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    "results": [
        {
            "id": 40550,
            "url": "https://svs.gsfc.nasa.gov/gallery/voyager/",
            "result_type": "Gallery",
            "release_date": "2026-03-04T00:00:00-05:00",
            "title": "Voyager",
            "description": "Launched in 1977, the twin Voyager spacecraft are NASA’s longest operating and most distant spacecraft. Hurtling through space at over 38,000 miles per hour, Voyager 1 and 2 were the first confirmed human-made objects to cross the threshold into interstellar space. After completing an in-depth reconnaissance of the outer planets, the Voyager spacecraft departed the heliosphere, the protective bubble of particles and magnetic fields generated by the Sun, in two separate directions and are now exploring the edges of interstellar space. \n\nLearn more: https://science.nasa.gov/mission/voyager/",
            "hits": 408
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        {
            "id": 40521,
            "url": "https://svs.gsfc.nasa.gov/gallery/svsdbgallery2024goddardsummerfilmfest/",
            "result_type": "Gallery",
            "release_date": "2024-06-28T00:00:00-04:00",
            "title": "2024 Goddard Summer Film Fest",
            "description": "Hosted by the Goddard Office of Communications, the 15th annual Goddard Film Festival is a special two-day event this year, highlighting the center’s achievements over the past year in astrophysics, Earth science, heliophysics and planetary science.\n \nOn Wednesday, July 17th at 2 pm, the Goett Auditorium in Building 3 will host a screening that will feature missions and topics such as OSIRIS-REx, PACE, CLPS, Voyager, Hubble, black holes, solar eclipses and much more.",
            "hits": 105
        },
        {
            "id": 20390,
            "url": "https://svs.gsfc.nasa.gov/20390/",
            "result_type": "Animation",
            "release_date": "2024-05-21T11:00:00-04:00",
            "title": "Exploring Planet Uranus Resource Page",
            "description": "Uranus Beauty Pass 1 || Shot4_4kProRes.00001_print.jpg (1024x576) [58.6 KB] || Shot4_4kProRes.00001_searchweb.png (320x180) [29.0 KB] || Shot4_4kProRes.00001_thm.png (80x40) [2.8 KB] || Shot4_4kProRes.00001_web.png (320x180) [29.0 KB] || Shot4_4k_mp4.mp4 [62.1 MB] || Shot4_1k_mp4.mp4 [17.1 MB] || Shot4_4kProRes.mov [1.5 GB] || This page contains the animations that were created for the Exploring Planet Uranus video. The full movie is also available. || ",
            "hits": 212
        },
        {
            "id": 14580,
            "url": "https://svs.gsfc.nasa.gov/14580/",
            "result_type": "Produced Video",
            "release_date": "2024-05-13T10:00:00-04:00",
            "title": "Exploring Planet Uranus",
            "description": "In one of the least explored regions of our solar system, there is an ice giant that scientists believe can help us unlock some of the remaining mysteries of our universe.  This video takes us on a journey there to explore planet Uranus, as well as its rings and moons, highlighting many fascinating features.We also look back on what was discovered by NASA's Voyager 2 spacecraft, as well as subsequent findings by ground-based telescopes and the Hubble Space Telescope. The ongoing search for ocean worlds and life beyond Earth makes Uranus an exciting target for the James Webb Space Telescope and for future up-close exploration. || ",
            "hits": 306
        },
        {
            "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": 133
        },
        {
            "id": 40505,
            "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/",
            "result_type": "Gallery",
            "release_date": "2023-08-28T00:00:00-04:00",
            "title": "Hyperwall Power Playlist - Planetary Science Focus",
            "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide  for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.",
            "hits": 260
        },
        {
            "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": 82
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        {
            "id": 40459,
            "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles5-planetary-fantasia/",
            "result_type": "Gallery",
            "release_date": "2023-05-03T00:00:00-04:00",
            "title": "Cosmic Cycles 5 Planetary Fantasia",
            "description": "Earth’s siblings, the other planets were created at the birth of the solar system. They give us a glimpse of the variety possible in the universe and how rare Earth is. As we explore these other worlds, we fuel our adventurous spirit and discover new wonders at every turn: riverbeds on Mars, volcanoes on Jupiter’s moon Io, auroras on Saturn, and sulfuric-acid clouds on Venus.",
            "hits": 36
        },
        {
            "id": 5032,
            "url": "https://svs.gsfc.nasa.gov/5032/",
            "result_type": "Visualization",
            "release_date": "2022-09-28T14:00:00-04:00",
            "title": "November 8, 2022 Total Lunar Eclipse: Shadow View",
            "description": "Universal Time (UTC). The Moon moves right to left, passing through the penumbra and umbra, leaving in its wake an eclipse diagram with the times at various stages of the eclipse. || shadow_diagram_utc_202211_print.jpg (1024x576) [79.0 KB] || shadow_diagram_utc_202211_searchweb.png (320x180) [44.6 KB] || shadow_diagram_utc_202211_thm.png (80x40) [4.8 KB] || umbracam_utc_202211_1080p30.mp4 (1920x1080) [13.1 MB] || umbracam_utc_202211_720p30.mp4 (1280x720) [7.2 MB] || umbracam_utc_202211_720p30.webm (1280x720) [11.0 MB] || umbracam_utc_202211_2160p30.mp4 (3840x2160) [37.3 MB] || umbracam_utc_202211_360p30.mp4 (640x360) [2.6 MB] || utc (3840x2160) [0 Item(s)] || shadow_diagram_utc_202211.tif (3840x2160) [5.8 MB] || umbracam_utc_202211_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 168
        },
        {
            "id": 14022,
            "url": "https://svs.gsfc.nasa.gov/14022/",
            "result_type": "Produced Video",
            "release_date": "2021-11-18T12:55:00-05:00",
            "title": "Hubble’s Grand Tour of the Outer Solar System",
            "description": "From its vantage point high above Earth’s atmosphere, NASA’s Hubble Space Telescope has completed its annual grand tour of the outer solar system – returning crisp images that are almost as good as earlier snapshots from interplanetary spacecraft. This is the realm of the giant planets— Jupiter, Saturn, Uranus, and Neptune – extending as far as 30 times the distance between Earth and the Sun.For more information, visit https://nasa.gov/hubble.Music Credits: “Crescent Moon” by Laetitia Frenod [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music || ",
            "hits": 43
        },
        {
            "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": 103
        },
        {
            "id": 13645,
            "url": "https://svs.gsfc.nasa.gov/13645/",
            "result_type": "Produced Video",
            "release_date": "2020-06-22T10:00:00-04:00",
            "title": "NASA Scientist Simulates a Kaleidoscope of Sunsets on Other Worlds",
            "description": "A simulation of sunsets on other worlds by NASA Goddard scientist, Geronimo Villanueva.Music credits: \"Immense and Beautiful\" by Victoria Beits from Universal Production Music || 13645_THUMB.jpg (3840x2160) [506.0 KB] || 13645_Planet_Sunset_MASTER.03906_searchweb.png (320x180) [23.3 KB] || 13645_Planet_Sunset_MASTER.03906_thm.png (80x40) [3.1 KB] || 13645_Planet_Sunset_MASTER.webm (960x540) [10.7 MB] || 13645_Planet_Sunset_MASTER_facebook_720.mp4 (1280x720) [108.3 MB] || 13645_Planet_Sunset_MASTER_twitter_720.mp4 (1280x720) [30.8 MB] || 13645_Planet_Sunset_MASTER.mp4 (3840x2160) [133.5 MB] || 13645_PlanetSunset.en_US.srt [58 bytes] || 13645_PlanetSunset.en_US.vtt [66 bytes] || ",
            "hits": 52
        },
        {
            "id": 4666,
            "url": "https://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": 122
        },
        {
            "id": 4667,
            "url": "https://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": 242
        },
        {
            "id": 13006,
            "url": "https://svs.gsfc.nasa.gov/13006/",
            "result_type": "Produced Video",
            "release_date": "2018-07-26T17:00:00-04:00",
            "title": "Hubble Sees Summer Storms on Mars and Saturn",
            "description": "B-Roll || HubbleMarsSaturnBRoll.00001_print.jpg (1024x576) [61.7 KB] || STSCI-H-p1829d-f-1152x1152.png (1152x1152) [360.7 KB] || STSCI-H-p1829d-f-1152x1152_print.jpg (1024x1024) [56.0 KB] || HubbleMarsSaturnBRoll.00001_searchweb.png (320x180) [46.8 KB] || HubbleMarsSaturnBRoll.00001_thm.png (80x40) [5.2 KB] || HubbleMarsSaturnBRoll.00001_print_web.png (320x180) [52.2 KB] || HubbleMarsSaturnBRoll.00001_web.png (320x180) [47.2 KB] || STSCI-H-p1829d-f-1152x1152_web.png (320x320) [33.8 KB] || STSCI-H-p1829d-f-1152x1152_thm.png (80x40) [3.9 KB] || 05-broll.mov (1280x720) [1.2 GB] || HubbleMarsSaturnBRoll.mp4 (1280x720) [88.2 MB] || HubbleMarsSaturnBRoll.webm (1280x720) [12.5 MB] || ",
            "hits": 42
        },
        {
            "id": 12880,
            "url": "https://svs.gsfc.nasa.gov/12880/",
            "result_type": "Produced Video",
            "release_date": "2018-03-05T00:00:00-05:00",
            "title": "Cosmic Designs and The Planets",
            "description": "Greetings and welcome to “Cosmic Designs” a performance by the National Philharmonic presented in partnership with NASA’s Goddard Space Flight Center.“Cosmic Designs” is a voyage that blends together science and art. The pursuit of knowledge and the creative drive for artistic expression are inherent to the human condition. The melding of NASA imagery and symphonic music we present here showcases the imagination that underpins both and highlights how inspiring the combination can be. || CD_Intro_Image_print.jpg (1024x567) [135.2 KB] || CD_Intro_Image.png (2918x1618) [5.8 MB] || CD_Intro_Image_searchweb.png (320x180) [103.7 KB] || CD_Intro_Image_web.png (320x177) [101.8 KB] || CD_Intro_Image_thm.png (80x40) [7.6 KB] || 1.CosmicDesigns_Title_1080.mov (1920x1080) [1.0 GB] || 1.CosmicDesigns_Title_1080.mp4 (1920x1080) [35.9 MB] || 1.CosmicDesigns_Title_1080.webm (1920x1080) [3.3 MB] || 1.CosmicDesigns_Title_4K.mov (3840x2160) [4.3 GB] || 1.CosmicDesigns_Title_4K.mp4 (3840x2160) [55.1 MB] || ",
            "hits": 207
        },
        {
            "id": 12796,
            "url": "https://svs.gsfc.nasa.gov/12796/",
            "result_type": "Produced Video",
            "release_date": "2017-12-13T11:30:00-05:00",
            "title": "2017 AGU Habitability Press Conference",
            "description": "Spanning Disciplines to Search for Life Beyond EarthThe search for life beyond Earth is riding a surge of creativity and innovation. Following a gold rush of exoplanet discovery over the past two decades, it is time to tackle the next step: determining which of the known exoplanets are proper candidates for life. Scientists from NASA and two universities presented new results dedicated to this task in fields spanning astrophysics, Earth science, heliophysics and planetary science — demonstrating how a cross-disciplinary approach is essential to finding life on other worlds — at the fall meeting of the American Geophysical Union on Dec. 13, 2017, in New Orleans, Louisiana.PANELISTS:• Giada Arney, NASA’s Goddard Space Flight Center• Stephen Kane, University of California-Riverside• Katherine Garcia-Sage, NASA’s Goddard Space Flight Center/Catholic University of America• Dave Brain, University of Colorado-Boulder || ",
            "hits": 127
        },
        {
            "id": 4140,
            "url": "https://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": 418
        },
        {
            "id": 4144,
            "url": "https://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": 474
        },
        {
            "id": 4145,
            "url": "https://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": 316
        },
        {
            "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": 100
        },
        {
            "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": 959
        },
        {
            "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": 1098
        },
        {
            "id": 11921,
            "url": "https://svs.gsfc.nasa.gov/11921/",
            "result_type": "Produced Video",
            "release_date": "2015-10-13T11:00:00-04:00",
            "title": "Planetary Portrait",
            "description": "The Hubble Space Telescope provides new maps of Jupiter. || c-1920.jpg (1920x1080) [171.1 KB] || c-1280.jpg (1280x720) [116.9 KB] || c-1024.jpg (1024x576) [89.3 KB] || c-1024_print.jpg (1024x576) [94.5 KB] || c-1024_searchweb.png (320x180) [34.8 KB] || c-1024_web.png (320x180) [34.8 KB] || c-1024_thm.png (80x40) [3.3 KB] || ",
            "hits": 52
        },
        {
            "id": 40246,
            "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-planets/",
            "result_type": "Gallery",
            "release_date": "2015-07-24T00:00:00-04:00",
            "title": "Hyperwall Planets",
            "description": "Hyperwall-ready visualizations featuring planets, moon, and small bodies\nReturn to Main Hyperwall Gallery.",
            "hits": 93
        },
        {
            "id": 40223,
            "url": "https://svs.gsfc.nasa.gov/gallery/heliophysics-education-resources/",
            "result_type": "Gallery",
            "release_date": "2015-01-16T00:00:00-05:00",
            "title": "Heliophysics Education Resources",
            "description": "Visualizations useful for illustrating key concepts.",
            "hits": 119
        },
        {
            "id": 30355,
            "url": "https://svs.gsfc.nasa.gov/30355/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-22T12:00:00-04:00",
            "title": "Hubble Finds Many Bright Clouds on Uranus",
            "description": "This image, orignally published on hubblesite.org, has been prepared for use on the hyperwall.A 1998 Hubble Space Telescope view reveals Uranus surrounded by its four major rings and by 10 of its 17 known satellites. This false-color image was generated by Erich Karkoschka using data taken on August 8, 1998, with Hubble's Near Infrared Camera and Multi-Object Spectrometer. Hubble recently found about 20 clouds—nearly as many clouds on Uranus as the previous total in the history of modern observations.The Wide Field/Planetary Camera 2 was developed by the Jet Propulsion Laboratory and managed by the Goddard Space Flight Center for NASA's Office of Space Science. || ",
            "hits": 51
        },
        {
            "id": 30356,
            "url": "https://svs.gsfc.nasa.gov/30356/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-22T12:00:00-04:00",
            "title": "Uranus in True and False Color",
            "description": "These two pictures of Uranus — one in true color (left) and the other in false color — were compiled from images returned Jan. 17, 1986, by the narrow-angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. The picture is a composite of images taken through blue, green and orange filters. The darker shadings at the upper right of the disk correspond to the day-night boundary on the planet. Beyond this boundary lies the hidden northern hemisphere of Uranus, which currently remains in total darkness as the planet rotates. The blue-green color results from the absorption of red light by methane gas in Uranus' deep, cold and remarkably clear atmosphere. The picture at right uses false color and extreme contrast enhancement to bring out subtle details in the polar region of Uranus. Images obtained through ultraviolet, violet and orange filters were respectively converted to the same blue, green and red colors used to produce the picture at left. The very slight contrasts visible in true color are greatly exaggerated here. In this false-color picture, Uranus reveals a dark polar hood surrounded by a series of progressively lighter concentric bands.  One possible explanation is that a brownish haze or smog, concentrated over the pole, is arranged into bands by zonal motions of the upper atmosphere. The bright orange and yellow strip at the lower edge of the planet's limb is an artifact of the image enhancement. In fact, the limb is dark and uniform in color around the planet. The Voyager project is managed for NASA by the Jet Propulsion Laboratory. || ",
            "hits": 170
        },
        {
            "id": 3846,
            "url": "https://svs.gsfc.nasa.gov/3846/",
            "result_type": "Visualization",
            "release_date": "2011-12-16T00:00:00-05:00",
            "title": "From the Sun to the Earth: The View from STEREO-A with no CME Enhancement",
            "description": "This visualization shows the original dataset from STEREO-A used to extract the motion of the coronal mass ejection (CME) in ID 3890. The data are combined from the SECCHI instrument, which includes an ultraviolet image of the Sun (EUVI), two coronographs (COR-1 & COR-2), and the wide-angle Heliospheric Imagers (HI-1 & HI-2).On this scale, the CME is so faint as to be invisible. However, the Heliospheric Imagers support such a broad range of image intensity that it is possible to observe the CME propagating through the field of view by computing differences of images with the preceeding image. This process is shown in animation #3890.The Earth (left side) and Venus (middle) are so bright as to 'bloom' along the readout line of the CCD (Charge-coupled device) pixels, which creates the bright vertical lines that move slightly with time. The dark shape on the left of the field of view is created by an occulting tab that was installed to (occasionally) hide the bright Earth in the view.The little cross markers label three other planets in the view of STEREO. Uranus is almost invisible in the scale of this imagery, but is visible in full-resolution datasets. || ",
            "hits": 110
        },
        {
            "id": 3890,
            "url": "https://svs.gsfc.nasa.gov/3890/",
            "result_type": "Visualization",
            "release_date": "2011-12-06T00:00:00-05:00",
            "title": "From the Sun to the Earth: CME Enhancement",
            "description": "This visualization shows the dataset from STEREO-A processed to enhance the visibility of the coronal mass ejection (CME) in entry #3846. The data are combined from the SECCHI instrument, which includes an ultraviolet image of the Sun (EUVI), two coronographs (COR-1 & COR-2), and the wide-angle Heliospheric Imagers (HI-1 & HI-2).Because the enhancement process for the CME involves computing differences from a number of sequential HI-1 and HI-2 images, the Earth (left side) and Venus (middle) are masked and oversized icons are installed to mark their position. The dark shape on the left of the field of view is created by an occulting tab that was installed to (occasionally) hide the bright Earth in the view.The little cross markers label three other planets in the view of STEREO. Uranus is almost invisible in the scale of this imagery, but is visible in full-resolution datasets. || ",
            "hits": 52
        },
        {
            "id": 3595,
            "url": "https://svs.gsfc.nasa.gov/3595/",
            "result_type": "Visualization",
            "release_date": "2009-07-27T00:00:00-04:00",
            "title": "Sentinels of the Heliosphere",
            "description": "Heliophysics is a term to describe the study of the Sun, its atmosphere or the heliosphere, and the planets within it as a system. As a result, it encompasses the study of planetary atmospheres and their magnetic environment, or magnetospheres. These environments are important in the study of space weather.As a society dependent on technology, both in everyday life, and as part of our economic growth, space weather becomes increasingly important. Changes in space weather, either by solar events or geomagnetic events, can disrupt and even damage power grids and satellite communications. Space weather events can also generate x-rays and gamma-rays, as well as particle radiations, that can jeopardize the lives of astronauts living and working in space.This visualization tours the regions of near-Earth orbit; the Earth's magnetosphere, sometimes called geospace; the region between the Earth and the Sun; and finally out beyond Pluto, where Voyager 1 and 2 are exploring the boundary between the Sun and the rest of our Milky Way galaxy. Along the way, we see these regions patrolled by a fleet of satellites that make up NASA's Heliophysics Observatory Telescopes. Many of these spacecraft do not take images in the conventional sense but record fields, particle energies and fluxes in situ. Many of these missions are operated in conjunction with international partners, such as the European Space Agency (ESA) and the Japanese Space Agency (JAXA).The Earth and distances are to scale. Larger objects are used to represent the satellites and other planets for clarity.Here are the spacecraft featured in this movie:Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTRACE: Observes the Sun in visible and ultraviolet wavelengths. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. AIM: Images and measures noctilucent clouds. SVS pageGeospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of five satellites to study how magnetospheric instabilities produce substorms. SVS pageL1 Fleet: The L1 point is a Lagrange Point, a point between the Earth and the Sun where the gravitational pull is approximately equal. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. Wind: Measures particle flows and fields in the solar wind. Heliospheric FleetSTEREO-A and B: These two satellites observe the Sun, with imagers and particle detectors, off the Earth-Sun line, providing a 3-D view of solar activity. SVS pageHeliopause FleetVoyager 1 and 2: These spacecraft conducted the original 'Planetary Grand Tour' of the solar system in the 1970s and 1980s. They have now travelled further than any human-built spacecraft and are still returning measurements of the interplanetary medium. SVS pageThis enhanced, narrated visualization was shown at the SIGGRAPH 2009 Computer Animation Festival in New Orleans, LA in August 2009; an eariler version created for AGU was called NASA's Heliophysics Observatories Study the Sun and Geospace. || ",
            "hits": 121
        },
        {
            "id": 3570,
            "url": "https://svs.gsfc.nasa.gov/3570/",
            "result_type": "Visualization",
            "release_date": "2008-12-15T00:00:00-05:00",
            "title": "NASA's Heliophysics Observatories Study the Sun and Geospace",
            "description": "Heliophysics is a term to describe the study of the Sun, its atmosphere or the heliosphere, and the planets within it as a system. As a result, it encompasses the study of planetary atmospheres and their magnetic environment, or magnetospheres. These environments are important in the study of space weather.As a society dependent on technology, both in everyday life, and as part of our economic growth, space weather becomes increasingly important. Changes in space weather, either by solar events or geomagnetic events, can disrupt and even damage power grids and satellite communications. Space weather events can also generate x-rays and gamma-rays, as well as particle radiations, that can jeopardize the lives of astronauts living and working in space.This visualization tours the regions of near-Earth orbit; the Earth's magnetosphere, sometimes called geospace; the region between the Earth and the Sun; and finally out beyond Pluto, where Voyager 1 and 2 are exploring the boundary between the Sun and the rest of our Milky Way galaxy. Along the way, we see these regions patrolled by a fleet of satellites that make up NASA's Heliophysics Observatory Telescopes. Many of these spacecraft do not take images in the conventional sense but record fields, particle energies and fluxes in situ. Many of these missions are operated in conjunction with international partners, such as the European Space Agency (ESA) and the Japanese Space Agency (JAXA).The Earth and distances are to scale. Larger objects are used to represent the satellites and other planets for clarity.Here are the spacecraft featured in this movie:Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTRACE: Observes the Sun in visible and ultraviolet wavelengths. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. AIM: Images and measures noctilucent clouds. SVS pageGeospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of five satellites to study how magnetospheric instabilities produce substorms. SVS pageL1 Fleet: The L1 point is a Lagrange Point between the Sun and the Earth. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. Wind: Measures particle flows and fields in the solar wind. Heliospheric FleetSTEREO-A and B: These two satellites observe the Sun, with imagers and particle detectors, off the Earth-Sun line, providing a 3-D view of solar activity. SVS pageHeliopause FleetVoyager 1 and 2: These spacecraft conducted the original 'Planetary Grand Tour' of the solar system in the 1970s and 1980s. They have now travelled further than any human-built spacecraft and are still returning measurements of the interplanetary medium. SVS pageA refined and narrated version of this visualization, Sentinels of the Heliosphere, is now available. || ",
            "hits": 91
        }
    ]
}