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        {
            "id": 12078,
            "url": "https://svs.gsfc.nasa.gov/12078/",
            "result_type": "Produced Video",
            "release_date": "2015-12-31T11:00:00-05:00",
            "title": "Cosmic Fireworks",
            "description": "Astronomers predict high-energy explosions from a rare stellar encounter. || c-1024.jpg (1024x576) [99.4 KB] || c-1024_print.jpg (1024x576) [107.3 KB] || c-1024_searchweb.png (320x180) [69.4 KB] || c-1024_web.png (320x180) [69.4 KB] || c-1024_thm.png (80x40) [11.1 KB] || ",
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            "release_date": "2015-07-02T10:00:00-04:00",
            "title": "Astronomers Predict Cosmic Light Show from 2018 Stellar Encounter",
            "description": "Coming attraction: Astronomers are expecting high-energy explosions when pulsar J2032 swings around its massive companion star in early 2018. The pulsar will plunge through a disk of gas and dust surrounding the star, triggering cosmic fireworks. Scientists are planning a global campaign to watch the event across the spectrum, from radio waves to gamma rays. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Binary_Pulsar_Still.png (1920x1080) [2.0 MB] || Binary_Pulsar_Still_print.jpg (1024x576) [88.4 KB] || Binary_Pulsar_Still_searchweb.png (320x180) [74.7 KB] || Binary_Pulsar_Still_thm.png (80x40) [8.1 KB] || 11895_Fermi_Binary_Pulsar_.mov (1920x1080) [1.5 GB] || 11895_Fermi_Binary_Pulsar_-H264_Best_1920x1080_29.97.mov (1920x1080) [523.1 MB] || 11895_Fermi_Binary_Pulsar_-H264_Good_1080_29.97.mov (1920x1080) [77.1 MB] || YOUTUBE_HQ_G2015-051_Fermi_Binary_Pulsar_FINAL_VX-171746_youtube_hq.mov (1280x720) [174.9 MB] || 11895_Fermi_Binary_Pulsar_MPEG4_1920X1080_2997.mp4 (1920x1080) [53.1 MB] || WMV_G2015-051_Fermi_Binary_Pulsar_FINAL_VX-171746_1280x720.wmv (1280x720) [48.3 MB] || APPLE_TV_G2015-051_Fermi_Binary_Pulsar_FINAL_VX-171746_appletv.m4v (1280x720) [71.5 MB] || 11895_Fermi_Binary_Pulsar_.webm (1920x1080) [14.4 MB] || APPLE_TV_G2015-051_Fermi_Binary_Pulsar_FINAL_VX-171746_appletv_subtitles.m4v (1280x720) [71.6 MB] || 11895_Fermi_Binary_Pulsar_SRT_Captions.en_US.srt [1.8 KB] || 11895_Fermi_Binary_Pulsar_SRT_Captions.en_US.vtt [1.8 KB] || ",
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            "id": 20225,
            "url": "https://svs.gsfc.nasa.gov/20225/",
            "result_type": "Animation",
            "release_date": "2015-07-02T10:00:00-04:00",
            "title": "Binary Pulsar J2032 animation",
            "description": "Binary Pulsar J2032 animation || BinaryPulsar.png (1920x1080) [2.0 MB] || Cam1_00312_print.jpg (1024x576) [65.8 KB] || Cam1_00312_searchweb.png (320x180) [68.9 KB] || Cam1_00312_thm.png (80x40) [5.7 KB] || BinaryPulsar_1080p60.webm (1920x1080) [2.1 MB] || 1920x1080_16x9_60p (1920x1080) [32.0 KB] || BinaryPulsar_1080p60.mp4 (1920x1080) [11.6 MB] || Bin_pulsar_442.mov (1920x1080) [534.0 MB] || Bin_pulsar_H264.mov (1920x1080) [315.4 MB] || ",
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        {
            "id": 11216,
            "url": "https://svs.gsfc.nasa.gov/11216/",
            "result_type": "Produced Video",
            "release_date": "2014-02-20T11:00:00-05:00",
            "title": "Black Widow Pulsars Consume Their Mates",
            "description": "Black widow spiders and their Australian cousins, known as redbacks, are notorious for an unsettling tendency to kill and devour their male partners. Astronomers have noted similar behavior among two rare breeds of binary system that contain rapidly spinning neutron stars, also known as pulsars. The essential features of black widow and redback binaries are that they place a normal but very low-mass star in close proximity to a millisecond pulsar, which has disastrous consequences for the star. Black widow systems contain stars that are both physically smaller and of much lower mass than those found in redbacks.So far, astronomers have found at least 18 black widows and nine redbacks within the Milky Way, and additional members of each class have been discovered within the dense globular star clusters that orbit our galaxy. One black widow system, named PSR J1311-3430 and discovered in 2012, sets the record for the tightest orbit of its class and contains one of the heaviest neutron stars known. The pulsar's featherweight companion, which is only a dozen or so times the mass of Jupiter and just 60 percent of its size, completes an orbit every 93 minutes – less time than it takes to watch most movies. The side of the star facing the pulsar is heated to more than 21,000 degrees Fahrenheit (nearly 12,000 C), or more than twice as hot as the sun's surface. Recent studies allow a range of values extending down to 2 solar masses for the pulsar, making it one of the most massive neutron stars known. Watch the video to learn more about this system and its discovery from some of the scientists involved. || ",
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        },
        {
            "id": 10520,
            "url": "https://svs.gsfc.nasa.gov/10520/",
            "result_type": "Produced Video",
            "release_date": "2010-01-05T14:30:00-05:00",
            "title": "New Millisecond Radio Pulsars Found in Fermi LAT Unidentified Sources",
            "description": "Radio searches netted 17 new millisecond pulsars by examining the Fermi Gamma-ray Space Telescope's list of unidentified sources. Colored circles indicate the positions of the new pulsars on the Fermi one-year all-sky map. || ",
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