{ "count": 15, "next": null, "previous": null, "results": [ { "id": 14162, "url": "https://svs.gsfc.nasa.gov/14162/", "result_type": "Produced Video", "release_date": "2022-05-19T15:30:00-04:00", "title": "Saturn Through the Veil of Enceladus – Artist’s Concept", "description": "Artist’s concept of Saturn and its icy moons Enceladus (foreground), Titan (large crescent at upper left), and Rhea (small crescent). Based on imagery from the Cassini spacecraft. || SaturnMoonsConceptArt_print.jpg (1024x460) [68.0 KB] || SaturnMoonsConceptArt.png (4800x2160) [6.3 MB] || SaturnMoonsConceptArt.jpg (4800x2160) [502.7 KB] || SaturnMoonsConceptArt_searchweb.png (320x180) [61.1 KB] || SaturnMoonsConceptArt_thm.png (80x40) [4.9 KB] || ", "hits": 183 }, { "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": 129 }, { "id": 30901, "url": "https://svs.gsfc.nasa.gov/30901/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Cassini's Final Image", "description": "Cassini's final image || PIA21895_print.jpg (1024x1030) [71.7 KB] || PIA21895_searchweb.png (320x180) [29.7 KB] || PIA21895_thm.png (80x40) [2.5 KB] || PIA21895.tif (505x508) [190.2 KB] || cassinis-final-image.hwshow [260 bytes] || ", "hits": 100 }, { "id": 30902, "url": "https://svs.gsfc.nasa.gov/30902/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Cassini, So Far from Home", "description": "one of Cassini's last looks at Saturn & its main rings || PIA21345_print.jpg (1024x529) [51.6 KB] || PIA21345_searchweb.png (320x180) [43.9 KB] || PIA21345_thm.png (80x40) [4.7 KB] || PIA21345.tif (3545x1834) [9.4 MB] || cassini-so-far-from-home.hwshow [200 bytes] || ", "hits": 106 }, { "id": 30903, "url": "https://svs.gsfc.nasa.gov/30903/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Two Titans", "description": "Two views of Saturn's moon Titan || PIA21624_print.jpg (1024x518) [43.1 KB] || PIA21624_searchweb.png (320x180) [51.4 KB] || PIA21624_thm.png (80x40) [5.2 KB] || PIA21624.tif (2024x1024) [3.9 MB] || two-titans.hwshow [186 bytes] || ", "hits": 52 }, { "id": 12714, "url": "https://svs.gsfc.nasa.gov/12714/", "result_type": "Produced Video", "release_date": "2017-09-14T00:00:00-04:00", "title": "Goddard Team Reflects on 20 Years of Cassini", "description": "The people behind Cassini's Composite Infrared Spectrometer (CIRS) reflect on their years-long experience working with their team - relationships formed, children born, challenges conquered, and their feelings as the Cassini mission comes to an end. CIRS was built and is operated at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Cassini is making its final dive into Saturn on September 15, 2017.Read the web feature on nasa.gov. || ", "hits": 25 }, { "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": 67 }, { "id": 30883, "url": "https://svs.gsfc.nasa.gov/30883/", "result_type": "Hyperwall Visual", "release_date": "2017-06-07T12:00:00-04:00", "title": "Saturn's Hexagon as Summer Solstice Approaches", "description": "June 2013 vs. April 2017 || saturn_hex_color_1080p.00001_print.jpg (1024x576) [75.7 KB] || saturn_hex_color_1080p.00001_searchweb.png (320x180) [67.7 KB] || saturn_hex_color_1080p.00001_thm.png (80x40) [4.8 KB] || saturn_hex_color_1080p.mp4 (1920x1080) [5.4 MB] || saturn_hex_color_720p.mp4 (1280x720) [2.1 MB] || saturn_hex_color_1080p.webm (1920x1080) [1.1 MB] || saturn_hex_color_2304p.mp4 (4096x2304) [28.0 MB] || 4104x2304_16x9_30p (4104x2304) [32.0 KB] || ", "hits": 277 }, { "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": 1004 }, { "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": 86 }, { "id": 11204, "url": "https://svs.gsfc.nasa.gov/11204/", "result_type": "Produced Video", "release_date": "2013-03-14T14:30:00-04:00", "title": "Jupiter's Hot Spots", "description": "Jupiter's bright Equatorial Zone swirls with dark patches, dubbed \"hot spots\" for their infrared glow. These holes in the ammonia clouds at the top of the atmosphere allow a glimpse into Jupiter's darker, hotter layers below. In 1995 NASA's Galileo spacecraft dropped a probe directly into a hot spot, taking the first and only in situ measurements of Jupiter's atmosphere. Now, movies recorded by NASA's Cassini spacecraft reveal that hot spots are not just local weather phenomena, but are in fact linked to much larger-scale atmospheric structures called Rossby waves. || ", "hits": 36 }, { "id": 11038, "url": "https://svs.gsfc.nasa.gov/11038/", "result_type": "Produced Video", "release_date": "2012-10-25T09:00:00-04:00", "title": "Saturn's Record-Setting Storm", "description": "NASA scientist Brigette Hesman discusses extreme temperature changes in Saturn's 2010 Great White Spot. || ", "hits": 155 }, { "id": 10927, "url": "https://svs.gsfc.nasa.gov/10927/", "result_type": "Produced Video", "release_date": "2012-03-13T13:00:00-04:00", "title": "RATTLING JET STREAM ON JUPITER", "description": "New movies of Jupiter are the first to catch an invisible wave shaking up one of the giant planet's jet streams, an interaction that also takes place in Earth's atmosphere and influences the weather.For complete transcript, click here. || G2012-013_Jupiter_Weather_portal.00752_print.jpg (1024x576) [69.0 KB] || G2012-013_Jupiter_Weather_portal_web.png (320x180) [190.6 KB] || G2012-013_Jupiter_Weather_portal_thm.png (80x40) [16.5 KB] || G2012-013_Jupiter_Weather.wmv (1280x720) [62.8 MB] || G2012-013_Jupiter_Weather_youtube_hq.mov (1280x720) [70.4 MB] || G2012-013_Jupiter_Weather_appletv.m4v (960x540) [56.5 MB] || G2012-013_Jupiter_Weather_appletv.webmhd.webm (960x540) [27.4 MB] || G2012-013_Jupiter_Weather_portal.mov (640x360) [53.2 MB] || G2012-013_Jupiter_Weather_ipod_lg.m4v (640x360) [22.3 MB] || GSFC_20120313_Jupiter_m10927_Weather.en_US.vtt [2.7 KB] || G2012-013_Jupiter_Weather_prores.mov (1280x720) [1.9 GB] || G2012-013_Jupiter_Weather_ipod_sm.mp4 (320x240) [11.7 MB] || ", "hits": 47 }, { "id": 10790, "url": "https://svs.gsfc.nasa.gov/10790/", "result_type": "Produced Video", "release_date": "2011-06-09T12:00:00-04:00", "title": "Voyager Satellites Find Magnetic Bubbles at Edge of Solar System", "description": "The sun's magnetic field spins opposite directions on the north and south poles. These oppositely pointing magnetic fields are separated by a layer of current called the heliospheric current sheet. Due to the tilt of the magnetic axis in relation to the axis of rotation of the Sun, the heliospheric current sheet flaps like a flag in the wind. The flapping current sheet separates regions of oppositely pointing magnetic field, called sectors. As the solar wind speed decreases past the termination shock, the sectors squeeze together, bringing regions of opposite magnetic field closer to each other. The Voyager spacecraft have now found that when the separation of sectors becomes very small, the sectored magnetic field breaks up into a sea of nested \"magnetic bubbles\" in a phenomenon called magnetic reconnection. The region of nested bubbles is carried by the solar wind to the north and south filling out the entire front region of the heliopause and the sector region in the heliosheath.This discovery has prompted a complete revision of what the heliosheath region looks like. The smooth, streamlined look is gone, replaced with a bubbly, frothy outer layer. More animations about the Voyager magnetic bubbles discovery are available. || ", "hits": 172 }, { "id": 10705, "url": "https://svs.gsfc.nasa.gov/10705/", "result_type": "Produced Video", "release_date": "2010-12-16T00:00:00-05:00", "title": "Taking on Titan: An Interview With Carrie Anderson", "description": "Since she was a little girl, Carrie Anderson has wanted to be an astronomer. Now, as a space scientist at NASA Goddard Space Flight Center, Carrie studies the atmosphere on Titan, one of Saturn's moons and the second largest moon in the solar system. Titan is also a model for what the early Earth might have been like. To learn about Titan, she uses an instrument on the Cassini spacecraft called CIRS.For complete transcript, click here. || carrie_thumbnail1.png (1259x713) [678.5 KB] || carrie_thumbnail1_web.jpg (320x181) [35.5 KB] || carrie_thumbnail1_thm.png (80x40) [18.2 KB] || carrie_thumbnail1_web_searchweb.jpg (320x180) [71.6 KB] || G2010-138_Carrie_Anderson_Profile_appletv.m4v (960x540) [92.5 MB] || G2010-138_Carrie_Anderson_Profile.wmv (1280x720) [82.6 MB] || G2010-138_Carrie_Anderson_Profile_youtube_hq.mov (1280x720) [99.6 MB] || G2010-138_Carrie_Anderson_Profile_appletv.webmhd.webm (960x540) [32.3 MB] || G2010-138_Carrie_Anderson_Profile.mov (640x360) [2.6 GB] || G2010-138_Carrie_Anderson_Profile_ipod_lg.m4v (640x360) [31.3 MB] || GSFC_20101216_Titan_m10705_Anderson.en_US.srt [4.0 KB] || GSFC_20101216_Titan_m10705_Anderson.en_US.vtt [3.9 KB] || G2010-138_Carrie_Anderson_Profile_ipod_sm.mp4 (320x240) [15.6 MB] || G2010-138_Carrie_Anderson_Profile_SVS.mpg (512x288) [24.0 MB] || ", "hits": 36 } ] }