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        {
            "id": 14937,
            "url": "https://svs.gsfc.nasa.gov/14937/",
            "result_type": "Produced Video",
            "release_date": "2025-12-23T11:00:00-05:00",
            "title": "NASA's Roman Space Telescope: Widening Our Gaze",
            "description": "The NASA Astrophysics fleet of spacecraft has an impressive range of capabilities. What is the next step in exploring the cosmos? The Nancy Grace Roman Space Telescope, NASA’s upcoming flagship mission, will take Hubble’s resolution and widen its infrared view to more than 100 times the coverage in every single image. Roman is a survey telescope that can peer through the Milky Way’s obscuring dust, and see faint, distant galaxies. Roman’s rigid design allows it to scan large regions of sky very quickly. Hubble would take 1,000 years to observe what Roman can see in one. Roman’s 18 4k x 4k detectors create 300-megapixel images covering an area of sky slightly larger than the full Moon. Roman will also look at the same regions of space repeatedly over time, allowing astronomers to see changes and observe temporary events like supernovae. Roman’s surveys of deep space and the center of our Milky Way galaxy will find thousands of new exoplanets, survey millions of galaxies, help us understand dark matter and dark energy, and learn more about the evolution of the universe. || ",
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        },
        {
            "id": 14939,
            "url": "https://svs.gsfc.nasa.gov/14939/",
            "result_type": "Produced Video",
            "release_date": "2025-12-19T00:00:00-05:00",
            "title": "Multi-camera Time-lapse of Roman's Assembly Completion",
            "description": "NASA’s next big eye on the cosmos is now fully assembled. On Nov. 25, technicians joined the inner and outer portions of the Nancy Grace Roman Space Telescope in the largest clean room at the agency’s Goddard Space Flight Center in Greenbelt, Maryland. || ",
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        },
        {
            "id": 14869,
            "url": "https://svs.gsfc.nasa.gov/14869/",
            "result_type": "Produced Video",
            "release_date": "2025-07-18T11:00:00-04:00",
            "title": "STORIE Fit Test at NASA Goddard Space Flight Center",
            "description": "NASA’s STORIE mission, or Storm Time O+ Ring current Imaging Evolution, has completed its design, build, and testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its mission onboard the International Space Station (ISS). From its unique vantage point on the ISS, STORIE will use neutral atom imaging to provide an “inside out” view of Earth’s ring current – a region of the magnetosphere where energetic particles are trapped in near-Earth space. In addition to answering fundamental questions about the ring current’s intensity and composition, STORIE will also provide a more detailed understanding of how geomagnetic storms affect Earth.From NASA’s Goddard Space Flight Center, STORIE will be shipped to NASA’s Johnson Space Center in Houston, Texas, where it will be integrated onto a pallet to be installed outside the ISS’s Columbus Module. STORIE will head to the ISS aboard a SpaceX commercial resupply flight no earlier than spring 2026. || ",
            "hits": 32
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        {
            "id": 14836,
            "url": "https://svs.gsfc.nasa.gov/14836/",
            "result_type": "Infographic",
            "release_date": "2025-05-07T00:00:00-04:00",
            "title": "Roman Systems Infographic",
            "description": "This infographic shows the two major subsystems that make up NASA’s Nancy Grace Roman Space Telescope. The subsystems are each undergoing testing prior to being joined together this fall. || Roman_Systems_Infographic_V1_Final_print.jpg (1024x576) [160.5 KB] || Roman_Systems_Infographic_V1_Final_16bit.png (3840x2160) [30.7 MB] || Roman_Systems_Infographic_V1_Final_8bit.png (3840x2160) [8.2 MB] || Roman_Systems_Infographic_V1_Final.jpg (3840x2160) [1.2 MB] || Roman_Systems_Infographic_V1_Final_searchweb.png (320x180) [88.8 KB] || Roman_Systems_Infographic_V1_Final_thm.png [6.4 KB] || ",
            "hits": 109
        },
        {
            "id": 14759,
            "url": "https://svs.gsfc.nasa.gov/14759/",
            "result_type": "Produced Video",
            "release_date": "2025-01-21T00:00:00-05:00",
            "title": "Roman's Wide Field Instrument added to the Mirror Assembly",
            "description": "B-roll footage slowed from 60 frames per second and 30 frames per second of the Wide Field Instrument (WFI) installation. || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_print.jpg (1024x576) [202.4 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_searchweb.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_web.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly_ProRes.mov (3840x2160) [35.6 MB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_thm.png [6.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.mp4 (3840x2160) [3.8 GB] || ",
            "hits": 64
        },
        {
            "id": 14491,
            "url": "https://svs.gsfc.nasa.gov/14491/",
            "result_type": "Produced Video",
            "release_date": "2023-12-26T00:00:00-05:00",
            "title": "Roman Hardware Highlights",
            "description": "This video, covering the second half of 2025, opens with a person entering NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.The outside half of Roman, called OSD, contains the solar panels and protective layers. The Deployable Aperture Cover, which protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space. Then the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool.In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right, and forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as they anticipated.While these tests occur, Roman’s inside half, containing the mirrors, instruments and support equipment, move into Goddard’s largest thermal vacuum chamber, the SES (Space Environment Simulator). This 40-foot-tall chamber can simulate the vacuum of space and the wide temperature range that Roman will experience there: from -310° Fahrenheit (-190° C) to 302° Fahrenheit (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned both horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.Music credit: “Our Journey Begins,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_SummerFall2025_3.jpg (1280x720) [473.7 KB] || Roman_HH_Summer-Fall2025_10mbps.mp4 (1920x1080) [185.0 MB] || Roman_HH_Summer-Fall2025_25mbps.mp4 (1920x1080) [452.7 MB] || Roman_HH_Summer-Fall2025_YT.mp4 (1920x1080) [880.2 MB] || RomanHHLate2025Captions.en_US.srt [588 bytes] || RomanHHLate2025Captions.en_US.vtt [570 bytes] || Roman_HH_Summer-Fall2025_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || ",
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        },
        {
            "id": 14443,
            "url": "https://svs.gsfc.nasa.gov/14443/",
            "result_type": "B-Roll",
            "release_date": "2023-10-17T00:00:00-04:00",
            "title": "Aerial Views of Goddard: Integration and Test Facilities",
            "description": "Building 29, home of the largest high-bay clean room in the world, stands prominently in this panoramic aerial view of NASA's Goddard Space Flight Center in Greenbelt, Maryland. The clean room is as tall as an eight-story building and as wide as two basketball courts. The circular structure left of center houses the High Capacity Centrifuge, which is used to simulate launch and landing loads on spacecraft hardware. Imaged Oct. 5, 2023, looking south-southwest.Credit: NASA/Francis Reddy || B29_pano_01_10_05_2023_looking_SSW_1080.jpg (2434x1080) [1.7 MB] || B29_pano_01_10_05_2023_looking_SSW_3840.jpg (8653x3840) [16.5 MB] || B29_pano_01_10_05_2023_looking_SSW_1080_searchweb.png (320x180) [128.1 KB] || B29_pano_01_10_05_2023_looking_SSW_1080_thm.png (80x40) [23.3 KB] || B29_pano_01_10_05_2023_looking_SSW.tif (13745x6100) [479.8 MB] || ",
            "hits": 75
        },
        {
            "id": 14409,
            "url": "https://svs.gsfc.nasa.gov/14409/",
            "result_type": "Produced Video",
            "release_date": "2023-09-08T00:00:00-04:00",
            "title": "Roman High-Gain Antenna Dish Integration",
            "description": "The Nancy Grace Roman Space Telescope’s high-gain antenna system has been integrated onto the spacecraft’s communications panel. The almost-6-foot dish is integral to Roman’s communications process; once Roman is launched, the dish will “beam down” data to ground systems across the globe.Music: \"Chasing Rainbows\" from Universal Production MusicComplete transcript available. || HGA_Integration_16x9_Still.jpg (1920x1080) [943.8 KB] || HGA_Integration_16x9_Still_searchweb.png (320x180) [107.9 KB] || HGA_Integration_16x9_Still_thm.png (80x40) [7.9 KB] || HGA_Integration_1080.webm (1920x1080) [6.8 MB] || HGA_Integration_1080.mp4 (1920x1080) [122.5 MB] || HGA_Integration_ProRes_1920x1080_2997.mov (1920x1080) [897.2 MB] || ",
            "hits": 47
        },
        {
            "id": 13882,
            "url": "https://svs.gsfc.nasa.gov/13882/",
            "result_type": "Produced Video",
            "release_date": "2021-06-25T00:00:00-04:00",
            "title": "NASA Administrator Sen. Bill Nelson visits Goddard",
            "description": "B-ROLL: Goddard Employee Social with Administrator Nelson || Employee_Social.png (1680x942) [2.4 MB] || Employee_Social_print.jpg (1024x574) [134.4 KB] || Employee_Social_searchweb.png (320x180) [111.8 KB] || Employee_Social_thm.png (80x40) [14.0 KB] || 13882_Sen_Nelson_Visit_B-roll_1of3.mov (1920x1080) [1.7 GB] || 13882_Sen_Nelson_Visit_B-roll_1of3_youtube_1080.mp4 (1920x1080) [174.8 MB] || 13882_Sen_Nelson_Visit_B-roll_1of3_youtube_1080.webm (1920x1080) [13.5 MB] || ",
            "hits": 36
        },
        {
            "id": 13337,
            "url": "https://svs.gsfc.nasa.gov/13337/",
            "result_type": "Produced Video",
            "release_date": "2019-10-09T11:00:00-04:00",
            "title": "The James Webb Space Telescope is now an Assembled Observatory",
            "description": "Engineers from NASA and Northrop Grumman have successfully integrated the James Webb Space Telescope's optical telescope element and spacecraft element together at Northrop Grumman in Redondo Beach, CA. Thus completing the construction of the most complex and powerful telescope ever built.  Webb will explore the cosmos using infrared light from planets and moons within our solar system to the earliest and most distant galaxies.  Next up for Webb; Deploying the five-layer sunshield designed to keep Webb's mirror and scientific instruments super cold. || ",
            "hits": 75
        },
        {
            "id": 13317,
            "url": "https://svs.gsfc.nasa.gov/13317/",
            "result_type": "B-Roll",
            "release_date": "2019-09-23T00:00:00-04:00",
            "title": "James Webb Space Telescope Integration B-Roll",
            "description": "B-Roll footage from the first day of engineers integrating the James Webb Space Telescope's optical telescope element with the Instrument package (OTIS) to the spacecraft element at Northrop Grumman in Redondo Beach, CA. || Day_1_print.jpg (1024x575) [173.7 KB] || Day_1.png (3344x1878) [7.8 MB] || Day_1_searchweb.png (320x180) [119.1 KB] || Day_1_thm.png (80x40) [11.8 KB] || JWST_Integration_Day_1.mov (1920x1080) [7.8 GB] || JWST_Integration_Day_1.mp4 (1920x1080) [493.3 MB] || JWST_Integration_Day_1_.webm (1920x1080) [71.2 MB] || ",
            "hits": 30
        },
        {
            "id": 30988,
            "url": "https://svs.gsfc.nasa.gov/30988/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-08-29T00:00:00-04:00",
            "title": "Earth System Diagram",
            "description": "Diagram showing parts of the Earth system. || earth_system_diagram_print.jpg (1024x574) [115.6 KB] || earth_system_diagram.png (4104x2304) [1.2 MB] || earth_system_diagram_searchweb.png (320x180) [63.5 KB] || earth_system_diagram_thm.png (80x40) [6.6 KB] || earth_system_diagram.hwshow [208 bytes] || ",
            "hits": 444
        },
        {
            "id": 12917,
            "url": "https://svs.gsfc.nasa.gov/12917/",
            "result_type": "Produced Video",
            "release_date": "2018-04-13T19:00:00-04:00",
            "title": "Parker Solar Probe Travels to Florida",
            "description": "Parker Solar Probe Arrives in FloridaOn April 4, 2018, Parker Solar Probe project scientist Nicky Fox of Johns Hopkins APL describes the spacecraft's April 3 journey to Florida and arrival at Astrotech Space Operations, the probe's new home before a scheduled launch on July 31, 2018 from NASA's Kennedy Space Center. Credit: NASA/Johns Hopkins APL/Lee HobsonWatch this video on the Johns Hopkins APL YouTube channel. || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_print.jpg (1024x576) [103.8 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_thm.png (80x40) [7.1 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_web.png (320x180) [85.2 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_searchweb.png (320x180) [85.2 KB] || PRORES_B-ROLL_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_prores.mov (1280x720) [642.5 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv_subtitles.m4v (1280x720) [48.0 MB] || NASA_TV_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mpeg (1280x720) [309.1 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv.m4v (1280x720) [48.0 MB] || YOUTUBE_1080_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_1080.mp4 (1920x1080) [146.4 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.mp4 (3840x2160) [97.6 MB] || Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mp4 (3840x2160) [502.0 MB] || YOUTUBE_4K_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_4k.mp4 (3840x2160) [373.1 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.webm (3840x2160) [12.3 MB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.srt [1.3 KB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.vtt [1.3 KB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_Prores.mov (3840x2160) [4.9 GB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_ipod_sm.mp4 (320x240) [15.8 MB] || ",
            "hits": 179
        },
        {
            "id": 12843,
            "url": "https://svs.gsfc.nasa.gov/12843/",
            "result_type": "Produced Video",
            "release_date": "2018-02-08T11:00:00-05:00",
            "title": "TESS Undergoes Integration and Testing",
            "description": "See highlights from the assembly and testing of the TESS spacecraft.Music: \"Prototype\" and \"Trial\" both from Killer Tracks.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_IandT_Still.png (1920x1080) [2.1 MB] || TESS_IandT_Still_print.jpg (1024x576) [84.6 KB] || TESS_IandT_Still_searchweb.png (320x180) [67.2 KB] || TESS_IandT_Still_thm.png (80x40) [5.7 KB] || 12843_TESS_IntegrationandTesting_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || 12843_TESS_IntegrationandTesting_H264_Good.m4v (1920x1080) [212.7 MB] || 12843_TESS_IntegrationandTesting_H264_1080.mov (1920x1080) [321.5 MB] || 12843_TESS_IntegrationandTesting_FINAL.mp4 (1920x1080) [324.0 MB] || 12843_TESS_IntegrationandTesting_ProRes_1920x1080_2997.webm (1920x1080) [24.2 MB] || 12843_TESS_IntegrationandTesting_SRT_Captions.en_US.srt [2.7 KB] || 12843_TESS_IntegrationandTesting_SRT_Captions.en_US.vtt [2.7 KB] || ",
            "hits": 179
        },
        {
            "id": 11294,
            "url": "https://svs.gsfc.nasa.gov/11294/",
            "result_type": "Produced Video",
            "release_date": "2013-06-07T14:00:00-04:00",
            "title": "GPM High-resolution Still Images",
            "description": "These are images documenting the building, integration and testing of the Global Precipitation Measurement (GPM) mission. The most recent developments are listed first.For additional images please visit the Precipitation Measurement Missions Image Gallery. || Vibration testing of the horizontal axis of the spacecraft.Credit: NASA || GPM_horiz_vibe.png (3456x5184) [26.4 MB] || GPM_horiz_vibe_web.png (320x480) [312.0 KB] || GPM_horiz_vibe_thm.png (80x40) [10.5 KB] || ",
            "hits": 49
        },
        {
            "id": 4057,
            "url": "https://svs.gsfc.nasa.gov/4057/",
            "result_type": "Visualization",
            "release_date": "2013-03-25T00:00:00-04:00",
            "title": "LEND Looks for Water at the South Pole",
            "description": "Since Lunar Reconnaissance Orbiter (LRO) entered lunar orbit in 2009, its neutron detector, LEND, has been counting the neutrons coming from the Moon's surface.Neutrons are created when galactic cosmic rays strike atoms in the lunar regolith. These neutrons bounce from atom to atom like billiard balls, losing energy with each collision. Along the way, some of these neutrons escape into space, where LEND can detect them.The presence of hydrogen in the lunar soil reduces the number of neutrons that escape. To map out likely deposits of water ice, LEND scientists look for this deficit of neutrons in the epithermal (medium) energy range.If the deficit were simply due to random fluctuations, the hydrogen map would never coalesce into a sharp image, but as this animation shows, the map of epithermal neutron deficit at the south pole of the Moon improves over time and converges on particular spots. These include especially strong signals in the permanently shadowed parts of Cabeus and Shoemaker craters, where ice would be completely shielded from the sun. But LEND and other missions have found signs of water in places that aren't permanently shadowed while apparently excluding some places that are, both of which are surprising and exciting discoveries. || ",
            "hits": 516
        },
        {
            "id": 11053,
            "url": "https://svs.gsfc.nasa.gov/11053/",
            "result_type": "B-Roll",
            "release_date": "2012-07-30T00:00:00-04:00",
            "title": "MAVEN Broadcast-Quality Spacecraft and Instrument Footage",
            "description": "This page contains broadcast-quality footage of the MAVEN spacecraft and science instruments. The MAVEN bus was built at Lockheed Martin Space Systems in Littleton, Colorado. MAVEN's science instruments were built at the Space Sciences Laboratory (SSL) at the University of California, Berkeley; at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado, Boulder; and at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Launch operations were conducted at the Kennedy Space Center on Cape Canaveral, Florida. MAVEN was launched on November 18, 2013 and arrived at Mars on September 21, 2014 EDT. || ",
            "hits": 44
        },
        {
            "id": 10782,
            "url": "https://svs.gsfc.nasa.gov/10782/",
            "result_type": "Produced Video",
            "release_date": "2011-07-22T09:00:00-04:00",
            "title": "The How-To Guide to Satellites: Putting it Together",
            "description": "Building satellites isn't easy. They're complex, expensive, and not to mention hard to make! This is why whenever NASA makes a new satellite—like the MAVEN mission to Mars—its scientists and engineers do everything they can to make sure it's done right.Now, putting a satellite together is nothing like putting together, say, an office chair. A single bolt can take hours to install, and you can't even imagine how complex the electronics are! Find out more about the whole process in this video! || ",
            "hits": 20
        },
        {
            "id": 10471,
            "url": "https://svs.gsfc.nasa.gov/10471/",
            "result_type": "Produced Video",
            "release_date": "2009-09-04T00:00:00-04:00",
            "title": "SDO Engineers Create What Never Was",
            "description": "Scientists discover what there is, but engineers create that which never was. This special group of folks at Goddard Space Flight Center are creators, like any artist, but instead of working with art they are working wiht scientific, mechanical, or electrical things with fantastic problems to solve.  Watch engineers talk about what it is like to be an engineer as they build, assemble, integrate, and test the Solary Dynamics Observatory (SDO) soon to be launched in early 2010. If you have a strong tendancy towards science and mathematics, and enjoy working and building things with your hands, then you could also come up with creative solutions, to create something, to do a certain job and do it well. || ",
            "hits": 26
        },
        {
            "id": 10399,
            "url": "https://svs.gsfc.nasa.gov/10399/",
            "result_type": "B-Roll",
            "release_date": "2009-02-24T00:00:00-05:00",
            "title": "Glory Cleanroom B-roll, Orbital Sciences Corporation",
            "description": "In the lead up to launch, a number of critical spacecraft building and testing milestones took place at Orbital Sciences Corporation in Dulles, Virginia. This video b-roll was filmed in cleanrooms at Orbital Sciences Corporation, and provides documentation of critical Glory milestone moments. || ",
            "hits": 14
        },
        {
            "id": 10376,
            "url": "https://svs.gsfc.nasa.gov/10376/",
            "result_type": "Produced Video",
            "release_date": "2009-02-17T12:00:00-05:00",
            "title": "LRO's Team Spirit with Joanne Baker",
            "description": "The Lunar Reconnaissance Orbiter (LRO) is the first step to future missions to the Moon, Mars, and beyond. But a lot has to happen before we get there and one woman on the LRO team played a key role in 'putting it together.' || Joanne_Baker_Profile.01252_print.jpg (1024x576) [56.3 KB] || Joanne_Baker_Profile_web.png (320x180) [240.1 KB] || Joanne_Baker_Profile_thm.png (80x40) [16.3 KB] || Joanne_Baker_Profile_AppleTV.webmhd.webm (960x540) [30.2 MB] || Joanne_Baker_Profile_AppleTV.m4v (960x540) [57.0 MB] || Joanne_Baker_Profile.mov (1280x720) [82.9 MB] || Joanne_Baker_Profile.mpg (640x360) [31.5 MB] || Joanne_Baker_Profile_ipod.m4v (640x360) [26.2 MB] || Joanne_Baker_Profile.m4v (320x180) [11.8 MB] || Joanne_Baker_Profile.mp4 (320x240) [6.2 MB] || Joanne_Baker_Profile_SVSsmall.mpg (512x288) [21.1 MB] || Joanne_Baker_Profile.wmv (346x260) [19.4 MB] || ",
            "hits": 24
        },
        {
            "id": 10189,
            "url": "https://svs.gsfc.nasa.gov/10189/",
            "result_type": "Produced Video",
            "release_date": "2008-03-11T00:00:00-04:00",
            "title": "Stepping Stones to SDO",
            "description": "NASA's Solar Dynamics Observatory (SDO) is currently in the 'integration and test' phase of mission development, (i.e. observatory is now complete with the spacecraft bus, propulsion module and instruments), the ground system is being completed and flight software is being tested. Critical systems testing has already begun and environmental testing of he observatory will be conducted in the near future as they continue towards a launch readiness date of December 1, 2008. This series of short videos shows the SDO spacecraft being assembled and tested with narration by the engineers doing the work. It will be updated until SDO is ready for launch.For more information on SDO, visit the web site http://sdo.gsfc.nasa.gov || ",
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        }
    ]
}