👀 Sneak a peek at the deepest & sharpest infrared image of the early universe ever taken — all in a day’s work for the Webb telescope. (Literally, capturing it took less than a day!) This is Webb’s first image released as we begin to #UnfoldTheUniverse: http://nasa.gov/webbfirstimages/
Source: @NASAWebb
Full resolution in comments
Source: @NASAWebb
Full resolution in comments
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This isn’t the farthest back we’ve observed. Non-infrared missions like COBE & WMAP saw the universe closer to the Big Bang (~380,000 years after), when there was only microwave background radiation, but no stars or galaxies. Webb sees a few 100 million years after the Big Bang.
Source: @NASAWebb
Source: @NASAWebb
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The image taken by the JWST compared to one taken by Hubble, of the galaxy cluster SMACS 0723.
It's a gravitational lens, showing us the light of galaxies that are far behind the cluster in arcs around it. I tried to orient them the same. LOOK AT THE DIFFERENCE.
12.5 hours of exposure for Webb and 2 weeks for Hubble!
Source: @Astropartigirl
It's a gravitational lens, showing us the light of galaxies that are far behind the cluster in arcs around it. I tried to orient them the same. LOOK AT THE DIFFERENCE.
12.5 hours of exposure for Webb and 2 weeks for Hubble!
Source: @Astropartigirl
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NASA, in partnership with ESA (European Space Agency) and CSA (Canadian Space Agency), will release the James Webb Space Telescope’s first full-color images and spectroscopic data during a live broadcast beginning at 14:30 UTC Tuesday, July 12, from NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
Released one by one, these first images from the world’s largest and most powerful space telescope will demonstrate Webb at its full power as it begins its mission to unfold the infrared universe.
Each image will simultaneously be made available on social media, as well as on the agency’s website at:
http://www.nasa.gov/webbfirstimages
📺 Join us for the stream and
💬 comment on the live broadcast here
Released one by one, these first images from the world’s largest and most powerful space telescope will demonstrate Webb at its full power as it begins its mission to unfold the infrared universe.
Each image will simultaneously be made available on social media, as well as on the agency’s website at:
http://www.nasa.gov/webbfirstimages
📺 Join us for the stream and
💬 comment on the live broadcast here
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EverythingScience
The image taken by the JWST compared to one taken by Hubble, of the galaxy cluster SMACS 0723. It's a gravitational lens, showing us the light of galaxies that are far behind the cluster in arcs around it. I tried to orient them the same. LOOK AT THE DIFFERENCE.…
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Canada’s instrument NIRISS on #Webb reveals the distinct signature of water 💧 in the atmosphere of a hot, puffy gas giant planet orbiting a distant Sun-like star. It also shows evidence of haze and clouds that previous studies of this planet did not detect. ☁
The spectrum captured by NIRISS isn’t only the most detailed of its kind to date, but it also covers a remarkably wide range of wavelengths, including a portion of the spectrum that has not previously been accessible from other telescopes.
This part of the spectrum is particularly sensitive to water as well as other key molecules like oxygen, methane, and carbon dioxide. Webb will play a significant role in the search for potentially habitable planets in the coming years.
Each of the 141 data points (white circles) on this graph represents the amount of a specific wavelength of light that is blocked by the planet and absorbed by its atmosphere.
Credits: NASA, ESA, CSA, STScI, and the Webb ERO Production Team
Source: @csa_asc
The spectrum captured by NIRISS isn’t only the most detailed of its kind to date, but it also covers a remarkably wide range of wavelengths, including a portion of the spectrum that has not previously been accessible from other telescopes.
This part of the spectrum is particularly sensitive to water as well as other key molecules like oxygen, methane, and carbon dioxide. Webb will play a significant role in the search for potentially habitable planets in the coming years.
Each of the 141 data points (white circles) on this graph represents the amount of a specific wavelength of light that is blocked by the planet and absorbed by its atmosphere.
Credits: NASA, ESA, CSA, STScI, and the Webb ERO Production Team
Source: @csa_asc
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Why do some of the galaxies in this image appear bent? The combined mass of this galaxy cluster acts as a “gravitational lens,” bending light rays from more distant galaxies behind it, magnifying them. The light from the farthest galaxy here traveled 13.1 billion years to us.
Source: @NASAWebb
Source: @NASAWebb
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Some stars go out with a bang. In these images of the Southern Ring planetary nebula, @NASAWebb shows a dying star cloaked by dust and layers of light.
Compare views of the Southern Ring nebula and its pair of stars by Webb’s NIRCam (L) & MIRI (R) instruments. The dimmer, dying star is expelling gas and dust that Webb sees through in unprecedented detail
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
Compare views of the Southern Ring nebula and its pair of stars by Webb’s NIRCam (L) & MIRI (R) instruments. The dimmer, dying star is expelling gas and dust that Webb sees through in unprecedented detail
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
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In Webb’s image of Stephan’s Quintet, we see 5 galaxies, 4 of which interact. (The left galaxy is in the foreground!)
Webb will revolutionize our knowledge of star formation & gas interactions in these galaxies
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
Webb will revolutionize our knowledge of star formation & gas interactions in these galaxies
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
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Galaxies collide in Stephan’s Quintet, pulling and stretching each other in a gravitational dance. In the mid-infrared view here, see how Webb pierces through dust, giving new insight into how interactions like these may have driven galaxy evolution in the early universe.
Source: @NASAWebb
Source: @NASAWebb
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🌟 A star is born!
Behind the curtain of dust and gas in these “Cosmic Cliffs” are previously hidden baby stars, now uncovered by Webb. We know — this is a show-stopper. Just take a second to admire the Carina Nebula in all its glory
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
Behind the curtain of dust and gas in these “Cosmic Cliffs” are previously hidden baby stars, now uncovered by Webb. We know — this is a show-stopper. Just take a second to admire the Carina Nebula in all its glory
http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse
Source: @NASAWebb
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The “Cosmic Cliffs” build on the legacy of Hubble’s imagery of the Carina Nebula, seen here. Webb’s new view gives us a rare peek into stars in their earliest, rapid stages of formation. For an individual star, this period only lasts about 50,000 to 100,000 years.
Source: @NASAWebb
Source: @NASAWebb
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Two cameras are better than one, as seen in this combined view from Webb’s NIRCam & MIRI! In the near-infrared, we see hundreds of stars and background galaxies. Meanwhile, the mid-infrared shows us dusty planet-forming disks (in red and pink) around young stars.
Source: @NASAWebb
Source: @NASAWebb
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Stephan's Quintet (NIRCam and MIRI Composite Image).png
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Stephan's Quintet (NIRCam and MIRI Composite Image)
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).
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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).
Low-res
Read More
Stephan's Quintet (MIRI Image).png
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Stephan's Quintet (MIRI)
With its powerful, mid-infrared vision, the Mid-Infrared Instrument (MIRI) shows never-before-seen details of Stephan’s Quintet, a visual grouping of five galaxies. MIRI pierced through dust-enshrouded regions to reveal huge shock waves and tidal tails, gas and stars stripped from the outer regions of the galaxies by interactions. It also unveiled hidden areas of star formation. The new information from MIRI provides invaluable insights into how galactic interactions may have driven galaxy evolution in the early universe.
Low-res
Read More
With its powerful, mid-infrared vision, the Mid-Infrared Instrument (MIRI) shows never-before-seen details of Stephan’s Quintet, a visual grouping of five galaxies. MIRI pierced through dust-enshrouded regions to reveal huge shock waves and tidal tails, gas and stars stripped from the outer regions of the galaxies by interactions. It also unveiled hidden areas of star formation. The new information from MIRI provides invaluable insights into how galactic interactions may have driven galaxy evolution in the early universe.
Low-res
Read More
Southern Ring Nebula (NIRCam Image).png
21.3 MB
Southern Ring Nebula (NIRCam)
The bright star at the center of NGC 3132, 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.
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The bright star at the center of NGC 3132, 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.
Low-res
Read More
“Cosmic Cliffs” in the Carina Nebula (NIRCam Image).png
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“Cosmic Cliffs” in the Carina Nebula (NIRCam)
Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away.
Low-res
Read More
—————————
Enjoy this high-resolution version of JWST's first set of images. We'll be covering future images and discoveries on this channel so stay tuned!
@EverythingScience
Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away.
Low-res
Read More
—————————
Enjoy this high-resolution version of JWST's first set of images. We'll be covering future images and discoveries on this channel so stay tuned!
@EverythingScience
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