🌌 Cosmic Dance Unveiled! 🌌
Meet Stephan's Quintet: a spectacular galactic group where four galaxies sway together, 290 million light-years away, while a fifth, NGC 7320, glides closer at just 40 million light-years. Thanks to the James Webb Space Telescope, we now see this cosmic ballet in stunning clarity—a mosaic of 150 million pixels showing young stars, shock waves, and swirling gas trails!
But it’s not just eye candy. Webb’s insights into the supermassive black hole in NGC 7319 are rewriting what we know about galaxy evolution and black hole behavior. Discover the wonders hidden in Stephan’s Quintet! ✨ #JamesWebb #StephansQuintet
Today marks the one-year anniversary of a mind-blowing discovery made by the James Webb Space Telescope, and brace yourselves, it's like something straight out of a sci-fi flick! 🌠
🔭 Last year, on November 17, 2022, the Webb telescope, with its super cosmic detective skills, unveiled the outer reaches of the colossal galaxy cluster Abell 2744, dropping a jaw-dropping bombshell – the revelation of two of the most distant galaxies ever spotted!
📸 Feast your eyes on the awe-inspiring image captured by NASA, ESA, CSA, and the brilliant mind of Tommaso Treu (UCLA), with a touch of magic in image processing by Zolt G. Levay (STScI). 🌌✨
🌟 These two cosmic wonders were found between 350 and 450 million years after the big bang. Imagine, just a blink in the vast timeline of our universe! 🕰️ Astronomers are scratching their heads because these galaxies, though smaller than our Milky Way, are shining brighter than your favorite star. 💫✨ They're like the rockstars of the early galaxy scene, converting gas into stars at a mind-boggling rate!
🔍 Webb's gaze has revealed a hidden universe, where the first galaxies are throwing a celestial party, quite different from the mature galaxies we're used to. 🎉💫 It seems the stellar birth began only 100 million years after the big bang, opening our eyes to a cosmic cradle of creation.
In just four days of processing, Webb managed to snatch a glimpse of these elusive early galaxies, previously unseen by any other telescope. 🚀 Imagine what wonders await as we delve deeper into the cosmos!
🔍 Stay tuned for the unfolding cosmic drama as Webb continues to unravel the mysteries of our universe! 🚀🔭✨ #WebbTelescope #GalacticRevelations #CosmicExploration #LostInSpace #SpaceWonders
Read what scientists thinks will most likely happen - James Webb Discovery - If betelgeuse goes supernova will it affect earth ?
NASA's Chandra X-ray Observatory and James Webb Space Telescope have delivered breathtaking composite images showcasing the beauty of two galaxies, a nebula, and a star cluster. These images, which combine X-rays from Chandra and infrared data from Webb, provide a mesmerizing glimpse into the hidden wonders of the universe.
Invisible to the unaided eye, the X-rays captured by Chandra and the infrared data obtained by Webb are transformed into vibrant colors that humans can perceive. To create these stunning composite images, NASA also incorporated data from other powerful telescopes, including the Hubble Space Telescope, the retired Spitzer Space Telescope, the European Space Agency's XMM-Newton, and the European Southern Observatory's New Technology Telescope.
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Read full article here
🚨 Breaking Space News! 🚨 NASA's James Webb Space Telescope has just revealed mind-blowing details about Jupiter's Great Red Spot! 🌌🔭 The upper atmosphere, once thought to be dull, is bursting with intricate structures and mysterious waves. 🌪️✨
Explore the cosmic secrets uncovered by JWST! -> https://www.jameswebbdiscovery.com/discoveries/jupiters-upper-atmosphere-mysteries-unlocked-by-james-webb-telescope
#Space #NASA #JamesWebb #Jupiter #GreatRedSpot #Astronomy #Discovery #ScienceNews #CosmicWonders
New Image from James Webb Telescope release today! Learn more..
Webb observes galaxy cluster RX J2129 triply lens supernova hosting galaxy
NASA's James Webb Space Telescope has begun the study of one of the most renowned supernovae, SN 1987A (Supernova 1987A). Located 168,000 light-years away in the Large Magellanic Cloud, SN 1987A has been a target of intense observations at wavelengths ranging from gamma rays to radio for nearly 40 years, since its discovery in February of 1987. New observations by Webb's NIRCam (Near-Infrared Camera) provide a crucial clue to our understanding of how a supernova develops over time to shape its remnant.
This image reveals a central structure like a keyhole. This center is packed with clumpy gas and dust ejected by the supernova explosion. The dust is so dense that even near-infrared light that Webb detects can't penetrate it, shaping the dark "hole" in the keyhole.
A bright, equatorial ring surrounds the inner keyhole, forming a band around the waist that connects two faint arms of hourglass-shaped outer rings. The equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots, which appeared as the supernova's shock wave hit the ring. Now spots are found even exterior to the ring, with diffuse emission surrounding it. These are the locations of supernova shocks hitting more exterior material.
While these structures have been observed to varying degrees by NASA's Hubble and Spitzer Space Telescopes and Chandra X-ray Observatory, the unparalleled sensitivity and spatial resolution of Webb revealed a new feature in this supernova remnant—small crescent-like structures.
These crescents are thought to be a part of the outer layers of gas shot out from the supernova explosion. Their brightness may be an indication of limb brightening, an optical phenomenon that results from viewing the expanding material in three dimensions. In other words, our viewing angle makes it appear that there is more material in these two crescents than there actually may be.
The high resolution of these images is also noteworthy. Before Webb, the now-retired Spitzer telescope observed this supernova in infrared throughout its entire lifespan, yielding key data about how its emissions evolved over time. However, it was never able to observe the supernova with such clarity and detail.
Despite the decades of study since the supernova's initial discovery, there are several mysteries that remain, particularly surrounding the neutron star that should have been formed in the aftermath of the supernova explosion. Like Spitzer, Webb will continue to observe the supernova over time.
Its NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) instruments will offer astronomers the ability to capture new, high-fidelity infrared data over time and gain new insights into the newly identified crescent structures. Further, Webb will continue to collaborate with Hubble, Chandra, and other observatories to provide new insights into the past and future of this legendary supernova.
TOP IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A). At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
LOWER IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A), which has been annotated to highlight key structures. At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
NASA’s James Webb Space Telescope has captured a breathtaking image of Uranus, the solar system's ice giant. This impressive image shows Uranus' dramatic rings and bright features in its atmosphere. The sensitivity of Webb's data has allowed the observatory to detect even the faintest dusty rings, a feat that has only been accomplished by two other facilities: Voyager 2 spacecraft and the Keck Observatory. Read full article here -
Never miss another James Webb Discovery. Tracking all the amazing discoveries made by the James Webb Space Telescope at https://www.jameswebbdiscovery.com, Follow now!
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