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        {
            "id": 40550,
            "url": "https://svs.gsfc.nasa.gov/gallery/voyager/",
            "result_type": "Gallery",
            "release_date": "2026-03-04T00:00:00-05:00",
            "title": "Voyager",
            "description": "Launched in 1977, the twin Voyager spacecraft are NASA’s longest operating and most distant spacecraft. Hurtling through space at over 38,000 miles per hour, Voyager 1 and 2 were the first confirmed human-made objects to cross the threshold into interstellar space. After completing an in-depth reconnaissance of the outer planets, the Voyager spacecraft departed the heliosphere, the protective bubble of particles and magnetic fields generated by the Sun, in two separate directions and are now exploring the edges of interstellar space. \n\nLearn more: https://science.nasa.gov/mission/voyager/",
            "hits": 625
        },
        {
            "id": 14750,
            "url": "https://svs.gsfc.nasa.gov/14750/",
            "result_type": "Produced Video",
            "release_date": "2025-01-10T10:00:00-05:00",
            "title": "NASA to Study the Moon’s Interior",
            "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Human Behaviour\" and \"Overview Effect\" from Jan Telegra of Universal Production Music. || YT_THUMB_LMS.jpg (1280x720) [171.6 KB] || CLPS_MAIN_LMS_FINAL.01682_searchweb.png (320x180) [63.2 KB] || CLPS_MAIN_LMS_FINAL.mp4 (1440x1080) [22.5 MB] || CLPS_MAIN_LMS_socialversion.mp4 (1440x1080) [27.4 MB] || CLPS_MAIN_LMS.en_US.srt [2.5 KB] || CLPS_MAIN_LMS.en_US.vtt [2.4 KB] || CLPS_MAIN_LMS_FINAL.01682_thm.png [5.2 KB] || ",
            "hits": 190
        },
        {
            "id": 5213,
            "url": "https://svs.gsfc.nasa.gov/5213/",
            "result_type": "Visualization",
            "release_date": "2024-08-14T15:00:00-04:00",
            "title": "Changes in the Atmosphere and Ocean During a Transition From La Niña to El Niño",
            "description": "This is the final version of the ENSO visualization with narration.  There are HD and 4k versions available as mp4s.  There is also a high quality 4k version which is very large (3.8 Gbytes).  Other non-narrated formats including individual frames are available below this entry.This movie is also available on youtube here:https://youtu.be/jK20dl3g9R8?si=38LHf1e0iIzrfhRQlink || ENSO_99_final_4k.01200_print.jpg (1024x576) [82.0 KB] || ENSO_Locked_Final_1080.mp4 (1920x1080) [155.7 MB] || ENSO_Final_Audio.en_US.srt [8.6 KB] || ENSO_Final_Audio.en_US.vtt [8.7 KB] || ENSO_Locked_Final_2160.mp4 (3840x2160) [184.8 MB] || ENSO_Locked_Final_2160_HIGH_QUAL.mp4 (3840x2160) [3.7 GB] || ENSO_Locked_Final_2160.mp4.hwshow [188 bytes] || ",
            "hits": 292
        },
        {
            "id": 20362,
            "url": "https://svs.gsfc.nasa.gov/20362/",
            "result_type": "Animation",
            "release_date": "2022-07-07T15:20:00-04:00",
            "title": "Gravity on the Moon vs. Asteroid Bennu: Animation",
            "description": "The lunar surface is better at resisting impacts than the loose surface of asteroid Bennu – thanks to the Moon’s much stronger gravity. || OREX-MoonvsBennuMograph-ProRes.00240_print.jpg (1024x576) [74.2 KB] || OREX-MoonvsBennuMograph-ProRes.00240_searchweb.png (320x180) [60.3 KB] || OREX-MoonvsBennuMograph-ProRes.00240_thm.png (80x40) [4.3 KB] || OREX-MoonvsBennuMograph-ProRes_1080.mp4 (1920x1080) [58.2 MB] || 3840x2160_16x9_30p (3840x2160) [128.0 KB] || OREX-MoonvsBennuMograph-ProRes.webm (3840x2160) [8.7 MB] || OREX-MoonvsBennuMograph-ProRes.mov (3840x2160) [3.2 GB] || OREX-MoonvsBennuMograph-ProRes_4K.mp4 (3840x2160) [238.1 MB] || ",
            "hits": 259
        },
        {
            "id": 20360,
            "url": "https://svs.gsfc.nasa.gov/20360/",
            "result_type": "Animation",
            "release_date": "2022-07-07T14:30:00-04:00",
            "title": "Thirty Seconds on Asteroid Bennu: Animation",
            "description": "Data-driven animation showing how the OSIRIS-REx spacecraft impacted asteroid Bennu's surface when it touched down and collected a sample. || 20360_Orex_tag_h264_1080.00111_print.jpg (576x1024) [160.5 KB] || 20360_Orex_tag_h264_1080.00111_searchweb.png (320x180) [97.3 KB] || 20360_Orex_tag_h264_1080.00111_thm.png (80x40) [6.1 KB] || 20360_Orex_tag_h264_1080.webm (1920x1080) [13.2 MB] || 20360_Orex_tag_h264_1080.mp4 (1920x1080) [175.4 MB] || 20360_Orex_tag_h264_4K.mp4 (3840x2160) [86.5 MB] || OREx_Tag_PNG (3840x2160) [0 Item(s)] || 20360_Orex_Prores_4k.mov (3840x2160) [4.4 GB] || ",
            "hits": 158
        },
        {
            "id": 14179,
            "url": "https://svs.gsfc.nasa.gov/14179/",
            "result_type": "Produced Video",
            "release_date": "2022-07-07T14:00:00-04:00",
            "title": "Asteroid Bennu’s Surprising Surface Revealed by OSIRIS-REx",
            "description": "When OSIRIS-REx touched down on asteroid Bennu, it encountered a surface of loose rocks and pebbles just barely held together by gravity.Complete transcript available.Universal Production Music: “Subsurface” by Ben Niblett and Jon CottonWatch this video on the NASA Goddard YouTube channel. || TAG_Science_Preview_4_print.jpg (1024x576) [182.1 KB] || TAG_Science_Preview_4.png (3840x2160) [10.5 MB] || TAG_Science_Preview_4.jpg (3840x2160) [902.0 KB] || TAG_Science_Preview_4_searchweb.png (180x320) [109.2 KB] || TAG_Science_Preview_4_thm.png (80x40) [7.1 KB] || 14179_TAG_Science_SHORT_Twitter.mp4 (1280x720) [22.5 MB] || 14179_TAG_Science_SHORT_Twitter.webm (1280x720) [10.5 MB] || 14179_TAG_Science_SHORT_Facebook.mp4 (1920x1080) [127.7 MB] || 14179_TAG_Science_SHORT_Captions.en_US.srt [2.0 KB] || 14179_TAG_Science_SHORT_Captions.en_US.vtt [1.9 KB] || 14179_TAG_Science_SHORT_MASTER.mov (3840x2160) [5.0 GB] || ",
            "hits": 77
        },
        {
            "id": 14095,
            "url": "https://svs.gsfc.nasa.gov/14095/",
            "result_type": "Produced Video",
            "release_date": "2022-02-09T09:00:00-05:00",
            "title": "NASA’s New Views of Venus’ Surface From Space",
            "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ",
            "hits": 861
        },
        {
            "id": 13693,
            "url": "https://svs.gsfc.nasa.gov/13693/",
            "result_type": "Produced Video",
            "release_date": "2020-08-17T00:00:00-04:00",
            "title": "Ocean Worlds: The Search for Life",
            "description": "NASA scientists discuss the search for life on the ocean worlds of our solar system and beyond.Watch this video on the NASA Goddard YouTube channel.Universal Production Music: “Superluminal” by Lee Groves and Peter George Marett; “Earthrise,” “Prism Lights,” and “Uncertain Ahead” by Ben Niblett and Jon Cotton; “Infinite Sky” and “Human Architecture” by Andy Blythe and Marten Joustra; “Imagine If” by Paul WernerComplete transcript available. || 13693OceanWorldsThumbnail2_print.jpg (1024x576) [269.6 KB] || 13693OceanWorldsThumbnail2.jpg (1920x1080) [763.8 KB] || 13693OceanWorldsThumbnail2_searchweb.png (180x320) [88.2 KB] || 13693OceanWorldsThumbnail2_thm.png (80x40) [7.9 KB] || 13693_Ocean_Worlds_GSFC_YouTube.webm (1920x1080) [103.5 MB] || 13693OceanWorldsCaptionsV3.en_US.srt [19.9 KB] || 13693OceanWorldsCaptionsV3.en_US.vtt [19.0 KB] || 13693_Ocean_Worlds_GSFC_Facebook.mp4 (1920x1080) [1.1 GB] || 13693_Ocean_Worlds_GSFC_YouTube.mp4 (1920x1080) [2.9 GB] || 13693_Ocean_Worlds_GSFC_MASTER.mov (1920x1080) [11.8 GB] || ",
            "hits": 172
        },
        {
            "id": 13562,
            "url": "https://svs.gsfc.nasa.gov/13562/",
            "result_type": "Produced Video",
            "release_date": "2020-02-25T16:00:00-05:00",
            "title": "The Science of Dragonfly",
            "description": "Dragonfly’s suite of science instruments will investigate the chemistry and habitability of Titan.Universal Production Music: “Clediss” by Thomas Stempfle and Tom Sue, “Downloading Landscapes” by Andrew Michael Britton and David Stephen GoldsmithWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13562_Dragonfly_Science_MASTER_facebook_720.mp4 (1280x720) [145.8 MB] || DragonflySciencePreview_print.jpg (1024x576) [96.9 KB] || DragonflySciencePreview.jpg (3840x2160) [637.4 KB] || DragonflySciencePreview_searchweb.png (320x180) [72.4 KB] || DragonflySciencePreview_thm.png (80x40) [5.5 KB] || TWITTER_720_13562_Dragonfly_Science_MASTER_twitter_720.mp4 (1280x720) [27.2 MB] || 13562_Dragonfly_Science_MASTER.webm (960x540) [46.9 MB] || 13562_Dragonfly_Science_CAPTIONS.en_US.srt [3.4 KB] || 13562_Dragonfly_Science_CAPTIONS.en_US.vtt [3.4 KB] || 13562_Dragonfly_Science_YouTube.mp4 (3840x2160) [2.7 GB] || 13562_Dragonfly_Science_MASTER.mov (3840x2160) [16.6 GB] || ",
            "hits": 140
        },
        {
            "id": 20311,
            "url": "https://svs.gsfc.nasa.gov/20311/",
            "result_type": "Animation",
            "release_date": "2020-02-25T16:00:00-05:00",
            "title": "Dragonfly Animation Resource Page",
            "description": "Dragonfly on Titan || DF_End_Pan_4K_Prores.00420_print.jpg (1024x576) [77.6 KB] || DF_End_Pan_H264_1080.mp4 (1920x1080) [27.1 MB] || DF_End_Pan_4K_H264.mp4 (3840x2160) [15.4 MB] || DF_End_Pan_4K_Prores_PNG (3840x2160) [0 Item(s)] || DF_End_Pan_4K_Prores.webm (3840x2160) [7.0 MB] || DF_End_Pan_4K_Prores.mov (3840x2160) [1.7 GB] || ",
            "hits": 278
        },
        {
            "id": 4572,
            "url": "https://svs.gsfc.nasa.gov/4572/",
            "result_type": "Visualization",
            "release_date": "2018-11-14T14:00:00-05:00",
            "title": "The Hiawatha Impact Crater",
            "description": "The series of visualizations below are derived from satellite imagery and radar sounding. They portray both the location and size of the 31-kilometer-wide impact crater beneath Hiawatha Glacier. They also portray the structure of the glacier ice that flows into and fills the crater.The Hiawatha impact crater was first suspected to exist in the summer of 2015, from examination of a compilation of Greenland's sub-ice topography radar measurements made by NASA over two decades. The visualizations of the subsurface shown below are derived from a spring 2016 airborne survey by Germany's Alfred Wegener Institute, using a new ultrawideband radar sounder developed by the Center for Remote Sensing of Ice Sheets at The University of Kansas. Subsequent helicopter visits to the deglaciated terrain in front of Hiawatha Glacier by scientists from the Natural History Museum in Denmark recovered sediment samples from the main river that discharges water from beneath Hiawatha Glacier, through the northwestern rim breach. Laboratory examination revealed that these sediment samples contained shocked quartz and elevated platinum-group-element concentrations, both signs that the sediment records evidence of the impact of an iron asteroid more than one kilometer wide. The Hiawatha impact crater is potentially one of the youngest large impact craters on Earth.In the visualizations below, the elevation of the topography of the bed, the ice surface and the radar curtains have been exaggerated ten times in order to better illustrate their structure. || ",
            "hits": 189
        },
        {
            "id": 12385,
            "url": "https://svs.gsfc.nasa.gov/12385/",
            "result_type": "Produced Video",
            "release_date": "2016-10-13T11:00:00-04:00",
            "title": "Space Fountains",
            "description": "Are plumes of water erupting from Jupiter’s moon Europa? || pf-1024.jpg (1024x576) [167.6 KB] || pf-1280.jpg (1280x720) [232.1 KB] || pf-1024_print.jpg (1024x576) [171.1 KB] || pf-1024_searchweb.png (320x180) [69.2 KB] || pf-1024_web.png (320x180) [69.2 KB] || pf-1024_thm.png (80x40) [5.1 KB] || ",
            "hits": 81
        },
        {
            "id": 12375,
            "url": "https://svs.gsfc.nasa.gov/12375/",
            "result_type": "Produced Video",
            "release_date": "2016-09-26T14:00:00-04:00",
            "title": "Hubble Directly Images Possible Plumes on Europa",
            "description": "NASA's Hubble Space Telescope took direct ultraviolet images of the icy moon Europa transiting across the disk of Jupiter. Out of ten observations, Hubble saw what may be water vapor plumes on three of the images. This adds another piece of supporting evidence to the existence of water vapor plumes on Europa - Hubble also detected spectroscopic signatures of water vapor in 2012. The existence of water vapor plumes could provide NASA's Europa flyby mission the opportunity to study the conditions and habitability of Europa's subsurface ocean.Read the full nasa.gov story here: http://www.nasa.gov/press-release/nasa-s-hubble-spots-possible-water-plumes-erupting-on-jupiters-moon-europaRead the full science paper here: http://hubblesite.org/pubinfo/pdf/2016/33/pdf.pdfFull details on the images can be found on HubbleSite.org: http://hubblesite.org/newscenter/archive/releases/2016/33/Additional Resources:JPL's \"Europa: Tempting Target for Future Exploration\" video file is downloadable here: https://vimeo.com/118505538Read the Dec 2013 press release about Hubble's previous observations of Europa here: http://www.nasa.gov/content/goddard/hubble-europa-water-vapor || ",
            "hits": 91
        },
        {
            "id": 4433,
            "url": "https://svs.gsfc.nasa.gov/4433/",
            "result_type": "Visualization",
            "release_date": "2016-02-25T20:00:00-05:00",
            "title": "El Niño: GMAO Daily Sea Surface Temperature Anomaly from 1997/1998 and 2015/2016",
            "description": "This visualization shows how the Sea Surface Temperature Anomaly (SSTA) data and subsurface Temperature Anomaly from the 1997 El Nino year compares to the 2015 El Nino year.  The visualization shows how the 1997 event started from colder-than-average sea surface temperatures – but the 2015 event started with warmer-than-average temperatures not only in the Pacific but also in in the Atlantic and Indian Oceans.This video is also available on our YouTube channel. || SSTcompare1997_2015_0000_print.jpg (1024x576) [87.4 KB] || SSTcompare1997_2015_0000_searchweb.png (320x180) [53.0 KB] || SSTcompare1997_2015_0000_thm.png (80x40) [5.6 KB] || Compare1997_2015_SSTA.mp4 (1920x1080) [28.7 MB] || compare (1920x1080) [0 Item(s)] || Compare1997_2015_SSTA.webm (1920x1080) [1.5 MB] || Compare1997_2015_SSTA.m4v (640x360) [2.5 MB] || Compare1997_2015_SSTA.mp4.hwshow [187 bytes] || ",
            "hits": 85
        },
        {
            "id": 12157,
            "url": "https://svs.gsfc.nasa.gov/12157/",
            "result_type": "Produced Video",
            "release_date": "2016-02-25T14:00:00-05:00",
            "title": "El Niño Rainfall and Ocean Temperature Visualizations",
            "description": "Visualization showing sea surface temperature (SST) anomaly data from Jan. 1, 2015 through Feb. 14, 2016. || SST_15-1920-MASTER-1920_H.264_QT_for_16x9_Youtube_print.jpg (1024x576) [102.5 KB] || SST_15-1920-MASTER.mov (1920x1080) [253.6 MB] || SST_15-1920-MASTER-1920_H.264_QT_for_16x9_Youtube.mov (1920x1080) [4.2 MB] || SST_15-1920-MASTER-1920_H.264_QT_for_16x9_Youtube.webm (1920x1080) [1.6 MB] || ",
            "hits": 32
        },
        {
            "id": 11756,
            "url": "https://svs.gsfc.nasa.gov/11756/",
            "result_type": "Produced Video",
            "release_date": "2015-03-17T11:00:00-04:00",
            "title": "Water On The Moon",
            "description": "A NASA spacecraft has found evidence of water ice buried beneath the lunar surface. || c-1280.jpg (1280x720) [254.2 KB] || c-1024.jpg (1024x576) [188.7 KB] || c-1024_print.jpg (1024x576) [170.1 KB] || c-1024_searchweb.png (320x180) [90.3 KB] || c-1024_print_thm.png (80x40) [18.3 KB] || ",
            "hits": 442
        },
        {
            "id": 30578,
            "url": "https://svs.gsfc.nasa.gov/30578/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-01-16T16:00:00-05:00",
            "title": "Permafrost Extent in the Northern Hemisphere",
            "description": "Original 1997 permafrost map || permafrost_northern_hemisphere_orig_print.jpg (1024x724) [276.1 KB] || permafrost_northern_hemisphere_orig.png (4582x3240) [19.2 MB] || permafrost_northern_hemisphere_orig_web.jpg (320x226) [28.0 KB] || permafrost_northern_hemisphere_orig_searchweb.png (320x180) [109.5 KB] || permafrost_northern_hemisphere_orig_thm.png (80x40) [7.3 KB] || permafrost_extent_northern_hemi_30578.pptx [5.2 MB] || permafrost_extent_northern_hemi_30578.key [27.5 MB] || permafrost_northern_hemisphere_orig.hwshow [238 bytes] || ",
            "hits": 164
        },
        {
            "id": 12561,
            "url": "https://svs.gsfc.nasa.gov/12561/",
            "result_type": "Produced Video",
            "release_date": "2014-12-16T10:00:00-05:00",
            "title": "Possible Methane Sources and Sinks on Mars",
            "description": "There are several possible ways that methane can be created, stored, and released on Mars, including both biological and non-biological pathways. || Mars_Methane_Sources_Sinks_PIA19088.jpg (1440x1080) [227.6 KB] || Mars_Methane_Sources_Sinks_PIA19088_searchweb.png (320x180) [108.1 KB] || Mars_Methane_Sources_Sinks_PIA19088_thm.png (80x40) [6.9 KB] || Mars_Methane_Sources_Sinks_PIA19088.tif (1440x1080) [4.5 MB] || ",
            "hits": 183
        },
        {
            "id": 11537,
            "url": "https://svs.gsfc.nasa.gov/11537/",
            "result_type": "Produced Video",
            "release_date": "2014-05-22T00:00:00-04:00",
            "title": "Journey Of Light",
            "description": "The light that illuminates our planet is made deep inside the sun and takes some 40,000 years to travel through the sun’s layers. Particles of light form from atoms undergoing nuclear fusion in the sun’s innermost layer known as the core. The light then flows through the sun’s interior for millennia, slowly bubbling up like water in a boiling pot. It eventually bursts past the sun’s surface, called the photosphere, and rises into the solar atmosphere. Once in the atmosphere—made up of the chromosphere and corona—the light streams out through the solar system. Watch the video to see how light travels from the sun's interior to the surface. || ",
            "hits": 457
        },
        {
            "id": 30499,
            "url": "https://svs.gsfc.nasa.gov/30499/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-05-13T00:00:00-04:00",
            "title": "Ocean Salinity and Daily Argo Coverage",
            "description": "Salinity has been measured at sea for centuries, first using buckets to collect samples, and later (within the past few decades) with instruments known as “CTDs,” which simultaneously measure conductivity (as a proxy for salinity), temperature, and ocean depth (based on pressure). This technology is used to provide single point samples throughout the ocean. The Argo program has over 3500 profiling floats with CTDs currently deployed in all ocean basins. The Argo array of profiling floats is the first attempt to monitor the global subsurface (upper 2000 meters) ocean temperature and salinity fields in real time. The first floats were deployed in late 1999 and it took another 8 years to reach the global target of 3000 operating floats delivering data every 10 days. While ~3500 floats seem like a lot, on a daily basis the ocean is still very undersampled.This visualization shows ocean salinity at 150 meters as derived by an eddy-resolving ocean model. The gray dots represent the daily locations of Argo floats from January 1993 to December 2010. Ocean salinity and temperature data from Argo floats have proved extremely useful, and can be used in combination with data from other sources (such as from NASA’s Aquarius mission and other satellite missions) to observe and model long-term ocean signals related to climate change. || ",
            "hits": 97
        },
        {
            "id": 30176,
            "url": "https://svs.gsfc.nasa.gov/30176/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Subsidence in California's Central Valley",
            "description": "This animation shows, in exaggerated terms, how the surface of the southern Central Valley of California deformed from the period 2007 to 2011. Interferometric data from the Japanese ALOS PALSAR imaging radar was used to measure the deformation, shown in color overlaid on an ASTER image. The large subsidence \"bowl\" that developed over this time period was caused by withdrawal of groundwater, causing subsurface layers to compact. Interferometric synthetic aperture radar, or InSAR, can be used to monitor subsidence in order to prevent groundwater overdraft and irreversible compaction of aquifers. ALOS PALSAR data is copyright JAXA/METI and was provided by the GEO Supersites and the U.S. Government Research Consortium datapool at the Alaska Satellite Facility. || ",
            "hits": 30
        },
        {
            "id": 11176,
            "url": "https://svs.gsfc.nasa.gov/11176/",
            "result_type": "Produced Video",
            "release_date": "2013-01-31T00:00:00-05:00",
            "title": "Europa's Chaos Terrains",
            "description": "Hard layers of ice make up the surface of Jupiter's frozen moon Europa. Glacial cracks and ridges scar its frigid white plains, carving paths across an icy shell that conceals a deep ocean of liquid water. Closer inspection of the moon's fractured topography reveals highly disrupted areas, called chaos terrains, where blocks of ice appear to have broken off, drifted and refrozen to the surface. Searching for an explanation of how these features formed, researchers studying images of Europa taken by NASA's Galileo spacecraft have come up with an answer. As plumes of warm ocean water rise to the subsurface, massive lakes develop inside the moon's crust—some larger than North America's Great Lakes combined. Over time, the ice directly above these lakes collapses, splintering into floating geometric fragments that rotate, raft and resettle into all kinds of chaotic configurations. Watch the video to learn more about Europa's chaos terrains. || ",
            "hits": 211
        },
        {
            "id": 11058,
            "url": "https://svs.gsfc.nasa.gov/11058/",
            "result_type": "Produced Video",
            "release_date": "2012-08-02T00:00:00-04:00",
            "title": "Cruising With Curiosity",
            "description": "The Mars of today is desolate and cold, but has the planet ever been hospitable enough for life? NASA sent its Curiosity rover there to find out. Using a suite of instruments, Curiosity will explore the planet's habitability, past and present. Part of its payload consists of a trio of chemistry tools called SAM, short for Sample Analysis at Mars. SAM's job is to analyze samples scooped or drilled from the surface and \"sniff\" the Martian air for chemical clues about the environment. Roughly the size of a microwave oven, SAM can do the work of an entire chemistry lab and is the most advanced instrument of its kind ever sent to another planet. Watch the videos to learn more about SAM and see it in action. || ",
            "hits": 24
        },
        {
            "id": 10813,
            "url": "https://svs.gsfc.nasa.gov/10813/",
            "result_type": "Produced Video",
            "release_date": "2011-12-13T14:00:00-05:00",
            "title": "NASA Developing Comet Harpoon for Sample Return",
            "description": "Since the beginning of the space age NASA has explored our solar system, bringing back unprecedented scientific knowledge. However only a handful of missions over the past 50 years have actually collected and returned samples from these far off places. Scientists at NASA's Goddard Space Flight Center in Greenbelt, Md. are in the early stages of working out the best design for a sample-collecting comet harpoon. || ",
            "hits": 33
        },
        {
            "id": 40045,
            "url": "https://svs.gsfc.nasa.gov/gallery/mars-sd/",
            "result_type": "Gallery",
            "release_date": "2010-03-08T00:00:00-05:00",
            "title": "Mars Standard-Definition Materials",
            "description": "Mars has long been a focus of NASA missions and research. This gallery contains standard-definition visualizations of NASA's Mars data, missions, and science.",
            "hits": 33
        },
        {
            "id": 10201,
            "url": "https://svs.gsfc.nasa.gov/10201/",
            "result_type": "Produced Video",
            "release_date": "2008-04-14T00:00:00-04:00",
            "title": "LRO Instrument Integrations",
            "description": "The LRO payload, comprised of six instruments and one technology demonstration, will provide key data sets to enable a human return to the moon. Though built at a variety of partner institutions, all of LRO's instruments were integrated onto the spacecraft at NASA's Goddard Space Flight Center. || ",
            "hits": 81
        },
        {
            "id": 2946,
            "url": "https://svs.gsfc.nasa.gov/2946/",
            "result_type": "Visualization",
            "release_date": "2006-05-15T12:00:00-04:00",
            "title": "Europa's Synthetic Subsurface Heat Transport (Version 2)",
            "description": "Encounters with Jupiter's moon Europa by the Voyager and Galileo spacecraft indicated that a liquid salty ocean might exist below a layer of surface ice that is up to 10 kilometers thick. An ocean general circulation model developed to study the earth's oceans was used to investigate the tidally-forced ocean circulations on Europa. The orbit of Europa is 'gravity locked' so that the same side of Europa always faces Jupiter as is the case with the earth's moon. The icy surface of Europa heaves up and down 50 meters due to the strong tidal forces. This visualization shows the temperature changes induced from the flow fields calculated for a European ocean 50 kilometers deep. The warmest temperatures tend to be near the equator, not because of heating by the sun, but because the currents in the European ocean move the warmest waters to that location. Understanding the thermal and flow fields from these model runs will help to interpret observations from future missions to Europa such as the Jupiter's Icy Moons Orbiter mission proposed for launch in 2012. || ",
            "hits": 60
        },
        {
            "id": 2947,
            "url": "https://svs.gsfc.nasa.gov/2947/",
            "result_type": "Visualization",
            "release_date": "2006-05-15T12:00:00-04:00",
            "title": "Europa's Synthetic Subsurface Heat Transport (Version 1)",
            "description": "Under Europa's icy surface are vast extraterrestrial oceans.  This conceptual animation depicts simulated heat transport of these subsurface oceans.  Please note that the simulated heat transport in this animation is only conceptual and a more accurate representation can be found at animation #2946. || ",
            "hits": 43
        },
        {
            "id": 2232,
            "url": "https://svs.gsfc.nasa.gov/2232/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Investigates Solar Flows Under Sunspots",
            "description": "SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot.  Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. || ",
            "hits": 32
        },
        {
            "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": 10
        },
        {
            "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": 6
        },
        {
            "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": 25
        },
        {
            "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": 16
        },
        {
            "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": 8
        },
        {
            "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": 9
        },
        {
            "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": 15
        },
        {
            "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": 13
        },
        {
            "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": 19
        },
        {
            "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": 11
        },
        {
            "id": 1601,
            "url": "https://svs.gsfc.nasa.gov/1601/",
            "result_type": "Visualization",
            "release_date": "1990-07-10T12:00:00-04:00",
            "title": "Supporting Media for MOLA release",
            "description": "How the spacecraft made the gravity map.  Animation by Studio 13. || gravmapping_pre.jpg (320x240) [10.3 KB] || preview_made_from_dv.00070_print.png (320x240) [28.9 KB] || gravmapping.webmhd.webm (960x540) [567.8 KB] || gravmapping.mov (320x240) [1.7 MB] || ",
            "hits": 16
        }
    ]
}