{
    "count": 6,
    "next": null,
    "previous": null,
    "results": [
        {
            "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": 220
        },
        {
            "id": 14719,
            "url": "https://svs.gsfc.nasa.gov/14719/",
            "result_type": "Visualization",
            "release_date": "2024-11-13T09:00:00-05:00",
            "title": "Swift Studies Gas-Churning Monster Black Holes",
            "description": "Watch as a gas cloud encounters two supermassive black holes. The complex interplay of gravitational and frictional forces causes the cloud to condense and heat. Some of the gas is ejected from the system with each orbit of the black holes.Credit: F. Goicovic et al. 2016Music: \"Forgotten Fortunes,\" Magnum Opus [ASCAP] , Universal Production MusicComplete transcript available. || Sim_Video_Still.jpg (3840x2160) [744.6 KB] || Sim_Video_Still_searchweb.png (320x180) [37.6 KB] || Sim_Video_Still_thm.png (80x40) [3.4 KB] || BH_Binary_TD_Sim_1080_Final.mp4 (1920x1080) [38.5 MB] || BH_Binary_TD_Sim_4k_Final.mp4 (3840x2160) [45.5 MB] || BH_Binary_TD_Sim_4k_Final_best.mp4 (3840x2160) [67.9 MB] || 14719_BinaryBHTDE_Captions.en_US.srt [57 bytes] || 14719_BinaryBHTDE_Captions.en_US.vtt [67 bytes] || BH_Binary_TD_Sim_4k_Final_ProRes.mov (3840x2160) [1.5 GB] || ",
            "hits": 214
        },
        {
            "id": 14149,
            "url": "https://svs.gsfc.nasa.gov/14149/",
            "result_type": "Produced Video",
            "release_date": "2022-05-02T10:45:00-04:00",
            "title": "NASA's Black Hole Orrery",
            "description": "Learn more about the best-known black hole systems in our galaxy and its neighbor, the Large Magellanic Cloud. This visualization presents 22 X-ray binary systems that host confirmed black holes at the same scale, with their orbits sped up by about 22,000 times. The view of each system reflects how we see it from Earth. Star colors ranging from blue-white to reddish represent temperatures from 5 times hotter to 45% cooler than our Sun. In most of these systems, a stream of matter from the star forms an accretion disk around the black hole. In others, like the famous system called Cygnus X-1, the star produces a hefty outflow that is partly swept up by the black hole’s gravity to form the disk. The accretion disks use a different color scheme because they sport even higher temperatures than the stars. The largest disk shown, belonging to a binary called GRS 1915, spans a distance greater than that separating Mercury from our Sun. The black holes themselves are shown larger than in reality using spheres scaled to reflect their masses.Credit: NASA's Goddard Space Flight Center and Scientific Visualization StudioMusic: \"Event Horizon\" from Gravity. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Black_Hole_Orrery_Still.jpg (3840x2160) [321.9 KB] || Black_Hole_Orrery_Still_searchweb.png (320x180) [25.6 KB] || Black_Hole_Orrery_Still_thm.png (80x40) [4.1 KB] || 14149_Black_Hole_Orrery_FINAL_1080.mp4 (1920x1080) [118.8 MB] || 14149_Black_Hole_Orrery_FINAL_1080.webm (1920x1080) [12.4 MB] || 14149_Black_Hole_Orrery_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || 14149_Black_Hole_Orrery_FINAL_4k_Best.mp4 (3840x2160) [379.2 MB] || 14149_Black_Hole_Orrery_FINAL_4k.mp4 (3840x2160) [176.7 MB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.srt [1.9 KB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.vtt [1.9 KB] || ",
            "hits": 323
        },
        {
            "id": 20367,
            "url": "https://svs.gsfc.nasa.gov/20367/",
            "result_type": "Animation",
            "release_date": "2022-04-28T00:00:00-04:00",
            "title": "Gravitational Wave",
            "description": "Two black holes orbit around each other and generate space-time ripples called gravitational waves in this animation. As the black holes get closer, the waves increase in frequency. Eventually, the event horizons merge into a peanut-shaped object, generating one very high-frequency wave. Within a rotation, the black holes merge completely. One lower-frequency wave, called the ring down, ripples out after the merger.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || A_Gravitational_Wave_ProRes.00450_print.jpg (1024x576) [119.9 KB] || A_Gravitational_Wave_ProRes.00450_searchweb.png (320x180) [78.6 KB] || A_Gravitational_Wave_ProRes.00450_thm.png (80x40) [6.8 KB] || A_Gravitational_Wave_ProRes.mov (3840x2160) [2.2 GB] || A_Gravitational_Wave_h264.mp4 (3840x2160) [40.4 MB] || A_Gravitational_Wave (3840x2160) [128.0 KB] || A_Gravitational_Wave_ProRes.webm (3840x2160) [15.0 MB] || ",
            "hits": 274
        },
        {
            "id": 13831,
            "url": "https://svs.gsfc.nasa.gov/13831/",
            "result_type": "Produced Video",
            "release_date": "2021-04-15T13:00:00-04:00",
            "title": "NASA Visualization Probes the Doubly Warped World of Binary Black Holes",
            "description": "Explore how the extreme gravity of two orbiting supermassive black holes distorts our view. In this visualization, disks of bright, hot, churning gas encircle both black holes, shown in red and blue to better track the light source. The red disk orbits the larger black hole, which weighs 200 million times the mass of our Sun, while its smaller blue companion weighs half as much. Zooming into each black hole reveals multiple, increasingly warped images of its partner. Watch to learn more. Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman and Brian P. PowellMusic: \"Gravitational Field\" from Orbit.  Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Supermassive_BlackHole_Binary_Still.jpg (3840x2160) [726.7 KB] || Supermassive_BlackHole_Binary_Still_searchweb.png (320x180) [18.9 KB] || Supermassive_BlackHole_Binary_Still_thm.png (80x40) [2.5 KB] || 13831_BlackHoleBinary_Simulation_1080.webm (1920x1080) [23.8 MB] || 13831_BlackHoleBinary_Simulation_1080.mp4 (1920x1080) [234.7 MB] || 13831_BlackHoleBinary_Simulation_4k.mp4 (3840x2160) [348.3 MB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4 (3840x2160) [936.6 MB] || 13831_BlackHoleBinary_Simulation_ProRes_3840x2160_30.mov (3840x2160) [4.1 GB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4.hwshow [137 bytes] || ",
            "hits": 299
        },
        {
            "id": 10507,
            "url": "https://svs.gsfc.nasa.gov/10507/",
            "result_type": "Produced Video",
            "release_date": "2009-10-28T01:45:00-04:00",
            "title": "Gamma-Rays from High-Mass X-Ray Binaries",
            "description": "In its first year, NASA's Fermi Gamma-ray Space Telescope discovered GeV (billions of electron volts) intensity variations revealing orbital motion in high-mass X-ray binaries (HMXBs). These are systems where a compact companion, such as a neutron star or a black hole, rapidly orbits a hot, young, massive star. The first examples include LSI +61 303, which sports a 26-day orbital period, and LS 5039 (3.9 days). This animation shows such a system. When the compact object lies far from its host star, TeV (trillions of electron volts) gamma-rays (white) are seen by ground-based gamma-ray observatories. But, as the object plunges closer to the star, the TeV emission is quenched and GeV emission turns on. Interactions by accelerated particles from the compact source with gas encircling the star — or in some systems, the star's light itself — is thought to be responsible for this change. || ",
            "hits": 68
        }
    ]
}