NASA Webb’s First Full-Color Images, Data Are Set to Sound
There’s a new, immersive way to explore some of the first full-color infrared images and data from NASA’s James Webb Space Telescope – through sound. Listeners can enter the complex soundscape of the Cosmic Cliffs in the Carina Nebula, explore the contrasting tones of two images that depict the Southern Ring Nebula, and identify the individual data points in a transmission spectrum of hot gas giant exoplanet WASP-96 b. “Music taps into our emotional centers,” said Matt Russo, a musician and physics professor at the University of Toronto. “Our goal is to make Webb’s images and data understandable through sound – helping listeners create their own mental images.”
A team of scientists, musicians, and a member of the blind and visually impaired community worked to adapt Webb’s data, with support from the Webb mission and NASA’s Universe of Learning.
Webb’s Cosmic Cliffs Sonification
Credits: Image: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).
A near-infrared image of the Cosmic Cliffs in the Carina Nebula, captured by NASA’s Webb Telescope, has been mapped to a symphony of sounds. Musicians assigned unique notes to the semi-transparent, gauzy regions and very dense areas of gas and dust in the nebula, culminating in a buzzing soundscape.
The sonification scans the image from left to right. The soundtrack is vibrant and full, representing the detail in this gigantic, gaseous cavity that has the appearance of a mountain range. The gas and dust in the top half of the image are represented in blue hues and windy, drone-like sounds. The bottom half of the image, represented in ruddy shades of orange and red, has a clearer, more melodic composition.
Brighter light in the image is louder. The vertical position of light also dictates the frequency of sound. For example, bright light near the top of the image sounds loud and high, but bright light near the middle is loud and lower pitched. Dimmer, dust-obscured areas that appear lower in the image are represented by lower frequencies and clearer, undistorted notes.
Webb’s Southern Ring Nebula Sonification
Credits: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).
NASA’s Webb Telescope uncovered two views of the Southern Ring Nebula – in near-infrared light (at left) and mid-infrared light (at right) – and each has been adapted to sound.
In this sonification, the colors in the images were mapped to pitches of sound – frequencies of light converted directly to frequencies of sound. Near-infrared light is represented by a higher range of frequencies at the beginning of the track. Mid-way through, the notes change, becoming lower overall to reflect that mid-infrared includes longer wavelengths of light.
Listen carefully at 15 seconds and 44 seconds. These notes align with the centers of the near- and mid-infrared images, where the stars at the center of the “action” appear. In the near-infrared image that begins the track, only one star is heard clearly, with a louder clang. In the second half of the track, listeners will hear a low note just before a higher note, which denotes that two stars were detected in mid-infrared light. The lower note represents the redder star that created this nebula, and the second is the star that appears brighter and larger.
Webb’s Exoplanet WASP-96 b Sonification
Credits: Image: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).
NASA’s Webb Telescope observed the atmospheric characteristics of the hot gas giant exoplanet WASP-96 b – which contains clear signatures of water – and the resulting transmission spectrum’s individual data points were translated into sound.
The sonification scans the spectrum from left to right. From bottom to top, the y-axis ranges from less to more light blocked. The x-axis ranges from 0.6 microns on the left to 2.8 microns on the right. The pitches of each data point correspond to the frequencies of light each point represents. Longer wavelengths of light have lower frequencies and are heard as lower pitches. The volume indicates the amount of light detected in each data point.
The four water signatures are represented by the sound of water droplets falling. These sounds simplify the data – water is detected as a signature that has multiple data points. The sounds align only to the highest points in the data.
Mapping Data to Sound
These audio tracks support blind and low-vision listeners first, but are designed to be captivating to anyone who tunes in. “These compositions provide a different way to experience the detailed information in Webb’s first data. Similar to how written descriptions are unique translations of visual images, sonifications also translate the visual images by encoding information, like color, brightness, star locations, or water absorption signatures, as sounds,” said Quyen Hart, a senior education and outreach scientist at the Space Telescope Science Institute in Baltimore, Maryland. “Our teams are committed to ensuring astronomy is accessible to all.”
This project has parallels to the “curb-cut effect,” an accessibility requirement that supports a wide range of pedestrians. “When curbs are cut, they benefit people who use wheelchairs first, but also people who walk with a cane and parents pushing strollers,” explained Kimberly Arcand, a visualization scientist at the Chandra X-ray Center in Cambridge, Massachusetts, who led the initial data sonification project for NASA and now works on it on behalf of NASA’s Universe of Learning. “We hope these sonifications reach an equally broad audience.”
Preliminary results from a survey Arcand led showed that people who are blind or low vision, and people who are sighted, all reported that they learned something about astronomical images by listening. Participants also shared that auditory experiences deeply resonated with them. “Respondents’ reactions varied – from experiencing awe to feeling a bit jumpy,” Arcand continued. “One significant finding was from people who are sighted. They reported that the experience helped them understand how people who are blind or low vision access information differently.”
“One significant finding was from people who are sighted. They reported that the experience helped them understand how people who are blind or low vision access information differently.”
These tracks are not actual sounds recorded in space. Instead, Russo and his collaborator, musician Andrew Santaguida, mapped Webb’s data to sound, carefully composing music to accurately represent details the team would like listeners to focus on. In a way, these sonifications are like modern dance or abstract painting – they convert Webb’s images and data to a new medium to engage and inspire listeners.
Christine Malec, a member of the blind and low vision community who also supports this project, said she experiences the audio tracks with multiple senses. “When I first heard a sonification, it struck me in a visceral, emotional way that I imagine sighted people experience when they look up at the night sky.”
There are other profound benefits to these adaptations. “I want to understand every nuance of sound and every instrument choice, because this is primarily how I’m experiencing the image or data,” Malec continued. Overall, the team hopes that sonifications of Webb’s data help more listeners feel a stronger connection to the universe – and inspire everyone to follow the observatory’s upcoming astronomical discoveries.
The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
These sonifications are a result of a collaboration between the NASA’s Universe of Learning program and the James Webb Space Telescope. The Chandra X-ray Center (CXC) leads data sonification as a NASA’s Universe of Learning partner. Science experts affiliated with the Webb mission provide their expertise on Webb observations, data, and targets.
NASA's Universe of Learning is part of the NASA Science Activation program, from the Science Mission Directorate at NASA Headquarters. The Science Activation program connects NASA science experts, real content and experiences, and community leaders in a way that activates minds and promotes deeper understanding of our world and beyond. Using its direct connection to the science and the experts behind the science, NASA's Universe of Learning provides resources and experiences that enable youth, families, and lifelong learners to explore fundamental questions in science, experience how science is done, and discover the universe for themselves.
NASA's Universe of Learning materials are based upon work supported by NASA under cooperative agreement award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and Jet Propulsion Laboratory.
Quelle: NASA
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Update: 3.09.2022
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NASA’s Webb Takes Its First-Ever Direct Image of Distant World
For the first time, astronomers have used NASA’s James Webb Space Telescope to take a direct image of a planet outside our solar system. The exoplanet is a gas giant, meaning it has no rocky surface and could not be habitable.
The image, as seen through four different light filters, shows how Webb’s powerful infrared gaze can easily capture worlds beyond our solar system, pointing the way to future observations that will reveal more information than ever before about exoplanets.
“This is a transformative moment, not only for Webb but also for astronomy generally,” said Sasha Hinkley, associate professor of physics and astronomy at the University of Exeter in the United Kingdom, who led these observations with a large international collaboration. Webb is an international mission led by NASA in collaboration with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
The exoplanet in Webb’s image, called HIP 65426 b, is about six to 12 times the mass of Jupiter, and these observations could help narrow that down even further. It is young as planets go — about 15 to 20 million years old, compared to our 4.5-billion-year-old Earth.
Astronomers discovered the planet in 2017 using the SPHERE instrument on the European Southern Observatory’s Very Large Telescope in Chile and took images of it using short infrared wavelengths of light. Webb’s view, at longer infrared wavelengths, reveals new details that ground-based telescopes would not be able to detect because of the intrinsic infrared glow of Earth’s atmosphere.
Researchers have been analyzing the data from these observations and are preparing a paper they will submit to journals for peer review. But Webb’s first capture of an exoplanet already hints at future possibilities for studying distant worlds.
Since HIP 65426 b is about 100 times farther from its host star than Earth is from the Sun, it is sufficiently distant from the star that Webb can easily separate the planet from the star in the image.
Webb’s Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) are both equipped with coronagraphs, which are sets of tiny masks that block out starlight, enabling Webb to take direct images of certain exoplanets like this one. NASA’s Nancy Grace Roman Space Telescope, slated to launch later this decade, will demonstrate an even more advanced coronagraph.
“It was really impressive how well the Webb coronagraphs worked to suppress the light of the host star,” Hinkley said.
Taking direct images of exoplanets is challenging because stars are so much brighter than planets. The HIP 65426 b planet is more than 10,000 times fainter than its host star in the near-infrared, and a few thousand times fainter in the mid-infrared.
In each filter image, the planet appears as a slightly differently shaped blob of light. That is because of the particulars of Webb’s optical system and how it translates light through the different optics.
“Obtaining this image felt like digging for space treasure,” said Aarynn Carter, a postdoctoral researcher at the University of California, Santa Cruz, who led the analysis of the images. “At first all I could see was light from the star, but with careful image processing I was able to remove that light and uncover the planet.”
While this is not the first direct image of an exoplanet taken from space – the Hubble Space Telescope has captured direct exoplanet images previously – HIP 65426 b points the way forward for Webb’s exoplanet exploration.
“I think what’s most exciting is that we’ve only just begun,” Carter said. “There are many more images of exoplanets to come that will shape our overall understanding of their physics, chemistry, and formation. We may even discover previously unknown planets, too.”
Quelle: NASA
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Update: 6.09.2022
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Stunningly perfect 'Einstein ring' captured by James Webb Space Telescope
It is our best look yet at these weird gravitationally-warped halos of light.
A near-perfect Einstein ring from the galaxy JO418. (Image credit: Spaceguy44)
NASA's James Webb Space Telescope has snapped a perfect shot of an "Einstein ring."
The stunning halo is the result of light from a distant galaxy passing through warped space-time surrounding another galaxy aligned between the distant light source and Earth. The new James Webb Space Telescope image, which was created by a Reddit-based astronomy enthusiast, is one of the best examples of the trippy astronomical phenomenon ever captured.
The ring of light in the new image comes from the distant galaxy SPT-S J041839-4751.8 (or JO418 for short), which is around 12 billion light-years from Earth, making it one of the oldest galaxies in the universe. JO418 is orientated directly behind another galaxy — the bright blue light at the center of the ring — which is so massive that its gravitational pull warps the space-time around it. As light from JO418 reaches the foreground galaxy it travels through this warped space-time. From Earth, it looks as though the light has curved around the galaxy, but the electromagnetic waves we see have actually been traveling in a straight line the entire time.
This weird effect is similar to how glass lenses redirect light. Like magnifying glasses, this phenomenon also makes the light from distant galaxies appear much closer than they actually are. The only difference is that the lens is made from gravity-mangled space-time instead of glass. As a result, researchers have dubbed this trippy effect, gravitational lensing. Albert Einstein first predicted gravitational lensing in 1912, when he devised his theory of relativity.
Reddit user and astronomy grad student "Spaceguy44" posted the image of the JOS18 Einstein ring Aug. 23 in the subreddit r/Astronomy. The anonymous astronomer created the shot using publicly available data collected by the Mid-Infrared Instrument (MIRI) on the James Webb Space Telescope.
"We wouldn't be able to see J0418 if it weren't for the light-bending properties of gravity," Spaceguy44 wrote on Reddit. "Without the lensing effect, the galaxy would probably look like most distant galaxies: a small blob of light."
The new image is not the first glimpse of JO418, but it is by far the most detailed yet.
In 2020, researchers discovered the distant galaxy after spotting partial gravitational lensing with the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile; they reported the finding in a paper published that year in the journal Nature(opens in new tab).
On Aug. 13, Spaceguy44 released an image of JO418 using data collected by Webb's NIRCam instrument, but the initial shot had a much lower resolution and the ring of light was less visible, according to ScienceAlert(opens in new tab)
NASA's Hubble Space Telescope has captured images of several other Einstein rings, including one formed from warped quasar light(opens in new tab). However, none of these Einstein rings was as complete or as clearly visible as the one in the new image.
Perfectly-circular Einstein rings are extremely rare because they require both the distant and foreground galaxies to be perfectly aligned with the observer. However, the more advanced sensors on Webb should make it easier to spot them in the future.
In this mosaic image stretching 340 light-years across, Webb’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust. The most active region appears to sparkle with massive young stars, appearing pale blue.
Credits: NASA, ESA, CSA, STScI, Webb ERO Production Team
Once upon a space-time, a cosmic creation story unfolded: Thousands of never-before-seen young stars spotted in a stellar nursery called 30 Doradus, captured by NASA’s James Webb Space Telescope. Nicknamed the Tarantula Nebula for the appearance of its dusty filaments in previous telescope images, the nebula has long been a favorite for astronomers studying star formation. In addition to young stars, Webb reveals distant background galaxies, as well as the detailed structure and composition of the nebula’s gas and dust.
At only 161,000 light-years away in the Large Magellanic Cloud galaxy, the Tarantula Nebula is the largest and brightest star-forming region in the Local Group, the galaxies nearest our Milky Way. It is home to the hottest, most massive stars known. Astronomers focused three of Webb’s high-resolution infrared instruments on the Tarantula. Viewed with Webb’s Near-Infrared Camera (NIRCam), the region resembles a burrowing tarantula’s home, lined with its silk. The nebula’s cavity centered in the NIRCam image has been hollowed out by blistering radiation from a cluster of massive young stars, which sparkle pale blue in the image. Only the densest surrounding areas of the nebula resist erosion by these stars’ powerful stellar winds, forming pillars that appear to point back toward the cluster. These pillars contain forming protostars, which will eventually emerge from their dusty cocoons and take their turn shaping the nebula.
Webb’s Near-Infrared Spectrograph (NIRSpec) caught one very young star doing just that. Astronomers previously thought this star might be a bit older and already in the process of clearing out a bubble around itself. However, NIRSpec showed that the star was only just beginning to emerge from its pillar and still maintained an insulating cloud of dust around itself. Without Webb’s high-resolution spectra at infrared wavelengths, this episode of star formation-in-action could not have been revealed.
At the longer wavelengths of light captured by its Mid-Infrared Instrument (MIRI), Webb focuses on the area surrounding the central star cluster and unveils a very different view of the Tarantula Nebula. In this light, the young hot stars of the cluster fade in brilliance, and glowing gas and dust come forward. Abundant hydrocarbons light up the surfaces of the dust clouds, shown in blue and purple.
Credits: NASA, ESA, CSA, STScI, Webb ERO Production Team
The region takes on a different appearance when viewed in the longer infrared wavelengths detected by Webb’s Mid-infrared Instrument (MIRI). The hot stars fade, and the cooler gas and dust glow. Within the stellar nursery clouds, points of light indicate embedded protostars, still gaining mass. While shorter wavelengths of light are absorbed or scattered by dust grains in the nebula, and therefore never reach Webb to be detected, longer mid-infrared wavelengths penetrate that dust, ultimately revealing a previously unseen cosmic environment.
One of the reasons the Tarantula Nebula is interesting to astronomers is that the nebula has a similar type of chemical composition as the gigantic star-forming regions observed at the universe’s “cosmic noon,” when the cosmos was only a few billion years old and star formation was at its peak. Star-forming regions in our Milky Way galaxy are not producing stars at the same furious rate as the Tarantula Nebula, and have a different chemical composition. This makes the Tarantula the closest (i.e., easiest to see in detail) example of what was happening in the universe as it reached its brilliant high noon. Webb will provide astronomers the opportunity to compare and contrast observations of star formation in the Tarantula Nebula with the telescope’s deep observations of distant galaxies from the actual era of cosmic noon.
Despite humanity’s thousands of years of stargazing, the star-formation process still holds many mysteries – many of them due to our previous inability to get crisp images of what was happening behind the thick clouds of stellar nurseries. Webb has already begun revealing a universe never seen before, and is only getting started on rewriting the stellar creation story.
The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.
Quelle: NASA
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Update: 9.09.2022
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James Webb Space Telescope spots alien planet shrouded in weird sand-filled clouds
The exoplanet's atmosphere also contains methane and carbon dioxide.
Astronomers have long speculated that some types of brown dwarfs are wrapped in turbulent, fast-changing atmospheres.(Image credit: NASA/JPL-Caltech)
The James Webb Space Telescope has found a strange alien world shrouded in clouds of sand-like silicate grains.
The exoplanet discovery, described in a new paper as the first detection of its kind, was made by the James Webb Space Telescope's NIRSpec and MIRI instruments. In the data, astronomers spotted evidence of silicate-rich clouds around a brown dwarf nearly 20 times the size of Jupiter. The finding confirms some earlier theories about these odd planet-like worlds.
Brown dwarfs are strange objects that are not quite big enough to ignite into stars but a little too big for ordinary planets. While brown dwarfs can't burn regular hydrogen, they can produce their own light and heat by burning deuterium (a less common isotope of hydrogen that contains an extra neutron).
The brown dwarf in question is called VHS 1256 b and orbits two small red dwarfstars, some 72 light-years from Earth in the constellation Corvus, or crow, in the southern sky. Astronomers discovered the strange exoplanet in 2016 and it has puzzled them ever since due to its reddish glow. They believed that glow could be caused by some type of atmosphere. Observations from the James Webb Space Telescope have now confirmed those theories, revealing that VHS 1256 b must be wrapped in thick clouds full of sand-like silicate grains, according to Forbes(opens in new tab).
Webb also detected water, methane, carbon monoxide, carbon dioxide, sodium and potassium in the atmosphere of VHS 1256 b.
"We will know more from iterations on the data reduction," Brittany Miles, an astronomer at the University of California, Irvine, and lead researcher on the project, told Space.com in an email. "So far, it looks pretty similar to theoretical expectations."
The Webb data were so detailed they showed that the ratio of the various gases changes throughout VHS 1256 b's atmosphere, which suggests the atmosphere is not still, but instead wild and turbulent.
"In a calm atmosphere, there is an expected ratio of, say, methane and carbon monoxide," Sasha Hinkley, an astronomer at the University of Exeter in the U.K. and one of the study's co-authors, told Forbes(opens in new tab). "But in many exoplanet atmospheres we're finding that this ratio is very skewed, suggesting that there is turbulent vertical mixing in these atmospheres, dredging up carbon dioxide from deep down to mix with the methane higher up in the atmosphere."
VHS 1256 b is small for a brown dwarf, which means that the body is likely young. The exoplanet orbits 360 sun-Earth distances from its two parent stars, following an oval-shaped orbit that takes 17,000 years to complete.
The paper has not yet been published; an early version is currently available on the online preprint repository arXiv.org(opens in new tab).
Quelle: SC
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Update: 14.09.2022
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This New Webb Telescope Image Looks Like a Painting of the Cosmos
NASA and its partners released a new image Monday morning of the inner region of the famous Orion Nebula, located 1,350 light-years away, taken by the James Webb Space Telescope. Though the celestial structure is by no means a stranger to astronomers, Webb’s powerful cameras show the nebula in unprecedented beauty and detail.
The new image is really a composite of several photos taken using different filters. Combined, we get a glimpse of the nebula’s various components, including its youngest stars and caverns of dense gas. The most visible feature is the Orion Bar, a wall of gas and dust that stretches from left to right and contains a bright star called θ2 Orionis A.
“We are blown away by the breathtaking images of the Orion Nebula. We started this project in 2017, so we have been waiting more than five years to get these data,” Western University astrophysicist Els Peeters, who helped lead the latest observations, said in a press release. “These new observations allow us to better understand how massive stars transform the gas and dust cloud in which they are born.”
NASA/STScI/Rice Univ./C.O’Dell et al.
Previous views of the Orion Nebula taken by Hubble, although beautiful, pale in comparison to what Webb can observe. Much of that is thanks to the orbital observatory’s ability to view the universe in infrared and near-infrared light, which allows it to see past the gas and dust that enshrouds much of the inner region’s most captivating parts. This also means scientists can better study how structures like the nebula foster the birth and growth of infant stars.
Close up of the Orion Bar’s northern region. Can you spot the frog?
NASA, ESA, CSA
Webb also picked up a bonus image of the nebula as it zoomed in on the Orion Bar. If you look closely, you can spot a frog-like structure.