{ "count": 206, "next": "https://svs.gsfc.nasa.gov/api/search/?keywords=X-ray&limit=100&offset=100", "previous": null, "results": [ { "id": 15044, "url": "https://svs.gsfc.nasa.gov/15044/", "result_type": "Produced Video", "release_date": "2026-05-27T09:00:00-04:00", "title": "Testing for the Katalyst-NASA Swift Boost Mission", "description": "Kieran Wilson, LINK’s principal investigator, and Hunter Robertson, a space systems engineer, both at Katalyst Space, stand next to their spacecraft inside the SES (Space Environment Simulator) at NASA’s Goddard Space Flight Center in Greenbelt, Md., on April 17, 2026, ahead of thermal vacuum testing. During testing in the SES, LINK fired its three ion thrusters, deployed one of its three arms, and experienced space-like hot and cold temperatures. Credit: NASA/Sophia RobertsAlt text: Two people stand next to a spacecraft inside a large black chamber.Image description: Downward-looking view of two people in white clean suits standing next to a spacecraft at the bottom of a large black circular chamber. The spacecraft lies at center on a black circular plate crisscrossed with white lines. Around the perimeter of the chamber are ladders and various stands. Several small lamps near the chamber’s floor create pools of light. There is a door open to the outside of the chamber at about 1 o’clock. || Testing_Link_-_Thermal_Vacuum_Testing-5-half.jpg (4752x2672) [3.8 MB] || Testing_Link_-_Thermal_Vacuum_Testing-5.jpg (9504x5344) [33.7 MB] || Testing_Link_-_Thermal_Vacuum_Testing-5-half_searchweb.png (320x180) [77.6 KB] || Testing_Link_-_Thermal_Vacuum_Testing-5-half_thm.png (80x40) [8.6 KB] || ", "hits": 1005 }, { "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": 138 }, { "id": 14930, "url": "https://svs.gsfc.nasa.gov/14930/", "result_type": "Infographic", "release_date": "2025-12-18T10:00:00-05:00", "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles", "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel", "hits": 204 }, { "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": 602 }, { "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": 211 }, { "id": 14868, "url": "https://svs.gsfc.nasa.gov/14868/", "result_type": "Produced Video", "release_date": "2025-07-23T00:00:00-04:00", "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail", "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ", "hits": 45 }, { "id": 31353, "url": "https://svs.gsfc.nasa.gov/31353/", "result_type": "Animation", "release_date": "2025-06-09T18:59:59-04:00", "title": "Supermassive Black Holes", "description": "In this video NuSTAR (Nuclear Spectroscopic Telescope Array) lead scientist Peter Boorman explains how the NuSTAR penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)", "hits": 203 }, { "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": 70 }, { "id": 14798, "url": "https://svs.gsfc.nasa.gov/14798/", "result_type": "Produced Video", "release_date": "2025-05-27T20:56:00-04:00", "title": "Astrophysics Multiwavelength Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos that show multiwavelength content.", "hits": 173 }, { "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": 221 }, { "id": 14819, "url": "https://svs.gsfc.nasa.gov/14819/", "result_type": "Produced Video", "release_date": "2025-05-06T10:45:00-04:00", "title": "NASA's NICER Studies Recurring Cosmic Crashes", "description": "Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" by Lee Groves [PRS] and Peter Geogre Marett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_thumbnail_NICER_QPE.jpg (1280x720) [225.7 KB] || YTframe_thumbnail_NICER_QPE_searchweb.png (320x180) [95.5 KB] || YTframe_thumbnail_NICER_QPE_thm.png [8.7 KB] || 14819_NICER_QPE_Good.mp4 (1920x1080) [70.6 MB] || 14819_NICER_QPE_Best.mp4 (1920x1080) [172.3 MB] || 14819_NICER_QPE_Captions.en_US.srt [2.8 KB] || 14819_NICER_QPE_Captions.en_US.vtt [2.7 KB] || 14819_NICER_QPE_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ", "hits": 67 }, { "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": 103 }, { "id": 14762, "url": "https://svs.gsfc.nasa.gov/14762/", "result_type": "Produced Video", "release_date": "2025-01-16T14:15:00-05:00", "title": "2.5 Billion Pixel Image of Galaxy Shot by Hubble", "description": "The Andromeda galaxy holds over 1 trillion stars and has been a key to unlocking the secrets of the universe. Thanks to NASA’s Hubble Space Telescope, we’re now seeing Andromeda in stunning new detail, revealing its dynamic history and unique structure.Recent Hubble surveys mapped the galaxy’s entire disk—an effort spanning a decade and over 1,000 orbits—showing everything from young stars to remnants of past galactic collisions. Learn how new information about Andromeda is reshaping our understanding of galactic evolution and what it reveals about the fate of our own galaxy. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerMusic Credit:“Vitava From Ma Vlast \"My Country\"” by Bedrich Smetana [PD] and Robert J Walsh [BMI], via First Digital Music [BMI] and Universal Production Music. || ", "hits": 371 }, { "id": 14755, "url": "https://svs.gsfc.nasa.gov/14755/", "result_type": "Produced Video", "release_date": "2025-01-13T13:00:00-05:00", "title": "NASA Astrophysics 2024 Highlights", "description": "2024 was an exciting year for astrophysics. There were fascinating discoveries by missions new and old, new instruments launched, and older instruments getting ready for unprecedented repairs in space. Several upcoming missions continued their march toward completion, with SPHEREx launching in 2025, the Nancy Grace Roman Space Telescope launching no later than May of 2027, and the Habitable Worlds Observatory beginning development as a next-generation space telescope. Building off the incredible successes, 2025 will be a great year for astrophysics at NASA.Credit: NASAMusic credit: “Extrapolations,” Andrii Yefymov [BMI], Universal Production MusicYouTubeComplete transcript available. || ASD_2024_highlight_STILL.jpg (1920x1080) [561.4 KB] || ASD_2024_highlight_STILL_searchweb.png (320x180) [111.9 KB] || ASD_2024_Highlights_good.mp4 (1920x1080) [134.2 MB] || ASD_2024_Highlights_best.mp4 (1920x1080) [368.9 MB] || ASD2024HighlightsCaptions.en_US.srt [1.7 KB] || ASD2024HighlightsCaptions.en_US.vtt [1.6 KB] || ASD_2024_highlight_STILL_thm.png [8.2 KB] || ASD_2024_Highlights_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || ", "hits": 368 }, { "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": 133 }, { "id": 14680, "url": "https://svs.gsfc.nasa.gov/14680/", "result_type": "Produced Video", "release_date": "2025-01-09T00:00:00-05:00", "title": "Astronauts Prepare for NICER Repair Training", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague participated in a training exercise at the NBL (Neutral Buoyancy Laboratory) at NASA’s Johnson Space Center in Houston. They were rehearsing activities related to repairing NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.Before any spacewalk, astronauts practice and refine procedures in the NBL to simulate — as closely as possible on Earth — the conditions under which they’ll complete the task in space.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s X-ray measurements during orbital daytime.The NICER team developed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 98 }, { "id": 14678, "url": "https://svs.gsfc.nasa.gov/14678/", "result_type": "Produced Video", "release_date": "2025-01-07T00:00:00-05:00", "title": "Astronauts Practice NICER Repair", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague practiced a repair for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station. The training exercise took place in the (NBL) Neutral Buoyancy Laboratory at NASA’s Johnson Space Center in Houston.Before any spacewalk, astronauts rehearse activities in the NBL to simulate — as much as possible — the conditions under which they’ll complete the task in space.In May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the instrument. The damage allows sunlight to reach the detectors during the station’s daytime, saturating sensors and interfering with NICER’s X-ray measurements. The damage does not impact nighttime observations.The NICER team developed a plan to cover the largest areas of damage using five patches, each shaped like a piece of pie, to be inserted into the instrument’s sunshades and locked in place. || ", "hits": 88 }, { "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": 369 }, { "id": 14679, "url": "https://svs.gsfc.nasa.gov/14679/", "result_type": "Produced Video", "release_date": "2024-12-13T00:00:00-05:00", "title": "NICER Caddy Preparation", "description": "In Spring 2024, scientists and engineers at NASA prepared and packed a patch kit for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s measurements during orbital daytime.The NICER team designed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 66 }, { "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": 219 }, { "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": 70 }, { "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": 109 }, { "id": 31303, "url": "https://svs.gsfc.nasa.gov/31303/", "result_type": "Hyperwall Visual", "release_date": "2024-08-06T00:00:00-04:00", "title": "25 Images for Chandra's 25th: 25 Images to Celebrate!", "description": "25 images from 25 years, still image || 25th-chandra-hw_print.jpg (1024x576) [248.2 KB] || 25th-chandra-hw.png (5760x3240) [16.0 MB] || 25th-chandra-hw_searchweb.png (320x180) [92.1 KB] || 25th-chandra-hw_thm.png (80x40) [12.7 KB] || 25-images-to-celebrate-chandras-25th.hwshow [290 bytes] || ", "hits": 91 }, { "id": 14603, "url": "https://svs.gsfc.nasa.gov/14603/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "NICER Hardware and Patch Kit", "description": "This video shows different components of NICER (Neutron star Interior Composition Explorer). The damaged thermal shield is a flight spare used during the patch testing process.0:00 A NICER patch slowly rotates counterclockwise. 0:14 A top-down view of the same patch, still rotating. 0:21 Another side view of the patch rotating. A gloved hand enters from the right-hand side, picks up the patch, and turns it on its side. The patch begins rotating again, so the tab on the bottom becomes visible. 1:03 A gloved hand slowly tilts a damaged thermal shield. 1:41 The thermal shield rests in a container that slowly rotates. 2:08 A gloved hand rotates a NICER X-ray concentrator. 2:30The camera moves past the X-ray concentrator. 2:52 A hand places a NICER sunshade on the table. 2:58 The sunshade rotates counterclockwise. 3:00 The sunshade rotates on its side.Credit:NASA/Sophia Roberts and Scott Wiessinger || Studio_Shoot_Single_Components.00001_print.jpg (1024x540) [16.9 KB] || Studio_Shoot_Single_Components.00001_searchweb.png (320x180) [23.1 KB] || Studio_Shoot_Single_Components.00001_thm.png (80x40) [2.1 KB] || Studio_Shoot_Single_Components.mp4 (4096x2160) [1.9 GB] || Studio_Shoot_Single_Components.mov (4096x2160) [12.7 GB] || ", "hits": 49 }, { "id": 14609, "url": "https://svs.gsfc.nasa.gov/14609/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "Anodizing NICER’s Patches", "description": "This video shows engineering technician Katrina Harvey anodizing NICER’s patches at the Plating Laboratory at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.0:00 One of the NICER patch bodies hangs from a spiky stick by a wire. 0:05 Patch lids attached to a similar stick are seen submerged in a dark blue liquid. 0:07 Harvey lifts the lids and one patch body from a chemical bath and submerges them in a container of deionized water. 0:24 Several lids have been dyed black. 0:29 Harvey submerges the black lids into a chemical bath covered with white plastic balls. 0:42 Harvey lifts undyed patch bodies from a deionized water rinse. 0:47 Harvey lifts patch bodies from a chemical bath covered in white plastic balls and dunks them in deionized water. 1:07 A wider view of Harvey as she works on the patch bodies in the plating lab. 1:24 The patch bodies are shown submerged in a blue liquid. 1:28 A pan across patch bodies submerged in blue liquid. 1:34 Harvey lifts the patch bodies on their individual wires out of a well where nozzles spray them with deionized water. She then dunks them several times in a container of black dye. 1:54 She adds more patch bodies to the black dye. 2:22 She hangs the dyed bodies in a well where nozzles spray them with deionized water. 2:35 Harvey sprays the patches with deionized water. 2:40 Keith Gendreau (NASA), Steve Kenyon (NASA), and Isiah Holt (NASA) cluster together, looking at one of the dyed NICER patch bodies. 2:48 Harvey rinses dyed patch bodies. 2:58 Harvey holds several dyed patch bodies still on their wires. She lifts them and starts walking through the lab. 3:18 Gendreau and Kenyon help remove plugs from holes in the patch bodies. These protected screw threads during the anodizing process. 3:32: Someone dries one of the patch bodies with compressed air. 3:42 The dyed patch bodies rest on a table. 3:58 Close-ups of various features of the lab, like labels, knobs, readouts, buttons, clamps, and wires.Credit:NASA/Sophia Roberts and Scott Wiessinger || Anondizing_Patches_at_4k.00001_print.jpg (1024x576) [72.4 KB] || Anondizing_Patches_at_4k.00001_searchweb.png (320x180) [61.0 KB] || Anondizing_Patches_at_4k.00001_thm.png (80x40) [5.0 KB] || Anondizing_Patches_at_4k.webm (3840x2160) [99.1 MB] || Anondizing_Patches_at_4k.mp4 (3840x2160) [2.5 GB] || Anondizing_Patches_at_4k_ProRes.mov (3840x2160) [18.3 GB] || ", "hits": 53 }, { "id": 14610, "url": "https://svs.gsfc.nasa.gov/14610/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "Machining NICER’s Patches", "description": "This video shows Richard Koenecke, an engineer at NASA’s Goddard Space Flight Center, creating the body of one of the NICER (Neutron star Interior Composition Explorer) patches.0:00 Two blocks of aluminum sit on a counter in front of a laptop that displays the schematics for the NICER patches. 0:06 Koenecke puts one block on the bed of a saw littered with metal shavings and then trims the block. 0:23 Koenecke sands down the block’s rough edges. 0:30 Koenecke walks into another part of his workshop. 0:37 Koenecke preps the machining chamber. 0:49 Inside the chamber, the machine starts to carve out the shape of the patch. Fluid sprayed from the nozzles above the tool helps cool the metal. 0:56 Koenecke looks into the chamber. 0:59 The chamber is shown at different angles. 1:15 Koenecke walking up to the chamber window. 1:22 Inside the chamber, the patch’s shape is now visible amidst a sea of aluminum shavings. 1:25 The cutting tool refines the shape of the patch. 1:40 Koenecke looks at a computer readout for the machining chamber. 1:45 Inside the chamber, the cutting tool lowers to hollow out the patch. 1:56 Koenecke holds and turns a block of the aluminum. 2:45 Koenecke’s dog Sara guards his shop on the Eastern Shore. 2:53 Koenecke sands a block of aluminum. 3:01 He closes the doors to the machining chamber and adjusts the settings on a computer screen. 3:10 Numbers change on the chamber’s computer screen. 3:31 Koenecke holds and turns the fully machined patch body. 3:51 In slow motion, Koenecke walking through his shop. 4:25 In slow motion, Koenecke holds the patch in close-up shots.Credit: NASA/Sophia Roberts and Scott Wiessinger || Machine_Shop_B-roll_-_Part_1.03720_print.jpg (1024x576) [111.0 KB] || Machine_Shop_B-roll_-_Part_1.03720_searchweb.png (320x180) [82.6 KB] || Machine_Shop_B-roll_-_Part_1.03720_thm.png (80x40) [6.8 KB] || Machine_Shop_B-roll_-_Part_1.webm (3840x2160) [74.7 MB] || Machine_Shop_B-roll_-_Part_1.mp4 (3840x2160) [2.5 GB] || Machine_Shop_B-roll_-_Part_1_ProRes.mov (3840x2160) [18.0 GB] || ", "hits": 53 }, { "id": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 347 }, { "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": 73 }, { "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": 53 }, { "id": 31273, "url": "https://svs.gsfc.nasa.gov/31273/", "result_type": "Hyperwall Visual", "release_date": "2024-01-31T00:00:00-05:00", "title": "NASA Telescopes Chase Down \"Green Monster\" in Star's Debris", "description": "Animations of images originally published at https://chandra.harvard.edu/photo/2024/casa/ and https://www.nasa.gov/image-article/nasa-telescopes-chase-down-green-monster-in-stars-debris/.Astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure called the “Green Monster”. Composite images from Chandra, Webb, Hubble, NuSTAR, and Spitzer reveal where elements such as silicon, iron, and titanium are located. Comparing where certain elements are with the location of the blast wave, researchers conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it. || ", "hits": 41 }, { "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": 76 }, { "id": 14408, "url": "https://svs.gsfc.nasa.gov/14408/", "result_type": "Produced Video", "release_date": "2023-09-07T11:00:00-04:00", "title": "Swift Spots a Snacking Black Hole Using a New Trick", "description": "Watch to learn how an update to NASA’s Neil Gehrels Swift Observatory allowed it to catch a supersized black hole in a distant galaxy munching repeatedly on a circling star. Credit: NASA’s Goddard Space Flight CenterMusic: \"Teapot Waltz\" by Benjamin Parsons from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Repeating_TDE_Still.jpg (1920x1080) [446.8 KB] || Repeating_TDE_Still_searchweb.png (320x180) [63.3 KB] || Repeating_TDE_Still_thm.png (80x40) [4.6 KB] || 14408_Repeating_TDE_sub100.mp4 (1920x1080) [89.7 MB] || Repeating_TDE_SRT_Captions.en_US.srt [1.7 KB] || Repeating_TDE_SRT_Captions.en_US.vtt [1.6 KB] || 14408_Repeating_TDE_ProRes_1920x1080_2997.mov (1920x1080) [1.2 GB] || 14408_Repeating_TDE_1080.mp4 (1920x1080) [186.2 MB] || ", "hits": 111 }, { "id": 14405, "url": "https://svs.gsfc.nasa.gov/14405/", "result_type": "Produced Video", "release_date": "2023-08-25T10:00:00-04:00", "title": "XRISM: Exploring the Hidden X-ray Cosmos", "description": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim || YTframe_XRISM_Exploring_XrayCosmos.jpg (1280x720) [668.5 KB] || YTframe_XRISM_Exploring_XrayCosmos_searchweb.png (320x180) [100.3 KB] || YTframe_XRISM_Exploring_XrayCosmos_thm.png (80x40) [7.6 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.srt [7.8 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.vtt [7.4 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mov (3840x2160) [21.6 GB] || ", "hits": 185 }, { "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": 975 }, { "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": 25 }, { "id": 14323, "url": "https://svs.gsfc.nasa.gov/14323/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Echoes of the Big Bang\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Complete list of footage usedHERE. Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_print.jpg (1024x576) [73.5 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2.jpg (3840x2160) [511.8 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_searchweb.png (320x180) [40.4 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_thm.png (80x40) [5.4 KB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.webm (1920x1080) [130.2 MB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.mp4 (1920x1080) [1.7 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_50mbps.mp4 (1920x1080) [4.1 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_ProRes_1920x1080_2997.mov (1920x1080) [14.7 GB] || ", "hits": 138 }, { "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": 185 }, { "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": 38 }, { "id": 31210, "url": "https://svs.gsfc.nasa.gov/31210/", "result_type": "Hyperwall Visual", "release_date": "2022-12-01T00:00:00-05:00", "title": "AAS 241 student winner Austin Brenner", "description": "AAS 2023 Student winner Austin Brenner || flux_video000_print.jpg (1024x576) [64.0 KB] || flux_video000_searchweb.png (320x180) [51.0 KB] || flux_video000_thm.png (80x40) [4.4 KB] || flux (3840x2160) [32.0 KB] || open_close (3840x2160) [4.0 KB] || station (3840x2160) [64.0 KB] || open_closed_2160p30.mp4 (3840x2160) [2.5 MB] || flux_video_2160p30.mp4 (3840x2160) [86.5 MB] || open_closed_2160p30.webm (3840x2160) [877.4 KB] || station_mapping_2160p30.mp4 (3840x2160) [113.0 MB] || ", "hits": 27 }, { "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] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || 3840x2160_16x9_60p (3840x2160) [64.0 KB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || ", "hits": 88 }, { "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": 251 }, { "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": 128 }, { "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": 177 }, { "id": 14136, "url": "https://svs.gsfc.nasa.gov/14136/", "result_type": "Produced Video", "release_date": "2022-04-20T00:00:00-04:00", "title": "Webb Instrument Overview", "description": "A look at the instruments on the Webb Telescope. || Webb_Instruments-Thumbnail-2.jpg (1920x1080) [1.3 MB] || Webb_Instruments-Thumbnail-2_print.jpg (1024x576) [676.3 KB] || Webb_Instruments-Thumbnail-2_searchweb.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_web.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_thm.png (80x40) [13.8 KB] || WEBB_Instrument_Package-closecap.en_US.srt [4.9 KB] || WEBB_Instrument_Package.webm (4096x2160) [68.8 MB] || WEBB_Instrument_Package.mp4 (4096x2160) [276.0 MB] || ", "hits": 31 }, { "id": 14132, "url": "https://svs.gsfc.nasa.gov/14132/", "result_type": "Produced Video", "release_date": "2022-04-12T00:00:00-04:00", "title": "Black Hole Week: Black Hole GIFs", "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ", "hits": 495 }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "result_type": "Produced Video", "release_date": "2022-04-06T13:00:00-04:00", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "hits": 55 }, { "id": 14115, "url": "https://svs.gsfc.nasa.gov/14115/", "result_type": "Produced Video", "release_date": "2022-03-08T13:00:00-05:00", "title": "NASA's NICER Tracks a Magnetar's Hot Spots", "description": "Explore how NASA’s Neutron star Interior Composition Explorer (NICER) tracked brilliant hot spots on the surface of an erupting magnetar – from 13,000 light-years away. Credit: NASA's Goddard Space Flight CenterMusic: \"Particles and Fields\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_Still.jpg (1920x1080) [574.3 KB] || Magnetar_Still_print.jpg (1024x576) [229.0 KB] || Magnetar_Still_searchweb.png (320x180) [66.1 KB] || Magnetar_Still_thm.png (80x40) [5.2 KB] || 14115_Merging_Magnetar_HotSpots_1080_Best.webm (1920x1080) [17.4 MB] || 14115_Merging_Magnetar_HotSpots_1080.mp4 (1920x1080) [158.9 MB] || 14115_Merging_Magnetar_HotSpots_1080_Best.mp4 (1920x1080) [382.0 MB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.srt [2.1 KB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.vtt [2.1 KB] || 14115_Merging_Magnetar_HotSpots_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || ", "hits": 201 }, { "id": 14111, "url": "https://svs.gsfc.nasa.gov/14111/", "result_type": "Produced Video", "release_date": "2022-02-28T07:00:00-05:00", "title": "Webb's Mid-Infrared Instrument (MIRI) Light Path Animation", "description": "The spectrograph light path inside the Mid Infrared Instrument (MIRI) on the Webb Telescope. Versions with labels and without labels.Credit: European Space Agency || MIRI_SPECTRO_v2.00030_print.jpg (1024x576) [40.5 KB] || MIRI_SPECTRO_v2.00030_searchweb.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_web.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_thm.png (80x40) [2.1 KB] || MIRI_SPECTRO_v2.mp4 (1920x1080) [156.3 MB] || MIRI_SPECTRO_labels_v3.mp4 (1920x1080) [177.9 MB] || MIRI_SPECTRO_v2.webm (1920x1080) [9.0 MB] || ", "hits": 71 }, { "id": 14112, "url": "https://svs.gsfc.nasa.gov/14112/", "result_type": "Produced Video", "release_date": "2022-02-28T07:00:00-05:00", "title": "Webb's Near Infrared Spectrograph (NIRSpec) Instrument Light Path Animation", "description": "Animation of the light path inside the Near Infrared Spectrometer (NIRSpec) on the Webb Telescope. Showing simulated data.Credit: European Space Agency || NIRSPEC_IFU_with_graph_v3.00030_print.jpg (1024x576) [39.9 KB] || NIRSPEC_IFU_with_graph_v3.00030_searchweb.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_web.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_thm.png (80x40) [2.1 KB] || NIRSPEC_IFU_with_graph_v3.mp4 (1920x1080) [311.7 MB] || NIRSPEC_IFU_with_graph_v3.webm (1920x1080) [12.7 MB] || ", "hits": 73 }, { "id": 20359, "url": "https://svs.gsfc.nasa.gov/20359/", "result_type": "Animation", "release_date": "2022-02-08T13:00:00-05:00", "title": "Migrating Magnetar Hot Spot Animations", "description": "Animation showing a wide view of SGR 1830, a magnetar that underwent an outburst in October 2020. NICER measurements from the first day of the event show that the X-ray emission exhibited three close peaks with every rotation. Astronomers think the triple peak occurred when three individual surface regions much hotter than their surroundings spun into and out of our view from Earth. NICER tracked the magnetar nearly every day for more than a month. Over that time, the hot spots dimmed, drifted relative to each other, and two even merged – a phenomenon not seen before. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || 02_MAGNETAR_Wide_view_BlipOnly_Still.png (1920x1080) [2.3 MB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_print.jpg (1024x576) [44.5 KB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_searchweb.png (320x180) [52.6 KB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_thm.png (80x40) [4.4 KB] || 02_MAGNETAR_Wide_view_BlipOnly_1080.mp4 (1920x1080) [36.0 MB] || 02_MAGNETAR_Wide_view_BlipOnly_web.webm (1920x1080) [3.5 MB] || 02_Magnetar_Wide_BlipOnly1 (1920x1080) [0 Item(s)] || 02_MAGNETAR_Wide_view_BlipOnly_ProRes_1920x1080_2997.mov (1920x1080) [502.4 MB] || ", "hits": 176 }, { "id": 14064, "url": "https://svs.gsfc.nasa.gov/14064/", "result_type": "Produced Video", "release_date": "2022-01-31T00:00:00-05:00", "title": "The Webb Telescope Sunshield", "description": "The Webb Telescope sunshield feature. || Webb_Telescope_Sunshield_Feature_Cover_Image_3_print.jpg (1024x535) [365.6 KB] || Webb_Telescope_Sunshield_Feature_Cover_Image_3.jpg (3348x1752) [2.4 MB] || Webb_Telescope_Sunshield_Feature_Cover_Image_3_searchweb.png (320x180) [95.0 KB] || Webb_Telescope_Sunshield_Feature_Cover_Image_3_thm.png (80x40) [7.3 KB] || WEBB_Sunshield_Package_v2.webmhd.webm (1080x568) [37.0 MB] || WEBB_Sunshield_Package_v2.mp4 (4096x2160) [186.9 MB] || Sunshield_feature_Output.en_US.srt [3.4 KB] || Sunshield_feature_Output.en_US.vtt [3.4 KB] || ", "hits": 29 }, { "id": 14060, "url": "https://svs.gsfc.nasa.gov/14060/", "result_type": "Produced Video", "release_date": "2021-12-25T00:00:00-05:00", "title": "Complete Webb Telescope Launch Broadcast", "description": "Part 1 of the Webb Telescope launch broadcast || 14060_Webb_Full_Launch_Broadcast_1.jpg (1435x807) [154.8 KB] || 14060_Webb_Full_Launch_Broadcast_1_print.jpg (1024x575) [88.2 KB] || 14060_Webb_Full_Launch_Broadcast_1_searchweb.png (320x180) [54.4 KB] || 14060_Webb_Full_Launch_Broadcast_1_thm.png (80x40) [8.5 KB] || 14060_Webb_Full_Launch_Broadcast_1.mov (1920x1080) [61.9 GB] || 14060_Webb_Full_Launch_Broadcast_1.webmhd.webm (1080x606) [690.4 MB] || 14060_Webb_Full_Launch_Broadcast_1.mp4 (3840x2160) [1.0 GB] || 14060_Webb_Full_Launch_Broadcast_1.webm (3840x2160) [1.3 GB] || ", "hits": 76 }, { "id": 20342, "url": "https://svs.gsfc.nasa.gov/20342/", "result_type": "Animation", "release_date": "2021-12-15T12:00:00-05:00", "title": "WEBB Turn Arounds", "description": "WEBB Turn Around Above the Horizon || WEBB_TurnAround_AboveHorizon_ProRes4444.00001_print.jpg (1024x576) [35.8 KB] || WEBB_TurnAround_AboveHorizon_ProRes4444.00001_searchweb.png (320x180) [21.7 KB] || WEBB_TurnAround_AboveHorizon_ProRes4444.00001_thm.png (80x40) [2.5 KB] || WEBB_TurnAround_AboveHorizon_1000px_ProRes4444.mov (1000x563) [37.6 MB] || WEBB_TurnAround_AboveHorizon_ProRes4444.mov (3840x2160) [374.2 MB] || WEBB_TurnAround_AboveHorizon_ProRes.mov (3840x2160) [285.5 MB] || WEBB_TurnAround_AboveHorizon_PNGs (3840x2160) [16.0 KB] || WEBB_TurnAround_AboveHorizon_PNG_2160p30.mp4 (3840x2160) [11.7 MB] || WEBB_TurnAround_AboveHorizon_ProRes4444.webm [0 bytes] || ", "hits": 30 }, { "id": 14021, "url": "https://svs.gsfc.nasa.gov/14021/", "result_type": "Produced Video", "release_date": "2021-12-06T12:00:00-05:00", "title": "Webb Journey to Space EP5: Spacecraft Fueling", "description": "Webb Journey to Space EP5: Spacecraft Fueling || Webb_Journey_To_Space_5_Cover_Image_2_print.jpg (1024x574) [401.7 KB] || Webb_Journey_To_Space_5_Cover_Image_2.jpg (3342x1874) [2.3 MB] || Webb_Journey_To_Space_5_Cover_Image_2_searchweb.png (320x180) [90.5 KB] || Webb_Journey_To_Space_5_Cover_Image_2_thm.png (80x40) [6.5 KB] || Webbs_Journey_to_Space_-_Moving_to_S5B.mov (1920x1080) [1.4 GB] || Webbs_Journey_to_Space_-_Moving_to_S5B_graphics.mov (1920x1080) [1.4 GB] || Webbs_Journey_to_Space_-_Moving_to_S5B_Graphics.mp4 (1920x1080) [102.1 MB] || Webbs_Journey_to_Space_-_Moving_to_S5B_no_Graphics.mp4 (1920x1080) [102.1 MB] || Webbs_Journey_to_Space_-_Moving_to_S5B_Graphics.webm (1920x1080) [11.1 MB] || Webb_Journey_to_Space_-_Moving_On_to_Fueling.en_US.srt [1.5 KB] || Webb_Journey_to_Space_-_Moving_On_to_Fueling.en_US.vtt [1.5 KB] || ", "hits": 35 }, { "id": 14039, "url": "https://svs.gsfc.nasa.gov/14039/", "result_type": "Produced Video", "release_date": "2021-12-03T08:00:00-05:00", "title": "New NASA Spacecraft Will Help Unlock The Secrets Of Extreme Cosmic Objects Live Shots", "description": "Quick link to associated B-ROLL for the live shots.Quick link to canned interview with Martin Weisskopf IXPE Principal Investigator || IXPE_Advisory_Banner-2.png (1200x480) [762.4 KB] || IXPE_Advisory_Banner-2_print.jpg (1024x409) [117.3 KB] || IXPE_Advisory_Banner-2_searchweb.png (320x180) [106.3 KB] || IXPE_Advisory_Banner-2_thm.png (80x40) [8.4 KB] || ", "hits": 37 }, { "id": 14002, "url": "https://svs.gsfc.nasa.gov/14002/", "result_type": "Produced Video", "release_date": "2021-11-09T00:00:00-05:00", "title": "Elements of Webb: Series Introduction Ep0", "description": "Elements of Webb EP00: Introduction || EP00-_Elements_Series_Introduction.jpg (1920x1080) [738.1 KB] || EP00-_Elements_Series_Introduction_print.jpg (1024x576) [333.2 KB] || EP00-_Elements_Series_Introduction_searchweb.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_web.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_thm.png (80x40) [7.1 KB] || 0-Elements_of_Webb_-_Introduction_1.mp4 (1920x1080) [89.2 MB] || 0-Elements_of_Webb_-_Introduction_1.webm (1920x1080) [9.4 MB] || 0-Elements_of_Webb_-_Introduction_1.en_US.srt [1.3 KB] || 0-Elements_of_Webb_-_Introduction_1.en_US.vtt [1.3 KB] || 0-Elements_of_Webb_-_Introduction.mov (1920x1080) [1.1 GB] || elements-of-webb-series-introduction-ep0.hwshow [332 bytes] || ", "hits": 33 }, { "id": 13952, "url": "https://svs.gsfc.nasa.gov/13952/", "result_type": "B-Roll", "release_date": "2021-10-18T12:00:00-04:00", "title": "29 Days on the Edge", "description": "The greatest origin story of all unfolds with the James Webb Space Telescope. Webb's launch is a pivotal moment that exemplifies the dedication, innovation, and ambition behind NASA and its partners, the European Space Agency (ESA) and Canadian Space Agency (CSA), but it is only the beginning. The 29 days following liftoff will be an exciting but harrowing time. Thousands of parts must work correctly, in sequence, to unfold Webb and put it in its final configuration. All while Webb flies through the expanse of space, alone, to a destination nearly one million miles away from Earth. As the largest and most complex telescope ever sent into space, the James Webb Space Telescope is a technological marvel. By necessity, Webb takes on-orbit deployments to the extreme. Each step can be controlled expertly from the ground, giving Webb's Mission Operations Center full control to circumnavigate any unforseen issues with deployment. || ", "hits": 98 }, { "id": 13886, "url": "https://svs.gsfc.nasa.gov/13886/", "result_type": "Produced Video", "release_date": "2021-07-26T11:00:00-04:00", "title": "NASA's Fermi Spots 'Fizzled' Burst from Collapsing Star", "description": "Astronomers combined data from NASA's Fermi Gamma-ray Space Telescope, other space missions, and ground-based observatories to reveal the origin of GRB 200826A, a brief but powerful burst of radiation. It’s the shortest burst known to be powered by a collapsing star – and almost didn’t happen at all. Credit: NASA's Goddard Space Flight CenterMusic: \"Inducing Waves\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Fizzled_GRB_Still.jpg (1920x1080) [740.9 KB] || Fizzled_GRB_Still_print.jpg (1024x576) [286.8 KB] || Fizzled_GRB_Still_searchweb.png (320x180) [72.2 KB] || Fizzled_GRB_Still_thm.png (80x40) [4.9 KB] || 13886_Fizzled_GRB_1080.mp4 (1920x1080) [147.2 MB] || 13886_Fizzled_GRB_1080_Best.mp4 (1920x1080) [453.2 MB] || 13886_Fizzled_GRB_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || 13886_Fizzled_GRB_1080.webm (1920x1080) [22.5 MB] || ", "hits": 90 }, { "id": 13841, "url": "https://svs.gsfc.nasa.gov/13841/", "result_type": "Produced Video", "release_date": "2021-04-27T17:00:00-04:00", "title": "NASA’s NICER Telescope Examined a Star on the Edge of Becoming a Black Hole Live Shots", "description": "Quick link to canned interview in Spanish with Diego Altamirano: Principal Research Fellow, University of Southampton.Quick link to associated B-ROLL for live shots. || Unknown-2.png (1600x535) [1.1 MB] || Unknown-2_print.jpg (1024x342) [147.9 KB] || Unknown-2_searchweb.png (320x180) [95.0 KB] || Unknown-2_thm.png (80x40) [7.4 KB] || ", "hits": 106 }, { "id": 13832, "url": "https://svs.gsfc.nasa.gov/13832/", "result_type": "Produced Video", "release_date": "2021-04-17T11:00:00-04:00", "title": "NASA’s NICER Tests Matter’s Limits", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) is helping physicists peer into the hearts of neutron stars, the remains of massive stars that exploded in supernovae. Scientists want to explore the nature of matter inside these objects, where it exists on the verge of collapsing into black holes. To do so, scientists need precise measurements of neutron stars’ masses and sizes, which NICER and other efforts are now making possible.Credit: NASA’s Goddard Space Flight CenterMusic: \"Question Time\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Video_title_card_2.jpg (1920x1080) [206.4 KB] || Video_title_card_2_searchweb.png (320x180) [54.8 KB] || Video_title_card_2_thm.png (80x40) [5.7 KB] || 13832_NICER_TestsMattersLimits_Best_1080.webm (1920x1080) [28.5 MB] || 13832_NICER_TestsMattersLimits_1080.mp4 (1920x1080) [187.8 MB] || 13832_NICER_TestsMattersLimits_Best_1080.mp4 (1920x1080) [650.1 MB] || 13832_NICER_TestsMattersLimits_SRT_Captions.en_US.srt [4.7 KB] || 13832_NICER_TestsMattersLimits_SRT_Captions.en_US.vtt [4.8 KB] || 13832_NICER_TestsMattersLimits_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || ", "hits": 329 }, { "id": 13737, "url": "https://svs.gsfc.nasa.gov/13737/", "result_type": "Produced Video", "release_date": "2021-04-08T14:00:00-04:00", "title": "NASA’s NICER Finds X-ray Boosts in the Crab Pulsar’s Radio Bursts", "description": "Observations from NASA’s Neutron star Interior Composition Explorer (NICER) show X-ray boosts linked in the Crab pulsar's random giant radio pulses. Watch to learn more. Credit: NASA's Goddard Space Flight CenterMusic: \"The Awakening\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Crab_Radio_Still.jpg (1920x1080) [865.4 KB] || Crab_Radio_Still_searchweb.png (320x180) [65.9 KB] || Crab_Radio_Still_thm.png (80x40) [5.2 KB] || 13737_Crab_Pulsar_Radio_Bursts_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.mp4 (1920x1080) [275.3 MB] || 13737_Crab_Pulsar_Radio_Bursts_1080.mp4 (1920x1080) [114.7 MB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.webm (1920x1080) [15.2 MB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.srt [2.6 KB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.vtt [2.6 KB] || ", "hits": 321 }, { "id": 13805, "url": "https://svs.gsfc.nasa.gov/13805/", "result_type": "Produced Video", "release_date": "2021-02-22T11:00:00-05:00", "title": "Swift Links Neutrino to Star-destroying Black Hole", "description": "Watch how a monster black hole ripping apart a star may have launched a ghost particle toward Earth. Astronomers have long predicted that tidal disruption events could produce high-energy neutrinos, nearly massless particles from outside our galaxy traveling close to the speed of light. One recent event, named AT2019dsg, provides the first proof this prediction is true but has challenged scientists’ assumptions of where and when these elusive particles might form during these destructive outbursts. Credit: NASA’s Goddard Space Flight CenterMusic: \"Diagnostic Report\" from Universal Production MusicComplete transcript available. || AT2019dsg_prores_still.jpg (1920x1080) [299.2 KB] || AT2019dsg_prores_still_print.jpg (1024x576) [119.5 KB] || AT2019dsg_prores_still_searchweb.png (180x320) [42.6 KB] || AT2019dsg_prores_still_web.png (320x180) [42.6 KB] || AT2019dsg_prores_still_thm.png (80x40) [4.1 KB] || AT2019dsg_HQ.mp4 (1920x1080) [347.5 MB] || AT2019dsg_LQ.mp4 (1920x1080) [191.3 MB] || AT2019dsg_prores.mov (1920x1080) [1.7 GB] || AT2019dsg_LQ.webm (1920x1080) [21.5 MB] || AT2019dsg_LQ.en_US.srt [3.7 KB] || AT2019dsg_LQ.en_US.vtt [3.7 KB] || ", "hits": 447 }, { "id": 13792, "url": "https://svs.gsfc.nasa.gov/13792/", "result_type": "Produced Video", "release_date": "2021-01-13T12:15:00-05:00", "title": "NASA Missions Unveil Magnetar Eruptions in Nearby Galaxies", "description": "On April 15, 2020, a wave of X-rays and gamma rays lasting only a fraction of a second triggered detectors on NASA and European spacecraft. The event was a giant flare from a magnetar, a type of city-sized stellar remnant that boasts the strongest magnetic fields known. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Collision Course-Alternative Version\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MGF_Video_Still.jpg (1920x1080) [602.3 KB] || MGF_Video_Still_print.jpg (1024x576) [264.7 KB] || MGF_Video_Still_searchweb.png (320x180) [74.9 KB] || MGF_Video_Still_thm.png (80x40) [5.7 KB] || 13792_Magnetar_Giant_Flare_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13792_Magnetar_Giant_Flare_best_1080.mp4 (1920x1080) [498.6 MB] || 13792_Magnetar_Giant_Flare_good_1080.mp4 (1920x1080) [221.6 MB] || 13792_Magnetar_Giant_Flare_best_1080.webm (1920x1080) [24.0 MB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.srt [4.0 KB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.vtt [4.0 KB] || ", "hits": 275 }, { "id": 13751, "url": "https://svs.gsfc.nasa.gov/13751/", "result_type": "Produced Video", "release_date": "2020-11-04T11:00:00-05:00", "title": "NASA Missions Team Up to Study Unique Magnetar Outburst", "description": "On April 28, space- and ground-based observatories detected powerful, simultaneous X-ray and radio bursts from a source in our galaxy. Watch to see how this unique event helps solve the longstanding puzzle of fast radio bursts observed in other galaxies.Credit: NASA's Goddard Space Flight CenterMusic: \"Jupiter's Eye\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_FRB_Still.jpg (1920x1080) [535.5 KB] || Magnetar_FRB_Still_searchweb.png (320x180) [65.5 KB] || Magnetar_FRB_Still_thm.png (80x40) [4.8 KB] || 13751_Magnetar_FRB_Best_1080.webm (1920x1080) [25.7 MB] || 13751_Magnetar_FRB_1080.mp4 (1920x1080) [237.4 MB] || 13751_Magnetar_FRB_Best_1080.mp4 (1920x1080) [741.8 MB] || Fast_Radio_Burst_SRT_Captions.en_US.srt [4.5 KB] || Fast_Radio_Burst_SRT_Captions.en_US.vtt [4.5 KB] || 13751_Magnetar_FRB_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 381 }, { "id": 13280, "url": "https://svs.gsfc.nasa.gov/13280/", "result_type": "Produced Video", "release_date": "2020-08-19T00:00:00-04:00", "title": "Assembling XRISM's X-ray Mirrors", "description": "Team members Lawrence Lozipone of Stinger Ghaffarian Technologies, Inc. and Yang Soong, a researcher at the University of Maryland, College Park, work with flight mirrors for the X-ray Imaging and Spectroscopy Mission (XRISM). Nested aluminum mirror segments – 1,624 of them for each X-ray Mirror Assembly – focus the incoming X-rays for the satellite's science instruments. Credit: NASA's Goddard Space Flight Center || XRISM_Cleanroom_B-roll_1080Still.jpg (1920x1080) [727.5 KB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.mov (1920x1080) [7.0 GB] || XRISM_Cleanroom_B-roll_1080.mp4 (1920x1080) [991.6 MB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.webm (1920x1080) [52.0 MB] || ", "hits": 86 }, { "id": 13578, "url": "https://svs.gsfc.nasa.gov/13578/", "result_type": "Produced Video", "release_date": "2020-04-13T11:00:00-04:00", "title": "NASA Missions Study a Nova's Shock Waves", "description": "NASA’s Fermi and NuSTAR space telescopes, together with another satellite named BRITE-Toronto, are providing new insights into a nova explosion that erupted in 2018. Detailed measurements of bright flares in the explosion clearly show that shock waves power most of the nova's visible light. Credit: NASA’s Goddard Space Flight CenterMusic: \"Scientist\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || novastill01.jpg (3840x2160) [1.1 MB] || novastill01_searchweb.png (320x180) [76.8 KB] || novastill01_thm.png (80x40) [6.7 KB] || 13578_Nova_Carinae_Best.webm (1920x1080) [13.8 MB] || novastill01.tif (3840x2160) [31.7 MB] || 13578_Nova_Carinae_SRT_Captions.en_US.srt [2.2 KB] || 13578_Nova_Carinae_SRT_Captions.en_US.vtt [2.2 KB] || 13578_Nova_Carinae_Best.mp4 (1920x1080) [319.4 MB] || 13578_Nova_Carinae_Good.mp4 (1920x1080) [129.0 MB] || 13578_Nova_Carinae_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 141 }, { "id": 13531, "url": "https://svs.gsfc.nasa.gov/13531/", "result_type": "Produced Video", "release_date": "2020-01-31T00:00:00-05:00", "title": "XRISM: Calorimeter Spectrometer Insert and Mirror Tests", "description": "XRISM team members pose with the XRISM Calorimeter Spectrometer Insert in a NASA Goddard clean room. From left to right, they are Bryan James, Mike Sampson, Tomomi Watanabe, Pete Barfknecht, Scott Porter, and Sinclair Douglas.Credit: Larry Gilbert/NASA || GSFC_20191101__2020-2568_07.jpg (3000x1995) [3.6 MB] || GSFC_20191101__2020-2568_07_searchweb.png (320x180) [111.9 KB] || GSFC_20191101__2020-2568_07_thm.png (80x40) [7.7 KB] || ", "hits": 49 }, { "id": 13530, "url": "https://svs.gsfc.nasa.gov/13530/", "result_type": "Produced Video", "release_date": "2020-01-30T00:00:00-05:00", "title": "Mirror Quadrants for XRISM", "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ", "hits": 50 }, { "id": 13240, "url": "https://svs.gsfc.nasa.gov/13240/", "result_type": "Produced Video", "release_date": "2019-12-12T11:00:00-05:00", "title": "NASA’s NICER Sizes Up a Pulsar, Reveals First-ever Surface Map", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) has expanded our understanding of pulsars, the dense, spinning corpses of exploded stars. Pulsar J0030+0451 (J0030 for short), located 1,100 light-years away in the constellation Pisces, now has the most precise and reliable measurements of both a pulsar’s mass and size to date. The shapes and locations of its hot spots challenge textbook depictions of these incredible objects. Music: \"Uncertain Ahead\" and \"Flowing Cityscape\" (underscore). Both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Two_NS_Model_Still.jpg (1920x1080) [308.5 KB] || Two_NS_Model_Still_print.jpg (1024x576) [140.4 KB] || Two_NS_Model_Still_searchweb.png (320x180) [87.0 KB] || Two_NS_Model_Still_thm.png (80x40) [8.0 KB] || 13240_NICER_J0030_MassRadius_1080.webm (1920x1080) [33.5 MB] || 13240_NICER_J0030_MassRadius_1080.mp4 (1920x1080) [301.1 MB] || 13240_NICER_J0030_MassRadius_Best_1080.mp4 (1920x1080) [804.5 MB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.srt [5.9 KB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.vtt [5.9 KB] || 13240_NICER_J0030_MassRadius_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || ", "hits": 131 }, { "id": 13480, "url": "https://svs.gsfc.nasa.gov/13480/", "result_type": "Produced Video", "release_date": "2019-11-20T00:00:00-05:00", "title": "NASA Science Live: Black Hole 101 (Episode 11)", "description": "NASA Science Live: Black Hole 101 (Episode 11) || 13480_NSL_Blackhole_youtube_720.00001_print.jpg (1024x576) [79.3 KB] || 13480_NSL_Blackhole_youtube_720.00001_searchweb.png (320x180) [79.1 KB] || 13480_NSL_Blackhole_youtube_720.00001_thm.png (80x40) [5.5 KB] || 13480_NSL_Blackhole_lowres.mp4 (1280x720) [551.1 MB] || 13480_NSL_Blackhole_youtube_720.mp4 (1280x720) [3.1 GB] || 13480_NSL_Blackhole.mov (1280x720) [20.6 GB] || 13480_NSL_Blackhole_youtube_720.webm (1280x720) [223.1 MB] || 13480_NSL_Blackhole.en_US.srt [56.3 KB] || 13480_NSL_Blackhole.en_US.vtt [52.8 KB] || ", "hits": 153 }, { "id": 13419, "url": "https://svs.gsfc.nasa.gov/13419/", "result_type": "Animation", "release_date": "2019-11-07T13:00:00-05:00", "title": "NICER Catches Milestone X-ray Burst", "description": "At about 10:04 p.m. EDT on Aug. 20, NASA’s Neutron star Interior Composition Explorer (NICER) telescope on the International Space Station detected a sudden spike of X-rays caused by a massive thermonuclear flash on the surface of a pulsar, the crushed remains of a star that long ago exploded as a supernova. The X-ray burst, the brightest seen by NICER so far, came from an object named SAX J1808.4-3658, or J1808 for short. The observations reveal many phenomena that have never been seen together in a single burst. In addition, the subsiding fireball briefly brightened again for reasons astronomers cannot yet explain. The data reveal a two-step change in brightness, which scientists think is caused by the ejection of separate layers from the pulsar surface, and other features that will help them decode the physics of these powerful events.The explosion, which astronomers classify as a Type I X-ray burst, released as much energy in 20 seconds as the Sun does in nearly 10 days.J1808 is located about 11,000 light-years away in the constellation Sagittarius, spins at a dizzying 401 rotations each second, and is one member of a binary system. Its companion is a brown dwarf, an object larger than a giant planet yet too small to be a star. A steady stream of hydrogen gas flows from the companion toward the neutron star, and it accumulates in a vast storage structure called an accretion disk.Hydrogen raining onto the pulsar's surface forms a hot, ever-deepening global “sea.” At the base of this layer, temperatures and pressures increase until hydrogen nuclei fuse to form helium nuclei, which produces energy — a process at work in the core of our Sun. The helium settles out and builds up a layer of its own. Eventually, the conditions allow helium nuclei to fuse into carbon. The helium erupts explosively and unleashes a thermonuclear fireball across the entire pulsar surface.As the burst started, NICER data show that its X-ray brightness leveled off for almost a second before increasing again at a slower pace. The researchers interpret this “stall” as the moment when the energy of the blast built up enough to blow the pulsar’s hydrogen layer into space. The fireball continued to build for another two seconds and then reached its peak, blowing off the more massive helium layer. The helium expanded faster, overtook the hydrogen layer before it could dissipate, and then slowed, stopped and settled back down onto the pulsar’s surface. Following this phase, the pulsar briefly brightened again by roughly 20 percent for reasons the team does not yet understand. || ", "hits": 96 }, { "id": 13415, "url": "https://svs.gsfc.nasa.gov/13415/", "result_type": "Produced Video", "release_date": "2019-10-31T00:00:00-04:00", "title": "NASA Science Live: Galaxy of Horrors (Episode 10)", "description": "NASA Science Live: Galaxy of Horrors (Episode 10) || 13415_NSL_Galaxy_Ep10_youtube_720.00001_print.jpg (1024x576) [79.7 KB] || 13415_NSL_Galaxy_Ep10_youtube_720.00001_searchweb.png (320x180) [79.6 KB] || 13415_NSL_Galaxy_Ep10_youtube_720.00001_thm.png (80x40) [5.5 KB] || 13415_NSL_Galaxy_Ep10_lowres.mp4 (1280x720) [550.9 MB] || 13415_NSL_Galaxy_Ep10_youtube_720.mp4 (1280x720) [3.1 GB] || 13415_NSL_Galaxy_Ep10.mov (1280x720) [20.7 GB] || 13415_NSL_Galaxy_Ep10_youtube_720.webm (1280x720) [222.1 MB] || 13415_NSL_Galaxy_Ep10.en_US.srt [59.1 KB] || 13415_NSL_Galaxy_Ep10.en_US.vtt [55.9 KB] || ", "hits": 39 }, { "id": 13344, "url": "https://svs.gsfc.nasa.gov/13344/", "result_type": "Produced Video", "release_date": "2019-10-18T00:00:00-04:00", "title": "NASA Science Live: A Telescope Like a Time Machine (Episode 9)", "description": "NASA Science Live: A Telescope Like a Time Machine (Episode 9) || 13344_NSL_WEBB_Ep9.00001_print.jpg (1024x576) [81.9 KB] || 13344_NSL_WEBB_Ep9.00001_searchweb.png (320x180) [81.6 KB] || 13344_NSL_WEBB_Ep9.00001_thm.png (80x40) [5.7 KB] || 13344_NSL_WEBB_Ep9_lowres.mp4 (1280x720) [551.7 MB] || 13344_NSL_WEBB_Ep9_youtube_720.mp4 (1280x720) [3.2 GB] || 13344_NSL_WEBB_Ep9.mov (1280x720) [20.8 GB] || 13344_NSL_WEBB_Ep9.webm (1280x720) [224.0 MB] || 13344_NSL_WEBB_Ep9.en_US.srt [64.0 KB] || 13344_NSL_WEBB_Ep9.en_US.vtt [60.5 KB] || ", "hits": 25 }, { "id": 13237, "url": "https://svs.gsfc.nasa.gov/13237/", "result_type": "Produced Video", "release_date": "2019-09-26T11:00:00-04:00", "title": "TESS Catches Its First Star-destroying Black Hole", "description": "When a star strays too close to a black hole, intense tides break it apart into a stream of gas. The tail of the stream escapes the system, while the rest of it swings back around, surrounding the black hole with a disk of debris. This video includes images of a tidal disruption event called ASASSN-19bt taken by NASA’s Transiting Exoplanet Survey Satellite (TESS) and Swift missions, as well as an animation showing how the event unfolded. Credit: NASA’s Goddard Space Flight CenterMusic: \"Games Show Sphere 03\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_TDE_Still_print.jpg (1024x576) [87.3 KB] || TESS_TDE_Still.jpg (3840x2160) [629.6 KB] || TESS_TDE_Still_searchweb.png (320x180) [68.3 KB] || TESS_TDE_Still_thm.png (80x40) [5.3 KB] || 13237_TESS_TDE_ProRes_1920x1080.mov (1920x1080) [1.6 GB] || 13237_TESS_TDE_1080_Best.mp4 (1920x1080) [380.2 MB] || 13237_TESS_TDE_1080.mp4 (1920x1080) [125.6 MB] || 13237_TESS_TDE_1080_Best.webm (1920x1080) [12.6 MB] || 13237_TESS_TDE_SRT_Captions.en_US.srt [2.2 KB] || 13237_TESS_TDE_SRT_Captions.en_US.vtt [2.2 KB] || ", "hits": 102 }, { "id": 13326, "url": "https://svs.gsfc.nasa.gov/13326/", "result_type": "Produced Video", "release_date": "2019-09-25T13:00:00-04:00", "title": "Black Hole Accretion Disk Visualization", "description": "This movie shows a complete revolution around a simulated black hole and its accretion disk following a path that is perpendicular to the disk. The black hole’s extreme gravitational field redirects and distorts light coming from different parts of the disk, but exactly what we see depends on our viewing angle. The greatest distortion occurs when viewing the system nearly edgewise. As our viewpoint rotates around the black hole, we see different parts of the fast-moving gas in the accretion disk moving directly toward us. Due to a phenomenon called \"relativistic Doppler beaming,\" gas in the disk that's moving toward us makes that side of the disk appear brighter, the opposite side darker. This effect disappears when we're directly above or below the disk because, from that angle, none of the gas is moving directly toward us.When our viewpoint passes beneath the disk, it looks like the gas is moving in the opposite direction. This is no different that viewing a clock from behind, which would make it look like the hands are moving counter-clockwise.CORRECTION: In earlier versions of the 360-degree movies on this page, these important effects were not apparent. This was due to a minor mistake in orienting the camera relative to the disk. The fact that it was not initially discovered by the NASA scientist who made the movie reflects just how bizarre and counter-intuitive black holes can be! Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman || BH_Accretion_Disk_Sim_360_4k_Prores.00001_print.jpg (1024x1024) [33.2 KB] || BH_Accretion_Disk_Sim_360_4k_Prores.00001_searchweb.png (320x180) [17.0 KB] || BH_Accretion_Disk_Sim_360_4k_Prores.00001_thm.png (80x40) [1.9 KB] || BH_Accretion_Disk_Sim_360_1080.mp4 (1080x1080) [19.0 MB] || BH_Accretion_Disk_Sim_360_1080.webm (1080x1080) [2.8 MB] || 360 (3840x3840) [0 Item(s)] || BH_Accretion_Disk_Sim_360_4k.mp4 (3840x3840) [119.2 MB] || BH_Accretion_Disk_Sim_360_4k_Prores.mov (3840x3840) [1020.1 MB] || ", "hits": 3323 }, { "id": 13199, "url": "https://svs.gsfc.nasa.gov/13199/", "result_type": "Produced Video", "release_date": "2019-06-24T13:00:00-04:00", "title": "XMM-Newton Anniversary Products", "description": "Scientists reflect on XMM-Newton’s 20th anniversary. The mission, led by ESA (European Space Agency), has dramatically improved our understanding of the cosmos thanks to detailed X-ray observations. NASA funded two of its three instruments, including the Optical/UV Monitor Telescope, which made XMM-Newton one of the first multiwavelength observatories in space.Music: \"Passionate Research\" and \"Wondrous Planet\" both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XMM_Still1.jpg (1280x720) [553.6 KB] || XMM_Still1_print.jpg (1024x576) [451.3 KB] || XMM_20th_Anniversary_ProRes_1280x720_2997.mov (1280x720) [3.1 GB] || XMM_20th_Anniversary_Best_720.mp4 (1280x720) [891.1 MB] || XMM_20th_Anniversary_Good_720.mp4 (1280x720) [251.9 MB] || XMM_20th_Anniversary_Best_720.webm (1280x720) [52.7 MB] || XMM_20th_Anniversary_SRT_Captions.en_US.srt [9.6 KB] || XMM_20th_Anniversary_SRT_Captions.en_US.vtt [9.6 KB] || ", "hits": 26 }, { "id": 13214, "url": "https://svs.gsfc.nasa.gov/13214/", "result_type": "Produced Video", "release_date": "2019-05-30T10:45:00-04:00", "title": "NICER's Night Moves", "description": "This image of the whole sky shows 22 months of X-ray data recorded by NASA's Neutron star Interior Composition Explorer (NICER) payload aboard the International Space Station during its nighttime slews between targets. NICER frequently observes targets best suited to its core mission (“mass-radius” pulsars) and those whose regular pulses are ideal for the Station Explorer for X-ray Timing and Navigation Technology (SEXTANT) experiment. One day they could form the basis of a GPS-like system for navigating the solar system.Credits: NASA/NICER || NICERNightMoveslabels.jpg (3299x1650) [13.7 MB] || ", "hits": 105 }, { "id": 12854, "url": "https://svs.gsfc.nasa.gov/12854/", "result_type": "Produced Video", "release_date": "2019-01-30T12:30:00-05:00", "title": "NICER Charts the Area Around a New Black Hole", "description": "Watch how X-ray echoes, mapped by NASA’s Neutron star Interior Composition Explorer (NICER) revealed changes to the corona of black hole MAXI J1820+070.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" from Killer TracksComplete transcript available. || Black_Hole_Corona_Still.jpg (1920x1080) [317.0 KB] || Black_Hole_Corona_Still_print.jpg (1024x576) [109.5 KB] || Black_Hole_Corona_Still_searchweb.png (320x180) [87.9 KB] || Black_Hole_Corona_Still_thm.png (80x40) [6.6 KB] || 12854_Black_Hole_Corona_ProRes_1920x1080.mov (1920x1080) [3.3 GB] || 12854_Black_Hole_Corona_1080p.mov (1920x1080) [515.0 MB] || 12854_Black_Hole_Corona.mp4 (1920x1080) [335.5 MB] || 12854_Black_Hole_Corona_small.mp4 (1920x1080) [135.2 MB] || 12854_Black_Hole_Corona_ProRes_1920x1080.webm (1920x1080) [26.7 MB] || 12854_Black_Hole_Corona_SRT_Captions.en_US.srt [4.5 KB] || 12854_Black_Hole_Corona_SRT_Captions.en_US.vtt [4.5 KB] || ", "hits": 67 }, { "id": 12855, "url": "https://svs.gsfc.nasa.gov/12855/", "result_type": "Produced Video", "release_date": "2019-01-10T13:00:00-05:00", "title": "Mysterious ‘Cow’ Blast Studied with NASA Telescopes", "description": "Watch what scientists think happens when a black hole tears apart a hot, dense white dwarf star. A team working with observations from NASA’s Neil Gehrels Swift Observatory suggest this process explains a mysterious outburst known as AT2018cow. Credit: NASA's Goddard Space Flight CenterMusic: \"Curious Events\" from Killer TracksWatch this video on the JPL YouTube channel.Complete transcript available. || AT2018COW_Labeled_Still_3_print.jpg (1024x576) [66.0 KB] || AT2018COW_Labeled_Still_3.jpg (3840x2160) [494.0 KB] || AT2018COW_Labeled_Still_3_searchweb.png (320x180) [56.8 KB] || AT2018COW_Labeled_Still_3_thm.png (80x40) [5.5 KB] || AT2018COW_Labeled_Music_Intro_3_1080.mp4 (1920x1080) [116.5 MB] || AT2018COW_Labeled_Music_Intro_3_1080p.mov (1920x1080) [161.2 MB] || AT2018COW_Labeled_Music_Intro_3_1080.webm (1920x1080) [13.2 MB] || AT2018COW_Labeled_Music_Intro_3_ProRes_3840x2160.mov (3840x2160) [4.7 GB] || AT2018COW_Labeled_Music_Intro_3_4k.mp4 (3840x2160) [436.5 MB] || AT2018COW_Labeled_Music_Intro_3_4K.mov (3840x2160) [241.6 MB] || AT2018COW_SRT_Captions.en_US.srt [1.2 KB] || AT2018COW_SRT_Captions.en_US.vtt [1.3 KB] || ", "hits": 136 }, { "id": 13042, "url": "https://svs.gsfc.nasa.gov/13042/", "result_type": "Produced Video", "release_date": "2018-11-08T13:00:00-05:00", "title": "NASA's Fermi Mission Shows How Luck Favors the Prepared", "description": "Explore how more than a century of scientific progress with gravitational waves, gamma rays and neutrinos has helped bring about the age of multimessenger astronomy. Music: \"Family Tree,\" \"The Archives\" and \"Beyond Truth,\" all from Killer Tracks.Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Luck_Timeline_Still_print.jpg (1024x576) [140.7 KB] || Luck_Timeline_Still.jpg (3840x2160) [1.1 MB] || Luck_Timeline_Still_searchweb.png (320x180) [78.5 KB] || Luck_Timeline_Still_thm.png (80x40) [7.4 KB] || 13042_LuckFavorsThePrepared_1080p.mov (1920x1080) [550.2 MB] || 13042_LuckFavorsThePrepared_1080.mp4 (1920x1080) [373.6 MB] || 13042_LuckFavorsThePrepared_1080.m4v (1920x1080) [188.4 MB] || 13042_LuckFavorsThePrepared_1080p.webm (1920x1080) [39.3 MB] || 13042_LuckFavorsThePrepared_ProRes_3840x2160_2997.mov (3840x2160) [19.8 GB] || 13042_LuckFavorsThePrepared_2160.mp4 (3840x2160) [1.1 GB] || 13042_LuckFavorsThePrepared_4K.mov (3840x2160) [715.2 MB] || LuckFavorsThePrepared_SRT_Captions.en_US.srt [6.5 KB] || LuckFavorsThePrepared_SRT_Captions.en_US.vtt [6.3 KB] || ", "hits": 135 }, { "id": 13043, "url": "https://svs.gsfc.nasa.gov/13043/", "result_type": "Produced Video", "release_date": "2018-10-02T10:50:00-04:00", "title": "New Simulation Sheds Light on Spiraling Supermassive Black Holes", "description": "Gas glows brightly in this computer simulation of supermassive black holes only 40 orbits from merging. Models like this may eventually help scientists pinpoint real examples of these powerful binary systems. Credit: NASA's Goddard Space Flight Center/Scott Noble; simulation data, d'Ascoli et al. 2018Music: \"Games Show Sphere 01\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SMBH_Sim_Still_1.jpg (1920x1080) [333.8 KB] || SMBH_Sim_Still_1_print.jpg (1024x576) [138.8 KB] || SMBH_Sim_Still_1_searchweb.png (320x180) [69.3 KB] || SMBH_Sim_Still_1_thm.png (80x40) [6.4 KB] || 13043_SMBH_Simulation_1080.webm (1920x1080) [17.4 MB] || 13043_SMBH_Simulation_1080.mp4 (1920x1080) [202.8 MB] || SMBH_SRT_Captions.en_US.srt [2.0 KB] || SMBH_SRT_Captions.en_US.vtt [1.9 KB] || 13043_SMBH_Simulation_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || ", "hits": 279 }, { "id": 13086, "url": "https://svs.gsfc.nasa.gov/13086/", "result_type": "Produced Video", "release_date": "2018-10-02T10:50:00-04:00", "title": "Supermassive Black Hole Binary Simulation Visualizations in 4k", "description": "Simulation of the light emitted by a supermassive black hole binary system where the surrounding gas is optically thin (transparent). Viewed from 0 degrees inclination, or directly above the plane of the disk. The emitted light represents all wavelengths.Credit: NASA's Goddard Space Flight Center/Scott Noble; simulation data, d'Ascoli et al. 2018 || image-000-_000150_print.jpg (1024x576) [33.9 KB] || image-000-_000150.png (3840x2160) [5.1 MB] || 0Degrees (3840x2160) [0 Item(s)] || SMBH_Sim_Thin0_4kFull.mp4 (3840x2160) [15.0 MB] || SMBH_Sim_Thin0_4kFull.webm (3840x2160) [2.2 MB] || SMBH_Sim_Thin0_4kFull.mov (3840x2160) [427.6 MB] || ", "hits": 300 }, { "id": 12980, "url": "https://svs.gsfc.nasa.gov/12980/", "result_type": "Produced Video", "release_date": "2018-08-21T10:00:00-04:00", "title": "Swift Millionth Image Mosaic", "description": "This mosaic of the Neil Gehrels Swift Observatory is created from images of astronomical objects captured by the satellite’s Ultraviolet/Optical Telescope which recently captured its millionth image. Each tile is 52 x 39 pixels, and at maximum resolution, the entire mosaic is 5,252 x 3,744 pixels. Zoom in to see each tile more clearly. Credit: NASA/Swift and AndreaMosaic || Swift_Millionth_Image_Mosaic_2k.jpg (2000x1426) [593.8 KB] || Swift_Millionth_Image_Mosaic_2k_print.jpg (1024x730) [148.9 KB] || Swift_Millionth_Image_Mosaic.jpg (5252x3744) [3.2 MB] || Swift_Millionth_Image_Mosaic_2k_searchweb.png (320x180) [65.4 KB] || Swift_Millionth_Image_Mosaic_2k_thm.png (80x40) [5.1 KB] || ", "hits": 126 }, { "id": 13031, "url": "https://svs.gsfc.nasa.gov/13031/", "result_type": "Produced Video", "release_date": "2018-08-14T13:00:00-04:00", "title": "NASA'S NICER Does the Space Station Twist", "description": "NICER Video with Astro and Goddard end tagsMusic: \"Frames of Motion\" from Killer TracksComplete transcript available. || NICER_ISS_Goddard.mp4 (1920x1080) [94.9 MB] || NICER_ISS_Goddard.webm (1920x1080) [9.9 MB] || NICER_ISS_Goddard_SRT_Captions.en_US.srt [868 bytes] || NICER_ISS_Goddard_SRT_Captions.en_US.vtt [806 bytes] || ", "hits": 80 }, { "id": 12989, "url": "https://svs.gsfc.nasa.gov/12989/", "result_type": "Produced Video", "release_date": "2018-07-03T11:00:00-04:00", "title": "Superstar Eta Carinae Shoots Cosmic Rays", "description": "Zoom into Eta Carinae, where the outflows of two massive stars collide and shoot accelerated particles cosmic rays into space.Credit: NASA’s Goddard Space Flight Center Music: \"Expectant Aspect\" from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Eta_Car_CR_Still.jpg (1920x1080) [307.1 KB] || Eta_Car_CR_Still_print.jpg (1024x576) [127.9 KB] || Eta_Car_CR_Still_searchweb.png (320x180) [98.2 KB] || Eta_Car_CR_Still_thm.png (80x40) [7.3 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.webm (1920x1080) [16.1 MB] || 12989_Eta_Car_CosmicRay_1080.m4v (1920x1080) [155.6 MB] || 12989_Eta_Car_CosmicRay_1080.mp4 (1920x1080) [234.6 MB] || 12989_Eta_Car_CosmicRay_1080p.mov (1920x1080) [311.6 MB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.srt [2.0 KB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.vtt [2.0 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.mov (1920x1080) [2.1 GB] || ", "hits": 208 }, { "id": 30970, "url": "https://svs.gsfc.nasa.gov/30970/", "result_type": "Hyperwall Visual", "release_date": "2018-06-25T10:00:00-04:00", "title": "Kepler Supernova Remnant", "description": "This animation shows the remnant of Kepler's Supernova, shown first in infrared, then visible, then low energy X-ray, then high-energy X-ray emission and finally in combination. || STScI-H-KeplerSNR_1x-1920x1080.00001_print.jpg (1024x576) [18.4 KB] || STScI-H-KeplerSNR_1x-1920x1080.00001_searchweb.png (320x180) [15.9 KB] || STScI-H-KeplerSNR_1x-1920x1080.00001_thm.png (80x40) [2.1 KB] || STScI-H-KeplerSNR_1x-1280x720.mp4 (1280x720) [1.8 MB] || STScI-H-KeplerSNR_1x-1920x1080.mp4 (1920x1080) [3.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-KeplerSNR_1x-1920x1080.webm (1920x1080) [6.4 MB] || STScI-H-KeplerSNR_1x-640x360.mp4 (640x360) [708.9 KB] || STScI-H-KeplerSNR_1x-3840x2160.mp4 (3840x2160) [3.8 MB] || STScI-H-KeplerSNR_1x-H265-3840x2160.mp4 (3840x2160) [2.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 97 }, { "id": 30960, "url": "https://svs.gsfc.nasa.gov/30960/", "result_type": "Hyperwall Visual", "release_date": "2018-06-04T10:00:00-04:00", "title": "Eagle Nebula: M16 Wide", "description": "This series of images shows the environment around the Pillars of Creation, the Eagle Nebula, Messier 16. The images reveal the nebula in optical, X-ray, mid-infrared, and far-infrared light. || STScI-H-M16wide_1x-1920x1080.00001_print.jpg (1024x576) [163.7 KB] || STScI-H-M16wide_1x-1920x1080.00001_searchweb.png (320x180) [108.4 KB] || STScI-H-M16wide_1x-1920x1080.00001_thm.png (80x40) [6.9 KB] || STScI-H-M16wide_1x-1280x720.mp4 (1280x720) [8.5 MB] || STScI-H-M16wide_1x-1920x1080.mp4 (1920x1080) [17.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M16wide_1x-1920x1080.webm (1920x1080) [5.2 MB] || STScI-H-M16wide_1x-640x360.mp4 (640x360) [2.9 MB] || STScI-H-M16wide_1x-3840x2160.mp4 (3840x2160) [17.1 MB] || STScI-H-M16wide_1x-H265-3840x2160.mp4 (3840x2160) [7.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 172 }, { "id": 30961, "url": "https://svs.gsfc.nasa.gov/30961/", "result_type": "Hyperwall Visual", "release_date": "2018-06-04T10:00:00-04:00", "title": "Milky Way Center in Multiple Wavelengths", "description": "This animation reveals the center of our Milky Way galaxy, first in near-infrared, then mid-infrared, then X-ray light, and then all three in combination. || STScI-H-MWC_1x-1920x1080.00001_print.jpg (1024x576) [153.0 KB] || STScI-H-MWC_1x-1920x1080.00001_searchweb.png (320x180) [94.5 KB] || STScI-H-MWC_1x-1920x1080.00001_thm.png (80x40) [5.5 KB] || STScI-H-MWC_1x-1280x720.mp4 (1280x720) [8.4 MB] || STScI-H-MWC_1x-1920x1080.mp4 (1920x1080) [18.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-MWC_1x-1920x1080.webm (1920x1080) [4.5 MB] || STScI-H-MWC_1x-640x360.mp4 (640x360) [2.8 MB] || STScI-H-MWC_1x-3840x2160.mp4 (3840x2160) [15.7 MB] || STScI-H-MWC_1x-H265-3840x2160.mp4 (3840x2160) [8.8 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || ", "hits": 255 }, { "id": 30952, "url": "https://svs.gsfc.nasa.gov/30952/", "result_type": "Hyperwall Visual", "release_date": "2018-05-21T10:00:00-04:00", "title": "The Whirlpool Galaxy: Visible and X-ray Views", "description": "This animation contrasts the visible-light (Hubble Space Telescope) and X-ray (Chandra X-ray Observatory) images of Messier 51, the majestic Whirlpool galaxy. || STScI-H-M51-Whirlpool_1x-1920x1080.00001_print.jpg (1024x576) [193.0 KB] || STScI-H-M51-Whirlpool_1x-1920x1080.00001_searchweb.png (320x180) [105.6 KB] || STScI-H-M51-Whirlpool_1x-1920x1080.00001_thm.png (80x40) [6.7 KB] || STScI-H-M51-Whirlpool_1x-1280x720.mp4 (1280x720) [6.2 MB] || STScI-H-M51-Whirlpool_1x-1920x1080.mp4 (1920x1080) [14.5 MB] || STScI-H-M51-Whirlpool_1x-1920x1080.webm (1920x1080) [3.0 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M51-Whirlpool_1x-640x360.mp4 (640x360) [1.8 MB] || STScI-H-M51-Whirlpool_1x-3840x2160.mp4 (3840x2160) [12.4 MB] || STScI-H-M51-Whirlpool_1x-H265-3840x2160.mp4 (3840x2160) [6.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 185 }, { "id": 12938, "url": "https://svs.gsfc.nasa.gov/12938/", "result_type": "Produced Video", "release_date": "2018-05-10T13:00:00-04:00", "title": "NICER Finds X-ray Pulsar in Record-fast Orbit", "description": "Scientists analyzing the first data from the Neutron Star Interior Composition Explorer (NICER) mission have found two stars that revolve around each other every 38 minutes. One of the stars in the system, called IGR J17062–6143 (J17062 for short), is a rapidly spinning, superdense star called a pulsar. The other is probably a hydrogen-poor white dwarf. The discovery bestows the stellar pair with the record for the shortest-known orbital period for a certain class of pulsar binary system.Music: \"Games Show Sphere 2\" from Killer TracksComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || NICER_Binary_Still.jpg (1920x1080) [197.3 KB] || NICER_Binary_Still_print.jpg (1024x576) [89.4 KB] || NICER_Binary_Still_searchweb.png (320x180) [46.7 KB] || NICER_Binary_Still_thm.png (80x40) [4.0 KB] || 12938_NICER_Binary_1080.mp4 (1920x1080) [91.4 MB] || 12938_NICER_Binary_1080p.mov (1920x1080) [47.8 MB] || 12938_NICER_Binary_Good_1080.m4v (1920x1080) [44.7 MB] || 12938_NICER_Binary_1080p.webm (1920x1080) [7.0 MB] || 12938_NICER_Binary_ProRes_1920x1080_2997.mov (1920x1080) [456.9 MB] || NICER_Binary_SRT_Captions.en_US.srt [767 bytes] || NICER_Binary_SRT_Captions.en_US.vtt [741 bytes] || ", "hits": 105 }, { "id": 30944, "url": "https://svs.gsfc.nasa.gov/30944/", "result_type": "Hyperwall Visual", "release_date": "2018-05-07T10:00:00-04:00", "title": "Vision Across the Full Spectrum: The Crab Nebula, from Radio to X-ray", "description": "This animation shows the Crab Nebula from the lowest-frequency light (radio), to infrared, visible, ultraviolet, and finally X-ray. || STScI-H-CrabNebula_1x-1920x1080.00001_print.jpg (1024x576) [40.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_searchweb.png (320x180) [26.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_thm.png (80x40) [2.3 KB] || STScI-H-CrabNebula_1x-1280x720.mp4 (1280x720) [3.8 MB] || STScI-H-CrabNebula_1x-1920x1080.mp4 (1920x1080) [7.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-CrabNebula_1x-1920x1080.webm (1920x1080) [8.0 MB] || STScI-H-CrabNebula_1x-640x360.mp4 (640x360) [1.4 MB] || STScI-H-CrabNebula_1x-3840x2160.mp4 (3840x2160) [16.2 MB] || STScI-H-CrabNebula_1x-H265_3840x2160.mp4 (3840x2160) [3.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 341 }, { "id": 12934, "url": "https://svs.gsfc.nasa.gov/12934/", "result_type": "Produced Video", "release_date": "2018-05-01T09:50:00-04:00", "title": "RXTE Photos", "description": "Technicians work on RXTE in 1995.Credit: NASA’s Goddard Space Flight Center || 614636main_416240main_rxte-full.jpg (2307x2217) [7.1 MB] || RXTE_Crop_searchweb.png (320x180) [102.5 KB] || RXTE_Crop_thm.png (80x40) [7.2 KB] || Photos of the Rossi X-ray Timing Explorer satellite in 1995, prior to its Dec. 30 launch. RXTE provided unprecedented views into the extreme environments around white dwarfs, neutron stars and black holes until it was decomissioned on Jan. 4, 2012. || ", "hits": 27 }, { "id": 30941, "url": "https://svs.gsfc.nasa.gov/30941/", "result_type": "Hyperwall Visual", "release_date": "2018-04-23T10:00:00-04:00", "title": "Colliding Galaxies (NGC 2207)", "description": "This animation shows the interacting galaxy pair NGC 2207, first in optical light, then in infrared, in X-ray, and finally in combination. || STScI-H-NGC2207_1x-1920x1080.00001_print.jpg (1024x576) [157.8 KB] || STScI-H-NGC2207_1x-1920x1080.00001_searchweb.png (320x180) [92.0 KB] || STScI-H-NGC2207_1x-1920x1080.00001_thm.png (80x40) [6.5 KB] || STScI-H-NGC2207_1x-1280x720.mp4 (1280x720) [4.5 MB] || STScI-H-NGC2207_1x-1920x1080.mp4 (1920x1080) [9.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-NGC2207_1x-1920x1080.webm (1920x1080) [4.9 MB] || STScI-H-NGC2207_1x-640x360.mp4 (640x360) [1.5 MB] || STScI-H-NGC2207_1x-3840x2160.mp4 (3840x2160) [8.8 MB] || STScI-H-NGC2207_1x-H265-3840x2160.mp4 (3840x2160) [4.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 221 }, { "id": 12806, "url": "https://svs.gsfc.nasa.gov/12806/", "result_type": "Produced Video", "release_date": "2017-12-21T13:00:00-05:00", "title": "'Winking' Star May Be Devouring Wrecked Planets", "description": "Zoom into RZ Piscium, a star about 550 light-years away that undergoes erratic dips in brightness. This animation illustrates one possible interpretation of the system, with a giant planet near the star slowly dissolving. Gas and dust stream away from the planet, and these clouds occasionally eclipse the star as we view it from Earth.Music: \"Frozen Wonder\" from Killer Tracks Watch this video on the NASA Goddard YouTube channel.Credit NASA's Goddard Space Flight Center/CI LabComplete transcript available. || StarObscure_Plane_v06_PNG_00333.png (1920x1080) [6.1 MB] || StarObscure_Plane_v06_00333.jpg (1920x1080) [131.6 KB] || StarObscure_Plane_v06_00333_print.jpg (1024x576) [53.2 KB] || StarObscure_Plane_v06_00333_searchweb.png (320x180) [38.0 KB] || StarObscure_Plane_v06_00333_thm.png (80x40) [4.0 KB] || 12806_RZ_Piscium_ProRes_1920x1080_2997.mov (1920x1080) [942.8 MB] || 12806_RZ_Piscium_H264_Best_1080p.mov (1920x1080) [172.1 MB] || 12806_RZ_Piscium_1080.mp4 (1920x1080) [73.4 MB] || 12806_RZ_Piscium_H264_1080.m4v (1920x1080) [72.4 MB] || 12806_RZ_Piscium_H264_1080.webm (1920x1080) [7.9 MB] || R2Piscium.en_US.srt [805 bytes] || R2Piscium.en_US.vtt [818 bytes] || ", "hits": 118 }, { "id": 12640, "url": "https://svs.gsfc.nasa.gov/12640/", "result_type": "Produced Video", "release_date": "2017-11-16T14:00:00-05:00", "title": "How Solar Flares Affect Earth", "description": "A team of scientists —led by Laura Hayes, a solar physicist who splits her time between NASA Goddard and Trinity College in Dublin, Ireland— investigated a connection between solar flares and Earth’s atmosphere. They discovered pulses in the electrified layer of the atmosphere—called the ionosphere—mirrored X-ray oscillations during a July 24, 2016 flare. Music: \"Good Chat\" by Richard Anthony D Pike on Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || flarefluxthumb.jpg (1920x1080) [846.0 KB] || flarefluxthumb_searchweb.png (320x180) [85.6 KB] || flarefluxthumb_thm.png (80x40) [6.6 KB] || flarefluxthumb_web.png (320x180) [85.6 KB] || 12640_Flare_Flux_ProRes_1920x1080_2997.mov (1920x1080) [950.0 MB] || 12640_Flare_Flux-Best.mov (1920x1080) [142.7 MB] || 12640_Flare_Flux-Good.m4v (1920x1080) [69.0 MB] || 12640_Flare_Flux-Compatible.m4v (960x540) [25.4 MB] || 12640_Flare_Flux-Compatible.webm (960x540) [7.2 MB] || 12640_Flare_Flux_9.en_US.srt [1.2 KB] || 12640_Flare_Flux_9.en_US.vtt [1.2 KB] || ", "hits": 249 }, { "id": 12740, "url": "https://svs.gsfc.nasa.gov/12740/", "result_type": "Produced Video", "release_date": "2017-10-16T10:00:00-04:00", "title": "Doomed Neutron Stars Create Blast of Light and Gravitational Waves", "description": "This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue). Credit: NASA's Goddard Space Flight Center/CI LabMusic: \"Exploding Skies\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Neutron_Star_Merger_Still_2_new_1080.png (1920x1080) [2.5 MB] || Neutron_Star_Merger_Still_2_new_1080.jpg (1920x1080) [167.3 KB] || Neutron_Star_Merger_Still_2_new_print.jpg (1024x576) [50.4 KB] || Neutron_Star_Merger_Still_2_new.png (3840x2160) [7.7 MB] || Neutron_Star_Merger_Still_2_new.jpg (3840x2160) [1.0 MB] || Neutron_Star_Merger_Still_2_new_thm.png (80x40) [4.4 KB] || Neutron_Star_Merger_Still_2_new_searchweb.png (320x180) [51.4 KB] || 12740_NS_Merger_Update_1080.m4v (1920x1080) [50.3 MB] || 12740_NS_Merger_Update_H264_1080.mp4 (1920x1080) [96.9 MB] || 12740_NS_Merger_Update_1080p.mov (1920x1080) [101.9 MB] || NS_Merger_SRT_Captions.en_US.srt [417 bytes] || NS_Merger_SRT_Captions.en_US.vtt [399 bytes] || 12740_NS_Merger_4k_Update.webm (3840x2160) [10.0 MB] || 12740_NS_Merger_4k_Update_H264.mp4 (3840x2160) [254.9 MB] || 12740_NS_Merger_4k_Update_H264.mov (3840x2160) [516.7 MB] || 12740_NS_Merger_4k_Update_ProRes_3840x2160_5994.mov (3840x2160) [5.1 GB] || 12740_NS_Merger_4k_Update_H264.hwshow [90 bytes] || ", "hits": 632 }, { "id": 12630, "url": "https://svs.gsfc.nasa.gov/12630/", "result_type": "Produced Video", "release_date": "2017-06-01T00:00:00-04:00", "title": "NICER Mission Overview", "description": "The Neutron Star Interior Composition Explorer (NICER) payload, destined for the exterior of the space station, will study the physics of neutron stars, providing new insight into their nature and behavior. These stars are called “pulsars” because of the unique way they emit light – in a beam similar to a lighthouse beacon. As the star spins, the light sweeps past us, making it appear as if the star is pulsing. Neutron stars emit X-ray radiation, enabling the NICER technology to observe and record information about their structure, dynamics and energetics. The payload also includes a technology demonstration called the Station Explorer for X-ray Timing and Navigation Technology (SEXTANT) which will help researchers to develop a pulsar-based space navigation system. Pulsar navigation could work similarly to GPS on Earth, providing precise position and time for spacecraft throughout the solar system.The 2-in-1 mission launched on June 3, 2017 aboard SpaceX's eleventh contracted cargo resupply mission with NASA to the International Space Station. The payload arrived at the space station in the Dragon spacecraft, along with other cargo, on June 5, 2017. || ", "hits": 98 }, { "id": 12609, "url": "https://svs.gsfc.nasa.gov/12609/", "result_type": "B-Roll", "release_date": "2017-05-23T10:00:00-04:00", "title": "Webb Telescope Element Arrives at NASA JSC for Cryogenic Testing", "description": "Carried inside a U.S. Air Force C5M Super Galaxy aircraft, the James Webb Space Telescope arrives at Ellington Field Reserve Joint Base near Houston, Texas on May 5, 2017. The Webb Telescope team unloads the telescope and transports it by road to the NASA Johnson Space Center for cryogenic testing. During its transport from the NASA Goddard Space Flight Center to the NASA Johnson Space Center, the Webb Telescope is kept safe inside the Space Telescope Transport Air Rail and Sea (STTARS) container. At the NASA Johnson Space Center, engineers cleaned and moved STTARS into the Chamber A cleanroom where the Webb Telescope was unloaded and attached to a rollover fixture. || ", "hits": 51 }, { "id": 12587, "url": "https://svs.gsfc.nasa.gov/12587/", "result_type": "Produced Video", "release_date": "2017-05-02T13:00:00-04:00", "title": "Gigantic Wave Discovered in Perseus Galaxy Cluster", "description": "A wave spanning 200,000 light-years is rolling through the Perseus galaxy cluster, according to observations from NASA's Chandra X-ray Observatory coupled with a computer simulation. The simulation shows the gravitational disturbance resulting from the distant flyby of a galaxy cluster about a tenth the mass of the Perseus cluster. The event causes cooler gas at the heart of the Perseus cluster to form a vast expanding spiral, which ultimately forms giant waves lasting hundreds of millions of years at its periphery. Merger events like this are thought to occur as often as every three to four billion years in clusters like Perseus.Credit: NASA's Goddard Space Flight CenterMusic: \"The Undiscovered\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Perseus_Simulation_Final_Frame_print.jpg (1024x575) [47.6 KB] || Perseus_Simulation_Final_Frame.png (7342x4129) [4.0 MB] || Perseus_Simulation_Final_Frame_thm.png (80x40) [3.3 KB] || Perseus_Simulation_Final_Frame_searchweb.png (320x180) [39.3 KB] || 12587_Perseus_Wind_FINAL_VX-281959_appletv_subtitles.m4v (1280x720) [85.7 MB] || 12587_Perseus_Wind_1080.webm (1920x1080) [18.2 MB] || 12587_Perseus_Wind_FINAL_VX-281959_appletv.m4v (1280x720) [85.6 MB] || 12587_Perseus_Wind_1080.m4v (1920x1080) [160.3 MB] || 12587_Perseus_Wind_1080.mov (1920x1080) [241.7 MB] || 12587_Perseus_Wind_SRT_Caption.en_US.vtt [1.7 KB] || 12587_Perseus_Wind_SRT_Caption.en_US.srt [1.7 KB] || WMV_12587_Perseus_Wind_FINAL_VX-281959_HD.wmv (3840x2160) [154.8 MB] || 12587_Perseus_Wind.mp4 (3840x2160) [306.3 MB] || 12587_Perseus_Wind_Good_4k.mov (3840x2160) [468.4 MB] || 12587_Perseus_Wind_4K.m4v (3840x2160) [792.0 MB] || 12587_Perseus_Wind_FINAL_VX-281959_youtube_hq.mov (3840x2160) [1.2 GB] || 12587_Perseus_Wind_ProRes_3840x2160_2997.mov (3840x2160) [5.2 GB] || ", "hits": 99 }, { "id": 20268, "url": "https://svs.gsfc.nasa.gov/20268/", "result_type": "Animation", "release_date": "2017-04-26T00:00:00-04:00", "title": "NICER Lensing", "description": "The Neutron star Interior Composition Explorer (NICER) mission will study neutron stars, the densest known objects in the cosmos. These neutron star animations and graphics highlight some of their unique characteristics.For more information about NICER visit: nasa.gov/nicer. || ", "hits": 196 } ] }