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Preparations for Next Moonwalk Simulations Underway (and Underwater)
Robotics teams gather on the main floor of the 2025 Aerospace Valley FIRST Robotics Competition at Eastside High School in Lancaster, California, adjusting and testing the functions of their robots, on April 3, 2025NASA/Genaro Vavuris A group of attendees to the 2025 Aerospace Valley FIRST Robotics Competition gather outside Eastside High School’s gymnasium in Lancaster, California, to watch an F/A-18 from NASA’s Armstrong Flight Research Center, in Edwards, California, fly over the school to kick off the competition, on April 3, 2025.NASA/Genaro Vavuris Jose Vasquez, engineering technician at NASA’s Armstrong Flight Research Center at Edwards, California, machines parts for a robot inside NASA’s mobile machine shop at the 2025 Aerospace Valley FIRST Robotics Competition in Lancaster, California, on April 3, 2025.NASA/Genaro Vavuris Students from Eagle Robotics, Team 399, supported by volunteers from NASA’s Armstrong Flight Research Center in Edwards, California, adjust their robot during the 2025 Aerospace Valley FIRST Robotics Competition in Lancaster, California, on April 3, 2025.NASA/Genaro Vavuris When young minds come together to test their knowledge and creativity in technology and innovation, the results are truly inspiring. In its sixth year, Aerospace Valley Regional FIRST Robotics Competition at East High School in Lancaster, California, proved to be another success. During three action-packed days, hundreds of students from around the world showcased their skills in building and programming robots designed to tackle real-world challenges. Volunteers from NASA’s Armstrong Flight Research Center in Edwards, California, played a key role, mentoring students and sharing expertise to guide the next generation of engineers.
The Aerospace Valley Regional was started with NASA’s support through the Robotics Alliance Project, which has helped expand robotics programs nationwide. As part of the project, NASA Armstrong supports five local teams and fosters innovation and mentorship for young minds. “It’s more than just a game – it’s a launchpad for future innovators,” said David Voracek, NASA Armstrong’s chief technologist, who has volunteered for 20 years and is the primary logistics manager.
Brad Flick, NASA Armstrong center director, toured the venue and talked to students, highlighting NASA’s continued commitment to inspiring the next generation of engineers and innovators. The event kicked off with an exciting F/A-18 flyover by NASA Armstrong research test pilots Nils Larson and James Less.
Throughout the competition, NASA volunteers – judges, scorers, and machinists – offered guidance and ensured smooth operations. The mobile shop supported students by repairing and fabricating parts for their robots, completing 79 jobs during the event. “Almost everything we do needs to get done in minutes,” says Jose Vasquez, volunteer, and engineering technician at NASA Armstrong’s fabrication lab, who volunteered at the event.
Beyond the competition, students engaged with industry professionals and explored career opportunities. “They don’t just build robots; they build confidence, resilience, and real-world skills alongside mentors who inspire them and volunteers who make it all possible,” Voracek said. This event showcased the talent, determination, and creativity that will shape the future of technology and innovation.
NASA’s Robotics Alliance Project provides grants for high school teams across the country and supports FIRST Robotics competitions, encouraging students to pursue STEM careers.
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Last Updated Apr 17, 2025 EditorDede DiniusContactPriscila Valdezpriscila.valdez@nasa.gov Related Terms
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Explore This Section Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read With NASA’s Webb, Dying Star’s Energetic Display Comes Into Full Focus
NASA’s James Webb Space Telescope has taken the most detailed image of planetary nebula NGC 1514 to date thanks to its unique mid-infrared observations. Webb shows its rings as intricate clumps of dust. It’s also easier to see holes punched through the bright pink central region. Credits:
NASA, ESA, CSA, STScI, Michael Ressler (NASA-JPL), Dave Jones (IAC) Gas and dust ejected by a dying star at the heart of NGC 1514 came into complete focus thanks to mid-infrared data from NASA’s James Webb Space Telescope. Its rings, which are only detected in infrared light, now look like “fuzzy” clumps arranged in tangled patterns, and a network of clearer holes close to the central stars shows where faster material punched through.
“Before Webb, we weren’t able to detect most of this material, let alone observe it so clearly,” said Mike Ressler, a researcher and project scientist for Webb’s MIRI (Mid-Infrared Instrument) at NASA’s Jet Propulsion Laboratory in southern California. He discovered the rings around NGC 1514 in 2010 when he examined the image from NASA’s Wide-field Infrared Survey Explorer (WISE). “With MIRI’s data, we can now comprehensively examine the turbulent nature of this nebula,” he said.
This scene has been forming for at least 4,000 years — and will continue to change over many more millennia. At the center are two stars that appear as one in Webb’s observation, and are set off with brilliant diffraction spikes. The stars follow a tight, elongated nine-year orbit and are draped in an arc of dust represented in orange.
One of these stars, which used to be several times more massive than our Sun, took the lead role in producing this scene. “As it evolved, it puffed up, throwing off layers of gas and dust in in a very slow, dense stellar wind,” said David Jones, a senior scientist at the Institute of Astrophysics on the Canary Islands, who proved there is a binary star system at the center in 2017.
Once the star’s outer layers were expelled, only its hot, compact core remained. As a white dwarf star, its winds both sped up and weakened, which might have swept up material into thin shells.
Image A: Planetary Nebula NGC 1514 (MIRI Image)
NASA’s James Webb Space Telescope has taken the most detailed image of planetary nebula NGC 1514 to date thanks to its unique mid-infrared observations. Webb shows its rings as intricate clumps of dust. It’s also easier to see holes punched through the bright pink central region. NASA, ESA, CSA, STScI, Michael Ressler (NASA-JPL), Dave Jones (IAC) Image B: Planetary Nebula NGC 1514 (WISE and Webb Images Side by Side)
Two infrared views of NGC 1514. At left is an observation from NASA’s Wide-field Infrared Survey Explorer (WISE). At right is a more refined image from NASA’s James Webb Space Telescope. NASA, ESA, CSA, STScI, NASA-JPL, Caltech, UCLA, Michael Ressler (NASA-JPL), Dave Jones (IAC) Its Hourglass Shape
Webb’s observations show the nebula is tilted at a 60-degree angle, which makes it look like a can is being poured, but it’s far more likely that NGC 1514 takes the shape of an hourglass with the ends lopped off. Look for hints of its pinched waist near top left and bottom right, where the dust is orange and drifts into shallow V-shapes.
What might explain these contours? “When this star was at its peak of losing material, the companion could have gotten very, very close,” Jones said. “That interaction can lead to shapes that you wouldn’t expect. Instead of producing a sphere, this interaction might have formed these rings.”
Though the outline of NGC 1514 is clearest, the hourglass also has “sides” that are part of its three-dimensional shape. Look for the dim, semi-transparent orange clouds between its rings that give the nebula body.
A Network of Dappled Structures
The nebula’s two rings are unevenly illuminated in Webb’s observations, appearing more diffuse at bottom left and top right. They also look fuzzy, or textured. “We think the rings are primarily made up of very small dust grains,” Ressler said. “When those grains are hit by ultraviolet light from the white dwarf star, they heat up ever so slightly, which we think makes them just warm enough to be detected by Webb in mid-infrared light.”
In addition to dust, the telescope also revealed oxygen in its clumpy pink center, particularly at the edges of the bubbles or holes.
NGC 1514 is also notable for what is absent. Carbon and more complex versions of it, smoke-like material known as polycyclic aromatic hydrocarbons, are common in planetary nebulae (expanding shells of glowing gas expelled by stars late in their lives). Neither were detected in NGC 1514. More complex molecules might not have had time to form due to the orbit of the two central stars, which mixed up the ejected material. A simpler composition also means that the light from both stars reaches much farther, which is why we see the faint, cloud-like rings.
What about the bright blue star to the lower left with slightly smaller diffraction spikes than the central stars? It’s not part of this nebula. In fact, this star lies closer to us.
This planetary nebula has been studied by astronomers since the late 1700s. Astronomer William Herschel noted in 1790 that NGC 1514 was the first deep sky object to appear genuinely cloudy — he could not resolve what he saw into individual stars within a cluster, like other objects he cataloged. With Webb, our view is considerably clearer.
NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth.
The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.
To learn more about Webb, visit: https://science.nasa.gov/webb
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Laura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Claire Blome – cblome@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Science Advisor
Michael Ressler (NASA-JPL)
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