Uploaded November 2025 | Updated September 2026, 2 weeks ago
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: 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 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: svs.gsfc.nasa.gov/14929. For more information on NASA’s media guidelines, visit nasa.gov/nasa-brand-center/images-and-media/.
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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: 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 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: svs.gsfc.nasa.gov/14929. 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
· Instagram: instagram.com/nasagoddard
· X: twitter.com/NASAGoddard
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· Flickr: flickr.com/photos/gsfc
![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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· Flickr http://www.flickr.com/photos/gsfc Take a 360 Tour of COBEs Cosmic Baby Picture](https://i.ytimg.com/vi/ef3QboVd83Y/mqdefault.jpg)
![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/.
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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)
![NASAs Illuminate: Weathering an Invisible Storm
In May 2024, the Sun launched multiple, powerful eruptions toward Earth, causing the largest geomagnetic storm in over 20 years. The solar storm was so intense, it knocked out many GPS and communication systems and even sparked auroras as far south as Mexico. This scientific visualization shows how the storm affected Earth’s magnetosphere in real time.
Music Credit: “Work to Be Done” by Ross Stephen Gilmartin [PRS] via Universal Production Music
Sound Effects: pixabay.com
Video credit: NASA’s Goddard Space Flight Center
Producer: Beth Anthony (eMITS)
Visualizer: Andrew J Christensen (SSAI)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14779 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/14779
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 NASAs Illuminate: Weathering an Invisible Storm](https://i.ytimg.com/vi/fOuILDmCTL0/mqdefault.jpg)



![Mapping the Boundaries of Our Home in Space with NASA’s IMAP Mission
NASA’s new Interstellar Mapping and Acceleration Probe, or IMAP, will explore and map the very boundaries of our heliosphere — a huge bubble created by the Suns wind that encapsulates our solar system — and study how that boundary interacts with the local galactic neighborhood beyond.
As a modern-day celestial cartographer, IMAP will chart the vast range of particles in interplanetary space, helping to investigate two of the most important overarching issues in heliophysics — the energization of charged particles from the Sun, and the interaction of the solar wind with interstellar space. Additionally, IMAP will support near real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth.
IMAP is launching no earlier than Sept. 23, 2025, aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Learn more about IMAP science: https://science.nasa.gov/missions/nasas-imap-mission-to-study-boundaries-of-our-home-in-space/
Find out more about the IMAP mission: https://science.nasa.gov/mission/imap/
Music credit: Soaring Dreams” by Klas Johan Wahl and Anders Paul Niska [STIM], “Electric Works” by Philippe Lhommet [SACEM], and “Mercurial Temperment” by Christian Telfold [ASCAP] from Universal Production Music
Credit: NASAs Goddard Space Flight Center
Producer/Editor: Lacey Young (eMITS)
Writer: Mara Johnson-Groh (eMITS)
Narrator: Jake Richmond (NASA)
Animators: Jonathan North (eMITS), Adriana Manrique (eMITS), Krystofer Kim (eMITS)
Talent: Eric Christian (NASA), Dave McComas (Princeton University), Matina Gkioulidou (Johns Hopkins Applied Physics Laboratory)
Additional Video and Animations:
Princeton University
Sound Effects:
Pixabay
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14895. 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/14895. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/
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 Mapping the Boundaries of Our Home in Space with NASA’s IMAP Mission](https://i.ytimg.com/vi/gEOraINOI5c/mqdefault.jpg)
![NASAs Roman Space Telescope Hardware Highlights: Winter/Spring 2026
The Nancy Grace Roman Space Telescope is now complete. This video, which covers the first half of 2026, highlights some of the final hardware milestones from this journey.
It opens with an aerial view of the complete observatory inside NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.
Some parts of Roman stow for launch. Once in space, these deployable components move into their operational positions. Engineers test these deployments on the ground to make sure they will go as planned in space. Four of the six Solar Array Sun Shield panels deploy. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool. The Deployable Aperture Cover (DAC), which protects the mirrors during launch and then unfolds to help shield them from sunlight, also test deploys. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space.
In preparation for vibration and acoustic testing, technicians put a clean tent over Roman and transport it out of the clean room. They push it next to the massive vibration tables, one of which shakes horizontally and the other vertically. A crane lifts Roman and the tent onto the tables, and also performs a 90-degree rotation after one horizontal test so that Roman can be tested on a different axis with the same table. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as anticipated.
For the acoustic test, they push it into the test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. A thick door seals the chamber and prevents most of the sound from escaping, although ear protection is still required for anyone nearby during a test. These tests are mostly to ensure that Roman can survive the rigors of launch. Once in space, it won’t be subjected to nearly as much force.
Once the tests are successfully completed, Roman re-enters the clean room and the tent is removed. Technicians lift Roman to a special rollover fixture that can safely tilt and spin Roman’s 18,500 pound mass. Once Roman is tilted horizontal for the first time as a full observatory, engineers slowly spin it through 360 degrees to make sure everything stays in place like it is supposed to.
After the rotations, technicians carefully perform a manual opening of the DAC to reveal the mirror. In this position, they can inspect the entire optical path all the way back to the instrument sensors and perform surface cleaning on the inside of the protective outer barrel and DAC. This is also a chance for final goodbyes to the mirror. Once the DAC is closed, no one will ever see the mirror as clearly again.
With all the assembly and testing at Goddard completed, the team begins the delicate process of loading Roman into an airtight container known as the CHARIOT (Conditioned Housing for Air, Road, Imaging optics assembly, and Observatory Transport). First they attach arms which will form the interior sides and support Roman. Then they lift and move Roman into the lower bed of the CHARIOT. An inner lid goes on first, followed by a larger outer lid with ducting to keep the observatory the right temperature and preserve the clean environment. As the CHARIOT leaves the clean room, Roman takes its first step in the journey to space.
Music credit: “Touching Clouds,” Andre Jesus Oliveira and Andre Miguel Lopes Roque [PRS], Universal Production Music
Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Videographers: Sophia Roberts (eMITS)
Scott Wiessinger (eMITS)
Rob Andreoli (eMITS)
John Philyaw (eMITS)
Jolearra Tshiteya (ASRC Federal)
Drone Pilot: Francis Reddy (University of Maryland College Park)
Editor: Scott Wiessinger (eMITS)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14491. 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/14491. For more information on NASA’s media guidelines, visit https://www.nasa.gov/nasa-brand-center/images-and-media/.
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![Furious February Flares
In early February 2026, the Sun emitted more than 50 flares including several X-class events, which is the most intense category of solar flares. NASA’s Solar Dynamics Observatory watches the Sun 24/7 and captured these views of the Sun in multiple wavelengths of light.
The Sun’s activity, which includes flares, follows an approximately 11-year cycle that creates periods of high and low activity. After reaching the current cycle’s most active phase in 2024 — known as solar maximum — the Sun remains in a heightened period of activity.
For news of the recent flares: https://science.nasa.gov/blogs/solar-cycle-25/
Music credit: “Gravity” by Cy Samuels [PRS] via Universal Production Music
Credit: NASA
Producer: Joy Ng (eMITS)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14973. 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/14973. 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 Furious February Flares](https://i.ytimg.com/vi/gp7KmJXf2EQ/mqdefault.jpg)

