Uploaded June 2025 | Updated September 2026, 2 weeks ago
Researchers have now gathered a complete year of PACE data to tell a story about the health of land vegetation by detecting slight variations in leaf colors.
Previous missions allowed scientists to observe broad changes in chlorophyll, the pigment that gives plants their green color and also allows them to perform photosynthesis. But PACE now allows scientists to see three different pigments in vegetation: chlorophyll, anthocyanins, and carotenoids.
The combination of these three pigments helps scientists pinpoint even more information about plant health.
Music: "Natural Perfection," "Drops of Inspiration," "Android," "Tiny Moving Parts," Universal Production Music
Please give credit for this item to:
NASA's Goddard Space Flight Center
Producers:
Ryan Fitzgibbons (eMITS)
Interviewees:
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Videographer:
John Philyaw (eMITS)
Writers:
Ryan Fitzgibbons (eMITS)
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Editor:
Ryan Fitzgibbons (eMITS)
Animator:
Chris Burns (eMITS)
Narrator:
Ryan Fitzgibbons (eMITS)
Scientists:
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Animator:
Ryan Fitzgibbons (eMITS)
Visualizers:
Kel Elkins (SSAI)
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14850. 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/14850. For more information on NASA’s media guidelines, visit nasa.gov/multimedia/guidelines.
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Researchers have now gathered a complete year of PACE data to tell a story about the health of land vegetation by detecting slight variations in leaf colors.
Previous missions allowed scientists to observe broad changes in chlorophyll, the pigment that gives plants their green color and also allows them to perform photosynthesis. But PACE now allows scientists to see three different pigments in vegetation: chlorophyll, anthocyanins, and carotenoids.
The combination of these three pigments helps scientists pinpoint even more information about plant health.
Music: "Natural Perfection," "Drops of Inspiration," "Android," "Tiny Moving Parts," Universal Production Music
Please give credit for this item to:
NASA's Goddard Space Flight Center
Producers:
Ryan Fitzgibbons (eMITS)
Interviewees:
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Videographer:
John Philyaw (eMITS)
Writers:
Ryan Fitzgibbons (eMITS)
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Editor:
Ryan Fitzgibbons (eMITS)
Animator:
Chris Burns (eMITS)
Narrator:
Ryan Fitzgibbons (eMITS)
Scientists:
Morgaine McKibben (SSAI)
Fred Huemmrich (UMBC)
Animator:
Ryan Fitzgibbons (eMITS)
Visualizers:
Kel Elkins (SSAI)
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14850. 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/14850. For more information on NASA’s media guidelines, visit nasa.gov/multimedia/guidelines.
Follow NASA’s Goddard Space Flight Center:
· Instagram instagram.com/nasagoddard
· X twitter.com/NASAGoddard
· Facebook: facebook.com/NASAGoddard
· Flickr flickr.com/photos/gsfc

![Supercomputer Traces Neutron Stars’ Magnetic Tango
New simulations performed on NASA’s Pleiades supercomputer are providing scientists with the most comprehensive look yet into the interacting magnetic structures around city-sized neutron stars in the moments before they crash. The team identified potential signals emitted during the stars’ final moments that may be detectable by future observatories. Just before orbiting neutron stars merge, the magnetic fields and plasma around them, called magnetospheres, become entangled. The new simulations studied the last several orbits before the merger, when the magnetospheres undergo rapid and dramatic changes, and modeled potentially observable high-energy signals. Neutron star mergers produce a particular type of GRB (gamma-ray burst), the most powerful class of explosions in the cosmos. They create near-light-speed jets that emit gamma rays, powerful ripples in space-time called gravitational waves, and a so-called kilonova explosion that forges heavy elements like gold and platinum. So far, only one event, observed in 2017, has connected all three phenomena. Neutron stars pack more mass than our Sun into a ball about 15 miles (24 kilometers) across, roughly the length of Manhattan Island in New York City. Born out of supernova explosions, neutron stars can spin dozens of times a second and wield some of the strongest magnetic fields known, up to 10 trillion times stronger than a refrigerator magnet. That’s strong enough to directly transform gamma-rays into electrons and positrons and rapidly accelerate them to energies far beyond anything achievable in particle accelerators on Earth. In the simulations, which were performed on the Pleiades supercomputer at NASA’s Ames Research Center in California’s Silicon Valley, the linked magnetospheres behave like a magnetic circuit that continually rewires itself as the stars orbit. Field lines connect, break, and reconnect while currents surge through plasma moving at nearly the speed of light, and the rapidly varying fields can accelerate particles to high energies. The team ran hundreds of simulations of a system of two orbiting neutron stars, each with 1.4 solar masses. The goal was to explore how different magnetic field configurations affected the way electromagnetic energy light in all of its forms left the coalescing system. The research shows that the emitted light varies greatly in brightness and is not distributed evenly, so what a far-away observer might detect depends greatly on their perspective on the merger. In addition, the way the signals strengthen as the stars get closer and closer depends on the relative magnetic orientations of the neutron stars. If next-generation gravitational wave observatories can provide an early warning, future ground-based gamma-ray telescopes will be able to team up with space-based X-ray and gamma-ray telescopes to begin searching for the pre-merger emission seen in these simulations. Routine observation of events like these using two different “messengers” — light and gravitational waves — will provide a major leap forward in understanding this class of GRBs.
Music credit: “A Theory Develops,” Pip Heywood [PRS], Universal Production Music
Credit: NASAs Goddard Space Flight Center
Scott Wiessinger (eMITS): Producer/editor
Scott Wiessinger (eMITS): Narrator
Francis Reddy (University of Maryland College Park):Science Writer
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14884 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/14884. 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 Supercomputer Traces Neutron Stars’ Magnetic Tango](https://i.ytimg.com/vi/mt6vcy-hssA/mqdefault.jpg)


![Plunge: Behind the Scenes Creating a NASA Black Hole Visualization
Plunge into the story behind some of NASA’s most iconic black hole videos!
For Black Hole Week 2024, NASA released new visualizations showing flights around and into a black hole. These visually striking and scientifically accurate products resulted from months of work by a small team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, led by astrophysicist Jeremy Schnittman
Now, a new video reveals the backstage story of how these visualizations came about.
Schnittman developed computer code that models a supermassive black hole, its accretion disk, and its space-warping effects. Using a technique called ray tracing, the code also incorporated a virtual camera that tracked every photon, or particle of light, reaching it back to its source. For these visualizations, Schnittman also moved this camera through space, increasing the level of difficulty.
One set of visualizations sent the camera on a near-miss trajectory that looped around the black hole and escaped back into space. The other set plunged the camera straight into the black hole along the most direct path possible.
While his initial low-resolution test frames could be produced on a laptop computer, the final 8k versions required thousands of frames generated by a Goddard supercomputer called Discover. When played back in video form, the complete frame sets showed detailed views of familiar black hole features — as well as some Schnittman had never seen before.
No project is without some last-minute drama, though. Some frames revealed unexpected issues in the code that the team had to rush to deal with as the May deadline for Black Hole Week 2024 approached.
Watch the full behind-the-scenes video to learn how the team tackled these obstacles in time to produce these jaw-dropping videos.
Music:
Beautiful Awesome,” David Husband and James William Banbury [PRS], Universal Production Music “Games Show Sphere 01,” Anselm Kreuzer [GEMA], Universal Production Music “Rolling,” Jaremy Aiello and Mike Mullen [BMI], Universal Production Music “Question Time,” Paul Louis Reeves [PRS], Universal Production Music “Tactical Analysis,” Clinton Rusich, Matthew St Laurent, Christian Telford, and David Travis Edwards [ASCAP], Universal Production Music “Game Show Sphere 02,” Anselm Kreuzer [GEMA], Universal Production Music “Awakening Yearning,” David Ashok Ramani and Jonathan Elias [ASCAP], Universal Production Music “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music
Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Videographers: Sophia Roberts (eMITS)
Scott Wiessinger (eMITS)
Amogh Thakkar (Intern)
Karly Noetzel (Intern)
Interviewee: Jeremy Schnittman (NASA/GSFC)
Science Writer: Francis Reddy (University of Maryland College Park)
Data Visualizers: Jeremy Schnittman (NASA/GSFC)
Brian Powell (NASA/GSFC)
Narrator: Scott Wiessinger (eMITS)
Editor: Scott Wiessinger (eMITS)
Interviewers: Scott Wiessinger (eMITS)
Chiara Villanueva (Intern)
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14818. 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/14818. 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 Plunge: Behind the Scenes Creating a NASA Black Hole Visualization](https://i.ytimg.com/vi/nEO7n0lVskE/mqdefault.jpg)


![Hubble Uncovers Star’s Unusual Atmosphere
Astronomers using NASA’s Hubble Space Telescope have found a rare ultra massive white dwarf formed from a stellar merger.
The discovery was made possible by Hubble’s sensitive ultraviolet observations and suggests these unusual white dwarfs may be more common than once thought.
The white dwarf is 128 light-years away and 20 percent more massive than the Sun. In visible light it looked like a typical white dwarf, but Hubble’s ultraviolet data revealed something unusual…
For more information, visit science.nasa.gov/mission/hubble
Credit: NASAs Goddard Space Flight Center
Paul Morris: Lead Producer
Music Credit:
Zero Gravity Brice Davoli [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM] and Universal Production Music
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14877. 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/14877. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.
See more Hubble videos on YouTube: https://www.youtube.com/playlist?list=PLiuUQ9asub3Ta8mqP5LNiOhOygRzue8kN
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If you liked this video, subscribe to the NASA Goddard YouTube channel:
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· Flickr http://www.flickr.com/photos/gsfc Hubble Uncovers Star’s Unusual Atmosphere](https://i.ytimg.com/vi/nyWuLSIoosk/mqdefault.jpg)
![100,000 Computer Simulations Reveal Milky Ways Fate
For decades, astronomers believed that one thing was as certain as death and taxes: the Milky Way and our neighboring Andromeda galaxy were on a crash course… destined to collide in less than 5 billion years.
That galactic smash-up would spark massive star formation, scatter stars like cosmic billiard balls, and possibly throw our Sun into a whole new orbit.
But now… that future may not be so certain.
For more information, visit science.nasa.gov/mission/hubble
Credit: NASAs Goddard Space Flight Center
Paul Morris: Lead Producer
Video Credits:
Milky Way Timelapse
Stock Footage Provided By Pond5/lovemushroom
Artist Rendition of Gaia Spacecraft
ESA
Artist’s animation of the Sun becoming a red giant
ESA/Hubble (M. Kornmesser & L. L. Christensen)
Milky Way and Andromeda Collision Simulation
Visualization Credit: NASA, ESA, and F. Summers (STScI) Simulation Credit: NASA, ESA, G. Besla (Columbia University), and R. van der Marel (STScI)
Music Credit:
Lost to Eternity by Timothy James Cornick [PRS] via BBC Production Music [PRS] and Universal Production Music
This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14847. 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/14847. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.
See more Hubble videos on YouTube: https://www.youtube.com/playlist?list=PLiuUQ9asub3Ta8mqP5LNiOhOygRzue8kN
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If you liked this video, subscribe to the NASA Goddard YouTube channel:
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· Flickr http://www.flickr.com/photos/gsfc 100,000 Computer Simulations Reveal Milky Ways Fate](https://i.ytimg.com/vi/o2x_31dE04s/mqdefault.jpg)

