{ "count": 2771, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Animation%22", "previous": null, "results": [ { "id": 5629, "url": "https://svs.gsfc.nasa.gov/5629/", "result_type": "Visualization", "release_date": "2026-03-26T13:00:00-04:00", "title": "Arctic Sea Ice Maximum 2026", "description": "Arctic sea ice maximum extent 2026, still image || arctic_sea_ice_max_2026_print_print.jpg (1024x576) [157.5 KB] || arctic_sea_ice_max_2026_print.png (3840x2160) [6.2 MB] || arctic_sea_ice_max_2026_print_searchweb.png (320x180) [79.9 KB] || arctic_sea_ice_max_2026_print_web.png (320x180) [79.9 KB] || arctic_sea_ice_max_2026_print_thm.png (80x40) [6.2 KB] || ", "hits": 530 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 712 }, { "id": 14992, "url": "https://svs.gsfc.nasa.gov/14992/", "result_type": "Animation", "release_date": "2026-03-24T15:00:00-04:00", "title": "Lunar Near and Far Side Phases", "description": "These animations illustrate opposite lunar phases on the near and far sides of the Moon.", "hits": 5693 }, { "id": 40550, "url": "https://svs.gsfc.nasa.gov/gallery/voyager/", "result_type": "Gallery", "release_date": "2026-03-04T00:00:00-05:00", "title": "Voyager", "description": "Launched in 1977, the twin Voyager spacecraft are NASA’s longest operating and most distant spacecraft. Hurtling through space at over 38,000 miles per hour, Voyager 1 and 2 were the first confirmed human-made objects to cross the threshold into interstellar space. After completing an in-depth reconnaissance of the outer planets, the Voyager spacecraft departed the heliosphere, the protective bubble of particles and magnetic fields generated by the Sun, in two separate directions and are now exploring the edges of interstellar space. \n\nLearn more: https://science.nasa.gov/mission/voyager/", "hits": 630 }, { "id": 40549, "url": "https://svs.gsfc.nasa.gov/gallery/interstellar-boundary-explorer-ibex/", "result_type": "Gallery", "release_date": "2026-03-02T00:00:00-05:00", "title": "IBEX – Interstellar Boundary Explorer", "description": "The Interstellar Boundary Explorer (IBEX) is a NASA spacecraft studying how our heliosphere — the protective bubble surrounding the Sun and planets that is inflated by a constant stream of solar particles — interacts with interstellar space. IBEX created the first maps showing the interactions at that border, and how they change over time due to variations in the Sun’s activity. IBEX studies the heliosphere’s boundaries by measuring a type of uncharged particle called energetic neutral atoms.\n\nIBEX launched on Oct. 19, 2008, from the Ronald Reagan Ballistic Missile Defense Test Site, in the Republic of the Marshall Islands. \n\nLearn more: https://science.nasa.gov/mission/ibex/", "hits": 214 }, { "id": 31366, "url": "https://svs.gsfc.nasa.gov/31366/", "result_type": "Hyperwall Visual", "release_date": "2026-02-27T12:00:00-05:00", "title": "NASA Science Drives Exploration", "description": "Animations based on the 2026 NASA Science Calendar graphics", "hits": 360 }, { "id": 31367, "url": "https://svs.gsfc.nasa.gov/31367/", "result_type": "Hyperwall Visual", "release_date": "2026-02-27T12:00:00-05:00", "title": "NISAR Satellite and Science", "description": "Animation showing NISAR satellite insruments and scientific research.", "hits": 222 }, { "id": 14970, "url": "https://svs.gsfc.nasa.gov/14970/", "result_type": "Animation", "release_date": "2026-02-20T12:00:00-05:00", "title": "Roman Space Telescope Assembly Animation", "description": "This animation shows key systems assembling to form NASA's Nancy Grace Roman Space Telescope. It starts with the spacecraft bus and then adds the instrument carrier. Then the Coronagraph Instrument joins, followed by the mirror assembly and the Wide Field Instrument, completing the main half of the observatory. The outer portion, which contains the outer barrel assembly, solar array Sun shield, and deployable aperture cover, slides over the exposed mirror to complete the full observatory. This animation includes a version with a transparent alpha channel. || Roman_Assembly_Still.jpg (3840x2160) [377.3 KB] || Roman_Assembly_Still_searchweb.png (320x180) [18.8 KB] || Roman_Assembly_Still_thm.png (80x40) [2.3 KB] || Roman_Asssembly_1080.mp4 (1920x1080) [61.6 MB] || Roman_Asssembly_4k.mp4 (3840x2160) [308.1 MB] || Roman_Asssembly_ProRes_3840x2160_60.mov (3840x2160) [3.7 GB] || Roman_Asssembly_ProRes4444Alpha_3840x2160_60.mov (3840x2160) [7.1 GB] || ", "hits": 171 }, { "id": 14967, "url": "https://svs.gsfc.nasa.gov/14967/", "result_type": "Animation", "release_date": "2026-02-20T10:00:00-05:00", "title": "NASA's Roman Space Telescope Parts and Assembly", "description": "The Roman observatory is slated to launch no later than May 2027, with the team aiming for as early as fall 2026. The mission will revolutionize our understanding of the universe with its deep, crisp, sweeping views of space.More than a thousand technicians and engineers assembled Roman from millions of individual components. Many parts were built and tested simultaneously to save time. Now that the observatory is assembled, it will undergo a spate of testing prior to shipping to NASA's Kennedy Space Center in Florida in summer 2026.Learn more at Building Roman. Music credit: “Unseen,” by David Husband [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel. || YTframe_RomanAssembly.jpg (1280x720) [151.7 KB] || YTframe_RomanAssembly_searchweb.png (320x180) [55.4 KB] || YTframe_RomanAssembly_thm.png (80x40) [8.3 KB] || 14967_Roman_Assembly_1080.mp4 (1920x1080) [138.9 MB] || 14967RomanAssemblyCaptions.en_US.srt [1.9 KB] || 14967RomanAssemblyCaptions.en_US.vtt [1.8 KB] || 14967_Roman_Assembly_4k_Good.mp4 (3840x2160) [290.7 MB] || 14967_Roman_Assembly_4k_Best.mp4 (3840x2160) [368.4 MB] || 14967_Roman_Assembly_4k_YT.mp4 (3840x2160) [722.6 MB] || 14967_Roman_Assembly_ProRes_3840x2160_30.mov (3840x2160) [6.1 GB] || ", "hits": 416 }, { "id": 14971, "url": "https://svs.gsfc.nasa.gov/14971/", "result_type": "Animation", "release_date": "2026-02-20T09:00:00-05:00", "title": "2026 Roman Space Telescope 360 Animation", "description": "A 360-degree spin animation of NASA's Nancy Grace Roman Space Telescope. This version showcases the final design and configuration. It includes a version with a transparent background. || Roman2025_360Spin_Still.jpg (3840x2160) [487.8 KB] || Roman2025_360Spin_Still_searchweb.png (320x180) [34.3 KB] || Roman2025_360Spin_Still_thm.png (80x40) [3.8 KB] || Roman2025_360Spin_1080.mp4 (1920x1080) [47.5 MB] || Roman2025_360Spin_4k.mp4 (3840x2160) [236.7 MB] || Roman2025_360Spin_ProRes4444Alpha_3840x2160_30.mov (3840x2160) [4.5 GB] || ", "hits": 445 }, { "id": 14966, "url": "https://svs.gsfc.nasa.gov/14966/", "result_type": "Produced Video", "release_date": "2026-02-14T00:00:00-05:00", "title": "SPHEREx Spacecraft and Observing Animations", "description": "SPHEREx is a small, highly-capable astronomy satellite mission that will map out the entire sky in 102 colors of infrared light from its vantage point in a low-Earth orbit. The spacecraft bus is powered by Sun-facing, rectangular solar panels.The white, conical Sun shield keeps the inner telescope components at a cool temperature that enables the detectors to operate with high sensitivity. The Sun shields are faded out at the end of the sequence to provide an unobstructed view of the telescope components.Credit: NASA/JPL-CaltechWatch this video on the JPLraw YouTube channel.JPL Page || SPHEREx_SurveyAnimationShot1_Stlll.jpg (3840x2160) [658.9 KB] || SPHEREx_SurveyAnimationShot1_Stlll_searchweb.png (320x180) [63.1 KB] || SPHEREx_SurveyAnimationShot1_Stlll_thm.png (80x40) [4.5 KB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422.mov (1920x1080) [703.6 MB] || SPHEREx_Shot1_Caption.en_US.srt [49 bytes] || SPHEREx_Shot1_Caption.en_US.vtt [59 bytes] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_4K.mp4 (3840x2160) [154.7 MB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422_4K.mov (3840x2160) [2.0 GB] || ", "hits": 234 }, { "id": 5613, "url": "https://svs.gsfc.nasa.gov/5613/", "result_type": "Visualization", "release_date": "2026-02-04T00:00:00-05:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2025", "description": "The change in the distribution of land temperature anomalies over the years 1951 to 2025.", "hits": 555 }, { "id": 5611, "url": "https://svs.gsfc.nasa.gov/5611/", "result_type": "Visualization", "release_date": "2026-01-30T09:00:00-05:00", "title": "Global Mean Sea Level 1993-2025", "description": "This animation shows the rise in global mean sea level from 1993 to 2023 based on data from a series of five international satellites.", "hits": 489 }, { "id": 14959, "url": "https://svs.gsfc.nasa.gov/14959/", "result_type": "Interactive", "release_date": "2026-01-29T00:00:00-05:00", "title": "Moon 3D Models for Web, AR, and Animation", "description": "These models of the Moon are made with imagery and topographic data from NASA’s Lunar Reconnaissance Orbiter, which has been studying and mapping the lunar surface since 2009. The models are intended for use in web interactives, augmented reality (AR) applications, and animations. ||", "hits": 6409 }, { "id": 40542, "url": "https://svs.gsfc.nasa.gov/gallery/dark-energy/", "result_type": "Gallery", "release_date": "2026-01-28T00:00:00-05:00", "title": "Dark Energy", "description": "Some 13.8 billion years ago, the universe began with a rapid expansion we call the big bang. After this initial expansion, which lasted a fraction of a second, gravity started to slow the universe down. But the cosmos wouldn’t stay this way. Nine billion years after the universe began, its expansion started to speed up, driven by an unknown force that scientists have named dark energy.\n\nBut what exactly is dark energy?\n\nThe short answer is: We don't know. But we do know that it exists, it’s making the universe expand at an accelerating rate, and approximately 68.3 to 70% of the universe is dark energy.", "hits": 926 }, { "id": 5604, "url": "https://svs.gsfc.nasa.gov/5604/", "result_type": "Visualization", "release_date": "2026-01-27T18:00:00-05:00", "title": "March 3, 2026 Total Lunar Eclipse: Shadow View", "description": "On March 3, 2026, the Moon enters the Earth's shadow, creating a total lunar eclipse. This set of visualizations shows the view down the barrel of the Earth's shadow as the Moon moves through it, along with times at various stages.", "hits": 978 }, { "id": 5606, "url": "https://svs.gsfc.nasa.gov/5606/", "result_type": "Visualization", "release_date": "2026-01-27T18:00:00-05:00", "title": "March 3, 2026 Total Lunar Eclipse: Visibility Map", "description": "On March 3, 2026, the Moon enters the Earth's shadow, creating a total lunar eclipse. The media on this page show the region of the Earth where this event is visible.", "hits": 1341 }, { "id": 20412, "url": "https://svs.gsfc.nasa.gov/20412/", "result_type": "Animation", "release_date": "2026-01-21T11:00:00-05:00", "title": "Artemis II Flight Path Animations", "description": "Animated Flight Path of Artemis II and comparison with NASA's Lunar Reconnaissance Orbiter and the Apollo mission orbits.", "hits": 77303 }, { "id": 14942, "url": "https://svs.gsfc.nasa.gov/14942/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Roman and Webb Comparison Graphics from Far and Wide", "description": "This page contains individual animation clips from the Far and Wide series. These clips all focus on the relationship between the Nancy Grace Roman and James Webb space telescopes: how they are different and how they will work together. These animations may be useful in presentations and other video products. || ", "hits": 198 }, { "id": 14943, "url": "https://svs.gsfc.nasa.gov/14943/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Additional Graphics", "description": "This page houses animation clips from the Far and Wide video series, which may be useful in presentations or other video products. || ", "hits": 147 }, { "id": 14946, "url": "https://svs.gsfc.nasa.gov/14946/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Viewing an Exoplanet Transmission Spectrum", "description": "When planets orbiting distant stars are aligned just right, a host star's light can pass through its planet's atmosphere before reaching our telescopes. This alters the light, and by analyzing its spectrum, astronomers can find out what the planet’s atmosphere is made of. This animation is a quick visual representation of that process. || ", "hits": 363 }, { "id": 14947, "url": "https://svs.gsfc.nasa.gov/14947/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Webb Spectrum and Image Animations", "description": "These are animated versions of James Webb Space Telescope imagery and spectra. The spectra visualizations were created by the Space Telescope Science Institute and then animated at NASA's Goddard Space Flight Center. || ", "hits": 459 }, { "id": 14950, "url": "https://svs.gsfc.nasa.gov/14950/", "result_type": "Animation", "release_date": "2026-01-20T11:00:00-05:00", "title": "Flying Through Galaxies", "description": "This artist's concept animation imagines flying through the vast web of galaxies that fill the visible universe. || 14950_Galaxies_FlyThrough_Still.jpg (3840x2160) [814.5 KB] || 14950_Galaxies_FlyThrough_Still_searchweb.png (320x180) [75.2 KB] || 14950_Galaxies_FlyThrough_Still_thm.png (80x40) [5.8 KB] || 14950_Galaxies_FlyThrough_1080.mp4 (1920x1080) [49.2 MB] || 14950_Galaxies_FlyThrough_4k.mp4 (3840x2160) [141.8 MB] || 14950_Galaxies_FlyThrough_4k60_75mbps.mp4 (3840x2160) [355.6 MB] || 14950_Galaxies_FlyThrough_ProRes_3840x2160_60.mov (3840x2160) [5.3 GB] || ", "hits": 229 }, { "id": 20411, "url": "https://svs.gsfc.nasa.gov/20411/", "result_type": "Animation", "release_date": "2026-01-14T10:00:00-05:00", "title": "A Pathway to Protocells on Titan – Animations", "description": "These animations illustrate how simple protocells could form in the lakes of Titan, Saturn’s largest moon. When rain falls from Titan’s methane clouds into its hydrocarbon lakes, it can transport organic molecules like acrylonitrile that are attracted to both water and oil. Such amphiphile molecules are likely to collect in a thin film on the surface of Titan’s lakes. As large raindrops pelt the lakes, they could stir up this floating “pond scum” to form spherical droplets of methane coated in a bilayer of amphiphiles – structures called vesicles that resemble cell membranes on Earth.Although such vesicles have yet to be detected on Titan, a 2025 study by Christian Mayer and NASA scientist Conor Nixon lays out the process for their formation and evolution, and it proposes a mechanism for their discovery by a future mission to Titan. The paper also proposes that different mixtures of amphiphiles could stabilize vesicles and lead to the evolution of simple protocells on Titan. || ", "hits": 335 }, { "id": 3335, "url": "https://svs.gsfc.nasa.gov/3335/", "result_type": "Visualization", "release_date": "2025-12-31T00:00:00-05:00", "title": "Meteor Crater Topography", "description": "The Earth and Mars are two planets which evolved very differently. By studying locations on Earth whose environment might be similar with that of Mars, scientists are able to theorize about 'the red planet' as well. Meteor Crater is one such study site in the Colorado Plateau, 73 km east of Flagstaff, Arizona. After the meteorite hit the surface of the Arizona desert thousands of years ago, some of the rocks were pushed up along the edge to form a rim around the crater. High resolution (2 m) digital elevation of the site, collected by aerial overflights of the region, is shown here overlain with a natural color IKONOS image. || ", "hits": 57 }, { "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": 2422 }, { "id": 14935, "url": "https://svs.gsfc.nasa.gov/14935/", "result_type": "Infographic", "release_date": "2025-12-18T13:00:00-05:00", "title": "Milky Way Anatomy", "description": "This infographic with artist’s concept views of our Milky Way galaxy highlights its main components: the disk, bulge, stellar halo, and dark matter halo. Scientists have a pretty good idea of the Milky Way’s overall structure, but since we’re nestled inside it, fine details are hard to see. Astronomers have used observations from different telescopes to piece together our galaxy's anatomy, and future observatories like NASA's Nancy Grace Roman Space Telescope will make the picture even clearer. || Milky_Way_Anatomy_Infographic_Simple_Final_print.jpg (1024x512) [118.4 KB] || Milky_Way_Anatomy_Infographic_Simple_Final.jpg (4320x2160) [1.2 MB] || Milky_Way_Anatomy_Infographic_Simple_Final.png (4320x2160) [6.5 MB] || Milky_Way_Anatomy_Infographic_Simple_Final_searchweb.png (320x180) [68.0 KB] || Milky_Way_Anatomy_Infographic_Simple_Final_thm.png (80x40) [5.1 KB] || ", "hits": 2461 }, { "id": 14936, "url": "https://svs.gsfc.nasa.gov/14936/", "result_type": "Animation", "release_date": "2025-12-12T10:00:00-05:00", "title": "Chillin with Paige", "description": "Land Ice with ICESat-2 Deputy Project Scientist Denis FeliksonMusic: \"Think Things Out,\" Universal Production Music || chillin_landice_thumb.png (1182x2124) [2.2 MB] || chillin_landice_thumb_print.jpg (1024x1840) [231.6 KB] || chillin_landice_thumb_searchweb.png (320x180) [81.2 KB] || chillin_landice_thumb_thm.png (80x40) [9.6 KB] || Chillin_GlacierIce_NO-SIM-v2.mp4 (1080x1920) [81.4 MB] || Chillin_GlacierIce_SIM-OPEN-v2.mp4 (1080x1920) [93.6 MB] || ", "hits": 27 }, { "id": 5587, "url": "https://svs.gsfc.nasa.gov/5587/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 7705 }, { "id": 5588, "url": "https://svs.gsfc.nasa.gov/5588/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026 South Up", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 775 }, { "id": 14916, "url": "https://svs.gsfc.nasa.gov/14916/", "result_type": "Produced Video", "release_date": "2025-12-08T09:30:00-05:00", "title": "Black Hole Eats Star: The Longest GRB Ever Seen", "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ", "hits": 603 }, { "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": 379 }, { "id": 14906, "url": "https://svs.gsfc.nasa.gov/14906/", "result_type": "Produced Video", "release_date": "2025-09-30T15:00:00-04:00", "title": "Evolution of a Sun-Like Star", "description": "As a star ages, its spin and the number and sizes of its spots decreases as shown in this animation of a Sun-like star. Star spots are tied to local magnetic fields that have been amplified by the star’s rotation, so the phenomena are connected.A version without labels is available for download.Credit: NASA’s Goddard Space Flight Center || ThreeStars_Still.jpg (3840x2160) [586.8 KB] || ThreeStars_Still.png (3840x2160) [3.4 MB] || ThreeStars_Still_searchweb.png (320x180) [65.9 KB] || ThreeStars_Still_thm.png (80x40) [6.3 KB] || 14906_ThreeStars_NoText_1080.mp4 (1920x1080) [53.6 MB] || 14906_ThreeStars_1080.mp4 (1920x1080) [53.8 MB] || 14906_ThreeStars_4k.mp4 (3840x2160) [178.6 MB] || 14906_ThreeStars_NoText_4k.mp4 (3840x2160) [178.3 MB] || 14906_ThreeStars_NoText_ProRes_3840x2160_2997.mov (3840x2160) [1.8 GB] || 14906_ThreeStars_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || ", "hits": 358 }, { "id": 14732, "url": "https://svs.gsfc.nasa.gov/14732/", "result_type": "Produced Video", "release_date": "2025-09-21T09:00:00-04:00", "title": "Hubble’s Inside the Image: Saturn's Aurorae", "description": "NASA's Hubble Space Telescope has captured breathtaking ultraviolet images of Saturn’s aurorae, vibrant displays of light created by charged particles interacting with the planet’s magnetic field.In this video, Dr. Padi Boyd dives into the mesmerizing details of Saturn's aurorae and explains how Hubble's unique ultraviolet view sheds light on the dynamics of the planet's atmosphere and magnetic environment.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. Christensen Animation of Sun Passing Behind Saturn: ESA/Hubble - M. Kornmesser & L. CalçadaMusic Credits:\"Perennial Ice\" by Matthew Nicholson [PRS], and Suki Jeanette Finn [PRS] via Atmosphere Music Ltd. [PRS] and Universal Production Music\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music || ", "hits": 60 }, { "id": 5583, "url": "https://svs.gsfc.nasa.gov/5583/", "result_type": "Visualization", "release_date": "2025-09-17T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2025", "description": "Animation of Arctic sea ice from its maximum extent, March 22 2025, to its minimum, September 10, 2025, 4K version || sea_ice_2025_min_2160p60.2820_print.jpg (1024x576) [154.9 KB] || sea_ice_2025_min_2160p60.2820_searchweb.png (320x180) [74.1 KB] || sea_ice_2025_min_2160p60.2820_thm.png (80x40) [6.0 KB] || 3840x2160_16x9_60p (3840x2160) [3200 Item(s)] || sea_ice_2025_min_2160p60_p60.mp4 (3840x2160) [107.4 MB] || sea_ice_2025_min_2160p60_p60.mp4.hwshow [194 bytes] || ", "hits": 532 }, { "id": 14892, "url": "https://svs.gsfc.nasa.gov/14892/", "result_type": "Produced Video", "release_date": "2025-08-29T16:00:00-04:00", "title": "Solar Wind Animations", "description": "The Sun releases a constant stream of charged particles, called the solar wind. The solar wind originates in the outermost layer of the Sun’s atmosphere, the corona, when plasma is heated to a point that the Sun’s gravity can’t hold it down. When this plasma escapes – often reaching speeds of over one million miles per hour – it drags the Sun’s magnetic out across the solar system. When the solar wind encounters Earth, it is deflected by our planet's magnetic shield, causing most of the solar wind's energetic particles to flow around and beyond us. However, some of these high-energy particles can sneak past Earth’s natural magnetic defenses and produce hazardous conditions for satellites and astronauts, as well as power grids and infrastructure on Earth.Learn more about the solar wind: https://science.nasa.gov/sun/what-is-the-solar-wind/ || ", "hits": 933 }, { "id": 5576, "url": "https://svs.gsfc.nasa.gov/5576/", "result_type": "Visualization", "release_date": "2025-08-26T09:00:00-04:00", "title": "TROPICS Eyes Hurricane Erin", "description": "This animation tracks Hurricane Erin from August 10 through August 20, 2025. || Erin_v07_L1C_ch12_2025-08-28_121639.02708_print.jpg (1024x576) [138.3 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_searchweb.png (320x180) [86.9 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_thm.png (80x40) [6.2 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.mp4 (1920x1080) [17.4 MB] || channel_12 (1920x1080) [855 Item(s)] ||", "hits": 59 }, { "id": 20406, "url": "https://svs.gsfc.nasa.gov/20406/", "result_type": "Animation", "release_date": "2025-08-22T09:00:00-04:00", "title": "The Heliosphere Within The Milky Way Galaxy", "description": "Our solar system is nestled inside the Milky Way galaxy, home to more than 100 billion stars. Stretching for millions of miles around the solar system is a protective bubble called the heliosphere. Created by particles and magnetic fields from the Sun, the heliosphere separates our solar system from the vast galaxy beyond — and much of its harsh space radiation that can be damaging to life on Earth. || ", "hits": 851 }, { "id": 20408, "url": "https://svs.gsfc.nasa.gov/20408/", "result_type": "Animation", "release_date": "2025-08-22T09:00:00-04:00", "title": "Solar Particle Acceleration", "description": "The Sun constantly emits a stream of high energy particles that can be accelerated by magnetic fields and other processes to nearly the speed of light. These particles, made of protons, ions and electrons, can be damaging at Earth where they can impede the function of satellites and telecommunications. NASA’s IMAP (Interstellar Mapping and Acceleration Probe) studies particle acceleration to better understand the fundamental processes driving these particles. This information will help scientists better understand and prepare for their effects at Earth, collectively called space weather. || ", "hits": 121 }, { "id": 40543, "url": "https://svs.gsfc.nasa.gov/gallery/imap/", "result_type": "Gallery", "release_date": "2025-08-20T00:00:00-04:00", "title": "IMAP – Interstellar Mapping and Acceleration Probe", "description": "NASA's Interstellar Mapping and Acceleration Probe (IMAP) maps the boundaries of the heliosphere — the protective bubble surrounding the Sun and planets that is inflated by the constant stream of particles from the Sun called the solar wind. As a modern-day celestial cartographer, IMAP also explores and charts the vast range of particles in interplanetary space, helping to investigate important issues in heliophysics, the field studying the Sun and its sphere of influence. IMAP provides near-real-time information about the solar wind to provide advanced space weather warnings from its location at Lagrange point 1, one million miles from Earth toward the Sun.\n\nThe mission launched on Sept. 24, 2025, from NASA’s Kennedy Space Center in Florida.\n\nLearn more: https://science.nasa.gov/mission/imap/", "hits": 401 }, { "id": 5575, "url": "https://svs.gsfc.nasa.gov/5575/", "result_type": "Visualization", "release_date": "2025-08-19T11:00:00-04:00", "title": "Powerful Hurricane Erin forms in the Atlantic", "description": "Hurricane Erin on August 16, 2025 at approximately 10:23Z (6:23 EST) east of Puerto Rico and St. Thomas, U.S.V.I.", "hits": 182 }, { "id": 40539, "url": "https://svs.gsfc.nasa.gov/gallery/artemis-iiscience/", "result_type": "Gallery", "release_date": "2025-08-15T00:00:00-04:00", "title": "Moon Visualizations, Animations, Videos - Artemis II Lunar Science", "description": "While the Artemis II crew will be the first humans to test NASA’s Orion spacecraft in space, they will also conduct science investigations that will inform future deep space missions. During the 10-day past the Moon and back, the Orion capsule will fly by the far side of the Moon — the side that always faces away from Earth. During this three-hour period, astronauts will analyze and photograph geologic features, such as impact craters and ancient lava flows. They will rely on the extensive geology training they received in the classroom and in Moon-like places on Earth to describe nuances in shapes, textures, and colors — the type of information that reveals the geologic history of an area. These skills will be critical to exploring the Moon’s South Pole region through future missions.\n\nLearn more about Artemis II lunar science.\nLearn more about all Artemis II science experiments\nLearn more about the Moon at science.nasa.gov/moon.\n\n**Note: This page will be continually updated through the Artemis II mission. **\n\nMedia Contact: Lonnie Shekhtman NASA’s Goddard Space Flight Center in Greenbelt, Md.", "hits": 6549 }, { "id": 20410, "url": "https://svs.gsfc.nasa.gov/20410/", "result_type": "Animation", "release_date": "2025-08-14T00:00:00-04:00", "title": "IMAP Beauty Passes", "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) will explore and map the very boundaries of our heliosphere — a huge bubble created by the Sun's wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.As a modern-day celestial cartographer, IMAP will also explore and chart the vast range of particles in interplanetary space, helping to investigate two of the most important overarching issues in heliophysics — the energization of charged particles from the Sun, and the interaction of the solar wind at its boundary with interstellar space. Additionally, IMAP will support real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. The IMAP spacecraft will be located at Lagrange Point 1, or L1. Lagrange points are positions in space where objects sent there tend to stay put. At L1, which is around 1 million miles from Earth towards the Sun, the gravitational pull of the Sun and Earth are balanced, allowing spacecraft to reduce fuel consumption needed to remain in position. At L1, IMAP will have a clear view of the heliosphere and will also be positioned to provide advanced warning of incoming solar storms headed to Earth. Learn more about IMAP.Below are conceptual animations highlighting the IMAP spacecraft. || ", "hits": 305 }, { "id": 14881, "url": "https://svs.gsfc.nasa.gov/14881/", "result_type": "Animation", "release_date": "2025-08-13T00:00:00-04:00", "title": "Fermi Spacecraft Animations 2025", "description": "A beauty pass of NASA's Fermi Gamma-ray Space Telescope. The spacecraft fills the frame with a starry background at 0:05 and is fully in frame with Earth partially in the background at 0:11.Credit: NASA's Goddard Space Flight Center/CI Lab || Fermi_Beauty_Still.jpg (3840x2160) [250.1 KB] || Fermi_Beauty_Still_searchweb.png (320x180) [11.5 KB] || Fermi_Beauty_Still_thm.png (80x40) [1.6 KB] || Fermi_BeautyPass_1080.mp4 (1920x1080) [46.1 MB] || Fermi_BeautyPass_4k.mp4 (3840x2160) [113.7 MB] || Fermi_BeautyPass_V002_ProRes_4k.mov (3840x2160) [1.3 GB] || ", "hits": 92 }, { "id": 14882, "url": "https://svs.gsfc.nasa.gov/14882/", "result_type": "Produced Video", "release_date": "2025-08-07T09:55:00-04:00", "title": "Interstellar Visitor is Fastest Comet Ever Recorded", "description": "NASA's Hubble Space Telescope just captured an incredible image of interstellar comet 3I/ATLAS racing through our solar system at 130,000 mph!This cosmic wanderer from beyond our solar system may have been traveling for billions of years before astronomers spotted it.Watch now to discover what this ancient visitor reveals about our galaxy's history and why scientists are racing to study it before its close encounter with the Sun in 2025!For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerMusic Credit:\"God is in the Wind\" by Yat Fung Wong [CASH] via Universal Publishing Production Music Asia [CASH] and Universal Production MusicVideo Credits:Halley’s Comet Animation by Parky via Pond5Milky Way Timelapse via Pond5Comet Grazing the Sun (Tsuchinshan-ATLAS)Exocomets in Solar SystemESO/L. Calçada/N. RisingerComets orbiting White Dwarf StarESA/Hubble, NASA, ESO, M. KornmesserOumuamua ImageESA/Hubble, NASA, ESO, M. Kornmesser || ", "hits": 207 }, { "id": 20407, "url": "https://svs.gsfc.nasa.gov/20407/", "result_type": "Animation", "release_date": "2025-08-01T14:00:00-04:00", "title": "Carruthers Geocorona Animation", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.In this animation, atomic hydrogen floats in Earth’s exosphere. As the lightest chemical in existence, atomic hydrogen tends to float away, or evaporate, off the top of Earth’s atmosphere. When the Sun shines on these atoms, they scatter that light in all directions, causing a glow around Earth. This fuzzy halo of light that’s given off by those exospheric atoms is called the geocorona. || ", "hits": 70 }, { "id": 40538, "url": "https://svs.gsfc.nasa.gov/gallery/carruthers-geocorona-observatory/", "result_type": "Gallery", "release_date": "2025-07-25T00:00:00-04:00", "title": "Carruthers Geocorona Observatory", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at the Sun-Earth Lagrange point 1 (L1) where it uses advanced ultraviolet imagers to monitor Earth’s exosphere, the outermost layer of the atmosphere.. Carruthers is the first SmallSat to operate at L1 and the first mission dedicated to observing the exosphere, including its response to solar-driven space weather\n\nThe Carruthers Geocorona Observatory launched on Sept. 24, 2025, from NASA’s Kennedy Space Center in Florida.\n\nLearn more: https://science.nasa.gov/mission/carruthers-geocorona-observatory/", "hits": 167 }, { "id": 14873, "url": "https://svs.gsfc.nasa.gov/14873/", "result_type": "Produced Video", "release_date": "2025-07-22T17:00:00-04:00", "title": "Lagrange Point 1 Animation", "description": "Lagrange points are positions in space where objects sent there tend to stay put. At Lagrange points, the gravitational pull of two large masses precisely equals the centripetal force required for a small object to move with them. These points in space can be used by spacecraft to reduce fuel consumption needed to remain in position.Of the five Lagrange points, three are unstable and two are stable. The unstable Lagrange points - labeled L1, L2 and L3 - lie along the line connecting the two large masses. The stable Lagrange points - labeled L4 and L5 - form the apex of two equilateral triangles that have the large masses at their vertices. L4 leads the orbit of earth and L5 follows.The L1 point of the Earth-Sun system affords an uninterrupted view of the Sun and will be home to three new heliophysics missions in 2025 - NASA's Interstellar Mapping and Acceleration Probe (IMAP), NASA's Carruthers Geocorona Observatory, and NOAA's Space Weather Follow On-Lagrange 1 (SWFO-L1). || ", "hits": 668 }, { "id": 14867, "url": "https://svs.gsfc.nasa.gov/14867/", "result_type": "Produced Video", "release_date": "2025-07-15T14:00:00-04:00", "title": "GEMx Animations", "description": "Conceptual animation illustrating the ER-2 aircraft collecting spectroscopic mineral data over the American West. || GEMxThumbnail.png (1948x1052) [1.5 MB] || GEMxThumbnail_print.jpg (1024x553) [118.0 KB] || GEMxThumbnail_searchweb.png (320x180) [55.7 KB] || GEMxThumbnail_thm.png (80x40) [8.2 KB] || GEMx_Interface_1080p.mov (1920x1080) [37.6 MB] || GEMx_Interface_4k.mp4 (3840x2160) [36.0 MB] || GEMx_Interface_ProRes.mov (3840x2160) [4.1 GB] || ", "hits": 66 }, { "id": 5569, "url": "https://svs.gsfc.nasa.gov/5569/", "result_type": "Visualization", "release_date": "2025-07-11T09:30:59-04:00", "title": "Texas Hill Country Hit by Powerful Floods", "description": "GPM passed over the Texas storm on July 4th, 11am CT.", "hits": 87 }, { "id": 20405, "url": "https://svs.gsfc.nasa.gov/20405/", "result_type": "Animation", "release_date": "2025-07-08T16:00:00-04:00", "title": "Carruthers Atmospheric Layers Animation", "description": "Earth’s atmosphere is divided into five main layers, differentiated by factors such as temperature, chemical composition, and air density. The troposphere is the lowest layer, extending from Earth's surface up to about 10 miles above it, and is where almost all weather phenomena occur. Above the troposphere is the stratosphere, which reaches up to around 31 miles. It contains the ozone layer, which absorbs harmful ultraviolet (UV) radiation from the Sun. Next is the mesosphere, which extends from about 31 to 53 miles above Earth. It is the coldest layer of the atmosphere, and it is where most meteors burn up upon entering. Above the mesosphere is the thermosphere, ranging from about 53 to 375 miles above Earth. Known as the upper atmosphere, this region contains the ionosphere, a region filled with charged particles that enable radio communications and where auroras often occur. The outermost layer is the exosphere, which gradually transitions into outer space. It is extremely thin and composed mainly of hydrogen and helium. Together, these layers form a protective shield that regulates Earth’s energy balance and helps sustain life. || ", "hits": 1661 }, { "id": 5566, "url": "https://svs.gsfc.nasa.gov/5566/", "result_type": "Animation", "release_date": "2025-07-03T14:59:59-04:00", "title": "TEMPO Air Quality Monitoring: Three Example Cases", "description": "Three visualizations demonstrating the air quality monitoring capabilities of the TEMPO mission.", "hits": 126 }, { "id": 31345, "url": "https://svs.gsfc.nasa.gov/31345/", "result_type": "Visualization", "release_date": "2025-06-11T18:59:59-04:00", "title": "One Year of PACE OCI Chlorophyll", "description": "The Ocean Color Instrument (OCI) on the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite is a spectrometer designed to identify and quantify phytoplankton. This is a year-long visualization of the level 3 mapped chlorophyll data.", "hits": 147 }, { "id": 14857, "url": "https://svs.gsfc.nasa.gov/14857/", "result_type": "Produced Video", "release_date": "2025-06-11T14:10:00-04:00", "title": "NASA’s Webb Reveals Galaxy Population Driving Cosmic Renovation", "description": "Symbols mark the locations of young, low-mass galaxies bursting with new stars when the universe was about 800 million years old. Using a filter sensitive to such galaxies, NASA’s James Webb Space Telescope imaged them with the help of a natural gravitational lens created by the massive galaxy cluster Abell 2744. In all, 83 young galaxies were found, but only the 20 shown here (white diamonds) were selected for deeper study. The inset zooms into one of the galaxies. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025Alt text: Animation showing the locations of young, low-mass, starburst galaxies around galaxy cluster Abell 2744.Image description:White and yellow galaxies of various sizes and shapes appear against the blackness of space. Two bright stars in our own galaxy display prominent six-spike diffraction patterns with bluish rays, visible at center left and lower left. Then 20 white diamonds sweep across the image. One diamond enlarges to reveal an image of a young, low-mass, star-forming galaxy. It looks like a green oval against a red and green checked background. The enlarged image then shrinks back, and the diamonds sweep away. The sequence loops. || Pandora_stamp_60pct.gif (600x600) [961.0 KB] || ", "hits": 270 }, { "id": 14855, "url": "https://svs.gsfc.nasa.gov/14855/", "result_type": "Produced Video", "release_date": "2025-06-06T11:00:00-04:00", "title": "Carruthers Geocorona Observatory Beauty Pass Animations", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ", "hits": 44 }, { "id": 20404, "url": "https://svs.gsfc.nasa.gov/20404/", "result_type": "Animation", "release_date": "2025-06-02T12:00:00-04:00", "title": "TRACERS Science Animations", "description": "The TRACERS, or the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 203 }, { "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": 483 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 486 }, { "id": 31350, "url": "https://svs.gsfc.nasa.gov/31350/", "result_type": "Animation", "release_date": "2025-05-27T18:59:59-04:00", "title": "Your Name In Landsat", "description": "The Landsat program, a joint venture between NASA and the U.S. Geological Survey (USGS), has been observing Earth for over 50 years, collecting breathtaking imagery and invaluable data used to study our planet’s changing surface.\r\n\r\nOn the Your Name In Landsat project page, users can type in their name, then view and export the graphic of that name spelled out in Earth features found in Landsat images.", "hits": 92 }, { "id": 5475, "url": "https://svs.gsfc.nasa.gov/5475/", "result_type": "Visualization", "release_date": "2025-05-16T13:00:00-04:00", "title": "SOS - Change in Night Lights between 2012 and 2023", "description": "This animation of the Earth at night showcases NASA's Black Marble data. The animation begins by showing annual averages of nighttime lights from 2012 to 2023. The lights then fade away to reveal how night lights changed between 2012 and 2023, with regions of more light depicted in purple and regions with less light depicted in orange. ||", "hits": 308 }, { "id": 5476, "url": "https://svs.gsfc.nasa.gov/5476/", "result_type": "Visualization", "release_date": "2025-05-16T13:00:00-04:00", "title": "SOS - Earth Observing Fleet - Jan 2025", "description": "An animated view of NASA's Earth observing fleet", "hits": 324 }, { "id": 5477, "url": "https://svs.gsfc.nasa.gov/5477/", "result_type": "Visualization", "release_date": "2025-05-16T13:00:00-04:00", "title": "SOS - Day/Night cycle with Blue Marble and Black Marble Nightlights", "description": "This animation shows daylight and nighttime cycles of Earth over a three-day period in 2024 as the planet spins on it’s axis.", "hits": 1336 }, { "id": 5538, "url": "https://svs.gsfc.nasa.gov/5538/", "result_type": "Visualization", "release_date": "2025-05-15T13:00:00-04:00", "title": "Exploring High-Resolution Sea Surface Height Data from NASA’s SWOT Satellite", "description": "Exploring High-Resolution Sea Surface Height Data from NASA’s SWOT Satellite", "hits": 220 }, { "id": 20403, "url": "https://svs.gsfc.nasa.gov/20403/", "result_type": "Animation", "release_date": "2025-05-14T09:00:00-04:00", "title": "Titan science results from James Webb Space Telescope: animation resource page", "description": "Push into JWST to Saturn and Titan. || JWST_Titan_Intro_Final_V001.00957_print.jpg (1024x576) [145.8 KB] || JWST_Titan_Intro_Final_V001.00957_searchweb.png (320x180) [78.0 KB] || JWST_Titan_Intro_Final_V001.00957_thm.png [5.5 KB] || JWST_Titan_Intro_Final_1080.mp4 (1920x1080) [72.8 MB] || JWST_Titan_Intro_Final_V001.mp4 (3840x2160) [38.4 MB] || JWST_Titan_Intro_Final_V001.mov (3840x2160) [6.8 GB] || ", "hits": 155 }, { "id": 31343, "url": "https://svs.gsfc.nasa.gov/31343/", "result_type": "Animation", "release_date": "2025-05-01T04:00:00-04:00", "title": "Curiosity Mars rover panoramas", "description": "Animated zoom and pans of two Curiosity Mars rover panoramas from February 7, 2025 and March 9, 2025.", "hits": 766 }, { "id": 14821, "url": "https://svs.gsfc.nasa.gov/14821/", "result_type": "Produced Video", "release_date": "2025-04-14T14:00:00-04:00", "title": "Lucy Will Explore Asteroid Donaldjohanson", "description": "Lucy’s flyby of main-belt asteroid 52246 Donaldjohanson will provide the first close look at this surviving remnant of the solar system’s chaotic past.Complete transcript available.Universal Production Music: “Nico’s Journey” by Nicholas Smith [PRS]; “Knowing Half the Future” and “Temporal Timings” by Lee John Gretton [PRS]; “Poly Propulsion” by Alfie Solo [PRS] Watch this video on the NASA Goddard YouTube channel. || Lucy_DJ_Preview_Thumbnail_V3_print.jpg (1024x576) [240.8 KB] || Lucy_DJ_Preview_Thumbnail_V3.png (1280x720) [1.1 MB] || Lucy_DJ_Preview_Thumbnail_V3_searchweb.png (320x180) [81.6 KB] || 14821_Lucy_Asteroid_DJ_Preview_V2_720.mp4 (1280x720) [58.1 MB] || 14821_Lucy_Asteroid_DJ_Preview_V2_1080.mp4 (1920x1080) [325.2 MB] || LucyDJPreviewCaptions.en_US.srt [5.6 KB] || LucyDJPreviewCaptions.en_US.vtt [5.3 KB] || Lucy_DJ_Preview_Thumbnail_V3_thm.png [6.5 KB] || 14821_Lucy_Asteroid_DJ_Preview_V2_4K.mp4 (3840x2160) [4.0 GB] || 14821_Lucy_Asteroid_DJ_Preview_V2_ProRes.mov (3840x2160) [25.8 GB] || ", "hits": 74 }, { "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": 65 }, { "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": 312 }, { "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": 341 }, { "id": 20400, "url": "https://svs.gsfc.nasa.gov/20400/", "result_type": "Animation", "release_date": "2025-04-07T00:00:00-04:00", "title": "Habitable Worlds Observatory Ultra-stable Telescope", "description": "HWO ultra stable animation || UltraStableTelescope_Prores.00877_print.jpg (1024x576) [74.6 KB] || UltraStableTelescope_Prores.00877_searchweb.png (320x180) [65.2 KB] || UltraStableTelescope_1080_h264.mov [59.2 MB] || UltraStableTelescope_Prores.00877_thm.png [4.3 KB] || UltraStableTelescope_UHD_h264.mov (3840x2160) [141.7 MB] || UltraStableTelescope_Prores.mov (3840x2160) [2.7 GB] ||", "hits": 169 }, { "id": 14811, "url": "https://svs.gsfc.nasa.gov/14811/", "result_type": "Produced Video", "release_date": "2025-04-02T00:00:00-04:00", "title": "IMAP: Mapping The Heliosphere & Sun", "description": "The Interstellar Mapping and Acceleration Probe, or IMAP, will explore and map the very boundaries of our heliosphere — a huge bubble created by the Sun's wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.The mission’s investigation of the boundaries of the heliosphere will be primarily done with energetic neutral atoms, or ENAs. An ENA is a type of uncharged particle formed when an energetic positively charged ion runs into a slow-moving neutral atom. The ion picks up an extra negatively charged electron in the collision, making it neutral — hence the name energetic neutral atom. This process frequently happens wherever there is plasma in space, such as throughout the heliosphere, including its boundary.The IMAP-Lo, IMAP-HI, and IMAP-Ultra instruments on IMAP are imaging the energies and composition of ENAs.Learn more about IMAP: https://science.nasa.gov/mission/imap/ || ", "hits": 159 }, { "id": 14802, "url": "https://svs.gsfc.nasa.gov/14802/", "result_type": "Produced Video", "release_date": "2025-03-28T14:31:59-04:00", "title": "Earth to Space: A National Symphony Orchestra Concert", "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.", "hits": 116 }, { "id": 5522, "url": "https://svs.gsfc.nasa.gov/5522/", "result_type": "Visualization", "release_date": "2025-03-27T12:00:00-04:00", "title": "Arctic Sea Ice Maximum 2025", "description": "Arctic sea ice maximum extent 2025, still image || arctic_sea_ice_max_2025.png (3840x2160) [6.2 MB] || arctic_sea_ice_max_2025_print.jpg (1024x576) [150.6 KB] || arctic_sea_ice_max_2025_web.png (320x180) [73.6 KB] || arctic_sea_ice_max_2025_searchweb.png (320x180) [73.6 KB] || arctic_sea_ice_max_2025_thm.png [5.9 KB] || ", "hits": 329 }, { "id": 14805, "url": "https://svs.gsfc.nasa.gov/14805/", "result_type": "Animation", "release_date": "2025-03-24T12:00:00-04:00", "title": "TRACERS Spacecraft Beauty Passes", "description": "The TRACERS, or the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 118 }, { "id": 20398, "url": "https://svs.gsfc.nasa.gov/20398/", "result_type": "Animation", "release_date": "2025-03-19T11:00:00-04:00", "title": "Habitable Worlds Observatory (HWO) EAC 2 Design Animations", "description": "Animations and stills of design concept EAC 2 for the Habitable Worlds Observatory", "hits": 89 }, { "id": 20399, "url": "https://svs.gsfc.nasa.gov/20399/", "result_type": "Animation", "release_date": "2025-03-19T00:00:00-04:00", "title": "XMM-Newton spacecraft animations", "description": "Flyby animation of ESA's (European Space Agency's) XMM-Newton observatory as it orbits Earth.Credit: NASA/ESA || XMM_Beauty_Still.jpg (3840x2160) [449.2 KB] || XMM_Beauty_Still_searchweb.png (320x180) [38.6 KB] || XMM_Beauty_Shot_H264_V1.mp4 (3840x2160) [23.4 MB] || XMM_Beauty_Still_thm.png [3.3 KB] || XMM_Beauty_Shot_Prores_V1.mov (3840x2160) [807.2 MB] || ", "hits": 100 }, { "id": 5517, "url": "https://svs.gsfc.nasa.gov/5517/", "result_type": "Visualization", "release_date": "2025-03-12T00:00:00-04:00", "title": "Antarctic Sea Ice Minimum, 2025", "description": "Antarctic sea ice minimum extent, March 1 2025 || antarctic_sea_ice_min_2025_print.jpg (1024x576) [79.2 KB] || antarctic_sea_ice_min_2025.png (3840x2160) [2.8 MB] || ", "hits": 242 }, { "id": 5516, "url": "https://svs.gsfc.nasa.gov/5516/", "result_type": "Visualization", "release_date": "2025-03-11T00:00:00-04:00", "title": "Global Mean Sea Level 1993-2024", "description": "This animation shows the rise in global mean sea level from 1993 to 2024 based on data from a series of five international satellites.", "hits": 427 }, { "id": 14786, "url": "https://svs.gsfc.nasa.gov/14786/", "result_type": "Animation", "release_date": "2025-02-20T00:00:00-05:00", "title": "Swift Spacecraft Animations: 2025", "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || ", "hits": 104 }, { "id": 5471, "url": "https://svs.gsfc.nasa.gov/5471/", "result_type": "Visualization", "release_date": "2025-01-30T15:00:00-05:00", "title": "March 13-14, 2025 Total Lunar Eclipse: Shadow View", "description": "On March 13-14, 2025, the Moon enters the Earth's shadow, creating a total lunar eclipse. This animation shows the changing appearance of the Moon as it travels into and out of the Earth's shadow, along with times at various stages.", "hits": 474 }, { "id": 5473, "url": "https://svs.gsfc.nasa.gov/5473/", "result_type": "Visualization", "release_date": "2025-01-30T15:00:00-05:00", "title": "March 13-14, 2025 Total Lunar Eclipse: Visibility Map", "description": "On March 14, 2025 (the night of March 13), the Moon enters Earth's shadow, creating a total lunar eclipse. This animated map shows the region of the Earth where this eclipse is visible.", "hits": 615 }, { "id": 14772, "url": "https://svs.gsfc.nasa.gov/14772/", "result_type": "B-Roll", "release_date": "2025-01-29T11:00:00-05:00", "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics", "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ", "hits": 508 }, { "id": 14724, "url": "https://svs.gsfc.nasa.gov/14724/", "result_type": "Produced Video", "release_date": "2025-01-28T00:00:00-05:00", "title": "Significant Mission Milestones in OSIRIS-REx Journey to Bennu and Back", "description": "NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) capsule of rocks and dust collected from asteroid Bennu lands on Earth at, in a targeted area of the Department of Defense’s Utah Test and Training Range at 8:52 a.m. MDT (10:52 a.m. EDT) on Sunday. This video shows a compilation of spacecraft, airplane, and ground camera footage of the landing.Format: 1920 x 1080 px (HD) || OREX_LANDING_HD.00031_print.jpg (1024x576) [106.9 KB] || OREX_LANDING_HD.00031_searchweb.png (320x180) [45.2 KB] || OREX_LANDING_HD.00031_web.png (320x180) [45.2 KB] || OREX_LANDING_HD.00031_thm.png (80x40) [3.5 KB] || OREX_LANDING_HD.mp4 (1920x1080) [79.5 MB] || ", "hits": 28 }, { "id": 14771, "url": "https://svs.gsfc.nasa.gov/14771/", "result_type": "Produced Video", "release_date": "2025-01-24T14:00:00-05:00", "title": "PUNCH Instruments", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ", "hits": 81 }, { "id": 40532, "url": "https://svs.gsfc.nasa.gov/gallery/punch/", "result_type": "Gallery", "release_date": "2025-01-22T00:00:00-05:00", "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch", "hits": 232 }, { "id": 14747, "url": "https://svs.gsfc.nasa.gov/14747/", "result_type": "Produced Video", "release_date": "2025-01-16T10:15:00-05:00", "title": "Pandora Spacecraft Animations", "description": "Animated beauty pass of an artist's concept of the Pandora spacecraft, viewed without thermal blankets, set in a neutral gray volume. Credit: NASA's Goddard Space Flight Center/Conceptual Image LabAlt text: Pandora spacecraft animation no. 1Image description: An artist’s concept of NASA’s exoplanet explorer, Pandora, floats in a light gray background. The body of the small satellite looks like a black box with metal hardware. A long metallic cylinder extends upward from the body with multiple thin rings that slightly protrude from the surface and a flat metal rectangle on one side. On the underside of the body is a shiny dark circle. Pandora’s three solar panels extend from one side of the spacecraft’s body. The visible side is gray and laced with white wires, and the panels are connected with small silver fasteners. || Pandora_Beauty_S1_Still.jpg (3840x2160) [1.0 MB] || Pandora_Beauty_S1_Still_searchweb.png (320x180) [37.2 KB] || Pandora_Beauty_S1_Still_thm.png [4.0 KB] || Pandora_Beauty_S1_1080.mp4 (1920x1080) [14.7 MB] || Pandora_Beauty_S1_4k.mp4 (3840x2160) [36.6 MB] || Pandora_Beauty_S1_ProRes_3840x2160_30.mov (3840x2160) [1.1 GB] || ", "hits": 103 }, { "id": 5452, "url": "https://svs.gsfc.nasa.gov/5452/", "result_type": "Visualization", "release_date": "2025-01-10T11:00:00-05:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2024", "description": "The change in the distribution of land temperature anomalies over the years 1964 to 2024. This version is in Celsius, a Fahrenheit version is also available. || GISTEMPDist_2024_C.00850_print.jpg (1024x576) [45.7 KB] || GISTEMPDist_2024_C.00850_searchweb.png (320x180) [13.7 KB] || GISTEMPDist_2024_C.00850_thm.png [2.1 KB] || GISTEMPDist_2024_C.mp4 (3840x2160) [21.1 MB] ||", "hits": 274 }, { "id": 14741, "url": "https://svs.gsfc.nasa.gov/14741/", "result_type": "Produced Video", "release_date": "2024-12-27T13:00:00-05:00", "title": "Parker Solar Probe: Humanity’s Closest Encounter with the Sun", "description": "Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.Breaking its previous record by flying just 3.8 million miles above the surface of the Sun, NASA’s Parker Solar Probe hurtled through the solar atmosphere at a blazing 430,000 miles per hour — faster than any human-made object has ever moved. A beacon tone received in the late evening hours of Dec. 26 confirmed the spacecraft had made it through the encounter safely and is operating normally.This pass, the first of more to come at this distance, allows the spacecraft to conduct unrivaled scientific measurements with the potential to change our understanding of the Sun. || ", "hits": 579 }, { "id": 31327, "url": "https://svs.gsfc.nasa.gov/31327/", "result_type": "Hyperwall Visual", "release_date": "2024-12-23T12:30:00-05:00", "title": "GMAO – Topographic Resolution Over the Contiguous United States", "description": "TOPO resolution over CONUS || 3840x2160_16x9_30p [0 Item(s)] || Topo resolution over CONUS ||", "hits": 40 }, { "id": 14731, "url": "https://svs.gsfc.nasa.gov/14731/", "result_type": "Produced Video", "release_date": "2024-12-16T10:00:00-05:00", "title": "Hubble’s Inside the Image: Protoplanetary Disks", "description": "NASA's Hubble Space Telescope has captured stunning images of protoplanetary disks—dynamic, swirling structures of gas and dust surrounding young stars.In this video, Dr. Padi Boyd takes us on a journey through these remarkable objects, explaining how Hubble's observations are unraveling the mysteries of planet formation and providing a glimpse into the birthplaces of new solar systems.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. Christensen Exoplanet Animations: ESA/Hubble - M. Kornmesser & L. CalçadaMusic Credits:PREMIUM BEAT BY SHUTTERSTOCKThe Search by Northern Points\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music || ", "hits": 117 }, { "id": 5434, "url": "https://svs.gsfc.nasa.gov/5434/", "result_type": "Visualization", "release_date": "2024-12-10T10:00:00-05:00", "title": "Collecting Global Methane Emissions with EMIT", "description": "Animation that shows the data collection path of the EMIT instrument onboard the ISS. EMIT has a 75 kilometer swath width - which is relatively narrow, but you can see in this data visualization how it can get full global coverage over time. The violet dots are methane emission sources. || new_emit_v35_4K.0100_print.jpg (1024x576) [162.5 KB] || new_emit_v35_4K.0100_searchweb.png (320x180) [74.3 KB] || new_emit_v35_4K.0100_thm.png (80x40) [7.6 KB] || new_emit_v35_1080p30.mp4 (1920x1080) [28.2 MB] || new_emit_v35_4K_2160p30.mp4 (3840x2160) [86.9 MB] || 3840x2160_16x9_30p [0 Item(s)] || new_emit_v35_4K_2160p30.mp4.hwshow [189 bytes] || ", "hits": 222 }, { "id": 5423, "url": "https://svs.gsfc.nasa.gov/5423/", "result_type": "Visualization", "release_date": "2024-11-27T11:00:00-05:00", "title": "Gravity waves disturbing the stratospheric polar vortex", "description": "Animation 1: Changes in temperature and height on the surface of 850 Kelvin potential temperature. 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