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    "results": [
        {
            "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": 165
        },
        {
            "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": 1262
        },
        {
            "id": 4370,
            "url": "https://svs.gsfc.nasa.gov/4370/",
            "result_type": "Visualization",
            "release_date": "2015-11-05T14:00:00-05:00",
            "title": "Solar Wind Strips the Martian Atmosphere",
            "description": "Scientists have long suspected the solar wind of stripping the Martian upper atmosphere into space, turning Mars from a blue world to a red one. Now, NASA's MAVEN orbiter is observing this process in action, providing significant data on solar wind erosion at Mars.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.This video is also available on our YouTube channel. || MarsAtmoLossExplainPreview.jpg (1920x1080) [993.6 KB] || APPLE_TV_4370_MAVEN_Mars_Atmo_Loss_appletv_subtitles.m4v (1280x720) [53.7 MB] || WEBM_4370_MAVEN_Mars_Atmo_Loss_APR.webm (960x540) [44.7 MB] || 4370_MAVEN_Mars_Atmo_Loss_appletv.m4v (1280x720) [53.7 MB] || NASA_TV_4370_MAVEN_Mars_Atmo_Loss.mpeg (1280x720) [369.5 MB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.srt [2.3 KB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.vtt [2.3 KB] || LARGE_MP4_4370_MAVEN_Mars_Atmo_Loss_large.mp4 (3840x2160) [111.3 MB] || YOUTUBE_HQ_4370_MAVEN_Mars_Atmo_Loss_youtube_hq.mov (3840x2160) [2.2 GB] || 4370_MAVEN_Mars_Atmo_Loss_APR.mov (3840x2160) [5.9 GB] || ",
            "hits": 334
        },
        {
            "id": 4393,
            "url": "https://svs.gsfc.nasa.gov/4393/",
            "result_type": "Visualization",
            "release_date": "2015-11-05T14:00:00-05:00",
            "title": "Solar Wind and Mars Bow Shock",
            "description": "Simulation of the solar wind at Mars compared with MAVEN observations, showing the predicted bow shock. Available for download in up to 4k resolution. || final_shock01.2500_print.jpg (1024x576) [205.3 KB] || final_shock01.2500_searchweb.png (320x180) [100.4 KB] || final_shock01.2500_thm.png (80x40) [6.6 KB] || final_shock01_1920x1080_60fps.mp4 (1920x1080) [66.6 MB] || APPLE_TV_4393_Mars_Solar_Wind_Bow_Shock_1920x1080_appletv.m4v (1280x720) [19.0 MB] || WEBM_4393_Mars_Solar_Wind_Bow_Shock_1920x1080.webm (960x540) [15.1 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || NASA_TV_4393_Mars_Solar_Wind_Bow_Shock_1920x1080.mpeg (1280x720) [128.4 MB] || PRORES_B-ROLL_4393_Mars_Solar_Wind_Bow_Shock_1920x1080_prores.mov (1280x720) [537.1 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || 4393_Mars_Solar_Wind_Bow_Shock_1920x1080.mov (1920x1080) [1.0 GB] || final_shock01_4k_60fps.mp4 (3840x2160) [214.3 MB] || ",
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        },
        {
            "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": 837
        },
        {
            "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": 64
        },
        {
            "id": 30533,
            "url": "https://svs.gsfc.nasa.gov/30533/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-11-06T12:00:00-05:00",
            "title": "View into 'John Klein' Drill Hole in Martian Mudstone",
            "description": "The hole that NASA's Curiosity Mars rover drilled into target rock \"John Klein\". || view_into_martian_mudstone_pia17594_print.jpg (1024x698) [199.0 KB] || view_into_martian_mudstone_pia17594_web.jpg (320x218) [46.0 KB] || view_into_martian_mudstone_pia17594_searchweb.png (320x180) [116.5 KB] || view_into_martian_mudstone_pia17594_thm.png (80x40) [16.0 KB] || view_into_martian_mudstone_pia17594.tif (1264x862) [3.1 MB] || view_into_martian_mudstone_pia17594.hwshow [111 bytes] || ",
            "hits": 16
        },
        {
            "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": 61
        },
        {
            "id": 3896,
            "url": "https://svs.gsfc.nasa.gov/3896/",
            "result_type": "Visualization",
            "release_date": "2011-12-28T00:00:00-05:00",
            "title": "Mars Roll",
            "description": "A redux of entry #2455 using MGS/MOLA data for the Martian topography and MGS/MOC for the Martian surface color. The animation rolls Mars to show major features of the Martian topography. Major features depicted include: Olympus Mons, Valles Marineris, Hellas Basin, and the Martian North and South Poles. || ",
            "hits": 78
        },
        {
            "id": 2882,
            "url": "https://svs.gsfc.nasa.gov/2882/",
            "result_type": "Visualization",
            "release_date": "2004-05-02T12:00:00-04:00",
            "title": "Zoom down to the Gale Crater on Mars",
            "description": "This is a zoom down to the Gale Crater on MARS as seen by Viking and the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC).  These images show a very large area of sedimentation inside the Gale Crater.  The origin of the sedimentary material remains unanswered. Studying these layers of rocks could answer many questions about the history of MARS. || ",
            "hits": 15
        },
        {
            "id": 2864,
            "url": "https://svs.gsfc.nasa.gov/2864/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Final Composite",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, still dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is 10km. high compared to Olympus Mons at 23km. This post-produced animation composite was created using various elements from animations #2865 through #2872. || ",
            "hits": 110
        },
        {
            "id": 2868,
            "url": "https://svs.gsfc.nasa.gov/2868/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: True Color Mars",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing Mars in it's true color beauty. The beginning of this animation is match-framed to animations #2864 through #2872. || ",
            "hits": 80
        },
        {
            "id": 2869,
            "url": "https://svs.gsfc.nasa.gov/2869/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Elevation Color-Mapped Mars",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano.  When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km.  This animation is one element of the Earth-Mars comparison.  It shows Mars' differing terrain via an elevation color map.  Yellow indicates the mean elevation.  Green, blue, and purple are low lying areas.  Red, brown, and white are the highest elevations.  This animation is match-framed to animations #2864 through #2872 and uses the same color map as animation #2866. || ",
            "hits": 317
        },
        {
            "id": 2870,
            "url": "https://svs.gsfc.nasa.gov/2870/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: True Color Olympus Mons over Elevation Color-Mapped Earth Bathymetry with True Color Land Features",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, Olympus Mons obstructs the view of Mauna Loa, but gives the viewer a good perspective of the overall size of this giant volcano. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 95
        },
        {
            "id": 2871,
            "url": "https://svs.gsfc.nasa.gov/2871/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Transparent Olympus Mons over Elevation Color-Mapped Earth with True Color Land",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, a transparent Olympus Mons is juxtaposed over Mauna Loa, allowing the viewer to better see the size differences between these land masses. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 105
        },
        {
            "id": 2872,
            "url": "https://svs.gsfc.nasa.gov/2872/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Mars Inside a Transparent Earth",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation not only shows the relative size differences between Mauna Loa and Olympus Mons, but also shows the size difference between these 2 planets. The equatorial radius of Mars is approximately 3397 km. compared to Earth's equatorial radius of 6378.1 km. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 65
        },
        {
            "id": 2877,
            "url": "https://svs.gsfc.nasa.gov/2877/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Planet Comparisons (False Color with Axes and Orbit Plane)",
            "description": "This is a visualization showing the relative size of Mars compared to that of Earth. This version uses false color textures (there are corresponding true color versions as well). The colors correspond to the heights above/below 'sea level.' This version also includes pole axes and an orbit plane. || ",
            "hits": 81
        },
        {
            "id": 2880,
            "url": "https://svs.gsfc.nasa.gov/2880/",
            "result_type": "Visualization",
            "release_date": "2004-04-01T12:00:00-05:00",
            "title": "Great Zoom into Distributary Fan, Mars",
            "description": "This is a Great Zoom into the so-called Distributary Fan on Mars. It is located just northeast of Holden Crater. As seen from Martian orbit by the Mars Orbiter Camera (MOC) flying on the Mars Global Surveyor (MGS) spacecraft, this dramatic visualization shows us where liquid water likely flowed across the Martian surface sometime in the planet's past. || ",
            "hits": 54
        },
        {
            "id": 2883,
            "url": "https://svs.gsfc.nasa.gov/2883/",
            "result_type": "Visualization",
            "release_date": "2004-01-16T12:00:00-05:00",
            "title": "Mars: Olympus Mons",
            "description": "MOLA-based still image showing Martian topography of Olympus Mons as both color and elevation. || Olympus Mons on Mars, in false color || olympus_mons_false.jpg (1280x1024) [260.9 KB] || olympus_mons_false_web.jpg (320x256) [13.9 KB] || olympus_mons_false_thm.png (80x40) [4.8 KB] || olympus_mons_false_web_searchweb.jpg (320x180) [84.0 KB] || olympus_mons_false.tif (1280x1024) [1.9 MB] || ",
            "hits": 325
        },
        {
            "id": 2884,
            "url": "https://svs.gsfc.nasa.gov/2884/",
            "result_type": "Visualization",
            "release_date": "2004-01-16T12:00:00-05:00",
            "title": "Mars: Valles Marineris",
            "description": "MOLA-based still image showing Martian topography of Valles Marineris as both color and elevation. || Valles Marineris on Mars, in false color || valles_marineris_false.jpg (1280x1024) [263.4 KB] || valles_marineris_false_web.jpg (320x256) [22.8 KB] || valles_marineris_false_thm.png (80x40) [6.7 KB] || valles_marineris_false_web_searchweb.jpg (320x180) [103.9 KB] || valles_marineris_false.tif (1280x1024) [1.7 MB] || ",
            "hits": 72
        },
        {
            "id": 2778,
            "url": "https://svs.gsfc.nasa.gov/2778/",
            "result_type": "Visualization",
            "release_date": "2003-07-03T12:00:00-04:00",
            "title": "Mars Odyssey: Mars' Northern Hemisphere",
            "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 2779 and animation 2780. Its purpose is to establish a frame of reference using a true color data set. In this case, that data is from Viking. || ",
            "hits": 29
        },
        {
            "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": 14
        },
        {
            "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": 32
        },
        {
            "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": 17
        },
        {
            "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": 19
        },
        {
            "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": 13
        },
        {
            "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": 12
        },
        {
            "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": 12
        },
        {
            "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": 10
        },
        {
            "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": 14
        },
        {
            "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": 8
        },
        {
            "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": 29
        },
        {
            "id": 2427,
            "url": "https://svs.gsfc.nasa.gov/2427/",
            "result_type": "Visualization",
            "release_date": "2002-04-16T12:00:00-04:00",
            "title": "MOLA-based Flyover of Hellas Transitioning to Utopia Planitia",
            "description": "MOLA-based animations showing Martian topography as both color and elevation.  The exaggeration is 3x.  This was created for a talk James Garvin will give on The Hill in late April 2002. || ",
            "hits": 11
        },
        {
            "id": 2428,
            "url": "https://svs.gsfc.nasa.gov/2428/",
            "result_type": "Visualization",
            "release_date": "2002-04-16T12:00:00-04:00",
            "title": "MOLA-based Flyover of Tharsis Volcanos",
            "description": "MOLA-based animations showing Martian topography as both color and elevation.  The exaggeration is 3x.  This was created for a talk James Garvin will give on The Hill in late April 2002. || ",
            "hits": 15
        },
        {
            "id": 2429,
            "url": "https://svs.gsfc.nasa.gov/2429/",
            "result_type": "Visualization",
            "release_date": "2002-04-16T12:00:00-04:00",
            "title": "MOLA-based Flyover of Gusev Crater",
            "description": "MOLA-based animations showing Martian topography as both color and elevation.  The exaggeration is 3x.  This was created for a talk James Garvin will give on The Hill in late April 2002. || ",
            "hits": 11
        },
        {
            "id": 2430,
            "url": "https://svs.gsfc.nasa.gov/2430/",
            "result_type": "Visualization",
            "release_date": "2002-04-16T12:00:00-04:00",
            "title": "MOLA-based Flyover of Korolev Crater",
            "description": "MOLA-based animations showing Martian topography as both color and elevation.  The exaggeration is 3x.  This was created for a talk James Garvin will give on The Hill in late April 2002. || ",
            "hits": 14
        },
        {
            "id": 2324,
            "url": "https://svs.gsfc.nasa.gov/2324/",
            "result_type": "Visualization",
            "release_date": "2001-12-11T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Polar Images",
            "description": "Print resolution still images in support of the MOLA: Seasonal Snow Variation story || The north pole of Mars shown colored by elevation || marsNPoleFalseCol.jpg (2730x2048) [791.2 KB] || marsNPoleFalseCola_web.png (320x240) [83.6 KB] || marsNPoleFalseCola_thm.png (80x40) [5.0 KB] || marsNPoleFalseCola_searchweb.png (320x180) [62.0 KB] || marsNPoleFalseCol.tif (2730x2048) [6.1 MB] || marsNPoleFalseCol.tif.hwshow [189 bytes] || ",
            "hits": 34
        },
        {
            "id": 2292,
            "url": "https://svs.gsfc.nasa.gov/2292/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, Zoom to Martian North Pole: True Color",
            "description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a short zoom to an overhead view of the rotating north pole in true color. || ",
            "hits": 19
        },
        {
            "id": 2293,
            "url": "https://svs.gsfc.nasa.gov/2293/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Fast Zoom to Martian North Pole: False Color",
            "description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a fast zoom to the surface of the pole.  The surface color is based on the elevation of the topography. || ",
            "hits": 14
        },
        {
            "id": 2294,
            "url": "https://svs.gsfc.nasa.gov/2294/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, Fast Zoom out from Martian South Pole: False Color",
            "description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a fast zoom out from the surface of the pole. The surface color is based on the elevation of the topography. || ",
            "hits": 8
        },
        {
            "id": 2295,
            "url": "https://svs.gsfc.nasa.gov/2295/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Medium Zoom to Martian North Pole: False Color",
            "description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a medium speed zoom to the surface of the pole.  The surface color is based on the elevation of the topography. || ",
            "hits": 10
        },
        {
            "id": 2296,
            "url": "https://svs.gsfc.nasa.gov/2296/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, Medium Zoom out from Martian South Pole: False Color",
            "description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument.  This particular animation shows a medium zoom out from the surface of the pole. The surface color is based on the elevation of the topography. || ",
            "hits": 10
        },
        {
            "id": 2297,
            "url": "https://svs.gsfc.nasa.gov/2297/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Flyover of the Martian North Pole: False Color",
            "description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a slow zoom to the surface of the pole, a flyover of the polar cap and a slow zoom out.  The surface color is based on the elevation of the topography. || ",
            "hits": 8
        },
        {
            "id": 2298,
            "url": "https://svs.gsfc.nasa.gov/2298/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom out from the Martian North Pole: True Color",
            "description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2297. || ",
            "hits": 7
        },
        {
            "id": 2299,
            "url": "https://svs.gsfc.nasa.gov/2299/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Flyover of the Martian South Pole: False Color",
            "description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument.  This particular animation shows a slow zoom to the surface of the pole, a flyover of the polar cap and a slow zoom out.  The surface color is based on the elevation of the topography. || ",
            "hits": 8
        },
        {
            "id": 2300,
            "url": "https://svs.gsfc.nasa.gov/2300/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom to the Martian South Pole: True Color",
            "description": "This is a true color visualization of the topography near the Martian south pole as measured with the MOLA instrument.  This particular animation shows a slow zoom to the surface of the pole and is a frame-accurate match to the beginning ofanimation id #2299. || ",
            "hits": 6
        },
        {
            "id": 2301,
            "url": "https://svs.gsfc.nasa.gov/2301/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom to the Martian North Pole: True Color",
            "description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a slow zoom to the surface of the pole and is a frame-accurate match to the beginning of animation id #2297. || ",
            "hits": 12
        },
        {
            "id": 2302,
            "url": "https://svs.gsfc.nasa.gov/2302/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom Out from the Martian North Pole: True Color",
            "description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument.  This particular animation shows a slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2297. || ",
            "hits": 13
        },
        {
            "id": 2303,
            "url": "https://svs.gsfc.nasa.gov/2303/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars: Flyover and Slow Zoom out from Martian S. Pole: True Color",
            "description": "This is a true color visualization of the topography near the Martian south pole as measured with the MOLA instrument.  This particular animation shows a flyover and slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2299. || ",
            "hits": 13
        },
        {
            "id": 2306,
            "url": "https://svs.gsfc.nasa.gov/2306/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, Graph Showing Snow Variations at Both Poles, With Dates",
            "description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes both poles and the Martian year timestamp. || Seasonal Mars snow variations graph (with dates) showing both poles || a002306.00100_print.png (720x480) [269.8 KB] || mola_graph_pre.jpg (320x240) [6.5 KB] || a002306.webmhd.webm (960x540) [2.8 MB] || a002306.dv (720x480) [142.8 MB] || a002306.mp4 (640x480) [8.1 MB] || mola_graph.mpg (320x240) [220.3 KB] || ",
            "hits": 21
        },
        {
            "id": 2307,
            "url": "https://svs.gsfc.nasa.gov/2307/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at both poles, without dates",
            "description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes both poles and no Martian year timestamp. || ",
            "hits": 11
        },
        {
            "id": 2308,
            "url": "https://svs.gsfc.nasa.gov/2308/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at north pole, with dates",
            "description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes just the north pole and the Martian year timestamp. || ",
            "hits": 10
        },
        {
            "id": 2309,
            "url": "https://svs.gsfc.nasa.gov/2309/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at north pole, without dates",
            "description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes just the north pole without the Martian year timestamp. || ",
            "hits": 13
        },
        {
            "id": 2310,
            "url": "https://svs.gsfc.nasa.gov/2310/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, clouds at both poles, with dates, without contours",
            "description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows both poles, with dates, and without contours. || ",
            "hits": 5
        },
        {
            "id": 2311,
            "url": "https://svs.gsfc.nasa.gov/2311/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, clouds at both poles, with dates, with contours",
            "description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows both poles, with dates, and with contours. || ",
            "hits": 15
        },
        {
            "id": 2312,
            "url": "https://svs.gsfc.nasa.gov/2312/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, clouds at north pole, with dates, without contours",
            "description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows just the north pole, with dates, and without contours. || ",
            "hits": 9
        },
        {
            "id": 2313,
            "url": "https://svs.gsfc.nasa.gov/2313/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T12:00:00-05:00",
            "title": "MOLA: Seasonal Snow Variations on Mars, Clouds at North Pole, With Dates and Contours",
            "description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows just the north pole, with dates, and with contours. || ",
            "hits": 9
        },
        {
            "id": 2305,
            "url": "https://svs.gsfc.nasa.gov/2305/",
            "result_type": "Visualization",
            "release_date": "2001-12-06T00:00:00-05:00",
            "title": "FUSE/MOLA: Mars Once Had Oceans - match render w/o oceans",
            "description": "This visualization shows a match render of Mars without oceans to accompany the rendering of Mars with oceans (animation id 2291). || Spinning Mars with true color Viking texture || a002305.00005_print.png (720x480) [330.4 KB] || mars_ocean_nowater_pre.jpg (320x238) [4.6 KB] || a002305.webmhd.webm (960x540) [4.9 MB] || a002305.dv (720x480) [224.3 MB] || mars_ocean_nowater.mpg (352x240) [3.4 MB] || ",
            "hits": 13
        },
        {
            "id": 2291,
            "url": "https://svs.gsfc.nasa.gov/2291/",
            "result_type": "Visualization",
            "release_date": "2001-12-04T12:00:00-05:00",
            "title": "FUSE/MOLA: Mars Once had Oceans",
            "description": "This visualization shows how Mars might look with an ocean at -500m where the lowest point on Mars is about -8000m and the highest point is about 22000m.  Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theory. || ",
            "hits": 25
        },
        {
            "id": 2326,
            "url": "https://svs.gsfc.nasa.gov/2326/",
            "result_type": "Visualization",
            "release_date": "2001-12-01T12:00:00-05:00",
            "title": "MOLA Stills for possible cover of 'Nature'",
            "description": "These are draft renders of Mars using MOLA data for Topography and Viking data (true color) for the surface texture.  One of these was picked and used by Nature on the cover of 'Insight' on 12 July 2001.  The same image was used on the cover of the Planetary Report July/August 2001. || Mars MOLA true color image of Kasei Valles looking west to east (vertical exaggeration 3x, shading 6x) || mola_nature_3x6x0.2s.0001_tc.jpg (425x550) [24.7 KB] || ",
            "hits": 19
        },
        {
            "id": 2327,
            "url": "https://svs.gsfc.nasa.gov/2327/",
            "result_type": "Visualization",
            "release_date": "2001-12-01T12:00:00-05:00",
            "title": "MOLA Stills for possible cover of 'Science'",
            "description": "These stills were generated as possible cover images for Science.  Science did not select one of these - instead they selected a MOC image. || Mars MOLA true color image of the north pole || science2_fixed_true.0000.jpg (425x550) [27.3 KB] || Mars MOLA false color image of the north and south poles || science.0000_false_northAndSouth.jpg (425x550) [31.4 KB] || Mars MOLA false color image of the north pole || science.0007_false.jpg (425x550) [24.2 KB] || ",
            "hits": 16
        },
        {
            "id": 2089,
            "url": "https://svs.gsfc.nasa.gov/2089/",
            "result_type": "Visualization",
            "release_date": "2001-03-27T12:00:00-05:00",
            "title": "Views of Mars with MOLA and Viking data",
            "description": "These views of Mars were generated for the National Geographic Society as reference materials for their February 2001 'Mars Revealed' poster. || View looking into Chryse Plantia from the west || chryseA0010.jpg (640x480) [47.5 KB] || chryseA0010_web.jpg (320x240) [8.2 KB] || chryseA0010.tif (640x480) [301.0 KB] || View looking into Chryse Plantia from the west || chryseA0011.jpg (640x480) [55.1 KB] || chryseA0011_web.jpg (320x240) [9.1 KB] || chryseA0011.tif (640x480) [382.3 KB] || ",
            "hits": 17
        },
        {
            "id": 1096,
            "url": "https://svs.gsfc.nasa.gov/1096/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "MOLA Zooming Down to Reveal a Hidden Channel (Fast Version)",
            "description": "In this visualization, using MOLA data, we take a closerlook at where the hidden channel of water is located. || a001096.00005_print.png (720x480) [522.4 KB] || a001096_thm.png (80x40) [6.6 KB] || a001096_pre.jpg (320x242) [11.1 KB] || a001096_pre_searchweb.jpg (320x180) [81.5 KB] || a001096.webmhd.webm (960x540) [1.5 MB] || a001096.dv (720x480) [36.5 MB] || a001096.mp4 (640x480) [2.0 MB] || a001096.mpg (352x240) [1.4 MB] || ",
            "hits": 17
        },
        {
            "id": 1097,
            "url": "https://svs.gsfc.nasa.gov/1097/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "MOLA Zooming Down to Reveal a Hidden Channel (Slow)",
            "description": "In this visualization, using MOLA data, zooming down tolook at where the hidden channel of water located. || a001097.00005_print.png (720x480) [519.9 KB] || a001097_pre.jpg (320x240) [15.7 KB] || a001097.webmhd.webm (960x540) [1.8 MB] || a001097.dv (720x480) [40.5 MB] || a001097.mp4 (640x480) [2.1 MB] || a001097.mpg (320x240) [1.3 MB] || ",
            "hits": 11
        },
        {
            "id": 1098,
            "url": "https://svs.gsfc.nasa.gov/1098/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "Viking Texture Zooming Down to Reveal a Hidden Channel (Fast)",
            "description": "This animation is a set up visualization. Using theViking data, the camera zooms down towards the area where theremight be hidden water channels. || a001098.00005_print.png (720x480) [407.0 KB] || a001098_thm.png (80x40) [5.2 KB] || a001098_pre.jpg (320x242) [8.1 KB] || a001098_pre_searchweb.jpg (320x180) [64.2 KB] || a001098.webmhd.webm (960x540) [1.4 MB] || a001098.dv (720x480) [41.0 MB] || a001098.mp4 (640x480) [2.2 MB] || a001098.mpg (352x240) [1.4 MB] || ",
            "hits": 19
        },
        {
            "id": 1099,
            "url": "https://svs.gsfc.nasa.gov/1099/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "Viking Texture Zoom Down (Slow)",
            "description": "This animation is a set up visualization. Using theViking data, the camera zooms down slowly towards the area where theremight be hidden water channels. || a001099.00005_print.png (720x480) [409.7 KB] || a001099_thm.png (80x40) [5.2 KB] || a001099_pre.jpg (320x242) [8.1 KB] || a001099_pre_searchweb.jpg (320x180) [65.3 KB] || a001099.webmhd.webm (960x540) [1.6 MB] || a001099.dv (720x480) [46.1 MB] || a001099.mp4 (640x480) [2.5 MB] || a001099.mpg (352x240) [1.5 MB] || ",
            "hits": 19
        },
        {
            "id": 1100,
            "url": "https://svs.gsfc.nasa.gov/1100/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "Gravity Flat Image Showing Hidden Channel (Still)",
            "description": "MOLA Gravity map of Mars, showing a possible water channel underground. || This image is a possible hidden water channel. || short_channel_gravity.jpg (720x486) [58.9 KB] || short_channel_gravity_web.jpg (320x216) [17.4 KB] || short_channel_gravity_thm.png (80x40) [7.0 KB] || short_channel_gravity_web_searchweb.jpg (320x180) [91.7 KB] || short_channel_gravity.tif (720x486) [403.2 KB] || ",
            "hits": 10
        },
        {
            "id": 1103,
            "url": "https://svs.gsfc.nasa.gov/1103/",
            "result_type": "Visualization",
            "release_date": "2000-06-19T12:00:00-04:00",
            "title": "Viking Texture Zoom Down to Gravity Map Revealing Hidden Channel",
            "description": "Viking Texture zoom down to gravity map revealing hidden channel || a001103.00005_print.png (720x480) [406.2 KB] || a001103_thm.png (80x40) [5.3 KB] || a001103_pre.jpg (320x242) [8.1 KB] || a001103_pre_searchweb.jpg (320x180) [65.4 KB] || a001103.webmhd.webm (960x540) [1.8 MB] || a001103.dv (720x480) [54.7 MB] || a001103.mp4 (640x480) [3.0 MB] || a001103.mpg (352x240) [2.1 MB] || ",
            "hits": 14
        },
        {
            "id": 1104,
            "url": "https://svs.gsfc.nasa.gov/1104/",
            "result_type": "Visualization",
            "release_date": "2000-06-14T12:00:00-04:00",
            "title": "MOLA Texture Zoom Down to Gravity Map Revealing Hidden Channel",
            "description": "Initially looking at the MOLA false color surface of Mars, we zoom in and see gravity data.  The blue line indicates an area where water possibly flowed. || a001104.00005_print.png (720x480) [522.9 KB] || a001104_thm.png (80x40) [6.6 KB] || a001104_pre.jpg (320x242) [11.1 KB] || a001104_pre_searchweb.jpg (320x180) [81.8 KB] || a001104.webmhd.webm (960x540) [1.9 MB] || a001104.dv (720x480) [54.7 MB] || a001104.mp4 (640x480) [2.9 MB] || a001104.mpg (352x240) [1.7 MB] || ",
            "hits": 18
        },
        {
            "id": 1095,
            "url": "https://svs.gsfc.nasa.gov/1095/",
            "result_type": "Visualization",
            "release_date": "2000-03-15T12:00:00-05:00",
            "title": "Mars North Pole Flyover",
            "description": "MOLA takes elevation data of Mars North Pole combined with Viking colormap. || ",
            "hits": 24
        },
        {
            "id": 1088,
            "url": "https://svs.gsfc.nasa.gov/1088/",
            "result_type": "Visualization",
            "release_date": "2000-03-09T12:00:00-05:00",
            "title": "Valles Marineris Flyover (Long Version)",
            "description": "This view of Valles Marineris was constructed by combining the Viking color texture with MOLA altimetry data. There is no vertical exaggeration applied to the surface displacement. || ",
            "hits": 13
        },
        {
            "id": 1093,
            "url": "https://svs.gsfc.nasa.gov/1093/",
            "result_type": "Visualization",
            "release_date": "2000-03-09T12:00:00-05:00",
            "title": "Valles Marineris Flyover (Short Version)",
            "description": "This view of Valles Marineris was constructed by combining the Viking color texture with MOLA altimetry data. There is no vertical exaggeration applied to the surface displacement. || ",
            "hits": 24
        },
        {
            "id": 1094,
            "url": "https://svs.gsfc.nasa.gov/1094/",
            "result_type": "Visualization",
            "release_date": "2000-03-09T12:00:00-05:00",
            "title": "Olympus Mons Flyover",
            "description": "This view of Olympus Mons was constructed by combining the Viking color texture with MOLA altimetry data. There is no vertical exaggeration applied to the surface displacement. || ",
            "hits": 221
        },
        {
            "id": 1101,
            "url": "https://svs.gsfc.nasa.gov/1101/",
            "result_type": "Visualization",
            "release_date": "2000-03-09T12:00:00-05:00",
            "title": "Valles Marineris Flyover (Long Version)",
            "description": "This view of Valles Marineris  was constructed by combining the Viking color texture with MOLA altimetry data.  There is no vertical exaggeration applied to the surface displacement. || ",
            "hits": 31
        },
        {
            "id": 1089,
            "url": "https://svs.gsfc.nasa.gov/1089/",
            "result_type": "Visualization",
            "release_date": "2000-03-01T12:00:00-05:00",
            "title": "MOLA Surface Topography With Gravity Texture Map",
            "description": "Rotating Mars showing variations in gravity. || Rotating Mars with colors indicating the strength of the gravitational field. || a001089.00005_print.png (720x480) [489.9 KB] || Gravity_pre.jpg (320x240) [9.2 KB] || a001089_pre.jpg (320x242) [7.8 KB] || a001089.webmhd.webm (960x540) [4.9 MB] || a001089.dv (720x480) [179.2 MB] || a001089.mp4 (640x480) [9.8 MB] || Gravity.mov (320x240) [2.9 MB] || a001089.mpg (352x240) [7.1 MB] || ",
            "hits": 39
        },
        {
            "id": 1090,
            "url": "https://svs.gsfc.nasa.gov/1090/",
            "result_type": "Visualization",
            "release_date": "2000-03-01T12:00:00-05:00",
            "title": "MOLA Surface Topography With Surface Elevation Texture Map",
            "description": "Rotating Mars with MOLA Surface Topography and Surface Elevation Texture Map. || ",
            "hits": 33
        },
        {
            "id": 1091,
            "url": "https://svs.gsfc.nasa.gov/1091/",
            "result_type": "Visualization",
            "release_date": "2000-03-01T12:00:00-05:00",
            "title": "MOLA Surface Topography With Viking Texture Map",
            "description": "Rotating Mars with the MOLA Surface Topography with Viking Texture Map || Rotating Mars with Viking imagery applied to MOLA topography. || a001091.00005_print.png (720x480) [401.2 KB] || a001091_pre.jpg (320x240) [6.6 KB] || a001091.webmhd.webm (960x540) [3.0 MB] || a001091.dv (720x480) [178.3 MB] || a001091.mp4 (640x480) [9.7 MB] || a001091.mpg (352x240) [7.1 MB] || ",
            "hits": 84
        },
        {
            "id": 1092,
            "url": "https://svs.gsfc.nasa.gov/1092/",
            "result_type": "Visualization",
            "release_date": "2000-03-01T12:00:00-05:00",
            "title": "Mars Mantle (MOHO) Topography With Mantle Elevation Texture Map",
            "description": "Rotating Mars with MOLA Topography colored to indicate elevation. || ",
            "hits": 15
        },
        {
            "id": 1102,
            "url": "https://svs.gsfc.nasa.gov/1102/",
            "result_type": "Visualization",
            "release_date": "2000-03-01T12:00:00-05:00",
            "title": "Mars Cutaway",
            "description": "Mars Globe showing a cutaway revealing the MOHO data. || Mars MOLA surface and mantle topography shown in cutaway, with elevation texture maps. || a001102.00005_print.png (720x480) [456.2 KB] || Cutaway_pre.jpg (320x240) [5.9 KB] || a001102_pre.jpg (320x242) [7.4 KB] || a001102.webmhd.webm (960x540) [3.7 MB] || a001102.m2v (720x480) [29.5 MB] || a001102.dv (720x480) [179.1 MB] || a001102.mp4 (640x480) [10.1 MB] || Cutaway.mov (320x240) [3.0 MB] || a001102.mpg (352x240) [6.9 MB] || ",
            "hits": 20
        },
        {
            "id": 1105,
            "url": "https://svs.gsfc.nasa.gov/1105/",
            "result_type": "Visualization",
            "release_date": "2000-02-15T12:00:00-05:00",
            "title": "Mars Crust Thickness",
            "description": "Looking at a slice of Mars.  The slice depicts Mars from south (left) to north (right).  Notice the downward trend from right to left, showing that Mars is mostly downhill from North to South. || ",
            "hits": 16
        },
        {
            "id": 764,
            "url": "https://svs.gsfc.nasa.gov/764/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Mars Polar Lander Landing Site: Global View to False Color MOLA Inset",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The  400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 14
        },
        {
            "id": 765,
            "url": "https://svs.gsfc.nasa.gov/765/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Close Up Fly Over of Mars Polar Lander Landing Area in True Color",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 10
        },
        {
            "id": 766,
            "url": "https://svs.gsfc.nasa.gov/766/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Close Up Fly Over of Mars Polar Lander Landing Area in False Color",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 10
        },
        {
            "id": 767,
            "url": "https://svs.gsfc.nasa.gov/767/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "A Comparison of Visible and Topographic Data for the Martian South Pole: Version 1",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 16
        },
        {
            "id": 768,
            "url": "https://svs.gsfc.nasa.gov/768/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "A Comparison of Visible and Topographic Data for the Martian South Pole: Version 2",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 8
        },
        {
            "id": 769,
            "url": "https://svs.gsfc.nasa.gov/769/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "A Rotating True Color View of the Martian South Pole",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 15
        },
        {
            "id": 770,
            "url": "https://svs.gsfc.nasa.gov/770/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "A Rotating False Color View of the Martian South Pole from MOLA",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. The elevation of the landing site is about 2.4 km, midway into the polar layered terrain. The 400 meters (1/4 mile) resolution of the MOLA data gives a smoothed but vertically exaggerated view of the topography. At this scale it is impossible to ascertain the actual roughness at the lander's destination, forcing project directors to make their best guesses based on available data. || ",
            "hits": 32
        },
        {
            "id": 771,
            "url": "https://svs.gsfc.nasa.gov/771/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "A Rotating False Color View of the Martian South Pole from MOLA: New Color Map",
            "description": "This is one of a series of visualizations showing false-colored renderings of the Martian topography measured by MOLA in the vicinity of the Mars Polar Lander landing site. || ",
            "hits": 29
        },
        {
            "id": 773,
            "url": "https://svs.gsfc.nasa.gov/773/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Push in South of the Hellas Basin Showing Topography from MOLA",
            "description": "Zoom into the region of Mars just south of the Hellas Basin showing topography data from MOLA.  Blue tones represent elevations of less than 2 kilometers, while reddish tones are greater than about 2.8 kilometers, relative to the mean equatorial height of Mars. || a000773.00010_print.png (720x480) [508.9 KB] || a000773_pre.jpg (320x238) [7.8 KB] || a000773.webmhd.webm (960x540) [3.7 MB] || a000773.dv (720x480) [145.1 MB] || a000773.mp4 (640x480) [8.9 MB] || a000773.mpg (352x240) [5.7 MB] || ",
            "hits": 30
        },
        {
            "id": 774,
            "url": "https://svs.gsfc.nasa.gov/774/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Push in South of the Hellas Basin Showing Topography from MOLA: New Color Map",
            "description": "Zoom into the region of Mars just south of the Hellas Basin showing topography data from MOLA.  This animation uses a color table designed to highlight the topography at the south pole.  White colors indicate elevations in excess of 3012 meters, red shows elevations between 2500 and 3012 meters, yellow shows elevations from 2450 to 2500 meters, dark cyan shows elevations from 2150 to 2450 meters, dark violet shows elevations from 320 to 2150 meters. || a000774.00010_print.png (720x480) [401.1 KB] || a000774_pre.jpg (320x238) [6.0 KB] || a000774.webmhd.webm (960x540) [5.6 MB] || a000774.dv (720x480) [151.6 MB] || a000774.mp4 (640x480) [8.9 MB] || a000774.mpg (352x240) [1.8 MB] || ",
            "hits": 11
        },
        {
            "id": 776,
            "url": "https://svs.gsfc.nasa.gov/776/",
            "result_type": "Visualization",
            "release_date": "1999-11-22T12:00:00-05:00",
            "title": "Mars Southern Hemisphere Rotation in False Color from MOLA",
            "description": "Blue represents low topography and red or white represent areas of high topography. || Watching MOLA topography data of the southern hemisphere of Mars on a rotating globe || a000776.00010_print.png (720x480) [512.4 KB] || a000776_pre.jpg (320x238) [7.8 KB] || a000776.webmhd.webm (960x540) [3.9 MB] || a000776.dv (720x480) [122.5 MB] || a000776.mp4 (640x480) [7.0 MB] || a000776.mpg (352x240) [4.9 MB] || ",
            "hits": 60
        },
        {
            "id": 684,
            "url": "https://svs.gsfc.nasa.gov/684/",
            "result_type": "Visualization",
            "release_date": "1999-08-25T12:00:00-04:00",
            "title": "Polar Orbiter: Fly Up to 4 Possible Landing Sites (Yellow)",
            "description": "Mars true color Viking sphere rotating to four potential Polar Lander landing sites (in yellow) || a000684.00010_print.png (720x480) [496.0 KB] || a000684_thm.png (80x40) [5.0 KB] || a000684_pre.jpg (320x238) [8.3 KB] || a000684_pre_searchweb.jpg (320x180) [61.5 KB] || a000684.webmhd.webm (960x540) [5.8 MB] || a000684.dv (720x480) [91.6 MB] || a000684.mp4 (640x480) [5.0 MB] || a000684.mpg (352x240) [3.2 MB] || ",
            "hits": 38
        },
        {
            "id": 685,
            "url": "https://svs.gsfc.nasa.gov/685/",
            "result_type": "Visualization",
            "release_date": "1999-08-25T12:00:00-04:00",
            "title": "Polar Orbiter: Fly Up to 4 Possible Landing Sites (Primary in Green, Secondary in Yellow)",
            "description": "Mars true color Viking sphere rotating to four potential Polar Lander landing sites (primary in green, secondary in yellow) || a000685.00010_print.png (720x480) [494.8 KB] || a000685_thm.png (80x40) [5.0 KB] || a000685_pre.jpg (320x238) [8.3 KB] || a000685_pre_searchweb.jpg (320x180) [61.3 KB] || a000685.webmhd.webm (960x540) [5.9 MB] || a000685.dv (720x480) [91.6 MB] || a000685.mp4 (640x480) [5.0 MB] || a000685.mpg (352x240) [3.2 MB] || ",
            "hits": 37
        },
        {
            "id": 686,
            "url": "https://svs.gsfc.nasa.gov/686/",
            "result_type": "Visualization",
            "release_date": "1999-08-25T12:00:00-04:00",
            "title": "Polar Orbiter: Fly Up to the Primary Landing Site (Green)",
            "description": "Fly up to primary Polar Lander landing site || a000686.00010_print.png (720x480) [496.9 KB] || a000686_thm.png (80x40) [5.0 KB] || a000686_pre.jpg (320x238) [8.2 KB] || a000686_pre_searchweb.jpg (320x180) [61.1 KB] || a000686.webmhd.webm (960x540) [5.8 MB] || a000686.dv (720x480) [92.1 MB] || a000686.mp4 (640x480) [5.1 MB] || a000686.mpg (352x240) [3.2 MB] || ",
            "hits": 43
        },
        {
            "id": 687,
            "url": "https://svs.gsfc.nasa.gov/687/",
            "result_type": "Visualization",
            "release_date": "1999-08-25T12:00:00-04:00",
            "title": "Polar Orbiter: Fly Up to Primary Landing Site with Roughness Map",
            "description": "dark blue = smooth, green = rough || Mars true color Viking sphere rotating to Polar Lander site in MOLA roughness false color || a000687.00010_print.png (720x480) [498.0 KB] || a000687_thm.png (80x40) [5.0 KB] || a000687_pre.jpg (320x238) [8.3 KB] || a000687_pre_searchweb.jpg (320x180) [61.0 KB] || a000687.webmhd.webm (960x540) [5.8 MB] || a000687.dv (720x480) [92.2 MB] || a000687.mp4 (640x480) [5.1 MB] || a000687.mpg (352x240) [3.1 MB] || ",
            "hits": 36
        },
        {
            "id": 688,
            "url": "https://svs.gsfc.nasa.gov/688/",
            "result_type": "Visualization",
            "release_date": "1999-08-25T12:00:00-04:00",
            "title": "Polar Orbiter: Fly Up to Primary Landing Site with Altitude Map",
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