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    "results": [
        {
            "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": 215
        },
        {
            "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": 353
        },
        {
            "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": 194
        },
        {
            "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": 80
        },
        {
            "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": 159
        },
        {
            "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": 133
        },
        {
            "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": 411
        },
        {
            "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": 116
        },
        {
            "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": 918
        },
        {
            "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": 78
        },
        {
            "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": 200
        }
    ]
}