{
    "count": 5,
    "next": null,
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    "results": [
        {
            "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": 86
        },
        {
            "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": 54
        },
        {
            "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": 65
        },
        {
            "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": 43
        },
        {
            "id": 10362,
            "url": "https://svs.gsfc.nasa.gov/10362/",
            "result_type": "Produced Video",
            "release_date": "2009-01-15T00:00:00-05:00",
            "title": "Radiolytic Production of Methane by Microbial Life",
            "description": "Animation depicting how 'extreme microbes' on Earth produce methane. || ",
            "hits": 45
        }
    ]
}