In the News

Galaxy pair Arp 143 contains distorted star-forming spiral galaxy NGC 2445 (right) with lots of young bright blue stars and several pink star-forming regions. The less flashy companion galaxy NGC 2444 (left) glows soft yellow with a wispy distorted loop.

For the first time, STScI served as the news office for two operating NASA flagship missions.

About This Article

With two world-class observatories doing amazing science, it is difficult to choose just a few news-making discoveries to highlight. In its first six months of science operations, NASA’s James Webb Space Telescope made more than 38,000 observations, while NASA’s Hubble Space Telescope has racked up 1.5 million over the course of its nearly 33-year career. Together, the dynamic space duo is opening up the universe, and our sense of wonder, all over again. Revisit some of their 2022 news highlights below. 

 

NOVEMBER 2022 ׀ WEBB

NASA's Webb Draws Back Curtain on Universe's Early Galaxies

Graphic titled “Abell 2744 GLASS; JWST/NIRCam,” with two large square images, one on the left and one on the right, and two smaller images in between, one stacked above the other. The small images are zoom-ins that show details in the large images. The large image on the left shows many galaxies of different colors, shapes, and sizes, and several bright foreground stars. On the left side is a box around a galaxy, labeled “1,” which zooms in to a red galaxy shown in the top small center pullout image. Pullout image 1 is labeled “z ~ 10.5” to indicate that the galaxy’s redshift is roughly 10.5. The image on the right also shows many galaxies of different colors, shapes, and sizes, but without any prominent diffraction spikes seen in the left image. It includes a box on the left side, labeled “2,” which zooms into a red galaxy, shown in the bottom center image. Pullout image 2 is labeled “z ~ 12.5” to indicate that the galaxy’s redshift is roughly 12.5.Just days after officially starting science operations, Webb found an unexpectedly rich “undiscovered country” of early galaxies that has been largely hidden until now. Webb is unveiling the first forming galaxies, which look remarkably different from the mature galaxies seen around us today. With just four days of analysis, researchers found two exceptionally bright galaxies that existed approximately 450 and 350 million years after the big bang (with redshifts of approximately 10.5 and 12.5, respectively). The initial findings are from a broader Webb research initiative involving two Early Release Science (ERS) programs: the Grism Lens-Amplified Survey from Space (GLASS), and the Cosmic Evolution Early Release Science Survey (CEERS). Discover the early universe with Webb.

 

OCTOBER 2022 ׀ WEBB

NASA’s Webb Takes Star-Filled Portrait of Pillars of Creation

Cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.With its Near-Infrared Camera, Webb delivered the most detailed near-infrared-light image ever captured of the iconic Pillars of Creation in the Eagle Nebula. This is a region where young stars are forming, or have barely burst from their dusty cocoons as they continue to form. Webb’s new view will help researchers revamp their models of star formation by identifying far more precise counts of newly formed stars, along with the quantities of gas and dust in the region. Over time, they will begin to build a clearer understanding of how stars form and burst out of these dusty clouds over millions of years. View the Pillars of Creation like never before.

 

SEPTEMBER 2022 ׀ HUBBLE AND WEBB

Webb, Hubble Capture Detailed Views of DART Impact

Two images side by side: At left, a photo with a black background and a bright blue spot at the center, labeled as Hubble. There is a bright haze around the dot, which is the Didymos-Dimorphos system, along with 5 diffraction spikes extending outward. The photo on the right is a black background with a bright red spot toward the middle of the image. The spot, which is the asteroid the Didymos-Dimorphos system after impact from DART, has 8 diffraction spikes extending out from its center. Also surrounding the asteroid is a haze of bright light with wispy tendrils extending outward.In September 2022, Webb and Hubble teamed up in their first collaborative observation of the same celestial target. The target itself was another first: a unique NASA experiment, the Double Asteroid Redirection Test (DART), humanity's first-ever in-space test for planetary defense. The DART spacecraft intentionally slammed into Dimorphos, the asteroid moonlet in the double-asteroid system of Didymos, at nearly 15,000 miles per hour.

Both Webb and Hubble observed the asteroid before and after the collision took place. They captured the impact in different wavelengths of light, Webb in infrared and Hubble in visible. Scientists are using the combined observations to learn about the surface of Dimorphos, how much material was ejected by the collision, how fast it was ejected, and the distribution of particle sizes in the expanding dust cloud. The telescopes' combined capabilities will also allow scientists to analyze a wide array of data relating to the makeup and history of our solar system. “Webb and Hubble show what we’ve always known to be true at NASA: We learn more when we work together,” said NASA Administrator Bill Nelson. Read more about Hubble and Webb’s first joint effort.

 

SEPTEMBER 2022 ׀ WEBB

New Webb Image Captures Clearest View of Neptune’s Rings in Decades

Mostly dark background with one extremely bright point of light that dominates the upper left quadrant of the image and a glowing sphere, which is the planet Neptune, toward the bottom middle of the image. The extremely bright point of light, which is Neptune’s moon Triton, at the upper left of the image has 8 spikes pointing out from a center bright point like a compass. Neptune is mostly white with a few extremely bright patches representing methane-ice clouds. The planet is accompanied by several narrow, faint rings and 6 tiny white dots, which are Neptune's moons. Splattered throughout the mostly black background are about 10 small, dim, blurry circles are distant galaxies.Webb captured the clearest view of Neptune’s rings in more than 30 years and revealed the ice giant in a whole new light. Webb’s Near-Infrared Camera images objects in the near-infrared range from 0.6 to 5 microns, so Neptune does not appear blue to Webb. Methane-ice clouds are prominent as bright streaks and spots. In addition to several bright, narrow rings, Webb’s precise image quality clearly shows Neptune’s fainter dust bands.

Webb also captured seven of Neptune’s 14 known moons. The largest moon, Triton, dominates the image as a very bright point of light sporting Webb’s signature diffraction spikes. Covered in a frozen sheen of condensed nitrogen, Triton reflects an average of 70 percent of the sunlight that hits it. It far outshines Neptune in this image because the planet’s atmosphere is darkened by methane absorption at these near-infrared wavelengths. See Neptune in a new light with Webb.

 

AUGUST 2022 ׀ WEBB

NASA’s Webb Detects Carbon Dioxide in Exoplanet Atmosphere

Graphic titled “Hot Gas Giant Exoplanet WASP-39 b Atmosphere Composition, NIRSpec Bright Object Time-Series Spectroscopy.” The graphic shows the transmission spectrum of the hot gas giant exoplanet WASP-39 b captured using Webb's NIRSpec Bright Object Time-Series Spectroscopy mode, with an illustration of the planet and its star in the background. The data points are plotted as white circles with grey error bars on a graph of amount of light blocked in percent on the vertical y axis versus wavelength of light in microns on the horizontal x axis. The y axis ranges from 2.00 percent (less light blocked) to 2.35 percent (more light blocked). The x axis ranges from 3.00 microns to 5.6 microns. A curvy blue line represents a best-fit model. One broad, prominent peak visible in the data and model is labeled “Carbon Dioxide, C O 2.” The carbon dioxide peak is centered around 4.3 microns and has a y value of between 2.25 and 2.30 percent of light blocked. The baseline is between 2.10 and 2.17 percent.Webb ushered in a new era of exoplanet science with the first unequivocal detection of carbon dioxide in a planetary atmosphere outside our solar system. The research team used Webb’s Near-Infrared Spectrograph to observe the hot gas-giant planet WASP 39 b, which orbits a Sun-like star 700 light-years away. No observatory has ever measured such subtle differences in brightness across the 3 to 5.5-micron range of light in an exoplanet transmission spectrum before. Access to this part of the electromagnetic spectrum is crucial for measuring abundances of gases like water and methane, as well as carbon dioxide, which are thought to exist in many different types of exoplanets. This early discovery with Webb holds promise for the future study of a wide variety of exoplanets, including smaller, cooler, rocky planets, providing insights into the composition, formation, and evolution of planets across the galaxy. Learn more about this groundbreaking discovery.

 

AUGUST 2022 ׀ HUBBLE

Hubble Sees Red Supergiant Star Betelgeuse Slowly Recovering After Blowing Its Top

This illustration plots changes in the brightness of the red supergiant star Betelgeuse. The top third shows four illustrations of the star, which is various shades of orange. From left to right: the illustration, labeled Jan-Mar 2019, shows a bright region at its southern point; Sept-Nov 2019 shows the bright region becoming larger and circular, but still connected to the star; Jan-Feb 2020 shows what looks like a dark brown cloud of gas extending just beyond the bottom left of where the bright region was; March 2020 shows no ejection, and a blurred star. At the bottom, the chart maps Change in Brightness on the y-axis and Time on the x-axis. A dotted blue line is labeled, predicted 400-day brightness, following a regular wave pattern. A continuous red line, which appears only periodically, is irregular and does not follow the predicted dotted line.Based on data from Hubble and other observatories, astronomers concluded that the bright red supergiant star Betelgeuse quite literally blew its top in 2019, losing a substantial part of its visible surface and producing a gigantic surface mass ejection. This is something never before seen in a normal star's behavior. Betelgeuse blasted off 400 billion times as much mass as a routine ejection by the Sun. These new observations yield clues as to how red stars lose mass late in their lives as their nuclear fusion furnaces burn out, before exploding as supernovae. However, Betelgeuse's behavior is not evidence the star is about to blow up anytime soon. "It's a totally new phenomenon that we can observe directly and resolve surface details with Hubble. We're watching stellar evolution in real time," said astronomer Andrea Dupree. Keep reading about Betelgeuse.

 

JULY 2022 ׀ WEBB

NASA Reveals Webb Telescope’s First Images of Unseen Universe

Illustration representing Webb science. The background is deep blue with scattered points of light of different size and brightness. Running from left to right through the middle is a jagged line representing a light spectrum (a graph of brightness versus wavelength of light). The area below the spectrum has a rainbow pattern from red on the left to purple on the right. The coloring is semi-transparent (the blue starry background is visible behind it) and fades out toward the bottom. In the middle, superimposed on the starry background and part of the spectrum is a large hexagon outlined in gold, with two hexagonal outlines behind it. Within the hexagon is an illustration of space with shapes representing objects and materials at different distances and points in time that Webb is investigating: a large planet with hints of cloud formations; beams of matter jetting out from the center of a galaxy; galaxies of different shapes and sizes; nebulous cloudy wisps; and stars with 8-pointed diffraction patterns.The much-anticipated first full-color images from NASA’s James Webb Space Telescope were released to the public in July 2022, beginning with a special broadcast from the White House on July 11. NASA Administrator Bill Nelson presented Webb’s First Deep Field image to President Biden and Vice-President Harris, and STScI’s then-Deputy Director Nancy Levenson attended to provide additional briefing, along with other experts. The following day, a full package of images and accompanying news releases and materials were issued, covering four additional celestial targets related to various areas of astronomy Webb will pursue during its mission: WASP-96 b (other worlds), the Southern Ring Nebula (stellar life cycle), Stephan’s Quintet (galaxies through time), and the Carina Nebula (star formation). Read the release that kicked off the start of Webb’s science operations.

 

JUNE 2022 ׀ HUBBLE

Dead Star Caught Ripping Up Planetary System

Illustration of a close-up view of a white dwarf system. A tiny star lies at the center, surrounded by a faint disk of material. Rocky-metallic bodies are shown falling into the star.Using archival data from NASA's Hubble Space Telescope and other NASA observatories, a white dwarf star has been found for the first time pulling both rocky-metallic and icy material onto its surface from its planetary system. A white dwarf is what remains after a star like our sun sheds its outer layers and ends nuclear fusion. This study confirms the true scale of this chaotic process, showing that within 100 million years after the beginning of its white dwarf phase, the star is able to simultaneously capture and consume material that originated in its asteroid belt and Kuiper belt-like regions. The makeup of the bodies detected raining onto the white dwarf implies that icy reservoirs might be common among planetary systems. This could have implications for our own solar system, and the theory that water was first delivered to Earth via comets and asteroids. Get details on the dead star here.

 

JUNE 2022 ׀ HUBBLE

Hubble Determines Mass of Isolated Black Hole Roaming Our Milky Way Galaxy

A crowded starfield with text at upper left, which reads Microlensing Black Hole. Small square around stars at center breaks out into a four-part graphic at the bottom of the image, with an arrow indicating a star dimming over time. Boxes are labeled with dates reading, from left, August 8, 2011; October 31, 2011; September 9, 2012; and August 29, 2017.For the first time ever, astronomers found direct evidence for a lone black hole drifting through interstellar space. Hubble made a mass measurement of the phantom object, following six years of meticulous observations. Until now, all black hole masses have been inferred statistically or through interactions in binary systems or in the cores of galaxies. Stellar-mass black holes are usually found due to the presence of a companion star, making this one unusual.

Hubble measured the amount of deflection of a background star's image by the black hole's warping of space. The star's image was offset from where it normally would be by about one milliarcsecond. That's equivalent to measuring the diameter of a 25-cent coin in Los Angeles as seen from New York City. Keep reading about the lone black hole.

 

APRIL 2022 ׀ HUBBLE

Hubble Confirms Largest Comet Nucleus Ever Seen

Diagram title reads, Comparison of Comet Nucleus Sizes. The rocky illustrations begin very small at left, like a pinpoint and extend almost to the height of the image at right. From left to right, shows P/2006 JQ5, 1 mile; 1P/Halley, 7 miles; C/2011 Kp36, 29 miles; C/Hale-Bopp, 46 miles; C/2002 VQ94, 60 miles; C/2014 UN271, 85 miles.Hubble has determined the size of the largest icy comet nucleus yet discovered. The estimated diameter is approximately 80 miles across, making it larger than the state of Rhode Island. The nucleus is about 50 times larger than those found at the heart of most known comets. Its mass is estimated to be a staggering 500 trillion tons, a hundred thousand times greater than the mass of a typical comet found much closer to the Sun. The behemoth comet, C/2014 UN271 (Bernardinelli-Bernstein) is barreling this way at 22,000 miles per hour from the edge of the Solar System. But not to worry. It will never get closer than 1 billion miles away from the Sun, which is slightly farther than the distance of the planet Saturn. Continue reading about the comet's nucleus.

 

MARCH 2022 ׀ HUBBLE

Record Broken: Hubble Spots Farthest Star Ever Seen

Field of stars and galaxies set against a black background includes an outline around an area toward the bottom center of the image. It is blown up larger, appearing toward the top of the image to show a lensed star along an arc.Hubble established an extraordinary new benchmark with its detection of a star that existed within the first billion years after the universe's birth in the big bang—the farthest individual star ever seen to date. Nicknamed Earendel, the star is so far away that its light has taken 12.9 billion years to reach Earth, appearing to us as it did when the universe was only 7 percent of its current age, at redshift 6.2. Even Hubble's power needed a boost from nature to detect it: Earendel is positioned along a ripple in space-time that gives it extreme magnification. The star's discovery was a huge leap further back in time from the previous single-star record holder, also detected by Hubble in 2018, which existed when the universe was about 4 billion years old, or 30 percent of its current age, at redshift 1.5. Read more about Earendel.

 

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