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    "results": [
        {
            "id": 14951,
            "url": "https://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] || ",
            "hits": 402
        },
        {
            "id": 20403,
            "url": "https://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": 198
        },
        {
            "id": 5530,
            "url": "https://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": 143
        },
        {
            "id": 14843,
            "url": "https://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": 181
        },
        {
            "id": 31271,
            "url": "https://svs.gsfc.nasa.gov/31271/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-01-26T00:00:00-05:00",
            "title": "Webb Views the Outer Planets",
            "description": "Images by Webb’s Near-Infrared Camera (NIRCam) show Jupiter, Saturn, Uranus, and Neptune. || ",
            "hits": 194
        },
        {
            "id": 20384,
            "url": "https://svs.gsfc.nasa.gov/20384/",
            "result_type": "Animation",
            "release_date": "2023-05-24T00:00:00-04:00",
            "title": "Enceladus",
            "description": "On Enceladus under a crust of ice lies a global ocean of salty water. Jets, supplied by that ocean, gush from the surface of the moon and feed into the entire system of Saturn. NASA’s James Webb Space Telescope first look at this ocean world is revealing that a plume spouts water out more than 20 times the size of the moon itself. Enceladus, together with its sub-surface ocean, is one of the most exciting scientific targets in our solar system in the search for life beyond Earth. Sandwiched between the moon’s icy outer crust and its rocky core is a global reservoir of salty water. Geyser-like volcanos spew jets of ice particles, water vapor, and organic chemicals out of crevices in the moon’s surface informally called ‘tiger stripes.’ In this video, we show a possible scenario of how water could be being sourced from hydrothermal vents in the sub-surface ocean to generate the observed plumes. || ",
            "hits": 521
        },
        {
            "id": 14321,
            "url": "https://svs.gsfc.nasa.gov/14321/",
            "result_type": "Produced Video",
            "release_date": "2023-05-11T15:00:00-04:00",
            "title": "Cosmic Cycles 5: Planetary Fantasia",
            "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Planetary Fantasia\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger.  Courtesy of the composer.Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Planetary_Fantasia_V2_print.jpg (1024x576) [60.4 KB] || Cosmic_Cycles_Planetary_Fantasia_V2.jpg (3840x2160) [465.1 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_searchweb.png (320x180) [40.9 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_thm.png (80x40) [5.2 KB] || Cosmic_Cycles_Planetary_Fantasia.webm (1920x1080) [98.0 MB] || Cosmic_Cycles_Planetary_Fantasia.mp4 (1920x1080) [415.1 MB] || Cosmic_Cycles-Planetary_Fantasia_Online_50mbps.mp4 (1920x1080) [3.5 GB] || Cosmic_Cycles-Planetary_Fantasia_Online_ProRes_1920x1080_2997.mov (1920x1080) [10.9 GB] || ",
            "hits": 80
        },
        {
            "id": 14162,
            "url": "https://svs.gsfc.nasa.gov/14162/",
            "result_type": "Produced Video",
            "release_date": "2022-05-19T15:30:00-04:00",
            "title": "Saturn Through the Veil of Enceladus – Artist’s Concept",
            "description": "Artist’s concept of Saturn and its icy moons Enceladus (foreground), Titan (large crescent at upper left), and Rhea (small crescent). Based on imagery from the Cassini spacecraft. || SaturnMoonsConceptArt_print.jpg (1024x460) [68.0 KB] || SaturnMoonsConceptArt.png (4800x2160) [6.3 MB] || SaturnMoonsConceptArt.jpg (4800x2160) [502.7 KB] || SaturnMoonsConceptArt_searchweb.png (320x180) [61.1 KB] || SaturnMoonsConceptArt_thm.png (80x40) [4.9 KB] || ",
            "hits": 178
        },
        {
            "id": 13809,
            "url": "https://svs.gsfc.nasa.gov/13809/",
            "result_type": "Produced Video",
            "release_date": "2021-02-10T09:55:00-05:00",
            "title": "Exploring Our Solar System with Dr. Amy Simon",
            "description": "Dr. Amy Simon has always been fascinated with space. From a young age she dreamed of lifting off in the Space Shuttle, just like her hero Sally Ride. Over the years her interest in space remained, and she eventually found herself working at NASA.Dr. Simon is the Senior Scientist for Planetary Atmospheres Research in the Solar System Exploration Division at the NASA Goddard Space Flight Center. Her scientific research involves the study of the composition, dynamics, and cloud structure in jovian planet atmospheres, primarily from spacecraft observations like the Hubble Space Telescope.Dr. Simon is also involved in multiple robotic flight missions, as well as future mission concept development. She was a co-investigator on the Cassini Composite Infrared Spectrometer (CIRS) and is the Deputy Instrument Scientist for the OSIRIS-REx Visible and near-IR Spectrometer (OVIRS), as well as the Landsat 9 TIRS2 instrument, and the Lucy L'Ralph instrument Deputy PI. She is PI of the Hubble Outer Planet Atmospheres Legacy (OPAL) program. She recently served as science co-lead of the NASA Ice Giants Mission Concept study.This inspiring woman shows the world that anything is possible, and that you should always work hard to follow your passion in life.For more information, visit https://nasa.gov/hubble. Music Credits: \"Falling Freet\" by Christian Tschuggnall [AKM] and Michael Edwards [APRA] via Atmosphere Music Ltd. [PRS] and Universal Production Music.“Darwin’s Extraordinary Journey” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music. || ",
            "hits": 273
        },
        {
            "id": 13783,
            "url": "https://svs.gsfc.nasa.gov/13783/",
            "result_type": "Produced Video",
            "release_date": "2020-12-15T14:55:00-05:00",
            "title": "The Outer Planets: Hubble’s Continuing Legacy",
            "description": "What is OPAL?OPAL (Outer Planet Atmospheres Legacy) is a project to obtain long time baseline observations of the outer planets in order to understand their atmospheric dynamics and evolution as gas giants. The yearly observations from OPAL throughout the remainder of Hubble's operation will provide an important legacy of time-domain images for use by planetary scientists. Viewers might notice that some of the images of the same planets appear to be different colors. This is due to the fact that over the years, from Voyager to Hubble, many different instruments, and many different filters have been used. For more information, visit https://nasa.gov/hubble. Music Credits: “The Granted Wish” by Nicholas Techer [BMI] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music.“Voyage Spectacular” by Rob Lane [PRS] via Abbey Road Masters [PRS], and Universal Production Music.“Celestial Waves” by Harry Vaman [SACEM] via Koka Media [SACEM], and Universal Production Music.“Solar Horizons” by David Rogers [PRS] and Paul Shaw [PRS] via Atmosphere Music Ltd [PRS], and Universal Production Music.“Visionary” by Andy Blythe [PRS] and Marten Joustra [PRS] via Ingenious Music Publishing Ltd. [PRS], and Universal Production Music. || ",
            "hits": 159
        },
        {
            "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": 154
        },
        {
            "id": 13562,
            "url": "https://svs.gsfc.nasa.gov/13562/",
            "result_type": "Produced Video",
            "release_date": "2020-02-25T16:00:00-05:00",
            "title": "The Science of Dragonfly",
            "description": "Dragonfly’s suite of science instruments will investigate the chemistry and habitability of Titan.Universal Production Music: “Clediss” by Thomas Stempfle and Tom Sue, “Downloading Landscapes” by Andrew Michael Britton and David Stephen GoldsmithWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13562_Dragonfly_Science_MASTER_facebook_720.mp4 (1280x720) [145.8 MB] || DragonflySciencePreview_print.jpg (1024x576) [96.9 KB] || DragonflySciencePreview.jpg (3840x2160) [637.4 KB] || DragonflySciencePreview_searchweb.png (320x180) [72.4 KB] || DragonflySciencePreview_thm.png (80x40) [5.5 KB] || TWITTER_720_13562_Dragonfly_Science_MASTER_twitter_720.mp4 (1280x720) [27.2 MB] || 13562_Dragonfly_Science_MASTER.webm (960x540) [46.9 MB] || 13562_Dragonfly_Science_CAPTIONS.en_US.srt [3.4 KB] || 13562_Dragonfly_Science_CAPTIONS.en_US.vtt [3.4 KB] || 13562_Dragonfly_Science_YouTube.mp4 (3840x2160) [2.7 GB] || 13562_Dragonfly_Science_MASTER.mov (3840x2160) [16.6 GB] || ",
            "hits": 171
        },
        {
            "id": 20311,
            "url": "https://svs.gsfc.nasa.gov/20311/",
            "result_type": "Animation",
            "release_date": "2020-02-25T16:00:00-05:00",
            "title": "Dragonfly Animation Resource Page",
            "description": "Dragonfly on Titan || DF_End_Pan_4K_Prores.00420_print.jpg (1024x576) [77.6 KB] || DF_End_Pan_H264_1080.mp4 (1920x1080) [27.1 MB] || DF_End_Pan_4K_H264.mp4 (3840x2160) [15.4 MB] || DF_End_Pan_4K_Prores_PNG (3840x2160) [0 Item(s)] || DF_End_Pan_4K_Prores.webm (3840x2160) [7.0 MB] || DF_End_Pan_4K_Prores.mov (3840x2160) [1.7 GB] || ",
            "hits": 362
        },
        {
            "id": 13307,
            "url": "https://svs.gsfc.nasa.gov/13307/",
            "result_type": "Produced Video",
            "release_date": "2019-09-12T09:55:00-04:00",
            "title": "Hubble’s Brand New Image of Saturn",
            "description": "This new Hubble Space Telescope view of Saturn, taken in late June of 2019, reveals the giant planet's iconic rings. Saturn’s amber colors come from summer smog-like hazes, produced in photochemical reactions driven by solar ultraviolet radiation. Below the haze lie clouds of ammonia ice crystals, as well as deeper, unseen lower-level clouds of ammonium hydrosulfide and water. The planet’s banded structure is caused by winds and clouds at different altitudes. Hubble’s Wide Field Camera 3 observed Saturn on June 20, 2019, as the planet made its closest approach to Earth, at about 845 million miles away.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight CenterPaul R. Morris (USRA): Lead Producer Music credits: \"Momentum\" by Guillaume Bernard [SACEM]; Killer Tracks Production Music || ",
            "hits": 135
        },
        {
            "id": 12672,
            "url": "https://svs.gsfc.nasa.gov/12672/",
            "result_type": "Produced Video",
            "release_date": "2018-12-17T11:00:00-05:00",
            "title": "Saturn's Rings Are Disappearing",
            "description": "Scientists from NASA Goddard have discovered that not only are Saturn's rings younger than previously thought, but also that the rings are actually disappearing at a rapid pace through a process called \"ring rain.\" Learn more about this phenomena in this animated video.Video narrated by: Jerome HruskaMusic Provided by Killer Tracks: \"The Butterfly Effect\" - Gresby Race NashWatch this video on the NASA Goddard YouTube channel. || SaturnRingRainThumbnail1.jpg (1920x1080) [591.1 KB] || SaturnRingRainThumbnail2.jpg (1920x1080) [530.2 KB] || SaturnRingRainThumbnail1_searchweb.png (320x180) [56.1 KB] || SaturnRingRainThumbnail1_thm.png (80x40) [3.6 KB] || 12672_SaturnRingsDisappearing_Twitter.mp4 (1280x720) [27.1 MB] || 12672_SaturnRingsDisappearing_YouTubeHD.webm (1920x1080) [13.7 MB] || 12672_SaturnRingsDisappearing_YouTubeHD.mp4 (1920x1080) [187.2 MB] || 12672_SaturnRingsDisappearing_Facebook.mp4 (1920x1080) [144.4 MB] || SaturnRingsDisappearingCaptions.en_US.srt [2.3 KB] || SaturnRingsDisappearingCaptions.en_US.vtt [2.3 KB] || 12672_SaturnRingsDisappearing_MASTER.mov (1920x1080) [1.6 GB] || ",
            "hits": 282
        },
        {
            "id": 4665,
            "url": "https://svs.gsfc.nasa.gov/4665/",
            "result_type": "Visualization",
            "release_date": "2018-07-27T00:00:00-04:00",
            "title": "Saturn's Magnetosphere",
            "description": "A basic view of Saturn's magnetosphere. || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_print.jpg (1024x576) [186.2 KB] || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_searchweb.png (320x180) [107.8 KB] || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_thm.png (80x40) [7.1 KB] || SaturnBasic-noglyph (1920x1080) [0 Item(s)] || Saturn_SaturnBasic_Dayside.HD1080i_p30.webm (1920x1080) [22.1 MB] || Saturn_SaturnBasic_Dayside.HD1080i_p30.mp4 (1920x1080) [365.5 MB] || SaturnBasic-noglyph (3840x2160) [0 Item(s)] || Saturn_SaturnBasic_Dayside_2160p30.mp4 (3840x2160) [938.9 MB] || Saturn_SaturnBasic_Dayside.HD1080i_p30.mp4.hwshow || ",
            "hits": 141
        },
        {
            "id": 13006,
            "url": "https://svs.gsfc.nasa.gov/13006/",
            "result_type": "Produced Video",
            "release_date": "2018-07-26T17:00:00-04:00",
            "title": "Hubble Sees Summer Storms on Mars and Saturn",
            "description": "B-Roll || HubbleMarsSaturnBRoll.00001_print.jpg (1024x576) [61.7 KB] || STSCI-H-p1829d-f-1152x1152.png (1152x1152) [360.7 KB] || STSCI-H-p1829d-f-1152x1152_print.jpg (1024x1024) [56.0 KB] || HubbleMarsSaturnBRoll.00001_searchweb.png (320x180) [46.8 KB] || HubbleMarsSaturnBRoll.00001_thm.png (80x40) [5.2 KB] || HubbleMarsSaturnBRoll.00001_print_web.png (320x180) [52.2 KB] || HubbleMarsSaturnBRoll.00001_web.png (320x180) [47.2 KB] || STSCI-H-p1829d-f-1152x1152_web.png (320x320) [33.8 KB] || STSCI-H-p1829d-f-1152x1152_thm.png (80x40) [3.9 KB] || 05-broll.mov (1280x720) [1.2 GB] || HubbleMarsSaturnBRoll.mp4 (1280x720) [88.2 MB] || HubbleMarsSaturnBRoll.webm (1280x720) [12.5 MB] || ",
            "hits": 42
        },
        {
            "id": 30978,
            "url": "https://svs.gsfc.nasa.gov/30978/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-07-20T00:00:00-04:00",
            "title": "Seeing Titan with Infrared Eyes",
            "description": "Six infrared views of Saturn's moon Titan. || titan_infrared_eyes_PIA21923_print.jpg (1024x576) [89.4 KB] || titan_infrared_eyes_PIA21923.png (5760x3240) [9.4 MB] || titan_infrared_eyes_PIA21923_searchweb.png (320x180) [65.1 KB] || titan_infrared_eyes_PIA21923_thm.png (80x40) [6.1 KB] || titan_infrared_eyes_PIA21923.hwshow [218 bytes] || ",
            "hits": 94
        },
        {
            "id": 30901,
            "url": "https://svs.gsfc.nasa.gov/30901/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-10-03T00:00:00-04:00",
            "title": "Cassini's Final Image",
            "description": "Cassini's final image || PIA21895_print.jpg (1024x1030) [71.7 KB] || PIA21895_searchweb.png (320x180) [29.7 KB] || PIA21895_thm.png (80x40) [2.5 KB] || PIA21895.tif (505x508) [190.2 KB] || cassinis-final-image.hwshow [260 bytes] || ",
            "hits": 89
        },
        {
            "id": 30902,
            "url": "https://svs.gsfc.nasa.gov/30902/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-10-03T00:00:00-04:00",
            "title": "Cassini, So Far from Home",
            "description": "one of Cassini's last looks at Saturn & its main rings || PIA21345_print.jpg (1024x529) [51.6 KB] || PIA21345_searchweb.png (320x180) [43.9 KB] || PIA21345_thm.png (80x40) [4.7 KB] || PIA21345.tif (3545x1834) [9.4 MB] || cassini-so-far-from-home.hwshow [200 bytes] || ",
            "hits": 94
        },
        {
            "id": 30903,
            "url": "https://svs.gsfc.nasa.gov/30903/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-10-03T00:00:00-04:00",
            "title": "Two Titans",
            "description": "Two views of Saturn's moon Titan || PIA21624_print.jpg (1024x518) [43.1 KB] || PIA21624_searchweb.png (320x180) [51.4 KB] || PIA21624_thm.png (80x40) [5.2 KB] || PIA21624.tif (2024x1024) [3.9 MB] || two-titans.hwshow [186 bytes] || ",
            "hits": 66
        },
        {
            "id": 12709,
            "url": "https://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": 74
        },
        {
            "id": 12467,
            "url": "https://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": 112
        },
        {
            "id": 4143,
            "url": "https://svs.gsfc.nasa.gov/4143/",
            "result_type": "Visualization",
            "release_date": "2017-07-12T10:01:00-04:00",
            "title": "Saturn's Magnetosphere",
            "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind.  Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer.  That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s.  The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959.  But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes).  The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets.  They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s.  The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. For these visualizations, the magnetic field structure is represented by gold/copper lines.  Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun.  The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis.  The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis.  It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included.  When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current.  This is a variation of the simple Luhmann-Friesen magnetosphere model.  They are meant to be representative of the basic characteristics of the planetary magnetic fields.  Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center.  ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann & Friesen, A simple model of the magnetosphereLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ",
            "hits": 83
        },
        {
            "id": 30883,
            "url": "https://svs.gsfc.nasa.gov/30883/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-06-07T12:00:00-04:00",
            "title": "Saturn's Hexagon as Summer Solstice Approaches",
            "description": "June 2013 vs. April 2017 || saturn_hex_color_1080p.00001_print.jpg (1024x576) [75.7 KB] || saturn_hex_color_1080p.00001_searchweb.png (320x180) [67.7 KB] || saturn_hex_color_1080p.00001_thm.png (80x40) [4.8 KB] || saturn_hex_color_1080p.mp4 (1920x1080) [5.4 MB] || saturn_hex_color_720p.mp4 (1280x720) [2.1 MB] || saturn_hex_color_1080p.webm (1920x1080) [1.1 MB] || saturn_hex_color_2304p.mp4 (4096x2304) [28.0 MB] || 4104x2304_16x9_30p (4104x2304) [32.0 KB] || ",
            "hits": 229
        },
        {
            "id": 12260,
            "url": "https://svs.gsfc.nasa.gov/12260/",
            "result_type": "Produced Video",
            "release_date": "2016-05-19T13:00:00-04:00",
            "title": "Hubble's New View of Mars and Planets",
            "description": "60-second video for social mediaMusic: \"Season of Swag\" by David Travis Edwards and Kenneth Barbee, Killer Tracks [BMI] and Soundcast Music [SESAC] || Hubble_Mars_Instagram_29.97.00148_print.jpg (1024x576) [42.9 KB] || Hubble_Mars_Instagram_29.97.00148_searchweb.png (320x180) [35.3 KB] || Hubble_Mars_Instagram_29.97.00148_web.png (320x180) [35.3 KB] || Hubble_Mars_Instagram_29.97.00148_thm.png (80x40) [3.5 KB] || Hubble_Mars_Instagram_29.97.mp4 (1280x720) [74.4 MB] || Hubble_Mars_Instagram.mp4 (1280x720) [74.1 MB] || Hubble_Mars_Instagram.mov (1280x720) [853.7 MB] || Hubble_Mars_Instagram_29.97.webm (1280x720) [15.1 MB] || Hubble_Mars_Instagram.en_US.srt [1.7 KB] || Hubble_Mars_Instagram.en_US.vtt [1.7 KB] || ",
            "hits": 116
        },
        {
            "id": 30710,
            "url": "https://svs.gsfc.nasa.gov/30710/",
            "result_type": "Hyperwall Visual",
            "release_date": "2016-03-15T12:00:00-04:00",
            "title": "Our Solar System",
            "description": "The 8 planets plus Pluto with planetary axis tilt || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_print.jpg (1024x576) [75.1 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_searchweb.png (320x180) [49.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_web.png (320x180) [50.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.mp4 (1920x1080) [9.2 MB] || planets3x3_pluto_colorMercury_axis_tilt_720p.mp4 (1280x720) [4.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.webm (1920x1080) [2.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_2160p.mp4 (3840x2160) [28.7 MB] || 3x3_pluto_tilt (4104x2304) [0 Item(s)] || 100-science-overview-001.hwshow || ",
            "hits": 918
        },
        {
            "id": 12018,
            "url": "https://svs.gsfc.nasa.gov/12018/",
            "result_type": "Produced Video",
            "release_date": "2015-10-30T12:45:00-04:00",
            "title": "Looking for the Shadows of New Worlds",
            "description": "NASA Goddard astrophysicist Daniel Angerhausen discusses how astronomers may be able to maximize transit photometry to find planets like those in our solar system around other stars -- and possibly moons, rings, and asteroid groups as well. Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Photometry_Still_2.jpg (1280x720) [139.8 KB] || Photometry_Still_2_print.jpg (1024x576) [103.0 KB] || Photometry_Still_2_searchweb.png (320x180) [76.9 KB] || Photometry_Still_2_thm.png (80x40) [6.0 KB] || Photometry_FINAL_ProRes_1280x720_5994.mov (1280x720) [3.6 GB] || Photometry_FINAL-H264_Best_1280x720_5994.mov (1280x720) [1.5 GB] || G2015-081_Photometry_FINAL_V2_youtube_hq.mov (1280x720) [604.7 MB] || Photometry_FINAL-H264_Good_1280x720_2997.mov (1280x720) [123.6 MB] || Photometry_FINAL-MPEG4_1280X720_2997.mp4 (1280x720) [63.2 MB] || G2015-081_Photometry_FINAL_V2_HD.wmv (1280x720) [59.0 MB] || G2015-081_Photometry_FINAL_V2_appletv.m4v (1280x720) [151.8 MB] || Photometry_FINAL_ProRes_1280x720_5994.webm (1280x720) [27.3 MB] || G2015-081_Photometry_FINAL_V2_appletv_subtitles.m4v (1280x720) [149.2 MB] || Photometry_Final_SRT_Captions2.en_US.srt [5.1 KB] || Photometry_Final_SRT_Captions2.en_US.vtt [5.1 KB] || NASA_PODCAST_G2015-081_Photometry_FINAL_V2_ipod_sm.mp4 (320x240) [48.5 MB] || ",
            "hits": 90
        },
        {
            "id": 30520,
            "url": "https://svs.gsfc.nasa.gov/30520/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-08-07T12:00:00-04:00",
            "title": "The Day the Earth Smiled",
            "description": "On July 19, 2013, in an event celebrated the world over, NASA's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings, and, in the background, our home planet, Earth. With the sun's powerful and potentially damaging rays eclipsed by Saturn itself, Cassini's onboard cameras were able to take advantage of this unique viewing geometry. They acquired a panoramic mosaic of the Saturn system that allows scientists to see details in the rings and throughout the system as they are backlit by the sun.With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilometers) across. || ",
            "hits": 202
        },
        {
            "id": 30518,
            "url": "https://svs.gsfc.nasa.gov/30518/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-08-06T14:00:00-04:00",
            "title": "Earth From the Outer Solar System",
            "description": "On July 19, 2013, the wide-angle camera on NASA’s Cassini spacecraft had the unusual opportunity to image the whole Saturn system as well as our home planet, Earth, and its moon. In this rare image, Earth is 898 million miles (1.44 billion kilometers) away and appears as a blue dot while the moon can be seen as a fainter protrusion off its right side. Opportunities to image Earth from the outer solar system are few and far between and special care must be taken to avoid damaging the cameras onboard the spacecraft. NASA informed the public about their planet’s portrait being taken from interplanetary distances and invited them to celebrate by finding Saturn in their part of the sky and waving at the ringed planet.This is one of many images that scientists will stich together to create a mosaic of the diffuse rings that encircle Saturn and check for change over time. The previous mosaic of the Saturn system captured by Cassini in 2006 revealed that the dusty E ring, which is fed by the water-ice plume of the moon Enceladus, had unexpectedly large variations in brightness and color around its orbit. Scientists want to see how the E ring looks seven Earth years later, in hopes that it will provide clues about the forces at work in the Saturn system. || ",
            "hits": 175
        },
        {
            "id": 11339,
            "url": "https://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": 143
        },
        {
            "id": 30353,
            "url": "https://svs.gsfc.nasa.gov/30353/",
            "result_type": "Hyperwall Visual",
            "release_date": "2012-12-20T12:00:00-05:00",
            "title": "Splendid Saturn",
            "description": "NASA's Cassini spacecraft has delivered a glorious view of Saturn, taken while the spacecraft was in Saturn's shadow. The cameras were turned toward Saturn and the sun so that the planet and rings are backlit. (The sun is behind the planet, which is shielding the cameras from direct sunlight.) In addition to the visual splendor, this special, very-high-phase viewing geometry allows scientists to study ring and atmosphere phenomena not easily seen at a lower phase.Since images like this can only be taken while the sun is behind the planet, this beautiful view is all the more precious for its rarity. Also captured in this image are two of Saturn's moons: Enceladus and Tethys. Both appear on the left side of the planet, below the rings. Enceladus is closer to the rings; Tethys is below and to the left.This view looks toward the non-illuminated side of the rings from about 19 degrees below the ring plane. The image was obtained with the Cassini spacecraft wide-angle camera on Oct. 17, 2012 at a distance of approximately 500,000 miles (800,000 kilometers) from Saturn. Image scale at Saturn is about 30 miles per pixel (50 kilometers per pixel). || ",
            "hits": 130
        },
        {
            "id": 11038,
            "url": "https://svs.gsfc.nasa.gov/11038/",
            "result_type": "Produced Video",
            "release_date": "2012-10-25T09:00:00-04:00",
            "title": "Saturn's Record-Setting Storm",
            "description": "NASA scientist Brigette Hesman discusses extreme temperature changes in Saturn's 2010 Great White Spot. || ",
            "hits": 106
        },
        {
            "id": 10958,
            "url": "https://svs.gsfc.nasa.gov/10958/",
            "result_type": "Produced Video",
            "release_date": "2012-05-02T08:00:00-04:00",
            "title": "Pursuit of Light",
            "description": "Perhaps more than all other federal agencies, NASA tells stories about big things: big places, big data, big ideas. Using extraordinarily high resolution data sets from some of the most innovative and powerful scientific instruments ever built, the media team at NASA Goddard presents PURSUIT OF LIGHT. The presentation showcases top level goals of NASA's Science Mission Directorate, with an eye toward capturing the imagination of mainstream audiences. Data visualizations at resolutions far greater than HDTV present NASA's science goals like never before. Interspersed with inventive live action footage also designed to make use of that vast canvas, this six and a half minute presentation captivates and moves viewers.PURSUIT OF LIGHT was designed expressly for a screen technology called The Hyperwall, a system largely perfected at NASA Goddard Space Flight Center. The Hyperwall itself is a platform best suited for big themes. With colossal screen resolution and an ultrawide presentational style, moving images played there take on a vast sense of scale and power. PURSUIT OF LIGHT employs the strength of this remarkable system and pushes it further than ever before, presenting stories about the Earth, The Moon, The Sun, The Planets, and the deep sky, wrapped in poetic implication about the humanity's imperative need to explore. This show will play prominently on touring Hyperwalls around the country as well as on the web. || ",
            "hits": 28
        },
        {
            "id": 30346,
            "url": "https://svs.gsfc.nasa.gov/30346/",
            "result_type": "Hyperwall Visual",
            "release_date": "2011-11-20T12:00:00-05:00",
            "title": "Two Storm Views on Saturn",
            "description": "Two false-color views of Saturn show detailed patterns that change during one Saturn day within a huge storm in the planet's Northern Hemisphere. The dramatic colors arise from a false-color combination of images taken by the Cassini spacecraft narrow-angle camera: images filtered at 889 nanometers are projected as blue, images filtered at 727 nanometers are projected as green, and images filtered at 750 nanometers are projected as red.Cassini scientists study the fine details contained in these mosaics to learn about wind speeds and cloud depths in the storm. For example, a red curlicue that indicates a deep cloud is present in the top mosaic, but it does not appear in bottom mosaic taken 11 hours later. || ",
            "hits": 49
        },
        {
            "id": 30347,
            "url": "https://svs.gsfc.nasa.gov/30347/",
            "result_type": "Hyperwall Visual",
            "release_date": "2011-11-20T12:00:00-05:00",
            "title": "Six Storm Views on Saturn",
            "description": "This series of images from NASA's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true-color and composite near-true-color views chronicle the storm from its start in late 2010 through mid-2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. || ",
            "hits": 114
        },
        {
            "id": 30352,
            "url": "https://svs.gsfc.nasa.gov/30352/",
            "result_type": "Hyperwall Visual",
            "release_date": "2007-03-29T12:00:00-04:00",
            "title": "Saturn's Active North Pole",
            "description": "A bizarre six-sided feature encircling the north pole of Saturn near 78 degrees north latitude has been spied by the visual and infrared mapping spectrometer on NASA's Cassini spacecraft.This image was acquired on Oct. 29, 2006, from an average distance of 902,000 kilometers (560,400 miles) above the cloud tops of Saturn, and is one of the first clear images ever taken of the north polar region as seen from a unique polar perspective.Originally discovered and last observed by a spacecraft during NASA's Voyager flybys of the early 1980's, the new views of this polar hexagon taken in late 2006 prove that this is an unusually long-lived feature on Saturn. || ",
            "hits": 104
        },
        {
            "id": 30348,
            "url": "https://svs.gsfc.nasa.gov/30348/",
            "result_type": "Hyperwall Visual",
            "release_date": "2005-02-28T12:00:00-05:00",
            "title": "True Saturn",
            "description": "While cruising around Saturn in early October 2004, Cassini captured a series of images that have been composed into this large global natural color view of Saturn and its rings. This grand mosaic consists of 126 images acquired in a tile-like fashion, covering one end of Saturn's rings to the other and the entire planet in between. The images were taken over the course of two hours on Oct. 6, 2004, while Cassini was approximately 6.3 million km (3.9 million miles) from Saturn. Since the view seen by Cassini during this time changed very little, no re-projection or alteration of any of the images was necessary. Three images (red, green and blue) were taken of each of 42 locations, or \"footprints,\" across the planet. The full color footprints were put together to produce a mosaic that is 8,888 pixels across and 4,544 pixels tall. The smallest features seen here are 38 km (24 miles) across. Many of Saturn's splendid features noted previously in single frames taken by Cassini are visible in this one detailed, all-encompassing view: subtle color variations across the rings, the thread-like F ring, ring shadows cast against the blue northern hemisphere, the planet's shadow making its way across the rings to the left, and blue-grey storms in Saturn's southern hemisphere to the right.  Tiny Mimas and even smaller Janus are both faintly visible at the lower left. The Sun-Saturn-Cassini, or phase, angle at the time was 72 degrees; hence, the partial illumination of Saturn in this portrait. Later in the mission, when the spacecraft's trajectory takes it far from Saturn and also into the direction of the Sun, Cassini will be able to look back and view Saturn and its rings in a more fully-illuminated geometry. || ",
            "hits": 141
        }
    ]
}