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        {
            "id": 13007,
            "url": "https://svs.gsfc.nasa.gov/13007/",
            "result_type": "Animation",
            "release_date": "2018-04-11T00:00:00-04:00",
            "title": "Jupiter Magnetic Tour",
            "description": "Take a tour of Jupiter's dynamo, the source of its giant magnetic field, in this new global map from the Juno mission. Watch this video on the NASA.gov Video YouTube channel. || JupiterMagneticTourSmall.mp4 (1920x1080) [71.9 MB] || JupiterMagneticTourPreview.jpg (3840x2160) [1.2 MB] || JupiterMagneticTourPreview_searchweb.png (320x180) [57.0 KB] || JupiterMagneticTourPreview_thm.png (80x40) [3.5 KB] || JupiterMagneticTourProRes.webm (960x540) [28.4 MB] || JupiterMagneticTour1080.mp4 (1920x1080) [193.9 MB] || Foreground_Jupiter_Frames (3840x2160) [0 Item(s)] || Background_Star_Frames (3840x2160) [0 Item(s)] || JupiterMagneticTour4k.mp4 (3840x2160) [492.1 MB] || JupiterMagneticTourProRes.mov (3840x2160) [4.1 GB] || ",
            "hits": 240
        },
        {
            "id": 4601,
            "url": "https://svs.gsfc.nasa.gov/4601/",
            "result_type": "Visualization",
            "release_date": "2017-12-18T11:00:00-05:00",
            "title": "Jupiter Quasi-Quadrennial Oscillation",
            "description": "Climate patterns on Jupiter can have striking similarities to those on Earth, making the gas giant a natural laboratory for understanding planetary atmospheres. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Lights,\" \"Times Waits,\" \"The Space Between\" || JupiterQQOpreview.jpg (1920x1080) [456.5 KB] || TWITTER_720_4601_Jupiter_QQO_Master_APR_twitter_720.mp4 (1280x720) [37.7 MB] || 4601_Jupiter_QQO_Master.webm (960x540) [72.7 MB] || FACEBOOK_720_4601_Jupiter_QQO_Master_APR_facebook_720.mp4 (1280x720) [218.0 MB] || YOUTUBE_HQ_4601_Jupiter_QQO_Master_APR_youtube_hq.mov (1920x1080) [875.9 MB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.srt [3.8 KB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.vtt [3.8 KB] || 4601_Jupiter_QQO_Master_APR.mov (1920x1080) [2.4 GB] || ",
            "hits": 54
        },
        {
            "id": 12709,
            "url": "https://svs.gsfc.nasa.gov/12709/",
            "result_type": "Produced Video",
            "release_date": "2017-09-12T10:00:00-04:00",
            "title": "Cassini's Infrared Saturn",
            "description": "Since arriving at Saturn in 2004, Cassini has used its Composite Infrared Spectrometer (CIRS) to study the ringed planet and its moons in heat radiation. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Particle Waves,\" \"Odyssey,\" \"Solaris,\" \"Expansive,\"\"Horizon Ahead,\" \"Ion Bridge,\" \"Outer Space\" || CassiniCIRSpreviewShort.jpg (1920x1080) [591.6 KB] || CassiniCIRSpreviewShort_searchweb.png (320x180) [125.9 KB] || CassiniCIRSpreviewShort_thm.png (80x40) [8.4 KB] || 12709_Cassini_CIRS_Short_TWTR.mp4 (1280x720) [102.0 MB] || WEBM-12709_Cassini_CIRS_Short_APR.webm (960x540) [191.9 MB] || 12709_Cassini_CIRS_Short_FB.mp4 (1280x720) [574.1 MB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.srt [10.3 KB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.vtt [10.3 KB] || 12709_Cassini_CIRS_Short_YT.mp4 (1920x1080) [1.2 GB] || 12709_Cassini_CIRS_Short_APR.mov (1920x1080) [6.0 GB] || 12709_Cassini_CIRS_Short_YT.hwshow [96 bytes] || ",
            "hits": 66
        },
        {
            "id": 4574,
            "url": "https://svs.gsfc.nasa.gov/4574/",
            "result_type": "Visualization",
            "release_date": "2017-05-31T10:00:00-04:00",
            "title": "Temperature, Reflectance Point to Frost near the Moon's Poles",
            "description": "A view of the south pole of the Moon showing where reflectance and temperature data indicate the possible presence of surface water ice. Includes music and narration. Music by Killer Tracks: Full Charge - Zubin Thakkar. || 4574_LROMoonFrost_YouTube.00780_print.jpg (1024x576) [236.8 KB] || 4574_LROMoonFrost_YouTube.mp4 (1920x1080) [75.8 MB] || 4574_LROMoonFrost_Facebook.mp4 (1280x720) [65.4 MB] || 4574_LROMoonFrost_Twitter.mp4 (1280x720) [11.8 MB] || 4574_LROMoonFrost_Facebook.webm (1280x720) [5.2 MB] || 4574_LROMoonFrost_MASTER.mov (1920x1080) [639.4 MB] || 4574_LroMoonFrost_Captions.en_US.srt [761 bytes] || 4574_LroMoonFrost_Captions.en_US.vtt [774 bytes] || 4574_LROMoonFrost_YouTube.mp4.hwshow [191 bytes] || ",
            "hits": 153
        },
        {
            "id": 4559,
            "url": "https://svs.gsfc.nasa.gov/4559/",
            "result_type": "Visualization",
            "release_date": "2017-04-27T10:00:00-04:00",
            "title": "Kepler Stares at Neptune",
            "description": "In late 2014 and early 2015, NASA's Kepler telescope observed the eighth planet in our solar system, Neptune. Kepler detected Neptune's daily rotation, the movement of clouds, and even minute changes in the sun's brightness, paving the way for future studies of weather and climate beyond our solar system. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks:\"Lost Contact\" – Adam Salkeld & Neil Pollard\"Processing Thoughts\" – Theo Golding || Neptune-Triton-Zoom-Thumbnail.jpg (1920x1080) [1.2 MB] || 4559_Kepler_Neptune_Twitter_720.mp4 (1280x720) [30.6 MB] || WEBM-4559_Kepler_Neptune_APR.webm (960x540) [58.6 MB] || Neptune-Triton-Zoom-Thumbnail_Big.tiff (1920x1080) [11.9 MB] || 4559_Kepler_Neptune_Facebook_720.mp4 (1280x720) [173.0 MB] || 4559_Kepler_Neptune_Captions_Output.en_US.srt [2.8 KB] || 4559_Kepler_Neptune_Captions_Output.en_US.vtt [2.9 KB] || 4559_Kepler_Neptune_APR.mov (1920x1080) [1.9 GB] || 4559_Kepler_Neptune_APR_4444.mov (1920x1080) [4.1 GB] || 4559_Kepler_Neptune_APR.mov.hwshow [205 bytes] || ",
            "hits": 112
        },
        {
            "id": 12322,
            "url": "https://svs.gsfc.nasa.gov/12322/",
            "result_type": "Produced Video",
            "release_date": "2016-08-04T11:00:00-04:00",
            "title": "Sampling An Asteroid",
            "description": "NASA is sending a robotic spacecraft to collect material from an asteroid and return it to Earth. || c-1024.jpg (1024x576) [160.1 KB] || c-1280.jpg (1280x720) [225.7 KB] || c-1920.jpg (1920x1080) [337.4 KB] || c-1024_print.jpg (1024x576) [169.1 KB] || c-1024_searchweb.png (320x180) [79.8 KB] || c-1024_web.png (320x180) [79.8 KB] || c-1024_thm.png (80x40) [6.6 KB] || ",
            "hits": 27
        },
        {
            "id": 12304,
            "url": "https://svs.gsfc.nasa.gov/12304/",
            "result_type": "Produced Video",
            "release_date": "2016-07-14T11:00:00-04:00",
            "title": "Cool Craters",
            "description": "On dwarf planet Ceres, scientists map craters where ice can accumulate. || cf-1024.jpg (1024x576) [155.4 KB] || cf-1280.jpg (1280x720) [221.7 KB] || cf-1920.jpg (1920x1080) [357.8 KB] || cf-1024_print.jpg (1024x576) [157.7 KB] || cf-1024_searchweb.png (320x180) [62.8 KB] || cf-1024_web.png (320x180) [62.8 KB] || cf-1024_thm.png (80x40) [4.5 KB] || ",
            "hits": 36
        },
        {
            "id": 12293,
            "url": "https://svs.gsfc.nasa.gov/12293/",
            "result_type": "Produced Video",
            "release_date": "2016-06-30T11:00:00-04:00",
            "title": "Exploring Jupiter’s Magnetism",
            "description": "NASA’s Juno spacecraft will create a detailed map of Jupiter’s magnetic field. || c-1024.jpg (1024x576) [240.2 KB] || c-1280.jpg (1280x720) [323.9 KB] || c-1920.jpg (1920x1080) [480.4 KB] || c-1024_print.jpg (1024x576) [249.9 KB] || c-1024_searchweb.png (320x180) [142.9 KB] || c-1024_web.png (320x180) [142.9 KB] || c-1024_thm.png (80x40) [28.7 KB] || ",
            "hits": 73
        },
        {
            "id": 12296,
            "url": "https://svs.gsfc.nasa.gov/12296/",
            "result_type": "Produced Video",
            "release_date": "2016-06-29T09:00:00-04:00",
            "title": "Exploring Jupiter's Magnetic Field",
            "description": "NASA is sending the Juno spacecraft to peer beneath the cloudy surface of Jupiter. Juno's twin magnetometers, built at Goddard Space Flight Center, will give scientists their first look at the dynamo that drives Jupiter's vast magnetic field. Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || JupiterMagnetometerPreview.jpg (1920x1080) [591.9 KB] || JupiterMagnetometerPreview_searchweb.png (320x180) [118.7 KB] || JupiterMagnetometerPreview_thm.png (80x40) [8.0 KB] || 12296_Juno_Magnetometer_appletv.m4v (1280x720) [159.8 MB] || WEBM_12296_Juno_Magnetometer_APR.webm (960x540) [124.4 MB] || 12296_Juno_Magnetometer_appletv_subtitles.m4v (1280x720) [159.9 MB] || LARGE_MP4_12296_Juno_Magnetometer_APR_large.mp4 (1920x1080) [311.4 MB] || 12296_Juno_Magnetometer_APR_Output.en_US.srt [6.2 KB] || 12296_Juno_Magnetometer_APR_Output.en_US.vtt [6.2 KB] || 12296_Juno_Magnetometer_ipod_sm.mp4 (320x240) [53.1 MB] || 12296_Juno_Magnetometer_APR.mov (1920x1080) [4.1 GB] || ",
            "hits": 182
        },
        {
            "id": 12079,
            "url": "https://svs.gsfc.nasa.gov/12079/",
            "result_type": "Produced Video",
            "release_date": "2015-12-29T11:00:00-05:00",
            "title": "Falling Apart",
            "description": "Weird marks on Phobos’ surface are early signs of the end for this moon of Mars. || c-1280.jpg (1280x720) [107.5 KB] || c-1024.jpg (1024x576) [75.5 KB] || c-1024_print.jpg (1024x576) [67.4 KB] || c-1024_searchweb.png (320x180) [24.6 KB] || c-1024_web.png (320x180) [24.6 KB] || c-1024_thm.png (80x40) [11.2 KB] || ",
            "hits": 88
        },
        {
            "id": 12021,
            "url": "https://svs.gsfc.nasa.gov/12021/",
            "result_type": "Produced Video",
            "release_date": "2015-10-13T13:00:00-04:00",
            "title": "Hubble Maps Jupiter in 4k Ultra HD",
            "description": "New imagery from the Hubble Space Telescope is revealing details never before seen on Jupiter. Hubble’s new Jupiter maps were used to create this Ultra HD animation.Watch this video on the NASA Explorer YouTube channel. || JupiterThumbnailSmall.png (2160x1215) [1.4 MB] || G2015-085_Jupiter720_MASTER_appletv_appletv_subtitles.m4v (1280x720) [39.0 MB] || G2015-085_Jupiter720_MASTER_appletv.m4v (1280x720) [39.0 MB] || WEBM_G2015-085_Jupiter4k_MASTER_YouTube.webm (960x540) [28.5 MB] || G2015-085_Jupiter720_MASTER.mp4 (1280x720) [98.9 MB] || G2015-085_Jupiter720_MASTER_nasa_tv.mpeg (1280x720) [249.3 MB] || G2015-085_Jupiter720_MASTER_prores.mov (1280x720) [917.9 MB] || G2015-085_Jupiter720_MASTER.en_US.srt [98 bytes] || G2015-085_Jupiter720_MASTER.en_US.vtt [111 bytes] || G2015-085_Jupiter720_.key [41.8 MB] || G2015-085_Jupiter720_.pptx [39.3 MB] || G2015-085_Jupiter720_MASTER_12021.key [41.7 MB] || G2015-085_Jupiter720_MASTER_12021.pptx [39.3 MB] || G2015-085_Jupiter4k_MASTER_YouTube.mp4 (3840x2160) [495.9 MB] || G2015-085_Jupiter4k_MASTER.mov (3840x2160) [4.5 GB] || G2015-085_Jupiter4k_MASTER_YouTube.hwshow [94 bytes] || G2015-085_Jupiter720_MASTER_appletv.m4v.hwshow [88 bytes] || ",
            "hits": 960
        },
        {
            "id": 11921,
            "url": "https://svs.gsfc.nasa.gov/11921/",
            "result_type": "Produced Video",
            "release_date": "2015-10-13T11:00:00-04:00",
            "title": "Planetary Portrait",
            "description": "The Hubble Space Telescope provides new maps of Jupiter. || c-1920.jpg (1920x1080) [171.1 KB] || c-1280.jpg (1280x720) [116.9 KB] || c-1024.jpg (1024x576) [89.3 KB] || c-1024_print.jpg (1024x576) [94.5 KB] || c-1024_searchweb.png (320x180) [34.8 KB] || c-1024_web.png (320x180) [34.8 KB] || c-1024_thm.png (80x40) [3.3 KB] || ",
            "hits": 61
        },
        {
            "id": 11898,
            "url": "https://svs.gsfc.nasa.gov/11898/",
            "result_type": "Produced Video",
            "release_date": "2015-06-12T12:30:00-04:00",
            "title": "Hubble Detects \"Sunscreen\" Layer on Distant Planet",
            "description": "ANIMATION Using NASA’s Hubble Telescope, scientists detected a stratosphere on the planet WASP-33b. A stratosphere occurs when molecules in the atmosphere absorb ultraviolet and visible light from the star. This absorption warms the stratosphere and acts as a kind of sunscreen layer for the planet below.Watch this video on YouTube. || CoolHotAll3av8_print.jpg (1024x576) [49.2 KB] || CoolHotAll3av8_searchweb.png (320x180) [48.2 KB] || CoolHotAll3av8_thm.png (80x40) [4.6 KB] || CoolHotAll3av8.mp4 (1920x1080) [46.7 MB] || CoolHotAll3av8sm.mp4 (1280x720) [16.4 MB] || CoolHotAll3av8sm.webm (1280x720) [2.2 MB] || ",
            "hits": 74
        },
        {
            "id": 11760,
            "url": "https://svs.gsfc.nasa.gov/11760/",
            "result_type": "Produced Video",
            "release_date": "2015-03-31T11:00:00-04:00",
            "title": "A Once-Blue Planet",
            "description": "NASA research suggests an ocean once covered the surface of Mars. || c-1280.jpg (1280x720) [229.4 KB] || c-1024.jpg (1024x576) [157.9 KB] || c-1024_print.jpg (1024x576) [150.3 KB] || c-1024_searchweb.png (320x180) [80.7 KB] || c-1024_print_thm.png (80x40) [18.5 KB] || ",
            "hits": 73
        },
        {
            "id": 11796,
            "url": "https://svs.gsfc.nasa.gov/11796/",
            "result_type": "Produced Video",
            "release_date": "2015-03-05T14:00:00-05:00",
            "title": "Mars’ Ancient Ocean",
            "description": "NASA planetary scientists Geronimo Villanueva and Michael Mumma discuss their findings regarding the ancient ocean of Mars.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Mars_Ocean_still_print.jpg (1024x576) [113.5 KB] || Mars_Ocean_still.png (1920x1080) [3.0 MB] || Mars_Ocean_still_web.jpg (320x180) [16.0 KB] || Mars_Ocean_still_searchweb.png (320x180) [86.4 KB] || Mars_Ocean_still_thm.png (80x40) [8.2 KB] || G2015-011_MarsOcean_MASTER_appletv.webm (960x540) [30.9 MB] || G2015-011_MarsOcean_MASTER_ipod_lg.m4v (640x360) [46.0 MB] || G2015-011_MarsOcean_MASTER_ipod_sm.mp4 (320x240) [24.8 MB] || G2015-011_MarsOcean_MASTER.en_US.srt [4.4 KB] || G2015-011_MarsOcean_MASTER.en_US.vtt [4.4 KB] || G2015-011_MarsOcean_MASTER_prores.mov (1280x720) [4.0 GB] || G2015-011_MarsOcean_MASTER_youtube_hq.mov (1280x720) [187.8 MB] || G2015-011_MarsOcean_MASTER_appletv.m4v (960x540) [116.1 MB] || G2015-011_MarsOcean_MASTER_1280x720.wmv (1280x720) [136.4 MB] || G2015-011_MarsOcean_MASTER_appletv_subtitles.m4v (960x540) [116.0 MB] || G2015-011_MarsOcean_MASTER_nasaportal.mov (640x360) [112.8 MB] || ",
            "hits": 358
        },
        {
            "id": 11673,
            "url": "https://svs.gsfc.nasa.gov/11673/",
            "result_type": "Produced Video",
            "release_date": "2014-10-14T11:45:00-04:00",
            "title": "MAVEN at Mars",
            "description": "On September 21, 2014, NASA’s Mars Atmosphere and Volatile Evolution, or MAVEN, spacecraft completed its 10-month journey and entered orbit around the Red Planet. As the first mission devoted to observing the tenuous upper atmosphere of Mars, MAVEN will help scientists determine how much of the atmosphere has been lost throughout the planet’s history and which processes have driven that loss. The spacecraft has already conducted preliminary observations of important gases in the planet’s upper atmosphere and sent those images back to Earth. Watch the videos to learn more about the MAVEN mission. || ",
            "hits": 49
        },
        {
            "id": 11443,
            "url": "https://svs.gsfc.nasa.gov/11443/",
            "result_type": "Produced Video",
            "release_date": "2014-01-21T00:00:00-05:00",
            "title": "Water Worlds",
            "description": "Earth, the blue planet, is our idea of a water world. But a planet doesn't have to be earthlike to have water. Using NASA's Hubble Space Telescope, scientists found faint signals of water in the atmospheres of five distant planets. All five—HD 209458b, WASP-12b, WASP-17b, WASP-19b and XO-1b—are a type of exoplanet known as hot Jupiters, massive worlds that orbit very close to their stars. Although the planets were quite hazy, the researchers could tell that two of them had stronger water signals than the other three. Being able to compare planets this way is a key step in figuring out why some worlds wind up with plentiful water yet others don't. Watch the video to see an animation of a hot Jupiter orbiting its star. || ",
            "hits": 59
        },
        {
            "id": 11428,
            "url": "https://svs.gsfc.nasa.gov/11428/",
            "result_type": "Produced Video",
            "release_date": "2013-12-03T12:00:00-05:00",
            "title": "Alien Atmospheres",
            "description": "Since the early 1990's, astronomers have known that extrasolar planets, or \"exoplanets,\" orbit stars light-years beyond our own solar system. Although most exoplanets are too distant to be directly imaged, detailed studies have been made of their size, composition, and even atmospheric makeup - but how? By observing periodic variations in the parent star's brightness and color, astronomers can indirectly determine an exoplanet's distance from its star, its size, and its mass. But to truly understand an exoplanet astronomers must study its atmosphere, and they do so by splitting apart the parent star's light during a planetary transit. || ",
            "hits": 238
        },
        {
            "id": 11372,
            "url": "https://svs.gsfc.nasa.gov/11372/",
            "result_type": "Produced Video",
            "release_date": "2013-11-28T00:00:00-05:00",
            "title": "Mars Evolution",
            "description": "What does catastrophic climate change look like? Mars can help answer that question. The Red Planet today is a desert world, cold and dry. Billions of years ago, however, Mars probably had a thick atmosphere that kept the planet warm enough to have water flowing on the surface. To investigate how Mars lost that abundant atmosphere, NASA launched the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft on November 18, 2013. The spacecraft will orbit Mars and examine the processes that are stripping away what remains of the planet’s fragile upper atmosphere. Understanding what happened on Mars will give us new insight into the habitability of planets and global climate change. Watch the video to see what Mars's radical transformation might have looked like. || ",
            "hits": 203
        },
        {
            "id": 11371,
            "url": "https://svs.gsfc.nasa.gov/11371/",
            "result_type": "Produced Video",
            "release_date": "2013-11-14T00:00:00-05:00",
            "title": "Crude Matter",
            "description": "What do car bumpers and computer speakers have in common? Both can be created from raw materials found on Earth or on Titan, Saturn’s largest moon. Titan is the only moon in the solar system with a significant atmosphere. In some ways its atmosphere is similar to Earth’s, but rather than being rich in oxygen, it’s rich in hydrocarbons—chemical compounds made of the elements carbon and hydrogen. In 1980, NASA's Voyager 1 spacecraft flew by Titan and detected different types of hydrocarbons in its atmosphere, including methane, ethane and propane. Now, NASA’s Cassini spacecraft has added one more to the list: propylene, a chemical building block used in the manufacture of plastic consumer goods. Watch the video to learn more. || ",
            "hits": 37
        },
        {
            "id": 11339,
            "url": "https://svs.gsfc.nasa.gov/11339/",
            "result_type": "Produced Video",
            "release_date": "2013-09-30T12:00:00-04:00",
            "title": "Propylene on Titan",
            "description": "With a thick atmosphere, clouds, a rain cycle and giant lakes, Saturn's large moon Titan is a surprisingly Earthlike place. But unlike on Earth, Titan's surface is far too cold for liquid water - instead, Titan's clouds, rain, and lakes consist of liquid hydrocarbons like methane and ethane (which exist as gases here on Earth). When these hydrocarbons evaporate and encounter ultraviolet radiation in Titan's upper atmosphere, some of the molecules are broken apart and reassembled into longer hydrocarbons like ethylene and propane.NASA's Voyager 1 spacecraft first revealed the presence of several species of atmospheric hydrocarbons when it flew by Titan in 1980, but one molecule was curiously missing - propylene, the main ingredient in plastic number 5. Now, thanks to NASA's Cassini spacecraft, scientists have detected propylene on Titan for the first time, solving a long-standing mystery about the solar system's most Earthlike moon. || ",
            "hits": 64
        },
        {
            "id": 11276,
            "url": "https://svs.gsfc.nasa.gov/11276/",
            "result_type": "Produced Video",
            "release_date": "2013-07-02T00:00:00-04:00",
            "title": "Drilling On Mars",
            "description": "NASA's Curiosity rover is the first robot to collect a sample drilled from the surface of Mars. On February 8, 2013, the tool at the end of Curiosity's robotic arm successfully drove a drill bit about two and a half inches into a flat patch of rock. Analysis of the powdery sample collected from the rock, now named John Klein, showed environmental conditions that could have been favorable for microbial life. This rock lies in Glenelg, a region where scientists found evidence of past water. The rover drilled into a second rock nearby, called Cumberland, on May 19 to confirm the results of the initial tests. This time, Curiosity made use of its new capability to stow some of the sample, in case more tests need to be conducted later. Watch the video and animation to see how Curiosity drills. || ",
            "hits": 92
        },
        {
            "id": 11237,
            "url": "https://svs.gsfc.nasa.gov/11237/",
            "result_type": "Produced Video",
            "release_date": "2013-04-25T00:00:00-04:00",
            "title": "Jupiter's Hot Spots",
            "description": "Jupiter is a planet known for clouds, from its distinctive orange and white stripes to the swirling vortex known as the Great Red Spot. But its cloudless patches are just as interesting—and so unusual that the big ones get the special name \"hot spots.\" Exactly how they form and why they're only found near the equator have long been mysteries. To study hot spots in motion, scientists made movies from images taken when NASA's Cassini spacecraft flew past the planet in 2000. The movies reveal new evidence that Jupiter's hot spots are created by an atmospheric phenomenon known as a Rossby wave. As the wave glides up and down in Jupiter's atmosphere like a horse on a merry-go-round, it creates holes in the clouds by displacing cold air. This results in a line of cloud-free warm air pockets, or hot spots, seen around the planet. Watch the video to learn more. || ",
            "hits": 55
        },
        {
            "id": 11217,
            "url": "https://svs.gsfc.nasa.gov/11217/",
            "result_type": "Produced Video",
            "release_date": "2013-03-04T12:00:00-05:00",
            "title": "Cosmic Ice Lab Studies Reactions Occurring in Deep Space",
            "description": "At the NASA Goddard Cosmic Ice Lab, scientists are studying ice to help us understand the unusual chemical reactions that occur in space. Ice in space is amorphous, lacking the crystalline structure of the ice found on Earth. In space, this ice is often dirty, containing different kinds of particles and organic molecules. Recent discoveries have found that compounds trapped in amorphous ice are involved in a kind of chemistry unlike anything known on Earth. At the Goddard Cosmic Ice Lab, scientists are recreating the conditions of space to study the properties of amorphous ice firsthand. Their research will help astronomers to interpret observations of the far reaches of space, and further our understanding of the potential for the existence life beyond Earth. || ",
            "hits": 57
        },
        {
            "id": 11184,
            "url": "https://svs.gsfc.nasa.gov/11184/",
            "result_type": "Produced Video",
            "release_date": "2013-02-05T00:00:00-05:00",
            "title": "Mercury's Ice Lockers",
            "description": "Mercury, the closest planet to the sun, sits in the hot seat, with temperatures soaring up to 800 degrees Fahrenheit. Certain spots at the planet's north and south poles, however, remain extremely cold—so cold, in fact, that scientists long suspected this sun-scorched planet of harboring ice. Sure enough, in 2012 NASA's MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) mission reported finding deposits of ice and frozen chemicals at Mercury's north pole. Granted, Mercury doesn't have the same kind of ice cap Earth does. But if all the deposits were added up, there would be enough ice to bury Washington, D.C., under a layer two miles thick. Watch the animation to see just how bone-chillingly dark Mercury's north pole can be, especially in deep craters, where the sun may never shine. || ",
            "hits": 627
        },
        {
            "id": 11148,
            "url": "https://svs.gsfc.nasa.gov/11148/",
            "result_type": "Produced Video",
            "release_date": "2012-12-25T00:00:00-05:00",
            "title": "Road Trip",
            "description": "The Curiosity rover's main destination is Mount Sharp and its intriguing rock layers. But before heading there, the rover took a road trip east to check out Glenelg, an area where three types of Martian terrain come together. Along the way, Curiosity made several stops, especially at Rocknest, where it took its first sniffs of the Martian atmosphere and its first scoops of soil. After analyzing those samples, the rover was back on the move toward Point Lake, a spot near Glenelg where Curiosity will look for a place to try out its drill. Some highlights of the rover's trip are captured in the videos and these pictures, starting with Curiosity's view of the landing site as it neared touchdown. || ",
            "hits": 6
        },
        {
            "id": 11127,
            "url": "https://svs.gsfc.nasa.gov/11127/",
            "result_type": "Produced Video",
            "release_date": "2012-11-15T00:00:00-05:00",
            "title": "Saturn's Superstorm",
            "description": "A spectacular storm, massive enough to be seen from Earth, erupted in Saturn's northern hemisphere in December 2010. The storm spawned bright clouds that wrapped all the way around the planet, while its powerful vortex grew larger than Jupiter's Great Red Spot. But the greatest surprises came six months after the storm began, as visible signs started to fade. That's when NASA's Cassini spacecraft and ground-based observers caught Saturn letting out an unprecedented belch of energy and releasing a huge amount of ethylene gas. The energy sent temperatures soaring in Saturn's atmosphere, a spike comparable in scale to jumping straight from deep winter in Fairbanks, Alaska, to high summer in the Mojave Desert. Scientists are still puzzled by the mysterious release of ethylene, a gas not typically observed on Saturn. Watch the videos to learn more about this rare and surprising superstorm. || ",
            "hits": 246
        },
        {
            "id": 11088,
            "url": "https://svs.gsfc.nasa.gov/11088/",
            "result_type": "Produced Video",
            "release_date": "2012-10-09T00:00:00-04:00",
            "title": "Thin Air",
            "description": "Did ancient Mars have a thick atmosphere and cloudy skies? Did liquid water flow on its surface? It's hard to imagine either one on the dry, dusty Mars of today. But scientists think the conditions on Mars could have been quite different before the planet started to lose its atmosphere. Exactly how Mars' atmosphere thinned is still being investigated, but there are several possibilities. One is a process called sputtering, a kind of atomic billiards game in which high-energy particles from the sun collide with molecules in the atmosphere and knock them away. NASA's MAVEN mission, scheduled to launch in 2013, will study why and how quickly the atmosphere surrounding Mars turned into thin air. Watch the video to explore the idea that Mars' once-thick atmosphere sputtered away. || ",
            "hits": 133
        },
        {
            "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": 21
        },
        {
            "id": 11010,
            "url": "https://svs.gsfc.nasa.gov/11010/",
            "result_type": "Produced Video",
            "release_date": "2012-07-10T00:00:00-04:00",
            "title": "Sizing Up Earth",
            "description": "At a given point in time, Earth usually seems stable. But over centuries, lands rise and sink, continents move and the balance of the ocean shifts. These changes are tracked through the science of geodesy, dedicated to measuring and precisely charting the size and shape of Earth. Geodesy began more than 2,000 years ago, when the Greek scholar Eratosthenes calculated the circumference of Earth with impressive accuracy. In modern geodesy, scientists use multiple techniques to map the world's ice sheets, watch sea level creep up and monitor the impact of earthquakes, droughts and floods. This animated video looks at the long history of geodesy and highlights some of the technologies NASA uses, such as radio telescopes and long-range lasers, to take the basic measure of our planet. || ",
            "hits": 368
        },
        {
            "id": 10981,
            "url": "https://svs.gsfc.nasa.gov/10981/",
            "result_type": "Produced Video",
            "release_date": "2012-06-05T00:00:00-04:00",
            "title": "Jupiter's Jet Streams",
            "description": "Jupiter is the largest and most massive planet in our solar system. You might not think of it as a place to learn about Earth's atmosphere and weather, but Jupiter, like our home planet, has cyclones (the Jovian equivalent of hurricanes) and anticyclones, along with fast-moving jet streams that circle its globe. Revealed in a sequence of black-and-white images taken by the Cassini spacecraft during its flyby of Jupiter are chevrons, dark V-shaped features that travel within a band of powerful winds near the equator. By tracking chevrons, NASA scientists were not only able to gauge the jet stream's speed, but also witness its subtle, wavelike movement as it zoomed around the planet—something never before seen. Studying this motion can help scientists better understand similar weather patterns on Earth. Learn more about this discovery and see footage of Jupiter's jet streams by watching the videos below. || ",
            "hits": 107
        },
        {
            "id": 10974,
            "url": "https://svs.gsfc.nasa.gov/10974/",
            "result_type": "Produced Video",
            "release_date": "2012-05-17T00:00:00-04:00",
            "title": "Most Wanted",
            "description": "There are about 600,000 asteroids in the solar system. That's roughly one for every person living in Washington, D.C. And with more of these rocky objects being found all the time, it's becoming harder to keep track of them all. That's why NASA scientists have assembled a most-wanted list of about six-dozen asteroids that, with the help of amateur astronomers, will be studied in preparation for the first U.S. asteroid sample return mission. Scheduled for launch in 2016, NASA's OSIRIS-REx spacecraft will orbit asteroid 1999 RQ36 and collect a sample from the surface that is returned to Earth. Analysis of the primitive material will not only reveal new information about the molecular origins of life and how the early solar system formed, but also provide insight into the behavior and movement of near-Earth objects in space. Watch the video below to see how the spacecraft will obtain a sample from the asteroid. || ",
            "hits": 30
        },
        {
            "id": 10951,
            "url": "https://svs.gsfc.nasa.gov/10951/",
            "result_type": "Produced Video",
            "release_date": "2012-04-19T00:00:00-04:00",
            "title": "Earthrise 2.0",
            "description": "On December 24, 1968, three Apollo astronauts circled the moon, becoming the first humans ever to do so. On their fourth orbit, Apollo 8 Commander Frank Borman interrupted the studies of the moon's cratered terrain to roll the spacecraft, bringing the three main windows around to face the direction of travel. All of a sudden, a bright sliver of light appeared from behind the lunar horizon. Within seconds, a sphere with dazzling white swirls and vivid shades of blue came into view. The astronauts quickly positioned the onboard cameras, first capturing a black-and-white image of Earth rising, and then snapping a color photo of the Blue Planet floating above the horizon. This breathtaking color image would later become known as the iconic Earthrise photograph. The visualization uses data collected by NASA's Terra satellite and Lunar Reconnaissance Orbiter to re-create this historic moment in space exploration. || ",
            "hits": 162
        },
        {
            "id": 10931,
            "url": "https://svs.gsfc.nasa.gov/10931/",
            "result_type": "Produced Video",
            "release_date": "2012-03-15T00:00:00-04:00",
            "title": "Moon Struck",
            "description": "Long before the first humans gazed up into the velvety blackness of the night sky, the moon was young and fresh-faced. These were the early days, before the patchwork of inky stains called the Man in the Moon, before the brilliant starburst patterns called ray craters decorated the surface, before a colossal crash turned one-fifth of its real estate into the South Pole-Aitken basin. Fast-forward to the present, and the moon's once smooth contour appears flawed and disfigured, punished by explosive volcanic eruptions and raining interstellar objects that bombarded its surface over eons. In the visualizations below, see some of the clearest views of the moon yet, courtesy of NASA's Lunar Reconnaissance Orbiter, and witness a recreation of the destructive, 4.5-billion-year evolution of Earth's natural satellite. || ",
            "hits": 80
        }
    ]
}