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    "results": [
        {
            "id": 12028,
            "url": "https://svs.gsfc.nasa.gov/12028/",
            "result_type": "Produced Video",
            "release_date": "2015-10-26T10:00:00-04:00",
            "title": "Suzaku Finds Common Chemical Composition at Largest Cosmic Scales",
            "description": "Suzaku mapped iron, magnesium, silicon and sulfur in four directions all across the Virgo Galaxy Cluster for the first time. The northern arm of the survey (top) extends 5 million light-years from M87 (center), the massive galaxy at the cluster's heart. Ratios of these elements are constant throughout the cluster, which means they were mixed well early in cosmic history. The dashed circle shows what astronomers call the virial radius, the boundary where gas clouds are just entering the cluster. Some prominent members of the cluster are labeled as well. The background image is part of the all-sky X-ray survey acquired by the German ROSAT satellite. The blue box at center indicates the area shown in the visible light image.    Credit: A. Simionescu (JAXA) and Hans Boehringer (MPE) || Suzaku_probes_Virgo_Cluster_labeled_print.jpg (1024x1259) [574.7 KB] || Suzaku_probes_Virgo_Cluster_labeled.jpg (2218x2729) [1.6 MB] || Suzaku_probes_Virgo_Cluster_labeled_web.png (320x393) [122.4 KB] || Suzaku_crop_searchweb.png (320x180) [64.0 KB] || Suzaku_crop_thm.png (80x40) [6.7 KB] || ",
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        {
            "id": 11821,
            "url": "https://svs.gsfc.nasa.gov/11821/",
            "result_type": "Produced Video",
            "release_date": "2015-03-25T14:00:00-04:00",
            "title": "Suzaku, Herschel Link a Black-hole 'Wind' to a Galactic Gush",
            "description": "This movie illustrates how black-hole feedback works in quasars. Dense gas and dust in the center simultaneously fuels the black hole and shrouds it from view. The black-hole wind propels large-scale outflows of cold gas and powers a shock wave that clears gas and dust from the central galaxy.Video credit: NASA's Goddard Space Flight Center || Suzaku_Quasar_Wind_STILL.png (1920x1080) [8.1 MB] || Suzaku_Quasar_Wind_STILL_print.jpg (1024x576) [41.8 KB] || Suzaku_Quasar_Wind_STILL_searchweb.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_web.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_thm.png (80x40) [7.9 KB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.webm (960x540) [3.3 MB] || 11821_Suzaku_Quasar_Wind_FINAL.mov (1920x1080) [333.5 MB] || 1920x1080_16x9_30p (1920x1080) [32.0 KB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Best_1920x1080_2997.mov (1920x1080) [295.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Good_1920x1080_2997.mov (1920x1080) [36.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL-MPEG4_1920X1080_2997.mp4 (1920x1080) [13.0 MB] || 11821_Suzaku_Quasar_Wind_FINAL_1280x720.wmv (1280x720) [13.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.m4v (960x540) [13.6 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_lg.m4v (640x360) [5.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_sm.mp4 (320x240) [2.6 MB] || ",
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        },
        {
            "id": 11725,
            "url": "https://svs.gsfc.nasa.gov/11725/",
            "result_type": "Produced Video",
            "release_date": "2015-01-07T13:15:00-05:00",
            "title": "NASA Missions Take an Unparalleled Look into Superstar Eta Carinae",
            "description": "Explore Eta Carinae from the inside out with the help of supercomputer simulations and data from NASA satellites and ground-based observatories. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Eta_Car_Density_XY_R10_R100_STILL_1920.jpg (1920x1080) [804.4 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_print.jpg (1024x576) [52.0 KB] || Eta_Car_Density_XY_R10_R100_STILL.jpg (4928x2772) [874.1 KB] || Eta_Car_Density_XY_R10_R100_STILL.png (4928x2772) [36.6 MB] || Eta_Car_Density_XY_R10_R100_STILL_1920_web.jpg (320x180) [13.1 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_searchweb.png (320x180) [55.9 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_thm.png (80x40) [8.0 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920.tiff (1920x1080) [11.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.webm (960x540) [30.5 MB] || G2015-001_Eta_Car_Binary_Final_ipod_lg.m4v (640x360) [43.2 MB] || G2015-001_Eta_Car_Binary.en_US.vtt [5.2 KB] || G2015-001_Eta_Car_Binary.en_US.srt [5.2 KB] || G2015-001_Eta_Car_Binary_Final_ipod_sm.mp4 (320x240) [22.8 MB] || G2015-001_Eta_Car_Binary_Final_appletv_subtitles.m4v (960x540) [103.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.m4v (960x540) [104.0 MB] || G2015-001_Eta_Car_Binary_Final_1280x720.wmv (1280x720) [107.6 MB] || 11725_Eta_Car_Binary2_MPEG4_1920X1080_2997.mp4 (1920x1080) [116.9 MB] || 11725_Eta_Car_Binary2_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || 11725_Eta_Car_Binary2_H264_Best_1920x1080_2997.mov (1920x1080) [2.6 GB] || 11725_Eta_Car_Binary2_H264_Good_1920x1080_2997.mov (1920x1080) [506.2 MB] || Eta_Car_Density_XY_R10_R100_STILL.tiff (4928x2772) [104.2 MB] || ",
            "hits": 98
        },
        {
            "id": 11388,
            "url": "https://svs.gsfc.nasa.gov/11388/",
            "result_type": "Produced Video",
            "release_date": "2013-10-30T14:00:00-04:00",
            "title": "Suzaku Study Points to Early Cosmic 'Seeding'",
            "description": "Most of the universe's heavy elements, including the iron in our blood, formed early in cosmic history and spread throughout the universe, according to a new study of the Perseus Galaxy Cluster using Japan's Suzaku satellite. Between 2009 and 2011, researchers from the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly run by Stanford University and the Department of Energy's SLAC National Accelerator Laboratory in California, used Suzaku's unique capabilities to map the distribution of iron throughout the Perseus Galaxy Cluster. What they found is remarkable: Across the cluster, which spans more than 11 million light-years of space, the concentration of X-ray-emitting iron is essentially uniform in all directions.This tells astronomers that iron — and by extension other heavy elements — already was widely dispersed throughout the universe when the cluster began to form. Explaining this helps scientists better understand what the universe was like 10 to 12 billion years ago, a time when rapid-fire supernova explosions were common and black holes were especially active. || ",
            "hits": 200
        },
        {
            "id": 10874,
            "url": "https://svs.gsfc.nasa.gov/10874/",
            "result_type": "Produced Video",
            "release_date": "2013-04-17T16:00:00-04:00",
            "title": "Science in the Media Press Conference",
            "description": "This video supports the Science in the Media curriculum module, which culminates with students playing the role of reporters viewing this simulated press conference and writing a story about it. The findings discussed in the video are actual results from the Suzaku satellite.Science in the Media curriculum module here. || ",
            "hits": 51
        },
        {
            "id": 10991,
            "url": "https://svs.gsfc.nasa.gov/10991/",
            "result_type": "Produced Video",
            "release_date": "2012-07-03T08:00:00-04:00",
            "title": "A Young Star Flaunts its X-ray Spots",
            "description": "Using combined data from a trio of orbiting X-ray telescopes, including NASA's Chandra X-ray Observatory and the Japan-led Suzaku satellite, astronomers have obtained a rare glimpse of the powerful phenomena that accompany a still-forming star. A new study based on these observations indicates that intense magnetic fields drive torrents of gas into the stellar surface, where they heat large areas to millions of degrees. X-rays emitted by these hot spots betray the newborn star's rapid rotation.Astronomers first took notice of the young star, known as V1647 Orionis, in January 2004, near the peak of an outburst. The eruption had brightened the star so much that it illuminated a conical patch of dust now known as McNeil's Nebula. Both the star and the nebula are located about 1,300 light-years away in the constellation Orion. Astronomers quickly determined that V1647 Ori was a protostar, a stellar infant still partly swaddled in its birth cloud. Protostars have not yet developed the energy-generating capabilities of a normal star such as the sun, which fuses hydrogen into helium in its core. For V1647 Ori, that stage lies millions of years in the future. Until then, the protostar shines from the heat energy released by the gas that continues to fall onto it, much of which originates in a rotating circumstellar disk.The mass of V1647 Ori is likely only about 80 percent of the sun's, but its low density bloats it to nearly five times the sun's size. Infrared measurements show that most of the star's surface has a temperature around 6,400 degrees Fahrenheit (3,500 C), or about a third cooler than the sun's. Yet during outbursts, the protostar's X-ray brightness increases by 100 times and the temperature of its X-ray-emitting regions reaches about 90 million F (50 million C). The team found strong similarities among 11 separate X-ray light curves based on data from Chandra, Suzaku and the European Space Agency's XMM-Newton satellites. These similarities allowed them to identify cyclic X-ray variations establishing that the star spins once each day. V1647 Ori is among the youngest stars whose spin rates have been determined using an X-ray-based technique.The cyclic X-ray changes represent the appearance and disappearance of hot regions on the star that rotate in and out of view. The model that best agrees with the observations, say the researchers, involves two hot spots of unequal brightness located on opposite sides of the star. Both spots are thought to be pancake-shaped areas about the size of the sun, but the more southerly spot is about five times brighter. || ",
            "hits": 51
        },
        {
            "id": 10533,
            "url": "https://svs.gsfc.nasa.gov/10533/",
            "result_type": "Produced Video",
            "release_date": "2010-01-12T00:00:00-05:00",
            "title": "Suzaku (formerly Astro-E2) Spacecraft",
            "description": "An animation depicting the Suzaku/Astro-E2 spacecraft on orbit. Suzaku maintains a low Earth orbit while it observes X-rays from the Universe. The satellite was developed at the Japanese Institute of Space and Astronautical Science (ISAS, which is part of the Japan Aerospace Exploration Agency, JAXA.) in collaboration with Japanese and US institutions including NASA. || ",
            "hits": 41
        },
        {
            "id": 10536,
            "url": "https://svs.gsfc.nasa.gov/10536/",
            "result_type": "Produced Video",
            "release_date": "2009-12-02T06:00:00-05:00",
            "title": "Suzaku: Intergalactic Prospector",
            "description": "Recently astronomers used the Suzaku orbiting X-ray observatory, operated jointly by NASA and the Japanese space agency, to discover the largest known reservoir of rare metals in the universe.  Suzaku detected the elements chromium and manganese while observing the central region of the Perseus galaxy cluster. The metallic atoms are part of the hot gas, or \"intergalactic medium,\" that lies between galaxies. Exploding stars, or supernovas, forge the heavy elements. The supernovas also create vast outflows, called superwinds. These galactic gusts transport heavy elements into the intergalactic void. || ",
            "hits": 33
        }
    ]
}