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            "id": 14847,
            "url": "https://svs.gsfc.nasa.gov/14847/",
            "result_type": "Produced Video",
            "release_date": "2025-06-02T11:00:00-04:00",
            "title": "100,000 Computer Simulations Reveal Milky Way's Fate",
            "description": "For decades, astronomers believed that one thing was as certain as death and taxes: the Milky Way and our neighboring Andromeda galaxy were on a crash course… destined to collide in less than 5 billion years.That galactic smash-up would spark massive star formation, scatter stars like cosmic billiard balls, and possibly throw our Sun into a whole new orbit.But now… that future may not be so certain.For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerVideo Credits:Milky Way TimelapseStock Footage Provided By Pond5/lovemushroomArtist Rendition of Gaia SpacecraftESAArtist’s animation of the Sun becoming a red giantESA/Hubble (M. Kornmesser & L. L. Christensen)Milky Way and Andromeda Collision SimulationVisualization Credit: NASA, ESA, and F. Summers (STScI) Simulation Credit: NASA, ESA, G. Besla (Columbia University), and R. van der Marel (STScI)Music Credit:\"Lost to Eternity\" by Timothy James Cornick [PRS] via BBC Production Music [PRS] and Universal Production Music || ",
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        {
            "id": 13412,
            "url": "https://svs.gsfc.nasa.gov/13412/",
            "result_type": "Produced Video",
            "release_date": "2019-10-28T09:55:00-04:00",
            "title": "Hubble's Scary New Halloween Image",
            "description": "NASA’s Hubble Space Telescope has unveiled a spooky new image staring out from the depths of the cosmos. The new image reveals the twin galaxies AM 2026-424 — a pair of interacting galaxies that may foreshadow our Milky Way’s own frightening fate.For more information, visit https://nasa.gov/hubble.Music Credits:\"Bad and Spooky\" by Brett Engel [ASCAP], Universal Production Music“Scream Dreams” by  Matthew Harris [PRS], Universal Production Music || ",
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        {
            "id": 30958,
            "url": "https://svs.gsfc.nasa.gov/30958/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-25T11:00:00-04:00",
            "title": "A Rose of Galaxies: Interacting Galaxies Arp 273",
            "description": "Known as Arp 273, these two galaxies have been distorted by their mutual gravitaional pull into a shape resembling a long-stemmed rose. || arp273-example_frame-1920x1080.png (1920x1080) [331.0 KB] || arp273-example_frame-1920x1080_print.jpg (1024x576) [25.1 KB] || arp273-example_frame-1920x1080_searchweb.png (320x180) [17.4 KB] || arp273-example_frame-1920x1080_thm.png (80x40) [2.4 KB] || arp273-1920x1080p30.mov (1920x1080) [34.7 MB] || arp273-1920x1080.webm (1920x1080) [15.1 MB] || arp273-1920x1080.mp4 (1920x1080) [34.9 MB] || arp273-1920x1080.wmv (1920x1080) [4.0 MB] || a-rose-of-galaxies-interacting-galaxies-arp-273.hwshow [234 bytes] || ",
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        },
        {
            "id": 30955,
            "url": "https://svs.gsfc.nasa.gov/30955/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-23T15:00:00-04:00",
            "title": "Crash of the Titans: Milky Way & Andromeda Collision",
            "description": "This scientific visualization of a computer simulation depicts the joint evolution of the Milky Way and Andromeda galaxies over the next several billion years and features the inevitable massive collision. || mw_m31_m33_a-example_frame2-1920x1080.png (1920x1080) [224.3 KB] || mw_m31_m33_a-example_frame2-1920x1080_print.jpg (1024x576) [40.3 KB] || mw_m31_m33_a-example_frame2-1920x1080_searchweb.png (320x180) [22.9 KB] || mw_m31_m33_a-example_frame2-1920x1080_thm.png (80x40) [2.0 KB] || mw_m31_m33_a-b-1920x1080.m4v (1920x1080) [59.1 MB] || mw_m31_m33_a-b-1920x1080.wmv (1920x1080) [60.1 MB] || mw_m31_m33_a-b-1920x1080.webm (1920x1080) [59.4 MB] || mw_m31_m33_a-b-3840x2160.mp4 (3840x2160) [369.1 MB] || crash-of-the-titans-milky-way-andromeda-collision.hwshow [319 bytes] || crash-of-the-titans-milky-way-andromeda-collision-hd.hwshow [322 bytes] || ",
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        {
            "id": 11965,
            "url": "https://svs.gsfc.nasa.gov/11965/",
            "result_type": "Produced Video",
            "release_date": "2015-07-27T15:00:00-04:00",
            "title": "Close Approach",
            "description": "Video about close calls on orbit. || Close_Approach_youtube_hq_print.jpg (1024x576) [95.1 KB] || Close_Approach_youtube_hq_searchweb.png (320x180) [67.5 KB] || Close_Approach_youtube_hq_thm.png (80x40) [4.9 KB] || Close_Approach_prores.mov (1280x720) [3.1 GB] || Close_Approach_youtube_hq.mov (1280x720) [364.1 MB] || Close_Approach_appletv.m4v (1280x720) [106.0 MB] || Close_Approach.webm (960x540) [89.3 MB] || Close_Approach_1280x720.wmv (1280x720) [103.0 MB] || Close_Approach_ipod_sm.mp4 (320x240) [38.7 MB] || ",
            "hits": 39
        },
        {
            "id": 10747,
            "url": "https://svs.gsfc.nasa.gov/10747/",
            "result_type": "Produced Video",
            "release_date": "2011-04-28T09:00:00-04:00",
            "title": "Swift and Hubble Probe an Asteroid Crash",
            "description": "Late last year, astronomers noticed that an asteroid named Scheila had unexpectedly brightened and it was sporting short-lived plumes. Data from NASA's Swift satellite and Hubble Space Telescope show that these changes likely occurred after Scheila was struck by a much smaller asteroid. On Dec. 11, 2010, images from the University of Arizona's Catalina Sky Survey, a project of NASA's Near Earth Object Observations Program, revealed the Scheila to be twice as bright as expected and immersed in a faint comet-like glow. Looking through the survey's archived images, astronomers inferred the outburst began between Nov. 11 and Dec. 3. Three days after the outburst was announced, Swift's Ultraviolet/Optical Telescope (UVOT) captured multiple images and a spectrum of the asteroid. Ultraviolet sunlight breaks up the gas molecules surrounding comets; water, for example, is transformed into hydroxyl (OH) and hydrogen (H). But none of the emissions most commonly identified in comets — such as hydroxyl or cyanogen (CN) — show up in the UVOT spectrum. The absence of gas around Scheila led the Swift team to reject scenarios where exposed ice accounted for the activity.Images show the asteroid was flanked in the north by a bright dust plume and in the south by a fainter one. The dual plumes formed as small dust particles excavated by the impact were pushed away from the asteroid by sunlight. Hubble observed the asteroid's fading dust cloud on Dec. 27, 2010, and Jan. 4, 2011.The two teams found the observations were best explained by a collision with a small asteroid impacting Scheila's surface at an angle of less than 30 degrees, leaving a crater 1,000 feet across. Laboratory experiments show a more direct strike probably wouldn't have produced two distinct dust plumes. The researchers estimated the crash ejected more than 660,000 tons of dust—equivalent to nearly twice the mass of the Empire State Building.For the collision animation go to #10759. || ",
            "hits": 43
        },
        {
            "id": 10759,
            "url": "https://svs.gsfc.nasa.gov/10759/",
            "result_type": "Produced Video",
            "release_date": "2011-04-28T09:00:00-04:00",
            "title": "(596) Scheila Asteroid Collision Animation",
            "description": "Late last year, astronomers noticed that an asteroid named Scheila had brightened unexpectedly and was sporting a short-lived tail. Now, data from NASA's Swift satellite and Hubble Space Telescope show that these changes likely occurred after Scheila was struck by a much smaller asteroid. || ",
            "hits": 44
        },
        {
            "id": 10740,
            "url": "https://svs.gsfc.nasa.gov/10740/",
            "result_type": "Produced Video",
            "release_date": "2011-04-07T09:00:00-04:00",
            "title": "When Neutron Stars Collide",
            "description": "Armed with state-of-the-art supercomputer models, scientists have shown that colliding neutron stars can produce the energetic jet required for a gamma-ray burst. Earlier simulations demonstrated that mergers could make black holes. Others had shown that the high-speed particle jets needed to make a gamma-ray burst would continue if placed in the swirling wreckage of a recent merger. Now, the simulations reveal the middle step of the process—how the merging stars' magnetic field organizes itself into outwardly directed components capable of forming a jet. The Damiana supercomputer at Germany's Max Planck Institute for Gravitational Physics needed six weeks to reveal the details of a process that unfolds in just 35 thousandths of a second—less than the blink of an eye.For the researchers' website, with more video and stills of their simulations, go here. || ",
            "hits": 472
        },
        {
            "id": 10658,
            "url": "https://svs.gsfc.nasa.gov/10658/",
            "result_type": "Produced Video",
            "release_date": "2010-10-28T00:00:00-04:00",
            "title": "Webb Science Feature - Colliding Galaxies",
            "description": "Deep surveys by the James Webb Space Telescope will capture the full panorama of galaxy evolution, from the earliest dwarf galaxies that formed to the familiar galaxies we see today. The Webb Telescope will help us understand how the shape, structure and chemical content of galaxies change over the sweep of cosmic history. || ",
            "hits": 47
        }
    ]
}