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            "id": 14111,
            "url": "https://svs.gsfc.nasa.gov/14111/",
            "result_type": "Produced Video",
            "release_date": "2022-02-28T07:00:00-05:00",
            "title": "Webb's Mid-Infrared Instrument (MIRI) Light Path Animation",
            "description": "The spectrograph light path inside the Mid Infrared Instrument (MIRI) on the Webb Telescope.  Versions with labels and without labels.Credit:  European Space Agency || MIRI_SPECTRO_v2.00030_print.jpg (1024x576) [40.5 KB] || MIRI_SPECTRO_v2.00030_searchweb.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_web.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_thm.png (80x40) [2.1 KB] || MIRI_SPECTRO_v2.mp4 (1920x1080) [156.3 MB] || MIRI_SPECTRO_labels_v3.mp4 (1920x1080) [177.9 MB] || MIRI_SPECTRO_v2.webm (1920x1080) [9.0 MB] || ",
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        {
            "id": 13970,
            "url": "https://svs.gsfc.nasa.gov/13970/",
            "result_type": "B-Roll",
            "release_date": "2021-10-21T00:00:00-04:00",
            "title": "Webb Journey to Space Part 3 Arrival & Off loaded",
            "description": "The MN Colibri with the Webb Telescope safely inside the cargo hold has arrived at Kourou in French Guiana, the location of the launch site for Webb.  The journey from Los Angeles to Kourou took a total of 16 days.  Once the MN Colibri made port, the team of engineers unload Webb still inside the protective transport container from the ship and moved it to Guiana Space Centre. || ",
            "hits": 27
        },
        {
            "id": 13532,
            "url": "https://svs.gsfc.nasa.gov/13532/",
            "result_type": "Produced Video",
            "release_date": "2020-01-27T16:00:00-05:00",
            "title": "Solar Orbiter's Orbit",
            "description": "An animation showing the trajectory of Solar Orbiter around the Sun, highlighting the gravity assist manoeuvres that will enable the spacecraft to change inclination to observe the Sun from different perspectives.During the initial cruise phase, which lasts until November 2021, Solar Orbiter will perform two gravity-assist manoeuvres around Venus and one around Earth to alter the spacecraft’s trajectory, guiding it towards the innermost regions of the Solar System. At the same time, Solar Orbiter will acquire in situ data and characterise and calibrate its remote-sensing instruments. The first close solar pass will take place in 2022 at around a third of Earth’s distance from the Sun.The spacecraft’s orbit has been chosen to be ‘in resonance’ with Venus, which means that it will return to the planet’s vicinity every few orbits and can again use the planet’s gravity to alter or tilt its orbit. Initially Solar Orbiter will be confined to the same plane as the planets, but each encounter of Venus will increase its orbital inclination. For example, after the 2025 Venus encounter it will make its first solar pass at 17º inclination, increasing to 33º during a proposed mission extension phase, bringing even more of the polar regions into direct view. || ",
            "hits": 124
        },
        {
            "id": 13505,
            "url": "https://svs.gsfc.nasa.gov/13505/",
            "result_type": "Produced Video",
            "release_date": "2019-12-11T15:00:00-05:00",
            "title": "Solar Orbiter - ESA Animations",
            "description": "Solar Orbiter is an European Space Agency (ESA) mission with strong NASA participation. Its mission is to perform unprecedented close-up observations of the Sun and from high-latitudes, providing the first images of the uncharted polar regions of the Sun, and investigating the Sun-Earth connection. || ",
            "hits": 260
        },
        {
            "id": 12981,
            "url": "https://svs.gsfc.nasa.gov/12981/",
            "result_type": "Produced Video",
            "release_date": "2018-06-11T13:00:00-04:00",
            "title": "Webb Telescope Optical Telescope Element Engineering History Presentation Supporting Video",
            "description": "Supporting produced video for Webb Telescope Optical Telescope Element Engineering History presentation. || OTE-Engineering-History.00150_print.jpg (1024x576) [59.7 KB] || OTE-Engineering-History.00150_searchweb.png (320x180) [48.0 KB] || OTE-Engineering-History.00150_web.png (320x180) [48.0 KB] || OTE-Engineering-History.00150_thm.png (80x40) [4.6 KB] || OTE-Engineering-History.mp4 (1920x1080) [255.0 MB] || OTE-Engineering-History.webm (1920x1080) [27.0 MB] || OTE-Engineering-History-close_cap-SRT.en_US.srt [2.3 KB] || OTE-Engineering-History-close_cap-SRT.en_US.vtt [2.3 KB] || ",
            "hits": 29
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        {
            "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": 119
        },
        {
            "id": 12453,
            "url": "https://svs.gsfc.nasa.gov/12453/",
            "result_type": "Produced Video",
            "release_date": "2017-04-17T13:00:00-04:00",
            "title": "NASA Team Explores Using LISA Pathfinder as a 'Comet Crumb' Detector",
            "description": "In a proof-of-concept study, NASA scientists are exploring using the European Space Agency's LISA Pathfinder spacecraft as a micrometeoroid detector. When tiny particles shed by asteroids and comets impact LISA Pathfinder, its thrusters work to quickly counteract any change in the spacecraft's motion. Researchers are monitoring these signals to learn more about the impacting particles.Credit: NASA's Goddard Space Flight CenterMusic: \"Electrovoltaic\" and \"Disks in the Sky\" from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || LPF_MM_Still_print.jpg (1024x576) [49.7 KB] || LPF_MM_Still.jpg (3840x2160) [516.9 KB] || LPF_MM_Still.png (3840x2160) [12.0 MB] || LPF_MM_Still_thm.png (80x40) [3.6 KB] || LPF_MM_Still_web.png (320x180) [36.9 KB] || LPF_MM_Still_searchweb.png (320x180) [36.9 KB] || 12453_LISA_Pathfinder_MM_FINAL2_youtube_hq.mov (1920x1080) [781.6 MB] || 12453_LISA_Pathfinder_MM_FINAL2-Compatible.webm (960x540) [27.3 MB] || 12453_LISA_Pathfinder_MM_FINAL_appletv_subtitles.m4v (1280x720) [136.2 MB] || WMV_12453_LISA_Pathfinder_MM_FINAL2_HD.wmv (1920x1080) [125.2 MB] || 12453_LISA_Pathfinder_MM_FINAL2-Compatible.m4v (960x540) [98.3 MB] || 12453_LISA_Pathfinder_MM_FINAL2_appletv.m4v (1280x720) [136.1 MB] || 12453_LISA_Pathfinder_MM_FINAL2_1080.m4v (1920x1080) [258.2 MB] || 12453_LISA_Pathfinder_MM_FINAL2_Good_1080p.mov (1920x1080) [386.0 MB] || 12453_LISA_Pathfinder_MM_FINAL2_ProRes_1920x1080_2997.mov (1920x1080) [3.4 GB] || 12453_LISA_Pathfinder_MM_SRT-Captions.en_US.vtt [4.5 KB] || 12453_LISA_Pathfinder_MM_SRT-Captions.en_US.srt [4.5 KB] || ",
            "hits": 40
        },
        {
            "id": 12286,
            "url": "https://svs.gsfc.nasa.gov/12286/",
            "result_type": "Produced Video",
            "release_date": "2016-06-20T11:00:00-04:00",
            "title": "Instagram: The Electric Wind of Venus",
            "description": "In many ways, Venus is the most similar planet to Earth. Not only are its size and gravity comparable to Earth’s, but there’s evidence that Venus once had lots of water – oceans’ worth! – in the distant past. So what happened? New NASA-funded research using data from ESA’s Venus Express reveal that it may have been Venus’ electric field that stripped the planet of water. Venus’ electric field is about 5-10 times stronger than Earth’s. That electric force is enough to rip particles – including the building blocks of water – out of Venus’ atmosphere. Over time, this “electric wind” could leave a watery planet bone-dry, making it a key factor in whether or not a planet is hospitable to life. Understanding this process will help scientists pinpoint where potentially habitable planets could be lurking around other stars. || ",
            "hits": 100
        },
        {
            "id": 4414,
            "url": "https://svs.gsfc.nasa.gov/4414/",
            "result_type": "Visualization",
            "release_date": "2016-03-21T12:30:00-04:00",
            "title": "The Mars Fleet",
            "description": "A fleet of landers, rovers, and orbiters is exploring the Red Planet, providing mission controllers with a remote presence on Mars. This visualization is available for download in 4K Ultra HD. || MarsFleetClosePreview.jpg (1920x1080) [168.3 KB] || MarsFleetClosePreview_searchweb.png (320x180) [55.1 KB] || MarsFleetClosePreview_thm.png (80x40) [5.4 KB] || Mars_Fleet_SVS_4414.00015_searchweb.png (320x180) [66.1 KB] || mars_fleet_Mar2016_4k_2160p30.00015_searchweb.png (320x180) [61.1 KB] || mars_fleet_Mar2016_HD_1080p60.mp4 (1920x1080) [14.9 MB] || version1 (1920x1080) [0 Item(s)] || mars_fleet_Jan2016_1080p30.webm (1920x1080) [4.3 MB] || mars_fleet_Mar2016_4k_2160p30.mp4 (3840x2160) [48.6 MB] || mars_fleet_Mar2016_640x360.m4v (640x360) [6.7 MB] || version1 (3840x2160) [0 Item(s)] || Mars_Fleet_SVS_4414.mov (1920x1080) [1.2 GB] || Mars_Fleet_SVS_4414_4k.mov (3840x2160) [4.6 GB] || mars-fleet-and-landings.hwshow || mars_solar_wind_compiled.hwshow || ",
            "hits": 103
        },
        {
            "id": 11906,
            "url": "https://svs.gsfc.nasa.gov/11906/",
            "result_type": "Produced Video",
            "release_date": "2015-06-24T12:00:00-04:00",
            "title": "NASA On Air: NASA Aids European Space Agency In Measuring Upper Air Arctic Winds (6/24/2015)",
            "description": "LEAD: In 2016 the European Space Agency, ESA, will launch a ‘first-of-its-kind' satellite to measure key elements in the earth's wind fields.1. The Aeolus satellite, named after the mythical Greek god of the winds, will measure worldwide upper level winds to help improve weather and climate forecasts.2. NASA recently helped ESA calibrate its new wind instrument by taking simultaneous wind measurements with two Doppler lidars aboard its DC-8 aircraft.TAG: The flights focused over the Arctic since this area holds particular interest due to the continued rise in Arctic temperatures. || WC_Aeolus-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [101.4 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [68.2 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_web.png (320x180) [68.2 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_thm.png (80x40) [5.7 KB] || WC_Aeolus-1920-MASTER_1920x1080.mov (1920x1080) [625.6 MB] || WC_Aeolus-1920-MASTER_1280x720.mov (1280x720) [711.7 MB] || WC_Aeolus-1920-MASTER_NBC_Today.mov (1920x1080) [269.7 MB] || WC_Aeolus-1920-MASTER_WEA_CEN.wmv (1280x720) [16.1 MB] || WC_Aeolus_converted.avi (1280x720) [16.8 MB] || WC_Aeolus-1920-MASTER_baron.mp4 (1920x1080) [12.6 MB] || WC_Aeolus-1920-MASTER_prores.mov (1920x1080) [435.3 MB] || WC_Aeolus-1920-MASTER_iPad_960x540.m4v (960x540) [80.1 MB] || WC_Aeolus-1920-MASTER_iPad_1280x720.m4v (1280x720) [134.5 MB] || WC_Aeolus-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [269.7 MB] || WC_Aeolus-1920-MASTER_iPad_1920x0180.webm (1920x1080) [3.1 MB] || ",
            "hits": 29
        },
        {
            "id": 11570,
            "url": "https://svs.gsfc.nasa.gov/11570/",
            "result_type": "Produced Video",
            "release_date": "2014-06-16T10:00:00-04:00",
            "title": "JWST ISIM Structure moves into SES <br>for Second Cryogenic Test",
            "description": "Engineers move the heart of the Webb Telescope holding all four science instruments out of the clean room at NASA's Goddard Space Flight Center and into the huge Space Environment Simulator for several months of testing at temperatures reaching 20 Kelvin or -425 Fahrenheit. || ",
            "hits": 34
        },
        {
            "id": 10956,
            "url": "https://svs.gsfc.nasa.gov/10956/",
            "result_type": "B-Roll",
            "release_date": "2012-04-09T00:00:00-04:00",
            "title": "Webb Telescope Flight Mirror Cryogenic Testing at Marshall Space Flight Center",
            "description": "The Webb Telescope's primary mirror has 18 hexagonal mirror segments. This footage taken at the NASA Marshall Space Flight Center shows 6 primary mirror segments being prepared readied for cryogenic testing. || ",
            "hits": 29
        }
    ]
}