{ "count": 77, "next": null, "previous": null, "results": [ { "id": 14983, "url": "https://svs.gsfc.nasa.gov/14983/", "result_type": "Produced Video", "release_date": "2026-05-08T10:18:00-04:00", "title": "“Cosmic Echoes” Audio Activation", "description": "The experience guides listeners through a narrative journey across space exploration and science.", "hits": 142 }, { "id": 31349, "url": "https://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": 178 }, { "id": 5429, "url": "https://svs.gsfc.nasa.gov/5429/", "result_type": "Visualization", "release_date": "2024-12-05T10:00:00-05:00", "title": "Lucy Earth Gravity Assist 2 Trajectory Visualizations", "description": "Ride-along view of Lucy’s second Earth gravity assist (EGA). The camera follows Lucy as the spacecraft approaches the sunlit side of Earth before crossing into Earth’s shadow as it slingshots around the planet. || lucy_ega2_pov-full.02400_print.jpg (1024x576) [73.5 KB] || lucy_ega2_pov-full.02400_searchweb.png (320x180) [55.6 KB] || lucy_ega2_pov-full.02400_thm.png (80x40) [3.5 KB] || lucy_ega2_pov-full_1080p60.mp4 (1920x1080) [8.5 MB] || lucy_ega2_pov-full [0 Item(s)] || lucy_ega2_pov-full_2160p30.mp4 (3840x2160) [36.4 MB] || lucy_ega2_pov-full_2160p60.mp4 (3840x2160) [34.7 MB] || lucy_ega2_pov-full_2160p60_prores.mov (3840x2160) [3.2 GB] || lucy_ega2_pov-full_2160p60.mp4.hwshow || ", "hits": 94 }, { "id": 31271, "url": "https://svs.gsfc.nasa.gov/31271/", "result_type": "Hyperwall Visual", "release_date": "2024-01-26T00:00:00-05:00", "title": "Webb Views the Outer Planets", "description": "Images by Webb’s Near-Infrared Camera (NIRCam) show Jupiter, Saturn, Uranus, and Neptune. || ", "hits": 105 }, { "id": 14321, "url": "https://svs.gsfc.nasa.gov/14321/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 5: Planetary Fantasia", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Planetary Fantasia\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Planetary_Fantasia_V2_print.jpg (1024x576) [60.4 KB] || Cosmic_Cycles_Planetary_Fantasia_V2.jpg (3840x2160) [465.1 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_searchweb.png (320x180) [40.9 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_thm.png (80x40) [5.2 KB] || Cosmic_Cycles_Planetary_Fantasia.webm (1920x1080) [98.0 MB] || Cosmic_Cycles_Planetary_Fantasia.mp4 (1920x1080) [415.1 MB] || Cosmic_Cycles-Planetary_Fantasia_Online_50mbps.mp4 (1920x1080) [3.5 GB] || Cosmic_Cycles-Planetary_Fantasia_Online_ProRes_1920x1080_2997.mov (1920x1080) [10.9 GB] || ", "hits": 43 }, { "id": 31191, "url": "https://svs.gsfc.nasa.gov/31191/", "result_type": "Hyperwall Visual", "release_date": "2022-08-29T00:00:00-04:00", "title": "Webb’s Jupiter Images Showcase Auroras and Hazes", "description": "A wide field view showcases Jupiter in the upper right quadrant. The planet’s swirling horizontal stripes are rendered in blues, browns, and cream. Electric blue auroras (labeled Northern and Southern Aurora) glow above Jupiter’s north and south poles. A white glow emanates out from the auroras. Along the planet’s equator, rings glow in a faint white. These rings are one million times fainter than the planet itself! At the far left edge of the rings, a moon (labeled as Andrastea) appears as a tiny white dot. Slightly further to the left, another moon (labeled as Amalthea) glows with tiny white diffraction spikes. The rest of the image is the blackness of space, with faintly glowing white galaxies in the distance. Also labeled are spikes of light eminating from the Southern Aurora, which are diffraction spikes. At far left there is also another faint line labeled as a diffraction spike from Jupiter's moon Io. || webb-jupiter-first-image_print.jpg (1024x576) [47.7 KB] || webb-jupiter-first-image.png (3840x2160) [2.9 MB] || webb-jupiter-first-image_searchweb.png (320x180) [31.3 KB] || webb-jupiter-first-image_thm.png (80x40) [3.0 KB] || webbs-jupiter-images-showcase-auroras-and-hazes.hwshow [319 bytes] || ", "hits": 167 }, { "id": 14186, "url": "https://svs.gsfc.nasa.gov/14186/", "result_type": "Produced Video", "release_date": "2022-08-03T14:00:00-04:00", "title": "Lucy’s Solar Powered Journey Continues", "description": "Shortly after Lucy launched, one of its solar arrays failed to fully deploy, putting the mission at risk. Complete transcript available.Universal Production Music: “Hypervelocity” by Sophy Olivia PurnellWatch this video on the NASA Goddard YouTube channel. || Lucy_Solar_Array_Preview_print.jpg (1024x576) [312.0 KB] || Lucy_Solar_Array_Preview.png (3840x2160) [10.3 MB] || Lucy_Solar_Array_Preview.jpg (3840x2160) [1.3 MB] || Lucy_Solar_Array_Preview_searchweb.png (320x180) [101.6 KB] || Lucy_Solar_Array_Preview_thm.png (80x40) [6.6 KB] || 14186_Lucy_Solar_Array_Twitter.mp4 (1280x720) [24.6 MB] || 14186_Lucy_Solar_Array_Twitter.webm (1280x720) [12.3 MB] || 14186_Lucy_Solar_Array_Facebook.mp4 (1920x1080) [138.1 MB] || 14186_Lucy_Solar_Array_Captions.en_US.srt [2.4 KB] || 14186_Lucy_Solar_Array_Captions.en_US.vtt [2.3 KB] || 14186_Lucy_Solar_Array_YouTube.mp4 (3840x2160) [1.3 GB] || 14186_Lucy_Solar_Array_MASTER_V2.mov (3840x2160) [5.4 GB] || ", "hits": 71 }, { "id": 20366, "url": "https://svs.gsfc.nasa.gov/20366/", "result_type": "Animation", "release_date": "2022-08-03T14:00:00-04:00", "title": "Lucy Solar Array Anomaly: Animation", "description": "ANIMATION – Shortly after Lucy launched, one of its solar arrays failed to fully deploy, putting the mission at risk. || Lucy_SP_update_h264_1080.00495_print.jpg (1024x576) [272.9 KB] || Lucy_SP_update_h264_1080.00495_searchweb.png (320x180) [88.7 KB] || Lucy_SP_update_h264_1080.00495_thm.png (80x40) [6.3 KB] || Lucy_SP_update_h264_1080.mp4 (1920x1080) [55.3 MB] || Lucy_SP_update_h264_1080.webm (1920x1080) [2.7 MB] || Lucy_SP_update.mov (3840x2160) [1.5 GB] || Lucy_SP_update_h264_4K.mp4 (3840x2160) [29.5 MB] || Lucy_SP_Update_PNG (3840x2160) [64.0 KB] || ", "hits": 42 }, { "id": 13966, "url": "https://svs.gsfc.nasa.gov/13966/", "result_type": "Produced Video", "release_date": "2021-10-14T10:55:00-04:00", "title": "Water Vapor Detected In Europa’s Atmosphere", "description": "NASA's Hubble Space Telescope observations of Jupiter's icy moon Europa have revealed the presence of persistent water vapor — but, mysteriously, only in one hemisphere. Europa harbors a vast ocean underneath its icy surface, which might offer conditions hospitable for life. This result advances astronomers' understanding of the atmospheric structure of icy moons, and helps lay the groundwork for planned science missions to the Jovian system to, in part, explore whether an environment half-a-billion miles from the Sun could support life. For more information, visit https://nasa.gov/hubble. Additional Credits:Artist’s Impressions of a Water Atmosphere on Europa: ESA/Hubble, J. da SilvaGalileo Spacecraft’s Image of Europa: NASA/JPL-Caltech/SETI InstituteMusic Credits: \"Maps of Deception\" by Idriss-El-Mehdi Bennani [SACEM], Olivier Louis Perrot [SACEM], and Philippe Andre Vandenhende [SACEM] via Sound Pocket Music [PRS] and Universal Production Music. || ", "hits": 168 }, { "id": 13948, "url": "https://svs.gsfc.nasa.gov/13948/", "result_type": "Produced Video", "release_date": "2021-10-05T09:00:00-04:00", "title": "Designing Lucy’s Path to the Trojan Asteroids", "description": "Explore Lucy’s journey to one main-belt asteroid and seven Jupiter Trojans.Complete transcript available.Universal Production Music: “Ocean Simulation” & “The Sequencer Paradox” by Laetitia Frenod; “The Chess Game” by David James Elliott & Martin Gratton; “Tale of Time” by Markus GleissnerWatch this video on the NASA Goddard YouTube channel. || DesigningLucyPreview_print.jpg (1024x576) [277.3 KB] || DesigningLucyPreview.png (3840x2160) [11.6 MB] || DesigningLucyPreview.jpg (3840x2160) [3.2 MB] || DesigningLucyPreview_searchweb.png (320x180) [105.7 KB] || DesigningLucyPreview_thm.png (80x40) [7.2 KB] || 13948_Designing_Lucy_Twitter.webm (1280x720) [50.5 MB] || 13948_Designing_Lucy_Twitter.mp4 (1280x720) [101.0 MB] || 13948_Designing_Lucy_Facebook.mp4 (1920x1080) [559.4 MB] || 13948_Designing_Lucy_Captions.en_US.srt [10.8 KB] || 13948_Designing_Lucy_Captions.en_US.vtt [10.4 KB] || 13948_Designing_Lucy_YouTube.mp4 (3840x2160) [4.4 GB] || 13948_Designing_Lucy_MASTER.mov (3840x2160) [21.6 GB] || ", "hits": 147 }, { "id": 13939, "url": "https://svs.gsfc.nasa.gov/13939/", "result_type": "Produced Video", "release_date": "2021-09-27T09:55:00-04:00", "title": "Hubble Observes Jupiter’s Great Red Spot Changing", "description": "Like the speed of an advancing race car driver, the winds in the outermost “lane” of Jupiter’s Great Red Spot are accelerating – a discovery only made possible by NASA’s Hubble Space Telescope, which has monitored the planet for more than a decade. Researchers analyzing Hubble’s regular “storm reports” found that the average wind speed just within the boundaries of the storm, known as a high-speed ring, has increased by up to 8 percent from 2009 to 2020. In contrast, the winds near the red spot’s innermost region are moving significantly more slowly, like someone cruising lazily on a sunny Sunday afternoon. For more information, visit https://nasa.gov/hubble. Music Credits: \"Underneath the same Moon\" by JC Lemay [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music. || ", "hits": 191 }, { "id": 13892, "url": "https://svs.gsfc.nasa.gov/13892/", "result_type": "Produced Video", "release_date": "2021-07-26T10:55:00-04:00", "title": "Hubble Finds Evidence of Water Vapor at Jupiter’s Moon Ganymede", "description": "Astronomers have used new and archival datasets from NASA’s Hubble Space Telescope to uncover evidence of water vapor in the atmosphere of Jupiter’s moon Ganymede. The vapor is present due to the thermal excitation of water molecules from the moon’s icy surface. Previous research has offered circumstantial evidence for the moon containing more water than all of Earth's oceans. However, temperatures there are so cold that water on the surface freezes and the ocean lies roughly 100 miles below the crust.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Andrea Gianopoulos: Science WriterTracy Vogel: Science WriterAdditional Credits:Artist’s Impression of Ganymede: Credit: ESA/Hubble, M. GarlickArtist’s Impression of a Sublimated Water Atmosphere on Ganymede: Credit: ESA/Hubble, J. daSilvaNASA’s Juno Spacecraft Observation of Ganymede in June 2021Video Artist’s Impression of Ganymede: Credit: ESA/Hubble, M. GarlickGanymede Spinning Globe: Credit: USGS Astrogeology Science CenterMusic Credits: \"Mysterious Discoveries\" by Bertrand Allagnat [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music. || ", "hits": 47 }, { "id": 4839, "url": "https://svs.gsfc.nasa.gov/4839/", "result_type": "Animation", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Interplanetary Dust: Visualizations", "description": "This visualization depicts a region of interplanetary dust that was detected by the Juno spacecraft. The visualization begins with a solar system view of Juno departing Earth and heading to Jupiter. The camera rotates down and a region of dust is revealed between Earth and Mars. Two distinct regions of density are represented using different colors. As the camera pushes into the volume, a portion of the volume is removed to show the interior shape and how it corresponds to the orbit of Mars. || juno_22.3000_print.jpg (1024x576) [69.0 KB] || juno_22.3000_searchweb.png (320x180) [53.2 KB] || juno_22.3000_thm.png (80x40) [3.6 KB] || juno_dust_1080p30.mp4 (1920x1080) [32.3 MB] || juno_dust_1080p60.mp4 (1920x1080) [34.5 MB] || juno_dust_1080p30.webm (1920x1080) [5.9 MB] || juno_dust (3840x2160) [0 Item(s)] || juno_dust_2160p30.mp4 (3840x2160) [170.8 MB] || juno_dust_2160p60.mp4 (3840x2160) [185.7 MB] || juno_dust_1080p30.mp4.hwshow [183 bytes] || ", "hits": 67 }, { "id": 13821, "url": "https://svs.gsfc.nasa.gov/13821/", "result_type": "Produced Video", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Discovers Mars’ Dust Storms Fill Solar System", "description": "NASA’s Juno spacecraft has made a serendipitous discovery: Mars may be ejecting dust into space, creating an interplanetary dust cloud that reflects sunlight, and which can be seen from Earth as the zodiacal light. Complete transcript available.Original musical score by Vangelis, used with permission.Watch this video on the NASA Goddard YouTube channel. || JunoDustCloudPreview_print.jpg (1024x576) [80.3 KB] || JunoDustCloudPreview.png (3840x2160) [8.3 MB] || JunoDustCloudPreview_searchweb.png (320x180) [47.0 KB] || JunoDustCloudPreview_thm.png (80x40) [3.5 KB] || YOUTUBE_1080_13821_Juno_Dust_MASTER_youtube_1080.mp4 (1920x1080) [147.0 MB] || FACEBOOK_720_13821_Juno_Dust_MASTER_facebook_720.mp4 (1280x720) [116.1 MB] || TWITTER_720_13821_Juno_Dust_MASTER_twitter_720.mp4 (1280x720) [19.5 MB] || 13821_Juno_Dust_MASTER.webm (960x540) [41.5 MB] || 13821_Juno_Dust_MASTER.mov (3840x2160) [10.4 GB] || 13821_Juno_Dust_MASTER.mp4 (3840x2160) [888.4 MB] || 13821_Juno_Dust_Captions.en_US.srt [1.8 KB] || 13821_Juno_Dust_Captions.en_US.vtt [1.7 KB] || ", "hits": 227 }, { "id": 20321, "url": "https://svs.gsfc.nasa.gov/20321/", "result_type": "Animation", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Interplanetary Dust: Animations", "description": "Juno during its outbound cruise to Jupiter. Available with and without text. || Juno_Animation_Shot01.00090_print.jpg (1024x576) [53.0 KB] || Juno_Animation_Shot01.00090_searchweb.png (320x180) [40.0 KB] || Juno_Animation_Shot01.00090_thm.png (80x40) [2.4 KB] || Juno_Animation_Shot01.mp4 (3840x2160) [10.3 MB] || Juno_Animation_Shot01 (3840x2160) [0 Item(s)] || Juno_Animation_Shot01_Textless (3840x2160) [0 Item(s)] || Juno_Animation_Shot01.webm (3840x2160) [1.6 MB] || Juno_Animation_Shot01_.mov (3840x2160) [963.3 MB] || Juno_Animation_Shot01_Textless.mov (3840x2160) [962.7 MB] || ", "hits": 50 }, { "id": 13817, "url": "https://svs.gsfc.nasa.gov/13817/", "result_type": "Produced Video", "release_date": "2021-02-25T11:55:00-05:00", "title": "Hubble Spots Comet Near Jupiter", "description": "After traveling several billion miles toward the Sun, a wayward young comet-like object orbiting among the giant planets has found a temporary parking place along the way. The object has settled near a family of captured ancient asteroids, called Trojans, that are orbiting the Sun alongside Jupiter. This is the first time a comet-like object has been spotted near the Trojan population.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Jupiter orbit with Trojan Asteroids: Kel ElkinsJupiter orbit with Trojan Asteroids: Ernie WrightKupier Belt Visualization: Scott WiessingerJupiter’s Wake Visualization: Dan GallagherMusic Credits: \"Infinity\" by Axel Tenner [GEMA], Michael Schluecker [GEMA], and Raphael Schalz [GEMA] via Ed.Berlin Production Music / Universal Production Music GmbH [GEMA] and Universal Production Music. || ", "hits": 71 }, { "id": 13809, "url": "https://svs.gsfc.nasa.gov/13809/", "result_type": "Produced Video", "release_date": "2021-02-10T09:55:00-05:00", "title": "Exploring Our Solar System with Dr. Amy Simon", "description": "Dr. Amy Simon has always been fascinated with space. From a young age she dreamed of lifting off in the Space Shuttle, just like her hero Sally Ride. Over the years her interest in space remained, and she eventually found herself working at NASA.Dr. Simon is the Senior Scientist for Planetary Atmospheres Research in the Solar System Exploration Division at the NASA Goddard Space Flight Center. Her scientific research involves the study of the composition, dynamics, and cloud structure in jovian planet atmospheres, primarily from spacecraft observations like the Hubble Space Telescope.Dr. Simon is also involved in multiple robotic flight missions, as well as future mission concept development. She was a co-investigator on the Cassini Composite Infrared Spectrometer (CIRS) and is the Deputy Instrument Scientist for the OSIRIS-REx Visible and near-IR Spectrometer (OVIRS), as well as the Landsat 9 TIRS2 instrument, and the Lucy L'Ralph instrument Deputy PI. She is PI of the Hubble Outer Planet Atmospheres Legacy (OPAL) program. She recently served as science co-lead of the NASA Ice Giants Mission Concept study.This inspiring woman shows the world that anything is possible, and that you should always work hard to follow your passion in life.For more information, visit https://nasa.gov/hubble. Music Credits: \"Falling Freet\" by Christian Tschuggnall [AKM] and Michael Edwards [APRA] via Atmosphere Music Ltd. [PRS] and Universal Production Music.“Darwin’s Extraordinary Journey” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music. || ", "hits": 39 }, { "id": 13783, "url": "https://svs.gsfc.nasa.gov/13783/", "result_type": "Produced Video", "release_date": "2020-12-15T14:55:00-05:00", "title": "The Outer Planets: Hubble’s Continuing Legacy", "description": "What is OPAL?OPAL (Outer Planet Atmospheres Legacy) is a project to obtain long time baseline observations of the outer planets in order to understand their atmospheric dynamics and evolution as gas giants. The yearly observations from OPAL throughout the remainder of Hubble's operation will provide an important legacy of time-domain images for use by planetary scientists. Viewers might notice that some of the images of the same planets appear to be different colors. This is due to the fact that over the years, from Voyager to Hubble, many different instruments, and many different filters have been used. For more information, visit https://nasa.gov/hubble. Music Credits: “The Granted Wish” by Nicholas Techer [BMI] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music.“Voyage Spectacular” by Rob Lane [PRS] via Abbey Road Masters [PRS], and Universal Production Music.“Celestial Waves” by Harry Vaman [SACEM] via Koka Media [SACEM], and Universal Production Music.“Solar Horizons” by David Rogers [PRS] and Paul Shaw [PRS] via Atmosphere Music Ltd [PRS], and Universal Production Music.“Visionary” by Andy Blythe [PRS] and Marten Joustra [PRS] via Ingenious Music Publishing Ltd. [PRS], and Universal Production Music. || ", "hits": 100 }, { "id": 13693, "url": "https://svs.gsfc.nasa.gov/13693/", "result_type": "Produced Video", "release_date": "2020-08-17T00:00:00-04:00", "title": "Ocean Worlds: The Search for Life", "description": "NASA scientists discuss the search for life on the ocean worlds of our solar system and beyond.Watch this video on the NASA Goddard YouTube channel.Universal Production Music: “Superluminal” by Lee Groves and Peter George Marett; “Earthrise,” “Prism Lights,” and “Uncertain Ahead” by Ben Niblett and Jon Cotton; “Infinite Sky” and “Human Architecture” by Andy Blythe and Marten Joustra; “Imagine If” by Paul WernerComplete transcript available. || 13693OceanWorldsThumbnail2_print.jpg (1024x576) [269.6 KB] || 13693OceanWorldsThumbnail2.jpg (1920x1080) [763.8 KB] || 13693OceanWorldsThumbnail2_searchweb.png (180x320) [88.2 KB] || 13693OceanWorldsThumbnail2_thm.png (80x40) [7.9 KB] || 13693_Ocean_Worlds_GSFC_YouTube.webm (1920x1080) [103.5 MB] || 13693OceanWorldsCaptionsV3.en_US.srt [19.9 KB] || 13693OceanWorldsCaptionsV3.en_US.vtt [19.0 KB] || 13693_Ocean_Worlds_GSFC_Facebook.mp4 (1920x1080) [1.1 GB] || 13693_Ocean_Worlds_GSFC_YouTube.mp4 (1920x1080) [2.9 GB] || 13693_Ocean_Worlds_GSFC_MASTER.mov (1920x1080) [11.8 GB] || ", "hits": 135 }, { "id": 13482, "url": "https://svs.gsfc.nasa.gov/13482/", "result_type": "Produced Video", "release_date": "2020-01-13T10:00:00-05:00", "title": "Lucy Mission Overview: Journey to Explore the Trojan Asteroids", "description": "An overview of the Lucy Mission and its targets, the Trojan Asteroids. This overview features interviews with Hal Levison (Principal Investigator) and Cathy Olkin (Deputy Principal Investigator) from the Southwest Research Institute in Boulder, Colorado. Music is \"Life Choices\" by Universal Production Music. || LUCY_OVERVIEW_MASTER.00035_print.jpg (1024x576) [157.1 KB] || LUCY_THUMB.jpg (3840x2160) [1.4 MB] || LUCY_OVERVIEW_MASTER.00035_searchweb.png (320x180) [88.7 KB] || LUCY_OVERVIEW_MASTER.00035_thm.png (80x40) [6.2 KB] || LUCY_OVERVIEW_MASTER_VX-310983.webm (960x540) [73.8 MB] || LUCY_OVERVIEW_MASTER_VX-310983_facebook_720.mp4 (1280x720) [252.2 MB] || LUCY_OVERVIEW_MASTER_VX-310983_twitter_720.mp4 (1280x720) [41.4 MB] || LUCY_MASTER_SMALLERSIZE.mp4 (3840x2160) [263.2 MB] || Lucy_Subtitles.en_US.srt [5.0 KB] || Lucy_Subtitles.en_US.vtt [5.0 KB] || LUCY_OVERVIEW_MASTER.mov (3840x2160) [13.1 GB] || ", "hits": 87 }, { "id": 13163, "url": "https://svs.gsfc.nasa.gov/13163/", "result_type": "Produced Video", "release_date": "2019-11-18T11:00:00-05:00", "title": "Water Vapor Plumes on Europa", "description": "An international research team led out of NASA’s Goddard Space Flight Center have obtained the first direct detection of water vapor on Jupiter’s moon, Europa. This video explains the findings.Music provided by Killer Tracks: \"Cross the Line\" - Wally Gagel & Xandy BarryKeck Observatory visuals provided by: Sean Goebel/W. M. Keck Observatory || WaterPlumeEuropa_print.jpg (1024x576) [63.5 KB] || EuropaAndJupiter.jpg (1920x1080) [572.4 KB] || WaterPlumeEuropa_searchweb.png (320x180) [79.4 KB] || WaterPlumeEuropa_thm.png (80x40) [6.5 KB] || WaterPlumeEuropa.tif (1920x1080) [7.9 MB] || 13163_WaterVaporEuropa_YouTubeHD.webm (1920x1080) [13.7 MB] || 13163_WaterVaporEuropa_FacebookHD.mp4 (1920x1080) [155.3 MB] || 13163_WaterVaporEuropa_YouTubeHD.mp4 (1920x1080) [201.4 MB] || 13163_WaterVaporEuropa_Captions.en_US.srt [2.4 KB] || 13163_WaterVaporEuropa_Captions.en_US.vtt [2.4 KB] || 13163_WaterVaporEuropa_MASTER.mov (1920x1080) [1.5 GB] || ", "hits": 89 }, { "id": 4719, "url": "https://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": 149 }, { "id": 13352, "url": "https://svs.gsfc.nasa.gov/13352/", "result_type": "Animation", "release_date": "2019-10-21T10:00:00-04:00", "title": "Lucy Trojan Asteroid Mission: Teaser", "description": "Lucy will explore the Jupiter Trojan asteroids – thought to be \"fossils of planet formation.\"Universal Production Music: Canyon of DreamsComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || Lucy_Flyby_CILab_Preview_print.jpg (1024x576) [407.7 KB] || Lucy_Flyby_CILab_Preview.jpg (1920x1080) [1007.3 KB] || Lucy_Flyby_CILab_Preview_searchweb.png (320x180) [79.8 KB] || Lucy_Flyby_CILab_Preview_thm.png (80x40) [5.9 KB] || Lucy_Flyby_CILab_Preview_web.png (320x180) [79.8 KB] || FACEBOOK_720_13352_Lucy_Teaser_MASTER_facebook_720.mp4 (1280x720) [81.1 MB] || TWITTER_720_13352_Lucy_Teaser_MASTER_twitter_720.mp4 (1280x720) [13.7 MB] || 13352_Lucy_Teaser_MASTER.webm (960x540) [29.5 MB] || 13352_Lucy_Teaser_MASTER.mov (3840x2160) [3.6 GB] || YOUTUBE_4K_13352_Lucy_Teaser_MASTER_youtube_4k.mp4 (3840x2160) [495.7 MB] || 13352_Lucy_Teaser_MASTER_Output_V2.en_US.srt [793 bytes] || 13352_Lucy_Teaser_MASTER_Output_V2.en_US.vtt [805 bytes] || ", "hits": 67 }, { "id": 20301, "url": "https://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": 63 }, { "id": 13279, "url": "https://svs.gsfc.nasa.gov/13279/", "result_type": "Produced Video", "release_date": "2019-08-08T09:55:00-04:00", "title": "Hubble’s Brand New Image of Jupiter", "description": "This new Hubble Space Telescope view of Jupiter, taken on June 27, 2019, reveals the giant planet's trademark Great Red Spot, and a more intense color palette in the clouds swirling in Jupiter's turbulent atmosphere than seen in previous years. The colors, and their changes, provide important clues to ongoing processes in planetary atmospheres. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center/Paul Morris/Tracy VogelMusic credits: \"Solaris\" by Axel Tenner [GEMA], Michael Schluecker [GEMA] and Raphael Schalz [GEMA]; Killer Tracks Production Music || ", "hits": 41 }, { "id": 31036, "url": "https://svs.gsfc.nasa.gov/31036/", "result_type": "Hyperwall Visual", "release_date": "2019-04-30T00:00:00-04:00", "title": "Jupiter or Earth?", "description": "Side by side images show similar features despite being from different planets. || jupiter_earth_with_scalebar_print.jpg (1024x576) [100.2 KB] || jupiter_earth_with_scalebar.png (3840x2160) [5.6 MB] || jupiter_earth_with_scalebar_searchweb.png (320x180) [93.5 KB] || jupiter_earth_with_scalebar_thm.png (80x40) [6.7 KB] || jupiter_earth_with_scalebar.hwshow [216 bytes] || ", "hits": 127 }, { "id": 4707, "url": "https://svs.gsfc.nasa.gov/4707/", "result_type": "Infographic", "release_date": "2019-02-22T00:00:00-05:00", "title": "Solar Wind Infographic", "description": "Large image version. PDF for posters linked below. || Solar_Wind_Infographic_Final.jpg (2418x3000) [1.3 MB] || Solar_Wind_Infographic_Final_searchweb.png (320x180) [97.7 KB] || Solar_Wind_Infographic_Final_thm.png (80x40) [7.6 KB] || ", "hits": 64 }, { "id": 4664, "url": "https://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": 191 }, { "id": 13007, "url": "https://svs.gsfc.nasa.gov/13007/", "result_type": "Animation", "release_date": "2018-04-11T00:00:00-04:00", "title": "Jupiter Magnetic Tour", "description": "Take a tour of Jupiter's dynamo, the source of its giant magnetic field, in this new global map from the Juno mission. Watch this video on the NASA.gov Video YouTube channel. || JupiterMagneticTourSmall.mp4 (1920x1080) [71.9 MB] || JupiterMagneticTourPreview.jpg (3840x2160) [1.2 MB] || JupiterMagneticTourPreview_searchweb.png (320x180) [57.0 KB] || JupiterMagneticTourPreview_thm.png (80x40) [3.5 KB] || JupiterMagneticTourProRes.webm (960x540) [28.4 MB] || JupiterMagneticTour1080.mp4 (1920x1080) [193.9 MB] || Foreground_Jupiter_Frames (3840x2160) [0 Item(s)] || Background_Star_Frames (3840x2160) [0 Item(s)] || JupiterMagneticTour4k.mp4 (3840x2160) [492.1 MB] || JupiterMagneticTourProRes.mov (3840x2160) [4.1 GB] || ", "hits": 210 }, { "id": 12878, "url": "https://svs.gsfc.nasa.gov/12878/", "result_type": "Produced Video", "release_date": "2018-03-13T13:00:00-04:00", "title": "Jupiter's Great Red Spot Shrinks and Grows", "description": "NASA scientists have found that not only is Jupiter's Great Red Spot shrinking, but it is actually growing taller and its color is deepening.Music provided by Killer Tracks: \"Moon Leaving\" by Maksim Tyutmanov and Victoria BeitsWatch this video on the NASA.gov Video YouTube channel. || 12878GRSthumbnail_print.jpg (1024x576) [38.9 KB] || 12878GRSthumbnail_searchweb.png (320x180) [29.5 KB] || 12878GRSthumbnail_thm.png (80x40) [3.1 KB] || 12878_GreatRedSpot_YouTubeHD.mp4 (1920x1080) [227.1 MB] || 12878_GreatRedSpot_MASTER.mov (1920x1080) [1.7 GB] || 12878_GreatRedSpot_FacebookHD.mp4 (1920x1080) [182.6 MB] || 12878_GreatRedSpot-Twitter.mp4 (1280x720) [32.9 MB] || 12878_GreatRedSpot_YouTubeHD.webm (1920x1080) [17.1 MB] || 12878GRSthumbnail.tiff (1920x1080) [5.9 MB] || 12878_GreatRedSpot_Captions.en_US.srt [2.5 KB] || 12878_GreatRedSpot_Captions.en_US.vtt [2.5 KB] || ", "hits": 82 }, { "id": 4601, "url": "https://svs.gsfc.nasa.gov/4601/", "result_type": "Visualization", "release_date": "2017-12-18T11:00:00-05:00", "title": "Jupiter Quasi-Quadrennial Oscillation", "description": "Climate patterns on Jupiter can have striking similarities to those on Earth, making the gas giant a natural laboratory for understanding planetary atmospheres. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Lights,\" \"Times Waits,\" \"The Space Between\" || JupiterQQOpreview.jpg (1920x1080) [456.5 KB] || TWITTER_720_4601_Jupiter_QQO_Master_APR_twitter_720.mp4 (1280x720) [37.7 MB] || 4601_Jupiter_QQO_Master.webm (960x540) [72.7 MB] || FACEBOOK_720_4601_Jupiter_QQO_Master_APR_facebook_720.mp4 (1280x720) [218.0 MB] || YOUTUBE_HQ_4601_Jupiter_QQO_Master_APR_youtube_hq.mov (1920x1080) [875.9 MB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.srt [3.8 KB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.vtt [3.8 KB] || 4601_Jupiter_QQO_Master_APR.mov (1920x1080) [2.4 GB] || ", "hits": 116 }, { "id": 4598, "url": "https://svs.gsfc.nasa.gov/4598/", "result_type": "Infographic", "release_date": "2017-11-24T00:00:00-05:00", "title": "Juno Infographic", "description": "TIFF image of the PDF poster (linked below). || Juno_Infographic_print.jpg (1024x975) [242.5 KB] || Juno_Infographic_searchweb.png (320x180) [76.7 KB] || Juno_Infographic_thm.png (80x40) [6.7 KB] || Juno_Infographic.tiff (4743x4517) [12.1 MB] || Some graphics and facts about the Juno mission at Jupiter. || ", "hits": 13 }, { "id": 30904, "url": "https://svs.gsfc.nasa.gov/30904/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "95 Minutes Over Jupiter", "description": "sequence of Juno images across Jupiter || PIA21967_print.jpg (1024x188) [44.5 KB] || PIA21967_searchweb.png (320x180) [72.3 KB] || PIA21967_thm.png (80x40) [5.8 KB] || PIA21967.tif (16000x2952) [77.2 MB] || ", "hits": 36 }, { "id": 30905, "url": "https://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": 76 }, { "id": 30906, "url": "https://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": 97 }, { "id": 30907, "url": "https://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": 29 }, { "id": 12732, "url": "https://svs.gsfc.nasa.gov/12732/", "result_type": "Produced Video", "release_date": "2017-09-25T00:00:00-04:00", "title": "Waves and Changes in Jupiter's Atmosphere", "description": "The movement of Jupiter’s clouds can be seen when comparing these two global maps, in which Jupiter’s cloud bands are laid out as a flat projection. Scientists produced these maps of Jupiter using Hubble Space Telescope observations for the Outer Planet Atmospheres Legacy program taken on January 19, 2015, from 2:00 UT to 12:30 UT and from 15:00 UT to 23:40 UT. In Jupiter’s North Equatorial Belt, Hubble imaged an elusive wave that had been spotted on the planet only once before, decades earlier, by Voyager 2. In Voyager’s images, the wave is barely visible, and nothing like it was seen again until the recent Hubble observations. In the Hubble images, the wave appears as nearly vertical lines passing through the top of the dark, central cloud belt. The wave was found traveling in a region dotted with cyclones and anticyclones. Similar waves—called baroclinic waves—sometimes appear in Earth’s atmosphere where cyclones are forming. The wave may originate in a clear layer beneath the clouds, only becoming visible when it propagates up into the cloud deck. || JupiterBlink6.00001_print.jpg (1024x576) [109.1 KB] || JupiterBlink6.00001_searchweb.png (320x180) [86.8 KB] || JupiterBlink6.00001_thm.png (80x40) [5.5 KB] || JupiterBlink6.mp4 (1920x1080) [14.7 MB] || JupiterBlink6.webm (1920x1080) [840.9 KB] || ", "hits": 38 }, { "id": 12660, "url": "https://svs.gsfc.nasa.gov/12660/", "result_type": "Produced Video", "release_date": "2017-07-17T13:00:00-04:00", "title": "New Brown Dwarf Found by NASA-funded Citizen Science Project", "description": "This illustration shows the average brown dwarf is much smaller than our sun and low mass stars and only slightly larger than the planet Jupiter. Credit: NASA’s Goddard Space Flight Center || Dwarf_Scale_Final_1080.png (1920x1080) [11.3 MB] || Dwarf_Scale_Final_1080.jpg (1920x1080) [764.2 KB] || Dwarf_Scale_Final_1080_print.jpg (1024x576) [278.7 KB] || Dwarf_Scale_Final_5k.png (5760x3240) [92.8 MB] || Dwarf_Scale_Final_5k.jpg (5760x3240) [4.1 MB] || Dwarf_Scale_Final_4k.png (3840x2160) [43.1 MB] || Dwarf_Scale_Final_4k.jpg (3840x2160) [1.7 MB] || ", "hits": 57 }, { "id": 4142, "url": "https://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": 243 }, { "id": 12585, "url": "https://svs.gsfc.nasa.gov/12585/", "result_type": "Produced Video", "release_date": "2017-04-13T14:00:00-04:00", "title": "Europa Water Vapor Plumes - More Hubble Evidence", "description": "The Hubble Space Telescope has captured even more evidence of water vapor plumes on Jupiter's icy moon Europa. The probable plumes appear to be repeating in the same location and correspond with a relatively warm region on Europa's surface observed by the Galileo spacecraft.Read the press release here - https://www.nasa.gov/press-release/nasa-missions-provide-new-insights-into-ocean-worlds-in-our-solar-systemView the release images on the HubbleSite here - http://hubblesite.org/news_release/news/2017-17Read the science paper here - http://iopscience.iop.org/article/10.3847/2041-8213/aa67f8/pdf || ", "hits": 175 }, { "id": 12570, "url": "https://svs.gsfc.nasa.gov/12570/", "result_type": "Produced Video", "release_date": "2017-04-06T13:00:00-04:00", "title": "Hubble Views Jupiter at Opposition", "description": "The Hubble Space Telescope observed Jupiter on April 3rd, 2017 - just days before Jupiter is in opposition on April 7th. This new image of Jupiter is part of Hubble's Outer Planets Atmospheres Legacy program, which is one of many ways Hubble provides science on the Jupiter system. View the NASA.gov web story here - nasa.gov/feature/goddard/2017/hubble-takes-close-up-portrait-of-jupiterEView the HubbleSite release images here - hubblesite.org/news_release/news/2017-15Learn more about Hubble's OPAL program here - archive.stsci.edu/prepds/opal/Learn more about NASA's Juno mission here - nasa.gov/junoLearn more about NASA's planned Europa Clipper mission here - nasa.gov/europa || ", "hits": 58 }, { "id": 12568, "url": "https://svs.gsfc.nasa.gov/12568/", "result_type": "Produced Video", "release_date": "2017-04-04T17:00:00-04:00", "title": "New Hubble Views Of Jupiter Live Shots", "description": "View story about the new Hubble imageClick here fort HubbleSite release images. || HubbleUpdateImage.jpg (720x540) [133.8 KB] || HubbleUpdateImage_print.jpg (1024x768) [212.3 KB] || HubbleUpdateImage_searchweb.png (320x180) [83.6 KB] || HubbleUpdateImage_thm.png (80x40) [6.5 KB] || ", "hits": 140 }, { "id": 30816, "url": "https://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": 33 }, { "id": 30807, "url": "https://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": 80 }, { "id": 12296, "url": "https://svs.gsfc.nasa.gov/12296/", "result_type": "Produced Video", "release_date": "2016-06-29T09:00:00-04:00", "title": "Exploring Jupiter's Magnetic Field", "description": "NASA is sending the Juno spacecraft to peer beneath the cloudy surface of Jupiter. Juno's twin magnetometers, built at Goddard Space Flight Center, will give scientists their first look at the dynamo that drives Jupiter's vast magnetic field. Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || JupiterMagnetometerPreview.jpg (1920x1080) [591.9 KB] || JupiterMagnetometerPreview_searchweb.png (320x180) [118.7 KB] || JupiterMagnetometerPreview_thm.png (80x40) [8.0 KB] || 12296_Juno_Magnetometer_appletv.m4v (1280x720) [159.8 MB] || WEBM_12296_Juno_Magnetometer_APR.webm (960x540) [124.4 MB] || 12296_Juno_Magnetometer_appletv_subtitles.m4v (1280x720) [159.9 MB] || LARGE_MP4_12296_Juno_Magnetometer_APR_large.mp4 (1920x1080) [311.4 MB] || 12296_Juno_Magnetometer_APR_Output.en_US.srt [6.2 KB] || 12296_Juno_Magnetometer_APR_Output.en_US.vtt [6.2 KB] || 12296_Juno_Magnetometer_ipod_sm.mp4 (320x240) [53.1 MB] || 12296_Juno_Magnetometer_APR.mov (1920x1080) [4.1 GB] || ", "hits": 190 }, { "id": 12260, "url": "https://svs.gsfc.nasa.gov/12260/", "result_type": "Produced Video", "release_date": "2016-05-19T13:00:00-04:00", "title": "Hubble's New View of Mars and Planets", "description": "60-second video for social mediaMusic: \"Season of Swag\" by David Travis Edwards and Kenneth Barbee, Killer Tracks [BMI] and Soundcast Music [SESAC] || Hubble_Mars_Instagram_29.97.00148_print.jpg (1024x576) [42.9 KB] || Hubble_Mars_Instagram_29.97.00148_searchweb.png (320x180) [35.3 KB] || Hubble_Mars_Instagram_29.97.00148_web.png (320x180) [35.3 KB] || Hubble_Mars_Instagram_29.97.00148_thm.png (80x40) [3.5 KB] || Hubble_Mars_Instagram_29.97.mp4 (1280x720) [74.4 MB] || Hubble_Mars_Instagram.mp4 (1280x720) [74.1 MB] || Hubble_Mars_Instagram.mov (1280x720) [853.7 MB] || Hubble_Mars_Instagram_29.97.webm (1280x720) [15.1 MB] || Hubble_Mars_Instagram.en_US.srt [1.7 KB] || Hubble_Mars_Instagram.en_US.vtt [1.7 KB] || ", "hits": 59 }, { "id": 11822, "url": "https://svs.gsfc.nasa.gov/11822/", "result_type": "Produced Video", "release_date": "2016-04-14T12:55:00-04:00", "title": "Hubble Memorable Moments", "description": "4. Hubble Memorable Moments: Comet ImpactIn July 1994, the Hubble Space Telescope was poised to use its newly fixed optics to observe one of the most impressive astronomical events of the century - the 21 fragments of Comet Shoemaker-Levy 9 impacting Jupiter. But these observations almost didn’t happen.Watch this video on the NASA Goddard YouTube channel. || Hubble_Memorable_Moments.png (1276x717) [1004.3 KB] || Hubble_Memorable_Moments_print.jpg (1024x575) [98.6 KB] || Hubble_Memorable_Moments_web.png (320x180) [78.1 KB] || Hubble_Memorable_Moments_thm.png (80x40) [7.7 KB] || mem.jpg (320x180) [9.8 KB] || HubbleMemorableMoments_CometImpact.webm (1280x720) [52.1 MB] || HubbleMemorableMoments_CometImpact.mp4 (1280x720) [763.6 MB] || HubbleMemorableMoments_CometImpact.en_US.srt [9.6 KB] || HubbleMemorableMoments_CometImpact.en_US.vtt [9.6 KB] || HubbleMemorableMoments_CometImpact.mov (1280x720) [6.4 GB] || ", "hits": 47 }, { "id": 30710, "url": "https://svs.gsfc.nasa.gov/30710/", "result_type": "Hyperwall Visual", "release_date": "2016-03-15T12:00:00-04:00", "title": "Our Solar System", "description": "The 8 planets plus Pluto with planetary axis tilt || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_print.jpg (1024x576) [75.1 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_searchweb.png (320x180) [49.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_web.png (320x180) [50.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.mp4 (1920x1080) [9.2 MB] || planets3x3_pluto_colorMercury_axis_tilt_720p.mp4 (1280x720) [4.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.webm (1920x1080) [2.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_2160p.mp4 (3840x2160) [28.7 MB] || 3x3_pluto_tilt (4104x2304) [0 Item(s)] || 100-science-overview-001.hwshow || ", "hits": 881 }, { "id": 12018, "url": "https://svs.gsfc.nasa.gov/12018/", "result_type": "Produced Video", "release_date": "2015-10-30T12:45:00-04:00", "title": "Looking for the Shadows of New Worlds", "description": "NASA Goddard astrophysicist Daniel Angerhausen discusses how astronomers may be able to maximize transit photometry to find planets like those in our solar system around other stars -- and possibly moons, rings, and asteroid groups as well. Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Photometry_Still_2.jpg (1280x720) [139.8 KB] || Photometry_Still_2_print.jpg (1024x576) [103.0 KB] || Photometry_Still_2_searchweb.png (320x180) [76.9 KB] || Photometry_Still_2_thm.png (80x40) [6.0 KB] || Photometry_FINAL_ProRes_1280x720_5994.mov (1280x720) [3.6 GB] || Photometry_FINAL-H264_Best_1280x720_5994.mov (1280x720) [1.5 GB] || G2015-081_Photometry_FINAL_V2_youtube_hq.mov (1280x720) [604.7 MB] || Photometry_FINAL-H264_Good_1280x720_2997.mov (1280x720) [123.6 MB] || Photometry_FINAL-MPEG4_1280X720_2997.mp4 (1280x720) [63.2 MB] || G2015-081_Photometry_FINAL_V2_HD.wmv (1280x720) [59.0 MB] || G2015-081_Photometry_FINAL_V2_appletv.m4v (1280x720) [151.8 MB] || Photometry_FINAL_ProRes_1280x720_5994.webm (1280x720) [27.3 MB] || G2015-081_Photometry_FINAL_V2_appletv_subtitles.m4v (1280x720) [149.2 MB] || Photometry_Final_SRT_Captions2.en_US.srt [5.1 KB] || Photometry_Final_SRT_Captions2.en_US.vtt [5.1 KB] || NASA_PODCAST_G2015-081_Photometry_FINAL_V2_ipod_sm.mp4 (320x240) [48.5 MB] || ", "hits": 70 }, { "id": 12021, "url": "https://svs.gsfc.nasa.gov/12021/", "result_type": "Produced Video", "release_date": "2015-10-13T13:00:00-04:00", "title": "Hubble Maps Jupiter in 4k Ultra HD", "description": "New imagery from the Hubble Space Telescope is revealing details never before seen on Jupiter. Hubble’s new Jupiter maps were used to create this Ultra HD animation.Watch this video on the NASA Explorer YouTube channel. || JupiterThumbnailSmall.png (2160x1215) [1.4 MB] || G2015-085_Jupiter720_MASTER_appletv_appletv_subtitles.m4v (1280x720) [39.0 MB] || G2015-085_Jupiter720_MASTER_appletv.m4v (1280x720) [39.0 MB] || WEBM_G2015-085_Jupiter4k_MASTER_YouTube.webm (960x540) [28.5 MB] || G2015-085_Jupiter720_MASTER.mp4 (1280x720) [98.9 MB] || G2015-085_Jupiter720_MASTER_nasa_tv.mpeg (1280x720) [249.3 MB] || G2015-085_Jupiter720_MASTER_prores.mov (1280x720) [917.9 MB] || G2015-085_Jupiter720_MASTER.en_US.srt [98 bytes] || G2015-085_Jupiter720_MASTER.en_US.vtt [111 bytes] || G2015-085_Jupiter720_.key [41.8 MB] || G2015-085_Jupiter720_.pptx [39.3 MB] || G2015-085_Jupiter720_MASTER_12021.key [41.7 MB] || G2015-085_Jupiter720_MASTER_12021.pptx [39.3 MB] || G2015-085_Jupiter4k_MASTER_YouTube.mp4 (3840x2160) [495.9 MB] || G2015-085_Jupiter4k_MASTER.mov (3840x2160) [4.5 GB] || G2015-085_Jupiter4k_MASTER_YouTube.hwshow [94 bytes] || G2015-085_Jupiter720_MASTER_appletv.m4v.hwshow [88 bytes] || ", "hits": 596 }, { "id": 30319, "url": "https://svs.gsfc.nasa.gov/30319/", "result_type": "Hyperwall Visual", "release_date": "2013-10-21T12:00:00-04:00", "title": "Jupiter Globe from Cassini", "description": "This true-color simulated view of Jupiter is composed of four images taken by NASA's Cassini spacecraft. These images were combined and the cylindrical map projected onto a globe in order to illustrate what Jupiter would look like if the cameras used to image this planet had a field-of-view large enough to capture the entire planet. The resolution is about 144 kilometers (89 miles) per pixel. Jupiter's moon Europa is casting the shadow on the planet. || ", "hits": 43 }, { "id": 30138, "url": "https://svs.gsfc.nasa.gov/30138/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "SOFIA view Jupiter in Infrared", "description": "Infrared image of Jupiter from SOFIA's First Light flight composed of individual images at wavelengths of 5.4 (blue), 24 (green) and 37 microns (red) made by Cornell University's FORCAST camera. Ground-based infrared observations are impossible at 5.4 and 37 microns and normally very difficult at 24 microns even from high mountaintop observatories such as Mauna Kea due to absorption by water and other molecules in Earth's atmosphere. The white stripe in the infrared image is a region of relatively transparent clouds through which the warm interior of Jupiter can be seen. A recent visual-wavelength picture of approximately the same side of Jupiter is shown for comparison. (Images are oriented with Jupiter's south pole at the top.) || ", "hits": 36 }, { "id": 11204, "url": "https://svs.gsfc.nasa.gov/11204/", "result_type": "Produced Video", "release_date": "2013-03-14T14:30:00-04:00", "title": "Jupiter's Hot Spots", "description": "Jupiter's bright Equatorial Zone swirls with dark patches, dubbed \"hot spots\" for their infrared glow. These holes in the ammonia clouds at the top of the atmosphere allow a glimpse into Jupiter's darker, hotter layers below. In 1995 NASA's Galileo spacecraft dropped a probe directly into a hot spot, taking the first and only in situ measurements of Jupiter's atmosphere. Now, movies recorded by NASA's Cassini spacecraft reveal that hot spots are not just local weather phenomena, but are in fact linked to much larger-scale atmospheric structures called Rossby waves. || ", "hits": 46 }, { "id": 11036, "url": "https://svs.gsfc.nasa.gov/11036/", "result_type": "Produced Video", "release_date": "2012-09-11T00:00:00-04:00", "title": "Laser Comm: That's a Bright Idea", "description": "Laser light made records obsolete. NASA is on the verge of doing the same thing with space based communications. Before the end of the decade, the Laser Communication Relay Demonstration (LCRD) mission will revolutionize the way we move tons of data from orbit to ground and all around the solar system. || ", "hits": 32 }, { "id": 10958, "url": "https://svs.gsfc.nasa.gov/10958/", "result_type": "Produced Video", "release_date": "2012-05-02T08:00:00-04:00", "title": "Pursuit of Light", "description": "Perhaps more than all other federal agencies, NASA tells stories about big things: big places, big data, big ideas. Using extraordinarily high resolution data sets from some of the most innovative and powerful scientific instruments ever built, the media team at NASA Goddard presents PURSUIT OF LIGHT. The presentation showcases top level goals of NASA's Science Mission Directorate, with an eye toward capturing the imagination of mainstream audiences. Data visualizations at resolutions far greater than HDTV present NASA's science goals like never before. Interspersed with inventive live action footage also designed to make use of that vast canvas, this six and a half minute presentation captivates and moves viewers.PURSUIT OF LIGHT was designed expressly for a screen technology called The Hyperwall, a system largely perfected at NASA Goddard Space Flight Center. The Hyperwall itself is a platform best suited for big themes. With colossal screen resolution and an ultrawide presentational style, moving images played there take on a vast sense of scale and power. PURSUIT OF LIGHT employs the strength of this remarkable system and pushes it further than ever before, presenting stories about the Earth, The Moon, The Sun, The Planets, and the deep sky, wrapped in poetic implication about the humanity's imperative need to explore. This show will play prominently on touring Hyperwalls around the country as well as on the web. || ", "hits": 52 }, { "id": 10927, "url": "https://svs.gsfc.nasa.gov/10927/", "result_type": "Produced Video", "release_date": "2012-03-13T13:00:00-04:00", "title": "RATTLING JET STREAM ON JUPITER", "description": "New movies of Jupiter are the first to catch an invisible wave shaking up one of the giant planet's jet streams, an interaction that also takes place in Earth's atmosphere and influences the weather.For complete transcript, click here. || G2012-013_Jupiter_Weather_portal.00752_print.jpg (1024x576) [69.0 KB] || G2012-013_Jupiter_Weather_portal_web.png (320x180) [190.6 KB] || G2012-013_Jupiter_Weather_portal_thm.png (80x40) [16.5 KB] || G2012-013_Jupiter_Weather.wmv (1280x720) [62.8 MB] || G2012-013_Jupiter_Weather_youtube_hq.mov (1280x720) [70.4 MB] || G2012-013_Jupiter_Weather_appletv.m4v (960x540) [56.5 MB] || G2012-013_Jupiter_Weather_appletv.webmhd.webm (960x540) [27.4 MB] || G2012-013_Jupiter_Weather_portal.mov (640x360) [53.2 MB] || G2012-013_Jupiter_Weather_ipod_lg.m4v (640x360) [22.3 MB] || GSFC_20120313_Jupiter_m10927_Weather.en_US.vtt [2.7 KB] || G2012-013_Jupiter_Weather_prores.mov (1280x720) [1.9 GB] || G2012-013_Jupiter_Weather_ipod_sm.mp4 (320x240) [11.7 MB] || ", "hits": 59 }, { "id": 10848, "url": "https://svs.gsfc.nasa.gov/10848/", "result_type": "Produced Video", "release_date": "2011-10-25T12:00:00-04:00", "title": "Laser Comm: The Next Generation of Space Communications", "description": "NASA is looking for the next generation of space communications technology and Laser Comm may be the answer. Optical communications provide higher bandwidth, which allows for faster data flow and even opens the door to streaming high-def video from distant planets to ground stations on Earth. The Laser Communications Relay Demonstration (LCRD) mission will be put to the test in 2017 on a Loral commercial satellite. There will be ground stations based at JPL in California and White Sands Complex in New Mexico and the demonstration is expected to run for two to three years.(Updated Information) || ", "hits": 41 }, { "id": 10679, "url": "https://svs.gsfc.nasa.gov/10679/", "result_type": "Produced Video", "release_date": "2010-11-02T09:00:00-04:00", "title": "Using Color to Search for Alien Earths", "description": "NASA astronomer Lucy McFadden and UCLA graduate Carolyn Crow recently made a discovery that will help identify characteristics of extrasolar planets, such as the compositions of their surfaces and atmospheres. By comparing the reflected red, blue, and green light from planets in our solar system, a team led by Crow and McFadden was able to group the planets according to their similarities. As it turns out, the planets fall into very distinct regions on this plot, where the vertical direction indicates the relative amount of blue light, and the horizontal direction the relative amount of red light. This technique works even when the source of the reflected light is visible only as a point, like exoplanets appear when observed through a telescope. Therefore, scientists can use it to identify earthlike planets more easily. || ", "hits": 203 }, { "id": 3636, "url": "https://svs.gsfc.nasa.gov/3636/", "result_type": "Visualization", "release_date": "2009-09-25T00:00:00-04:00", "title": "Hubble Space Telescope Observes the Comet P/Shoemaker-Levy 9 Collision with Jupiter", "description": "From July 16 through July 22, 1994, pieces of an object designated as Comet P/Shoemaker-Levy 9 collided with Jupiter. This is the first collision of two solar system bodies ever to be observed, and the effects of the comet impacts on Jupiter's atmosphere have been simply spectacular and beyond expectations. Comet Shoemaker-Levy 9 consisted of at least 21 discernable fragments with diameters estimated at up to 2 kilometers. IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ", "hits": 51 }, { "id": 3520, "url": "https://svs.gsfc.nasa.gov/3520/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Flow Field Representation of Jupiter's Great Red Spot", "description": "This visualization shows a simple simulated flow field representation of Jupiter's Great Red Spot. The flow field is static (i.e., the wind directions don't change over time). This visualization was created in support of the Science On a Sphere film called \"Largest\" which is about Jupiter. These frames were rendered \"flat\" and are intended to be duplicated several times around the sphere. || ", "hits": 16 }, { "id": 3604, "url": "https://svs.gsfc.nasa.gov/3604/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Pull out from Jupiter Showing Moon Orbits", "description": "NOTE: The orbital plane of the moons in these visualizations is incorrect. The Galilean moons should be aligned to Jupiter's equator.This visualization shows jupiter and 63 of its moons. We start close in to Jupiter showing relativly fast moving inner moons that are generally in the same orbital plane including the so called 'Galilean moons': Europa, Io, Ganymede, and Callisto. Other inner moons are: Amalthea, Thebe, Adrastea, and Metis. These inner moons orbit Jupiter as fast as about every 7 hours to about every 17 days. These moons are also relativly close to Jupiter: from around 100 thousand to a couple of million kilometers away.We pull back revealing many smaller moons much farther away (tens of millions of kilometers) in much longer orbits (up to several years). Time speeds up to show the motion of these moons in irregular orbits. The following outer moons are displayed: Himalia, Elara, Pasiphae, Sinope, Lysithea, Carme, Ananke, Leda, Callirrhoe, Themisto, Megaclite, Taygete, Chaldene, Harpalyke, Kalyke, Iocaste, Erinome, Isonoe, Praxidike, Autonoe, Thyone, Hermippe, Aitne, Eurydome, Euanthe, Euporie, Orthosie, Sponde, Kale, Pasithee, Hegemone, Mneme, Aoede, Thelxinoe, Arche, Kallichore, Helike, Carpo, Eukelade, Cyllene, Kore, S/2000 J11, S/2003 J2, S/2003 J3, S/2003 J4, S/2003 J5, S/2003 J9 ,S/2003 J10, S/2003 J12, S/2003 J15, S/2003 J16, S/2003 J17, S/2003 J18, S/2003 J19, and S/2003 J23.This visualization was created in support of the Science On a Sphere film called \"Largest\" which is about Jupiter. The visualziation was choreographed to fit into \"Largest\" as a layer that is Intended to be composited with other layers including a background starfield. Three copies of this shot are arranged with orbits that fade on as we pull back in order to facilitate a seamless inset (without orbits falling off the boarder) on the Science On a Sphere composited frames. || ", "hits": 197 }, { "id": 3607, "url": "https://svs.gsfc.nasa.gov/3607/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Shoemaker-Levy 9 Hitting Jupiter with Orbit Trails", "description": "This visualziation shows the major fragments of comet Showmaker-Levy 9 colliding with Jupiter. The orbits are driven using ephemeris data. The impacts occurred over a series of about six Earth days which is why Jupiter (which rotates about once every Earth 10 hours) appears to be rotating so fast in this visualization; time is is depicted at about 7 hours per second of animation.The comet fragments shown are: \"a\", \"b\", \"c\", \"d\", \"e\", \"f\", \"g\", \"h\", \"k\", \"l\", \"n\", \"p\", \"p\", \"q\", \"q\", \"r\", \"s\", \"t\", \"u\", \"v\", and \"w\". Several letters were skipped (due to lack of ephemeris) and 2 letters \"p\" and \"q\" appear twice; these are also known as \"p1\", \"p2\", \"q1\", and \"q2\".This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layer that is intended to be composited with other layers including a match-rendered background star field. Three copies of this shot are arranged in order to facilitate a seamless inset on the Science On a Sphere composited frames. || ", "hits": 74 }, { "id": 3608, "url": "https://svs.gsfc.nasa.gov/3608/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "One Thousand Earths Could Fit Inside Jupiter", "description": "This animation illustrates that it would take about 1000 Earths to fill a volume the size of Jupiter.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layer that is intended to be composited with other layers. In this case, mulitple layers are provided to make the it appear as if a sphere were filling up with Earths. These frames are in cylindrical equidistant projection and are intended to be viewed wrapped to a sphere. A sample composite of the layers is provided to show how the shot might be composed from the source layers. || ", "hits": 219 }, { "id": 3609, "url": "https://svs.gsfc.nasa.gov/3609/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Rotation Period Comparison Between Earth and Jupiter", "description": "This animation illustrates the difference in the rotational period between the Earth and Jupiter. Earth rotates once in 24 hours; whereas, Jupiter rotates more quickly, taking only about 10 hours. This means that Jupiter rotates about 2 1/2 times faster than the Earth. However, Jupiter is about 11 times bigger than the Earth, so matter near the outer 'surface' of Jupiter is travelling much faster (about 30 times faster) than matter at the outer 'surface' of Earth.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layers intended to be composited. The 2 animations of Earth and Jupiter are match rendered so that if played back at the same frame rate (say 30 frames per second), the relative rotational speed differences will be accurate. An example composite is provided for reference; in this composite, only a portion of Jupiter is shown so that the relative sizes of the planets are also represented. The composited shot is designed to be repeated around the scienice on a sphere display several times. || ", "hits": 984 }, { "id": 3610, "url": "https://svs.gsfc.nasa.gov/3610/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Jupiter Cloud Sequence from Cassini", "description": "When the Cassini mission flew by the planet Jupiter in late 2000, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation. The elapsed time between each interpolated frame corresponds to about 1 hour. More info on the image sequence is available at Jupiter Mosaics and Movies - Rings, Satellites, AtmosphereIMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ", "hits": 121 }, { "id": 3611, "url": "https://svs.gsfc.nasa.gov/3611/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Jupiter Cloud Sequence from Voyager 1", "description": "When the Voyager 1 mission flew by the planet Jupiter in March of 1979, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping and data gaps. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ", "hits": 52 }, { "id": 3614, "url": "https://svs.gsfc.nasa.gov/3614/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Jupiter Cloud Sequence from Voyager 2", "description": "When the Voyager 2 mission flew by the planet Jupiter in July of 1979, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping and data gaps. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ", "hits": 42 }, { "id": 3616, "url": "https://svs.gsfc.nasa.gov/3616/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Galilean moon orbits from Callisto into Jupiter", "description": "NOTE: The orbital plane of the moons in these visualizations is incorrect. The Galilean moons should be aligned to Jupiter's equator.This visualization starts close in on Jupiter's moon Callisto. We pull back and start moving in towards Jupiter, passing Ganymede on the way. Io and Europa are off in the distance behind Jupiter as we push in and Jupiter fills the screen.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layers to be composited in post-production. There are five separate layers that were designed to give the editors flexibility in reagrds to when particular objects faded in/out. There are three layers that are identical except that Callisto and Jupiter are offset 0, 120, and 240 degrees; this is for a zoom out/in effect that transitions quickly to fully wrapped images of Callisto/Jupiter. A background layer contains only Io and Europa. Finally a layer with Jupiter as a gray ball in included for use in masking. All of the layers are intended to be composited over a starfield. Since there is very little camera motion other than a push in, a moving starfield is not provided for this shot.A composite movie is included to illustrate how the layers were intended to be used. || ", "hits": 87 }, { "id": 3617, "url": "https://svs.gsfc.nasa.gov/3617/", "result_type": "Visualization", "release_date": "2009-09-21T00:00:00-04:00", "title": "Inner moons of Jupiter Push In to Europa", "description": "This visualization starts showing the orbits of Jupiter's inner moons (Europa, Io, Ganymede, Callisto, Amalthea, Thebe, Adrastea, and Metis). As the orbits procede we begin to zero in on Europa. Other moons and orbits fade away as we push in to Europa filling the screen.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. Mulitple layer offset 120 degrees from each other are intended to overlay the orbits. A Europa label is provided so that it can be faded out in post production. A separate layer for Jupiter is also provided so that the other moons and orbit trails can also be faded out, leaving only Jupiter. || ", "hits": 85 }, { "id": 10477, "url": "https://svs.gsfc.nasa.gov/10477/", "result_type": "Produced Video", "release_date": "2009-09-04T00:00:00-04:00", "title": "LARGEST: A Spherical Movie About Jupiter", "description": "NASA's home for spherical films on Magic Planet. Download the Magic Planet-ready movie file here.Three hundred and eighty million miles from Earth, the solar system's largest planet spins like a sizzling top in the night, massive and powerful beyond all comparison short of the sun itself. It's therefore only fitting—and certainly about time—that the fifth planet receive its proper cinematic due, set naturally on the most appropriate cinematic platform. With the movie LARGEST, Jupiter comes to Science On a Sphere.LARGEST examines the gas giant like a work of art, like a destination of celestial wonder. Starting with the basics, the movie examines the gross anatomy of the immense planet. From swirling winds to astounding rotational velocity to unimaginable size, Jupiter demands nothing less than a list of superlatives. But where general description sets the stage, LARGEST parts the curtains on humanity's experience with the fifth planet. The movie takes us on a journey to this immense sphere via dramatic fly-bys with some of the most astounding robotic probes ever designed. Then, with NASA instruments trained on the striped behemoth, the drama really begins.NASA released LARGEST on September 15, 2009. It is one in a series of spherical movies created entirely by staff at the NASA Goddard Space Flight Center. But while the process to create a fully spherical movie is something of an in-house Goddard creation, the Science On a Sphere projection system itself is an invention of the space agency's sibling NOAA.This film has been prepared exclusively for playback on spherical projections systems. It will not play properly on a traditional computer or television screen. If you are interested in downloading the complete final movie file for spherical playback, please visit ftp://public.sos.noaa.gov/extras/.For more information about the movie itself, visit the main website at www.nasa.gov/largest. || ", "hits": 67 }, { "id": 2946, "url": "https://svs.gsfc.nasa.gov/2946/", "result_type": "Visualization", "release_date": "2006-05-15T12:00:00-04:00", "title": "Europa's Synthetic Subsurface Heat Transport (Version 2)", "description": "Encounters with Jupiter's moon Europa by the Voyager and Galileo spacecraft indicated that a liquid salty ocean might exist below a layer of surface ice that is up to 10 kilometers thick. An ocean general circulation model developed to study the earth's oceans was used to investigate the tidally-forced ocean circulations on Europa. The orbit of Europa is 'gravity locked' so that the same side of Europa always faces Jupiter as is the case with the earth's moon. The icy surface of Europa heaves up and down 50 meters due to the strong tidal forces. This visualization shows the temperature changes induced from the flow fields calculated for a European ocean 50 kilometers deep. The warmest temperatures tend to be near the equator, not because of heating by the sun, but because the currents in the European ocean move the warmest waters to that location. Understanding the thermal and flow fields from these model runs will help to interpret observations from future missions to Europa such as the Jupiter's Icy Moons Orbiter mission proposed for launch in 2012. || ", "hits": 39 }, { "id": 2947, "url": "https://svs.gsfc.nasa.gov/2947/", "result_type": "Visualization", "release_date": "2006-05-15T12:00:00-04:00", "title": "Europa's Synthetic Subsurface Heat Transport (Version 1)", "description": "Under Europa's icy surface are vast extraterrestrial oceans. This conceptual animation depicts simulated heat transport of these subsurface oceans. Please note that the simulated heat transport in this animation is only conceptual and a more accurate representation can be found at animation #2946. || ", "hits": 47 }, { "id": 20043, "url": "https://svs.gsfc.nasa.gov/20043/", "result_type": "Animation", "release_date": "2004-12-03T12:00:00-05:00", "title": "Coronal Mass Ejections Blast their Way Through the Solar System", "description": "A coronal mass ejection erupts from the Sun and propagates out through the Solar System. Along the way it is detected by the spacecraft at Jupiter and Saturn. Eventually it is detected by the two Voyager spacecraft beyond the orbit of Pluto. || XflareLRG_pre.00002_print.jpg (1024x768) [90.5 KB] || XflareLRG_pre.jpg (320x240) [65.8 KB] || XFlares_pre.jpg (320x238) [11.3 KB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || XflareLRG.webmhd.webm (960x540) [5.4 MB] || CME_SS0001.mp4 (1920x1080) [17.7 MB] || XflareLRG.mpg (720x486) [10.7 MB] || XFlares.mpg (320x240) [7.0 MB] || ", "hits": 55 }, { "id": 3041, "url": "https://svs.gsfc.nasa.gov/3041/", "result_type": "Visualization", "release_date": "2004-11-01T12:00:00-05:00", "title": "Lunar Fly By and Earth Approach", "description": "This is an animation flying over the surface of the moon then approaching the earth. It was created in support of a presentation at the National Air and Space Museum (NASM) in October 2004. Scales are not accurate in this visualization. The Earth is about 3 times larger than it would actually appear. The source of the moon texture is unknown; it is thought to be a composite from several missions. The Earth texture was captured as the Galileo spacecraft swung by the Earth in 1990 for a gravity assist on its way to Jupiter. || ", "hits": 85 }, { "id": 2963, "url": "https://svs.gsfc.nasa.gov/2963/", "result_type": "Visualization", "release_date": "2004-07-08T12:00:00-04:00", "title": "The NOAA POES Satellite Detects Record Particle Flows into the Earth's Upper Atmosphere", "description": "This set of still images from the NOAA/POES satellite are derived from measurements by particle detectors in low Earth orbit. The data are sampled along the orbit track and then interpolated in time and position for the rest of the polar region. This interpolation is responsible for the curved block-shaped artifacts in the images. || ", "hits": 35 }, { "id": 84, "url": "https://svs.gsfc.nasa.gov/84/", "result_type": "Visualization", "release_date": "1995-03-24T12:00:00-05:00", "title": "Simulations of the Breakup of Comet Shoemaker-Levy 9 Employing a Swarm Model: Initial Conditions", "description": "The breakup of comet Shoemaker-Levy 9 due to its gravitational interaction with Jupiter in July, 1994 is simulated using a swarm model. In this simulation, the comet is modeled as an initially spherical distribution of 16,384 particles. The particles interact with the tidal field of Jupiter and with each other through inter-particle gravitation and collisions. All simulations were performed on the Maspar MP-2 at NASA/GSFC. || ", "hits": 25 }, { "id": 85, "url": "https://svs.gsfc.nasa.gov/85/", "result_type": "Visualization", "release_date": "1995-03-24T12:00:00-05:00", "title": "Simulations of the Breakup of Comet Shoemaker-Levy 9 Employing a Swarm Model: Dynamical Evolution", "description": "The breakup of comet Shoemaker-Levy 9 due to its gravitational interaction with Jupiter in July, 1994 is simulated using a swarm model. In this simulation, the comet is modeled as an initially spherical distribution of 16,384 particles. The particles interact with the tidal field of Jupiter and with each other through inter-particle gravitation and collisions. All simulations were performed on the Maspar MP-2 at NASA/GSFC. || ", "hits": 70 } ] }