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    "results": [
        {
            "id": 14261,
            "url": "https://svs.gsfc.nasa.gov/14261/",
            "result_type": "Produced Video",
            "release_date": "2023-01-19T16:00:00-05:00",
            "title": "Leaders in Lidar",
            "description": "In this series, we dive into the legacy of Goddard's lead role in developing laser altimetry, which has revolutionized the way we map our planet, the Moon and other planets. Each chapter looks at the successes and failures of these lidar instruments, beginning with the Mars Observer Laser Altimeter in the late 1980s, through the current generation of laser altimeters on ICESat-2 and GEDI. Through dozens of interviews and archival footage, the history, challenges and legacy of lidar are uncovered. || ",
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        {
            "id": 4041,
            "url": "https://svs.gsfc.nasa.gov/4041/",
            "result_type": "Visualization",
            "release_date": "2013-02-08T00:00:00-05:00",
            "title": "GRAIL Free-Air Gravity Map for the Cover of <em>Science</em>",
            "description": "These print-resolution stills were created for the cover of the February 8, 2013 issue of Science. They show the free-air gravity map developed by the Gravity Recovery and Interior Laboratory (GRAIL) mission.If the Moon were a perfectly smooth sphere of uniform density, the gravity map would be a single, featureless color, indicating that the force of gravity at a given elevation was the same everywhere. But like other rocky bodies in the solar system, including Earth, the Moon has both a bumpy surface and a lumpy interior. Spacecraft in orbit around the Moon experience slight variations in gravity caused by both of these irregularities.The free-air gravity map shows deviations from the mean, the gravity that a cueball Moon would have. The deviations are measured in milliGals, a unit of acceleration. On the map, dark purple is at the low end of the range, at around -400 mGals, and red is at the high end near +400 mGals. Yellow denotes the mean.These views show a part of the Moon's surface that's never visible from Earth. They are centered on lunar coordinates 29°N 142°E. The large, multi-ringed impact feature near the center is Mare Moscoviense. The crater Mendeleev is south of this. The digital elevation model for the terrain is from the Lunar Reconnaissance Orbiter laser altimeter (LOLA). Merely for plausibility, the sun angle and starry background are accurate for specific dates (December 21, 2012, 0:00 UT and January 8, 2013, 14:00 UT, respectively). || ",
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        },
        {
            "id": 737,
            "url": "https://svs.gsfc.nasa.gov/737/",
            "result_type": "Visualization",
            "release_date": "1999-10-15T12:00:00-04:00",
            "title": "Images of Earth and Space: SC99 Edition",
            "description": "From our home planet to distant neutron stars, this narrated video tape presents recent scientific visualizations of observation and simulation data. We begin with a dramatic journey over SC99 host city Portland and its surroundings. Later explorations accompany the X-33 aerospace plane on its first test flight, witness Mississippi River flooding, and follow global life over 22 months. New views of Mars reveal a basin that could swallow Mount Everest, while a simulation tests how rovers would navigate the red planet's terrain. We conclude with the first-ever supercomputer model producing a black hole from two merging neutron stars. || ",
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        }
    ]
}