This allows accurate an unambiguous identification (red circle) of counterparts in complementary data at many other wavelengths: including (from top to bottom) optical images from the Subaru 8m telescope, Spitzer Space Telescope mid-infrared images at 24 and 3.6 microns, and VLA radio maps. A team of Canadian astronomers, including experts from the Dunlap Institute for Astronomy & Astrophysics in the University of Toronto's Faculty of Arts & Science, have used the James Webb Telescope (JWST) to identify the most distant globular clusters ever discovered - dense groups of millions of stars that may be relics containing the first and oldest stars in the universe. The James Webb Telescope has captured a stunning image of a cluster of billion year old galaxies. The James Webb Telescope recently beamed its first official photo of deep space to NASA officials This telescope will spy distant galaxies using 168 off-the-shelf Canon lenses The Dragonfly Telephoto Array installed in New Mexico. It presently uses 48 Canon 400mm lenses (in two arrays), but that number will be increasing by quite a bit. Image by Pieter van Dokkum, Yale University The combined mass of this galaxy cluster acts as a gravitational lens, magnifying much more distant galaxies behind it, NASA said in a press release. The image was unveiled by US President WASHINGTON, July 21 — Just a week after its first images were shown to the world, the James Webb Space Telescope may have found a galaxy that existed 13.5 billion years ago, a scientist who analysed the data said Wednesday. Known as GLASS-z13, the galaxy dates back to 300 million years after the Big Bang, about 100 million years earlier than The first image from the $10 billion James Webb Space Telescope was released Monday at the White House — a jumble of distant galaxies that went deeper into the cosmos than humanity has ever seen Tue 12 Jul 2022 // 00:05 UTC Pic On Monday, NASA released its first image from the James Webb Space Telescope, or JWST, providing the sharpest and deepest glimpse yet of distant galaxies from the very early universe. . It has been an exciting week with the release of breathtaking photos of our Universe by the James Webb Space Telescope JWST. Images such as the one below give us a chance to see faint distant galaxies as they were more than 13 billion years ago. The SMACS 0723 deep field image was taken with only a exposure. Faint galaxies in this image emitted this light more than 13 billion years ago. NASA, ESA, CSA, and STScI It’s the perfect time to step back and appreciate our first-class ticket to the depths of the Universe and how these images allow us to look back in time. These images also raise interesting points about how the expansion of the Universe factors into the way we calculate distances at a cosmological scale. Modern time travel Looking back in time might sound like a strange concept, but it’s what space researchers do every single day. Our Universe is bound by the rules of physics, with one of the best-known “rules” being the speed of light. And when we talk about “light”, we’re actually referring to all the wavelengths across the electromagnetic spectrum, which travel at around a whooping 300,000 kilometres per second. Light travels so fast that in our everyday lives it appears to be instantaneous. Even at these break-neck speeds, it still takes some time to travel anywhere across the cosmos. When you look at the Moon, you actually see it as it was seconds ago. It’s only a tiny peek back in time, but it’s still the past. It’s the same with sunlight, except the photons light particles emitted from the Sun’s surface travel just over eight minutes before they finally reach Earth. Our galaxy, the Milky Way, spans 100,000+ light-years. And the beautiful newborn stars seen in JWST’s Carina Nebula image are 7,500 light-years away. In other words, this nebula as pictured is from a time roughly 2,000 years earlier than when the first ever writing is thought to have been invented in ancient Mesopotamia. The Carina Nebula is a birthplace for stars. NASA, ESA, CSA, and STScI Anytime we look away from the Earth, we’re looking back in time to how things once were. This is a superpower for astronomers because we can use light, as observed throughout time, to try to puzzle together the mystery of our universe. What makes JWST spectacular Space-based telescopes let us see certain ranges of light that are unable to pass through Earth’s dense atmosphere. The Hubble space telescope was designed and optimised to use both ultraviolet UV and visible parts of the electromagnetic spectrum. The JWST was designed to use a broad range of infrared light. And this is a key reason the JWST can see further back in time than Hubble. The electromagnetic spectrum with Hubble and JWST’s ranges. Hubble is optimised to see shorter wavelengths. These two telescopes complement each other, giving us a fuller picture of the universe. NASA, J. Olmsted STScI Galaxies emit a range of wavelengths on the electromagnetic spectrum, from gamma rays to radio waves, and everything in between. All of these give us important information about the different physics occurring in a galaxy. When galaxies are near us, their light hasn’t changed that much since being emitted, and we can probe a vast range of these wavelengths to understand what’s happening inside them. But when galaxies are extremely far away, we no longer have that luxury. The light from the most distant galaxies, as we see it now, has been stretched to longer and redder wavelengths due to the expansion of the universe. This means some of the light that would have been visible to our eyes when it was first emitted has since lost energy as the universe expanded. It’s now in a completely different region of the electromagnetic spectrum. This is a phenomenon called “cosmological redshift”. And this is where the JWST really shines. The broad range of infrared wavelengths detectable by JWST allow it to see galaxies Hubble never could. Combine this capability with the JWST’s enormous mirror and superb pixel resolution, and you have the most powerful time machine in the known universe. Read more Two experts break down the James Webb Space Telescope's first images, and explain what we've already learnt Light age does not equal distance Using the JWST, we will be able to capture extremely distant galaxies as they were only 100 million years after the Big Bang – which happened around billion years ago. So we will be able to see light from billion years ago. What’s about to hurt your brain, however, is that those galaxies are not billion light-years away. The actual distance to those galaxies today would be ~46 billion light-years. This discrepancy is all thanks to the expanding universe, and makes working on a very large scale tricky. The universe is expending due to something called “dark energy”. It’s thought to be a universal constant, acting equally in all areas of space-time the fabric of our universe. And the more the universe expands, the greater the effect dark energy has on its expansion. This is why even though the universe is billion years old, it’s actually about 93 billion light-years across. We can’t see the effect of dark energy on a galactic scale within the Milky Way but we can see it over much greater cosmological distances. Sit back and enjoy We live in a remarkable time of technology. Just 100 years ago, we didn’t know there were galaxies outside our own. Now we estimate there are trillions, and we are spoilt for choice. For the foreseeable future, the JWST will be taking us on a journey through space and time each and every week. You can stay up to date with the latest news as NASA releases it. Editor’s Note Sign up for CNN’s Wonder Theory science Explore the universe with news on fascinating discoveries, scientific advancements and more. CNN — Astronomers have detected the most distant known organic molecules in the universe using the James Webb Space Telescope. It’s the first time Webb has detected complex molecules in the distant universe. The complex molecules were found in a galaxy known as SPT0418-47, located more than 12 billion light-years away. The discovery sheds light on the chemical interactions that occurred within the earliest galaxies in the universe and how they relate to star formation. On Earth, the molecules, called polycyclic aromatic hydrocarbons, can be found in smoke, soot, smog, engine exhaust and forest fires. The base of the organic molecules is carbon, considered to be one of the building blocks of life because it’s a key element in amino acids, which form proteins. A study detailing the findings was published Monday in the journal Nature. The light from the dusty galaxy began traveling across the cosmos when the universe was less than billion years old, just 10% of its current age of billion years. The galaxy was first spotted in 2013 by the National Science Foundation’s South Pole Telescope. Other observatories, such as the Hubble Space Telescope and the Atacama Large Millimeter/submillimeter Array in Chile, have observed it since. But the Webb telescope’s infrared capabilities, which can see light invisible to the human eye and peer through cosmic dust, was able to capture new details about the galaxy. And the space observatory received a helping hand from a phenomenon called gravitational lensing. “This magnification happens when two galaxies are almost perfectly aligned from the Earth’s point of view, and light from the background galaxy is warped and magnified by the foreground galaxy into a ring-like shape, known as an Einstein ring,” said study coauthor Joaquin Vieira, professor of astronomy and physics at the University of Illinois Urbana-Champaign, in a statement. Gravitational lensing was originally predicted in Albert Einstein’s theory of relativity. “By combining Webb’s amazing capabilities with a natural ‘cosmic magnifying glass,’ we were able to see even more detail than we otherwise could,” said lead study author Justin Spilker, an assistant professor of physics and astronomy at Texas A&M University, in a statement. “That level of magnification is actually what made us interested in looking at this galaxy with Webb in the first place, because it really lets us see all the rich details of what makes up a galaxy in the early universe that we could never do otherwise,” said Spilker, who is also a member of Texas A&M’s George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy. Astronomers spotted the signature of the organic molecules during a careful analysis of Webb’s data. The molecules are common in space. Here on Earth, they are part of cancer-causing hydrocarbon emissions that contribute to the planet’s atmospheric pollution. Previously, astronomers thought polycyclic aromatic hydrocarbons were a sign of star formation because they have observed the large molecules near bright young stars. But Webb’s data revealed the presence of these molecules may not have been an indicator of star birth in the early days of the universe. “Thanks to the high-definition images from Webb, we found a lot of regions with smoke but no star formation, and others with new stars forming but no smoke,” Spilker said. The unexpected finding is helping astronomers piece together answers to some of the lingering questions about the beginning of the universe. “Discoveries like this are precisely what Webb was built to do understand the earliest stages of the universe in new and exciting ways,” said study coauthor Kedar Phadke, a doctoral student of astronomy at the University of Illinois Urbana-Champaign, in a statement. “It’s amazing that we can identify molecules billions of light-years away that we’re familiar with here on Earth, even if they show up in ways we don’t like, like smog and smoke. It’s also a powerful statement about the amazing capabilities of Webb that we’ve never had The researchers are looking forward to flexing Webb’s capabilities more in the future as they search for even more distant galaxies. “Now that we’ve shown this is possible for the first time, we’re looking forward to trying to understand whether it’s really true that where there’s smoke, there’s fire,” Spilker said. “Maybe we’ll even be able to find galaxies that are so young that complex molecules like these haven’t had time to form in the vacuum of space yet, so galaxies are all fire and no smoke. The only way to know for sure is to look at more galaxies, hopefully even further away than this NASA's James Webb Space Telescope has shared a mesmerising and never-before-seen picture showing more than 45,000 galaxies in one frame. The picture was of a portion of the sky known as GOODS-Sout. James Webb Space Telescope captured the image as part of the JWST Advanced Deep Extragalactic Survey per the space agency, around 32 days of the telescope time will be devoted to the JADES programme to uncover and characterise distant and faint galaxies as astronomers make efforts to understand how the first stars and galaxies were formed. Although the data is still pouring in, hundreds of galaxies have already been discovered that existed when the universe had not completed 600 million years. Galaxies, which were sparkling along with a number of young, hot stars, have also been identified by the of the JADES programme and professor at the University of Arizona in Tucson Marcia Rieke said, "With JADES, we want to answer a lot of questions, like How did the earliest galaxies assemble themselves? How fast did they form stars? Why do some galaxies stop forming stars?"The part of the sky was previously observed by the Hubble telescope. You're looking at 45,000+ galaxies. This image was taken as part of the JWST Advanced Deep Extragalactic Survey JADES — a massive science program that’s revolutionizing what we know about galaxies in the early universe Here are the highlights ⬇️ — NASA Webb Telescope NASAWebb June 5, 2023 × Investigation into galaxies that existed 500 to 850 million years after the big bang University of Texas' Ryan Endsley headed the investigation into galaxies which existed 500 to 850 million years after the big bang occurred. "For hundreds of millions of years after the big bang, the universe was filled with a gaseous fog that made it opaque to energetic light. By one billion years after the big bang, the fog had cleared and the universe became transparent, a process known as reionisation. Scientists have debated whether active, supermassive black holes or galaxies full of hot, young stars were the primary cause of reionisation," the space agency explained. The researchers found evidence of young galaxies going through rapid star formation interspersed with short periods where fewer stars formed. WATCH NASA mission to Saturn's moon Titan may unravel secrets behind origin of life “Almost every single galaxy that we are finding shows these unusually strong emission line signatures indicating intense recent star formation. These early galaxies were very good at creating hot, massive stars,” stated Ryan Endsley of the University of Texas, who headed the investigation.“Previously, the earliest galaxies we could see just looked like little smudges. And yet those smudges represent millions or even billions of stars at the beginning of the universe. Now, we can see that some of them are actually extended objects with visible structures. We can see groupings of stars being born only a few hundred million years after the beginning of time,” stated Kevin Hainline of the University of Arizona, in a statement. "We're finding star formation in the early universe is much more complicated than we thought," Rieke stated. You can now write for and be a part of the community. Share your stories and opinions with us WION LIVE HERE Researchers have detected complex organic molecules in a galaxy more than 12 billion light-years away from Earth - the most distant galaxy in which these molecules are now known to exist. Thanks to the capabilities of the recently launched James Webb Space Telescope and careful analyses from the research team, a new study lends critical insight into the complex chemical interactions that occur in the first galaxies in the early universe. University of Illinois Urbana-Champaign astronomy and physics professor Joaquin Vieira and graduate student Kedar Phadke collaborated with researchers at Texas A&M University and an international team of scientists to differentiate between infrared signals generated by some of the more massive and larger dust grains in the galaxy and those of the newly observed hydrocarbon molecules. The study findings are published in the journal Nature. "This project started when I was in graduate school studying hard-to-detect, very distant galaxies obscured by dust," Vieira said. "Dust grains absorb and re-emit about half of the stellar radiation produced in the universe, making infrared light from distant objects extremely faint or undetectable through ground-based telescopes." In the new study, the JWST received a boost from what the researchers call "nature's magnifying glass" - a phenomenon called gravitational lensing. "This magnification happens when two galaxies are almost perfectly aligned from the Earth's point of view, and light from the background galaxy is warped and magnified by the foreground galaxy into a ring-like shape, known as an Einstein ring," Vieira said. The team focused the JWST on SPT0418-47 - an object discovered using the National Science Foundation's South Pole Telescope and previously identified as a dust-obscured galaxy magnified by a factor of about 30 to 35 by gravitational lensing. SPT0418-47 is 12 billion light-years from Earth, corresponding to a time when the universe was less than billion years old, or about 10% of its current age, the researchers said. "Before having access to the combined power of gravitational lensing and the JWST, we could neither see nor spatially resolve the actual background galaxy through all of the dust," Vieira said. Spectroscopic data from the JWST suggest that the obscured interstellar gas in SPT0418-47 is enriched in heavy elements, indicating that generations of stars have already lived and died. The specific compound the researchers detected is a type of molecule called polycyclic aromatic hydrocarbon, or PAH. On Earth, these molecules can be found in the exhaust produced by combustion engines or forest fires. Being comprised of carbon chains, these organic molecules are considered the basic building blocks for the earliest forms of life, the researchers said. "What this research is telling us right now - and we are still learning - is that we can see all of the regions where these smaller dust grains are located - regions that we could never see before the JWST," Phadke said. "The new spectroscopic data lets us observe the galaxy's atomic and molecular composition, providing very important insights into the formation of galaxies, their lifecycle and how they evolve." "We didn't expect this," Vieira said. "Detecting these complex organic molecules at such a vast distance is game-changing regarding future observations. This work is just the first step, and we're just now learning how to use it and learn its capabilities. We are very excited to see how this plays out." "It's extremely cool that galaxies I discovered while writing my thesis would one day be observed by the JWST," Vieira said. "I am grateful to the taxpayers, the NSF and NASA for funding and supporting both the SPT and the JWST. Without these instruments, this discovery could have never been made." Vieira also is the director of the Center for AstroPhysical Surveys, funded by the National Center for Supercomputing Applications at Illinois. Phadke is a CAPS graduate fellow. The Space Telescope Science Institute operates the JWST under the management of the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. The bright star at the center of NGC 3132, Southern Nebula Ring, while prominent when viewed by NASA's Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula. A second star, barely visible at lower left along one of the bright star's diffraction spikes, is the nebula's source. It has ejected at least eight layers of gas and dust over thousands of years. NASA, ESA, CSA, STScI hide caption toggle caption NASA, ESA, CSA, STScI The bright star at the center of NGC 3132, Southern Nebula Ring, while prominent when viewed by NASA's Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula. A second star, barely visible at lower left along one of the bright star's diffraction spikes, is the nebula's source. It has ejected at least eight layers of gas and dust over thousands of years. NASA, ESA, CSA, STScI The universe's splendor and breadth are on display like never before, thanks to a new batch of images that NASA released from the James Webb Space Telescope on Tuesday. The images from the new telescope are "really gorgeous," said NASA's Jane Rigby, the operations project scientist for the James Webb Space Telescope. "That's something that has been true for every image we've gotten with Webb," she added. "We can't take blank sky [images]. Everywhere we look, there's galaxies everywhere." The images reflect five areas of space that researchers agreed to target the exoplanet WASP-96 b; the Southern Ring Nebula; the Carina Nebula; Stephan's Quintet five galaxies in the constellation Pegasus; and the galaxy cluster SMACS 0723. A nursery for the stars One of the most eye-popping images released on Tuesday depicts what looks to be cosmic cliffs, valleys and mountains — albeit with mountains that stretch to seven light-years in height. What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera NIRCam on NASA's James Webb Space Telescope, this image reveals previously obscured areas of star birth. NASA, ESA, CSA, STScI hide caption toggle caption NASA, ESA, CSA, STScI What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera NIRCam on NASA's James Webb Space Telescope, this image reveals previously obscured areas of star birth. NASA, ESA, CSA, STScI The image captures part of a "stellar nursery called NGC 3324 at the northwest corner of the Carina Nebula," NASA said. It's roughly 7,600 light-years from Earth. "The blistering, ultraviolet radiation from the young stars is sculpting the nebula's wall by slowly eroding it away," the agency added. "Dramatic pillars tower above the glowing wall of gas, resisting this radiation. The 'steam' that appears to rise from the celestial 'mountains' is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation." Galaxies from 'It's a Wonderful Life' stun scientists The tight galaxy group called Stephan's Quintet is a "laboratory" for scientists to study the powerful effects galaxies can exert on each other, thanks to new data from the Webb telescope. An enormous mosaic of Stephan's Quintet is the largest image to date from NASA's James Webb Space Telescope, covering about one-fifth of the Moon's diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The visual grouping of five galaxies was captured by Webb's Near-Infrared Camera NIRCam and Mid-Infrared Instrument MIRI. NASA, ESA, CSA, STScI hide caption toggle caption NASA, ESA, CSA, STScI An enormous mosaic of Stephan's Quintet is the largest image to date from NASA's James Webb Space Telescope, covering about one-fifth of the Moon's diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The visual grouping of five galaxies was captured by Webb's Near-Infrared Camera NIRCam and Mid-Infrared Instrument MIRI. NASA, ESA, CSA, STScI Researchers hope to learn more about how galaxies merge and interact, including triggering each other to form new stars, and how those processes might be impacted by supermassive black holes. The image casts the quintet in a new light, after they represented angels in Frank Capra's class film It's a Wonderful Life. "This enormous mosaic is Webb's largest image to date, covering about one-fifth of the Moon's diameter," NASA said. "It contains over 150 million pixels and is constructed from almost 1,000 separate image files." Catch a dying star Webb pulled the veil back on the second star in the Southern Ring Nebula, using mid-infrared wavelengths to capture it in extraordinary detail. "The star closely orbits its companion as it periodically ejects layers of gas and dust," NASA said. "Together, the swirling duo have created a fantastic landscape of asymmetrical shells." The new image shows the nebula from a nearly head-on view. But if we could see it from its edge, NASA says, "its three-dimensional shape would more clearly look like two bowls placed together at the bottom, opening away from one another with a large hole at the center." Webb delivers a portrait of a puffy giant "WASP-96 b is a giant planet outside our solar system, composed mainly of gas," NASA said. "The planet, located nearly 1,150 light-years from Earth, orbits its star every days. It has about half the mass of Jupiter, and its discovery was announced in 2014." The agency didn't release a photo but rather a spectrum analysis of WASP-96 b's atmosphere, garnered from Webb sighting the WASP-96 b as it transited in front of a star. A transmission spectrum made from a single observation using Webb's Near-Infrared Imager and Slitless Spectrograph NIRISS reveals atmospheric characteristics of the hot gas giant exoplanet WASP-96 b. Illustration NASA, ESA, CSA, STScI hide caption toggle caption Illustration NASA, ESA, CSA, STScI A transmission spectrum made from a single observation using Webb's Near-Infrared Imager and Slitless Spectrograph NIRISS reveals atmospheric characteristics of the hot gas giant exoplanet WASP-96 b. Illustration NASA, ESA, CSA, STScI A light curve from Webb's Near-Infrared Imager and Slitless Spectrograph NIRISS shows the change in brightness of light from the WASP-96 star system over time as the planet transits the star. A transit occurs when an orbiting planet moves between the star and the telescope, blocking some of the light from the star. Illustration NASA, ESA, CSA, STScI hide caption toggle caption Illustration NASA, ESA, CSA, STScI A light curve from Webb's Near-Infrared Imager and Slitless Spectrograph NIRISS shows the change in brightness of light from the WASP-96 star system over time as the planet transits the star. A transit occurs when an orbiting planet moves between the star and the telescope, blocking some of the light from the star. Illustration NASA, ESA, CSA, STScI The analysis found the "chemical fingerprint" of water in the atmosphere, said Knicole Colon, a research astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Md. A look at some of the universe's first galaxies ever The trove of images comes one day after a jaw-dropping first image was published by NASA and the White House, more than six months after the telescope was launched from Earth. That first image showed the galaxy cluster SMACS 0723, known as Webb's First Deep Field. NASA's James Webb Space Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this composite image of galaxy cluster SMACS 0723 is overflowing with detail. The image shows the galaxy cluster SMACS 0723 as it appeared billion years ago. NASA, ESA, CSA, and STScI hide caption toggle caption NASA, ESA, CSA, and STScI NASA's James Webb Space Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this composite image of galaxy cluster SMACS 0723 is overflowing with detail. The image shows the galaxy cluster SMACS 0723 as it appeared billion years ago. NASA, ESA, CSA, and STScI "If you held a grain of sand on the tip of your finger at arm's length, that is the part of the universe you are seeing — just one little speck of the universe," NASA Administrator Bill Nelson said on Monday. But that speck contains multitudes. And thanks to the telescope's deep and sharp infrared images, Earthlings are getting a more detailed look at distant galaxies than was ever possible. That first image comprises thousands of galaxies, with even faint and diffuse structures visible for the first time. "This deep field, taken by Webb's Near-Infrared Camera NIRCam, is a composite made from images at different wavelengths, totaling hours – achieving depths at infrared wavelengths beyond the Hubble Space Telescope's deepest fields, which took weeks," NASA said. The stunning displays amount to a rich lesson in the history of the universe some of the galaxies are more than 13 billion years old, meaning they formed relatively soon after the Big Bang. For instance, the image of galaxy cluster SMACS 0723 amounts to a snapshot from billion years ago. Aside from gaping at stunning views like everyone else, researchers will use data from the Webb telescope "to learn more about the galaxies' masses, ages, histories, and compositions," according to NASA. The Webb Space Telescope is the culmination of an international program led by NASA. Its partners include the European Space Agency, or ESA, and the Canadian Space Agency.

the telescope will photograph distant galaxies