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    "results": [
        {
            "id": 20411,
            "url": "https://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": 215
        },
        {
            "id": 14932,
            "url": "https://svs.gsfc.nasa.gov/14932/",
            "result_type": "Produced Video",
            "release_date": "2025-12-02T08:00:00-05:00",
            "title": "Bio-Essential Sugars Discovered in Samples from Asteroid Bennu",
            "description": "OSIRIS-REx Project Scientist Daniel Glavin discusses the discovery of ribose and glucose in samples of asteroid Bennu, and the implications for the formation and evolution of life on Earth.Complete transcript available.Watch this video on the NASA.gov Video YouTube channel. || Bennu-Sugars-Thumbnail_print.jpg (1024x576) [175.2 KB] || Bennu-Sugars-Thumbnail.jpg (1280x720) [534.2 KB] || Bennu-Sugars-Thumbnail.png (1280x720) [892.3 KB] || Bennu-Sugars-Thumbnail_searchweb.png (320x180) [77.4 KB] || Bennu-Sugars-Thumbnail_thm.png (80x40) [6.8 KB] || 14932_Bennu_Sugars_Interview_Glavin_720.mp4 (1280x720) [180.6 MB] || 14932_Bennu_Sugars_Interview_Glavin_1080.mp4 (1920x1080) [1011.6 MB] || BennuSugarsGlavinCaptionsV2.en_US.srt [18.4 KB] || BennuSugarsGlavinCaptionsV2.en_US.vtt [17.5 KB] || 14932_Bennu_Sugars_Interview_Glavin_4K.mp4 (3840x2160) [6.2 GB] || 14932_Bennu_Sugars_Interview_Glavin_ProRes.mov (3840x2160) [47.0 GB] || ",
            "hits": 192
        },
        {
            "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": 180
        },
        {
            "id": 14772,
            "url": "https://svs.gsfc.nasa.gov/14772/",
            "result_type": "B-Roll",
            "release_date": "2025-01-29T11:00:00-05:00",
            "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics",
            "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ",
            "hits": 705
        },
        {
            "id": 14774,
            "url": "https://svs.gsfc.nasa.gov/14774/",
            "result_type": "Produced Video",
            "release_date": "2025-01-29T11:00:00-05:00",
            "title": "NASA Finds Ingredients of Life in Fragments of Lost World",
            "description": "Scientists studying the Bennu samples have discovered evidence of a wet, salty environment from 4.5 billion years ago that created the molecular building blocks of life.Complete transcript available.Universal Production Music: “Future Tense” by Gresby Race Nash [PRS]; “Take Off” by Nicholas Smith [PRS]; “Big Decision” by Gresby Race Nash [PRS]; “Waiting for the Answer” by Gresby Race Nash [PRS]Watch this video on the NASA Goddard YouTube channel. || 14774-Bennu-Organics-Thumbnail-V4_print.jpg (1024x576) [395.9 KB] || 14774-Bennu-Organics-Thumbnail-V4.jpg (1280x720) [1.2 MB] || 14774-Bennu-Organics-Thumbnail-V4.png (1280x720) [1.8 MB] || 14774-Bennu-Organics-Thumbnail-V4_searchweb.png (320x180) [120.2 KB] || 14774-Bennu-Organics-Thumbnail-V4_thm.png [8.3 KB] || 14774_OSIRIS-REx_Bennu_Organics_720.mp4 (1280x720) [66.1 MB] || 14774_OSIRIS-REx_Bennu_Organics_1080.mp4 (1920x1080) [370.5 MB] || BennuOrganicsCaptions.en_US.srt [6.4 KB] || BennuOrganicsCaptions.en_US.vtt [6.0 KB] || 14774_OSIRIS-REx_Bennu_Organics_4K.mp4 (3840x2160) [2.3 GB] || 14774_OSIRIS-REx_Bennu_Organics_ProRes.mov (3840x2160) [14.5 GB] || ",
            "hits": 401
        },
        {
            "id": 14089,
            "url": "https://svs.gsfc.nasa.gov/14089/",
            "result_type": "Produced Video",
            "release_date": "2022-09-05T10:00:00-04:00",
            "title": "A Box of Treasure from Asteroid Ryugu",
            "description": "NASA scientist Heather Graham receives a shipment of asteroid Ryugu samples from her colleagues at the Japan Aerospace Exploration Agency (JAXA). Transcript available.Universal Production Music: “The Ocean and the Moon” & “On Your Game” by Andy Blythe and Marten JoustraWatch this video on the NASA Goddard YouTube channel. || Ryugu_Treasure_Preview_V7_print.jpg (1024x576) [110.4 KB] || Ryugu_Treasure_Preview_V7.png (3840x2160) [6.0 MB] || Ryugu_Treasure_Preview_V7.jpg (3840x2160) [1.2 MB] || Ryugu_Treasure_Preview_V7_searchweb.png (320x180) [62.7 KB] || Ryugu_Treasure_Preview_V7_thm.png (80x40) [5.7 KB] || 14089_Ryugu_Sample_V4_Twitter.mp4 (1280x720) [33.5 MB] || 14089_Ryugu_Sample_V2_Twitter.webm (1280x720) [16.2 MB] || 14089_Ryugu_Sample_V4_Facebook.mp4 (1920x1080) [189.1 MB] || 14089_Ryugu_Sample_V2_Captions.en_US.srt [3.7 KB] || 14089_Ryugu_Sample_V2_Captions.en_US.vtt [3.5 KB] || 14089_Ryugu_Sample_V4_YouTube.mp4 (3840x2160) [1.8 GB] || 14089_Ryugu_Sample_V4_MASTER.mov (3840x2160) [7.7 GB] || ",
            "hits": 192
        },
        {
            "id": 14037,
            "url": "https://svs.gsfc.nasa.gov/14037/",
            "result_type": "Produced Video",
            "release_date": "2021-12-01T12:00:00-05:00",
            "title": "Ozone 101: What Is the Ozone Hole?",
            "description": "Ozone 101 is the first in a series of explainer videos outlining the fundamentals of popular Earth science topics. Let’s back up to the basics and understand what caused the Ozone Hole, its effects on the planet, and what scientists predict will happen in future decades. || ",
            "hits": 128
        },
        {
            "id": 14004,
            "url": "https://svs.gsfc.nasa.gov/14004/",
            "result_type": "Produced Video",
            "release_date": "2021-11-17T00:00:00-05:00",
            "title": "Elements of Webb: Gold Part 2 Ep02",
            "description": "Elements of Webb EP02: Gold Part Two || 2-Gold_2_-_Dark.jpg (1920x1080) [1.1 MB] || 2-Gold_2_-_Dark_print.jpg (1024x576) [473.1 KB] || 2-Gold_2_-_Dark_searchweb.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_web.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_thm.png (80x40) [7.5 KB] || 2-Elements_-_Gold_2.webm (1920x1080) [34.9 MB] || 2-Elements_-_Gold_2.en_US.srt [5.8 KB] || 2-Elements_-_Gold_2.en_US.vtt [5.8 KB] || 2-Elements_-_Gold_2_ProRes.mov (1920x1080) [4.2 GB] || 2-Elements_-_Gold_2.mp4 (1920x1080) [324.5 MB] || elements-of-webb-gold-part-2-ep02.hwshow [293 bytes] || ",
            "hits": 33
        },
        {
            "id": 14003,
            "url": "https://svs.gsfc.nasa.gov/14003/",
            "result_type": "Produced Video",
            "release_date": "2021-11-10T00:00:00-05:00",
            "title": "Elements of Webb: Gold Part 1 Ep01",
            "description": "Elements of Webb EP01: Gold Part One || 1-Gold_1_-_Dark.jpg (1920x1080) [958.4 KB] || 1-Gold_1_-_Dark_print.jpg (1024x576) [388.7 KB] || 1-Gold_1_-_Dark_searchweb.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_web.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_thm.png (80x40) [7.4 KB] || 1-Elements-_Gold_1.webm (1920x1080) [25.6 MB] || 1-Elements-_Gold_1.en_US.srt [4.1 KB] || 1-Elements-_Gold_1_ProRes.mov (1920x1080) [3.2 GB] || 1-Elements-_Gold_1.mp4 (1920x1080) [239.5 MB] || elements-of-webb-gold-part-1-ep01.hwshow [291 bytes] || ",
            "hits": 29
        },
        {
            "id": 14002,
            "url": "https://svs.gsfc.nasa.gov/14002/",
            "result_type": "Produced Video",
            "release_date": "2021-11-09T00:00:00-05:00",
            "title": "Elements of Webb: Series Introduction Ep0",
            "description": "Elements of Webb EP00: Introduction || EP00-_Elements_Series_Introduction.jpg (1920x1080) [738.1 KB] || EP00-_Elements_Series_Introduction_print.jpg (1024x576) [333.2 KB] || EP00-_Elements_Series_Introduction_searchweb.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_web.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_thm.png (80x40) [7.1 KB] || 0-Elements_of_Webb_-_Introduction_1.mp4 (1920x1080) [89.2 MB] || 0-Elements_of_Webb_-_Introduction_1.webm (1920x1080) [9.4 MB] || 0-Elements_of_Webb_-_Introduction_1.en_US.srt [1.3 KB] || 0-Elements_of_Webb_-_Introduction_1.en_US.vtt [1.3 KB] || 0-Elements_of_Webb_-_Introduction.mov (1920x1080) [1.1 GB] || elements-of-webb-series-introduction-ep0.hwshow [332 bytes] || ",
            "hits": 28
        },
        {
            "id": 13871,
            "url": "https://svs.gsfc.nasa.gov/13871/",
            "result_type": "Produced Video",
            "release_date": "2021-06-09T13:30:00-04:00",
            "title": "NASA Finds Local Lockdowns Brought Global Ozone Reductions",
            "description": "This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery is provided by pond5.com and is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.Music Credit:Universal Production Music: Waiting For Results - Adam John Salkeld [PRS], Neil Pollard [PRS]Complete transcript available. || 13871_Still_Image.jpg (1920x1080) [626.3 KB] || 13871_Still_Image_searchweb.png (320x180) [77.2 KB] || 13871_Still_Image_thm.png (80x40) [7.0 KB] || 13871_COVIDNOx.mov (1920x1080) [1.9 GB] || 13871_COVIDNOx.mp4 (1920x1080) [199.0 MB] || 13871_COVIDNOx.webm (1920x1080) [15.2 MB] || COVIDNOX.en_US.srt [2.1 KB] || COVIDNOX.en_US.vtt [2.1 KB] || ",
            "hits": 23
        },
        {
            "id": 13807,
            "url": "https://svs.gsfc.nasa.gov/13807/",
            "result_type": "Produced Video",
            "release_date": "2021-02-17T11:00:00-05:00",
            "title": "NASA Helps Identify Uptick in Emissions of Ozone-Depleting Compounds",
            "description": "Music: \"Hidden Movement\" Universal Production Music Complete transcript available. || Screen_Shot_2021-02-10_at_9.41.20_AM_print.jpg (1024x569) [115.7 KB] || Screen_Shot_2021-02-10_at_9.41.20_AM.png (2267x1261) [3.1 MB] || Screen_Shot_2021-02-10_at_9.41.20_AM_searchweb.png (320x180) [87.6 KB] || Screen_Shot_2021-02-10_at_9.41.20_AM_thm.png (80x40) [6.9 KB] || CFC_11_RC_5.webm (1920x1080) [6.5 MB] || 13807_CFC11.mp4 (1920x1080) [389.2 MB] || CFC11RC5.en_US.srt [3.4 KB] || ",
            "hits": 274
        },
        {
            "id": 13753,
            "url": "https://svs.gsfc.nasa.gov/13753/",
            "result_type": "Produced Video",
            "release_date": "2020-11-17T11:00:00-05:00",
            "title": "NASA Studies How COVID-19 Shutdowns Affect Emissions",
            "description": "Music: \"Lab Analysis\" from Universal Production MusicComplete transcript available.Coming soon to our YouTube channel. || Screen_Shot_2020-11-13_at_1.08.17_PM_print.jpg (1024x572) [164.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM.png (3568x1994) [6.4 MB] || Screen_Shot_2020-11-13_at_1.08.17_PM_searchweb.png (320x180) [85.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM_thm.png (80x40) [9.8 KB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.mp4 (1920x1080) [442.5 MB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.webm (1920x1080) [25.9 MB] || COVIDNO2.en_US.srt [4.4 KB] || COVIDNO2.en_US.vtt [4.4 KB] || ",
            "hits": 83
        },
        {
            "id": 13559,
            "url": "https://svs.gsfc.nasa.gov/13559/",
            "result_type": "Produced Video",
            "release_date": "2020-03-23T10:00:00-04:00",
            "title": "NASA Models Methane Sources and Movement Around the Globe",
            "description": "Complete transcript available.Music: \"Reported Missing\" by Andrew Michael Britton [PRS] and David Stephen Goldsmith [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html. || Methane_Still.jpg (1920x1080) [408.5 KB] || Methane_Still_print.jpg (1024x576) [181.8 KB] || Methane_Still_searchweb.png (180x320) [71.4 KB] || Methane_Still_web.png (320x180) [71.4 KB] || Methane_Still_thm.png (80x40) [6.4 KB] || 13559_Methane_Final.webm (960x540) [62.2 MB] || TWITTER_720_13559_Methane_Final_twitter_720.mp4 (1280x720) [28.5 MB] || 13559_Methane_Final_lowres.mp4 (1280x720) [43.6 MB] || 13559_Methane_Final.mp4 (1920x1080) [272.5 MB] || Mathen_captions.en_US.srt [3.2 KB] || Mathen_captions.en_US.vtt [3.3 KB] || 13559_Methane_Final.mov (1920x1080) [3.4 GB] || ",
            "hits": 81
        },
        {
            "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. || 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] || FACEBOOK_720_13562_Dragonfly_Science_MASTER_facebook_720.mp4 (1280x720) [145.8 MB] || 13562_Dragonfly_Science_CAPTIONS.en_US.srt [3.4 KB] || 13562_Dragonfly_Science_CAPTIONS.en_US.vtt [3.4 KB] || 13562_Dragonfly_Science_4K_Small.mp4 (3840x2160) [363.0 MB] || 13562_Dragonfly_Science_YouTube.mp4 (3840x2160) [2.7 GB] || 13562_Dragonfly_Science_MASTER.mov (3840x2160) [16.6 GB] || ",
            "hits": 127
        },
        {
            "id": 4754,
            "url": "https://svs.gsfc.nasa.gov/4754/",
            "result_type": "Visualization",
            "release_date": "2019-12-09T00:00:00-05:00",
            "title": "The Complex Chemistry of Surface Ozone Depicted in a New GEOS Simulation",
            "description": "96 chemical species are shown from a GEOS atmospheric simulation || gmao_chem_3x3_pass02_09.05630_no_overlay_print.jpg (1024x576) [126.9 KB] || gmao_chem_3x3_pass02_09.05630_no_overlay.png (5760x3240) [2.5 MB] || gmao_chem_3x3_pass02_09.05630_no_overlay_searchweb.png (320x180) [82.3 KB] || gmao_chem_3x3_pass02_09.05630_no_overlay_thm.png (80x40) [6.8 KB] || 1920x1080_16x9_p30 (1920x1080) [0 Item(s)] || gmao_chem_HD_1080p30.webm (1920x1080) [36.0 MB] || gmao_chem_HD_1080p30.mp4 (1920x1080) [267.3 MB] || 9600x3240_16x9_30p (9600x3240) [0 Item(s)] || 3840x2160_16x9_p30 (3840x2160) [0 Item(s)] || gmao_chem_5x3_preview.mp4 (3200x1080) [429.0 MB] || gmao_chem_4k_2160p30.mp4 (3840x2160) [762.1 MB] || gmao_chem_HD_1080p30.mp4.hwshow [212 bytes] || ",
            "hits": 219
        },
        {
            "id": 13784,
            "url": "https://svs.gsfc.nasa.gov/13784/",
            "result_type": "Produced Video",
            "release_date": "2019-11-13T00:00:00-05:00",
            "title": "Seasonal Variations in Oxygen at Gale Crater",
            "description": "For the first time in the history of space exploration, scientists have measured the seasonal changes in the gases that fill the air directly above the surface of Gale Crater on Mars. As a result, they noticed something baffling: oxygen, the gas many Earth creatures use to breathe, behaves in a way that so far scientists cannot explain through any known chemical processes. || ",
            "hits": 205
        },
        {
            "id": 4764,
            "url": "https://svs.gsfc.nasa.gov/4764/",
            "result_type": "Visualization",
            "release_date": "2019-11-07T00:00:00-05:00",
            "title": "Simulation of Surface Ozone",
            "description": "Global surface ozone from a GEOS model run || ozone_only_4k.00000_print.jpg (1024x576) [65.8 KB] || ozone_only_4k.00000_searchweb.png (320x180) [58.9 KB] || ozone_only_4k.00000_thm.png (80x40) [5.1 KB] || ozone_only_1080p30.mp4 (1920x1080) [24.5 MB] || ozone_only_1080p30.webm (1920x1080) [7.2 MB] || ozone_only_2160p30.mp4 (3840x2160) [70.8 MB] || ozone_only (3840x2160) [0 Item(s)] || ozone_only (5760x3240) [0 Item(s)] || ozone_only_1080p30.mp4.hwshow [208 bytes] || ",
            "hits": 81
        },
        {
            "id": 13222,
            "url": "https://svs.gsfc.nasa.gov/13222/",
            "result_type": "B-Roll",
            "release_date": "2019-06-06T00:00:00-04:00",
            "title": "Goddard Astrobiology Analytical Laboratory (Footage)",
            "description": "Highlight reel of the NASA Goddard Astrobiology Analytical Laboratory. Available for download in broadcast-quality Apple ProRes. || Astrobiology_Lab_Preview_print.jpg (1024x576) [151.9 KB] || Astrobiology_Lab_Preview.jpg (1920x1080) [302.5 KB] || Astrobiology_Lab_Preview_searchweb.png (320x180) [98.9 KB] || Astrobiology_Lab_Preview_thm.png (80x40) [7.5 KB] || TWITTER_720_Astrobiology_Lab_Highlights_V2_twitter_720.mp4 (1280x720) [25.1 MB] || Astrobiology_Lab_Highlights_V2.webm (960x540) [59.9 MB] || FACEBOOK_720_Astrobiology_Lab_Highlights_V2_facebook_720.mp4 (1280x720) [159.2 MB] || Astrobiology_Lab_Highlights_V2.mp4 (1920x1080) [233.7 MB] || YOUTUBE_1080_Astrobiology_Lab_Highlights_V2_youtube_1080.mp4 (1920x1080) [220.9 MB] || Astrobiology_Lab_Highlights_V2.mov (1920x1080) [4.5 GB] || ",
            "hits": 29
        },
        {
            "id": 12967,
            "url": "https://svs.gsfc.nasa.gov/12967/",
            "result_type": "Produced Video",
            "release_date": "2018-06-07T13:00:00-04:00",
            "title": "Ancient Organics Discovered on Mars - Broadcast Graphics",
            "description": "NASA-TV graphics illustrating Curiosity's findings on Mars, broadcast on June 7, 2018 from Goddard Space Flight Center. All clips are formatted in 1280x720 or higher resolution. Learn more about this discovery. || ",
            "hits": 298
        },
        {
            "id": 20231,
            "url": "https://svs.gsfc.nasa.gov/20231/",
            "result_type": "Animation",
            "release_date": "2018-05-24T13:00:00-04:00",
            "title": "Mars Organic Molecule Analyzer: Animations",
            "description": "MOMA uses ultraviolet laser pulses to release and ionize organic compounds captured within crushed Martian surface and near-surface materials. Because each laser pulse lasts less than two billionths of a second, this process effectively ionizes more heat-resistant materials than those accessed by traditional oven-heating (pyrolysis) methods. Pulsed laser processing preserves weak molecular bonds, and enables the identification of organic compounds even in the presence of highly reactive perchlorates commonly found in Martian surface materials. || MOMAposterFull.jpg (1920x1080) [130.9 KB] || MOMAposterFull_print.jpg (1024x576) [73.3 KB] || MOMAposterFull_searchweb.png (320x180) [36.8 KB] || MOMAposterFull_web.png (320x180) [36.8 KB] || MOMAposterFull_thm.png (80x40) [3.7 KB] || ldms (1920x1080) [0 Item(s)] || MOMA-LDMS_h264.mp4 (1920x1080) [91.5 MB] || MOMA-LDMS_1080p60.mp4 (1920x1080) [24.4 MB] || MOMA-LDMS_1080p60.webm (1920x1080) [8.3 MB] || MOMA-LDMS.mov (1920x1080) [2.1 GB] || Moma-LDMS.hwshow [67 bytes] || ",
            "hits": 118
        },
        {
            "id": 4184,
            "url": "https://svs.gsfc.nasa.gov/4184/",
            "result_type": "Visualization",
            "release_date": "2014-06-30T00:00:00-04:00",
            "title": "2014 Update Aqua/AIRS Carbon Dioxide with Mauna Loa Carbon Dioxide",
            "description": "This visualization is a time-series of the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft. For comparison, it is overlain by a graph of the seasonal variation and interannual increase of carbon dioxide observed at the Mauna Loa, Hawaii observatory.The graph shows data, commonly called the Keeling Curve, from the Scripps measurements of monthly carbon dioxide concentration at Mauna Loa Observatory. The collection of this data was started by C. David Keeling of the Scripps Institution of Oceanography in March of 1958 at a facility of the National Oceanic and Atmospheric Administration [Keeling, 1976]. The two most notable features of this visualization are the seasonal variation of carbon dioxide and the trend of increase in its concentration from year to year. The global map clearly shows that the carbon dioxide in the Northern Hemisphere peaks in April-May and then drops to a minimum in September-October. Although the seasonal cycle is less pronounced in the Southern Hemisphere it is opposite to that in the Northern Hemisphere. This seasonal cycle is governed by the growth cycle of plants. The Northern Hemisphere has the majority of the land masses, and so the amplitude of the cycle is greater in that hemisphere. The overall color of the map shifts toward the red with advancing time due to the annual increase of carbon dioxide.The concentration of carbon dioxide in the mid-troposphere lags the concentration found at the surface as mixing from the lower to upper altitudes usually takes days to weeks.More information about AIRS can be found at http://airs.jpl.nasa.gov.  More information about the carbon dioxide concentration at Mauna Loa Observatory can be found at http://scrippsco2.ucsd.edu/ || ",
            "hits": 24
        },
        {
            "id": 11217,
            "url": "https://svs.gsfc.nasa.gov/11217/",
            "result_type": "Produced Video",
            "release_date": "2013-03-04T12:00:00-05:00",
            "title": "Cosmic Ice Lab Studies Reactions Occurring in Deep Space",
            "description": "At the NASA Goddard Cosmic Ice Lab, scientists are studying ice to help us understand the unusual chemical reactions that occur in space. Ice in space is amorphous, lacking the crystalline structure of the ice found on Earth. In space, this ice is often dirty, containing different kinds of particles and organic molecules. Recent discoveries have found that compounds trapped in amorphous ice are involved in a kind of chemistry unlike anything known on Earth. At the Goddard Cosmic Ice Lab, scientists are recreating the conditions of space to study the properties of amorphous ice firsthand. Their research will help astronomers to interpret observations of the far reaches of space, and further our understanding of the potential for the existence life beyond Earth. || ",
            "hits": 47
        },
        {
            "id": 3685,
            "url": "https://svs.gsfc.nasa.gov/3685/",
            "result_type": "Visualization",
            "release_date": "2010-03-15T23:00:00-04:00",
            "title": "Aqua/AIRS Carbon Dioxide, 2002-2009, With Mauna Loa Carbon Dioxide Graph",
            "description": "This visualization is a time-series of the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft. For comparison, it is overlain by a graph of the seasonal variation and interannual increase of carbon dioxide observed at the Mauna Loa, Hawaii observatory. The AIRS data show the average concentration (parts per million) over an altitude range of 3 km to 13 km, whereas the Mauna Loa data show the concentration at an altitude of 3.4 km and its annual increase at a rate of approximately 2 parts per million (ppm) per year. The two most notable features of this visualization are the seasonal variation of CO2 and the trend of increase in its concentration from year to year. The global map clearly shows that the CO2 in the northern hemisphere peaks in April-May and then drops to a minimum in September-October. Although the seasonal cycle is less pronounced in the southern hemisphere it is opposite to that in the northern hemisphere. This seasonal cycle is governed by the growth cycle of plants. The northern hemisphere has the majority of the land masses, and so the amplitude of the cycle is greater in that hemisphere. The overall color of the map shifts toward the red with advancing time due to the annual increase of CO2. Although the mid-latitude jet streams are not visible in the map, we can see their influence upon the distribution of CO2 around the globe. These rivers of air occur at an altitude of about 5 km and rapidly transport CO2 around the globe at that altitude. In the northern hemisphere, the mid-latitude jet stream squirms like a released garden hose over the period of a few days due to the continental landmasses. In the southern hemisphere the jet stream flow is more directly West to East, and during the period from July to October the CO2 concentration is enhanced in a belt delineated by the jet stream and lofting of CO2 into the free troposphere by the high Andes is visible in this period. The zonal flow of CO2 around the globe at the latitude of South Africa, southern Australia and southern South America is readily apparent. Eastward flow of CO2 from Indonesia and the Celebes sea can be seen in the November to February time frame. || ",
            "hits": 127
        },
        {
            "id": 10474,
            "url": "https://svs.gsfc.nasa.gov/10474/",
            "result_type": "Produced Video",
            "release_date": "2009-07-27T00:00:00-04:00",
            "title": "Hubble Career Profiles",
            "description": "These profiles begin to explore what systems engineering is as seen through the roles of Benjamin Reed and Jackie Townsend on the Hubble Space Telescope. Reed is a materials assurance engineer who has a background in chemistry and has most recently worked on improving Hubble's outer blanket layer. Townsend came to Goddard with a background in physics and has served as the instrument manager of Hubble's newest imager, Wide Field Camera 3. Through their personal backgrounds and current work, Reed and Townsend show that great engineers share patience, tenacity, and a passion for problem solving. || ",
            "hits": 34
        },
        {
            "id": 3562,
            "url": "https://svs.gsfc.nasa.gov/3562/",
            "result_type": "Visualization",
            "release_date": "2008-10-08T23:00:00-04:00",
            "title": "Aqua/AIRS Carbon Dioxide with Mauna Loa Carbon Dioxide Overlaid",
            "description": "A NASA/university study of the first-ever global satellite maps of carbon dioxide in Earth's atmosphere has revealed new information on how this key greenhouse gas linked to climate change is distributed and moves around our world. Moustafa Chahine, lead study author and AIRS science team leader at NASA's Jet Propulsion Laboratory, Pasadena, Calif., said the maps, which cover from September 2002 to July 2008, will be used by scientists to refine how climate models represent the processes that transport carbon dioxide within Earth's atmosphere. 'These data capture global variations in the distribution of carbon dioxide over time that are not represented in the existing models used to determine where carbon dioxide is created and stored,' he said. Chahine said the previous scientific consensus was that carbon dioxide was evenly mixed in the free troposphere, decreasing as you move farther south of the equator. 'Our results show carbon dioxide there can vary by nearly one percent and that the free troposphere is like international waters-what's produced in one place is free to travel elsewhere,' he said.This visualization is a time-series of the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft. For comparison, it is overlain by a graph of the seasonal variation and interannual increase of carbon dioxide observed at the Mauna Loa, Hawaii observatory. The AIRS data show the average concentration (parts per million) over an altitude range of 3 km to 13 km, whereas the Mauna Loa data show the concentration at an altitude of 3.4 km and its annual increase at a rate of approximately 2 parts per million (ppmv) per year. The two most notable features of this visualization are the seasonal variation of CO2 and the trend of increase in its concentration from year to year. The global map clearly shows that the CO2 in the northern hemisphere peaks in April-May and then drops to a minimum in September-October. Although the seasonal cycle is less pronounced in the southern hemisphere it is opposite to that in the northern hemisphere. This seasonal cycle is governed by the growth cycle of plants. The northern hemisphere has the majority of the land masses, and so the amplitude of the cycle is greater in that hemisphere. The overall color of the map shifts toward the red with advancing time due to the annual increase of CO2. Although the mid-latitude jet streams are not visible in the map, we can see their influence upon the distribution of CO2 around the globe. These rivers of air occur at an altitude of about 5 km and rapidly transport CO2 around the globe at that altitude. In the northern hemisphere, the mid-latitude jet stream squirms like a released garden hose over the period of a few days due to the continental landmasses. In the southern hemisphere the jet stream flow is more directly West to East, and during the period from July to October the CO2 concentration is enhanced in a belt delineated by the jet stream and lofting of CO2 into the free troposphere by the high Andes is visible in this period. The zonal flow of CO2 around the globe at the latitude of South Africa, southern Australia and southern South America is readily apparent. Eastward flow of CO2 from Indonesia and the Celebes sea can be seen in the November to February time frame. || ",
            "hits": 29
        },
        {
            "id": 3555,
            "url": "https://svs.gsfc.nasa.gov/3555/",
            "result_type": "Visualization",
            "release_date": "2008-10-08T00:00:00-04:00",
            "title": "Aqua/AIRS Sees Belt of Carbon Dioxide in Southern Hemisphere with Winds",
            "description": "Although originally designed to measure atmospheric water vapor and temperature profiles for weather forecasting, data from the Atmospheric Infrared Sounder (AIRS) instrument on NASA's Aqua spacecraft are now also being used by scientists to observe atmospheric carbon dioxide. This visualization shows Aqua/AIRS mid-tropospheric carbon dioxide from July 2003. Low concentrations, 360 ppm, are shown in blue and high concentrations, 385 ppm, are shown in red. Notice that despite carbon dioxide's high degree of mixing, the regional patterns of atmospheric sources and sinks are still apparent in mid-troposphere carbon dioxide concentrations.  In the southern hemisphere the jet stream flow is more directly West to East, and during the period from July to October the CO2 concentration is enhanced in a belt delineated by the jet stream and lofting of CO2 into the free troposphere by the high Andes is visible in this period. The zonal flow of CO2 around the globe at the latitude of South Africa, southern Australia and southern South America is readily apparent.For more information on AIRS, visit the AIRS Project Web Site: http://airs.jpl.nasa.gov. The AIRS data products are available at http://daac.gsfc.nasa.gov/AIRS/index.shtml. || ",
            "hits": 22
        },
        {
            "id": 3554,
            "url": "https://svs.gsfc.nasa.gov/3554/",
            "result_type": "Visualization",
            "release_date": "2008-10-07T16:00:00-04:00",
            "title": "Aqua/AIRS Sees Belt of Carbon Dioxide in Southern Hemisphere",
            "description": "Although originally designed to measure atmospheric water vapor and temperature profiles for weather forecasting, data from the Atmospheric Infrared Sounder (AIRS) instrument on NASA's Aqua spacecraft are now also being used by scientists to observe atmospheric carbon dioxide. In the southern hemisphere, a belt of mid-tropospheric air containing enhanced concentrations of carbon dioxide emerged between 30 and 40 degrees south latitude. This belt had not previously been seen in any chemistry transport model. Subtropical storms track through this region, as do the cloud bands of the intertropical convergence zone near the equator, an area of low atmospheric pressure that forms where northeast and southeast trade winds meet.The researchers believe strong convection (thunderstorms) in this belt, and South America's high Andes Mountains, lift carbon dioxide from major sources on Earth's surface, such as the respiration of plants, forest fires and facilities for producing synthetic fuels and generating power. This carbon dioxide is then carried into the 'free troposphere,' the part of the troposphere that is too high to be influenced by Earth's surface. There, it becomes trapped in the mid-latitude jet stream, which transports it rapidly around the world. For more information on AIRS, visit the AIRS Project Web Site: http://airs.jpl.nasa.gov. The AIRS data products are available at http://daac.gsfc.nasa.gov/AIRS/index.shtml. || ",
            "hits": 15
        },
        {
            "id": 3440,
            "url": "https://svs.gsfc.nasa.gov/3440/",
            "result_type": "Visualization",
            "release_date": "2007-12-30T12:00:00-05:00",
            "title": "Aqua/AIRS Global Carbon Dioxide",
            "description": "Although originally designed to measure atmospheric water vapor and temperature profiles for weather forecasting, data from the Atmospheric Infrared Sounder (AIRS) instrument on NASA's Aqua spacecraft are now also being used by scientists to observe atmospheric carbon dioxide. Scientists from NASA; the National Oceanic and Atmospheric Administration; the European Center for Medium-Range Weather Forecasts; the University of Maryland, Baltimore County; Princeton University, Princeton, New Jersey; and the California Institute of Technology (Caltech), Pasadena, Calif., are using several different methods to measure the concentration of carbon dioxide in the mid-troposphere (about eight kilometers, or five miles, above the surface).  This visualization shows Aqua/AIRS mid-tropospheric carbon dioxide from July 2003.  Low concentrations, 360 ppm,  are shown in blue and high concentrations, 385 ppm, are shown in red.   Notice that despite carbon dioxide's  high degree of mixing, the regional patterns of atmospheric sources and sinks are still apparent in mid-troposphere carbon dioxide concentrations. This pattern of high carbon dioxide in the Northern Hemisphere (North America, Atlantic Ocean, and Central Asia) is consistent with model predictions.For more information on AIRS, visit the AIRS Project Web Site: http://airs.jpl.nasa.gov. The AIRS data products are available at http://daac.gsfc.nasa.gov/AIRS/index.shtml. || ",
            "hits": 19
        },
        {
            "id": 3441,
            "url": "https://svs.gsfc.nasa.gov/3441/",
            "result_type": "Visualization",
            "release_date": "2007-12-30T12:00:00-05:00",
            "title": "Aqua/AIRS Carbon Dioxide with Winds",
            "description": "Although originally designed to measure atmospheric water vapor and temperature profiles for weather forecasting, data from the Atmospheric Infrared Sounder (AIRS) instrument on NASA's Aqua spacecraft are now also being used by scientists to observe atmospheric carbon dioxide. Scientists from NASA; the National Oceanic and Atmospheric Administration; the European Center for Medium-Range Weather Forecasts; the University of Maryland, Baltimore County; Princeton University, Princeton, New Jersey; and the California Institute of Technology (Caltech), Pasadena, Calif., are using several different methods to measure the concentration of carbon dioxide in the mid-troposphere (about eight kilometers, or five miles, above the surface). This visualization shows Aqua/AIRS mid-tropospheric carbon dioxide from July 2003. Low concentrations, 360 ppm, are shown in blue and high concentrations, 385 ppm, are shown in red. Notice that despite carbon dioxide's high degree of mixing, the regional patterns of atmospheric sources and sinks are still apparent in mid-troposphere carbon dioxide concentrations. This pattern of high carbon dioxide in the Northern Hemisphere (North America, Atlantic Ocean, and Central Asia) is consistent with model predictions.For more information on AIRS, visit the AIRS Project Web Site: http://airs.jpl.nasa.gov. The AIRS data products are available at http://daac.gsfc.nasa.gov/AIRS/index.shtml. || ",
            "hits": 16
        },
        {
            "id": 10133,
            "url": "https://svs.gsfc.nasa.gov/10133/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Helium Atom",
            "description": "Helium nuclei were created in the Big Bang and contain two protons and two neutrons each. Helium is the second most abundant element, comprising roughly one quarter of the mass of the Universe. This animation zooms into a standard helium atom, showing its protons (green), neutrons (white), and electrons (blue). || ",
            "hits": 282
        },
        {
            "id": 3112,
            "url": "https://svs.gsfc.nasa.gov/3112/",
            "result_type": "Visualization",
            "release_date": "2005-02-15T12:00:00-05:00",
            "title": "Aral Sea Evaporation (WMS)",
            "description": "The Aral Sea is actually not a sea at all, but an immense fresh water lake. In the last thirty years, more than sixty percent of the lake has disappeared because much of the river flow feeding the lake was diverted to irrigate cotton fields and rice paddies. Concentrations of salts and minerals began to rise in the shrinking body of water, leading to staggering alterations in the lake's ecology and precipitous drops in the Aral's fish population. Powerful winds that blow across this part of Asia routinely pick up and deposit the now exposed lake bed soil. This has contributed to a significant reduction in breathable air quality, and crop yields have been appreciably affected due to heavily salt laden particles falling on arable land. This series of Landsat images taken in 1973, 1987 and 2000 show the profound reduction in overall area at the north end of the Aral, and a commensurate increase in land area as the floor of the sea now lies exposed. || ",
            "hits": 61
        },
        {
            "id": 2623,
            "url": "https://svs.gsfc.nasa.gov/2623/",
            "result_type": "Visualization",
            "release_date": "2002-10-15T12:00:00-04:00",
            "title": "West Coast Chlorophyll Bloom",
            "description": "Sea-viewing Wide Field-of-view Sensor (SeaWiFS) on board the Orbview 2 satellite captured the phytoplankton bloom October 6, 2002 .  Red represents high concentration of chlorophyll, follow by orange, yellow and green. Land and cloud portions of the image are presented in natural color.SeaWiFS monitors ocean plant life by measuring the amount of chlorophyll in the ocean.  Large phytoplankton blooms tend to coincide with natural phenomena that drive that nutrient-rich water to the surface. The process is called upwelling.  Winds coming off principal land masses push surface layers of water away from the shore. Into the resulting wind-driven void deeper water underneath the surface layers rushes in toward the coast, bringing with it nutrients for life to bloom.  This upwelling fuel the growth of marine phytoplankton which, along with larger seaweeds, nourishes the incredible diversity of creatures found along the northern and central California coast. || ",
            "hits": 31
        },
        {
            "id": 2105,
            "url": "https://svs.gsfc.nasa.gov/2105/",
            "result_type": "Visualization",
            "release_date": "2001-04-19T12:00:00-04:00",
            "title": "Dramatic Evaporation of the Aral Sea",
            "description": "Disappearing Water: The Aral Sea Over Time (From 1973 to 2001) A time series is a powerful illustrative tool. Where in the case of Las Vegas we see the direct effects of people on the land, in the case of the Aral Sea, separating the countries of Kazakhstan and Uzbekistan, we see indirect, but no less dramatic effects on a different part of the world. The Aral Sea is actually not a sea at all. It is an immense lake, a body of fresh water, although that particular description of its contents might now be more a figure of speech than practical fact. In the last thirty years, more than sixty percent of the lake has disappeared. As you'll see in the visualization, the change over time is dramatic. In the 1970s, farmers and state offices opened significant diversions from the rivers supplying water to the lake, sending millions of gallons to irrigate cotton fields and rice paddies. So voluminous were these irrigation sluices that concentrations of salts and minerals began to rise in the shrinking body of water. That change in chemistry has led to staggering alterations in the lake's ecology, causing precipitous drops in the Aral's fish population. A secondary effect of this reduction in the Aral Sea's overall size is the rapid exposure of the lake bed. Powerful winds that blow across this part of Asia routinely pick up and deposit tens of thousands of tons of now exposed soil every year. This has not only contributed to significant reduction in breathable air quality for nearby residents, but also appreciably affected crop yields due to those heavily salt laden particles falling on arable land. In the following sequence of images, we see a series of Landsat scenes taken several years apart. As the years pass, we see the profound reduction in overall area covered by the Aral, and a commensurate increase in land area as the floor of the sea now lies exposed. || ",
            "hits": 174
        },
        {
            "id": 2117,
            "url": "https://svs.gsfc.nasa.gov/2117/",
            "result_type": "Visualization",
            "release_date": "2001-04-19T12:00:00-04:00",
            "title": "Dramatic Evaporation of the Aral Sea (With Dates)",
            "description": "Disappearing Water: The Aral Sea Over Time (From 1973 to 2001) A time series is a powerful illustrative tool. Where in the case of Las Vegas we see the direct effects of people on the land, in the case of the Aral Sea, separating the countries of Kazakhstan and Uzbekistan, we see indirect, but no less dramatic effects on a different part of the world. The Aral Sea is actually not a sea at all. It is an immense lake, a body of fresh water, although that particular description of its contents might now be more a figure of speech than practical fact. In the last thirty years, more than sixty percent of the lake has disappeared. As you'll see in the visualization, the change over time is dramatic. In the 1970s, farmers and state offices opened significant diversions from the rivers supplying water to the lake, sending millions of gallons to irrigate cotton fields and rice paddies. So voluminous were these irrigation sluices that concentrations of salts and minerals began to rise in the shrinking body of water. That change in chemistry has led to staggering alterations in the lake's ecology, causing precipitous drops in the Aral's fish population. A secondary effect of this reduction in the Aral Sea's overall size is the rapid exposure of the lake bed. Powerful winds that blow across this part of Asia routinely pick up and deposit tens of thousands of tons of now exposed soil every year. This has not only contributed to significant reduction in breathable air quality for nearby residents, but also appreciably affected crop yields due to those heavily salt laden particles falling on arable land. In the following sequence of images, we see a series of Landsat scenes taken several years apart. As the years pass, we see the profound reduction in overall area covered by the Aral, and a commensurate increase in land area as the floor of the sea now lies exposed. || ",
            "hits": 143
        },
        {
            "id": 579,
            "url": "https://svs.gsfc.nasa.gov/579/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS: The Upper Atmosphere Research Satellite",
            "description": "This video summarizes science and data obtained by the Upper Atmosphere Research Satellite (UARS) mission.  UARS was launched in 1991 to study ozone depletion and the processes that control the stratospheric ozone layer.  Although the mission was intended to last only 18 months, UARS continued to operate 7.5 years after launch with 8 of the 10 instruments at the time this video was made. UARS has been one of the most successful NASA satellite programs. The spacecraft was developed and is managed by NASA's Goddard Space Flight Center. || ",
            "hits": 58
        },
        {
            "id": 823,
            "url": "https://svs.gsfc.nasa.gov/823/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of O2 being Broken Up and Reforming as O3",
            "description": "Ozone is formed when high energy ultra-violet radiation from the sun breaks apart  molecular oxygen.  An oxygen atom then combines with an oxygen molecule producing a new molecule with three atoms of oxygen, ozone. || ",
            "hits": 623
        },
        {
            "id": 837,
            "url": "https://svs.gsfc.nasa.gov/837/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Ozone and Chlorine Monoxide over Antarctica from MLS (1/12/93 - 9/17/93)",
            "description": "The  Microwave Limb Sounder (MLS) measures microwave emission from ozone and chlorine monoxide, a major ozone destroying radical.  Right after UARS was launched, MLS began to measure large concentrations of chlorine monoxide over the south pole.  These dramatic images clearly showed the extent of the south polar ozone destruction and confirmed the connection between man-made chlorine and the formation to  the Antarctic ozone hole. Why is so much  chlorine monoxide found over the Antarctic?  UARS measurements have confirmed that CFCs enter the stratosphere in the tropics.  As they rise above the ozone layer, ultraviolet molecules release chlorine, which then can react with methane to form hydrogen chloride.  Chlorine can also react with ozone forming the radical chlorine monoxide.  Chlorine monoxide then combines with the radical nitrogen dioxide to form stable chlorine nitrate.  Chlorine nitrate and hydrogen chloride are called reservoir gases for the chlorine radical.  These reservoir gases usually contain more than ninety percent of the chlorine in the lower stratosphere. || ",
            "hits": 139
        },
        {
            "id": 182,
            "url": "https://svs.gsfc.nasa.gov/182/",
            "result_type": "Visualization",
            "release_date": "1998-01-01T12:00:00-05:00",
            "title": "Positron-electron Annihilation",
            "description": "Animation of positron-electron annihilation || a000182.00030_print.png (720x480) [453.0 KB] || a000182_pre.jpg (320x242) [5.2 KB] || a000182.webmhd.webm (960x540) [1.7 MB] || a000182.dv (720x480) [35.5 MB] || a000182.mp4 (640x480) [2.0 MB] || a000182.mpg (352x240) [1.4 MB] || ",
            "hits": 512
        },
        {
            "id": 1603,
            "url": "https://svs.gsfc.nasa.gov/1603/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Support Animations/Stills for SOLVE",
            "description": "The polar vortex || Vortex.jpg (640x480) [47.7 KB] || newVORTEX_pre.jpg (320x240) [9.5 KB] || Vortex_thm.png (80x40) [5.5 KB] || newVORTEX_pre_searchweb.jpg (180x320) [66.0 KB] || newVORTEX.webmhd.webm (960x540) [1.6 MB] || Vortex.tif (640x480) [253.9 KB] || newVORTEX.mov (320x240) [4.2 MB] || ",
            "hits": 26
        }
    ]
}