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.
Druk op onderstaande knop om te reageren in mijn forum
Zoeken in blog
Deze blog is opgedragen aan mijn overleden echtgenote Lucienne.
In 2012 verloor ze haar moedige strijd tegen kanker!
In 2011 startte ik deze blog, omdat ik niet mocht stoppen met mijn UFO-onderzoek.
BEDANKT!!!
Een interessant adres?
UFO'S of UAP'S, ASTRONOMIE, RUIMTEVAART, ARCHEOLOGIE, OUDHEIDKUNDE, SF-SNUFJES EN ANDERE ESOTERISCHE WETENSCHAPPEN - DE ALLERLAATSTE NIEUWTJES
UFO's of UAP'S in België en de rest van de wereld Ontdek de Fascinerende Wereld van UFO's en UAP's: Jouw Bron voor Onthullende Informatie!
Ben jij ook gefascineerd door het onbekende? Wil je meer weten over UFO's en UAP's, niet alleen in België, maar over de hele wereld? Dan ben je op de juiste plek!
België: Het Kloppend Hart van UFO-onderzoek
In België is BUFON (Belgisch UFO-Netwerk) dé autoriteit op het gebied van UFO-onderzoek. Voor betrouwbare en objectieve informatie over deze intrigerende fenomenen, bezoek je zeker onze Facebook-pagina en deze blog. Maar dat is nog niet alles! Ontdek ook het Belgisch UFO-meldpunt en Caelestia, twee organisaties die diepgaand onderzoek verrichten, al zijn ze soms kritisch of sceptisch.
Nederland: Een Schat aan Informatie
Voor onze Nederlandse buren is er de schitterende website www.ufowijzer.nl, beheerd door Paul Harmans. Deze site biedt een schat aan informatie en artikelen die je niet wilt missen!
Internationaal: MUFON - De Wereldwijde Autoriteit
Neem ook een kijkje bij MUFON (Mutual UFO Network Inc.), een gerenommeerde Amerikaanse UFO-vereniging met afdelingen in de VS en wereldwijd. MUFON is toegewijd aan de wetenschappelijke en analytische studie van het UFO-fenomeen, en hun maandelijkse tijdschrift, The MUFON UFO-Journal, is een must-read voor elke UFO-enthousiasteling. Bezoek hun website op www.mufon.com voor meer informatie.
Samenwerking en Toekomstvisie
Sinds 1 februari 2020 is Pieter niet alleen ex-president van BUFON, maar ook de voormalige nationale directeur van MUFON in Vlaanderen en Nederland. Dit creëert een sterke samenwerking met de Franse MUFON Reseau MUFON/EUROP, wat ons in staat stelt om nog meer waardevolle inzichten te delen.
Let op: Nepprofielen en Nieuwe Groeperingen
Pas op voor een nieuwe groepering die zich ook BUFON noemt, maar geen enkele connectie heeft met onze gevestigde organisatie. Hoewel zij de naam geregistreerd hebben, kunnen ze het rijke verleden en de expertise van onze groep niet evenaren. We wensen hen veel succes, maar we blijven de autoriteit in UFO-onderzoek!
Blijf Op De Hoogte!
Wil jij de laatste nieuwtjes over UFO's, ruimtevaart, archeologie, en meer? Volg ons dan en duik samen met ons in de fascinerende wereld van het onbekende! Sluit je aan bij de gemeenschap van nieuwsgierige geesten die net als jij verlangen naar antwoorden en avonturen in de sterren!
Heb je vragen of wil je meer weten? Aarzel dan niet om contact met ons op te nemen! Samen ontrafelen we het mysterie van de lucht en daarbuiten.
18-04-2025
A Hole Opened Up in the Sun's Corona and Vented Helium-3
A Hole Opened Up in the Sun's Corona and Vented Helium-3
By Laurence Tognetti, MSc
SwRI scientists located the source of highest-ever concentration of a rare helium isotope emitted by the Sun. In this Solar Dynamics Observatory extreme ultraviolet image, the blue arrow marks a small bright point located at the edge of a coronal hole (outlined in red) that was the source of the phenomenon. (Credit: NASA/SDO/AIA)
What can Helium-3 (3He) being discharged from the Sun teach us about 3He creation and the Sun’s activity? This is what a recent study published in The Astrophysical Journal hopes to address as an international team of researchers investigated 3He-rich solar energetic particles (SEPs) emitted by the Sun in late 2023. This study has the potential to help astronomers better understand how solar activity could contribute to the production of 3He, the latter of which remains one of the most desired substances due to its potential for nuclear fusion technology on Earth.
For the study, the researchers used the joint NASA-ESA Solar Orbiter to observe the SEPs between October 24-25, 2023, which is currently located at 0.47 astronomical units (AU) from the Sun, or just under halfway between the Sun and the Earth. While SEPs are produced from solar flares or coronal mass ejections (CMEs), which happen regularly, SEPs typically release substances with increased levels of heavy ions like iron. Heavy ions are classified as possessing an atomic number (Z) greater than 10. However, the iron content (Z= 26) in this SEP was found to be normal, with the researchers surprised to discover increased levels of carbon (Z = 6), nitrogen (Z = 7), silicon (Z = 14), and sulfur (Z = 16) within the SEP.
The team then conducted a follow-up observation with NASA’s Solar Dynamics Observatory, which orbits the Earth in a circular, geosynchronous orbit at an altitude of 35,789 kilometers (22,238 miles), so significantly farther from the Sun than Solar Orbiter. In the end, SDO successfully identified the source of the SEP as a solar jet emanating from coronal hole, which is an area of the Sun where open magnetic field lines enable solar winds to escape to space and are often darker in color compared to the rest of the Sun’s surface.
“Surprisingly, the magnetic field strength in this region was weak, more typical of quiet solar areas rather than active regions,” said Dr. Radoslav Bučík, who is an astrophysicist at the Southwest Research Institute and lead author of the study. “This finding supports earlier theories suggesting that 3He enrichment is more likely in weakly magnetized plasma, where turbulence is minimal.”
Other Helium-3 Sources
The Sun produces 3He from the nuclear fusion occurring in its massive core when it converts hydrogen to helium. While this is part of the Sun’s natural processes that enable our planet to sustain life, producing 3He in a laboratory or other Earth-based setting has proven incredibly difficult due to the massive temperatures that have to be duplicated, often requiring a minimum of 100 million degrees Celsius (180 million degrees Fahrenheit).
While the Earth’s mantle contains traces of 3He from the planet’s formation, its decay over billions of years has converted most of the original 3He to Helium-4 (4He). Therefore, scientists have hypothesized that the closest location to obtain active samples of 3He is the lunar surface due to the solar wind’s daily bombardment, resulting in 3He becoming embedded in the lunar regolith (dust). However, it is estimated that successful processing of 1 gram (0.025 ounces) of 3He would require approximately 150 tons of lunar regolith to be mined. Additionally, successful nuclear fusion here on Earth has yet to be realized.
While humanity continues to struggle with nuclear fusion and the need for 3He, this study demonstrates the awesome power of the Sun and how much we still don’t know about its complex and intricate processes responsible for providing life-giving power here on Earth.
What new discoveries about solar activity and 3He will astronomers make in the coming years and decades? Only time will tell, and this is why we science!
Is There Life on an Alien Planet? Fresh Findings Revive the Debate
Is There Life on an Alien Planet? Fresh Findings Revive the Debate
By Alan Boyle
An artist's conception shows the planet K2-18 b and its host star. (ESA / Hubble / M. Kornmesser)
Two new studies have sparked fresh debate about a faraway planet with a weird atmosphere. One of the studies claims additional evidence for the presence of life on the planet K2-18 b, based on chemical clues. The other study argues that such clues can be produced on a lifeless world covered with hot magma.
The hubbub illustrates how tricky it can be to determine whether life exists beyond Earth by looking for "biosignatures" with powerful telescopes — in this case, NASA's James Webb Space Telescope. It also illustrates the potential pitfalls of reporting provocative results.
A study published today in the Astrophysical Journal Letters attracted widespread attention when it reported that the chemical signatures of dimethyl sulfide and dimethyl disulfide had been found in K2-18 b's atmosphere. The findings were a follow-up to an earlier study published by the same researchers, which detected carbon-bearing molecules including methane and carbon dioxide in the atmosphere.
What's so special about dimethyl sulfide and dimethyl disulfide? The study noted that on Earth, those two chemicals are produced only by life, primarily microbial life such as marine plankton. The researchers claimed that the findings were consistent with their view that K2-18 b was what's known as a Hycean planet — a habitable, ocean-covered world with a hydrogen-rich atmosphere.
"Given everything we know about this planet, a Hycean world with an ocean that is teeming with life is the scenario that best fits the data we have," Cambridge astronomer Nikku Madhusudhan, the study's lead researcher, said in a news release.
The teeming-with-life scenario drew skeptical comments from an assortment of other scientists who have been studying the potential for exoplanetary life. The planetary science community has long debated the case for Hycean planets and detecting life on such planets.
"This paper adds (weak) evidence to one model amongst many of a complicated planet atmosphere," Oxford astronomer Chris Lintott wrote in a series of posts to Bluesky. "Currently, it's not much more of a hint of life as the lottery ticket in my back pocket is a hint of my having a million quid by Monday."
Arguing against the teeming-with-life scenario, researchers have noted that the chemical signature of dimethyl sulfide has been detected in the lifeless environments of a comet and the interstellar medium. One study, published last year, suggested that the sort of atmospheric chemistry documented previously by JWST could be due to interactions with a boiling-hot ocean of magma.
The magma hypothesis is front and center in a study that's just been accepted for publication in the Astrophysical Journal. That study was based on JWST observations of a different sub-Neptune planet, a cousin of K2-18 b known as TOI-270 d. A research team led by Christopher Glein of the Southwest Research Institute found that TOI-270 d's weird atmospheric chemistry could be explained by cooking methane and carbon dioxide in the presence of hot hydrogen and magma.
Glein said the findings could apply to K2-18b as well. "There appears to be a lack of diagnostic evidence for a Hycean state on these types of planets, at least on the ones we've observed so far," he said in an email.
John Stott, an astrophysicist at Lancaster University, phrased a similar assessment more colorfully in a Bluesky quip: "It will probably turn out to be vulcanism rather than Vulcans."
The questions surrounding dimethyl sulfide (DMS) and dimethyl disulfide (DMDS) are still up in the air. "I have not yet looked into whether this model can produce DMS and DMDS to the reported abundances (I just learned about this new work a day ago)," Glein wrote. "That's an important question, but first we need to confirm that these species are confidently detected."
The confidence level for the JWST observations reported in Madhusudhan's paper is at the 3-sigma level. That's statistically significant, but it doesn't quite hit the 5-sigma level that's associated with a confirmed discovery. Madhusudhan and his colleagues say that 16 to 24 hours of follow-up observation time with JWST may help them reach the 5-sigma level.
In a news release, Glein said the study of alien atmospheric chemistry was worthwhile even if it doesn't produce conclusive evidence of extraterrestrial life.
“While it is a bit disappointing to find that TOI-270 d is unlikely to be habitable, this planet still offers a fantastic opportunity to explore alternative paths of planetary origins and evolution,” Glein said. “We are learning much more about the crazy configurations of planets that nature comes up with.”
This week's debate raises a larger issue about the search for chemical biosignatures. How strong would the evidence have to be to convince scientists that the chemical compounds associated with life on Earth could only be produced by biological activity?
Stott was skeptical any such evidence would be strong enough.
"If we ever did find an exoplanet with robust biomarkers, it would be interesting philosophically," he wrote. "Personally, I'd only believe it if either: 1. We had a physical sample of the life (impossible anytime soon unless in solar system); or 2. A clear broadcast signal from intelligent life."
An Interesting Solution to the Hubble Tension: The Universe is Slowly Spinning
An Interesting Solution to the Hubble Tension: The Universe is Slowly Spinning
By Brian Koberlein
The magnificent Whirlpool galaxy, also known as Messier 51. Credit: NASA/ESA
Everything in the Universe spins. Galaxies, planets, stars, and black holes all rotate, even if just a bit. It comes from the fact that the clouds of scattered gas and dust of the cosmos are never perfectly symmetrical. But the Universe as a whole does not rotate. Some objects spin one way, some another, but add them all up, and the total rotation is zero. At least that's what we've thought. But a new study suggests that the Universe does rotate, and this rotation solves the big mystery of cosmology known as the Hubble tension.
The idea of a rotating universe isn't new. Even Einstein contemplated the idea. Most famously, Kurt Gödel devised a rotating model universe that is a solution to Einstein's field equations. The Gödel metric, as it's known, has some really strange properties. While standard cosmology metrics such as the one used in our standard model have space plus one time dimension, Gödel's model has two time-like dimensions. Distant galaxies would have a strange rotational bias to them, and light would spontaneously polarize. Even more bizarre is that the universe would be filled with time loops. Known as closed timelike curves (CTCs), they would allow you to meet yourself in the past simply by traveling through space.
Gödel's model is an interesting exploration of the theoretical limits of relativity, but it doesn't resemble the real Universe in any significant way. Astronomers have looked for things like galactic spin bias and asymmetries in the cosmic microwave background that would suggest cosmic rotation, and they all support a non-rotating universe to the limits of observation.
But our observational limits have gotten better over time, and they seem to have painted us into a theoretical quandary. We know the Universe began in a hot, dense state we call the Big Bang, and since that time, about 13.8 billion years ago, the cosmos has expanded. It continues to expand at an ever-increasing rate, thanks to dark energy. But what that increasing rate is, exactly, is a bit of a mystery. Observations of fluctuations in the cosmic microwave background find that the Universe expands at about 67 km/s per Mpc. However, observations of supernovae and Cepheid variables in distant galaxies find the Universe expanding at a faster rate of 73 km/s per Mpc. According to the standard model, these values should agree. The fact that they don't is known as the Hubble tension. This mystery stands at the heart of modern cosmology, so it isn't surprising that all sorts of wild solutions have been proposed. Modified gravity, quintessence, exotic supersymmetry particles—you name it. So why not reconsider the rotating universe model?
Matching cosmic rotation to observed Hubble values.
Credit: Szigeti, et al
This new model doesn't use the Gödel metric, but instead presumes the Universe is filled with a uniform rotating fluid. Non-rotating versions of this fluid have been proposed to explain dark energy, but the addition of rotation means that spacetime is given a twist, similar to the frame-dragging effect we've observed for rotating masses such as Earth. As the authors show, the rotating fluid would bias our observation of cosmic expansion with increasing distance. In other words, the more distant our measure of the Hubble parameter, the smaller it would appear.
Taking the nearby observations of cosmic expansion as the most accurate, the team assumes the 73 km/s per Mpc value is correct and then asks how fast the fluid would have to rotate to match the 67 km/s per Mpc observations of the cosmic microwave background. Matching the data, they obtained a rotation rate of ω = 3.5 radians per billion years. On a basic level, cosmic rotation can solve the Hubble tension problem. Interestingly, the rotation rate the authors found is just under the limit that would create closed timelike curves. The model rotates as fast as it possibly can before all temporal logic is tossed out the window.
While it's a fascinating result, there are plenty of caveats. To begin with, the model is a tweak model. The authors assume it's true to prove it works. There's nothing inherently wrong with tweak models, but tweak models are weak models, as the saying goes. Just because it can solve the problem doesn't mean it's the solution. Additionally, the introduction of a rotating fluid will affect things such as galactic evolution and galaxy clustering. The authors are aware of this and note that their next goal is to determine observable tests of their model. Time (and space) will tell if the model works in the end.
New and ‘strongest evidence yet’ has emerged suggesting that there is another world that could have life on it.
Scientists have discovered early signs that a distant planet in space called K2-18b could have some life.
The promising finding was made by the Cambridge University team studying the atmosphere
They detected signs of chemical molecules, which on Earth are produced by living organisms such as marine algae.
This is what a ‘Hycean’ world could look like (Picture: Reuters)
The scientists used the James Webb Space Telescope – the largest telescope in space armed with a high-resolution equipment that can reach further into space than its predecessor the Hubble Space Telescope.
However, the expert team stressed that more evidence is needed after the promising find.
How far is planet K2-18b?
The chemical fingerprints were of dimethyl sulfide (DMS) and/or dimethyl disulfide (DMDS), located in the atmosphere of K2-18b.
A report said: ‘While an unknown chemical process may be the source of these molecules in K2-18b’s atmosphere, the results are the strongest evidence yet that life may exist on a planet outside our solar system.’
K2-18b is the only exoplanet known to host both water and temperatures that could support life (Picture: AFP/Getty)
K2-18b isn’t a short journey away – it lives around seven hundred trillion miles from Earth.
For conventional spacecraft to travel that distance, it would take possibly hundreds of years.
Why is the finding significant?
This was the first time astronomers found carbon-based molecules in the atmosphere of an exoplanet in the habitable zone of space.
Scientists suspect it could be a ‘Hycean’ planet – a habitable, ocean-covered world.
Professor Nikku Madhusudhan, from Cambridge’s Institute of Astronomy and the research lead, said: ‘Earlier theoretical work had predicted that high levels of sulfur-based gases like DMS and DMDS are possible on Hycean worlds.
‘And now we’ve observed it, in line with what was predicted. Given everything we know about this planet, a Hycean world with an ocean that is teeming with life is the scenario that best fits the data we have.’
He said there were major questions concerning the processes that might be producing the chemicals.
As with any research, it was ‘important that we’re deeply sceptical of our own results’ and that rigorous further testing was needed despite the excitement.
The prof continued: ‘Decades from now, we may look back at this point in time and recognise it was when the living universe came within reach.
‘This could be the tipping point, where suddenly the fundamental question of whether we’re alone in the universe is one we’re capable of answering.’
The possibility of alien life continues to drive scientists determined to find evidence that we are not the only living things in the galaxy.
Strongest Evidence of Alien Life Yet Found 124 Light-Years Away
Strongest Evidence of Alien Life Yet Found 124 Light-Years Away
By Daniel Lawler, AFP
Artist's impression of an exoplanet near a red star.
(A. Smith, N. Madhusudhan/University of Cambridge)
Astronomers announced Thursday that they had detected the most promising "hints" of potential life on a planet beyond our Solar System, though other scientists expressed scepticism.
There has been vigorous debate in scientific circles about whether the planet K2-18b, which is 124 light years away in the Leo constellation, could be an ocean world capable of hosting microbial life.
Using the James Webb Space Telescope, a British-US team of researchers detected signs of two chemicals in the planet's atmosphere long considered to be "biosignatures" indicating extraterrestrial life.
On Earth, the chemicals dimethyl sulfide (DMS) and dimethyl disulfide are produced only by life, mostly microscopic marine algae called phytoplankton.
The graph shows the observed transmission spectrum of the habitable zone exoplanet K2-18 b using the JWST MIRI spectrograph. (A. Smith, N. Madhusudhan/University of Cambridge)
The researchers emphasised caution, saying that more observations were needed to confirm these findings, and that they were not announcing a definitive discovery.
But the implications could be huge, according to Nikku Madhusudhan, a Cambridge University astrophysicist and lead author of the study, published in The Astrophysical Journal Letters.
"What we are finding at this point are hints of possible biological activity outside the solar system," he told a press conference.
"Frankly, I think this is the closest we have come to seeing a feature that we can attribute to life."
But outside experts pointed to disputes over previous discoveries about the exoplanet, adding that these chemicals could have been created by unknown means having nothing to do with life.
Chemical clues
More than eight times the mass of Earth and 2.5 times as big, K2-18b is a rare exoplanet that orbits its star in a habitable or "goldilocks" zone.
This means it is neither too hot nor too cold to have liquid water, considered the most important ingredient for life.
Telescopes observe such far-off exoplanets when they cross in front of their star, allowing astronomers to analyse how molecules block the light streaming through their atmosphere.
In 2023, the Webb telescope detected methane and carbon dioxide in K2-18b's atmosphere, the first time such carbon-based molecules were detected on an exoplanet in a habitable zone.
It also detected weak signals of the chemical DMS, leading astronomers to turn Webb towards the planet again a year ago, this time using its mid-infrared instrument to detect different wavelengths of light.
They found much stronger signs of the chemicals, though still well below the "five sigma" threshold of statistical significance scientists seek for such discoveries.
Even if the results are confirmed, it would not necessarily mean that the planet is home to life.
Last year, scientists found traces of DMS on a comet, which suggested it can be produced in non-organic ways.
However the concentration of the chemical observed on K2-18b appears to be thousands of times stronger than levels on Earth, strongly suggesting a biological origin, Madhusudhan said.
Are we alone in the universe?
K2-18b has long been considered the premier candidate for a "hycean planet" – an ocean world bigger than Earth with a hydrogen-rich atmosphere.
These planets would not be expected to be home to intelligent alien life, but rather tiny microbes similar to those in Earth's oceans billions of years ago.
Some research has questioned whether the currently proposed hycean planets are too close to their stars to support liquid water, including K2-18b, which orbits its star every 33 days.
Raymond Pierrehumbert, a planetary physics professor at Oxford University, has conducted separate research indicating K2-18b is too hot for life.
If the planet did have water, it would be "hellishly hot" and uninhabitable, he told AFP, adding that oceans of lava were more plausible.
Sara Seager, a professor of planetary science at MIT, called for patience, pointing to previous claims of water vapour in K2-18b's atmosphere that turned out to be a different gas.
And within our solar system, Mars, Venus and moons such as Saturn's Enceladus all have "more chance to be realised as life-hosting," she told AFP.
Madhusudhan estimated that it would take just 16 to 24 more hours of Webb's time to confirm their findings, which could happen in the next few years.
Even beyond K2-18b, Madhusudhan said Webb and future telescopes could allow humanity to discover life outside our home planet sooner than one might think.
"This could be the tipping point, where suddenly the fundamental question of whether we're alone in the universe is one we're capable of answering," he said.
"Sterkste bewijs tot nog toe": wetenschappers zien aanwijzingen voor buitenaards leven op verre planeet
Een illustratie van de Universiteit van Cambridge over hoe K2-18b er zou kunnen uitzien
"Sterkste bewijs tot nog toe": wetenschappers zien aanwijzingen voor buitenaards leven op verre planeet
Artikel door Stien Schoofs
Wetenschappers van de Universiteit van Cambridge die al enkele jaren de planeet K2-18b bestuderen, vermoeden dat de planeet vol zit met microbieel leven. Dat hebben ze ontdekt door naar de chemische samenstelling van de atmosfeer te kijken met de James Webb ruimtetelescoop.
In die chemische samenstelling hebben ze gassen met de naam dimethylslfide (DMS) en/of dimethyldisulfide (DMDS) ontdekt. Dat staat te lezen in hun onderzoek in The Astrophysical Journal Letters. Op aarde kennen we die ook, want die worden geproduceerd door algen en fytoplankton in het water.
Fytoplankton zijn een soort algen en dus een levend organisme. Aangezien DMS en DMDS enkel nog maar bij levende organismen zijn gevonden, veronderstellen de onderzoekers dat het op de planeet K2-18b krioelt van het leven.
"Bovendien is de hoeveelheid van die gassen op K2-18b duizenden keren hoger dan wat we op aarde hebben", vertelt professor Nikku Madhusudhan, die het onderzoek op de Universiteit van Cambridge leidt, aan de BBC.
99,99999 procent zekerheid nodig
Het is voor alle duidelijkheid een veronderstelling. Eentje die ze in 2023 ook al eens deden, maar toen waren de onderzoekers maar voor 68 procent zeker. Omdat ze nu, 2 jaar later, kunnen spreken van een 99,7 procent zekerheid, brengen ze het nieuws nog eens naar buiten.
De wetenschappers benadrukken zelf dat er nog bijkomend onderzoek nodig is .Toch zijn ze hoopvol. "Dit is het sterkste bewijs tot nu toe dat er mogelijk buitenaards leven is. Realistisch gezien kan ik zeggen dat we dit nieuws kunnen bevestigen binnen 1 of 2 jaar", klinkt het bij Madhusudhan.
Onduidelijkheid over oorsprong gassen
"Als we bevestigen dat er leven is op K2-18b, zou dat in feite moeten bevestigen dat leven heel gewoon is in het sterrenstelsel", gaat hij enthousiast verder. Hij geeft ook wel duidelijk aan dat er nog veel vragen zijn in dit stadium van het onderzoek.
Los van het feit dat er nog geen 99,99999 procent zekerheid is over de resultaten, is er ook geen absolute zekerheid over de oorsprong van de gassen. "Het is niet omdat het op aarde afkomstig is van micro-organismes, dat het op andere planeten ook zo is", stelt professor Catherine Heymans van de Universiteit van Edinburgh.
ESA/Hubble, M. Kornmesser
Heymans heeft niets met het onderzoek te maken, en plaatst er nog vraagtekens bij. "In het universum gebeuren veel vreemde dingen", zegt ze aan BBC. "We weten niet welke andere geologische activiteiten plaatsvinden op de planeet die misschien die gassen produceren."
We hebben nog een grote wetenschappelijke berg te beklimmen als we een van de grootste vragen in de wetenschap willen beantwoorden
Er is nog een andere optie: intense komeetinslagen zouden voor die gassen kunnen zorgen. "Leven is een van de opties, maar het is een van de vele", zegt dr. Nora Hänni aan de universiteit van Bern. "We zouden alle andere opties strikt moeten uitsluiten voordat we leven claimen."
Ook het team van onderzoekers van Cambridge University weten dat die mogelijkheid er is en doen daarom onderzoek om te zien of DMS of DMDS ook geproduceerd kan worden zonder levende organismen.
Hoe dan ook voelt het voor de onderzoekers van Cambridge wel als een doorbraak. "We hebben nog een grote wetenschappelijke berg te beklimmen als we een van de grootste vragen in de wetenschap willen beantwoorden. Maar ik geloof dat we op de goede weg zijn", sluit Madhusudhan af.
Snel meer duidelijkheid over buitenaards leven?
Het is duidelijk: collega-wetenschappers willen meer duidelijkheid voordat ze aannemen dat er leven is op de planeet K2-18b. "Wetenschap is anders dan bijvoorbeeld de juridische wereld", verklaart Decin. "In de rechtbank ben je onschuldig tot het tegendeel bewezen is, terwijl in de wetenschap een hypothese overeind blijft tot iemand ze ontkracht."
En wetenschappers doen er alles aan om die hypothese te ontkrachten, net omdat dat de hypothese sterker maakt als dat niet lukt. "Dat neemt niet weg dat dit een heel belangrijke stap is."
Een stap die ons snel kan vertellen of er een kans is op buitenaards leven? "Nee, dan moeten we nog wel wat stappen zetten om die zekerheid te hebben", nuanceert Decin.
"Je moet je voorstellen dat je als buitenaards wezen naar de aarde kijkt. Je ziet ons daar ook niet op lopen", maakt ze de vergelijking. "Je zal zien dat er water aanwezig is en methaan bijvoorbeeld. Dat is niet genoeg om te bevestigen dat er leven mogelijk is. Dan moet je ook bijkomend onderzoek doen, net zoals we hier nog lang zullen moeten doen voor we zekerheid hebben over buitenaards leven."
GERELATEERDE VIDEO'S
Is K2-18b a Hycean Exoworld? With Dr. Nikku Madhusudhan
K2-18b: an exoplanet fit for life?
NASA's Astonishing Find Super-Earth(K2-18b): A Planet with a sign of life!
Roadmap for Obtaining First Sample Returns from Mercury and Venus
Roadmap for Obtaining First Sample Returns from Mercury and Venus
By Laurence Tognetti
Ultraviolet image of Venus (left) and optical imageof Mercury (right) obtained by NASA's Mariner 10 spacecraft during its mission in the 1970s. (Credit: NASA)
How can we successfully collect and return samples from Mercury and Venus to Earth? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a pair of researchers from the California Institute of Technology (Caltech) discussed how future missions could successfully conduct sample return missions from the two innermost planets in our solar system. This study has the potential to help scientists, engineers, and mission planners better understand new methods for conducting sample returns throughout the solar system, and specifically from hard-to-reach destinations.
Here, Universe Today discusses this incredible research with Teng Ee (Tony) Yap, who is a PhD student at Caltech and lead author of the study, regarding the motivation behind the study, significant takeaways, next steps for developing sample return missions, and the importance of returning samples from Mercury and Venus. Therefore, what was the motivation behind the study?
Yap tells Universe Today. “This study came out of a workshop held by the Keck Institute of Space Studies (KISS) at Caltech on Sample Return across the Solar System, which brought together experts in geo/cosmochemistry, orbital dynamics, mission science, etc. (as well as early career scientists like myself) to discuss the highest priority scientific objectives that can be achieved through sample return from bodies spanning the whole solar system, and what technologies need to be developed for those missions to be feasible.”
For the study, the researchers discussed the pros and cons of obtaining samples from Mercury and Venus, specifically mentioning the absence of meteorites that originate from the inner solar system, as all collected meteorites have originated from beyond the Earth’s orbit, specifically the main asteroid belt, Mars, and the Kuiper Belt. The researchers emphasized that along with the lack of meteorites from the inner solar system comes a lack of knowledge regarding the planetary building materials, such as carbonaceous and non-carbonaceous materials, and what materials could have existed in the inner solar system during its early formation billions of years ago.
Additionally, the researchers made a case for sample returns from both Mercury and Venus by using past and current missions like NASA’s MESSENGER to Mercury, active missions like the European Space Agency’s BepiColombo to Mercury, and proposed future NASA missions like DAVINCI and VERITAS to Venus. Therefore, what are the most significant takeaways from this study?
“We do not have a single sample, in the form of a meteorite, from Mercury and Venus,” Yap tells Universe Today. “The building blocks of both planets are derived from the innermost Solar System, and we need to know what these blocks look like geochemically to better understand the evolution in the early Solar System ~4.6 billion years ago and figure out if they represent the missing component needed to explain the Earth’s composition. A sample return mission to Mercury is possible with the development of nuclear thermal propulsion – it is unclear when this technology will come online’, however. A sample return mission to Venus doesn’t appear to be feasible, even with nuclear propulsion (largely due to its large mass; tough to get down to the surface and back to Earth). Balloon-based technologies (imagine a lab floating in a Venusian cloud layer) are being considered.”
Getting a space mission approved for flight is often a lengthy and time-consuming process taking anywhere from several years to decades to go from a proposal to a fully operational and launch-ready space mission. To facilitate this process, NASA incorporates its Technology Readiness Levels system to gauge each step of development for a mission, including laboratory and real-world demonstrations for all systems and subsystems. Each level often involves countless tests, evaluations, re-designs, more tests, and more evaluations until the spacecraft is finally ready for flight.
For example, while NASA’s Mariner 10 was the first spacecraft to conduct a detailed study of Mercury in 1975, it would be another 23 years before another spacecraft was proposed to travel to the closest planet to the Sun. This is because traveling that close to the Sun is very dangerous to the Sun’s enormous gravity that would pull in any spacecraft traveling too close. Therefore, multiple gravity assists and planetary flybys were utilized to slow a spacecraft to the necessary speeds to orbit Mercury.
The MESSENGER spacecraft was proposed in 1998 and launched in 2004, but didn’t enter Mercury orbit until 2011. Therefore, what are the next steps for developing future missions to return samples from Mercury and Venus, along with what is the importance of returning samples from Mercury and Venus?
Yap tells Universe Today, “Pushing for the development of nuclear propulsion and balloon-based technologies! Getting the community excited about looking ‘in’ towards Mercury and Venus, in addition to looking ‘out’ towards the giant planets and their moons. Strengthening the science case for sample return to those planets (i.e., figuring out how to make the most of, say, 1 gram of rock scraped or drilled from their surfaces).”
Yap continues, “Mercury and Venus have the potential to solve a major and longstanding problem in the field of cosmochemistry: tracing the building blocks of the Earth. Ironically, we don’t know how to ‘build’ the Earth from materials we know; there is no mixture of meteorites we know that yields the Earth’s composition.”
How will returned samples from Mercury and Venus help scientists better understand the history of the planets and the solar system in the coming years and decades? Only time will tell, and this is why we science!
The most distant object ever explored up close might just have revealed one of the earliest stages of planet formation.
This is Arrokoth, which resides in our solar system’s Kuiper Belt, a region of objects beyond Neptune. On January 1, 2019, NASA’s New Horizons spacecraft found some unusual mounds on Arrokoth, which scientists say are some of the original building blocks of our solar system, from billions of years ago.
Image via NASA/ Johns Hopkins/ Southwest Research Institute/ Roman Tkachenkou.
Arrokoth, the Kuiper belt object known for its reddish hue and bi-lobed snowman shape, has bumpy mounds all over its larger lobe, and these may be the remnants of boulders that once smooshed together to create the whole object.
Using data from the New Horizons spacecraft, which flew past Arrokoth around 44.6 astronomical units from the Sun in 2019, a team led by planetary scientist Alan Stern of the Southwest Research Institute made a close study of the lobe, known as Wenu.
They discovered 12 bumps that have more or less the same size, shape, color, and reflectivity, suggesting that these are the units from which Wenu was assembled.
"It's amazing to see this object so well preserved that its shape directly reveals these details of its assembly from a set of building blocks all very similar to one another," says astronomer Will Grundy of Lowell Observatory. "Arrokoth almost looks like a raspberry, made of little sub-units."
Arrokoth, hanging out far from the Sun, past Pluto, in the Kuiper Belt of icy rocks, is thought to be a seed of a planet that never made it to full growth. Moreover, because of its location, its alteration by solar radiation is thought to be minimal; it is the most primitive and pristine object we've ever observed.
Previous studies have shown that Arrokoth was once two smaller objects in a binary orbit that gradually came together and fused, but there's a lot more to its formation history. A 2020 paper showed that it was actually a whole bunch of objects in a complex orbital dance that gently came together under gravity at low speeds to form a larger rock.
Color-coded images of Arrokoth that show the mounds. (SwRI)
This supports the notion that planet growth starts with a bunch of smaller objects from the same part of the cloud of debris that surrounds a newborn star. And the new discovery further supports this scenario.
Arrokoth measures about 35 kilometers (22 miles) in length, by 20 kilometers (12 miles) in width, and 10 kilometers (6 miles) in thickness. And Wenu, New Horizons observations revealed, wasn't smooth, but was covered in a series of interlocking mounds, or bumps, that incited curiosity about how it formed.
Using two close-up images from the New Horizons flyby, Stern and his colleagues conducted an in-depth analysis of the mounds of Wenu. They counted, in total, 12 mounds, generally about 5 kilometers across, and with similar length-to-width ratios, in addition to other similarities.
To figure out how Wenu got that way, the researchers conducted simulations, focusing on two formation scenarios: smaller objects, about 3 kilometers across, slamming together at high speed; or larger objects, about 5 kilometers across, gently glomming together at low speed.
The first scenario, the high-speed one, is unlikely to be how Wenu formed. The resulting object was too smooth, since the rocks shattered and smushed on impact. The slow formation scenario, however, produced a lumpy blob that looked a heck of a lot like Wenu.
The lumpy object resulting from low-speed simulations (left) compared to Wenu (right). (Stern et al., PSJ, 2023)
This fits previous findings about the slow and gentle formation of Arrokoth, but it raises another question: why are the rocks all more or less the same size? That's a question we might need more modeling – and more observations of other planetesimals – to answer.
"Similarities including in sizes and other properties of Arrokoth's mound structures suggest new insights into its formation," Stern says. "If the mounds are indeed representative of the building blocks of ancient planetesimals like Arrokoth, then planetesimal formation models will need to explain the preferred size for these building blocks."
As for the smaller of the two lobes, Weeyo, at first glance, it doesn't look a lot like Wenu, with its large crater. However, the team was able to tentatively identify three mound-like structures. So it's not impossible that Weeyo formed the same way.
A NASA mission, Lucy, is currently underway to explore the populations of asteroids that share the orbit of Jupiter. Looking for signs of mounds among these objects will help scientists understand exactly how common this formation process might be.
Blue Origin All Female Crew, Including Katy Perry Scream All The Way Back To Earth!, UFO UAP Sighting News.
Blue Origin All Female Crew, Including Katy Perry Scream All The Way Back To Earth!, UFO UAP Sighting News.
Date of landing: April 14, 2025
So an all woman crew...every guy has thought about such sci-fi epic stories...and yet Earth had just such a historical moment today...as they landed in the desert in a space capsule. You might by chance notice a little screaming every now and then. The screams are as if they saw an alien for the first time, but it's not, it's just the sudden G force change as they drop, the parachute opens and they hit the ground. I sure hope Katy Perry can sing again after all that screaming but hey, if not, there is an opening on the space station she might take.
Frozen Lava Domes on Europa Might Provide Future Habitats!
Frozen Lava Domes on Europa Might Provide Future Habitats!
By Mark Thompson
Ridges disrupted by the localized formation of domes may be indicative of thermal upwelling of water from beneath Europa's crust (Credit : NASA/JPL/Southwest Research Institute)
Europa is one of the four satellites of Jupiter that were discovered by Galileo over 400 years ago. It’s slightly smaller than Earth’s Moon and is covered by a thick shell of ice, beneath which lies a global subsurface ocean kept liquid by tidal heating from Jupiter’s strong gravitational pull. Its surface is marked by cracks, ridges, and smooth plains, suggesting ongoing geological activity. There are features like domes and ridged terrains indicate that material from the interior may be interacting with the surface, possibly through processes like cryovolcanism.
This is Europa in true colour from Juno's flyby
(Credit : NASA/JPL-Caltech/SwRI/MSSS/Kevin M. Gill)
The Galileo spacecraft’s Solid State Imager revealed that Jupiter’s moon Europa has a geologically young and diverse surface, Some of the domes, particularly those with circular or lobate shapes and smooth surfaces, are believed to be cryovolcanic in origin, formed by the eruption of water or slushy ice rather than molten rock. Various formation mechanisms have been proposed, including diapirism (upward movement of warmer ice) and cryovolcanic emplacement. Previous studies have identified 38 candidate cryolava domes in Europa’s Conamara region, with a third modelled using a volume flux approach that suggested the erupted cryolava was far less viscous than previously estimated.
Artist's Image of NASA's Galileo Spacecraft Flying Past Jupiter's moon Io
(Credit : NASA)
A recent piece of research led by Kierra A. Wilk from the NASA Goddard Space Flight Center has expanded the study to include 186 domes, providing deeper insight into the behaviour of Europa’s cryolava and the potential for exchange between the surface and the subsurface ocean making it an environment that could be suitable for life. Using images and elevation data from Galileo’s E6, E14, E15, and E17 flybys, the team identified and mapped potential cryovolcanic domes on Europa, noting their geological context, such as whether they intersect ridges, sit in depressions, or show signs of flow lobes.
For each dome, three topographic profiles were created with adjustments made for surrounding terrain to estimate relative dome heights. The average diameter and height of each dome were then used in models based on fluid dynamics to understand how they formed. While Earth’s lava domes can take months to decades to form, Europa’s cryolava domes are estimated to have formed in as little as one month to up to 50 years, depending on how quickly the cryolava cooled and solidified.
The new study uses the maximum dome height rather than the average based on previous studies, as using average height can underestimate cryolava viscosity by up to 100 times. The estimated formation time for the domes matches earlier studies, but viscosity may be higher if cooling and formation happened over the same period.
These findings suggest Europa's cryolava may behave like basaltic to andesitic lava on Earth and could be made of thick, particle-rich brine. Viscosity differences hint at varying temperatures or compositions in Europa’s interior. Upcoming high-resolution data from the Europa Clipper mission will help identify more domes and active areas, offering deeper insight into Europa's geological activity and the potential habitability of its subsurface reservoirs.
How Crater Shapes Are Revealing More About Titan’s Icy Crust
How Crater Shapes Are Revealing More About Titan’s Icy Crust
By Mark Thompson
Artist Illustration of Titan's Thin Icy Crust (Credit : NASA/JPL)
Titan, Saturn's largest moon, is a fascinating world that is unique among moons of the outer Solar System. It’s shrouded in a thick, hazy atmosphere rich in nitrogen and methane and it's the only moon with a substantial atmosphere and the only place besides Earth known to have stable bodies of surface liquid. These aren't water lakes and seas, however, but collections of liquid hydrocarbons (primarily methane and ethane) that form a complex cycle similar to Earth's water cycle. Beneath this alien landscape lies a mysterious interior: likely a water-ice crust floating atop a subsurface ocean of liquid water mixed with ammonia.
Saturn's moon Titan
(Credit: NASA/Kevin Gill)
A new paper reveals how a team of researchers from Imperial College London, UK have compared real craters on Titan with computer-simulated ones to determine the thickness of its icy shell. This information is important for understanding Titan's interior structure, how it evolved thermally, and its potential to produce organic molecules—making it significant for astrobiology research.
Impact simulations for Titan used special hydrodynamic code that simulates crater impact processes on planetary surfaces. They ran simulations with vertical impact velocities at 10.5 km/s, testing three impactor sizes (2, 5, and 10 km). The models incorporated strength and damage parameters for methane clathrate (where methane gas is trapped inside water) and water ice based on previous studies, using a model that simulates how rock and debris behaves like a fluid during high energy impact events.
Image showing surface detail on Titan
(Credit : NASA)
They also employed an ANEOS equation of state to describe how water ice behaves under extreme conditions, this was also used for methane clathrate too since there is limited data on this state. The simulations used adaptive resolution (starting at 40 cells per projectile radius) and continued until crater dimensions stabilised, with error margins of about 15% for dimensions and two grid cells for depth measurements.
All of the simulated impact craters appeared deeper than those actually observed on Titan. Among the tested models, the 10 km methane clathrate-capped scenario produced craters closest to reality, though still hundreds of meters too deep. Pure ice models performed worst, creating craters over a kilometre deeper than observed, but results improved as the ice lid thickness decreased.
When comparing Titan's actual craters to computer simulations, researchers found the 10 km methane clathrate model best matched reality. This model produced craters with central peaks and sharp rims like the observed Selk crater, though slightly deeper—likely due to sand filling in the craters over time. Pure ice models created much simpler yet significantly deeper craters that couldn't be explained by erosion or infill. The most accurate model appears to be a 10 km methane clathrate layer above 5 km of conductive ice, with warm convective ice beneath at 256.5 K.
Is it possible to build a Dyson sphere that isn't catastrophically unstable? New research says yes, but only in one type of star system.
(Image credit: cokada via Getty Images)
Dyson spheres, the hypothetical mega-structures that advanced alien civilizations might use to enclose a star and harness its energy, suffer from a fatal flaw: They are catastrophically unstable. But now an engineer claims to have figured out a way to stabilize these structures — and all it takes is two stars.
In the 1960s, physicist and polymath Freeman Dyson cooked up the idea of these eponymous spheres. He envisioned that a sufficiently advanced society would have an insatiable need for living space and energy. And if they were industrious enough, they could solve both challenges by taking apart a planet and turning it into an enormous spherical shell. This sphere would enclose a star, providing billions of planets' worth of surface area and capturing vast amounts of solar energy.
Dyson calculated that a shell made from a planet with the mass of Jupiter could completely enclose the sun at roughly the orbit of Earth. But the gravity inside a hollow shell cancels out, which means there's nothing tethering the shell to the star. They are free to move in independent directions, which means that soon enough a star hosting a Dyson sphere will simply crash into the shell, destroying it.
In apaper published Jan. 29in the journal Monthly Notices of the Royal Astronomical Society,Colin McInnes, an engineer at the University of Glasgow, found a way to theoretically stabilize a Dyson sphere. The trick is that you need a system with at least two stars.
Hunting for stable Dyson spheres
McInnes started by searching for any points within a binary star system that could host a stable Dyson sphere arrangement, where the sphere could stay in place and the gravitational forces exerted on it would be uniform. He found one arrangement, where the sphere surrounds both stars. But that situation was only mildly stable and likely to suffer the same problem as the single-star case.
Another stable point arises when the sphere orbits independently, surrounding neither star. While this might be useful for space station outposts, it doesn't provide the energy-capturing benefits of englobing a star.
But McInnes did find one stable — and useful — configuration. This only happens in binary systems in which one star is much smaller than the other. In that specific case, the Dyson sphere can enclose the smaller of the two stars. The motion of that smaller star acts like a gravitational anchor, keeping the Dyson sphere in motion with the same orbit around the larger star, preventing a catastrophic collision.
There are several caveats to this. The smaller star has to be no bigger than around one tenth the mass of the larger companion, otherwise the gravitational stable point disappears. And the sphere has to be extremely light and thin compared with the two stars, otherwise its own gravitational influence mixes into the dynamics of the system and destroys the stability.
And, of course, this analysis ignores any practical engineering considerations, like the stresses and tensions the sphere might experience, or how to build the thing in the first place.
While it's unlikely humans will build a Dyson sphere in the distant future — if ever — this research does help inform searches for extraterrestrial civilizations. Presumably, a sufficiently advanced civilization would have made the same realization before building its own Dyson sphere, and so we shouldn't look for them around solitary stars.
Instead, scientists could look for large, bright stars with a diffuse, infrared companion — the telltale sign of the heat leaking out of a Dyson sphere enclosing the smaller star of a larger companion.
The research proposes looking for extraterrestrial life in so-called “computational zones” that could encompass a much wider range of habitats than traditional “habitable zones,” which are areas where liquid water might exist on a planetary surface in similar conditions to those found on Earth when the earliest forms of life emerged.
Computational zones, in contrast, are areas in which information can be processed, and could include any environment with three principal characteristics—capacity, energy, and instantiation (or substrate)—which could include overlooked substellar objects, such as brown dwarfs, the subsurface oceans of ice moons like Europa, or massive artificial structures, such as Dyson spheres.
Earth is the only world we know of that hosts life, leaving us with a rather limited sample to work with on the important question of whether we are alone in the universe. For this reason, it makes sense for scientists searching for life to focus their efforts on worlds that are similar to our own, and to especially prioritize the presence of surface liquid water, given how important this key ingredient has been to life on Earth.
That said, life may arise in many unexpected places that could be well beyond the limits of our imaginations. This problem inspired Caleb Scharf, a senior scientist for astrobiology at NASA’s Ames Research Center, and Olaf Witkowski, an expert on artificial intelligence (AI) and director of Cross Labs in Tokyo, Japan, to think of new ways to expand the scope of our search for aliens.
Now, the pair have unveiled a strategy to look for life that is built on the idea of computation, which the researchers define as “a set of physical processes that act on information represented by states of matter” and that “encompasses biological systems, digital systems, and other constructs,” according to a study recently published on the preprint server arxiv.
“One key piece of the computational zone idea is that it’s this very natural way to merge all the factors we look for in searching for life into one neat package—if you look for where computation can happen you naturally look at environmental conditions, energy, and what things are built out of,” Scharf said in an email. “It’s very agnostic though” in that “it doesn’t presume much about what life will be like except it must process information.”
“For example, this makes the interiors of icy moons like Europa or Enceladus just as important as the surface of a rocky planet, and puts these places on much more equal footing,” he continued. “Computational zones also give a new way to think about the outward signatures of life—if information processing is the core feature, what might that do to the world around it? And that creates a very natural bridge to questions of technology (or what we call technology) or how life might expand and ‘outsource’ its needs.”
The idea of computational zones emerged over the course of years as Scharf and Witkowski collaborated with each other on projects, while also delving into their own unique fields of astrobiology and AI research. Like many researchers who work in these fields, Scharf and Witkowski hoped to both develop a more unbiased method of evaluating the cosmos for the presence of life that didn’t depend so much on parameters linked to Earth.
“We may be introducing a lot of Earth biases when trying to project our knowledge onto other systems distant from Earth,” Witkowski told Motherboard in an email. “We essentially make a lot of assumptions about the nature of life, its necessary ingredients, and its characteristic signatures that may be detected when we point our equipment in its general direction.”
“One way to escape this limitation is to consider universal characteristics of life: what are possible or likely invariants of living systems which evolve anywhere in our universe?” he continued. “When one looks at life through the lens of information, one may see patterns and properties that are present regardless of the environment or substrate in which the living systems evolve. They all perform a certain type of computation, which we want to ultimately be able to detect. This may cast a larger and more adequate net over the systems which may contain life.”
The “Bingo moment,” as Scharf described it, was the team’s realization that fundamental physical rules about the limits of energy required for computation should be applicable to both biological and digital information processes.
“This paper is kind of the opening salvo on expressing this idea and showing how it might be applied to get us all the way to real-world measurements and strategies for looking for life that doesn’t make too many assumptions about how that life is built—it could be biological, digital, or something else,” Scharf explained.
“In this sense computational zones offer a less-contentious way to think more out of the box without going full ‘Borg’ in our hypothetical extrapolations!” he noted.
The new study, which has been submitted for publication in The Astrobiology Journal, runs with this idea by outlining the three major components of computation in the context of a search for life. Capacity describes the number of available states for carrying information, which includes factors such as the chemical ingredients available for computation. Energy refers to power sources that can support computation, such as sunlight or hydrothermal vents. Last, instantiation refers to the platform or substrate upon which the computation takes place.
This fresh perspective on one of humanity’s oldest questions could expose hidden opportunities to look for life beyond the conventional habitable zones where liquid water might flow. To that end, the team plans to continue developing the concept so that it can inform and expand the search for other beings in the universe, whether they are biological, artificial, or something else entirely.
“We’re starting to think about ways to accurately describe the computational hierarchy of life’s processes,” Scharf said. “Should metabolism be classified as computational or is it just a support process for computation? How does computation differ between microbial life and complex life? Just how much computation does life carry out—we estimate some of this in the paper, but what’s the net total computation of Earth, for example? (and yes, it’s very Hitchhiker’s Guide to the Galaxy!)”
“By adding this additional lens of computation, we don’t mean to replace current tools, but rather extend their perspective on complex life that may be found in the universe,” added Witkowski. “Hopefully, this leads directly to some ways to better understand and find more strands of it. Maybe it also leads to ways of looking at Earth and our solar system too, and the computation that is available within it. We can imagine designing new models to determine promising areas in the universe worth looking at in priority for traces of life. This is a fascinating new tool that we’re looking forward to developing further.”
Researchers have proposed many origins for a gravity anomaly in Wilkes Land, East Antarctica, but the latest evidence suggests the subglacial hole is an impact crater measuring 315 miles across.
Because it is buried beneath the Antarctic ice sheet, the Wilkes Land crater can only be seen through gravity and other forms of mapping. In this map, the crater is located in the bottom right corner and forms a light-colored U-shape surrounded by darker areas.
(Image credit: Klokočník, Kostelecký & Bezděk. Earth Planets Space (2018). Reshared under the terms of Creative Commons (CC BY 4.0))
Why it's incredible: Evidence suggests it could be the greatest known impact crater on Earth.
The Wilkes Land crater is a hole in the bedrock beneath East Antarctica's ice sheet measuring 315 miles (510 kilometers) across. Researchers have been trying to explain its existence since the 1960s, and the most recent evidence suggests it was born from a cataclysmic meteorite impact.
The crater was first detected as a huge dent in Earth's gravitational field. Initial ground-based seismic and gravity surveys already indicated that the crater was huge — around 150 miles (240 km) across — but newer techniques reveal that it is likely more than double this size.
The Largest Impact Crater on the Planet; Hidden in Antarctica & 300 Miles Wide
According to a 2018 study, the Wilkes Land crater sits about 1 mile (1.6 km) beneath the surface of Antarctica's ice sheet. The study showed the crater in more detail than ever before and examined its potential link with southern Australia, which was connected to East Antarctica until around 35 million years ago. While the origin of the crater remains uncertain, the results of the study suggest the event that created the hole likely occurred before the continents separated.
Researchers have proposed several explanations for the Wilkes Land crater, including that it could be a volcanic structure, a sedimentary basin, a deeply eroded valley or a meteor impact crater, according to a 2015 paper. For that paper, scientists used satellite remote sensing techniques to map the crater and determine its physical characteristics. In the middle of the hole in Earth's gravitational field, known as a negative gravity anomaly, they found a positive gravity anomaly, with the ice sheet filling the gap around this central peak like a huge, frosty donut.
The central peak is likely a structure known as a mass concentration, or a "mascon," according to the study. Mascons can occur within meteor impact structures due to the meteor crashing through Earth's crust and affecting the mantle beneath. Following the impact, the mantle may recoil and form a dense plug, resulting in a positive gravity anomaly, the study authors wrote.
A map of Antarctica showing gravity data across the frozen continent. Wilkes Land is situated in the bottom right corner of the map. A patch resembling a U-shape surrounded by dark blue is the Wilkes Land crater. (Image credit: Klokočník, Kostelecký & Bezděk. Earth Planets Space (2018). Reshared under the terms of Creative Commons (CC BY 4.0))
The Wilkes Land crater and its mascon aren't perfectly circular and instead form a U-shape, according to the 2018 study, whose results support the conclusion that the crater was caused by a meteor impact. The northern side of the crater is fragmented, perhaps as a result of tectonic processes that ripped Australia and Antarctica apart, the authors noted. Parts of the crater are clearly visible in southern Australia, they added.
If the Wilkes Land crater is an impact crater, then it "would be the greatest impact crater known" on Earth in terms of its size, the authors wrote.
In the 2015 study, researchers found that the crater's diameter matches the speed and size of space rocks that regularly crashed into Earth during its early history between 4.1 billion and 3.8 billion years ago. "The WLA [Wilkes Land Anomaly] could have been created by such bolides," they wrote in the study.
"Nonetheless, because of the constraints imposed by the overlying continental ice sheet, [...], we believe that the other explanations for the subglacial structure remain viable," they added.
Discover more incredible places, where we highlight the fantastic history and science behind some of the most dramatic landscapes on Earth.
Geologists Find Clues In Crater Left by Dinosaur-Killing Asteroid
Geologists Find Clues In Crater Left by Dinosaur-Killing Asteroid
Geophysicists announced this week that they have successfully collected key samples from the site of the asteroid strike that likely wiped out the dinosaurs.
(Joe Tucciarone/Science Source)
Scientists have had a literal breakthrough off the coast of Mexico.
After weeks of drilling from an offshore platform in the Gulf of Mexico, they have reached rocks left over from the day the Earthwas hit by a killer asteroid.
The cataclysm is believed to have wiped out the dinosaurs. “This was probably the most important event in the last 100 million years,” says Joanna Morgan, a geophysicist at Imperial College in London and a leader of the expedition.
Liftboat Myrtle is a drilling platform normally used for oil operations. Since April, geologists have been using it in the Gulf of Mexico to drill into the crater Chicxulub. (DSmith/ECORD/IODP)
Since the 1980s, researchers have known about the impact site, located near the present-day Yucatan Peninsula. Known as Chicxulub, the crater is approximately 125 miles across. It was created when an asteroid the size of Staten Island, N.Y., struck Earth around 66 million years ago. The initial explosion from the impact would have made a nuclear bomb look like a firecracker. The searing heat started wildfires many hundreds of miles away.
After that, came an unscheduled winter. Sulfur, ash and debris clouded the sky. Darkness fell and, for a while, Earth was not itself.
“I think it was a bad few months, really,” Morgan says.
That’s an understatement: Scientists believe 75 percent of life went extinct during this dark chapter in Earth’s history, including the dinosaurs.
Researchers have sampled Chicxulub before, but this expedition by the European Consortium for Ocean Research Drilling precisely targets a key part of the crater yet to be studied: a ring of mountains left by the asteroid. This “peak ring” is a fundamental feature of the strike and should tell researchers much more about it, says Sean Gulick, a geophysicist at the University of Texas at Austin, who co-leads the team with Morgan.
For weeks, they’ve been drilling — and going back in time. Each layer of rock they pass through is connected to a part of Earth’s history.
Scientists on Myrtle have been drilling around-the-clock. This week, they finally reached a buried ring of mountains created by the asteroid. (ELeBer/ECORD/IODP)
“We went through a remarkable amount of the post-impact world. All the way into the Eocene times — so between 50 and 55 million years ago,” Gulick says.
The rocks they’ve pulled out show how life began to recover after the cataclysm, Gulick says. “We’ve got all these limestones and rocks that contain the fossils from the world after the impact, all the things that evolved from the few organisms that survived.”
The research team finally reached the top of the peak ring this week. It appears to be a thick layer of broken, melted rock just beneath a layer of sandstone that may be the leavings of a huge tsunami that was triggered when the asteroid struck.
Gulick thinks the rocks hold clues. For example, if any microscopic organisms survived near the site of the strike, their fossils might be in these samples. In June, the rock cores will be sent back to a lab in Germany for further study.
The asteroid strike marked the end of an era. But the creatures that made it through that catastrophe went on to shape the world again, says Morgan.
“The mammals survived,” she says. “And that led on to our own evolution.”
At the site of the dinosaur-killing crater, scientists find a surprise
When colossal asteroids rock Earth, it's not all doom and gloom.
The menacing asteroid that wiped out non-avian dinosaurs left a colossal marine crater in what's now the Yucatan Peninsula. But after analyzing deeply drilled rock core from the impact site created by the six-mile-wide asteroid, geologists have found compelling evidence that life soon thrived in the basin following the seismic episode.
The asteroid's impact stoked nutrients and chemicals to be released from beneath the seafloor, a process called hydrothermal activity. Similar activity naturally occurs today in the deep sea, where hydrothermal vents emit superheated chemical-rich fluid into the water, feeding unique colonies of life, including huge tubeworms, crabs, fish, microorganisms, and beyond.
"This study reveals that impact cratering events, while primarily destructive, can in some cases also lead to significant hydrothermal activity,” Steven Goderis, a researcher at Vrije Universiteit Brussel in Belgium who co-authored the study, said in a statement. “In the case of Chicxulub, this process played a vital role in the rapid recovery of marine ecosystems.”
The research was published this week in the peer-reviewed journal Nature Communications.
The colossal impact event, which triggered a mass extinction event over much of Earth's land and ocean environments, also filled the present-day Gulf of Mexico with nutrients for at least 700,000 years, the researchers concluded.
In the core drilled from the impact site, called "Chicxulub crater" (which you should Google for a novel Google-created search result), researchers found a ratio of the metallic element osmium that is associated with asteroid remnants. When the asteroid struck this region, its pulverized particles — which contained osmium — mixed beneath the seafloor and were emitted into the water, before eventually settling back down on the seafloor. When scientists drilled into the ocean bottom, they brought up this ancient seafloor, revealing that hydrothermal fluid containing asteroid remnants flowed into the gulf for hundreds of thousands of years.
The impact, which precipitated widespread hydrothermal activity, ultimately created a nutrient-rich oceanic bath, the researchers say.
"After the asteroid impact, the Gulf of Mexico records an ecological recovery process that is quite different from that of the global ocean, as continuous hydrothermal activity has created a unique marine environment," Honami Sato, an earth scientist at Japan's Kyushu University who led the research, explained.
If such a cataclysmic event could create extremely habitable conditions on a region of Earth, the same might happen on other worlds, too. It could happen on ocean moons, or in a related way, perhaps even on desert worlds. Mars, for example, is a planet bombarded with meteor strikes. Such impacts could melt the plentiful water ice in parts of Mars' subsurface, creating an inviting environment for microbes to thrive.
The risks of an asteroid impact
Fortunately for us earthling land-dwellers, the odds of a cataclysmic space rock impact are exceedingly small. Here are today's general risks from asteroids or comets both tiny and very large. Importantly, even relatively small rocks can still be threatening, as the surprise 56-foot (17-meter) rock that exploded over Russia and blew out people's windows in 2013 proved.
Every single day about 100 tons of dust and sand-sized particles fall through Earth's atmosphere and promptly burn up.
Every year, on average, an "automobile-sized asteroid" plummets through our sky and explodes, according to NASA.
Impacts by objects around 460 feet (140 meters wide) in diameter occur every 10,000 to 20,000 years.
A "dinosaur-killing" impact from a rock perhaps a half-mile across or larger happens on 100-million-year timescales.
Scientific Report on Communication Signals from Extraterrestrial Civilizations
Scientific Report on Communication Signals from Extraterrestrial Civilizations
Abstract
The search for extraterrestrial intelligence (SETI) has long fascinated scientists. This report explores various potential communication methods that extraterrestrial civilizations might employ, including neutrino signals, laser communications, gravitational waves, radio waves, and quantum codes. Each method's descriptions, advantages, disadvantages, and future perspectives are discussed to evaluate their feasibility as means of contact with intelligent life beyond Earth.
1. Neutrino Signals: A Potential Medium for Cosmic Communication
Introduction
Neutrinos are among the most fascinating subatomic particles known to science. Produced during nuclear reactions, such as those occurring in stars, they are incredibly weakly interacting, allowing them to traverse vast distances without being absorbed or deflected by matter. This unique property of neutrinos has sparked interest in their potential use as a medium for communication across astronomical distances. In this essay, we will explore the nature of neutrinos, their capabilities as a communication medium, the advantages and disadvantages of using them for communication, and the future perspectives for neutrino communication technology.
Nature of Neutrinos
Neutrinos are fundamental particles that belong to the lepton family, which also includes electrons and their heavier counterparts, muons and taus. They come in three types, or "flavors": electron neutrinos, muon neutrinos, and tau neutrinos. Neutrinos are produced in a variety of processes, including nuclear fusion in stars, radioactive decay, and cosmic events like supernovae. Despite their abundance—trillions of them pass through our bodies every second—neutrinos are notoriously difficult to detect because they interact with matter only through the weak nuclear force. This weak interaction means that neutrinos can travel through light-years of material without being significantly affected, making them an intriguing candidate for communication over astronomical distances.
Communication Medium
The concept of using neutrinos for communication is rooted in their unique properties. Unlike electromagnetic signals, which can be absorbed or scattered by interstellar dust, gas, and cosmic radiation, neutrinos can pass through celestial bodies, including planets and stars. This characteristic makes them particularly appealing for sending messages across vast expanses of space, where traditional communication methods may falter. In theory, a civilization could send neutrino signals that are undetectable by conventional means, effectively hiding their communication from the noise of electromagnetic radiation that fills the universe.
Neutrinos could carry information regarding the sender's location, intentions, or even complex data encoded in specific patterns of neutrino emissions. This encoding is essential for any communication system, as it allows the recipient to interpret the information being sent. While the concept remains largely theoretical at this stage, it opens up exciting possibilities for interstellar communication.
Advantages of Neutrino Communication
Penetrative Ability: One of the most significant advantages of neutrinos is their ability to penetrate dense materials. Unlike photons, which can be absorbed or scattered by matter, neutrinos can travel through celestial bodies with ease. This means that a signal could potentially be sent from one star system to another, passing through intervening matter without loss of clarity.
Low Noise: Neutrinos interact so weakly with matter that background noise from other cosmic phenomena is minimized. This low noise environment can enhance the clarity of the signals, making it easier for recipients to distinguish between meaningful information and random fluctuations.
Universality: Since neutrinos are produced in a variety of astrophysical processes, they can be generated by numerous sources, including stars, supernovae, and artificial means. This universality allows for a wide range of potential communication scenarios, from natural signals emitted by stars to intentional messages sent by advanced civilizations.
Disadvantages of Neutrino Communication
Despite the advantages, there are considerable challenges associated with neutrino communication.
Detection Difficulty: Detecting neutrinos is a significant hurdle. Specialized detectors, such as large underground or underwater observatories, are necessary to capture and interpret neutrino signals. These detectors often require sophisticated technology and substantial resources, making it difficult to establish a reliable communication system.
Energy Requirements: Generating a sufficient flux of neutrinos for communication purposes requires immense energy. The energy needed to produce neutrinos on the scale required for interstellar communication may be beyond the capabilities of many civilizations. This limitation raises questions about the practicality of neutrino communication as a viable means of contact.
Signal Decay and Noise: While neutrinos are less susceptible to interference than electromagnetic signals, they are still subject to potential decay or scattering over long distances. Ensuring that signals remain intact and distinguishable over vast distances remains an unresolved challenge.
Future Perspectives
Research into neutrino communication is still in its infancy, but advancements in particle physics and detector technology could pave the way for practical applications in the future. As our understanding of neutrinos deepens, we may develop new methods for generating and detecting these elusive particles more efficiently. This progress could enhance our ability to use neutrinos for communication, potentially enabling contact with other civilizations or enhancing our understanding of the cosmos.
Moreover, interdisciplinary collaboration between physicists, engineers, and communication experts will be crucial in overcoming the existing challenges. By addressing the technical hurdles associated with neutrino generation and detection, we may unlock the potential for a new frontier in cosmic communication.
Conclusion
Neutrinos present a unique and compelling opportunity for communication across astronomical distances. Their weakly interacting nature allows them to traverse vast expanses of space, potentially enabling civilizations to send messages that remain undetectable by conventional means. While there are considerable challenges to overcome, including detection difficulties and energy requirements, the exploration of neutrino communication is a promising avenue for future research. As technology advances, the dream of communicating across the cosmos using neutrinos may one day become a reality, opening new doors to our understanding of the universe and our place within it.
Artist’s impression of a Dyson Sphere, a proposed alien megastructure that is the target of SETI surveys. Finding one of these qualifies in a “first contact” scenario.
Credit: Breakthrough Listen / Danielle Futselaar
2. Laser Communications: A Comprehensive Analysis
Description Lasers are remarkable devices capable of producing highly focused beams of light, which can efficiently carry information over extensive distances with minimal attenuation. This technology has revolutionized the way we communicate, akin to the ease and immediacy of texting in our contemporary world. The potential applications of lasers extend beyond terrestrial communication, as researchers and scientists have actively explored their utility for interstellar messaging. The ability to modulate laser beams enables the encoding of messages, transforming simple light into sophisticated communication channels that could one day bridge the vast expanses of space.
Communication Medium The essence of laser communication lies in the transmission of encoded light signals through the vacuum of space. These signals can be meticulously received by advanced optical telescopes or specialized detectors, either stationed on Earth or positioned on other celestial bodies. This method of communication harnesses the speed of light, facilitating the rapid transfer of information across astronomical distances. By using lasers, scientists aim to establish a communication framework that could potentially reach distant star systems, allowing for the exchange of messages with hypothetical extraterrestrial civilizations.
Advantages Laser communication presents several significant advantages that enhance its appeal as a medium for information transmission:
High Data Rate: One of the most compelling benefits of laser communication is its capability to transmit vast amounts of data at remarkable speeds. This high data rate makes it particularly suitable for conveying complex messages, which can be crucial in scenarios where detailed information is essential, such as scientific data or urgent communications.
Directional Beam: The inherently focused nature of laser beams enables targeted communication. This precision significantly reduces the likelihood of signal interference, especially from cosmic background noise. The ability to direct beams toward specific points in space enhances the clarity and integrity of the transmitted information, making laser communication a reliable option for long-distance transmissions.
Disadvantages Despite its many advantages, laser communication is not without its challenges:
Line of Sight: A critical limitation of laser signals is their dependence on a clear line of sight. The effectiveness of laser communication diminishes if there are obstacles obstructing the path between the transmitter and receiver. This requirement can complicate communication efforts, particularly in environments where physical barriers are prevalent.
Atmospheric Interference: When communicating from Earth, laser signals must traverse the atmosphere, which can introduce various forms of distortion or absorption. Atmospheric conditions, such as clouds, fog, or even pollution, can significantly complicate the efforts to maintain a stable communication link. This interference poses challenges for planetary communication, as it can distort the signals and hinder the clarity of the transmitted information.
Future Perspectives Looking ahead, the future of laser communication appears promising, especially with the continuous advancements in laser technologies and optical systems. As researchers refine these technologies, laser communication has the potential to evolve into a primary method for interstellar messaging. Future missions could leverage sophisticated laser systems to send out signals aimed at reaching potential extraterrestrial civilizations. The prospect of establishing communication with intelligent life beyond Earth is an exciting endeavor that could redefine our understanding of the universe.
In addition to interstellar applications, the advancements in laser communication could also enhance terrestrial communication systems. The integration of laser technology into existing networks could lead to faster and more efficient data transmission, benefiting various sectors, including telecommunications, space exploration, and scientific research. As the demand for high-speed data transfer continues to grow, laser communication stands poised to play a pivotal role in meeting these needs.
In conclusion, laser communication represents a groundbreaking advancement in the field of information transmission. Its ability to deliver high data rates through focused beams of light offers a unique solution for both terrestrial and potential interstellar messaging. While challenges such as line of sight and atmospheric interference remain, ongoing research and technological innovations hold the promise of overcoming these obstacles. As we continue to explore the possibilities of laser communication, we may one day be able to send and receive messages across the cosmos, enriching our understanding of the universe and our place within it.
3. Gravitational Waves
Description
Gravitational waves are perturbations in the fabric of spacetime, generated by the acceleration of massive celestial bodies. These phenomena are often produced during cataclysmic events such as the merging of black holes or neutron stars. When such massive objects collide, they create ripples that propagate outward at the speed of light. The study of gravitational waves has opened new avenues in astrophysics, allowing scientists to observe and understand events that are otherwise invisible to traditional telescopes. As research progresses, there is a growing interest in the potential of gravitational waves to serve as a medium for communication, suggesting a fascinating intersection between astrophysics and information technology.
Communication Medium
Gravitational waves have the unique ability to carry detailed information about their origins. Each wave contains a signature that reflects the dynamics of the astronomical event that created it. This characteristic raises the possibility of manipulating gravitational waves to encode messages. By varying the waveforms or frequencies of the waves, one could theoretically transmit information across vast distances. This concept aligns with the fundamental principles of wave mechanics, where information can be encoded in various parameters of a wave, such as its amplitude, frequency, or phase.
Advantages
Universality: One of the most significant advantages of using gravitational waves as a communication medium is their ability to traverse any medium without attenuation. Unlike electromagnetic waves, which can be absorbed or scattered by matter, gravitational waves are fundamentally different in that they interact very weakly with the material universe. This means that they can propagate through the cosmos unimpeded, allowing for potential communication across immense distances, even between galaxies.
Low Background Noise: The detection of gravitational waves is less susceptible to interference from electromagnetic noise, which can often obscure signals in traditional communication methods. For example, radio waves can be drowned out by background radiation from various sources, including cosmic rays and man-made signals. Gravitational waves, however, are less affected by these disturbances, making them a clearer medium for communication in certain contexts. This characteristic could provide a more reliable means of transmitting information, especially in environments with high electromagnetic interference.
Disadvantages
Detection Challenges: Despite the intriguing potential of gravitational waves for communication, the technology required to detect these waves is currently highly specialized and complex. Instruments like the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo are designed to measure the minuscule distortions in spacetime caused by passing gravitational waves. These facilities rely on advanced technology, including extremely precise lasers and vacuum systems, which limits their accessibility and practicality for widespread application. As a result, the ability to detect and utilize gravitational waves for communication remains a significant challenge.
Energy Requirements: Another substantial barrier to the practical use of gravitational waves for communication is the immense energy required to generate detectable signals. The events that produce significant gravitational waves, such as the merger of black holes, involve massive amounts of energy, far beyond what can be harnessed by most civilizations. This limitation raises questions about the feasibility of creating artificial gravitational waves for communication, as only highly advanced technological societies might possess the capability to generate such energy levels.
Future Perspectives
Looking ahead, the field of gravitational wave astronomy is poised for significant advancements. As technology continues to evolve, researchers are actively exploring innovative methods to utilize gravitational waves for communication. The development of more sensitive detectors is a key area of focus. Future instruments may enhance our ability to detect weaker gravitational waves, opening up new possibilities for their application beyond traditional astrophysics.
Furthermore, interdisciplinary collaboration between physicists, engineers, and communication specialists could lead to novel approaches for encoding and transmitting information through gravitational waves. As our understanding of these phenomena deepens, the potential to harness gravitational waves as a communication medium may become more feasible.
In conclusion, while gravitational waves present both compelling advantages and formidable challenges as a medium for communication, ongoing research and technological advancements may one day unlock their potential. As we continue to explore the universe and the fundamental laws governing it, the idea of communicating through gravitational waves remains an exciting and thought-provoking possibility that could reshape our understanding of information transmission across the cosmos.
4. Radio Waves
Description
Radio waves are an established medium for communication, extensively utilized across the globe for various forms of broadcasting. Their unique properties make them an essential component of modern communication technologies. Notably, radio waves have been harnessed in the quest for extraterrestrial signals, exemplified by initiatives such as the Search for Extraterrestrial Intelligence (SETI). This ongoing exploration underscores the importance of radio waves not only in terrestrial applications but also in the broader context of interstellar communication.
Communication Medium
One of the most significant characteristics of radio waves is their ability to be transmitted over long distances. This capability allows for the transmission of information encoded within their frequencies and amplitudes. The modulation of these properties enables radio waves to carry complex data, making them versatile for various communication needs. For instance, in terrestrial applications, radio waves are used for broadcasting television, radio shows, and even for wireless internet signals. In the context of space exploration, they serve as a vital link for communicating with spacecraft and satellites, enabling data exchange and command transmission over vast distances.
Advantages
The advantages of using radio waves as a communication medium are numerous.
Established Technology: Radio communication is a well-understood and mature technology with a long history of successful implementation. From its inception in the late 19th century to its current applications, radio communication has proven its reliability and effectiveness in both terrestrial and extraterrestrial contexts.
Wide Range: Another significant advantage is the ability of radio signals to travel vast distances. They can penetrate various cosmic materials, such as dust and gas in space, making them an ideal choice for interstellar communication. This characteristic is particularly valuable when attempting to communicate across the immense distances that separate celestial bodies.
Disadvantages
Despite the advantages, there are notable disadvantages associated with the use of radio waves for communication.
Signal Degradation: One of the primary challenges is signal degradation. Over long distances, radio signals can weaken significantly. Various cosmic phenomena, such as solar flares or cosmic background radiation, can introduce interference that degrades the integrity of messages being transmitted. This degradation poses challenges for maintaining clear communication.
Signal Detection: Another critical disadvantage is the difficulty in signal detection. The vastness of space means that distinguishing genuine signals from background noise can be a formidable task. This challenge is especially pronounced in the search for extraterrestrial signals, where the faintness of potential signals can be easily lost amidst the cosmic cacophony of noise.
Future Perspectives
Looking ahead, the future of radio wave technology holds promising developments that could enhance our ability to detect and utilize extraterrestrial radio signals. Continuous advancements in radio technology and techniques are being pursued, including the development of phased array systems and sophisticated algorithms for signal processing.
Phased array systems, for instance, allow for the rapid scanning of the sky without the need to physically move antennas. This technology could significantly improve the efficiency of searches for extraterrestrial signals by enabling the simultaneous monitoring of multiple frequencies and areas of the sky. Additionally, advanced signal processing algorithms can help filter out background noise and enhance the detection of faint signals, improving the likelihood of discovering meaningful communications from other civilizations.
Moreover, future missions may leverage radio waves for targeted communication efforts. As our understanding of the cosmos deepens, missions could be designed to send intentional signals to specific star systems that are deemed most likely to harbor intelligent life. This proactive approach, combined with enhanced detection capabilities, could usher in a new era of interstellar communication.
In summary, radio waves remain a cornerstone of communication, with well-established applications on Earth and promising potential in the search for extraterrestrial life. While challenges such as signal degradation and detection difficulties exist, ongoing advancements in technology and methodologies are paving the way for improved communication capabilities. As we continue to explore the cosmos, radio waves will undoubtedly play a crucial role in our quest to connect with potential extraterrestrial civilizations. The future holds exciting possibilities as we strive to unlock the mysteries of the universe, utilizing radio waves as a bridge to the stars.
5. Quantum Codes
Description
Quantum communication is a cutting-edge method that utilizes the principles of quantum mechanics, specifically quantum entanglement, to enable the secure and instantaneous transmission of information over considerable distances. This innovative approach is regarded as the most advanced form of communication available today. The unique characteristics of quantum mechanics, such as the peculiar behavior of particles at the quantum level, allow for a level of security and speed in information exchange that classical communication methods cannot achieve.
Communication Medium
Quantum codes serve as the backbone for creating secure communication channels. These channels leverage quantum properties to ensure that any attempt by eavesdroppers to intercept messages is detected. Essentially, the fundamental principles of quantum mechanics guarantee that any observation or interaction with the quantum state of the system will alter the information being transmitted. Consequently, this makes it theoretically impossible for unauthorized parties to access the transmitted data without leaving a trace. This level of security is a significant advancement over classical encryption methods, which can be vulnerable to sophisticated hacking techniques.
Advantages
Security: One of the most compelling advantages of quantum communication is its inherent security. Due to the nature of quantum states, any attempt to observe or interfere with the transmission alters the state itself, thereby alerting the communicating parties to potential eavesdropping. This provides a robust defense against unauthorized access and ensures the confidentiality of the information being exchanged.
Speed: Quantum entanglement presents a fascinating opportunity for instantaneous communication across vast distances. This phenomenon challenges traditional notions of information transfer limits, suggesting that it may be possible to convey information almost instantaneously, regardless of the distance separating the sender and receiver. Such a breakthrough could revolutionize not only communication technology but also various fields reliant on rapid data transfer.
Disadvantages
Technological Limitations:Despite its potential, quantum communication faces significant technological hurdles. The current methods for generating and maintaining entangled states are still in their infancy and often require complex setups that are difficult to implement on a large scale. As a result, practical applications of quantum communication remain limited at this stage, hindering its widespread adoption.
Scalability: Another key challenge is the scalability of quantum communication networks. The fragility of quantum states makes it difficult to establish robust networks that can operate efficiently across extensive geographic areas. Developing infrastructure that can consistently maintain entangled states over long distances is a substantial challenge that researchers and engineers must overcome to realize the full potential of quantum communication.
Future Perspectives
Looking ahead, as advancements in quantum technology continue to progress, the potential for quantum communication to facilitate contact with extraterrestrial civilizations becomes increasingly tantalizing. The unique properties of quantum communication may enable the transmission of messages across interstellar distances, providing a new avenue for exploring the cosmos and potentially establishing communication with intelligent life beyond our planet. Research in this field could lead to groundbreaking discoveries and innovations that make quantum communication not only feasible but also practical for interstellar messaging.
In addition to interstellar communication, the future development of quantum networks may lead to significant benefits for various sectors, including secure data transmission for financial institutions, enhanced cybersecurity measures, and improved communication systems for governmental and military applications. As the technology matures and becomes more accessible, we can anticipate a paradigm shift in how information is transmitted globally, transcending the limitations imposed by classical communication methods.
Moreover, with ongoing research and investment in quantum technologies, there is the potential for collaborative efforts between nations and private enterprises to create a standardized framework for quantum communication. This could foster an international quantum communication infrastructure that enhances global connectivity and security.
In conclusion, quantum codes represent a revolutionary approach to communication that harnesses the principles of quantum mechanics to provide unparalleled security and speed. While challenges remain in terms of technology and scalability, the future of quantum communication holds immense promise. As the field evolves, it could not only transform our understanding of communication but also open new frontiers in our quest for knowledge and interaction with the universe beyond our own. The ongoing exploration of quantum communication may well lead to unforeseen applications and opportunities that could reshape the fabric of human interaction in the years to come.
Conclusion
The exploration of potential communication methods from extraterrestrial civilizations reveals a diverse array of possibilities, each with its unique advantages and challenges. As technology continues to evolve, the feasibility of these communication mediums will be tested in our ongoing search for extraterrestrial intelligence. Future advancements in detection, transmission, and signal processing will be crucial in enhancing our capabilities to communicate with civilizations beyond our planet.
In addition to radio waves and light signals, other forms of communication may exist that transcend our current understanding. For instance, some researchers speculate on the potential of using gravitational waves as a means of communication. Gravitational waves, ripples in spacetime caused by massive celestial events like merging black holes, could theoretically carry information across vast distances. While this concept is still largely theoretical, it highlights the diversity of potential communication forms that could exist in the universe.
Another intriguing possibility is the use of quantum communication. Quantum entanglement allows particles to be interconnected in such a way that the state of one can instantaneously influence the state of another, regardless of distance. If extraterrestrial civilizations have mastered quantum communication, they could send messages that are impervious to interception or eavesdropping, vastly improving the security of their communications. However, such methods would require a deep understanding of quantum mechanics and advanced technology, which may or may not align with the capabilities of other civilizations.
Moreover, visual communication methods, such as lasers or even complex patterns of light modulation, can also be considered. The use of lasers has been proposed as a means of signaling across interstellar distances. This method could involve sending modulated pulses of light that convey information, similar to how we use fiber optics on Earth. The challenge with such methods lies in accurately targeting distant stars and the need for powerful enough lasers to ensure the message reaches its destination without significant loss of intensity.
When discussing the question of whether aliens have tried to contact us, it is essential to consider the vastness of the universe and the time scales involved. The Fermi Paradox raises the question of why, given the high probability of life elsewhere in the universe, we have yet to encounter any definitive evidence of extraterrestrial intelligence. Some theorists argue that advanced civilizations may adopt a policy of non-interference, choosing not to communicate with less developed species, akin to the Prime Directive in science fiction narratives. This perspective suggests that any attempts at communication may go unnoticed or misinterpreted by humanity.
On the other hand, several scientific initiatives have been established to actively search for extraterrestrial signals. Projects like the Search for Extraterrestrial Intelligence (SETI) use radio telescopes to scan the cosmos for signs of intelligent life. So far, while many signals have been detected, none have been conclusively identified as artificial or originating from extraterrestrial sources. This ongoing search emphasizes both the optimism and the challenges we face in our quest for contact.
Additionally, the discovery of exoplanets in the habitable zone of their stars has expanded our understanding of where life might exist. Future missions to these planets could provide invaluable insights into their atmospheres and potential signals, further enhancing our chances of making contact. The recent advancements in astrobiology, combined with technological innovations in communication and detection, increase the likelihood that we may one day receive a message from beyond our world.
In conclusion, the quest for communication with extraterrestrial civilizations encompasses a wide range of methods, each with its own set of challenges and potential. The evolution of our technology and understanding of physics may eventually allow us to bridge the vast distances between stars and engage in meaningful dialogue with other intelligent beings. While the question of whether aliens have already attempted to contact us remains unanswered, the ongoing search fuels our curiosity and drives scientific inquiry, reminding us of our place in the cosmos and the possibility of connection beyond our own world. As we continue to explore and innovate, the dream of interstellar communication may one day become a reality, opening new avenues of understanding and collaboration across the universe.
Exploring the Moon with Biologically-Inspired Subsurface Robots
Exploring the Moon with Biologically-Inspired Subsurface Robots
By Matthew Williams
Thanks to the Apollo missions and countless robotic explorers, our understanding of the physical conditions, composition, and geological history of the Moon has advanced considerably. For example, analysis of lunar rocks, regolith, and seismic measurements of the Moon's interior structure led to the theory that the Earth and Moon formed roughly 4.5 billion years ago. Since the turn of the century, missions have also revealed that there is water on the Moon, most of which consists of ice in Permanently Shadowed Regions (PSRs) around the poles.
To learn more about the Moon and ensure long-term habitability, missions that can explore the subsurface are needed. That is the recommendation a team of researchers made in a recent study, which explores the possibility of using a robot—Persistent Lunar Exploration with Autonomous SubsurfacE Robots (PLEASER)—to accomplish these tasks. These missions would be able to explore one of the most promising environments for future lunar bases and habitats while also revealing more about the Moon's formation, evolution, and properties.
Subsurface lava tubes and recesses on the Moon have become a major focal point in recent years. Based on data obtained by multiple orbiters, landers, and rovers, scientists have learned that these features—common to Earth—are significantly larger on the Moon. On Earth, lava tubes do not exceed 30 meters (100 ft) in diameter. But owing to the Moon's lower gravity, scientists have estimated that these features could measure 385 m (1,260 ft) or more in diameter.
Like lava tubes on Earth, some lunar tubes are accessible thanks to collapsed sections known as "skylights." As part of their long-term visions for lunar exploration and development, NASA and other space agencies (notably China) are considering establishing habitats in these tubes to take advantage of the protection they offer. These include warmer temperatures (~20° C, 70° F) and natural shielding from extreme temperature variations, the vacuum of space, and micrometeoroids.
To accomplish this and learn more about the Moon's properties, composition, and geological history, NASA and other space agencies need dedicated missions to explore these features. As Long-Fox told Universe Today via email, their concept for a subsurface robot would enable all of this by being able to interact with both the surface and subsurface regolith directly:
"Just like on Earth, the different layers (stratigraphy) tell the history of the area you are in. On the Moon, there is no wind or flowing water, so the main processes that shape the surface are impacts. The impacts, big or small, eject regolith and rocks that get thrown elsewhere on the surface. This means that there will be different layers deposited from different impacts, and understanding this evolution of the surface will really help us understand the history and current state of the Moon."
As part of their study, the team explored multiple methods for powering the robots, design considerations, and the potential applications and benefits this mission could have. The result was their PLEASER concept, which calls for a deployable/retractable regolith probe within a snake-like robot. The snake configuration would allow PLEASER to penetrate the surrounding lunar regolith to measure its strength, thermal conductivity, and dielectric properties. It could also burrow into the surface or slither its way into skylights, seeking out subsurface structures for further investigation. As Long-Fox further explained:
"This robot would the physical state of the regolith, informing not only on geologic history but also the presence of volatiles such as water ice or the suitability of the area being explored for infrastructure development like habitats, roadways, launch/landing pads, and more. Just by the nature of the robot traversing in the subsurface, it will need to displace the regolith around it. We envision doing this with a scooping system, and by measuring forces it takes to scoop the regolith as well as resistance to the serpentine motion of the robot, we can estimate critical properties of the surface and subsurface regolith.
In terms of power, the team considered multiple options, including external power, a cable connected to a power source, a Radioisotope Thermoelectric Generator (RTG),and solar panels. One design they considered featured solar panels embedded along the snake-like body (see above image) that could be deployed and retracted. As Stoica indicated:
"Solar panels that are folded inside the body and deploy outside of the body when the robot comes to the surface to 'bathe in the Sun,' so to speak, to get energy. We mostly considered a fusiform body snake/worm shape. Others have done studies of sand snake movements - I am aware of some universities that produce some nice simulations and demos for earth conditions - in sandy soil."
The team hopes their study will help produce concepts for a mobile platform that can directly explore the lunar surface and subsurface, regardless of whether it is lunar day or night. Robots of this nature will also be able to search for subsurface areas more suitable for developing a lunar base, road, or other infrastructure elements. As noted, the scientific returns are also promising, as subsurface robots would create unprecedented opportunities for exploring the Moon's geology.
In addition to studying lunar regolith and rocks in situ, this robot could deploy subsurface sensors like seismometers. Not only would these reveal more about the Moon's interior structure, but they are notoriously difficult to deploy on the surface. Lastly, as Stoica added, these robots may someday be able to create subsurface tunnels that could house lunar habitats:
"[A]fter the initial stages, once routes/tunnels (for fun, I would just call them 'artificial/fake lava tubes'), other equipment would be more like surface robots. So, in this respect, these may be like the machines that build underground tunnels (drilling, burrowing) but perhaps more in the formation of teams/swarms rather than a big machine. This is pure speculation at this point, no tradeoffs were made, and how many exactly and how big is undetermined. Though I have looked at swarms in my life, I am very cautious when it comes to throwing words like swarms, etc., in terms of operational space robotics in the next 1-2 decades, while the concept we refer to may only be a few years ahead."
The colors of the arrows represent the direction of motion. Relative to the LMC, located at the bottom left of the image, most red arrows show movement towards the LMC, whereas most light blue arrows show movement away from the LMC, suggesting they are being pulled apart. Credit Credit: Satoya Nakano
The Magellanic Clouds are two irregular dwarf galaxies visible from the Southern Hemisphere that orbit our own Milky Way Galaxy. Named after the explorer Ferdinand Magellan who documented them during his voyage in the 16th century, they consist of the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC). Located approximately 160,000 and 200,000 light-years away respectively, these satellite galaxies are rich in gas and young stars. The Magellanic Clouds are connected by a stream of gas called the Magellanic Bridge and are slowly being torn apart by tidal forces from our galaxy, with the material forming the trailing Magellanic Stream that extends across much of our southern sky.
The Large and Small Magellanic Clouds
( Credit : ESO/S. Brunier)
A team of researchers at Nagoya University have discovered evidence that the SMC is potentially being torn apart by gravitational forces from its larger companion, the LMC. Led by Satoya Nakano and Kengo Tachihara, the team identified unexpected patterns in the movement of massive stars within the SMC, revealing dynamics that could significantly alter our understanding of how galaxies interact and evolve. The findings, published in The Astrophysical Journal Supplement Series, initially seemed so surprising that the team questioned their analytical methods, but further investigation confirmed the validity of their results.
The team were able to track and study about 7,000 massive stars within the SM. These stars (each over eight times our Sun's mass and markers for hydrogen-rich regions) were observed moving in opposite directions across the galaxy. Some approach the nearby LMC while others recede from it, indicating the SMC is being gravitationally pulled apart by its larger companion. This discovery provides compelling evidence of an ongoing galactic disruption that may eventually lead to the SMC's destruction.
The Smalll Magellanic Cloud
(Credit : ESA Hubble)
Anoter key discovery from the research was the unexpected lack of rotational movement among the SMC's massive stars, contrasting with galaxies like our Milky Way where stars and gas rotate together. Typically, young massive stars move in tandem with their birth gas clouds before decoupling, but the SMC's stars show no rotational pattern, suggesting the gas itself isn't rotating! Nakano noted this may necessitate revising calculations of the SMC's mass and its interactions with the LMC and the Milky Way, potentially transforming our understanding of the complex three-body gravitational relationship among these galaxies.”
The study offers valuable insights into how galaxies interact and evolve, especially in the early epochs of the Universe. The SMC, with its similarities to primordial galaxies, serves as key for understanding galaxy formation. Observing stellar motion in the SMC and LMC, helps researchers connect star formation with galactic dynamics, potentially reshaping our understanding of the Cosmos
The surface of Mars looks like an empty red wasteland. But if you look a bit closer, the remnants of an ancient alien civilization begin to take shape.
At least, that's the conclusion of George J. Haas, the founder and premier investigator of the Mars research group known as The Cydonia Institute.
In his new book, 'The Great Architects of Mars,' Haas analyzed dozens of photos of structures on the Martian surface that he is sure are man-made.
Those include pyramids, a keyhole-shaped formation and even one that looks like a parrot.
According to the author, these formations may be the remnants of once-magnificent cities, towering pyramids, gigantic geoglyphs and more.
Geometry, Haas said, is the marker of civilization. He has spent more than 30 years meticulously studying NASAimages of the Martian surface to look for geometric features and patterns that can't be explained by nature alone.
As a formally trained artist, Haas has an eye for deciphering the subtle differences between a natural formation and an object that was intentionally crafted.
'You don't have to be a geologist to know the difference between a rock and a sculpture — something that's geometric,' he told DailyMail.com.
The 'keyhole' structure on the surface of Mars consists of two main parts: a wedge-shaped formation and an attached circular dome
However, scientists have said Haas' claims are a result of 'pareidolia,' a common brain phenomenon in which a person sees faces in random images or patterns.
'Sometimes we see faces that aren't really there,' explained Robin Kramer, Senior Lecturer in the School of Psychology, at University of Lincoln, in an article for The Conversation.
'You may be looking at the front of a car or a burnt piece of toast when you notice a face-like pattern.
'This is called face pareidolia and is a mistake made by the brain's face detection system.'
Even so, Haas is sure that the structures in the images prove there is life on Mars.
1. The keyhole
In 2011, NASA's Mars Reconnaissance Orbiter (MRO) spacecraft snapped a photo of a bizarre formation on the surface of Libya Montes, an area of high-elevation on Mars.
The raised structure consists of two main parts: a wedge-shaped formation and an attached circular dome. Together, they resemble an enormous exclamation mark.
The Mars keyhole structure bears resemblance to the Kofun Tomb in Japan (pictured)
'Traditionally, the basic shape of a conjoined wedge and dome formation are commonly referred to as a keyhole,' Haas wrote.
In 2013, the 'exquisite' geometry of this strange landform captured his attention.
Three years later, Haas and several colleagues published a formal analysis of the keyhole in the Journal of Space Exploration, concluding that its geometry and symmetry suggest it could have been intelligently built.
Without considering that possibility, 'there's no way you can explain that keyhole formation,' Haas said.
'While there are known geological mechanisms that are capable of creating and destroying the individual angles and planes presented in this formation, the natural creation of two opposing geometrically designed formations seems to go well beyond the probability of chance,' the author explained.
Haas also pointed out the keyhole's similarity to monuments constructed by New World, Middle Eastern, and Japanese cultures, such as the Kofun Tomb in Japan.
2. Parrot geoglyph
The parrot geoglyph has 22 points of anatomical correctness, according to Haas
A sketch of the parrot geoglyphs' shape
In 2002, independent researcher Wilmer Faust noticed an odd shape captured in a Mars Global Surveyor image of the large-impact crater known as Argyre Basin.
He showed the image to Haas and his colleagues at The Cydonia Institute, highlighting features throughout the area's topography that looked like a head with an eye and beak, a mound-shaped body, a leg and foot, and an extended wing with feathers.
In his new book, 'The Great Architects of Mars,' George J. Haas analyzed dozens of photos of structures on the Martian surface that appear to be man-made
'After seeing the image, I immediately saw the parrot formation,' Haas noted.
This bizarre structure has since become known as the 'parrot geoglyph,' or 'Parrotopia.'
A geoglyph is a large design or image made on the ground using stones, gravel, mounds of earth or other natural objects.
The human brain tends to look for familiar patterns in abstract shapes, like when you see a face in the clouds. But the parrot geoglyph is different.
'[Cloud shapes] are usually just silhouettes,' Haas explained. 'They don't have a lot of secondary or tertiary detail. There's no eyes, there's no irises, there's no eyelids, there's no eyebrows... That's what we have with the parrot.'
'It's got 22 points of anatomical correctness... It's a sculpture, it's a work of art,' Haas contended. Five different veterinarians, including an avian specialist, confirmed the lifelike anatomy of this Martian structure, the author added.
Geoglyphs can be found in many different locations on Earth, such as Peru, Israel, England, Australia, and even in the US.
However, Haas wrote that there are no geoglyphs anywhere on Earth which match the fine detail of the parrot on Mars.
3. The Sagan pyramids
The Sagan pyramids are three-sided pyramids located on Mars that caught the attention of famed astronomer Carl Sagan in the 1970s
While gathering information about Mars' atmosphere and mapping the planet's surface in 1972, NASA's Mariner 9 spacecraft captured an image of anomalous formations in the Elysium area — the second largest volcanic region on the planet.
These triangular, three-sided pyramids stood out amid steep-sided volcanic cones and impact craters. At an average height of more than 3,200 feet and a width of nearly 10,000 feet, they would dwarf even the largest pyramids on Earth.
George J. Haas is the founder and premier investigator of the Mars research group known as The Cydonia Institute, and the author of 'The Great Architects of Mars'
The pyramids caught the attention of renowned astronomer Carl Sagan, who speculated that they might have been made by high winds and harsh sand blasting large mounds of rock and dirt into pyramid shapes.
But even the late astronomer acknowledged that scientists would need to observe these formations up close to actually determine what they are and how they were made.
While Haas does not rule out Sagan's explanation, he thinks it's possible that these pyramids were built by intelligent beings, and notes that there is some evidence to suggest this region of Mars could have supported ancient life.
'Recent data suggests that volcanic activity may have occurred as recently as 53,000 years ago, creating an environment that was suitable for supporting life,' Haas said. 'Water had also left its mark on the region in the form of riverbeds and canyons.'
What's more, Haas argued that natural pyramid formations tend to be cone-shaped and lack similarly-sized faces.
And while three-sided pyramids are very rare on Earth, they do exist. One of them lies just 65 miles north of Las Vegas, Nevada in the top secret military base known as Area 51. This pyramid is part of the Big Explosives Experimental Facility at the Nevada National Security Site.
'I believe it is fair to say that this triangular formation looks a lot like the three-sided pyramid that Sagan saw in the original Mariner 9 images,' Haas noted.
4. The Martian Atlantis Complex
A detailed view of the Martian Atlantis Complex
The Martian Atlantis Complex resembles the city of Al-Ula in Saudi Arabia (pictured)
The Atlantis Chaos region of Mars, located in the planet's southern hemisphere, is characterized by areas of blocky, steep-sided mesas interspersed with deep valleys.
Scientists generally believe this terrain resulted from the slow erosion of a once-continuous solid plateau, according to the European Space Agency (ESA).
But in 2019, Greg Orme of the Society for Planetary SETI Research pointed out that part of the Atlantis Chaos region captured in a NASA image contained the remains of a 'tightly-knit grid of cellular formations.'
Then, independent researcher Javed Raza took a closer look at the image and began highlighting linear formations that appeared to be part of a 'massive city-like complex.'
'Raza suggested that the arrangements of these evenly spaced foundations with broken walls and towers are typical of the kind of remains one would see in built-up areas on Earth,' Haas wrote.
Further analysis revealed that the entire 'city complex' can be divided into two distinct 'twin' cities, one Eastern and the other Western.
The cubic grid design of the Eastern City resembles the remains of mudbrick and stone adobe houses built throughout the midwestern US and at Al-Ula in Saudi Arabia — a once-bustling city that became largely unoccupied in the 1980s.
The Western City also shares similarities with another terrestrial metropolis: Berlin. Specifically, a small section of this Martian terrain resembles a bombed-out area of the German city during World War II.
5. The starburst structure
The starburst structure on the surface of Mars
The starburst structure is roughly the same shape as Fort Henry in Tennessee (pictured)
While studying ESA images of the Nepenthes Mensae region of Mars, a rugged, flat-topped plateau in the planet's eastern hemisphere, an odd-shaped formation caught Haas' eye.
The raised patch of land resembled an irregular star shape 'with five radiating arms that stretch out like a giant starfish.'
'There is a large mound positioned at its northernmost point and three smaller mounds of various sizes located at its center. The formation projects so much energy in its shape and design that I have titled it Starburst,' Haas said.
The author believes the Starburst bears strong resemblance to a star fort with triangular bastions at each corner, which were commonly found in Europe in the 16th and 17th centuries, and in America during colonization and the Civil War period.
'Many of these star-shaped fortifications included interior buildings and had raised platforms within their main structure allowing military fire over the main ramparts,' he explained.
The Starburst looks especially similar to Fort Henry, which was built on the eastern bank of the Tennessee River in 1861 to defend the river and the critical railroad route between Bowling Green, Kentucky, and Memphis, Tennessee.
'When Fort Henry is compared to the Starburst structure found on Mars their common polygonal star design is remarkably similar,' Haas continued.
'Notice the various sizes and shapes of the extending bastions of Fort Henry and its truncated star point at the tip. It is this truncated section of Fort Henry that looks very similar to the blunted star point observed on the Starburst structure on Mars.'
Uncovering a lost alien civilization
Haas' work raises intriguing questions about how certain structures on the Martian surface came to be.
But in order to confirm his theory that these formations are the remnants of an ancient alien civilization, scientists would need to take a much closer look.
Although humans have never stepped foot on the Red Planet before, that could become a reality within the next decade.
'Elon [Musk] wants to go there next year,' Haas said. Indeed, the SpaceX Chief Executive has set an ambitious goal of launching the first uncrewed Starship mission to Mars in 2026, and hopes to send astronauts there by 2029.
Haas hopes that once humanity establishes a presence on the Red Planet, scientists can actually begin investigating some of these unusual structures to learn how they formed — or were built.
'Mars is just going to be a treasure trove of technology and all kinds of information,' he told DailyMail.com.
Although these changes might be small on the planetary scale, scientists warn they could cause havoc for satellite navigation.
As the Earth turns on its axis, changes in the oceans, atmosphere, and deep within the molten mantle cause the planet to wobble like a spinning top.
While most of the planet's wobbles are regular and predictable, scientists from ETH Zurich have found that human-caused changes will soon outweigh the natural shifts.
Since satellites and deep space telescopes work out their position by referring to the Earth's axis of rotation, any change in the North Pole could cause serious issues.
Lead author Dr Mostafa Kiani Shahvandi, now at the University of Vienna, told MailOnline this could cause inaccuracies 'from a few metres to hundreds of metres'.
Earth's North Pole is on the move and could shift by as much as 90 feet (27 metres) by 2100, according to scientists
Like anything spinning on its axis, big changes in the Earth's distribution of mass cause it to shift on its axis.
Most of the time this is a normal and predictable process caused by factors such as regular cycles of ocean currents.
However, as the planet's ice sheets and glaciers melt, this is causing a more rapid redistribution of weight than scientists have observed in the past, which is causing the pole to shift.
Dr Shahvandi and his co-author measured the movement of the poles between 1908 and 2000 and compared this with projections of ice melt to see how far they might move in the future.
In the worst-case scenario, in which greenhouse gas emissions are not reduced, the dramatic melting of the ice sheets will have moved the poles 89 feet between 1900 and 2100.
In a more optimistic scenario in which greenhouse gas emissions are reduced, the North Pole will still move as much as 39 feet (12 metres).
For now, human-caused effects aren't moving the poles as much as natural causes.
As the ice caps melt in the warming climate, Earth's weight is redistributed around the planet. Like a spinning top, this shift alters the axis about which the Earth spins and moves the geographical North Pole
In the worst-case scenario (red) climate change could trigger the pole to move 89 feet between 1900 and 2100. In a more optimistic scenario (green) in which greenhouse gas emissions are reduced, the North Pole will still move as much as 39 feet (12 metres)
During the ice age, the Earth's crust sunk down under the weight of glaciers and has risen up since they melted, redistributing the planet’s weight.
Even though the last ice age ended over 10,000 years ago, the rebound effects can still be seen in the natural shift of the North Pole.
However, in the near future the scientists say that human-caused climate change will overtake the ice age rebound as the biggest contributor.
Dr Shahvandi says: 'Currently, the natural processes dominate polar motion, but if climate change continues and ice sheets melt more and more, then in the last decades of the 21st century the human-induced climate change will certainly dominate.'
Arctic sea ice covered an area six per cent smaller than average, marking the fourth month in a row when sea ice extents have seen record-breaking lows.
Likewise, Antarctic sea ice hit its fourth lowest monthly extent for March, standing 24 per cent lower than average.
The biggest contributors to the shift were the Antarctic ice sheet and the Greenland Ice Sheet (pictured) which is melting at an accelerating rate
This graph shows how much the melting of the Greenland Ice Sheet could shift the pole on the X (top) and Y (bottom) axes by 2100. The red line shows the worst-case scenario in which emissions do not reduce and the blue line shows the more optimistic scenario
This could cause serious problems for satellite navigation and for space-based telescopes like the James Webb Space Telescope (pictured) which use the Earth's axis as a reference point for navigation. This could cause errors on the scale of kilometres
The researchers discovered that the biggest sources of polar shift are the melting of the Greenland Ice sheet and the Antarctic Ice sheet.
If this change continues, it is likely to cause issues for the sensitive navigation systems of satellites and space telescopes such as the James Webb Space Telescope.
In their paper, published in the journal Geophysical Research Letters, the researchers write: 'Since prediction of polar motion is crucial for applications such as spacecraft navigation and orientation of deep-space telescopes, the reduced predictability of polar motion under climate change might impact the operational accuracy of such applications.'
That would be bad for navigation systems here on Earth but even more perilous for spacecraft since it will become harder to work out their exact location.
Dr Shahvandi says this could create errors of 'kilometres' for spacecraft probing distant planets.
Global sea levels could rise as much as 1.2 metres (4 feet) by 2300 even if we meet the 2015 Paris climate goals, scientists have warned.
The long-term change will be driven by a thaw of ice from Greenland to Antarctica that is set to re-draw global coastlines.
Sea level rise threatens cities from Shanghai to London, to low-lying swathes of Florida or Bangladesh, and to entire nations such as the Maldives.
It is vital that we curb emissions as soon as possible to avoid an even greater rise, a German-led team of researchers said in a new report.
By 2300, the report projected that sea levels would gain by 0.7-1.2 metres, even if almost 200 nations fully meet goals under the 2015 Paris Agreement.
Targets set by the accords include cutting greenhouse gas emissions to net zero in the second half of this century.
Ocean levels will rise inexorably because heat-trapping industrial gases already emitted will linger in the atmosphere, melting more ice, it said.
In addition, water naturally expands as it warms above four degrees Celsius (39.2°F).
Every five years of delay beyond 2020 in peaking global emissions would mean an extra 8 inches (20 centimetres) of sea level rise by 2300.
'Sea level is often communicated as a really slow process that you can't do much about ... but the next 30 years really matter,' said lead author Dr Matthias Mengel, of the Potsdam Institute for Climate Impact Research, in Potsdam, Germany.
None of the nearly 200 governments to sign the Paris Accords are on track to meet its pledges.
Beste bezoeker, Heb je zelf al ooit een vreemde waarneming gedaan, laat dit dan even weten via email aan Frederick Delaere opwww.ufomeldpunt.be. Deze onderzoekers behandelen jouw melding in volledige anonimiteit en met alle respect voor jouw privacy. Ze zijn kritisch, objectief maar open minded aangelegd en zullen jou steeds een verklaring geven voor jouw waarneming! DUS AARZEL NIET, ALS JE EEN ANTWOORD OP JOUW VRAGEN WENST, CONTACTEER FREDERICK. BIJ VOORBAAT DANK...
Druk op onderstaande knop om je bestand , jouw artikel naar mij te verzenden. INDIEN HET DE MOEITE WAARD IS, PLAATS IK HET OP DE BLOG ONDER DIVERSEN MET JOUW NAAM...
Druk op onderstaande knop om een berichtje achter te laten in mijn gastenboek
Alvast bedankt voor al jouw bezoekjes en jouw reacties. Nog een prettige dag verder!!!
Over mijzelf
Ik ben Pieter, en gebruik soms ook wel de schuilnaam Peter2011.
Ik ben een man en woon in Linter (België) en mijn beroep is Ik ben op rust..
Ik ben geboren op 18/10/1950 en ben nu dus 75 jaar jong.
Mijn hobby's zijn: Ufologie en andere esoterische onderwerpen.
Op deze blog vind je onder artikels, werk van mezelf. Mijn dank gaat ook naar André, Ingrid, Oliver, Paul, Vincent, Georges Filer en MUFON voor de bijdragen voor de verschillende categorieën...
Veel leesplezier en geef je mening over deze blog.