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            "id": 5633,
            "url": "https://svs.gsfc.nasa.gov/5633/",
            "result_type": "Visualization",
            "release_date": "2026-04-06T10:30:00-04:00",
            "title": "Simulating the Artemis II Lunar Flyby on April 6, 2026",
            "description": "This visualization simulates what the crew of Artemis II will see out the window on the day of their closest approach to the Moon on April 6, 2026. It covers the period of their scheduled science observations that begins at 18:45 UTC and spans seven hours, flying the virtual camera on the actual post-TLI trajectory that swings the spacecraft around the Moon's far side.",
            "hits": 33468
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        {
            "id": 14934,
            "url": "https://svs.gsfc.nasa.gov/14934/",
            "result_type": "Produced Video",
            "release_date": "2026-03-26T16:00:00-04:00",
            "title": "NASA Interview Opportunity: Moonbound! NASA’s Artemis II Mission Days From Launch — First Crewed Journey Around the Moon in More Than 50 Years!",
            "description": "Click here for the Artemis II PRESS KIT. || ARTEMIS_II_BANNER_english2.jpeg (1800x720) [342.6 KB] || ARTEMIS_II_BANNER_english2_print.jpg (1024x409) [139.2 KB] || ARTEMIS_II_BANNER_english2_searchweb.png (320x180) [86.2 KB] || ARTEMIS_II_BANNER_english2_thm.png (80x40) [7.7 KB] || ",
            "hits": 3908
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        {
            "id": 14989,
            "url": "https://svs.gsfc.nasa.gov/14989/",
            "result_type": "Produced Video",
            "release_date": "2026-03-18T09:55:00-04:00",
            "title": "Hubble Accidentally Catches Comet Breaking Up",
            "description": "In a happy twist of fate, NASA’s Hubble Space Telescope just witnessed a comet in the act of breaking apart. The chance of that happening while Hubble watched is extraordinarily miniscule. Comet K1, whose full name is Comet C/2025 K1 (ATLAS)—not to be confused with interstellar comet 3I/ATLAS—was not the original target of the Hubble study.Before it fragmented, K1 was likely a bit larger than an average comet, probably around 5 miles across. The team estimates the comet began to disintegrate eight days before Hubble viewed it. Hubble took three 20-second images, one on each day from November 8 through November 10, 2025. As it watched the comet, one of K1’s smaller pieces also broke up. Because Hubble’s sharp vision can distinguish extremely fine details, the team could trace the history of the fragments back to when they were one piece. That allowed them to reconstruct the timeline. But in doing so, they uncovered a mystery: Why was there a delay between when the comet broke up and when bright outbursts were seen from the ground? When the comet fragmented and exposed fresh ice, why didn’t it brighten almost instantaneously?Sometimes the best science happens by accident!For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerOriginal Story Written by: Ann Jenkins / Christine Pulliam of the Space Telescope Science InstituteVideo Credits:Milky Way with comets timelapse. Credit: POND5Comet Shoemaker Levy colliding with Jupiter from ESA's movie \"15 Years of Discovery\". Credit: ESA/Hubble (M. Kornmesser & L. L. Christensen)Comet K1 Image. Credit: NASA, ESA, D. Bodewits (Auburn). Image processing: J. DePasquale (STScI).Diagram of K1’s path through the Solar System. Credit: NASA, ESA, R. Crawford (STScI)Music Credit:“Le nozze di Figaro” by Wolfgang Amadeus Mozart via Chappell Recorded Music Library Ltd [PRS] and Universal Production Music || ",
            "hits": 319
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            "id": 14988,
            "url": "https://svs.gsfc.nasa.gov/14988/",
            "result_type": "Produced Video",
            "release_date": "2026-03-16T14:00:00-04:00",
            "title": "Artemis II: Into the Path of Solar Eruptions",
            "description": "For the first time in half a century, four astronauts are leaving Earth’s protective magnetic field. They’ll enter a realm where massive solar eruptions can unleash more energy than a billion hydrogen bombs. The Artemis II crew will fly through a dangerous environment, but they’re not going it alone. On the voyage, the astronauts and their Orion capsule are outfitted with radiation trackers as ground teams monitor solar eruptions 24/7. Here’s how NASA and the National Oceanic and Atmospheric Administration (NOAA) are protecting explorers from the most powerful eruptions in the solar system. Learn more: https://science.nasa.gov/missions/artemis/artemis-2/to-protect-artemis-ii-astronauts-nasa-experts-keep-eyes-on-sun/ || ",
            "hits": 1996
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        {
            "id": 31347,
            "url": "https://svs.gsfc.nasa.gov/31347/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-03-03T18:59:59-05:00",
            "title": "Astronaut Don Pettit’s Photos from Space",
            "description": "hyperwall hwshows for photos from https://www.nasa.gov/gallery/astronaut-don-pettits-photos-from-space/",
            "hits": 990
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            "id": 40548,
            "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/",
            "result_type": "Gallery",
            "release_date": "2026-03-03T00:00:00-05:00",
            "title": "SOHO – Solar and Heliospheric Observatory",
            "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/",
            "hits": 475
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            "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.",
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            "id": 5586,
            "url": "https://svs.gsfc.nasa.gov/5586/",
            "result_type": "Visualization",
            "release_date": "2026-01-20T12:00:00-05:00",
            "title": "Extreme Mass Ratio Black Hole Inspirals (EMRIs)",
            "description": "Shows seven unique black hole inspirals.",
            "hits": 398
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            "id": 14951,
            "url": "https://svs.gsfc.nasa.gov/14951/",
            "result_type": "Produced Video",
            "release_date": "2026-01-14T10:00:00-05:00",
            "title": "Are Titan’s Lakes Teeming with Primitive Cells?",
            "description": "Titan’s hydrocarbon lakes could contain structures called vesicles that strongly resemble cell membranes on Earth. A recent study coauthored by NASA shows that rainfall might provide the energy needed for these vesicles to form.Complete transcript available.Universal Production Music: “Perpetual Resonance” by Lee John Gretton [PRS]Watch this video on the NASA Goddard YouTube channel and Facebook. || Titan-Vesicles-Thumbnail-V3_print.jpg (1024x576) [112.3 KB] || Titan-Vesicles-Thumbnail-V3.jpg (1280x720) [362.4 KB] || Titan-Vesicles-Thumbnail-V3.png (1280x720) [734.2 KB] || Titan-Vesicles-Thumbnail-V3_searchweb.png (320x180) [62.2 KB] || Titan-Vesicles-Thumbnail-V3_thm.png (80x40) [6.0 KB] || 14951_Titan_Vesicles_Explainer_720.mp4 (1280x720) [39.0 MB] || 14951_Titan_Vesicles_Explainer_1080.mp4 (1920x1080) [218.4 MB] || TitanVesiclesCaptions.en_US.srt [3.8 KB] || TitanVesiclesCaptions.en_US.vtt [3.6 KB] || 14951_Titan_Vesicles_Explainer_4K.mp4 (3840x2160) [1.3 GB] || 14951_Titan_Vesicles_Explainer_ProRes.mov (3840x2160) [8.0 GB] || ",
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            "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. || ",
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            "id": 14945,
            "url": "https://svs.gsfc.nasa.gov/14945/",
            "result_type": "Produced Video",
            "release_date": "2026-01-09T09:00:00-05:00",
            "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars",
            "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ",
            "hits": 460
        },
        {
            "id": 14930,
            "url": "https://svs.gsfc.nasa.gov/14930/",
            "result_type": "Infographic",
            "release_date": "2025-12-18T10:00:00-05:00",
            "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles",
            "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel",
            "hits": 132
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        {
            "id": 5577,
            "url": "https://svs.gsfc.nasa.gov/5577/",
            "result_type": "Animation",
            "release_date": "2025-11-20T09:00:00-05:00",
            "title": "SDO Sun This Week",
            "description": "This visualization shows SDO AIA-304 imagery from the past 7 days with a color table and image processing applied. Archive folders are provided in the Download menu.",
            "hits": 0
        },
        {
            "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": 369
        },
        {
            "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": 378
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        {
            "id": 5536,
            "url": "https://svs.gsfc.nasa.gov/5536/",
            "result_type": "Visualization",
            "release_date": "2025-08-15T09:00:00-04:00",
            "title": "Simulated Artemis II Lunar Flyby",
            "description": "This visualization simulates what the crew of Artemis II might see out the window on the day of their closest approach to the Moon.",
            "hits": 16328
        },
        {
            "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.",
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        {
            "id": 5532,
            "url": "https://svs.gsfc.nasa.gov/5532/",
            "result_type": "Visualization",
            "release_date": "2025-07-18T08:00:00-04:00",
            "title": "Comparing ISS and ICESat-2 Coverage Across the Earth",
            "description": "These visualizations explore the orbits of the International Space Station (ISS) and the ICESat-2 satellite. The ISS reaches a maximum latitude of approximately ±51.6°, while ICESat-2 extends to about ±88°, allowing it to observe much closer to the poles.",
            "hits": 157
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        {
            "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": 198
        },
        {
            "id": 5525,
            "url": "https://svs.gsfc.nasa.gov/5525/",
            "result_type": "Visualization",
            "release_date": "2025-04-14T13:00:00-04:00",
            "title": "Lucy Flyby of Asteroid Donaldjohanson Trajectory Visualizations",
            "description": "NASA’s Lucy mission is heading to the Jupiter Trojans – an unexplored population of asteroids considered to be the fossils of planetary formation. Along the way, Lucy is traveling through the main asteroid belt, on course to fly past 52246 Donaldjohanson on April 20, 2025.",
            "hits": 97
        },
        {
            "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": 145
        },
        {
            "id": 5519,
            "url": "https://svs.gsfc.nasa.gov/5519/",
            "result_type": "Visualization",
            "release_date": "2025-03-18T17:05:00-04:00",
            "title": "Surface Water and Ocean Topography (SWOT) Vertical Gravity Gradient",
            "description": "No description available.",
            "hits": 563
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        {
            "id": 5510,
            "url": "https://svs.gsfc.nasa.gov/5510/",
            "result_type": "Visualization",
            "release_date": "2025-02-25T17:10:00-05:00",
            "title": "Map of the March 29, 2025 Partial Solar Eclipse",
            "description": "On Saturday, March 29, 2025, the Moon passes in front of the Sun, casting its shadow across the Atlantic Ocean. Observers in Europe, western Africa, and eastern Canada are positioned to see a partial eclipse.",
            "hits": 357
        },
        {
            "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": 211
        },
        {
            "id": 14722,
            "url": "https://svs.gsfc.nasa.gov/14722/",
            "result_type": "Produced Video",
            "release_date": "2024-12-06T15:00:00-05:00",
            "title": "NASA Interview Opportunity: NASA Spacecraft Days Away From Historic Close Approach to the Sun",
            "description": "Scroll down the page for associated cut b-roll for the live shots and pre-recorded soundbites.Find out more about NASA's Parker Solar Probe here! nasa.gov/parker || Screenshot_2024-12-06_at_2.24.02 PM.png (1546x606) [1.9 MB] || Screenshot_2024-12-06_at_2.24.02 PM_print.jpg (1024x401) [195.3 KB] || Screenshot_2024-12-06_at_2.24.02 PM_searchweb.png (320x180) [128.7 KB] || Screenshot_2024-12-06_at_2.24.02 PM_thm.png (80x40) [12.2 KB] || ",
            "hits": 130
        },
        {
            "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": 190
        },
        {
            "id": 14707,
            "url": "https://svs.gsfc.nasa.gov/14707/",
            "result_type": "Produced Video",
            "release_date": "2024-11-25T11:00:00-05:00",
            "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3",
            "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ",
            "hits": 649
        },
        {
            "id": 31319,
            "url": "https://svs.gsfc.nasa.gov/31319/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-10-23T00:00:00-04:00",
            "title": "2025 NASA Science Calendar",
            "description": "Images from the 2025 NASA Science Calendar",
            "hits": 124
        },
        {
            "id": 14695,
            "url": "https://svs.gsfc.nasa.gov/14695/",
            "result_type": "Produced Video",
            "release_date": "2024-10-16T12:00:00-04:00",
            "title": "Roman's Outer Barrel Assembly Testing Time Lapse",
            "description": "Watch a condensed seven-minute version of the time-lapse with labels explaining the steps.Credit: NASA's Goddard Space Flight CenterMusic credit: \"Concave Hexagon\" from the album Geometric Shapes. Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_OBA_TL.jpg (1280x720) [367.9 KB] || YTframe_OBA_TL_searchweb.png (320x180) [102.0 KB] || YTframe_OBA_TL_thm.png (80x40) [10.3 KB] || 14695_OBA_Timelapse_Medium_1080.mp4 (1920x1080) [259.0 MB] || 14695OBATimelapseMedium.en_US.srt [2.6 KB] || 14695OBATimelapseMedium.en_US.vtt [2.5 KB] || 14695_OBA_Timelapse_Medium_4k.mp4 (3840x2160) [495.7 MB] || 14695_OBA_Timelapse_Medium_4k_HighQuality.mp4 (3840x2160) [2.3 GB] || 14695_OBA_Timelapse_Medium_ProRes_3840x2160_2997.mov (3840x2160) [26.3 GB] || ",
            "hits": 52
        },
        {
            "id": 5301,
            "url": "https://svs.gsfc.nasa.gov/5301/",
            "result_type": "Visualization",
            "release_date": "2024-09-30T00:00:00-04:00",
            "title": "Atlantic Ocean Surface Drift Patterns from the Caribbean in 2010 and 2011",
            "description": "Simulated particle backtrack with windage and timelineThis  visualization shows simulated particles released during 2010 and 2011 traced back in time to show their path based on the ocean surface velocities from Global HYCOM model with 1% windage applied.  Simulated particles were released between December through April and tracked back in time.  The gold balls under the timeline indicate the months when particles were released.  Flow lines represent the movement of a particle over a 20-day period.  Particles that venture above the 23 degree north latitude line (shown in red) during their lifespan are colored gold while particles that stayed south of it are colored green. || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_print.jpg (1024x576) [193.3 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_searchweb.png (320x180) [76.7 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_thm.png (80x40) [6.2 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_1080p60.mp4 (1920x1080) [52.6 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_1080p30.mp4 (1920x1080) [54.0 MB] || composite_wWind [0 Item(s)] || composite_wWind [0 Item(s)] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4 (3840x2160) [151.2 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_2160p30.mp4 (3840x2160) [158.8 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4.hwshow [226 bytes] || ",
            "hits": 37
        },
        {
            "id": 5343,
            "url": "https://svs.gsfc.nasa.gov/5343/",
            "result_type": "Visualization",
            "release_date": "2024-09-23T00:00:00-04:00",
            "title": "NEX GDDP CMIP6 Historical and Predicted Global Maximum Monthly Temperature from 1950 - 2100",
            "description": "No description available.",
            "hits": 177
        },
        {
            "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": 78
        },
        {
            "id": 14686,
            "url": "https://svs.gsfc.nasa.gov/14686/",
            "result_type": "B-Roll",
            "release_date": "2024-09-18T11:00:00-04:00",
            "title": "Eclipse Ballooning Project Featuring the University of Maryland",
            "description": "The NASA-sponsored Nationwide Eclipse Ballooning Project (NEBP) immerses teams of STEM learners from a wide range of higher education institutions in an innovative NASA-mission-like adventure in data acquisition and analysis through scientific ballooning during the Oct. 14, 2023, annular and April 8, 2024, total solar eclipses.NEBP includes development and implementation of two learner-centered activity tracks – engineering and atmospheric science. At sites along the eclipse path, student teams in the engineering track use innovative larger balloon systems to live stream video to the NASA eclipse website, observe in situ perturbations in atmospheric phenomena, and conduct individually designed experiments. Atmospheric science track teams make frequent observations by launching hourly radiosondes on helium-filled weather balloons. Student participants work with atmospheric science experts throughout the project and will publish results in peer-reviewed journals.The project fully supports 53 teams divided into nine pods to facilitate effective education. NEBP provides a learning environment that uses evidence and equity-based practices to make certain the 750+ participants are (and feel) supported, engaged, and valued. In addition, NEBP provides infrastructure tools and best practices to help participating institutions build collaborations that could continue far beyond the scope of this project.Learn more: https://science.nasa.gov/sciact-team/nationwide-eclipse-ballooning-project/ || ",
            "hits": 38
        },
        {
            "id": 5378,
            "url": "https://svs.gsfc.nasa.gov/5378/",
            "result_type": "Visualization",
            "release_date": "2024-09-07T15:30:00-04:00",
            "title": "Map of the October 2, 2024 Annular Solar Eclipse",
            "description": "On Wednesday, October 2, 2024, the Moon passes in front of the Sun, casting its shadow across the Pacific Ocean. Observers on Rapa Nui (Easter Island) and in far southern Chile and Argentina are in the path of the annular eclipse. Hawai'i, parts of Antarctica, and the southern half of South America see a partial eclipse.",
            "hits": 237
        },
        {
            "id": 5362,
            "url": "https://svs.gsfc.nasa.gov/5362/",
            "result_type": "Visualization",
            "release_date": "2024-08-23T00:00:00-04:00",
            "title": "TROPICS Tracks Hurricane Debby",
            "description": "This data visualization starts by showing the constellation of cubesats that make up the TROPICS mission collecting data across the globe. The camera then pushes in tighter to show Tropical Depression Debby over Haiti. We then follow Debby's path over Cuba as it begins to organize into a Tropical Storm. It then strengthens to a category 1 hurricane in the Gulf of Mexico right before hitting Florida, where it quickly weakens back into a Tropical Storm. It then slowly moves over Georgia and South Carolina flooding both those states. || tropics_debbyL1c_v90_2024-08-15_1016.02928_print.jpg (1024x576) [146.7 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_searchweb.png (320x180) [86.0 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_thm.png (80x40) [6.4 KB] || tropics_debbyL1c_v90_2024-08-15_1016_1080p30.mp4 (1920x1080) [31.8 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4 (3840x2160) [94.7 MB] || 3840x2160_16x9_30p [0 Item(s)] || tropics_debbyL1c_v90_2024-08-15_1016.webm (3840x2160) [20.4 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4.hwshow || ",
            "hits": 38
        },
        {
            "id": 14652,
            "url": "https://svs.gsfc.nasa.gov/14652/",
            "result_type": "Produced Video",
            "release_date": "2024-08-15T17:00:00-04:00",
            "title": "Exploring Volcanoes with NASA’s GEODES Team",
            "description": "Enjoy this music video of NASA’s GEODES team exploring lunar-like landscapes.Complete transcript available.Music credit: “Aerial” by Ben Cosgrove” and \"Volcano\" by Ben Cosgrove. Used with permission from the artist.Watch this video on the NASA Goddard YouTube channel. || ExploringVolcanoes_Thumbnail_print.jpg (1024x576) [185.0 KB] || ExploringVolcanoes_Thumbnail.png (1280x720) [1.2 MB] || ExploringVolcanoes_Thumbnail_searchweb.png (320x180) [106.5 KB] || ExploringVolcanoes_Thumbnail_thm.png (80x40) [8.4 KB] || ExploringVolcanoes_720.mp4 (1280x720) [67.0 MB] || EXPLORING_VOLCANOES_Captions_Final.en_US.srt [2.1 KB] || EXPLORING_VOLCANOES_Captions_Final.en_US.vtt [2.0 KB] || ExploringVolcanoes.mp4 (1920x1080) [471.1 MB] || ",
            "hits": 45
        },
        {
            "id": 5326,
            "url": "https://svs.gsfc.nasa.gov/5326/",
            "result_type": "Visualization",
            "release_date": "2024-07-18T12:00:00-04:00",
            "title": "Moon Essentials: Orbit",
            "description": "The mean (average) orbit of the Moon as it changes over the course of 8.5 years. Shows the tilt of the orbit and the slow rotation of the nodes (where the Moon's orbit intersects the orbit plane of the Earth) and the apses (the near and far points). This is a simplified model that ignores the short-term influence of the Sun and the rest of the solar system. || simple.1351_print.jpg (1024x576) [62.0 KB] || simple.1351_searchweb.png (320x180) [39.1 KB] || simple.1351_thm.png (80x40) [3.0 KB] || simple [0 Item(s)] || moon_orbit_simple_1080p30.mp4 (1920x1080) [9.1 MB] || moon_orbit_simple_720p30.mp4 (1280x720) [5.0 MB] || moon_orbit_simple_360p30.mp4 (640x360) [2.3 MB] || ",
            "hits": 4552
        },
        {
            "id": 14619,
            "url": "https://svs.gsfc.nasa.gov/14619/",
            "result_type": "Produced Video",
            "release_date": "2024-07-17T10:00:00-04:00",
            "title": "Black Hole with Accretion Disk Visualization",
            "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole surrounded by a rapidly-rotating disk of gas and dust. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The speed at which material, in what is known as an accretion disk, orbits the black hole increases with proximity. The orbital speed of material closest to the event horizon approaches the speed of light. This produces an effect known as “relativistic doppler beaming” which enhances the brightness of material moving towards us along our line of sight, and correspondingly dims the brightness of material moving away.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.The light from the orbiting material is likewise distorted, making the flat accretion disk appear to bend completely around the black hole’s shadow and have the disk behind the black hole appear to be both above and below it. Yet despite these strange visual distortions that change with viewing angle, the accretion disk itself physically remains flat.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance of a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
            "hits": 880
        },
        {
            "id": 14620,
            "url": "https://svs.gsfc.nasa.gov/14620/",
            "result_type": "Produced Video",
            "release_date": "2024-07-17T10:00:00-04:00",
            "title": "Isolated Black Hole Visualization",
            "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
            "hits": 1128
        },
        {
            "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": 368
        },
        {
            "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": 1661
        },
        {
            "id": 14574,
            "url": "https://svs.gsfc.nasa.gov/14574/",
            "result_type": "Produced Video",
            "release_date": "2024-05-06T10:00:00-04:00",
            "title": "Black Hole Week 2024 Poster and Media",
            "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.",
            "hits": 193
        },
        {
            "id": 14562,
            "url": "https://svs.gsfc.nasa.gov/14562/",
            "result_type": "Produced Video",
            "release_date": "2024-04-03T14:30:00-04:00",
            "title": "Chasing The 2024 Total Solar Eclipse With NASA Jets",
            "description": "The April 8, 2024, total solar eclipse will produce stunning views across North America. While anyone along the eclipse path with a clear sky will see the spectacular event, the best view might be 50,000 feet in the air, aboard NASA’s WB-57 jet planes. That’s where a trio of NASA-funded teams are sending their scientific instruments to take measurements of the eclipse.Two teams will image the Sun’s outer atmosphere – the corona – and a third will measure the ionosphere, the upper electrically charged layer of Earth’s atmosphere. This information will help scientists better understand the structure and temperature of the corona, the effects of the Sun on Earth’s atmosphere, and even aid in the search of asteroids that may orbit near the Sun. || ",
            "hits": 77
        },
        {
            "id": 5247,
            "url": "https://svs.gsfc.nasa.gov/5247/",
            "result_type": "Visualization",
            "release_date": "2024-03-26T00:00:00-04:00",
            "title": "Ang 2024 Total Solar Eclipse",
            "description": "This page is a Tagalog version of #5123 (The 2024 Total Solar Eclipse). || ",
            "hits": 40
        },
        {
            "id": 5248,
            "url": "https://svs.gsfc.nasa.gov/5248/",
            "result_type": "Visualization",
            "release_date": "2024-03-25T13:30:00-04:00",
            "title": "Insolation during the 2024 Eclipse",
            "description": "Insolation (the amount of sunlight reaching the ground) is affected dramatically by the Moon's shadow during the April 8, 2024 total solar eclipse. || insol.0765_print.jpg (1024x576) [144.8 KB] || insol.0765_searchweb.png (320x180) [73.2 KB] || insol.0765_thm.png (80x40) [6.1 KB] || eclipse2024_insol_720p30.mp4 (1280x720) [10.4 MB] || eclipse2024_insol_1080p30.mp4 (1920x1080) [21.3 MB] || eclipse2024_insol_2160p30.mp4 (3840x2160) [66.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || eclipse2024_insol_360p30.mp4 (640x360) [3.2 MB] || ",
            "hits": 52
        },
        {
            "id": 14551,
            "url": "https://svs.gsfc.nasa.gov/14551/",
            "result_type": "Produced Video",
            "release_date": "2024-03-25T06:00:00-04:00",
            "title": "The Countdown Is On For The Historic Solar Eclipse On April 8th That Will Sweep Across the U.S. Are You Ready for It?",
            "description": "Scroll down the page for the cut b-roll for the live shots and a canned interview available for easy download || Total_Solar_Eclipse_Banner_4.3.24.jpg (1800x720) [134.2 KB] || Total_Solar_Eclipse_Banner_4.3.24_print.jpg (1024x409) [62.3 KB] || Total_Solar_Eclipse_Banner_4.3.24_searchweb.png (320x180) [32.4 KB] || Total_Solar_Eclipse_Banner_4.3.24_thm.png (80x40) [5.0 KB] || ",
            "hits": 114
        },
        {
            "id": 14555,
            "url": "https://svs.gsfc.nasa.gov/14555/",
            "result_type": "Produced Video",
            "release_date": "2024-03-20T09:00:00-04:00",
            "title": "How to Observe with GLOBE Eclipse",
            "description": "Music Credit:  \"Silly Goose\" by Reveille from Soundstripe || EclipseEnglish.00001_print.jpg (1024x576) [198.7 KB] || EclipseEnglish.00001_searchweb.png (320x180) [104.0 KB] || EclipseEnglish.en_US.srt [4.2 KB] || EclipseEnglish.en_US.vtt [4.0 KB] || EclipseEnglish.mp4 (1920x1080) [362.6 MB] || ",
            "hits": 26
        },
        {
            "id": 5236,
            "url": "https://svs.gsfc.nasa.gov/5236/",
            "result_type": "Visualization",
            "release_date": "2024-03-13T17:30:00-04:00",
            "title": "5000 Years of Total Solar Eclipses: The Movie",
            "description": "An animated heatmap showing the accumulation of total solar eclipse paths over the 5000 years from 2000 BCE to 3000 CE. || heatmap.0090_print.jpg (1024x576) [282.2 KB] || heatmap.0090_searchweb.png (320x180) [93.8 KB] || heatmap.0090_thm.png (80x40) [7.5 KB] || heatmap_720p30.mp4 (1280x720) [20.0 MB] || heatmap_1080p30.mp4 (1920x1080) [38.1 MB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || heatmap_360p30.mp4 (640x360) [6.2 MB] || heatmap_2160p30.mp4 (3840x2160) [120.6 MB] || ",
            "hits": 75
        },
        {
            "id": 14547,
            "url": "https://svs.gsfc.nasa.gov/14547/",
            "result_type": "Produced Video",
            "release_date": "2024-03-12T11:00:00-04:00",
            "title": "Citizen CATE 2024",
            "description": "Led by Amir Caspi of the Southwest Research Institute in Colorado, the Citizen Continental-America Telescopic Eclipse (CATE) 2024 project will place 35 teams in the eclipse path from Texas to Maine to capture the corona in polarized light.Light travels in waves, but those waves can be oriented in different directions, or polarization angles. Caspi explains that light we see from the corona is sunlight that gets bounced around by the corona before it reaches our eyes. Citizen CATE 2024 is one of many participatory science projects happening during the 2024 total solar eclipse. Read more: https://science.nasa.gov/solar-system/skywatching/eclipse-photographers-help-study-sun-during-disappearing-act/ || ",
            "hits": 37
        },
        {
            "id": 14541,
            "url": "https://svs.gsfc.nasa.gov/14541/",
            "result_type": "Produced Video",
            "release_date": "2024-03-12T09:00:00-04:00",
            "title": "Dynamic Eclipse Broadcast (DEB) Initiative",
            "description": "In visible wavelengths of light, the Sun’s surface is much brighter than its corona. During a total solar eclipse, however, observers can see the corona – and scientists can investigate how solar material moves out from the Sun to form the solar wind, an ever-flowing particle stream that impacts Earth and our entire solar system.The Dynamic Eclipse Broadcast (DEB) Initiative, led by Bob Baer and Matt Penn of Southern Illinois University in Carbondale, organizes volunteers as they capture images of the corona during the 2024 eclipse. Using identical instruments at more than 70 different locations across North America, participants document the moment-by-moment appearance of the corona throughout the eclipse. Comparing these images across locations, scientists track plumes of solar material in the difficult-to-study inner corona, estimating their speed and rate of acceleration and linking these observations to those from NASA spacecraft.The project expands on the team’s efforts during the 2017 total solar eclipse, this time including observation sites outside the path of totality, where part of the solar disk will remain visible. Images from these locations will reveal the source of solar material later observed as outflows in the corona, allowing the team to trace them back to their origins on the Sun.DEB Initiative is one of many participatory science projects happening during the 2024 total solar eclipse. Click here to learn more. || ",
            "hits": 51
        },
        {
            "id": 14527,
            "url": "https://svs.gsfc.nasa.gov/14527/",
            "result_type": "Produced Video",
            "release_date": "2024-02-28T09:00:00-05:00",
            "title": "The Moon and the 2024 Total Solar Eclipse",
            "description": "This video explores the role of the Moon in the 2024 total solar eclipse that can be seen in the United States, Canada, and Mexico.Music provided by Universal Production Music: \"On the Up\" - David Stephen WestlakeWatch this video on the NASA Goddard YouTube channel. || Moon2024TSE_Thumbnail.jpg (1920x1080) [220.8 KB] || Moon2024TSE_Thumbnail_print.jpg (1024x576) [79.4 KB] || Moon2024TSE_Thumbnail_searchweb.png (320x180) [22.0 KB] || Moon2024TSE_Thumbnail_thm.png (80x40) [2.6 KB] || 14527_Moonand2024TSE_YouTubeHD.mp4 (1920x1080) [397.1 MB] || 14527_Moonand2024TSE_MASTER.mov (1920x1080) [2.8 GB] || 14527_Moonand2024TSE_TwitterX.mp4 (1280x720) [397.5 MB] || 14527_Moonand2024TSE_YouTubeHD.webm (1920x1080) [27.9 MB] || 14527_Moonand2024TSE_CAPTIONS.en_US.srt [5.7 KB] || 14527_Moonand2024TSE_CAPTIONS.en_US.vtt [5.4 KB] || ",
            "hits": 194
        },
        {
            "id": 5222,
            "url": "https://svs.gsfc.nasa.gov/5222/",
            "result_type": "Visualization",
            "release_date": "2024-02-20T12:07:00-05:00",
            "title": "5000 Years of Total Solar Eclipses",
            "description": "A heatmap showing the frequency of total solar eclipses over the 5000 years from 2000 BCE to 3000 CE. Includes versions without the color key and without the continent outlines. || eclipse_freq_heatmap_print.jpg (1024x512) [323.0 KB] || eclipse_freq_heatmap_searchweb.png (320x180) [120.8 KB] || eclipse_freq_heatmap_thm.png (80x40) [17.8 KB] || eclipse_freq_heatmap.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_nocbar.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_noland.tif (5400x2700) [17.0 MB] || ",
            "hits": 910
        },
        {
            "id": 5219,
            "url": "https://svs.gsfc.nasa.gov/5219/",
            "result_type": "Visualization",
            "release_date": "2024-02-13T09:00:00-05:00",
            "title": "2024 Path of Totality",
            "description": "This visualization closely follows the Moon's umbra shadow as it crosses North America during the April 8, 2024 total solar eclipse. It covers the one hour and 50 minutes between 10:57 a.m. Pacific Standard Time and 4:47 p.m. Atlantic Daylight Time. Annotations include a running clock and the location of the center of the shadow. Everyone within the dark oval sees totality. || flyover.2101_print.jpg (1024x576) [348.8 KB] || flyover.2101_searchweb.png (180x320) [129.1 KB] || flyover.2101_thm.png (80x40) [7.6 KB] || text (1920x1080) [0 Item(s)] || eclipse2024_flyover_720p30.mp4 (1280x720) [59.2 MB] || eclipse2024_flyover_1080p30.mp4 (1920x1080) [108.3 MB] || eclipse2024_flyover_360p30.mp4 (640x360) [24.3 MB] || text (3840x2160) [0 Item(s)] || eclipse2024_flyover_2160p30.mp4 (3840x2160) [360.5 MB] || eclipse2024_flyover_1080p30.mp4.hwshow [193 bytes] || ",
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        {
            "id": 14520,
            "url": "https://svs.gsfc.nasa.gov/14520/",
            "result_type": "Produced Video",
            "release_date": "2024-02-08T08:00:00-05:00",
            "title": "NASA's 2024 Total Solar Eclipse Broadcast (Official Trailer)",
            "description": "On April 8, 2024,  a total solar eclipse will travel through Mexico, cross the United States from Texas to Maine, and exit North America along Canada’s coast. A total solar eclipse occurs when the Moon passes between the Sun and Earth and briefly covers the full disk of the Sun. This reveals the Sun’s wispy, white outer atmosphere, called the corona.Weather permitting, people throughout most of North and Central America, including all of the contiguous United States, will be able to view at least a partial solar eclipse. A partial solar eclipse is when the Moon only covers part of the Sun. People in Hawaii and parts of Alaska will also experience a partial solar eclipse. Click here to learn more about when and where the solar eclipse will be visible: go.nasa.gov/Eclipse2024MapWARNING: Except during the brief total phase of a total solar eclipse, when the Moon completely blocks the Sun’s bright face, it is not safe to look directly at the Sun without specialized eye protection for solar viewing. Indirect viewing methods, such as pinhole projectors, can also be used to experience an eclipse. For more on how to safely view this eclipse: go.nasa.gov/Eclipse2024SafetyNot in the path of the eclipse? Watch with us from anywhere in the world. We will provide live broadcast coverage on April 8 from 1:00 p.m. to 4:00 p.m. EDT (17:00 to 20:00 UTC) on NASA TV, NASA.gov, the NASA app, and on YouTube.Learn more about the upcoming total solar eclipse: go.nasa.gov/Eclipse2024 || ",
            "hits": 231
        },
        {
            "id": 31275,
            "url": "https://svs.gsfc.nasa.gov/31275/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-02-03T00:00:00-05:00",
            "title": "NASA’s Laser Communications Experiment Streamed From Deep Space",
            "description": "This 15-second ultra-high-definition video featuring a cat named Taters was streamed via laser from deep space by NASA on Dec. 11, 2023. The video was inspired by the first television test broadcast of Felix the Cat in 1928, and the influence that cat videos have had on popular culture. It was part of the technology demonstration known as Deep Space Optical Communications (DSOC), which is attached to the Psyche spacecraft traveling to the asteroid belt between Mars and Jupiter.Uploaded before launch, the short ultra-high definition video features an orange tabby cat named Taters, the pet of a JPL employee, chasing a laser pointer, with overlayed graphics. The graphics illustrate several features from the tech demo, such as Psyche’s orbital path, Palomar’s telescope dome, and technical information about the laser and its data bit rate. Tater’s heart rate, color, and breed are also on display. || ",
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        },
        {
            "id": 14519,
            "url": "https://svs.gsfc.nasa.gov/14519/",
            "result_type": "Produced Video",
            "release_date": "2024-02-02T16:00:00-05:00",
            "title": "AMS Media Briefing: The 2024 Total Solar Eclipse & NASA",
            "description": "On Wednesday, Jan. 31, 2024, at the 104th American Meteorological Society Annual Meeting, NASA scientists participated in an informative media briefing about the April 8, 2024, total solar eclipse. In this briefing, panelists discussed what viewers can see across the path of totality, how they can safely watch the eclipse, and at-home activities to learn about and watch the eclipse. NASA scientists also shared a unique perspective on what it means to see this eclipse during solar maximum, when the Sun is at a period of high activity, as well as the parallels between space weather and meteorology, and space weather’s impact on Earth. || ",
            "hits": 37
        },
        {
            "id": 5212,
            "url": "https://svs.gsfc.nasa.gov/5212/",
            "result_type": "Visualization",
            "release_date": "2024-01-20T00:00:00-05:00",
            "title": "April 8, 2024 Total Solar Eclipse Path for Spherical Displays",
            "description": "A map-like view of the Earth during the total solar eclipse of April 8, 2024, showing the umbra (small black oval), penumbra (purple outline), and the path of totality (red). This equirectangular projection is suitable for spherical displays and for spherical mapping in 3D animation software. || eclipse.0850_print.jpg (1024x512) [122.8 KB] || eclipse.0850_searchweb.png (320x180) [72.5 KB] || eclipse.0850_thm.png (80x40) [6.2 KB] || eclipse_sos_1024p30.mp4 (2048x1024) [21.4 MB] || eclipse_sos_2048p30.mp4 (4096x2048) [64.0 MB] || 4096x2048_2x1_30p (4096x2048) [0 Item(s)] || eclipse_sos_256p30.mp4 (512x256) [2.1 MB] || eclipse_sos_512p30.mp4 (1024x512) [6.8 MB] || ",
            "hits": 295
        },
        {
            "id": 14491,
            "url": "https://svs.gsfc.nasa.gov/14491/",
            "result_type": "Produced Video",
            "release_date": "2023-12-26T00:00:00-05:00",
            "title": "Roman Hardware Highlights",
            "description": "This video, covering the second half of 2025, opens with a person entering NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.The outside half of Roman, called OSD, contains the solar panels and protective layers. The Deployable Aperture Cover, which protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space. Then the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool.In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right, and forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as they anticipated.While these tests occur, Roman’s inside half, containing the mirrors, instruments and support equipment, move into Goddard’s largest thermal vacuum chamber, the SES (Space Environment Simulator). This 40-foot-tall chamber can simulate the vacuum of space and the wide temperature range that Roman will experience there: from -310° Fahrenheit (-190° C) to 302° Fahrenheit (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned both horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.Music credit: “Our Journey Begins,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_SummerFall2025_3.jpg (1280x720) [473.7 KB] || Roman_HH_Summer-Fall2025_10mbps.mp4 (1920x1080) [185.0 MB] || Roman_HH_Summer-Fall2025_25mbps.mp4 (1920x1080) [452.7 MB] || Roman_HH_Summer-Fall2025_YT.mp4 (1920x1080) [880.2 MB] || RomanHHLate2025Captions.en_US.srt [588 bytes] || RomanHHLate2025Captions.en_US.vtt [570 bytes] || Roman_HH_Summer-Fall2025_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || ",
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        },
        {
            "id": 14399,
            "url": "https://svs.gsfc.nasa.gov/14399/",
            "result_type": "Produced Video",
            "release_date": "2023-12-20T11:00:00-05:00",
            "title": "Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky",
            "description": "From solar flares to black hole jets: NASA’s Fermi Gamma-ray Space Telescope has produced a unique time-lapse tour of the dynamic high-energy sky. Fermi Deputy Project Scientist Judy Racusin narrates this movie, which compresses 14 years of gamma-ray observations into 6 minutes. Credit: NASA’s Goddard Space Flight Center and NASA/DOE/LAT CollaborationMusic: \"Expanding Shell\" written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Video descriptive text available. || Fermi_14Year_Narrated_Still_print.jpg (1024x576) [157.6 KB] || Fermi_14Year_Narrated_Still.jpg (3840x2160) [891.9 KB] || Fermi_14Year_Narrated_Still_searchweb.png (320x180) [39.2 KB] || Fermi_14Year_Narrated_Still_thm.png (80x40) [4.2 KB] || 14399_Fermi_14Year_Narrated_sub100.mp4 (1920x1080) [90.5 MB] || 14399_Fermi_14Year_Narrated_1080.webm (1920x1080) [49.4 MB] || 14399_Fermi_14Year_Narrated_1080.mp4 (1920x1080) [908.7 MB] || Fermi_14Year_Narrated_SRT_Captions.en_US.srt [8.4 KB] || Fermi_14Year_Narrated_SRT_Captions.en_US.vtt [8.0 KB] || 14399_Fermi_14Year_Narrated_4k.mp4 (3840x2160) [2.2 GB] || 14399_Fermi_14Year_Narrated_ProRes_3840x2160_2997.mov (3840x2160) [19.4 GB] || ",
            "hits": 101
        },
        {
            "id": 14483,
            "url": "https://svs.gsfc.nasa.gov/14483/",
            "result_type": "B-Roll",
            "release_date": "2023-12-18T00:00:00-05:00",
            "title": "Aerial Views of Goddard: Buildings 21 and 11",
            "description": "This sequence shows the northeast corner of Building 21, with the Goddard Library, near sunset and in fall colors, looking southwest. The first shot approaches the building horizontally at low altitude. The next shows a descent from moderate altitude, with Building 11 visible in the background; the following shot shows a rise to similar height and a similar descent. The next shot features a slow descent from several hundred feet, looking southwest into the sun and toward Building 11, followed by an ascent at similar pace and height. Captured Nov.14, 2023. Credit: NASA/Francis Reddy || Building_21_Library_Corner_Sunset_Still.jpg (3840x2160) [2.3 MB] || Building_21_Library_Corner_Sunset_Still_searchweb.png (320x180) [85.5 KB] || Building_21_Library_Corner_Sunset_Still_thm.png (80x40) [6.2 KB] || Goddard_Bldg21CornerSunset_clips_11132023_1080_30_15mbps.mp4 (1920x1080) [383.1 MB] || Goddard_Bldg21CornerSunset_clips_11132023_4k60_25mbps.mp4 (3840x2160) [638.6 MB] || Goddard_Bldg21CornerSunset_clips_11132023_4k60_100mbps.mp4 (3840x2160) [2.5 GB] || ",
            "hits": 21
        },
        {
            "id": 14484,
            "url": "https://svs.gsfc.nasa.gov/14484/",
            "result_type": "B-Roll",
            "release_date": "2023-12-18T00:00:00-05:00",
            "title": "Aerial Views of Goddard: Miscellaneous",
            "description": "Views in the vicinity of the pond and wooded area in the northwest of Goddard's campus. The first sequence is an ascent, followed by a  descent, looking northwest. The next clip flies horizontally across the pond at low altitude. The following clip transitions from a position just above the pond, flying southeast, and rises to reveal Buildings 20, 28, and the broader Goddard campus. The next shot flies the same path in reverse at slower speed. Credit: NASA/Francis Reddy || Goddard_Pond_Still.jpg (3840x2160) [3.4 MB] || Goddard_Pond_Still_searchweb.png (320x180) [106.0 KB] || Goddard_Pond_Still_thm.png (80x40) [6.8 KB] || Goddard_Pond_clips_11092023_1080_30_15mbps.mp4 (1920x1080) [459.2 MB] || Goddard_Pond_clips_11092023_4k60_25mbps.mp4 (3840x2160) [765.3 MB] || Goddard_Pond_clips_11092023_4k60_100mbps.mp4 (3840x2160) [3.0 GB] || ",
            "hits": 16
        },
        {
            "id": 14474,
            "url": "https://svs.gsfc.nasa.gov/14474/",
            "result_type": "Produced Video",
            "release_date": "2023-12-08T11:00:00-05:00",
            "title": "A Tour of NASA’s 2024 Total Solar Eclipse Map",
            "description": "On April 8, 2024, a total solar eclipse will cross North America, passing over Mexico, the United States, and Canada. A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. The sky will darken as if it were dawn or dusk, and those standing in the path of totality may see the Sun’s outermost atmosphere (the corona) if weather permits.A map developed using data from a variety of NASA sources shows the total eclipse path as a dark band. Outside this path, purple lines indicate how much of the Sun will become covered by the Moon during the partial eclipse.This video shows different areas of the map, explaining these and other features that describe what observers across the country can expect to see during the total eclipse. Explore and download the eclipse map here. || ",
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        },
        {
            "id": 5186,
            "url": "https://svs.gsfc.nasa.gov/5186/",
            "result_type": "Visualization",
            "release_date": "2023-11-13T08:00:00-05:00",
            "title": "Flying Around The 2024 Eclipse Shadow",
            "description": "The virtual camera flies from the night side of the Earth and Moon to the day side, revealing the path of the Moon's shadow during the April 8, 2024, total solar eclipse. Includes narration by the visualizer.Music provided by Universal Production Music: “ Bright Determination” – Julien VonarbThis video can also be viewed on the NASA Goddard YouTube channel. || flyaround.0900.n_print.jpg (1024x576) [196.9 KB] || eclipse24_flyaround_narrated.mp4 (1920x1080) [85.2 MB] || eclipse24_flyaround_narrated.webm (1920x1080) [6.2 MB] || eclipse24_flyaround_narrated_prores.mov (1920x1080) [626.7 MB] || eclipse24_flyaround_captions.en-US.en_US.srt [1.2 KB] || eclipse24_flyaround_captions.en-US.en_US.vtt [1.1 KB] || eclipse24_flyaround_narrated.mp4.hwshow || ",
            "hits": 265
        },
        {
            "id": 14450,
            "url": "https://svs.gsfc.nasa.gov/14450/",
            "result_type": "Produced Video",
            "release_date": "2023-11-01T12:00:00-04:00",
            "title": "NASA Annular Eclipse Imagery",
            "description": "On Oct. 14, 2023, an annular solar eclipse crossed North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere experienced this eclipse.An annular solar eclipse happens when the Moon passes between the Sun and Earth while it is at or near its farthest point from Earth. Because the Moon is farther away from Earth than usual, it appears smaller than the Sun and does not completely cover the Sun's disk. Because of this, the Sun will appear like a “ring of fire” in the sky for those in the path of annularity.During an annular eclipse, it is never safe to look directly at the Sun without specialized eye protection designed for solar viewing.To learn more about eclipses visit: science.nasa.gov/eclipses. || ",
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        },
        {
            "id": 14401,
            "url": "https://svs.gsfc.nasa.gov/14401/",
            "result_type": "Produced Video",
            "release_date": "2023-10-31T10:00:00-04:00",
            "title": "NASA’s Eclipse Art",
            "description": "“The greatest scientists are artists as well.” ~Albert EinsteinArt and science have been treated as separate disciplines but have more in common than is often realized. Creativity is critical to making scientific breakthroughs, and art is often an expression (or product) of scientific knowledge. And both art and science begin in the experience of awe, of beholding something grand. The experience of a solar eclipse is a prime example of where these two human endeavors meet.Eclipses are celestial events we can predict with extreme precision, and their occurrence reveals fundamental truths about our place in the universe. Yet, as many eclipse watchers will attest, there is no anticipating how you will feel when experiencing one. The emotional resonance of eclipses is underlined by their presence in artforms in cultures across the world going back millennia.To celebrate the special role of eclipses in connecting art and science, creatives across NASA will be sharing their eclipse-inspired artwork in anticipation of two solar eclipses that will cross the United States on October 14, 2023, and April 8, 2024.The first two pieces in the series are presented below, with short biographies of their creators. || ",
            "hits": 82
        },
        {
            "id": 40502,
            "url": "https://svs.gsfc.nasa.gov/gallery/2024total-solar-eclipse-gallery/",
            "result_type": "Gallery",
            "release_date": "2023-10-31T00:00:00-04:00",
            "title": "2024 Total Solar Eclipse",
            "description": "On April 8, 2024, a total solar eclipse will cross North America, passing over Mexico, the United States, and Canada. A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. The sky will darken as if it were dawn or dusk.A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. People viewing the eclipse from locations where the Moon’s shadow completely covers the Sun – known as the path of totality – will experience a total solar eclipse. The sky will darken, as if it were dawn or dusk. Weather permitting, people along the path of totality will see the Sun’s corona, or outer atmosphere, which is usually obscured by the bright face of the Sun.Learn more about this total solar eclipse: solarsystem.nasa.gov/eclipses/2024\n",
            "hits": 398
        },
        {
            "id": 14446,
            "url": "https://svs.gsfc.nasa.gov/14446/",
            "result_type": "Produced Video",
            "release_date": "2023-10-27T11:00:00-04:00",
            "title": "The Ring of Fire: 2023 Annular Solar Eclipse (NASA Recap)",
            "description": "On Oct. 14, 2023, an annular solar eclipse crossed North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere were able to experience this “ring of fire” eclipse. NASA’s official broadcast and outreach teams were located in Kerrville, TX, and Albuquerque, NM, to capture the event and celebrate with the communities in the path of annularity. For more information: • Official NASA Broadcast• Interactive Eclipse Map Explorer || ",
            "hits": 105
        },
        {
            "id": 14430,
            "url": "https://svs.gsfc.nasa.gov/14430/",
            "result_type": "Produced Video",
            "release_date": "2023-10-14T13:00:00-04:00",
            "title": "Capturing the Sounds of a Solar Eclipse",
            "description": "In April 2024, volunteers can join the Eclipse Soundscapes project to help NASA scientists better understand how wildlife is impacted by solar eclipses. Volunteers will gather sound recordings, make observations using any of their senses, and even help with data analysis from across the path of the eclipse. This video features interviews from Eclipse Soundscapes experts MaryKay Severino, Dr. William “Trae” Winter III, and Dr. William Oestreich, and highlights natural resource manager Dr. Chace Holzhueser at Hot Springs National Park in Arkansas, who will be conducting a similar study for the total solar eclipse on April 8, 2024.Visit https://science.nasa.gov/eclipses/citizen-science/ to learn more! || ",
            "hits": 35
        },
        {
            "id": 14424,
            "url": "https://svs.gsfc.nasa.gov/14424/",
            "result_type": "Produced Video",
            "release_date": "2023-10-12T21:00:00-04:00",
            "title": "NASA Interview Opportunity: Ring of Fire THIS Weekend With Annular Solar Eclipse",
            "description": "Associated cut broll for the live shots will be added by 4:00 p.m. EST on Thursday, Oct 12 || english_final.png (7560x2484) [3.0 MB] || english_final_print.jpg (1024x336) [84.8 KB] || english_final_searchweb.png (320x180) [40.8 KB] || english_final_thm.png (80x40) [5.5 KB] || ",
            "hits": 64
        },
        {
            "id": 31244,
            "url": "https://svs.gsfc.nasa.gov/31244/",
            "result_type": "Hyperwall Visual",
            "release_date": "2023-09-25T00:00:00-04:00",
            "title": "OSIRIS-REx Tags Asteroid Bennu Videos",
            "description": "Touch-And-Go (TAG) sample collection || osiris-rex-tag_1000_print.jpg (1024x576) [124.1 KB] || osiris-rex-tag_1000_searchweb.png (320x180) [78.7 KB] || osiris-rex-tag_1000_thm.png (80x40) [5.0 KB] || osiris-rex-tag_1080p30.mp4 (1920x1080) [10.3 MB] || osiris-rex-tag_1080p30.webm (1920x1080) [1.4 MB] || osiris-rex-tag_2160p30.mp4 (3840x2160) [29.9 MB] || tag (3840x2160) [0 Item(s)] || ",
            "hits": 247
        },
        {
            "id": 14416,
            "url": "https://svs.gsfc.nasa.gov/14416/",
            "result_type": "B-Roll",
            "release_date": "2023-09-24T09:00:00-04:00",
            "title": "OSIRIS-REx Sample Return Broadcast Media",
            "description": "On September 24, 2023, NASA’s OSIRIS-REx spacecraft delivered a sample of the pristine asteroid Bennu to Earth. Its sample return capsule, containing rocks and dust collected from Bennu, touched down at the Department of Defense Utah Test and Training Range shortly before 9:00 am, Mountain Time. This page contains video packages and graphics that were broadcast by NASA during the event. View the OSIRIS-REx Sample Return Broadcast and Landing Highlights. || ",
            "hits": 201
        },
        {
            "id": 40500,
            "url": "https://svs.gsfc.nasa.gov/gallery/annular-solar-eclipse2023/",
            "result_type": "Gallery",
            "release_date": "2023-09-19T00:00:00-04:00",
            "title": "2023 Annular Solar Eclipse",
            "description": "On Oct. 14, 2023, an annular solar eclipse will cross North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere can experience this eclipse.\n\nAn annular solar eclipse happens when the Moon passes between the Sun and Earth while it is at or near its farthest point from Earth. Because the Moon is farther away from Earth than usual, it appears smaller than the Sun and does not completely cover the star. Because of this, the Sun will appear like a “ring of fire” in the sky for those in the path of annularity.\n\nDuring an annular eclipse, it is never safe to look directly at the Sun without specialized eye protection designed for solar viewing.\n\nLearn more about this annular solar eclipse: solarsystem.nasa.gov/eclipses/2023",
            "hits": 134
        },
        {
            "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": 334
        },
        {
            "id": 40507,
            "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/",
            "result_type": "Gallery",
            "release_date": "2023-08-28T00:00:00-04:00",
            "title": "Hyperwall Power Playlist - Heliophysics 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": 189
        },
        {
            "id": 14374,
            "url": "https://svs.gsfc.nasa.gov/14374/",
            "result_type": "Infographic",
            "release_date": "2023-08-03T11:00:00-04:00",
            "title": "A Guide to Cosmic Temperatures",
            "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ",
            "hits": 1061
        },
        {
            "id": 14385,
            "url": "https://svs.gsfc.nasa.gov/14385/",
            "result_type": "Produced Video",
            "release_date": "2023-07-20T10:00:00-04:00",
            "title": "OSIRIS-REx Returns – Teaser",
            "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Path of a Hero\" Caleb Jordan Swift of Universal Production Music. || OREX_PROMO_FINAL_SEP24.00867_print.jpg (1024x576) [182.9 KB] || OREX_PROMO_FINAL_SEP24.00867_searchweb.png (320x180) [75.6 KB] || OREX_PROMO_FINAL_SEP24.00867_thm.png (80x40) [6.1 KB] || OREX_PROMO_FINAL.en_US.srt [587 bytes] || OREX_PROMO_FINAL.en_US.vtt [565 bytes] || OREX_PROMO_14385.mp4 (3840x2160) [44.4 MB] || ",
            "hits": 89
        },
        {
            "id": 5123,
            "url": "https://svs.gsfc.nasa.gov/5123/",
            "result_type": "Visualization",
            "release_date": "2023-07-10T14:00:00-04:00",
            "title": "The 2024 Total Solar Eclipse",
            "description": "This page is also available in the following languages:Tagalog (Wikang Tagalog)Vietnamese (tiếng Việt)Simplified Chinese (汉语)Traditional Chinese (漢語)Arabic (بهاس ملايو)Korean (한국어) || ",
            "hits": 640
        },
        {
            "id": 5124,
            "url": "https://svs.gsfc.nasa.gov/5124/",
            "result_type": "Visualization",
            "release_date": "2023-07-10T14:00:00-04:00",
            "title": "The 2023 Annular Solar Eclipse",
            "description": "The path of annularity and partial contours crossing the U.S. for the 2023 annular solar eclipse occurring on October 14, 2023. || eclipse_map_2023_QR_1920.png (1920x960) [3.4 MB] || eclipse_map_2023_QR_10800.png (10800x5400) [77.3 MB] || eclipse_map_2023_QR_5400.png (5400x2700) [23.1 MB] || eclipse_map_2023_QR_1920_searchweb.png (320x180) [111.9 KB] || eclipse_map_2023_QR_1920_thm.png (80x40) [7.2 KB] || eclipse_map_2023_QR.png (22500x11250) [129.8 MB] || the-2023-annular-solar-eclipse.hwshow [302 bytes] || ",
            "hits": 107
        },
        {
            "id": 14282,
            "url": "https://svs.gsfc.nasa.gov/14282/",
            "result_type": "Produced Video",
            "release_date": "2023-05-17T11:00:00-04:00",
            "title": "Spitzer, TESS Find Potential Earth-Size World Covered in Volcanoes",
            "description": "LP 791-18 d, illustrated here in an artist's concept, is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system. Astronomers discovered and studied the planet using data from NASA’s Spitzer Space Telescope and TESS (Transiting Exoplanet Survey Satellite) along with many other observatories.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || LP79118d_BeautyShot.jpg (2048x1152) [130.9 KB] || LP79118d_Temperate_Earth_BeautyShot_Full.jpg (5760x3240) [2.2 MB] || LP79118d_Temperate_Earth_BeautyShot_Full.png (5760x3240) [12.4 MB] || LP79118d_BeautyShot_searchweb.png (320x180) [59.9 KB] || LP79118d_BeautyShot_thm.png (80x40) [5.1 KB] || ",
            "hits": 61
        },
        {
            "id": 14309,
            "url": "https://svs.gsfc.nasa.gov/14309/",
            "result_type": "Produced Video",
            "release_date": "2023-03-15T11:00:00-04:00",
            "title": "Fermi Captures Dynamic Gamma-ray Sky",
            "description": "Watch a cosmic gamma-ray fireworks show in this animation using just a year of data from the Large Area Telescope (LAT) aboard NASA’s Fermi Gamma-ray Space Telescope. Each object’s magenta circle grows as it brightens and shrinks as it dims. The yellow circle represents the Sun following its apparent annual path across the sky. The animation shows a subset of the LAT gamma-ray records now available for more than 1,500 objects in a new, continually updated repository. Over 90% of these sources are a type of galaxy called a blazar, powered by the activity of a supermassive black hole.Credit: NASA’s Marshall Space Flight Center/Daniel Kocevski || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_ProRes_3840x2160.mov (3840x2160) [170.3 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1600.gif (1600x900) [6.5 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1050.gif (1050x590) [3.2 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark.gif (800x450) [2.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.mp4 (3840x2160) [12.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.webm (3840x2160) [1.9 MB] || ",
            "hits": 108
        },
        {
            "id": 5073,
            "url": "https://svs.gsfc.nasa.gov/5073/",
            "result_type": "Visualization",
            "release_date": "2023-03-08T14:00:00-05:00",
            "title": "The 2023 and 2024 Solar Eclipses: Map and Data",
            "description": "The map was updated on March 15, 2023, to correct times in Mexico along the total eclipse path. || ",
            "hits": 1000
        },
        {
            "id": 5086,
            "url": "https://svs.gsfc.nasa.gov/5086/",
            "result_type": "Visualization",
            "release_date": "2023-03-08T14:00:00-05:00",
            "title": "A Tour of NASA’s Solar Eclipse Map for 2023 and 2024",
            "description": "The map was updated on March 15, 2023, to correct times in Mexico along the total eclipse path.Two solar eclipses will cross the United States in 2023 and 2024. On October 14, 2023, an annular solar eclipse will create a “ring of fire” in the sky from Oregon to Texas. On April 8, 2024, a total solar eclipse will darken the skies from Texas to Maine. On both dates, all 48 contiguous states in the U.S. will experience a partial solar eclipse. || ",
            "hits": 137
        },
        {
            "id": 14230,
            "url": "https://svs.gsfc.nasa.gov/14230/",
            "result_type": "Produced Video",
            "release_date": "2022-11-01T08:00:00-04:00",
            "title": "Skywatcher’s Delight: Find out how you can catch the Nov. 8 total lunar eclipse",
            "description": "Click here to find out everything you need to know about Tuesday's LUNAR ECLIPSE Click here for quick link to table of ECLIPSE TIMESClick here for quick link to canned interview in Spanish with Francisco AndolzQuick link to edited B-ROLL for interviewsClick here for a quick link to a canned interview with Noah Petro || What_you_need_to_know_about_next_weeks_lunar_eclipse.jpg (6912x3456) [1.6 MB] || What_you_need_to_know_about_next_weeks_lunar_eclipse_print.jpg (1024x512) [89.3 KB] || What_you_need_to_know_about_next_weeks_lunar_eclipse_searchweb.png (320x180) [57.2 KB] || What_you_need_to_know_about_next_weeks_lunar_eclipse_thm.png (80x40) [6.5 KB] || ",
            "hits": 175
        },
        {
            "id": 5038,
            "url": "https://svs.gsfc.nasa.gov/5038/",
            "result_type": "Visualization",
            "release_date": "2022-10-05T16:15:00-04:00",
            "title": "The Sun's Path at Different Lunar Latitudes",
            "description": "The path of the Sun in the lunar sky is shown at four latitudes, including the South Pole. An arrow points toward the Sun. Annotations include the subsolar longitude and the elapsed time in Earth days. || moon.0330_print.jpg (1024x576) [135.4 KB] || moon.0330_searchweb.png (320x180) [76.0 KB] || moon.0330_thm.png (80x40) [5.9 KB] || sun_paths_1080p30.mp4 (1920x1080) [18.0 MB] || sun_paths_720p30.mp4 (1280x720) [8.8 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || sun_paths_720p30.webm (1280x720) [4.5 MB] || sun_paths_360p30.mp4 (640x360) [3.0 MB] || sun_paths_1080p30.mp4.hwshow [183 bytes] || ",
            "hits": 1016
        },
        {
            "id": 31194,
            "url": "https://svs.gsfc.nasa.gov/31194/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-10-04T00:00:00-04:00",
            "title": "DART: Double Asteroid Redirection Test",
            "description": "The DART mission is NASA's demonstration of kinetic impactor technology, impacting an asteroid to adjust its speed and path. DART was the first-ever space mission to demonstrate asteroid deflection by kinetic impactor. It impacted the moonlet Dimorphos on September 26, 2022. || ",
            "hits": 289
        },
        {
            "id": 14215,
            "url": "https://svs.gsfc.nasa.gov/14215/",
            "result_type": "Produced Video",
            "release_date": "2022-09-29T12:15:00-04:00",
            "title": "Hubble Views Aftermath of DART Impact",
            "description": "The DART mission will deploy a kinetic impactor to smack the small moon Dimorphos of the asteroid Didymos on the evening of Sept. 26. This is an on-orbit demonstration of asteroid deflection, a key test of NASA's kinetic impactor technology, designed to impact an asteroid to adjust its speed and path.  This particular asteroid moon is NOT a threat to Earth, but is technology being explored to use for when we DO find a potentially hazardous asteroid.The Hubble Space Telescope captured these extraordinary views of the asteroid moon soon after the successful impact.For more information, visit https://nasa.gov/hubble. Music & Sound“The Beauty Beyond” by Jeremy Noel William Abbott [PRS] and Vasco [PRS] via Freshworx Music Limited [PRS] and Universal Production Music || ",
            "hits": 111
        },
        {
            "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": 119
        },
        {
            "id": 31183,
            "url": "https://svs.gsfc.nasa.gov/31183/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-04-07T00:00:00-04:00",
            "title": "Typhoon Surigae Rain Rate and Accumulation",
            "description": "This animation shows the rain rates (blue/yellow shading) and accumulations (green/purple shading) produced by Typhoon Surigae from April 12-25, 2021, estimated by NASA's Integrated Multi-satellitE Retrievals for GPM (IMERG) algorithm. Cloudiness is shown in shades of white/gray below the rain rates, based on geosynchronous satellite infrared observations. Surigae's intensity is shown by the multi-colored line, based on estimates by the U.S. Navy-Air Force Joint Typhoon Warning Center (JTWC) using the Saffir-Simpson hurricane wind scale from 1 to 5. Typhoon Surigae formed over the Western Pacific Ocean on April 13, 2021, intensifying to a Category 1-equivalent storm by April 16 as it passed north of Palau. Surigae continued to intensify as it approached the Philippines, reaching Category-5 intensity by April 17 before gradually weakening as its path recurved to the northeast. Although Surigae didn't make landfall, it left heavy rainfall accumulations in its path, including over Palau, which IMERG estimated received over 300 millimeters (12 inches) of rainfall during the period of the animation. Local rain gauges showed similar accumulations during the same period of time.NASA's IMERG product is a multi-satellite global estimate of rainfall produced in near real-time at half-hourly intervals. The global span of IMERG covers the oceans as well as land areas, which is a major advantage over ground-based radar and rain gauge measurements. IMERG allows atmospheric scientists to study extreme weather events, such as typhoons, and better understand the mechanisms that drive them, leading to better preparedness for future events. || ",
            "hits": 49
        },
        {
            "id": 14118,
            "url": "https://svs.gsfc.nasa.gov/14118/",
            "result_type": "B-Roll",
            "release_date": "2022-03-16T10:00:00-04:00",
            "title": "NASA’s Webb Reaches Alignment Milestone, Optics Working Successfully",
            "description": "NASA’s Webb Reaches Alignment Milestone, Optics Working SuccessfullyFollowing the completion of critical mirror alignment steps, the James Webb Space Telescope team has great confidence that the observatory’s optical performance will meet or exceed the science goals it was built to achieve.On March 11, the Webb team completed the stage of alignment known as “fine phasing” – and at this key stage in the commissioning of Webb’s Optical Telescope Element, every optical parameter that has been checked and tested is performing at, or above, expectations. The team found no critical issues and no measurable contamination or blockages to Webb’s optical path. The observatory is able to successfully gather light from distant objects and deliver it to its instruments without issue.Although there are months to go before Webb ultimately delivers its new view of the cosmos, achieving this milestone means the team is confident that Webb’s first-of-its-kind optical system is working as well as possible.Music Credit:  Emerging Discovery Instrumental by Carter / Universal Production Music || ",
            "hits": 37
        },
        {
            "id": 14111,
            "url": "https://svs.gsfc.nasa.gov/14111/",
            "result_type": "Produced Video",
            "release_date": "2022-02-28T07:00:00-05:00",
            "title": "Webb's Mid-Infrared Instrument (MIRI) Light Path Animation",
            "description": "The spectrograph light path inside the Mid Infrared Instrument (MIRI) on the Webb Telescope.  Versions with labels and without labels.Credit:  European Space Agency || MIRI_SPECTRO_v2.00030_print.jpg (1024x576) [40.5 KB] || MIRI_SPECTRO_v2.00030_searchweb.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_web.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_thm.png (80x40) [2.1 KB] || MIRI_SPECTRO_v2.mp4 (1920x1080) [156.3 MB] || MIRI_SPECTRO_labels_v3.mp4 (1920x1080) [177.9 MB] || MIRI_SPECTRO_v2.webm (1920x1080) [9.0 MB] || ",
            "hits": 65
        },
        {
            "id": 14112,
            "url": "https://svs.gsfc.nasa.gov/14112/",
            "result_type": "Produced Video",
            "release_date": "2022-02-28T07:00:00-05:00",
            "title": "Webb's Near Infrared Spectrograph (NIRSpec) Instrument Light Path Animation",
            "description": "Animation of the light path inside the Near Infrared Spectrometer (NIRSpec) on the Webb Telescope.  Showing simulated data.Credit:  European Space Agency || NIRSPEC_IFU_with_graph_v3.00030_print.jpg (1024x576) [39.9 KB] || NIRSPEC_IFU_with_graph_v3.00030_searchweb.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_web.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_thm.png (80x40) [2.1 KB] || NIRSPEC_IFU_with_graph_v3.mp4 (1920x1080) [311.7 MB] || NIRSPEC_IFU_with_graph_v3.webm (1920x1080) [12.7 MB] || ",
            "hits": 57
        },
        {
            "id": 14098,
            "url": "https://svs.gsfc.nasa.gov/14098/",
            "result_type": "Produced Video",
            "release_date": "2022-02-10T10:30:00-05:00",
            "title": "IMPACTS 2022: NASA Planes Fly into Snowstorms to Study Snowfall",
            "description": "NASA’s Investigation of Microphysics and Precipitation for Atlantic Coast-Threatening Storms (IMPACTS) mission, which began in January and is planned to wrap up at the end of February, has seen upwards of 10 flights so far. Ultimately, what the IMPACTS team learns about snowstorms will improve meteorological models and our ability to use satellite data to predict how much snow will fall and where.Music credit: “Struggles” and “Natural Time Cycles” from Universal Production MusicComplete transcript available. || Thumbnail.jpg (1920x1080) [737.2 KB] || Thumbnail_print.jpg (1024x576) [275.6 KB] || Thumbnail_searchweb.png (320x180) [100.7 KB] || IMPACTS_Final_Cut.webm (1920x1080) [21.1 MB] || IMPACTS_Final_Cut.mp4 (1920x1080) [378.3 MB] || IMPACTS_Final_1_otter_ai.en_US.srt [3.2 KB] || IMPACTS_Final_1_otter_ai.en_US.vtt [3.2 KB] || ",
            "hits": 25
        },
        {
            "id": 20354,
            "url": "https://svs.gsfc.nasa.gov/20354/",
            "result_type": "Animation",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "Animation: Origins of Switchbacks",
            "description": "On recent solar encounters, Parker Solar Probe collected data pinpointing the origin of zig-zag-shaped structures in the solar wind, called switchbacks. The data showed one spot switchbacks originate is at the visible surface of the Sun – the photosphere. By the time it reaches Earth, 93 million miles away, the solar wind is an unrelenting headwind of particles and magnetic fields. But as it escapes the Sun, the solar wind is structured and patchy. In the mid-1990s, the NASA-European Space Agency mission Ulysses flew over the Sun’s poles and discovered a handful of bizarre S-shaped kinks in the solar wind’s magnetic field lines, which detoured charged particles on a zig-zag path as they escaped the Sun. For decades, scientists thought these occasional switchbacks were oddities confined to the Sun’s polar regions.   In 2019, at 34 solar radii from the Sun, Parker Solar Probe discovered that switchbacks were not rare, but common in the solar wind. This renewed interest in the features raised new questions: Where are they coming from and how do they form and evolve? Were they forged at the surface of the Sun, or shaped by some process kinking magnetic fields in the solar atmosphere? The new findings, in press at the Astrophysical Journal, finally confirm one origin point near the solar surface. More information here. || ",
            "hits": 78
        },
        {
            "id": 40433,
            "url": "https://svs.gsfc.nasa.gov/gallery/science-ona-sphere-gallery/",
            "result_type": "Gallery",
            "release_date": "2021-11-23T00:00:00-05:00",
            "title": "Science On a Sphere Gallery",
            "description": "Content for NOAA's Science on a Sphere and related spherical display platforms.",
            "hits": 279
        },
        {
            "id": 13985,
            "url": "https://svs.gsfc.nasa.gov/13985/",
            "result_type": "Produced Video",
            "release_date": "2021-11-16T06:00:00-05:00",
            "title": "NASA Just Days Away From Launching Humanity’s First-Ever Asteroid-Deflecting Mission Live Shots",
            "description": "Click here for the DART PRESS KITClick here for B-ROLL resourcesQuick link for cut Live Shot B-ROLLClick here for quick link to CANNED INTERVIEW with Tom Statler / DART Program Scientist || DART_banner_2.png (3214x804) [3.0 MB] || DART_banner_2_print.jpg (1024x256) [74.4 KB] || DART_banner_2_searchweb.png (320x180) [78.8 KB] || DART_banner_2_thm.png (80x40) [9.8 KB] || ",
            "hits": 114
        },
        {
            "id": 13943,
            "url": "https://svs.gsfc.nasa.gov/13943/",
            "result_type": "Produced Video",
            "release_date": "2021-10-25T06:00:00-04:00",
            "title": "Ready For Liftoff! NASA and SpaceX to Launch A Four-Member Crew to the International Space Station Live Shots",
            "description": "Click here for associated B-ROLL for the live shotsClick here for canned interview with NASA Administrator Bill NelsonClick here for canned interview with Crew3 Mission Commandar Raja ChariClick here for details about Crew3 Media briefings and other schedule logistics.Click here for Crew3 Press Kit with additional canned interviews, b-roll, training video, and other material || banner3_print.jpg (1024x156) [80.5 KB] || banner3_searchweb.png (320x180) [5.8 MB] || banner3_thm.png (80x40) [5.8 MB] || banner3.tif (3034x464) [11.1 MB] || ",
            "hits": 34
        },
        {
            "id": 13944,
            "url": "https://svs.gsfc.nasa.gov/13944/",
            "result_type": "Produced Video",
            "release_date": "2021-10-14T14:00:00-04:00",
            "title": "Lucy L-2 Engineering Briefing",
            "description": "NASA will hold a virtual media briefing at 3 p.m. EDT Thursday, October 14th, to preview the engineering behind the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun. The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Lucy engineering briefing participants include:• Joan Salute, associate director for flight programs, Planetary Science Division, NASA Headquarters.• Katie Oakman, Lucy structures and mechanisms lead, Lockheed Martin Space.• Jessica Lounsbury, Lucy project systems engineer, Goddard.• Coralie Adam, deputy navigation team chief, KinetX Aerospace.Over its 12-year primary mission, Lucy will explore a record-breaking number of asteroids. The spacecraft will fly by one asteroid in the solar system’s main belt and seven Trojan asteroids. Lucy’s path will circle back to Earth three times for gravity assists, which will make it the first spacecraft ever to return to our planet’s vicinity from the outer solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida. Lucy’s principal investigator is based out of the Boulder, Colorado, branch of Southwest Research Institute (SwRI), headquartered in San Antonio, Texas. NASA’s Goddard Space Flight Center in Greenbelt, Maryland provides overall mission management, systems engineering, and safety and mission assurance. Lockheed Martin Space in Littleton, Colorado, built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the agency’s Science Mission Directorate in Washington. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida. || ",
            "hits": 28
        },
        {
            "id": 13945,
            "url": "https://svs.gsfc.nasa.gov/13945/",
            "result_type": "Produced Video",
            "release_date": "2021-10-14T10:00:00-04:00",
            "title": "Lucy L-2 Science and Instrument Briefing",
            "description": "NASA will hold a virtual media briefing at 1 p.m. EDT Thursday, October 14th, to preview the launch of the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun.The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Participants in Thursday's briefing will include:• Alana Johnson, Senior Communications Specialist, NASA Planetary Science Division• Adriana Ocampo, Lucy Program Executive, NASA Headquarters• Cathy Olkin, Lucy Deputy Principal Investigator, Southwest Research Institute   • Keith Noll, Lucy Project Scientist, NASA's Goddard Space Flight Center• Hal Weaver, L’LORRI Instrument PI, Johns Hopkins University Applied Physics Laboratory • Phil Christensen, L’TES Instrument PI, Arizona State University • Dennis Reuter, L’RALPH Instrument PI, NASA's Goddard Space Flight Center  Over its 12-year primary mission, Lucy will explore a record number of asteroids in separate orbits around the Sun. The spacecraft will fly by one asteroid in the solar system’s main belt, located between the orbits of Mars and Jupiter, followed by seven Trojans. In addition, Lucy’s path will circle back to Earth three times for gravity assists, making it the first spacecraft ever to travel out to the distance of Jupiter and return to the vicinity of Earth.The Lucy mission is named after the fossilized skeleton of an early hominin (pre-human ancestor) discovered in Ethiopia in 1974 and named “Lucy” by the team of paleoanthropologists who discovered it. Just as the Lucy fossil provided unique insights into humanity’s evolution, the Lucy mission promises to revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida.Southwest Research Institute is the home institution of the principal investigator. NASA Goddard Space provides overall mission management, systems engineering, plus safety and mission assurance. Lockheed Martin Space built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the Science Mission Directorate. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida.For more information about Lucy, visit: http://www.nasa.gov/lucy || ",
            "hits": 22
        },
        {
            "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",
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        {
            "id": 13950,
            "url": "https://svs.gsfc.nasa.gov/13950/",
            "result_type": "Produced Video",
            "release_date": "2021-10-05T06:00:00-04:00",
            "title": "NASA Just Days Away From Launching Probe To Mysterious Asteroid Belt To Explore \"Fossils\" Of The Early Solar System Live Shots",
            "description": "Quick link to edited B-ROLL for the live shotsQuick link to canned interview with Donya Douglas-Bradshaw  Lucy Project ManagerQuick link to canned interview with Cory Prykull, Lockheed Martin Space, Lucy Assembly, Test & Launch Operations Lead || Lucy_banner.png (1550x464) [1.3 MB] || Lucy_banner_print.jpg (1024x306) [134.8 KB] || Lucy_banner_searchweb.png (320x180) [139.1 KB] || Lucy_banner_thm.png (80x40) [12.5 KB] || ",
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    ]
}