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        {
            "id": 13692,
            "url": "https://svs.gsfc.nasa.gov/13692/",
            "result_type": "Produced Video",
            "release_date": "2020-08-17T10:00:00-04:00",
            "title": "Ocean Worlds Social Videos",
            "description": "Europa Plumes || Europa_thumb.jpg (1920x1080) [84.7 KB] || Europa_13692.01157_searchweb.png (320x180) [28.7 KB] || Europa_13692.01157_thm.png (80x40) [3.4 KB] || Europa_13692.mp4 (1920x1080) [49.4 MB] || Europa_13692_facebook_720.mp4 (1280x720) [54.2 MB] || Europa_13692_twitter_720.mp4 (1280x720) [9.0 MB] || Europa_13692.webm (960x540) [18.6 MB] || Europa_captioned.en_US.srt [981 bytes] || Europa_captioned.en_US.vtt [945 bytes] || ",
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        },
        {
            "id": 13693,
            "url": "https://svs.gsfc.nasa.gov/13693/",
            "result_type": "Produced Video",
            "release_date": "2020-08-17T00:00:00-04:00",
            "title": "Ocean Worlds: The Search for Life",
            "description": "NASA scientists discuss the search for life on the ocean worlds of our solar system and beyond.Watch this video on the NASA Goddard YouTube channel.Universal Production Music: “Superluminal” by Lee Groves and Peter George Marett; “Earthrise,” “Prism Lights,” and “Uncertain Ahead” by Ben Niblett and Jon Cotton; “Infinite Sky” and “Human Architecture” by Andy Blythe and Marten Joustra; “Imagine If” by Paul WernerComplete transcript available. || 13693OceanWorldsThumbnail2_print.jpg (1024x576) [269.6 KB] || 13693OceanWorldsThumbnail2.jpg (1920x1080) [763.8 KB] || 13693OceanWorldsThumbnail2_searchweb.png (180x320) [88.2 KB] || 13693OceanWorldsThumbnail2_thm.png (80x40) [7.9 KB] || 13693_Ocean_Worlds_GSFC_YouTube.webm (1920x1080) [103.5 MB] || 13693OceanWorldsCaptionsV3.en_US.srt [19.9 KB] || 13693OceanWorldsCaptionsV3.en_US.vtt [19.0 KB] || 13693_Ocean_Worlds_GSFC_Facebook.mp4 (1920x1080) [1.1 GB] || 13693_Ocean_Worlds_GSFC_YouTube.mp4 (1920x1080) [2.9 GB] || 13693_Ocean_Worlds_GSFC_MASTER.mov (1920x1080) [11.8 GB] || ",
            "hits": 252
        },
        {
            "id": 4777,
            "url": "https://svs.gsfc.nasa.gov/4777/",
            "result_type": "Visualization",
            "release_date": "2020-01-23T09:00:00-05:00",
            "title": "Proxima Centauri b Climate Model Scenarios",
            "description": "Proxima b as a water planet with no land and no ocean circulation. Notice the large ocean on Proxima b's starside. || thermo.0026__cameraShape1_beauty.2000_print.jpg (1024x576) [279.0 KB] || Thermo (3840x2160) [0 Item(s)] || thermo.0026__cameraShape1_beauty.webm (3840x2160) [54.6 MB] || thermo.0026__cameraShape1_beauty.mp4 (3840x2160) [671.5 MB] || ",
            "hits": 379
        },
        {
            "id": 4778,
            "url": "https://svs.gsfc.nasa.gov/4778/",
            "result_type": "Visualization",
            "release_date": "2020-01-23T09:00:00-05:00",
            "title": "Earth Versus Proxima Centauri b Rotation Rates",
            "description": "Earth spins on its axis every 24 hours. Proxima B is tidally locked and therefore always faces it's star, much like how the moon has one side that always faces Earth. || near_evb.00333_print.jpg (1024x576) [88.2 KB] || near_evb.00333_searchweb.png (320x180) [55.2 KB] || near_evb.00333_thm.png (80x40) [5.5 KB] || Composite (1920x1080) [0 Item(s)] || near_evb_1080p30_2.webm (1920x1080) [72.6 MB] || near_evb_1080p30_2.mp4 (1920x1080) [367.4 MB] || ",
            "hits": 387
        },
        {
            "id": 4779,
            "url": "https://svs.gsfc.nasa.gov/4779/",
            "result_type": "Visualization",
            "release_date": "2020-01-23T09:00:00-05:00",
            "title": "Orbital Differences Between Earth and Proxima Centauri b",
            "description": "This data visualization compares the relative distances and speeds of Proxima B's orbit to the Earth's orbit. Proxima B rapidly orbits its sun every 11.2 days. || evb_orbits_comp.0333_print.jpg (1024x576) [78.7 KB] || evb_orbits_comp.0333_searchweb.png (320x180) [48.9 KB] || evb_orbits_comp.0333_thm.png (80x40) [4.7 KB] || evb_orbits_comp_1080p30.mp4 (1920x1080) [5.3 MB] || Composite (1920x1080) [0 Item(s)] || evb_orbits_comp_1080p30.webm (1920x1080) [1.8 MB] || ",
            "hits": 567
        },
        {
            "id": 4780,
            "url": "https://svs.gsfc.nasa.gov/4780/",
            "result_type": "Visualization",
            "release_date": "2020-01-23T09:00:00-05:00",
            "title": "Where is Proxima B?",
            "description": "This animation shows where Proxima Centauri B can be located in the Southern sky. It starts with a view of Earth and the camera moves to a view of the Southern sky, revealing the star constellations. Proxima Centauri is then highlighted and we quickly fly to it. Eventually, the planet unwraps into a flat plane showing a potential planetary surface without clouds. || prox_b_intro.0460_print.jpg (1024x576) [89.7 KB] || prox_b_intro.0460_searchweb.png (320x180) [78.9 KB] || prox_b_intro.0460_thm.png (80x40) [5.1 KB] || prox_b_intro_1080p30.mp4 (1920x1080) [30.3 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || prox_b_intro_1080p30.webm (1920x1080) [6.3 MB] || ",
            "hits": 402
        },
        {
            "id": 13518,
            "url": "https://svs.gsfc.nasa.gov/13518/",
            "result_type": "Produced Video",
            "release_date": "2020-01-23T00:00:00-05:00",
            "title": "Earth Climate Models Bring Exoplanet To Life",
            "description": "Music: \"Machine Learning\" by Jon Cotton and Ben Niblett; \"No Wave\" by Julien Vignon; \"The Missing Star\" by Matthew Charles Gilbert Davidson; all from Universal Production MusicComplete transcript available. || ProxCenB_Thumbnail_print.jpg (1024x576) [315.6 KB] || ProxCenB_Thumbnail.png (3840x2160) [18.9 MB] || ProxCenB_Thumbnail_searchweb.png (320x180) [145.7 KB] || ProxCenB_Thumbnail_thm.png (80x40) [7.6 KB] || ProxCenB.mp4 (1920x1080) [369.8 MB] || ProxCenB.webm (1920x1080) [48.9 MB] || ProxCenB.en_US.srt [7.3 KB] || ProxCenB.en_US.vtt [7.3 KB] || ProxCenB.mov (3840x2160) [28.4 GB] || ",
            "hits": 62
        },
        {
            "id": 12804,
            "url": "https://svs.gsfc.nasa.gov/12804/",
            "result_type": "Produced Video",
            "release_date": "2018-03-15T07:00:00-04:00",
            "title": "SEEC AAS Hyperwall Presentation January 2018",
            "description": "This animation illustrates the Kepler-186 system, whose fifth world is the first Earth-sized exoplanet to be found orbiting within its star’s habitable zone. The animation closes with a simulated image from a coronagraph showing how such a planet might appear when directly imaged.Credit: NASA/Ames/SETI Institute/JPL-Caltech || Kepler186_Coronagraph_Combined_LongPause.01270_print.jpg (1024x576) [35.2 KB] || Kepler186_Coronagraph_Combined_LongPause.webm (1920x1080) [14.0 MB] || Kepler186_Coronagraph_Combined_LongPause.mov (1920x1080) [180.7 MB] || ",
            "hits": 49
        },
        {
            "id": 11898,
            "url": "https://svs.gsfc.nasa.gov/11898/",
            "result_type": "Produced Video",
            "release_date": "2015-06-12T12:30:00-04:00",
            "title": "Hubble Detects \"Sunscreen\" Layer on Distant Planet",
            "description": "ANIMATION Using NASA’s Hubble Telescope, scientists detected a stratosphere on the planet WASP-33b. A stratosphere occurs when molecules in the atmosphere absorb ultraviolet and visible light from the star. This absorption warms the stratosphere and acts as a kind of sunscreen layer for the planet below.Watch this video on YouTube. || CoolHotAll3av8_print.jpg (1024x576) [49.2 KB] || CoolHotAll3av8_searchweb.png (320x180) [48.2 KB] || CoolHotAll3av8_thm.png (80x40) [4.6 KB] || CoolHotAll3av8.mp4 (1920x1080) [46.7 MB] || CoolHotAll3av8sm.mp4 (1280x720) [16.4 MB] || CoolHotAll3av8sm.webm (1280x720) [2.2 MB] || ",
            "hits": 54
        },
        {
            "id": 11443,
            "url": "https://svs.gsfc.nasa.gov/11443/",
            "result_type": "Produced Video",
            "release_date": "2014-01-21T00:00:00-05:00",
            "title": "Water Worlds",
            "description": "Earth, the blue planet, is our idea of a water world. But a planet doesn't have to be earthlike to have water. Using NASA's Hubble Space Telescope, scientists found faint signals of water in the atmospheres of five distant planets. All five—HD 209458b, WASP-12b, WASP-17b, WASP-19b and XO-1b—are a type of exoplanet known as hot Jupiters, massive worlds that orbit very close to their stars. Although the planets were quite hazy, the researchers could tell that two of them had stronger water signals than the other three. Being able to compare planets this way is a key step in figuring out why some worlds wind up with plentiful water yet others don't. Watch the video to see an animation of a hot Jupiter orbiting its star. || ",
            "hits": 166
        },
        {
            "id": 11413,
            "url": "https://svs.gsfc.nasa.gov/11413/",
            "result_type": "Produced Video",
            "release_date": "2013-12-17T00:00:00-05:00",
            "title": "Exploring Outer Worlds",
            "description": "Since the early 1990s, astronomers have known that distant planets orbit stars light-years from Earth. Although most of these alien worlds, called exoplanets, are too far away to be imaged directly, scientists have made detailed observations of their size and composition. One method of study involves watching a planet as it transits its host star. By measuring how the brightness and color of a star changes when a planet crosses in front of its disk, astronomers can indirectly determine the mass of the planet and the proximity of its orbit. Similar measurements can provide other key information, like the chemical makeup of a planet's atmosphere. Watch the video to learn more. || ",
            "hits": 33
        },
        {
            "id": 11428,
            "url": "https://svs.gsfc.nasa.gov/11428/",
            "result_type": "Produced Video",
            "release_date": "2013-12-03T12:00:00-05:00",
            "title": "Alien Atmospheres",
            "description": "Since the early 1990's, astronomers have known that extrasolar planets, or \"exoplanets,\" orbit stars light-years beyond our own solar system. Although most exoplanets are too distant to be directly imaged, detailed studies have been made of their size, composition, and even atmospheric makeup - but how? By observing periodic variations in the parent star's brightness and color, astronomers can indirectly determine an exoplanet's distance from its star, its size, and its mass. But to truly understand an exoplanet astronomers must study its atmosphere, and they do so by splitting apart the parent star's light during a planetary transit. || ",
            "hits": 256
        }
    ]
}