{
    "count": 5,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 5127,
            "url": "https://svs.gsfc.nasa.gov/5127/",
            "result_type": "Visualization",
            "release_date": "2023-07-22T00:00:00-04:00",
            "title": "Lunar South Pole Terrain in Coded Color",
            "description": "A visualization of the south pole of the Moon with labeled craters and elevations in coded color. The view begins with a nearly full Moon as viewed from Earth, flies quickly to the south pole, then circles the pole.",
            "hits": 707
        },
        {
            "id": 3727,
            "url": "https://svs.gsfc.nasa.gov/3727/",
            "result_type": "Visualization",
            "release_date": "2010-06-11T00:00:00-04:00",
            "title": "LOLA Lunar Topography in False Color",
            "description": "This animation is a brief tour of several prominent features of the Moon's terrain: Tycho crater, the south pole, and the South Pole-Aitken basin. The height of the terrain is color-coded, with blues and greens representing low altitudes and reds representing high altitudes. The view is match-moved to a companion piece showing the Moon in natural colors.This is an update of animation 3582, which was produced before the launch of Lunar Reconnaissance Orbiter. Except for the Tycho crater inset, the elevation map in this updated version is based entirely on early results of the Lunar Orbiter Laser Altimeter onboard LRO. These results already represent a substantial improvement in our knowledge of the Moon's topography. || ",
            "hits": 426
        },
        {
            "id": 3686,
            "url": "https://svs.gsfc.nasa.gov/3686/",
            "result_type": "Visualization",
            "release_date": "2010-03-15T00:00:00-04:00",
            "title": "LRO/LOLA Lunar South Pole Flyover",
            "description": "The Lunar Reconnaissance Oribiter (LRO) was launched on June 18, 2009. Its mission is to map the moon's surface, find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology. One of the instruments on board is the  Lunar Orbiter Laser Altimeter (LOLA) which measures landing site slopes, lunar surface roughness, and has begun generation of a high resolution 3D map of the Moon.This visualization uses Clementine data for the global view of the moon, but then transitions to using only LRO/LOLA DEM with a neutral gray texture when flying around the lunar south pole. The DEM by itself creates an amazingly realistic view of the lunar southpole. As better maps are created from the other instruments aboard LRO, an even clearer picture of the moon will emerge.Please note that this visualization is match-frame rendered to The Moon's South Pole in 3D via LRO/LOLA First Light Data (#3633). || ",
            "hits": 308
        },
        {
            "id": 3633,
            "url": "https://svs.gsfc.nasa.gov/3633/",
            "result_type": "Visualization",
            "release_date": "2009-09-16T00:00:00-04:00",
            "title": "The Moon's South Pole in 3D via LRO/LOLA First Light Data",
            "description": "The Lunar Reconnaissance Oribiter (LRO) was launched on June 18, 2009. Its mission is to map the moon's surface, find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology. One of the instruments on board is the  Lunar Orbiter Laser Altimeter (LOLA) which measures landing site slopes, lunar surface roughness, and has begun generation of a high resolution 3D map of the Moon. The animation depicted here is the beginning of  LOLA's mapping project and shows the lunar south pole through digital elevation map data collected by the  LOLA instrument during the spacecraft commissioning phase. During the commissioning phase, LRO was in a highly elliptical orbit coming closer to the lunar south pole than the north pole. Furthermore, since  LOLA uses laser pulses to measure the surface, the accuracy of its measurements are greatly affected by the instrument's distance to the surface. This is why there is virtually no data of the lunar north pole, and much better coverage of the south pole. The topographic data shown here is currently processed to show at approximately 30 meters per pixel.The colors in this animation depict the relative heights of the lunar surface with respect to the surface mean. Warm colors (brown, red, magenta, and tan) indicate areas above the mean. Cooler colors (green, cyan, blue, and violet) are areas below the mean. || ",
            "hits": 247
        },
        {
            "id": 3628,
            "url": "https://svs.gsfc.nasa.gov/3628/",
            "result_type": "Visualization",
            "release_date": "2009-07-17T00:00:00-04:00",
            "title": "Galapagos Islands Flyby",
            "description": "Straddling the equator approximately 1000 kilometers to the west of the South American mainland, the Galapagos Islands lie within the heart of the equatorial current system.  Rising from the sea floor, the volcanic islands of the Galapagos are set on top of a large submarine platform.  The main portion of the Galapagos platform is relatively flat and less than 1000 meters in depth.  The steepest slopes are found along the western and southern flanks of the platform with a gradual slope towards the east.  The interactions of the Galapagos and the oceanic currents create vastly different environmental regimes which not only isolates one part of the Archipelago from the other but allows penguins to live along the equator on the western part of the Archipelago and tropical corals around the islands to the north.  The islands are relatively new in geologic terms with the youngest islands in the west still exhibiting periodic eruptions from their massive volcanic craters. || ",
            "hits": 30
        }
    ]
}