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        {
            "id": 13272,
            "url": "https://svs.gsfc.nasa.gov/13272/",
            "result_type": "Produced Video",
            "release_date": "2019-08-09T00:00:00-04:00",
            "title": "Fermi and Gamma Rays: A Cartoon Look",
            "description": "NASA’s Fermi Gamma-ray Space Telescope detects gamma rays — the highest-energy form of light — often produced by objects like pulsars, the remnants of exploding stars and active galaxies powered by supermassive black holes. The satellite does not look for aliens, extraterrestrial life or anything of the sort. If aliens were to pass by the Fermi spacecraft, they would just slip by undetected. Unless, of course, that alien ship was powered by processes that left behind traces of gamma rays.Credit: NASA's Goddard Space Flight Center/Gabby Garcia || Alien_00121.jpg (1920x1080) [395.7 KB] || Alien_00121_print.jpg (1024x576) [143.1 KB] || Alien_00121_searchweb.png (320x180) [41.7 KB] || Alien_00121_thm.png (80x40) [4.4 KB] || Fermi_Alien_Animation_ProRes_1920x1080_24.mov (1920x1080) [76.6 MB] || 1920x1080_16x9_24p (1920x1080) [8.0 KB] || Fermi_Alien_Animation_1080.mp4 (1920x1080) [5.3 MB] || Fermi_Alien_Animation_ProRes_1920x1080_24.webm (1920x1080) [966.5 KB] || ",
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        {
            "id": 4714,
            "url": "https://svs.gsfc.nasa.gov/4714/",
            "result_type": "Visualization",
            "release_date": "2019-05-13T11:00:00-04:00",
            "title": "Lee Lincoln Scarp at the Apollo 17 Landing Site",
            "description": "An animated view of Lee Lincoln scarp from above and from near ground level. This visualization is created from Lunar Reconnaissance Orbiter photographs and elevation mapping. The scarp is at the western end of the Taurus-Littrow valley, landing site of Apollo 17, and was explored by the astronauts on their second moonwalk. || scarp.0510_print.jpg (1024x576) [101.8 KB] || scarp.0510_searchweb.png (320x180) [63.7 KB] || scarp.0510_thm.png (80x40) [5.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || scarp_1080p30.mp4 (1920x1080) [15.7 MB] || scarp_720p30.mp4 (1280x720) [8.7 MB] || scarp_720p30.webm (1280x720) [3.5 MB] || scarp_1080p30_prores.mov (1920x1080) [657.9 MB] || scarp_360p30.mp4 (640x360) [3.3 MB] || scarp_1080p30.mp4.hwshow || ",
            "hits": 93
        },
        {
            "id": 13095,
            "url": "https://svs.gsfc.nasa.gov/13095/",
            "result_type": "Produced Video",
            "release_date": "2018-11-19T12:00:00-05:00",
            "title": "Bright Spots",
            "description": "Curious bright spots mark the surface of Ceres. || PIA20182_16x9_1024x576.jpg (1024x576) [112.7 KB] || PIA20182_16x9_searchweb.png (320x180) [62.1 KB] || PIA20182_16x9_web.png (320x180) [62.1 KB] || PIA20182_16x9_thm.png (80x40) [5.6 KB] || PIA20182_16x9.tif (1920x1080) [1.8 MB] || ",
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        {
            "id": 20231,
            "url": "https://svs.gsfc.nasa.gov/20231/",
            "result_type": "Animation",
            "release_date": "2018-05-24T13:00:00-04:00",
            "title": "Mars Organic Molecule Analyzer: Animations",
            "description": "MOMA uses ultraviolet laser pulses to release and ionize organic compounds captured within crushed Martian surface and near-surface materials. Because each laser pulse lasts less than two billionths of a second, this process effectively ionizes more heat-resistant materials than those accessed by traditional oven-heating (pyrolysis) methods. Pulsed laser processing preserves weak molecular bonds, and enables the identification of organic compounds even in the presence of highly reactive perchlorates commonly found in Martian surface materials. || MOMAposterFull.jpg (1920x1080) [130.9 KB] || MOMAposterFull_print.jpg (1024x576) [73.3 KB] || MOMAposterFull_searchweb.png (320x180) [36.8 KB] || MOMAposterFull_web.png (320x180) [36.8 KB] || MOMAposterFull_thm.png (80x40) [3.7 KB] || ldms (1920x1080) [0 Item(s)] || MOMA-LDMS_h264.mp4 (1920x1080) [91.5 MB] || MOMA-LDMS_1080p60.mp4 (1920x1080) [24.4 MB] || MOMA-LDMS_1080p60.webm (1920x1080) [8.3 MB] || MOMA-LDMS.mov (1920x1080) [2.1 GB] || Moma-LDMS.hwshow [67 bytes] || ",
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        },
        {
            "id": 12360,
            "url": "https://svs.gsfc.nasa.gov/12360/",
            "result_type": "Animation",
            "release_date": "2016-09-06T10:00:00-04:00",
            "title": "To Bennu and Back",
            "description": "NASA's latest New Frontiers mission, OSIRIS-REx, will venture to a near-Earth asteroid to discover clues about the unique resources asteroids hold, processes that affect asteroids' orbital paths and their potential for impacting Earth, and the origins of life in the solar system. In addition, OSIRIS-REx will collect a sample from the surface of the asteroid and return it to Earth for generations of scientists to study and analyze, making this the first American asteroid sample return mission and the largest sample returned from an extraterrestrial body since Apollo. OSIRIS-REx's launch window opens September 8, 2016. This is the journey #ToBennuAndBack. || ",
            "hits": 41
        },
        {
            "id": 11688,
            "url": "https://svs.gsfc.nasa.gov/11688/",
            "result_type": "Produced Video",
            "release_date": "2014-12-04T11:00:00-05:00",
            "title": "The Fountains of Enceladus",
            "description": "Enceladus, a tiny moon orbiting Saturn, is one of the solar system's most active objects. More than 100 distinct jets of water burst through four massive cracks near the moon's south pole. The water simultaneously freezes and boils when it hits the cold vacuum of space. Hundreds of miles above, the jets merge into a single plume of ice particles. Larger particles fall back, while smaller, faster ones escape to form Saturn’s gossamer E ring. NASA’s Cassini spacecraft has snapped hundreds of images of the geysers during several close flybys of Enceladus. Researchers believe gravitational force from Saturn alternately compresses and stretches the moon in its oblong orbit. Models predict this same tidal energy warms a sea of liquid water beneath the ice, providing a source for the geysers and a potential abode for extraterrestrial life. Watch the video to see close-ups of the moon and its icy plumes taken by Cassini. || ",
            "hits": 517
        },
        {
            "id": 10822,
            "url": "https://svs.gsfc.nasa.gov/10822/",
            "result_type": "Produced Video",
            "release_date": "2011-09-15T00:00:00-04:00",
            "title": "Does DNA Have Extraterrestrial Origins?",
            "description": "If terms like adenine and guanine bring back unpleasant memories of Genetics 101 here's one reason to give the words a second thought: A team of scientists has discovered that these and other DNA building blocks can form in outer space and have been deposited on Earth's surface by meteorites. To reach this eye-opening conclusion, researchers ground up and analyzed a set of twelve meteorites collected from Antarctica and Australia. Within them, the scientists found a treasure trove of molecules that may have played a key role in allowing early forms of life to form. Adenine, which helps make up the rungs of DNA's spiraling, ladder-like structure, turned up in eleven of the meteorites. Guanine, another key building block of DNA, was present in eight. Two of the twelve meteorites also contained something extraordinary—exotic molecules that are so rare on Earth that they prove the DNA building blocks must have formed in outer space. The discovery lends support to the theory that a kit of pre-made parts from meteorites or a comet might have kick-started life on Earth. Learn more about the breakthrough in the video below. || ",
            "hits": 1092
        },
        {
            "id": 10698,
            "url": "https://svs.gsfc.nasa.gov/10698/",
            "result_type": "Produced Video",
            "release_date": "2011-01-20T09:00:00-05:00",
            "title": "NASA's Swift Finds 'Missing' Active Galaxies",
            "description": "Most large galaxies contain a giant central black hole. In an active galaxy, matter falling toward the supermassive black hole powers high-energy emissions so intense that two classes of active galaxies, quasars and blazars, rank as the most luminous objects in the universe. Thick clouds of dust and gas near the central black hole screens out ultraviolet, optical and low-energy (or soft) X-ray light. Although there are many different types of active galaxy, astronomers explain the different observed properties based on how the galaxy angles into our line of sight. We view the brightest ones nearly face on, but as the angle increases, the surrounding ring of gas and dust absorbs increasing amounts of the black hole's emissions. || ",
            "hits": 157
        },
        {
            "id": 2947,
            "url": "https://svs.gsfc.nasa.gov/2947/",
            "result_type": "Visualization",
            "release_date": "2006-05-15T12:00:00-04:00",
            "title": "Europa's Synthetic Subsurface Heat Transport (Version 1)",
            "description": "Under Europa's icy surface are vast extraterrestrial oceans.  This conceptual animation depicts simulated heat transport of these subsurface oceans.  Please note that the simulated heat transport in this animation is only conceptual and a more accurate representation can be found at animation #2946. || ",
            "hits": 37
        }
    ]
}