{
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    "results": [
        {
            "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": 142
        },
        {
            "id": 30967,
            "url": "https://svs.gsfc.nasa.gov/30967/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-06-11T10:00:00-04:00",
            "title": "30 Doradus: A Massive Star-Forming Region",
            "description": "This animation of the active star-forming region 30 Doradus showcases Hubble's entire wavelength range, from ultraviolet to infrared. || STScI-H-30_Dor_1x-1920x1080.00001_print.jpg (1024x576) [150.5 KB] || STScI-H-30_Dor_1x-1920x1080.00001_searchweb.png (320x180) [89.3 KB] || STScI-H-30_Dor_1x-1920x1080.00001_thm.png (80x40) [6.0 KB] || STScI-H-30_Dor_1x-1280x720.mp4 (1280x720) [2.9 MB] || STScI-H-30_Dor_1x-1920x1080.mp4 (1920x1080) [5.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-30_Dor_1x-1920x1080.webm (1920x1080) [1.8 MB] || STScI-H-30_Dor_1x-640x360.mp4 (640x360) [1.0 MB] || STScI-H-30_Dor_1x-3840x2160.mp4 (3840x2160) [4.9 MB] || STScI-H-30_Dor_1x-H265-3840x2160.mp4 (3840x2160) [2.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 72
        },
        {
            "id": 30773,
            "url": "https://svs.gsfc.nasa.gov/30773/",
            "result_type": "Hyperwall Visual",
            "release_date": "2016-04-21T00:00:00-04:00",
            "title": "The Bubble Nebula (NGC 7635) from Hubble",
            "description": "To mark Hubble's 26th birthday, astronomers captured this balloon-like sphere of gas. || bubble-hst-7857x7462_print.jpg (1024x972) [193.4 KB] || bubble-hst-7857x7462.png (7857x7462) [73.8 MB] || bubble-hst-3412x3240.png (3412x3240) [16.3 MB] || bubble-hst-7857x7462_searchweb.png (320x180) [97.1 KB] || bubble-hst-7857x7462_thm.png (80x40) [19.5 KB] || the-bubble-nebula-ngc-7635-from-hubble.hwshow [302 bytes] || ",
            "hits": 49
        },
        {
            "id": 1,
            "url": "https://svs.gsfc.nasa.gov/1/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Tidal Streams in Massive X-ray Binary Systems",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own.  The high luminosity of the massive star drives a strong wind from its surface.  The neutron star crashes through this wind at over 300 kilometers per second.  The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star.  In this simulation, the tidal distortion of the primary star and the resultant tidal stream is shown.  The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 86
        },
        {
            "id": 2,
            "url": "https://svs.gsfc.nasa.gov/2/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Tidal Streams in Massive X-ray Binary Systems: Neutron Star Close-up",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own.  The high luminosity of the massive star drives a strong wind from its surface.  The neutron star crashes through this wind at over 300 kilometers per second.  The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star.  In this simulation, the tidal distortion of the primary star and the resultant tidal stream is shown.  The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 57
        },
        {
            "id": 4,
            "url": "https://svs.gsfc.nasa.gov/4/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Stellar Wind Disruption by an Orbiting Neutron Star: Low X-Ray Luminosity",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own.  The high luminosity of the massive star drives a strong wind from its surface.  The neutron star crashes through this wind at over 300 kilometers per second.  The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star.  This simulation, in the reference frame of the neutron star, shows conditions of low X-ray luminosity. in which there is a small accretion radius, a slight asymmetry, and short timescales for variability.The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 64
        },
        {
            "id": 5,
            "url": "https://svs.gsfc.nasa.gov/5/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Stellar Wind Disruption by an Orbiting Neutron Star: Moderate X-Ray Luminosity",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own.  The high luminosity of the massive star drives a strong wind from its surface.  The neutron star crashes through this wind at over 300 kilometers per second.  The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star.  This simulation, in the reference frame of the neutron star, shows conditions of low X-ray luminosity. in which there is a large accretion radius, significant asymmetry, and long timescales for variability.The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 54
        },
        {
            "id": 6,
            "url": "https://svs.gsfc.nasa.gov/6/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Stellar Wind Disruption by an Orbiting Neutron Star: High X-Ray Luminosity",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own. The high luminosity of the massive star drives a strong wind from its surface. The neutron star crashes through this wind at over 300 kilometers per second. The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star. This simulation, in the reference frame of the neutron star, shows conditions of high X-ray luminosity, in which there is a weak bow shock, no oscillation, and a large photoionization wake. The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 53
        },
        {
            "id": 7,
            "url": "https://svs.gsfc.nasa.gov/7/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Stellar Wind Disruption by an Orbiting Neutron Star: Neutron Star Close-up",
            "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own.  The high luminosity of the massive star drives a strong wind from its surface.  The neutron star crashes through this wind at over 300 kilometers per second.  The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star.  The large scale structure seen in the accretion wake is powered by the release of gravitational potential energy near the surface of the neutron star.The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ",
            "hits": 58
        }
    ]
}