{ "count": 384, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&people=Francis+Reddy", "previous": null, "results": [ { "id": 15099, "url": "https://svs.gsfc.nasa.gov/15099/", "result_type": "Produced Video", "release_date": "2026-09-18T14:00:00-04:00", "title": "NASA-JAXA XRISM Mission Sees Pulsar Accreting Companion's 'Wind'", "description": "This artist’s concept of the BP Crucis system follows the pulsar on a passage through the dense stream of plasma flowing from its companion, a blue hypergiant 40 times the Sun’s mass. During each four-day passage, the pulsar’s X-ray brightness flares as it pulls in some of the gas. At first, the gas forms a messy, turbulent accretion disk around the pulsar, and plasma spirals down to it. But as the pulsar moves deeper into the stream, there’s not enough angular momentum to support the disk, and it breaks up. At this point, plasma falls straight onto the pulsar. Later, as the pulsar nears the end of its passage, a messy accretion disk rebuilds, this time spinning in the opposite direction of the earlier disk. Credit: NASA’s Goddard Space Flight Center Conceptual Image LaboratoryAlt text: Animation of the BP Crucis system0:00 A wide view, showing the giant star, its gas stream, and the pulsar nearing it. 0:08 The camera zooms into the pulsar as it encounters the stream. 0:10 Gas flowing past the pulsar forms a clockwise-spinning accretion disk. 0:17 The disk breaks up. The gas now flows directly onto the pulsar. 0:35 As the pulsar nears the end of its passage through the stream, a new disk, spinning counterclockwise, forms. 0:51 The disk breaks up and the pulsar exits the stream. 0:52 Return to a wide view of the system. || Still2.jpg (3840x2160) [1.6 MB] || XRISM2.mp4 (1920x1080) [73.7 MB] || XRISM.en_US.srt [49 bytes] || XRISM.en_US.vtt [59 bytes] || XRISM_1.mp4 (3840x2160) [184.3 MB] || XRISM.mp4 (3840x2160) [725.6 MB] || XRISMNO_TexT.mov (3840x2160) [3.7 GB] || XRISMFinalText.mov (3840x2160) [3.9 GB] || ", "hits": 947 }, { "id": 20417, "url": "https://svs.gsfc.nasa.gov/20417/", "result_type": "Animation", "release_date": "2026-09-18T14:00:00-04:00", "title": "Wind-Accreting Pulsar Visualization", "description": "Visualization of the BP Crucis system showing the pulsar near closest approach to its companion, a blue hypergiant 40 times the Sun’s mass. Twice each orbit, the pulsar passes throuh a dense stream of plasma flowing from the companion, flaring up in X-rays as it does. In this sequence, the pulsar approaches, enters, and exits the stream. || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_print.jpg (1024x576) [84.0 KB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_searchweb.png (320x180) [62.1 KB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.00012_thm.png (80x40) [5.0 KB] || XRISM_IM_SHOT_01_alt_30fps_1080p_proRes.mov (1920x1080) [352.2 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_h264.mp4 (3840x2160) [26.2 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_proRes.webm (3840x2160) [5.9 MB] || XRISM_IM_SHOT_01_alt_30fps_4k_proRes.mov (3840x2160) [1.3 GB] || ", "hits": 448 }, { "id": 15080, "url": "https://svs.gsfc.nasa.gov/15080/", "result_type": "Produced Video", "release_date": "2026-08-28T13:00:00-04:00", "title": "Roman: Go For Launch", "description": "NASA’s Nancy Grace Roman Space Telescope is prepped for launch, and one phase of Roman is ending. It began with the 2010 Astronomy and Astrophysics Decadal Survey, where the community called for a wide-field infrared survey telescope: WFIRST. This was Roman’s start. Institutes and businesses across the country began developing new hardware to support this mission. At the observatory’s heart was a mirror the same size as Hubble’s and a set of 18 state-of-the-art detectors that allowed for both a massive field of view and extremely high angular resolution. This combination would allow Roman to create vast and detailed surveys of the universe unlike anything seen before. Roman also holds a Coronagraph Instrument to test hardware never before flown in space. It will be able to see distant planets orbiting other stars and is a major step toward finding life outside the solar system.Much of Roman’s hardware was developed and built in-house at NASA’s Goddard Space Flight Center. Other key systems came from places like NASA’s JPL (Jet Propulsion Laboratory), BAE Systems, and L3Harris. Beginning in 2023, all the parts converged on Goddard. Inside Goddard’s enormous clean room, a team of dedicated engineers and technicians spent over three years assembling the pieces. Throughout the process, they also used Goddard’s testing facilities to evaluate the hardware’s ability to survive launch and space. Pieces, assembled sections, and finally the entire observatory were subjected to tests like vibration and acoustic shaking, thermal vacuum freezing, and centrifuge g-force loading.The early completion and future success of the Roman Space Telescope is a testament to the unwavering commitment and effort of thousands of people working together toward a common goal. Thanks to all their efforts, Roman will broaden our understanding of the universe and our place within it.Music: “Caelum,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || RomanGoForLaunch_Still.jpg (3840x2160) [1.6 MB] || RomanGoForLaunch_Still_searchweb.png (320x180) [88.5 KB] || RomanGoForLaunch_Still_thm.png (80x40) [7.5 KB] || 15080_RomanGoForLaunch_1080.mp4 (1920x1080) [170.3 MB] || RomanGoForLaunchCaptions.en_US.srt [3.0 KB] || RomanGoForLaunchCaptions.en_US.vtt [2.8 KB] || 15080_RomanGoForLaunch_4k.mp4 (3840x2160) [354.2 MB] || 15080_RomanGoForLaunch_4k_Best.mp4 (3840x2160) [699.6 MB] || 15080_RomanGoForLaunch_ProRes_3840x2160_2997.mov (3840x2160) [12.2 GB] || ", "hits": 352 }, { "id": 15082, "url": "https://svs.gsfc.nasa.gov/15082/", "result_type": "Produced Video", "release_date": "2026-08-27T00:00:00-04:00", "title": "Curious Universe: Why Roman Will Make Unexpected Discoveries", "description": "In this special episode of the Curious Universe podcast, we take a deep dive into the science of NASA’s Nancy Grace Roman Space Telescope with Julie McEnery, Roman's senior project scientist. Learn why Roman’s survey data will be so detailed that they could cover a 4K screen the size of dozens of city blocks and why Julie says she doesn’t hope Roman changes our understanding of the universe—she knows it will.Watch this video on the NASA Goddard YouTube channel. || CU_Julie_Thumb_v1.png (1280x720) [1.4 MB] || CU_Julie_Thumb_v1_print.jpg (1024x576) [251.1 KB] || CU_Julie_Thumb_v1_searchweb.png (320x180) [108.4 KB] || CU_Julie_Thumb_v1_thm.png (80x40) [8.0 KB] || CU_Roman_McEnery_Final.webm (1920x1080) [199.5 MB] || CU_Roman_McEnery_Final.mp4 (1920x1080) [3.7 GB] || ", "hits": 156 }, { "id": 15081, "url": "https://svs.gsfc.nasa.gov/15081/", "result_type": "Produced Video", "release_date": "2026-08-24T12:00:00-04:00", "title": "NASA's Nancy Grace Roman Space Telescope: Official Mission Trailer", "description": "Named after NASA’s first chief astronomer, the ‘mother of the Hubble Space Telescope,’ the Nancy Grace Roman Space Telescope will have a field of view at least 100 times larger than Hubble's, measuring light from more than a billion galaxies during its five-year primary mission. This observatory will also be able to block starlight to directly see exoplanets and planet-forming disks, complete a statistical census of planetary systems in our galaxy, and settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics. || ", "hits": 273 }, { "id": 14974, "url": "https://svs.gsfc.nasa.gov/14974/", "result_type": "Infographic", "release_date": "2026-08-20T09:00:00-04:00", "title": "Infographic: NASA’s Pandora Mission", "description": "Pandora is a NASA small satellite (SmallSat) mission designed to study exoplanet atmospheres and their host stars. In its first year, it will observe about 20 exoplanets using visible and near-infrared light, revisiting each planet 10 times for 24-hour observations to separate the planet’s signal from its star and reveal the composition of the planet’s atmosphere. || ", "hits": 377 }, { "id": 15064, "url": "https://svs.gsfc.nasa.gov/15064/", "result_type": "Produced Video", "release_date": "2026-07-28T12:00:00-04:00", "title": "NASA's Roman Space Telescope's Transport from Goddard to Kennedy", "description": "Watch this video to see how Roman was transported from NASA's Goddard Space Flight Center down to the Kennedy Space Center. Includes a version with no text overlays.Music credit: “Unity for Liberty,” Lucas Napoleone and François Rousselot [SACEM], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_RomanTRANSPORT_Still.jpg (1280x720) [285.7 KB] || YTframe_RomanTRANSPORT_Still_searchweb.png (320x180) [91.7 KB] || YTframe_RomanTRANSPORT_Still_thm.png (80x40) [9.9 KB] || RomanTransportCaptions.en_US.srt [682 bytes] || RomanTransportCaptions.en_US.vtt [656 bytes] || 15064_RomanTransport_1080.mp4 (3840x2160) [175.8 MB] || 15064_RomanTransport_15mbps_4k.mp4 (3840x2160) [261.6 MB] || 15064_RomanTransport_25mbps_4k.mp4 (3840x2160) [432.6 MB] || 15064_RomanTransport_NoText_4k.mp4 (3840x2160) [1.3 GB] || 15064_RomanTransport_ProRes_3840x2160_2997.mov (3840x2160) [7.8 GB] || ", "hits": 413 }, { "id": 15067, "url": "https://svs.gsfc.nasa.gov/15067/", "result_type": "B-Roll", "release_date": "2026-07-28T12:00:00-04:00", "title": "Roman Pegasus Transport B-roll", "description": "Select drone shots of Pegasus sailing from Baltimore Harbor and under the Chesapeake Bay Bridge. Captured by Rob Fortunato and Christopher Albert. || Drone_Selects_Still.jpg (3840x2160) [2.5 MB] || Drone_Selects_Still_searchweb.png (320x180) [69.8 KB] || Drone_Selects_Still_thm.png (80x40) [4.3 KB] || Pegasus_Drone_Selects_Albert-Fortunato_June132026.mp4 (3840x2160) [690.8 MB] || ", "hits": 74 }, { "id": 15058, "url": "https://svs.gsfc.nasa.gov/15058/", "result_type": "Produced Video", "release_date": "2026-07-08T14:00:00-04:00", "title": "Roman Space Telescope and The Journey to Space", "description": "NASA's Nancy Grace Roman Space Telescope recently completed an epic 8-day voyage, the culmination of more than a decade of dedicated cross-country teamwork. This video retraces Roman's journey from humble beginnings as individual components spread across the country to the observatory's completion at NASA's Goddard Space Flight Center in Greenbelt, Md., and finally to the launch site at NASA's Kennedy Space Center in Florida. Next, Roman will undergo final preparations prior to launch, which is slated for Aug. 30.Narrated by John Rhys-DaviesMusic: “Comic Book Hero,” Adam Saunders [PRS] and Mark Stephen Cousins [PRS], Universal Production Music Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Map_Video_Thumbnail_V2.jpg (1920x1080) [1.3 MB] || Roman_Map_Video_Thumbnail_V2_searchweb.png (320x180) [110.9 KB] || Roman_Map_Video_Thumbnail_V2_thm.png (80x40) [8.3 KB] || 15058_Roman_Map_Good.mp4 (1920x1080) [137.5 MB] || 15058_Roman_Map_YT.mp4 (1920x1080) [434.3 MB] || RomanMapCaptions.en_US.srt [1.3 KB] || RomanMapCaptions.en_US.vtt [1.3 KB] || 15058_Roman_Map_ProRes_1920x1080_2997.mov (1920x1080) [1.2 GB] || ", "hits": 213 }, { "id": 15053, "url": "https://svs.gsfc.nasa.gov/15053/", "result_type": "Produced Video", "release_date": "2026-06-17T13:15:00-04:00", "title": "NASA’s Fermi Mission Reveals Related Supernova Remnants", "description": "This multiwavelength scene shows the Jellyfish Nebula supernova remnant (right), the interstellar cloud it’s interacting with, and a distinctive curving filament to its upper left. The filament, which is shown here both in optical and ultraviolet (UV) light, is the visible part of an overlapping supernova remnant, G189.6+3.3, that is more prominent in radio and X-rays. Data inlcudes NASA’s Neil Gehrels Swift Observatory and NASA’s retired WISE (Wide-field Infrared Survey Explorer) mission.", "hits": 332 }, { "id": 15041, "url": "https://svs.gsfc.nasa.gov/15041/", "result_type": "Produced Video", "release_date": "2026-05-20T09:00:00-04:00", "title": "NASA's Fermi Spies a Supercharged Supernova", "description": "Gamma rays detected by NASA’s Fermi Gamma-ray Space Telescope gave scientists a look under the hood of a rare supernova that produced much more light than normal.Credit: NASA’s Goddard Space Flight CenterMusic credits:\"Granular Game\" by John Bisset \"In The Zone\" by Daniel Migdal, Jonas Pomo\"Ornaments\" by Lisa Van Hal || Fermi_Spies_a_Supercharged_Supernova_Thumbnail.jpg (1280x720) [231.5 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.en_US.srt [2.2 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.en_US.vtt [2.1 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.webm (3840x2160) [34.1 MB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.mp4 (3840x2160) [892.9 MB] || 15041-_Fermi_Spies_a_Supercharged_Supernova_ProRes.mov (3840x2160) [6.3 GB] || ", "hits": 410 }, { "id": 20413, "url": "https://svs.gsfc.nasa.gov/20413/", "result_type": "Animation", "release_date": "2026-05-20T09:00:00-04:00", "title": "Supernova explosion animation, with & without pulsar", "description": "This animation shows a supernova — the explosion of a massive star — and the formation of an expanding cloud of debris called a supernova remnant. As the brightness fades, a pulsing light source appears at the center, surrounded by a small expanding nebula. The pulsing object is a pulsar, a type of neutron star, which represents the core of the massive star that exploded. The cloud around it is a pulsar wind nebula, which is formed and maintained by an outflow of particles streaming away from the neutron star. A version of the animation is available without the pulsar.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || SN_HQ_Full_H264_V001.00750_print.jpg (1024x576) [120.0 KB] || SN_HQ_Full_H264_V001.00750_searchweb.png (320x180) [77.3 KB] || SN_HQ_Full_H264_V001.00750_web.png (320x180) [77.3 KB] || SN_HQ_Full_H264_V001.00750_thm.png (80x40) [5.9 KB] || SN_HQ_Full_1080_V001.mp4 (1920x1080) [97.4 MB] || SN_HQ_Full_H264_V001.mp4 (3840x2160) [63.7 MB] || SN_HQ_Full_onlypulsar_V001.mov (3840x2160) [119.4 MB] || SN_HQ_Full_V001.mov (3840x2160) [2.5 GB] || SN_HQ_Full_nopulsar_V001.mov (3840x2160) [2.5 GB] || ", "hits": 1591 }, { "id": 15033, "url": "https://svs.gsfc.nasa.gov/15033/", "result_type": "Produced Video", "release_date": "2026-05-12T00:00:00-04:00", "title": "TESS Finds Possible New Worlds Using Stellar Eclipses", "description": "A gas giant planet looms in the foreground at right, illuminated by a pair of stars, in this artist’s concept of a world in a binary system. NASA’s TESS (Transiting Exoplanet Survey Satellite) has found planets in two binary star systems by looking for stellar dimming as the planets cross in front of one of the stars. Astronomers have now demonstrated a new method of finding planets in these systems by focusing on the timing of the stars’ mutual eclipses. Credit: NASA's Goddard Space Flight Center/Chris Smith (USRA)Alt text: Planet orbiting a binary systemImage description: Against a starry sky suffused with an orange glow, a gas giant planet with purple and white clouds appears in its crescent phase at right. Two bright stars illuminate the scene, one large and whitish at left, the other smaller and more orange near the center. || circumbinary_planet_AC.png (3991x2160) [3.7 MB] || circumbinary_planet_AC_print.jpg (1024x554) [71.5 KB] || circumbinary_planet_no_text.png (3991x2160) [3.7 MB] || ", "hits": 409 }, { "id": 15004, "url": "https://svs.gsfc.nasa.gov/15004/", "result_type": "Produced Video", "release_date": "2026-04-21T13:00:00-04:00", "title": "Nancy Grace Roman Space Telescope is Ready for Launch", "description": "The Nancy Grace Roman Space Telescope is scheduled to launch in September 2026. That is nearly eight months ahead of its required launch readiness date of May 2027.In its final years of construction, the observatory underwent rigorous environmental tests designed to prove it can withstand the demanding journey from Earth to space.These environmental tests included blasting the telescope with the intense sound of a rocket launch, vibrating the observatory while enclosed in a protective clean tent, another launch simulation, and placing it inside a thermal vacuum chamber where it was cooled to the extreme operating temperatures of space.Each of these tests proved Roman's worthiness for early flight and is a testament to the hard work from the entire team. || ", "hits": 542 }, { "id": 14997, "url": "https://svs.gsfc.nasa.gov/14997/", "result_type": "Produced Video", "release_date": "2026-04-08T16:00:00-04:00", "title": "Drone Footage of The Nancy Grace Roman Space Telescope Fully Deployed", "description": "The Nancy Grace Roman Space Telescope stands fully deployed as it will be in space. The solar panels reach their full width of over 14 feet (4.3 meters), and with the Deployable Aperture Cover standing tall, this observatory towers over 42 feet (12.8 meters) high –– taller than any other telescope created at NASA's Goddard Space Flight Center.This is the first drone footage captured inside a NASA cleanroom, fitting for Goddard's largest telescope. || ", "hits": 236 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 430 }, { "id": 14976, "url": "https://svs.gsfc.nasa.gov/14976/", "result_type": "Produced Video", "release_date": "2026-02-20T00:00:00-05:00", "title": "Fermi's 15-year View of the Gamma-Ray Sky", "description": "This image shows the entire sky as seen by Fermi's Large Area Telescope. Lighter colors indicate brighter gamma-ray sources. The map is centered on the center of our galaxy. The most prominent feature is the bright, diffuse glow running along the middle of the map, which marks the central plane of our Milky Way galaxy. The gamma rays there are mostly produced when energetic particles accelerated in the shock waves of supernova remnants collide with gas atoms and even light between the stars. Many of the star-like features above and below the Milky Way plane are distant galaxies powered by supermassive black holes. Many of the bright sources along the plane are pulsars. The image was constructed from 15 years of observations using front-converting gamma rays with energies greater than 1 GeV. Hammer projection with black background.Credit: NASA/DOE/Fermi LAT CollaborationAlt text: Fermi 15-year all-sky gamma-ray mapImage description: A colorful oval map sits in the middle of a black background. The oval is predominantly royal blue, striped with an irregular bright red, orange, and yellow band horizontally across the center, which shows the plane of our Milky Way galaxy. Smaller dots and splotches in red, orange, yellow, and white appear throughout the oval. || intens_ait_180m_gt1000_psf3_gal_0p1.png (3600x1800) [2.9 MB] || intens_ait_180m_gt1000_psf3_gal_0p1_print.jpg (1024x512) [290.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_searchweb.png (320x180) [74.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_thm.png (80x40) [4.6 KB] || ", "hits": 166 }, { "id": 14884, "url": "https://svs.gsfc.nasa.gov/14884/", "result_type": "Produced Video", "release_date": "2026-01-29T11:00:00-05:00", "title": "NASA Supercomputer Probes Tangled Magnetospheres of Merging Neutron Stars", "description": "New supercomputer simulations explore the tangled magnetic structures around merging neutron stars. These structures, called magnetospheres, interact as the city-sized stars enter their final orbits. Magnetic field lines can connect both stars, break, and reconnect, while currents surge through surrounding plasma moving at nearly the speed of light. The simulations show that these systems may produce X-rays and gamma rays that future observatories should be able to detect. Credit: NASA’s Goddard Space Flight CenterAlt text: Narrated video introducing simulations of merging neutron star magnetospheresMusic: “A Theory Develops,” Pip Heywood [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NS_Binary_Sim_Still.jpg (5760x3240) [1.4 MB] || NS_Binary_Sim_Still_searchweb.png (320x180) [67.6 KB] || NS_Binary_Sim_Still_thm.png (80x40) [5.2 KB] || 14884_NeutronStarBinarySim2_good.mp4 (1920x1080) [220.4 MB] || 14884_NeutronStarBinarySim2_best.mp4 (1920x1080) [363.9 MB] || NeutronStarBinarySimulationCaptions.en_US.srt [2.4 KB] || NeutronStarBinarySimulationCaptions.en_US.vtt [2.2 KB] || 14884_NeutronStarBinarySim2_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || ", "hits": 296 }, { "id": 14891, "url": "https://svs.gsfc.nasa.gov/14891/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Roman and Webb's Overlapping Roles in Understanding Our Universe", "description": "The four Roman/Webb Far and Wide videos that detail the differences between the two missions, why we need both, what they will do and how they will work together.", "hits": 425 }, { "id": 14943, "url": "https://svs.gsfc.nasa.gov/14943/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Additional Graphics", "description": "This page houses animation clips from the Far and Wide video series, which may be useful in presentations or other video products. || ", "hits": 111 }, { "id": 14916, "url": "https://svs.gsfc.nasa.gov/14916/", "result_type": "Produced Video", "release_date": "2025-12-08T09:30:00-05:00", "title": "Black Hole Eats Star: The Longest GRB Ever Seen", "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ", "hits": 483 }, { "id": 14933, "url": "https://svs.gsfc.nasa.gov/14933/", "result_type": "Produced Video", "release_date": "2025-12-04T09:00:00-05:00", "title": "XRISM Finds Elemental Bounty in Supernova Remnant", "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ", "hits": 110 }, { "id": 14928, "url": "https://svs.gsfc.nasa.gov/14928/", "result_type": "Produced Video", "release_date": "2025-11-20T10:00:00-05:00", "title": "TESS Triples Size of Pleiades Star Cluster", "description": "These young, hot blue stars are members of the Pleiades open star cluster and reside about 430 light-years away in the northern constellation Taurus. The brightest stars are visible to the unaided eye during evenings from October to April. A new study finds the cluster to be triple the size previously thought — and shows that its stars are scattered across the night sky. The Schmidt telescope at the Palomar Observatory in California captured this color-composite image. Credit: NASA, ESA, and AURA/CaltechAlt text: Members of the Pleiades shine in blue. Image description: The Pleiades are shown in this image. Six of the stars, all blue-white, are larger than the others and have diffraction spikes and faint blue circles around them. Other, smaller blue stars are also scattered across the image. Patches of swirling blue dust surround some of the stars. || STScI-01EVVEYWX1TA3MGBK5F6EFQVGQ.jpg (4877x3513) [1.1 MB] || ", "hits": 288 }, { "id": 14818, "url": "https://svs.gsfc.nasa.gov/14818/", "result_type": "Produced Video", "release_date": "2025-09-26T12:00:00-04:00", "title": "Plunge: Behind the Scenes Creating NASA's Black Hole Visualization", "description": "Behind the scenes video about the Black Hole visualization from 2024", "hits": 270 }, { "id": 14881, "url": "https://svs.gsfc.nasa.gov/14881/", "result_type": "Animation", "release_date": "2025-08-13T00:00:00-04:00", "title": "Fermi Spacecraft Animations 2025", "description": "A beauty pass of NASA's Fermi Gamma-ray Space Telescope. The spacecraft fills the frame with a starry background at 0:05 and is fully in frame with Earth partially in the background at 0:11.Credit: NASA's Goddard Space Flight Center/CI Lab || Fermi_Beauty_Still.jpg (3840x2160) [250.1 KB] || Fermi_Beauty_Still_searchweb.png (320x180) [11.5 KB] || Fermi_Beauty_Still_thm.png (80x40) [1.6 KB] || Fermi_BeautyPass_1080.mp4 (1920x1080) [46.1 MB] || Fermi_BeautyPass_4k.mp4 (3840x2160) [113.7 MB] || Fermi_BeautyPass_V002_ProRes_4k.mov (3840x2160) [1.3 GB] || ", "hits": 88 }, { "id": 14859, "url": "https://svs.gsfc.nasa.gov/14859/", "result_type": "Produced Video", "release_date": "2025-06-21T00:00:00-04:00", "title": "Webb Stellarium", "description": "Stellarium is an installation video designed for the Goddard Space Flight Center visitor center. It is playing temporarily in the room designed for Solarium, and installation built around Sun footage from the Solar Dynamics Observatory (SDO).\r\n\r\nStellarium sources James Webb Space Telescope imagery processed and provided by the Space Telescope Science Institute and available here.", "hits": 112 }, { "id": 14857, "url": "https://svs.gsfc.nasa.gov/14857/", "result_type": "Produced Video", "release_date": "2025-06-11T14:10:00-04:00", "title": "NASA’s Webb Reveals Galaxy Population Driving Cosmic Renovation", "description": "Symbols mark the locations of young, low-mass galaxies bursting with new stars when the universe was about 800 million years old. Using a filter sensitive to such galaxies, NASA’s James Webb Space Telescope imaged them with the help of a natural gravitational lens created by the massive galaxy cluster Abell 2744. In all, 83 young galaxies were found, but only the 20 shown here (white diamonds) were selected for deeper study. The inset zooms into one of the galaxies. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025Alt text: Animation showing the locations of young, low-mass, starburst galaxies around galaxy cluster Abell 2744.Image description:White and yellow galaxies of various sizes and shapes appear against the blackness of space. Two bright stars in our own galaxy display prominent six-spike diffraction patterns with bluish rays, visible at center left and lower left. Then 20 white diamonds sweep across the image. One diamond enlarges to reveal an image of a young, low-mass, star-forming galaxy. It looks like a green oval against a red and green checked background. The enlarged image then shrinks back, and the diamonds sweep away. The sequence loops. || Pandora_stamp_60pct.gif (600x600) [961.0 KB] || ", "hits": 130 }, { "id": 14792, "url": "https://svs.gsfc.nasa.gov/14792/", "result_type": "Produced Video", "release_date": "2025-05-27T20:57:00-04:00", "title": "Astrophysics Missions Vertical Video", "description": "This page collects vertical videos related to specific Astrophysics missions and their hardware or capabilities.", "hits": 57 }, { "id": 14793, "url": "https://svs.gsfc.nasa.gov/14793/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Black Holes Vertical Video", "description": "This page collects Astrophysics vertical videos with black-hole-related content", "hits": 1189 }, { "id": 14797, "url": "https://svs.gsfc.nasa.gov/14797/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Exoplanets Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to the topic of exoplanets.", "hits": 130 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 238 }, { "id": 14842, "url": "https://svs.gsfc.nasa.gov/14842/", "result_type": "B-Roll", "release_date": "2025-05-19T00:00:00-04:00", "title": "Roman Space Telescope's Outer Shell Passes Thermal Test - Drone Footage", "description": "The outer portion of the Nancy Grace Roman Space Telescope recently passed a major milestone: thermal cycling. Drone footage captures its emergence from the test facility and return to the clean room. The Roman Space Telescope is a NASA observatory designed to perform wide-field imaging and surveys of the near-infrared sky. || ", "hits": 81 }, { "id": 14834, "url": "https://svs.gsfc.nasa.gov/14834/", "result_type": "Produced Video", "release_date": "2025-05-12T00:00:00-04:00", "title": "Cosmic Dawn: The Untold Story of the James Webb Space Telescope", "description": "For more than three decades, NASA and an international team of scientists and engineers pushed the limits of technology, innovation, and perseverance to build and launch the James Webb Space Telescope, the most powerful space observatory ever created. Cosmic Dawn brings audiences behind the scenes with the Webb film crew, and never-before-heard testimonies revealing the real story of how this telescope overcame all odds. ||", "hits": 283 }, { "id": 20399, "url": "https://svs.gsfc.nasa.gov/20399/", "result_type": "Animation", "release_date": "2025-03-19T00:00:00-04:00", "title": "XMM-Newton spacecraft animations", "description": "Flyby animation of ESA's (European Space Agency's) XMM-Newton observatory as it orbits Earth.Credit: NASA/ESA || XMM_Beauty_Still.jpg (3840x2160) [449.2 KB] || XMM_Beauty_Still_searchweb.png (320x180) [38.6 KB] || XMM_Beauty_Shot_H264_V1.mp4 (3840x2160) [23.4 MB] || XMM_Beauty_Still_thm.png [3.3 KB] || XMM_Beauty_Shot_Prores_V1.mov (3840x2160) [807.2 MB] || ", "hits": 91 }, { "id": 14786, "url": "https://svs.gsfc.nasa.gov/14786/", "result_type": "Animation", "release_date": "2025-02-20T00:00:00-05:00", "title": "Swift Spacecraft Animations: 2025", "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || Swift_S1_v2_4k60.hwshow [423 bytes] || ", "hits": 169 }, { "id": 14778, "url": "https://svs.gsfc.nasa.gov/14778/", "result_type": "Produced Video", "release_date": "2025-02-05T21:00:00-05:00", "title": "Fast Field Trips", "description": "Thermal Blanket Technician Paula Cain gives us a tour of the lab, including a special look at how she created the Artemis II zero-gravity indicator \"Rise.\"\"Found in a Dream,\" \"Looking Back,\" Universal Production Music.Complete transcript available. || FFT_ThermalBlanketxRise_thumb.png (1080x1920) [1.6 MB] || FFT_ThermalBlanketxRise_thumb_print.jpg (1024x1820) [312.1 KB] || FFT_ThermalBlanketxRise_thumb_searchweb.png (320x180) [104.5 KB] || FFT_ThermalBlanketxRise_thumb_thm.png (80x40) [6.9 KB] || FFT_ThermalBlanketxRise_NoCap.webm (1080x1920) [17.6 MB] || FFT_ThermalBlanketxRise_IG.mp4 (1080x1920) [165.4 MB] || FFT_ThermalBlanketxRise_NoCap.mp4 (1080x1920) [165.3 MB] || FFT_ThermalBlanketxRise.en_US.srt [5.2 KB] || FFT_ThermalBlanketxRise.en_US.vtt [4.9 KB] || ", "hits": 110 }, { "id": 14747, "url": "https://svs.gsfc.nasa.gov/14747/", "result_type": "Produced Video", "release_date": "2025-01-16T10:15:00-05:00", "title": "Pandora Spacecraft Animations", "description": "Animated beauty pass of an artist's concept of the Pandora spacecraft, viewed without thermal blankets, set in a neutral gray volume. Credit: NASA's Goddard Space Flight Center/Conceptual Image LabAlt text: Pandora spacecraft animation no. 1Image description: An artist’s concept of NASA’s exoplanet explorer, Pandora, floats in a light gray background. The body of the small satellite looks like a black box with metal hardware. A long metallic cylinder extends upward from the body with multiple thin rings that slightly protrude from the surface and a flat metal rectangle on one side. On the underside of the body is a shiny dark circle. Pandora’s three solar panels extend from one side of the spacecraft’s body. The visible side is gray and laced with white wires, and the panels are connected with small silver fasteners. || Pandora_Beauty_S1_Still.jpg (3840x2160) [1.0 MB] || Pandora_Beauty_S1_Still_searchweb.png (320x180) [37.2 KB] || Pandora_Beauty_S1_Still_thm.png [4.0 KB] || Pandora_Beauty_S1_1080.mp4 (1920x1080) [14.7 MB] || Pandora_Beauty_S1_4k.mp4 (3840x2160) [36.6 MB] || Pandora_Beauty_S1_ProRes_3840x2160_30.mov (3840x2160) [1.1 GB] || ", "hits": 127 }, { "id": 14754, "url": "https://svs.gsfc.nasa.gov/14754/", "result_type": "Produced Video", "release_date": "2025-01-16T10:14:00-05:00", "title": "NASA’s Pandora Mission Closer To Probing Alien Atmospheres", "description": "Basic overview of NASA's Pandora mission, which will revolutionize the study of exoplanet atmospheres.", "hits": 230 }, { "id": 14753, "url": "https://svs.gsfc.nasa.gov/14753/", "result_type": "Produced Video", "release_date": "2025-01-13T10:14:00-05:00", "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole", "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ", "hits": 105 }, { "id": 14738, "url": "https://svs.gsfc.nasa.gov/14738/", "result_type": "Produced Video", "release_date": "2024-12-20T10:00:00-05:00", "title": "What Are Gamma-ray Bursts?", "description": "Watch to learn more about gamma-ray bursts, the most powerful explosions in the cosmos. They first came to the attention of astronomers in the 1970s when new satellites detected this surprising phenomenon. Over decades, scientists have found that these blasts could be detected somewhere in the sky almost every day, and that they were both extremely distant — the closest known is over 100 million light-years away — and enormously powerful. Gamma-ray bursts are now linked to the explosive deaths of massive stars and to mergers of compact objects, like neutron stars and black holes, but many puzzles remain. Credit: NASA’s Goddard Space Flight CenterMusic: “Time Science,” Steve Fawcett [ASCAP] and Katherine F Martin [BMI], Universal Production Music Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_ASD_GRB.jpg (1280x720) [221.2 KB] || YTframe_ASD_GRB_searchweb.png (320x180) [81.7 KB] || YTframe_ASD_GRB_thm.png (80x40) [9.6 KB] || 14738_GRBexplainer_Small.mp4 (1920x1080) [117.7 MB] || 14738_GRBexplainer_Best.mp4 (1920x1080) [526.7 MB] || 14738GRBexplainerCaptions.en_US.srt [4.4 KB] || 14738GRBexplainerCaptions.en_US.vtt [4.2 KB] || 14738_GRBexplainer_ProRes_1920x1080_2997.mov (1920x1080) [2.9 GB] || ", "hits": 547 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 159 }, { "id": 14720, "url": "https://svs.gsfc.nasa.gov/14720/", "result_type": "Produced Video", "release_date": "2024-11-22T10:00:00-05:00", "title": "COBE All-Sky Map 360 Video With Narration", "description": "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.(This video is formatted for 360-degree use.)Credit: NASA's Goddard Space Flight CenterMusic: “Meetings in Underwater Ruins,” Philippe Andre Vandenhende [SACEM], Olivier Louis Perrot [SACEM] and Idriss-El-Mehdi Bennani [SACEM], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Design_hybrid_COBE_360.jpg (1280x720) [235.1 KB] || YTframe_Design_hybrid_COBE_360_searchweb.png (320x180) [80.8 KB] || YTframe_Design_hybrid_COBE_360_thm.png (80x40) [9.2 KB] || 14720_COBE_360_Captions.en_US.srt [4.7 KB] || 14720_COBE_360_Captions.en_US.vtt [4.4 KB] || 14720_COBE_360_Narrated_Good.mp4 (8192x4096) [131.8 MB] || 14720_COBE_360_Narrated_Best.mp4 (8192x4096) [503.2 MB] || ", "hits": 184 }, { "id": 14721, "url": "https://svs.gsfc.nasa.gov/14721/", "result_type": "Produced Video", "release_date": "2024-11-20T10:00:00-05:00", "title": "What's In A Name? NASA's Swift Mission", "description": "Watch to learn how NASA’s Neil Gehrels Swift Observatory got its name.Credit: NASA’s Goddard Space Flight CenterMusic: “In a Conundrum,” Pip Heywood [PRS], Universal Production Music“Spinning Particles,” Christian Telford [ASCAP] and Koichi Sanchez-Imahashi [ASCAP], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Swift_Name_20_Thumbnail2.jpg (1280x720) [308.5 KB] || Swift_Name_20_Thumbnail2_searchweb.png (320x180) [103.9 KB] || Swift_Name_20_Thumbnail2_thm.png (80x40) [9.3 KB] || 14721_Swift20_WhatsInAName_Good.mp4 (1920x1080) [199.2 MB] || 14721_Swift20_WhatsInAName_Best.mp4 (1920x1080) [883.1 MB] || 14721_Swift20_WhatsInAName_Captions.en_US.srt [3.7 KB] || 14721_Swift20_WhatsInAName_Captions.en_US.vtt [3.5 KB] || 14721_Swift20_WhatsInAName_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || ", "hits": 125 }, { "id": 11738, "url": "https://svs.gsfc.nasa.gov/11738/", "result_type": "Infographic", "release_date": "2024-11-20T00:00:00-05:00", "title": "Infographic: NASA's Neil Gehrels Swift Observatory", "description": "This infographic summarizes key aspects of NASA's Swift mission, from its instruments to scientific results gleaned from 20 years of operations. Swift is still going strong, and the observatory remains a key part of NASA’s strategy to monitor the changing sky with multiple telescopes using different approaches for studying the cosmos.Credit: NASA's Goddard Space Flight CenterClick the download button to select from a range of sizes. || Swift_20_Infographic_Quarter.jpg (1550x1991) [1.2 MB] || Swfit_20_Poster_CMYK.jpg (6200x7965) [19.2 MB] || Swift_20_Infographic_Full.jpg (6200x7965) [7.4 MB] || Swift_20_Infographic_Full.png (6200x7965) [34.2 MB] || Swift_20_Infographic_Half.jpg (3100x3983) [3.2 MB] || Swift_20_Infographic_Half.png (3100x3983) [10.5 MB] || Swift_20_Infographic_Full.jpg.dzi [178 bytes] || Swift_20_Infographic_Full.jpg_files [4.0 KB] || ", "hits": 301 }, { "id": 14715, "url": "https://svs.gsfc.nasa.gov/14715/", "result_type": "Produced Video", "release_date": "2024-11-18T00:00:00-05:00", "title": "COBE Celebrates 35th Launch Anniversary", "description": "Technicians work on the COBE (Cosmic Background Explorer) spacecraft in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission launched into an Earth orbit in 1989 to make an all-sky map of the cosmic microwave background, the oldest light in the universe. The conical silver shield protects the scientific instruments from direct radiation from the Sun and Earth, isolates them from radio-frequency interference from the spacecraft transmitters and terrestrial sources, and provides thermal isolation for a dewar containing liquid helium coolant.Credit: NASA/COBE Science Team || COBE_in_gfsc_clean_room_1.jpg (1629x1600) [552.8 KB] || ", "hits": 138 }, { "id": 20393, "url": "https://svs.gsfc.nasa.gov/20393/", "result_type": "Animation", "release_date": "2024-11-04T11:00:00-05:00", "title": "T Coronae Borealis Nova Animations", "description": "Located 3,000 light-years away, T Coronae Borealis — T CrB for short — contains two stars that orbit each other: a red giant nearing the end of its life and an Earth-sized stellar remnant known as a white dwarf. The dwarf’s intense gravity rounds up some of the gas flowing off of the red giant, forming a flattened cloud of gas around the dwarf — an accretion disk. Gas in the disk gradually works its way inward, eventually flowing onto the white dwarf nestled at its center. Credit: NASA's Goddard Space Flight Center Conceptual Image LabAlt text: Animation showing the T CrB system || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.00300_print.jpg (1024x576) [91.6 KB] || T_CrB_NOVA_SHOT_1_4k_30fps_h264.mp4 (3840x2160) [18.1 MB] || T_CrB_Nova_S1 [0 Item(s)] || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.webm (3840x2160) [4.5 MB] || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.mov (3840x2160) [984.5 MB] || ", "hits": 844 }, { "id": 14698, "url": "https://svs.gsfc.nasa.gov/14698/", "result_type": "Produced Video", "release_date": "2024-10-22T11:00:00-04:00", "title": "NASA Reveals LISA Engineering Development Unit Telescope", "description": "NASA has revealed the first look at a full-scale prototype for six telescopes that will enable, in the next decade, the space-based detection of gravitational waves — ripples in space-time caused by merging black holes and other cosmic sources.The LISA (Laser Interferometer Space Antenna) mission is led by ESA (European Space Agency) in partnership with NASA to detect gravitational waves by using lasers to measure precise distances — down to picometers, or trillionths of a meter — between a trio of spacecraft distributed in a vast configuration larger than the Sun. Each side of the triangular array will measure nearly 1.6 million miles, or 2.5 million kilometers.Twin telescopes aboard each spacecraft will both transmit and receive infrared laser beams to track their companions, and NASA is supplying all six of them to the LISA mission. The prototype, called the Engineering Development Unit Telescope, will provide guidance as engineers and scientists work toward building the flight hardware.In May, the prototype, which was manufactured and assembled by L3Harris Technologies in Rochester, New York, arrived at NASA's Goddard Space Flight Center in Greenbelt, Maryland. The primary mirror is coated in gold to better reflect the infrared lasers and to reduce heat loss from a surface exposed to cold space since the telescope will operate best when close to room temperature. The prototype is made entirely from an amber-colored glass-ceramic called Zerodur, manufactured by Schott in Mainz, Germany. The material is widely used for telescope mirrors and other applications requiring high precision because its shape changes very little over a wide range of temperatures. || ", "hits": 182 }, { "id": 14694, "url": "https://svs.gsfc.nasa.gov/14694/", "result_type": "Produced Video", "release_date": "2024-10-03T11:00:00-04:00", "title": "Legacy of Light Concluding Video", "description": "This video appeared at the conclusion of the Legacy of Light event on September 25, 2024. It foregrounds the importance of the Hubble, Webb and Roman observatories in enabling the Habitable Worlds Observatory, which could answer one of our most fundamental questions: are we alone?Credit: NASA's Goddard Space Flight CenterMusic: \"Infinite Horizons,\" Dan Thiessen [BMI] Universal Production MusicComplete transcript available. || NASM_HWO_Still.jpg (1920x1080) [409.5 KB] || NASM_HWO_Still_searchweb.png (320x180) [35.4 KB] || NASM_HWO_Still_thm.png (80x40) [3.3 KB] || LegacyOfLightConclusionCaptions.en_US.srt [972 bytes] || LegacyOfLightConclusionCaptions.en_US.vtt [934 bytes] || LegacyOfLightConclusion_ProRes_1920x1080_2398.mov (1920x1080) [2.0 GB] || LegacyOfLightConclusion_better.mp4 (1920x1080) [455.3 MB] || LegacyOfLightConclusion_good.mp4 (1920x1080) [204.0 MB] || LegacyOfLightConclusion_YT.mp4 (1920x1080) [842.2 MB] || ", "hits": 65 }, { "id": 14693, "url": "https://svs.gsfc.nasa.gov/14693/", "result_type": "Produced Video", "release_date": "2024-10-02T12:00:00-04:00", "title": "NASA's Nancy Grace Roman Space Telescope: Systems, Assemble!", "description": "In September 2024, the Nancy Grace Roman Space Telescope passed a key milestone and was approved for the next stage of construction. Work on the main systems that will make up the final spacecraft is finishing, and the team at NASA’s Goddard Space Flight Center is ready to begin integration, the process of connecting them together. This video celebrates the effort to reach the final stages of assembly.Music: “The Call,” Torsti Juhani Spoof [BMI] Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Building_Roman_Main2.jpg (1280x720) [451.7 KB] || YTframe_Building_Roman_Main2_searchweb.png (320x180) [124.6 KB] || YTframe_Building_Roman_Main2_thm.png (80x40) [11.0 KB] || 14693_RomanSystemsAssemble_Good.mp4 (1920x1080) [234.1 MB] || 14693_RomanSystemsAssemble_Better.mp4 (1920x1080) [444.0 MB] || 14693RomanSystemsAssembleCaptions.en_US.srt [491 bytes] || 14693RomanSystemsAssembleCaptions.en_US.vtt [475 bytes] || 14693_RomanSystemsAssemble_YouTube.mp4 (1920x1080) [1012.1 MB] || 14693_RomanSystemsAssemble_ProRes1920x1080_2997.mov (1920x1080) [2.8 GB] || 14693_RomanSystemsAssemble_Better.hwshow [508 bytes] || ", "hits": 79 }, { "id": 14634, "url": "https://svs.gsfc.nasa.gov/14634/", "result_type": "Produced Video", "release_date": "2024-07-25T14:00:00-04:00", "title": "Fermi Finds Novel Feature in BOAT Gamma-Ray Burst", "description": "The brightest gamma-ray burst yet recorded gave scientists a new high-energy feature to study. Learn what NASA’s Fermi mission saw, and what this feature may be telling us about the burst’s light-speed jets. Credit: NASA's Goddard Space Flight CenterMusic: “Tides,” Jon Cotton [PRS] and Ben Niblett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Distant_GRB_still.jpg (3840x2160) [2.5 MB] || 14634_Fermi_GRB_Emission_Line_Under100.mp4 (1920x1080) [90.7 MB] || 14634_Fermi_GRB_Emission_Line_Best.mp4 (1920x1080) [422.0 MB] || 14634FermiGRBEmissionLine_Captions.en_US.srt [4.4 KB] || 14634FermiGRBEmissionLine_Captions.en_US.vtt [4.2 KB] || 14634_Fermi_GRB_Emission_Line_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || ", "hits": 119 }, { "id": 14581, "url": "https://svs.gsfc.nasa.gov/14581/", "result_type": "Produced Video", "release_date": "2024-05-23T10:00:00-04:00", "title": "Gliese 12 b: An Intriguing World Sized Between Earth and Venus", "description": "Gliese 12 b’s estimated size may be as large as Earth or slightly smaller — comparable to Venus in our solar system. This artist’s concept compares Earth with different possible Gliese 12 b interpretations, from no atmosphere to a thick Venus-like one. Follow-up observations with NASA’s James Webb Space Telescope will help determine just how much atmosphere the planet retains as well as its composition.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Alt text: Illustration of Earth compared to various models of Gliese 12 b Image description: At left, against a black background, floats an artist's concept of a nearly half-illuminated Earth, with clouds, blue oceans, and land areas rendered in green, tan, brown, and white. At right are three similarly illuminated planets, slightly smaller than Earth and each representing a possible interpretation of Gliese 12 b. The version on the left has a surface of blotchy reddish and brownish features and no atmosphere. The middle version has the same surface texture partly obscured by a hazy atmosphere. And the rightmost and smallest version of the planet has a thick, Venus-like atmosphere that obscures the surface completely. || Gl12b_Earth_Comparison_ac.jpg (3840x2160) [935.8 KB] || Gl12b_Earth_Comparison_ac_print.jpg (1024x576) [126.0 KB] || Gl12b_Earth_Comparison.jpg (3840x2160) [929.5 KB] || Gl12b_Earth_Comparison_ac_searchweb.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_web.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_thm.png (80x40) [9.8 KB] || Gl12b_Earth_Comparison.tif (3840x2160) [6.4 MB] || ", "hits": 512 }, { "id": 14584, "url": "https://svs.gsfc.nasa.gov/14584/", "result_type": "Produced Video", "release_date": "2024-05-08T09:00:00-04:00", "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy", "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ", "hits": 78 }, { "id": 14524, "url": "https://svs.gsfc.nasa.gov/14524/", "result_type": "Infographic", "release_date": "2024-05-07T10:00:00-04:00", "title": "Primordial Black Holes", "description": "This artist's concept takes a fanciful approach to imagining small primordial black holes. In reality, such tiny black holes would have a difficult time forming the accretion disks that make them visible here.Credit: NASA's Goddard Space Flight Center || Primordial_Black_Hole_Still_1080.jpg (1920x1080) [275.1 KB] || Primordial_Black_Hole_Still_4k_print.jpg (1024x576) [51.1 KB] || Primordial_Black_Hole_Still_4k.jpg (3840x2160) [2.5 MB] || Primordial_Black_Hole_Still_4k.png (3840x2160) [7.3 MB] || Primordial_Black_Hole_Still_4k_searchweb.png (320x180) [61.5 KB] || Primordial_Black_Hole_Still_4k_thm.png (80x40) [5.6 KB] || ", "hits": 1045 }, { "id": 14576, "url": "https://svs.gsfc.nasa.gov/14576/", "result_type": "Visualization", "release_date": "2024-05-06T13:00:00-04:00", "title": "NASA Black Hole Visualization Takes Viewers Beyond the Brink", "description": "In this flight toward a supermassive black hole, labels highlight many of the fascinating features produced by the effects of general relativity along the way. This supercomputer visualization tracks a camera as it approaches, briefly orbits, and then crosses the event horizon — the point of no return — of a supersized black hole similar in mass to the one at the center of our galaxy. Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. PowellMusic: “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music“Memories” from Digital Juice“Path Finder,” Eric Jacobsen [TONO] and Lorenzo Castellarin [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14576_BHPlunge_Explain_Still.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail_searchweb.png (180x320) [85.0 KB] || 14576_PageThumbnail_thm.png (80x40) [9.6 KB] || 14576_BHPlunge_Explainer_1080.mp4 (1920x1080) [319.5 MB] || 14576_BHPlunge_Explainer_Captions.en_US.srt [2.5 KB] || 14576_BHPlunge_Explainer_Captions.en_US.vtt [2.4 KB] || 14576_BHPlunge_Explainer_4k.mp4 (3840x2160) [1.5 GB] || 14576_BHPlunge_Explainer_4kYouTube.mp4 (3840x2160) [3.0 GB] || 14576_BHPlunge_Explainer_ProRes_3840x2160_2997.mov (3840x2160) [12.8 GB] || ", "hits": 3331 }, { "id": 14574, "url": "https://svs.gsfc.nasa.gov/14574/", "result_type": "Produced Video", "release_date": "2024-05-06T10:00:00-04:00", "title": "Black Hole Week 2024 Poster and Media", "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.", "hits": 158 }, { "id": 14585, "url": "https://svs.gsfc.nasa.gov/14585/", "result_type": "Visualization", "release_date": "2024-05-06T00:00:00-04:00", "title": "Beyond the Brink: Tracking a Simulated Plunge into a Black Hole", "description": "In this all-sky view, the camera approaches a supermassive black hole weighing 4.3 million Suns. It is about 70 million miles (113 million kilometers) from the black hole’s event horizon, the boundary of no return. It’s moving inward at 19% the speed of light — nearly 127 million mph (205 million kph). A flat, swirling cloud of hot, glowing gas called an accretion disk surrounds the black hole and serves as a visual reference during the fall, as do glowing structures called photon rings, which form closer to the black hole from light that has orbited it one or more times. A backdrop of the starry sky completes the scene.Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. Powell || 1_BH_Viz_20_rg_019c.jpg (8192x4096) [6.1 MB] || ", "hits": 530 }, { "id": 14463, "url": "https://svs.gsfc.nasa.gov/14463/", "result_type": "Produced Video", "release_date": "2024-04-30T11:00:00-04:00", "title": "XRISM Mission Captures Unmatched Data With Just 36 Pixels", "description": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XRISM_36_Pixels_Still.jpg (1920x1080) [959.9 KB] || XRISM_36_Pixels_Still_searchweb.png (320x180) [94.7 KB] || XRISM_36_Pixels_Still_thm.png (80x40) [7.0 KB] || 14463_XRISM_36Pixels_Good.mp4 (1920x1080) [148.9 MB] || 14463_XRISM_36Pixels_Best.mp4 (1920x1080) [514.8 MB] || 14463_XRISM_36Pixels_Captions.en_US.srt [4.6 KB] || 14463_XRISM_36Pixels_Captions.en_US.vtt [4.4 KB] || 14463_XRISM_36Pixels_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || ", "hits": 69 }, { "id": 14512, "url": "https://svs.gsfc.nasa.gov/14512/", "result_type": "B-Roll", "release_date": "2024-01-28T00:00:00-05:00", "title": "Aerial Views of Goddard: 2023 Wildfire Smoke", "description": "This panorama of NASA Goddard was taken on the morning of June 7, 2023, when smoke from raging wildfires in Eastern Canada wafted over the Mid-Atlantic region. The Integration and Test complex is located at top center in this view, looking north.Credit: NASA/Francis Reddy || Wildfire_Smoke_am_GSFC_06072023_looking_N.jpg (7500x3167) [7.9 MB] || Wildfire_Smoke_am_GSFC_06072023_looking_N_print.jpg (1024x432) [292.8 KB] || Wildfire_Smoke_am_GSFC_06072023_looking_N_searchweb.png (320x180) [111.8 KB] || Wildfire_Smoke_am_GSFC_06072023_looking_N_thm.png (80x40) [20.7 KB] || ", "hits": 61 }, { "id": 14727, "url": "https://svs.gsfc.nasa.gov/14727/", "result_type": "Produced Video", "release_date": "2024-01-22T00:00:00-05:00", "title": "Fort Sumner, New Mexico: 2024 Drone Views", "description": "This clip contains various shots of the NASA payload processing facility at Fort Sumner as well as general views of the surrounding area, acquired Aug. 23, 2024. Credit: NASA/Francis ReddyVideo playback is at half speed (30 fps). 0:00 A slow, early morning approach to the staging facility as its doors open, revealing the EXCITE (EXoplanet Climate Infrared TElescope) payload. 0:45 The camera descends, with the rising sun moving behind the staging facility. 0:58 A closer, lower approach to the EXCITE payload. 1:10 A higher, more distant arc that starts by showing the low sun and the NASA sign on the staging facility, moving north. 1:41 A slow ascent looking toward EXCITE and the morning sun. 1:28 Hovering as the doors close on EXCITE. 03:20 Overview flying back across the airport revealing various vehicles and structures. 4:41 Similar, but at higher altitude and flying in a different direction. || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.00001_print.jpg (1024x576) [139.0 KB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.webm (3840x2160) [67.5 MB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.mp4 (3840x2160) [2.9 GB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility_ProRes.mov (3840x2160) [22.1 GB] || ", "hits": 75 }, { "id": 14476, "url": "https://svs.gsfc.nasa.gov/14476/", "result_type": "Produced Video", "release_date": "2024-01-11T11:10:00-05:00", "title": "Fermi Mission Detects Surprising Gamma-Ray Feature Beyond Our Galaxy", "description": "This artist’s concept shows the entire sky in gamma rays with magenta circles illustrating the uncertainty in the direction from which more high-energy gamma rays than average seem to be arriving. In this view, the plane of our galaxy runs across the middle of the map. The circles enclose regions with a 68% (inner) and a 95% chance of containing the origin of these gamma rays. Credit: NASA’s Goddard Space Flight Center || Dark_Fermi_Dipole.jpg (3840x2160) [506.2 KB] || Dark_Fermi_Dipole.png (3840x2160) [8.9 MB] || Dark_Fermi_Dipole_searchweb.png (320x180) [57.6 KB] || Dark_Fermi_Dipole_thm.png (80x40) [5.4 KB] || ", "hits": 124 }, { "id": 14492, "url": "https://svs.gsfc.nasa.gov/14492/", "result_type": "Produced Video", "release_date": "2024-01-05T08:50:00-05:00", "title": "XRISM Reveals Its First Look at X-ray Cosmos", "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ", "hits": 112 }, { "id": 14491, "url": "https://svs.gsfc.nasa.gov/14491/", "result_type": "Produced Video", "release_date": "2023-12-26T00:00:00-05:00", "title": "Roman Hardware Highlights", "description": "This video 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. After a deployment test of the High-Gain Antenna, done on a structure called the Pantheon, 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 MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_WinterSpring2026_7.jpg (1280x720) [331.6 KB] || Roman_HH_Winter-Spring2026_10mbps.mp4 (1920x1080) [233.2 MB] || Roman_HH_Winter-Spring2026_20mbps.mp4 (1920x1080) [477.4 MB] || RomanHHEarly2026Captions.en_US.srt [2.0 KB] || RomanHHEarly2026Captions.en_US.vtt [1.9 KB] || Roman_HH_Winter-Spring2026_NoText.mp4 (1920x1080) [1.1 GB] || Roman_HH_Winter-Spring2026_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 159 }, { "id": 14399, "url": "https://svs.gsfc.nasa.gov/14399/", "result_type": "Produced Video", "release_date": "2023-12-20T11:00:00-05:00", "title": "Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky", "description": "From solar flares to black hole jets: NASA’s Fermi Gamma-ray Space Telescope has produced a unique time-lapse tour of the dynamic high-energy sky. Fermi Deputy Project Scientist Judy Racusin narrates this movie, which compresses 14 years of gamma-ray observations into 6 minutes. Credit: NASA’s Goddard Space Flight Center and NASA/DOE/LAT CollaborationMusic: \"Expanding Shell\" written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Video descriptive text available. || Fermi_14Year_Narrated_Still_print.jpg (1024x576) [157.6 KB] || Fermi_14Year_Narrated_Still.jpg (3840x2160) [891.9 KB] || Fermi_14Year_Narrated_Still_searchweb.png (320x180) [39.2 KB] || Fermi_14Year_Narrated_Still_thm.png (80x40) [4.2 KB] || 14399_Fermi_14Year_Narrated_sub100.mp4 (1920x1080) [90.5 MB] || 14399_Fermi_14Year_Narrated_1080.webm (1920x1080) [49.4 MB] || 14399_Fermi_14Year_Narrated_1080.mp4 (1920x1080) [908.7 MB] || Fermi_14Year_Narrated_SRT_Captions.en_US.srt [8.4 KB] || Fermi_14Year_Narrated_SRT_Captions.en_US.vtt [8.0 KB] || 14399_Fermi_14Year_Narrated_4k.mp4 (3840x2160) [2.2 GB] || 14399_Fermi_14Year_Narrated_ProRes_3840x2160_2997.mov (3840x2160) [19.4 GB] || ", "hits": 155 }, { "id": 14480, "url": "https://svs.gsfc.nasa.gov/14480/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: 180- and 360-Degree Panoramas", "description": "Two 180-degree pans from above the Goddard Main Gate sign in midday sun and fall colors. The first is fairly slow, the return pan is faster. Greenbelt Road is prominent at the start and end. Captured Nov. 9, 2023.Credit: NASA/Francis Reddy || Goddard_Panorama_From_Main_Gate_Still.jpg (3840x2160) [3.5 MB] || Goddard_Panorama_From_Main_Gate_Still_searchweb.png (320x180) [120.0 KB] || Goddard_Panorama_From_Main_Gate_Still_thm.png (80x40) [7.8 KB] || Goddard_PanoramaFromMainGate_clip_11132023_1080_30_15mbps.mp4 (1920x1080) [306.9 MB] || Goddard_PanoramaFromMainGate_clip_11092023_4k60_25mbps.mp4 (3840x2160) [511.6 MB] || Goddard_PanoramaFromMainGate_clip_11092023_4k60_100mbps.mp4 (3840x2160) [2.0 GB] || ", "hits": 62 }, { "id": 14481, "url": "https://svs.gsfc.nasa.gov/14481/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: Main Gate", "description": "Views of the Goddard Main Gate sign. The first clip shows the sign up close, then the camera pulls back swiftly. The other clips begin close to the sign and rise over the center at different speeds, looking northwest. Captured Nov. 9, 2023.Credit: NASA/Francis Reddy || Main_Gate_Still.jpg (3840x2160) [4.1 MB] || Main_Gate_Still_searchweb.png (320x180) [123.3 KB] || Main_Gate_Still_thm.png (80x40) [7.6 KB] || Goddard_MainGate_clips_11092023_1080_30_15mbps.mp4 (1920x1080) [209.6 MB] || Goddard_MainGate_clips_11092023_4k60_25mbps.mp4 (3840x2160) [346.5 MB] || Goddard_MainGate_clips_11092023_4k60_100mbps.mp4 (3840x2160) [1.3 GB] || ", "hits": 61 }, { "id": 14482, "url": "https://svs.gsfc.nasa.gov/14482/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: Buildings 32 and 33", "description": "Views of the east side of Building 32 in morning light and fall colors. Several clips fly toward and away from the east entrance. The next set of clips rise to various heights above the building. The final shot stays above the building and pulls back, looking west. Captured Nov. 9, 2023.Credit: NASA/Francis Reddy || Building_32_East_Corner_Close_Still.jpg (3840x2160) [3.3 MB] || Building_32_East_Corner_Close_Still_searchweb.png (320x180) [104.5 KB] || Building_32_East_Corner_Close_Still_thm.png (80x40) [6.7 KB] || Goddard_Bldg32EastCornerClose_clips_11092023_1080_30_15mbps.mp4 (1920x1080) [306.8 MB] || Goddard_Bldg32EastCornerClose_clips_11092023_4k60_25mbps.mp4 (3840x2160) [511.5 MB] || Goddard_Bldg32EastCornerClose_clips_11092023_4k60_100mbps.mp4 (3840x2160) [2.0 GB] || ", "hits": 71 }, { "id": 14483, "url": "https://svs.gsfc.nasa.gov/14483/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: Buildings 21 and 11", "description": "This sequence shows the northeast corner of Building 21, with the Goddard Library, near sunset and in fall colors, looking southwest. The first shot approaches the building horizontally at low altitude. The next shows a descent from moderate altitude, with Building 11 visible in the background; the following shot shows a rise to similar height and a similar descent. The next shot features a slow descent from several hundred feet, looking southwest into the sun and toward Building 11, followed by an ascent at similar pace and height. Captured Nov.14, 2023. Credit: NASA/Francis Reddy || Building_21_Library_Corner_Sunset_Still.jpg (3840x2160) [2.3 MB] || Building_21_Library_Corner_Sunset_Still_searchweb.png (320x180) [85.5 KB] || Building_21_Library_Corner_Sunset_Still_thm.png (80x40) [6.2 KB] || Goddard_Bldg21CornerSunset_clips_11132023_1080_30_15mbps.mp4 (1920x1080) [383.1 MB] || Goddard_Bldg21CornerSunset_clips_11132023_4k60_25mbps.mp4 (3840x2160) [638.6 MB] || Goddard_Bldg21CornerSunset_clips_11132023_4k60_100mbps.mp4 (3840x2160) [2.5 GB] || ", "hits": 53 }, { "id": 14484, "url": "https://svs.gsfc.nasa.gov/14484/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: Miscellaneous", "description": "Views in the vicinity of the pond and wooded area in the northwest of Goddard's campus. The first sequence is an ascent, followed by a descent, looking northwest. The next clip flies horizontally across the pond at low altitude. The following clip transitions from a position just above the pond, flying southeast, and rises to reveal Buildings 20, 28, and the broader Goddard campus. The next shot flies the same path in reverse at slower speed. Credit: NASA/Francis Reddy || Goddard_Pond_Still.jpg (3840x2160) [3.4 MB] || Goddard_Pond_Still_searchweb.png (320x180) [106.0 KB] || Goddard_Pond_Still_thm.png (80x40) [6.8 KB] || Goddard_Pond_clips_11092023_1080_30_15mbps.mp4 (1920x1080) [459.2 MB] || Goddard_Pond_clips_11092023_4k60_25mbps.mp4 (3840x2160) [765.3 MB] || Goddard_Pond_clips_11092023_4k60_100mbps.mp4 (3840x2160) [3.0 GB] || ", "hits": 42 }, { "id": 14485, "url": "https://svs.gsfc.nasa.gov/14485/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: General Campus", "description": "Views of the Goddard campus, from various heights, looking northeast from above Building 21, with fall colors in the late afternoon and magic hour. Several shots rise from below the tree line. Others fly forward or backward, looking toward the Integration and Test facilities prominent in the background.Credit: NASA/Francis Reddy || Goddard_from_Building_21_Sunset_Still.jpg (3840x2160) [3.0 MB] || Goddard_from_Building_21_Sunset_Still_searchweb.png (320x180) [105.1 KB] || Goddard_from_Building_21_Sunset_Still_thm.png (80x40) [7.0 KB] || Goddard_CampusSunsetFrom21_clips_11132023_1080_30_15mbps.mp4 (1920x1080) [675.6 MB] || Goddard_CampusSunsetFrom21_clips_11132023_4k60_25mbps.mp4 (3840x2160) [1.1 GB] || Goddard_CampusSunsetFrom21_clips_11132023_4k60_100mbps.mp4 (3840x2160) [4.4 GB] || ", "hits": 57 }, { "id": 14486, "url": "https://svs.gsfc.nasa.gov/14486/", "result_type": "B-Roll", "release_date": "2023-12-18T00:00:00-05:00", "title": "Aerial Views of Goddard: Buildings 20 and 28", "description": "A variety of clips showing flights from the wooded area in the northwest of the Goddard campus favoring Buildings 20 and 28, looking east. Some shots ascend from below the tree tops to reveal the center; others descend below the tree tops. Captured Nov. 9, 2023.Credit: NASA/Francis Reddy || Buildings_20_and_28_Still.jpg (3840x2160) [3.5 MB] || Buildings_20_and_28_Still_searchweb.png (320x180) [112.8 KB] || Buildings_20_and_28_Still_thm.png (80x40) [7.6 KB] || Goddard_Bldg20and28_clips_11132023_1080_30_15mbps.mp4 (1920x1080) [760.6 MB] || Goddard_Bldg20and28_clips_11132023_4k60_25mbps.mp4 (3840x2160) [1.2 GB] || Goddard_Bldg20and28_clips_11132023_4k60_100mbps.mp4 (3840x2160) [4.9 GB] || ", "hits": 49 }, { "id": 5144, "url": "https://svs.gsfc.nasa.gov/5144/", "result_type": "Interactive", "release_date": "2023-11-28T09:20:00-05:00", "title": "Fermi Gamma-ray Pulsar Catalog WorldWide Telescope Interactive", "description": "Before NASA’s Fermi Gamma-ray Space Telescope launched in 2008, only a handful of pulsars, including the Crab, Vela, and Geminga, were known to emit gamma-rays, the highest-energy form of light. Shown here are 294 gamma-ray pulsars detected by Fermi. Young pulsars, formed when massive stars explode, are the slowest rotators, typically spinning about 10 times a second. Paradoxically, their older siblings, called millisecond pulsars (MSPs), spin much faster, up to hundreds of times a second, thanks to the effects of a stream of matter pulled from a companion star. In spider systems, the companion is all but consumed. The most energetic spiders may fully evaporate their companions, leaving behind only an isolated MSP. Studying pulsars provides insights into the interplay of gravity, radiation, and magnetic fields with matter in the most extreme state we can observe directly.The WorldWide Telescope is a tool for showcasing astronomical data and knowledge. It’s not a physical telescope — it’s a suite of free and open source software and data sets that combine to create stunning scientific visualizations and stories. || ", "hits": 73 }, { "id": 5157, "url": "https://svs.gsfc.nasa.gov/5157/", "result_type": "Visualization", "release_date": "2023-11-28T09:20:00-05:00", "title": "Fermi Catalog of Gamma-ray Pulsars", "description": "A visualization of the 294 pulsars in the Fermi gamma-ray pulsar catalog. The visualization starts with a full-sky Hammer projection view of the catalog. Different types of pulsars are indicated by different markers. The pulsar markers oscillate in size according to the object's pulsation frequency at actual speed. Millisecond pulsars are just shown as solid markers. The map then morphs into the full 3D view of the pulsar distribution, and we then fly out to give a top down view showing the distribution of gamma-ray pulsars in our galaxy. || pulsar3DMap_2160p30.00200_print.jpg (1024x576) [174.0 KB] || pulsar3DMap_2160p30.00200_searchweb.png (320x180) [72.3 KB] || pulsar3DMap_2160p30.00200_thm.png (80x40) [5.4 KB] || full (3840x2160) [0 Item(s)] || pulsar3DMap_2160p30.mp4 (3840x2160) [240.8 MB] || ", "hits": 111 }, { "id": 14434, "url": "https://svs.gsfc.nasa.gov/14434/", "result_type": "Produced Video", "release_date": "2023-11-28T09:20:00-05:00", "title": "NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars", "description": "This visualization shows 294 gamma-ray pulsars, first plotted on an image of the entire starry sky as seen from Earth and then transitioning to a view from above our galaxy. The symbols show different types of pulsars. Young pulsars blink in real time except for the Crab, which pulses slower because its rate is only slightly lower than the video frame rate. Millisecond pulsars remain steady, pulsing too quickly to see. The Crab, Vela, and Geminga were among the 11 gamma-ray pulsars known before Fermi launched. Other notable objects are also highlighted. Distances are shown in light-years (abbreviated ly).Credit: NASA’s Goddard Space Flight CenterMusic: \"Fascination\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Pulsar_Still.jpg (3840x2160) [3.5 MB] || Pulsar_Still_searchweb.png (320x180) [105.5 KB] || Pulsar_Still_thm.png (80x40) [7.0 KB] || 14434_Fermi_Pulsar_Locations_1080.mp4 (1920x1080) [93.9 MB] || 14434_Fermi_Pulsar_Locations_1080.webm (1920x1080) [10.0 MB] || Pulsar_Captions.en_US.srt [46 bytes] || Pulsar_Captions.en_US.vtt [56 bytes] || 14434_Fermi_Pulsar_Locations_4k_Good.mp4 (3840x2160) [112.8 MB] || 14434_Fermi_Pulsar_Locations_4k_Best.mp4 (3840x2160) [689.2 MB] || 14434_Fermi_Pulsar_Locations_ProRes_3840x2160_2997.mov (3840x2160) [4.5 GB] || ", "hits": 273 }, { "id": 14435, "url": "https://svs.gsfc.nasa.gov/14435/", "result_type": "B-Roll", "release_date": "2023-10-17T00:00:00-04:00", "title": "Aerial Views of Goddard: Visitor Center", "description": "General afternoon drone footage of the rocket garden, flights between the Visitor Center and Gift Shop toward and away from the rocket garden, and ascents and descents along the Delta B looking west-northwest into the center. Captured June 13, 2023.Credit: NASA/Francis Reddy || Summer_VC_general_still.jpg (3840x2160) [2.5 MB] || Goddard_VCSummerGeneral_1080_30_15mbps.webm (1920x1080) [24.7 MB] || Goddard_VCSummerGeneral_1080_30_15mbps.mp4 (1920x1080) [370.4 MB] || Goddard_VCSummerGeneral_4k60_25mbps.mp4 (3840x2160) [617.5 MB] || Goddard_VCSummer_General_4k60_100mbps.mp4 (3840x2160) [2.4 GB] || ", "hits": 103 }, { "id": 14443, "url": "https://svs.gsfc.nasa.gov/14443/", "result_type": "B-Roll", "release_date": "2023-10-17T00:00:00-04:00", "title": "Aerial Views of Goddard: Integration and Test Facilities", "description": "Building 29, home of the largest high-bay clean room in the world, stands prominently in this panoramic aerial view of NASA's Goddard Space Flight Center in Greenbelt, Maryland. The clean room is as tall as an eight-story building and as wide as two basketball courts. The circular structure left of center houses the High Capacity Centrifuge, which is used to simulate launch and landing loads on spacecraft hardware. Imaged Oct. 5, 2023, looking south-southwest.Credit: NASA/Francis Reddy || B29_pano_01_10_05_2023_looking_SSW_1080.jpg (2434x1080) [1.7 MB] || B29_pano_01_10_05_2023_looking_SSW_3840.jpg (8653x3840) [16.5 MB] || B29_pano_01_10_05_2023_looking_SSW_1080_searchweb.png (320x180) [128.1 KB] || B29_pano_01_10_05_2023_looking_SSW_1080_thm.png (80x40) [23.3 KB] || B29_pano_01_10_05_2023_looking_SSW.tif (13745x6100) [479.8 MB] || ", "hits": 194 }, { "id": 14402, "url": "https://svs.gsfc.nasa.gov/14402/", "result_type": "Produced Video", "release_date": "2023-09-20T13:00:00-04:00", "title": "Simulated Gravitational Wave All-Sky Image", "description": "Watch as gravitational waves from a simulated population of compact binary systems combine into a synthetic map of the entire sky. Such systems contain white dwarfs, neutron stars, or black holes in tight orbits. Maps like this using real data will be possible once space-based gravitational wave observatories become active in the next decade. The center of our Milky Way galaxy lies at the center of this all-sky view, with the galactic plane extending across the middle. Brighter spots indicate sources with stronger signals and lighter colors indicate those with higher frequencies. Larger colored patches show sources whose positions are less well known. The inset shows the frequency and strength of the gravitational signal, as well as the sensitivity limit for LISA (Laser Interferometer Space Antenna), an observatory now being designed by ESA (European Space Agency) in collaboration with NASA for launch in the 2030s.Credit: NASA’s Goddard Space Flight CenterMusic: \"Shadowless\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || LISA_AllSky_withInset_Still.jpg (2985x1497) [795.1 KB] || LISA_AllSky_1080.mp4 (1920x1080) [22.8 MB] || LISA_AllSky_1080.webm (1920x1080) [2.5 MB] || LISA_AllSky_4k.mp4 (3840x2160) [60.4 MB] || LISA_AllSky_SRT_Captions.en_US.srt [205 bytes] || LISA_AllSky_SRT_Captions.en_US.vtt [218 bytes] || LISA_AllSky_ProRes_3840x2160_30.mov (3840x2160) [992.4 MB] || ", "hits": 86 }, { "id": 20378, "url": "https://svs.gsfc.nasa.gov/20378/", "result_type": "Animation", "release_date": "2023-09-19T18:00:00-04:00", "title": "Long Gamma-Ray Burst", "description": "Complete animation sequence.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GRB_Sequence_Still.jpg (3840x2160) [1.6 MB] || 20378_GRB_Sequence_1080.mp4 (1920x1080) [41.7 MB] || 20378_GRB_Sequence_4k.mp4 (3840x2160) [109.7 MB] || 20378_GRB_Sequence_ProRes_3840x2160_30.mov (3840x2160) [1.4 GB] || ", "hits": 318 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 61 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 837 }, { "id": 14389, "url": "https://svs.gsfc.nasa.gov/14389/", "result_type": "Produced Video", "release_date": "2023-08-01T13:00:00-04:00", "title": "XRISM Additional Images", "description": "The XRISM spacecraft during acoustic testing at JAXA's Tsukuba Space Center in December 2022. These and other tests confirm that the spacecraft can withstand the severe vibrations and sounds of its rocket launch.Credit: JAXA || XRISM_Acoustic_12_23_22.jpg (2832x4240) [6.9 MB] || ", "hits": 39 }, { "id": 14335, "url": "https://svs.gsfc.nasa.gov/14335/", "result_type": "Produced Video", "release_date": "2023-05-01T10:45:00-04:00", "title": "NASA Animation Sizes Up the Universe’s Biggest Black Holes", "description": "All monster black holes are not equal. Watch this video to see how they compare to each other and to our solar system. The black holes shown, which range from 100,000 to more than 60 billion times our Sun’s mass, are scaled according to the sizes of their shadows – a circular zone about twice the size of their event horizons. Only one of these colossal objects resides in our own galaxy, and it lies 26,000 light-years away. Smaller black holes are shown in bluish colors because their gas is expected to be hotter than that orbiting larger ones. Scientists think all of these objects shine most intensely in ultraviolet light. Credit: NASA's Goddard Space Flight Center Conceptual Image LabMusic: \"In the Stars\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SMBH_Scale_Still_1.jpg (3840x2160) [3.0 MB] || SMBH_Scale_Still_1_searchweb.png (180x320) [71.4 KB] || SMBH_Scale_Still_1_thm.png (80x40) [4.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.mp4 (1920x1080) [166.0 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080.mp4 (1920x1080) [102.7 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.webm (1920x1080) [13.3 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_ProRes_3840x2160_60.mov (3840x2160) [12.6 GB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_4k_Best.mp4 (3840x2160) [314.2 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.srt [2.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.vtt [2.2 KB] || ", "hits": 1831 }, { "id": 14317, "url": "https://svs.gsfc.nasa.gov/14317/", "result_type": "Produced Video", "release_date": "2023-03-28T13:50:00-04:00", "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst", "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ", "hits": 388 }, { "id": 14265, "url": "https://svs.gsfc.nasa.gov/14265/", "result_type": "Produced Video", "release_date": "2023-01-20T00:00:00-05:00", "title": "TESS 2022 Sky Views", "description": "This all-sky mosaic was constructed from 912 TESS images. By late October 2022, when the last image of this mosaic was captured, TESS had discovered 266 exoplanets and 4,258 candidates. The north and south ecliptic poles – the ends of imaginary lines extending above and below the center of Earth's orbit around the Sun – lie at the top and bottom of the image. The Andromeda galaxy is the small, bright oval near the upper right edge. The Lage Magellanic Cloud can be seen along the bottom edge just left of center. Above and to the left of it shine the Small Magellanic Cloud and the bright star cluster 47 Tucanae. Molleweide projection. Credit: NASA/MIT/TESS and Ethan Kruse (University of Maryland College Park) || TESS_NandS_12-2022.png (15000x7500) [85.3 MB] || TESS_NandS_12-2022.jpg (15000x7500) [43.4 MB] || TESS_NandS_12-2022_5k.jpg (5000x2500) [4.0 MB] || TESS_NandS_12-2022_5k_print.jpg (1024x512) [104.0 KB] || TESS_NandS_12-2022_5k_searchweb.png (320x180) [55.7 KB] || TESS_NandS_12-2022_5k_thm.png (80x40) [4.8 KB] || ", "hits": 90 }, { "id": 14209, "url": "https://svs.gsfc.nasa.gov/14209/", "result_type": "Produced Video", "release_date": "2023-01-09T17:10:00-05:00", "title": "NASA’s Compton Mission Glimpses Supersized Neutron Stars", "description": "This simulation tracks the gravitational wave and density changes as two orbiting neutron stars crash together. Dark purple colors represent the lowest densities, while yellow-white shows the highest. An audible tone and a visual frequency scale (at left) track the steady rise in the frequency of gravitational waves as the neutron stars close. When the objects merge at 42 seconds, the gravitational waves suddenly jump to frequencies of thousands of hertz and bounce between two primary tones (quasiperiodic oscillations, or QPOs). The presence of these signals in such simulations led to the search and discovery of similar phenomena in the light emitted by short gamma-ray bursts.Credit: NASA's Goddard Space Flight Center and STAG Research Centre/Peter HammondComplete transcript available.Watch this video on the NASA Goddard YouTube channel.Visual description:On a black background with a faint gray grid, two multicolored blobs representing merging neutron stars circle and close. The colors indicate density. Yellow-white indicates the highest densities, at the centers of the objects. The colors change to orange and red at their periphery, with purple colors representing matter torn from and swirling with the neutron stars as they orbit. The grid shrinks as the camera pulls back to capture a wider view of the merger. A pale orange display at left shows the changing frequency of the gravitational waves generated, which is also indicated by the rising tone. As the merger occurs, the screen shows a spinning yellow blob at center immersed in a large cloud of magneta and purple debris. || Merger_Simulation_Annotated_Still_2.jpg (1920x1080) [180.7 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.webm (1920x1080) [12.1 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.mp4 (1920x1080) [129.3 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_BEST_1080.mp4 (1920x1080) [161.8 MB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.srt [1.6 KB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.vtt [1.6 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_ProRes_1920x1080_2997.mov (1920x1080) [1.0 GB] || ", "hits": 219 }, { "id": 14269, "url": "https://svs.gsfc.nasa.gov/14269/", "result_type": "Produced Video", "release_date": "2023-01-09T13:10:00-05:00", "title": "NASA’s Webb Telescope Links Galaxies Near and Far", "description": "A trio of faint objects (circled) captured in the James Webb Space Telescope’s deep image of the galaxy cluster SMACS 0723 exhibit properties remarkably similar to rare, small galaxies called “green peas” found much closer to home. The cluster’s mass makes it a gravitational lens, which both magnifies and distorts the appearance of background galaxies. We view these early peas as they existed when the universe was about 5% its current age of 13.8 billion years. The farthest pea, at left, contains just 2% the oxygen abundance of a galaxy like our own and might be the most chemically primitive galaxy yet identified. Credit: NASA, ESA, CSA, and STScI || early_peas_behind_SMACS_0723_1080_print.jpg (1024x880) [161.9 KB] || early_peas_behind_SMACS_0723_1080.png (2513x2160) [3.8 MB] || early_peas_behind_SMACS_0723_2160.png (2513x2160) [3.8 MB] || early_peas_behind_SMACS_0723_full.png (3840x3302) [8.2 MB] || early_peas_behind_SMACS_0723_1080_searchweb.png (320x180) [71.2 KB] || early_peas_behind_SMACS_0723_1080_web.png (320x275) [103.8 KB] || early_peas_behind_SMACS_0723_1080_thm.png (80x40) [5.1 KB] || ", "hits": 341 }, { "id": 20374, "url": "https://svs.gsfc.nasa.gov/20374/", "result_type": "Animation", "release_date": "2022-12-12T00:00:00-05:00", "title": "XRISM Beauty Shots", "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ", "hits": 92 }, { "id": 14255, "url": "https://svs.gsfc.nasa.gov/14255/", "result_type": "Produced Video", "release_date": "2022-12-07T11:00:00-05:00", "title": "NASA’s Fermi, Swift Capture Revolutionary Gamma-Ray Burst", "description": "Watch to learn how an event called GRB 211211A rocked scientists’s understanding of gamma-ray bursts – the most powerful explosions in the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic Credits: \"Finished Plate\" by Airglo and \"Binary Fission\" by Tom KaneWatch this video on the NASA Goddard YouTube channel. || Title_Card_Revolutionary_GRB.jpg (1920x1080) [1.5 MB] || Title_Card_Revolutionary_GRB_searchweb.png (320x180) [100.7 KB] || Title_Card_Revolutionary_GRB_thm.png (80x40) [7.3 KB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.mp4 (1920x1080) [171.9 MB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst_ProRes.mov (1920x1080) [2.2 GB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.webm (1920x1080) [18.4 MB] || Long_GRB_Captions.en_US.srt [2.8 KB] || Long_GRB_Captions.en_US.vtt [2.8 KB] || ", "hits": 171 }, { "id": 14244, "url": "https://svs.gsfc.nasa.gov/14244/", "result_type": "Produced Video", "release_date": "2022-11-25T00:00:00-05:00", "title": "XRISM Resolve Animation", "description": "This animation illustrates how the microcalorimeter array at the heart of XRISM's revolutionary Resolve soft X-ray spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to 50 millikelvins, just above absolute zero, detects this minute temperature change.Credit: NASA's Goddard Space Flight Center || XRISM_Calorimeter-STILL_print.jpg (1024x576) [64.0 KB] || XRISM_Calorimeter-STILL.jpg (3840x2160) [716.3 KB] || XRISM_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL_thm.png (80x40) [5.5 KB] || XRISM_Calorimeter-STILL_web.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || ", "hits": 127 }, { "id": 14203, "url": "https://svs.gsfc.nasa.gov/14203/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Simulations of Weak Black Hole Jets", "description": "This sequence shows the simulated evolution of weak jets (orange, pink, and purple) formed by a supermassive black hole as they interact with stars and gas clouds (green, yellow) at the center of a galaxy. The jet is angled about 15 degrees toward the plane of its galaxy and is shown in 12 time steps, with each interval representing 50,000 years. The image at bottom right shows the jets 600,000 years after they formed. Each step is available as a 4K video and as frames by selecting \"Download Options.\"Credit: NASA's Goddard Space Flight Center/R. Tanner and K. Weaver || AGN_time_series_Numbered_print.jpg (1024x576) [109.6 KB] || AGN_time_series_Numbered.jpg (3840x2160) [982.9 KB] || Step1 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.webm (4000x4000) [3.2 MB] || Step12 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step12_4k_30.mp4 (4000x4000) [15.0 MB] || Step11 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step11_4k_30.mp4 (4000x4000) [15.0 MB] || Step10 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step10_4k_30.mp4 (4000x4000) [14.9 MB] || Step9 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step9_4k_30.mp4 (4000x4000) [15.0 MB] || Step8 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step8_4k_30.mp4 (4000x4000) [15.0 MB] || Step7 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step7_4k_30.mp4 (4000x4000) [15.0 MB] || Step6 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.mp4 (4000x4000) [15.1 MB] || Step5 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step5_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step2_4k_30.mp4 (4000x4000) [15.0 MB] || Step4 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step4_4k_30.mp4 (4000x4000) [15.0 MB] || Step2 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step6_4k_30.mp4 (4000x4000) [14.9 MB] || Step3 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step3_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step10_ProRes_4k_30.mov (4000x4000) [3.1 GB] || AGNwinds_TimeEvolution_Step1_ProRes_4k_30.mov (4000x4000) [387.2 MB] || AGNwinds_TimeEvolution_Step2_ProRes_4k_30.mov (4000x4000) [864.7 MB] || AGNwinds_TimeEvolution_Step12_ProRes_4k_30.mov (4000x4000) [3.3 GB] || AGNwinds_TimeEvolution_Step3_ProRes_4k_30.mov (4000x4000) [1.4 GB] || AGNwinds_TimeEvolution_Step11_ProRes_4k_30.mov (4000x4000) [3.2 GB] || AGNwinds_TimeEvolution_Step4_ProRes_4k_30.mov (4000x4000) [1.9 GB] || AGNwinds_TimeEvolution_Step9_ProRes_4k_30.mov (4000x4000) [2.9 GB] || AGNwinds_TimeEvolution_Step5_ProRes_4k_30.mov (4000x4000) [2.4 GB] || AGNwinds_TimeEvolution_Step8_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step7_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step6_ProRes_4k_30.mov (4000x4000) [2.7 GB] || ", "hits": 158 }, { "id": 14217, "url": "https://svs.gsfc.nasa.gov/14217/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Creating Black Hole Jets With a NASA Supercomputer", "description": "New simulations carried out on the NASA Center for Climate Simulation’s Discover supercomputer show how weaker, low-luminosity jets produced by a galaxy's monster black hole interact with their galactic environment. Because these jets are more difficult to detect, the simulations help astronomers link these interactions to features they can observe, such as various gas motions and optical and X-ray emissions.Credit: NASA's Goddard Space Flight CenterMusic credit: \"Lost Time;\" \"Ascension;\" \"Flowing Cityscape;\" \"Jupiter's Eye;\" \"Pizzicato Piece;\" \"Facts;\" \"Final Words\" all from Universal Production MusicVideo Descriptive Text available.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14217_AGN_OUtflow_Still.jpg (1920x1080) [1.0 MB] || 14217_AGN_OUtflow_Still_searchweb.png (320x180) [92.9 KB] || 14217_AGN_OUtflow_Still_thm.png (80x40) [6.7 KB] || 14217_AGN_Outflow_FINAL_1080.webm (1920x1080) [67.5 MB] || AGN_Outflow_SRT_Captions.en_US.srt [11.4 KB] || 14217_AGN_Outflow_FINAL_1080.mp4 (1920x1080) [632.4 MB] || 14217_AGN_Outflow_FINAL_1080_Best.mp4 (1920x1080) [1.5 GB] || 14217_AGN_Outflow_FINAL_ProRes_1920x1080_24.mov (1920x1080) [6.4 GB] || ", "hits": 3137 }, { "id": 14167, "url": "https://svs.gsfc.nasa.gov/14167/", "result_type": "Produced Video", "release_date": "2022-10-31T11:00:00-04:00", "title": "BurstCube Integration", "description": "BurstCube is a mission under development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. This CubeSat will detect short gamma-ray bursts, which are important sources for gravitational wave discoveries and multimessenger astronomy. The satellite is expected to launch in March 2024. || ", "hits": 90 }, { "id": 20371, "url": "https://svs.gsfc.nasa.gov/20371/", "result_type": "Animation", "release_date": "2022-10-28T14:00:00-04:00", "title": "BurstCube Animations", "description": "BurstCube is a mission under development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. This CubeSat will detect short gamma-ray bursts, which are important sources for gravitational wave discoveries and multimessenger astronomy. The satellite is expected to launch in 2023. || ", "hits": 49 }, { "id": 14227, "url": "https://svs.gsfc.nasa.gov/14227/", "result_type": "Produced Video", "release_date": "2022-10-13T15:30:00-04:00", "title": "NASA Missions Detect Record-Breaking Burst", "description": "Swift’s X-Ray Telescope captured the afterglow of GRB 221009A about an hour after it was first detected. The bright rings form as a result of X-rays scattered by otherwise unobservable dust layers within our galaxy that lie in the direction of the burst. The dark vertical line is an artifact of the imaging system.Credit: NASA/Swift/A. Beardmore (University of Leicester) || XRT_image_crop.jpg (1084x1080) [629.3 KB] || XRT_image_crop_print.jpg (1024x1020) [657.0 KB] || XRT_image_crop_searchweb.png (320x180) [133.7 KB] || XRT_image_crop_web.png (320x318) [191.7 KB] || XRT_image_crop_thm.png (80x40) [26.1 KB] || ", "hits": 279 }, { "id": 14189, "url": "https://svs.gsfc.nasa.gov/14189/", "result_type": "Produced Video", "release_date": "2022-08-19T12:45:00-04:00", "title": "50th Anniversary of NASA's Copernicus Mission", "description": "Watch: This vintage segment on Copernicus comes from a 1973 edition of “The Science Report,” a long-running film series produced by the U.S. Information Agency. Credit: National Archives (306-SR-138B)Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || OAO-CopernicusFilm.02735_print.jpg (1024x768) [108.8 KB] || OAO-CopernicusFilm.mov (1440x1080) [2.1 GB] || OAO-CopernicusFilm.mp4 (1440x1080) [235.2 MB] || OAO-CopernicusFilm.webm (1440x1080) [24.5 MB] || OAO-CopernicusFilm.en_US.srt [3.8 KB] || OAO-CopernicusFilm.en_US.vtt [3.8 KB] || ", "hits": 123 }, { "id": 14170, "url": "https://svs.gsfc.nasa.gov/14170/", "result_type": "Produced Video", "release_date": "2022-08-10T10:00:00-04:00", "title": "NASA’s Fermi Confirms 'PeVatron' Supernova Remnant", "description": "Explore how astronomers located a supernova remnant that fires up protons to energies 10 times greater than the most powerful particle accelerator on Earth.Credit: NASA’s Goddard Space Flight CenterMusic: New Philosopher by Laurent Dury; Universal Production MusicWatch this video on the NASA Goddard YouTube channelComplete transcript available. || 14170-Found__A_PeVatron.01978_print.jpg (1024x576) [61.1 KB] || 14170-_PeVatron.webm (1920x1080) [15.1 MB] || 14170-_PeVatron.mp4 (1920x1080) [136.6 MB] || 14170-PeVatron.en_US.vtt [2.3 KB] || 14170-PeVatron.mov (1920x1080) [1.8 GB] || ", "hits": 193 }, { "id": 14148, "url": "https://svs.gsfc.nasa.gov/14148/", "result_type": "Produced Video", "release_date": "2022-05-05T12:45:00-04:00", "title": "Magnetic Flip Drives Flare-Up of Monster Black Hole", "description": "Explore the unusual eruption of 1ES 1927+654, a galaxy located 236 million light-years away in the constellation Draco. A sudden reversal of the magnetic field around its million-solar-mass black hole may have triggered the outburst.Credit: NASA’s Goddard Space Flight Center Music: \"Water Dance\" and \"Alternate Worlds\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ChangingLookAGN_Still1.jpg (1920x1080) [822.9 KB] || ChangingLookAGN_Still1_searchweb.png (320x180) [79.5 KB] || ChangingLookAGN_Still1_thm.png (80x40) [6.2 KB] || 14148_ChangingLook_AGN_1080.webm (1920x1080) [24.8 MB] || 14148_ChangingLook_AGN_Sub100MB.mp4 (1920x1080) [91.5 MB] || 14148_ChangingLook_AGN_1080.mp4 (1920x1080) [246.5 MB] || 14148_ChangingLook_AGN_Best_1080.mp4 (1920x1080) [534.7 MB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.srt [4.2 KB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.vtt [4.3 KB] || 14148_ChangingLook_AGN_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 135 }, { "id": 14146, "url": "https://svs.gsfc.nasa.gov/14146/", "result_type": "Produced Video", "release_date": "2022-05-04T00:00:00-04:00", "title": "Black Hole Desktop & Phone Wallpapers", "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ", "hits": 4930 }, { "id": 14149, "url": "https://svs.gsfc.nasa.gov/14149/", "result_type": "Produced Video", "release_date": "2022-05-02T10:45:00-04:00", "title": "NASA's Black Hole Orrery", "description": "Learn more about the best-known black hole systems in our galaxy and its neighbor, the Large Magellanic Cloud. This visualization presents 22 X-ray binary systems that host confirmed black holes at the same scale, with their orbits sped up by about 22,000 times. The view of each system reflects how we see it from Earth. Star colors ranging from blue-white to reddish represent temperatures from 5 times hotter to 45% cooler than our Sun. In most of these systems, a stream of matter from the star forms an accretion disk around the black hole. In others, like the famous system called Cygnus X-1, the star produces a hefty outflow that is partly swept up by the black hole’s gravity to form the disk. The accretion disks use a different color scheme because they sport even higher temperatures than the stars. The largest disk shown, belonging to a binary called GRS 1915, spans a distance greater than that separating Mercury from our Sun. The black holes themselves are shown larger than in reality using spheres scaled to reflect their masses.Credit: NASA's Goddard Space Flight Center and Scientific Visualization StudioMusic: \"Event Horizon\" from Gravity. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Black_Hole_Orrery_Still.jpg (3840x2160) [321.9 KB] || Black_Hole_Orrery_Still_searchweb.png (320x180) [25.6 KB] || Black_Hole_Orrery_Still_thm.png (80x40) [4.1 KB] || 14149_Black_Hole_Orrery_FINAL_1080.mp4 (1920x1080) [118.8 MB] || 14149_Black_Hole_Orrery_FINAL_1080.webm (1920x1080) [12.4 MB] || 14149_Black_Hole_Orrery_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || 14149_Black_Hole_Orrery_FINAL_4k_Best.mp4 (3840x2160) [379.2 MB] || 14149_Black_Hole_Orrery_FINAL_4k.mp4 (3840x2160) [176.7 MB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.srt [1.9 KB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.vtt [1.9 KB] || ", "hits": 303 }, { "id": 4996, "url": "https://svs.gsfc.nasa.gov/4996/", "result_type": "Visualization", "release_date": "2022-05-02T10:15:00-04:00", "title": "An Orrery of Black Holes and Their Companions", "description": "Full visualization of the binary system black hole orrery with labels and legend included.Credit: NASA's Scientific Visualization Studio || explainerComp_5-27-2022a_2160p60.02000_print.jpg (1024x576) [54.7 KB] || explainerComp_5-27-2022a (3840x2160) [0 Item(s)] || explainerComp_5-27-2022a_2160p60.mp4 (3840x2160) [35.7 MB] || explainerComp_5-27-2022a_2160p60.webm (3840x2160) [26.6 MB] || ", "hits": 150 }, { "id": 4997, "url": "https://svs.gsfc.nasa.gov/4997/", "result_type": "Visualization", "release_date": "2022-05-02T10:15:00-04:00", "title": "Black Holes and Their Companions Close Up", "description": "Close up view of GRS 1915.Credit: NASA's Scientific Visualization Studio || closeupGlow_withOrbits_GRS1915_4k_4-25-2022a_2160p30.00001_print.jpg (1024x576) [25.6 KB] || withOrbitLines_EXR (3840x2160) [0 Item(s)] || withOrbitLines_PNG (3840x2160) [0 Item(s)] || withOrbitLines_EXR (3840x2160) [0 Item(s)] || withOrbitLines_PNG (3840x2160) [0 Item(s)] || closeupGlow_withOrbits_GRS1915_4k_4-25-2022a_2160p30.webm (3840x2160) [10.3 MB] || noOrbitLines_EXR (3840x2160) [0 Item(s)] || noOrbitLines_PNG (3840x2160) [0 Item(s)] || closeupGlow_withOrbits_GRS1915_4k_5-2-2022a_2160p60.mp4 (3840x2160) [180.1 MB] || ", "hits": 127 } ] }