{
    "count": 18,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 30835,
            "url": "https://svs.gsfc.nasa.gov/30835/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-08-30T00:00:00-04:00",
            "title": "NASA's Planetary Fleets, Including Mars, Venus, Discovery Missions, and Small Body Missions",
            "description": "The Planetary Fleet || planetary_fleet_spiral_04017024_print.jpg (1024x576) [208.9 KB] || planetary_fleet_spiral_04017024.png (3840x2160) [9.8 MB] || planetary_fleet_spiral_04017024_searchweb.png (320x180) [89.8 KB] || planetary_fleet_spiral_04017024_web.png (320x180) [89.8 KB] || planetary_fleet_spiral_04017024_thm.png (80x40) [6.5 KB] || nasas-planetary-fleet.hwshow [307 bytes] ||",
            "hits": 226
        },
        {
            "id": 4414,
            "url": "https://svs.gsfc.nasa.gov/4414/",
            "result_type": "Visualization",
            "release_date": "2016-03-21T12:30:00-04:00",
            "title": "The Mars Fleet",
            "description": "A fleet of landers, rovers, and orbiters is exploring the Red Planet, providing mission controllers with a remote presence on Mars. This visualization is available for download in 4K Ultra HD. || MarsFleetClosePreview.jpg (1920x1080) [168.3 KB] || MarsFleetClosePreview_searchweb.png (320x180) [55.1 KB] || MarsFleetClosePreview_thm.png (80x40) [5.4 KB] || Mars_Fleet_SVS_4414.00015_searchweb.png (320x180) [66.1 KB] || mars_fleet_Mar2016_4k_2160p30.00015_searchweb.png (320x180) [61.1 KB] || mars_fleet_Mar2016_HD_1080p60.mp4 (1920x1080) [14.9 MB] || version1 (1920x1080) [0 Item(s)] || mars_fleet_Jan2016_1080p30.webm (1920x1080) [4.3 MB] || mars_fleet_Mar2016_4k_2160p30.mp4 (3840x2160) [48.6 MB] || mars_fleet_Mar2016_640x360.m4v (640x360) [6.7 MB] || version1 (3840x2160) [0 Item(s)] || Mars_Fleet_SVS_4414.mov (1920x1080) [1.2 GB] || Mars_Fleet_SVS_4414_4k.mov (3840x2160) [4.6 GB] || mars-fleet-and-landings.hwshow || mars_solar_wind_compiled.hwshow || ",
            "hits": 99
        },
        {
            "id": 4436,
            "url": "https://svs.gsfc.nasa.gov/4436/",
            "result_type": "Visualization",
            "release_date": "2016-03-21T12:30:00-04:00",
            "title": "GMM-3 Mars Gravity Map",
            "description": "Scientists have used small fluctuations in the orbits of three NASA spacecraft to map the gravity field of Mars.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.This video is also available on our YouTube channel. || MarsGravityMapYouTube.png (1920x1080) [7.9 MB] || MarsGravityMapYouTube.jpg (1920x1080) [706.6 KB] || APPLE_TV_G2016-003_Mars_Gravity_Map_MASTER_appletv.m4v (1280x720) [51.0 MB] || WEBM_G2016-003_Mars_Gravity_Map_MASTER.webm (960x540) [43.4 MB] || APPLE_TV_G2016-003_Mars_Gravity_Map_MASTER_appletv_appletv_subtitles.m4v (1280x720) [15.5 MB] || LARGE_MP4_G2016-003_Mars_Gravity_Map_MASTER_large.mp4 (1920x1080) [109.0 MB] || NASA_TV_G2016-003_Mars_Gravity_Map_MASTER.mpeg (1280x720) [362.0 MB] || G2016-003_Mars_Gravity_Map_MASTER_GoogOut.en_US.srt [1.8 KB] || G2016-003_Mars_Gravity_Map_MASTER_GoogOut.en_US.vtt [1.9 KB] || G2016-003_Mars_Gravity_Map_MASTER.mov (1920x1080) [2.9 GB] || ",
            "hits": 133
        },
        {
            "id": 11875,
            "url": "https://svs.gsfc.nasa.gov/11875/",
            "result_type": "Produced Video",
            "release_date": "2015-05-21T06:00:00-04:00",
            "title": "NASA On Air: NASA’s Curiosity Sees Blue Sunset On Mars (5/21/2015)",
            "description": "LEAD: NASA’s Curiosity rover captured its first Mars sunset in color and indicates the sky is blue.1. This Martian sunset sequence was captured over seven minutes on April 15, 2015.2. Why is it blue?3. On Earth our sunsets are red because the molecules in the atmosphere scatter or filter out the blue wavelength light.4. On Mars the Martian dust particles permit blue light to penetrate the atmosphere more efficiently than light that is red in color.TAG: Dust in the Martian atmosphere is common during its spring season. || WC_MarsSunset-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [69.5 KB] || WC_MarsSunset-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [58.6 KB] || WC_MarsSunset-1920-MASTER_iPad_1920x0180_web.png (320x180) [58.6 KB] || WC_MarsSunset-1920-MASTER_iPad_1920x0180_thm.png (80x40) [4.6 KB] || WC_MarsSunset-1920-MASTER_1920x1080.mov (1920x1080) [296.0 MB] || WC_MarsSunset-1920-MASTER_1280x720.mov (1280x720) [325.0 MB] || WC_MarsSunset-1920-MASTER_NBC_Today.mov (1920x1080) [32.0 MB] || WC_MarsSunset-1920-MASTER_WEA_CEN.wmv (1280x720) [5.6 MB] || WC_MarSunset_1920-MASTER.avi (1280x720) [5.0 MB] || WC_MarsSunset-1920-MASTER_baron.mp4 (1920x1080) [13.7 MB] || WC_MarsSunset-1920-MASTER_prores.mov (1920x1080) [275.7 MB] || WC_MarsSunset-1920-MASTER_iPad_960x540.m4v (960x540) [17.1 MB] || WC_MarsSunset-1920-MASTER_iPad_1280x720.m4v (1280x720) [31.7 MB] || WC_MarsSunset-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [44.0 MB] || WC_MarsSunset-1920-MASTER_iPad_1920x0180.webm (1920x1080) [1.8 MB] || ",
            "hits": 852
        },
        {
            "id": 11859,
            "url": "https://svs.gsfc.nasa.gov/11859/",
            "result_type": "Produced Video",
            "release_date": "2015-04-17T14:00:00-04:00",
            "title": "NASA On Air: NASA Mars Rover Weather Data Bolsters Case For Salty Water (4/17/2015)",
            "description": "LEAD: A year’s worth of weather data from Mars indicates conditions are favorable for small quantities of salty water (brine) to form at night at Gale crater.1. Mars’ soil contains perchlorate salts that can pull water vapor out of the air.  On cold nights when the relative humidity is high, they pull so much water that they dissolve into liquid, forming a salty brine.2. NASA’s Mars Curiosity rover weather station shows winter daytime temperature highs of around 0 Degrees Fahrenheit. But nighttime lows are near minus 135 Degrees Fahrenheit with relative humidity at 60%.TAG: Despite this evidence, the low temperatures and high salinity levels are likely to make the water unsuitable for life. || WC-Mars-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [222.7 KB] || WC-Mars-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [115.4 KB] || WC-Mars-1920-MASTER_iPad_1920x0180_web.png (320x180) [115.4 KB] || WC-Mars-1920-MASTER_iPad_1920x0180_thm.png (80x40) [7.4 KB] || WC-Mars-1920-MASTER_1920x1080.mov (1920x1080) [734.2 MB] || WC-Mars-1920-MASTER_1280x720.mov (1280x720) [819.4 MB] || WC-Mars-1920-MASTER_NBC_Today.mov (1920x1080) [194.0 MB] || WC-Mars-1920-MASTER_WEA_CEN.wmv (1280x720) [13.8 MB] || WC_Mars.avi (1280x720) [16.2 MB] || WC-Mars-1920-MASTER_baron.mp4 (1920x1080) [18.1 MB] || WC-Mars-1920-MASTER_prores.mov (1920x1080) [432.2 MB] || WC-Mars-1920-MASTER_iPad_960x540.m4v (960x540) [68.9 MB] || WC-Mars-1920-MASTER_iPad_1280x720.m4v (1280x720) [105.0 MB] || WC-Mars-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [205.1 MB] || WC-Mars-1920-MASTER_iPad_1920x0180.webm (1920x1080) [2.9 MB] || ",
            "hits": 91
        },
        {
            "id": 30336,
            "url": "https://svs.gsfc.nasa.gov/30336/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-21T12:00:00-04:00",
            "title": "Exploring Mars",
            "description": "Since our first close-up picture of Mars in 1965, spacecraft voyages to the Red Planet have revealed a world strangely familiar, yet different enough to challenge our perceptions of what makes a planet work. Every time we feel close to understanding Mars, new discoveries send us straight back to the drawing board.Over the past several decades, spacecraft have shown us that Mars is rocky, cold, and desolate beneath its hazy, pink sky. We've discovered that today's Martian wasteland hints at a formerly volatile world where volcanoes once raged and flash floods rushed over the land.Among our many discoveries about Mars, one stands out above all others: the evidence for past surface water on Mars. Water is key because almost everywhere we find water on Earth, we find life. With our robotic spacecraft, we've found evidence that liquid water once flowed in ancient Martian environments that could have supported microbial life. Armed with that knowledge, we now can seek signs of whether such life actually arose. Is there any evidence of life in the planet's past? If so, could any of these tiny living creatures still exist today? Imagine how exciting it would be to answer, \"Yes!!\" || ",
            "hits": 99
        },
        {
            "id": 2779,
            "url": "https://svs.gsfc.nasa.gov/2779/",
            "result_type": "Visualization",
            "release_date": "2003-07-03T12:00:00-04:00",
            "title": "Mars Odyssey: Water Ice/Winter Observations",
            "description": "NASA's Mars Odyssey detected water ice in the northern hemisphere. During the winter months, the icy soil is covered by a thick layer of carbon dioxide ('dry ice') frost obscuring the water ice signature.This animation is match-framed to animation #2778 and animation #2780. It shows the areas of ice during a martian winter. || ",
            "hits": 48
        },
        {
            "id": 2780,
            "url": "https://svs.gsfc.nasa.gov/2780/",
            "result_type": "Visualization",
            "release_date": "2003-07-03T12:00:00-04:00",
            "title": "Mars Odyssey: Water Ice/Summer Observations",
            "description": "NASA's Mars Odyssey detected water ice in the northern hemisphere. During the winter months, the icy soil is covered by a thick layer of carbon dioxide ('dry ice') frost obscuring the water ice signature.This animation is match-framed to #2778 and #2779. It shows the areas of ice during a martian summer. || ",
            "hits": 45
        },
        {
            "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": 27
        },
        {
            "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": 9
        },
        {
            "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": 6
        },
        {
            "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": 9
        },
        {
            "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": 8
        },
        {
            "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": 9
        },
        {
            "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": 1
        },
        {
            "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": 11
        }
    ]
}