Uploaded January 2026 | Updated September 2026, 2 weeks ago
The James Webb Space Telescope, which is actively observing the universe from a million miles away, and the Nancy Grace Roman Space Telescope, set to launch in 2026, are NASA's two latest flagship astrophysics observatories. Although both are studying myriad cosmic objects to answer fundamental questions about our universe, they have very different designs and capabilities. The universe is such a vast and complex place that it takes many telescopes with different abilities to thoroughly study it. This four-part video series explores the differences and synergies of Roman and Webb.
Webb’s giant mirror, ultracold instruments and infrared vision help it observe the farthest observable reaches of the cosmos. Using its narrow field of view, it can measure distant galaxies and planets outside our solar system with unprecedented detail.
Roman has a large field of view and will capture giant, 300-megapixel images, enabling it to survey the sky 1,000 times faster than the Hubble Space Telescope can while maintaining resolution similar to Hubble’s. Roman will also observe regions repeatedly over time, allowing astronomers to see changes and detect transient events like exploding stars and the movement of planets near the center of our galaxy.
Learn more at science.nasa.gov/roman-and-webb
Music credit: “Light Trails,” Max Cameron Concors [ASCAP], Universal Production Music “Relentless Data,” Jay Price [PRS], Universal Production Music
Credit: NASA's Goddard Space Flight Center
Scott Wiessinger (eMITS): Producer/editor
Barb Mattson (University of Maryland College Park): Narrator
Scott Wiessinger (eMITS): Writer
Ashley Balzer (eMITS): Science Writer
Francis Reddy (University of Maryland College Park):Science Writer
Claire Andreoli (NASA/GSFC): Public Affairs Officer
Adriana Manrique Gutierrez (eMITS): Animator
Scott Wiessinger (eMITS): Animator
Krystofer Kim (eMITS): Animator
Jenny McElligott (Advocates in Manpower Management, Inc.): Animator
Jonathan North (eMITS): Animator
Chris Smith (KBRWyle): Animator
Dominic Benford (NASA/HQ): Science Advisor
Rob Zellem (NASA/GSFC): Science Advisor
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14891. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: svs.gsfc.nasa.gov/14891. For more information on NASA’s media guidelines, visit nasa.gov/nasa-brand-center/images-and-media/.
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The James Webb Space Telescope, which is actively observing the universe from a million miles away, and the Nancy Grace Roman Space Telescope, set to launch in 2026, are NASA's two latest flagship astrophysics observatories. Although both are studying myriad cosmic objects to answer fundamental questions about our universe, they have very different designs and capabilities. The universe is such a vast and complex place that it takes many telescopes with different abilities to thoroughly study it. This four-part video series explores the differences and synergies of Roman and Webb.
Webb’s giant mirror, ultracold instruments and infrared vision help it observe the farthest observable reaches of the cosmos. Using its narrow field of view, it can measure distant galaxies and planets outside our solar system with unprecedented detail.
Roman has a large field of view and will capture giant, 300-megapixel images, enabling it to survey the sky 1,000 times faster than the Hubble Space Telescope can while maintaining resolution similar to Hubble’s. Roman will also observe regions repeatedly over time, allowing astronomers to see changes and detect transient events like exploding stars and the movement of planets near the center of our galaxy.
Learn more at science.nasa.gov/roman-and-webb
Music credit: “Light Trails,” Max Cameron Concors [ASCAP], Universal Production Music “Relentless Data,” Jay Price [PRS], Universal Production Music
Credit: NASA's Goddard Space Flight Center
Scott Wiessinger (eMITS): Producer/editor
Barb Mattson (University of Maryland College Park): Narrator
Scott Wiessinger (eMITS): Writer
Ashley Balzer (eMITS): Science Writer
Francis Reddy (University of Maryland College Park):Science Writer
Claire Andreoli (NASA/GSFC): Public Affairs Officer
Adriana Manrique Gutierrez (eMITS): Animator
Scott Wiessinger (eMITS): Animator
Krystofer Kim (eMITS): Animator
Jenny McElligott (Advocates in Manpower Management, Inc.): Animator
Jonathan North (eMITS): Animator
Chris Smith (KBRWyle): Animator
Dominic Benford (NASA/HQ): Science Advisor
Rob Zellem (NASA/GSFC): Science Advisor
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14891. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: svs.gsfc.nasa.gov/14891. For more information on NASA’s media guidelines, visit nasa.gov/nasa-brand-center/images-and-media/.
If you liked this video, subscribe to the NASA Goddard YouTube channel: youtube.com/NASAGoddard
Follow NASA’s Goddard Space Flight Center
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· Flickr: flickr.com/photos/gsfc
![NASA’S PUNCH Mission
NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun’s corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.
Watch the video to learn how imaging the Sun’s corona and the solar wind together will help scientists better understand the entire inner heliosphere — Sun, solar wind, and Earth — as a single connected system.
Music Credit: “Crafted with Science Instrumental” by Zak McNeil [ASCAP] via Universal Production Music
Video credit: NASA’s Goddard Space Flight Center
Producer: Beth Anthony (eMITS)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14773 While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here:
https://svs.gsfc.nasa.gov/14773
For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
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· Flickr: http://www.flickr.com/photos/gsfc NASA’S PUNCH Mission](https://i.ytimg.com/vi/bOi8fDGtmZo/mqdefault.jpg)
![Artemis II: Into the Path of Solar Eruptions
For the first time in half a century, four astronauts are leaving Earth’s protective magnetic field. They’ll enter a realm where massive solar eruptions can unleash more energy than a billion hydrogen bombs.
The Artemis II crew will fly through a dangerous environment, but they’re not going it alone. On the voyage, the astronauts and their Orion capsule are outfitted with radiation trackers as ground teams monitor solar eruptions 24/7. Here’s how NASA and the National Oceanic and Atmospheric Administration (NOAA) are protecting explorers from the most powerful eruptions in the solar system. 🛡️
Video credit: NASA/Joy Ng
Music credit: “Again and Again” by Laurent Dury [SACEM] via Universal Production Music
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14988 While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14988. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
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![Parker Solar Probe: Humanity’s Closest Encounter with the Sun
Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.
Breaking its previous record by flying just 3.8 million miles above the surface of the Sun, NASA’s Parker Solar Probe hurtled through the solar atmosphere at a blazing 430,000 miles per hour — faster than any human-made object has ever moved. A beacon tone received in the late evening hours of Dec. 26 confirmed the spacecraft had made it through the encounter safely and is operating normally.
This pass, the first of more to come at this distance, allows the spacecraft to conduct unrivaled scientific measurements with the potential to change our understanding of the Sun.
Read more: https://science.nasa.gov/science-research/heliophysics/nasas-parker-solar-probe-makes-history-with-closest-pass-to-sun/
Music credits: “Altitude” by Thomas Daniel Bellingham [PRS]; “Our Velocity Vibrant” by Jeremy Noel William Abbott [PRS]; “Omega Centauri” by Timothy James Cornick [PRS]; “Earthrise” by Alasdair Neil Parkinson [ASCA]; “The Big Revelation” by Richard James Neale [PRS], Jason Glover [PRS]; “Snuggling You” by Daniel Backes [GEMA], Peter Moslener [GEMA] from Universal Production Music.
Video Credit: NASA
Editors: Joy Ng (eMITS), Beth Anthony (eMITS)
Lead Heat Shield Engineer: Betsy Congdon (Johns Hopkins APL)
Associate Administrator: Nicola Fox (NASA)
Mission Designer: Yanping Guo (Johns Hopkins APL)
Heliophysicist: Kelly Korreck (NASA)
Lead Producer: Joy Ng (eMITS)
Project Scientist: Nour Rawafi (Johns Hopkins APL)
Heliophysics Division Director: Joseph Westlake (NASA)
Mission Systems Engineer: John Wirzburger (Johns Hopkins APL)
Videographers: Lacey Young, Beth Anthony, Joy Ng (eMITS)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14741 While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14741
For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard
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· Flickr: http://www.flickr.com/photos/gsfc Parker Solar Probe: Humanity’s Closest Encounter with the Sun](https://i.ytimg.com/vi/c80TzqNoqMg/mqdefault.jpg)

![Intense Solar Storm Shifts ESCAPADE Launch
NASA’s ESCAPADE mission launched on Nov. 13, 2025!
But it wasn’t without any hiccups — or maybe a series of violent burps? — from the Sun! ☀️🌬️
The launch of ESCAPADE, our next mission to Mars, was delayed by a day due to the most powerful geomagnetic storm of 2025. The storm was caused by multiple flares and eruptions known as coronal mass ejections heading toward Earth.
With the help of NASA satellites and models, the team could monitor when the storm subsided and by the following day, it was safe to launch.
Music credit: Machine Learning” by Ben Niblett and Jon Cotton [PRS] from Universal Production Music
Credit: NASAs Goddard Space Flight Center
Producer: Lacey Young (eMITS)
Videographer: John Sackman (eMITS), Chris Stevens (eMITS)
Writer: Erin Mahoney (Booz Allen Hamilton Inc.), Abbey Interrante (NCS), Joy Ng (eMITS)
Talent: Joe Westlake (NASA)
Additional Video and Animations:
Blue Origin
Rocket Lab
Storyblocks
Sound Effects:
Pixabay
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14925. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14925. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/
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![Planting an Artemis I Moon Tree
On Nov. 16, 2022, NASA launched the Artemis I test flight, sending an uncrewed Orion capsule beyond the Moon and back. On board were seeds from five species of trees, to be planted after returning to Earth. On Nov. 7, 2024, a seedling from the Artemis I flight was planted at the NASA Goddard Visitor Center by Artemis I Mission Manager Mike Sarafin, Artemis II Camera Lead Marie Henderson, Artemis III Project Scientist Noah Petro, Artemis IV Project Scientist Barbara Cohen, and others. In commemorating the event, Dr. Petro noted that planting a seedling is, like space exploration, an act of hope intended to bring fruit to future generations.
Learn more: https://www.nasa.gov/learning-resources/nasa-stem-artemis-moon-trees/
Credit: NASA’s Goddard Space Flight Center
Dan Gallagher: Producer/Editor
Noah Petro: Scientist
John D. Philyaw: Videographer
Lonnie Shekhtman: Public Affairs
Caela Barry: Support
Staci Horvath: Support
Kathryn Mersmann: Support
Derrol Nail: Launch Commentator
Aaron E. Lepsch: Technical Support
Universal Production Music: “Positive Progression” by Harry Gregson Williams [BMI] and Ben Andrew [PRS]; “Timeless” by Joshua Benjamin Pacey [PRS] and Harry Gregson Williams [BMI]
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14929. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14929. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
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· Flickr: http://www.flickr.com/photos/gsfc Planting an Artemis I Moon Tree](https://i.ytimg.com/vi/e9E3POsQthk/mqdefault.jpg)
![Take a 360 Tour of COBEs Cosmic Baby Picture
View the entire sky with the microwave eyes of NASA’s COBE (Cosmic Background Explorer) satellite in this immersive video. COBE took the first baby picture of the universe, revealing slight temperature variations when the cosmos was just 380,000 years old. This image shows the entire sky using four years of observations by COBE’s Differential Microwave Radiometer. The central plane of our galaxy runs across the middle, and its center is marked by a white X. Red indicates hotter regions, blue colder. The fluctuations are extremely faint, varying by only 1 part in 100,000 from the average temperature. They represent density variations in the early universe thought to have given rise to the structures we see today. After stripping away foreground emission arising from dust, hot gas, and charged particles interacting with magnetic fields in our galaxy, COBE data revealed tiny variations in the temperature of the cosmic microwave background — the oldest light in the universe — for the first time.
Music credit: “Meetings in Underwater Ruins,” Philippe Andre Vandenhende [SACEM], Olivier Louis Perrot [SACEM] and Idriss-El-Mehdi Bennani [SACEM], Universal Production Music.
Credit: NASA’s Goddard Space Flight Center
Image credit: NASA/COBE Science Team
Producer: Scott Wiessinger (eMITS)
Narrator: Thomas Essinger-Hileman (NASA/GSFC)
Science Writer: Francis Reddy (University of Maryland College Park)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14720. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14720. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines.
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![One Last Look at Romans Mirror
The primary mirror for NASAs Nancy Grace Roman Space Telescope has passed its final inspection. On May 20 and 21, engineers at NASAs Goddard Space Flight Center in Greenbelt, Md., confirmed that no specks fell onto the mirrors during testing and that there are no defects in the coating or alignment. With this milestone complete, the primary mirror is ready for its next view: space.
Music: “All This Time,” Joseph Michael Robbins [PRS], Universal Production Music
Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Videographers: Scott Wiessinger (eMITS)
Sophia Roberts (eMITS)
Public affairs officer: Claire Andreoli (NASA/GSFC)
Editor: Scott Wiessinger (eMITS)
Science Writer: Ashley Balzer (eMITS)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/15049. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/15049. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard
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· Flickr http://www.flickr.com/photos/gsfc One Last Look at Romans Mirror](https://i.ytimg.com/vi/fAgrztFvWyk/mqdefault.jpg)