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    "results": [
        {
            "id": 14868,
            "url": "https://svs.gsfc.nasa.gov/14868/",
            "result_type": "Produced Video",
            "release_date": "2025-07-23T00:00:00-04:00",
            "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail",
            "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ",
            "hits": 127
        },
        {
            "id": 14788,
            "url": "https://svs.gsfc.nasa.gov/14788/",
            "result_type": "Produced Video",
            "release_date": "2025-03-03T00:00:00-05:00",
            "title": "Roman Vertical Video",
            "description": "This page collects all the vertically-formatted videos produced for the Nancy Grace Roman Space Telescope mission. ||",
            "hits": 221
        },
        {
            "id": 14777,
            "url": "https://svs.gsfc.nasa.gov/14777/",
            "result_type": "Produced Video",
            "release_date": "2025-01-31T11:00:00-05:00",
            "title": "Coming Together : Roman's Internal Pieces are now Installed",
            "description": "NASA's Nancy Grace Roman Space Telescope is in the SCIPA configuation or the Spacecraft Integrated Payload Assembly. It includes the spacecraft bus, with all the support systems and electronics, the Wide Field Instrument, the Coronagraph Instrument, and the Optical Telescope Assembly, which is built around the 2.4 meter (7.9 foot) primary mirror. || ",
            "hits": 92
        },
        {
            "id": 14746,
            "url": "https://svs.gsfc.nasa.gov/14746/",
            "result_type": "Produced Video",
            "release_date": "2025-01-14T13:00:00-05:00",
            "title": "Roman SCIPA Hyperwall Time-lapse",
            "description": "This 3x3-hyperwall-resolution time-lapse video of Roman shows the major integration steps of the key systems to form SCIPA, or the Spacecraft Integrated Payload Assembly. It includes the spacecraft bus, with all the support systems and electronics, the Wide Field Instrument, the Coronagraph Instrument, and the Optical Telescope Assembly, which is built around the 2.4 meter (7.9 foot) primary mirror. This sequence does not have sound and is available as video and frames.Credit: NASA's Goddard Space Flight Center || Roman_SCIPA_TL_Still.jpg (5760x3240) [8.6 MB] || Roman_SCIPA_TL_Still_searchweb.png (320x180) [126.8 KB] || Roman_SCIPA_TL_Still_thm.png [8.3 KB] || 5760x3240_16x9_30p (5760x3240) [17806 Item(s)] || Roman_SCIPA_TL_Still.jpg.dzi [178 bytes] || Roman_SCIPA_TL_Still.jpg_files [4.0 KB] || Roman_SCIPA_Time-lapse_D4.mp4 (5760x3240) [1.4 GB] || ",
            "hits": 75
        },
        {
            "id": 14582,
            "url": "https://svs.gsfc.nasa.gov/14582/",
            "result_type": "Produced Video",
            "release_date": "2024-05-14T10:00:00-04:00",
            "title": "DAVINCI Drop Testing at UTTR",
            "description": "The DAVINCI Project is led by NASA GSFC with primary partners at Lockheed Martin as well as from NASA’s JPL, JHU’s APL, Malin Space Science Systems, NASA’s LaRC, NASA ARC, University of Michigan, and Kinetx.The PI, Deputy PI’s and Program management team are at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The artwork shown here was developed for the DAVINCI team by CI Labs and the SVS.   Special data analysis by the PI and Project Science team led by Dr. Jim Garvin, Dr. Stephanie Getty, and Dr. Giada Areny with Dr. Natasha Johnson and Dr. Erika Kohler is included.    NASA Langley (LaRC) partners include Dr. S. Dutta and his team who developed the probe aerodynamic drop test experiment for the DAVINCI project.  Narration is by Dr. Jim Garvin, PI for the DAVINCI mission to Venus.  The DAVINCI Project acknowledges the continuing support of NASA’s Discovery Program, with DAVINCI Program Executive Andrea Riley and Program scientist Nick Lang, and Mission Manager Kevin Sykes.  Music is \"Great Secrets\" by Thomas Alexander Farnon of Universal Production Music. || DAVINCI_REEL_THUMB.jpg (1080x1920) [584.4 KB] || DAVINCI_UTTR.01191_searchweb.png (320x180) [71.8 KB] || DAVINCI_UTTR.01191_thm.png (80x40) [6.4 KB] || DAVINCI_UTTR.en_US.srt [2.5 KB] || DAVINCI_UTTR.en_US.vtt [2.3 KB] || DAVINCI_UTTR.mp4 [30.7 MB] || ",
            "hits": 75
        },
        {
            "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] || ",
            "hits": 292
        },
        {
            "id": 14438,
            "url": "https://svs.gsfc.nasa.gov/14438/",
            "result_type": "Produced Video",
            "release_date": "2023-10-24T10:00:00-04:00",
            "title": "Why NASA's Roman Mission Will Study Milky Way's Flickering Lights",
            "description": "Watch this video to learn about time-domain astronomy and how time will be a key element in the Nancy Grace Roman Space Telescope's galactic bulge survey.Music: \"Elapsing Time\" and \"Beyond Truth\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_TDA-GBS_Still.jpg (1920x1080) [716.0 KB] || Roman_TDA-GBS_Still_print.jpg (1024x576) [206.4 KB] || Roman_TDA-GBS_Still_searchweb.png (320x180) [95.5 KB] || Roman_TDA-GBS_Still_thm.png (80x40) [7.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Sub100.mp4 (1920x1080) [91.9 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.webm (1920x1080) [32.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.mp4 (1920x1080) [215.7 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Best.mp4 (1920x1080) [744.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Captions.en_US.srt [6.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || ",
            "hits": 105
        },
        {
            "id": 14426,
            "url": "https://svs.gsfc.nasa.gov/14426/",
            "result_type": "Produced Video",
            "release_date": "2023-10-19T13:00:00-04:00",
            "title": "NASA's Lucy Mission Flyby of Asteroid Dinkinesh",
            "description": "Video: NASA's Lucy Mission Flies By Asteroid DinkineshMusic provided by Universal Production Music: \"Pioneer\" - Lorenzo CastellarinWatch this video on the NASA Goddard YouTube channel. || DinkineshFlyby_Thumbnail.jpg (1920x1080) [681.4 KB] || DinkineshFlyby_Thumbnail_print.jpg (1024x576) [238.9 KB] || DinkineshFlyby_Thumbnail_searchweb.png (320x180) [68.0 KB] || DinkineshFlyby_Thumbnail_thm.png (80x40) [4.8 KB] || 14426_LucyDinkineshFlyby_YouTubeHD.webm (1920x1080) [27.0 MB] || 14426_LucyDinkineshFlyby_TwitterX.mp4 (1280x720) [52.8 MB] || 14426_LucyDinkineshFlyby_YouTubeHD.mp4 (1920x1080) [391.9 MB] || 14426_LucyDinkineshFlyby_Captions.en_US.srt [5.0 KB] || 14426_LucyDinkineshFlyby_Captions.en_US.vtt [4.8 KB] || 14426_LucyDinkineshFlyby_MASTER.mov (1920x1080) [3.2 GB] || ",
            "hits": 69
        },
        {
            "id": 14422,
            "url": "https://svs.gsfc.nasa.gov/14422/",
            "result_type": "Produced Video",
            "release_date": "2023-10-06T00:00:00-04:00",
            "title": "Roman's Instrument Carrier Arrives",
            "description": "The Nancy Grace Roman Space Telescope's Instrument Carrier arrives at NASA's Goddard Space Flight Center.  The workers remove the grid-like structure from the truck container that brought it and move it into a clean tent.  Once there, engineers remove the protective wrapping and inspect the carbon fiber struts.  The Instrument Carrier sits between the primary mirror and spacecraft bus and will hold Roman's  Wide Field Instrument and Coronagraph technology demonstration.Music: \"Knowledge and Process\" from Universal Production MusicComplete transcript available. || Roman_Instrument_Carrier.jpg (1849x1004) [426.6 KB] || Roman_Instrument_Carrier_searchweb.png (320x180) [105.1 KB] || Roman_Instrument_Carrier_thm.png (80x40) [10.6 KB] || Roman_Instrument_Carrier_Arrival_Good.webm (1920x1080) [13.2 MB] || Roman_Instrument_Carrier_Arrival_Good.mp4 (1920x1080) [105.1 MB] || Roman_Instrument_Carrier_Arrival_Best.mp4 (1920x1080) [257.6 MB] || Roman_Instrument_Carrier_Arrival_Captions.en_US.srt [894 bytes] || Roman_Instrument_Carrier_Arrival_Captions.en_US.vtt [907 bytes] || Roman_Instrument_Carrier_Arrival_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ",
            "hits": 56
        },
        {
            "id": 40503,
            "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/",
            "result_type": "Gallery",
            "release_date": "2023-08-28T00:00:00-04:00",
            "title": "Hyperwall Power Playlist - Earth Science Focus",
            "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide  for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.",
            "hits": 272
        },
        {
            "id": 5051,
            "url": "https://svs.gsfc.nasa.gov/5051/",
            "result_type": "Visualization",
            "release_date": "2022-12-12T00:00:00-05:00",
            "title": "Drought conditions set the stage for an intense fire season in California in 2021",
            "description": "NASA’s Earth Information System (EIS) analysis captures the onset of drought and heightened fire conditions in mid-August 2021, with seasonal deficits of rainfall, exceptionally dry soils, onset of acute vegetation stress, and reduced plant growth. || fire_hyro_VIZ01_final_HD.02350_print.jpg (1024x576) [135.1 KB] || fire_hyro_VIZ01_final_HD.02350_searchweb.png (320x180) [73.4 KB] || fire_hyro_VIZ01_final_HD.02350_thm.png (80x40) [5.1 KB] || fire_hyro_VIZ01_final_HD_1080p59.94.mp4 (1920x1080) [20.6 MB] || 1920x1080_16x9_60p (1920x1080) [256.0 KB] || fire_hyro_VIZ01_final_HD_1080p59.94.webm (1920x1080) [6.7 MB] || fire_hyro_VIZ01_final_4k_2160p59.94.mp4 (3840x2160) [66.2 MB] || 3840x2160_16x9_60p (3840x2160) [256.0 KB] || 9600x3240_16x9_30p (9600x3240) [256.0 KB] || ",
            "hits": 29
        },
        {
            "id": 14217,
            "url": "https://svs.gsfc.nasa.gov/14217/",
            "result_type": "Produced Video",
            "release_date": "2022-11-15T13:00:00-05:00",
            "title": "Creating Black Hole Jets With a NASA Supercomputer",
            "description": "New simulations carried out on the NASA Center for Climate Simulation’s Discover supercomputer show how weaker, low-luminosity jets produced by a galaxy's monster black hole interact with their galactic environment. Because these jets are more difficult to detect, the simulations help astronomers link these interactions to features they can observe, such as various gas motions and optical and X-ray emissions.Credit: NASA's Goddard Space Flight CenterMusic credit: \"Lost Time;\" \"Ascension;\" \"Flowing Cityscape;\" \"Jupiter's Eye;\" \"Pizzicato Piece;\" \"Facts;\" \"Final Words\" all from Universal Production MusicVideo Descriptive Text available.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14217_AGN_OUtflow_Still.jpg (1920x1080) [1.0 MB] || 14217_AGN_OUtflow_Still_searchweb.png (320x180) [92.9 KB] || 14217_AGN_OUtflow_Still_thm.png (80x40) [6.7 KB] || 14217_AGN_Outflow_FINAL_1080.webm (1920x1080) [67.5 MB] || AGN_Outflow_SRT_Captions.en_US.srt [11.4 KB] || 14217_AGN_Outflow_FINAL_1080.mp4 (1920x1080) [632.4 MB] || 14217_AGN_Outflow_FINAL_1080_Best.mp4 (1920x1080) [1.5 GB] || 14217_AGN_Outflow_FINAL_ProRes_1920x1080_24.mov (1920x1080) [6.4 GB] || ",
            "hits": 223
        },
        {
            "id": 14194,
            "url": "https://svs.gsfc.nasa.gov/14194/",
            "result_type": "Produced Video",
            "release_date": "2022-08-12T00:00:00-04:00",
            "title": "Roman Interactive Promo",
            "description": "Short promotional video for the Nancy Grace Roman Interactive.Music: \"Braniacs and Machines\" from Universal Production Music.Complete transcript available. || Interactive_zoom_STILL.jpg (1920x1080) [302.4 KB] || Interactive_zoom_STILL_searchweb.png (320x180) [85.1 KB] || Interactive_zoom_STILL_thm.png (80x40) [7.4 KB] || Interactive_Teaser_V3.mp4 (1920x1080) [33.5 MB] || Interactive_Teaser_V3.webm (1920x1080) [2.2 MB] || Roman_Interactive_Teaser_ProRes_1920x1080_24.mov (1920x1080) [252.7 MB] || Interactive_Teaser_SRT_Captions.en_US.srt [246 bytes] || Interactive_Teaser_SRT_Captions.en_US.vtt [259 bytes] || ",
            "hits": 74
        },
        {
            "id": 4971,
            "url": "https://svs.gsfc.nasa.gov/4971/",
            "result_type": "Visualization",
            "release_date": "2022-06-07T10:00:00-04:00",
            "title": "Monitoring Changing Waters using the Gulf of Maine Atlantic Time Series (GNATS)",
            "description": "Visualization of 20 years of data from the Gulf of Maine North Atlantic Time Series (GNATS).   The data shown are temperatures at the water's surface and below the surface.  Satellite based sea surface temperatures are also shown.  This version does not include date or color bar overlays. || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_print.jpg (1024x576) [149.8 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_thm.png (80x40) [6.1 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_searchweb.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_web.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.mp4 (1920x1080) [76.4 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.webm (1920x1080) [12.0 MB] || 3840x2160_16x9_60p (3840x2160) [1.0 MB] || 9600x3240_16x9_30p (9600x3240) [1.0 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_2160p59.94.mp4 (3840x2160) [249.3 MB] || preview_5x3_hyperwall_gulf_of_maine.mp4 (2400x810) [129.1 MB] || ",
            "hits": 91
        },
        {
            "id": 14100,
            "url": "https://svs.gsfc.nasa.gov/14100/",
            "result_type": "Produced Video",
            "release_date": "2022-02-11T10:25:00-05:00",
            "title": "Photons Received: Webb Sees Its First Star – 18 Times",
            "description": "The James Webb Space Telescope is nearing completion of the first phase of the months-long process of aligning the observatory’s primary mirror using the Near Infrared Camera (NIRCam) instrument. The team's challenge was twofold: confirm that NIRCam was ready to collect light from celestial objects, and then identify starlight from the same star in each of the 18 primary mirror segments. The result is an image mosaic of 18 randomly organized dots of starlight, the product of Webb's unaligned mirror segments all reflecting light from the same star back at Webb's secondary mirror and into NIRCam's detectors.What looks like a simple image of blurry starlight now becomes the foundation to align and focus the telescope in order for Webb to deliver unprecedented views of the universe this summer. Over the next month or so, the team will gradually adjust the mirror segments until the 18 images become a single star. || Webb_Mirror_Alignment_Update-h264.00150_print.jpg (1024x576) [110.1 KB] || Webb_First_Star-OTE_print.jpg (1024x576) [232.8 KB] || Webb_First_Star-OTE.jpg (4608x2592) [1.3 MB] || Webb_Mirror_Alignment_Update-h264.00150_searchweb.png (320x180) [83.9 KB] || Webb_Mirror_Alignment_Update-h264.00150_web.png (320x180) [83.9 KB] || Webb_Mirror_Alignment_Update-h264.00150_thm.png (80x40) [6.7 KB] || Webb_First_Star-OTE_searchweb.png (320x180) [64.4 KB] || Webb_First_Star-OTE_web.png (320x180) [64.4 KB] || Webb_First_Star-OTE_thm.png (80x40) [21.3 KB] || Webb_Mirror_Alignment_Update-h264.mp4 (1920x1080) [220.5 MB] || Webb_Mirror_Alignment_Update-h264.webm (1920x1080) [22.4 MB] || Webb_Mirror_Alignment_Update-prores-1080p.mov (4608x2592) [13.6 GB] || Webb_Mirror_Alignment_Update-4k-prores.mov (4608x2592) [13.6 GB] || Webb_Mirror_Alignment_Update-v4-closecap.en_US.srt [4.3 KB] || Webb_Mirror_Alignment_Update-v4-closecap.en_US.vtt [4.3 KB] || Webb_Mirror_Alignment_Update-4k-h264.mp4 (4608x2592) [222.5 MB] || ",
            "hits": 40
        },
        {
            "id": 31173,
            "url": "https://svs.gsfc.nasa.gov/31173/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-01-18T00:00:00-05:00",
            "title": "Satellite View of the Blue Economy",
            "description": "Laura Lorenzoni's \"Satellite View of the Blue Economy\" presentation for COP26 || COP26_title_slide_Lorenzoni.001_print.jpg (1024x576) [559.1 KB] || COP26_title_slide_Lorenzoni.001.jpeg (5760x3240) [12.8 MB] || COP26_title_slide_Lorenzoni.001_searchweb.png (180x320) [94.4 KB] || COP26_title_slide_Lorenzoni.001_thm.png (80x40) [7.6 KB] || lorenzoni_2021_cop26_sub_720p30.webm (1280x720) [81.7 MB] || lorenzoni_2021_cop26_sub_1080p30.mp4 (1920x1080) [882.1 MB] || lorenzoni_2021_cop26_sub_720p30.mp4 (1280x720) [475.1 MB] || lorenzoni_2021_cop26_sub_2160p30.mp4 (3840x2160) [2.6 GB] || ",
            "hits": 42
        },
        {
            "id": 14005,
            "url": "https://svs.gsfc.nasa.gov/14005/",
            "result_type": "Produced Video",
            "release_date": "2021-11-24T00:00:00-05:00",
            "title": "Elements of Webb: Beryllium Part 1 Ep03",
            "description": "Have you heard of beryllium? It’s a rare lightweight metal used as the primary material on the Webb Telescope. This episode explores the reason this expensive metal is perfect for Webb. Special thanks to LA Gauge for hosting  the media team. #UnfoldTheUniverse || Beryllium_1_dark.jpg (1920x1080) [898.1 KB] || Beryllium_1_dark_print.jpg (1024x576) [388.6 KB] || Beryllium_1_dark_searchweb.png (320x180) [85.0 KB] || Beryllium_1_dark_web.png (320x180) [85.0 KB] || Beryllium_1_dark_thm.png (80x40) [7.1 KB] || 03-Elements-Beryllium_1_ProRes.mov (1920x1080) [3.1 GB] || 3-Elements-Beryllium_1.mp4 (1920x1080) [241.4 MB] || 3-Elements-Beryllium_1.webm (1920x1080) [25.7 MB] || 03-Elements-Beryllium_1.en_US.srt [4.2 KB] || 03-Elements-Beryllium_1.en_US.vtt [4.2 KB] || ",
            "hits": 82
        },
        {
            "id": 14002,
            "url": "https://svs.gsfc.nasa.gov/14002/",
            "result_type": "Produced Video",
            "release_date": "2021-11-09T00:00:00-05:00",
            "title": "Elements of Webb: Series Introduction Ep0",
            "description": "Elements of Webb EP00: Introduction || EP00-_Elements_Series_Introduction.jpg (1920x1080) [738.1 KB] || EP00-_Elements_Series_Introduction_print.jpg (1024x576) [333.2 KB] || EP00-_Elements_Series_Introduction_searchweb.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_web.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_thm.png (80x40) [7.1 KB] || 0-Elements_of_Webb_-_Introduction_1.mp4 (1920x1080) [89.2 MB] || 0-Elements_of_Webb_-_Introduction_1.webm (1920x1080) [9.4 MB] || 0-Elements_of_Webb_-_Introduction_1.en_US.srt [1.3 KB] || 0-Elements_of_Webb_-_Introduction_1.en_US.vtt [1.3 KB] || 0-Elements_of_Webb_-_Introduction.mov (1920x1080) [1.1 GB] || elements-of-webb-series-introduction-ep0.hwshow [332 bytes] || ",
            "hits": 54
        },
        {
            "id": 13852,
            "url": "https://svs.gsfc.nasa.gov/13852/",
            "result_type": "Produced Video",
            "release_date": "2021-05-26T10:00:00-04:00",
            "title": "NASA’s Roman Mission to Probe Cosmic Secrets Using Exploding Stars",
            "description": "NASA’s upcoming Nancy Grace Roman Space Telescope will see thousands of exploding stars called supernovae across vast stretches of time and space. Using these observations, astronomers aim to shine a light on several cosmic mysteries, providing a window onto the universe’s distant past and hazy present.Credit: NASA's Goddard Space Flight CenterMusic: \"Relentless Data\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Supernova_IA_1285_print.jpg (1024x576) [53.0 KB] || Supernova_IA_1285.png (3840x2160) [5.0 MB] || Supernova_IA_1285_searchweb.png (320x180) [46.9 KB] || Supernova_IA_1285_thm.png (80x40) [4.6 KB] || 13852_Roman_Standard_Candle_Supernovae_1080_Best.webm (1920x1080) [28.3 MB] || 13852_Roman_Standard_Candle_Supernovae_1080.mp4 (1920x1080) [136.7 MB] || 13852_Roman_Standard_Candle_Supernovae_1080_Best.mp4 (1920x1080) [654.2 MB] || 13852RomanStandardCandleSupernovaeCaptionsFix.en_US.srt [4.7 KB] || 13852RomanStandardCandleSupernovaeCaptionsFix.en_US.vtt [4.7 KB] || 13852_Roman_Standard_Candle_Supernovae_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ",
            "hits": 127
        },
        {
            "id": 13806,
            "url": "https://svs.gsfc.nasa.gov/13806/",
            "result_type": "Produced Video",
            "release_date": "2021-03-12T11:00:00-05:00",
            "title": "Scientists Build a Detailed Image of U Mon Binary",
            "description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ",
            "hits": 62
        },
        {
            "id": 13774,
            "url": "https://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": 95
        },
        {
            "id": 13738,
            "url": "https://svs.gsfc.nasa.gov/13738/",
            "result_type": "Produced Video",
            "release_date": "2020-10-19T11:30:00-04:00",
            "title": "OSIRIS-REx Science and Engineering Briefing",
            "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ",
            "hits": 65
        },
        {
            "id": 13724,
            "url": "https://svs.gsfc.nasa.gov/13724/",
            "result_type": "Produced Video",
            "release_date": "2020-09-24T14:25:00-04:00",
            "title": "OSIRIS-REx: Countdown to TAG",
            "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ",
            "hits": 79
        },
        {
            "id": 13686,
            "url": "https://svs.gsfc.nasa.gov/13686/",
            "result_type": "Produced Video",
            "release_date": "2020-08-12T11:00:00-04:00",
            "title": "Hubble Trivia",
            "description": "The Hubble Space Telescope has been answering questions about the universe for over 30 years. Now it’s your turn to answer some questions about Hubble! Hubble Trivia is a miniseries featuring some frequently asked questions and surprising facts about the famous space telescope. See if you can answer each trivia question before the answer is revealed! || ",
            "hits": 176
        },
        {
            "id": 13663,
            "url": "https://svs.gsfc.nasa.gov/13663/",
            "result_type": "Produced Video",
            "release_date": "2020-08-11T11:00:00-04:00",
            "title": "TESS Completes Its Primary Mission",
            "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) has completed its two-year primary mission and is continuing its search for new worlds. Watch to review some of TESS’s most interesting discoveries so far.Credit: NASA’s Goddard Space Flight CenterMusic: \"Drive to Succeed\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_2_Still.jpg (1920x1080) [661.7 KB] || TESS_2_Still_print.jpg (1024x576) [187.0 KB] || 13663_TESS_2nd_Anniversary_Highlights.mp4 (1920x1080) [215.9 MB] || 13663_TESS_2nd_Anniversary_Highlights_Best.mp4 (1920x1080) [611.5 MB] || 13663_TESS_2nd_Anniversary_Highlights_ProRes_1920x1080_2997.mov (1920x1080) [2.7 GB] || 13663_TESS_2nd_Anniversary_Highlights.webm (1920x1080) [23.4 MB] || TESS_2nd_Anniversary_Highlights_SRT_Captions.en_US.srt [4.0 KB] || TESS_2nd_Anniversary_Highlights_SRT_Captions.en_US.vtt [4.0 KB] || ",
            "hits": 173
        },
        {
            "id": 13639,
            "url": "https://svs.gsfc.nasa.gov/13639/",
            "result_type": "Produced Video",
            "release_date": "2020-06-09T14:00:00-04:00",
            "title": "Tower Extension Test a Success for NASA’s James Webb Space Telescope",
            "description": "Technicians test the James Webb Space Telescope's Deployable Tower Assembly in the cleanroom.  Social media release version.Music credit: Universal Production Music: Timelapse Clouds by Blythe Joustra || Webb_Tower_Deployment_Test-Main-h264-a.00167_print.jpg (1024x576) [234.2 KB] || Webb_Tower_Deployment_Test-Main-h264-a.00167_searchweb.png (320x180) [109.5 KB] || Webb_Tower_Deployment_Test-Main-h264-a.00167_web.png (320x180) [109.5 KB] || Webb_Tower_Deployment_Test-Main-h264-a.00167_thm.png (80x40) [7.7 KB] || Webb_Tower_Deployment_Test-Main-h264-a.mp4 (1920x1080) [71.8 MB] || Webb_Tower_Deployment_Test-Main-prores-a.mov (1920x1080) [1.5 GB] || Webb_Tower_Deployment_Test-Main-h264-a.webm (1920x1080) [7.8 MB] || Webb_Tower_Deployment_Test-2-srt-closecap.en_US.srt [1.3 KB] || Webb_Tower_Deployment_Test-2-srt-closecap.en_US.vtt [1.3 KB] || ",
            "hits": 33
        },
        {
            "id": 13606,
            "url": "https://svs.gsfc.nasa.gov/13606/",
            "result_type": "Produced Video",
            "release_date": "2020-05-20T11:00:00-04:00",
            "title": "A New Portrait of the Cosmos is Coming",
            "description": "Welcome to NASA's upcoming infrared survey mission, taking a wider view of the cosmos.Credit: NASA's Goddard Space Flight CenterMusic: \"The Decision (alternate)\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Trailer_still_1_print.jpg (1024x576) [181.5 KB] || Trailer_still_1.jpg (3840x2160) [2.0 MB] || Trailer_still_1_searchweb.png (180x320) [104.8 KB] || Trailer_still_1_thm.png (80x40) [7.9 KB] || Roman_Space_Telescope_Trailer_ProRes_1920x1080_2997.mov (1920x1080) [797.0 MB] || Roman_Space_Telescope_Trailer_Best_1080.mp4 (1920x1080) [281.5 MB] || Roman_Space_Telescope_Trailer_1080.mp4 (1920x1080) [132.9 MB] || Roman_Space_Telescope_Trailer_1080.webm (1920x1080) [7.2 MB] || Roman_Trailer_SRT_Captions.en_US.srt [740 bytes] || Roman_Trailer_SRT_Captions.en_US.vtt [753 bytes] || ",
            "hits": 105
        },
        {
            "id": 13565,
            "url": "https://svs.gsfc.nasa.gov/13565/",
            "result_type": "Produced Video",
            "release_date": "2020-02-27T15:00:00-05:00",
            "title": "Asteroid Bennu: Selecting Site Nightingale",
            "description": "After a year of studying asteroid Bennu, the OSIRIS-REx mission chose a location called “Nightingale” as the primary sample collection site.Universal Production Music: “Extreme Measures” by John Sands and Marc Ferrari, “Ice Echoes” by Dominik Luke Marsden Johnson, “Look at the Mirror” by Jonathan FigoliWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Bennu20cmGlobalPreviewV3_print.jpg (1024x576) [150.9 KB] || Bennu20cmGlobalPreviewV3.jpg (3840x2160) [2.4 MB] || Bennu20cmGlobalPreviewV3_web.png (320x180) [19.5 KB] || Bennu20cmGlobalPreviewV3_searchweb.png (320x180) [19.5 KB] || Bennu20cmGlobalPreviewV3_thm.png (80x40) [2.1 KB] || TWITTER_720_13565_Bennu_Nightingale_MASTER_twitter_720.mp4 (1280x720) [42.3 MB] || 13565_Bennu_Nightingale_MASTER.webm (960x540) [96.1 MB] || FACEBOOK_720_13565_Bennu_Nightingale_MASTER_facebook_720.mp4 (1280x720) [252.3 MB] || YOUTUBE_1080_13565_Bennu_Nightingale_MASTER_youtube_1080.mp4 (1920x1080) [319.9 MB] || 13565_Bennu_Nightingale_CAPTIONS.en_US.srt [5.3 KB] || 13565_Bennu_Nightingale_CAPTIONS.en_US.vtt [5.3 KB] || 13565_Bennu_Nightingale_MASTER.mp4 (3840x2160) [4.8 GB] || 13565_Bennu_Nightingale_MASTER.mov (3840x2160) [13.4 GB] || ",
            "hits": 61
        },
        {
            "id": 13497,
            "url": "https://svs.gsfc.nasa.gov/13497/",
            "result_type": "Produced Video",
            "release_date": "2020-01-05T14:00:00-05:00",
            "title": "Simulated Image Demonstrates the Power of NASA’s Nancy Grace Roman Space Telescope",
            "description": "Watch the video to learn more about the Roman Space Telescope's simulated image.Credit: NASA's Goddard Space Flight CenterMusic: \"Flight Impressions\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Simulated_Image_Still.jpg (1920x1080) [891.1 KB] || 13497_Simulated_Image_Roman_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13497_Simulated_Image_Roman_Best_1080.mp4 (1920x1080) [936.5 MB] || 13497_Simulated_Image_Roman_1080.mp4 (1920x1080) [291.8 MB] || 13497_Simulated_Image_Roman_1080.webm (1920x1080) [22.4 MB] || Simulated_Image_Roman_SRT_Captions.en_US.srt [3.6 KB] || Simulated_Image_Roman_SRT_Captions.en_US.vtt [3.6 KB] || ",
            "hits": 89
        },
        {
            "id": 13314,
            "url": "https://svs.gsfc.nasa.gov/13314/",
            "result_type": "Produced Video",
            "release_date": "2019-09-13T10:00:00-04:00",
            "title": "Unraveling the Mysteries of Dark Energy with NASA's WFIRST",
            "description": "Watch this video to learn more about dark energy and how WFIRST will study it.Music: \"Searching Everywhere\" from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Dark_Energy_Expansion_Still_print.jpg (1024x576) [164.5 KB] || Dark_Energy_Expansion_Still.jpg (3840x2160) [942.3 KB] || Dark_Energy_Expansion_Still_searchweb.png (320x180) [50.3 KB] || Dark_Energy_Expansion_Still_thm.png (80x40) [5.0 KB] || 13314_Dark_Energy_1080_good.mp4 (1920x1080) [236.4 MB] || 13314_Dark_Energy_1080.mp4 (1920x1080) [125.1 MB] || 13314_Dark_Energy_1080.webm (1920x1080) [25.4 MB] || 13314_Dark_Energy_ProRes_3840x2160_2997.mov (3840x2160) [5.5 GB] || 13314_Dark_Energy_4k_best.mp4 (3840x2160) [558.4 MB] || 13314_Dark_Energy_SRT_Captions.en_US.srt [5.0 KB] || 13314_Dark_Energy_SRT_Captions.en_US.vtt [4.9 KB] || ",
            "hits": 336
        },
        {
            "id": 40348,
            "url": "https://svs.gsfc.nasa.gov/gallery/esddatafor-societal-benefits/",
            "result_type": "Gallery",
            "release_date": "2018-04-24T00:00:00-04:00",
            "title": "ESD data for Societal Benefit",
            "description": "No description available.",
            "hits": 220
        },
        {
            "id": 11886,
            "url": "https://svs.gsfc.nasa.gov/11886/",
            "result_type": "Produced Video",
            "release_date": "2015-06-03T14:00:00-04:00",
            "title": "JWST Arm Over-Deploy at GSFC",
            "description": "JWST Arm-Over Deploy || Screen_Shot_2015-06-03_at_10.40.24_AM.png (1409x752) [1.2 MB] || Screen_Shot_2015-06-03_at_10.40.24_AM_print.jpg (1024x546) [126.5 KB] || Screen_Shot_2015-06-03_at_10.40.24_AM_searchweb.png (320x180) [97.3 KB] || Screen_Shot_2015-06-03_at_10.40.24_AM_web.png (320x170) [92.9 KB] || Screen_Shot_2015-06-03_at_10.40.24_AM_thm.png (80x40) [10.4 KB] || JWST_Arm_Over-Deploy_ProRes_appletv.m4v (960x540) [88.4 MB] || JWST_Arm_Over-Deploy_ProRes_prores.mov (1280x720) [3.1 GB] || JWST_Arm_Over-Deploy_ProRes_1280x720.wmv (1280x720) [110.0 MB] || JWST_Arm_Over-Deploy_ProRes_youtube_hq.mov (1280x720) [336.3 MB] || JWST_Arm_Over-Deploy_ProRes_youtube_hq.webm (1280x720) [23.1 MB] || JWST_Arm_Over-Deploy_ProRes_ipod_lg.m4v (640x360) [34.5 MB] || JWST_Arm_Over-Deploy_ProRes_ipod_sm.mp4 (320x240) [18.3 MB] || ",
            "hits": 43
        },
        {
            "id": 30584,
            "url": "https://svs.gsfc.nasa.gov/30584/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-02-13T00:00:00-05:00",
            "title": "AXIOM-1 Ocean chlorophyll, Sea Ice Thickness and Atmospheric Precipitable Water",
            "description": "This animation shows ocean surface chlorophyll concentration, sea ice thickness, and atmospheric precipitable water. || 0001_print.jpg (1024x576) [236.0 KB] || 0001_searchweb.png (320x180) [121.0 KB] || 0001_web.png (320x180) [121.0 KB] || 0001_thm.png (80x40) [8.0 KB] || chl-1920x1080.webm (1920x1080) [15.9 MB] || axiom_chl_720p.mp4 (1280x720) [161.2 MB] || axiom_chl_h265_720p.mp4 (1280x720) [105.5 MB] || chl-1920x1080.mp4 (1920x1080) [889.5 MB] || chl (5760x3240) [128.0 KB] || axiom_chl_h265_2304p.mp4 (4096x2304) [913.8 MB] || chlorophyll_ice_thickness_precip_water_30584.key [896.4 MB] || chlorophyll_ice_thickness_precip_water_30584.pptx [893.1 MB] || axiom_chl_2304p.mp4 (4096x2304) [1.4 GB] || ",
            "hits": 38
        },
        {
            "id": 30380,
            "url": "https://svs.gsfc.nasa.gov/30380/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-24T12:00:00-04:00",
            "title": "Monthly Net Primary Productivity",
            "description": "Plants play an important role in the movements of carbon dioxide throughout Earth's environment. Living plants both take in carbon dioxide from the air and put out carbon dioxide to the air. Called net primary productivity, these maps show where and how much carbon dioxide is taken in by vegetation during photosynthesis minus how much carbon dioxide is released when plants respire on a monthly basis, from February 2000 to the present. Created using data from the Moderate Resolutions Imaging Spectroradiometer (MODIS) instrument onboard NASA’s Terra satellite, the colors on these maps indicate how fast carbon was taken in for every square meter of land. Values range from -1.0 grams of carbon per square meter per day (tan) to 6.5 grams per square meter per day (dark green). A negative value means decomposition or respiration overpowered carbon absorption; more carbon was released to the atmosphere than the plants took in. Maps such as these allow scientists to routinely monitor plants' role in the global carbon cycle. || ",
            "hits": 225
        },
        {
            "id": 3927,
            "url": "https://svs.gsfc.nasa.gov/3927/",
            "result_type": "Visualization",
            "release_date": "2012-06-07T12:00:00-04:00",
            "title": "ICESCAPE Mission Measures High Chlorophyll-a Under the Ice",
            "description": "ICESCAPE is a multi-year NASA mission to study biogeochemical and ecological impacts of climate change in the Chukchi and Beaufort Seas in the Arctic. During 2011, the ICESCAPE mission acquired data while sailing on the US Coast Guard Cutter Healy. This visualization shows both the technique used by the ICESCAPE mission to take data measurements as well as some of the data that was taken.The visualization shows the ICESCAPE ship's path through the Chukchi and Beaufort seas north of Alaska from July 3, 2011 through July 8, 2011. The ship stops and takes measurements along the way. The measurements are taken by canisters lowered to various depths that sample the water. The measurement depths range from 1.8 meters to 149.3 meters below sea level. The sets of measurements are broken into two transects. The first transect is the trip out into the ice. The second transect is the trip back. Topography (above sea level) is exaggerated 10 times. Bathymetry (below sea level) is exaggerated 200 times in order differentiate the measurements.The colors of the measurements (i.e,. stations) correspond to the color bar below which represent chlorophyll-a concentrations. Measurements that are depicted by spheres were acquired while the ship was in open water while measurements depicted by cubes were acquired when the ship was in ice. As data is collected, a wall of interpolated data is generated.An important finding of this research was that high concentrations of chlorophyll-a were found under the ice. || ",
            "hits": 48
        },
        {
            "id": 3804,
            "url": "https://svs.gsfc.nasa.gov/3804/",
            "result_type": "Visualization",
            "release_date": "2010-12-12T00:00:00-05:00",
            "title": "Human Consumption of Global Plant Production, 2005",
            "description": "On Dec. 14, 2010 NASA Goddard researchers conducted a press briefing at the American Geophysical Union Fall 2010 meeting, entitled, \"Satellite Supported Estimates of Human Rate of NPP carbon Use on Land: Challenges Ahead.\" In the first measurement of this trend, the research showed humans are using an increasing amount of Earth's annual production of photosynthetic land plants due to both increases in population and per capita consumption, and that amount of Net Primary Production (NPP) required rose from 20 to 25 percent from 1995 to 2005.This visualization illustrates the relationship between human acquistition of net primary productivity (HANPP) and NPP itself, by presenting the ratio of HANPP to NPP.  It is a carbon balance sheet showing the percent of terrestrial net primary production that is required to provide food, fiber, and wood-based fuels for the world's global population in 2005.Measured in terms of carbon, regions where the populations are consuming more than is generated on the landscape show up as yellows and reds.  The colors are presented on a logarithmic scale, meaning that the value of the data at each unit on the scale is ten times that of the previous unit; i.e. areas in red are 100 times (or greater) the value of areas in green.  Therefore yellow, for example, with a value of HANPP/NPP = 10^0, or 1, represents regions were people require an amount of NPP that is 100 percent of the regional production, and red represents regions where people require more production than is locally available, up to 1000 percent and beyond. Values of less than 10 percent are not shown.  This map shows where populations are highly dependent upon a food and fiber distribution system and are arguably potentially vulnerable to climate change. || ",
            "hits": 16
        },
        {
            "id": 40087,
            "url": "https://svs.gsfc.nasa.gov/gallery/hanppagu2010/",
            "result_type": "Gallery",
            "release_date": "2010-12-09T00:00:00-05:00",
            "title": "Carbon Consumption and the Earth's Carrying Capacity",
            "description": "No description available.",
            "hits": 81
        },
        {
            "id": 3764,
            "url": "https://svs.gsfc.nasa.gov/3764/",
            "result_type": "Visualization",
            "release_date": "2010-08-19T14:00:00-04:00",
            "title": "How Much Carbon do Plants Take from the Atmosphere?",
            "description": "Plant life converts atmospheric carbon dioxide into biomass through photosynthesis, a process called 'fixing'. This is one of the main ways in which carbon dioxide is removed from the atmosphere and is a major part of the carbon cycle. The amount of carbon removed is called the gross primary productivity (GPP), and the change in GPP due to rising global temperatures is very important factor in the response of the Earth to climate change.Data from the MODIS instrument on NASA's Terra satellite has been recently used to calculate the GPP for the whole world for the last 10 years. This animation shows a time sequence of GPP on land as measured by MODIS during the years 2000 through 2009. Two things to note are the year-long productivity of the tropical regions and the large seasonal productivity in the northern hemisphere. A close look at the animation also reveals major urban areas for which the productivity is negligible.For a look at why the decade from 2000 through 2009 meant lower productivity, see the page 'How has the Atmospheric Carbon Uptake from Plants Changed in the Last Decade?' || ",
            "hits": 147
        },
        {
            "id": 3765,
            "url": "https://svs.gsfc.nasa.gov/3765/",
            "result_type": "Visualization",
            "release_date": "2010-08-19T14:00:00-04:00",
            "title": "How has the Atmospheric Carbon Uptake from Plants Changed in the Last Decade?",
            "description": "Plant life converts atmospheric carbon dioxide into biomass through photosynthesis. This process, called fixing, is one of the main ways in which carbon dioxide is removed from the atmosphere and is a major part of the carbon cycle. Plants release a fraction of this fixed carbon by respiration in order to get energy to live and to move carbon to other organs. The amount of carbon removed minus the amount of carbon respired is called the net primary productivity (NPP) and is the amount of carbon turned into biomass.The change in NPP due to rising global temperatures is a very important factor in the response of the Earth to climate change. Measurements of radiation and leaf area from the MODIS instrument on NASA's Terra satellite have recently been used to calculate the change in NPP for the whole world for the last 10 years. This animation shows a time sequence of annual NPP deviation from normal (or 'anomaly') on land as measured by MODIS during the years 2000 through 2009. Annual NPP, especially its departures from a long-term mean condition, will demonstrate the effects of environmental drivers such as ENSO (El Niño) events, climate change, droughts, pollution episodes, land degradation, and agricultural expansion.Earlier studies of productivity between 1982 and 1999 showed that prouctivity went up as global temperatures rose, because longer, warmer growing seasons were better for plant growth. This new study indicates that this is still true in the northern hemisphere, but that increased temperatures have meant increased drought and dryness in the tropics and the southern hemisphere. As a result, the global net productivity has actually decreased in the period from 2000 through 2009.Regionally, negative annual NPP anomalies were mainly caused by large-scale droughts. In 2000, droughts reduced NPP in North America and China; in 2002, droughts reduced NPP in North America and Australia; in 2003, drought caused by a major heat wave reduced NPP in Europe; in 2005, severe droughts in the Amazon, Africa, and Australia greatly reduced both regional and global NPP; from 2007 through 2009 over large parts of Australia, continuous droughts reduced continental NPP.For an animation of daily productivity, see the page How Much Carbon do Plants Take from the Atmosphere?. || ",
            "hits": 90
        },
        {
            "id": 10630,
            "url": "https://svs.gsfc.nasa.gov/10630/",
            "result_type": "Produced Video",
            "release_date": "2010-08-19T14:00:00-04:00",
            "title": "Plant Productivity in a Warming World",
            "description": "The past decade is the warmest on record since instrumental measurements began in the 1880s. Previous research suggested that in the '80s and '90s, warmer global temperatures and higher levels of precipitation — factors associated with climate change — were generally good for plant productivity. An updated analysis published this week in Science indicates that as temperatures have continued to rise, the benefits to plants are now overwhelmed by longer and more frequent droughts. High-resolution data from the Moderate Resolution Imaging Spectroradiometer, or MODIS, indicate a net decrease in NPP from 2000-2009, as compared to the previous two decades. || ",
            "hits": 29
        },
        {
            "id": 3459,
            "url": "https://svs.gsfc.nasa.gov/3459/",
            "result_type": "Visualization",
            "release_date": "2007-09-15T00:00:00-04:00",
            "title": "Multivariate ENSO Index Correlation with Ocean Net Primary Production Data over the North Atlantic",
            "description": "The SeaWiFS instrument aboard the Seastar satellite has been collecting ocean data since 1997. A check up of the Earth's planetary health reveals that the lowest rung in the ocean food chain is shrinking. For the past 20 years (early 1980s to present), phytoplankton concentrations declined as much as 30 percent in northern oceans. Scientists from NASA, the National Oceanic and Atmospheric Administration (NOAA), and Oregon State University say warmer ocean temperatures and low winds may be depriving the tiny ocean plants of necessary nutrients. However, they still do not know if the loss of phytoplankton is a long-term trend or a climate oscillation. Scientists can monitor ocean and planetary health through phytoplankton. Since the whole ocean food chain depends on the health and productivity of phytoplankton, a significant change could indicate a shift in our climate. Phytoplankton consists of many diverse species of microscopic free-floating ocean plants that form the base of the ocean's food chain. These plants thrive on sunlight and nutrients. Limit either one and phytoplankton will not grow. This animation shows the Multivariate ENSO Index (MEI) in red and the net primary production NPP anomaly in units of Tgrams carbon per month in green. The MEI is a multivariate index that incorporates sea level pressure, surface zonal and meridional wind components, sea surface temperature, surface air temperature, and cloudiness (Wolter and Timlin, 1998). The MEI index is calculated for the tropical Pacific (i.e., between 10 degrees North and 10 degrees South, from Asia to the Americas) with units of kg m-3. The Net Primary Production (NPP) data was generated from the Vertically Generalized Production Model (VGPM). The VGPM data set is available at the following URL: http://web.science.oregonstate.eduocean.productivity/ . As the sea surface temperature warms, the production levels decrease. || ",
            "hits": 56
        },
        {
            "id": 20120,
            "url": "https://svs.gsfc.nasa.gov/20120/",
            "result_type": "Animation",
            "release_date": "2007-09-14T00:00:00-04:00",
            "title": "360 Degrees of GLAST",
            "description": "GLAST will carry two instruments: the Large Area Telescope (LAT) and the GLAST Burst Monitor (GBM). The LAT is GLAST's primary instrument and consists of four components: the Tracker, the Calorimeter, the Anticoincidence Detector (ACD), and the Data Acquisition System (DAQ). These instrument components working together will detect gamma rays by using Einstein's famous equation (E=mc(squared) in a technique known as pair production. The GLAST Burst Monitor is a complementary instrument and consists of low-energy detectors, high-energy detectors, and data processing unit. The GBM can see all directions at once, except for the area where Earth blocks its view. When the GBM detects a bright gamma-ray burst, it immediately sends a signal to the LAT to observe that area of the sky. || ",
            "hits": 55
        },
        {
            "id": 40116,
            "url": "https://svs.gsfc.nasa.gov/gallery/jwst/",
            "result_type": "Gallery",
            "release_date": "2000-01-01T00:00:00-05:00",
            "title": "James Webb Space Telescope",
            "description": "The James Webb Space Telescope (sometimes called JWST) is a large, infrared-optimized space telescope. The observatory launched into space on an Ariane 5 rocket from the Guiana Space Centre in Kourou, French Guiana on December 25, 2021.  After launch, the observatory was successfully unfolded and is being readied for science. \n\nWebb will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy. Webb will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System. Webb's instruments are designed to work primarily in the infrared range of the electromagnetic spectrum, with some capability in the visible range.\n\nWebb has a large primary mirror, 6.5 meters (21.3 feet) in diameter and a sunshield the size of a tennis court. Both the mirror and sunshade are too large to fit onto the Ariane 5 rocket fully open, so both were folded which meant they needed to be unfolded in space. \n\nWebb is currently in its operational orbit about 1.5 million km (1 million miles) from the Earth at a location known as Lagrange Point 2 (L2).\n\nThe James Webb Space Telescope was named after the NASA Administrator who crafted the Apollo program, and who was a staunch supporter of space science.",
            "hits": 841
        }
    ]
}