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    "next": null,
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    "results": [
        {
            "id": 2510,
            "url": "https://svs.gsfc.nasa.gov/2510/",
            "result_type": "Visualization",
            "release_date": "2002-08-28T12:00:00-04:00",
            "title": "Mars Odyssey Science Cover Image",
            "description": "This still was created to for the cover of the journal Science (5 July 2002 issue).  It shows epithermal neutron data represented by the colors overlayed on Mars topography.  The blue colors represent high concentrations of hydrogen, indicating the strong possibility that water ice exists in those regions.The vertical exaggeration is 5x normal and the shading exaggeration is 50x normal. || ",
            "hits": 15
        },
        {
            "id": 2447,
            "url": "https://svs.gsfc.nasa.gov/2447/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Smoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole.  This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts). A series of animations was generated to support a Space Science Update (SSU) on the topic.  These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 14
        },
        {
            "id": 2448,
            "url": "https://svs.gsfc.nasa.gov/2448/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Unsmoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole.  This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second.  The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).  A series of animations was generated to support a Space Science Update (SSU) on the topic.  These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 11
        },
        {
            "id": 2449,
            "url": "https://svs.gsfc.nasa.gov/2449/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Viking True Color)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole.  This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second.  The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic.  These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 10
        },
        {
            "id": 2450,
            "url": "https://svs.gsfc.nasa.gov/2450/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Smoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole.  This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second.  The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic.  These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 10
        },
        {
            "id": 2451,
            "url": "https://svs.gsfc.nasa.gov/2451/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Unsmoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 10
        },
        {
            "id": 2452,
            "url": "https://svs.gsfc.nasa.gov/2452/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Viking True Color)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 13
        },
        {
            "id": 2453,
            "url": "https://svs.gsfc.nasa.gov/2453/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Smoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 11
        },
        {
            "id": 2454,
            "url": "https://svs.gsfc.nasa.gov/2454/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Unsmoothed)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 10
        },
        {
            "id": 2455,
            "url": "https://svs.gsfc.nasa.gov/2455/",
            "result_type": "Visualization",
            "release_date": "2002-05-31T12:00:00-04:00",
            "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Viking True Color)",
            "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ",
            "hits": 21
        }
    ]
}