Catherine Stoddard

Astronomer’s at NASA discovered a supermassive black hole that has a Death Star-like jet shooting out at the core of a huge galaxy and it appears that stars along the beam’s trajectory are exploding.

"We don't know what's going on, but it's just a very exciting finding," said Alec Lessing of Stanford University, lead author of the paper published in The Astrophysical Journal. "This means there's something missing from our understanding of how black hole jets interact with their surroundings."

Stars are exploding but not destroyed

The stars that are exploding along the trajectory of the giant blowtorch-like beam are called novae.

The Hubble found that twice as many novae near the beam of plasma are exploding twice as much as compared to anywhere else in the galaxy during the surveyed time period.

These stars typically erupt in a double-star system where an aging star begins to spill hydrogen into a burned out white dwarf star companion, NASA explained. 

When the dwarf star has its fill of hydrogen, it explodes like a giant nuclear bomb. But the dwarf is not destroyed in this process, it simply starts this cycle over again.

While it has been theorized that the heat from the jet is leading to the novae explosions, researchers said it is not nearly hot enough in the observed locations to have this type of impact on the stars.

Researchers are still trying to figure out what’s going on.

"There's something that the jet is doing to the star systems that wander into the surrounding  neighborhood. Maybe the jet somehow snowplows hydrogen fuel onto the white dwarfs, causing them to erupt more frequently," said Lessing. "But it's not clear that it's a physical pushing. It could be the effect of the pressure of the light emanating from the jet. When you deliver hydrogen faster, you get eruptions faster. Something might be doubling the mass transfer rate onto the white dwarfs near the jet."

What is the jet of light?

A Hubble Space Telescope image of the giant galaxy M87 shows a 3,000-light-year-long jet of plasma blasting from the galaxy's 6.5-billion-solar-mass central black hole.

(NASA, ESA, STScI, Alec Lessing (Stanford University), Mike Shara (AMNH))

The jet is being shot out by a 6.5 billion-solar-mass central black hole which is engorged with infalling matter, NASA said.

The black hole is launching a 3,000-light-year-long jet of plasma that is blazing through space nearly at the speed of light.

Anything that is caught directly, or near, the jet "would be sizzled."

The Source

• Information for this article was gathered from NASA. This story was reported from Los Angeles. 

{ https://www.yahoo.com/news/ }

01-10-2024 om 22:26 geschreven door peter  

NASA engineers have successfully reactivated a set of thrusters on Voyager 1, unused for decades, to keep the 47-year-old spacecraft communicating with Earth. With the probe billions of miles from our planet, this maneuver was critical to ensuring it stays on course. The aging spacecraft continues to surprise with its resilience.

By Julian James

Voyager 1’s Ongoing Journey

NASA's Voyager 1 Fires Dormant Thrusters After Decades

© Provided by Ever-Growing

Voyager 1, launched in 1977, has far exceeded its expected lifespan, continuing to transmit data from interstellar space. Currently about 15 billion miles from Earth, the probe travels beyond the heliosphere, the Sun’s protective bubble of magnetic fields. As its components age, new challenges arise, requiring NASA engineers to find creative solutions to keep the mission alive. One such challenge emerged this year when the spacecraft’s thrusters started clogging, threatening its ability to communicate.

01-10-2024 om 21:59 geschreven door peter  

{ https://scientias.nl/ }

01-10-2024 om 00:29 geschreven door peter  

Een nieuwe studie werpt licht op het intrigerende mysterie van Mars’ ontbrekende atmosfeer. Want mogelijk verbergt die zich wel vol in het zicht…

Mars was niet altijd de kille woestijn die we nu kennen. Er zijn steeds meer aanwijzingen dat er miljarden jaren geleden water over het oppervlak van de rode planeet stroomde. En als er water was, dan moet er ook een dikke atmosfeer zijn geweest om te voorkomen dat het bevroor. Maar zo’n 3,5 miljard jaar geleden droogde het water op en de lucht, die ooit vol koolstofdioxide zat, werd aanzienlijk dunner. Hierdoor wordt onze naaste buur nu nog slechts omhuld door een flinterdunne atmosfeer. Een vraag waar wetenschappers zich al jaren het hoofd over breken, is wat er precies met de Martiaanse atmosfeer is gebeurd. Twee geologen komen nu in het vakblad Science Advances met een verrassende theorie.

Klei
Volgens de twee geologen zou het antwoord mogelijk te vinden kunnen zijn in de klei van de planeet. In hun artikel suggereren ze dat een aanzienlijk deel van de verloren atmosfeer van Mars mogelijk is opgeslagen in de kleiachtige korst. Ze stellen dat het vloeibare water dat ooit zo rijkelijk over Mars stroomde, door bepaalde soorten gesteente had kunnen sijpelen, wat een langzame kettingreactie zou hebben opgestart. Deze reactie zou geleidelijk koolstofdioxide uit de atmosfeer hebben onttrokken en omgezet in methaan — een vorm van koolstof die gedurende lange tijd in de klei van de planeet kan worden opgeslagen.

Aarde
Deze theorie is niet eens zo vergezocht. Vergelijkbare processen komen namelijk ook voor in bepaalde gebieden op aarde. De onderzoekers hebben dan ook hun kennis van de interacties tussen gesteenten en gassen op aarde gebruikt om te begrijpen hoe soortgelijke processen op Mars zouden kunnen werken. Ze ontdekten dat, rekening houdend met de geschatte hoeveelheid klei die het oppervlak van Mars bedekt, deze klei tot 1,7 bar koolstofdioxide zou kunnen vasthouden. Dit zou ongeveer 80 procent van de oorspronkelijke atmosfeer van de planeet vertegenwoordigen.

Deze afbeelding toont de geleidelijke verandering van ijzerrijke rotsen op Mars wanneer deze in contact komen met water dat CO2 uit de atmosfeer bevat. In de loop van miljarden jaren zou dit proces voldoende CO2 in de kleilaag hebben kunnen opslaan, in de vorm van methaan, om het grootste deel van het CO2 te verklaren dat uit de vroege atmosfeer van de planeet is verdwenen.

Afbeelding: Courtesy of Joshua Murray, Oliver Jagoutz, et al.

Smectiet
Concreet zou de Martiaanse atmosfeer weleens opgegaan kunnen zijn in een soort oppervlakte-klei mineraal genaamd smectiet, dat bekend staat als een zeer efficiënte opslagplaats voor koolstof. In een enkele korrel smectiet zitten talloze ‘plooien’ waarin koolstof miljarden jaren lang ongestoord kan blijven. De onderzoekers hebben aangetoond dat de aanwezigheid van smectiet op aarde waarschijnlijk het resultaat is van tektonische activiteit. Zodra het aan het oppervlak kwam, konden de kleimineralen genoeg koolstofdioxide uit de atmosfeer opnemen en opslaan, waardoor de planeet gedurende miljoenen jaren afkoelde. Ook Mars blijkt bedekt te zijn met dezelfde smectiet-klei. De onderzoekers vroegen zich daarom af of deze klei op Mars een vergelijkbare functie zou kunnen hebben gehad in het vasthouden van koolstof. En als dat het geval is, hoeveel koolstof zou de klei dan kunnen opslaan?

Smectiet-klei op Mars
Zoals je hierboven kunt lezen, ontstaat smectiet op aarde door de beweging van continentale platen en het naar boven brengen van rotsen uit de mantel. Mars kent echter geen soortgelijke tektonische activiteit. Hoe het kan dat Mars dan toch bedekt is met smectiet-klei? In de loop van ongeveer een miljard jaar zou het water dat door de korst sijpelde geleidelijk reageren met olivijn. Wetenschappers denken dat de Martiaanse korst voornamelijk uit stollingsgesteente bestaat dat rijk is aan olivijn, een mineraal dat een gereduceerde vorm van ijzer bevat. Zuurstofmoleculen in het water zouden zich aan het ijzer hechten, waardoor waterstof vrijkomt en het rode geoxideerde ijzer ontstaat dat de planeet zijn herkenbare kleur geeft. Deze vrijgekomen waterstof zou vervolgens met koolstofdioxide in het water hebben gereageerd om methaan te vormen. Naarmate deze reactie in de loop van de tijd vorderde, zou olivijn langzaam zijn omgevormd tot een ander soort ijzerrijk gesteente, bekend als serpentijn, dat daarna bleef reageren met water om smectiet te vormen.

Na een rekensommetje kwamen de onderzoekers tot een interessante ontdekking. Als Mars bedekt is met een laag smectiet van 1.100 meter diep, zou deze hoeveelheid klei in staat zijn om een enorme hoeveelheid methaan op te slaan. Dit zou overeenkomen met het merendeel van het koolstofdioxide in de atmosfeer dat sinds het opdrogen van de planeet verloren is gegaan. “We constateren dat de schattingen van de wereldwijde klei-volumes op Mars overeenkomen met een groot deel van de oorspronkelijke CO2 van de planeet, dat is vastgelegd als organische verbindingen in de kleirijke korst,” zegt onderzoeker Joshua Murray. “In zekere zin zou de ontbrekende atmosfeer van Mars zich weleens in het volle zicht kunnen verbergen.”

Kortom, de onderzoekers hypothetiseren dat de verloren koolstofdioxide mogelijk is opgeslagen in de kleiachtige oppervlakken van Mars. “Mogelijk hebben zich dus op de aarde en Mars soortgelijke processen voorgedaan,” denkt onderzoeker Oliver Jagoutz. “Grote hoeveelheden atmosferisch CO2 zouden kunnen zijn omgezet in methaan en in de klei zijn opgeslagen.” Deze ontdekking is niet alleen belangrijk voor de wetenschap van Mars, maar heeft ook implicaties voor toekomstige missies naar de planeet. Zo suggereren de onderzoekers dat deze opgeslagen Martiaanse koolstof op een dag weer kan worden teruggewonnen en omgezet in brandstof. “Mogelijk is er nog steeds methaan aanwezig,” stelt Jagoutz. “Dit zou in de toekomst als energiebron op Mars kunnen worden gebruikt.”

Bronmateriaal

• "Mars’ missing atmosphere could be hiding in plain sight" - Massachusetts Institute of Technology (via EurekAlert)
  
• Afbeelding bovenaan dit artikel: via Canva Pro

{ https://scientias.nl/ }

30-09-2024 om 23:53 geschreven door peter  

The brains of NASA's Europa Clipper spacecraft are stored in a metal vault.

It's where the large exploration vehicle — the length of a basketball court — safeguards its computers, software, and many electronics. The craft is about to launch to Jupiter's moon Europa, a world planetary scientists suspect harbors an ocean twice the volume of Earth's. With around 50 close swoops by Europa, NASA will be able to confidently answer the question of whether this ocean realm also hosts the ingredients, such as an energy source and telltale materials, to support life.

Credit: NASA / JPL-Caltech

Yet the radiation environs there are particularly harsh.

"The charged particle environment at Europa's location is immense," Cynthia Phillips, a NASA planetary geologist and project staff scientist for the space agency's Europa Clipper mission, told Mashable.

Jupiter, a gas giant planet 317 times more massive than Earth, generates a massive magnetic field shooting out between 600,000 to 2 million miles (1 to 3 million kilometers) toward the sun. It's created by the planet's liquid metal core, which spins and creates electrical currents (moving electric charges make magnetic fields). Crucially, this magnetic field grabs and then accelerates particles from the relentless solar wind — a stream of rapidly traveling charged particles emitted by the sun — which creates potent radiation belts around Jupiter.

"It bombards everything."

Any craft traveling around the planet will almost certainly pass through these hazardous zones and expose instruments to harmful particles, which can damage computer chips and electronics. "It bombards everything," Curt Niebur, Europa Clipper's program scientist, said at a press conference leading up to the mission's launch. Decades ago, during the Voyager mission, NASA's engineers were worried about the craft passing by Jupiter. A person hypothetically riding aboard Voyager as it passed Jupiter would have gotten hit with a radiation dose 1,000 times the lethal level.

A depiction of Jupiter's sprawling magnetic field. If was visible to the naked eye, "it would appear two to three times the size of the sun or moon to viewers on Earth," NASA explained.

Hence, the vault. "The vault seriously reduces the harmful radiation these electronics get," Phillips said. (NASA's Juno craft, exploring the greater Jupiter system, also carries a vault.)

Yet there are electronics outside this protective metallic box. And in May NASA received test data that suggested some transistors — which are electrical switches that control how electricity flows around the spacecraft — couldn't withstand the high radiation environs around Europa. Fortunately, intensive follow-up testing showed these switches will work as the craft makes some 50 flybys over three and a half years. "They unequivocally passed that review today," Nicola Fox, who heads NASA's Science Mission Directorate, said following a pivotal September decision to green-light the mission.

Related video:

• https://youtu.be/9rm8LMWxag8

• ISS Humanity’s Space Lab! (Newsworthy Women)
  

But mission engineers will be watching these transistors closely. As the New York Times reported, NASA bolted a late add-on to the craft, a small "canary box" holding the different types of transistors. If any show signs of damage or dysfunction as Europa Clipper swoops through belts of radiation, planners could adapt the mission.

In this graphic, the box illuminated in red shows the Europa Clipper's vault on the center of the spacecraft.

Already, the mission's orbital plan — which is to zip away from damaging regions after making close flybys of the ice-covered moon — minimizes the time the craft is exposed to high radiation zones. During each orbit around Jupiter, the craft will spend under a day in an irradiated zone, before swooping out. It won't return for between two to three weeks.

"You get out of there," Phillips told Mashable.

"You get out of there."

The robotic spacecraft's exposure to radiation, however, comes with rewards. When the probe dips close to Europa between 2031 and 2034, it will have the chance to view, scan, and investigate Europa in unprecedented detail. A ground-penetrating radar will look under the ice, and potentially see areas of liquid water or even where the ice meets the alien ocean. An instrument called the SUrface Dust Analyzer, or SUDA, will literally sample particles of Europa that have been ejected into space by tiny meteorites. And, of course, Europa Clipper will capture a bounty of images.

"The images are going to be spectacular," said Laurie Leshin, director of NASA’s Jet Propulsion Laboratory, the agency center that built the craft.

In sum, with this orbiting laboratory of instruments, NASA will be able to determine if the ocean moon has the right stuff — energy sources, a long-lived stable ocean, organic compounds (like carbon) — for life. If so, the agency plans to return to Europa and land on the icy crust. This time, they won't just be looking to see if it's habitable. They'll drill into the ice, looking to see if it's inhabited.

"We'll be knocking on the door for a second mission," Niebur said.

{ https://www.msn.com/en-us/ }

30-09-2024 om 23:22 geschreven door peter  

New Map Reveals Impressive Megastructures in Local Universe

The newly-developed map of the local Universe is based on the motions of 56,000 galaxies, according to a team of astrophysicists from the Leibniz Institute for Astrophysics Potsdam.

This map shows the distribution of matter in the local Universe; it shows how matter flows, i.e. along which trajectories (thin lines) the galaxies move.

Image credit: Valade et al., doi: 10.1038/s41550-024-02370-0.

“Mapping the Universe has always been one of the most challenging tasks in astronomy,” said lead author Dr. Aurelien Valade and colleagues.

“Inaccurate observations, observational errors and incomplete data make this work extremely difficult.”

“In addition, the observed galaxies make up only a small part of the total mass in the Universe, as much of the matter exists in the form of invisible dark matter.”

“Furthermore, galaxies are not bound to be formed in such a way that they accurately trace the underlying matter well, which makes them an uncertain indicator of the matter distribution in the Universe.”

“Therefore, in order to create a map of our cosmic environment, we also look at the motion of galaxies.”

“On the one hand, galaxies move away from us with the expansion of the Universe, but on the other hand they also attract each other due to gravity.”

“These movements can be mapped and reveal the cosmic currents — the rivers and gulf-streams throughout the cosmos on which galaxies move.”

“Since the motion is caused by gravity, it can thus be used to see the invisible.”

To create a map of the local Universe, the authors used data on the motions of 56,000 galaxies from the Cosmic Flows-4 catalogue.

“Since the measurements of each galaxy’s velocity are error prone and fairly uncertain, there are various possible cosmographic maps that would fit the observational data,” they explained.

“Thus, we developed a new approach: a ‘probabilistic’ map of the Universe.”

“Such a map indicates how likely it is that a certain feature, such as a ‘basin of attraction,’ actually exists.”

“A basin of attraction is a region which, absent the cosmic expansion, would collapse to a single point.”

With this new method, the researchers obtained a reliable picture of the large-scale distribution of matter and revealed astonishing structures of our cosmic neighborhood.

“Laniakea, the supercluster to which many believed that our Galaxy belongs, is probably merely an appendage of the much larger Shapley basin. It may not even exist as a separate entity,” they said.

“Even more astonishing is the fact that the Sloan Great Wall — an immense wall composed of hundreds of thousands of galaxies — at around a thousand trillion trillion cubic light years is currently the largest known structure in this cosmic network of galaxies.”

“It is perhaps unsurprising that the further into the cosmos we look, we find that our home supercluster is more connected and more extensive than we thought,” said Dr. Noam Libeskind, co-author on the study.

“Discovering that there is a good chance that we are part of a much larger structure is exciting.”

{ https://www.sci.news/ }

30-09-2024 om 21:52 geschreven door peter  

Earth to Pass Through the Same Taurid Meteor Stream in 2032 That May Have Triggered a Mass Extinction 12,800 Years Ago

Earth will travel right in front of the same Taurid meteor stream in 2032 that caused a mass extinction and worldwide flood ~12,800 years ago, plunging Earth into a mini-Ice Age for 1,300 years. Graham Hancock was right all this time but we did not listen to him.

Our solar system is a dangerous place, and every month Earth inches closer to one of its riskier places, the “Taurid swarm” of meteors. Our planet is predicted to pass directly through the “Taurid swarm” in November 2032.

An ancient monument found in Turkey might be more than just a monument—it could be the world’s oldest solar calendar. Researchers from the University of Edinburgh studied symbols carved on the pillars of Göbekli Tepe, a large, ancient site in southern Turkey. They think these carvings were used to track days, seasons, and years, like a calendar. (Source)

The team noticed that each “V” shape carved on the pillars might represent one day. One pillar even had 365 “V”s, the same number as days in a year. They also found that a special “V” around the neck of a bird-like figure could represent the summer solstice—the longest day of the year. This might explain why the “V” symbol shows up on many other statues in the area, often around the necks of figures connected to time and creation.

Mini Ice Age

The ancient calendar focused on tracking day, night, and seasonal changes, which might have become more important after a major comet hit Earth around 10,850 B.C. This event likely caused a mini-ice age that wiped out many species. According to Martin Sweatman, a researcher from the University of Edinburgh, the people at Gobekli Tepe were careful observers of the sky, possibly because the comet strike had changed their world.

This disaster may have sparked the beginning of civilization by starting new religious beliefs and pushing people to develop agriculture to survive the colder climate. Their carvings might be some of the earliest attempts at writing. These carvings also tracked the cycles of the Moon and Sun, long before similar calendars were made. They may have even shown for the first time that comet strikes are more likely to happen when Earth crosses the path of comet fragments, something that modern scientists have confirmed.

To help support this theory, the team points to another pillar at the site appearing to picture the Taurid meteor stream lasting 27 days, which was quite possibly the source of the ancient comet strike. The researchers believe that the temple carvings show the ancient civilization was recording dates precisely, noting how the movement of constellations across the sky differed based on the time of the year. This would be 10,000 years before Hipparchus of ancient Greece documented the wobble in the Earth’s axis in 150 BC, making this newfound calendar well ahead of its time.

The Younger Dryas boundary (YDB) cosmic-impact hypothesis suggests that around 12,800 years ago, Earth was hit by pieces of a large comet, which broke apart as it entered the inner solar system. This event likely caused a chain reaction, leading to an “impact winter” (a period of intense cold) and a climate change episode called the Younger Dryas (YD). (Source)

The collision is also believed to have caused massive wildfires, the extinction of large animals like mammoths, and changes in human cultures and population decline. Evidence of this impact includes unusually high levels of platinum found at 26 sites across the Northern Hemisphere, including in ice cores from Greenland, which show platinum deposits over a 21-year period.

The start of the Younger Dryas also shows an increase in dust and chemicals linked to wildfires, like ammonium and other burning aerosols, found in ice cores from Greenland, Antarctica, and Russia. These signs point to one of the biggest wildfire events in over 120,000 years, with about 9% of Earth’s forests burned, covering 10 million square kilometers.

This large-scale burning and the cooling effect of the impact may have triggered the Younger Dryas climate change, according to the theory.

A 2021 study (Taurid complex smoking gun) found that 88 near-Earth asteroids, hidden in the debris that creates the Taurid Meteor Shower, likely came from the breakup of a single comet about 20,000 years ago. Astronomers at the University of Antioquia in Colombia studied the ‘Taurid complex’ to learn more about where these objects came from.

In the 1980s, scientists William Napier and Victor Clube noticed large asteroids in the Taurid stream. They suggested these asteroids had the same origin as Comet Encke, which orbits the Sun every three years. However, some asteroids are over a mile wide, meaning they couldn’t have come from Comet Encke itself. Scientists Ignacio Ferrín and Vincenzo Orofino reviewed old research and measured light reflected from the larger asteroids.

They found more evidence that both Comet Encke and the big asteroids came from the breakup of a huge ice comet, 62 miles wide, about 20,000 years ago. The team warned that these asteroids could be dangerous to Earth, and others from the ancient comet might have already hit our planet in the past. Every year, Earth passes through a stream of debris, causing shooting stars to appear in October in the southern hemisphere and November in the north.

Comet Encke, first seen in 1786, left a trail of debris as it got closer to the sun, like other comets. This trail, made up of rocks, dust, and debris, sometimes comes close to Earth, leading to lots of scientific study. Some studies focus on larger asteroids.

Experts think impacts from the Taurid stream may have contributed to the extinction of ancient cultures and global cooling during the Younger Dryas period. The 1908 Tunguska event, where a small asteroid exploded above Russia, destroying millions of trees, is believed to be connected to this debris stream.

In 2013, the Chelyabinsk meteor, which injured over 1,500 people in Russia, may have also come from the Taurid stream. In 2005, NASA astronomer Rob Suggs observed a flash from a meteor hitting the moon, which was part of the Taurid meteor shower.

A team of Colombian researchers, along with astronomers from Italy’s University of Salento, reviewed many studies on space impacts. They confirmed that a group of space objects contains up to 88 large pieces. Using a method called secular light curves, they noticed changes in the brightness of these objects and found that 67% showed signs of “comet-like” activity. This supported the idea that these objects came from a common origin.

Napier, another scientist, supported their findings. He said that these asteroids, which have orbits like Comet Encke, could either be affected by unknown forces or are pieces of a larger, older comet that lost its gases. This original comet may have been a “rubble pile” – a mix of rocks and other materials held together by ice. Over time, this pile could have broken apart, possibly due to forces from the Sun or another object, creating smaller fragments.

One asteroid, Oljato, is an example of a rubble pile. It’s still held together by ice, which gives it comet-like activity, but it’s much smaller than its parent. Bigger inactive objects like Morpheus are similar, but their ice is trapped inside. Smaller objects, like 2006 SO198, might be the original rocky pieces. The team explained that even if an object looks like a regular asteroid, it could still have a comet-like origin.

Taurid meteors, part of this group, are usually larger than normal meteors. They shine brightly and go deeper into the Earth’s atmosphere, sometimes creating fireballs. While this is mostly harmless, the discovery of larger asteroids in one “dangerous” part of the meteor stream could be a real threat.

Earth passes through this risky area every few years, leading to more shooting stars and possibly large objects hitting Earth instead of burning up in the atmosphere. Future encounters are expected in 2022, 2025, 2032, and 2039.

In 2021, David Asher, Armagh Observatory astronomer predicted that in 2032 and 2036 we are likely to pass through the centre of the Taurid complex, where there will be a ‘noticeable enhancement of fireballs.’ According to study [Taurid complex smoking gun] authors Ignacio Ferrín and Vincenzo Orofino, outgassing from comet-like objects within the complex could be hiding smaller, but still potentially dangerous, asteroids that might hit the Earth.

‘The Tunguska cosmic body was 60 to 90 meters in diameter,’ he told Discover Magazine, adding that we ‘now believe the complex may contain many more objects of that size. It is not the tame, simple and innocent complex we thought it was.’

{ https://howandwhys.com/ }

30-09-2024 om 21:11 geschreven door peter  

China transformeerde maangrond in water: de eerste stap naar echte kolonisatie?

door Janine

NASA

Dat China plannen heeft om de maan en haar grondstoffen te gebruiken is zeker geen mysterie. Tegelijkertijd heeft het Aziatische land de afgelopen jaren verschillende sondes naar onze satelliet gestuurd, waaronder naar de verborgen kant. Meer recent is echter het nieuws dat een team van Chinese wetenschappers enkele monsters die door de Chang'e 5-missie naar de aarde zijn teruggebracht, heeft gebruikt om water te produceren. Zou dit de eerste stap kunnen zijn naar een toekomstige menselijke aanwezigheid op de maan? Laten we het samen uitzoeken!

Chang'e 5 en de maanmonsters teruggebracht naar de aarde

Zoals de naam al doet vermoeden, is de Chang'e 5-missie zeker niet de eerste die op de maan is gearriveerd. Het bijzondere aan deze missie is dat er voor het eerst in 44 jaar monsters van de maanbodem naar de aarde zijn teruggebracht. Ondanks de daaropvolgende Chang'e 6-missie, waarbij in plaats daarvan de verborgen kant van onze satelliet werd betrokken, zijn de resultaten van Chang'e 5 simpelweg buitengewoon. Zoals te lezen is in een recente studie gepubliceerd in het tijdschrift The Innovation, hebben Chinese wetenschappers ontdekt dat de mineralen waaruit de bodem van de maan bestaat rijk zijn aan waterstof en kunnen worden gebruikt om ter plekke water te produceren. Maar hoe?

De methode waarmee je water uit eenvoudige grond kunt halen, vereist het verwarmen van de mineralen waaruit het bestaat tot extreem hoge temperaturen, om een ​​chemische reactie van de elementen met waterstof te veroorzaken en daardoor tot de vorming van waterdamp te leiden.

Hoe je water van de Maan krijgt

Chen et al./The Innovation - 2024

Dankzij de innovatieve methode van Chinese wetenschappers kan uit elke ton maangrond ongeveer 50 liter water worden gewonnen. Het lijkt misschien niet veel, en het is ongetwijfeld een proces dat om verschillende redenen op aarde geen zin zou hebben. Op de maan verandert dit echter: 50 liter water kan voorzien in de dagelijkse behoeften van de leden van een hypothetische menselijke missie op een hypothetische maanbasis. De maanbasis vormt een concreet doel van de Chinese ruimteverkenning: het ter plekke kunnen produceren van water zou een enorm voordeel betekenen.

In feite wil China vòòr 2035 een permanent onderzoeksstation op de maan bouwen, terwijl China vòòr 2045 een ruimtestation in een baan rond de satelliet wil bouwen. Als Chang'e 5 na 44 jaar de eerste missie was die maanmonsters terugbracht, is de Chang'e 6-missie de eerste die monsters van de andere kant van de maan terugbracht. Kortom: China lijkt het serieus te nemen.

Naar een toekomstige maanbasis... en verder

Dat het mogelijk is om water rechtstreeks uit de maanbodem te halen is buitengewoon nieuws dat echter ook een aantal overwegingen met zich meebrengt. Allereerst moeten we begrijpen hoeveel energie er nodig is om de bodem te verwarmen en welke andere elementen betrokken zijn bij het proces van waterdampvorming. Ten tweede mogen we de geopolitieke implicaties niet vergeten van de belangstelling die China toont voor onze satelliet: de concurrentie om maanbronnen zal in de toekomst steeds levendiger worden. En mogelijk ook heviger.

Kortom, de resultaten van de Chinese Academie van Wetenschappen laten zien hoe het mogelijk is om steeds dichter bij het idee van een permanente aanwezigheid van de mens op de maan te komen. Aan de andere kant zijn er tientallen jaren verstreken sinds de laatste keer dat een astronaut een wandeling maakte op onze satelliet. De volgende zou wel eens een ruimtestation op de maan kunnen bewonen, op haar grond kunnen lopen... en haar water kunnen drinken.

{ https://www.curioctopus.nl/ }

30-09-2024 om 18:48 geschreven door peter  

Artikel door businessam.be

 

Revolutie in de ruimtevaart: nieuw aandrijfsysteem maakt oneindige ruimtereizen mogelijk

Key takeaways

• Super Magdrive gebruikt direct beschikbare metalen in de ruimte als brandstof.
• Traditionele raketmotoren zijn afhankelijk van schaarse bronnen zoals xenon of krypton.
• Dit nieuwe systeem maakt gebruik van metalen zoals ijzer, aluminium en koper.

Onderzoekers van de Universiteit van Southampton ontwikkelen een baanbrekend aandrijvingssysteem dat direct beschikbare metalen uit de ruimte gebruikt als brandstof. Deze innovatieve technologie, bekend als Super Magdrive, zou ruimtetuigen in staat kunnen stellen om oneindige reizen door de kosmos te maken.

Traditionele raketmotoren zijn afhankelijk van schaarse grondstoffen zoals xenon of krypton, die overvloedig aanwezig zijn op aarde maar moeilijk te verkrijgen zijn in de diepe ruimte. Dit nieuwe systeem maakt daarentegen gebruik van metalen zoals ijzer, aluminium en koper, die in overvloed aanwezig zijn in ons zonnestelsel. Hoofdonderzoeker Dr. Minkwan Kim benadrukt in een gesprek met Sky News dat dit een revolutionaire benadering van ruimteverkenning is, waardoor ruimtetuigen zich ver in de kosmos kunnen wagen en gedurende langere perioden kunnen werken.

Kritische ontwikkelingen en samenwerkingsverbanden

Het team van Dr. Kim werkte samen met het Britse ruimtevaartbedrijf Magdrive aan de ontwikkeling van Super Magdrive. De Britse overheid heeft 1 miljoen pond beschikbaar gesteld om dit project te ondersteunen. Dr. Kim ziet deze technologie als een hoeksteen voor toekomstige missies in de diepe ruimte, die mogelijk tot ongekende ontdekkingen kunnen leiden.

Toekomstige implicaties en verwachtingen

Hij gelooft dat het een revolutie teweeg kan brengen in ons vermogen om nieuwe planeten te verkennen, naar buitenaards leven te zoeken en de grenzen van menselijke verkenning te verleggen door reizen mogelijk te maken die verder gaan dan eerder bedachte grenzen.

De ruimtevaart van de toekomst documentaire fragment

{ https://www.msn.com/nl-be/ }

30-09-2024 om 18:01 geschreven door peter  

SpaceX launches mission to rescue astronauts stranded at ISS

A SpaceX spacecraft has lifted off to rescue two astronauts stranded at the International Space Station (ISS) due to technical issues.

NASA astronaut Nick Hague and Russian astronaut Aleksandr Gorbunov took off on Saturday from Cape Canaveral, Florida to bring back Suni Williams and Barry Wilmore.

The Dragon spacecraft, operated by SpaceX, the private company founded by billionaire Elon Musk, is set to arrive at the ISS on Sunday.

Originally, astronauts Zena Cardman and Stephanie Wilson were set to be part of NASA’s SpaceX Crew-9 mission.

However, they gave up their spots to accommodate Williams and Wilmore, astronauts stranded on the ISS due to technical issues with the Starliner spacecraft.

Williams and Wilmore were originally scheduled to return to Earth on June 13, after their Boeing Starliner capsule launched its first crewed flight from Florida’s Cape Canaveral Space Force Station on June 5. But the Starliner had been plagued with issues, even before the June 5 launch. A previous launch attempt was scrapped on June 1 just moments before launch because of a ground control computer performance issue.

During the 25-hour flight to the International Space Station, the spacecraft experienced several helium leaks and a malfunctioning thruster. Then, when the Starliner arrived on June 6 and attempted to dock at the ISS, four more of the 28 thrusters malfunctioned causing the ship’s arrival to be delayed.

Saturday’s launch of NASA’s mission had been delayed for several days due to the effects of Hurricane Helene. Weather concerns persisted until the last minute, with rain and storms posing risks to the mission.

“The crewmates will conduct more than 200 scientific investigations, including blood clotting studies, moisture effects on plants grown in space, and vision changes in astronauts during their mission,” read a NASA statement.

Williams and Wilmore are expected to return to Earth in February 2025, along with Hague and Gorbunov.

Related video:

{ https://www.msn.com/en-us/ }

29-09-2024 om 23:51 geschreven door peter  

Story by Joe Hindy

 

29-09-2024 om 23:14 geschreven door peter  

Since Earth and the Moon have similar geological history, it made sense to look around on our planet for materials to simulate lunar dust. For LUNA, the agency partners created something called EAC-1. It’s based on volcanic powder spread out over the Eifel region in Germany some 45 million years ago. ESA has been working with this material for some years now, creating “moon bricks” that lunar colonists could use to build roads, launch pads, and habitats. Not only that, but lunar soil (like the EAC-1) contains a high percentage of oxygen. If astronauts can practice “cracking” that soil at LUNA, that would provide them with experience doing the same thing to tap in situ sources of oxygen they can use to survive.

Two astronauts simulate a training session in the new Luna Hall as part of the opening ceremony at the European Astronaut Centre (EAC) in Cologne.

Photo: picture alliance/dpa | Benjamin Westhoff

More about LUNA

The LUNA main hall isn’t just a soil pit, however. It also has a specialized illumination simulator. That allows astronauts to recreate and practice their work under lunar day-and-night cycles. The Moon’s “day” is 14 Earth days long and a lunar night is the same length. Future astronauts and colonists will need to adapt their living and working conditions to those cycles.

Eventually, LUNA will also incorporate gravity off-loading systems. These are simulations of reduced gravity environments. Since the Moon’s gravity is one-sixth that of Earth’s, it’s important for astronauts to train in lower-gravity environments. Plans include a system similar to the Active Response Gravity Offload System (ARGOS) gravity system that NASA uses. It’s a device that suspends an astronaut trainee in a special trainer and uses sensors and other feedback that provide a simulated low-gravity environment.

In addition to astronaut training for low gravity and working with soil, LUNA will act as a testbed for operating robotic systems such as rovers and other tools. It will enable advanced science testing and activities, and teach astronauts how to build, manipulate, and operate energy systems. For example, researchers at the facility will test the regolith to understand the effects of moon dust on equipment space agencies plan to bring to the moon.

Preparing for Artemis and Beyond

All these activities should help future astronauts and mission planners develop solutions to challenges the Artemis and other explorers will face on the Moon. LUNA will also contain a unique habitat training area called FLEXHab. It is planned as a simulated habitat that will connect to the main facility.

Finally, ESA and DLR plan to repurpose a food production facility called EDEN-ISS. It’s actually a greenhouse that hosted a five-year-long food cultivation experiment. It will become part of the LUNA laboratory and is aimed at helping astronauts figure out how to grow and prepare food during their stay on the Moon.

Building accurate replicas of the lunar environment is a big training step toward permanent habitation on the Moon. The Artemis project will be one mission to take advantage of LUNA. Its mission timeline has slipped, but astronauts will still likely be headed toward the Moon within the decade. Test sites such as LUNA will play an important role in their training and eventual colonization activities.

For More Information

• New LUNA Facility Will prepare Astronauts for Moon Landings
• Full-Size Reduced Gravity Simulator For Humans, Robots, and Test Objects
  Bricks from Moon Dust

{ https://www.universetoday.com/ }

29-09-2024 om 00:47 geschreven door peter  

A mosaic of the images of 378 satellites across 101 Milky Way-like systems.

Credit: Yao-Yuan Mao (Utah), with images from the DESI Legacy Surveys Sky Viewer

This would seem to indicate that the Milky Way is rather typical. But then the team looked at those galaxies with a large companion, like the Large Magellanic Cloud we see in the southern hemisphere. For those galaxies the number of satellites is typically much larger than four. The Milky Way has an unusually low number of satellites. One reason for this may be that the Large Magellanic Cloud entered our sphere of influence rather recently on the cosmic timeline.

A second study based on the SAGA data looked at star formation in the satellite galaxies. It found that the closer a satellite is to the main galaxy the more likely it is to still be producing stars. This is similar to what we see among the Milky Way satellites. So it seems that while the Milky Way is a little unusual, it isn’t unique among galaxies of similar mass.

But it will always be our special spiral galaxy.

Reference: 

• Mao, Yao-Yuan, et al. “The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies.” arXiv preprint arXiv:2404.14498 (2024).

Reference: 

• Geha, Marla, et al. “The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies.” arXiv preprint arXiv:2404.14499 (2024).

{ https://www.universetoday.com/ }

29-09-2024 om 00:25 geschreven door peter  

Ceres is Former Ocean World, Planetary Scientists Say

Ceres is a key object in understanding the evolution of small bodies and is the only dwarf planet to have been orbited by a spacecraft, NASA’s Dawn mission. Dawn data paint an inconclusive picture of Ceres’ internal structure, composition and evolutionary pathway. New research shows that a crust with nearly 90% ice near the surface, which gradually decreases to 0% at 117 km depth, simultaneously matches the Dawn observations. This crustal structure results from a frozen ocean that became more impurity rich as it solidified top-down. Therefore, the Dawn data are consistent with an icy Ceres that evolved through freezing of an ancient, impure ocean.

This false-color image shows the dwarf planet Ceres. Scientists use false color to examine differences in surface materials. The color blue on Ceres is generally associated with bright material, found in more than 130 locations, and seems to be consistent with salts.

Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA.

“Ceres is the largest object in the asteroid belt, and a dwarf planet. I think sometimes people think of small, lumpy things as asteroids (and most of them are!), but Ceres really looks more like a planet,” said Purdue University researcher Mike Sori.

“It is a big sphere, diameter 950 km or so, and has surface features like craters, volcanoes, and landslides.”

“We think that there’s lots of water-ice near Ceres surface, and that it gets gradually less icy as you go deeper and deeper.”

“People used to think that if Ceres was very icy, the craters would deform quickly over time, like glaciers flowing on Earth, or like gooey flowing honey.”

“However, we’ve shown through our simulations that ice can be much stronger in conditions on Ceres than previously predicted if you mix in just a little bit of solid rock.”

This discovery is contradictory to the previous belief that Ceres was relatively dry.

The common assumption was that Ceres was less than 30% ice, but Sori’s team now believes the surface is more like 90% ice.

“Our interpretation of all this is that Ceres used to be an ocean world like Europa (one of Jupiter’s moons), but with a dirty, muddy ocean,’” Dr. Sori said.

“As that muddy ocean froze over time, it created an icy crust with a little bit of rocky material trapped in it.”

The authors used computer simulations to model how relaxation occurs for craters on Ceres over billions of years.

“Even solids will flow over long timescales, and ice flows more readily than rock,” said Purdue University Ph.D. student Ian Pamerleau.

“Craters have deep bowls which produce high stresses that then relax to a lower stress state, resulting in a shallower bowl via solid state flow.”

“So the conclusion after NASA’s Dawn mission was that due to the lack of relaxed, shallow craters, the crust could not be that icy.”

“Our computer simulations account for a new way that ice can flow with only a little bit of non-ice impurities mixed in, which would allow for a very ice-rich crust to barely flow even over billions of years.”

“Therefore, we could get an ice-rich Ceres that still matches the observed lack of crater relaxation.”

“We tested different crustal structures in these simulations and found that a gradational crust with a high ice content near the surface that grades down to lower ice with depth was the best way to limit relaxation of Cerean craters.”

“To me the exciting part of all this, if we’re right, is that we have a frozen ocean world pretty close to Earth,” Dr. Sori said.

“Ceres may be a valuable point of comparison for the ocean-hosting icy moons of the outer Solar System, like Jupiter’s moon Europa and Saturn’s moon Enceladus.”

“Ceres, we think, is therefore the most accessible icy world in the Universe. That makes it a great target for future spacecraft missions.”

{ https://www.sci.news/ }

28-09-2024 om 23:05 geschreven door peter  

De Aarde had ook zijn planetaire ringen, net als Saturnus: dat stelt een onderzoek

door Janine

Kevin M. Gill/Wikimedia Commons - CC BY 2.0

We kennen allemaal Saturnus, een van de meest iconische planeten in het zonnestelsel vanwege zijn spectaculaire planetaire ringen. Natuurlijk hebben Uranus en Neptunus ook iets dergelijks, en hetzelfde kan gezegd worden van Jupiter, maar deze structuren hebben niet dezelfde charme. Onlangs is er echter een onderzoek gedaan dat suggereert dat ook de aarde zo'n 460 miljoen jaar geleden haar eigen ringenstelsel kan hebben gehad. Laten we eens kijken hoe dit mogelijk is!

Had de Aarde ook planetaire ringen?

Een team onderzoekers van de Monash University in Melbourne stelt deze hypothese voor in een studie die is gepubliceerd in het tijdschrift Earth and Planetary Science Letters. De wetenschappers analyseerden inslagkraters die werden gecreëerd door asteroïden tijdens het Ordovicium, tussen 485 en 443 miljoen jaar geleden. Het probleem is dit: er werden 21 kraters geïdentificeerd die zich binnen 30 graden van de evenaar bevonden, maar de verdeling is te afwijkend om in traditionele theorieën te passen. Kortom, waarom zijn alle kraters geconcentreerd in deze gordel als meer dan tweederde van de aardkorst daarbuiten ligt?

Volgens de onderzoekers is het antwoord duidelijk: zo'n 460 miljoen jaar geleden zou een grote asteroïde de aarde hebben benaderd tot hij de limiet van Roche passeerde, waarna hij werd beïnvloed door getijdenkrachten. Als gevolg daarvan zou de asteroïde zijn gaan fragmenteren en deze fragmenten zouden hebben geholpen bij het vormen van een ring van puin rond de aarde. Net als bij Saturnus en andere gasreuzen.

Planeetringen en ijstijden

Oliver Hull/Monash University

Wat is het verband tussen de vorming van planetaire ringen en de concentratie inslagkraters die Australische onderzoekers hebben ontdekt? Simpel: na de vorming zouden de brokstukken die de ring vormden in de loop van miljoenen jaren beetje bij beetje op de aarde zijn gevallen en zo de piek in kraters hebben veroorzaakt. Maar dat is nog niet alles, want de studie probeerde ook bewijs te vinden voor de klimatologische gevolgen die een ringsysteem zeker zou hebben gehad op de aarde.

Vanuit dit perspectief zouden de planetaire ringen een deel van het zonlicht hebben kunnen tegenhouden en hebben bijgedragen aan de wereldwijde afkoeling. En in feite vindt precies aan het einde van het Ordovicium de Hirnatien-ijstijd plaats, die wordt beschouwd als een van de koudste periodes van de afgelopen 500 miljoen jaar. Bovendien is het deze ijstijd die de massa-uitsterving in het Ordovicium veroorzaakte, de eerste van de vijf grote massa-uitstervingen in de geschiedenis van de aarde. Gebeurde dit allemaal door 'onze' planeetringen?

Perspectieven van het onderzoek

De ontdekking door Australische onderzoekers kan veel bredere gevolgen hebben dan verwacht. In de praktijk gaat het niet alleen om het idee dat de Aarde ook een eigen planetair ringenstelsel kan hebben gehad, maar om overwegingen van complexere aard:

• ten eerste, wat er in het laatste deel van het Ordovicium gebeurde, zou ook gebeurd kunnen zijn in de 4 miljard jaar van de vorige geschiedenis van de Aarde;
• ten tweede kan de vorming en het daaropvolgende verval van een planetaire ring belangrijke gevolgen hebben gehad voor het klimaat op aarde;
• ten slotte spelen astronomische gebeurtenissen, waaronder de vorming van planeetringen, een veel belangrijkere rol in de geschiedenis van een planeet dan verwacht.

Kortom, als de hypothese van het onderzoek gegrond blijkt te zijn, staan we mogelijk aan het begin van een geheel nieuw onderzoeksgebied over de interactie tussen de aarde en de kosmos. Met gevolgen voor de hele evolutionaire geschiedenis van onze planeet.

{ https://www.curioctopus.nl/ }

28-09-2024 om 22:04 geschreven door peter  

A photo recently captured by NASA's Perseverance rover on Mars has revealed a surprising object that stands out from the planet's natural landscape. 

The object in question looks like an artificial piece of glass or eventual a mirror, (the contours of the glass/mirror are clearly visible), partially located behind a rock formation. 

The fact that it could be a mirror is because the reflection in the mirror seems to show a part of what appears to be a metallic rectangular object what lies in front of the mirror. 

Both the glass/mirror and the metallic object seem to be remnants of something either abandoned or wrecked long ago. They clearly do not belong to the rover's equipment or any known NASA gear.  

This discovery joins a growing list of mysterious objects found on Mars hinting at the possibility that intelligent civilizations may have once existed on the planet potentially wiped out due to a catastrophic event which made life on the planet impossible. 

Link to the photo uploaded by Neville Thompson on his Gigapan page.

• http://www.gigapan.com/gigapans/236036

{ https://ufosightingshotspot.blogspot.com/ }

28-09-2024 om 21:46 geschreven door peter  

We spent 45 days in a simulated Mars habitat built by NASA - this is the brutal reality of life on Red Planet

• READ MORE: New map of Mars reveals hidden 'structures' below the surface

By Ellyn Lapointe For Dailymail.Com

Four volunteer scientists have just emerged from a 45-day stay inside NASA's most realistic Mars simulation yet.

The crew remained completely isolated inside the Human Exploration Research Analog (HERA) - a 650-square-foot habitat at NASA's Johnson Space Center in Houston, Texas - until Monday, when the hatch opened and they finally 'returned to Earth.'

While inside, they completed 18 different studies that will help NASA and other space agencies learn how humans respond to the confinement, demanding work-life conditions and remote environments of deep-space missions, according to NASA

NASA has set a goal to get humans to Mars by the 2030s. With that deadline fast approaching, simulated missions like HERA provide key insights into how astronauts might survive the farthest crewed space mission ever attempted. 

The four person crew - comprised of Sergii Iakymov, Sarah Elizabeth McCandless, Erin Anderson, and Brandon Kent (L to R) - was the third to enter the HERA habitat

Above, a 3D-rendered image of the red planet Mars - as virtual as the team's HERA experience

The four person crew - comprised of Erin Anderson, Sergii Iakymov, Sarah Elizabeth McCandless and Brandon Kent - was the third to enter the HERA habitat.

Their mission was unique in that it included the more detailed assignments designed to closely replicate the living and working experience on Mars.

During the month-and-a-half-long simulation, the crew performed a wide range of tasks.

Their assignments included harvesting plants from a hydroponic garden, growing shrimp, deploying a small satellite, conducting a virtual 'walk' across the surface of Mars and flying simulated drones over Martian terrain. 

'These activities are designed to immerse the crew in the task-focused mindset of astronauts,' NASA wrote in a statement.

NASA even simulated the communication delays that real astronauts could one day face on Mars. During a real Mars mission, communications from Earth could take up to 20 minutes to reach astronauts on the red planet, and vice versa. 

All the while, the crew was being monitored by NASA scientists to assess how their day-to-day tasks, routine, and the isolation and confinement of their habitat affected their behavior and performance. 

When they weren't hard at work, the crew read books, played cards, built Legos and listened to music. 

The HERA mission three crew entered the habitat on August 9

Their mission was unique in that it included the more detailed assignments designed to closely replicate the living and working experience on Mars, including growing hydroponic plants

The volunteers also grew shrimp, deployed a small satellite, conducted a virtual 'walk' across the surface of Mars and flew simulated drones over Martian terrain

On Monday afternoon, the crew finally emerged from their tiny habitat, marking the end of their mission. 

'Following our safe passage to Mars, and our safe return to Earth, as the crew of Campaign 7, Mission 3, we hereby officially transfer this exploration vessel to the flight analogs operations team,' said Kent upon exiting HERA.

'We hope this vessel continues to serve as a safe home for future HERA crews,' he added. 

NASA also runs another, bigger simulated Mars habitat called the Crew Health and Performance Exploration Analog, or CHAPEA. This 1,700-square-foot is large enough to sustain volunteers for up to a year. 

The first CHAPEA volunteer crew emerged from their habitat in July. 

If you think you have what it takes to spend weeks inside cramped Mars simulation, NASA is actively seeking non-smoking volunteers between the ages of 30 and 55 for the next HERA mission. 

{ https://www.dailymail.co.uk/ }

28-09-2024 om 21:31 geschreven door peter  

Story by And¸elika

©And¸elika

NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
With all of the worrying things happening here, on earth, one way to take your mind off them is to look at the beauty of the cosmos. Luckily, NASA is still out there exploring outer space and providing us with the latest wonders. Recently The National Aeronautics and Space Administration released the brand new imagery of Jupiter. The captivating display of the stormy southern hemisphere of the planet which exists 484 million miles away from us, prompted us to share a list of most fascinating photos NASA has taken of the planet.
Nasa's Juno spacecraft has been taking snaps of the planet since it's first close pass by Jupiter in 2016. Since then, Juno took stunning images of and it, helping scientists learn the important information about the gas giant.

©NASA

#1 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
NASA’s Juno spacecraft was a little more than one Earth diameter from Jupiter when it captured this mind-bending, color-enhanced view of the planet’s tumultuous atmosphere.

©NASA

#2 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
A multitude of swirling clouds in Jupiter's dynamic North North Temperate Belt is captured in this image from NASA's Juno spacecraft. Appearing in the scene are several bright-white “pop-up” clouds as well as an anticyclonic storm, known as a white oval.

©NASA

#3 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image captures the swirling cloud formations around the south pole of Jupiter, looking up toward the equatorial region.

©NASA

#4 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
See Jovian clouds in striking shades of blue in this new view taken by NASA’s Juno spacecraft.

©NASA

#5 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
During its 24th close flyby of Jupiter, NASA’s Juno spacecraft captured this view of a chaotic, stormy area of the planet’s northern hemisphere known as a folded filamentary region. Jupiter has no solid surface in the same way Earth does. Data collected by Juno indicate that some of the giant planet’s winds run deeper and last longer than similar atmospheric processes on Earth.

©NASA

#6 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Jupiter’s volcanically active moon Io casts its shadow on the planet in this dramatic image from NASA’s Juno spacecraft. As with solar eclipses on the Earth, within the dark circle racing across Jupiter’s cloud tops one would witness a full solar eclipse as Io passes in front of the Sun.

©NASA

#7 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
NASA’s Juno mission captured this look at Jupiter’s tumultuous northern regions during the spacecraft’s close approach to the planet on Feb. 17, 2020.

©NASA

#8 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This striking view of Jupiter’s Great Red Spot and turbulent southern hemisphere was captured by NASA’s Juno spacecraft as it performed a close pass of the gas giant planet.

©NASA

#9 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image of Jupiter’s turbulent southern hemisphere was captured by NASA’s Juno spacecraft as it performed its most recent close flyby of the gas giant planet on Dec. 21, 2018

©NASA

#10 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Thick white clouds are present in this JunoCam image of Jupiter's equatorial zone. These clouds complicate the interpretation of infrared measurements of water. At microwave frequencies, the same clouds are transparent, allowing Juno's Microwave Radiometer to measure water deep into Jupiter's atmosphere. The image was acquired during Juno's flyby of the gas giant on Dec. 16, 2017.

©NASA

#11 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image captures swirling cloud belts and tumultuous vortices within Jupiter’s northern hemisphere.

©NASA

#12 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image shows Jupiter’s south pole, as seen by NASA’s Juno spacecraft from an altitude of 32,000 miles (52,000 kilometers). The oval features are cyclones, up to 600 miles (1,000 kilometers) in diameter. Multiple images taken with the JunoCam instrument on three separate orbits were combined to show all areas in daylight, enhanced color, and stereographic projection.

 

©NASA

#13 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This view from NASA's Juno spacecraft captures colorful, intricate patterns in a jet stream region of Jupiter's northern hemisphere known as "Jet N3."

©NASA

#14 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
NASA’s Juno spacecraft captured this view of an area within a Jovian jet stream showing a vortex that has an intensely dark center. Nearby, other features display bright, high altitude clouds that have puffed up into the sunlight.

©NASA

#15 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
A dynamic storm at the southern edge of Jupiter’s northern polar region dominates this Jovian cloudscape, courtesy of NASA’s Juno spacecraft.

©NASA

#16 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image of Jupiter’s iconic Great Red Spot and surrounding turbulent zones was captured by NASA’s Juno spacecraft.

©NASA

#17 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image of Jupiter’s swirling south polar region was captured by NASA’s Juno spacecraft as it neared completion of its tenth close flyby of the gas giant planet.

©NASA

#18 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
See Jupiter’s southern hemisphere in beautiful detail in this new image taken by NASA’s Juno spacecraft. The color-enhanced view captures one of the white ovals in the “String of Pearls,” one of eight massive rotating storms at 40 degrees south latitude on the gas giant planet.

©NASA

#19 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This view of Jupiter’s atmosphere from NASA’s Juno spacecraft includes something remarkable: two storms caught in the act of merging.

©NASA

#20 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Colorful swirling cloud belts dominate Jupiter’s southern hemisphere in this image captured by NASA’s Juno spacecraft.

 

©NASA

#21 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This color-enhanced image of a massive, raging storm in Jupiter’s northern hemisphere was captured by NASA’s Juno spacecraft during its ninth close flyby of the gas giant planet.

©NASA

#22 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
See intricate cloud patterns in the northern hemisphere of Jupiter in this new view taken by NASA’s Juno spacecraft.

©NASA

#23 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Dramatic atmospheric features in Jupiter’s northern hemisphere are captured in this view from NASA’s Juno spacecraft. The new perspective shows swirling clouds that surround a circular feature within a jet stream region called "Jet N6."

©NASA

#24 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This image captures the intensity of the jets and vortices in Jupiter’s North North Temperate Belt.

©NASA

#25 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Small bright clouds dot Jupiter’s entire south tropical zone in this image acquired by JunoCam on NASA’s Juno spacecraft on May 19, 2017, at an altitude of 7,990 miles (12,858 kilometers). Although the bright clouds appear tiny in this vast Jovian cloudscape, they actually are cloud towers roughly 30 miles (50 kilometers) wide and 30 miles (50 kilometers) high that cast shadows on the clouds below. On Jupiter, clouds this high are almost certainly composed of water and/or ammonia ice, and they may be sources of lightning. This is the first time so many cloud towers have been visible, possibly because the late-afternoon lighting is particularly good at this

©NASA

#26 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
Colorful swirling clouds in Jupiter's North Equatorial Belt practically fill this image from NASA's Juno spacecraft. This is the closest image captured of the Jovian clouds during this recent flyby of the gas giant planet.

©NASA

#27 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
See swirling cloud formations in the northern area of Jupiter's north temperate belt in this new view taken by NASA’s Juno spacecraft.

©NASA

#28 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
NASA’s Juno mission captured this look at the southern hemisphere of Jupiter on Feb. 17, 2020, during the spacecraft’s most recent close approach to the giant planet.

©NASA

#29 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
This extraordinary view of Jupiter was captured by NASA’s Juno spacecraft on the outbound leg of its 12th close flyby of the gas giant planet.

©NASA

#30 NASA Released 30 Amazing High-Def Photos Of The Largest Planet In Our Solar System—Jupiter
A swirling, oval white cloud in Jupiter’s South South Temperate Belt is captured in this image from NASA's Juno spacecraft. Known as White Oval A5, the feature is an anticyclonic storm. An anticyclone is a weather phenomenon where winds around the storm flow in the direction opposite to those of the flow around a region of low pressure.

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27-09-2024 om 23:15 geschreven door peter  

Early Martian Atmosphere Could Be Locked Up in Planet’s Clay Surface

Geological observations of Mars indicate a dense early atmosphere ranging from 0.25 to 4 bar of carbon dioxide. But 3.5 billion years ago, the Martian atmosphere thinned rapidly to approximately 0.054 bar, suggesting a substantial loss of atmospheric carbon dioxide, either to space or the lithosphere. The mechanism by which Mars lost its carbon dioxide remains poorly understood. For MIT geologists Joshua Murray and Oliver Jagoutz, the answer may lie in the planet’s clay-covered crust. The researchers used their knowledge of interactions between rocks and gases on Earth and applied that to how similar processes could play out on Mars. They found that, given how much clay is estimated to cover the Martian surface, the planet’s clay could hold up to 1.7 bar of carbon dioxide, which would be equivalent to around 80% of the planet’s initial, early atmosphere. It’s possible that this sequestered Martian carbon could one day be recovered and converted into propellant to fuel future missions between Mars and Earth, the researchers propose.

This schematic illustrates the progressive alteration of iron-rich rocks on Mars as the rocks interact with water containing carbon dioxide from the atmosphere.

Image credit: Joshua Murray & Oliver Jagoutz, doi: 10.1126/sciadv.adm8443.

“Based on our findings on Earth, we show that similar processes likely operated on Mars, and that copious amounts of atmospheric carbon dioxide could have transformed to methane and been sequestered in clays,” Professor Jagoutz said.

“This methane could still be present and maybe even used as an energy source on Mars in the future.”

Professor Jagoutz and Murray seek to identify the geologic processes and interactions that drive the evolution of Earth’s lithosphere — the hard and brittle outer layer that includes the crust and upper mantle, where tectonic plates lie.

In 2023, they focused on a type of surface clay mineral called smectite, which is known to be a highly effective trap for carbon.

Within a single grain of smectite are a multitude of folds, within which carbon can sit undisturbed for billions of years.

They showed that smectite on Earth was likely a product of tectonic activity, and that, once exposed at the surface, the clay minerals acted to draw down and store enough carbon dioxide from the atmosphere to cool the planet over millions of years.

Soon after they reported their results, Professor Jagoutz happened to look at a map of the surface of Mars and realized that much of that planet’s surface was covered in the same smectite clays.

An illustration shows an misty atmosphere around the Red Planet Mars. Could this envelop of gas have "gone to ground" billions of years ago?

 (Image credit: Robert Lea (created with Canva)/NASA)

Could the clays have had a similar carbon-trapping effect on Mars, and if so, how much carbon could the clays hold?

Unlike on Earth, where smectite is a consequence of continental plates shifting and uplifting to bring rocks from the mantle to the surface, there is no such tectonic activity on Mars.

The scientists looked for ways in which the clays could have formed on Mars, based on what they know of the planet’s history and composition.

For instance, some remote measurements of Mars’ surface suggest that at least part of the planet’s crust contains ultramafic igneous rocks, similar to those that produce smectites through weathering on Earth.

Other observations reveal geologic patterns similar to terrestrial rivers and tributaries, where water could have flowed and reacted with the underlying rock.

The authors wondered whether water could have reacted with Mars’ deep ultramafic rocks in a way that would produce the clays that cover the surface today.

They developed a simple model of rock chemistry, based on what is known of how igneous rocks interact with their environment on Earth.

They applied this model to Mars, where scientists believe the crust is mostly made up of igneous rock that is rich in the mineral olivine.

The team used the model to estimate the changes that olivine-rich rock might undergo, assuming that water existed on the surface for at least a billion years, and the atmosphere was thick with carbon dioxide.

“At this time in Mars’ history, we think carbon dioxide is everywhere, in every nook and cranny, and water percolating through the rocks is full of carbon dioxide too,” Murray said.

Over about a billion years, water trickling through the crust would have slowly reacted with olivine — a mineral that is rich in a reduced form of iron.

Oxygen molecules in water would have bound to the iron, releasing hydrogen as a result and forming the red oxidized iron which gives the planet its iconic color.

An image of a dust devil sweeping over Mars captured by the Opportunity Rover in March 2016 as the robot investigated smectites in Marathon Valley. 

(Image credit: NASA/JPL-Caltech)

This free hydrogen would then have combined with carbon dioxide in the water, to form methane.

As this reaction progressed over time, olivine would have slowly transformed into another type of iron-rich rock known as serpentine, which then continued to react with water to form smectite.

“These smectite clays have so much capacity to store carbon,” Murray said.

“So then we used existing knowledge of how these minerals are stored in clays on Earth, and extrapolate to say, if the Martian surface has this much clay in it, how much methane can you store in those clays?”

The researchers found that if Mars is covered in a layer of smectite that is 1,100 m deep, this amount of clay could store a huge amount of methane, equivalent to most of the carbon dioxide in the atmosphere that is thought to have disappeared since the planet dried up.

“We find that estimates of global clay volumes on Mars are consistent with a significant fraction of Mars’ initial carbon dioxide being sequestered as organic compounds within the clay-rich crust,” Murray said.

“In some ways, Mars’ missing atmosphere could be hiding in plain sight.”

• The results appear in the journal Science Advances.
• Joshua Murray & Oliver Jagoutz. 2024. Olivine alteration and the loss of Mars’ early atmospheric carbon. Science Advances 10 (39); doi: 10.1126/sciadv.adm8443
• This article is based on a press-release provided by MIT.

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27-09-2024 om 21:24 geschreven door peter  

New map of Mars reveals hidden 'structures' below the Martian surface

• READ MORE:  Scientists discover smiley-face on Mars that may hold signs of life

By Ellyn Lapointe For Dailymail.Com

A new map of Mars has revealed mysterious structures hiding beneath the sediment layers of a lost ocean.

The researchers detected about 20 features scattered around the planet's north polar cap that are significantly denser than their surroundings. 

The structures vary in shape and size, with one resembling the shape of a dog, leaving the team puzzled because they do not know exactly what the formations are or where they came from. But they do have some theories.

One idea is that the structures were compacted by ancient meteor strikes, or  formed by volcanic activity, but more research is needed to get to the bottom of these underground anomalies. 

A new analysis of Mars' gravitational field has revealed mysterious structures lurking beneath the planet's surface

The team of researchers from Denmark's TU Delft and Utrecht University presented their findings at the Europlanetary Science Conference in Berlin this week.

The team used tiny deviations in satellite orbits to create a picture of Mars' gravitational field, or the region of space around a planet where its gravitational force can be felt. 

They did this to look for clues about how mass is distributed throughout the planet's subsurface. 

The team then combined these observations with data on the thickness and flexibility of the Mars' crust, as well as the dynamics of the planet's mantle and deep interior. 

These observations were collected by NASA's InSIGHT lander, which completed its study of Mars' crust, mantle and core in 2022.

This allowed the researchers to create a global density map of Mars that revealed the existence of 20 previously unknown underground structures scattered around the planet's north polar cap.

The structures are about 19 to 25 pounds per cubic foot denser than their surroundings, and vary in shape and size. 

Additionally, they are covered by a thick, smooth layer of sediment that may have once been a seabed. 

The researchers used tiny deviations in satellite orbits and data from NASA's InSIGHT lander to create a global density map of Mars

Their analysis revealed 20 previously unknown underground structures scattered around the planet's north polar cap

Billions of years ago, Mars was not the desert planet we know today. It was once covered in oceans and rivers, but water dried up in an extreme climactic shift. 

Now, the only evidence of these bodies of water lies in Mars' geologic record - like this sediment layer. 

As for the structures that lie beneath, 'there seems to be no trace of them at the surface,' lead author Bart Root, an assistant professor at TU Delft, said. 

'However, through gravity data, we have a tantalizing glimpse into the older history of the northern hemisphere of Mars.' 

This isn't the first time that scientists have uncovered oddities beneath the surface of Mars. 

In December 2023, China's Zhurong found large honeycomb-shaped crevasses buried dozens of meters beneath Mars' equator that likely formed when drastic temperature dips contract and fracture the ground.

But Root and his team are having a harder time figuring out what these most recently structures are, and where they came from. Right now, they have two main theories. 

Either the structures were compacted by ancient impact events, like meteor strikes, or they were formed by some kind of volcanic activity. This latter idea challenges scientists' longstanding view of Mars as a geologically inactive planet. 

But while studies have shown that Mars does not have as much geological activity as Earth, a growing body of evidence suggests that it isn't completely 'dead.'

Root's study adds to this evidence not just by discovering structures that may be volcanically formed, but through a totally separate finding. 

In addition to finding the mysterious structures, the team's analysis revealed that Mars' mantle may still host active geological processes that could be feeding Olympus Mons, the largest known volcano in the solar system.

Olympus Mons is located in the Tharsis Montes region near Mars' equator. Scientists estimate that it hasn't erupted for 25 million years.

The subterranean geology of the Tharsis region is incredibly dense, but Root and his team detected a much lighter mass lying 700 miles beneath the surface. 

He believes this mass is an enormous plume of magma that stretches 1,000 miles across in Mars' mantle. What's more, this plume might be in the process of bubbling to the surface.

'This means we need to rethink how we understand the support for the Olympus Mons volcano and its surroundings,' Root said. 

'It shows that Mars might still have active movements happening inside it, affecting and possibly making new volcanic features on the surface.' 

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27-09-2024 om 20:50 geschreven door peter