{
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    "results": [
        {
            "id": 15084,
            "url": "http://svs.gsfc.nasa.gov/15084/",
            "result_type": "Visualization",
            "release_date": "2026-08-30T00:00:00-04:00",
            "title": "Brunei Bay Boats",
            "description": "Brunei Bay, located on the northwest coast of Borneo, serves as a major anchorage for commercial vessels, including large cargo ships and oil tankers. This time series of Harmonized Landsat and Sentinel-2 (HLS) imagery captures the dynamic nature of this maritime hub. As ships arrive, wait at anchor, and eventually depart, changing ocean currents and tides cause the anchored vessels to rotate and sway, creating a dynamic display of ship traffic over time.",
            "hits": 89
        },
        {
            "id": 5625,
            "url": "http://svs.gsfc.nasa.gov/5625/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami",
            "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.",
            "hits": 105
        },
        {
            "id": 5626,
            "url": "http://svs.gsfc.nasa.gov/5626/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)",
            "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.",
            "hits": 69
        },
        {
            "id": 14634,
            "url": "http://svs.gsfc.nasa.gov/14634/",
            "result_type": "Produced Video",
            "release_date": "2024-07-25T14:00:00-04:00",
            "title": "Fermi Finds Novel Feature in BOAT Gamma-Ray Burst",
            "description": "The brightest gamma-ray burst yet recorded gave scientists a new high-energy feature to study. Learn what NASA’s Fermi mission saw, and what this feature may be telling us about the burst’s light-speed jets. Credit: NASA's Goddard Space Flight CenterMusic: “Tides,” Jon Cotton [PRS] and Ben Niblett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Distant_GRB_still.jpg (3840x2160) [2.5 MB] || 14634_Fermi_GRB_Emission_Line_Under100.mp4 (1920x1080) [90.7 MB] || 14634_Fermi_GRB_Emission_Line_Best.mp4 (1920x1080) [422.0 MB] || 14634FermiGRBEmissionLine_Captions.en_US.srt [4.4 KB] || 14634FermiGRBEmissionLine_Captions.en_US.vtt [4.2 KB] || 14634_Fermi_GRB_Emission_Line_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || ",
            "hits": 71
        },
        {
            "id": 14408,
            "url": "http://svs.gsfc.nasa.gov/14408/",
            "result_type": "Produced Video",
            "release_date": "2023-09-07T11:00:00-04:00",
            "title": "Swift Spots a Snacking Black Hole Using a New Trick",
            "description": "Watch to learn how an update to NASA’s Neil Gehrels Swift Observatory allowed it to catch a supersized black hole in a distant galaxy munching repeatedly on a circling star. Credit: NASA’s Goddard Space Flight CenterMusic: \"Teapot Waltz\" by Benjamin Parsons from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Repeating_TDE_Still.jpg (1920x1080) [446.8 KB] || Repeating_TDE_Still_searchweb.png (320x180) [63.3 KB] || Repeating_TDE_Still_thm.png (80x40) [4.6 KB] || 14408_Repeating_TDE_sub100.mp4 (1920x1080) [89.7 MB] || Repeating_TDE_SRT_Captions.en_US.srt [1.7 KB] || Repeating_TDE_SRT_Captions.en_US.vtt [1.6 KB] || 14408_Repeating_TDE_ProRes_1920x1080_2997.mov (1920x1080) [1.2 GB] || 14408_Repeating_TDE_1080.mp4 (1920x1080) [186.2 MB] || ",
            "hits": 100
        },
        {
            "id": 40462,
            "url": "http://svs.gsfc.nasa.gov/gallery/cosmic-cycles3-earthas-art/",
            "result_type": "Gallery",
            "release_date": "2023-05-01T00:00:00-04:00",
            "title": "Cosmic Cycles 3 Earth as Art",
            "description": "Starting in 1972, nine Landsat satellites have orbited Earth, taking images of the surface. This unprecedented coverage has been tremendously useful to the scientific community, but it has also produced thousands of beautiful high-resolution images of the complex patterns of our world. From the fractal patterns of mountain ranges and river deltas to the precise geometry of agriculture, Landsat has rendered Earth as a work of art.",
            "hits": 32
        },
        {
            "id": 14132,
            "url": "http://svs.gsfc.nasa.gov/14132/",
            "result_type": "Produced Video",
            "release_date": "2022-04-12T00:00:00-04:00",
            "title": "Black Hole Week: Black Hole GIFs",
            "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ",
            "hits": 385
        },
        {
            "id": 14095,
            "url": "http://svs.gsfc.nasa.gov/14095/",
            "result_type": "Produced Video",
            "release_date": "2022-02-09T09:00:00-05:00",
            "title": "NASA’s New Views of Venus’ Surface From Space",
            "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ",
            "hits": 524
        },
        {
            "id": 14025,
            "url": "http://svs.gsfc.nasa.gov/14025/",
            "result_type": "Produced Video",
            "release_date": "2021-11-29T11:00:00-05:00",
            "title": "Strong Winds Power Electric Fields in the Upper Atmosphere",
            "description": "Using observations from NASA’s ICON mission, scientists presented the first direct measurements of Earth’s long-theorized dynamo on the edge of space: a wind-driven electrical generator that spans the globe 60-plus miles above our heads. The dynamo churns in the ionosphere, the electrically charged boundary between Earth and space. It’s powered by tidal winds in the upper atmosphere that are faster than most hurricanes and rise from the lower atmosphere, creating an electrical environment that can affect satellites and technology on Earth. The new work, published today in Nature Geoscience, improves our understanding of the ionosphere, which helps scientists better predict space weather and protect our technology from its effects.More information: https://www.nasa.gov/feature/goddard/2021/strong-winds-power-electric-fields-in-upper-atmosphere-icon/ || ",
            "hits": 90
        },
        {
            "id": 13880,
            "url": "http://svs.gsfc.nasa.gov/13880/",
            "result_type": "Produced Video",
            "release_date": "2021-07-12T11:00:00-04:00",
            "title": "How NASA Saw 2020’s Record-Breaking Atlantic Hurricane Season From Space",
            "description": "Tides by Ben Niblett [PRS] and Jon Cotton [PRS]Complete transcript available. || Screen_Shot_2021-07-09_at_3.36.03_PM_print.jpg (1024x574) [210.3 KB] || Screen_Shot_2021-07-09_at_3.36.03_PM.png (3204x1798) [8.1 MB] || Screen_Shot_2021-07-09_at_3.36.03_PM_searchweb.png (320x180) [117.4 KB] || Screen_Shot_2021-07-09_at_3.36.03_PM_thm.png (80x40) [11.2 KB] || Hurricanes_Final.webm (1920x1080) [36.2 MB] || Hurricanes_Final.mp4 (1920x1080) [436.6 MB] || Hurricanes.en_US.srt [3.6 KB] || Hurricanes.en_US.vtt [3.6 KB] || ",
            "hits": 22
        },
        {
            "id": 13848,
            "url": "http://svs.gsfc.nasa.gov/13848/",
            "result_type": "Produced Video",
            "release_date": "2021-04-29T11:00:00-04:00",
            "title": "NASA Sees Tides Under the Ocean’s Surface",
            "description": "Internal tides, or internal waves, can reach hundreds of feet underneath the ocean surface, but might only be a few inches high on the surface. Even though they're underwater, NASA can see these tides from satellites. They provide oceanographers with a unique way to map and study the much larger internal water motion. || ",
            "hits": 60
        },
        {
            "id": 4850,
            "url": "http://svs.gsfc.nasa.gov/4850/",
            "result_type": "Visualization",
            "release_date": "2021-04-29T00:00:00-04:00",
            "title": "Internal Ocean Tides",
            "description": "Data visualization featuring internal tides data from NASA Goddard's Space Flight Center simulation run. The visualization sequence starts with a view of the Americas and the Pacific Ocean and soon after exposes the undersea mountain range along the Hawaiian Ridge. Internal tides data appear on the water surface and the direction of the waves reveal the interplay between the steep bathymetry and the tidal energy generated in the region. Zooming out to a global view, we spot other areas around the globe where large tides are generated, such as Tahiti, Southwest Indian Ocean and Luzon Strait and observe the motions and patterns presented by data. || InternalTides_1024x576_2944.jpg (1024x576) [614.4 KB] || InternalTides_1024x576_2944_searchweb.png (320x180) [134.6 KB] || InternalTides_1024x576_2944_web.png (320x180) [134.6 KB] || InternalTides_1024x576_2944_thm.png (80x40) [21.2 KB] || InternalTides_1280x720p30.mp4 (1280x720) [62.4 MB] || InternalTides_1920x1080_60fps_2944.tif (1920x1080) [7.9 MB] || InternalTides_1280x720p30.webm (1280x720) [15.1 MB] || InternalTides_1920x1080p30.mp4 (1920x1080) [120.7 MB] || InternalTides (3840x2160) [0 Item(s)] || InternalTides_3840x2160_60fps_2944.tif (3840x2160) [31.6 MB] || InternalTides_3840x2160_p30.mp4 (3840x2160) [376.1 MB] || InternalTides_1920x1080p30.mp4.hwshow [192 bytes] || ",
            "hits": 175
        },
        {
            "id": 4879,
            "url": "http://svs.gsfc.nasa.gov/4879/",
            "result_type": "Visualization",
            "release_date": "2021-04-29T00:00:00-04:00",
            "title": "Internal Tides: Global Views",
            "description": "Data visualization featuring energetic internal tides on a rotating Earth. The visualization simulates data over a period of a day (24 hours) and showcases the largest internal tides on water bodies around the world. The largest internal tides are generated in regions with steep bathymetry and along mid-ocean ridges, such as in the Hawaiian Ridge, Tahiti, Macquarie Ridge and Luzon Strait. || LargeTides_Composite_1920x1080_0000.png (1024x576) [511.0 KB] || LargeTides_Composite_1920x1080_0000_print.jpg (1024x576) [128.5 KB] || LargeTides_Composite_1920x1080_0000_searchweb.png (320x180) [51.6 KB] || LargeTides_Composite_1920x1080_0000_thm.png (80x40) [4.3 KB] || LargeTides_Composite (1920x1080) [0 Item(s)] || LargeTides_Composite_1280x720p30.mp4 (1280x720) [62.8 MB] || LargeTides_Composite_1920x1080_0000.tif (1920x1080) [11.9 MB] || LargeTides_Composite_1920x1080p30.mp4 (1920x1080) [113.6 MB] || LargeTides_Composite (3840x2160) [0 Item(s)] || LargeTides_Composite_3840x2160_p30.webm (3840x2160) [28.7 MB] || LargeTides_Composite_3840x2160_p30.mp4 (3840x2160) [260.3 MB] || LargeTides_Composite_1920x1080p30.mp4.hwshow [199 bytes] || ",
            "hits": 68
        },
        {
            "id": 13805,
            "url": "http://svs.gsfc.nasa.gov/13805/",
            "result_type": "Produced Video",
            "release_date": "2021-02-22T11:00:00-05:00",
            "title": "Swift Links Neutrino to Star-destroying Black Hole",
            "description": "Watch how a monster black hole ripping apart a star may have launched a ghost particle toward Earth. Astronomers have long predicted that tidal disruption events could produce high-energy neutrinos, nearly massless particles from outside our galaxy traveling close to the speed of light. One recent event, named AT2019dsg, provides the first proof this prediction is true but has challenged scientists’ assumptions of where and when these elusive particles might form during these destructive outbursts. Credit: NASA’s Goddard Space Flight CenterMusic: \"Diagnostic Report\" from Universal Production MusicComplete transcript available. || AT2019dsg_prores_still.jpg (1920x1080) [299.2 KB] || AT2019dsg_prores_still_print.jpg (1024x576) [119.5 KB] || AT2019dsg_prores_still_searchweb.png (180x320) [42.6 KB] || AT2019dsg_prores_still_web.png (320x180) [42.6 KB] || AT2019dsg_prores_still_thm.png (80x40) [4.1 KB] || AT2019dsg_HQ.mp4 (1920x1080) [347.5 MB] || AT2019dsg_LQ.mp4 (1920x1080) [191.3 MB] || AT2019dsg_prores.mov (1920x1080) [1.7 GB] || AT2019dsg_LQ.webm (1920x1080) [21.5 MB] || AT2019dsg_LQ.en_US.srt [3.7 KB] || AT2019dsg_LQ.en_US.vtt [3.7 KB] || ",
            "hits": 281
        },
        {
            "id": 13798,
            "url": "http://svs.gsfc.nasa.gov/13798/",
            "result_type": "Produced Video",
            "release_date": "2021-01-12T12:15:00-05:00",
            "title": "Swift, TESS Catch Eruptions from an Active Galaxy",
            "description": "Watch as a monster black hole partially consumes an orbiting giant star. In this illustration, the gas pulled from the star collides with the black hole’s debris disk and causes a flare. Astronomers have named this repeating event ASASSN-14ko. The flares are the most predictable and frequent yet seen from an active galaxy. Credit: NASA’s Goddard Space Flight CenterMusic: \"Ruminations\" from Universal Production MusicComplete transcript available. || periodic_AGN_still.jpg (1920x1080) [512.8 KB] || periodic_AGN_still_print.jpg (1024x576) [229.4 KB] || periodic_AGN_still_searchweb.png (320x180) [77.1 KB] || periodic_AGN_still_web.png (320x180) [77.1 KB] || periodic_AGN_still_thm.png (80x40) [6.3 KB] || periodic_AGN_HQ.mp4 (1920x1080) [230.6 MB] || periodic_AGN_LQ.mp4 (1920x1080) [123.5 MB] || periodic_AGN_prores.mov (1920x1080) [1.3 GB] || periodic_AGN_LQ.webm (1920x1080) [13.2 MB] || periodic_AGN_prores.mov.en_US.srt [1.6 KB] || periodic_AGN_prores.mov.en_US.vtt [1.6 KB] || ",
            "hits": 75
        },
        {
            "id": 13774,
            "url": "http://svs.gsfc.nasa.gov/13774/",
            "result_type": "Produced Video",
            "release_date": "2020-12-02T09:55:00-05:00",
            "title": "Hubble’s Servicing Mission 1",
            "description": "Shortly after the Hubble Space Telescope was deployed in 1990, the observatory's primary mirror was discovered to have an aberration that affected the clarity of the telescope's early images. Fortunately, Hubble, orbiting 353 miles (569 km) above the surface of the Earth, was the first telescope designed to be visited in space by astronauts to perform repairs, replace parts, and update its technology with new instruments. Servicing Mission 1, launched in December 1993, was the first opportunity to conduct planned maintenance on the telescope. In addition, new instruments were installed and the optics of the flaw in Hubble's primary mirror was corrected.For more information, visit https://nasa.gov/hubble. Music Credits: \"Sleep Patterns\" by Oliver Worth [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music.\"Tides\" by Ben Niblett [PRS], and Jon Cotton [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music.\"Mirrored Cubes\" by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.\"Natural Time Cycles by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.Motion Graphics Template Media Credits:Lower Thirds Auto Self Resizing by cayman via Motion Array || ",
            "hits": 47
        },
        {
            "id": 13765,
            "url": "http://svs.gsfc.nasa.gov/13765/",
            "result_type": "Produced Video",
            "release_date": "2020-11-05T12:00:00-05:00",
            "title": "High Tide Flooding",
            "description": "Complete transcript available. || SLR_2020_High_Tide_Flooding_Final_1080.02397_print.jpg (1024x576) [140.1 KB] || SLR_2020_High_Tide_Flooding_Final_1080.02397_web.png (320x180) [86.8 KB] || SLR_2020_High_Tide_Flooding_Final_1080.02397_thm.png (80x40) [6.1 KB] || SLR_2020_High_Tide_Flooding_Final_1080.02397_searchweb.png (320x180) [86.8 KB] || SLR_2020_High_Tide_Flooding_Final_1080.mp4 (1920x1080) [670.8 MB] || SLR_2020_High_Tide_Flooding_Final_1080.webm (1920x1080) [57.4 MB] || SLR_2020_High_Tide_Flooding_Final.mp4 (3840x2160) [2.0 GB] || high_tide_flooding_12.en_US.srt [10.0 KB] || high_tide_flooding_12.en_US.vtt [10.0 KB] || ",
            "hits": 31
        },
        {
            "id": 4821,
            "url": "http://svs.gsfc.nasa.gov/4821/",
            "result_type": "Visualization",
            "release_date": "2020-11-05T00:00:00-05:00",
            "title": "Barotropic Global Ocean Tides",
            "description": "This animation with voiceover narration shows the barotropic global ocean tides as a complex system of rotating and trapped waves with a mixture of frequencies.Complete transcript available.This video is also available on our YouTube channel. || tides04_final_HD_voiceoverVer04.01000_print.jpg (1024x576) [142.7 KB] || tides04_final_HD_voiceoverVer04.webm (1920x1080) [16.9 MB] || tides04_final_HD_voiceoverVer04.mp4 (1920x1080) [322.9 MB] || BarotropicGlobalOceanTidesVer04.en_US.srt [2.3 KB] || BarotropicGlobalOceanTidesVer04.en_US.vtt [2.3 KB] || tides04_final_HD_voiceoverVer04.mp4.hwshow || ",
            "hits": 286
        },
        {
            "id": 13708,
            "url": "http://svs.gsfc.nasa.gov/13708/",
            "result_type": "Produced Video",
            "release_date": "2020-09-16T11:00:00-04:00",
            "title": "Potential Giant World Circles a Tiny Star",
            "description": "Watch to learn how a possible giant planet may have survived its tiny star’s chaotic history. Jupiter-size WD 1856 b is nearly seven times larger than the white dwarf it orbits every day and a half. Astronomers discovered it using data from NASA’s Transiting Exoplanet Survey Satellite and now-retired Spitzer Space Telescope.Credit: NASA/JPL-Caltech/NASA's Goddard Space Flight CenterMusic: \"Titanium\" from Killer Tracks.Complete transcript available. || wd_1856_still.jpg (1920x1080) [306.2 KB] || wd_1856_still_print.jpg (1024x576) [106.2 KB] || wd_1856_still_searchweb.png (320x180) [46.5 KB] || wd_1856_still_web.png (320x180) [46.5 KB] || wd_1856_still_thm.png (80x40) [4.2 KB] || WD_1856_HQ.mp4 (1920x1080) [279.8 MB] || WD_1856_LQ.mp4 (1920x1080) [146.4 MB] || WD_1856_prores.mov (1920x1080) [1.5 GB] || WD_1856_LQ.webm (1920x1080) [17.1 MB] || WD_1856_prores.en_US.srt [3.0 KB] || WD_1856_prores.en_US.vtt [2.9 KB] || ",
            "hits": 121
        },
        {
            "id": 13608,
            "url": "http://svs.gsfc.nasa.gov/13608/",
            "result_type": "Produced Video",
            "release_date": "2020-05-22T10:00:00-04:00",
            "title": "NASA Names Upcoming Telescope to Honor the \"Mother of Hubble\"",
            "description": "Learn about Nancy Grace Roman, her contribution to NASA missions, and how NASA has honored her.Credit: NASA's Goddard Space Flight CenterMusic: \"Rising Tides\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NGR_Still_1.jpg (1920x1080) [1023.4 KB] || NGR_Still_1_searchweb.png (320x180) [100.8 KB] || NGR_Still_1_thm.png (80x40) [7.6 KB] || Roman_Biography_1080.webm (1920x1080) [23.7 MB] || Roman_Biography_1080.mp4 (1920x1080) [330.8 MB] || Roman_Biography_Best_1080.mp4 (1920x1080) [956.8 MB] || Roman_Biography_SRT_Captions.en_US.srt [4.0 KB] || Roman_Biography_SRT_Captions.en_US.vtt [4.0 KB] || Roman_Biography_ProRes_1920x1080_2997.mov (1920x1080) [2.9 GB] || ",
            "hits": 58
        },
        {
            "id": 13582,
            "url": "http://svs.gsfc.nasa.gov/13582/",
            "result_type": "Produced Video",
            "release_date": "2020-04-20T11:00:00-04:00",
            "title": "NASA Reveals Alien Composition of 2I/Borisov, First Interstellar Comet",
            "description": "When amateur astronomer Gennady Borisov discovered an interstellar comet zipping through our solar system on Aug. 30, 2019, scientists promptly turned their telescopes towards it hoping to catch a glimpse of this rare and ephemeral event. When the scientists peeked inside the halo of gas that formed around the comet as it came closer to the Sun and its ices began to vaporize, they detected something peculiar. 2I/Borisov was releasing gas with a greater concentration of carbon monoxide (CO) than anyone had detected in any comet at a similar distance from the Sun.Song is \"Tides\" from Universal Production Music. || 13582_thumb2.jpg (3840x2160) [335.5 KB] || 13582_Comet_Borisov_YouTube_MASTER.00435_searchweb.png (320x180) [77.0 KB] || 13582_Comet_Borisov_YouTube_MASTER.00435_thm.png (80x40) [4.0 KB] || 13582_Comet_Borisov_MASTER_twitter_720.mp4 (1280x720) [26.3 MB] || 13582_Comet_Borisov_facebook_720.mp4 (1280x720) [151.3 MB] || 13582_Comet_Borisov.webm (960x540) [48.7 MB] || 13582_Comet_Borisov_MASTER.mov.en_US.srt [2.8 KB] || 13582_Comet_Borisov_MASTER.mov.en_US.vtt [2.7 KB] || 13582_Comet_Borisov_YouTube_MASTER.mp4 (3840x2160) [155.4 MB] || ",
            "hits": 34
        },
        {
            "id": 13237,
            "url": "http://svs.gsfc.nasa.gov/13237/",
            "result_type": "Produced Video",
            "release_date": "2019-09-26T11:00:00-04:00",
            "title": "TESS Catches Its First Star-destroying Black Hole",
            "description": "When a star strays too close to a black hole, intense tides break it apart into a stream of gas. The tail of the stream escapes the system, while the rest of it swings back around, surrounding the black hole with a disk of debris. This video includes images of a tidal disruption event called ASASSN-19bt taken by NASA’s Transiting Exoplanet Survey Satellite (TESS) and Swift missions, as well as an animation showing how the event unfolded. Credit: NASA’s Goddard Space Flight CenterMusic: \"Games Show Sphere 03\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_TDE_Still_print.jpg (1024x576) [87.3 KB] || TESS_TDE_Still.jpg (3840x2160) [629.6 KB] || TESS_TDE_Still_searchweb.png (320x180) [68.3 KB] || TESS_TDE_Still_thm.png (80x40) [5.3 KB] || 13237_TESS_TDE_ProRes_1920x1080.mov (1920x1080) [1.6 GB] || 13237_TESS_TDE_1080_Best.mp4 (1920x1080) [380.2 MB] || 13237_TESS_TDE_1080.mp4 (1920x1080) [125.6 MB] || 13237_TESS_TDE_1080_Best.webm (1920x1080) [12.6 MB] || 13237_TESS_TDE_SRT_Captions.en_US.srt [2.2 KB] || 13237_TESS_TDE_SRT_Captions.en_US.vtt [2.2 KB] || ",
            "hits": 147
        },
        {
            "id": 13233,
            "url": "http://svs.gsfc.nasa.gov/13233/",
            "result_type": "Produced Video",
            "release_date": "2019-06-19T14:00:00-04:00",
            "title": "Modeling the Future of the Greenland Ice Sheet",
            "description": "Music: Tides by Jon Cotton [PRS], Ben Niblett [PRS]Complete transcript available. || Greenland_Still_Two.jpg (1920x1080) [941.0 KB] || Greenland_Still_Two_searchweb.png (320x180) [152.3 KB] || Greenland_Still_Two_thm.png (80x40) [8.8 KB] || 13233_Greenland_Outlet_FINAL.mp4 (1920x1080) [253.2 MB] || 13233_Greenland_Outlet_FINAL.mov (1920x1080) [3.4 GB] || 13233_Greenland_Outlet_FINAL.webm (1920x1080) [17.2 MB] || 13233_Greenland_Outlet_FINAL_VX-303985.webm (960x540) [54.0 MB] || GreenlandOutletModel_Fine_V2.en_US.srt [2.9 KB] || GreenlandOutletModel_Fine_V2.en_US.vtt [2.9 KB] || ",
            "hits": 75
        },
        {
            "id": 13092,
            "url": "http://svs.gsfc.nasa.gov/13092/",
            "result_type": "Produced Video",
            "release_date": "2019-03-25T12:00:00-04:00",
            "title": "Greenland's Jakobshavn Glacier Reacts to Changing Ocean Temperatures",
            "description": "NASA's Oceans Melting Greenland (OMG) mission uses ships and planes to measure how ocean temperatures affect Greenland's vast icy expanses. Jakobshavn Glacier, known in Greenlandic as Sermeq Kujalle, on Greenland's central western side, has been one of the island's largest contributor's to sea level rise, losing mass at an accelerating rate. In a new study, the OMG team found that between 2016 and 2017, Jakobshavn Glacier grew slightly and the rate of mass loss slowed down. They traced the causes of this thickening to a temporary cooling of ocean temperatures in the region. || ",
            "hits": 25
        },
        {
            "id": 13147,
            "url": "http://svs.gsfc.nasa.gov/13147/",
            "result_type": "Produced Video",
            "release_date": "2019-02-19T00:00:00-05:00",
            "title": "Volunteer Discovers Record-Setting White Dwarf Star",
            "description": "In this illustration, an asteroid (bottom left) breaks apart under the powerful gravity of LSPM J0207+3331, the oldest, coldest white dwarf known to be surrounded by a ring of dusty debris. Scientists think the system’s infrared signal is best explained by two distinct rings composed of dust supplied by crumbling asteroids.Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || White_Dwarf_Disk_FINAL_1080.png (1920x1080) [11.5 MB] || White_Dwarf_Disk_FINAL_1080.jpg (1920x1080) [372.7 KB] || White_Dwarf_Disk_FINAL_1080_print.jpg (1024x576) [98.1 KB] || White_Dwarf_Disk_FINAL_4k.png (3840x2160) [48.9 MB] || White_Dwarf_Disk_FINAL_4k.jpg (3840x2160) [1.2 MB] || White_Dwarf_Disk_FINAL_1080_searchweb.png (320x180) [52.9 KB] || White_Dwarf_Disk_FINAL_1080_thm.png (80x40) [4.3 KB] || ",
            "hits": 117
        },
        {
            "id": 12994,
            "url": "http://svs.gsfc.nasa.gov/12994/",
            "result_type": "Produced Video",
            "release_date": "2018-07-12T11:00:00-04:00",
            "title": "NASA's Fermi Links Cosmic Neutrino to Monster Black Hole",
            "description": "The discovery of a high-energy neutrino on Sept. 22, 2017, sent astronomers on a chase to locate its source -- a supermassive black hole in a distant galaxy. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Hidden Tides\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Blazar.00590_print.jpg (1024x576) [61.2 KB] || Blazar.00590.png (3840x2160) [5.2 MB] || Blazar.00590.jpg (3840x2160) [536.3 KB] || Blazar.00590_searchweb.png (320x180) [46.6 KB] || Blazar.00590_thm.png (80x40) [4.6 KB] || 12994_Fermi_Blazar_Neutrino_1080p.webm (1920x1080) [17.1 MB] || 12994_Fermi_Blazar_Neutrino_1080.mp4 (1920x1080) [154.8 MB] || 12994_Fermi_Blazar_Neutrino_1080p.mov (1920x1080) [229.5 MB] || 12994_Fermi_Blazar_Neutrino_SRT_Captions.en_US.srt [2.8 KB] || 12994_Fermi_Blazar_Neutrino_SRT_Captions.en_US.vtt [2.7 KB] || 12994_Fermi_Blazar_Neutrino_H264_4k_2997.mp4 (3840x2160) [380.3 MB] || 12994_Fermi_Blazar_Neutrino_4K.mov (3840x2160) [445.0 MB] || 12994_Fermi_Blazar_Neutrino_ProRes_4k_2997.mov (3840x2160) [6.5 GB] || ",
            "hits": 384
        },
        {
            "id": 12696,
            "url": "http://svs.gsfc.nasa.gov/12696/",
            "result_type": "Produced Video",
            "release_date": "2018-05-31T14:00:00-04:00",
            "title": "PACE -- Skies, Oceans, Life",
            "description": "Red tides can come from harmful algal blooms near shore for a variety of reasons. PACE will help scientists monitor red tides. || TWITTER_720-PACE_Red_Tide_w_logo.01000_print.jpg (1024x576) [177.1 KB] || APPLE_TV-PACE_Red_Tide_w_logo.m4v (1280x720) [42.0 MB] || FACEBOOK_720-PACE_Red_Tide_w_logo.mp4 (1280x720) [106.7 MB] || LARGE_MP4-PACE_Red_Tide_w_logo_large.mp4 (1920x1080) [73.8 MB] || TWITTER_720-PACE_Red_Tide_w_logo.mp4 (1280x720) [18.0 MB] || WEBM-PACE_Red_Tide_w_logo.webm (960x540) [29.5 MB] || YOUTUBE_1080-PACE_Red_Tide_w_logo.mp4 (1920x1080) [134.6 MB] || YOUTUBE_720-PACE_Red_Tide_w_logo.mp4 (1280x720) [138.2 MB] || PACE_Red_Tide_w_logo.en_US.srt [587 bytes] || PACE_Red_Tide_w_logo.en_US.vtt [600 bytes] || PACE_Red_Tide_w_logo_lowres.mp4 (480x272) [10.0 MB] || ",
            "hits": 28
        },
        {
            "id": 12806,
            "url": "http://svs.gsfc.nasa.gov/12806/",
            "result_type": "Produced Video",
            "release_date": "2017-12-21T13:00:00-05:00",
            "title": "'Winking' Star May Be Devouring Wrecked Planets",
            "description": "Zoom into RZ Piscium, a star about 550 light-years away that undergoes erratic dips in brightness. This animation illustrates one possible interpretation of the system, with a giant planet near the star slowly dissolving. Gas and dust stream away from the planet, and these clouds occasionally eclipse the star as we view it from Earth.Music: \"Frozen Wonder\" from Killer Tracks Watch this video on the NASA Goddard YouTube channel.Credit NASA's Goddard Space Flight Center/CI LabComplete transcript available. || StarObscure_Plane_v06_PNG_00333.png (1920x1080) [6.1 MB] || StarObscure_Plane_v06_00333.jpg (1920x1080) [131.6 KB] || StarObscure_Plane_v06_00333_print.jpg (1024x576) [53.2 KB] || StarObscure_Plane_v06_00333_searchweb.png (320x180) [38.0 KB] || StarObscure_Plane_v06_00333_thm.png (80x40) [4.0 KB] || 12806_RZ_Piscium_ProRes_1920x1080_2997.mov (1920x1080) [942.8 MB] || 12806_RZ_Piscium_H264_Best_1080p.mov (1920x1080) [172.1 MB] || 12806_RZ_Piscium_1080.mp4 (1920x1080) [73.4 MB] || 12806_RZ_Piscium_H264_1080.m4v (1920x1080) [72.4 MB] || 12806_RZ_Piscium_H264_1080.webm (1920x1080) [7.9 MB] || R2Piscium.en_US.srt [805 bytes] || R2Piscium.en_US.vtt [818 bytes] || ",
            "hits": 34
        },
        {
            "id": 12666,
            "url": "http://svs.gsfc.nasa.gov/12666/",
            "result_type": "Produced Video",
            "release_date": "2017-08-11T16:00:00-04:00",
            "title": "Scientists Bury GPS in Antarctic Ice to Measure Effects of Tides",
            "description": "NASA scientists and ice sheet modelers, Ryan Walker and Christine Dow, traveled to a remote location on the coast of Antarctic to investigate how tides affect the movement and stability of the Nansen Ice Shelf, a 695-mile extension of ice protruding into Antarctica’s Ross Sea. Relatively understudied, Nansen’s manageable size lends itself to becoming a proxy for predicting how larger ice shelves will contribute to sea level rise in the decades and centuries to come. By studying the impact of tides, Walker and Dow are able to determine how the rise and fall of floating ice sheets may impact the likelihood of an eventual ice shelf collapse.Complete transcript available.Music: Tiptoe Marimba by Brightside Studio || LARGE_MP4-Nansen_0711217_FINAL_V3_large.00001_print.jpg (1024x576) [78.0 KB] || LARGE_MP4-Nansen_0711217_FINAL_V3_large.00001_searchweb.png (320x180) [57.6 KB] || LARGE_MP4-Nansen_0711217_FINAL_V3_large.00001_thm.png (80x40) [4.4 KB] || LARGE_MP4-Nansen_0711217_FINAL_V3_large.00001_web.png (320x180) [57.6 KB] || APPLE_TV-Nansen_0711217_FINAL_V3_appletv.m4v (1280x720) [129.6 MB] || FACEBOOK_720-Nansen_0711217_FINAL_V3_facebook_720.mp4 (1280x720) [302.8 MB] || LARGE_MP4-Nansen_0711217_FINAL_V3_large.mp4 (1280x720) [244.4 MB] || Nansen_0711217_FINAL_V3.mov (1280x720) [2.6 GB] || TWITTER_720-Nansen_0711217_FINAL_V3_twitter_720.mp4 (1280x720) [53.9 MB] || WEBM-Nansen_0711217_FINAL_V3.webm (960x540) [97.5 MB] || YOUTUBE_1080-Nansen_0711217_FINAL_V3_youtube_1080.mp4 (1920x1080) [403.4 MB] || YOUTUBE_720-Nansen_0711217_FINAL_V3_youtube_720.mp4 (1280x720) [404.4 MB] || APPLE_TV-Nansen_0711217_FINAL_V3_appletv_subtitles.m4v (1280x720) [129.7 MB] || 12666_Nansen_080717.en_US.srt [4.4 KB] || 12666_Nansen_080717.en_US.vtt [4.4 KB] || Nansen_0711217_FINAL_V3_lowres.mp4 (480x272) [32.5 MB] || ",
            "hits": 17
        },
        {
            "id": 30890,
            "url": "http://svs.gsfc.nasa.gov/30890/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-08-03T00:00:00-04:00",
            "title": "Landsat 'Sees in the Dark' the Evolution of Antarctica’s Delaware-Sized Iceberg",
            "description": "Evolution of Larsen C ice shelf leading up to and following the calving || larsencriftevolution20162017v5.png (3427x1650) [5.0 MB] || larsencriftevolution20162017v5_print.jpg (1024x493) [158.0 KB] || larsencriftevolution20162017v5_searchweb.png (320x180) [69.6 KB] || larsencriftevolution20162017v5_thm.png (80x40) [6.3 KB] || ",
            "hits": 32
        },
        {
            "id": 12614,
            "url": "http://svs.gsfc.nasa.gov/12614/",
            "result_type": "Produced Video",
            "release_date": "2017-06-02T11:00:00-04:00",
            "title": "SDO Anniversary Series",
            "description": "The sun is always changing and NASA's Solar Dynamics Observatory is always watching. Launched on Feb. 11, 2010, SDO keeps a 24-hour eye on the entire disk of the sun, with a prime view of the graceful dance of solar material coursing through the sun's atmosphere, the corona.Year 1 || ",
            "hits": 56
        },
        {
            "id": 12477,
            "url": "http://svs.gsfc.nasa.gov/12477/",
            "result_type": "Produced Video",
            "release_date": "2017-05-15T12:00:00-04:00",
            "title": "Marine Magnetism",
            "description": "A new method uses Earth's magnetic field to detect changes in the heat stored in the ocean. || TidalMagFL_frames_30fps.0272.png (1920x1080) [4.1 MB] || TidalMagFL_frames_30fps.0272_1024x576.jpg (1024x576) [183.8 KB] || TidalMagFL_frames_30fps.0272_1280x720.jpg (1280x720) [291.4 KB] || TidalMagFL_frames_30fps.0272_1024x576_print.jpg (1024x576) [183.2 KB] || TidalMagFL_frames_30fps.0272_thm.png (80x40) [5.8 KB] || TidalMagFL_frames_30fps.0272_1024x576_searchweb.png (320x180) [103.7 KB] || ",
            "hits": 35
        },
        {
            "id": 12499,
            "url": "http://svs.gsfc.nasa.gov/12499/",
            "result_type": "Produced Video",
            "release_date": "2017-03-20T14:00:00-04:00",
            "title": "Swift Charts a Star's 'Death Spiral' into Black Hole",
            "description": "This animation illustrates how debris from a tidally disrupted star collides with itself, creating shock waves that emit ultraviolet and optical light far from the black hole. According to Swift observations of ASASSN-14li, these clumps took about a month to fall back to the black hole, where they produced changes in the X-ray emission that correlated with the earlier UV and optical changes.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || TD_Shocks_Still_print.jpg (1024x576) [115.2 KB] || TD_Shocks_Still.png (3840x2160) [32.6 MB] || TD_Shocks_Still.jpg (3840x2160) [922.7 KB] || TD_Shocks_Still_searchweb.png (320x180) [59.5 KB] || TD_Shocks_Still_thm.png (80x40) [4.8 KB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_1080.mov (1920x1080) [50.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_youtube_hq.mov (1920x1080) [25.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Good_1080.m4v (1920x1080) [44.4 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.m4v (960x540) [10.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_HD.wmv (1920x1080) [6.9 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.webm (960x540) [3.8 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv_subtitles.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_SRT_Captions.en_US.srt [509 bytes] || 12499_Tidal_Disruption_SRT_Captions.en_US.vtt [522 bytes] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_ProRes_1920x1080_2997.mov (1920x1080) [591.1 MB] || ",
            "hits": 132
        },
        {
            "id": 40317,
            "url": "http://svs.gsfc.nasa.gov/gallery/vcearth-video-wall/",
            "result_type": "Gallery",
            "release_date": "2017-02-02T00:00:00-05:00",
            "title": "VC Earth Video Wall",
            "description": "list of videos to display on video wall in Earth science exhibit at Goddard Visitor Center",
            "hits": 10
        },
        {
            "id": 4541,
            "url": "http://svs.gsfc.nasa.gov/4541/",
            "result_type": "Visualization",
            "release_date": "2016-12-30T00:00:00-05:00",
            "title": "Ocean Tides and Magnetic Fields",
            "description": "Earth’s magnetic field is built up from many contributing sources ranging from the planet’s core to the magnetosphere in space. Untangling and identifying the different sources allows geomagnetic scientists to gather information about the individual processes that combine to create the full field.One contributor is the ocean. But how do the tides affect Earth’s magnetic field? Seawater is an electrical conductor, and therefore interacts with the magnetic field. As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along. Because the salty water is a good, but not great, conductor, the interaction is relatively weak. The strongest component is from the regular lunar tide that happens about twice per day (actually 12.42 hours). Other contributions come from ocean swell, eddies, and even tsunamis.The strength of the interaction also depends on the temperature of the ocean water. Scientists are now able to determine how much heat is being stored in the entire ocean, from wave top to sea floor by observations of the Earth's magnetic field. || ",
            "hits": 219
        },
        {
            "id": 12456,
            "url": "http://svs.gsfc.nasa.gov/12456/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:45:00-05:00",
            "title": "Tracking Ocean Heat With Magnetic Fields",
            "description": "As Earth warms, much of the extra heat is stored in the planet’s ocean – but monitoring the magnitude of that heat content is a difficult task. A surprising feature of the tides could help, however. Scientists at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, are developing a new way to use satellite observations of magnetic fields to measure heat stored in the ocean.Music: War Torn by Brad Smith [BMI] Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12456-ocean-heat-AGU-web.jpg (1920x1080) [354.1 KB] || 12456-ocean-heat-AGU-web_searchweb.png (320x180) [122.0 KB] || 12456-ocean-heat-AGU-web_thm.png (80x40) [7.7 KB] || 12456-ocean-heat-APR_VX-680579_large.mp4 (1920x1080) [59.1 MB] || 12456-ocean-heat-APR_VX-680579_appletv.m4v (1280x720) [30.6 MB] || 12456-ocean-heat-AGU-720p.mp4 (1280x720) [59.5 MB] || 12456-ocean-heat-AGU.mp4 (1920x1080) [59.9 MB] || 12456-ocean-heat-APR_VX-680579.webm (960x540) [23.6 MB] || 12456-ocean-heat-APR_VX-680579_appletv_subtitles.m4v (1280x720) [30.7 MB] || 12456-ocean-heat-captions.en_US.srt [891 bytes] || 12456-ocean-heat-captions.en_US.vtt [904 bytes] || 12456-ocean-heat-APR_VX-680579_ipod_sm.mp4 (320x240) [10.9 MB] || 12456-ocean-heat-APR_VX-680579_prores.mov (1280x720) [791.2 MB] || 12456-ocean-heat-APR_VX-680579_youtube_hq.mov (1920x1080) [212.0 MB] || 12456-ocean-heat-APR_VX-680579.mpeg (1280x720) [196.6 MB] || ",
            "hits": 28
        },
        {
            "id": 12450,
            "url": "http://svs.gsfc.nasa.gov/12450/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:30:00-05:00",
            "title": "Ocean Tides and Magnetic Fields",
            "description": "Seawater is an electrical conductor, and therefore interacts with the magnetic field.  As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along.Because the salty water is a good, but not great, conductor, the interaction is relatively weak.  Scientists at NASA Goddard Space Flight Center are developing improved methods to isolate the signal from ocean tides and use that information to determine the heat content of the ocean.Music: \"Memory Of A Lifetime\" by J Ehrlich [SESAC], Jean-Christophe Beck [BMI]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12450-Tidal-Magnetic-Animation-APR_large.00545_print.jpg (1024x576) [189.1 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_searchweb.png (320x180) [93.6 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_thm.png (80x40) [5.8 KB] || 12450-Tidal-Magnetic-Animation-APR.webm (960x540) [26.5 MB] || 12450-Tidal-Magnetic-Animation-APR_prores.mov (1280x720) [989.0 MB] || 12450-Tidal-Magnetic-Animation-APR_large.mp4 (1920x1080) [66.1 MB] || 12450-Tidal-Magnetic-Animation-APR_youtube_hq.mov (1920x1080) [1.0 GB] || 12450-Tidal-Magnetic-Animation-APR_appletv.m4v (1280x720) [32.1 MB] || 12450-Tidal-Magnetic-Animation-APR_appletv_subtitles.m4v (1280x720) [32.2 MB] || 1920x1080_16x9_30p (1920x1080) [128.0 KB] || 12450-Tidal-Magnetic-Animation.en_US.srt [1.4 KB] || 12450-Tidal-Magnetic-Animation.en_US.vtt [1.4 KB] || 12450-Tidal-Magnetic-Animation-APR_ipod_sm.mp4 (320x240) [11.5 MB] || ",
            "hits": 190
        },
        {
            "id": 4492,
            "url": "http://svs.gsfc.nasa.gov/4492/",
            "result_type": "Visualization",
            "release_date": "2016-11-09T15:00:00-05:00",
            "title": "ICESat-2 Measurements Over Antarctica (prelaunch)",
            "description": "ICESat-2 has 3 pairs of lasers that will measure the heights of ice and snow at very high resolution || walls75.1870_print.jpg (1024x576) [34.7 KB] || walls75.1870_searchweb.png (320x180) [29.8 KB] || walls75.1870_thm.png (80x40) [3.4 KB] || walls_1080p30.mp4 (1920x1080) [50.0 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || walls_1080p30.webm (1920x1080) [11.9 MB] || walls_360p30.mp4 (640x360) [8.1 MB] || Slide1.hwshow || ",
            "hits": 32
        },
        {
            "id": 12126,
            "url": "http://svs.gsfc.nasa.gov/12126/",
            "result_type": "Produced Video",
            "release_date": "2016-05-16T11:00:00-04:00",
            "title": "Science On a Sphere: A Global Tour of Precipitation from NASA",
            "description": "Precipitation (falling rain and snow) is our fresh water reservoir in the sky and is fundamental to life on Earth. A Global Tour of Precipitation from NASA shows how rain and snowfall moves around the world from the vantage of space using measurements from the Global Precipitation Measurement Core Observatory, or GPM. This is a joint mission between NASA and the Japanese Aerospace Exploration Agency (JAXA) and offers the most detailed and worldwide view of rain and snowfall ever created.This narrated movie is created for Science On a Sphere, a platform designed by NOAA that displays movies on a spherical screen. Audiences can view the movie from any side of the sphere and can see any part of Earth. During this show viewers will be guided through a variety of precipitation patterns and display features such as the persistent band of the heaviest rainfall around the equator and tight swirls of tropical storms in the Northern Hemisphere. At subtropical latitudes in both hemispheres there are persistent dry areas and this is where most of the major deserts reside. Sea surface temperature and winds are also shown to highlight the interconnectedness of the Earth system. The movie concludes with near real-time global precipitation data from GPM, which is provided to Science On a Sphere roughly six hours after the observation.To download this movie formatted for a spherical screen, visit NOAA's official Science On a Sphere website below:‌• A Global Tour of Precipitation from NASA‌• Near Real-Time Global Precipitation Data || ",
            "hits": 49
        },
        {
            "id": 12144,
            "url": "http://svs.gsfc.nasa.gov/12144/",
            "result_type": "Produced Video",
            "release_date": "2016-02-12T09:00:00-05:00",
            "title": "SDO: Year 6",
            "description": "This ultra-high definition (3840x2160) video shows the sun in the 171 angstrom wavelength of extreme ultraviolet light. It covers a time period of January 2, 2015 to January 28, 2016 at a cadence of one frame every hour, or 24 frames per day.  This timelapse is repeated with narration by solar scientist Nicholeen Viall and contains close-ups and annotations. 171 angstrom light highlights material around 600,000 Kelvin and shows features in the upper transition region and quiet corona of the sun. The video is available to download here at 59.94 frames per second, double the rate YouTube currently allows for UHD content.  The music is titled \"Tides\" and is from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SDO_Year6_HCblend_HD.png (1920x1080) [5.3 MB] || SDO_Year6_HCblend_HD.jpg (1920x1080) [545.9 KB] || SDO_Year6_HCblend_HD_print.jpg (1024x576) [179.5 KB] || SDO_Year6_HCblend_UHD.png (3840x2160) [19.7 MB] || SDO_Year6_HCblend_UHD.jpg (3840x2160) [1.2 MB] || SDO_Year6_HCblend_HD_searchweb.png (180x320) [59.6 KB] || SDO_Year6_HCblend_HD_thm.png (80x40) [4.8 KB] || 12144_SDO_Year_6_appletv.webm (1280x720) [50.5 MB] || 12144_SDO_Year_6_appletv.m4v (1280x720) [241.9 MB] || 12144_SDO_Year_6_appletv_appletv_subtitles.m4v (1280x720) [242.1 MB] || SDO_Year_6_SRT_Captions.en_US.srt [6.3 KB] || SDO_Year_6_SRT_Captions.en_US.vtt [6.3 KB] || 12144_SDO_Year_6_H264_Good_1920x1080_2997.mov (1920x1080) [1.4 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_2997.mov (3840x2160) [9.1 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_5994.mov (3840x2160) [10.2 GB] || 12144_SDO_Year_6_ProRes_3840x2160_5994.mov (3840x2160) [50.3 GB] || ",
            "hits": 118
        },
        {
            "id": 40249,
            "url": "http://svs.gsfc.nasa.gov/gallery/rising-seas/",
            "result_type": "Gallery",
            "release_date": "2015-08-25T00:00:00-04:00",
            "title": "Sea Level Rise",
            "description": "Earth’s seas are rising, a direct result of a changing climate. Ocean temperatures are increasing, leading to ocean expansion. And as ice sheets and glaciers melt, they add more water. A fleet of increasingly sophisticated instruments deployed by NASA across the oceans, on polar ice and in orbit, reveals significant changes among globally interlocking factors that are driving sea levels higher.",
            "hits": 146
        },
        {
            "id": 40213,
            "url": "http://svs.gsfc.nasa.gov/gallery/swift-black-holes/",
            "result_type": "Gallery",
            "release_date": "2014-11-13T00:00:00-05:00",
            "title": "Swift: Black Holes",
            "description": "No description available.",
            "hits": 37
        },
        {
            "id": 11587,
            "url": "http://svs.gsfc.nasa.gov/11587/",
            "result_type": "Produced Video",
            "release_date": "2014-07-17T11:00:00-04:00",
            "title": "The Moving Shoreline",
            "description": "Beaches are dynamic, living landscapes, and the prime example of their evolution is the coastal barrier. These islands and spits run parallel to the mainland and protect it from the full force of ocean winds and waves. More than 2,100 barriers front about 10 percent of the world’s continental shorelines. These sandy barriers are constantly raised up, shifted, and torn down by the natural ebb and flow of waves, currents, winds, and tides. Hooks form, inlets open and close, and beaches slowly march across their back bays and lagoons toward the mainland. This process allows them to naturally move ever upwards as sea levels rise. Since 1984, USGS-NASA Landsat satellites have observed coastline changes off of Chatham, Massachusetts, on the southeastern elbow of Cape Cod. Over the past 30 years, three major breaches opened, and barrier islands connected to the coastline and to each other. Watch the video to see the changes unfold. || ",
            "hits": 43
        },
        {
            "id": 11530,
            "url": "http://svs.gsfc.nasa.gov/11530/",
            "result_type": "Produced Video",
            "release_date": "2014-05-13T10:00:00-04:00",
            "title": "Neutron Stars Rip Each Other Apart to Form Black Hole",
            "description": "This supercomputer simulation shows one of the most violent events in the universe: a pair of neutron stars colliding, merging and forming a black hole.  A neutron star is the compressed core left behind when a star born with between eight and 30 times the sun's mass explodes as a supernova. Neutron stars pack about 1.5 times the mass of the sun — equivalent to about half a million Earths — into a ball just 12 miles (20 km) across.  As the simulation begins, we view an unequally matched pair of neutron stars weighing 1.4 and 1.7 solar masses. They are separated by only about 11 miles, slightly less distance than their own diameters. Redder colors show regions of progressively lower density.  As the stars spiral toward each other, intense tides begin to deform them, possibly cracking their crusts. Neutron stars possess incredible density, but their surfaces are comparatively thin, with densities about a million times greater than gold. Their interiors crush matter to a much greater degree densities rise by 100 million times in their centers. To begin to imagine such mind-boggling densities, consider that a cubic centimeter of neutron star matter outweighs Mount Everest. By 7 milliseconds, tidal forces overwhelm and shatter the lesser star. Its superdense contents erupt into the system and curl a spiral arm of incredibly hot material. At 13 milliseconds, the more massive star has accumulated too much mass to support it against gravity and collapses, and a new black hole is born. The black hole's event horizon — its point of no return — is shown by the gray sphere. While most of the matter from both neutron stars will fall into the black hole, some of the less dense, faster moving matter manages to orbit around it, quickly forming a large and rapidly rotating torus. This torus extends for about 124 miles (200 km) and contains the equivalent of 1/5th the mass of our sun.  The entire simulation covers only 20 milliseconds.Scientists think neutron star mergers like this produce short gamma-ray bursts (GRBs). Short GRBs last less than two seconds yet unleash as much energy as all the stars in our galaxy produce over one year. The rapidly fading afterglow of these explosions presents a challenge to astronomers. A key element in understanding GRBs is getting instruments on large ground-based telescopes to capture afterglows as soon as possible after the burst. The rapid notification and accurate positions provided by NASA's Swift mission creates a vibrant synergy with ground-based observatories that has led to dramatically improved understanding of GRBs, especially for short bursts. || ",
            "hits": 450
        },
        {
            "id": 30494,
            "url": "http://svs.gsfc.nasa.gov/30494/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-03-01T00:00:00-05:00",
            "title": "Simulated Sea Surface Speeds",
            "description": "This simulation shows sea surface speed in ultra-high resolution. Several oceanic characteristics are included in the simulation and are visible in its output; including tides, atmospheric pressure forcing, diurnal cycles, and dynamic/thermodynamic sea ice . The model has a .75 to 2.2 km horizontal grid spacing and 90 vertical levels, with 1-m vertical levels near the surface. The full 3D grid is output at hourly intervals.Yellow shades represent relatively fast sea surface speeds, while red shades represent slower speeds. The simulation was carried out using the Massachusetts Institute of Technology general circulation model (mitgcm.org) by the Estimating the Circulation and Climate of the Ocean (ECCO) group. Credits: C. Hill, G. Forget (MIT)C. Henze, B. Nelson, B. Ciotti (Ames)D. Menemenlis (JPL)A. Chaudhuri (AER)MITgcm/ECCO developers and usersSGI and NAS computer scientists and engineers || ",
            "hits": 18
        },
        {
            "id": 10807,
            "url": "http://svs.gsfc.nasa.gov/10807/",
            "result_type": "Produced Video",
            "release_date": "2011-08-24T13:00:00-04:00",
            "title": "NASA's Swift Satellite Spots Black Hole Devouring A Star",
            "description": "In late March 2011, NASA's Swift satellite alerted astronomers to intense and unusual high-energy flares from a new source in the constellation Draco. They soon realized that the source, which is now known as Swift J1644+57, was the result of a truly extraordinary event — the awakening of a distant galaxy's dormant black hole as it shredded and consumed a star. The galaxy is so far away that the radiation from the blast has traveled 3.9 billion years before reaching Earth. Most galaxies, including our own, possess a central supersized black hole weighing millions of times the sun's mass. According to the new studies, the black hole in the galaxy hosting Swift J1644+57 may be twice the mass of the four-million-solar-mass black hole lurking at the center of our own Milky Way galaxy. As a star falls toward a black hole, it is ripped apart by intense tides. The gas is corralled into a disk that swirls around the black hole and becomes rapidly heated to temperatures of millions of degrees. The innermost gas in the disk spirals toward the black hole, where rapid motion and magnetism creates dual, oppositely directed \"funnels\" through which some particles may escape. Particle jets driving matter at velocities greater than 80-90 percent the speed of light form along the black hole's spin axis. In the case of Swift J1644+57, one of these jets happened to point straight at Earth.Theoretical studies of tidally disrupted stars suggested that they would appear as flares at optical and ultraviolet energies. The brightness and energy of a black hole's jet is greatly enhanced when viewed head-on. The phenomenon, called relativistic beaming, explains why Swift J1644+57 was seen at X-ray energies and appeared so strikingly luminous. When first detected on March 28, the flares were initially assumed to signal a gamma-ray burst, one of the nearly daily short blasts of high-energy radiation often associated with the death of a massive star and the birth of a black hole in the distant universe. But as the emission continued to brighten and flare, astronomers realized that the most plausible explanation was the tidal disruption of a sun-like star seen as beamed emission. || ",
            "hits": 160
        },
        {
            "id": 10656,
            "url": "http://svs.gsfc.nasa.gov/10656/",
            "result_type": "Produced Video",
            "release_date": "2010-11-01T00:00:00-04:00",
            "title": "JWST Feature - Evolution of the Universe",
            "description": "Astrophyscists and astonomers will use the James Webb Space Telescope to unravel mysteries about the evolution of the Universe. The Webb telscope will help observe how the first stars gathered into the first galaxies, and those first galaxies collided and merged into larger galaxies and evolved into the Universe we see today. || ",
            "hits": 91
        },
        {
            "id": 10657,
            "url": "http://svs.gsfc.nasa.gov/10657/",
            "result_type": "Produced Video",
            "release_date": "2010-11-01T00:00:00-04:00",
            "title": "JWST Feature - Galaxy Evolution",
            "description": "Astrophysicists and astronomers will use the James Webb Space Telescope to see further than Hubble to witness the origin and development of galaxies. || ",
            "hits": 36
        },
        {
            "id": 10658,
            "url": "http://svs.gsfc.nasa.gov/10658/",
            "result_type": "Produced Video",
            "release_date": "2010-10-28T00:00:00-04:00",
            "title": "Webb Science Feature - Colliding Galaxies",
            "description": "Deep surveys by the James Webb Space Telescope will capture the full panorama of galaxy evolution, from the earliest dwarf galaxies that formed to the familiar galaxies we see today. The Webb Telescope will help us understand how the shape, structure and chemical content of galaxies change over the sweep of cosmic history. || ",
            "hits": 60
        },
        {
            "id": 10659,
            "url": "http://svs.gsfc.nasa.gov/10659/",
            "result_type": "Produced Video",
            "release_date": "2010-10-28T00:00:00-04:00",
            "title": "JWST Feature - Planetary Evolution",
            "description": "A fully produced video about planetary evolution and how the Webb Telelscope's ability to see inside dense clouds of gas and dust will help us better understand solar system formation and evolution. || ",
            "hits": 90
        },
        {
            "id": 40078,
            "url": "http://svs.gsfc.nasa.gov/gallery/earth-science-education/",
            "result_type": "Gallery",
            "release_date": "2010-09-26T00:00:00-04:00",
            "title": "Earth Science Educator Resources",
            "description": "On this page is a collection of Goddard video pieces that have been created for education related events.  You will find recordings of past webcasts, earth science web shorts and professional development resources.  We hope this will become your first stop when shopping for multimedia lesson objects to apply in your classroom.",
            "hits": 43
        },
        {
            "id": 40075,
            "url": "http://svs.gsfc.nasa.gov/gallery/energy-essentials/",
            "result_type": "Gallery",
            "release_date": "2010-08-17T00:00:00-04:00",
            "title": "Energy Essentials",
            "description": "Energy. What do we really know about it? Where does the energy we use come from? How does energy flow through the systems of our planet? How is our energy consumption changing our climate? Who uses the most energy? In celebration of Earth Science Week's 2010 theme, Exploring Energy, NASA presents a multimedia gallery that helps answer some of these questions.  The images, data visualizations, animations and videos in this gallery highlight how NASA satellite data and research help us better understand how much is reaching Earth from the Sun, how it's distributed across the Earth, where humans are tapping into that energy, and the many ways in which our energy use is transforming our planet. You can download the imagery in a variety of formats directly from this site. For more multimedia resources on energy and other topics, search the Scientific Visualization Studio. To learn more about Earth Science Week 2010, visit the Earth Science Week web site.",
            "hits": 74
        },
        {
            "id": 10497,
            "url": "http://svs.gsfc.nasa.gov/10497/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "The Ocean's Green Machines",
            "description": "One tiny marine plant makes life on Earth possible: phytoplankton.  These microscopic photosynthetic drifters form the basis of the marine food web, they regulate carbon in the atmosphere, and are responsible for half of the photosynthesis that takes place on this planet.  Earth's climate is changing at an unprecedented rate, and as our home planet warms, so does the ocean.  Warming waters have big consequences for phytoplankton and for the planet.  For complete transcript, click here. || Oceans_Green_Machines_640x480_ESWpage.00427_print.jpg (1024x576) [65.8 KB] || Oceans_Green_Machines_640x480_ESWpage_web.png (320x180) [135.9 KB] || Oceans_Green_Machines_640x480_ESWpage_thm.png (80x40) [15.0 KB] || Oceans_Green_Machines_AppleTV.webmhd.webm (960x540) [80.8 MB] || Oceans_Green_Machines_1280x720_ProRes.mov (1280x720) [4.9 GB] || Oceans_Green_Machines_1280x720_H264.mov (1280x720) [176.1 MB] || Oceans_Green_Machines_1280x720_ESWpage.mp4 (1280x720) [115.8 MB] || Oceans_Green_Machines_AppleTV.m4v (960x540) [195.1 MB] || Oceans_Green_Machines_640x360_ipod.m4v (640x360) [62.2 MB] || Oceans_Green_Machines_640x480_ESWpage.mp4 (640x360) [62.2 MB] || Oceans_Green_Machines_512x288.mpg (512x288) [113.3 MB] || Oceans_Green_Machines_320x180.mp4 (320x180) [27.7 MB] || Oceans_Green_Machines.wmv (320x176) [37.8 MB] || ",
            "hits": 68
        },
        {
            "id": 10498,
            "url": "http://svs.gsfc.nasa.gov/10498/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Keeping Up With Carbon",
            "description": "Carbon is all around us.  This unique atom is the basic building block of life, and its compounds form solids, liquids, or gases. Carbon helps form the bodies of living organisms; it dissolves in the ocean; mixes in the atmosphere; and can be stored in the crust of the planet. A carbon atom could spend millions of years moving through this complex cycle. The ocean plays the most critical role in regulating Earth's carbon balance, and understanding how the carbon cycle is changing is key to understanding Earth's changing climate. For complete transcript, click here. || Keeping_Up_with_Carbon_640x360_ESWpage.00577_print.jpg (1024x576) [71.2 KB] || Keeping_Up_with_Carbon_640x360_ESWpage_web.png (320x180) [128.6 KB] || Keeping_Up_with_Carbon_640x360_ESWpage_thm.png (80x40) [13.9 KB] || Keeping_Up_with_Carbon_AppleTV.webmhd.webm (960x540) [84.1 MB] || Keeping_Up_with_Carbon_1280x720_ProRes.mov (1280x720) [5.1 GB] || Keeping_Up_with_Carbon_1280x720_H264.mov (1280x720) [159.3 MB] || Keeping_Up_with_Carbon_1280x720_ESWpage.mp4 (1280x720) [133.5 MB] || Keeping_Up_with_Carbon_AppleTV.m4v (960x540) [201.6 MB] || Keeping_Up_with_Carbon_640x360_ipod.m4v (640x360) [63.2 MB] || Keeping_Up_with_Carbon_640x360_ESWpage.mp4 (640x360) [63.2 MB] || Keeping_Up_with_Carbon_512x288.mpg (512x288) [123.9 MB] || Keeping_Up_with_Carbon_320x180.mp4 (320x180) [26.0 MB] || Keeping_Up_with_Carbon.wmv (320x176) [39.0 MB] || ",
            "hits": 75
        },
        {
            "id": 10502,
            "url": "http://svs.gsfc.nasa.gov/10502/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Climate Change and the Global Ocean",
            "description": "We know climate change can affect us, but does climate change alter something as vast, deep and mysterious as our oceans? For years, scientists have studied the world's oceans by sending out ships and divers, deploying data-gathering buoys, and by taking aerial measurements from planes. But one of the better ways to understand oceans is to gain an even broader perspective - the view from space. NASA's Earth observing satellites do more than just take pictures of our planet. High-tech sensors gather data, including ocean surface temperature, surface winds, sea level, circulation, and even marine life. Information the satellites obtain help us understand the complex interactions driving the world's oceans today - and gain valuable insight into how the impacts of climate change on oceans might affect us on dry land.For complete transcript, click here. || Global_Ocean_ipod_320x240.01252_print.jpg (1024x576) [77.3 KB] || Global_Ocean_ipod_320x240_web.png (320x180) [84.7 KB] || Global_Ocean_ipod_320x240_thm.png (80x40) [16.1 KB] || Global_Ocean_appletv.webmhd.webm (960x540) [78.2 MB] || Global_Ocean_broll_prores.mov (1280x720) [5.3 GB] || Global_Ocean_1280x720.mp4 (1280x720) [159.8 MB] || Global_Ocean_appletv.m4v (960x540) [187.1 MB] || Global_Ocean_H264_1280x720_30fps.mov (1280x720) [167.6 MB] || Global_Ocean_youtube_1280x720.mov (1280x720) [79.2 MB] || Global_Ocean_ipod_640x480.m4v (640x360) [59.9 MB] || Global_Ocean_ipod_320x240.m4v (320x180) [25.9 MB] || Global_Ocean.wmv (346x260) [39.1 MB] || ",
            "hits": 32
        },
        {
            "id": 3538,
            "url": "http://svs.gsfc.nasa.gov/3538/",
            "result_type": "Visualization",
            "release_date": "2008-10-31T12:00:00-04:00",
            "title": "Landsat Image Mosaic of Antarctica Flyover of Pine Island Glacier",
            "description": "The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. This area of the West Antarctic Ice Sheet is also believed to be the most susceptible to collapse. The evolution of this glacier is therefore of great interest to the scientific community. It is an area of Antarctica which is experiencing rapid changes. The grounding line of Pine Island Glacier is retreating, the glacier is thinning rapidly, and its ice flow is accelerating. Additionally, the sea ice cover in front of the glacier has been decreasing steadily for several decades. The Landsat Image Mosaic of Antarctica (LIMA) is a data product funded by the National Science Foundation (NSF) and jointly produced by the U.S. Geological Survey (USGS), the British Antarctic Survey (BAS), and the National Aeronautics and Space Administration (NASA). The LIMA data shown here uses the pan-chromatic band and has a resolution of 15 meters per pixel. The 13 swaths used to generate this sample mosaic where acquired between December 25, 1999 and December 31, 2001. The elevation data shown has no vertical exaggeration (1x) and is courtesy of the Radarsat Antarctic Mapping Project (RAMP) Digital Elevation Model (DEM). || ",
            "hits": 33
        },
        {
            "id": 1332,
            "url": "http://svs.gsfc.nasa.gov/1332/",
            "result_type": "Visualization",
            "release_date": "2000-06-15T12:00:00-04:00",
            "title": "TOPEX/Poseidon Flat Earth Tide Height Model",
            "description": "Data from TOPEX/Poseidon was used to produce a computer model of 16 days of tide height.  Blue is below sea level, red is above sea level. || ",
            "hits": 41
        },
        {
            "id": 1333,
            "url": "http://svs.gsfc.nasa.gov/1333/",
            "result_type": "Visualization",
            "release_date": "2000-06-15T12:00:00-04:00",
            "title": "TOPEX/Poseidon Western Hemisphere: Tide Height Model",
            "description": "Data from TOPEX/Poseidon was used to produce a computer model of 16 days of tide height.  Blue  indicates below sea level; red indicates above sea level. || ",
            "hits": 24
        },
        {
            "id": 1334,
            "url": "http://svs.gsfc.nasa.gov/1334/",
            "result_type": "Visualization",
            "release_date": "2000-06-15T12:00:00-04:00",
            "title": "TOPEX/Poseidon Eastern Hemisphere Tide Height Model",
            "description": "Data from TOPEX/Poseidon was used to produce a computer model of 16 days of tide height.  Blue indicates below sea level; red indicates above sea level. || ",
            "hits": 14
        }
    ]
}