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    "results": [
        {
            "id": 14818,
            "url": "https://svs.gsfc.nasa.gov/14818/",
            "result_type": "Produced Video",
            "release_date": "2025-09-26T12:00:00-04:00",
            "title": "Plunge: Behind the Scenes Creating NASA's Black Hole Visualization",
            "description": "Behind the scenes video about the Black Hole visualization from 2024",
            "hits": 314
        },
        {
            "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": 148
        },
        {
            "id": 14793,
            "url": "https://svs.gsfc.nasa.gov/14793/",
            "result_type": "Produced Video",
            "release_date": "2025-05-27T20:55:00-04:00",
            "title": "Black Holes Vertical Video",
            "description": "This page collects Astrophysics vertical videos with black-hole-related content",
            "hits": 1063
        },
        {
            "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": 110
        },
        {
            "id": 14737,
            "url": "https://svs.gsfc.nasa.gov/14737/",
            "result_type": "Produced Video",
            "release_date": "2024-12-17T09:00:00-05:00",
            "title": "Curious Universe Video Episode: The Mind-bending Math Inside Black Holes",
            "description": "This is a special video edition of NASA's podcast, Curious Universe.Black holes are mysterious, far away, and can bend the fabric of reality itself—but we're learning more about them all the time. Ronald Gamble, a NASA theoretical astrophysicist, uses math, computer coding, and a dash of creativity to peer inside some of the universe's most extreme objects. We'll explore what it would feel like to get pulled into a black hole and what people get wrong about black holes. And we'll answer questions from curious listeners, including, \"What would happen if a black hole ate nothing but magnetized material?\" || ",
            "hits": 85
        },
        {
            "id": 14619,
            "url": "https://svs.gsfc.nasa.gov/14619/",
            "result_type": "Produced Video",
            "release_date": "2024-07-17T10:00:00-04:00",
            "title": "Black Hole with Accretion Disk Visualization",
            "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole surrounded by a rapidly-rotating disk of gas and dust. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The speed at which material, in what is known as an accretion disk, orbits the black hole increases with proximity. The orbital speed of material closest to the event horizon approaches the speed of light. This produces an effect known as “relativistic doppler beaming” which enhances the brightness of material moving towards us along our line of sight, and correspondingly dims the brightness of material moving away.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.The light from the orbiting material is likewise distorted, making the flat accretion disk appear to bend completely around the black hole’s shadow and have the disk behind the black hole appear to be both above and below it. Yet despite these strange visual distortions that change with viewing angle, the accretion disk itself physically remains flat.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance of a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
            "hits": 1167
        },
        {
            "id": 14620,
            "url": "https://svs.gsfc.nasa.gov/14620/",
            "result_type": "Produced Video",
            "release_date": "2024-07-17T10:00:00-04:00",
            "title": "Isolated Black Hole Visualization",
            "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
            "hits": 1227
        },
        {
            "id": 14621,
            "url": "https://svs.gsfc.nasa.gov/14621/",
            "result_type": "Produced Video",
            "release_date": "2024-07-17T10:00:00-04:00",
            "title": "What is a black hole? Astro-Investigates Ep. 1",
            "description": "Black holes - what are they really? Learn this and more with “Astro-Investigates,” the video series that explores and explains big astrophysics topics with the help of NASA scientists. In this episode, you’ll hear from: Joanna Piotrowska - Astrophysicist at Caltech Varoujan Gorjian - NASA Research Astronomer Daniel Stern - NASA Astrophysicist Michele Vallisneri - NASA Theoretical physicist To learn more about black holes and NASA missions studying these mysterious objects, visit: [https://science.nasa.gov/universe/bla...](https://science.nasa.gov/universe/black-holes/) || JPL_Explainers_BH_FINAL.00096_print.jpg (1024x576) [76.6 KB] || JPL_Explainers_BH_FINAL.00096_searchweb.png (320x180) [61.4 KB] || JPL_Explainers_BH_FINAL.en_US.srt [9.2 KB] || JPL_Explainers_BH_FINAL.en_US.vtt [8.7 KB] || JPL_Explainers_BH_FINAL.mp4 (1920x1080) [812.8 MB] || JPL_Explainers_BH_FINAL_NoText.mp4 (1920x1080) [815.1 MB] || ",
            "hits": 222
        },
        {
            "id": 14576,
            "url": "https://svs.gsfc.nasa.gov/14576/",
            "result_type": "Visualization",
            "release_date": "2024-05-06T13:00:00-04:00",
            "title": "NASA Black Hole Visualization Takes Viewers Beyond the Brink",
            "description": "In this flight toward a supermassive black hole, labels highlight many of the fascinating features produced by the effects of general relativity along the way. This supercomputer visualization tracks a camera as it approaches, briefly orbits, and then crosses the event horizon — the point of no return — of a supersized black hole similar in mass to the one at the center of our galaxy.  Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. PowellMusic: “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music“Memories” from Digital Juice“Path Finder,” Eric Jacobsen [TONO] and Lorenzo Castellarin [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14576_BHPlunge_Explain_Still.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail_searchweb.png (180x320) [85.0 KB] || 14576_PageThumbnail_thm.png (80x40) [9.6 KB] || 14576_BHPlunge_Explainer_1080.mp4 (1920x1080) [319.5 MB] || 14576_BHPlunge_Explainer_Captions.en_US.srt [2.5 KB] || 14576_BHPlunge_Explainer_Captions.en_US.vtt [2.4 KB] || 14576_BHPlunge_Explainer_4k.mp4 (3840x2160) [1.5 GB] || 14576_BHPlunge_Explainer_4kYouTube.mp4 (3840x2160) [3.0 GB] || 14576_BHPlunge_Explainer_ProRes_3840x2160_2997.mov (3840x2160) [12.8 GB] || ",
            "hits": 2147
        },
        {
            "id": 14585,
            "url": "https://svs.gsfc.nasa.gov/14585/",
            "result_type": "Visualization",
            "release_date": "2024-05-06T00:00:00-04:00",
            "title": "Beyond the Brink: Tracking a Simulated Plunge into a Black Hole",
            "description": "In this all-sky view, the camera approaches a supermassive black hole weighing 4.3 million Suns. It is about 70 million miles (113 million kilometers) from the black hole’s event horizon, the boundary of no return. It’s moving inward at 19% the speed of light —  nearly 127 million mph (205 million kph). A flat, swirling cloud of hot, glowing gas called an accretion disk surrounds the black hole and serves as a visual reference during the fall, as do glowing structures called photon rings, which form closer to the black hole from light that has orbited it one or more times. A backdrop of the starry sky completes the scene.Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. Powell || 1_BH_Viz_20_rg_019c.jpg (8192x4096) [6.1 MB] || ",
            "hits": 470
        },
        {
            "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": 142
        },
        {
            "id": 14335,
            "url": "https://svs.gsfc.nasa.gov/14335/",
            "result_type": "Produced Video",
            "release_date": "2023-05-01T10:45:00-04:00",
            "title": "NASA Animation Sizes Up the Universe’s Biggest Black Holes",
            "description": "All monster black holes are not equal. Watch this video to see how they compare to each other and to our solar system. The black holes shown, which range from 100,000 to more than 60 billion times our Sun’s mass, are scaled according to the sizes of their shadows – a circular zone about twice the size of their event horizons. Only one of these colossal objects resides in our own galaxy, and it lies 26,000 light-years away. Smaller black holes are shown in bluish colors because their gas is expected to be hotter than that orbiting larger ones. Scientists think all of these objects shine most intensely in ultraviolet light. Credit: NASA's Goddard Space Flight Center Conceptual Image LabMusic: \"In the Stars\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SMBH_Scale_Still_1.jpg (3840x2160) [3.0 MB] || SMBH_Scale_Still_1_searchweb.png (180x320) [71.4 KB] || SMBH_Scale_Still_1_thm.png (80x40) [4.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.mp4 (1920x1080) [166.0 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080.mp4 (1920x1080) [102.7 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.webm (1920x1080) [13.3 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_ProRes_3840x2160_60.mov (3840x2160) [12.6 GB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_4k_Best.mp4 (3840x2160) [314.2 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.srt [2.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.vtt [2.2 KB] || ",
            "hits": 1608
        },
        {
            "id": 14130,
            "url": "https://svs.gsfc.nasa.gov/14130/",
            "result_type": "Produced Video",
            "release_date": "2022-04-07T14:00:00-04:00",
            "title": "Fermi Searches for Gravitational Waves From Monster Black Holes",
            "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ",
            "hits": 138
        },
        {
            "id": 14022,
            "url": "https://svs.gsfc.nasa.gov/14022/",
            "result_type": "Produced Video",
            "release_date": "2021-11-18T12:55:00-05:00",
            "title": "Hubble’s Grand Tour of the Outer Solar System",
            "description": "From its vantage point high above Earth’s atmosphere, NASA’s Hubble Space Telescope has completed its annual grand tour of the outer solar system – returning crisp images that are almost as good as earlier snapshots from interplanetary spacecraft. This is the realm of the giant planets— Jupiter, Saturn, Uranus, and Neptune – extending as far as 30 times the distance between Earth and the Sun.For more information, visit https://nasa.gov/hubble.Music Credits: “Crescent Moon” by Laetitia Frenod [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music || ",
            "hits": 57
        },
        {
            "id": 13834,
            "url": "https://svs.gsfc.nasa.gov/13834/",
            "result_type": "Produced Video",
            "release_date": "2021-04-12T10:00:00-04:00",
            "title": "NASA's Field Guide to Black Holes",
            "description": "Thinking about doing some black hole watching the next time you’re on an intergalactic vacation, but you’re not quite sure where to start? Well, look no further! This series of videos shows you everything you need to know. With topics ranging from basic black holes, to fancy black holes, to giant black holes and their companions, you’ll be more than ready for your next adventure.In addition to the videos, you can also download a printable guide that has even more information.Note: While these videos can be shared in their entirety without permission, their music has been licensed and may not be excised or remixed in other products. || ",
            "hits": 122
        },
        {
            "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": 128
        },
        {
            "id": 31021,
            "url": "https://svs.gsfc.nasa.gov/31021/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-02-11T18:00:00-05:00",
            "title": "Spiral Galaxy M106",
            "description": "This composite image of galaxy M106 focuses on its active center, where large amounts of gas are thought to be falling into and fueling a supermassive black hole. || STScI-H-M106_Legus_7910x6178_print.jpg (1024x799) [139.3 KB] || STScI-H-M106_Legus_7910x6178.png (7910x6178) [75.9 MB] || STScI-H-M106_Legus_7910x6178_searchweb.png (320x180) [83.3 KB] || STScI-H-M106_Legus_7910x6178_thm.png (80x40) [6.7 KB] || STScI-H-M106_Legus_7910x6178.png.dzi (7910x6178) [178 bytes] || STScI-H-M106_Legus_7910x6178.tif (7910x6178) [100.1 MB] || STScI-H-M106_Legus_7910x6178.png_files (1x1) [4.0 KB] || ",
            "hits": 69
        },
        {
            "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": 120
        },
        {
            "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": 253
        },
        {
            "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": 291
        },
        {
            "id": 12539,
            "url": "https://svs.gsfc.nasa.gov/12539/",
            "result_type": "Produced Video",
            "release_date": "2017-03-23T13:00:00-04:00",
            "title": "Hubble Detects a Rogue Supermassive Black Hole",
            "description": "The Hubble Space Telescope captured an image of a quasar named 3C 186 that is offset from the center of its galaxy. Astronomers hypothesize that this supermassive black hole was jettisoned from the center of its galaxy by the recoil from gravitational waves produced by the merging of two supermassive black holes. Read the press release here - https://www.nasa.gov/feature/goddard/2017/feature/gravitational-wave-kicks-monster-black-hole-out-of-galactic-coreDownload the Hubble images here - http://hubblesite.org/news_release/news/2017-12Read the science paper here - http://imgsrc.hubblesite.org/hvi/uploads/science_paper/file_attachment/231/3c186.pdf || ",
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        {
            "id": 12499,
            "url": "https://svs.gsfc.nasa.gov/12499/",
            "result_type": "Produced Video",
            "release_date": "2017-03-20T14:00:00-04:00",
            "title": "Swift Charts a Star's 'Death Spiral' into Black Hole",
            "description": "This animation illustrates how debris from a tidally disrupted star collides with itself, creating shock waves that emit ultraviolet and optical light far from the black hole. According to Swift observations of ASASSN-14li, these clumps took about a month to fall back to the black hole, where they produced changes in the X-ray emission that correlated with the earlier UV and optical changes.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || TD_Shocks_Still_print.jpg (1024x576) [115.2 KB] || TD_Shocks_Still.png (3840x2160) [32.6 MB] || TD_Shocks_Still.jpg (3840x2160) [922.7 KB] || TD_Shocks_Still_searchweb.png (320x180) [59.5 KB] || TD_Shocks_Still_thm.png (80x40) [4.8 KB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_1080.mov (1920x1080) [50.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_youtube_hq.mov (1920x1080) [25.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Good_1080.m4v (1920x1080) [44.4 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.m4v (960x540) [10.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_HD.wmv (1920x1080) [6.9 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.webm (960x540) [3.8 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv_subtitles.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_SRT_Captions.en_US.srt [509 bytes] || 12499_Tidal_Disruption_SRT_Captions.en_US.vtt [522 bytes] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_ProRes_1920x1080_2997.mov (1920x1080) [591.1 MB] || ",
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}