheduled to leave after Crew-12 arrived on a new SpaceX Dragon capsule no earlier than February 15.

    Until their arrival, a group including NASA astronaut Chris Williams, who arrived at the ISS aboard a Russian Soyuz spacecraft in November 2025, will be maintaining the station.

    The evacuation followed NASA's Spaceflight Human-System Standard, which mandates contingency return procedures whenever onboard medical resources are insufficient.

    Although statistical models have long predicted that such an event could occur roughly once every three years, the plan has never before been used.

    Located 250 miles above Earth, the ISS functions as a testbed for research that supports deeper space exploration, including eventual missions to return humans to the moon and onward to Mars. 

    The ISS is set to be decommissioned after 2030, with its orbit gradually lowered until it breaks up in the atmosphere over a remote part of the Pacific Ocean called Point Nemo, a spacecraft graveyard.

    RELATED VIDEOS

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

    15-01-2026 om 21:02 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 astronauts seen for first time since medical evacuation

    NASA astronauts seen for first time since medical evacuation

    Story by Matt Cannon

    Astronauts evacuated early from the International Space Station (ISS) due to a medical issue were seen for the first time back on Earth in the early hours of Thursday morning after their SpaceX Dragon craft splashed down off the Californian coast.

    NASA has not given details on who within Crew-11 was experiencing the issue or what the specific problem was, citing patient privacy. Officials have emphasized that it was not an emergency.

    Why It Matters

    This was the first evacuation prompted by a medical issue in NASA’s near 68-year history, and the first from the ISS since it became continuously inhabited in 2000.

    What To Know

    Splashdown occurred at 12:41 a.m. PT (3:41 a.m. ET) in calm waters off San Diego, following a nine-and-a-half-hour ride back to Earth. Crew members had been away from Earth for 167 days. The hatch opened at 1:10 a.m. PT (4:10 a.m. ET).

    The crew, launched in August, were scheduled to remain on the ISS until late February. But the mission was canceled on January 7, meaning a planned spacewalk by Zena Cardman and Michael Fincke the next day did not take place.

    The ailing astronaut is “stable, safe and well cared for,” outgoing space station commander Fincke said earlier this week via social media. “This was a deliberate decision to allow the right medical evaluations to happen on the ground, where the full range of diagnostic capability exists.”

    NASA astronaut Fincke was first to exit the craft before his fellow American, and mission commander, Cardman. JAXA (the Japan’s space agency) astronaut Kimiya Yu and then Roscosmos (Russia’s space agency) cosmonaut Oleg Platonov followed.

    Crew members were given an initial medical check by a SpaceX medical doctor as they disembarked, NASA said. The space agency’s live footage of the event showed all four crew members were carried away on stretchers.

    Pennsylvanian Fincke, a veteran of three previous ISS trips, was seen smiling and giving a thumbs-up as he was helped on to a stretcher.

    NASA astronauts Mike Fincke gives a thumbs-up.

    NASA astronauts Mike Fincke gives a thumbs-up.

    NASA astronaut Zena Cardman, the mission commander, returns.

    NASA astronaut Zena Cardman, the mission commander, returns.

    Mission commander Cardman, a Virginia native who was on her first ISS mission, was also seen smiling as she waved and pointed to someone out of shot.

    Yu gave a double wave as he was pushed away on a stretcher. He had just completed 300 days in space across two missions, NASA said.

    Platonov raised his arms and gave a double thumbs-up as he was carried away.

    NASA and Roscosmos take turns transporting each other’s astronauts or cosmonauts between Earth and the ISS under one of few remaining cooperation agreements between the United States and Russia following Moscow’s invasion of Ukraine.

    Japanese astronaut Kimiya Yu.

    Japanese astronaut Kimiya Yu.

    Russian cosmonaut Oleg Platonov.

    Russian cosmonaut Oleg Platonov.

    What People Are Saying 

    NASA announced on January 8 that the early evacuation would take place, saying: “NASA announced on Thursday its decision to return the agency’s SpaceX Crew-11 mission to Earth from the International Space Station earlier than originally planned as teams monitor a medical concern with a crew member currently living and working aboard the orbital laboratory.”

    Asked at a January 8 news conference about the medical issue, NASA administrator Jared Isaacman said: “This was a serious medical condition; that is why we’re pursuing this path. [The] Crew member’s stable. As we mentioned, we’re not electing an emergency deorbit. But obviously, as we’ve already communicated, the capability to diagnose and treat this properly does not live on the International Space Station. And I think there’s pretty broad agreement across our experts here on the ground, as well as the crew members in space. So I think there’s complete alignment around that point.”

    “Our timing of this departure is unexpected,” NASA astronaut Zena Cardman said before the return trip, “but what was not surprising to me was how well this crew came together as a family to help each other and just take care of each other.”

    What Happens Next

    NASA was scheduled to hold a news conference at 2:45 a.m. PT (5:45 a.m. ET).

    Update 1/15/2026 6:17 a.m. ET: This article has been updated with more information.

    The news cycle is loud. Algorithms push us to extremes. In the middle—where facts, ideas and progress live—there’s a void. At Newsweek, we fill it with fearless, fair and fiercely independent journalism.

    Common ground isn’t just possible—it’s essential. Our readers reflect America’s diversity, united by a desire for thoughtful, unbiased news. Independent ratings confirm our approach: NewsGuard gives us 100/100 for reliability, and AllSides places us firmly in the political center.

    In a polarized era, the center is dismissed as bland. Ours is different: The Courageous Center—it’s not “both sides,” it’s sharp, challenging and alive with ideas. We follow facts, not factions. If that sounds like the kind of journalism you want to see thrive, we need you..

    RELATED VIDEOS


    newsweek.com }

    15-01-2026 om 18:24 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART
    14-01-2026
    Klik hier om een link te hebben waarmee u dit artikel later terug kunt lezen.Scientists discover extraterrestrial relics in the first samples from moon's mysterious far side

    A human space probe has brought back an ancient extraterrestrial visitor from the moon, rewriting the early history of the solar system. 

    China's Chang'e-6 spacecraft made history in June 2024 by returning the first-ever samples from the moon's far side, a region humans had never explored before.

    In a new study, scientists examined the dusty soil from an ancient crater called the Apollo basin and found seven tiny rock pieces that didn't belong to anything that naturally formed on the moon's surface.

    These small fragments turned out to be leftovers from ancient asteroids that crashed into the moon billions of years ago.

    Unlike normal moon rocks, these pieces came from watery asteroids that floated into space between Mars and Jupiter, making them true 'extraterrestrial relics' from outside our planet.

    Moreover, scientists from the Chinese Academy of Sciences discovered that the relics came from the same type of space rocks that likely delivered chemicals necessary to spark life on planets like Earth billions of years ago.

    Asteroids like these delivered water and other key ingredients to the moon early in its history, possibly helping create its thin water ice deposits we see today.

    On a larger scale, the new findings have rewritten our understanding of how space rocks shaped the Earth and moon, since Earth's meteorite finds are limited by our atmosphere and gravity, burning up potential samples before they can be studied.

    China's Chang'e-6 lander (pictured) returned to Earth in June 2024 and scientists have just uncovered an extraterrestrial relic deposited by an asteroid in the moon samples

    China's Chang'e-6 lander (pictured) returned to Earth in June 2024 and scientists have just uncovered an extraterrestrial relic deposited by an asteroid in the moon samples 

    The samples (pictured) are completely foreign compared to the makeup of the moon, meaning asteroids likely brought the ice water found on the lunar surface

    The samples (pictured) are completely foreign compared to the makeup of the moon, meaning asteroids likely brought the ice water found on the lunar surface

    The far side of the moon is the hidden half we never see because our planet and the moon are tidally locked, meaning we always see the same face from our perspective.

    Specifically, the team identified these seven fragments as leftovers from a rare type of asteroid called CI-like carbonaceous chondrites.

    At the heart of these mysterious samples were tiny green crystals called olivine, which look like olive-shaped gems and make up the backbone of the asteroids they came from.

    Finding olivine in these space rocks was special because it's loaded with water trapped inside, plus just the right mix of iron, zinc, and other metals not seen across the relatively dry moon.

    The samples matched the composition of other nearby asteroids that astronomers and recently studied, including Ryugu, studied by Japan's Hayabusa2 mission, and Bennu, studied by NASA's OSIRIS-REx.

    The research in the Proceedings of the National Academy of Sciences (PNAS) noted that most of the rocks ever taken back from the moon formed there over time.

    Scientists knew the new samples from Chang'e-6 didn't form on the moon because of their makeup and hidden chemical fingerprints, which included 10 to 20 percent water trapped in clay-like minerals, amino acids, and tar-like carbon compounds.

    Scientists also uncovered lightweight gases like hydrogen, nitrogen, and sulfur, making these relics from space resemble soggy sponges carrying the seeds of oceans and air.

    The Chinese lander collected over four pounds of rocks from the lunar surface after successfully landing on the moon's far side in May 2024

    The Chinese lander collected over four pounds of rocks from the lunar surface after successfully landing on the moon's far side in May 2024

    article image

    Typical Moon rocks are mostly dry black lava stone and white feldspar, made from iron-heavy minerals, calcium, aluminum, and titanium, with almost no water at all.

    'This finding supports the hypothesis that asteroids played a role in delivering water and other volatiles to the lunar surface,' the researchers wrote.

    Experts believe these asteroid bits crashed into the moon's far side over four billion years ago, during the chaotic formation of the early solar system, when giant impacts blasted materials across planets.

    The discovery appeared to prove that a similar process involving water-carrying asteroids took place on the moon that scientists suspect occurred on Earth at the dawn of time.

    One theory argues that asteroid collisions like the ones found on the moon are believed to have slammed into our planet as well, creating oceans and scattering amino acids - the basic ingredients that kickstarted tiny life forms in Earth's warm pools.

    Scientists believe the same asteroid rain hit other planets, too, like Mars, where it might have created ancient rivers and maybe even early microbes hiding underground today.

    Even icy moons like Europa around Jupiter could have gotten a life-giving boost from these asteroids, delivering heat, water, and chemicals deep into their frozen oceans to brew something organic.

    NASA, China, and India have all announced that they will be sending additional missions to the moon before 2030, including manned missions by the US.

    RELATED VIDEOS

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

    14-01-2026 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.NASA sets historic date for returning Americans to the moon after 53 years

    NASA has announced that America is now just weeks away from a historic return to the moon for the first time in over 50 years.

    The space agency revealed on Tuesday that the earliest Artemis II, the first manned mission to the moon since 1972, will launch on February 6.

    NASA officials noted that the official launch window for Artemis II will remain open from January 31 to February 14, with several alternate dates also being picked out.

    The mission will take NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and Canadian Space Agency astronaut Jeremy Hansen on a 10-day journey around the moon and back to Earth.

    The Artemis II mission will not land on the moon's surface. The first lunar landing in the Artemis program is scheduled for Artemis III, currently planned to take place in 2027. 

    Artemis II can't launch on just any day. The timing will depend on precise orbital mechanics, such as where Earth and the moon are positioned, rocket performance, and weather conditions near the launch site at Kennedy Space Center in Florida.

    February 7, 8, 10, and 11 have been chosen as potential backup launch dates. If something prevents the launch in February, NASA has also picked out dates in early March and April for the upcoming moon mission.

    Artemis II will be the first space mission with a human crew in 53 years to go beyond low Earth orbit.

    (From left to right) Astronauts Jeremy Hansen, Victor Glover, Reid Wiseman, and Christina Koch pose in their flight suits for the Artemis II mission, scheduled for February 2026

    (From left to right) Astronauts Jeremy Hansen, Victor Glover, Reid Wiseman, and Christina Koch pose in their flight suits for the Artemis II mission, scheduled for February 2026

    NASA's new moon rocket lifted off from Launch Pad 39B at the Kennedy Space Center in Florida on November 16, 2022. It was the first test fight of the Artemis program

    NASA's new moon rocket lifted off from Launch Pad 39B at the Kennedy Space Center in Florida on November 16, 2022. It was the first test fight of the Artemis program

    As early as February 6, the astronauts will launch from Cape Canaveral in an Orion spacecraft, carried by NASA's powerful Space Launch System (SLS) rocket system.

    They'll first orbit Earth a couple of times to test the life support equipment and then head toward the moon for a lunar flyby, a close pass without orbiting or landing.

    The spacecraft will use the moon's gravity to slingshot back toward Earth in a 'free-return trajectory', meaning if anything goes wrong, it can safely return without extra use of its engines.

    The main goal of the mission will be to prove the rocket, spacecraft, and systems work perfectly with humans on board, paving the way for Artemis III's landing next year.

    NASA is less than a week away from the first part of this historic event, the rollout, set to begin as soon as January 17.

    The fully stacked SLS rocket and Orion spacecraft are scheduled to 'roll out' from NASA's Vehicle Assembly Building to Launch Pad 39B at Kennedy Space Center.

    It's a four-mile trip that uses a giant crawler-transporter to carry the rocket and can take up to 12 hours to complete.

    Once at the pad, teams will connect power and fuel lines and do final rocket testing before the astronauts start their walkthrough for the flight.

    Join the debate

    Should NASA focus on returning to the moon or prioritize missions to Mars instead?

    Comment now
    NASA’s SLS (Space Launch System) rocket, which will carry the Artemis II spacecraft, is seen inside High Bay 3 of the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida

    NASA's SLS (Space Launch System) rocket, which will carry the Artemis II spacecraft, is seen inside High Bay 3 of the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida

    article image

    Once Artemis II is on the launch pad, NASA crews will go through what's called a 'wet dress rehearsal' and 'tanking' procedure.

    They'll load the SLS rocket with over 700,000 gallons of super-cold liquid hydrogen and oxygen, which act as the propellants that ignite and blast the craft into space.

    NASA will even run through a fake countdown to launch, practice holds and restarts, and then safely drain the tanks of the fuel until it's time for the real launch.

    The rehearsal tests the space agency's fueling procedures and helps check for any problems with the rocket, such as leaks in the rocket tanks or valves.

    If any problems are spotted, NASA will likely need to run multiple rehearsals and possibly delay the launch.

    In September 2025, former NASA Administrator Sean Duffy publicly announced that 'about a year and a half' after the Artemis II mission, the Artemis III astronaut mission would 'land and establish a long-term presence of life on the moon led by America'.

    He continued by saying that what astronauts learn from the renewed missions to the moon will help in future efforts to 'put American boots on Mars'.

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

    14-01-2026 om 22:50 geschreven door peter  

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    Categorie:ASTRONOMIE / RUIMTEVAART


    Hello GIFs – Fun Animated Images to Greet Anyone - Funimada.com

    Item preview, Colorful UFO Design with Hello Text designed and sold by Rue Market.

    Ufo GIFs | Tenor


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