{ "count": 259, "next": "http://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Flyby%22", "previous": null, "results": [ { "id": 5651, "url": "http://svs.gsfc.nasa.gov/5651/", "result_type": "Visualization", "release_date": "2026-09-23T11:00:00-04:00", "title": "Asteroid Apophis 2029 Earth Flyby – Orbit Visualizations", "description": "Orbit visualizations showing the April 2029 Earth flyby of asteroid Apophis and the OSIRIS-APEX spacecraft.", "hits": 1029 }, { "id": 15101, "url": "http://svs.gsfc.nasa.gov/15101/", "result_type": "Produced Video", "release_date": "2026-09-23T11:00:00-04:00", "title": "NASA’s OSIRIS-APEX Mission Will Explore Asteroid Apophis", "description": "NASA’s OSIRIS-APEX mission will rendezvous with Apophis in mid-2029, following the asteroid’s historically close flyby of Earth.", "hits": 827 }, { "id": 20414, "url": "http://svs.gsfc.nasa.gov/20414/", "result_type": "Animation", "release_date": "2026-09-23T11:00:00-04:00", "title": "Asteroid Apophis 2029 Earth Flyby – Animations", "description": "OSIRIS-APEX will rendezvous with asteroid Apophis in mid-2029, following its historically close flyby with Earth. || OREX_APEX_Rendezvous_1080_30fps_h264.00940_print.jpg (1024x576) [137.7 KB] || OREX_APEX_Rendezvous_1080_30fps_h264.00940_searchweb.png (320x180) [69.5 KB] || OREX_APEX_Rendezvous_1080_30fps_h264.00940_thm.png (80x40) [4.7 KB] || OREX_APEX_Rendezvous_1080_30fps_h264.mp4 (1920x1080) [40.9 MB] || OREX_APEX_Rendezvous_1080_30fps_proRes.mov (1920x1080) [524.1 MB] || OREX_APEX_Rendezvous_4k_30fps_h264.mp4 (3840x2160) [41.5 MB] || OREX_APEX_Rendezvous_4k_30fps_proRes.webm (3840x2160) [8.4 MB] || OREX_APEX_Rendezvous_4k_30fps_proRes.mov (3840x2160) [1.8 GB] || ", "hits": 997 }, { "id": 5628, "url": "http://svs.gsfc.nasa.gov/5628/", "result_type": "Visualization", "release_date": "2026-06-18T14:10:00-04:00", "title": "Lucy Observations of Asteroid Donaldjohanson", "description": "Lucy Observations of Asteroid Donaldjohanson", "hits": 176 }, { "id": 31395, "url": "http://svs.gsfc.nasa.gov/31395/", "result_type": "Hyperwall Visual", "release_date": "2026-05-30T18:59:59-04:00", "title": "Psyche Mission", "description": "Psyche is a NASA mission to study a metal-rich asteroid with the same name, located in the main asteroid belt between Mars and Jupiter. This is NASA’s first mission to study an asteroid that has more metal than rock or ice. No description available.", "hits": 287 }, { "id": 5633, "url": "http://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": 2539 }, { "id": 14934, "url": "http://svs.gsfc.nasa.gov/14934/", "result_type": "Produced Video", "release_date": "2026-03-26T16:00:00-04:00", "title": "NASA Interview Opportunity: Moonbound! 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During the 10-day past the Moon and back, the Orion capsule will fly by the far side of the Moon — the side that always faces away from Earth. During this three-hour period, astronauts will analyze and photograph geologic features, such as impact craters and ancient lava flows. They will rely on the extensive geology training they received in the classroom and in Moon-like places on Earth to describe nuances in shapes, textures, and colors — the type of information that reveals the geologic history of an area. These skills will be critical to exploring the Moon’s South Pole region through future missions.\n\nLearn more about Artemis II lunar science.\nLearn more about all Artemis II science experiments\nLearn more about the Moon at science.nasa.gov/moon.\n\n**Note: This page will be continually updated through the Artemis II mission. **\n\nMedia Contact: Lonnie Shekhtman NASA’s Goddard Space Flight Center in Greenbelt, Md.", "hits": 2612 }, { "id": 14865, "url": "http://svs.gsfc.nasa.gov/14865/", "result_type": "Produced Video", "release_date": "2025-07-10T14:00:00-04:00", "title": "The Closest Images Ever Taken of the Sun’s Atmosphere", "description": "On its record-breaking pass by the Sun in December 2024, NASA’s Parker Solar Probe captured stunning new images from within the Sun’s atmosphere. These newly released images — taken closer to the Sun than we’ve ever been before — are helping scientists better understand the Sun’s influence across the solar system, including events that can affect Earth.Parker Solar Probe started its closest approach to the Sun on Dec. 24, 2024, flying just 3.8 million miles from the solar surface. As it skimmed through the Sun’s outer atmosphere, called the corona, in the days around the perihelion, it collected data with an array of scientific instruments, including the Wide-Field Imager for Solar Probe, or WISPR.Learn more - https://science.nasa.gov/science-research/heliophysics/nasas-parker-solar-probe-snaps-closest-ever-images-to-sun/Find the latest WISPR imagery here. || ", "hits": 816 }, { "id": 5534, "url": "http://svs.gsfc.nasa.gov/5534/", "result_type": "Visualization", "release_date": "2025-06-18T11:23:00-04:00", "title": "Parker Solar Probe - Extended Mission", "description": "After it's ultimate perihelion in December 2024, the Parker Solar Probe will continue it's orbits around the Sun. This visualization presents a projection of it's current orbit through 2029.", "hits": 585 }, { "id": 31349, "url": "http://svs.gsfc.nasa.gov/31349/", "result_type": "Hyperwall Visual", "release_date": "2025-05-28T18:59:59-04:00", "title": "Juno images, 2024 - early 2025", "description": "Several recent images from the JunoCam and Jovian Infrared Auroral Mapper (JIRAM) instruments show volcanic hot spots on IO, polar storms and Jupiter's moon Amalthea.", "hits": 102 }, { "id": 14799, "url": "http://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 262 }, { "id": 14821, "url": "http://svs.gsfc.nasa.gov/14821/", "result_type": "Produced Video", "release_date": "2025-04-14T14:00:00-04:00", "title": "Lucy Will Explore Asteroid Donaldjohanson", "description": "Lucy’s flyby of main-belt asteroid 52246 Donaldjohanson will provide the first close look at this surviving remnant of the solar system’s chaotic past.Complete transcript available.Universal Production Music: “Nico’s Journey” by Nicholas Smith [PRS]; “Knowing Half the Future” and “Temporal Timings” by Lee John Gretton [PRS]; “Poly Propulsion” by Alfie Solo [PRS] Watch this video on the NASA Goddard YouTube channel. || Lucy_DJ_Preview_Thumbnail_V3_print.jpg (1024x576) [240.8 KB] || Lucy_DJ_Preview_Thumbnail_V3.png (1280x720) [1.1 MB] || Lucy_DJ_Preview_Thumbnail_V3_searchweb.png (320x180) [81.6 KB] || 14821_Lucy_Asteroid_DJ_Preview_V2_720.mp4 (1280x720) [58.1 MB] || 14821_Lucy_Asteroid_DJ_Preview_V2_1080.mp4 (1920x1080) [325.2 MB] || LucyDJPreviewCaptions.en_US.srt [5.6 KB] || LucyDJPreviewCaptions.en_US.vtt [5.3 KB] || Lucy_DJ_Preview_Thumbnail_V3_thm.png [6.5 KB] || 14821_Lucy_Asteroid_DJ_Preview_V2_4K.mp4 (3840x2160) [4.0 GB] || 14821_Lucy_Asteroid_DJ_Preview_V2_ProRes.mov (3840x2160) [25.8 GB] || ", "hits": 76 }, { "id": 20402, "url": "http://svs.gsfc.nasa.gov/20402/", "result_type": "Animation", "release_date": "2025-04-14T14:00:00-04:00", "title": "Lucy Flyby of Asteroid Donaldjohanson: Animations", "description": "Close up of Lucy's APP swiveling to keep DJ in frame. || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_print.jpg (1024x576) [79.5 KB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_searchweb.png (320x180) [48.0 KB] || LUCY_DJ_CloseUp_30fps_4k_h264_v02.mp4 (3840x2160) [73.9 MB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.00001_thm.png [4.4 KB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.webm (3840x2160) [11.9 MB] || LUCY_DJ_CloseUp_30fps_4k_proRes_v02.mov (3840x2160) [3.3 GB] || ", "hits": 78 }, { "id": 5525, "url": "http://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": 71 }, { "id": 20399, "url": "http://svs.gsfc.nasa.gov/20399/", "result_type": "Animation", "release_date": "2025-03-19T00:00:00-04:00", "title": "XMM-Newton spacecraft animations", "description": "Flyby animation of ESA's (European Space Agency's) XMM-Newton observatory as it orbits Earth.Credit: NASA/ESA || XMM_Beauty_Still.jpg (3840x2160) [449.2 KB] || XMM_Beauty_Still_searchweb.png (320x180) [38.6 KB] || XMM_Beauty_Shot_H264_V1.mp4 (3840x2160) [23.4 MB] || XMM_Beauty_Still_thm.png [3.3 KB] || XMM_Beauty_Shot_Prores_V1.mov (3840x2160) [807.2 MB] || ", "hits": 134 }, { "id": 5443, "url": "http://svs.gsfc.nasa.gov/5443/", "result_type": "Visualization", "release_date": "2024-12-17T00:00:00-05:00", "title": "Heliophysics Sentinels 2024", "description": "There have been some changes since the 2022 Heliophysics Fleet. AIM and ICON have been decommissioned while two other instruments have been added. AWE is an instrument mounted on the ISS, and RAD is a particle detector on the Curiosity Mars rover. As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause. || ", "hits": 338 }, { "id": 14734, "url": "http://svs.gsfc.nasa.gov/14734/", "result_type": "Produced Video", "release_date": "2024-12-10T10:00:00-05:00", "title": "Lucy Spacecraft’s Second Slingshot of Earth", "description": "NASA’s Lucy spacecraft will make its second of three Earth gravity assists on Dec. 12, 2024.Complete transcript available.Universal Production Music: “Determined Arrival 4-5” by Joel Goodman [ASCAP]; “Floating” by Nicholas Smith [PRS]; “Subtle Confidence 3” by Joel Goodman [ASCAP]Watch this video on the NASA Goddard YouTube channel. || Lucy-EGA2-Preview-V4_print.jpg (1024x576) [162.5 KB] || Lucy-EGA2-Preview-V4.jpg (1280x720) [574.7 KB] || Lucy-EGA2-Preview-V4.png (1280x720) [1.1 MB] || Lucy-EGA2-Preview-V4_searchweb.png (320x180) [84.0 KB] || Lucy-EGA2-Preview-V4_thm.png (80x40) [6.1 KB] || 14734_Lucy_EGA2_Overview_720.mp4 (1280x720) [40.2 MB] || 14734_Lucy_EGA2_Overview_1080.mp4 (1920x1080) [225.1 MB] || LucyEGA2Captions.en_US.srt [3.5 KB] || LucyEGA2Captions.en_US.vtt [3.3 KB] || 14734_Lucy_EGA2_Overview_4K.mp4 (3840x2160) [2.7 GB] || 14734_Lucy_EGA2_Overview_ProRes.mov (3840x2160) [16.6 GB] || 14734_Lucy_EGA2_Overview_4K.hwshow [478 bytes] || ", "hits": 75 }, { "id": 14722, "url": "http://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": 104 }, { "id": 5428, "url": "http://svs.gsfc.nasa.gov/5428/", "result_type": "Visualization", "release_date": "2024-11-25T00:00:00-05:00", "title": "Parker Solar Probe Towards its Ultimate Perihelion", "description": "Parker Solar Probe is making its final planned orbits around the Sun.On Wednesday, November 6, 2024, NASA's Parker Solar Probe completed it's final Venus gravity assist maneuver, passing within 233 miles (376 kilometers) of Venus' surface. The flyby adjusted Parker's trajectory into its final orbital configuration, bringing the spacecraft to within an unprecedented 3.86 million miles from the solar surface on December 24, 2024. It will be the closest any human-made object has been to the Sun. || ", "hits": 301 }, { "id": 31319, "url": "http://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": 86 }, { "id": 14596, "url": "http://svs.gsfc.nasa.gov/14596/", "result_type": "Produced Video", "release_date": "2024-05-29T11:00:00-04:00", "title": "Lucy Sees Asteroid Dinkinesh in Detail", "description": "Narrated video of Lucy’s encounter with the main-belt asteroid Dinkinesh and its satellite, Selam, on Nov. 1, 2023.Complete transcript available.Universal Production Music: “Gaining Positivity” by Ho Ling Tang [BMI] and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || Dinkinesh_Detailed_View_V2_print.jpg (1024x576) [64.4 KB] || Dinkinesh_Detailed_View_V2.jpg (1280x720) [159.2 KB] || Dinkinesh_Detailed_View_V2.png (1280x720) [165.4 KB] || Dinkinesh_Detailed_View_V2_searchweb.png (320x180) [13.4 KB] || Dinkinesh_Detailed_View_V2_thm.png (80x40) [1.9 KB] || 14596_Dinkinesh_Detailed_View_1080.mp4 (1920x1080) [55.5 MB] || 14596_Dinkinesh_Detailed_View_720.mp4 (1280x720) [11.4 MB] || DinkineshDetailedCaptions.en_US.srt [1.2 KB] || DinkineshDetailedCaptions.en_US.vtt [1.1 KB] || 14596_Dinkinesh_Detailed_View_4K.mp4 (3840x2160) [539.3 MB] || 14596_Dinkinesh_Detailed_View_ProRes.mov (3840x2160) [3.3 GB] || ", "hits": 117 }, { "id": 14576, "url": "http://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": 3855 }, { "id": 14426, "url": "http://svs.gsfc.nasa.gov/14426/", "result_type": "Produced Video", "release_date": "2023-10-19T13:00:00-04:00", "title": "NASA's Lucy Mission Flyby of Asteroid Dinkinesh", "description": "Video: NASA's Lucy Mission Flies By Asteroid DinkineshMusic provided by Universal Production Music: \"Pioneer\" - Lorenzo CastellarinWatch this video on the NASA Goddard YouTube channel. || DinkineshFlyby_Thumbnail.jpg (1920x1080) [681.4 KB] || DinkineshFlyby_Thumbnail_print.jpg (1024x576) [238.9 KB] || DinkineshFlyby_Thumbnail_searchweb.png (320x180) [68.0 KB] || DinkineshFlyby_Thumbnail_thm.png (80x40) [4.8 KB] || 14426_LucyDinkineshFlyby_YouTubeHD.webm (1920x1080) [27.0 MB] || 14426_LucyDinkineshFlyby_TwitterX.mp4 (1280x720) [52.8 MB] || 14426_LucyDinkineshFlyby_YouTubeHD.mp4 (1920x1080) [391.9 MB] || 14426_LucyDinkineshFlyby_Captions.en_US.srt [5.0 KB] || 14426_LucyDinkineshFlyby_Captions.en_US.vtt [4.8 KB] || 14426_LucyDinkineshFlyby_MASTER.mov (1920x1080) [3.2 GB] || ", "hits": 62 }, { "id": 5155, "url": "http://svs.gsfc.nasa.gov/5155/", "result_type": "Visualization", "release_date": "2023-10-01T00:00:00-04:00", "title": "Lucy - Asteroid Dinkinesh Flyby", "description": "A top-down view of the inner solar system, with planets shown in gray, Lucy in teal, and Dinkinesh in pink. The Lucy/Dinkinesh close approach will occur on November 1, 2023. || lucy_dinkinesh_withDates.00385_print.jpg (1024x576) [66.1 KB] || lucy_dinkinesh_withDates.00385_searchweb.png (320x180) [54.9 KB] || lucy_dinkinesh_withDates.00385_thm.png (80x40) [4.0 KB] || lucy_dinkinesh_withDates_1080p60.mp4 (1920x1080) [3.4 MB] || lucy_dinkinesh_withDates (3840x2160) [64.0 KB] || lucy_dinkinesh_withDates_2160p60.mp4 (3840x2160) [16.0 MB] || lucy_dinkinesh_withDates_2160p30.mp4 (3840x2160) [20.0 MB] || lucy_dinkinesh_withDates.prores.mov (3840x2160) [3.0 GB] || ", "hits": 57 }, { "id": 20381, "url": "http://svs.gsfc.nasa.gov/20381/", "result_type": "Animation", "release_date": "2023-08-30T16:30:00-04:00", "title": "OSIRIS-REx Sample Return: Animations", "description": "Ride along with OSIRIS-REx on the thrilling finale of its journey to Bennu and back.Universal Production Music: “Rise to the Challenge” by Daniel Marantz and Michael James Burns, Raydia Music library [PRS]; “Fragments of Time” by Timothy Robert Shortell, Scores of Hypersonic Music [BMI]Watch this video on the NASA.gov Video YouTube channel. || Shot11_DivertBurn_Thumbnail_print.jpg (1024x576) [63.3 KB] || Shot11_DivertBurn_Thumbnail.jpg (3840x2160) [1.1 MB] || Shot11_DivertBurn_Thumbnail.png (3840x2160) [9.9 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_720.mp4 (1280x720) [42.8 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_1080.mp4 (1920x1080) [298.0 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_4K.mp4 (3840x2160) [2.9 GB] || 20381_OSIRIS-REx_RETURN_MONTAGE_ProRes.mov (3840x2160) [20.4 GB] || 20381_OSIRIS-REx_RETURN_MONTAGE_4K.hwshow [513 bytes] || ", "hits": 1971 }, { "id": 40518, "url": "http://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics 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": 131 }, { "id": 5069, "url": "http://svs.gsfc.nasa.gov/5069/", "result_type": "Visualization", "release_date": "2023-02-09T00:00:00-05:00", "title": "Asteroid Bennu 3D Models", "description": "These 3D models and images were created using data from NASA’s OSIRIS-REx spacecraft collected while in orbit around asteroid Bennu. These are some of the 3D models that were used to create several SVS Bennu data visualizations, including Tour of Asteroid Bennu, Detailed Global Views of Asteroid Bennu, and Bennu TAG Surface Change. || ", "hits": 430 }, { "id": 20374, "url": "http://svs.gsfc.nasa.gov/20374/", "result_type": "Animation", "release_date": "2022-12-12T00:00:00-05:00", "title": "XRISM Beauty Shots", "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ", "hits": 127 }, { "id": 20372, "url": "http://svs.gsfc.nasa.gov/20372/", "result_type": "Animation", "release_date": "2022-10-19T00:00:00-04:00", "title": "Lucy Earth Gravity Assist One: Animations", "description": "NASA’s Lucy mission is heading to the Jupiter Trojans – two swarms of primitive asteroids trapped in Jupiter’s orbit that may hold clues to the formation of the planets. Lucy launched on October 16, 2021, spent a year in orbit around the Sun, and returned home on its launch anniversary for the first of three Earth gravity assists. The maneuver boosted Lucy’s speed and elongated its orbit around the Sun, setting it track for a second flyby of Earth in December 2024. This page provides artist concept animations depicting Lucy’s first Earth gravity assist.Learn more about Lucy's first Earth gravity assist. || ", "hits": 119 }, { "id": 14225, "url": "http://svs.gsfc.nasa.gov/14225/", "result_type": "Produced Video", "release_date": "2022-10-13T11:00:00-04:00", "title": "Lucy Spacecraft Will Slingshot Around Earth", "description": "NASA’s Lucy spacecraft will make an exceptionally close flyby of Earth on Oct. 16, 2022. Complete transcript available.Universal Production Music: “Determined Arrival 5” by Joel Goodman; “Finding Solace” by Eric Chevalier; “Subtle Confidence 3” by Joel GoodmanWatch this video on the NASA Goddard YouTube channel. || Lucy_EGA1_Preview_2_print.jpg (1024x576) [112.3 KB] || Lucy_EGA1_Preview_2.png (3840x2160) [12.5 MB] || Lucy_EGA1_Preview_2.jpg (3840x2160) [773.2 KB] || Lucy_EGA1_Preview_2_thm.png (80x40) [5.3 KB] || Lucy_EGA1_Preview_2_searchweb.png (180x320) [76.5 KB] || 14225_Lucy_EGA1_Twitter_V2.mp4 (1280x720) [52.4 MB] || 14225_Lucy_EGA1_Twitter_V2.webm (1280x720) [26.0 MB] || 14225_Lucy_EGA1_Facebook_V2.mp4 (1920x1080) [294.2 MB] || 14225_Lucy_EGA1_Captions_FINAL.en_US.srt [5.6 KB] || 14225_Lucy_EGA1_Captions_FINAL.en_US.vtt [5.3 KB] || 14225_Lucy_EGA1_YouTube_V2.mp4 (3840x2160) [3.6 GB] || 14225_Lucy_EGA1_MASTER_V2.mov (3840x2160) [23.8 GB] || ", "hits": 102 }, { "id": 14095, "url": "http://svs.gsfc.nasa.gov/14095/", "result_type": "Produced Video", "release_date": "2022-02-09T09:00:00-05:00", "title": "NASA’s New Views of Venus’ Surface From Space", "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ", "hits": 556 }, { "id": 14035, "url": "http://svs.gsfc.nasa.gov/14035/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "AGU 2021 - Major discoveries as NASA’s Parker Solar Probe closes in on the Sun", "description": "NASA’s Parker Solar Probe has now done what no spacecraft has done before—it has officially touched the Sun. Launched in 2018 to study the Sun’s biggest mysteries, the spacecraft has now grazed the edge of the solar atmosphere and gathered new close-up observations of our star. This is allowing us to see the Sun as never before—including the findings in two new papers, which were presented at AGU, that are helping scientists answer fundamental questions about the Sun.PANELISTSDr. Nicola Fox• Heliophysics Division Director of the Science Mission Directorate at NASA HeadquartersDr. Nour Raouafi• Project Scientist for NASA’s Parker Solar Probe• The Johns Hopkins Applied Physics Laboratory Dr. Justin Kasper• Principal Investigator for Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Parker Solar Probe • BWX Technologies, Inc., University of MichiganProf. Stuart D. Bale• Principal Investigator for Fields Experiment (FIELDS) on Parker Solar Probe • University of California, Berkeley Dr. Kelly Korreck• Program Scientist at NASA Headquarters• Smithsonian Astrophysical Observatory || ", "hits": 89 }, { "id": 14036, "url": "http://svs.gsfc.nasa.gov/14036/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "Animation: NASA's Parker Solar Probe Enters Solar Atmosphere", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. The new milestone marks one major step for Parker Solar Probe and one giant leap for solar science. Just as landing on the Moon allowed scientists to understand how it was formed, touching the very stuff the Sun is made of will help scientists uncover critical information about our closest star and its influence on the solar system. On April 28, 2021, during its eighth flyby of the Sun, Parker Solar Probe encountered the specific magnetic and particle conditions at 18.8 solar radii (8.127 million miles) above the solar surface that told scientists it had crossed the Alfvén critical surface for the first time and finally entered the solar atmosphere.More information here. || ", "hits": 231 }, { "id": 14045, "url": "http://svs.gsfc.nasa.gov/14045/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "NASA's Parker Solar Probe Touches The Sun For The First Time", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. The new milestone marks one major step for Parker Solar Probe and one giant leap for solar science. Just as landing on the Moon allowed scientists to understand how it was formed, touching the very stuff the Sun is made of will help scientists uncover critical information about our closest star and its influence on the solar system. More information here. || ", "hits": 191 }, { "id": 13951, "url": "http://svs.gsfc.nasa.gov/13951/", "result_type": "Produced Video", "release_date": "2021-10-07T10:00:00-04:00", "title": "Lucy's Journey: Episode 5 - \"The First Flyby\"", "description": "The fifth in a series of six episodes in the Lucy's Journey cartoon series.Music is \"Frantic Funk Out\" by Anders Johan Greger Lewen, \"Jewel\" by Arnaud Rignon and Sebastien Langolff and \"Shaken and Stirred\" by Steve Martin of Universal Production Music.Watch this video on the NASA Goddard YouTube channel. || 13951_lucythumb.jpg (3840x2160) [1.0 MB] || 13951_EPISODE5.00170_searchweb.png (320x180) [66.7 KB] || 13951_EPISODE5.00170_thm.png (80x40) [4.6 KB] || 13951_EPISODE5_facebook_720.mp4 (1280x720) [108.4 MB] || 13951_EPISODE5_twitter_720.mp4 (1280x720) [19.5 MB] || 13951_EPISODE5_facebook_720.webm (1280x720) [11.4 MB] || 13951_EPISODE5.mp4 (3840x2160) [108.3 MB] || 13951_caption.en_US.srt [1.2 KB] || 13951_caption.en_US.vtt [1.1 KB] || ", "hits": 46 }, { "id": 4943, "url": "http://svs.gsfc.nasa.gov/4943/", "result_type": "Visualization", "release_date": "2021-09-28T09:00:00-04:00", "title": "Lucy Mission Trajectory 'Over-the-Shoulder' Views", "description": "This visualization is a view from the Lucy spacecraft as it travels through the solar system, represented in a Jupiter-rotating reference frame. In this reference frame, Jupiter appears fixed in space. This visualization spans from launch through the flyby of the main belt asteroid DonaldJohanson. (Part 1 of 3) || lucy_pov_p1.2520_print.jpg (1024x576) [47.5 KB] || lucy_pov_p1.2520_searchweb.png (320x180) [39.2 KB] || lucy_pov_p1.2520_thm.png (80x40) [2.4 KB] || lucy_pov_p1_2160p60.mp4 (3840x2160) [69.7 MB] || lucy_pov_p1_2160p60.webm (3840x2160) [18.9 MB] || lucy_pov_p1 (3840x2160) [0 Item(s)] || lucy_pov_p1_prores.mov (3840x2160) [9.5 GB] || ", "hits": 64 }, { "id": 4921, "url": "http://svs.gsfc.nasa.gov/4921/", "result_type": "Visualization", "release_date": "2021-08-11T13:00:00-04:00", "title": "Bennu 2135/2182 orbits", "description": "Visualization depicting the 2135 Bennu-Earth flyby. Bennu’s orbit is represented in white. Earth’s orbit is represented in light blue. || bennu_2135_comp_0000_print.jpg (1024x576) [35.1 KB] || bennu_2135_comp_0000_searchweb.png (320x180) [13.4 KB] || bennu_2135_comp_0000_thm.png (80x40) [4.1 KB] || bennu_2135_comp_1080p30.webm (1920x1080) [3.7 MB] || bennu_2135_comp_1080p30.mp4 (1920x1080) [1.7 MB] || bennu_2135_comp_1080p60.mp4 (1920x1080) [1.7 MB] || bennu_orbit_2135 (3840x2160) [0 Item(s)] || bennu_2135_comp_2160p30.mp4 (3840x2160) [3.4 MB] || bennu_2135_comp_2160p60.mp4 (3840x2160) [3.5 MB] || osiris-rex_animations.hwshow || ", "hits": 280 }, { "id": 13896, "url": "http://svs.gsfc.nasa.gov/13896/", "result_type": "Animation", "release_date": "2021-08-11T13:00:00-04:00", "title": "OSIRIS-REx Sheds Light on Hazardous Asteroid Bennu", "description": "OSIRIS-REx is improving our understanding of asteroid Bennu’s future impact hazard.Complete transcript available.Universal Production Music: “Time Particles” by Laetitia FrenodWatch this video on the NASA Goddard YouTube channel. || BennuImpactHazardPreview_print.jpg (1024x576) [110.3 KB] || BennuImpactHazardPreview.png (3840x2160) [5.2 MB] || BennuImpactHazardPreview.jpg (3840x2160) [1.1 MB] || BennuImpactHazardPreview_searchweb.png (180x320) [45.8 KB] || BennuImpactHazardPreview_thm.png (80x40) [3.5 KB] || TWITTER_720_13896_Bennu_Impact_Hazard_MASTER_twitter_720.mp4 (1280x720) [29.3 MB] || 13896_Bennu_Impact_Hazard_MASTER.webm (960x540) [47.1 MB] || FACEBOOK_720_13896_Bennu_Impact_Hazard_MASTER_facebook_720.mp4 (1280x720) [180.0 MB] || 13896_Bennu_Impact_Hazard_Captions.en_US.srt [4.0 KB] || 13896_Bennu_Impact_Hazard_Captions.en_US.vtt [3.8 KB] || 13896_Bennu_Impact_Hazard_SPANISH.mp4 (3840x2160) [200.8 MB] || 13896_Bennu_Impact_Hazard_YouTube.mp4 (3840x2160) [1.7 GB] || 13896_Bennu_Impact_Hazard_MASTER.mov (3840x2160) [18.6 GB] || ", "hits": 123 }, { "id": 13906, "url": "http://svs.gsfc.nasa.gov/13906/", "result_type": "Produced Video", "release_date": "2021-08-11T12:00:00-04:00", "title": "OSIRIS-REx Bennu Impact Probability – Media Telecon", "description": "NASA will host a media teleconference at 1 p.m. EDT Wednesday, Aug. 11, to discuss an important finding from NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft.OSIRIS-REx spent over two years near the asteroid Bennu, which is a third of a mile (500 meters) wide. During that time, the spacecraft gathered information about Bennu’s size, shape, mass, and composition while monitoring its spin and orbital trajectory. Before leaving the near-Earth object May 10, 2021, the spacecraft scooped up a sample of rock and dust from the asteroid’s surface. OSIRIS-REx will return the sample to Earth Sept. 24, 2023, for further scientific study.The teleconference will stream live online at: http://www.nasa.gov/liveParticipants in the briefing will be:•Dante Lauretta, study co-author and OSIRIS-REx principal investigator at the University of Arizona in Tucson•Davide Farnocchia, study lead author and scientist with the Center for Near Earth Object Studies at NASA’s Jet Propulsion Laboratory in Southern California•Jason Dworkin, OSIRIS-REx project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland•Lindley Johnson, planetary defense officer at NASA’s Planetary Defense Coordination Office at NASA Headquarters in WashingtonFor more information about the OSIRIS-REx mission to Bennu, visit: https://www.nasa.gov/osiris-rexLearn more about asteroid Bennu’s updated impact hazard.Read the science paper on Icarus. || ", "hits": 106 }, { "id": 20356, "url": "http://svs.gsfc.nasa.gov/20356/", "result_type": "Animation", "release_date": "2021-08-11T00:00:00-04:00", "title": "Asteroid Bennu Impact Hazard: Animations", "description": "On September 25, 2135, an asteroid called Bennu will make a close flyby of Earth. Our planet’s gravity will tweak Bennu’s path, making it a challenge to calculate its future trajectory and the odds of a potential impact late in the 22nd century. This media resource page provides broadcast-quality animations related to asteroid Bennu’s impact hazard. Learn more from NASA.Watch the produced video on the NASA Goddard YouTube Channel. || ", "hits": 212 }, { "id": 13864, "url": "http://svs.gsfc.nasa.gov/13864/", "result_type": "Produced Video", "release_date": "2021-05-20T12:55:00-04:00", "title": "Hubble Tracks Origins Of Energy Blasts", "description": "Fast radio bursts or FRBs, are extraordinary events that generate as much energy in a thousandth of a second as the Sun does in an entire year!Astronomers, using NASA’s Hubble Space Telescope have traced the locations of eight brief, powerful FRBs; five of which are near or on their host galaxy’s spiral arms. The research helped rule out some of the possible stellar objects originally thought to cause these brilliant flares.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Sunrise over the Pacific: ArtbeatsAnimation of Magnetar: Scott WiessingerFRB Locations Animation: Scott Wiessinger and Chris SmithGamma Ray Burst Illustration: Michael StarobinNeutron Star Merger: Michael StarobinMagnetar Flyby Animation: Chris SmithMagnetar Flare Sequence: Chris SmithMusic Credits: \"Deep Caverns\" by JC Lemay [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music. || ", "hits": 108 }, { "id": 13840, "url": "http://svs.gsfc.nasa.gov/13840/", "result_type": "Produced Video", "release_date": "2021-04-23T08:55:00-04:00", "title": "Hubble's 31st Anniversary: Giant Star on the Edge of Destruction", "description": "In celebration of the 31st anniversary of the launching of NASA’s Hubble Space Telescope, astronomers aimed the renowned observatory at a brilliant “celebrity star,” one of the brightest stars seen in our galaxy, surrounded by a glowing halo of gas and dust.Hubble's senior project scientist, Dr. Jennifer Wiseman, takes us on a tour of this stunning new image, describes the telescope's current health, and summarizes some of Hubble's contributions to astronomy from the past year.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Flyby of AG CarinaeVideo credit: Leah Hustak, Frank Summers, Alyssa Pagan, Joseph DePasquale, Greg Bacon (STSci)Artist’s Impression of the Black Hole Concentration in NGC 6397Video credit: ESA/Hubble, N. BartmannAnimation of of Exoplanet GJ 1132 bVideo credit: Robert HurtMusic Credits: \"Himalayan Temple\" by Jan Pham Huu Tri [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music. || ", "hits": 63 }, { "id": 13751, "url": "http://svs.gsfc.nasa.gov/13751/", "result_type": "Produced Video", "release_date": "2020-11-04T11:00:00-05:00", "title": "NASA Missions Team Up to Study Unique Magnetar Outburst", "description": "On April 28, space- and ground-based observatories detected powerful, simultaneous X-ray and radio bursts from a source in our galaxy. Watch to see how this unique event helps solve the longstanding puzzle of fast radio bursts observed in other galaxies.Credit: NASA's Goddard Space Flight CenterMusic: \"Jupiter's Eye\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_FRB_Still.jpg (1920x1080) [535.5 KB] || Magnetar_FRB_Still_searchweb.png (320x180) [65.5 KB] || Magnetar_FRB_Still_thm.png (80x40) [4.8 KB] || 13751_Magnetar_FRB_Best_1080.webm (1920x1080) [25.7 MB] || 13751_Magnetar_FRB_1080.mp4 (1920x1080) [237.4 MB] || 13751_Magnetar_FRB_Best_1080.mp4 (1920x1080) [741.8 MB] || Fast_Radio_Burst_SRT_Captions.en_US.srt [4.5 KB] || Fast_Radio_Burst_SRT_Captions.en_US.vtt [4.5 KB] || 13751_Magnetar_FRB_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 433 }, { "id": 40423, "url": "http://svs.gsfc.nasa.gov/gallery/lucy/", "result_type": "Gallery", "release_date": "2020-11-02T00:00:00-05:00", "title": "Lucy", "description": "Launching in 2021, NASA's Lucy spacecraft will be the first space mission to study the outer Solar System asteroids known as the Trojans, which are orbiting the same distance from the Sun as Jupiter. These fly-by encounters are planned to take place over a 12-year period. The instruments on board will collect data on surface geology, surface color and composition, the asteroids' interior and bulk properties, as well as any satellites and rings.\n\nLucy is named for the famous Australopithecus afarensis hominid fossil that shed light on our early human ancestors. By making the first exploration of the Trojan asteroids, the Lucy mission will improve our understanding of the early solar system, and be the first to uncover these fossils of planet formation.", "hits": 0 }, { "id": 13738, "url": "http://svs.gsfc.nasa.gov/13738/", "result_type": "Produced Video", "release_date": "2020-10-19T11:30:00-04:00", "title": "OSIRIS-REx Science and Engineering Briefing", "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ", "hits": 95 }, { "id": 40161, "url": "http://svs.gsfc.nasa.gov/gallery/osirisrex/", "result_type": "Gallery", "release_date": "2020-09-29T00:00:00-04:00", "title": "OSIRIS-REx", "description": "NASA’s OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid, will return to Earth on Sept. 24, 2023, with material from asteroid Bennu. When it arrives, the OSIRIS-REx spacecraft will release the sample capsule for a safe landing in the Utah desert. Generations of scientists will study the material from Bennu in laboratories on Earth to better understand how the solar system evolved and where the chemical ingredients for life may have originated.\r\rKeep up with sample-landing news and updates on the OSIRIS-REx blog.Watch OSIRIS-REx videos on this YouTube channel.Learn more about OSIRIS-REx from NASA.", "hits": 345 }, { "id": 13724, "url": "http://svs.gsfc.nasa.gov/13724/", "result_type": "Produced Video", "release_date": "2020-09-24T14:25:00-04:00", "title": "OSIRIS-REx: Countdown to TAG", "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ", "hits": 78 }, { "id": 4857, "url": "http://svs.gsfc.nasa.gov/4857/", "result_type": "Animation", "release_date": "2020-09-21T00:00:00-04:00", "title": "OSIRIS-REx – Detailed Global Views of Asteroid Bennu", "description": "Looping animation of asteroid Bennu rotating. This 3D model of Bennu was created using 20cm resolution laser altimetry data and imagery taken by OSIRIS-REx. || bennu_spin_v3_02.1000_print.jpg (1024x576) [75.3 KB] || bennu_spin_v3_02.1000_searchweb.png (320x180) [18.4 KB] || bennu_spin_v3_02.1000_thm.png (80x40) [1.6 KB] || bennu_spin_v3_1080p30.mp4 (1920x1080) [77.5 MB] || Bennu_GlobalSpin_20cm_v2 (3840x2160) [0 Item(s)] || bennu_spin_v3_2160p30.webm (3840x2160) [32.4 MB] || bennu_spin_v3_2160p30.mp4 (3840x2160) [242.3 MB] || 4857_Bennu_Global_Spin_20cm.mov (3840x2160) [12.0 GB] || 01_dworkin_bennu.hwshow || ", "hits": 268 }, { "id": 13664, "url": "http://svs.gsfc.nasa.gov/13664/", "result_type": "Produced Video", "release_date": "2020-07-16T08:00:00-04:00", "title": "ESA and NASA Release First Images From Solar Orbiter Mission", "description": "Scientists from ESA (European Space Agency) and NASA will present the first images captured by Solar Orbiter, the joint ESA/NASA mission to study the Sun, during an online news briefing at 8 a.m. EDT Thursday, July 16. Launched on Feb. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun. The flyby captured the closest images ever taken of the Sun. During the briefing, mission experts will discuss what these closeup images reveal about our star, including what we can learn from Solar Orbiter’s new measurements of particles and magnetic fields flowing from the Sun.The briefing will stream live at:https://www.nasa.gov/solarorbiterfirstlight/Participants in the call include:•Daniel Müller – Solar Orbiter Project Scientist at ESA•Holly R. Gilbert – Solar Orbiter Project Scientist at NASA•José Luis Pellón Bailón – Solar Orbiter Deputy Spacecraft Operations Manager at ESA•David Berghmans – Principal investigator of the Extreme Ultraviolet Imager (EUI) at the Royal Observatory of Belgium•Sami Solanki – Principal investigator of the Polarimetric and Helioseismic Imager (PHI) and director of the Max Planck Institute for Solar System Research•Christopher J. Owen – Principal investigator of the Solar Wind Analyser (SWA) at Mullard Space Science Laboratory, University College London•ESA’s first light images•ESA press release •NASA feature story || ", "hits": 127 }, { "id": 13628, "url": "http://svs.gsfc.nasa.gov/13628/", "result_type": "Produced Video", "release_date": "2020-06-12T10:00:00-04:00", "title": "Parker Solar Probe Teams Up with Observatories Around the Solar System for Fourth Solar Encounter", "description": "At the heart of understanding our space environment is the knowledge that conditions throughout space — from the Sun to the atmospheres of planets to the radiation environment in deep space — are connected.Studying this connection – a field of science called heliophysics — is a complex task: Researchers track sudden eruptions of material, radiation, and particles against the background of the ubiquitous outflow of solar material.A confluence of events in early 2020 created a nearly ideal space-based laboratory, combining the alignment of some of humanity’s best observatories — including Parker Solar Probe, during its fourth solar flyby — with a quiet period in the Sun’s activity, when it’s easiest to study those background conditions. These conditions provided a unique opportunity for scientists to study how the Sun influences conditions at points throughout space, with multiple angles of observation and at different distances from the Sun. || ", "hits": 41 }, { "id": 13599, "url": "http://svs.gsfc.nasa.gov/13599/", "result_type": "Produced Video", "release_date": "2020-04-29T13:00:00-04:00", "title": "Hubble's Cosmic Reef Image Flyby", "description": "This science visualization presents the dramatic landscape of two nebulas in the Large Magellanic Cloud. The video takes viewers on a close-up tour of the nebulas' three-dimensional structures, as deduced by scientists and artists. The visualization is an interpretation of the nebulas' complex structure and is based on images by NASA's Hubble Space Telescope.For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble.Visualization Credits:Greg Bacon, Joseph DePasquale, Leah Hustak, Joseph Olmsted, Alyssa Pagan, Dani Player, and Frank Summers [ STScI ]Music credits: \"Cosmic Reef\" by J. DePasquale [ STScI ] || ", "hits": 95 }, { "id": 13505, "url": "http://svs.gsfc.nasa.gov/13505/", "result_type": "Produced Video", "release_date": "2019-12-11T15:00:00-05:00", "title": "Solar Orbiter - ESA Animations", "description": "Solar Orbiter is an European Space Agency (ESA) mission with strong NASA participation. Its mission is to perform unprecedented close-up observations of the Sun and from high-latitudes, providing the first images of the uncharted polar regions of the Sun, and investigating the Sun-Earth connection. || ", "hits": 91 }, { "id": 4719, "url": "http://svs.gsfc.nasa.gov/4719/", "result_type": "Visualization", "release_date": "2019-10-21T10:00:00-04:00", "title": "Lucy mission trajectory", "description": "Jupiter's swarms of Trojan asteroids may be remnants of the primordial material that formed the outer planets, and serve as time capsules from the birth of our Solar System more than 4 billion years ago. The Trojans orbit in two loose groups that orbit the Sun, with one group always ahead of Jupiter in its path, the other always behind. At these two Lagrange points the bodies are stabilized by the Sun and Jupiter in a gravitational balancing act. These primitive bodies hold vital clues to deciphering the history of the solar system, and perhaps even the origins of life and organic material on Earth.Lucy will be the first space mission to study the Trojans. The mission takes its name from the fossilized human ancestor (called “Lucy” by her discoverers) whose skeleton provided unique insight into humanity's evolution. Likewise, the Lucy mission will revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy will launch in October 2021 and, with boosts from Earth's gravity, will complete a twelve-year journey to eight different asteroids — a Main Belt asteroid and seven Jupiter Trojans, the last two members of a “two-for-the-price-of-one” binary system. Lucy’s complex path will take it to both clusters of Trojans and give us our first close-up view of all three major types of bodies in the swarms (so-called C-, P- and D-types). || ", "hits": 168 }, { "id": 20301, "url": "http://svs.gsfc.nasa.gov/20301/", "result_type": "Animation", "release_date": "2019-10-21T00:00:00-04:00", "title": "Lucy Mission Animations", "description": "Lucy flies by its final target, the binary asteroid Patroclus/Menoetius. When it completes this flyby, Lucy will have visited an unprecedented seven asteroids. || Lucy_Flyby_main_seq_00315_print.jpg (1024x576) [85.2 KB] || Lucy_Flyby_main_seq_00315_searchweb.png (320x180) [77.9 KB] || Lucy_Flyby_main_seq_00315_thm.png (80x40) [6.1 KB] || Lucy_Flyby_main_1080_H264.mp4 (1920x1080) [45.0 MB] || Lucy_Flyby_main_1080_H264.webm (1920x1080) [2.8 MB] || Lucy_Flyby_1080_ProRes.mov (1920x1080) [282.0 MB] || Lucy_flyby_4k_prores_seq (3840x2160) [0 Item(s)] || Lucy_Flyby_main_4k_H264.mp4 (3840x2160) [27.5 MB] || Lucy_Flyby_main_4k_H264.webm (3840x2160) [5.9 MB] || Lucy_Flyby_main_4k.mov (3840x2160) [758.8 MB] || ", "hits": 88 }, { "id": 4758, "url": "http://svs.gsfc.nasa.gov/4758/", "result_type": "Visualization", "release_date": "2019-10-16T00:00:00-04:00", "title": "The Path of Comet 2I/Borisov", "description": "Follow 2I/Borisov from September 2018 to April 2020 as it flies through our solar system. || flyby.0396_print.jpg (1024x576) [117.5 KB] || flyby.0396_searchweb.png (320x180) [71.4 KB] || flyby.0396_thm.png (80x40) [4.3 KB] || flyby_1080p30.mp4 (1920x1080) [11.4 MB] || flyby_720p30.mp4 (1280x720) [6.0 MB] || flyby_720p30.webm (1280x720) [2.4 MB] || flyby_dates (1920x1080) [0 Item(s)] || flyby_360p30.mp4 (640x360) [2.1 MB] || flyby_1080p30.mp4.hwshow [179 bytes] || ", "hits": 156 }, { "id": 31024, "url": "http://svs.gsfc.nasa.gov/31024/", "result_type": "Hyperwall Visual", "release_date": "2019-02-25T11:00:00-05:00", "title": "A Flyby of the Whirlpool Galaxy", "description": "This flight across the Whirlpool Galaxy is visualized using observations from the Hubble Space Telescope. || m51-example_frame-1920x1080.png (1920x1080) [1.8 MB] || m51-example_frame-1920x1080_print.jpg (1024x576) [68.7 KB] || m51-example_frame-3840x2160.png (3840x2160) [6.1 MB] || m51-example_frame-1920x1080_searchweb.png (320x180) [53.4 KB] || m51-example_frame-1920x1080_thm.png (80x40) [4.4 KB] || m51_flyby_hw-1920x1080.webm (1920x1080) [7.0 MB] || m51_flyby_hw-1920x1080.mp4 (1920x1080) [104.9 MB] || m51_flyby_hw-3840x2160.mp4 (3840x2160) [258.3 MB] || ", "hits": 106 }, { "id": 13113, "url": "http://svs.gsfc.nasa.gov/13113/", "result_type": "Produced Video", "release_date": "2018-12-12T15:00:00-05:00", "title": "AGU 2018 - Expected Data and Scientific Discovery from NASA’s Parker Solar Probe", "description": "Animation of NASA's Parker Solar Probe in the solar wind. Credit: NASA/GSFC/CIL/Brian Monroe || 1_Nicky_ParkerBeautyPass_1.00200_print.jpg (1024x576) [34.0 KB] || 1_Nicky_ParkerBeautyPass_1.mp4 (1920x1080) [24.5 MB] || 1_Nicky_ParkerBeautyPass_1.webm (1920x1080) [2.4 MB] || ", "hits": 48 }, { "id": 40365, "url": "http://svs.gsfc.nasa.gov/gallery/earth-science-oct2018-briefing/", "result_type": "Gallery", "release_date": "2018-10-18T00:00:00-04:00", "title": "Earth Science Overview Oct 2018 Briefing", "description": "No description available.", "hits": 95 }, { "id": 4680, "url": "http://svs.gsfc.nasa.gov/4680/", "result_type": "Visualization", "release_date": "2018-10-04T00:00:00-04:00", "title": "Space Weather to the Edge of the Solar System - Revisited", "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_print.jpg (1024x576) [97.2 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_searchweb.png (320x180) [79.1 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_thm.png (80x40) [5.0 KB] || TopView (1920x1080) [0 Item(s)] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4 (1920x1080) [41.0 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.webm (1920x1080) [6.6 MB] || TopView (3840x2160) [0 Item(s)] || NewHorizons.topfixed_HAE.UHD3840_2160p30.mp4 (3840x2160) [125.3 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4.hwshow [202 bytes] || ", "hits": 87 }, { "id": 4682, "url": "http://svs.gsfc.nasa.gov/4682/", "result_type": "Visualization", "release_date": "2018-09-19T00:00:00-04:00", "title": "GPM Captures Super Typhoon Mangkhut Approaching The Philippines", "description": "At nearly the same time that the US East Coast was experiencing the arrival of Hurricane Florence, a much more powerful storm was also arriving half a world away in the Philippines—Super Typhoon Mangkhut. While the slow-moving Florence arrived as a Category 1 hurricane that brought record flooding to the Carolinas, less than 7 hours later Mangkhut (known as Ompong in the Philippines) made landfall on the northern main island of Luzon as a full on Category 5 super typhoon with sustained winds reported at 165 mph. The visualization starts with a view of Integrated Multi-satellitE Retrievals for GPM (IMERG) precipitation rates from 15:11 UTC (11:11 pm PST) 12 September to 15:41 UTC (11:41 pm PST) 13 September 2018 as the storm was making its way across the Philippine Sea headed for Luzon. Before entering the Philippine Sea, Mangkhut passed just north of Guam on the evening of the 10th as a Category 2 typhoon with sustained winds reported at 105 mph by the Joint Typhoon Warning Center (JTWC) causing widespread power outages. The next day on the 11th as it entered the eastern Philippine Sea, Mangkhut underwent a rapid intensification cycle wherein the storm’s intensity shot from Category 2 on the afternoon of the 10th (local time) to Category 5 with sustained winds estimated at 160 mph by JTWC by the evening of the 11th (local time). Mangkhut is estimated to have reached its peak intensity at 18:00 UTC on the 12th (2:00 am PST 13 September) with maximum sustained winds estimated at 180 mph by JTWC, making it the strongest tropical cyclone of the year thus far.At the start of the visualization, Mangkhut was an extremely powerful Category 5 super typhoon and just approaching its peak intensity. Over the next 24 hours, Mangkhut’s intensity leveled out such that when the GPM core satellite over flew the storm, Mangkhut’s peak intensity was estimated at 165 mph, a still very powerful Category 5 storm. The end of the visualization shows the surface rainfall within Mangkhut as well as a 3D flyby of the storm courtesy of the GPM core satellite, which passed over the storm at around 15:40 UTC (11:40 pm PST) on the 13th. At the surface, a distinct eye is present surrounded by a large area of very heavy to intense rain (shown in dark red and magenta). Further out, heavy rain bands are rotating counter clockwise around the storm’s center. The flyby shows a 3D rendering of the radar structure of Mangkhut using data collected from GPM’s Dual-frequency Precipitation Radar or DPR. At the heart of the storm surrounding the eye is a ring of elevated echo tops associated with Mangkhut’s eyewall. The strong symmetry and continuity of the ring is consistent with an intense tropical cyclone and suggests no inhibiting effects such as dry air or wind shear are affecting the storm. In fact, after these images were taken, Mangkhut would continue on to strike the northern part of Luzon at the same estimated intensity, becoming the strongest typhoon to hit the Philippines since Super Typhoon Haiyan in 2013. So far the storm is being blamed for at least 95 fatalities in the Philippines, many due to a large landslide around the town of Itogon. After crossing Luzon, Mangkhut continued on to strike Hong Kong with winds reported at 121 mph before dissipating over mainland China, where it is being blamed for 6 fatalities. GPM data is part of the toolbox of satellite data used by forecasters and scientists to understand how storms behave. GPM is a joint mission between NASA and the Japan Aerospace Exploration Agency. Current and future data sets are available with free registration to users from NASA Goddard's Precipitation Processing Center website. || ", "hits": 122 }, { "id": 4681, "url": "http://svs.gsfc.nasa.gov/4681/", "result_type": "Visualization", "release_date": "2018-09-12T10:00:00-04:00", "title": "GOES and GPM Capture Florence Trying to Intensify Over the Atlantic", "description": "Hurricane Florence originally formed from an African Easterly wave that emerged off the west coast of Africa back on the 30th of August. When it reached the vicinity of the Cape Verde Islands the next day, it was organized enough to become a tropical depression. The following day the depression strengthened enough to become a tropical storm and Florence was born on the 1st of September. Over the next 3 days, Florence gradually strengthened as it moved in a general west-northwest direction into the central Atlantic. Then, on the 4th of September, Florence began to rapidly intensify. By the morning of the 5th, Florence was a Category 3 hurricane before reaching Category 4 intensity later that afternoon with maximum sustained winds estimated at 130 mph by the National Hurricane Center (NHC). At this point, Florence became the victim of increasingly strong southwesterly wind shear, which greatly weakened the storm all the way back down to a tropical storm the by evening of the 6th.The following GOES-East Infrared (IR) loop shows Florence from 17:54 UTC (1:54 pm EDT) 6 September to 19:27 UTC (3:27 pm EDT) 7 September when it was struggling against the strong southwesterly wind shear in the Central Atlantic. A very interesting looking feature is the arc-shaped cloud that propagates outward from the storm towards the west. This cloud feature is occurring at upper-levels and is likely tied to a gravity wave propagating outward from an area of intense convection that erupted from deep within the storm. When the tops of these smaller scale storms within a storm reach the upper troposphere, they can trigger gravity waves. As these waves progagate outward they can enhance cloud formation where they induce rising motion and erode cloud where they induce downward motion or subsidence. As this arc-shaped cloud is able to propagate outward uniformly from the center, it must be occurring above the shear layer. Compensating areas of subsidence can also surround the strong rising motion occurring within the tall convective clouds. This can help to erode surrounding clouds and may be contributing to the clearing that occurs between the arc-shaped cloud and the mainarea of convection.The end of the loop shows surface rainfall and a 3D flyby of Florence courtesy of the GPM core satellite, which passed over the storm at around 19:21 UTC (3:21 pm EDT) on the 7th. At the surface, two areas of intense rain (shown in magenta) reveal the presence of two areas of strong thunderstorms within Florence north and northeast of the center. The flyby shows a 3D rendering of the radar structure of the storm. The darker blue tower indicates an area of deep convection that has penetrated well over 10 km high and is associated with the southernmost area of intense rain just north of the center. It is these areas of deep convection that fuel the storm by releasing heat, known as latent heat, mainly from condensation, near the core. Although it would be nearly 2 days before Florence re-gained hurricane intensity, these convective towers are what helped Florence to survive the effects of the wind shear and eventually grow back into a Category 4 hurricane.GPM is a joint mission between NASA and the Japanese space agency JAXA.Caption by Stephen Lang (SSAI/NASA GSFC) and Joe Munchak (GSFC). || ", "hits": 88 }, { "id": 13029, "url": "http://svs.gsfc.nasa.gov/13029/", "result_type": "Produced Video", "release_date": "2018-08-09T00:00:00-04:00", "title": "Parker Solar Probe Pre-Launch Briefing", "description": "Hosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Scott Messer - Program Manager, NASA Programs, United Launch AllianceOmar Baez - Launch Director, NASA, Kennedy Space CenterKathy Rice - Launch Weather Officer, 45th Weather Squadron, Cape Canaveral Air Force StationThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASANicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAndy Dreisman - Project Manger The Johns Hopkins University Applied Physics Lab || ", "hits": 59 }, { "id": 4664, "url": "http://svs.gsfc.nasa.gov/4664/", "result_type": "Visualization", "release_date": "2018-07-27T00:00:00-04:00", "title": "Jupiter's Magnetosphere", "description": "Jupiter's magnetosphere - a basic view. || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_print.jpg (1024x576) [245.3 KB] || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_searchweb.png (320x180) [132.5 KB] || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_thm.png (80x40) [8.3 KB] || JupiterBasic-noglyph (1920x1080) [0 Item(s)] || Jupiter_JupiterBasic_Dayside.HD1080i_p30.webm (1920x1080) [32.8 MB] || Jupiter_JupiterBasic_Dayside.HD1080i_p30.mp4 (1920x1080) [406.6 MB] || JupiterBasic-noglyph (3840x2160) [0 Item(s)] || Jupiter_JupiterBasic_Dayside_2160p30.mp4 (3840x2160) [984.8 MB] || Jupiter_JupiterBasic_Dayside.HD1080i_p30.mp4.hwshow [206 bytes] || ", "hits": 226 }, { "id": 4665, "url": "http://svs.gsfc.nasa.gov/4665/", "result_type": "Visualization", "release_date": "2018-07-27T00:00:00-04:00", "title": "Saturn's Magnetosphere", "description": "A basic view of Saturn's magnetosphere. || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_print.jpg (1024x576) [186.2 KB] || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_searchweb.png (320x180) [107.8 KB] || Saturn_SaturnBasic_Dayside.slate_BaseRig.HD1080i.1500_thm.png (80x40) [7.1 KB] || SaturnBasic-noglyph (1920x1080) [0 Item(s)] || Saturn_SaturnBasic_Dayside.HD1080i_p30.webm (1920x1080) [22.1 MB] || Saturn_SaturnBasic_Dayside.HD1080i_p30.mp4 (1920x1080) [365.5 MB] || SaturnBasic-noglyph (3840x2160) [0 Item(s)] || Saturn_SaturnBasic_Dayside_2160p30.mp4 (3840x2160) [938.9 MB] || Saturn_SaturnBasic_Dayside.HD1080i_p30.mp4.hwshow || ", "hits": 173 }, { "id": 4666, "url": "http://svs.gsfc.nasa.gov/4666/", "result_type": "Visualization", "release_date": "2018-07-27T00:00:00-04:00", "title": "Uranus' Magnetosphere", "description": "A basic view of the Uranian magnetosphere when the rotation axis is perpendicular to the Uranus-Sun line and days and nights are of equal duration. || Uranus_UranusEquinox_Dayside.slate_BaseRig.HD1080i.1500_print.jpg (1024x576) [197.1 KB] || Uranus_UranusEquinox_Dayside.slate_BaseRig.HD1080i.1500_searchweb.png (320x180) [107.3 KB] || Uranus_UranusEquinox_Dayside.slate_BaseRig.HD1080i.1500_thm.png (80x40) [6.8 KB] || UranusEquinox-noglyph (1920x1080) [0 Item(s)] || Uranus_UranusEquinox_Dayside.HD1080i_p30.webm (1920x1080) [20.9 MB] || Uranus_UranusEquinox_Dayside.HD1080i_p30.mp4 (1920x1080) [308.1 MB] || UranusEquinox-noglyph (3840x2160) [0 Item(s)] || Uranus_UranusEquinox_Dayside_2160p30.mp4 (3840x2160) [758.5 MB] || Uranus_UranusEquinox_Dayside.HD1080i_p30.mp4.hwshow [206 bytes] || ", "hits": 160 }, { "id": 4667, "url": "http://svs.gsfc.nasa.gov/4667/", "result_type": "Visualization", "release_date": "2018-07-27T00:00:00-04:00", "title": "Neptune's Magnetosphere", "description": "A basic view of the Neptunian magnetosphere when the southern side of the rotation axis is directed sunward (southern summer) || Neptune_NeptuneSouthSummer_Dayside.slate_BaseRig.HD1080i.1500_print.jpg (1024x576) [195.5 KB] || Neptune_NeptuneSouthSummer_Dayside.slate_BaseRig.HD1080i.1500_searchweb.png (320x180) [108.2 KB] || Neptune_NeptuneSouthSummer_Dayside.slate_BaseRig.HD1080i.1500_thm.png (80x40) [6.8 KB] || NeptuneSouthSummer-noglyph (1920x1080) [0 Item(s)] || Neptune_NeptuneSouthSummer_Dayside.HD1080i_p30.webm (1920x1080) [21.4 MB] || Neptune_NeptuneSouthSummer_Dayside.HD1080i_p30.mp4 (1920x1080) [328.8 MB] || NeptuneSouthSummer-noglyph (3840x2160) [0 Item(s)] || Neptune_NeptuneSouthSummer_Dayside_2160p30.mp4 (3840x2160) [820.2 MB] || Neptune_NeptuneSouthSummer_Dayside.HD1080i_p30.mp4.hwshow [212 bytes] || ", "hits": 107 }, { "id": 13003, "url": "http://svs.gsfc.nasa.gov/13003/", "result_type": "Produced Video", "release_date": "2018-07-20T12:30:00-04:00", "title": "Parker Solar Probe Science Briefing - Visual Resources", "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ", "hits": 177 }, { "id": 13000, "url": "http://svs.gsfc.nasa.gov/13000/", "result_type": "Produced Video", "release_date": "2018-07-16T12:00:00-04:00", "title": "Pluto's Underground Ocean", "description": "Pluto and Charon may keep their interiors warm enough to support liquid water oceans. || PIA19717_1024x576.jpg (1024x576) [6.1 KB] || PIA19717_print.jpg (1024x576) [6.4 KB] || PIA19717_thm.png (80x40) [1.1 KB] || PIA19717_searchweb.png (320x180) [4.5 KB] || PIA19717.tif (1280x720) [2.6 MB] || ", "hits": 365 }, { "id": 4591, "url": "http://svs.gsfc.nasa.gov/4591/", "result_type": "Visualization", "release_date": "2017-10-10T16:00:00-04:00", "title": "GPM Catches Hurricane Nate's Landfall...Twice", "description": "NASA's GPM satellite helped track Nate's progress through the Gulf of Mexico and also captured Nate's landfall on the north central Gulf Coast. This animation shows instantaneous rainrate estimates from NASA's Integrated Multi-satellitE Retrievals for GPM or IMERG product over North America and the surrounding waters beginning on Thursday October 5th when Nate first became a tropical storm near the northeast coast of Nicaragua in the western Caribbean until its eventual landfall on the northern Gulf Coast on Sunday October 8th. IMERG estimates precipitation from a combination of space-borne passive microwave sensors, including the GMI microwave sensor onboard the GPM core satellite, and geostationary IR (infrared) data. The animation shows Nate moving rapidly northward through the Gulf of Mexico on the 7th. Nate's rapid movement from 20 to as much as 26 mph did not allow the storm much time to strengthen despite being over very warm waters and in a relatively low wind shear environment. Nate reached a peak intensity of 90 mph sustained winds, which it maintained while passing over the Gulf of Mexico, but it did not intensify any further before making landfall. The animation also shows two 3D flyby's of Nate captured by the GPM core satellite as it overflew the storm just before landfall at 22:58 UTC (5:58 CDT) on Saturday October 7th and again at 08:42 UTC (3:42 CDT) on Sunday October 8th soon after Nate's second landfall. The 3D precipitation tops (shown in blue) are from GPM's DPR as are the vertical cross sections of precipitation intensity. The first overpass shows that Nate is a very asymmetric storm with most of the rainbands associated with Nate located north and east of the center. With it's rapid movement, Nate was unable to fully develop and lacks the classic ring of intense thunderstorms associated a fully developed eyewall. Although overall much the same, the second overpass shows an area of deep, intense convection producing heavy rains over southwest Alabama. || nate.1890_print.jpg (1024x576) [166.6 KB] || nate.1890_searchweb.png (320x180) [92.3 KB] || nate.1890_thm.png (80x40) [7.5 KB] || nate.mp4 (1920x1080) [37.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || nate.webm (1920x1080) [5.1 MB] || nate.mp4.hwshow [170 bytes] || ", "hits": 54 }, { "id": 30905, "url": "http://svs.gsfc.nasa.gov/30905/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Juno's Eighth Close Approach to Jupiter", "description": "Jupiter image sequence || PIA21780_print.jpg (1024x801) [159.5 KB] || PIA21780_searchweb.png (320x180) [88.9 KB] || PIA21780_thm.png (80x40) [6.9 KB] || PIA21780.tif (6392x5000) [54.0 MB] || ", "hits": 42 }, { "id": 30906, "url": "http://svs.gsfc.nasa.gov/30906/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Jupiter: A New Point of View", "description": "Jupiter || PIA21778_print.jpg (1024x457) [104.5 KB] || PIA21778_searchweb.png (320x180) [98.5 KB] || PIA21778_thm.png (80x40) [6.1 KB] || PIA21778.tif (10123x4523) [93.8 MB] || ", "hits": 33 }, { "id": 30907, "url": "http://svs.gsfc.nasa.gov/30907/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Jupiter Storm of the High North", "description": "A storm on Jupiter || PIA21776_print.jpg (1024x1193) [247.1 KB] || PIA21776_searchweb.png (320x180) [87.9 KB] || PIA21776_thm.png (80x40) [5.9 KB] || PIA21776.tif (2119x2470) [11.9 MB] || -jupiter-storm-of-the-high-north.hwshow [208 bytes] || ", "hits": 44 }, { "id": 20251, "url": "http://svs.gsfc.nasa.gov/20251/", "result_type": "Animation", "release_date": "2017-09-22T09:00:00-04:00", "title": "OSIRIS-REx Earth Gravity Assist", "description": "When OSIRIS-REx flies by Earth on September 22, 2017, it will use our planet's gravity as a slingshot to catch asteroid Bennu. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks:\"Origin\" by Axel Tenner, Michael Schluecker, and Raphael Schalz || 20251_OSIRIS-REx_Earth_Gravity_Assist_FB.mp4 (1280x720) [138.9 MB] || EGA_1_Flyby_Preview.jpg (3840x2160) [742.5 KB] || EGA_1_Flyby_Preview_searchweb.png (320x180) [79.0 KB] || EGA_1_Flyby_Preview_thm.png (80x40) [5.5 KB] || 20251_OSIRIS-REx_Earth_Gravity_Assist_TWTR.mp4 (1280x720) [24.6 MB] || WEBM-20251_OSIRIS-REx_Earth_Gravity_Assist_APR.webm (960x540) [46.8 MB] || 20251_OSIRIS-REx_Earth_Gravity_Assist_FB_Output.en_US.srt [1.4 KB] || 20251_OSIRIS-REx_Earth_Gravity_Assist_FB_Output.en_US.vtt [1.4 KB] || 20251_OSIRIS-REx_Earth_Gravity_Assist_YT.mp4 (3840x2160) [1.7 GB] || 20251_OSIRIS-REx_Earth_Gravity_Assist_APR.mov (3840x2160) [10.2 GB] || ", "hits": 117 }, { "id": 4139, "url": "http://svs.gsfc.nasa.gov/4139/", "result_type": "Visualization", "release_date": "2017-08-31T14:00:00-04:00", "title": "Voyager 1 Trajectory through the Solar System", "description": "This visualization tracks the trajectory of the Voyager 1 spacecraft through the solar system. Launched on September 5, 1977, it was one of two spacecraft sent to visit the giant planets of the outer solar system. Voyager 1 flew by Jupiter and Saturn before being directed out of the solar system.To fit the 40 year history of the mission into a short visualization, the pacing of time accelerates through most of the movie, starting at about 5 days per second at the beginning and speeding up to about 11 months per second after the planet flybys are past.The termination shock and heliopause are the 'boundaries' created when the plasma between the stars interacts with the plasma flowing outward from the Sun. They are represented with simple grid models and oriented so their 'nose' is pointed in the direction (Right Ascension = 17h 24m, declination = 17 degrees south) represented by more recent measurements from other missions. || ", "hits": 1026 }, { "id": 4140, "url": "http://svs.gsfc.nasa.gov/4140/", "result_type": "Visualization", "release_date": "2017-08-31T14:00:00-04:00", "title": "Voyager 2 Trajectory through the Solar System", "description": "This visualization tracks the trajectory of the Voyager 2 spacecraft through the solar system. Launched on August 20, 1977, it was one of two spacecraft sent to visit the giant planets of the outer solar system. Like Voyager 1, Voyager 2 flew by Jupiter and Saturn, but the Voyager 2 mission was extended to fly by Uranus and Neptune before being directed out of the solar system.To fit the 40 year history of the mission into a short visualization, the pacing of time accelerates through most of the movie, starting at about 5 days per second at the beginning and speeding up to about 11 months per second after the planet flybys are past.The termination shock and heliopause are the 'boundaries' created when the plasma between the stars interacts with the plasma flowing outward from the Sun. They are represented with simple grid models and oriented so their 'nose' is pointed in the direction (Right Ascension = 17h 24m, declination = 17 degrees south) represented by more recent measurements from other missions. || ", "hits": 355 }, { "id": 4143, "url": "http://svs.gsfc.nasa.gov/4143/", "result_type": "Visualization", "release_date": "2017-07-12T10:01:00-04:00", "title": "Saturn's Magnetosphere", "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer. That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959. But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes). The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included. When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current. This is a variation of the simple Luhmann-Friesen magnetosphere model. They are meant to be representative of the basic characteristics of the planetary magnetic fields. Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center. ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann & Friesen, A simple model of the magnetosphereLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ", "hits": 131 }, { "id": 4141, "url": "http://svs.gsfc.nasa.gov/4141/", "result_type": "Visualization", "release_date": "2017-07-12T10:00:00-04:00", "title": "Earth's Magnetosphere", "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer. That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959. But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes). The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. For this Earth visualization, note that the north magnetic pole points out of the southern hemisphere.For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included. When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current. This is a variation of the simple Luhmann-Friesen magnetosphere model. They are meant to be representative of the basic characteristics of the planetary magnetic fields. Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center. ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann and Friesen, A simple model of the magnetosphereLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ", "hits": 314 }, { "id": 4142, "url": "http://svs.gsfc.nasa.gov/4142/", "result_type": "Visualization", "release_date": "2017-07-12T10:00:00-04:00", "title": "Jupiter's Magnetosphere", "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer. That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959. But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes). The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. The volcanic activity on Jupiter's moon Io launches a large amount of sulfur-based compounds along its orbit, which is subsequently ionized by solar ultraviolet radiation. This is represented in the visualization by the yellowish structure along the orbit of Io. This creates a plasma torus and ring current around Jupiter, which alters the planet's magnetic field, forming some of the perturbations in Jupiter's magnetic field along the orbit of Io.For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included. When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current. This is a variation of the simple Luhmann-Friesen magnetosphere model. They are meant to be representative of the basic characteristics of the planetary magnetic fields. Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center. ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann and Friesen, A simple model of the magnetosphereLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ", "hits": 254 }, { "id": 4144, "url": "http://svs.gsfc.nasa.gov/4144/", "result_type": "Visualization", "release_date": "2017-07-12T10:00:00-04:00", "title": "Uranus' Magnetosphere", "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer. That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959. But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes). The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. The rotation axis of Uranus is tilted over ninety degrees relative to the revolution axis of the solar system, placing it roughly in the plane of the solar system. In addition, the magnetic axis has a large tilt relative to the rotation axis. These effects combine to not only give Uranus a more a more variable magnetosphere, but suggest the planet's magnetic field may be generated by a different mechanism than that of Earth, Jupiter and Saturn.For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included. When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current. This is a variation of the simple Luhmann-Friesen magnetosphere model. They are meant to be representative of the basic characteristics of the planetary magnetic fields. Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center. ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann & Friesen, A simple model of the magnetosphereMagnetic reconnection at Uranus' magnetopauseLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ", "hits": 328 }, { "id": 4145, "url": "http://svs.gsfc.nasa.gov/4145/", "result_type": "Visualization", "release_date": "2017-07-12T10:00:00-04:00", "title": "Neptune's Magnetosphere", "description": "Earth's magnetic field creates a 'bubble' around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer. That this field might form a type of 'bubble' around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term 'magnetosphere' was applied to magnetic bubble by Thomas Gold in 1959. But it wasn't until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes). The Voyager program , two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the 'Grand Tour' of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurments of the strength, extent and diversity of the magnetospheres of the outer planets.In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes. The rotation axis of Neptune is highly tilted relative to the revolution axis of the solar system, but nowhere near as extreme as Uranus. It's magnetic axis also has a large tilt relative to the rotation axis. These effects combine to not only give Uranus a more a more variable magnetosphere, but suggest the planet's magnetic field may be generated by a different mechanism than that of Earth, Jupiter and Saturn.For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.Major satellites of the planetary system are also included. When appropriate for the time window of the visualization, the Voyager flyby trajectories are indicated.The models are constructed by combining the fields of a simple magnetic dipole, a current sheet (whose intensity is tuned match the scale of the magnetotail), and occasionally a ring current. This is a variation of the simple Luhmann-Friesen magnetosphere model. They are meant to be representative of the basic characteristics of the planetary magnetic fields. Some features NOT included are longitudes of magnetic poles to a standard planetary coordinate system and offsets of the dipole center from the planetary center. ReferencesT. Gold, Motions in the Magnetosphere of the EarthLuhmann & Friesen, A simple model of the magnetosphereMagnetic reconnection at Neptune's magnetopauseLASP: Polarity of planetary magnetic fieldsWikipedia: The Solar Storm of 1859Wikipedia: Kristian BirkelandWikipedia: Carl StørmerSpecial thanks to Arik Posner (NASA/HQ) and Gina DiBraccio (UMBC/GSFC) for helpful pointers on orientation of planetary rotation and magnetic axes. || ", "hits": 288 }, { "id": 12659, "url": "http://svs.gsfc.nasa.gov/12659/", "result_type": "Produced Video", "release_date": "2017-07-10T12:00:00-04:00", "title": "Colossal Cosmic Waves", "description": "When a small galaxy cluster disturbs a larger one, giant waves emanate for millions of years. || AM06_beta200_t_417_1024x576.jpg (1024x576) [52.5 KB] || AM06_beta200_t_417_1920x1080.jpg (1920x1080) [140.8 KB] || AM06_beta200_t_417.png (7344x4130) [3.5 MB] || AM06_beta200_t_417_searchweb.png (320x180) [37.8 KB] || AM06_beta200_t_417_thm.png (80x40) [3.1 KB] || ", "hits": 65 }, { "id": 12587, "url": "http://svs.gsfc.nasa.gov/12587/", "result_type": "Produced Video", "release_date": "2017-05-02T13:00:00-04:00", "title": "Gigantic Wave Discovered in Perseus Galaxy Cluster", "description": "A wave spanning 200,000 light-years is rolling through the Perseus galaxy cluster, according to observations from NASA's Chandra X-ray Observatory coupled with a computer simulation. The simulation shows the gravitational disturbance resulting from the distant flyby of a galaxy cluster about a tenth the mass of the Perseus cluster. The event causes cooler gas at the heart of the Perseus cluster to form a vast expanding spiral, which ultimately forms giant waves lasting hundreds of millions of years at its periphery. Merger events like this are thought to occur as often as every three to four billion years in clusters like Perseus.Credit: NASA's Goddard Space Flight CenterMusic: \"The Undiscovered\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Perseus_Simulation_Final_Frame_print.jpg (1024x575) [47.6 KB] || Perseus_Simulation_Final_Frame.png (7342x4129) [4.0 MB] || Perseus_Simulation_Final_Frame_thm.png (80x40) [3.3 KB] || Perseus_Simulation_Final_Frame_searchweb.png (320x180) [39.3 KB] || 12587_Perseus_Wind_FINAL_VX-281959_appletv_subtitles.m4v (1280x720) [85.7 MB] || 12587_Perseus_Wind_1080.webm (1920x1080) [18.2 MB] || 12587_Perseus_Wind_FINAL_VX-281959_appletv.m4v (1280x720) [85.6 MB] || 12587_Perseus_Wind_1080.m4v (1920x1080) [160.3 MB] || 12587_Perseus_Wind_1080.mov (1920x1080) [241.7 MB] || 12587_Perseus_Wind_SRT_Caption.en_US.vtt [1.7 KB] || 12587_Perseus_Wind_SRT_Caption.en_US.srt [1.7 KB] || WMV_12587_Perseus_Wind_FINAL_VX-281959_HD.wmv (3840x2160) [154.8 MB] || 12587_Perseus_Wind.mp4 (3840x2160) [306.3 MB] || 12587_Perseus_Wind_Good_4k.mov (3840x2160) [468.4 MB] || 12587_Perseus_Wind_4K.m4v (3840x2160) [792.0 MB] || 12587_Perseus_Wind_FINAL_VX-281959_youtube_hq.mov (3840x2160) [1.2 GB] || 12587_Perseus_Wind_ProRes_3840x2160_2997.mov (3840x2160) [5.2 GB] || ", "hits": 128 }, { "id": 4559, "url": "http://svs.gsfc.nasa.gov/4559/", "result_type": "Visualization", "release_date": "2017-04-27T10:00:00-04:00", "title": "Kepler Stares at Neptune", "description": "In late 2014 and early 2015, NASA's Kepler telescope observed the eighth planet in our solar system, Neptune. Kepler detected Neptune's daily rotation, the movement of clouds, and even minute changes in the sun's brightness, paving the way for future studies of weather and climate beyond our solar system. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks:\"Lost Contact\" – Adam Salkeld & Neil Pollard\"Processing Thoughts\" – Theo Golding || Neptune-Triton-Zoom-Thumbnail.jpg (1920x1080) [1.2 MB] || 4559_Kepler_Neptune_Twitter_720.mp4 (1280x720) [30.6 MB] || WEBM-4559_Kepler_Neptune_APR.webm (960x540) [58.6 MB] || Neptune-Triton-Zoom-Thumbnail_Big.tiff (1920x1080) [11.9 MB] || 4559_Kepler_Neptune_Facebook_720.mp4 (1280x720) [173.0 MB] || 4559_Kepler_Neptune_Captions_Output.en_US.srt [2.8 KB] || 4559_Kepler_Neptune_Captions_Output.en_US.vtt [2.9 KB] || 4559_Kepler_Neptune_APR.mov (1920x1080) [1.9 GB] || 4559_Kepler_Neptune_APR_4444.mov (1920x1080) [4.1 GB] || 4559_Kepler_Neptune_APR.mov.hwshow [205 bytes] || ", "hits": 234 }, { "id": 4548, "url": "http://svs.gsfc.nasa.gov/4548/", "result_type": "Visualization", "release_date": "2017-01-22T11:59:00-05:00", "title": "Category 4 Hurricane Matthew on October 2, 2016", "description": "This data visualization tracks Hurricane Matthew as it intensifies to a Category 5 Hurricane and stops as Matthew turns into a Category 4 Hurricane on October 2, 2016. GPM's GPROF and DPR data swathes are then revealed to show the internal precipitation structure of this strong storm. After most of the DPR data is pulled away, a static 3D wind field is then shown to reveal the flow of air within the structure. DPR is then draped back over the wind fields to show the two datasets together. The winds are derived from GEOS-5. || flyby.1100_print.jpg (1024x576) [116.1 KB] || flyby.1100_searchweb.png (320x180) [68.6 KB] || flyby.1100_thm.png (80x40) [5.2 KB] || flyby_1080p30.mp4 (1920x1080) [31.3 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || flyby_1080p30.webm (1920x1080) [5.8 MB] || flyby4K_2160p30.mp4 (3840x2160) [93.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || flyby_4548.key [33.8 MB] || flyby_4548.pptx [33.5 MB] || flyby_1080p30.mp4.hwshow [179 bytes] || ", "hits": 87 }, { "id": 30816, "url": "http://svs.gsfc.nasa.gov/30816/", "result_type": "Hyperwall Visual", "release_date": "2016-10-10T00:00:00-04:00", "title": "Juno's first flyby of Jupiter", "description": "Image releases from NASA's Juno mission's first orbital flyby of Jupiter include images from JunoCam and the Jovian Infrared Auroral Mapper (JIRAM) instrument.Juno will perform 36 orbital flybys of Jupiter during its mission, which is scheduled to end in February 2018. || ", "hits": 44 }, { "id": 30807, "url": "http://svs.gsfc.nasa.gov/30807/", "result_type": "Hyperwall Visual", "release_date": "2016-09-27T12:00:00-04:00", "title": "Jupiter's North Pole Unlike Anything Encountered in Our Solar System", "description": "NASA's Juno spacecraft sent back this image of Jupiter's north pole taken on August 27, 2016. || pia21030_main_2_north_polar_full-disk_a.png (1558x875) [637.8 KB] || pia21030_main_2_north_polar_full-disk_a_print.jpg (1024x575) [35.7 KB] || pia21030_main_2_north_polar_full-disk_a_searchweb.png (320x180) [30.9 KB] || pia21030_main_2_north_polar_full-disk_a_thm.png (80x40) [2.5 KB] || Jupiter_north_pole_30807.key [3.0 MB] || Jupiter_north_pole_30807.pptx [707.1 KB] || jupiters-north-pole.hwshow [226 bytes] || ", "hits": 51 }, { "id": 12375, "url": "http://svs.gsfc.nasa.gov/12375/", "result_type": "Produced Video", "release_date": "2016-09-26T14:00:00-04:00", "title": "Hubble Directly Images Possible Plumes on Europa", "description": "NASA's Hubble Space Telescope took direct ultraviolet images of the icy moon Europa transiting across the disk of Jupiter. Out of ten observations, Hubble saw what may be water vapor plumes on three of the images. This adds another piece of supporting evidence to the existence of water vapor plumes on Europa - Hubble also detected spectroscopic signatures of water vapor in 2012. The existence of water vapor plumes could provide NASA's Europa flyby mission the opportunity to study the conditions and habitability of Europa's subsurface ocean.Read the full nasa.gov story here: http://www.nasa.gov/press-release/nasa-s-hubble-spots-possible-water-plumes-erupting-on-jupiters-moon-europaRead the full science paper here: http://hubblesite.org/pubinfo/pdf/2016/33/pdf.pdfFull details on the images can be found on HubbleSite.org: http://hubblesite.org/newscenter/archive/releases/2016/33/Additional Resources:JPL's \"Europa: Tempting Target for Future Exploration\" video file is downloadable here: https://vimeo.com/118505538Read the Dec 2013 press release about Hubble's previous observations of Europa here: http://www.nasa.gov/content/goddard/hubble-europa-water-vapor || ", "hits": 111 }, { "id": 12367, "url": "http://svs.gsfc.nasa.gov/12367/", "result_type": "Produced Video", "release_date": "2016-09-08T11:00:00-04:00", "title": "Seeing Jupiter Up Close", "description": "NASA’s Juno spacecraft beams back new images of the solar system’s largest planet. || c-1024.jpg (1024x576) [103.3 KB] || c-1280.jpg (1280x720) [135.3 KB] || c-1024_print.jpg (1024x576) [107.0 KB] || c-1024_searchweb.png (320x180) [57.0 KB] || c-1024_web.png (320x180) [57.0 KB] || c-1024_thm.png (80x40) [5.0 KB] || ", "hits": 57 }, { "id": 40302, "url": "http://svs.gsfc.nasa.gov/gallery/svsyoutube-candidates/", "result_type": "Gallery", "release_date": "2016-06-03T00:00:00-04:00", "title": "SVS YouTube Candidates", "description": "These are the proposed visualization candidates to be included in the SVS YouTube Channel.", "hits": 43 }, { "id": 12080, "url": "http://svs.gsfc.nasa.gov/12080/", "result_type": "Produced Video", "release_date": "2016-02-26T13:15:50-05:00", "title": "A Close Look At Pluto", "description": "NASA’s New Horizons spacecraft reveals features on Pluto never before seen. || c-1920.jpg (1920x1080) [529.9 KB] || c-1280.jpg (1280x720) [344.5 KB] || c-1024.jpg (1024x576) [249.5 KB] || c-1024_print.jpg (1024x576) [258.8 KB] || c-1024_searchweb.png (320x180) [114.3 KB] || c-1024_web.png (320x180) [114.3 KB] || c-1024_thm.png (80x40) [24.1 KB] || ", "hits": 192 }, { "id": 12081, "url": "http://svs.gsfc.nasa.gov/12081/", "result_type": "Produced Video", "release_date": "2016-02-23T11:00:00-05:00", "title": "Charon Makes Its Debut", "description": "NASA’s New Horizons spacecraft provides the first up-close view of Pluto’s largest moon. || c-1280.jpg (1280x720) [113.6 KB] || c-1024.jpg (1024x576) [86.7 KB] || c-1024_print.jpg (1024x576) [84.8 KB] || c-1024_searchweb.png (320x180) [48.9 KB] || c-1024_web.png (320x180) [48.9 KB] || c-1024_thm.png (80x40) [15.6 KB] || ", "hits": 103 }, { "id": 4392, "url": "http://svs.gsfc.nasa.gov/4392/", "result_type": "Visualization", "release_date": "2015-12-08T10:00:00-05:00", "title": "Space Weather to the Edge of the Solar System", "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons2015_40AU.NoSTEREO_1080p30.01000_print.jpg (1024x576) [72.7 KB] || NewHorizons2015_40AU.NoSTEREO_1080p30.mp4 (1920x1080) [27.9 MB] || NewHorizons2015_40AU.NoSTEREO_1080p30.webm (1920x1080) [6.6 MB] || NewHorizons2015_40AU.NoSTEREO.3840x2160_p30.mp4 (3840x2160) [82.5 MB] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || NoSTEREO (3840x2160) [0 Item(s)] || space-weather-to-the-edge-of-the-solar-system-hd1080-movie.hwshow [336 bytes] || ", "hits": 77 }, { "id": 40262, "url": "http://svs.gsfc.nasa.gov/gallery/hubble-space-telescope/", "result_type": "Gallery", "release_date": "2015-12-04T00:00:00-05:00", "title": "Hubble Space Telescope", "description": "Since its launch in 1990, the Hubble Space Telescope has changed our fundamental understanding of the universe. Hubble’s unique design, allowing it to be repaired and upgraded with advanced technology by astronauts, has made it one of NASA’s longest-living and most valuable observatories. Today, Hubble continues to provide views of cosmic wonders never before seen and is still at the forefront of astronomy.\nThe Hubble Space Telescope is an international collaboration between NASA and the European Space Agency (ESA).For more information visit us at https://nasa.gov/hubble or follow us on social media @NASAHubble.", "hits": 330 }, { "id": 40277, "url": "http://svs.gsfc.nasa.gov/gallery/hyperwall20-nov2015/", "result_type": "Gallery", "release_date": "2015-10-10T00:00:00-04:00", "title": "Hyperwall 20 Nov 2015", "description": "Content from the November 20, 2015 Hyperwall Content News mailing list", "hits": 15 }, { "id": 30684, "url": "http://svs.gsfc.nasa.gov/30684/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T15:00:00-04:00", "title": "Flyby of JWST at L2 Point", "description": "A flyby of the James Webb Space Telescope at the second LaGrange point || jwst_flyby-example_frame-1920x1080.png (1920x1080) [1.4 MB] || jwst_flyby-example_frame-1920x1080.jpg (1080x1920) [148.1 KB] || jwst_flyby-example_frame-1920x1080_searchweb.png (180x320) [52.2 KB] || jwst_flyby-example_frame-1920x1080_thm.png (80x40) [4.1 KB] || jwst_flyby-b-1920x1080.wmv (1920x1080) [31.2 MB] || jwst_flyby-b-1280x720.wmv (1280x720) [19.6 MB] || jwst_flyby-b-1280x720.m4v (1280x720) [19.1 MB] || jwst_flyby-b-1920x1080.m4v (1920x1080) [31.1 MB] || jwst_flyby-b-1920x1080p24.webm (1920x1080) [4.6 MB] || jwst_flyby-b-30684.key [22.3 MB] || jwst_flyby-b-30684.pptx [19.9 MB] || jwst_flyby-b-1920x1080p24.mov (1920x1080) [176.2 MB] || flyby-of-jwst-at-l2-point.hwshow [218 bytes] || ", "hits": 52 } ] }