{ "count": 386, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Simulation%22", "previous": null, "results": [ { "id": 31383, "url": "https://svs.gsfc.nasa.gov/31383/", "result_type": "Hyperwall Visual", "release_date": "2026-04-01T12:00:00-04:00", "title": "Water Droplet Science with Astronaut Don Pettit on the ISS", "description": "NASA astronaut Don Pettit demonstrates electrostatic forces using charged water droplets and a knitting needle made of Teflon.", "hits": 542 }, { "id": 5625, "url": "https://svs.gsfc.nasa.gov/5625/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami", "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.", "hits": 514 }, { "id": 5626, "url": "https://svs.gsfc.nasa.gov/5626/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)", "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.", "hits": 178 }, { "id": 14924, "url": "https://svs.gsfc.nasa.gov/14924/", "result_type": "Produced Video", "release_date": "2026-02-18T09:55:00-05:00", "title": "\"Dark Galaxy\" Identified by Hubble", "description": "Master VersionHorizontal version. This is for use on any YouTube or non-YouTube platform where you want to display the video horizontally. || 14924_DARK_WIDE_PRINT.jpg (1920x1080) [759.2 KB] || 14924_DARK_WIDE_THUMB.jpg (1920x1080) [759.2 KB] || 14924_DARK_WIDE_SEARCH.jpg (320x180) [32.1 KB] || 14924_DARK_WIDE_MP4.mp4 (1920x1080) [239.9 MB] || 14924_DARK_WIDE_MP4.en_US.srt [3.6 KB] || 14924_DARK_WIDE_MP4.en_US.vtt [3.6 KB] || ", "hits": 280 }, { "id": 14884, "url": "https://svs.gsfc.nasa.gov/14884/", "result_type": "Produced Video", "release_date": "2026-01-29T11:00:00-05:00", "title": "NASA Supercomputer Probes Tangled Magnetospheres of Merging Neutron Stars", "description": "New supercomputer simulations explore the tangled magnetic structures around merging neutron stars. These structures, called magnetospheres, interact as the city-sized stars enter their final orbits. Magnetic field lines can connect both stars, break, and reconnect, while currents surge through surrounding plasma moving at nearly the speed of light. The simulations show that these systems may produce X-rays and gamma rays that future observatories should be able to detect. Credit: NASA’s Goddard Space Flight CenterAlt text: Narrated video introducing simulations of merging neutron star magnetospheresMusic: “A Theory Develops,” Pip Heywood [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NS_Binary_Sim_Still.jpg (5760x3240) [1.4 MB] || NS_Binary_Sim_Still_searchweb.png (320x180) [67.6 KB] || NS_Binary_Sim_Still_thm.png (80x40) [5.2 KB] || 14884_NeutronStarBinarySim2_good.mp4 (1920x1080) [220.4 MB] || 14884_NeutronStarBinarySim2_best.mp4 (1920x1080) [363.9 MB] || NeutronStarBinarySimulationCaptions.en_US.srt [2.4 KB] || NeutronStarBinarySimulationCaptions.en_US.vtt [2.2 KB] || 14884_NeutronStarBinarySim2_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || ", "hits": 448 }, { "id": 14938, "url": "https://svs.gsfc.nasa.gov/14938/", "result_type": "Visualization", "release_date": "2025-12-22T11:00:00-05:00", "title": "Artemis Science: Visualizing NASA’s Next Lunar Flyby", "description": "Artemis II visualization lead Ernie Wright explains how his data-driven animations are helping astronauts to prepare for a historic flyby of the Moon.Complete transcript available.Universal Production Music: “Black Cloud” and “Magic Trick” by Hugo Dubery [SACEM] and Philippe Galtier [SACEM]; “Connecting Ideas” by Christopher Timothy White [PRS]; “Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS]Watch this video on the NASA Goddard YouTube channel and Facebook. || Artemis-Sci-Wright-A2Sim-Thumbnail_print.jpg (1024x576) [102.1 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail.jpg (1920x1080) [533.4 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail.png (1920x1080) [1.2 MB] || Artemis-Sci-Wright-A2Sim-Thumbnail_searchweb.png (320x180) [64.7 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail_thm.png (80x40) [6.2 KB] || 14938_Artemis_Sci_Wright_A2Sim_720.mp4 (1280x720) [93.2 MB] || 14938_Artemis_Sci_Wright_A2Sim_1080.mp4 (1920x1080) [520.8 MB] || ArtemisSciWrightA2SimCaptions.en_US.srt [9.1 KB] || ArtemisSciWrightA2SimCaptions.en_US.vtt [8.7 KB] || 14938_Artemis_Sci_Wright_A2Sim_4K.mp4 (3840x2160) [3.2 GB] || 14938_Artemis_Sci_Wright_A2Sim_ProRes.mov (3840x2160) [20.2 GB] || ", "hits": 3768 }, { "id": 5503, "url": "https://svs.gsfc.nasa.gov/5503/", "result_type": "Visualization", "release_date": "2025-11-19T12:00:00-05:00", "title": "ESCAPADE Theoretical Flight Through Active Mars Magnetosphere", "description": "NASA's Escape and Plasma Acceleration Dynamics Explorers mission, or ESCAPADE, aims to study Mars' real-time response to the solar wind and how the Martian magnetosphere changes over time, helping us better understand Mars' climate history. In this data visualization, we use the September 13, 2017 solar storm that arrived at Mars as an example of a storm that the twin ESCAPADE spacecraft might study.", "hits": 396 }, { "id": 14818, "url": "https://svs.gsfc.nasa.gov/14818/", "result_type": "Produced Video", "release_date": "2025-09-26T12:00:00-04:00", "title": "Plunge: Behind the Scenes Creating NASA's Black Hole Visualization", "description": "Behind the scenes video about the Black Hole visualization from 2024", "hits": 359 }, { "id": 5375, "url": "https://svs.gsfc.nasa.gov/5375/", "result_type": "Visualization", "release_date": "2025-08-07T14:00:00-04:00", "title": "Carrington Class Coronal Mass Ejection - ENLIL Simulation of A Series of CMEs", "description": "A series of visualizations of the simulation of a series of CMEs between July 2012 and August 2012, including a carrington class coronal mass ejection that hit STEREO-A.", "hits": 310 }, { "id": 14847, "url": "https://svs.gsfc.nasa.gov/14847/", "result_type": "Produced Video", "release_date": "2025-06-02T11:00:00-04:00", "title": "100,000 Computer Simulations Reveal Milky Way's Fate", "description": "For decades, astronomers believed that one thing was as certain as death and taxes: the Milky Way and our neighboring Andromeda galaxy were on a crash course… destined to collide in less than 5 billion years.That galactic smash-up would spark massive star formation, scatter stars like cosmic billiard balls, and possibly throw our Sun into a whole new orbit.But now… that future may not be so certain.For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerVideo Credits:Milky Way TimelapseStock Footage Provided By Pond5/lovemushroomArtist Rendition of Gaia SpacecraftESAArtist’s animation of the Sun becoming a red giantESA/Hubble (M. Kornmesser & L. L. Christensen)Milky Way and Andromeda Collision SimulationVisualization Credit: NASA, ESA, and F. Summers (STScI) Simulation Credit: NASA, ESA, G. Besla (Columbia University), and R. van der Marel (STScI)Music Credit:\"Lost to Eternity\" by Timothy James Cornick [PRS] via BBC Production Music [PRS] and Universal Production Music || ", "hits": 463 }, { "id": 14793, "url": "https://svs.gsfc.nasa.gov/14793/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Black Holes Vertical Video", "description": "This page collects Astrophysics vertical videos with black-hole-related content", "hits": 1400 }, { "id": 5530, "url": "https://svs.gsfc.nasa.gov/5530/", "result_type": "Visualization", "release_date": "2025-05-14T08:00:59-04:00", "title": "Webb Confirms Seasonal Variations in Titan Climate Model", "description": "This global circulation model simulates a year of weather on Titan, depicting seasonal variations in wind currents, methane cloud cover, and sunlight over the course of a Saturn year (approximately 29.5 Earth years). New observations from the James Webb Science Telescope confirm this seasonal variation.", "hits": 181 }, { "id": 14835, "url": "https://svs.gsfc.nasa.gov/14835/", "result_type": "Produced Video", "release_date": "2025-05-09T15:00:00-04:00", "title": "What Happened During the Biggest Geomagnetic Storm in Over 20 Years", "description": "On May 10, 2024, the first G5 or “severe” geomagnetic storm in over two decades hit Earth. The event did not cause any catastrophic damages, but it did produce surprising effects on Earth. The storm, which has been called the best-documented geomagnetic storm in history, spread auroras to unusually low latitudes and produced effects spanning from the ground to near-Earth space. Data captured during this historic event will be analyzed for years to come, revealing new lessons about the nature of geomagnetic storms and how best to weather them.Learn more:• What NASA Is Learning from the Biggest Geomagnetic Storm in 20 Years• How NASA Tracked the Most Intense Solar Storm in Decades || ", "hits": 525 }, { "id": 20402, "url": "https://svs.gsfc.nasa.gov/20402/", "result_type": "Animation", "release_date": "2025-04-14T14:00:00-04:00", "title": "Lucy Flyby of Asteroid Donaldjohanson: Animations", "description": "Close up of Lucy's APP swiveling to keep DJ in frame. || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_print.jpg (1024x576) [79.5 KB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_searchweb.png (320x180) [48.0 KB] || LUCY_DJ_CloseUp_30fps_4k_h264_v02.mp4 (3840x2160) [73.9 MB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_thm.png [4.4 KB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.webm (3840x2160) [11.9 MB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.mov (3840x2160) [3.3 GB] || ", "hits": 46 }, { "id": 5514, "url": "https://svs.gsfc.nasa.gov/5514/", "result_type": "Visualization", "release_date": "2025-04-07T09:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere for Fulldome", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents and magnetic fields combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 276 }, { "id": 5502, "url": "https://svs.gsfc.nasa.gov/5502/", "result_type": "Visualization", "release_date": "2025-04-07T00:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents (green colors) and magnetic fields (pink lines) combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 342 }, { "id": 14749, "url": "https://svs.gsfc.nasa.gov/14749/", "result_type": "Produced Video", "release_date": "2025-01-14T10:00:00-05:00", "title": "OpenUniverse: Simulated Universe Views for Roman", "description": "This video begins with a tiny one-square-degree portion of the full OpenUniverse simulation area (about 70 square degrees, equivalent to an area of sky covered by more than 300 full moons). It spirals in toward a particularly galaxy-dense region, zooming by a factor of 75. This simulation showcases the cosmos as NASA’s Nancy Grace Roman Space Telescope could see it, allowing scientists to preview the next generation of cosmic discovery now. Roman’s real future surveys will enable a deep dive into the universe with highly resolved imaging, as demonstrated in this video.Credit: NASA’s Goddard Space Flight Center and M. Troxel || OpenUniverseFullZoom_4k_Best.00001_print.jpg (1024x576) [111.9 KB] || OpenUniverseFullZoom_4k_Good.mp4 (3840x2160) [101.9 MB] || OpenUniverseFullZoom_4k_Best.mp4 (3840x2160) [249.3 MB] || OpenUniverseFullZoom_ProRes_3840x2160_30.mov (3840x2160) [2.9 GB] || ", "hits": 129 }, { "id": 14739, "url": "https://svs.gsfc.nasa.gov/14739/", "result_type": "Produced Video", "release_date": "2025-01-03T12:00:00-05:00", "title": "From the Moon, NASA’s LEXI Will Reveal Earth’s Magnetic Shield", "description": "NASA’s next mission to the Moon will carry an instrument called LEXI (the Lunar Environment Heliospheric X-ray Imager), which will provide the first-ever global view of the magnetic environment that shields Earth from solar radiation.From the surface of the Moon, LEXI will capture wide-field images of Earth's magnetic environment, or magnetosphere, in low-energy (or \"soft\") X-rays. LEXI will study changes in the magnetosphere and help us learn more about how it interacts with a stream of particles from the Sun called the solar wind, which can pose hazards for Artemis astronauts traveling to the Moon.Learn more about LEXI and its CLPS (Commercial Lunar Payload Services) flight to the Moon from Hyunju Connor, LEXI co-investigator at NASA’s Goddard Space Flight Center.More on LEXI: https://science.nasa.gov/science-research/heliophysics/nasas-lexi-will-provide-x-ray-vision-of-earths-magnetosphere/ || ", "hits": 198 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 297 }, { "id": 5394, "url": "https://svs.gsfc.nasa.gov/5394/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "How much does the Gulf of Mexico Contribute to the Gulf Stream?", "description": "Animation 1: Lagrangian particles colored by temperature viewed from above with fixed camera. || GM_experiment22_2024-11-01_1336_final_flatT.01638_print.jpg (1024x576) [232.7 KB] || GM_experiment22_2024-11-01_1336_final_flatT.01638_searchweb.png (320x180) [103.9 KB] || GM_experiment22_2024-11-01_1336_final_flatT.01638_thm.png (80x40) [6.5 KB] || GM_experiment_flatT_1080p30.mp4 (1920x1080) [58.9 MB] || flatT [0 Item(s)] || GM_experiment22_final_flatT.mp4 (3840x2160) [196.8 MB] || GM_experiment22_final_flatT.mp4.hwshow [193 bytes] || ", "hits": 174 }, { "id": 14719, "url": "https://svs.gsfc.nasa.gov/14719/", "result_type": "Visualization", "release_date": "2024-11-13T09:00:00-05:00", "title": "Swift Studies Gas-Churning Monster Black Holes", "description": "Watch as a gas cloud encounters two supermassive black holes. The complex interplay of gravitational and frictional forces causes the cloud to condense and heat. Some of the gas is ejected from the system with each orbit of the black holes.Credit: F. Goicovic et al. 2016Music: \"Forgotten Fortunes,\" Magnum Opus [ASCAP] , Universal Production MusicComplete transcript available. || Sim_Video_Still.jpg (3840x2160) [744.6 KB] || Sim_Video_Still_searchweb.png (320x180) [37.6 KB] || Sim_Video_Still_thm.png (80x40) [3.4 KB] || BH_Binary_TD_Sim_1080_Final.mp4 (1920x1080) [38.5 MB] || BH_Binary_TD_Sim_4k_Final.mp4 (3840x2160) [45.5 MB] || BH_Binary_TD_Sim_4k_Final_best.mp4 (3840x2160) [67.9 MB] || 14719_BinaryBHTDE_Captions.en_US.srt [57 bytes] || 14719_BinaryBHTDE_Captions.en_US.vtt [67 bytes] || BH_Binary_TD_Sim_4k_Final_ProRes.mov (3840x2160) [1.5 GB] || ", "hits": 124 }, { "id": 5365, "url": "https://svs.gsfc.nasa.gov/5365/", "result_type": "Visualization", "release_date": "2024-09-19T11:00:00-04:00", "title": "Broken Annular Baily's Beads Simulation", "description": "Simulation of Baily's beads from 21:55:20.5 to 21:55:35.5 UTC during the April 8, 2005 hybrid solar eclipse, as viewed from 94.02587°W, 6.45677°N. The movie runs in real time. || beads.0150_print.jpg (1024x576) [53.4 KB] || beads.0150_searchweb.png (320x180) [33.3 KB] || beads.0150_thm.png (80x40) [3.5 KB] || beads_1080p30.mp4 (1920x1080) [3.4 MB] || beads_720p30.mp4 (1280x720) [1.5 MB] || beads_360p30.mp4 (640x360) [416.0 KB] || 1920x1080_16x9_30p [16.0 KB] || ", "hits": 82 }, { "id": 14655, "url": "https://svs.gsfc.nasa.gov/14655/", "result_type": "Produced Video", "release_date": "2024-08-14T11:50:00-04:00", "title": "Globular Star Cluster Exploration (Dome Version)", "description": "Globular Star Cluster Exploration || THUMB.jpg (1920x1080) [90.1 KB] || PRINT_2.jpg (1920x1080) [90.1 KB] || Search.jpg (320x180) [11.5 KB] || Globular_Star_Cluster_Exploration_Dome_Version.mp4 (1280x720) [73.9 MB] || 3800x3800_1x1_30p [256.0 KB] || ", "hits": 66 }, { "id": 14656, "url": "https://svs.gsfc.nasa.gov/14656/", "result_type": "Produced Video", "release_date": "2024-08-14T11:00:00-04:00", "title": "Galaxy Collision Simulation (Dome Version)", "description": "Galaxy Collision Simulation || PRINT.jpg (1920x1080) [62.5 KB] || THUMB.jpg (1920x1080) [62.5 KB] || SEARCH.jpg (320x180) [8.3 KB] || Galaxy_Collision_Simulation_Dome_Version.mp4 (1280x720) [28.6 MB] || 1024x1024_1x1_30p [128.0 KB] || 2048x2048_1x1_30p [128.0 KB] || 3200x3200_1x1_30p [128.0 KB] || 3800x3800_1x1_30p [128.0 KB] || ", "hits": 119 }, { "id": 14647, "url": "https://svs.gsfc.nasa.gov/14647/", "result_type": "B-Roll", "release_date": "2024-08-12T13:00:00-04:00", "title": "CODEX – Coronal Diagnostic Experiment", "description": "The Coronal Diagnostic Experiment (CODEX) is a solar coronagraph that will be installed on the International Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contribution from Italy's National Institute for Astrophysics (INAF).Learn more: https://science.nasa.gov/mission/codex/ || ", "hits": 78 }, { "id": 14631, "url": "https://svs.gsfc.nasa.gov/14631/", "result_type": "Produced Video", "release_date": "2024-07-22T11:00:00-04:00", "title": "Model Behavior: Visualizing Global CO2", "description": "Universal Production Music: Prismatic by David Stephen Goldsmith [ PRS ]Complete transcript available. || 14631_DYAMONDThumbnailHorz.jpg (1280x720) [291.1 KB] || 14631_DYAMONDThumbnailHorz_print.jpg (1024x576) [222.2 KB] || 14631_DYAMONDThumbnailHorz_searchweb.png (320x180) [91.4 KB] || 14631_DYAMONDThumbnailHorz_thm.png (80x40) [7.1 KB] || 14631_dyamondhorz_US.en.en_US.srt [2.3 KB] || 14631_dyamondhorz_US.en.en_US.vtt [2.2 KB] || 14631_DYAMOND_Horz.webm (3840x2160) [32.4 MB] || 14631_DYAMOND_Horz.mp4 (3840x2160) [267.6 MB] || ", "hits": 387 }, { "id": 40521, "url": "https://svs.gsfc.nasa.gov/gallery/svsdbgallery2024goddardsummerfilmfest/", "result_type": "Gallery", "release_date": "2024-06-28T00:00:00-04:00", "title": "2024 Goddard Summer Film Fest", "description": "Hosted by the Goddard Office of Communications, the 15th annual Goddard Film Festival is a special two-day event this year, highlighting the center’s achievements over the past year in astrophysics, Earth science, heliophysics and planetary science.\n \nOn Wednesday, July 17th at 2 pm, the Goett Auditorium in Building 3 will host a screening that will feature missions and topics such as OSIRIS-REx, PACE, CLPS, Voyager, Hubble, black holes, solar eclipses and much more.", "hits": 72 }, { "id": 14604, "url": "https://svs.gsfc.nasa.gov/14604/", "result_type": "Produced Video", "release_date": "2024-06-12T10:00:00-04:00", "title": "NASA’s Roman Mission Gets Cosmic ‘Sneak Peek’ From Supercomputers", "description": "This graphic highlights part of a new simulation of what NASA’s Nancy Grace Roman Space Telescope could see when it launches by May 2027. The background spans about 0.11 square degrees (roughly equivalent to half of the area of sky covered by a full Moon), representing less than half the area Roman will see in a single snapshot. The inset zooms in to a region 300 times smaller, showcasing a swath of brilliant synthetic galaxies at Roman’s full resolution. Having such a realistic simulation helps scientists study the physics behind cosmic images –– both synthetic ones like these and future real ones. Researchers will use the observations for many types of science, including testing our understanding of the origin, evolution, and ultimate fate of the universe.Credit: C. Hirata and K. Cao (OSU) and NASA’s Goddard Space Flight Center || Roman_Simulation_Popout_2k_deg.jpg (2048x2048) [979.2 KB] || ", "hits": 58 }, { "id": 14598, "url": "https://svs.gsfc.nasa.gov/14598/", "result_type": "Produced Video", "release_date": "2024-06-07T00:00:00-04:00", "title": "Cruising the Cosmic Web (Dome Version)", "description": "Cruising the Cosmic Web || PRINT.jpg (1920x1080) [250.5 KB] || THUMB.jpg (1920x1080) [250.5 KB] || SEARCH.jpg (320x180) [20.0 KB] || Cruising_the_Cosmic_Web,_V2_Dome_Version.mp4 (1280x720) [36.0 MB] || 1024x1024_1x1_30p [256.0 KB] || 2200x2200_1x1_30p [256.0 KB] || ", "hits": 348 }, { "id": 14583, "url": "https://svs.gsfc.nasa.gov/14583/", "result_type": "Produced Video", "release_date": "2024-05-08T00:00:00-04:00", "title": "Artemis & JETT5 Interview with Kelsey Young", "description": "Dr. Kelsey Young is the Artemis Science Flight Operations Lead and works at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.Complete transcript available.Dr. Young discusses the JETT5 mission, which was conducted May 13-17. During JETT5, astronauts performed a series of simulated moonwalks in the San Francisco Volcanic Field near Flagstaff, Arizona, while flight controllers and scientists at NASA’s Johnson Space Center in Houston, Texas guided and provided feedback on their progress. JETT5 was designed to prepare crew members for the historic Artemis III mission that will land near the Moon’s south pole.00:00:00:00 – What is your role in NASA’s Artemis missions?00:00:58:03 – What was the JETT5 mission, and what activities did it include?00:01:49:03 – Why are mission simulations like JETT5 critical?00:02:32:20 – Why was Arizona chosen as the site of the JETT5 field test?00:03:44:18 – Why were the field tests conducted both in daytime and at night?00:04:39:13 – Where were Mission Control team members and scientists located?00:05:21:26 – What is the Science Evaluation Room for the Artemis missions?00:06:10:17 – What are the activities and roles within the Science Evaluation Room?00:06:49:00 – What science payloads will the Artemis crew deploy on the lunar surface?00:07:22:28 – What goes into creating a scientifically well-trained crew member? || Kelsey_Young_Interview_Preview_print.jpg (1024x576) [89.8 KB] || Kelsey_Young_Interview_Preview.png (3840x2160) [11.8 MB] || Kelsey_Young_Interview_Preview.jpg (3840x2160) [2.7 MB] || Kelsey_Young_Interview_Preview_searchweb.png (320x180) [76.3 KB] || Kelsey_Young_Interview_Preview_thm.png (80x40) [6.6 KB] || Kelsey_Young_Interview_JETT5_720.mp4 (1280x720) [122.5 MB] || Kelsey_Young_Interview_JETT5_1080.mp4 (1920x1080) [685.7 MB] || KelseyYoungInterviewJETT5.en_US.srt [14.0 KB] || KelseyYoungInterviewJETT5.en_US.vtt [13.4 KB] || Kelsey_Young_Interview_JETT5_4K.mp4 (3840x2160) [4.2 GB] || Kelsey_Young_Interview_JETT5_ProRes.mov (3840x2160) [32.5 GB] || ", "hits": 938 }, { "id": 14576, "url": "https://svs.gsfc.nasa.gov/14576/", "result_type": "Visualization", "release_date": "2024-05-06T13:00:00-04:00", "title": "NASA Black Hole Visualization Takes Viewers Beyond the Brink", "description": "In this flight toward a supermassive black hole, labels highlight many of the fascinating features produced by the effects of general relativity along the way. This supercomputer visualization tracks a camera as it approaches, briefly orbits, and then crosses the event horizon — the point of no return — of a supersized black hole similar in mass to the one at the center of our galaxy. Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. PowellMusic: “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music“Memories” from Digital Juice“Path Finder,” Eric Jacobsen [TONO] and Lorenzo Castellarin [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14576_BHPlunge_Explain_Still.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail_searchweb.png (180x320) [85.0 KB] || 14576_PageThumbnail_thm.png (80x40) [9.6 KB] || 14576_BHPlunge_Explainer_1080.mp4 (1920x1080) [319.5 MB] || 14576_BHPlunge_Explainer_Captions.en_US.srt [2.5 KB] || 14576_BHPlunge_Explainer_Captions.en_US.vtt [2.4 KB] || 14576_BHPlunge_Explainer_4k.mp4 (3840x2160) [1.5 GB] || 14576_BHPlunge_Explainer_4kYouTube.mp4 (3840x2160) [3.0 GB] || 14576_BHPlunge_Explainer_ProRes_3840x2160_2997.mov (3840x2160) [12.8 GB] || ", "hits": 1612 }, { "id": 14585, "url": "https://svs.gsfc.nasa.gov/14585/", "result_type": "Visualization", "release_date": "2024-05-06T00:00:00-04:00", "title": "Beyond the Brink: Tracking a Simulated Plunge into a Black Hole", "description": "In this all-sky view, the camera approaches a supermassive black hole weighing 4.3 million Suns. It is about 70 million miles (113 million kilometers) from the black hole’s event horizon, the boundary of no return. It’s moving inward at 19% the speed of light — nearly 127 million mph (205 million kph). A flat, swirling cloud of hot, glowing gas called an accretion disk surrounds the black hole and serves as a visual reference during the fall, as do glowing structures called photon rings, which form closer to the black hole from light that has orbited it one or more times. A backdrop of the starry sky completes the scene.Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. Powell || 1_BH_Viz_20_rg_019c.jpg (8192x4096) [6.1 MB] || ", "hits": 420 }, { "id": 5214, "url": "https://svs.gsfc.nasa.gov/5214/", "result_type": "Visualization", "release_date": "2024-02-08T08:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss for Fulldome", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events.This is 4k fulldome imagery intended for projection in a planetarium or other hemispherical dome theater. || ", "hits": 96 }, { "id": 5193, "url": "https://svs.gsfc.nasa.gov/5193/", "result_type": "Visualization", "release_date": "2023-12-11T09:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events. || ", "hits": 484 }, { "id": 5169, "url": "https://svs.gsfc.nasa.gov/5169/", "result_type": "Interactive", "release_date": "2023-10-02T09:00:00-04:00", "title": "NASA Eclipse Explorer: An interactive guide to the 2017, 2023, and 2024 Solar Eclipses", "description": "|| An embedded version of the NASA Eclipse Explorer. The standalone version is available at https://go.nasa.gov/EclipseExplorer. || eclipse_explorer_screenshot_print.jpg (1024x661) [170.8 KB] || eclipse_explorer_screenshot.png (3456x2234) [6.1 MB] || eclipse_explorer_screenshot_searchweb.png (320x180) [73.4 KB] || eclipse_explorer_screenshot_thm.png (80x40) [8.9 KB] ||", "hits": 107 }, { "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": 255 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary 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": 339 }, { "id": 40483, "url": "https://svs.gsfc.nasa.gov/gallery/air-qualityin-dc/", "result_type": "Gallery", "release_date": "2023-06-08T00:00:00-04:00", "title": "Air Quality in DC", "description": "NASA-supported scientist Susan Anenberg reviews air pollution data from satellites, airplanes, and ground sensors and combines it with data on race, ethnicity, poverty, and health. In doing so Anenberg unveils the both the big picture of air pollution and individual neighborhood effects. Information that lets community leaders and other decision makers to make better decisions and address long standing inequities.", "hits": 6 }, { "id": 40487, "url": "https://svs.gsfc.nasa.gov/gallery/nasaand-hurricanes/", "result_type": "Gallery", "release_date": "2023-06-08T00:00:00-04:00", "title": "NASA and Hurricanes", "description": "Hurricanes are getting stronger due to climate change warming the air and oceans. NASA atmospheric scientist Mara Fuentes says NASA sees deep into hurricanes to better their power, track storms through the night, and precisely map flooding in real time. NASA shares this information with partners like NOAA for weather forecasts and FEME to support emergency responders. Before, during, and after a hurricane, NASA data is put to use by decision makers to make critical decisions.", "hits": 124 }, { "id": 14331, "url": "https://svs.gsfc.nasa.gov/14331/", "result_type": "Produced Video", "release_date": "2023-04-06T09:55:00-04:00", "title": "Hubble Catches Possible Runaway Black Hole", "description": "There’s an invisible monster on the loose! It’s barreling through intergalactic space fast enough to travel from Earth to the Moon in 14 minutes. But don’t worry, luckily this beast is very, very far away!This potential supermassive black hole, weighing as much as 20 million Suns, has left behind a never-before-seen 200,000 light-year-long trail of newborn stars. The streamer is twice the diameter of our Milky Way galaxy. It’s likely the result of a rare, bizarre game of galactic billiards among three massive black holes.For more information, visit https://nasa.gov/hubble. Video Credit:Black Hole AnimationNASA’s Goddard Space Flight Center/Jeremy SchnittmanImage of Chandra X-Ray ObservatoryNASA/CXC and J. Vaughan3 Black Hole Orbits and SlingshotsImage from paper “A candidate runaway supermassive black hole identified by shocks and star formation in its wake” by PI Pieter Von Dokkum et al.Schematic illustration of the runaway SMBH scenario as an explanation of the key observed features. Panels 1–5 show a “classical” slingshot scenario (e.g., Saslaw et al. 1974). The background of panel 6 is a frame from an Illustris TNG simulation (Pillepich et al. 2018)Music Credit:“Unclaimed Space” by Peter Nickalls [PRS] via Atmosphere Music Ltd. [PRS] and Universal Production Music. || ", "hits": 40 }, { "id": 40461, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles7-echoesofthe-big-bang/", "result_type": "Gallery", "release_date": "2023-03-27T00:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "NASA studies the makeup and workings of the universe, from the smallest particles of matter and energy to its large-scale structure and evolution. Scientists look far back in space and time to learn the full cosmic history of stars and galaxies. They tease out details of the environments around black holes and observe the most powerful explosions since the big bang. NASA is discovering numerous planets beyond our solar system, decoding how planetary systems form, and learning how environments hospitable for life develop.\n\nWant to know more?\nNASA Universe Webb Space Telescope images Hubble Space Telescope", "hits": 56 }, { "id": 14301, "url": "https://svs.gsfc.nasa.gov/14301/", "result_type": "Produced Video", "release_date": "2023-03-08T10:00:00-05:00", "title": "Millions of Galaxies Emerge in New Simulated Images From NASA's Roman", "description": "This video begins by showing the most distant galaxies in the simulated deep field image in red. As it zooms out, layers of nearer (yellow and white) galaxies are added to the frame. By studying different cosmic epochs, Roman will be able to trace the universe's expansion history, study how galaxies developed over time, and much more.Credit: Caltech-IPAC/R. Hurt and M. Troxel || Roman_Zoom_still.jpg (1920x1080) [515.9 KB] || Roman_Zoom_still_searchweb.png (320x180) [106.4 KB] || Roman_Zoom_still_thm.png (80x40) [6.6 KB] || Roman_Zoom-HD2K.mp4 (1920x1080) [25.3 MB] || Roman_Zoom-HD2K.webm (1920x1080) [2.7 MB] || ", "hits": 72 }, { "id": 14297, "url": "https://svs.gsfc.nasa.gov/14297/", "result_type": "Produced Video", "release_date": "2023-03-01T10:00:00-05:00", "title": "How NASA's Roman Space Telescope Will Rewind the Universe", "description": "In this simulated view of the deep cosmos, each dot represents a galaxy. The three small squares show Hubble's field of view, and each reveals a different region of the synthetic universe. Roman will be able to quickly survey an area as large as the whole zoomed-out image, which will give us a glimpse of the universe’s largest structures.Credits: NASA’s Goddard Space Flight Center/A. Yung || Yung_Stucture_Survey-Hubble.gif (800x800) [10.9 MB] || Yung_Structure_Survey-Hubble_ProRes.mov (800x800) [36.3 MB] || Yung_Structure_Survey-Hubble_800.mp4 (800x800) [6.4 MB] || Yung_Structure_Survey-Hubble_800.webm (800x800) [1.6 MB] || ", "hits": 93 }, { "id": 14209, "url": "https://svs.gsfc.nasa.gov/14209/", "result_type": "Produced Video", "release_date": "2023-01-09T17:10:00-05:00", "title": "NASA’s Compton Mission Glimpses Supersized Neutron Stars", "description": "This simulation tracks the gravitational wave and density changes as two orbiting neutron stars crash together. Dark purple colors represent the lowest densities, while yellow-white shows the highest. An audible tone and a visual frequency scale (at left) track the steady rise in the frequency of gravitational waves as the neutron stars close. When the objects merge at 42 seconds, the gravitational waves suddenly jump to frequencies of thousands of hertz and bounce between two primary tones (quasiperiodic oscillations, or QPOs). The presence of these signals in such simulations led to the search and discovery of similar phenomena in the light emitted by short gamma-ray bursts.Credit: NASA's Goddard Space Flight Center and STAG Research Centre/Peter HammondComplete transcript available.Watch this video on the NASA Goddard YouTube channel.Visual description:On a black background with a faint gray grid, two multicolored blobs representing merging neutron stars circle and close. The colors indicate density. Yellow-white indicates the highest densities, at the centers of the objects. The colors change to orange and red at their periphery, with purple colors representing matter torn from and swirling with the neutron stars as they orbit. The grid shrinks as the camera pulls back to capture a wider view of the merger. A pale orange display at left shows the changing frequency of the gravitational waves generated, which is also indicated by the rising tone. As the merger occurs, the screen shows a spinning yellow blob at center immersed in a large cloud of magneta and purple debris. || Merger_Simulation_Annotated_Still_2.jpg (1920x1080) [180.7 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.webm (1920x1080) [12.1 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.mp4 (1920x1080) [129.3 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_BEST_1080.mp4 (1920x1080) [161.8 MB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.srt [1.6 KB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.vtt [1.6 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_ProRes_1920x1080_2997.mov (1920x1080) [1.0 GB] || ", "hits": 261 }, { "id": 14203, "url": "https://svs.gsfc.nasa.gov/14203/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Simulations of Weak Black Hole Jets", "description": "This sequence shows the simulated evolution of weak jets (orange, pink, and purple) formed by a supermassive black hole as they interact with stars and gas clouds (green, yellow) at the center of a galaxy. The jet is angled about 15 degrees toward the plane of its galaxy and is shown in 12 time steps, with each interval representing 50,000 years. The image at bottom right shows the jets 600,000 years after they formed. Each step is available as a 4K video and as frames by selecting \"Download Options.\"Credit: NASA's Goddard Space Flight Center/R. Tanner and K. Weaver || AGN_time_series_Numbered_print.jpg (1024x576) [109.6 KB] || AGN_time_series_Numbered.jpg (3840x2160) [982.9 KB] || Step1 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.webm (4000x4000) [3.2 MB] || Step12 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step12_4k_30.mp4 (4000x4000) [15.0 MB] || Step11 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step11_4k_30.mp4 (4000x4000) [15.0 MB] || Step10 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step10_4k_30.mp4 (4000x4000) [14.9 MB] || Step9 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step9_4k_30.mp4 (4000x4000) [15.0 MB] || Step8 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step8_4k_30.mp4 (4000x4000) [15.0 MB] || Step7 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step7_4k_30.mp4 (4000x4000) [15.0 MB] || Step6 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.mp4 (4000x4000) [15.1 MB] || Step5 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step5_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step2_4k_30.mp4 (4000x4000) [15.0 MB] || Step4 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step4_4k_30.mp4 (4000x4000) [15.0 MB] || Step2 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step6_4k_30.mp4 (4000x4000) [14.9 MB] || Step3 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step3_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step10_ProRes_4k_30.mov (4000x4000) [3.1 GB] || AGNwinds_TimeEvolution_Step1_ProRes_4k_30.mov (4000x4000) [387.2 MB] || AGNwinds_TimeEvolution_Step2_ProRes_4k_30.mov (4000x4000) [864.7 MB] || AGNwinds_TimeEvolution_Step12_ProRes_4k_30.mov (4000x4000) [3.3 GB] || AGNwinds_TimeEvolution_Step3_ProRes_4k_30.mov (4000x4000) [1.4 GB] || AGNwinds_TimeEvolution_Step11_ProRes_4k_30.mov (4000x4000) [3.2 GB] || AGNwinds_TimeEvolution_Step4_ProRes_4k_30.mov (4000x4000) [1.9 GB] || AGNwinds_TimeEvolution_Step9_ProRes_4k_30.mov (4000x4000) [2.9 GB] || AGNwinds_TimeEvolution_Step5_ProRes_4k_30.mov (4000x4000) [2.4 GB] || AGNwinds_TimeEvolution_Step8_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step7_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step6_ProRes_4k_30.mov (4000x4000) [2.7 GB] || ", "hits": 183 }, { "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": 171 }, { "id": 5023, "url": "https://svs.gsfc.nasa.gov/5023/", "result_type": "Visualization", "release_date": "2022-09-19T09:30:00-04:00", "title": "Lunar Polar Wander", "description": "The wandering path of the lunar South Pole is shown over a period from 4.25 billion years ago to the present.This video can also be viewed on the SVS YouTube channel. || tpw.0750_print.jpg (1024x576) [250.9 KB] || tpw.0750_searchweb.png (320x180) [109.2 KB] || tpw.0750_thm.png (80x40) [7.6 KB] || tpw_1080p30.mp4 (1920x1080) [46.9 MB] || tpw_720p30.mp4 (1280x720) [22.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || tpw_720p30.webm (1280x720) [5.6 MB] || tpw_360p30.mp4 (640x360) [8.1 MB] || tpw_1080p30.mp4.hwshow [177 bytes] || ", "hits": 129 }, { "id": 40447, "url": "https://svs.gsfc.nasa.gov/gallery/visualizationsfor-educators/", "result_type": "Gallery", "release_date": "2022-08-17T00:00:00-04:00", "title": "Visualizations for Educators", "description": "Phenomena are observable events that occur in nature. Data visualizations can offer new ways for students to experience and explore Earth and space phenomena that happen over large scales of time and at great distances. This gallery includes visualizations of phenomena that support topics that are taught in middle and high school and are aligned with select Next Generation Science Standards.\n\n\nThis gallery was curated by Anne Arundle County Science Teachers Margaret Graham and Jeremy Milligan with support from Dr. Rachel Connolly during the summer of 2022. A video showing how Jeremy Milligan uses SVS resources to develop a phenomena-based lesson is also available.", "hits": 286 }, { "id": 20360, "url": "https://svs.gsfc.nasa.gov/20360/", "result_type": "Animation", "release_date": "2022-07-07T14:30:00-04:00", "title": "Thirty Seconds on Asteroid Bennu: Animation", "description": "Data-driven animation showing how the OSIRIS-REx spacecraft impacted asteroid Bennu's surface when it touched down and collected a sample. || 20360_Orex_tag_h264_1080.00111_print.jpg (576x1024) [160.5 KB] || 20360_Orex_tag_h264_1080.00111_searchweb.png (320x180) [97.3 KB] || 20360_Orex_tag_h264_1080.00111_thm.png (80x40) [6.1 KB] || 20360_Orex_tag_h264_1080.webm (1920x1080) [13.2 MB] || 20360_Orex_tag_h264_1080.mp4 (1920x1080) [175.4 MB] || 20360_Orex_tag_h264_4K.mp4 (3840x2160) [86.5 MB] || OREx_Tag_PNG (3840x2160) [0 Item(s)] || 20360_Orex_Prores_4k.mov (3840x2160) [4.4 GB] || ", "hits": 158 }, { "id": 14172, "url": "https://svs.gsfc.nasa.gov/14172/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Dominic Benford 2022 AAS Roman Hyperwall Talk", "description": "Static title card.Credit: NASA's Goddard Space Flight Center || dominic_benford_roman_title_slide_print.jpg (1024x576) [262.4 KB] || dominic_benford_roman_title_slide.png (3840x2160) [10.2 MB] || dominic_benford_roman_title_slide_searchweb.png (320x180) [113.1 KB] || dominic_benford_roman_title_slide_thm.png (80x40) [7.9 KB] || ", "hits": 21 }, { "id": 14174, "url": "https://svs.gsfc.nasa.gov/14174/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Rebekah Hounsell 2022 AAS Roman Hyperwall Talk", "description": "Title slide.Credit: NASA's Goddard Space Flight Center || rebekah_hounsell_roman_title_print.jpg (1024x576) [250.4 KB] || rebekah_hounsell_roman_title.png (3840x2160) [10.3 MB] || rebekah_hounsell_roman_title_searchweb.png (320x180) [111.8 KB] || rebekah_hounsell_roman_title_thm.png (80x40) [8.1 KB] || ", "hits": 34 }, { "id": 14175, "url": "https://svs.gsfc.nasa.gov/14175/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Expanding Our View (2022 STScI presentation)", "description": "Complete PowerPoint file with all slides and notes || PPT_still.jpg (3840x2160) [750.6 KB] || roman-expanding-our-view-presentation.pptx [76.2 MB] || Slide #1 – Onscreen before presentation begins and during introductionCredit: STScI, NASA || Slide1_print.jpg (1024x576) [98.1 KB] || Slide1.png (3840x2160) [3.4 MB] || Slide1.jpg (3840x2160) [750.6 KB] || Slide1_searchweb.png (320x180) [63.9 KB] || Slide1_thm.png (80x40) [5.6 KB] || ", "hits": 55 }, { "id": 14146, "url": "https://svs.gsfc.nasa.gov/14146/", "result_type": "Produced Video", "release_date": "2022-05-04T00:00:00-04:00", "title": "Black Hole Desktop & Phone Wallpapers", "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ", "hits": 9142 }, { "id": 14134, "url": "https://svs.gsfc.nasa.gov/14134/", "result_type": "Produced Video", "release_date": "2022-05-02T13:00:00-04:00", "title": "NASA Simulation Suggests Some Volcanoes Might Warm Climate, Destroy Ozone Layer", "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Good Omens\" by Count Zero and Rohan Stevenson and \"Blue Moons\" by Gresby Race Nash of Universal Production Music || 14134_thumb.jpg (1920x1080) [450.5 KB] || volcanism_14134.00242_searchweb.png (320x180) [71.1 KB] || volcanism_14134.00242_thm.png (80x40) [5.5 KB] || volcanism_14134.mp4 (1920x1080) [377.7 MB] || volcanism_14134.webm (1920x1080) [27.0 MB] || volcanism_14134_caption.en_US.srt [4.9 KB] || volcanism_14134_caption.en_US.vtt [4.7 KB] || ", "hits": 99 }, { "id": 4987, "url": "https://svs.gsfc.nasa.gov/4987/", "result_type": "Visualization", "release_date": "2022-04-28T11:00:00-04:00", "title": "Fast Magnetic Reconnection and the Hall Effect", "description": "Magnetic reconnection is one of the most complex processes known for converting energy from magnetic fields to particle motion. It takes place in solar flares and regions of planetary (and stellar) magnetospheres. Having been studied since the 1950s, many details of the process are still undergoing study.One of the key components in magnetic reconnection is the collision of two magnetic field regions with opposite-directed field lines, imbedded in a plasma. The field and plasma combination forms an X-shaped configuration at their closest, and most intense point.These visualizations are plotted from a reconnection model generated by VPIC (Vector Particle-In-Cell) code. Quantities are plotted in 'dimensionless' coordinates, that are normalized to the ion inertial length (di). || ", "hits": 167 }, { "id": 14132, "url": "https://svs.gsfc.nasa.gov/14132/", "result_type": "Produced Video", "release_date": "2022-04-12T00:00:00-04:00", "title": "Black Hole Week: Black Hole GIFs", "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ", "hits": 434 }, { "id": 14130, "url": "https://svs.gsfc.nasa.gov/14130/", "result_type": "Produced Video", "release_date": "2022-04-07T14:00:00-04:00", "title": "Fermi Searches for Gravitational Waves From Monster Black Holes", "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ", "hits": 104 }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "result_type": "Produced Video", "release_date": "2022-04-06T13:00:00-04:00", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "hits": 46 }, { "id": 14105, "url": "https://svs.gsfc.nasa.gov/14105/", "result_type": "Produced Video", "release_date": "2022-03-22T10:00:00-04:00", "title": "Simulated Galaxy Redshift Cubes", "description": "This video dissolves between the entire collection of redshift cubes in 55 seconds. A shorter, faster version is available below.Credit: NASA’s Goddard Space Flight Center/F. Reddy and Z. Zhai, Y. Wang (IPAC) and A. Benson (Carnegie Observatories)Watch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Cube_Spin_110-Short_mkII_still.jpg (1920x1080) [577.0 KB] || Cube_Spin_110-Short_mkII_still_print.jpg (1024x576) [158.1 KB] || Cube_Spin_110-Short_mkII_still_thm.png (80x40) [6.3 KB] || Cube_Spin_110-Short_mkII_still_searchweb.png (320x180) [79.4 KB] || 14105_110_RedshiftGalaxyCube_Dissolve_1080.mp4 (1920x1080) [59.2 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_ProRes_1920x1080_2997.mov (1920x1080) [970.0 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_1080.webm (1920x1080) [7.0 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_SRT_Captions.en_US.srt [956 bytes] || 14105_110_RedshiftGalaxyCube_Dissolve_SRT_Captions.en_US.vtt [969 bytes] || ", "hits": 185 }, { "id": 14116, "url": "https://svs.gsfc.nasa.gov/14116/", "result_type": "Produced Video", "release_date": "2022-03-18T00:00:00-04:00", "title": "Two Scientists Have a Frank and Honest Discussion about Antarctica", "description": "NASA Glaciologists Kelly Brunt and Alex Gardner discuss the history, challenges and evolution of mapping the Antarctic continent and what it means for science and society. || ", "hits": 32 }, { "id": 20358, "url": "https://svs.gsfc.nasa.gov/20358/", "result_type": "Animation", "release_date": "2022-02-16T12:00:00-05:00", "title": "Webb Mirror Alignment Animations", "description": "Crowded field yields light on NIRCam instrument to check it's properly functioning for its key role in aligning Webb's mirrors. || WEBB_FL_4k_30fps_ProRes.00125_print.jpg (1024x576) [194.9 KB] || WEBB_FL_1K_30fps.mp4 (1000x562) [2.4 MB] || WEBB_FL_HD_30fps.mp4 (1920x1080) [4.9 MB] || WEBB_FL_4k_30fps_ProRes.mov (3840x2160) [450.6 MB] || WEBB_FL_4k_30fps_h264.mp4 (3840x2160) [5.5 MB] || WEBB_FL_4k (3840x2160) [8.0 KB] || WEBB_FL_4k_30fps_h264.webm (3840x2160) [1.2 MB] || ", "hits": 143 }, { "id": 40436, "url": "https://svs.gsfc.nasa.gov/gallery/black-hole-week/", "result_type": "Gallery", "release_date": "2022-02-12T00:00:00-05:00", "title": "Black Hole Week", "description": "This gallery brings together resources related to NASA’s Black Hole Week — videos, social media products, news stories, still images, and assets. This week is a celebration of celestial objects with gravity so intense that even light cannot escape them. Our goal is that no matter where people turn that week they will run into a black hole. (Figuratively, of course — we don’t want anyone falling in!)", "hits": 284 }, { "id": 13921, "url": "https://svs.gsfc.nasa.gov/13921/", "result_type": "Produced Video", "release_date": "2022-01-10T10:00:00-05:00", "title": "The Roman Space Telescope's Simulated Ultra-Deep Field Image", "description": "This video demonstrates how Roman could expand on Hubble’s iconic Ultra Deep Field image. While a similar Roman observation would be just as sharp as Hubble’s and see equally far back in time, it could reveal an area 300 times larger, offering a much broader view of cosmic ecosystems. Credit: NASA’s Goddard Space Flight CenterMusic: \"Subterranean Secret\" and \"Expectant Aspect\" from Universal Production Music.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SUDF_Footprint_print.jpg (1024x576) [232.0 KB] || SUDF_Footprint.jpg (3840x2160) [2.7 MB] || SUDF_Footprint_thm.png (80x40) [4.3 KB] || SUDF_Footprint_searchweb.png (320x180) [71.2 KB] || SUDF_Footprint_web.png (320x180) [71.2 KB] || 13921_Roman_Simulated_UDF_1080.webm (1920x1080) [24.4 MB] || 13921_Roman_Simulated_UDF_SRT_Captions.en_US.srt [3.8 KB] || 13921_Roman_Simulated_UDF_SRT_Captions.en_US.vtt [3.9 KB] || 13921_Roman_Simulated_UDF_ProRes_1920x1080_2997.mov (1920x1080) [3.0 GB] || 13921_Roman_Simulated_UDF_1080_Best.mp4 (1920x1080) [439.7 MB] || 13921_Roman_Simulated_UDF_1080.mp4 (1920x1080) [228.8 MB] || ", "hits": 85 }, { "id": 4959, "url": "https://svs.gsfc.nasa.gov/4959/", "result_type": "Visualization", "release_date": "2021-12-13T00:00:00-05:00", "title": "Reduction in Tropospheric NOx and Ozone Corresponding to Worldwide COVID-19 Lockdowns", "description": "When the world went into lockdown to slow the spread of COVID-19, air pollution emissions started to rapidly decrease leaving a global atmospheric fingerprint detected by a team of scientists at NASA’s Jet Propulsion Laboratory using satellite measurements. These traces provided an unexpected window into what low-emissions world could look like, thus providing a means for identifying effective environmental policies. While many countries in the last few decades have implemented environmental policies to reduce human health risk from air pollution by controlling emissions, the impacts of those policies have not always been clear. The global lockdowns in response to COVID-19 represent a well-observed “scenario-of-opportunity” that allows us to assess how atmospheric emission and composition responds to reduced human activity. COVID-19 lockdowns effectively showed how reducing NOx emissions affects the global atmosphere. Its identifying signature shows up as in the atmosphere’s altered ability to produce harmful ozone pollution and ozone’s reduced influence on Earth’s heat balance that affects climate. These effects are not uniform across the world and depend on the location and season of the emission reductions.The results of this research indicate that in order to design effective environmental policies which benefit both air quality and climate, decision-makers need to carefully consider the complex relationships between emissions and atmospheric composition. || ", "hits": 40 }, { "id": 40432, "url": "https://svs.gsfc.nasa.gov/gallery/360and-vrgallery/", "result_type": "Gallery", "release_date": "2021-11-23T00:00:00-05:00", "title": "360 and VR Gallery", "description": "Visualizations in 360 and VR formats", "hits": 161 }, { "id": 13954, "url": "https://svs.gsfc.nasa.gov/13954/", "result_type": "Produced Video", "release_date": "2021-10-06T04:00:00-04:00", "title": "With NASA Data, Researchers Find Standing Waves at Edge of Earth’s Magnetic Bubble", "description": "Earth sails the solar system in a ship of its own making: the magnetosphere, the magnetic field that envelops and protects our planet. The celestial sea we find ourselves in is filled with charged particles flowing from the Sun, known as the solar wind. Just as ocean waves follow the wind, scientists expected that waves traveling along the magnetosphere should ripple in the direction of the solar wind. But a new study reveals some waves do just the opposite.Studying these magnetospheric waves, which transport energy, helps scientists understand the complicated ways that solar activity plays out in the space around Earth. Changing conditions in space driven by the Sun are known as space weather. That weather can impact our technology from communications satellites in orbit to power lines on the ground. “Understanding the boundaries of any system is a key problem,” said Martin Archer, a space physicist at Imperial College London who led the new study, published today in Nature Communications. “That’s how stuff gets in: energy, momentum, matter.” || ", "hits": 185 }, { "id": 13948, "url": "https://svs.gsfc.nasa.gov/13948/", "result_type": "Produced Video", "release_date": "2021-10-05T09:00:00-04:00", "title": "Designing Lucy’s Path to the Trojan Asteroids", "description": "Explore Lucy’s journey to one main-belt asteroid and seven Jupiter Trojans.Complete transcript available.Universal Production Music: “Ocean Simulation” & “The Sequencer Paradox” by Laetitia Frenod; “The Chess Game” by David James Elliott & Martin Gratton; “Tale of Time” by Markus GleissnerWatch this video on the NASA Goddard YouTube channel. || DesigningLucyPreview_print.jpg (1024x576) [277.3 KB] || DesigningLucyPreview.png (3840x2160) [11.6 MB] || DesigningLucyPreview.jpg (3840x2160) [3.2 MB] || DesigningLucyPreview_searchweb.png (320x180) [105.7 KB] || DesigningLucyPreview_thm.png (80x40) [7.2 KB] || 13948_Designing_Lucy_Twitter.webm (1280x720) [50.5 MB] || 13948_Designing_Lucy_Twitter.mp4 (1280x720) [101.0 MB] || 13948_Designing_Lucy_Facebook.mp4 (1920x1080) [559.4 MB] || 13948_Designing_Lucy_Captions.en_US.srt [10.8 KB] || 13948_Designing_Lucy_Captions.en_US.vtt [10.4 KB] || 13948_Designing_Lucy_YouTube.mp4 (3840x2160) [4.4 GB] || 13948_Designing_Lucy_MASTER.mov (3840x2160) [21.6 GB] || ", "hits": 57 }, { "id": 13872, "url": "https://svs.gsfc.nasa.gov/13872/", "result_type": "Produced Video", "release_date": "2021-06-17T10:55:00-04:00", "title": "Mystery of Galaxy's Missing Dark Matter Deepens", "description": "When astronomers using NASA’s Hubble Space Telescope uncovered an oddball galaxy that looks like it doesn’t have much dark matter, some thought the finding was hard to believe and looked for a simpler explanation. Dark matter, after all, is the invisible glue that makes up the bulk of the universe’s contents. All galaxies are dominated by it; in fact, galaxies are thought to form inside immense halos of dark matter. So, finding a galaxy lacking the invisible stuff is an extraordinary claim that challenges conventional wisdom. It would have the potential to upset theories of galaxy formation and evolution.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Galaxy Motion Simulation: Credit: ESO/L. Calçada.Dark Matter Simulation: Credit: Additional Visualizations:Galaxy Motion Simulation: Credit: ESO/L. Calçada.Dark Matter Simulation: Credit: Wu, Hahn, Wechsler, Abel(KIPAC), Visualization: Kaehler (KIPAC)Music Credits: \"Aphelion Horizon\" by Alistair Hetherington [PRS] via Atmosphere Music Ltd. [PRS], and Universal Production Music. || ", "hits": 226 }, { "id": 12772, "url": "https://svs.gsfc.nasa.gov/12772/", "result_type": "Produced Video", "release_date": "2021-05-05T10:25:00-04:00", "title": "2017 Hurricanes and Aerosols Simulation", "description": "Tracking aerosols over land and water from August 1 to November 1, 2017. Hurricanes and tropical storms are obvious from the large amounts of sea salt particles caught up in their swirling winds. The dust blowing off the Sahara, however, gets caught by water droplets and is rained out of the storm system. Smoke from the massive fires in the Pacific Northwest region of North America are blown across the Atlantic to the UK and Europe. This visualization is a result of combining NASA satellite data with sophisticated mathematical models that describe the underlying physical processes.Music: Elapsing Time by Christian Telford [ASCAP], Robert Anthony Navarro [ASCAP]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12772_hurricanes_and_aerosols_1080p_youtube_1080.00001_print.jpg (1024x576) [161.7 KB] || 12772_hurricanes_and_aerosols_1080p_youtube_1080.00001_searchweb.png (180x320) [108.8 KB] || 12772_hurricanes_and_aerosols_1080p_youtube_1080.00001_thm.png (80x40) [7.5 KB] || 12772_hurricanes_and_aerosols_appletv.m4v (1280x720) [78.1 MB] || 12772_hurricanes_and_aerosols_twitter_720.mp4 (1280x720) [34.1 MB] || 12772_hurricanes_and_aerosols.webm (960x540) [65.0 MB] || 12772_hurricanes_and_aerosols_appletv_subtitles.m4v (1280x720) [78.1 MB] || 12772_hurricanes_and_aerosols_1080p_large.mp4 (1920x1080) [163.1 MB] || 12772_hurricanes_and_aerosols_facebook_720.mp4 (1280x720) [184.9 MB] || 12772_hurricanes_and_aerosols_youtube_1080.mp4 (1920x1080) [247.2 MB] || 12772_hurricanes_and_aerosols_youtube_720.mp4 (1280x720) [247.9 MB] || 12772_hurricanes_aerosols_captions.en_US.srt [3.1 KB] || 12772_hurricanes_aerosols_captions.en_US.vtt [3.1 KB] || 12772_hurricanes_and_aerosols_UHD.mp4 (3840x2160) [739.9 MB] || 12772_hurricanes_and_aerosols_1080p-prores.mov (1920x1080) [4.3 GB] || 12772_hurricanes_and_aerosols_UHD_4444.mov (3840x2160) [40.1 GB] || ", "hits": 230 }, { "id": 4850, "url": "https://svs.gsfc.nasa.gov/4850/", "result_type": "Visualization", "release_date": "2021-04-29T00:00:00-04:00", "title": "Internal Ocean Tides", "description": "Data visualization featuring internal tides data from NASA Goddard's Space Flight Center simulation run. The visualization sequence starts with a view of the Americas and the Pacific Ocean and soon after exposes the undersea mountain range along the Hawaiian Ridge. Internal tides data appear on the water surface and the direction of the waves reveal the interplay between the steep bathymetry and the tidal energy generated in the region. Zooming out to a global view, we spot other areas around the globe where large tides are generated, such as Tahiti, Southwest Indian Ocean and Luzon Strait and observe the motions and patterns presented by data. || InternalTides_1024x576_2944.jpg (1024x576) [614.4 KB] || InternalTides_1024x576_2944_searchweb.png (320x180) [134.6 KB] || InternalTides_1024x576_2944_web.png (320x180) [134.6 KB] || InternalTides_1024x576_2944_thm.png (80x40) [21.2 KB] || InternalTides_1280x720p30.mp4 (1280x720) [62.4 MB] || InternalTides_1920x1080_60fps_2944.tif (1920x1080) [7.9 MB] || InternalTides_1280x720p30.webm (1280x720) [15.1 MB] || InternalTides_1920x1080p30.mp4 (1920x1080) [120.7 MB] || InternalTides (3840x2160) [0 Item(s)] || InternalTides_3840x2160_60fps_2944.tif (3840x2160) [31.6 MB] || InternalTides_3840x2160_p30.mp4 (3840x2160) [376.1 MB] || InternalTides_1920x1080p30.mp4.hwshow [192 bytes] || ", "hits": 129 }, { "id": 4879, "url": "https://svs.gsfc.nasa.gov/4879/", "result_type": "Visualization", "release_date": "2021-04-29T00:00:00-04:00", "title": "Internal Tides: Global Views", "description": "Data visualization featuring energetic internal tides on a rotating Earth. The visualization simulates data over a period of a day (24 hours) and showcases the largest internal tides on water bodies around the world. The largest internal tides are generated in regions with steep bathymetry and along mid-ocean ridges, such as in the Hawaiian Ridge, Tahiti, Macquarie Ridge and Luzon Strait. || LargeTides_Composite_1920x1080_0000.png (1024x576) [511.0 KB] || LargeTides_Composite_1920x1080_0000_print.jpg (1024x576) [128.5 KB] || LargeTides_Composite_1920x1080_0000_searchweb.png (320x180) [51.6 KB] || LargeTides_Composite_1920x1080_0000_thm.png (80x40) [4.3 KB] || LargeTides_Composite (1920x1080) [0 Item(s)] || LargeTides_Composite_1280x720p30.mp4 (1280x720) [62.8 MB] || LargeTides_Composite_1920x1080_0000.tif (1920x1080) [11.9 MB] || LargeTides_Composite_1920x1080p30.mp4 (1920x1080) [113.6 MB] || LargeTides_Composite (3840x2160) [0 Item(s)] || LargeTides_Composite_3840x2160_p30.webm (3840x2160) [28.7 MB] || LargeTides_Composite_3840x2160_p30.mp4 (3840x2160) [260.3 MB] || LargeTides_Composite_1920x1080p30.mp4.hwshow [199 bytes] || ", "hits": 58 }, { "id": 13831, "url": "https://svs.gsfc.nasa.gov/13831/", "result_type": "Produced Video", "release_date": "2021-04-15T13:00:00-04:00", "title": "NASA Visualization Probes the Doubly Warped World of Binary Black Holes", "description": "Explore how the extreme gravity of two orbiting supermassive black holes distorts our view. In this visualization, disks of bright, hot, churning gas encircle both black holes, shown in red and blue to better track the light source. The red disk orbits the larger black hole, which weighs 200 million times the mass of our Sun, while its smaller blue companion weighs half as much. Zooming into each black hole reveals multiple, increasingly warped images of its partner. Watch to learn more. Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman and Brian P. PowellMusic: \"Gravitational Field\" from Orbit. Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Supermassive_BlackHole_Binary_Still.jpg (3840x2160) [726.7 KB] || Supermassive_BlackHole_Binary_Still_searchweb.png (320x180) [18.9 KB] || Supermassive_BlackHole_Binary_Still_thm.png (80x40) [2.5 KB] || 13831_BlackHoleBinary_Simulation_1080.webm (1920x1080) [23.8 MB] || 13831_BlackHoleBinary_Simulation_1080.mp4 (1920x1080) [234.7 MB] || 13831_BlackHoleBinary_Simulation_4k.mp4 (3840x2160) [348.3 MB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4 (3840x2160) [936.6 MB] || 13831_BlackHoleBinary_Simulation_ProRes_3840x2160_30.mov (3840x2160) [4.1 GB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4.hwshow [137 bytes] || ", "hits": 273 }, { "id": 10662, "url": "https://svs.gsfc.nasa.gov/10662/", "result_type": "Produced Video", "release_date": "2021-04-14T00:00:00-04:00", "title": "Webb Science Simulations: Planetary Systems and Origins of Life", "description": "Supercomputer simulations of planeratry evolution. Part 1: Turbulent Molecular Cloud Nebula with Protostellar ObjectsThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Drs. Alexei Kritsuk and Michael Norman to visualize a computational data set of a turbulent molecular cloud nebula forming protostellar objects and accretion disks approximately 100 AU in diameter, on the order of the size of our solar system. AVL used its Amore software to interpolate and render the Adaptive Mesh Refinement (AMR) simulation generated from ENZO code for cosmology and astrophysics. The AMR simulation was developed by Drs. Kritsuk and Norman at the Laboratory for Computational Astrophysics. The AMR simulation generated more than 2 terabytes of data and follows star formation processes in a self-gravitating turbulent molecular cloud with a dynamic range of half-a-million in linear scale, resolving both the large-scale filamentary structure of the molecular cloud (~5 parsec) and accretion disks around emerging young protostellar objects (down to 2 AU). Part 2: Protoplanetary Disk and Planet FormationThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Dr. Aaron Boley to visualize the 16,000 year evolution of a young, isolated protoplanetary disk which surrounds a newly-formed protostar. The disk forms spiral arms and a dense clump as a result of gravitational collapse. Dr. Aaron Boley developed this computational model to investigate the response of young disks to mass accretion from their surrounding envelopes, including the direct formation of planets and brown dwarfs through gravitational instability. The main formation mechanism for gas giant planets has been debated within the scientific community for over a decade. One of these theories is 'direct formation through gravitational instability.' If the self-gravity of the gas overwhelms the disk's thermal pressure and the stabilizing effect of differential rotation, the gas closest to the protostar rotates faster than gas farther away. In this scenario, regions of the gaseous disk collapse and form a planet directly. The study, presented in Boley (2009), explores whether mass accretion in the outer regions of disks can lead to such disk fragmentation. The simulations show that clumps can form in situ at large disk radii. If the clumps survive, they can become gas giants on wide orbits, e.g., Fomalhaut b, or even more massive objects called brown dwarfs. Whether a disk forms planets at large radii and, if so, the number of planets that form, depend on how much of the envelope mass is distributed at large distances from the protostar. The results of the simulations suggest that there are two modes of gas giant planet formation. The first mode occurs early in the disk's lifetime, at large radii, and through the disk instability mechanism. After the main accretion phase is over, gas giants can form in the inner disk, over a period of a million years, through the core accretion mechanism, which researchers are addressing in other studies.Thanks to R. H. Durisen, L. Mayer, and G. Lake for comments and discussions relating to this research. This study was supported in part by the University of Zurich, Institute for Theoretical Physics, and by a Swiss Federal Grant. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.AVL at NCSA, University of Illinois. || ", "hits": 218 }, { "id": 13776, "url": "https://svs.gsfc.nasa.gov/13776/", "result_type": "Produced Video", "release_date": "2020-12-15T21:00:00-05:00", "title": "2020 AGU Roundtable: What will we learn from Solar Cycle 25?", "description": "Solar Cycle 25 is here, ushering in the next season of space weather from the Sun. As our star’s activity ramps up—a natural part of its roughly 11-year cycle—scientists are eager to test their predictions. In this AGU 2020 media roundtable, scientists will discuss outstanding questions in solar cycle science, what opportunities this new cycle provides researchers, and how we track progress in predictions. || ", "hits": 91 }, { "id": 13753, "url": "https://svs.gsfc.nasa.gov/13753/", "result_type": "Produced Video", "release_date": "2020-11-17T11:00:00-05:00", "title": "NASA Studies How COVID-19 Shutdowns Affect Emissions", "description": "Music: \"Lab Analysis\" from Universal Production MusicComplete transcript available.Coming soon to our YouTube channel. || Screen_Shot_2020-11-13_at_1.08.17_PM_print.jpg (1024x572) [164.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM.png (3568x1994) [6.4 MB] || Screen_Shot_2020-11-13_at_1.08.17_PM_searchweb.png (320x180) [85.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM_thm.png (80x40) [9.8 KB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.mp4 (1920x1080) [442.5 MB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.webm (1920x1080) [25.9 MB] || COVIDNO2.en_US.srt [4.4 KB] || COVIDNO2.en_US.vtt [4.4 KB] || ", "hits": 72 }, { "id": 4872, "url": "https://svs.gsfc.nasa.gov/4872/", "result_type": "Visualization", "release_date": "2020-11-17T00:00:00-05:00", "title": "Deviation of Modeled Normal Pollution Levels from Measurements Following COVID-19 Lockdown", "description": "Deviation from modeled normal nitrogen dioxide levels after COVID-19 lockdowns || covid_19_7_day_no2.0810_print.jpg (1024x576) [207.7 KB] || covid_19_7_day_no2.0810_searchweb.png (320x180) [83.4 KB] || covid_19_7_day_no2.0810_thm.png (80x40) [6.4 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || covid_19_7_day_no2_1080p30.mp4 (1920x1080) [25.3 MB] || covid_19_7_day_no2_1080p30.webm (1920x1080) [5.0 MB] || covid_19_7_day_no2_1080p30.mp4.hwshow [192 bytes] || ", "hits": 34 }, { "id": 4873, "url": "https://svs.gsfc.nasa.gov/4873/", "result_type": "Visualization", "release_date": "2020-11-10T09:00:00-05:00", "title": "Ocean Surface CO2 Flux with Surface Winds", "description": "Ocean surface winds and CO2 flux. Blue areas are where CO2 is absorbed by the ocean and red areas are where CO2 is outgassed from the oceanComing soon to our YouTube channel. || co2flux_final_001.1000_print.jpg (1024x576) [55.2 KB] || co2flux_final_001.1000_searchweb.png (180x320) [47.6 KB] || co2flux_final_001.1000_thm.png (80x40) [4.3 KB] || co2flux_final_with_cbar_1080p30.webm (1920x1080) [14.3 MB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || captions_silent.30528.en_US.srt [43 bytes] || co2flux_final_with_cbar_1080p30.mp4 (1920x1080) [185.4 MB] || co2flux_final_no_cbar_1080p30.mp4 (1920x1080) [203.6 MB] || co2flux_final_with_cbar2160p30.mp4 (3840x2160) [791.2 MB] || co2flux_final_no_cbar_2160p30.mp4 (3840x2160) [852.2 MB] || co2flux_final_with_cbar_1080p30.mp4.hwshow [234 bytes] || ", "hits": 43 }, { "id": 4821, "url": "https://svs.gsfc.nasa.gov/4821/", "result_type": "Visualization", "release_date": "2020-11-05T00:00:00-05:00", "title": "Barotropic Global Ocean Tides", "description": "This animation with voiceover narration shows the barotropic global ocean tides as a complex system of rotating and trapped waves with a mixture of frequencies.Complete transcript available.This video is also available on our YouTube channel. || tides04_final_HD_voiceoverVer04.01000_print.jpg (1024x576) [142.7 KB] || tides04_final_HD_voiceoverVer04.webm (1920x1080) [16.9 MB] || tides04_final_HD_voiceoverVer04.mp4 (1920x1080) [322.9 MB] || BarotropicGlobalOceanTidesVer04.en_US.srt [2.3 KB] || BarotropicGlobalOceanTidesVer04.en_US.vtt [2.3 KB] || tides04_final_HD_voiceoverVer04.mp4.hwshow || ", "hits": 266 }, { "id": 13759, "url": "https://svs.gsfc.nasa.gov/13759/", "result_type": "B-Roll", "release_date": "2020-11-02T05:30:00-05:00", "title": "James Webb Space Telescope Media Resource Animation Reel", "description": "A media reel of animations regarding the James Webb Space Telescope. || Screen_Shot_2020-10-29_at_2.27.33_PM_print.jpg (1024x574) [62.9 KB] || Screen_Shot_2020-10-29_at_2.27.33_PM.png (3346x1876) [3.3 MB] || Screen_Shot_2020-10-29_at_2.27.33_PM_searchweb.png (320x180) [55.8 KB] || Screen_Shot_2020-10-29_at_2.27.33_PM_thm.png (80x40) [7.4 KB] || JWST_Media_Resource_Animation_Reel_1080p_A2.mov (1920x1080) [4.2 GB] || JWST_Media_Resource_Animation_Reel_1080p_A2.mp4 (1920x1080) [332.5 MB] || JWST_Media_Resource_Animation_Reel_1080p_A2.webm (1920x1080) [32.3 MB] || ", "hits": 97 }, { "id": 20326, "url": "https://svs.gsfc.nasa.gov/20326/", "result_type": "Animation", "release_date": "2020-10-20T00:00:00-04:00", "title": "OSIRIS-REx TAG Event: Real-time Animation", "description": "Real-time animation of the OSIRIS-REx Touch-And-Go (TAG) Event. This animation accurately depicts the spacecraft's journey to the surface of Bennu. || OrexTagRealtimePreview2_print.jpg (1024x576) [94.4 KB] || OrexTagRealtimePreview2.png (1920x1080) [1.5 MB] || OrexTagRealtimePreview2_searchweb.png (320x180) [58.3 KB] || OrexTagRealtimePreview2_thm.png (80x40) [4.2 KB] || Orex_Tag_1080_29.97fps.webm (1920x1080) [515.7 MB] || Slew_to_TAG_Attitude (3840x2160) [0 Item(s)] || Y_Wing (3840x2160) [0 Item(s)] || Checkpoint (3840x2160) [0 Item(s)] || Matchpoint (3840x2160) [0 Item(s)] || Slew_to_Pegasus_Attitude (3840x2160) [0 Item(s)] || Orex_Tag_4K_30fps.webm (3840x2160) [893.7 MB] || Orex_Tag_4K_30fps.mp4 (3840x2160) [5.6 GB] || Orex_Tag_1080_29.97fps.mp4 (1920x1080) [9.1 GB] || Orex_Tag_4K_ProRes_30fps.mov (3840x2160) [275.1 GB] || ", "hits": 99 }, { "id": 4804, "url": "https://svs.gsfc.nasa.gov/4804/", "result_type": "Visualization", "release_date": "2020-10-13T00:00:00-04:00", "title": "Greenland Ice Sheet: Three Futures", "description": "This movie shows the evolution of several regions of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios. Each scenario reflects a potential future climate outcome based on current and future greenhouse gas emmisions. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008. || Greenland_NE_2008_2300_HD_still.2127.jpg (1920x1080) [1.0 MB] || Greenland_NE_2008_2300_HD_still.2127_print.jpg (1024x576) [159.2 KB] || Greenland_NE_2008_2300_HD_still.2127_searchweb.png (320x180) [81.1 KB] || Greenland_NE_2008_2300_HD_still.2127_thm.png (80x40) [7.1 KB] || GreenlandVizV5.webm (1920x1080) [19.7 MB] || Greenland_NE_2008_2300_HD_still.2127.tif (1920x1080) [2.0 MB] || GreenlandVizV5.mp4 (1920x1080) [181.9 MB] || GreenlandViz_FINAL.mov (1920x1080) [5.8 GB] || GreenlandVizV5.mp4.hwshow [378 bytes] || ", "hits": 212 }, { "id": 13685, "url": "https://svs.gsfc.nasa.gov/13685/", "result_type": "Produced Video", "release_date": "2020-08-12T11:00:00-04:00", "title": "5 Things that Changed Weather Forecasting Forever", "description": "Complete transcript available.Watch this video on the NASA Goddard YouTube Channel || Weather_forecasting_history_FINAL_smallest.00180_print.jpg (1024x576) [114.4 KB] || Weather_forecasting_history_FINAL_smallest.00180_searchweb.png (320x180) [43.1 KB] || Weather_forecasting_history_FINAL_smallest.00180_web.png (320x180) [43.1 KB] || Weather_forecasting_history_FINAL_smallest.00180_thm.png (80x40) [3.0 KB] || Weather_forecasting_history_FINAL_smallest.mp4 (1920x1080) [653.6 MB] || Weather_forecasting_history_FINAL_smaller.mp4 (1920x1080) [1.1 GB] || Weather_forecasting_history_FINAL_smallest.webm (1920x1080) [123.4 MB] || Weather_forecasting_history_FINAL.mp4 (3840x2160) [1.2 GB] || Weather_forecasting_final.en_US.vtt [22.5 KB] || Weather_forecasting_final_corrected.en_US.srt [21.7 KB] || Weather_forecasting_final_corrected.en_US.vtt [21.6 KB] || ", "hits": 35 }, { "id": 13645, "url": "https://svs.gsfc.nasa.gov/13645/", "result_type": "Produced Video", "release_date": "2020-06-22T10:00:00-04:00", "title": "NASA Scientist Simulates a Kaleidoscope of Sunsets on Other Worlds", "description": "A simulation of sunsets on other worlds by NASA Goddard scientist, Geronimo Villanueva.Music credits: \"Immense and Beautiful\" by Victoria Beits from Universal Production Music || 13645_THUMB.jpg (3840x2160) [506.0 KB] || 13645_Planet_Sunset_MASTER.03906_searchweb.png (320x180) [23.3 KB] || 13645_Planet_Sunset_MASTER.03906_thm.png (80x40) [3.1 KB] || 13645_Planet_Sunset_MASTER.webm (960x540) [10.7 MB] || 13645_Planet_Sunset_MASTER_facebook_720.mp4 (1280x720) [108.3 MB] || 13645_Planet_Sunset_MASTER_twitter_720.mp4 (1280x720) [30.8 MB] || 13645_Planet_Sunset_MASTER.mp4 (3840x2160) [133.5 MB] || 13645_PlanetSunset.en_US.srt [58 bytes] || 13645_PlanetSunset.en_US.vtt [66 bytes] || ", "hits": 42 }, { "id": 40418, "url": "https://svs.gsfc.nasa.gov/gallery/themis/", "result_type": "Gallery", "release_date": "2020-06-08T00:00:00-04:00", "title": "THEMIS – Time History of Events and Macroscale Interactions during Substorms", "description": "The Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission was launched on Feb. 17, 2007, to measure the magnetic and plasma environment around Earth to better understand a space weather phenomenon known as a substorm, which initiates auroras. With THEMIS, we now have a much better understanding of substorms, which can help us predict and mitigate space weather effects near Earth — including helping to ensure safety for astronauts and spacecraft operating around Earth.\n\nIn 2010, after THEMIS successfully completed its prime mission, two of the five spacecraft were sent on a new mission: into orbit around the Moon to begin the first systematic measurements of conditions in the magnetotail — the distant tail of Earth’s magnetic environment. The new mission is known as the Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon’s Interaction with the Sun, or THEMIS-ARTEMIS.\n\nLearn more: https://science.nasa.gov/mission/themis/", "hits": 108 }, { "id": 4825, "url": "https://svs.gsfc.nasa.gov/4825/", "result_type": "Visualization", "release_date": "2020-05-25T00:00:00-04:00", "title": "MAVEN – Mars and Solar Wind Simulation", "description": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded. || maven_cme44.03600_print.jpg (1024x512) [253.9 KB] || maven_cme44.03600_searchweb.png (320x180) [92.7 KB] || maven_cme44.03600_thm.png (80x40) [5.2 KB] || 1920x1080_16x9_30p (2048x1024) [0 Item(s)] || maven_cme44_1024p30.webm (2048x1024) [5.9 MB] || maven_cme44_1024p30.mp4 (2048x1024) [195.1 MB] || maven_cme44_1024p30.mp4.hwshow [58 bytes] || ", "hits": 52 }, { "id": 13580, "url": "https://svs.gsfc.nasa.gov/13580/", "result_type": "Produced Video", "release_date": "2020-04-14T10:30:00-04:00", "title": "NASA Models the Complex Chemistry of Earth's Atmosphere", "description": "Music: \"Interconnecting Threads\" by Axel Tenner [GEMA]; \"Night Drift\" by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS], from Universal Production MusicWatch this video on the NASA Goddard YouTube channel. Complete transcript available. || ChemicalSpecies_Still_print.jpg (1024x576) [313.1 KB] || ChemicalSpecies_Still.jpg (3840x2160) [2.0 MB] || ChemicalSpecies_Still_searchweb.png (320x180) [104.5 KB] || ChemicalSpecies_Still_web.png (320x180) [104.5 KB] || ChemicalSpecies_Still_thm.png (80x40) [7.8 KB] || 13580_ChemSpecies_Final.mov (1920x1080) [1.8 GB] || 13580_ChemSpecies_Final_lowres.mp4 (1280x720) [82.5 MB] || 13580_ChemSpecies_Final.mp4 (1920x1080) [467.4 MB] || 13580_ChemSpecies_Final.webm (1920x1080) [2.7 MB] || ChemicalSpecies.en_US.srt [4.2 KB] || ChemicalSpecies.en_US.vtt [4.2 KB] || ", "hits": 40 }, { "id": 13559, "url": "https://svs.gsfc.nasa.gov/13559/", "result_type": "Produced Video", "release_date": "2020-03-23T10:00:00-04:00", "title": "NASA Models Methane Sources and Movement Around the Globe", "description": "Complete transcript available.Music: \"Reported Missing\" by Andrew Michael Britton [PRS] and David Stephen Goldsmith [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html. || Methane_Still.jpg (1920x1080) [408.5 KB] || Methane_Still_print.jpg (1024x576) [181.8 KB] || Methane_Still_searchweb.png (180x320) [71.4 KB] || Methane_Still_web.png (320x180) [71.4 KB] || Methane_Still_thm.png (80x40) [6.4 KB] || 13559_Methane_Final.webm (960x540) [62.2 MB] || TWITTER_720_13559_Methane_Final_twitter_720.mp4 (1280x720) [28.5 MB] || 13559_Methane_Final_lowres.mp4 (1280x720) [43.6 MB] || 13559_Methane_Final.mp4 (1920x1080) [272.5 MB] || Mathen_captions.en_US.srt [3.2 KB] || Mathen_captions.en_US.vtt [3.3 KB] || 13559_Methane_Final.mov (1920x1080) [3.4 GB] || ", "hits": 74 }, { "id": 13567, "url": "https://svs.gsfc.nasa.gov/13567/", "result_type": "Produced Video", "release_date": "2020-03-06T09:00:00-05:00", "title": "How Does NASA Model Atmospheric Patterns?", "description": "Music: Favor by Victor Maitre [SACEM]Complete transcript available. || GMAOThumb.jpg (1920x1080) [251.3 KB] || GMAOThumb_print.jpg (1024x576) [131.2 KB] || GMAOThumb_searchweb.png (180x320) [82.2 KB] || GMAOThumb_web.png (320x180) [82.2 KB] || GMAOThumb_thm.png (80x40) [6.4 KB] || 13567_GMAO_Atmospheric_Model.mp4 (1920x1080) [88.5 MB] || 13567_GMAO_Atmospheric_Model.webm (1920x1080) [10.2 MB] || 13567_GMAO_Atmospheric_Model.mov (1920x1080) [673.0 MB] || captions.en_US.srt [1.3 KB] || captions.en_US.vtt [1.4 KB] || ", "hits": 28 }, { "id": 13556, "url": "https://svs.gsfc.nasa.gov/13556/", "result_type": "Produced Video", "release_date": "2020-02-14T03:00:00-05:00", "title": "Astrophysics Valentines", "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ", "hits": 80 }, { "id": 13197, "url": "https://svs.gsfc.nasa.gov/13197/", "result_type": "Produced Video", "release_date": "2020-02-11T09:00:00-05:00", "title": "Gravitational Wave Simulations of Merging Black Holes: 1080 and 8k Resolutions", "description": "This visualization shows gravitational waves emitted by two black holes (black spheres) of nearly equal mass as they spiral together and merge. Yellow structures near the black holes illustrate the strong curvature of space-time in the region. Orange ripples represent distortions of space-time caused by the rapidly orbiting masses. These distortions spread out and weaken, ultimately becoming gravitational waves (purple). The merger timescale depends on the masses of the black holes. For a system containing black holes with about 30 times the sun’s mass, similar to the one detected by LIGO in 2015, the orbital period at the start of the movie is just 65 milliseconds, with the black holes moving at about 15 percent the speed of light. Space-time distortions radiate away orbital energy and cause the binary to contract quickly. As the two black holes near each other, they merge into a single black hole that settles into its \"ringdown\" phase, where the final gravitational waves are emitted. For the 2015 LIGO detection, these events played out in little more than a quarter of a second. This simulation was performed on the Pleiades supercomputer at NASA's Ames Research Center. Fixed view.Credit: NASA/Bernard J. Kelly (Goddard and Univ. of Maryland Baltimore County), Chris Henze (Ames) and Tim Sandstrom (CSC Government Solutions LLC)Watch this video on the NASAgovVideo YouTube channel. || Merger_Fixed_Still.png (1920x1080) [1.2 MB] || Merger_Fixed_Still_print.jpg (1024x576) [59.6 KB] || BH_merger_fixed_camera_close_H264_YouTube_720p.mp4 (1280x720) [65.5 MB] || BH_merger_fixed_camera_close_H264_YouTube_1080p.mp4 (1920x1080) [65.2 MB] || BH_merger_fixed_camera_close_H264_YouTube_720p.webm (1280x720) [3.9 MB] || BH_merger_fixed_camera_close_ProRes_1920x1080.mov (1920x1080) [1.1 GB] || ", "hits": 366 }, { "id": 13528, "url": "https://svs.gsfc.nasa.gov/13528/", "result_type": "Produced Video", "release_date": "2020-01-27T13:50:00-05:00", "title": "Solar Orbiter Media Telecon", "description": "NASA and ESA scientists will present Solar Orbiter, the ESA/NASA collaboration soon to start its journey to the Sun, during a media teleconference on Monday, Jan. 27, 2020 at 2 p.m. EST. Mission experts will discuss Solar Obiter’s uniquely tilted orbit, how the mission will capture the first images of the Sun’s North and South poles, and its ability to tackle major solar mysteries with its comprehensive suite of ten different instruments. The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:•Nicola Fox, director of the Heliophysics Division in the Science Mission Directorate at NASA Headquarters in Washington•Chris St. Cyr, former NASA project scientist for the mission at NASA Goddard•Yannis Zouganelis, ESA deputy project scientist for Solar Orbiter at the European Space Astronomy Centre in Madrid, Spain•Anne Pacros, ESA Mission and Payload Manager || ", "hits": 32 }, { "id": 40409, "url": "https://svs.gsfc.nasa.gov/gallery/fermi-stills/", "result_type": "Gallery", "release_date": "2020-01-22T00:00:00-05:00", "title": "Fermi Stills", "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.", "hits": 271 }, { "id": 13496, "url": "https://svs.gsfc.nasa.gov/13496/", "result_type": "Produced Video", "release_date": "2020-01-06T19:15:00-05:00", "title": "TESS Mission’s First Earth-size World in Star’s Habitable-zone", "description": "Take a tour through TOI 700, a planetary system 100 light-years away in the constellation Dorado. One of the system’s residents is TOI 700 d, the first Earth-size habitable-zone planet discovered by NASA’s Transiting Exoplanet Survey Satellite. Credit: NASA’s Goddard Space Flight Center.Music: \"Family Tree\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TOI_700d.jpg (1920x1080) [397.4 KB] || TOI_700d_print.jpg (1024x576) [128.3 KB] || TOI_700d_searchweb.png (320x180) [65.8 KB] || TOI_700d_thm.png (80x40) [5.5 KB] || 13496_TOI700_Earth-size_1080.webm (1920x1080) [25.7 MB] || 13496_TOI700_Earth-size_1080.mp4 (1920x1080) [229.2 MB] || 13496_TOI700_Earth-size_1080_Best.mp4 (1920x1080) [394.2 MB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.srt [4.4 KB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.vtt [4.4 KB] || 13496_TOI700_Earth-size_ProRes_1920x1080.mov (1920x1080) [2.7 GB] || ", "hits": 464 }, { "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": 66 }, { "id": 13240, "url": "https://svs.gsfc.nasa.gov/13240/", "result_type": "Produced Video", "release_date": "2019-12-12T11:00:00-05:00", "title": "NASA’s NICER Sizes Up a Pulsar, Reveals First-ever Surface Map", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) has expanded our understanding of pulsars, the dense, spinning corpses of exploded stars. Pulsar J0030+0451 (J0030 for short), located 1,100 light-years away in the constellation Pisces, now has the most precise and reliable measurements of both a pulsar’s mass and size to date. The shapes and locations of its hot spots challenge textbook depictions of these incredible objects. Music: \"Uncertain Ahead\" and \"Flowing Cityscape\" (underscore). Both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Two_NS_Model_Still.jpg (1920x1080) [308.5 KB] || Two_NS_Model_Still_print.jpg (1024x576) [140.4 KB] || Two_NS_Model_Still_searchweb.png (320x180) [87.0 KB] || Two_NS_Model_Still_thm.png (80x40) [8.0 KB] || 13240_NICER_J0030_MassRadius_1080.webm (1920x1080) [33.5 MB] || 13240_NICER_J0030_MassRadius_1080.mp4 (1920x1080) [301.1 MB] || 13240_NICER_J0030_MassRadius_Best_1080.mp4 (1920x1080) [804.5 MB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.srt [5.9 KB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.vtt [5.9 KB] || 13240_NICER_J0030_MassRadius_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || ", "hits": 163 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ", "hits": 101 }, { "id": 4754, "url": "https://svs.gsfc.nasa.gov/4754/", "result_type": "Visualization", "release_date": "2019-12-09T00:00:00-05:00", "title": "The Complex Chemistry of Surface Ozone Depicted in a New GEOS Simulation", "description": "96 chemical species are shown from a GEOS atmospheric simulation || gmao_chem_3x3_pass02_09.05630_no_overlay_print.jpg (1024x576) [126.9 KB] || gmao_chem_3x3_pass02_09.05630_no_overlay.png (5760x3240) [2.5 MB] || gmao_chem_3x3_pass02_09.05630_no_overlay_searchweb.png (320x180) [82.3 KB] || gmao_chem_3x3_pass02_09.05630_no_overlay_thm.png (80x40) [6.8 KB] || 1920x1080_16x9_p30 (1920x1080) [0 Item(s)] || gmao_chem_HD_1080p30.webm (1920x1080) [36.0 MB] || gmao_chem_HD_1080p30.mp4 (1920x1080) [267.3 MB] || 9600x3240_16x9_30p (9600x3240) [0 Item(s)] || 3840x2160_16x9_p30 (3840x2160) [0 Item(s)] || gmao_chem_5x3_preview.mp4 (3200x1080) [429.0 MB] || gmao_chem_4k_2160p30.mp4 (3840x2160) [762.1 MB] || gmao_chem_HD_1080p30.mp4.hwshow [212 bytes] || ", "hits": 161 }, { "id": 4764, "url": "https://svs.gsfc.nasa.gov/4764/", "result_type": "Visualization", "release_date": "2019-11-07T00:00:00-05:00", "title": "Simulation of Surface Ozone", "description": "Global surface ozone from a GEOS model run || ozone_only_4k.00000_print.jpg (1024x576) [65.8 KB] || ozone_only_4k.00000_searchweb.png (320x180) [58.9 KB] || ozone_only_4k.00000_thm.png (80x40) [5.1 KB] || ozone_only_1080p30.mp4 (1920x1080) [24.5 MB] || ozone_only_1080p30.webm (1920x1080) [7.2 MB] || ozone_only_2160p30.mp4 (3840x2160) [70.8 MB] || ozone_only (3840x2160) [0 Item(s)] || ozone_only (5760x3240) [0 Item(s)] || ozone_only_1080p30.mp4.hwshow [208 bytes] || ", "hits": 75 }, { "id": 40388, "url": "https://svs.gsfc.nasa.gov/gallery/nasaearth-science/", "result_type": "Gallery", "release_date": "2019-09-13T10:53:37-04:00", "title": "NASA Earth Science", "description": "NASA’s Earth Science Division (ESD) missions help us to understand our planet’s interconnected systems, from a global scale down to minute processes. Working in concert with a satellite network of international partners, ESD can measure precipitation around the world, and it can employ its own constellation of small satellites to look into the eye of a hurricane. ESD technology can track dust storms across continents and mosquito habitats across cities.\n\nFor more information:\nhttps://science.nasa.gov/earth-science", "hits": 192 }, { "id": 4743, "url": "https://svs.gsfc.nasa.gov/4743/", "result_type": "Visualization", "release_date": "2019-07-30T00:00:00-04:00", "title": "Greenland's Jakobshavn Region: Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Jakobshavn region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model . All data sets for this study are publicly available at the NSF Arctic Data Center || ", "hits": 20 } ] }