Mission Operations Center for NASA's Webb Space Telescope. Also operating the Hubble Space Telescope and the upcoming Roman Space Telescope. We help humanity explore the universe with advanced space telescopes and ever-growing data archives.
Unique, twisting dust lanes are prominent in this Hubble image—an edge-on view of lenticular galaxy NGC 4753. That dust likely was pulled in during a merger with a dwarf galaxy more than 1 billion years ago.
Credit: NASA, ESA, and L. Kelsey. 🔭 🧪
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This region, called G35.2-0.7N, is a hotbed of high-mass star formation. Much of this nebula is dark and dusty. However, massive jets, like the one that is launching toward us, pierce through the darkness, giving us a view inside.
Credit: ESA/Hubble & NASA, R. Fedriani, J. Tan. 🔭 🧪
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"Hubble isn't just a satellite; it's about humanity's quest for knowledge."
— John M. Grunsfeld, NASA astronaut who worked on the Hubble Space Telescope 🔭 🧪
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Watch as STScI’s Dr. Frank Summers explores the Pillars of Creation in three dimensions with a brand-new visible and infrared fly-through visualization—TODAY at 8:00 p.m. ET. 🔭 🧪
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This image of L1527 was taken by #NASAWebb in mid-infrared. The protostar in this image is tiny. It resides in the red center at less than a pixel in size, but the white areas above and below it show just how much dust it stirs as it develops: webbtelescope.pub/4bxsqcm 🔭 🧪
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Happy Canada Day! Canadian scientists are taking part in the James Webb Space Telescope's exciting science mission that promises to change our understanding of the universe. 🔭 🧪
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In July, look to Scorpius to find Antares, one of the largest known stars, and globular star cluster M4. Stay tuned for space-based images of the Swan and Trifid nebulas. And mark your calendar for the Delta Aquarid meteor shower.
Watch “Tonight’s Sky.” 🔭 🧪
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The Coma Cluster acts as a database for studies of galaxy evolution. The center, shown here, contains mostly elliptical galaxies. Outside of the center, lenticular and spiral galaxies become relatively more common.
Explore these types of galaxies: bit.ly/3wsBzok 🔭 🧪
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Watch the full video of the Pillars of Creation and download the 3D printer file. (7/7) 🔭 🧪
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A bonus product from this visualization is a new 3D printable model of the Pillars of Creation. The base model of the four pillars used in the visualization has been adapted to the STL file format so that viewers can download the model file and print it out on 3D printers. (6/7)
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Hubble sees objects that glow in visible light, at thousands of degrees. Webb's infrared vision, which is sensitive to cooler objects with temperatures of just hundreds of degrees, pierces through obscuring dust to see stars embedded in the pillars. (5/7)
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The movie takes visitors into the three-dimensional structures of the pillars. Rather than an artistic interpretation, the video is based on observational data. The visualization helps viewers experience how two of the world's most powerful space telescopes work together. (4/7)
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The four Pillars of Creation, made primarily of cool molecular hydrogen and dust, are being eroded by the fierce winds and punishing ultraviolet light of nearby hot, young stars. Finger-like structures larger than the solar system protrude from the tops of the pillars. (3/7)
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This is the most comprehensive, detailed, multiwavelength movie yet of these iconic star-birthing clouds. Pillars of Creation in the heart of the Eagle Nebula have captured imaginations worldwide with their arresting, ethereal beauty since 1995. (2/7)
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Combining data from the Hubble and James Webb space telescopes, a team from NASA's Universe of Learning at STScI has produced a breathtaking new 3D visualization of the towering "Pillars of Creation" in the Eagle Nebula. (1/7)
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On Tuesday, Dr. Frank Summers will detail the features of the Pillars of Creation, which involves the interplay of stars and dust, and explain the knowledge gained through multiwavelength observations from Hubble and #NASAWebb. 🔭 🧪
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Over 12 billion years. More than 7,500 galaxies. One telescope.
Hubble captured galaxies in various stages of assembly throughout most of the history of the universe.
Click to explore: bit.ly/4bnEjC0 🔭 🧪
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NEW: Wind through the iconic Pillars of Creation, switching between Hubble’s visible-light observations and #NASAWebb’s infrared view, and see how they are being eroded by the fierce winds of nearby hot, young stars.
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Take the tour of the Pillars of Creation with NASA’s Universe of Learning! Move through the three-dimensional structures of the pillars. Rather than an artistic interpretation, the video is based on observational data from telescopes. 🔭 🧪
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This video tours the Serpens Nebula, a star-forming region that lies 1,300 light-years away from Earth.
A new image of Serpens from #NASAWebb shows an intriguing group of aligned protostellar outflows within one region of the nebula.
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Us looking at NGC 3351: 👁️ 👄 👁️
NGC 3351: 👁️
This barred spiral galaxy is located about 33 million light-years away in the constellation Leo. #NASAWebb took this face-on image of NGC 3351, revealing the spindly structure of the galaxy’s gas and dust: bit.ly/4a9q4zQ 🔭 🧪
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Our face-on view of spiral galaxy NGC 1015 gives the perfect perspective to appreciate its central bulge, bar, and ring of stars. Scientists snapped this image with Hubble in 2013 to study a type of exploding star, or supernova.
Credit: NASA, ESA, and A. Riess (STScI/JHU). 🔭 🧪
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Need to reset? Trace the diffuse brown pillars in Hubble’s image of star-forming region Westerlund 2. Each pillar is a few light-years tall. For context, one light-year is about 6 trillion miles (9 trillion kilometers).
Credit: NASA, ESA, STScI. 🔭 🧪
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Spot the difference with Hubble! These 2020 images compare Jupiter in visible light at left, and with ultraviolet and near-infrared light added on the right, giving scientists insight into the planet’s huge storms.
Discover more: hubblesite.org/contents/med... 🔭 🧪
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NGC 1277 has long since stopped forming new stars. The telltale signs lie in the globular clusters around it. It is surrounded by reddish clusters, which hold older star populations, while younger, blue star clusters are absent.
Read about its history: bit.ly/4a9QbH0 🔭 🧪
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It’s summer! Temps are high, school is out, pools are open, grills are stoked—and the earth’s tilt is in place. What does ‘summer solstice’ mean, and is it really the longest day of the year? Baltimore's WYPR asks our Kelly Lepo to break it down. 🔭 🧪 ☀️
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In the Webb image, these jets are signified by bright clumpy streaks that appear red, which are shockwaves from the jet hitting surrounding gas and dust. Here, the red color represents the presence of molecular hydrogen and carbon monoxide. (7/7) 🔭 🧪
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A disk of material forms around the young star to transport material down, like a whirlpool around a drain. The swirling magnetic fields in the inner disk launch some of the material into twin jets that shoot outward in opposite directions. (6/7)
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As an interstellar gas cloud crashes in on itself to form a star, it spins more rapidly. The only way for the gas to continue moving inward is for some of the spin (known as angular momentum) to be removed. (5/7)
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“Astronomers have long assumed that as clouds collapse to form stars, the stars will tend to spin in the same direction,” said @NASAJPL’s Klaus Pontoppidan. “These aligned, elongated structures are a historical record of the fundamental way that stars are born.” (4/7)
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Here, however, they are slanted in the same direction, to the same degree, like sleet pouring down during a storm. The discovery of these aligned objects is providing information into the fundamentals of how stars are born. (3/7)
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Astronomers found an intriguing group of protostellar outflows, formed when jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds. Typically, these objects have varied orientations within one region. (2/7)
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For the first time, a phenomenon astronomers have long hoped to directly image has been captured by #NASAWebb’s Near-Infrared Camera. In this stunning image of the Serpens Nebula, the discovery lies in the upper left of this image—a young, nearby star-forming region. (1/7) 🔭 🧪 🧵
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Watch our view of the Serpens Nebula transform as it’s observed in different wavelengths of light and different resolutions: Hubble’s visible light view, Spitzer’s infrared look, and #NASAWebb’s crisp near-infrared image: webbtelescope.pub/3Vmca9d 🔭 🧪
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FS Tau was recently observed by Hubble, showing us the blue jets streaming out from the newly formed FS Tau B, the star on the far right that is hidden by a tiny vertical line of dust. The bright object in the center is two stars closely orbiting each other. Credit: NASA, ESA. 🔭 🧪
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What's going on with Cassiopeia A? How did this star tear itself apart? What does it tell us about how the elements for life in the universe came to be?
Learn more about this dynamic dead star, the target for this season of NASA's #AstrophotoChallenge: mo-www.cfa.harvard.edu/OWN/astropho... 🔭 🧪
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One way of observing exoplanets is by blocking out their stars’ light. Space telescopes like Hubble and Webb use devices inside the observatory to do this, known as coronagraphs, allowing telescopes to see dimmer exoplanets, as shown in this animation. Credit: NASA. 🔭 🧪
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What have we learned about the Crab Nebula with #NASAWebb? More than just a pinch! 🦀
With the data:
• Astronomers are closer to understanding the origins of this supernova remnant.
• Some of the Crab’s main components have been mapped in isolation. webbtelescope.pub/3XwLGDL 🔭 🧪
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"Symbiotic stars like HM Sge are rare in our galaxy, and witnessing a nova-like explosion is even rarer. This unique event is a treasure for astrophysicists spanning decades," said STScI’s Steven Goldman. (5/5) 🔭 🧪
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Its presence shows that the estimated temperature of the white dwarf and accretion disk increased from less than 400,000 degrees Fahrenheit in 1989 to greater than 450,000 degrees Fahrenheit now. (4/5)
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The latest Hubble ultraviolet observations show that the binary system has gotten hotter. A strong emission line of highly ionized magnesium that was not present in earlier published spectra from 1990 appeared in 2021 data. (3/5)
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New data from Hubble and the retired SOFIA observatory was used to revisit HM Sagittae, one of the strangest binary star systems in our galaxy—40 years after it burst onto the scene as a bright and long-lived nova. (2/5)
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A strange event happened in 1975, when a nova called HM Sagittae grew 250 times brighter as it ingested gas from a bloated red giant companion it is orbiting. It never really faded away as novas commonly do, but has maintained its brightness for decades. (1/5) 🧵 🔭 🧪
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“We are trying to identify whether distant supernovae are fundamentally different from or very much like what we see in the nearby universe,” said Justin Pierel, a NASA Einstein Fellow at STScI. (5/5) 🔭 🧪
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Astronomers compared multiple images taken up to one year apart and looked for sources that disappeared or appeared in those images. In all, they uncovered about 80 supernovas in a patch of sky only about the thickness of a grain of rice held at arm’s length. (4/5)
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Previously, researchers used Hubble to view supernovas from when the universe was in the "young adult" stage. With JADES, scientists are seeing supernovas when the universe was in its “teens” or “pre-teens.” (3/5)
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To make these discoveries, the team analyzed imaging data obtained as part of the JWST Advanced Deep Extragalactic Survey (JADES) program. Webb is ideal for finding extremely distant supernovae because their light is stretched into longer wavelengths. (2/5)
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Supernovas can’t hide from #NASAWebb. Using data from a deep Webb survey of the early universe, astronomers have identified 10 times more far-off supernovae than were previously known. (1/5) 🧵 🔭 🧪
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Dr. Macarena Garcia Marin speaks to the gathered scientists about the James Webb Space Telescope at the American Astronomical Society annual meeting in Madison, Wisconsin, today. #AAS244 #NASAWebb 🔭 🧪
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"Beta Pictoris is at an age when planet formation in the terrestrial planet zone is still ongoing through giant asteroid collisions, so what we could be seeing here is basically how rocky planets and other bodies are forming in real time." — STScI's Christine Chen 🔭 🧪
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