{ "count": 82, "next": null, "previous": null, "results": [ { "id": 14916, "url": "https://svs.gsfc.nasa.gov/14916/", "result_type": "Produced Video", "release_date": "2025-12-08T09:30:00-05:00", "title": "Black Hole Eats Star: The Longest GRB Ever Seen", "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ", "hits": 610 }, { "id": 14886, "url": "https://svs.gsfc.nasa.gov/14886/", "result_type": "Produced Video", "release_date": "2025-08-22T11:00:00-04:00", "title": "Artemis Science: Exploring the Moon’s South Pole", "description": "By sending astronauts to collect samples from the Moon’s South Pole, NASA’s Artemis missions may uncover clues to the formation of the solar system.Complete transcript available.Universal Production Music: “Transitions” by Harry Gregson Williams [BMI] and Ben Andrew [PRS]; “Love on the Moon” by Sebastian Barnaby Robertson [BMI] and Yaacov Kobi Hokima [BMI]Watch this video on the NASA Goddard YouTube channel. || Artemis_Sci_Young_S_Pole_Preview.png (1920x1080) [1.5 MB] || Artemis_Sci_Young_S_Pole_Preview.jpg (1920x1080) [721.6 KB] || Artemis_Sci_Young_S_Pole_Preview_print.jpg (1024x576) [139.2 KB] || Artemis_Sci_Young_S_Pole_Preview_searchweb.png (320x180) [84.1 KB] || Artemis_Sci_Young_S_Pole_Preview_thm.png (80x40) [6.7 KB] || 14886_Artemis_Sci_Young_SPole_720.mp4 (1280x720) [37.3 MB] || 14886_Artemis_Sci_Young_SPole_1080.mp4 (1920x1080) [208.1 MB] || ArtemisSciYoungSPoleCaptions.en_US.srt [4.0 KB] || ArtemisSciYoungSPoleCaptions.en_US.vtt [3.8 KB] || 14886_Artemis_Sci_Young_SPole_4K_Small.mp4 (3840x2160) [155.7 MB] || 14886_Artemis_Sci_Young_SPole_4K.mp4 (3840x2160) [1.3 GB] || 14886_Artemis_Sci_Young_SPole_ProRes.mov (3840x2160) [7.4 GB] || ", "hits": 509 }, { "id": 14690, "url": "https://svs.gsfc.nasa.gov/14690/", "result_type": "Produced Video", "release_date": "2024-09-23T14:00:00-04:00", "title": "Ten Years at Mars with NASA’s MAVEN Mission", "description": "During its first decade at Mars, MAVEN has helped to explain how the Red Planet evolved from warm and wet into the cold, dry world we see today. Complete transcript available.Universal Production Music: “Executive Deceit” by Samuel Karl Bohn [PRS], Chalk Music [PRS]; “Quasar” by Ross Stephen Gilmartin [PRS], Chappell Recorded Music Library Ltd [PRS]; “Modular Odyssey” and “Synthology” by Laetitia Frenod [SACEM], Koka Media [SACEM]Watch this video on the NASA Goddard YouTube channel. || MAVEN-10th-Anniversary-Preview_print.jpg (1024x576) [160.7 KB] || MAVEN-10th-Anniversary-Preview.jpg (1280x720) [622.5 KB] || MAVEN-10th-Anniversary-Preview.png (1280x720) [1.2 MB] || MAVEN-10th-Anniversary-Preview_searchweb.png (320x180) [80.6 KB] || MAVEN-10th-Anniversary-Preview_thm.png (80x40) [6.3 KB] || 14690_MAVEN_10th_Anniversary_720.mp4 (1280x720) [92.2 MB] || 14690_MAVEN_10th_Anniversary_1080.mp4 (1920x1080) [516.6 MB] || Maven10thAnniversaryCaptionsV3.en_US.srt [8.9 KB] || Maven10thAnniversaryCaptionsV3.en_US.vtt [8.5 KB] || 14690_MAVEN_10th_Anniversary_4K.mp4 (3840x2160) [6.3 GB] || 14690_MAVEN_10th_Anniversary_ProRes.mov (3840x2160) [36.5 GB] || ", "hits": 91 }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "result_type": "Produced Video", "release_date": "2022-04-06T13:00:00-04:00", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "hits": 70 }, { "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": 144 }, { "id": 13663, "url": "https://svs.gsfc.nasa.gov/13663/", "result_type": "Produced Video", "release_date": "2020-08-11T11:00:00-04:00", "title": "TESS Completes Its Primary Mission", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) has completed its two-year primary mission and is continuing its search for new worlds. Watch to review some of TESS’s most interesting discoveries so far.Credit: NASA’s Goddard Space Flight CenterMusic: \"Drive to Succeed\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_2_Still.jpg (1920x1080) [661.7 KB] || TESS_2_Still_print.jpg (1024x576) [187.0 KB] || 13663_TESS_2nd_Anniversary_Highlights.mp4 (1920x1080) [215.9 MB] || 13663_TESS_2nd_Anniversary_Highlights_Best.mp4 (1920x1080) [611.5 MB] || 13663_TESS_2nd_Anniversary_Highlights_ProRes_1920x1080_2997.mov (1920x1080) [2.7 GB] || 13663_TESS_2nd_Anniversary_Highlights.webm (1920x1080) [23.4 MB] || TESS_2nd_Anniversary_Highlights_SRT_Captions.en_US.srt [4.0 KB] || TESS_2nd_Anniversary_Highlights_SRT_Captions.en_US.vtt [4.0 KB] || ", "hits": 92 }, { "id": 13665, "url": "https://svs.gsfc.nasa.gov/13665/", "result_type": "Produced Video", "release_date": "2020-07-16T10:00:00-04:00", "title": "The Webb Telescope is Folded For Final Testing", "description": "NASA’s James Webb Space Telescope is folded and ready for its final suite of testing. || Cover_Image_Text.jpg (1920x1080) [860.6 KB] || Cover_Image_Text_print.jpg (1024x576) [382.7 KB] || Cover_Image_Text_searchweb.png (320x180) [113.4 KB] || Cover_Image_Text_web.png (320x180) [113.4 KB] || Cover_Image_Text_thm.png (80x40) [24.0 KB] || WebbFoldsforFinalTestingProres.mov (1920x1080) [1.0 GB] || WebbFoldsforFinalTesting.mp4 (1920x1080) [75.9 MB] || WebbFoldsforFinalTesting.webm (1920x1080) [8.1 MB] || WebbFoldsforFinalTesting-closecap1.en_US.srt [802 bytes] || WebbFoldsforFinalTesting-closecap1.en_US.vtt [815 bytes] || ", "hits": 44 }, { "id": 13635, "url": "https://svs.gsfc.nasa.gov/13635/", "result_type": "Produced Video", "release_date": "2020-06-30T10:50:00-04:00", "title": "NASA’s TESS Provides New Insights Into an Ultrahot World", "description": "Explore KELT-9 b, one of the hottest planets known. Observations from NASA's Transiting Exoplanet Survey Satellite (TESS) have revealed new details about the planet’s environment. The planet follows a close, polar orbit around a squashed star with different surface temperatures, factors that make peculiar seasons for KELT-9 b. Credit: NASA's Goddard Space Flight CenterMusic: \"Migrating Species\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Kelt9b_Still.jpg (1920x1080) [711.8 KB] || Kelt9b_Still_searchweb.png (320x180) [77.8 KB] || Kelt9b_Still_thm.png (80x40) [6.0 KB] || 13635_KELT-9b_1080.mp4 (1920x1080) [146.6 MB] || 13635_KELT-9b_Best_1080.mp4 (1920x1080) [418.4 MB] || 13635_KELT-9b_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || 13635_KELT-9b_1080.webm (1920x1080) [15.9 MB] || 13635_KELT-9b_SRT_Captions.en_US.srt [2.7 KB] || 13635_KELT-9b_SRT_Captions.en_US.vtt [2.7 KB] || ", "hits": 88 }, { "id": 20307, "url": "https://svs.gsfc.nasa.gov/20307/", "result_type": "Animation", "release_date": "2020-01-28T11:00:00-05:00", "title": "NASA's Conceptual Image Lab 2020 Demo Reel", "description": "Conceptual Image Lab Demo Reel with Text discriptions. || CILDemoReel2020Text4K.00420_print.jpg (1024x576) [33.3 KB] || CILDemoReel2020Text4K.00420_searchweb.png (320x180) [51.3 KB] || CILDemoReel2020Text4K.00420_thm.png (80x40) [4.7 KB] || CILDemoReel2020Text1080.mov (1920x1080) [362.8 MB] || CILDemoReel2020Text4K.webm (3840x2160) [87.7 MB] || CILDemoReel2020Text4K.mov (3840x2160) [867.6 MB] || ", "hits": 54 }, { "id": 13527, "url": "https://svs.gsfc.nasa.gov/13527/", "result_type": "Produced Video", "release_date": "2020-01-27T12:00:00-05:00", "title": "New Mission Will Take First Peek at Sun’s Poles", "description": "A new spacecraft is journeying to the Sun to snap the first pictures of the Sun’s north and south poles. Solar Orbiter, a collaboration between ESA (the European Space Agency) and NASA will have its first opportunity to launch from Cape Canaveral on Feb. 7, 2020, at 11:15 p.m. EST. Launching on a United Launch Alliance Atlas V rocket, the spacecraft will use Venus’ and Earth’s gravity to swing itself out of the ecliptic plane — the swath of space, roughly aligned with the Sun’s equator, where all planets orbit. From there, Solar Orbiter's bird’s eye view will give it the first-ever look at the Sun's poles.Read more: https://www.nasa.gov/feature/goddard/2020/new-mission-will-take-first-peek-at-sun-s-poles || ", "hits": 70 }, { "id": 13275, "url": "https://svs.gsfc.nasa.gov/13275/", "result_type": "Produced Video", "release_date": "2019-08-07T11:30:00-04:00", "title": "How NASA Will Protect Astronauts From Space Radiation", "description": "Today, the Apollo-era flares serve as a reminder of the threat of radiation exposure for technology and astronauts in space. Understanding and predicting solar eruptions is crucial for safe space exploration. Almost 50 years since those 1972 storms, the data, technology and resources available to NASA have improved, enabling advancements towards space weather forecasts and astronaut protection — key to NASA’s Artemis program to return astronauts to the Moon.", "hits": 285 }, { "id": 13238, "url": "https://svs.gsfc.nasa.gov/13238/", "result_type": "Produced Video", "release_date": "2019-07-25T09:50:00-04:00", "title": "Highlights From TESS's First Year", "description": "Here are highlights from TESS's first year of science operations. All exoplanet animations are illustrations.Credit: NASA's Goddard Space Flight CenterMusic: \"Elapsing Time\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_First_Year_Still.jpg (1920x1080) [515.9 KB] || TESS_First_Year_Still_print.jpg (1024x576) [182.2 KB] || TESS_First_Year_Still_searchweb.png (320x180) [70.7 KB] || TESS_First_Year_Still_thm.png (80x40) [5.3 KB] || 13238_TESS_First_Year_ProRes_1920x1080.mov (1920x1080) [2.4 GB] || 13238_TESS_First_Year_Best.mp4 (1920x1080) [483.9 MB] || 13238_TESS_First_Year_Good.mp4 (1920x1080) [184.7 MB] || 13238_TESS_First_Year_ProRes_1920x1080.webm (1920x1080) [20.0 MB] || TESS_First_Year_SRT_Captions.en_US.srt [3.7 KB] || TESS_First_Year_SRT_Captions.en_US.vtt [3.7 KB] || ", "hits": 68 }, { "id": 12589, "url": "https://svs.gsfc.nasa.gov/12589/", "result_type": "Produced Video", "release_date": "2019-06-10T10:00:00-04:00", "title": "Getting SET - The Mission to Protect Satellites from Radiation", "description": "SET is the latest addition to NASA’s fleet of heliophysics observatories. NASA heliophysics missions study a vast interconnected system from the Sun to the space surrounding Earth and other planets, and to the farthest limits of the Sun’s constantly flowing stream of solar wind. SET’s observations provide key information on the Sun’s effects on our spacecraft, enabling further exploration of space. Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credits: Night Moves by Max Cameron Concors, Wavelengths by Max Cameron Concors, and Alpha Helix by David Travis Edwards, Robert Anthony Navarro, Matthew St Laurent, and Christian Telford. End tag music credits: Radiant Energy by Chris Constantinou, Paul Frazer || SETThumb.jpg (1920x1080) [191.0 KB] || SETThumb_searchweb.png (320x180) [79.4 KB] || SETThumb_thm.png (80x40) [6.2 KB] || 12589_SET.V3.webm (1920x1080) [31.1 MB] || captions.en_US.srt [4.4 KB] || captions.en_US.vtt [4.2 KB] || 12589_SET.en_US.srt [4.2 KB] || 12589_SET.en_US.vtt [4.2 KB] || 12589_SET.V3.mov (1920x1080) [5.5 GB] || 12589_SET.V3.mp4 (1920x1080) [206.9 MB] || 12589_SET.V3FB1080.mp4 (1920x1080) [241.6 MB] || ", "hits": 45 }, { "id": 13078, "url": "https://svs.gsfc.nasa.gov/13078/", "result_type": "Produced Video", "release_date": "2019-04-15T11:00:00-04:00", "title": "Water Released from Moon During Meteor Showers", "description": "Data from the LADEE spacecraft reveal that the lunar surface is periodically releasing water.Music provided by Killer Tracks: Virtual MemoryComplete transcript available. Watch this video on the NASA Goddard YouTube channel. || LADEE_Moon_Earth_Preview_V4_print.jpg (1024x576) [181.9 KB] || LADEE_Moon_Earth_Preview_V4.jpg (1280x720) [281.6 KB] || LADEE_Moon_Earth_Preview_V4_searchweb.png (180x320) [46.5 KB] || LADEE_Moon_Earth_Preview_V4_thm.png (80x40) [3.9 KB] || TWITTER_720_13078_LADEE_Water_Short_MASTER_twitter_720.mp4 (1280x720) [21.1 MB] || 13078_LADEE_Water_Short_MASTER.webm (960x540) [48.9 MB] || YOUTUBE_1080_13078_LADEE_Water_Short_MASTER_youtube_1080.mp4 (1920x1080) [176.0 MB] || FACEBOOK_720_13078_LADEE_Water_Short_MASTER_facebook_720.mp4 (1280x720) [134.7 MB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.srt [2.6 KB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.vtt [2.6 KB] || 13078_LADEE_Water_Short_MASTER.mp4 (3840x2160) [940.5 MB] || 13078_LADEE_Water_Short_MASTER.mov (3840x2160) [5.5 GB] || ", "hits": 66 }, { "id": 20278, "url": "https://svs.gsfc.nasa.gov/20278/", "result_type": "Animation", "release_date": "2019-04-15T11:00:00-04:00", "title": "Water Released from Moon During Meteor Showers: Animations", "description": "Scientists have discovered that water is being released from the moon during meteor showers. When a speck of comet debris strikes the moon it vaporizes on impact, creating a shock wave in the lunar soil. For a sufficiently large impactor, this shock wave can breach the soil’s dry upper layer and release water molecules from a hydrated layer below. The LADEE spacecraft detects these water molecules as they enter the tenuous lunar atmosphere. || ", "hits": 233 }, { "id": 12941, "url": "https://svs.gsfc.nasa.gov/12941/", "result_type": "Produced Video", "release_date": "2018-11-14T13:50:00-05:00", "title": "Massive Crater Discovered under Greenland Ice", "description": "It took the combined efforts of an international team of scientists to unravel the mystery of the Hiawatha crater. This video shows how that discovery came together. Complete transcript available. || combined_cut_8.0_1.00540_print.jpg (1024x576) [126.7 KB] || combined_cut_8.0_1.00540_searchweb.png (320x180) [92.1 KB] || combined_cut_8.0_1.00540_web.png (320x180) [92.1 KB] || combined_cut_8.0_1.00540_thm.png (80x40) [6.2 KB] || combined_cut_8.0_1.webm (1920x1080) [34.6 MB] || Greenland_crater_discovery_final_720.mov (1280x720) [232.3 MB] || Greenland_crater_discovery_final_1080.mov (1920x1080) [329.3 MB] || Greenland_crater_discovery.en_US.srt [5.5 KB] || Greenland_crater_discovery.en_US.vtt [5.5 KB] || Greenland_meteor_crater_1920.mp4 (1920x1080) [2.3 GB] || Greenland_crater_discovery_final.mp4 (3840x2160) [2.8 GB] || ", "hits": 77 }, { "id": 13042, "url": "https://svs.gsfc.nasa.gov/13042/", "result_type": "Produced Video", "release_date": "2018-11-08T13:00:00-05:00", "title": "NASA's Fermi Mission Shows How Luck Favors the Prepared", "description": "Explore how more than a century of scientific progress with gravitational waves, gamma rays and neutrinos has helped bring about the age of multimessenger astronomy. Music: \"Family Tree,\" \"The Archives\" and \"Beyond Truth,\" all from Killer Tracks.Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Luck_Timeline_Still_print.jpg (1024x576) [140.7 KB] || Luck_Timeline_Still.jpg (3840x2160) [1.1 MB] || Luck_Timeline_Still_searchweb.png (320x180) [78.5 KB] || Luck_Timeline_Still_thm.png (80x40) [7.4 KB] || 13042_LuckFavorsThePrepared_1080p.mov (1920x1080) [550.2 MB] || 13042_LuckFavorsThePrepared_1080.mp4 (1920x1080) [373.6 MB] || 13042_LuckFavorsThePrepared_1080.m4v (1920x1080) [188.4 MB] || 13042_LuckFavorsThePrepared_1080p.webm (1920x1080) [39.3 MB] || 13042_LuckFavorsThePrepared_ProRes_3840x2160_2997.mov (3840x2160) [19.8 GB] || 13042_LuckFavorsThePrepared_2160.mp4 (3840x2160) [1.1 GB] || 13042_LuckFavorsThePrepared_4K.mov (3840x2160) [715.2 MB] || LuckFavorsThePrepared_SRT_Captions.en_US.srt [6.5 KB] || LuckFavorsThePrepared_SRT_Captions.en_US.vtt [6.3 KB] || ", "hits": 190 }, { "id": 20285, "url": "https://svs.gsfc.nasa.gov/20285/", "result_type": "Animation", "release_date": "2018-10-24T00:00:00-04:00", "title": "Laser Communications Relay Demonstration (LCRD) Overview Video and Resources", "description": "Laser Communications Relay Demonstration Overview VideoMusic Credit: Universal Production MusicTrack 1: Time Shift EqualibriumTrack 2: Frames of MotionTrack 3: Inducing Waves || 20285_LCRD_Logo_2021.png (1674x939) [1.2 MB] || 20285_LCRD_Overview_2021_lowres.mp4 (1280x720) [35.5 MB] || 20285_LCRD_Overview_2021.mp4 (1920x1080) [202.4 MB] || 20285_LCRD_Overview_2021.mov (1920x1080) [3.5 GB] || 20285_LCRD_Overview_2021.webm (1920x1080) [18.2 MB] || 20285_LCRD_Overview_2021.en_US.srt [3.1 KB] || 20285_LCRD_Overview_2021.en_US.vtt [3.0 KB] || ", "hits": 130 }, { "id": 13001, "url": "https://svs.gsfc.nasa.gov/13001/", "result_type": "Produced Video", "release_date": "2018-07-30T11:50:00-04:00", "title": "Parker Solar Probe", "description": "NASA's mission to touch the Sun begins its journey in 2018 || 01_Cover_forStory.png (1280x720) [920.1 KB] || 01_Cover_forStory_print.jpg (1024x576) [74.5 KB] || 01_Cover_forStory_thm.png (80x40) [5.2 KB] || 01_Cover_forStory_searchweb.png (320x180) [71.7 KB] || ", "hits": 101 }, { "id": 12978, "url": "https://svs.gsfc.nasa.gov/12978/", "result_type": "Produced Video", "release_date": "2018-07-20T13:00:00-04:00", "title": "Parker Solar Probe--Mission Overview", "description": "Parker Solar Probe will swoop to within 4 million miles of the sun's surface, facing heat and radiation like no spacecraft before it. Launching in 2018, Parker Solar Probe will provide new data on solar activity and make critical contributions to our ability to forecast major space-weather events that impact life on Earth.In order to unlock the mysteries of the corona, but also to protect a society that is increasingly dependent on technology from the threats of space weather, we will send Parker Solar Probe to touch the Sun.In 2017, the mission was renamed for Eugene Parker, the S. Chandrasekhar Distinguished Service Professor Emeritus, Department of Astronomy and Astrophysics at the University of Chicago. In the 1950s, Parker proposed a number of concepts about how stars—including our Sun—give off energy. He called this cascade of energy the solar wind, and he described an entire complex system of plasmas, magnetic fields, and energetic particles that make up this phenomenon. Parker also theorized an explanation for the superheated solar atmosphere, the corona, which is – contrary to what was expected by physics laws -- hotter than the surface of the sun itself. This is the first NASA mission that has been named for a living individual. || a012978_ParkerThumbnail_print.jpg (1024x576) [115.8 KB] || a012978_ParkerThumbnail.png (2327x1311) [5.5 MB] || a012978_ParkerThumbnail_thm.png (80x40) [6.6 KB] || a012978_ParkerThumbnail_searchweb.png (320x180) [83.0 KB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_twitter_720.mp4 (1920x1080) [58.8 MB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_youtube_1080.webm (1920x1080) [103.7 MB] || 12978_PSP_Overview_MASTER_appletv_subtitles.m4v (1280x720) [151.8 MB] || 12978_PSP_Overview_MASTER_appletv.m4v (1280x720) [151.7 MB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_large_mp4.mp4 (1920x1080) [261.7 MB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_youtube_720.mp4 (1920x1080) [330.9 MB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_youtube_1080.mp4 (1920x1080) [444.0 MB] || PSP_CC.en_US.srt [5.0 KB] || PSP_CC.en_US.vtt [5.0 KB] || 12978_PSP_Overview_MASTER_ipod_sm.mp4 (320x240) [46.0 MB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version_lowres.mp4 (480x272) [34.8 MB] || CH28_12978_PSP_Overview_MASTER_ch28.mov (1280x720) [2.3 GB] || SVS_12978_PSP_OVERVIEW_PKG_FINAL_Version.mov (1920x1080) [6.8 GB] || ", "hits": 146 }, { "id": 13003, "url": "https://svs.gsfc.nasa.gov/13003/", "result_type": "Produced Video", "release_date": "2018-07-20T12:30:00-04:00", "title": "Parker Solar Probe Science Briefing - Visual Resources", "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ", "hits": 33 }, { "id": 12867, "url": "https://svs.gsfc.nasa.gov/12867/", "result_type": "Produced Video", "release_date": "2018-07-19T15:00:00-04:00", "title": "Why Won't it Melt? How NASA's Solar Probe will Survive the Sun", "description": "Music credit: Cheeky Chappy [Main Track] by Jimmy Kaleth, Ross Andrew McLean from www.killertracks.com This music requires a license for use.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || meltthumb.jpg (1920x1080) [311.2 KB] || meltthumb_searchweb.png (320x180) [76.6 KB] || meltthumb_thm.png (80x40) [5.4 KB] || 12867WhyWontItMeltV8.mov (1920x1080) [5.4 GB] || 12867WhyWontItMeltV8.webm (1920x1080) [23.3 MB] || 12867WhyWontItMeltV8_appletv.m4v (1280x720) [148.8 MB] || 12867WhyWontItMeltV8_youtube_1080.mp4 (1920x1080) [443.5 MB] || 12867WhyWontItMeltV8_youtube_hq.mov (1920x1080) [1.3 GB] || 12867WhyWontItMeltV8_appletv_subtitles.m4v (1280x720) [148.9 MB] || 12867WhyWontItMeltV8.en_US.srt [4.2 KB] || 12867WhyWontItMeltV8.en_US.vtt [4.2 KB] || 12867WhyWontItMeltV8_ipod_sm.mp4 (320x240) [38.2 MB] || ", "hits": 33 }, { "id": 12949, "url": "https://svs.gsfc.nasa.gov/12949/", "result_type": "Produced Video", "release_date": "2018-07-02T13:00:00-04:00", "title": "Star Collision", "description": "Light bursts from the collision of two neutron stars. || Neutron_Star_Merger_Still_1_1024x576.jpg (1024x576) [148.9 KB] || Neutron_Star_Merger_Still_1.jpg (3840x2160) [2.4 MB] || Neutron_Star_Merger_Still_1_searchweb.png (320x180) [88.4 KB] || Neutron_Star_Merger_Still_1_thm.png (80x40) [7.3 KB] || ", "hits": 621 }, { "id": 12967, "url": "https://svs.gsfc.nasa.gov/12967/", "result_type": "Produced Video", "release_date": "2018-06-07T13:00:00-04:00", "title": "Ancient Organics Discovered on Mars - Broadcast Graphics", "description": "NASA-TV graphics illustrating Curiosity's findings on Mars, broadcast on June 7, 2018 from Goddard Space Flight Center. All clips are formatted in 1280x720 or higher resolution. Learn more about this discovery. || ", "hits": 274 }, { "id": 12901, "url": "https://svs.gsfc.nasa.gov/12901/", "result_type": "Produced Video", "release_date": "2018-05-09T13:00:00-04:00", "title": "NASA Spacecraft Finds New Magnetic Process in Turbulent Space", "description": "Though close to home, the space immediately around Earth is full of hidden secrets and invisible processes. In a new discovery reported in the journal Nature, scientists working with NASA’s Magnetospheric Multiscale spacecraft — MMS — have uncovered a new type of magnetic event in our near-Earth environment by using an innovative technique to squeeze extra information out of the data.Magnetic reconnection is one of the most important processes in the space — filled with charged particles known as plasma — around Earth. This fundamental process dissipates magnetic energy and propels charged particles, both of which contribute to a dynamic space weather system that scientists want to better understand, and even someday predict, as we do terrestrial weather. Reconnection occurs when crossed magnetic field lines snap, explosively flinging away nearby particles at high speeds. The new discovery found reconnection where it has never been seen before — in turbulent plasma. || ", "hits": 83 }, { "id": 12884, "url": "https://svs.gsfc.nasa.gov/12884/", "result_type": "Produced Video", "release_date": "2018-04-03T12:00:00-04:00", "title": "TESS Shorts", "description": "The Unique Orbit of NASA’s Newest Planet HunterNASA's Transiting Exoplanet Survey Satellite - TESS will fly in an orbit that completes two circuits around the Earth every time the Moon orbits. This special orbit will allow TESS’s cameras to monitor each patch of sky continuously from nearly a month at a time. To get into this orbit, TESS will make a series of loops culminating in a lunar gravitational-assist, which will give it the push it needs. TESS will reach its orbit about 60 days after launch.Music: \"Drive to Succeed\" from Killer TracksComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || TESS_Orbit_Still_print.jpg (1024x576) [69.4 KB] || TESS_Orbit_Still.jpg (3840x2160) [364.7 KB] || TESS_Orbit_Still_searchweb.png (320x180) [12.1 KB] || TESS_Orbit_Still_thm.png (80x40) [2.1 KB] || 12884_TESS_Orbit_Final_1080.mp4 (1920x1080) [92.9 MB] || 12884_TESS_Orbit_1080p.webm (1920x1080) [10.6 MB] || 12884_TESS_Orbit_1080p.mov (1920x1080) [301.8 MB] || 12884_TESS_Orbit_Final_4k.mp4 (3840x2160) [95.2 MB] || TESS_Orbit_SRT_Captions.en_US.srt [1.6 KB] || TESS_Orbit_SRT_Captions.en_US.vtt [1.6 KB] || 12884_TESS_Orbit_4K.mov (3840x2160) [690.3 MB] || 12884_TESS_Orbit_ProRes_3840x2160_2997.mov (3840x2160) [4.3 GB] || ", "hits": 200 }, { "id": 12618, "url": "https://svs.gsfc.nasa.gov/12618/", "result_type": "Produced Video", "release_date": "2018-04-02T12:00:00-04:00", "title": "How Plasma Transports Energy", "description": "For the first time, NASA scientists see how energy is transported in a plasma. || Story_Cover_AlfvenWaveParticles.Kinetic.MediumGyro.vzAlfvenDG4_staticXclose_inertial.HD1080i.0200_print.jpg (1024x576) [142.6 KB] || Story_Cover_AlfvenWaveParticles.Kinetic.MediumGyro.vzAlfvenDG4_staticXclose_inertial.HD1080i.0200_print_print.jpg (1024x576) [139.9 KB] || Story_Cover_AlfvenWaveParticles.Kinetic.MediumGyro.vzAlfvenDG4_staticXclose_inertial.HD1080i.0200_print_searchweb.png (320x180) [84.0 KB] || Story_Cover_AlfvenWaveParticles.Kinetic.MediumGyro.vzAlfvenDG4_staticXclose_inertial.HD1080i.0200_print_thm.png (80x40) [6.2 KB] || ", "hits": 119 }, { "id": 12850, "url": "https://svs.gsfc.nasa.gov/12850/", "result_type": "Produced Video", "release_date": "2018-03-28T13:00:00-04:00", "title": "NASA's New Planet Hunter: TESS", "description": "Watch an overview of the TESS mission.Music: \"Drive to Succeed\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Still_B1_00812_print.jpg (1024x576) [56.9 KB] || TESS_Still_B1_00812.png (3840x2160) [5.6 MB] || TESS_Still_B1_00812_searchweb.png (320x180) [53.1 KB] || TESS_Still_B1_00812_thm.png (80x40) [4.8 KB] || 12850_TESS_Overview_1080.webm (1920x1080) [34.9 MB] || 12850_TESS_Overview_1080.m4v (1920x1080) [321.6 MB] || TESS_Overview_SRT_Captions.en_US.srt [5.8 KB] || TESS_Overview_SRT_Captions.en_US.vtt [5.8 KB] || 12850_TESS_Overview_4K_Good_H264.mov (3840x2160) [931.4 MB] || 12850_TESS_Overview_4K_Best_H264.m4v (3840x2160) [1.5 GB] || 12850_TESS_Overview.mp4 (3840x2160) [1.6 GB] || 12850_TESS_Overview_YOUTUBE.mov (3840x2160) [3.2 GB] || 12850_TESS_Overview_Prores_3840x2160_2997.mov (3840x2160) [17.2 GB] || ", "hits": 208 }, { "id": 12887, "url": "https://svs.gsfc.nasa.gov/12887/", "result_type": "Produced Video", "release_date": "2018-03-28T12:45:00-04:00", "title": "TESS Coverage Animations", "description": "Animation showing the TESS spacecraft and the coverage of its four cameras. Each camera covers a 24 degrees-square patch of sky and the four cameras are arranged in a vertical strip called an observation sector. || TESS_FOVAnimation_SH1_Text_frame.1687.png (1920x1080) [3.1 MB] || TESS_FOVAnimation_SH1_Text_frame.1687_print.jpg (1024x576) [106.2 KB] || TESS_FOVAnimation_SH1_4K_Text_frame.1687.png (3840x2160) [12.0 MB] || TESS_FOVAnimation_SH1_Text_frame.1687_searchweb.png (320x180) [75.3 KB] || TESS_FOVAnimation_SH1_Text_frame.1687_thm.png (80x40) [4.9 KB] || TESS_FOVAnimation_SH1_Final_v01-HD_1080p.mov (1920x1080) [86.8 MB] || TESS_FOVAnimation_SH1_Final_v01.webm (1920x1080) [4.2 MB] || FOV (3840x2160) [0 Item(s)] || TESS_FOVAnimation_SH1_Final_4K_Text_v01_H264.mov (3840x2160) [133.1 MB] || TESS_FOVAnimation_SH1_Final_v01.mov (1920x1080) [2.0 GB] || TESS_FOVAnimation_SH1_Final_4K_Text_v01.mov (3840x2160) [8.0 GB] || ", "hits": 168 }, { "id": 12880, "url": "https://svs.gsfc.nasa.gov/12880/", "result_type": "Produced Video", "release_date": "2018-03-05T00:00:00-05:00", "title": "Cosmic Designs and The Planets", "description": "Greetings and welcome to “Cosmic Designs” a performance by the National Philharmonic presented in partnership with NASA’s Goddard Space Flight Center.“Cosmic Designs” is a voyage that blends together science and art. The pursuit of knowledge and the creative drive for artistic expression are inherent to the human condition. The melding of NASA imagery and symphonic music we present here showcases the imagination that underpins both and highlights how inspiring the combination can be. || CD_Intro_Image_print.jpg (1024x567) [135.2 KB] || CD_Intro_Image.png (2918x1618) [5.8 MB] || CD_Intro_Image_searchweb.png (320x180) [103.7 KB] || CD_Intro_Image_web.png (320x177) [101.8 KB] || CD_Intro_Image_thm.png (80x40) [7.6 KB] || 1.CosmicDesigns_Title_1080.mov (1920x1080) [1.0 GB] || 1.CosmicDesigns_Title_1080.mp4 (1920x1080) [35.9 MB] || 1.CosmicDesigns_Title_1080.webm (1920x1080) [3.3 MB] || 1.CosmicDesigns_Title_4K.mov (3840x2160) [4.3 GB] || 1.CosmicDesigns_Title_4K.mp4 (3840x2160) [55.1 MB] || ", "hits": 203 }, { "id": 12870, "url": "https://svs.gsfc.nasa.gov/12870/", "result_type": "Produced Video", "release_date": "2018-02-26T08:00:00-05:00", "title": "GOES-S in Space Covers the Western US", "description": "GOES-S is the latest in a series of new weather satellites, a powerful asset in the nation's fleet. It is part of of the Geostationary Operational Environmental Satellite (GOES) – R Series. These are the nation’s most advanced in terms of geostationary weather satellites. The GOES-R Series significantly improves the detection and observation of environmental phenomena that directly affect public safety, protection of property and our nation’s economic health and prosperity.The satellites provide advanced imaging with increased spatial resolution and faster coverage for more accurate forecasts, real-time mapping of lightning activity, and improved monitoring of solar activity and space weather.The GOES-R Series is a four-satellite program (GOES-R/S/T/U) that will extend the availability of the operational GOES satellite system through 2036. || GOESR_Conceptual_3_V2_print.jpg (1024x576) [129.2 KB] || GOES-S_FINAL_DRAFT_twitter_720.00537_searchweb.png (320x180) [33.2 KB] || GOES-S_FINAL_DRAFT_twitter_720.00537_thm.png (80x40) [3.6 KB] || GOES-S_FINAL_DRAFT.mov (1920x1080) [4.7 GB] || GOES-S_FINAL_DRAFT.webm (960x540) [142.6 MB] || GOES-S_FINAL_DRAFT_facebook_720.mp4 (1280x720) [424.6 MB] || GOES-S_FINAL_DRAFT_twitter_720.mp4 (1280x720) [86.7 MB] || GOES-S_FINAL_DRAFT_youtube_1080.mp4 (1920x1080) [580.4 MB] || GOES-S_FINAL_DRAFT_youtube_720.mp4 (1280x720) [553.5 MB] || GOES-S_FINAL_DRAFT_twitter_720.webm (1280x720) [39.0 MB] || GOES-S_FINAL.en_US.srt [6.9 KB] || GOES-S_FINAL.en_US.vtt [6.9 KB] || ", "hits": 43 }, { "id": 12700, "url": "https://svs.gsfc.nasa.gov/12700/", "result_type": "Produced Video", "release_date": "2017-12-08T10:00:00-05:00", "title": "Can Data from Space Save Dolphins?", "description": "In an unprecedented collaboration between NASA’s Goddard Space Flight Center, the International Fund for Animal Welfare, and the Bureau of Ocean Energy Management, scientists from a cross-section of fields pooled massive data sets together to investigate the possible connection between space weather and marine mammal mass stranding events. Music credits: Long Travels - Boris Nonte, Gregg LehrmanSpiritual Migration - Giles Robert LambCrystal Sound Bath - James Alexander DormanThe Space Between - Max ConcorsInducing Waves - Ben Niblett, Jon CottonEnchanted - Gregg Lehrman, Boris Nonte, Daniel Louis WalterComplete transcript available.Watch this video on the NASA Goddard YouTube channel.Credit: NASA’s Goddard Space Flight Center/Genna Duberstein/Scott Wiessinger || StrandingsPosterFrameTextv03.jpg (3840x2160) [3.0 MB] || 12700_NASA_Data_and_Dolphins_ProRes_FINAL.mov (1920x1080) [8.1 GB] || 12700_NASA_Data_and_Dolphins_FINAL_youtube_hq.mov (1920x1080) [4.5 GB] || YOUTUBE_1080_12700_NASA_Data_and_Dolphins_FINAL_youtube_1080.mp4 (1920x1080) [1.1 GB] || 12700_NASA_Data_and_Dolphins_H264_FINAL.mp4 (1920x1080) [716.4 MB] || 12700_NASA_Data_and_Dolphins_FINAL_large.mp4 (1920x1080) [613.7 MB] || YOUTUBE_1080_12700_NASA_Data_and_Dolphins_FINAL_youtube_1080.webm (1920x1080) [66.9 MB] || 12700_data_and_dolphins.en_US.srt [11.6 KB] || 12700_data_and_dolphins.en_US.vtt [11.5 KB] || ", "hits": 41 }, { "id": 12740, "url": "https://svs.gsfc.nasa.gov/12740/", "result_type": "Produced Video", "release_date": "2017-10-16T10:00:00-04:00", "title": "Doomed Neutron Stars Create Blast of Light and Gravitational Waves", "description": "This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue). Credit: NASA's Goddard Space Flight Center/CI LabMusic: \"Exploding Skies\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Neutron_Star_Merger_Still_2_new_1080.png (1920x1080) [2.5 MB] || Neutron_Star_Merger_Still_2_new_1080.jpg (1920x1080) [167.3 KB] || Neutron_Star_Merger_Still_2_new_print.jpg (1024x576) [50.4 KB] || Neutron_Star_Merger_Still_2_new.png (3840x2160) [7.7 MB] || Neutron_Star_Merger_Still_2_new.jpg (3840x2160) [1.0 MB] || Neutron_Star_Merger_Still_2_new_thm.png (80x40) [4.4 KB] || Neutron_Star_Merger_Still_2_new_searchweb.png (320x180) [51.4 KB] || 12740_NS_Merger_Update_1080.m4v (1920x1080) [50.3 MB] || 12740_NS_Merger_Update_H264_1080.mp4 (1920x1080) [96.9 MB] || 12740_NS_Merger_Update_1080p.mov (1920x1080) [101.9 MB] || NS_Merger_SRT_Captions.en_US.srt [417 bytes] || NS_Merger_SRT_Captions.en_US.vtt [399 bytes] || 12740_NS_Merger_4k_Update.webm (3840x2160) [10.0 MB] || 12740_NS_Merger_4k_Update_H264.mp4 (3840x2160) [254.9 MB] || 12740_NS_Merger_4k_Update_H264.mov (3840x2160) [516.7 MB] || 12740_NS_Merger_4k_Update_ProRes_3840x2160_5994.mov (3840x2160) [5.1 GB] || 12740_NS_Merger_4k_Update_H264.hwshow [90 bytes] || ", "hits": 600 }, { "id": 12639, "url": "https://svs.gsfc.nasa.gov/12639/", "result_type": "Produced Video", "release_date": "2017-09-05T10:00:00-04:00", "title": "Where is the Edge of the Solar System?", "description": "Complete transcript available.Music credit: Dream Girl 3 by Yuri Sazonoff || EdgeofSolarSystem_ThumbnailOption2_print.jpg (1024x576) [252.4 KB] || EdgeofSolarSystem_ThumbnailOption2.png (3840x2160) [14.7 MB] || EdgeofSolarSystem_ThumbnailOption2_thm.png (80x40) [7.0 KB] || EdgeofSolarSystem_ThumbnailOption2_searchweb.png (320x180) [115.1 KB] || 12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_appletv.m4v (1280x720) [28.8 MB] || 12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_appletv_subtitles.m4v (1280x720) [28.8 MB] || YOUTUBE_1080_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_youtube_1080.webm (1920x1080) [7.2 MB] || TWITTER_720_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_twitter_720.mp4 (1280x720) [12.3 MB] || YOUTUBE_1080_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_youtube_1080.mp4 (1920x1080) [95.1 MB] || FACEBOOK_720_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_facebook_720.mp4 (1280x720) [70.5 MB] || YOUTUBE_720_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_youtube_720.mp4 (1280x720) [96.0 MB] || PRORES_B-ROLL_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_prores.mov (1280x720) [403.5 MB] || 12639_Edge_of_the_Solar_System.en_US.srt [810 bytes] || 12639_Edge_of_the_Solar_System.en_US.vtt [823 bytes] || YOUTUBE_4K_12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_youtube_4k.mp4 (3840x2160) [246.9 MB] || 12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_lowres.mp4 (480x272) [9.5 MB] || 12639_EdgeofSolarSystem_Final_24fps_v02_VX-718267_youtube_hq.mov (3840x2160) [1.8 GB] || 12639_EdgeofSolarSystem_Final_24fps_v02.mov (3840x2160) [3.0 GB] || 12639_EdgeofSolarSystem_Final_2997fps_v02.mov (3840x2160) [3.7 GB] || ", "hits": 576 }, { "id": 12676, "url": "https://svs.gsfc.nasa.gov/12676/", "result_type": "Produced Video", "release_date": "2017-08-11T00:00:00-04:00", "title": "Science Goals of the James Webb Space Telescope", "description": "Complete transcript available. || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.00385_print.jpg (1024x576) [108.8 KB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.00385_searchweb.png (180x320) [89.3 KB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.00385_thm.png (80x40) [7.1 KB] || 12676_-_Science_Goals_of_JWST_FINAL.mov (1920x1080) [4.3 GB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.mp4 (1920x1080) [326.7 MB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.webm (1920x1080) [36.4 MB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.en_US.srt [6.2 KB] || 12676_-_Science_Goals_of_the_James_Webb_Space_Telescope.en_US.vtt [6.2 KB] || ", "hits": 47 }, { "id": 12477, "url": "https://svs.gsfc.nasa.gov/12477/", "result_type": "Produced Video", "release_date": "2017-05-15T12:00:00-04:00", "title": "Marine Magnetism", "description": "A new method uses Earth's magnetic field to detect changes in the heat stored in the ocean. || TidalMagFL_frames_30fps.0272.png (1920x1080) [4.1 MB] || TidalMagFL_frames_30fps.0272_1024x576.jpg (1024x576) [183.8 KB] || TidalMagFL_frames_30fps.0272_1280x720.jpg (1280x720) [291.4 KB] || TidalMagFL_frames_30fps.0272_1024x576_print.jpg (1024x576) [183.2 KB] || TidalMagFL_frames_30fps.0272_thm.png (80x40) [5.8 KB] || TidalMagFL_frames_30fps.0272_1024x576_searchweb.png (320x180) [103.7 KB] || ", "hits": 48 }, { "id": 12479, "url": "https://svs.gsfc.nasa.gov/12479/", "result_type": "Produced Video", "release_date": "2017-02-11T11:58:00-05:00", "title": "NASM 2016: The Search For Life", "description": "Complete transcript available. || Thumbnail_print.jpg (1024x578) [142.3 KB] || Thumbnail.png (3348x1890) [8.3 MB] || Thumbnail_searchweb.png (320x180) [98.0 KB] || Thumbnail_web.png (320x180) [98.5 KB] || Thumbnail_thm.png (80x40) [7.3 KB] || The-Search-For-Life-NASM2016.mov (1920x1080) [52.0 GB] || APPLE_TV-The-Search-For-Life-NASM2016_appletv.m4v (1280x720) [1.0 GB] || NASA_TV-The-Search-For-Life-NASM2016.mpeg (1280x720) [6.8 GB] || The-Search-For-Life-NASM2016.webm (1920x1080) [233.9 MB] || NASMOnline.mp4 (1920x1080) [2.1 GB] || YOUTUBE_HQ-NASMOnline_youtube_hq.mov (1920x1080) [4.8 GB] || APPLE_TV-The-Search-For-Life-NASM2016_appletv_subtitles.m4v (1280x720) [1.0 GB] || NASMOnline.en_US.srt [38.3 KB] || NASMOnline.en_US.vtt [36.5 KB] || The-Search-For-Life-NASM2016_lowres.mp4 (480x272) [280.4 MB] || ", "hits": 18 }, { "id": 12450, "url": "https://svs.gsfc.nasa.gov/12450/", "result_type": "Produced Video", "release_date": "2016-12-12T18:30:00-05:00", "title": "Ocean Tides and Magnetic Fields", "description": "Seawater is an electrical conductor, and therefore interacts with the magnetic field. As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along.Because the salty water is a good, but not great, conductor, the interaction is relatively weak. Scientists at NASA Goddard Space Flight Center are developing improved methods to isolate the signal from ocean tides and use that information to determine the heat content of the ocean.Music: \"Memory Of A Lifetime\" by J Ehrlich [SESAC], Jean-Christophe Beck [BMI]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12450-Tidal-Magnetic-Animation-APR_large.00545_print.jpg (1024x576) [189.1 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_searchweb.png (320x180) [93.6 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_thm.png (80x40) [5.8 KB] || 12450-Tidal-Magnetic-Animation-APR.webm (960x540) [26.5 MB] || 12450-Tidal-Magnetic-Animation-APR_prores.mov (1280x720) [989.0 MB] || 12450-Tidal-Magnetic-Animation-APR_large.mp4 (1920x1080) [66.1 MB] || 12450-Tidal-Magnetic-Animation-APR_youtube_hq.mov (1920x1080) [1.0 GB] || 12450-Tidal-Magnetic-Animation-APR_appletv.m4v (1280x720) [32.1 MB] || 12450-Tidal-Magnetic-Animation-APR_appletv_subtitles.m4v (1280x720) [32.2 MB] || 1920x1080_16x9_30p (1920x1080) [128.0 KB] || 12450-Tidal-Magnetic-Animation.en_US.srt [1.4 KB] || 12450-Tidal-Magnetic-Animation.en_US.vtt [1.4 KB] || 12450-Tidal-Magnetic-Animation-APR_ipod_sm.mp4 (320x240) [11.5 MB] || ", "hits": 395 }, { "id": 20241, "url": "https://svs.gsfc.nasa.gov/20241/", "result_type": "Animation", "release_date": "2016-09-20T14:00:00-04:00", "title": "The Electromagnetic Spectrum", "description": "Animation depicting the electromagnetic spectrum and the different characteristics of each wavelength type. 4k resolution. || WFirst_ElectromagneticSpectrum.0830_print.jpg (1024x576) [228.7 KB] || WFirst_ElectromagneticSpectrum.0830.png (3840x2160) [13.8 MB] || WFirst_ElectromagneticSpectrum.0830_searchweb.png (320x180) [105.9 KB] || WFirst_ElectromagneticSpectrum.0830_thm.png (80x40) [7.1 KB] || WFirst_LightSpectrum_Final_H264_HD_1080p.mov (1920x1080) [150.2 MB] || WFirst_LightSpectrum_Final_H264_HD_1080p.webm (1920x1080) [8.7 MB] || WFirst_LightSpectrum_Final_4K_ProRes.mov (3840x2160) [5.6 GB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || WFirst_LightSpectrum_Final_H264-4K.mov (3840x2160) [196.0 MB] || ", "hits": 200 }, { "id": 20248, "url": "https://svs.gsfc.nasa.gov/20248/", "result_type": "Animation", "release_date": "2016-09-20T14:00:00-04:00", "title": "Generic Exoplanet Animations", "description": "Animation imagining what an ice-covered exoplanet might look like. || Icy_Exoplanet_Still_print.jpg (1024x576) [144.3 KB] || Icy_Exoplanet_Still.png (3840x2160) [7.6 MB] || Icy_Exoplanet_Still_searchweb.png (320x180) [89.2 KB] || Icy_Exoplanet_Still_thm.png (80x40) [6.2 KB] || Icy_Exoplanet_H264_1080p.mov (1920x1080) [30.1 MB] || Icy_Exoplanet_H264_1080p.webm (1920x1080) [1.9 MB] || Icy (3840x2160) [0 Item(s)] || Icy_Exoplanet_H264_4K.mov (3840x2160) [39.4 MB] || Icy_Exoplanet_4k_ProRes.mov (3840x2160) [2.2 GB] || ", "hits": 59 }, { "id": 12265, "url": "https://svs.gsfc.nasa.gov/12265/", "result_type": "Produced Video", "release_date": "2016-06-22T13:00:00-04:00", "title": "X-ray Echoes Map a 'Killer' Black Hole", "description": "NASA Goddard astronomer Erin Kara discusses the discovery of X-ray echoes from Swift J1644+57, a black hole that shattered a passing star. X-rays produced by flares near this million-solar-mass black hole bounced off the nascent accretion disk and revealed its structure. Credit: NASA's Goddard Space Flight CenterMusic: \"The Orion Arm\" and \"Particle Acceleration\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || TD_Still.png (1920x1080) [11.0 MB] || TD_Still_print.jpg (1024x576) [109.7 KB] || TD_Still_searchweb.png (180x320) [91.6 KB] || TD_Still_thm.png (80x40) [7.0 KB] || 12265_BH_Echoes_FINAL2_ProRes_1920x1080_2997.mov (1920x1080) [3.8 GB] || 12265_BH_Echoes_FINAL2_youtube_hq.mov (1920x1080) [1.6 GB] || 12265_BH_Echoes_FINAL2-HD_1080p.mov (1920x1080) [443.2 MB] || 12265_BH_Echoes_FINAL2-Apple_Devices_Best.m4v (1920x1080) [295.2 MB] || 12265_BH_Echoes_FINAL2_appletv.m4v (1280x720) [150.6 MB] || 12265_BH_Echoes_FINAL2-Apple_HD_Compatible.m4v (960x540) [118.9 MB] || 12265_BH_Echoes_FINAL2_appletv_subtitles.m4v (1280x720) [150.7 MB] || 12265_BH_Echoes_FINAL2-Apple_HD_Compatible.webm (960x540) [31.7 MB] || 12265_BH_Echoes_FINAL2_SRT_Captions.en_US.srt [5.3 KB] || 12265_BH_Echoes_FINAL2_SRT_Captions.en_US.vtt [5.3 KB] || 12265_BH_Echoes_FINAL2_lowres.mp4 (480x272) [39.9 MB] || ", "hits": 177 }, { "id": 12286, "url": "https://svs.gsfc.nasa.gov/12286/", "result_type": "Produced Video", "release_date": "2016-06-20T11:00:00-04:00", "title": "Instagram: The Electric Wind of Venus", "description": "In many ways, Venus is the most similar planet to Earth. Not only are its size and gravity comparable to Earth’s, but there’s evidence that Venus once had lots of water – oceans’ worth! – in the distant past. So what happened? New NASA-funded research using data from ESA’s Venus Express reveal that it may have been Venus’ electric field that stripped the planet of water. Venus’ electric field is about 5-10 times stronger than Earth’s. That electric force is enough to rip particles – including the building blocks of water – out of Venus’ atmosphere. Over time, this “electric wind” could leave a watery planet bone-dry, making it a key factor in whether or not a planet is hospitable to life. Understanding this process will help scientists pinpoint where potentially habitable planets could be lurking around other stars. || ", "hits": 141 }, { "id": 12208, "url": "https://svs.gsfc.nasa.gov/12208/", "result_type": "Produced Video", "release_date": "2016-06-20T09:00:00-04:00", "title": "The Electric Wind of Venus", "description": "Venus has an \"electric wind\" strong enough to remove the components of water from its upper atmosphere. This action may have played a significant role in stripping Earth's twin planet of its oceans, according to new research results from the European Space Agency's Venus Express mission led by NASA-funded researchers. Lead author of the research paper, Glyn Collinson, explains that \"electric wind\" can strip Earth-like planets of oceans and atmospheres. || ", "hits": 125 }, { "id": 12281, "url": "https://svs.gsfc.nasa.gov/12281/", "result_type": "Produced Video", "release_date": "2016-06-10T18:00:00-04:00", "title": "Instagram: Solar Storms May Have Been Key to Life on Earth", "description": "Our sun's adolescence was stormy—and new evidence shows that these tempests may have been just the key to seeding life as we know it.Some 4 billion years ago, the sun shone with only about three-quarters the brightness we see today, but its surface roiled with giant eruptions spewing enormous amounts of solar material and radiation out into space. These powerful solar explosions may have provided the crucial energy needed to warm Earth, despite the sun's faintness. The eruptions also may have furnished the energy needed to turn simple molecules into the complex molecules such as RNA and DNA that were necessary for life. The research was published in Nature Geoscience on May 23, 2016, by a team of scientists from NASA.Understanding what conditions were necessary for life on our planet helps us both trace the origins of life on Earth and guide the search for life on other planets. Until now, however, fully mapping Earth's evolution has been hindered by the simple fact that the young sun wasn't luminous enough to warm Earth.\"Back then, Earth received only about 70 percent of the energy from the sun than it does today,\" said Vladimir Airapetian, lead author of the paper and a solar scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. \"That means Earth should have been an icy ball. Instead, geological evidence says it was a warm globe with liquid water. We call this the Faint Young Sun Paradox. Our new research shows that solar storms could have been central to warming Earth.\" || ", "hits": 72 }, { "id": 12267, "url": "https://svs.gsfc.nasa.gov/12267/", "result_type": "Produced Video", "release_date": "2016-06-09T11:00:00-04:00", "title": "How Earth Lost Its Cool", "description": "Scientists think solar storms may have been key to warming our planet. || c-1024.jpg (1024x576) [165.2 KB] || c-1280.jpg (1280x720) [234.6 KB] || c-1920.jpg (1920x1080) [360.8 KB] || c-1024_print.jpg (1024x576) [172.3 KB] || c-1024_searchweb.png (320x180) [93.6 KB] || c-1024_web.png (320x180) [93.6 KB] || c-1024_thm.png (80x40) [20.3 KB] || ", "hits": 115 }, { "id": 12249, "url": "https://svs.gsfc.nasa.gov/12249/", "result_type": "Produced Video", "release_date": "2016-05-24T11:00:00-04:00", "title": "Earth's Magnetism In Action", "description": "Scientists make a breakthrough in observing the dynamic magnetic system surrounding our planet. || c-1024.jpg (1024x576) [385.4 KB] || c-1280.jpg (1280x720) [576.4 KB] || c-1024_print.jpg (1024x576) [403.6 KB] || c-1024_searchweb.png (320x180) [137.4 KB] || c-1024_web.png (320x180) [137.4 KB] || c-1024_thm.png (80x40) [24.5 KB] || ", "hits": 96 }, { "id": 11853, "url": "https://svs.gsfc.nasa.gov/11853/", "result_type": "Produced Video", "release_date": "2016-05-23T11:00:00-04:00", "title": "The Faint Young Star Paradox: Solar Storms May Have Been Key to Life on Earth", "description": "Energy from our young sun – 4 billion years ago -- aided in creating molecules in Earth's atmosphere that allowed it to warm up enough to incubate life. Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || faintyoung.jpg (1280x720) [105.6 KB] || faintyoung_searchweb.png (320x180) [81.4 KB] || faintyoung_thm.png (80x40) [15.3 KB] || WEBM_G2015-036_FaintYoungStarParadox_V2.webm (960x540) [39.6 MB] || G2015-036_FaintYoungStarParadox_V2.mov (1920x1080) [1.4 GB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv.m4v (1280x720) [54.0 MB] || YOUTUBE_HQ_G2015-036_FaintYoungStarParadox_V2_youtube_hq.mov (1920x1080) [318.5 MB] || NASA_TV_G2015-036_FaintYoungStarParadox_V2.mpeg (1280x720) [346.1 MB] || PRORES_B-ROLL_G2015-036_FaintYoungStarParadox_V2_prores.mov (1280x720) [719.8 MB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv_subtitles.m4v (1280x720) [54.0 MB] || G2015-036FaintYoungStarParadox_V2.en_US.srt [1.8 KB] || G2015-036FaintYoungStarParadox_V2.en_US.vtt [1.8 KB] || NASA_PODCAST_G2015-036_FaintYoungStarParadox_V2_ipod_sm.mp4 (320x240) [18.8 MB] || G2015-036_FaintYoungStarParadox_V2_lowres.mp4 (480x272) [14.8 MB] || ", "hits": 182 }, { "id": 20237, "url": "https://svs.gsfc.nasa.gov/20237/", "result_type": "Animation", "release_date": "2016-05-12T14:00:00-04:00", "title": "Beyond Earth - Earth's Geomagnetic Activity", "description": "Space is a better vacuum than any we can create on Earth, but it's nonetheless bustling with activity. It overflows with energy, particles and a complex system of magnetic field lines. This animation shows the busy-ness of near-Earth space, where the magnetic environment around Earth can trap electrons and charged particles. || beyondearth.jpg (1280x720) [261.9 KB] || beyondearth_searchweb.png (320x180) [136.2 KB] || beyondearth_thm.png (80x40) [22.8 KB] || BeyondEarthAnimatedGIFFinal30fpsv02.webm (1920x1080) [4.4 MB] || BeyondEarthAnimatedGIFFinal30fpsv02.mov (1920x1080) [429.8 MB] || BeyondEarthAnimatedGIFFinal60fpsv02.mov (1920x1080) [429.8 MB] || beyond-earth-earths-geomagnetic-activity.hwshow || ", "hits": 253 }, { "id": 12239, "url": "https://svs.gsfc.nasa.gov/12239/", "result_type": "Produced Video", "release_date": "2016-05-12T13:00:00-04:00", "title": "MMS First Results", "description": "This short video outlines the MMS mission and its first results. Since it launched, MMS has made more than 4,000 trips through the magnetic boundaries around Earth, each time gathering information about the way the magnetic fields and particles move. A surprising result was that at the moment of interconnection between the sun’s magnetic field lines and those of Earth the crescents turned abruptly so that the electrons flowed along the field lines. By watching these electron tracers, MMS made the first observation of the predicted breaking and interconnection of magnetic fields in space. Credit: NASA/GSFCWatch this video on the NASA Goddard YouTube channel. || mmsthumb.jpg (1280x720) [139.4 KB] || mmsthumb_print.jpg (1024x576) [161.8 KB] || mmsthumb_searchweb.png (320x180) [104.3 KB] || mmsthumb_web.png (320x180) [104.3 KB] || mmsthumb_thm.png (80x40) [6.8 KB] || 12239_MMS_First_ResultsV2_appletv.m4v (1280x720) [76.9 MB] || 12239_MMS_First_ResultsV2.webm (1920x1080) [18.1 MB] || 12239_MMS_First_ResultsV2_appletv_subtitles.m4v (1280x720) [77.0 MB] || 12239_MMS_First_ResultsV2.en_US.srt [3.0 KB] || 12239_MMS_First_ResultsV2.en_US.vtt [3.0 KB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov (1920x1080) [1.1 GB] || 12239_MMS_First_ResultsV2_lowres.mp4 (480x272) [21.6 MB] || 12239_MMS_First_ResultsV2_ipod_sm.mp4 (320x240) [26.3 MB] || PRORES_B-ROLL_12239_MMS_First_ResultsV2_prores.mov (1280x720) [2.2 GB] || 12239_MMS_First_ResultsV2.mov (1920x1080) [4.2 GB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov.hwshow [100 bytes] || ", "hits": 179 }, { "id": 20228, "url": "https://svs.gsfc.nasa.gov/20228/", "result_type": "Animation", "release_date": "2016-04-06T11:00:00-04:00", "title": "Massive Black Hole Shreds Passing Star (Animation Only)", "description": "A star approaching too close to a massive black hole is torn apart by tidal forces, as shown in this artist's rendering. Filaments containing much of the star's mass fall toward the black hole. Eventually these gaseous filaments merge into a smooth, hot disc glowing brightly in X-rays. As the disk forms, it's central region heats up tremendously, which drives a flow of material, called a wind, away from the disk.Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || BlackHoleAnimation.1675_print.jpg (1024x576) [119.5 KB] || BlackHoleAnimation.1675_searchweb.png (320x180) [88.0 KB] || BlackHoleAnimation.1675_thm.png (80x40) [5.9 KB] || 20228_Swift_Tidal_ProRes_1920x1080_5994.webm (1920x1080) [4.8 MB] || 1920x1080_16x9_60p (1920x1080) [256.0 KB] || 20228_Swift_Tidal_ProRes_1920x1080_5994.mov (1920x1080) [1.4 GB] || 20228_Swift_Tidal_H264_1920x1080_5994.mov (1920x1080) [813.8 MB] || ", "hits": 182 }, { "id": 20234, "url": "https://svs.gsfc.nasa.gov/20234/", "result_type": "Animation", "release_date": "2016-03-07T11:00:00-05:00", "title": "Conceptual Image Lab Demo Reel", "description": "CI Lab Demo Reel || CI_Labs_Demo_-_APR_Master_print.00105.jpg (1024x576) [14.7 KB] || CI_Labs_Demo_-_APR_Master_searchweb.png (320x180) [6.0 KB] || CI_Labs_Demo_-_APR_Master_thm.png (80x40) [954 bytes] || CI_Labs_Demo_-_APR_Master.mov (1920x1080) [2.4 GB] || CI_Labs_Demo_-_H264_Master.mov (1920x1080) [119.5 MB] || CI_Labs_Demo.mp4 (1920x1074) [94.8 MB] || CI_Labs_Demo_-_H264_Master.webm (1920x1080) [20.7 MB] || CILab_demo.en_US.vtt [384 bytes] || CILab_demo.en_US.srt [370 bytes] || ", "hits": 59 }, { "id": 12027, "url": "https://svs.gsfc.nasa.gov/12027/", "result_type": "Produced Video", "release_date": "2015-11-23T11:00:00-05:00", "title": "NASM 2015: Our Violent Universe", "description": "NASM 2015 Presentation - Our Violent Universe || poster-VX-73356-00-00-25,41.jpg (1280x720) [159.6 KB] || poster-VX-73356-00-00-25,41_searchweb.png (320x180) [94.7 KB] || poster-VX-73356-00-00-25,41_thm.png (80x40) [6.8 KB] || APPLE_TV_G2015-086_NASM_2015_appletv.m4v (1280x720) [1.6 GB] || NASA_TV_G2015-086_NASM_2015.mpeg (1280x720) [10.9 GB] || WMV_G2015-086_NASM_2015_HD.wmv (1280x720) [630.3 MB] || YOUTUBE_HQ_G2015-086_NASM_2015_youtube_hq.mov (1280x720) [8.3 GB] || G2015-086_NASM_2015_edited.mov (1280x720) [29.2 GB] || WEBM_G2015-086_NASM_2015.webm (960x540) [1.3 GB] || APPLE_TV_G2015-086_NASM_2015_appletv_subtitles.m4v (1280x720) [1.6 GB] || G2015-086_NASM2015.en_US.srt [77.0 KB] || G2015-086_NASM2015.en_US.vtt [72.4 KB] || NASA_PODCAST_G2015-086_NASM_2015_ipod_sm.mp4 (320x240) [589.1 MB] || ", "hits": 68 }, { "id": 12046, "url": "https://svs.gsfc.nasa.gov/12046/", "result_type": "Produced Video", "release_date": "2015-11-10T11:00:00-05:00", "title": "Stripping the Martian Atmosphere", "description": "A NASA mission reveals how gases in Mars' upper atmosphere are stripped away by the sun's solar wind. || c-1920.jpg (1920x1080) [991.0 KB] || c-1280.jpg (1280x720) [567.7 KB] || c-1024.jpg (1024x576) [389.5 KB] || c-1024_print.jpg (1024x576) [397.5 KB] || c-1024_searchweb.png (320x180) [121.3 KB] || c-1024_web.png (320x180) [121.3 KB] || c-1024_thm.png (80x40) [7.2 KB] || ", "hits": 337 }, { "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": 425 }, { "id": 12033, "url": "https://svs.gsfc.nasa.gov/12033/", "result_type": "Produced Video", "release_date": "2015-10-29T11:00:00-04:00", "title": "A Star Is Torn", "description": "Scientists uncover new details about what happens when a black hole destroys a star. || c-1920.jpg (1920x1080) [746.6 KB] || c-1280.jpg (1280x720) [362.0 KB] || c-1024.jpg (1024x576) [226.8 KB] || c-1024_print.jpg (1024x576) [242.9 KB] || c-1024_searchweb.png (320x180) [108.1 KB] || c-1024_web.png (320x180) [108.1 KB] || c-1024_thm.png (80x40) [16.9 KB] || ", "hits": 84 }, { "id": 12005, "url": "https://svs.gsfc.nasa.gov/12005/", "result_type": "Produced Video", "release_date": "2015-10-21T13:00:00-04:00", "title": "Massive Black Hole Shreds Passing Star", "description": "A star approaching too close to a massive black hole is torn apart by tidal forces, as shown in this artist's rendering. Filaments containing much of the star's mass fall toward the black hole. Eventually these gaseous filaments merge into a smooth, hot disk glowing brightly in X-rays. As the disk forms, its central region heats up tremendously, which drives a flow of material, called a wind, away from the disk. Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Swift_Tidal_Disruption_2_Still_print.jpg (1024x576) [172.7 KB] || Swift_Tidal_Disruption_2_Still.jpg (1920x1080) [606.7 KB] || Swift_Tidal_Disruption_2_Still_web.png (320x180) [98.5 KB] || Swift_Tidal_Disruption_2_Still_thm.png (80x40) [6.8 KB] || Swift_Tidal_Disruption_2_Still_searchweb.png (320x180) [98.4 KB] || APPLE_TV_12005_Swift_Tidal_Music_FINAL_appletv_subtitles.m4v (1280x720) [37.5 MB] || 12005_Swift_Tidal_Music_MPEG4_1920X1080_2997.mp4 (1920x1080) [40.5 MB] || 12005_Swift_Tidal_Music_MPEG4_1920X1080_2997.webm (1920x1080) [7.7 MB] || WMV_12005_Swift_Tidal_Music_FINAL_HD.wmv (1920x1080) [49.6 MB] || APPLE_TV_12005_Swift_Tidal_Music_FINAL_appletv.m4v (1280x720) [37.4 MB] || 12005_Swift_Tidal_SRT_Captions.en_US.vtt [261 bytes] || 12005_Swift_Tidal_Music_FINAL_lowres.mp4 (480x272) [10.6 MB] || NASA_PODCAST_12005_Swift_Tidal_Music_FINAL_ipod_sm.mp4 (320x240) [12.3 MB] || 12005_Swift_Tidal_SRT_Captions.en_US.srt [248 bytes] || 12005_Swift_Tidal_Music_ProRes_1920x1080_5994.mov (1920x1080) [2.1 GB] || 12005_Swift_Tidal_Music_H264_Good_1920x1080_2997.mov (1920x1080) [301.2 MB] || 12005_Swift_Tidal_Music_FINAL_youtube_hq.mov (1920x1080) [1.3 GB] || 12005_Swift_Tidal_Music_H264_Best_1920x1080_5994.mov (1920x1080) [2.5 GB] || ", "hits": 269 }, { "id": 11929, "url": "https://svs.gsfc.nasa.gov/11929/", "result_type": "Produced Video", "release_date": "2015-09-08T11:45:00-04:00", "title": "Imaging Stars From Mars", "description": "A NASA spacecraft uses starlight to probe the composition of Mars’ upper atmosphere. || c-1920.jpg (1920x1080) [332.6 KB] || c-1280.jpg (1280x720) [185.3 KB] || c-1024.jpg (1024x576) [124.4 KB] || c-1024_print.jpg (1024x576) [134.3 KB] || c-1024_searchweb.png (320x180) [70.7 KB] || c-1024_web.png (320x180) [70.7 KB] || c-1024_thm.png (80x40) [13.1 KB] || ", "hits": 69 }, { "id": 11992, "url": "https://svs.gsfc.nasa.gov/11992/", "result_type": "Produced Video", "release_date": "2015-09-02T11:00:00-04:00", "title": "Mapping Mars' Upper Atmosphere", "description": "Principal Investigator Bruce Jakosky talks about MAVEN’s science observations at Mars.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Bruce_Jakosky_G2015-007_thumbnail.png (1920x1080) [1.8 MB] || Bruce_Jakosky_G2015-007_thumbnail_print.jpg (1024x576) [100.6 KB] || Bruce_Jakosky_G2015-007_thumbnail_searchweb.png (320x180) [90.5 KB] || Bruce_Jakosky_G2015-007_thumbnail_thm.png (80x40) [7.2 KB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv.m4v (1280x720) [123.4 MB] || WEBM_G2015-007_MAVEN_Early_Sci_MASTER.webm (960x540) [101.9 MB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv_subtitles.m4v (1280x720) [123.5 MB] || NASA_TV_G2015-007_MAVEN_Early_Sci_MASTER.mpeg (1280x720) [846.9 MB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.srt [4.1 KB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.vtt [4.2 KB] || G2015-007_MAVEN_Early_Sci_MASTER_H264.mov (1920x1080) [1.7 GB] || NASA_PODCAST_G2015-007_MAVEN_Early_Sci_MASTER_ipod_sm.mp4 (320x240) [44.1 MB] || PRORES_B-ROLL_G2015-007_MAVEN_Early_Sci_MASTER_prores.mov (1280x720) [3.4 GB] || G2015-007_MAVEN_Early_Sci_MASTER.mov (1920x1080) [6.5 GB] || ", "hits": 29 }, { "id": 20223, "url": "https://svs.gsfc.nasa.gov/20223/", "result_type": "Animation", "release_date": "2015-09-02T11:00:00-04:00", "title": "MAVEN Stellar Occultation", "description": "NASA's Mars Atmosphere and Volatile Evolution mission (MAVEN) is the first spacecraft specifically designed to study the upper atmosphere of Mars. MAVEN's goal is to determine how Mars lost its thick early atmosphere, and with it, its once hospitable climate.While previous Mars orbiters have peered down at the planet's surface, MAVEN is spending part of its time gazing at the stars, observing the Martian atmosphere through a series of stellar occultations. As Mars rolls beneath MAVEN, due to the spacecraft's own orbital motion, background stars rise and set behind the planet. Their light dims as it passes through the tenuous atmosphere, with specific gases absorbing specific wavelengths. MAVEN uses its Imaging Ultraviolet Spectrograph to break apart this light and see which wavelengths are absorbed, allowing it to determine atmospheric composition at varying altitudes. || ", "hits": 43 }, { "id": 11844, "url": "https://svs.gsfc.nasa.gov/11844/", "result_type": "Produced Video", "release_date": "2015-05-14T11:00:00-04:00", "title": "Big Ozone Holes Going Extinct", "description": "NASA scientists say large ozone holes will be a thing of the past by 2040. || f-1280.jpg (1280x720) [253.0 KB] || f-1920.jpg (1920x1080) [402.2 KB] || f-1024_print.jpg (1024x576) [163.6 KB] || f-1024_print_print.jpg (1024x576) [163.6 KB] || f-1024_print_searchweb.png (320x180) [102.6 KB] || ", "hits": 74 }, { "id": 11869, "url": "https://svs.gsfc.nasa.gov/11869/", "result_type": "Produced Video", "release_date": "2015-05-08T10:00:00-04:00", "title": "NASA On Air: Big Ozone Holes Headed For Extinction By 2040 (5/8/2015)", "description": "LEAD: NASA scientists report that the ozone hole over Antarctica is slowly recovering.1. The ozone hole is the result of man-made chlorine and bromine chemicals reacting with thin ice clouds at 60,000 feet where temperatures are bitterly cold, less than –110 Degrees Fahrenheit.2. The ozone hole varies from twice to three times the size of the United States.3. Since the Montreal Protocol agreement in 1987, emissions have been regulated and ozone-depleting chemical levels have been slowly declining.4. With a new analysis, NASA scientists say that the ozone hole will be consistently smaller than less than twice the United States.TAG: Scientists will continue to use satellites to monitor the recovery of the ozone hole and they hope to see its full recovery before the end of the century. || WC_Ozone2040-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [115.0 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [78.1 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_web.png (320x180) [78.1 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_thm.png (80x40) [5.4 KB] || WC_Ozone2040-1920-MASTER_1920x1080.mov (1920x1080) [648.2 MB] || WC_Ozone2040-1920-MASTER_1280x720.mov (1280x720) [766.3 MB] || WC_Ozone2040-1920-MASTER_NBC_Today.mov (1920x1080) [241.4 MB] || WC_Ozone2040-1920-MASTER_WEA_CEN.wmv (1280x720) [17.3 MB] || WC_Ozone2040-1920-MASTER_converted.avi (1280x720) [19.0 MB] || WC_Ozone2040-1920-MASTER_baron.mp4 (1920x1080) [20.6 MB] || WC_Ozone2040-1920-MASTER_prores.mov (1920x1080) [518.5 MB] || WC_Ozone2040-1920-MASTER_iPad_960x540.m4v (960x540) [71.1 MB] || WC_Ozone2040-1920-MASTER_iPad_1280x720.m4v (1280x720) [116.2 MB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [241.4 MB] || WC_Ozone2040-1920-MASTER_iPad_960x540.webm (960x540) [3.4 MB] || ", "hits": 89 }, { "id": 11781, "url": "https://svs.gsfc.nasa.gov/11781/", "result_type": "Produced Video", "release_date": "2015-05-06T12:00:00-04:00", "title": "Big Ozone Holes Headed For Extinction By 2040", "description": "The next three decades will see an end of the era of big ozone holes. In a new study, scientists from NASA Goddard Space Flight Center say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040.Ozone-depleting chemicals in the atmosphere cause an ozone hole to form over Antarctica during the winter months in the Southern Hemisphere. Since the Montreal Protocol agreement in 1987, emissions have been regulated and chemical levels have been declining. However, the ozone hole has still remained bigger than 8 million square miles since the early 1990s, with exact sizes varying from year to year.The size of the ozone hole varies due to both temperature and levels of ozone-depleting chemicals in the atmosphere. In order to get a more accurate picture of the future size of the ozone hole, scientists used NASA’s AURA satellite to determine how much the levels of these chemicals in the atmosphere varied each year. With this new knowledge, scientists can confidently say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040. Scientists will continue to use satellites to monitor the recovery of the ozone hole and they hope to see its full recovery before the end of the century.Research: Inorganic chlorine variability in the Antarctic vortex and implications for ozone recovery.Journal: Geophysical Research: Atmospheres, December 18, 2014.Link to paper: http://onlinelibrary.wiley.com/doi/10.1002/2014JD022295/abstract.Here is the YouTube video. || ", "hits": 133 }, { "id": 11829, "url": "https://svs.gsfc.nasa.gov/11829/", "result_type": "Produced Video", "release_date": "2015-03-31T14:00:00-04:00", "title": "A Week in the Life of Rain", "description": "A video highlighting several precipitation events that occurred between August 4 and August 11, 2014, using the IMERG dataset.For complete transcript, click here. || Week_in_the_Life_of_Rain_nasaportal_print.jpg (1024x576) [125.5 KB] || Week_in_the_Life_of_Rain_nasaportal_searchweb.png (320x180) [101.3 KB] || Week_in_the_Life_of_Rain_nasaportal_web.png (320x180) [101.3 KB] || Week_in_the_Life_of_Rain_nasaportal_thm.png (80x40) [6.9 KB] || Week_in_the_Life_of_Rain_1280x720.wmv (1280x720) [196.3 MB] || Week_in_the_Life_of_Rain_large.mp4 (1280x720) [419.8 MB] || Week_in_the_Life_of_Rain_youtube_hq.mov (1280x720) [742.6 MB] || Week_in_the_Life_of_Rain_720x480.webm (720x480) [44.2 MB] || Week_in_the_Life_of_Rain_ipod_lg.m4v (640x360) [66.1 MB] || WeekLifeRain.en_US.srt [8.5 KB] || WeekLifeRain.en_US.vtt [8.5 KB] || Week_in_the_Life_of_Rain_nasaportal.mov (640x360) [162.0 MB] || Week_in_the_Life_of_Rain_720x480.wmv (720x480) [187.9 MB] || Week_in_the_Life_of_Rain_ipod_sm.mp4 (320x240) [35.6 MB] || Week_in_the_Life_of_Rain-H264_Best_1280x720_59.94.mov (1280x720) [3.4 GB] || Week_in_the_Life_of_Rain_prores.mov (1280x720) [5.8 GB] || ", "hits": 25 }, { "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": 133 }, { "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": 427 }, { "id": 11751, "url": "https://svs.gsfc.nasa.gov/11751/", "result_type": "Produced Video", "release_date": "2015-02-26T11:00:00-05:00", "title": "Dust Crossing", "description": "What connects Earth's largest, hottest desert to its largest tropical rain forest? || c-1920.jpg (1920x1080) [364.1 KB] || c-1280.jpg (1280x720) [202.1 KB] || c-1024.jpg (1024x576) [136.8 KB] || c-1024_print.jpg (1024x576) [131.4 KB] || c-1024_searchweb.png (320x180) [75.1 KB] || c-1024_print_thm.png (80x40) [13.5 KB] || ", "hits": 271 }, { "id": 11785, "url": "https://svs.gsfc.nasa.gov/11785/", "result_type": "Produced Video", "release_date": "2015-02-24T13:00:00-05:00", "title": "NASA On Air: NASA Satellite Reveals How Much Dust Feeds Amazon’s Plants (2/24/2015)", "description": "LEAD: NASA scientists have made the first multi-year satellite-based estimate of how much Saharan dust in Africa floats all the way to South America’s Amazon rainforest.1. An estimated 28 million tons of African dust falls on the Amazon rainforest – more than 100,000 semi-truck loads.2. A small but very important ingredient in the dust is the phosphorus from an ancient dusty lake bed in Chad.3. The African phosphorus plays a critical role as a natural fertilizer for the Amazon rainforest growth.TAG: This dust transport is the largest on the planet. Satellite studies will also help determine its relationship to climate changes. || WC_Dust-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [105.3 KB] || WC_Dust-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [75.0 KB] || WC_Dust-1920-MASTER_iPad_1920x0180_web.png (320x180) [75.0 KB] || WC_Dust-1920-MASTER_iPad_1920x0180_thm.png (80x40) [5.5 KB] || WC_Dust-1920-MASTER_WEA_CEN.wmv (1280x720) [16.3 MB] || DUST_WC3.avi (1280x720) [16.9 MB] || WC_Dust-1920-MASTER_baron.mp4 (1920x1080) [20.9 MB] || WC_Dust-1920-MASTER_iPad_1920x0180.webm (1920x1080) [2.9 MB] || WC_Dust-1920-MASTER_iPad_960x540.m4v (960x540) [111.7 MB] || WC_Dust-1920-MASTER_iPad_1280x720.m4v (1280x720) [173.6 MB] || WC_Dust-1920-MASTER_NBC_Today.mov (1920x1080) [405.3 MB] || WC_Dust-1920-MASTER_prores.mov (1920x1080) [434.1 MB] || WC_Dust-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [405.3 MB] || WC_Dust-1920-MASTER_1920x1080.mov (1920x1080) [669.5 MB] || WC_Dust-1920-MASTER_1280x720.mov (1280x720) [769.1 MB] || ", "hits": 150 }, { "id": 11775, "url": "https://svs.gsfc.nasa.gov/11775/", "result_type": "Produced Video", "release_date": "2015-02-24T10:00:00-05:00", "title": "Satellite Tracks Saharan Dust To Amazon In 3-D", "description": "For the first time, a NASA satellite has quantified in three dimensions how much dust makes the trans-Atlantic journey from the Sahara Desert to the Amazon rainforest. Among this dust is phosphorus, an essential nutrient that acts like a fertilizer, which the Amazon depends on in order to flourish.The new dust transport estimates were derived from data collected by a lidar instrument on NASA's Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation, or CALIPSO, satellite from 2007 though 2013.An average of 27.7 million tons of dust per year – enough to fill 104,908 semi trucks – fall to the surface over the Amazon basin. The phosphorus portion, an estimated 22,000 tons per year, is about the same amount as that lost from rain and flooding. The finding is part of a bigger research effort to understand the role of dust and aerosols in the environment and on local and global climate.Research: The fertilizing role of African dust in the Amazon rainforest: A first multiyear assessment based on data from Cloud-Aerosol Lidar and Infrared Pathfinder Satellite ObservationsJournal: Geophysical Research LettersLink to paper: http://onlinelibrary.wiley.com/doi/10.1002/2015GL063040/fullHere is the YouTube video. || ", "hits": 459 }, { "id": 11743, "url": "https://svs.gsfc.nasa.gov/11743/", "result_type": "Produced Video", "release_date": "2015-01-27T16:00:00-05:00", "title": "SMAP Radiometer versus Radio Frequency Interference", "description": "The microwave radiometer on NASA's SMAP mission was designed and built at Goddard Space Flight Center to avoid unwanted radio frequency interference. Instrument Scientist Jeff Piepmeier explains how and why.For complete transcript, click here.Watch this video on the NASA Goddard YouTube channel. || G2015-009_SMAP_Radiometer_MASTER_nasaportal_print.jpg (1024x576) [57.7 KB] || G2015-009_SMAP_Radiometer_MASTER_nasaportal00802_print.jpg (1024x576) [57.0 KB] || G2015-009_SMAP_Radiometer_MASTER_nasaportal_thm.png (80x40) [5.1 KB] || G2015-009_SMAP_Radiometer_MASTER_nasaportal_web.png (320x180) [63.7 KB] || G2015-009_SMAP_Radiometer_MASTER_nasaportal_searchweb.png (320x180) [63.7 KB] || G2015-009_SMAP_Radiometer_MASTER_appletv.m4v (960x540) [84.6 MB] || G2015-009_SMAP_Radiometer_MASTER_appletv_subtitles.m4v (960x540) [84.5 MB] || G2015-009_SMAP_Radiometer_MASTER_1280x720.wmv (1280x720) [99.7 MB] || G2015-009_SMAP_Radiometer_MASTER_youtube_hq.mov (1280x720) [153.4 MB] || G2015-009_SMAP_Radiometer_MASTER_720x480.wmv (720x480) [78.6 MB] || G2015-009_SMAP_Radiometer_MASTER_720x480.webm (720x480) [22.3 MB] || G2015-009_SMAP_Radiometer_MASTER_ipod_lg.m4v (640x360) [33.5 MB] || G2015-009_SMAP_Radiometer_MASTER_nasaportal.mov (640x360) [84.1 MB] || G2015-009_SMAP_Radiometer-captions.en_US.srt [3.7 KB] || G2015-009_SMAP_Radiometer-captions.en_US.vtt [3.7 KB] || G2015-009_SMAP_Radiometer_MASTER_ipod_sm.mp4 (320x240) [17.9 MB] || G2015-009_SMAP_Radiometer_MASTER_prores.mov (1280x720) [3.0 GB] || ", "hits": 32 }, { "id": 11725, "url": "https://svs.gsfc.nasa.gov/11725/", "result_type": "Produced Video", "release_date": "2015-01-07T13:15:00-05:00", "title": "NASA Missions Take an Unparalleled Look into Superstar Eta Carinae", "description": "Explore Eta Carinae from the inside out with the help of supercomputer simulations and data from NASA satellites and ground-based observatories. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Eta_Car_Density_XY_R10_R100_STILL_1920.jpg (1920x1080) [804.4 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_print.jpg (1024x576) [52.0 KB] || Eta_Car_Density_XY_R10_R100_STILL.jpg (4928x2772) [874.1 KB] || Eta_Car_Density_XY_R10_R100_STILL.png (4928x2772) [36.6 MB] || Eta_Car_Density_XY_R10_R100_STILL_1920_web.jpg (320x180) [13.1 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_searchweb.png (320x180) [55.9 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_thm.png (80x40) [8.0 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920.tiff (1920x1080) [11.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.webm (960x540) [30.5 MB] || G2015-001_Eta_Car_Binary_Final_ipod_lg.m4v (640x360) [43.2 MB] || G2015-001_Eta_Car_Binary.en_US.vtt [5.2 KB] || G2015-001_Eta_Car_Binary.en_US.srt [5.2 KB] || G2015-001_Eta_Car_Binary_Final_ipod_sm.mp4 (320x240) [22.8 MB] || G2015-001_Eta_Car_Binary_Final_appletv_subtitles.m4v (960x540) [103.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.m4v (960x540) [104.0 MB] || G2015-001_Eta_Car_Binary_Final_1280x720.wmv (1280x720) [107.6 MB] || 11725_Eta_Car_Binary2_MPEG4_1920X1080_2997.mp4 (1920x1080) [116.9 MB] || 11725_Eta_Car_Binary2_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || 11725_Eta_Car_Binary2_H264_Best_1920x1080_2997.mov (1920x1080) [2.6 GB] || 11725_Eta_Car_Binary2_H264_Good_1920x1080_2997.mov (1920x1080) [506.2 MB] || Eta_Car_Density_XY_R10_R100_STILL.tiff (4928x2772) [104.2 MB] || ", "hits": 143 }, { "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": 220 }, { "id": 11690, "url": "https://svs.gsfc.nasa.gov/11690/", "result_type": "Produced Video", "release_date": "2014-12-11T11:00:00-05:00", "title": "CATS In Space", "description": "Earth's atmosphere may look empty, but it's actually chock-full of aerosols—tiny airborne particles such as dust, smoke and ash that seed clouds. Like clouds, these particles reflect and absorb sunlight, playing an important role in the cooling and warming of the planet. Now, with the help of a new instrument being launched this month to the International Space Station, scientists can better explore the properties of clouds and aerosols from space. The Cloud-Aerosol Transport System (CATS) is a refrigerator-sized probe that will bounce lasers into the atmosphere, collecting data on the location and composition of clouds and aerosols around the globe. The results will provide the closest look yet at how clouds form, sharpening computer models that use such information to project how cloud patterns may influence Earth's weather and climate. Watch the video for an animation that shows CATS scanning the atmosphere from orbit. || ", "hits": 26 }, { "id": 11685, "url": "https://svs.gsfc.nasa.gov/11685/", "result_type": "Produced Video", "release_date": "2014-11-25T11:00:00-05:00", "title": "Cloud Transformation", "description": "Volcanoes can spew lava, ash and smoke when they erupt. But even when they aren't erupting, gases can leak from their vents and form tiny particles in the atmosphere known as volcanic aerosols. Although smaller than a human hair, these particles can have a large effect on the properties of nearby clouds. A new study using NASA and European Space Agency satellite data has shown that volcanic aerosols can decrease the size of water droplets that make up clouds. The result may not seem significant, but clouds composed of smaller droplets tend to be brighter and reflect more sunlight back into space. This can affect weather patterns, such as altering winds and where rain falls. Watch the video to learn more. || ", "hits": 59 }, { "id": 11702, "url": "https://svs.gsfc.nasa.gov/11702/", "result_type": "Produced Video", "release_date": "2014-11-21T00:00:00-05:00", "title": "MMS Launch and Deploy - Narrated", "description": "In March of 2015, an unprecedented NASA mission will launch to study a process so mysterious that no one has ever directly measured it in action. To create the first-ever 3-dimensional maps of this process, a process called magnetic reconnection, which occurs all over the universe, the Magnetospheric Multiscale, or MMS, mission uses four separate spacecraft equipped with ultra high speed instruments. Launching four satellites into space simultaneously is a complicated process. In addition, each spacecraft has six booms that will unfold and extend in space once in orbit. A launch and deployment with so many moving parts must be meticulously planned. Watch the video to get a sneak preview of how MMS will make this journey: The four spacecraft are housed in a single rocket on their trip into space. One by one, each ejects out, before moving into a giant pyramid-shaped configuration. Next each spacecraft deploys its six booms. Once in orbit, MMS will fly through regions near Earth where this little-understood process of magnetic reconnection occurs. Magnetic reconnection happens in thin layers just miles thick, but can tap into enough power at times to create gigantic explosions many times the size of Earth. Reconnection happens when magnetic field lines explosively realign and release massive bursts of energy, while hurling particles out at nearly the speed of light in all directions. Magnetic reconnection powers eruptions on the sun and – closer to home – triggers the flow of material and energy from interplanetary space into near-Earth space. The MMS orbit will carry the four spacecraft through reconnection regions near Earth, using this nearby natural laboratory to better understand how reconnection occurs everywhere in space. For more information about MMS, visit: www.nasa.gov/mms || ", "hits": 25 }, { "id": 10183, "url": "https://svs.gsfc.nasa.gov/10183/", "result_type": "Produced Video", "release_date": "2014-11-13T13:00:00-05:00", "title": "How Do Active Volcanoes Change Clouds?", "description": "NASA Goddard Space Flight Center scientist Andrew Sayer talks about how emissions from volcanoes can affect clouds.This video provides an overview of research published in the Journal of Atmospheric Chemistry and Physics Research:Systematic satellite observations of the impact of aerosols from passive volcanic degassing on local cloud propertiesJournal of Atmospheric Chemistry and Physics, October 9, 2014 || ", "hits": 65 }, { "id": 11671, "url": "https://svs.gsfc.nasa.gov/11671/", "result_type": "Produced Video", "release_date": "2014-10-07T11:45:00-04:00", "title": "Sea Ice: Past, Present and Future", "description": "Sea ice has covered a portion of the Arctic Ocean for more than 10 million years. But only in the last hundred or so years have advancements in technology—from the beginnings of flight to the dawn of the space age—enabled humans to gain a complete view of the sea ice and an understanding of how it’s changing. Scientific accounts of Arctic sea ice can be traced back to the time of the Roman Empire. Early explorers traveled across land and by sea to witness firsthand the floating sheets of ice that blanket Earth's northern pole. By the mid- to late 20th century, observation of the Arctic’s frozen waters entered a new era. Remote-sensing instruments carried aboard research aircraft and satellites provided enhanced and eventually near-continuous monitoring of sea ice from space. Watch the videos for a closer look at select events in Arctic sea ice exploration. || ", "hits": 53 }, { "id": 20214, "url": "https://svs.gsfc.nasa.gov/20214/", "result_type": "Animation", "release_date": "2014-10-06T00:00:00-04:00", "title": "MMS Launch and Deployment", "description": "This animation follows Magnetosphere Multiscale(MMS) Mission from launch at Kennedy Space Center through deployment and on station doing science. The MMS mission is comprising four identically instrumented spacecraft that will use Earth’s magnetosphere as a laboratory to study the microphysics of three fundamental plasma processes: magnetic reconnection, energetic particle acceleration, and turbulence. || ", "hits": 17 }, { "id": 11639, "url": "https://svs.gsfc.nasa.gov/11639/", "result_type": "Produced Video", "release_date": "2014-09-11T11:30:00-04:00", "title": "Mini Nebula", "description": "Eta Carinae lies about 7,500 light-years away in the southern constellation of Carina and is one of the most massive binary star systems in our Milky Way galaxy. In the middle of the 19th century, it underwent an explosion that astronomers call the Great Eruption. As a part of this event, a gaseous shell containing at least 10 and perhaps as much as 40 times the sun's mass was shot into space. Using new observations, astronomers created the first high-resolution 3-D model of the expanding cloud produced by this outburst. The model suggests the twin-lobed dust-filled cloud known as the Homunculus Nebula—which is now about a light-year long and continues to expand at more than 1.3 million mph—was molded by interactions between Eta Carinae's two stars. Watch the video to learn more. || ", "hits": 84 }, { "id": 11440, "url": "https://svs.gsfc.nasa.gov/11440/", "result_type": "Produced Video", "release_date": "2014-09-11T09:30:00-04:00", "title": "Ionospheric Holes on Venus", "description": "The European Space Agency's Venus Express mission saw something it could not explain. It appeared that there were holes on the nightside of Venus' ionosphere. Researchers at NASA's Goddard Space Flight Center investigated these mysterious holes, and found evidence that the sun's magnetic field lines may be penetrating through the planet. || ", "hits": 97 }, { "id": 11637, "url": "https://svs.gsfc.nasa.gov/11637/", "result_type": "Produced Video", "release_date": "2014-09-08T10:15:00-04:00", "title": "CATS - New Remote-Sensing Instrument to Blaze a Trail on the International Space Station", "description": "The Cloud-Aerosol Transport System (CATS), a new instrument that will measure the character and worldwide distribution of the tiny particles that make up haze, dust, air pollutants, and smoke, will do more than gather data once it's deployed on the International Space Station in December. || ", "hits": 59 }, { "id": 11634, "url": "https://svs.gsfc.nasa.gov/11634/", "result_type": "Produced Video", "release_date": "2014-09-03T09:00:00-04:00", "title": "A Selective History of Arctic Sea Ice Observations", "description": "Arctic sea ice has been been the last frontier of the North for thousands of years, turning back seafarers, testing the mettle of explorers, and providing a way of life for people circling the top of the world. This animated timeline provides a quick (and highly selective) ride from the days of early Greek exploration to the dawn of the Space Age to the advanced capabilities we have today. || ", "hits": 31 }, { "id": 11568, "url": "https://svs.gsfc.nasa.gov/11568/", "result_type": "Produced Video", "release_date": "2014-07-08T10:00:00-04:00", "title": "Eta Carinae's Homunculus Nebula Now in 3D", "description": "An international team of astronomers has developed a 3D model of a giant cloud ejected by the massive binary system Eta Carinae during its 19th century outburst. Eta Carinae lies about 7,500 light-years away in the southern constellation of Carina and is one of the most massive binary systems astronomers can study in detail. The smaller star is about 30 times the mass of the sun and may be as much as a million times more luminous. The primary star contains about 90 solar masses and emits 5 million times the sun's energy output. Both stars are fated to end their lives in spectacular supernova explosions.Between 1838 and 1845, Eta Carinae underwent a period of unusual variability during which it briefly outshone Canopus, normally the second-brightest star. As a part of this event, which astronomers call the Great Eruption, a gaseous shell containing at least 10 and perhaps as much as 40 times the sun's mass was shot into space. This material forms a twin-lobed dust-filled cloud known as the Homunculus Nebula, which is now about a light-year long and continues to expand at more than 1.3 million mph (2.1 million km/h). Using the European Southern Observatory's Very Large Telescope and its X-Shooter spectrograph, the team imaged near-infrared, visible and ultraviolet wavelengths along 92 separate swaths across the nebula, making the most complete spectral map to date. The researchers have used the spatial and velocity information provided by this data to create the first high-resolution 3D model of the Homunculus Nebula.The shape model was developed using only a single emission line of near-infrared light emitted by molecular hydrogen gas. The characteristic 2.12-micron light shifts in wavelength slightly depending on the speed and direction of the expanding gas, allowing the team to probe even dust-obscured portions of the Homunculus that face away from Earth. || ", "hits": 147 } ] }