{
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    "next": null,
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    "results": [
        {
            "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": 5421
        },
        {
            "id": 30357,
            "url": "https://svs.gsfc.nasa.gov/30357/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-12-22T12:00:00-05:00",
            "title": "Computer-simulated Global View of Venus",
            "description": "This global view of the surface of Venus is centered at 180 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneer Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. || ",
            "hits": 106
        },
        {
            "id": 30358,
            "url": "https://svs.gsfc.nasa.gov/30358/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-22T12:00:00-04:00",
            "title": "Hemispheric View of Venus",
            "description": "The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98 percent of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km. A mosaic of the Magellan images (most with illumination from the west) forms the image base. Gaps in the Magellan coverage were filled with images from the Earth-based Arecibo radar in a region centered roughly on 0 degree latitude and longitude, and with a neutral tone elsewhere (primarily near the south pole). The composite image was processed to improve contrast and to emphasize small features, and was color-coded to represent elevation. Gaps in the elevation data from the Magellan radar altimeter were filled with altimetry from the Venera spacecraft and the U.S. Pioneer Venus missions. An orthographic projection was used, simulating a distant view of one hemisphere of the planet. || ",
            "hits": 216
        },
        {
            "id": 3728,
            "url": "https://svs.gsfc.nasa.gov/3728/",
            "result_type": "Visualization",
            "release_date": "2010-06-17T00:00:00-04:00",
            "title": "Magellan: Venus False-Color Terrain",
            "description": "This animation is a brief tour of the global terrain of the planet Venus as revealed by radar onboard the Magellan spacecraft. The height of the terrain is color-coded, with blues and greens representing low altitudes and reds representing high altitudes. Highlighted are two large \"continents,\" or highlands, Aphrodite Terra and Ishtar Terra; the Maxwell Montes mountain range; and Maat Mons, a large, currently dormant volcano.Magellan arrived at Venus in August of 1990 and spent four years there collecting data. The elevation map used here was created with data collected during the first mapping cycle. Many of the coverage gaps, represented here by black pixels, were filled in during later mapping cycles. || ",
            "hits": 284
        }
    ]
}