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    "results": [
        {
            "id": 14951,
            "url": "http://svs.gsfc.nasa.gov/14951/",
            "result_type": "Produced Video",
            "release_date": "2026-01-14T10:00:00-05:00",
            "title": "Are Titan’s Lakes Teeming with Primitive Cells?",
            "description": "Titan’s hydrocarbon lakes could contain structures called vesicles that strongly resemble cell membranes on Earth. A recent study coauthored by NASA shows that rainfall might provide the energy needed for these vesicles to form.Complete transcript available.Universal Production Music: “Perpetual Resonance” by Lee John Gretton [PRS]Watch this video on the NASA Goddard YouTube channel and Facebook. || Titan-Vesicles-Thumbnail-V3_print.jpg (1024x576) [112.3 KB] || Titan-Vesicles-Thumbnail-V3.jpg (1280x720) [362.4 KB] || Titan-Vesicles-Thumbnail-V3.png (1280x720) [734.2 KB] || Titan-Vesicles-Thumbnail-V3_searchweb.png (320x180) [62.2 KB] || Titan-Vesicles-Thumbnail-V3_thm.png (80x40) [6.0 KB] || 14951_Titan_Vesicles_Explainer_720.mp4 (1280x720) [39.0 MB] || 14951_Titan_Vesicles_Explainer_1080.mp4 (1920x1080) [218.4 MB] || TitanVesiclesCaptions.en_US.srt [3.8 KB] || TitanVesiclesCaptions.en_US.vtt [3.6 KB] || 14951_Titan_Vesicles_Explainer_4K.mp4 (3840x2160) [1.3 GB] || 14951_Titan_Vesicles_Explainer_ProRes.mov (3840x2160) [8.0 GB] || ",
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        {
            "id": 20411,
            "url": "http://svs.gsfc.nasa.gov/20411/",
            "result_type": "Animation",
            "release_date": "2026-01-14T10:00:00-05:00",
            "title": "A Pathway to Protocells on Titan – Animations",
            "description": "These animations illustrate how simple protocells could form in the lakes of Titan, Saturn’s largest moon. When rain falls from Titan’s methane clouds into its hydrocarbon lakes, it can transport organic molecules like acrylonitrile that are attracted to both water and oil. Such amphiphile molecules are likely to collect in a thin film on the surface of Titan’s lakes. As large raindrops pelt the lakes, they could stir up this floating “pond scum” to form spherical droplets of methane coated in a bilayer of amphiphiles – structures called vesicles that resemble cell membranes on Earth.Although such vesicles have yet to be detected on Titan, a 2025 study by Christian Mayer and NASA scientist Conor Nixon lays out the process for their formation and evolution, and it proposes a mechanism for their discovery by a future mission to Titan. The paper also proposes that different mixtures of amphiphiles could stabilize vesicles and lead to the evolution of simple protocells on Titan. || ",
            "hits": 152
        },
        {
            "id": 20403,
            "url": "http://svs.gsfc.nasa.gov/20403/",
            "result_type": "Animation",
            "release_date": "2025-05-14T09:00:00-04:00",
            "title": "Titan science results from James Webb Space Telescope: animation resource page",
            "description": "Push into JWST to Saturn and Titan. || JWST_Titan_Intro_Final_V001.00957_print.jpg (1024x576) [145.8 KB] || JWST_Titan_Intro_Final_V001.00957_searchweb.png (320x180) [78.0 KB] || JWST_Titan_Intro_Final_V001.00957_thm.png [5.5 KB] || JWST_Titan_Intro_Final_1080.mp4 (1920x1080) [72.8 MB] || JWST_Titan_Intro_Final_V001.mp4 (3840x2160) [38.4 MB] || JWST_Titan_Intro_Final_V001.mov (3840x2160) [6.8 GB] || ",
            "hits": 161
        },
        {
            "id": 5530,
            "url": "http://svs.gsfc.nasa.gov/5530/",
            "result_type": "Visualization",
            "release_date": "2025-05-14T08:00:59-04:00",
            "title": "Webb Confirms Seasonal Variations in Titan Climate Model",
            "description": "This global circulation model simulates a year of weather on Titan, depicting seasonal variations in wind currents, methane cloud cover, and sunlight over the course of a Saturn year (approximately 29.5 Earth years). New observations from the James Webb Science Telescope confirm this seasonal variation.",
            "hits": 177
        },
        {
            "id": 14843,
            "url": "http://svs.gsfc.nasa.gov/14843/",
            "result_type": "Produced Video",
            "release_date": "2025-05-14T08:00:00-04:00",
            "title": "Webb Spies Rain Clouds, New Molecule on Titan",
            "description": "NASA’s Webb Telescope has discovered a new molecule in Titan’s atmosphere – one that may have implications for the future of this surprisingly Earthlike world.Complete transcript available.Universal Production Music: “Barfuß Durch Die Stadt” by Edgar Möller [GEMA] and Lucia Wilke [GEMA]; “Into the Void” by Gage Boozan [ASCAP]; “Pulse of Progress” by Emma Zarobyan [SOCAN]; “Playing With The Narrative” by Cathleen Flynn [ASCAP] and Micah Barnes [BMI]; “Back From The Brink” by Daniel Gunnar Louis Trachtenberg [PRS]Watch this video on the James Webb Space Telescope YouTube channel. || Webb_Titan_Climate_Thumbnail_print.jpg (1024x576) [189.4 KB] || Webb_Titan_Climate_Thumbnail.jpg (1280x720) [872.3 KB] || Webb_Titan_Climate_Thumbnail.png (1280x720) [1.3 MB] || Webb_Titan_Climate_Thumbnail_searchweb.png (320x180) [88.6 KB] || Webb_Titan_Climate_Thumbnail_thm.png [6.7 KB] || 14843_Webb_Titan_Climate_720.mp4 (1280x720) [77.0 MB] || 14843_Webb_Titan_Climate_1080.mp4 (1920x1080) [431.4 MB] || WebbTitanClimate.en_US.srt [7.3 KB] || WebbTitanClimate.en_US.vtt [6.9 KB] || 14843_Webb_Titan_Climate_4K.mp4 (3840x2160) [4.9 GB] || 14843_Webb_Titan_Climate_ProRes.mov (3840x2160) [29.0 GB] || ",
            "hits": 114
        },
        {
            "id": 12736,
            "url": "http://svs.gsfc.nasa.gov/12736/",
            "result_type": "Produced Video",
            "release_date": "2018-06-04T12:00:00-04:00",
            "title": "Building Blocks for Surviving Titan",
            "description": "Saturn’s moon, Titan, may have a building block for potential cell membranes. || PIA14909_16x9.jpg (1024x576) [86.6 KB] || PIA14909_16x9_print.jpg (1024x576) [86.1 KB] || PIA14909_16x9_searchweb.png (320x180) [34.1 KB] || PIA14909_16x9_thm.png (80x40) [3.2 KB] || ",
            "hits": 113
        },
        {
            "id": 12709,
            "url": "http://svs.gsfc.nasa.gov/12709/",
            "result_type": "Produced Video",
            "release_date": "2017-09-12T10:00:00-04:00",
            "title": "Cassini's Infrared Saturn",
            "description": "Since arriving at Saturn in 2004, Cassini has used its Composite Infrared Spectrometer (CIRS) to study the ringed planet and its moons in heat radiation. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Particle Waves,\" \"Odyssey,\" \"Solaris,\" \"Expansive,\"\"Horizon Ahead,\" \"Ion Bridge,\" \"Outer Space\" || CassiniCIRSpreviewShort.jpg (1920x1080) [591.6 KB] || CassiniCIRSpreviewShort_searchweb.png (320x180) [125.9 KB] || CassiniCIRSpreviewShort_thm.png (80x40) [8.4 KB] || 12709_Cassini_CIRS_Short_TWTR.mp4 (1280x720) [102.0 MB] || WEBM-12709_Cassini_CIRS_Short_APR.webm (960x540) [191.9 MB] || 12709_Cassini_CIRS_Short_FB.mp4 (1280x720) [574.1 MB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.srt [10.3 KB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.vtt [10.3 KB] || 12709_Cassini_CIRS_Short_YT.mp4 (1920x1080) [1.2 GB] || 12709_Cassini_CIRS_Short_APR.mov (1920x1080) [6.0 GB] || 12709_Cassini_CIRS_Short_YT.hwshow [96 bytes] || ",
            "hits": 94
        },
        {
            "id": 12467,
            "url": "http://svs.gsfc.nasa.gov/12467/",
            "result_type": "Produced Video",
            "release_date": "2017-07-28T14:00:00-04:00",
            "title": "A Titan Discovery",
            "description": "NASA scientist Maureen Palmer narrates this video about the definitive detection of acrylonitrile on Titan.Music Provided by Killer Tracks: \"A Look Ahead\" - Matthew St Laurent. || TitanPreview.jpg (3840x2160) [5.4 MB] || TitanPreview-2.jpg (3840x2160) [1.4 MB] || TitanPreview_searchweb.png (320x180) [64.3 KB] || TitanPreview_thm.png (80x40) [5.2 KB] || A_Titan_Discovery_-_twitter.mp4 (1280x720) [26.0 MB] || A_Titan_Discovery_-_facebook.mp4 (1280x720) [149.3 MB] || A_Titan_Discovery.en_US.srt [1.8 KB] || A_Titan_Discovery.en_US.vtt [1.8 KB] || A_Titan_Discovery_-_youtube4k.webm (3840x2160) [16.7 MB] || A_Titan_Discovery_-_youtube4k.mp4 (3840x2160) [458.3 MB] || A_Titan_Discovery_-_MASTER.mov (3840x2160) [6.2 GB] || ",
            "hits": 47
        },
        {
            "id": 11371,
            "url": "http://svs.gsfc.nasa.gov/11371/",
            "result_type": "Produced Video",
            "release_date": "2013-11-14T00:00:00-05:00",
            "title": "Crude Matter",
            "description": "What do car bumpers and computer speakers have in common? Both can be created from raw materials found on Earth or on Titan, Saturn’s largest moon. Titan is the only moon in the solar system with a significant atmosphere. In some ways its atmosphere is similar to Earth’s, but rather than being rich in oxygen, it’s rich in hydrocarbons—chemical compounds made of the elements carbon and hydrogen. In 1980, NASA's Voyager 1 spacecraft flew by Titan and detected different types of hydrocarbons in its atmosphere, including methane, ethane and propane. Now, NASA’s Cassini spacecraft has added one more to the list: propylene, a chemical building block used in the manufacture of plastic consumer goods. Watch the video to learn more. || ",
            "hits": 31
        },
        {
            "id": 11339,
            "url": "http://svs.gsfc.nasa.gov/11339/",
            "result_type": "Produced Video",
            "release_date": "2013-09-30T12:00:00-04:00",
            "title": "Propylene on Titan",
            "description": "With a thick atmosphere, clouds, a rain cycle and giant lakes, Saturn's large moon Titan is a surprisingly Earthlike place. But unlike on Earth, Titan's surface is far too cold for liquid water - instead, Titan's clouds, rain, and lakes consist of liquid hydrocarbons like methane and ethane (which exist as gases here on Earth). When these hydrocarbons evaporate and encounter ultraviolet radiation in Titan's upper atmosphere, some of the molecules are broken apart and reassembled into longer hydrocarbons like ethylene and propane.NASA's Voyager 1 spacecraft first revealed the presence of several species of atmospheric hydrocarbons when it flew by Titan in 1980, but one molecule was curiously missing - propylene, the main ingredient in plastic number 5. Now, thanks to NASA's Cassini spacecraft, scientists have detected propylene on Titan for the first time, solving a long-standing mystery about the solar system's most Earthlike moon. || ",
            "hits": 60
        }
    ]
}