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            "description": "Astronomers are gearing up for high-energy fireworks coming in early 2018, when a stellar remnant the size of a city meets one of the brightest stars in our galaxy. The cosmic light show will occur when a pulsar discovered by NASA's Fermi Gamma-ray Space Telescope swings by its companion star. Scientists plan a global campaign to watch the event from radio wavelengths to the highest-energy gamma rays detectable.<br><br>The pulsar, known as J2032+4127 (J2032 for short), is the crushed core of a massive star that exploded as a supernova. It is a magnetized ball about 12 miles across, or about the size of Washington, weighing almost twice the sun's mass and spinning seven times a second. J2032's rapid spin and strong magnetic field together produce a lighthouse-like beam detectable when it sweeps our way. <br><br>The pulsar orbits a massive companion named MT91 213. Classified as a Be star, the companion is 15 times the mass of the sun and shines 10,000 times brighter. Be stars drive strong outflows, called stellar winds, and are embedded in large disks of gas and dust. <br><br>Following an elongated orbit lasting about 25 years, the pulsar passes closest to its partner once each circuit. Whipping around its companion in early 2018, the pulsar will plunge through the surrounding disk and trigger astrophysical fireworks. It will serve as a probe to help astronomers measure the massive star's gravity, magnetic field, stellar wind and disk properties.<br><br>Read more at <a href='http://www.nasa.gov/feature/goddard/astronomers-predict-fireworks-from-rare-stellar-encounter-in-2018'>http://www.nasa.gov/feature/goddard/astronomers-predict-fireworks-from-rare-stellar-encounter-in-2018</a>",
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            "page_type": "Animation",
            "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] || ",
            "release_date": "2015-07-02T10:00:00-04:00",
            "update_date": "2023-05-03T13:49:37.433299-04:00",
            "main_image": {
                "id": 442238,
                "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020200/a020225/Cam1_00312_print.jpg",
                "filename": "Cam1_00312_print.jpg",
                "media_type": "Image",
                "alt_text": "Binary Pulsar J2032 animation ",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 10798,
            "url": "https://svs.gsfc.nasa.gov/10798/",
            "page_type": "Produced Video",
            "title": "Stellar Odd Couple Makes Striking Flares",
            "description": "Every 3.4 years, pulsar B1259-63 dives twice through the gas disk surrounding the massive blue star it orbits. With each pass, it produces gamma rays. During the most recent event, NASA's Fermi Gamma-ray Space Telescope observed that the pulsar's gamma-ray flare was much more intense the second time it plunged through the disk. Astronomers don't yet know why.For the B1259 binary animation, go here. || ",
            "release_date": "2011-06-29T10:00:00-04:00",
            "update_date": "2023-05-03T13:53:43.940435-04:00",
            "main_image": {
                "id": 484924,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010798/GR_Disc0177.jpg",
                "filename": "GR_Disc0177.jpg",
                "media_type": "Image",
                "alt_text": "Short narrated video about B1259.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here.",
                "width": 1280,
                "height": 720,
                "pixels": 921600
            }
        }
    ],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}