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    "results": [
        {
            "id": 13184,
            "url": "https://svs.gsfc.nasa.gov/13184/",
            "result_type": "Produced Video",
            "release_date": "2019-04-29T00:00:00-04:00",
            "title": "Goddard at 60",
            "description": "On July 29, 1958, President Eisenhower signed the National Aeronautics and Space Act, establishing the National Aeronautics and Space Administration. When it began operations on October 1, 1958, NASA consisted mainly of the four laboratories and some 80 employees of the government's 46-year-old research agency, the National Advisory Committee for Aeronautics (NACA). Goddard Space Flight Center was established on May 1, 1959 as NASA's first space flight center.In celebration of its 60th year, we look back at the innovations and scientific impacts the women and men of Goddard have made throughout its history. || ",
            "hits": 106
        },
        {
            "id": 11760,
            "url": "https://svs.gsfc.nasa.gov/11760/",
            "result_type": "Produced Video",
            "release_date": "2015-03-31T11:00:00-04:00",
            "title": "A Once-Blue Planet",
            "description": "NASA research suggests an ocean once covered the surface of Mars. || c-1280.jpg (1280x720) [229.4 KB] || c-1024.jpg (1024x576) [157.9 KB] || c-1024_print.jpg (1024x576) [150.3 KB] || c-1024_searchweb.png (320x180) [80.7 KB] || c-1024_print_thm.png (80x40) [18.5 KB] || ",
            "hits": 121
        },
        {
            "id": 11796,
            "url": "https://svs.gsfc.nasa.gov/11796/",
            "result_type": "Produced Video",
            "release_date": "2015-03-05T14:00:00-05:00",
            "title": "Mars’ Ancient Ocean",
            "description": "NASA planetary scientists Geronimo Villanueva and Michael Mumma discuss their findings regarding the ancient ocean of Mars.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Mars_Ocean_still_print.jpg (1024x576) [113.5 KB] || Mars_Ocean_still.png (1920x1080) [3.0 MB] || Mars_Ocean_still_web.jpg (320x180) [16.0 KB] || Mars_Ocean_still_searchweb.png (320x180) [86.4 KB] || Mars_Ocean_still_thm.png (80x40) [8.2 KB] || G2015-011_MarsOcean_MASTER_appletv.webm (960x540) [30.9 MB] || G2015-011_MarsOcean_MASTER_ipod_lg.m4v (640x360) [46.0 MB] || G2015-011_MarsOcean_MASTER_ipod_sm.mp4 (320x240) [24.8 MB] || G2015-011_MarsOcean_MASTER.en_US.srt [4.4 KB] || G2015-011_MarsOcean_MASTER.en_US.vtt [4.4 KB] || G2015-011_MarsOcean_MASTER_prores.mov (1280x720) [4.0 GB] || G2015-011_MarsOcean_MASTER_youtube_hq.mov (1280x720) [187.8 MB] || G2015-011_MarsOcean_MASTER_appletv.m4v (960x540) [116.1 MB] || G2015-011_MarsOcean_MASTER_1280x720.wmv (1280x720) [136.4 MB] || G2015-011_MarsOcean_MASTER_appletv_subtitles.m4v (960x540) [116.0 MB] || G2015-011_MarsOcean_MASTER_nasaportal.mov (640x360) [112.8 MB] || ",
            "hits": 765
        },
        {
            "id": 11693,
            "url": "https://svs.gsfc.nasa.gov/11693/",
            "result_type": "Produced Video",
            "release_date": "2014-12-16T11:00:00-05:00",
            "title": "How Comets Are Born",
            "description": "Comets are small, icy objects that circle the sun. They can be thought of as floating time capsules, preserving a chemical record of the early solar system. Astronomers believe comets materialized more than 4.5 billion years ago from the dust and gas of the protoplanetary disk, a donut-shaped cloud of debris surrounding our newborn star. On the fringes of the disk, far from the sun’s heat, fine grains of dust coated with frozen gases and water ice began clumping together. Over time, clumps of dust assembled into ice-rich rocks, which later evolved into the mile-sized bodies that we observe today traveling among and far beyond the planets. Watch the video to see an artist’s interpretation of the birth of a comet. || ",
            "hits": 357
        },
        {
            "id": 10615,
            "url": "https://svs.gsfc.nasa.gov/10615/",
            "result_type": "Produced Video",
            "release_date": "2010-07-13T00:00:00-04:00",
            "title": "The Goddard Center for Astrobiology",
            "description": "Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe. The NASA Goddard Center for Astrobiology and the NASA Astrobiology Institute focus on this amazing field through research, experimentation, and work with scientists from all over the world. Learn more about some of the people at the Goddard Center for Astrobiology below! || ",
            "hits": 38
        },
        {
            "id": 3574,
            "url": "https://svs.gsfc.nasa.gov/3574/",
            "result_type": "Visualization",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "Methane Plume on Mars",
            "description": "The first definitive detection of methane in the atmosphere of Mars indicates the planet is alive in the sense that it still has geologic activity powered by heat from its interior, according to a team of NASA and university scientists. The team used spectrometer instruments attached to several telescopes to detect plumes of methane that were emitted from specific sites during the warmer seasons - spring and summer. Though nothing conclusive can yet be determined, it is possible that the detected methane was either produced by geologic processes such as the oxidation of iron (serpentinization) or by microscopic Martian life below the planet's surface. The methane released today could be produced currently, or it could be ancient methane trapped in ice 'cages' called clathrates or as gas below a sub-surface ice layer. || ",
            "hits": 61
        },
        {
            "id": 10358,
            "url": "https://svs.gsfc.nasa.gov/10358/",
            "result_type": "Produced Video",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "Geochemical Creation of Methane",
            "description": "Conceptual animation depicting how geochemical processes during the course of Mars' history may have produced the methane plumes now seen in Mars' atmosphere. Here, through a process called serpentinization, methane is generated as part of a reaction involving the conversion of liquid water (seen seeping into the planet's crust), iron oxide, and carbon dioxide energized by the planet's internal heat into serpentine minerals. || methane_geo_mpgLG00377_print.jpg (1024x576) [85.2 KB] || methane_geo_mpgLG_web.png (320x180) [184.0 KB] || methane_geo_mpgLG_thm.png (80x40) [16.0 KB] || methane_geo_h264fullres.webmhd.webm (960x540) [3.0 MB] || methane_geo_h264fullres.mov (1280x720) [12.3 MB] || methane_geo_prores.mov (1280x720) [535.3 MB] || methane_geo_YouTube.mov (1280x720) [5.8 MB] || methane_geo_ipodLG.m4v (640x360) [3.5 MB] || methane_geo_mpgLG.mpg (640x360) [4.7 MB] || methane_geo_ipodSM.m4v (320x180) [1.5 MB] || methane_geo_mp4SM.mp4 (320x240) [665.5 KB] || methane_geo_mpgSM.mpg (512x288) [3.1 MB] || ",
            "hits": 38
        },
        {
            "id": 10359,
            "url": "https://svs.gsfc.nasa.gov/10359/",
            "result_type": "Produced Video",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "Biological Creation of Methane",
            "description": "Conceptual animation depicting how biological organisms (shown as oval-shaped translucent structures) living beneath the surface of Mars may have produced methane (shown as blue spheres). || methane_bio_mpgLG00327_print.jpg (1024x576) [88.5 KB] || methane_bio_mpgLG_web.png (320x180) [202.1 KB] || methane_bio_mpgLG_thm.png (80x40) [16.4 KB] || methane_bio_h264fullres.webmhd.webm (960x540) [4.5 MB] || methane_bio_h264fullres.mov (1280x720) [12.3 MB] || methane_bio_prores.mov (1280x720) [505.6 MB] || methane_bio_ipodLG.m4v (640x360) [3.7 MB] || methane_bio_mpgLG.mpg (640x360) [4.6 MB] || methane_bio_ipodSM.m4v (320x180) [1.4 MB] || methane_bio_mp4SM.mp4 (320x240) [1.1 MB] || methane_bio_mpgSM.mpg (512x288) [3.1 MB] || ",
            "hits": 38
        },
        {
            "id": 10360,
            "url": "https://svs.gsfc.nasa.gov/10360/",
            "result_type": "Produced Video",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "Mars Methane Spectroscopy",
            "description": "Conceptual animation demonstrating the process of spectroscopy. The first animation demonstrates the general concept of visible-light spectroscopy by which white light is separated into its component wavelengths (colors) using a prism. The second animation demonstrates how this idea is applied to the discovery of methane in Mars' atmosphere. Because it absorbs specific wavelengths of electromagnetic energy, methane has a 'fingerprint' that can be seen as missing lines on the resulting spectograph. || Mars_Methane_Spectroscopy_mpgLG.00715_print.jpg (1024x576) [54.5 KB] || Mars_Methane_Spectroscopy_mpgLG_web.png (320x180) [60.4 KB] || Mars_Methane_Spectroscopy_mpgLG_thm.png (80x40) [6.9 KB] || Mars_Methane_Spectroscopy_h264fullres.webmhd.webm (960x540) [2.9 MB] || Mars_Methane_Spectroscopy_h264fullres.mov (1280x720) [9.7 MB] || Mars_Methane_Spectroscopy_prores.mov (1280x720) [140.3 MB] || Mars_Methane_Spectroscopy_YouTube.mov (1280x720) [6.8 MB] || Mars_Methane_Spectroscopy_ipodLG.m4v (640x360) [3.6 MB] || Mars_Methane_Spectroscopy_mpgLG.mpg (640x360) [6.2 MB] || Mars_Methane_Spectroscopy_ipodSM.m4v (320x180) [1017.7 KB] || Mars_Methane_Spectroscopy_mp4SM.mp4 (320x240) [658.4 KB] || Mars_Methane_Spectroscopy_mpgSM.mpg (512x288) [4.2 MB] || ",
            "hits": 50
        },
        {
            "id": 10363,
            "url": "https://svs.gsfc.nasa.gov/10363/",
            "result_type": "Produced Video",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "The Mystery of Martian Methane",
            "description": "Mike Mumma and his team of researchers at Goddard Space Flight Center have made the first definitive observations of methane in the atmosphere of Mars. The evidence of methane plumes only during certain seasons and the chemical processes that could lead to its possible sources both raise intriguing questions for future study.For complete transcript, click here. || methane_short_mpgLG.00377_print.jpg (1024x768) [55.1 KB] || methane_short_mpgLG_web.png (320x180) [154.8 KB] || methane_short_mpgLG_thm.png (80x40) [14.9 KB] || Methanev2_h264_appletv.webmhd.webm (960x540) [23.3 MB] || Methanev2_h264_YouTube.mov (1280x720) [40.0 MB] || Methanev2_h264_appletv.m4v (960x540) [82.2 MB] || Methanev2_h264_fullres.mov (1280x720) [85.4 MB] || Methanev2_svs_SM.mpg (512x288) [22.1 MB] || Methanev2_svs_LG.mpg (640x360) [32.9 MB] || Methanev2_h264_ipodLG.m4v (640x360) [27.9 MB] || Methanev2.mp4 (320x240) [4.7 MB] || Methanev2_h264_ipodSM.m4v (320x180) [11.3 MB] || ",
            "hits": 56
        },
        {
            "id": 97,
            "url": "https://svs.gsfc.nasa.gov/97/",
            "result_type": "Visualization",
            "release_date": "1996-02-08T12:00:00-05:00",
            "title": "Images of Earth and Space: The Role of Visualization in NASA Science",
            "description": "This compilation video contains visualizations of Earth and Space Sciences resulting from supercomputer models. The excerpted visualizations include: Ocean Planet, El Niño, Ozone 1991, Clouds, Changes in Glacier Bay, Alaska, Biosphere, Lunar Topography from the Clementine Mission, Musculoskeletal Modeling Dynamic Simulations, Simulations of the Breakup and Dynamical Evolution of Comet Shoemaker-Levy 9, Convective Penetration in Stellar Interiors, Topological Features of a Compressible Plasma Vortex Sheet: A Model for the Outer Heliospheric Solar Wind, R-Aquarii Jet, The Evolution of Distorted Black Holes, Rayleigh-Taylor Instability in a Supernova, Galaxy Harassment, N-Body Simulation of the Cold Dark Matter Cosmology. || ",
            "hits": 132
        },
        {
            "id": 84,
            "url": "https://svs.gsfc.nasa.gov/84/",
            "result_type": "Visualization",
            "release_date": "1995-03-24T12:00:00-05:00",
            "title": "Simulations of the Breakup of Comet Shoemaker-Levy 9 Employing a Swarm Model: Initial Conditions",
            "description": "The breakup of comet Shoemaker-Levy 9 due to its gravitational interaction with Jupiter in July, 1994 is simulated using a swarm model.  In this simulation, the comet is modeled as an initially spherical distribution of 16,384 particles.  The particles interact with the tidal field of Jupiter and with each other through inter-particle gravitation and collisions.  All simulations were performed on the Maspar MP-2 at NASA/GSFC. || ",
            "hits": 40
        },
        {
            "id": 85,
            "url": "https://svs.gsfc.nasa.gov/85/",
            "result_type": "Visualization",
            "release_date": "1995-03-24T12:00:00-05:00",
            "title": "Simulations of the Breakup of Comet Shoemaker-Levy 9 Employing a Swarm Model: Dynamical Evolution",
            "description": "The breakup of comet Shoemaker-Levy 9 due to its gravitational interaction with Jupiter in July, 1994 is simulated using a swarm model.  In this simulation, the comet is modeled as an initially spherical distribution of 16,384 particles.  The particles interact with the tidal field of Jupiter and with each other through inter-particle gravitation and collisions.  All simulations were performed on the Maspar MP-2 at NASA/GSFC. || ",
            "hits": 48
        }
    ]
}