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The Official *NASA* Webb X account. The world's most powerful space telescope. Launched: Dec. 25, 2021. First images revealed: July 12, 2022.

Lagrange Point 2
Joined April 2009
Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)Photo by NASA Webb Telescope (@NASAWebb)
This July was our 4th science anniversary, and the results have been fascinating! Bringing us previously unseen details from all throughout the universe to right here in our own solar system, Webb has given scientists, and the world, a powerful new set of tools.
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Happy Halloween! 👻 Like a spectral form rising out of a cold mist, @NASAHubble and Webb have captured a hauntingly dynamic star-forming scene, which lies within the vast Carina Nebula, a diffuse star-forming region located about 7,500 light-years away from Earth.
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The small, select area both telescopes observed is nicknamed the Cat’s Head Nebula because of its resemblance to a cat sitting with its back toward the viewer. The “head” of the cat is turned to the right, revealing a glowing eye.
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Pspspsp! Just in time for Halloween, NASA’s Hubble and James Webb Space Telescopes recently stared at an eerie star-forming scene within the Carina Nebula, a massive gas and dust cloud located approximately 7,500 light-years away from Earth.
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Rest easy, Captain. We have the helm. ✨ This is Webb’s look at Westerlund 1, a super star cluster. Because our galaxy is past its peak of star formation, and because stars live relatively short lives, only a few of these clusters exist to give us clues to that past era.
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Note for clarity: "because such stars live relatively short lives..." Massive stars are relatively short-lived.
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Replying to @NASAHubble
@NASAHubble and @NASAWebb captured a purr-fect view of the Cat’s Head Nebula. This long thin structure, made of dark, dense dust, looks like the head of a cat, its eye a newborn star still shrouded by the dust and gas from which it formed. science.nasa.gov/missions/hu…
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Double, double toil and trouble; Fire burn and cauldron bubble 🧙‍♀️ This turbulent cauldron of star formation, N159, resides about 161,000 light years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting our Milky Way. esawebb.org/images/potm2610a…
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This region has a lower metallicity (proportion of elements that are heavier than helium and hydrogen) than our Milky Way, revealing more about how stars formed in the conditions of the early universe.
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Fast radio bursts (FRBs) - enigmatic, millisecond-long flashes of radio emission from the distant universe - were first discovered in 2007. Their origins are difficult to pinpoint, but Webb found the host galaxy to the most distant FRB seen to date. go.nasa.gov/4emggqZ
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Happy World Space Week! If you're searching up space facts today, you might run into our newest image! 👇 Google.com
Brewing up new stars 🪄 Webb’s unique view of the stellar nursery known as NGC 7129 reveals numerous stars formerly hidden in this cosmic cauldron, helping astronomers study the star lifecycle in more depth. go.nasa.gov/4y9abFE
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Brewing up new stars 🪄 Webb’s unique view of the stellar nursery known as NGC 7129 reveals numerous stars formerly hidden in this cosmic cauldron, helping astronomers study the star lifecycle in more depth. go.nasa.gov/4y9abFE
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They say planet formation’s a cruel endeavor Violent collisions, like that between a proto-Earth and a Mars-sized object named Theia 4.5 billion years ago, shaped our home planet. Webb is helping compare other young stellar systems to our own. go.nasa.gov/4rL1UpN
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As a star ages, its environment changes. Material in its gas-rich protoplanetary disk form planetesimals, which can then create planets and moons, eventually leaving a gas-poor disk of debris analogous to the debris in our own solar system's asteroid and Kuiper belt.
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Seeing double… or quadruple! 👀 In this Webb image of galaxy cluster MACS J0454.1-0300, gravitational lensing shows us 4 or more images of the same galaxy. This is the first time researchers have spotted this more than once in the same galaxy cluster! esawebb.org/images/potm2609a…
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The brilliant golden galaxies visible in this image make up galaxy cluster MACS J0454.1-0300, but the orange galaxies are much farther away. Gravitational lensing occurs in this image due to the enormous mass of those golden galaxies. They bend and magnify the flight of the more distant orange galaxies.
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Free downloadable mini poster of Webb's look at Centaurus A! science.nasa.gov/asset/webb/…
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Within this star-forming nebula (captured by Webb) are the smallest brown dwarfs ever detected. Neither planet nor star, these objects are formed like stars, raising questions about the star formation process. go.nasa.gov/4y7RVwU
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Adding to their strangeness, one of these tiny brown dwarfs showed signs of a disk, suggesting small planets could be forming around an object that itself is only the mass of a planet.
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Scientists used Webb and @NASAHubble to study some of the most far-flung bodies in our solar system, Trans-Neptunian Objects, unexpectedly finding that the number and colors followed the same relationships as their larger family members. More: go.nasa.gov/4drPY6e
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“Being a star just means that you just find your own special place and that you shine where you are.” - Dolly Parton ✨ An irregular galaxy might seem like an odd place for so many new stars to shine, yet multitudes are forming within the gas that crowds Arp 263.
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It is thought that the irregular appearance of Arp 263 is actually due to a galactic merger. Galactic mergers cause gas and dust to crash together, and that process creates stars.
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How close is too close to a black hole? Asking for a friend. 😬 Webb just revealed dust and water surviving in the extreme environment of a star located near our Milky Way's supermassive black hole, Sagittarius A*! esawebb.org/images/weic2617d…
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IRS 3 is a star near the end of its life cycle, located just over half a light year away from Sgr A*. Similar huge, cool, luminous stars shed dust-producing gas with their powerful stellar winds. But do stars so close to a supermassive black hole produce dust?
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What animal do you see in this Webb image?! A bird? An elephant? A giraffe? Let your imagination run wild! This is Webb’s infrared view of part of the Carina Nebula, a star-forming region also home to the Cosmic Cliffs, which was one of the first images released by Webb.
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Here Webb captures a different aspect of Carina, a feature called the “Treasure Chest,” which is an object known as a cometary globule. A cometary globule is an isolated cloud of gas and dust with a dense, dark head and a sweeping tail.
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It's the circle of life… Webb's look at the Lion Nebula, the remains of a dying lower-mass star, is in both the mid and near-infrared. Though massive stars undergo supernova explosions at the end of their lives, lower-mass stars shed their outer layers.
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In the Lion Nebula’s case, its white dwarf is “cooking” everything from the inside and producing a bubble of ionized gas as it does. The gas bubble, which forms the lion’s face, is expanding over time and destroying dust that is in its path.
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Technical Trivia: Which of these techniques involve placing a specially designed mask with several small pinholes in the light path through a telescope? A: Coronagraphy B: Aperture masking interferometry C: Integral Field Unit Spectroscopy D: Multi-Object Spectroscopy
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B is correct, aperture masking interferometry! This observational technique allowed science teams to make detailed and unique observations of the massive binary star system Wolf-Rayet 137; PDS 70, a young, Sun-like star; and Jupiter’s moon Io. go.nasa.gov/4pVLXvO
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Who doesn't love a good mystery?! 🔍🔴 Little Red Dots (LRD), first detected by Webb, are very distant, seemed to emerge ~600 million years/mysteriously decline by ~1.5 billion years post-big bang. What if they didn’t disappear, they just evolved? go.nasa.gov/4h44W5g
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Researchers used Webb (infrared), Hubble (ultraviolet), and Chandra (X-rays) to look at a spiral galaxy that existed 3.3 billion years after the big bang with a Little Red Dot-like center. The galaxy’s central compact object fits the criteria for an LRD though it is nearer-by.
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