Members Can Post Anonymously On This Site
Have We Been to Uranus? We Asked a NASA Expert: Episode 56
-
Similar Topics
-
By NASA
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
NASA has announced the winners of it’s 31st Human Exploration Rover Challenge . The annual engineering competition – one of the agency’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. NASA NASA has announced the winning student teams in the 2025 Human Exploration Rover Challenge. This year’s competition challenged teams to design, build, and test a lunar rover powered by either human pilots or remote control. In the human-powered division, Parish Episcopal School in Dallas, Texas, earned first place in the high school division, and the Campbell University in Buies Creek, North Carolina, captured the college and university title. In the remote-control division, Bright Foundation in Surrey, British Columbia, Canada, earned first place in the middle and high school division, and the Instituto Tecnologico de Santa Domingo in the Dominican Republic, captured the college and university title.
The annual engineering competition – one of NASA’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. The complete list of 2025 award winners is provided below:
Human-Powered High School Division
First Place: Parish Episcopal School, Dallas, Texas Second Place: Ecambia High School, Pensacola, Florida Third Place: Centro Boliviano Americano – Santa Cruz, Bolivia Human-Powered College/University Division
First Place: Campbell University, Buies Creek, North Carolina Second Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Third Place: University of Alabama in Huntsville Remote-Control Middle School/High School Division
First Place: Bright Foundation, Surrey, British Columbia, Canada Second Place: Assumption College, Brangrak, Bangkok, Thailand Third Place: Erie High School, Erie, Colorado Remote-Control College/University Division
First Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Second Place: Campbell University, Buies Creek, North Carolina Third Place: Tecnologico de Monterey – Campus Cuernvaca, Xochitepec, Morelos, Mexico Ingenuity Award
Queen’s University, Kingston, Ontario, Canada Phoenix Award
Human-Powered High School Division: International Hope School of Bangladesh, Uttara, Dhaka, Bangladesh College/University Division: Auburn University, Auburn, Alabama Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Southwest Oklahoma State University, Weatherford, Oklahoma Task Challenge Award
Remote-Control Middle School/High School Division: Assumption College, Bangrak, Bangkok, Thailand College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Project Review Award
Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: Campbell University, Buies Creek, North Carolina Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Featherweight Award
Campbell University, Buies Creek, North Carolina Safety Award
Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: University of Alabama in Huntsville Crash and Burn Award
Universidad de Monterrey, Nuevo Leon, Mexico (Human-Powered Division) Team Spirit Award
Instituto Tecnologico de Santo Domingo, Dominican Republic (Human-Powered Division) STEM Engagement Award
Human-Powered High School Division: Albertville Innovation School, Albertville, Alabama College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Remote-Control Middle School/High School Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic College/University Division: Tecnologico de Monterrey, Nuevo Leon, Mexico Social Media Award
Human-Powered High School Division: International Hope School of Bagladesh, Uttara, Dhaka, Bangladesh College/University Division: Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Remote-Control Middle School/High School Division: ATLAS SkillTech University, Mumbai, Maharashtra, India College/University Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic Most Improved Performance Award
Human-Powered High School Division: Space Education Institute, Leipzig, Germany College/University Division: Purdue University Northwest, Hammond, Indiana Remote-Control Middle School/High School Division: Erie High School, Erie, Colorado College/University Division: Campbell University, Buies Creek, North Carolina Pit Crew Award
Human-Powered High School Division: Academy of Arts, Career, and Technology, Reno, Nevada College/University Division: Queen’s University, Kingston, Ontario, Canada Artemis Educator Award
Fabion Diaz Palacious from Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Rookie of the Year
Deira International School, Dubai, United Arab Emirates
More than 500 students with 75 teams from around the world participated in the 31st year of the competition. Participating teams represented 35 colleges and universities, 38 high schools, and two middle schools from 20 states, Puerto Rico, and 16 other nations. Teams were awarded points based on navigating a half-mile obstacle course, conducting mission-specific task challenges, and completing multiple safety and design reviews with NASA engineers.
NASA expanded the 2025 challenge to include a remote-control division, Remote-Operated Vehicular Research, and invited middle school students to participate.
“This student design challenge encourages the next generation of scientists and engineers to engage in the design process by providing innovative concepts and unique perspectives,” said Vemitra Alexander, who leads the challenge for NASA’s Office of STEM Engagement at Marshall. “This challenge also continues NASA’s legacy of providing valuable experiences to students who may be responsible for planning future space missions, including crewed missions to other worlds.”
The rover challenge is one of NASA’s eight Artemis Student Challenges reflecting the goals of the Artemis campaign, which will land Americans on the Moon while establishing a long-term presence for science and exploration, preparing for future human missions to Mars. NASA uses such challenges to encourage students to pursue degrees and careers in the fields of science, technology, engineering, and mathematics.
The competition is managed by NASA’s Southeast Regional Office of STEM Engagement at Marshall. Since its inception in 1994, more than 15,000 students have participated – with many former students now working at NASA, or within the aerospace industry.
To learn more about the Human Exploration Rover Challenge, please visit:
https://www.nasa.gov/roverchallenge/home/index.html
News Media Contact
Taylor Goodwin
Marshall Space Flight Center, Huntsville, Ala.
256.544.0034
taylor.goodwin@nasa.gov
View the full article
-
By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s Wallops Flight Facility commemorated the start of construction of its new Wallops Island causeway bridge during a groundbreaking ceremony at 10 a.m., Monday, April 14, 2025, on the island.
NASA’s Wallops Flight Facility commemorated the start of construction of its new Wallops Island causeway bridge during a groundbreaking ceremony at 10 a.m., Monday, April 14, 2025, on the island. NASA’s Wallops Flight Facility Facility Director David Pierce, NASA’s Goddard Space Flight Center Associate Center Director Ray Rubilotta, and Virgnia Sen. Bill DeSteph attended the ceremony.NASA/Danielle Johnson The ceremony was held at the base of the old Wallops Island causeway bridge. Virgina state Sen. Bill DeSteph attended the groundbreaking, along with staffers from the offices of Sen. Mark Warner, Sen. Tim Kaine, Congresswomen Jen Kiggans, Sen. Chris Van Hollen, and Sen. Angela Alsobrooks. NASA Wallops Facility Director David Pierce and NASA’s Goddard Space Flight Center Associate Center Director Ray Rubilotta attended on behalf of the agency.
“Much has changed over the decades, but one thing that has remained the same is our reliance on the causeway bridge as the only means for vehicular access to and from the island,” said Pierce. “Our bridge supports a growing portfolio of commercial launch and government partners. The work we do advances science, technology, and national security missions. This vital work for our nation is enabled by our bridge.”
In 2023, NASA Wallops was awarded $103 million in federal funds to fully construct and replace the current 65-year-old causeway bridge that serves as the only vehicular access from NASA Wallops Mainland facilities to its Wallops Island facilities and launch range. After years of exposure to coastal weather and repeated repairs to extend its viability, the existing causeway bridge is reaching the end of its service life.
The new causeway bridge, slated for completion in early 2028, will feature a flatter structure, capable of accommodating the increase in heavier loads transported to and from the island in support of an increased cadence of launch operations by NASA, its tenants, and commercial partners. This vital investment in NASA’s infrastructure supports the launch range’s continued growth, strengthening its role as a key asset in Virginia and the nation.
An architectural rendering showing the new Wallops Island causeway bridge next to the old causeway bridge.Courtesy of Kokosing NASA is partnering with the Federal Highway Administration to lead the delivery of the design-build project. The project has been awarded to Kokosing Construction Company.
For more information on NASA’s Wallops Flight Facility, visit www.nasa.gov/wallops.
Share
Details
Last Updated Apr 14, 2025 Related Terms
Wallops Flight Facility
View the full article
-
By NASA
A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands at Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Nov. 4, 2024, in preparation for the agency’s SpaceX 31st Commercial Resupply Services mission to the International Space Station.Credit: SpaceX NASA and SpaceX are targeting 4:15 a.m. EDT, Monday, April 21, for the next launch to deliver science investigations, supplies, and equipment to the International Space Station. This is the 32nd SpaceX commercial resupply services mission to the orbiting laboratory for the agency.
Filled with more than 6,400 pounds of supplies, a SpaceX Dragon spacecraft on a Falcon 9 rocket will lift off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Live launch coverage will begin at 3:55 a.m. on NASA+. Learn how to watch NASA content through a variety of platforms.
NASA’s coverage of Dragon’s arrival to the orbital outpost will begin at 6:45 a.m. Tuesday, April 22, on NASA+. The spacecraft will dock autonomously to the zenith port of the space station’s Harmony module.
Along with food and essential equipment for the crew, Dragon is delivering a variety of science experiments, including a demonstration of refined maneuvers for free-floating robots. Dragon also carries an enhanced air quality monitoring system that could protect crew members on exploration missions to the Moon and Mars, and two atomic clocks to examine fundamental physics concepts such as relativity and test worldwide synchronization of precision timepieces.
The Dragon spacecraft is scheduled to remain at the space station until May, when it will depart and return to Earth with research and cargo, splashing down off the coast of California.
NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):
Wednesday, April 16
1 p.m. – International Space Station National Lab Science Webinar with the following participants:
Jennifer Buchli, chief scientist, NASA’s International Space Station Program Michael Roberts, chief scientific officer, International Space Station National Lab Claire Fortenberry, research aerospace engineer, NASA’s Glenn Research Center in Cleveland Yupeng Chen, co-founder, Eascra Biotech Mari Anne Snow, CEO, Eascra Biotech Maj. Travis Tubbs, U.S. Air Force Academy Heath Mills, co-founder, Rhodium Scientific Sarah Wyatt, researcher, Ohio University Media who wish to participate must register for Zoom access no later than one hour before the start of the webinar.
Audio of the teleconference will stream live on the International Space Station National Lab website.
Friday, April 18
3 p.m. – Prelaunch media teleconference (no earlier than one hour after completion of the Launch Readiness Review) with the following participants:
Zebulon Scoville, deputy manager, Transportation Integration Office, NASA’s International Space Station Program Jennifer Buchli, chief scientist, NASA’s International Space Station Program Sarah Walker, director, Dragon Mission Management, SpaceX Jimmy Taeger, launch weather officer, 45th Weather Squadron, Cape Canaveral Space Force Station
Media who wish to participate by phone must request dial-in information by 5 p.m. Thursday, April 17, by emailing Kennedy’s newsroom at: ksc-media-accreditat@mail.nasa.gov.
Audio of the teleconference will stream live on the agency’s website.
Monday, April 21:
3:55 a.m. – Launch coverage begins on NASA+.
4:15 a.m. – Launch
Tuesday, April 22:
6:45 a.m. – Arrival coverage begins on NASA+.
8:20 a.m. – Docking
NASA website launch coverage
Launch day coverage of the mission will be available on the NASA website. Coverage will include live streaming and blog updates beginning no earlier than 3:55 a.m., April 21, as the countdown milestones occur. On-demand streaming video on NASA+ and photos of the launch will be available shortly after liftoff. For questions about countdown coverage, contact the NASA Kennedy newsroom at 321-867-2468. Follow countdown coverage on our International Space Station blog for updates.
Attend Launch Virtually
Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch.
Watch, Engage on Social Media
Let people know you’re watching the mission on X, Facebook, and Instagram by following and tagging these accounts:
X: @NASA, @NASAKennedy, @NASASocial, @Space_Station, @ISS_Research,
@ISS National Lab
Facebook: NASA, NASAKennedy, ISS, ISS National Lab
Instagram: @NASA, @NASAKennedy, @ISS, @ISSNationalLab
Coverage en Espanol
Did you know NASA has a Spanish section called NASA en Espanol? Check out NASA en Espanol on X, Instagram, Facebook, and YouTube for additional mission coverage.
Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo o Messod Bendayan a: antonia.jaramillobotero@nasa.gov o messod.c.bendayan@nasa.gov.
Learn more about the commercial resupply mission at:
https://www.nasa.gov/mission/nasas-spacex-crs-32/
-end-
Julian Coltre / Josh Finch
Headquarters, Washington
202-358-1100
julian.n.coltre@nasa.gov / joshua.a.finch@nasa.gov
Stephanie Plucinsky / Steven Siceloff
Kennedy Space Center, Florida
321-876-2468
stephanie.n.plucinsky@nasa.gov / steven.p.siceloff@nasa.gov
Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov
Share
Details
Last Updated Apr 14, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms
Commercial Resupply Humans in Space International Space Station (ISS) ISS Research SpaceX Commercial Resupply View the full article
-
By NASA
NASA’s Lucy spacecraft is 6 days and less than 50 million miles (80 million km) away from its second close encounter with an asteroid; this time, the small main belt asteroid Donaldjohanson.
Download high-resolution video and images from NASA’s Scientific Visualization Studio.
NASA/Dan Gallagher This upcoming event represents a comprehensive “dress rehearsal” for Lucy’s main mission over the next decade: the exploration of multiple Trojan asteroids that share Jupiter’s orbit around the Sun. Lucy’s first asteroid encounter – a flyby of the tiny main belt asteroid Dinkinesh and its satellite, Selam, on Nov. 1, 2023 – provided the team with an opportunity for a systems test that they will be building on during the upcoming flyby.
Lucy’s closest approach to Donaldjohanson will occur at 1:51pm EDT on April 20, at a distance of 596 miles (960 km). About 30 minutes before closest approach, Lucy will orient itself to track the asteroid, during which its high-gain antenna will turn away from Earth, suspending communication. Guided by its terminal tracking system, Lucy will autonomously rotate to keep Donaldjohanson in view. As it does this, Lucy will carry out a more complicated observing sequence than was used at Dinkinesh. All three science instruments – the high-resolution greyscale imager called L’LORRI, the color imager and infrared spectrometer called L’Ralph, and the far infrared spectrometer called L’TES – will carry out observation sequences very similar to the ones that will occur at the Trojan asteroids.
However, unlike with Dinkinesh, Lucy will stop tracking Donaldjohanson 40 seconds before the closest approach to protect its sensitive instruments from intense sunlight.
“If you were sitting on the asteroid watching the Lucy spacecraft approaching, you would have to shield your eyes staring at the Sun while waiting for Lucy to emerge from the glare. After Lucy passes the asteroid, the positions will be reversed, so we have to shield the instruments in the same way,” said encounter phase lead Michael Vincent of Southwest Research Institute (SwRI) in Boulder, Colorado. “These instruments are designed to photograph objects illuminated by sunlight 25 times dimmer than at Earth, so looking toward the Sun could damage our cameras.”
Fortunately, this is the only one of Lucy’s seven asteroid encounters with this challenging geometry. During the Trojan encounters, as with Dinkinesh, the spacecraft will be able to collect data throughout the entire encounter.
After closest approach, the spacecraft will “pitch back,” reorienting its solar arrays back toward the Sun. Approximately an hour later, the spacecraft will re-establish communication with Earth.
“One of the weird things to wrap your brain around with these deep space missions is how slow the speed of light is,” continued Vincent. “Lucy is 12.5 light minutes away from Earth, meaning it takes that long for any signal we send to reach the spacecraft. Then it takes another 12.5 minutes before we get Lucy’s response telling us we were heard. So, when we command the data playback after closest approach, it takes 25 minutes from when we ask to see the pictures before we get any of them to the ground.”
Once the spacecraft’s health is confirmed, engineers will command Lucy to transmit the science data from the encounter back to Earth, which is a process that will take several days.
Donaldjohanson is a fragment from a collision 150 million years ago, making it one of the youngest main belt asteroids ever visited by a spacecraft.
“Every asteroid has a different story to tell, and these stories weave together to paint the history of our solar system,” said Tom Statler, Lucy mission program scientist at NASA Headquarters in Washington. “The fact that each new asteroid we visit knocks our socks off means we’re only beginning to understand the depth and richness of that history. Telescopic observations are hinting that Donaldjohanson is going to have an interesting story, and I’m fully expecting to be surprised – again.”
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, designed and built the L’Ralph instrument and provides overall mission management, systems engineering and safety and mission assurance for Lucy. Hal Levison of SwRI’s office in Boulder, Colorado, is the principal investigator. SwRI, headquartered in San Antonio, also leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft, designed the original orbital trajectory and provides flight operations. Goddard and KinetX Aerospace are responsible for navigating the Lucy spacecraft. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, designed and built the L’LORRI (Lucy Long Range Reconnaissance Imager) instrument. Arizona State University in Tempe, Arizona, designed and build the L’TES (Lucy Thermal Emission Spectrometer) instrument. Lucy is the thirteenth mission in NASA’s Discovery Program, which is managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama.
By Katherine Kretke, Southwest Research Institute
Media Contact:
Karen Fox / Molly Wasser
Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
Nancy N. Jones
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Share
Details
Last Updated Apr 14, 2025 EditorMadison OlsonContactNancy N. Jonesnancy.n.jones@nasa.govLocationGoddard Space Flight Center Related Terms
Lucy Goddard Space Flight Center Planetary Science Explore More
4 min read New Modeling Assesses Age of Next Target Asteroid for NASA’s Lucy
Article 4 weeks ago 3 min read NASA’s Lucy Spacecraft Takes Its 1st Images of Asteroid Donaldjohanson
Article 2 months ago 3 min read NASA’s Lucy Asteroid Target Gets a Name
Article 2 years ago View the full article
-
By NASA
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
Downloads
Click any image to open a larger version.
View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
Media Contacts
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)
Related Information
Read more about other planetary nebulae
Watch: ViewSpace video about planetary nebulae
View images of other planetary nebulae on AstroPix
More Webb News
More Webb Images
Webb Science Themes
Webb Mission Page
Related For Kids
What is the Webb Telescope?
SpacePlace for Kids
En Español
Ciencia de la NASA
NASA en español
Space Place para niños
Keep Exploring Related Topics
James Webb Space Telescope
Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Stars
Stars Stories
Universe
Share
Details
Last Updated Apr 14, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
James Webb Space Telescope (JWST) Astrophysics Binary Stars Goddard Space Flight Center Nebulae Planetary Nebulae Science & Research Stars The Universe White Dwarfs View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.