Joined April 2009
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Beyond the Orion Nebula is a long and massive filament of cold gas and dust divided into four parts and collectively called the Orion Molecular Clouds. This image shows just a small portion of one of the clouds. esawebb.org/images/potm2605a…
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Go far and wide with @NASARoman! NASA’s next space telescope will be joining Webb in L2, a million miles away to join us and your name can come too! Get your boarding pass to send your name with Roman as we work to create the most complete picture of the universe yet: my.nasa.gov/specialevents/s/…
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NASA Webb Telescope retweeted
Have you ever wanted to have your name 'Roman' a million miles away? Now you can! Send your name along the Nancy Grace Roman Space Telescope, scheduled to launch Aug. 30, 2026! Sign up here: go.nasa.gov/4ejkRcR Submissions close July 12.
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Webb has delivered the strongest evidence yet that its discovery of mysterious Little Red Dots (LRD) are “black hole stars.” They appear starting ~600 million years after the big bang, and scientists are still working out exactly what they are. science.nasa.gov/missions/we…
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This gas accounts for why most LRDs are faint in X-rays; any X-rays given off are likely absorbed by the surrounding cocoons. More typical growing supermassive black holes are not embedded in dense gas, which allows UV light and X-rays from material orbiting them to escape.
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Ultimately this is one more piece of an ongoing puzzle discovered by, and potentially solvable by Webb.
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Beyond the Orion Nebula is a long and massive filament of cold gas and dust divided into four parts and collectively called the Orion Molecular Clouds. This image shows just a small portion of one of the clouds. esawebb.org/images/potm2605a…
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Every stage of star formation — from the youngest stellar embryos, to protoplanetary discs, to newly-minted pre-main sequence stars — is contained within just this scene (captured by Webb’s Near-Infared Camera) which stretches 150 light-years across.
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Webb is looking at the chemical fingerprints of interstellar comet 3I/ATLAS in the mid-infrared 🔎 New data points to a very different formation environment and chemistry for this object compared to most comets that formed in our own solar system. science.nasa.gov/blogs/3iatl…
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Which came first, galaxies or black holes? New Webb observations show that some supermassive black holes were enormous from their beginnings, shifting traditional ideas around how black holes form and grow. go.nasa.gov/4vaEASC
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NASA Webb Telescope retweeted
Westerlund 2 is a young cluster of thousands of stars located about 20,000 light-years from Earth. This close-up image, roughly 12 light-years across, combines observations from NASA's Chandra X-ray Observatory & @NASAWebb.✨
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NASA Webb Telescope retweeted
At the heart of galaxy NGC 1365, a supermassive black hole is basically feasting at an all‑you‑can‑eat buffet in this image from Chandra and @NASAWebb. Located about 60 million light-years from Earth, this gobbling black hole has a mass of roughly 2 million suns... and growing.⚫
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NASA Webb Telescope retweeted
There is a massive black hole in the center of almost every galaxy. How did it get there, and importantly, how does it grow? On May 19, we'll discuss what new #NASAWebb data is driving the biggest tensions in our understanding of the black hole phenomenon. youtube.com/live/KIMhXF-heAw…
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To MoM-z14 & back! 💐 Let a caregiver in your life know your appreciation for them reaches the farthest galaxy ever detected! Read more about MoM-z14: go.nasa.gov/4d1kt3l
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Don’t let anyone dull your shine 💫 The heart of galaxy M77 nearly outshines the galaxy itself in this mid-infrared Webb image. Gas rapidly orbits the central black hole, heating up, and radiating light. esawebb.org/images/potm2604a…
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This image is a composite of both mid and near infrared. The bright orange lines radiating out of the center are diffraction spikes. They aren't a physical feature of the galaxy, but an optical effect caused by the structure of the telescope.
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Light can bend (or be diffracted) around the edges of the telescope primary mirror and the struts that hold the secondary mirror. Bright objects in Webb images show a distinctive six-plus-two-pointed pattern. Hubble's have 4 point diffraction spikes due to its structure.
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