{
    "count": 28,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 13325,
            "url": "https://svs.gsfc.nasa.gov/13325/",
            "result_type": "Produced Video",
            "release_date": "2019-09-24T13:00:00-04:00",
            "title": "The Nancy Grace Roman Space Telescope's Coronagraph Instrument",
            "description": "Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.Credit: NASA's Goddard Space Flight CenterMusic: \"Concept of Motion\" from Universe Production MusicComplete transcript available. || Roman_CGI_Still.jpg (1920x1080) [396.1 KB] || 13325_Roman_CGI_1080.mp4 (1920x1080) [96.8 MB] || 13325_Roman_CGI_Final_ProRes_1920x1080_2997.mov (1920x1080) [1.3 GB] || 13325_Roman_CGI_1080.webm (1920x1080) [13.9 MB] || Roman_CGI_SRT_Captions.en_US.srt [2.4 KB] || Roman_CGI_SRT_Captions.en_US.vtt [2.4 KB] || ",
            "hits": 351
        },
        {
            "id": 13184,
            "url": "https://svs.gsfc.nasa.gov/13184/",
            "result_type": "Produced Video",
            "release_date": "2019-04-29T00:00:00-04:00",
            "title": "Goddard at 60",
            "description": "On July 29, 1958, President Eisenhower signed the National Aeronautics and Space Act, establishing the National Aeronautics and Space Administration. When it began operations on October 1, 1958, NASA consisted mainly of the four laboratories and some 80 employees of the government's 46-year-old research agency, the National Advisory Committee for Aeronautics (NACA). Goddard Space Flight Center was established on May 1, 1959 as NASA's first space flight center.In celebration of its 60th year, we look back at the innovations and scientific impacts the women and men of Goddard have made throughout its history. || ",
            "hits": 54
        },
        {
            "id": 12238,
            "url": "https://svs.gsfc.nasa.gov/12238/",
            "result_type": "Produced Video",
            "release_date": "2017-12-22T13:00:00-05:00",
            "title": "WFIRST Will See the Big Picture of the Universe",
            "description": "Learn about the Wide Field Infrared Survey Telescope (WFIRST) mission.Music: \"We Dissolve in Stars\" and \"Climb the Ladder\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WFIRST_Beauty_still_print.jpg (1024x576) [97.2 KB] || WFIRST_Beauty_still.png (3840x2160) [36.5 MB] || WFIRST_Beauty_still.jpg (3840x2160) [988.6 KB] || WFIRST_Beauty_still_searchweb.png (320x180) [72.0 KB] || WFIRST_Beauty_still_thm.png (80x40) [5.1 KB] || YOUTUBE_1080_12238_WFIRST_Overview_V3_FINAL.mp4 (1920x1080) [845.8 MB] || 12238_WFIRST_Overview_V3_H264_1080p.mov (1920x1080) [759.1 MB] || 12238_WFIRST_Overview_V3_H264_1080_2997.m4v (1920x1080) [377.3 MB] || 12238_WFIRST_Overview_V3_H264_1080p.webm (1920x1080) [41.2 MB] || 12238_WFIRST_Overview_V3_ProRes_3840x2160_2997.mov (3840x2160) [19.3 GB] || YOUTUBE_HQ_12238_WFIRST_Overview_V3_FINAL_4k.mov (3840x2160) [6.5 GB] || 12238_WFIRST_Overview_V3_H264_4K.mov (3840x2160) [1.1 GB] || WFIRST_overview_SRT_Captions.en_US.srt [6.7 KB] || WFIRST_overview_SRT_Captions.en_US.vtt [6.4 KB] || ",
            "hits": 178
        },
        {
            "id": 12527,
            "url": "https://svs.gsfc.nasa.gov/12527/",
            "result_type": "Produced Video",
            "release_date": "2017-03-01T09:00:00-05:00",
            "title": "Goddard Memorial Symposium Tribute",
            "description": "2017 Goddard Memorial Symposium Tribute VideoMusic Credit: Killer TracksWheel of Emotion [KOK2399]In Tribute [KT178]Sentimental Adagietto [KT210]Northern Lights [SDN008] || 12527_Goddard_Mem_Sym_poster.jpg (1280x720) [87.6 KB] || 12527_Goddard_Mem_Sym_poster_searchweb.png (320x180) [54.2 KB] || 12527_Goddard_Mem_Sym_poster_thm.png (80x40) [5.3 KB] || 12527_Goddard_Mem_Sym_Tribute_appletv.m4v (1280x720) [227.4 MB] || 12527_Goddard_Mem_Sym_Tribute_h264.mov (1280x720) [751.4 MB] || 12527_Goddard_Mem_Sym_Tribute.mov (1280x720) [4.9 GB] || 12527_Goddard_Mem_Sym_Tribute.webm (960x540) [161.2 MB] || 12527_Goddard_Mem_Sym_Tribute_appletv_subtitles.m4v (1280x720) [227.5 MB] || 12527_GoddardMemSymTribute.en_US.srt [8.0 KB] || 12527_GoddardMemSymTribute.en_US.vtt [7.5 KB] || ",
            "hits": 17
        },
        {
            "id": 12433,
            "url": "https://svs.gsfc.nasa.gov/12433/",
            "result_type": "Produced Video",
            "release_date": "2017-01-13T14:30:00-05:00",
            "title": "Dark Energy Expansion Graph",
            "description": "5760x3240 resolution animation designed for 3x3 hyperwalls. || ",
            "hits": 197
        },
        {
            "id": 12434,
            "url": "https://svs.gsfc.nasa.gov/12434/",
            "result_type": "Produced Video",
            "release_date": "2017-01-13T14:30:00-05:00",
            "title": "Astronomical Object Beauty Sequences",
            "description": "5760x320 resolution video designed for 3x3 hyperwall use. || ",
            "hits": 123
        },
        {
            "id": 12417,
            "url": "https://svs.gsfc.nasa.gov/12417/",
            "result_type": "Produced Video",
            "release_date": "2017-01-13T13:00:00-05:00",
            "title": "WFIRST 2017 AAS Hyperwall Presentation",
            "description": "New hyperwall resources for Neil Gehrels' 2017 AAS talk.  Most visuals are 5760x3240 and designed for a 3x3 hyperwall with 1920x1080 screens. || ",
            "hits": 120
        },
        {
            "id": 12308,
            "url": "https://svs.gsfc.nasa.gov/12308/",
            "result_type": "Produced Video",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Hubble vs Roman Space Telescope Image Size Comparisons",
            "description": "The Nancy Grace Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics. The telescope has a primary mirror that is 2.4 meters in diameter (7.9 feet), and is the same size as the Hubble Space Telescope's primary mirror. The Roman Space Telescope will have two instruments, the Wide Field Instrument, and the Coronagraph Instrument.The Wide Field Instrument will have a field of view that is 100 times greater than the Hubble infrared instrument, capturing more of the sky with less observing time. As the primary instrument, the Wide Field Instrument will measure light from a billion galaxies over the course of the mission lifetime. It will perform a microlensing survey of the inner Milky Way to find ~2,600 exoplanets. || ",
            "hits": 697
        },
        {
            "id": 20241,
            "url": "https://svs.gsfc.nasa.gov/20241/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "The Electromagnetic Spectrum",
            "description": "Animation depicting the electromagnetic spectrum and the different characteristics of each wavelength type. 4k resolution. || WFirst_ElectromagneticSpectrum.0830_print.jpg (1024x576) [228.7 KB] || WFirst_ElectromagneticSpectrum.0830.png (3840x2160) [13.8 MB] || WFirst_ElectromagneticSpectrum.0830_searchweb.png (320x180) [105.9 KB] || WFirst_ElectromagneticSpectrum.0830_thm.png (80x40) [7.1 KB] || WFirst_LightSpectrum_Final_H264_HD_1080p.mov (1920x1080) [150.2 MB] || WFirst_LightSpectrum_Final_H264_HD_1080p.webm (1920x1080) [8.7 MB] || WFirst_LightSpectrum_Final_4K_ProRes.mov (3840x2160) [5.6 GB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || WFirst_LightSpectrum_Final_H264-4K.mov (3840x2160) [196.0 MB] || ",
            "hits": 264
        },
        {
            "id": 20242,
            "url": "https://svs.gsfc.nasa.gov/20242/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Gravitational Microlensing Animation",
            "description": "Animation illustrating how gravitational microlensing works.  4k resolution. || Lensing_00789_print.jpg (1024x576) [60.5 KB] || Lensing_00789.png (3840x2160) [7.1 MB] || Lensing_00789_searchweb.png (320x180) [54.6 KB] || Lensing_00789_thm.png (80x40) [4.4 KB] || WFIRST_Microlensing_H264_1080p.mov (1920x1080) [57.6 MB] || WFIRST_Microlensing_H264_1080p.webm (1920x1080) [3.7 MB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || WFIRST_Microlensing_H264_4k.mov (3840x2160) [76.0 MB] || WFIRST_Microlensing.key [60.0 MB] || WFIRST_Microlensing.pptx [59.7 MB] || WFIRST_Microlensing_4k_ProRes.mov (3840x2160) [2.2 GB] || ",
            "hits": 324
        },
        {
            "id": 20243,
            "url": "https://svs.gsfc.nasa.gov/20243/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Roman Space Telescope Coronagraph Animation",
            "description": "Animation illustrating how a planet can disappear in a star's bright light, and how a coronagraph can reveal it. || Coronagraph_Still_print.jpg (1024x576) [23.5 KB] || Coronagraph_Still.png (3840x2160) [4.8 MB] || Coronagraph_Still_searchweb.png (320x180) [32.9 KB] || Coronagraph_Still_thm.png (80x40) [3.2 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.mov (1920x1080) [28.1 MB] || 3840x2160_16x9_60p (3840x2160) [128.0 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_4K.mov (3840x2160) [47.0 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.webm (3840x2160) [3.3 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.key [29.9 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.pptx [29.6 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.mov (3840x2160) [2.4 GB] || ",
            "hits": 256
        },
        {
            "id": 20244,
            "url": "https://svs.gsfc.nasa.gov/20244/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Dark Matter Gravitational Lensing Animation",
            "description": "Animation illustrating light from a cluster of galaxies being lensed by dark matter. || GravLens_fr_00168_print.jpg (1024x576) [59.0 KB] || GravLens_fr_00168.png (3840x2160) [3.1 MB] || GravLens_fr_00168_searchweb.png (320x180) [43.7 KB] || GravLens_fr_00168_thm.png (80x40) [4.4 KB] || GravLens_H2641080p.mov (1920x1080) [27.1 MB] || GravLens_H2641080p.webm (1920x1080) [1.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || GravLens_H264_4K.mov (3840x2160) [35.4 MB] || GravLens_4k_ProRes.mov (3840x2160) [1.4 GB] || ",
            "hits": 285
        },
        {
            "id": 20245,
            "url": "https://svs.gsfc.nasa.gov/20245/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Roman Space Telescope Orbit Diagrams",
            "description": "Animation showing Earth's orbit. Then the type of planet the Roman Space Telescope will be able to directly observe: roughly Neptune size in a 1.6AU or greater orbit. And, finally, the type of planet at the current limit of direct observation: Jupiter-size or larger and 40AU from its host star. || WFIRST_OrbitScale_REV_003_0806_print.jpg (1024x576) [99.9 KB] || WFIRST_OrbitScale_REV_003_0806.png (3840x2160) [6.0 MB] || WFIRST_OrbitScale_REV_003_0806.jpg (3840x2160) [1.2 MB] || WFIRST_OrbitScale_REV_003_0806_searchweb.png (320x180) [47.0 KB] || WFIRST_OrbitScale_REV_003_0806_thm.png (80x40) [2.9 KB] || WFIRST_OrbitScale_Rev003_1080p.mov (1920x1080) [42.1 MB] || WFIRST_OrbitScale_Rev003_1080.m4v (1920x1080) [21.7 MB] || WFIRST_OrbitScale_Rev003_1080p.webm (1920x1080) [2.3 MB] || WFIRST_OrbitScale_Rev003_4k_60_ProRes.mov (3840x2160) [3.0 GB] || 3840x2160_16x9_60p (3840x2160) [128.0 KB] || WFIRST_OrbitScale_Rev003_4k.mov (3840x2160) [59.4 MB] || ",
            "hits": 248
        },
        {
            "id": 20246,
            "url": "https://svs.gsfc.nasa.gov/20246/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Dark Energy Expansion",
            "description": "Animation illustrating the accelerating expansion of the universe. || WFirstExpansion_00599_print.jpg (1024x576) [151.6 KB] || WFirstExpansion_00599.png (3840x2160) [25.8 MB] || WFirstExpansion_00599_searchweb.png (180x320) [82.7 KB] || WFirstExpansion_00599_thm.png (80x40) [5.7 KB] || WFIRST_Dark_Energy_Expansion_H264_1080p.mov (1920x1078) [26.9 MB] || WFIRST_Dark_Energy_Expansion_H264_1080p.webm (1920x1078) [1.7 MB] || 3840x2160_16x9_30p (4104x2304) [0 Item(s)] || WFIRST_Dark_Energy_Expansion_H264_4K.mov (4096x2300) [36.0 MB] || WFIRST_Dark_Energy_Expansion_4k_ProRes.mov (4104x2304) [768.2 MB] || ",
            "hits": 699
        },
        {
            "id": 4470,
            "url": "https://svs.gsfc.nasa.gov/4470/",
            "result_type": "Visualization",
            "release_date": "2016-09-20T00:00:00-04:00",
            "title": "WFIRST: The Road to L2",
            "description": "This visualization follows the WFIRST telescope on its trajectory to the Sun-Earth Lagrange Two point. || WFIRST.path2L2.relative_RigRHS.HD1080i.1400_print.jpg (1024x576) [92.9 KB] || WFIRST.path2L2.relative_RigRHS.HD1080i.1400_searchweb.png (180x320) [60.8 KB] || WFIRST.path2L2.relative_RigRHS.HD1080i.1400_thm.png (80x40) [3.2 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || WFIRST.path2L2.relative.HD1080i_p30.mp4 (1920x1080) [50.6 MB] || WFIRST.path2L2.relative.HD1080i_p30.webm (1920x1080) [6.0 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || WFIRST.path2L2.relative.UHD2160_p30.mp4 (3840x2160) [178.1 MB] || WFIRST.path2L2.relative.HD1080i_p30.mp4.hwshow [201 bytes] || ",
            "hits": 156
        },
        {
            "id": 4471,
            "url": "https://svs.gsfc.nasa.gov/4471/",
            "result_type": "Visualization",
            "release_date": "2016-09-20T00:00:00-04:00",
            "title": "WFIRST: The Road to L2. The view from above",
            "description": "This visualization views the WFIRST trajectory to Sun-Earth Lagrange Two point from above the ecliptic plane. || WFIRST.polar.relative_RigRHS.HD1080i.1500_print.jpg (1024x576) [105.7 KB] || WFIRST.polar.relative_RigRHS.HD1080i.1500_searchweb.png (320x180) [66.6 KB] || WFIRST.polar.relative_RigRHS.HD1080i.1500_thm.png (80x40) [3.4 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || WFIRST.polar.relative.HD1080i_p30.mp4 (1920x1080) [90.4 MB] || WFIRST.polar.relative.HD1080i_p30.webm (1920x1080) [8.4 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || WFIRST.polar.relative.UHD2160_p30.mp4 (3840x2160) [314.8 MB] || WFIRST.polar.relative.HD1080i_p30.mp4.hwshow [199 bytes] || ",
            "hits": 89
        },
        {
            "id": 4472,
            "url": "https://svs.gsfc.nasa.gov/4472/",
            "result_type": "Visualization",
            "release_date": "2016-09-20T00:00:00-04:00",
            "title": "WFIRST: The Road to L2. Oblique view",
            "description": "This visualization views the WFIRST trajectory to Sun-Earth Lagrange Two point from above the ecliptic plane. || WFIRST.oblique.relative_RigRHS.HD1080i.1500_print.jpg (1024x576) [115.7 KB] || WFIRST.oblique.relative_RigRHS.HD1080i.1500_searchweb.png (320x180) [70.4 KB] || WFIRST.oblique.relative_RigRHS.HD1080i.1500_thm.png (80x40) [4.2 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || WFIRST.oblique.relative.HD1080i_p30.webm (1920x1080) [8.4 MB] || WFIRST.oblique.relative.HD1080i_p30.mp4 (1920x1080) [112.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || WFIRST.oblique.relative.UHD2160_p30.mp4 (3840x2160) [357.3 MB] || WFIRST.oblique.relative.HD1080i_p30.mp4.hwshow [201 bytes] || ",
            "hits": 73
        },
        {
            "id": 12153,
            "url": "https://svs.gsfc.nasa.gov/12153/",
            "result_type": "Produced Video",
            "release_date": "2016-02-18T11:00:00-05:00",
            "title": "WFIRST: The Best of Both Worlds",
            "description": "With a view 100 times bigger than that of NASA’s Hubble Space Telescope, the Wide Field Infrared Survey Telescope WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life.  Scientists participating in the mission discuss the spacecraft, the science, and its potential.  Slated to launch in the mid-2020s, the observatory will operate at a gravitational balance point known as Earth-sun L2, which is located about 930,000 miles from Earth and directly opposite the sun.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WfirstAfta-PrintStill2_print.jpg (1024x576) [79.3 KB] || WfirstAfta-PrintStill2.png (3840x2160) [4.7 MB] || WfirstAfta-PrintStill2_searchweb.png (320x180) [59.2 KB] || WfirstAfta-PrintStill2_thm.png (80x40) [4.6 KB] || 12153_WFIRST_Best_Both_Worlds_ProRes_1280x720_5994.mov (1280x720) [3.1 GB] || 12153_WFIRST_Best_Both_Worlds_H264_Best_1280x720_5994.mov (1280x720) [1.7 GB] || 12153_WFIRST_Best_Both_Worlds_FINAL_youtube_hq.mov (1280x720) [671.5 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.mov (1280x720) [174.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv.m4v (1280x720) [122.3 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.webm (1280x720) [25.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv_subtitles.m4v (1280x720) [122.4 MB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.srt [4.6 KB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.vtt [4.4 KB] || NASA_PODCAST_12153_WFIRST_Best_Both_Worlds_FINAL_ipod_sm.mp4 (320x240) [41.6 MB] || ",
            "hits": 156
        },
        {
            "id": 12027,
            "url": "https://svs.gsfc.nasa.gov/12027/",
            "result_type": "Produced Video",
            "release_date": "2015-11-23T11:00:00-05:00",
            "title": "NASM 2015: Our Violent Universe",
            "description": "NASM 2015 Presentation - Our Violent Universe || poster-VX-73356-00-00-25,41.jpg (1280x720) [159.6 KB] || poster-VX-73356-00-00-25,41_searchweb.png (320x180) [94.7 KB] || poster-VX-73356-00-00-25,41_thm.png (80x40) [6.8 KB] || APPLE_TV_G2015-086_NASM_2015_appletv.m4v (1280x720) [1.6 GB] || NASA_TV_G2015-086_NASM_2015.mpeg (1280x720) [10.9 GB] || WMV_G2015-086_NASM_2015_HD.wmv (1280x720) [630.3 MB] || YOUTUBE_HQ_G2015-086_NASM_2015_youtube_hq.mov (1280x720) [8.3 GB] || G2015-086_NASM_2015_edited.mov (1280x720) [29.2 GB] || WEBM_G2015-086_NASM_2015.webm (960x540) [1.3 GB] || APPLE_TV_G2015-086_NASM_2015_appletv_subtitles.m4v (1280x720) [1.6 GB] || G2015-086_NASM2015.en_US.srt [77.0 KB] || G2015-086_NASM2015.en_US.vtt [72.4 KB] || NASA_PODCAST_G2015-086_NASM_2015_ipod_sm.mp4 (320x240) [589.1 MB] || ",
            "hits": 92
        },
        {
            "id": 12055,
            "url": "https://svs.gsfc.nasa.gov/12055/",
            "result_type": "Produced Video",
            "release_date": "2015-11-12T11:00:00-05:00",
            "title": "1,000 and Counting",
            "description": "NASA's Swift spacecraft spots its thousandth gamma-ray burst. || c-1280.jpg (1280x720) [182.8 KB] || c-1024.jpg (1024x576) [132.0 KB] || c-1024_print.jpg (1024x576) [139.3 KB] || c-1024_searchweb.png (320x180) [74.7 KB] || c-1024_web.png (320x180) [74.7 KB] || c-1024_thm.png (80x40) [19.5 KB] || ",
            "hits": 44
        },
        {
            "id": 12038,
            "url": "https://svs.gsfc.nasa.gov/12038/",
            "result_type": "Produced Video",
            "release_date": "2015-11-06T13:00:00-05:00",
            "title": "NASA's Swift Catches its 1,000th Gamma-ray Burst",
            "description": "Labeled image. GRB 151027B, Swift's 1,000th burst (center), is shown in this composite X-ray, ultraviolet and optical image. X-rays were captured by Swift's X-Ray Telescope, which began observing the field 3.4 minutes after the Burst Alert Telescope detected the blast. Swift's Ultraviolet/Optical Telescope (UVOT) began observations seven seconds later and faintly detected the burst in visible light. The image includes X-rays with energies from 300 to 6,000 electron volts, primarily from the burst, and lower-energy light seen through the UVOT's visible, blue and ultraviolet filters (shown, respectively, in red, green and blue). The image has a cumulative exposure of 10.4 hours.  Credit: NASA/Swift/Phil Evans, Univ. of Leicester || grb151027B_UVOT_XRT_labeled_1080.jpg (912x1080) [403.9 KB] || grb151027B_UVOT_XRT_labeled_2160_print.jpg (1024x1213) [394.1 KB] || grb151027B_UVOT_XRT_labeled_2160.jpg (1823x2160) [1.0 MB] || grb151027B_UVOT_XRT_labeled_2160_searchweb.png (320x180) [43.8 KB] || grb151027B_UVOT_XRT_labeled_2160_thm.png (80x40) [3.6 KB] || ",
            "hits": 158
        },
        {
            "id": 11792,
            "url": "https://svs.gsfc.nasa.gov/11792/",
            "result_type": "Produced Video",
            "release_date": "2015-03-03T00:00:00-05:00",
            "title": "Inspiring Women in Science",
            "description": "Favorite ScienceWoman - Katrina's CutThis is a video Katrina edited of everyone talking about their favorite #ScienceWoman.For complete transcript, click here. || Favorite_ScienceWoman_Katrinas_cut_youtube_hq.00527_print.jpg (1024x576) [110.3 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_print.jpg (1024x576) [118.6 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_thm.png (80x40) [6.1 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_web.png (320x180) [85.7 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_searchweb.png (320x180) [85.7 KB] || Favorite_ScienceWoman_Katrinas_cut_1280x720.wmv (1280x720) [161.3 MB] || Favorite_ScienceWoman_Katrinas_cut_appletv_subtitles.m4v (960x540) [133.2 MB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq.mov (1280x720) [148.5 MB] || Favorite_ScienceWoman_Katrinas_cut_appletv.m4v (960x540) [133.3 MB] || Favorite_ScienceWoman_Katrinas_cut_prores.mov (1280x720) [4.8 GB] || Favorite_ScienceWoman_Katrinas_cut_720x480.webm (720x480) [35.5 MB] || Favorite_ScienceWoman_Katrinas_cut_720x480.wmv (720x480) [104.4 MB] || Favorite_ScienceWoman_Katrinas_cut_ipod_lg.m4v (640x360) [53.1 MB] || Favorite_ScienceWoman.en_US.srt [6.5 KB] || Favorite_ScienceWoman.en_US.vtt [6.5 KB] || Favorite_ScienceWoman_Katrinas_cut_nasaportal.mov (640x360) [127.5 MB] || Favorite_ScienceWoman_Katrinas_cut_ipod_sm.mp4 (320x240) [28.5 MB] || ",
            "hits": 18
        },
        {
            "id": 10171,
            "url": "https://svs.gsfc.nasa.gov/10171/",
            "result_type": "Produced Video",
            "release_date": "2014-11-20T14:00:00-05:00",
            "title": "Swift: A Decade of Game-Changing Astrophysics",
            "description": "Scientists participating in NASA's Swift mission discuss the spacecraft, the science, and recall their personal experiences as members of the team.Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Swift_Interview_Still_print.jpg (1024x576) [160.8 KB] || Swift_Interview_Still.png (2560x1440) [4.1 MB] || Swift_Interview_Still_web.jpg (180x320) [21.2 KB] || Swift_Interview_Still_thm.png (80x40) [9.1 KB] || Swift_Interview_Still_web.png (320x180) [95.3 KB] || Swift_Interview_Still_searchweb.png (180x320) [95.3 KB] || Swift_10_Interviews_MPEG4_1280X720_2997.mp4 (1280x720) [149.1 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.webmhd.webm (960x540) [98.0 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.m4v (960x540) [257.7 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv_subtitles.m4v (960x540) [257.5 MB] || G2014-067_Swift_10_Interviews_FINAL_1280x720.wmv (1280x720) [292.3 MB] || Swift_10_Interviews_H264_Good_1280x720_2997.mov (1280x720) [551.2 MB] || Swift_10_Interviews_H264_640x360_2997_iPhone.m4v (640x360) [94.6 MB] || G2014-067_Swift_10_Interviews.en_US.srt [11.7 KB] || G2014-067_Swift_10_Interviews.en_US.vtt [11.7 KB] || G2014-067_Swift_10_Interviews_FINAL_ipod_lg.m4v (640x360) [102.9 MB] || G2014-067_Swift_10_Interviews_FINAL_ipod_sm.mp4 (320x240) [51.9 MB] || Swift_10_Interviews_H264_Best_1280x720_5994.mov (1280x720) [3.9 GB] || Swift_10_Interviews_ProRes_1280x720_5994.mov (1280x720) [8.7 GB] || ",
            "hits": 100
        },
        {
            "id": 11553,
            "url": "https://svs.gsfc.nasa.gov/11553/",
            "result_type": "Produced Video",
            "release_date": "2014-05-30T13:00:00-04:00",
            "title": "WFIRST: Uncovering the Mysteries of the Universe",
            "description": "The Wide-Field Infrared Survey Telescope (WFIRST) is an upcoming space telescope designed to perform wide-field imaging and spectroscopy of the infrared sky. One of WFIRST’s objectives will be looking for clues about dark energy—the mysterious force that is accelerating the expansion of the universe.  Another objective of the mission will be finding and studying exoplanets. WFIRST uses the same 2.4 meter telescope size as Hubble, but with 18 cutting-edge fourth-generation image sensors compared to Hubble's single first-generation sensor. As a result, each WFIRST image will cover over 200 times as much as a Hubble Wide Field Camera 3/IR image and be 300 megapixels in size.  Hubble images reveal thousands of galaxies; a single WFIRST image will uncover millions.To help uncover the mystery of dark energy, WFIRST will make incredibly precise measurements of the universe.  These measurements, like the distance and position of galaxies, can be compared to other measurements—such as the cosmic microwave background from the WMAP mission—to determine how dark energy has changed over time.  WFIRST can also measure the slight distortions in light from distant galaxies as it passes more nearby mass concentrations.  These data will build a three dimensional picture of how mass is distributed throughout the universe, and provide independent confirmation of its structure.Because WFIRST has such a large and sensitive field of view, it can find thousands of new exoplanets through a process called microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the gravitational \"attraction\" of the foreground star. This \"lens\" star is then a virtual magnifying glass, amplifying the brightness of the background source star. If the lens star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source.  For closer planets, WFIRST will open a new era of direct observation.  Currently only a handful of planets are observable in light reflected off of them, and they are all large planets close to their stars.  WFIRST will be able to detect planets as small as Neptune, and as far from their stars as Saturn is from the sun.  This is possible thanks to newly developed  coronagraphs, which block the bright light from the star to make the planet more visible. || ",
            "hits": 109
        },
        {
            "id": 10861,
            "url": "https://svs.gsfc.nasa.gov/10861/",
            "result_type": "Produced Video",
            "release_date": "2011-11-03T14:00:00-04:00",
            "title": "Fermi Pulsar Interactive Videos",
            "description": "These videos originally accompanied a Fermi Pulsar Interactive.  That interactive is now available here. || ",
            "hits": 224
        },
        {
            "id": 10253,
            "url": "https://svs.gsfc.nasa.gov/10253/",
            "result_type": "Produced Video",
            "release_date": "2008-09-26T01:00:00-04:00",
            "title": "Scientists Watch Baby Black Hole Get to Work Fast",
            "description": "Scientists using NASA's Swift satellite say they have found newborn black holes, just seconds old, in a confused state of existence, sloppily gorging on material falling into them while somehow propelling other material away at great speeds. These black holes are born in massive star explosions. An initial blast obliterates the star. Yet the chaotic black hole activity appears to re-energize the explosion again and again over the course of several minutes. This is a dramatically different view of star death, one that entails multiple explosive outbursts and not just a single bang, as previously thought.When a massive star runs out of fuel, it no longer has the energy to support its mass. The core collapses and forms a black hole. Shockwaves bounce out and obliterate the outer shells of the star. Previously scientists thought that a single explosion is followed by a graceful afterglow of the dying embers. Now, according to Swift observations, it appears that a newborn black hole in the core somehow re-energizes the explosion again and again, creating multiple bursts all within a few minutes. || ",
            "hits": 123
        },
        {
            "id": 10251,
            "url": "https://svs.gsfc.nasa.gov/10251/",
            "result_type": "Produced Video",
            "release_date": "2008-05-31T00:00:00-04:00",
            "title": "GLAST Prelude, for Brass Quintet, Op.12",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institiutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S. Music composed by Nolan Gasser, © 2008 Music performed by the American Brass Quintet || ",
            "hits": 70
        },
        {
            "id": 20077,
            "url": "https://svs.gsfc.nasa.gov/20077/",
            "result_type": "Animation",
            "release_date": "2006-08-18T00:00:00-04:00",
            "title": "Cosmic Explosion Second Only to the Sun in Brightness",
            "description": "The gamma ray flare produced by neutron star SGR 1806-20, traveled 50,000 light years before impacting Earth. The burst was so powerful, that it disrupted Earth's ionosphere. Scientists know of only two other giant flares in the past 35 years, and this December 27, 2005 event was one hundred times more powerful than either of those || ",
            "hits": 248
        }
    ]
}