{ "count": 65, "next": null, "previous": null, "results": [ { "id": 14938, "url": "https://svs.gsfc.nasa.gov/14938/", "result_type": "Visualization", "release_date": "2025-12-22T11:00:00-05:00", "title": "Artemis Science: Visualizing NASA’s Next Lunar Flyby", "description": "Artemis II visualization lead Ernie Wright explains how his data-driven animations are helping astronauts to prepare for a historic flyby of the Moon.Complete transcript available.Universal Production Music: “Black Cloud” and “Magic Trick” by Hugo Dubery [SACEM] and Philippe Galtier [SACEM]; “Connecting Ideas” by Christopher Timothy White [PRS]; “Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS]Watch this video on the NASA Goddard YouTube channel and Facebook. || Artemis-Sci-Wright-A2Sim-Thumbnail_print.jpg (1024x576) [102.1 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail.jpg (1920x1080) [533.4 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail.png (1920x1080) [1.2 MB] || Artemis-Sci-Wright-A2Sim-Thumbnail_searchweb.png (320x180) [64.7 KB] || Artemis-Sci-Wright-A2Sim-Thumbnail_thm.png (80x40) [6.2 KB] || 14938_Artemis_Sci_Wright_A2Sim_720.mp4 (1280x720) [93.2 MB] || 14938_Artemis_Sci_Wright_A2Sim_1080.mp4 (1920x1080) [520.8 MB] || ArtemisSciWrightA2SimCaptions.en_US.srt [9.1 KB] || ArtemisSciWrightA2SimCaptions.en_US.vtt [8.7 KB] || 14938_Artemis_Sci_Wright_A2Sim_4K.mp4 (3840x2160) [3.2 GB] || 14938_Artemis_Sci_Wright_A2Sim_ProRes.mov (3840x2160) [20.2 GB] || ", "hits": 2422 }, { "id": 14932, "url": "https://svs.gsfc.nasa.gov/14932/", "result_type": "Produced Video", "release_date": "2025-12-02T08:00:00-05:00", "title": "Bio-Essential Sugars Discovered in Samples from Asteroid Bennu", "description": "OSIRIS-REx Project Scientist Daniel Glavin discusses the discovery of ribose and glucose in samples of asteroid Bennu, and the implications for the formation and evolution of life on Earth.Complete transcript available.Watch this video on the NASA.gov Video YouTube channel. || Bennu-Sugars-Thumbnail_print.jpg (1024x576) [175.2 KB] || Bennu-Sugars-Thumbnail.jpg (1280x720) [534.2 KB] || Bennu-Sugars-Thumbnail.png (1280x720) [892.3 KB] || Bennu-Sugars-Thumbnail_searchweb.png (320x180) [77.4 KB] || Bennu-Sugars-Thumbnail_thm.png (80x40) [6.8 KB] || 14932_Bennu_Sugars_Interview_Glavin_720.mp4 (1280x720) [180.6 MB] || 14932_Bennu_Sugars_Interview_Glavin_1080.mp4 (1920x1080) [1011.6 MB] || BennuSugarsGlavinCaptionsV2.en_US.srt [18.4 KB] || BennuSugarsGlavinCaptionsV2.en_US.vtt [17.5 KB] || 14932_Bennu_Sugars_Interview_Glavin_4K.mp4 (3840x2160) [6.2 GB] || 14932_Bennu_Sugars_Interview_Glavin_ProRes.mov (3840x2160) [47.0 GB] || ", "hits": 259 }, { "id": 14922, "url": "https://svs.gsfc.nasa.gov/14922/", "result_type": "Produced Video", "release_date": "2025-12-01T14:00:00-05:00", "title": "Anatomy of an Active Galactic Nucleus", "description": "An active galactic nucleus, or AGN, is a supermassive black hole at the center of a galaxy that is consuming surrounding matter. Although the black hole itself is not visible, the structures around it emit light across many wavelengths. The artist’s concepts here highlight distinct structures that can accompany an AGN — the photon ring, accretion disk, corona, dusty torus, and relativistic jets. || ", "hits": 436 }, { "id": 14905, "url": "https://svs.gsfc.nasa.gov/14905/", "result_type": "Produced Video", "release_date": "2025-11-28T09:00:00-05:00", "title": "Black Hole Environments, Explained", "description": "If light can’t escape black holes, how do we know where they are? The regions around them tell an incredible story. From blazing coronas and swirling accretion disks to powerful jets that stretch millions of miles, these extreme environments reveal black holes' secrets and how these mysterious objects shape the universe.Join host Sophia Roberts as she talks with researchers Jenna Cann and Cecilia Chirenti at NASA Goddard about how scientists study these mysterious structures, the challenges of observing the unseeable, and the discoveries that continue to change our understanding of black holes.Credit: NASA’s Goddard Space Flight CenterMusic credits from Universal Production Music:\"Breaking the Barrier,\" David Bertrand Holland\"Dust Spirals,\" Alexandre Prodhomme\"Miniature Universe,\" Geoffrey Wilkinson\"Urban Decay,\" Sarah Natasha Penelope Warne\"Solar Plexus,\" Brandon Seliga\"Polygraph,\" Eric Chevalier\"The Mischief Makers,\" Joaquim Badia\"Maelstrom Dream,\" Lucie Rose\"The Truth Will Out,\" Chris Dony and Beth Perry || 14905_-_BHE_Thumbnail.jpg (1280x720) [947.8 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.srt [15.7 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.vtt [14.8 KB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_1080.mp4 (1920x1080) [1.7 GB] || FINAL_-_14905_Black_Hole_Enviroments_Explained_4k.mp4 (3840x2160) [9.2 GB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_ProRes.mov (3840x2160) [39.3 GB] || ", "hits": 227 }, { "id": 14818, "url": "https://svs.gsfc.nasa.gov/14818/", "result_type": "Produced Video", "release_date": "2025-09-26T12:00:00-04:00", "title": "Plunge: Behind the Scenes Creating NASA's Black Hole Visualization", "description": "Behind the scenes video about the Black Hole visualization from 2024", "hits": 384 }, { "id": 14583, "url": "https://svs.gsfc.nasa.gov/14583/", "result_type": "Produced Video", "release_date": "2024-05-08T00:00:00-04:00", "title": "Artemis & JETT5 Interview with Kelsey Young", "description": "Dr. Kelsey Young is the Artemis Science Flight Operations Lead and works at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.Complete transcript available.Dr. Young discusses the JETT5 mission, which was conducted May 13-17. During JETT5, astronauts performed a series of simulated moonwalks in the San Francisco Volcanic Field near Flagstaff, Arizona, while flight controllers and scientists at NASA’s Johnson Space Center in Houston, Texas guided and provided feedback on their progress. JETT5 was designed to prepare crew members for the historic Artemis III mission that will land near the Moon’s south pole.00:00:00:00 – What is your role in NASA’s Artemis missions?00:00:58:03 – What was the JETT5 mission, and what activities did it include?00:01:49:03 – Why are mission simulations like JETT5 critical?00:02:32:20 – Why was Arizona chosen as the site of the JETT5 field test?00:03:44:18 – Why were the field tests conducted both in daytime and at night?00:04:39:13 – Where were Mission Control team members and scientists located?00:05:21:26 – What is the Science Evaluation Room for the Artemis missions?00:06:10:17 – What are the activities and roles within the Science Evaluation Room?00:06:49:00 – What science payloads will the Artemis crew deploy on the lunar surface?00:07:22:28 – What goes into creating a scientifically well-trained crew member? || Kelsey_Young_Interview_Preview_print.jpg (1024x576) [89.8 KB] || Kelsey_Young_Interview_Preview.png (3840x2160) [11.8 MB] || Kelsey_Young_Interview_Preview.jpg (3840x2160) [2.7 MB] || Kelsey_Young_Interview_Preview_searchweb.png (320x180) [76.3 KB] || Kelsey_Young_Interview_Preview_thm.png (80x40) [6.6 KB] || Kelsey_Young_Interview_JETT5_720.mp4 (1280x720) [122.5 MB] || Kelsey_Young_Interview_JETT5_1080.mp4 (1920x1080) [685.7 MB] || KelseyYoungInterviewJETT5.en_US.srt [14.0 KB] || KelseyYoungInterviewJETT5.en_US.vtt [13.4 KB] || Kelsey_Young_Interview_JETT5_4K.mp4 (3840x2160) [4.2 GB] || Kelsey_Young_Interview_JETT5_ProRes.mov (3840x2160) [32.5 GB] || ", "hits": 620 }, { "id": 14347, "url": "https://svs.gsfc.nasa.gov/14347/", "result_type": "B-Roll", "release_date": "2023-07-13T00:00:00-04:00", "title": "Unfolding the Universe with Webb", "description": "NASA's James Webb Space Telescope is unfolding the universe, and revealing sights humanity has never seen before. In this video, astronomers describe working with the telescope and how the images and data are collected. From first images to routine operations: experts at the Space Telescope Science Institute in Baltimore, MD explain how the images are processed, and turned from raw data to the spectacular full-color images seen on the internet. || ", "hits": 75 }, { "id": 14217, "url": "https://svs.gsfc.nasa.gov/14217/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Creating Black Hole Jets With a NASA Supercomputer", "description": "New simulations carried out on the NASA Center for Climate Simulation’s Discover supercomputer show how weaker, low-luminosity jets produced by a galaxy's monster black hole interact with their galactic environment. Because these jets are more difficult to detect, the simulations help astronomers link these interactions to features they can observe, such as various gas motions and optical and X-ray emissions.Credit: NASA's Goddard Space Flight CenterMusic credit: \"Lost Time;\" \"Ascension;\" \"Flowing Cityscape;\" \"Jupiter's Eye;\" \"Pizzicato Piece;\" \"Facts;\" \"Final Words\" all from Universal Production MusicVideo Descriptive Text available.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14217_AGN_OUtflow_Still.jpg (1920x1080) [1.0 MB] || 14217_AGN_OUtflow_Still_searchweb.png (320x180) [92.9 KB] || 14217_AGN_OUtflow_Still_thm.png (80x40) [6.7 KB] || 14217_AGN_Outflow_FINAL_1080.webm (1920x1080) [67.5 MB] || AGN_Outflow_SRT_Captions.en_US.srt [11.4 KB] || 14217_AGN_Outflow_FINAL_1080.mp4 (1920x1080) [632.4 MB] || 14217_AGN_Outflow_FINAL_1080_Best.mp4 (1920x1080) [1.5 GB] || 14217_AGN_Outflow_FINAL_ProRes_1920x1080_24.mov (1920x1080) [6.4 GB] || ", "hits": 205 }, { "id": 14226, "url": "https://svs.gsfc.nasa.gov/14226/", "result_type": "B-Roll", "release_date": "2022-10-12T00:00:00-04:00", "title": "Lee Feinberg Interview for Webb First Evaluation Image", "description": "Interview with Lee Feinberg regarding Webb's first evaluation image. || Lee_Feinberg_Interview_Cover_Image_print.jpg (1024x574) [131.9 KB] || Lee_Feinberg_Interview_Cover_Image.png (3340x1874) [8.2 MB] || Lee_Feinberg_Interview_Cover_Image_searchweb.png (320x180) [104.6 KB] || Lee_Feinberg_Interview_Cover_Image_thm.png (80x40) [11.2 KB] || Lee_Feinberg_Interview_for_Webb_First_Evaluation_Image_HD.mov (1920x1080) [4.5 GB] || Lee_Feinberg_Interview_for_Webb_First_Evaluation_Image_HD.mp4 (1920x1080) [985.4 MB] || Lee_Feinberg_Interview_for_Webb_First_Evaluation_Image_HD.webm (1920x1080) [54.3 MB] || Lee_Feinberg_Interview_for_Webb_First_Evaluation_Image_4K.mov (4608x2592) [29.7 GB] || Lee_Feinberg_Interview_for_Webb_First_Evaluation_Image_4K.mp4 (4608x2592) [984.7 MB] || ", "hits": 39 }, { "id": 13908, "url": "https://svs.gsfc.nasa.gov/13908/", "result_type": "Produced Video", "release_date": "2021-08-09T13:00:00-04:00", "title": "Exploring Asteroid Bennu Through Technology", "description": "Learn how “Tour of Asteroid Bennu” was created using data from OSIRIS-REx.Complete transcript available.Universal Production Music: “Spindrift” by Max Cameron Concors; “Unearthing Dark Secrets” by Andrew Joseph Carpenter and Mark Richmond PhillipsWatch this video on the NASA Goddard YouTube channel. || MakingTourBennuPreviewV4_print.jpg (1024x576) [133.2 KB] || MakingTourBennuPreviewV4.png (1920x1080) [1.9 MB] || MakingTourBennuPreviewV4.jpg (1920x1080) [753.9 KB] || MakingTourBennuPreviewV4_thm.png (80x40) [6.2 KB] || MakingTourBennuPreviewV4_searchweb.png (320x180) [81.7 KB] || TWITTER_720_13908_Making_Tour_Bennu_MASTER_twitter_720.mp4 (1280x720) [38.1 MB] || 13908_Making_Tour_Bennu_MASTER.webm (960x540) [87.9 MB] || FACEBOOK_720_13908_Making_Tour_Bennu_MASTER_facebook_720.mp4 (1280x720) [233.4 MB] || 13908_Making_Tour_Bennu_YouTube.mp4 (1920x1080) [990.0 MB] || 13908_Making_Tour_Bennu_Captions_V2.en_US.srt [6.2 KB] || 13908_Making_Tour_Bennu_Captions_V2.en_US.vtt [6.0 KB] || 13908_Making_Tour_Bennu_MASTER.mov (1920x1080) [3.0 GB] || ", "hits": 88 }, { "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": 158 }, { "id": 13608, "url": "https://svs.gsfc.nasa.gov/13608/", "result_type": "Produced Video", "release_date": "2020-05-22T10:00:00-04:00", "title": "NASA Names Upcoming Telescope to Honor the \"Mother of Hubble\"", "description": "Learn about Nancy Grace Roman, her contribution to NASA missions, and how NASA has honored her.Credit: NASA's Goddard Space Flight CenterMusic: \"Rising Tides\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NGR_Still_1.jpg (1920x1080) [1023.4 KB] || NGR_Still_1_searchweb.png (320x180) [100.8 KB] || NGR_Still_1_thm.png (80x40) [7.6 KB] || Roman_Biography_ProRes_1920x1080_2997.mov (1920x1080) [2.9 GB] || Roman_Biography_Best_1080.mp4 (1920x1080) [956.8 MB] || Roman_Biography_1080.mp4 (1920x1080) [330.8 MB] || Roman_Biography_1080.webm (1920x1080) [23.7 MB] || Roman_Biography_SRT_Captions.en_US.srt [4.0 KB] || Roman_Biography_SRT_Captions.en_US.vtt [4.0 KB] || ", "hits": 48 }, { "id": 13587, "url": "https://svs.gsfc.nasa.gov/13587/", "result_type": "Produced Video", "release_date": "2020-04-21T10:00:00-04:00", "title": "Tale of Two Telescopes: HST and WFIRST", "description": "AstrophysicsComplete transcript available. || Astrophysics.00144_print.jpg (1024x576) [113.3 KB] || Astrophysics.00144_searchweb.png (320x180) [82.1 KB] || Astrophysics.00144_thm.png (80x40) [6.6 KB] || Astrophysics.mp4 (1920x1080) [331.7 MB] || Astrophysics.mov (1920x1080) [3.3 GB] || Astrophysics.webm (1920x1080) [36.0 MB] || AStrophysics_SRT_Captions.en_US.srt [6.2 KB] || AStrophysics_SRT_Captions.en_US.vtt [6.3 KB] || ", "hits": 36 }, { "id": 13207, "url": "https://svs.gsfc.nasa.gov/13207/", "result_type": "Produced Video", "release_date": "2019-07-12T10:00:00-04:00", "title": "OSIRIS-REx Social Media Interviews", "description": "This page contains interviews with personnel from the Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) mission, edited for social media. The OSIRIS-REx spacecraft launched Sept. 8, 2016, and began orbiting asteroid Bennu on Dec. 31, 2018. Its primary science objective is to study Bennu and collect a sample for return to Earth in 2023. Bennu is a carbon-rich asteroid that records the earliest history of our solar system, and which may contain the raw ingredients of life. || ", "hits": 30 }, { "id": 12166, "url": "https://svs.gsfc.nasa.gov/12166/", "result_type": "Produced Video", "release_date": "2018-12-03T00:00:00-05:00", "title": "OSIRIS-REx Mission Arrives at Asteroid Bennu", "description": "OSIRIS-REx mission team members capture the excitement of arriving at asteroid Bennu. Music provided by Killer Tracks: Distant Echoes, Game Show Sphere 9Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 12166_Bennu_Arrival_Preview_print.jpg (1024x576) [101.3 KB] || 12166_Bennu_Arrival_Preview.jpg (1920x1080) [319.2 KB] || 12166_Bennu_Arrival_Preview_searchweb.png (320x180) [45.2 KB] || 12166_Bennu_Arrival_Preview_thm.png (80x40) [4.1 KB] || FACEBOOK_720_12166_OSIRIS-REx_Arrival_Bennu_MASTER_facebook_720.mp4 (1280x720) [473.9 MB] || TWITTER_720_12166_OSIRIS-REx_Arrival_Bennu_MASTER_twitter_720.mp4 (1280x720) [74.9 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.webm (960x540) [174.0 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.mov (3840x2160) [25.0 GB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.mp4 (3840x2160) [5.7 GB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small.mp4 (3840x2160) [490.1 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small_Output.en_US.srt [11.2 KB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small_Output.en_US.vtt [11.2 KB] || ", "hits": 57 }, { "id": 13023, "url": "https://svs.gsfc.nasa.gov/13023/", "result_type": "Produced Video", "release_date": "2018-10-22T00:00:00-04:00", "title": "Elegance: Music & Math", "description": "This past summer, sometimes before the start of the work day, Goddard interns Philip Lu and Gabriel Apaza played impromptu classical piano concerts on the Steinway in the Hinners Auditorium, tackling masters such as Liszt, Debussy, Bach, Schubert and Chopin.Lu is a physics doctoral student at UCLA. Apaza is a rising senior at Michigan State studying computer science and engineering with a math minor. Both agree that music and mathematics share a commonality of elegance and problem-solving. In this video, they explain how. || Elegance_Music_Math_V2.00001_print.jpg (1024x576) [3.8 KB] || Elegance_Music_Math_V2.00001_searchweb.png (320x180) [3.0 KB] || Elegance_Music_Math_V2.00001_thm.png (80x40) [594 bytes] || Elegance_Music_Math.mov (1920x1080) [7.2 GB] || Elegance_Music_Math.mp4 (1920x1080) [289.6 MB] || Elegance_Music_Math.webm (1920x1080) [30.6 MB] || Elegance_Music_Math_V2.en_US.srt [4.3 KB] || Elegance_Music_Math_V2.en_US.vtt [4.4 KB] || ", "hits": 26 }, { "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": 245 }, { "id": 12501, "url": "https://svs.gsfc.nasa.gov/12501/", "result_type": "Produced Video", "release_date": "2017-02-14T09:30:00-05:00", "title": "Raven is Heading to the International Space Station", "description": "The future of autonomous navigation capability is getting closer to being a reality. Killer Tracks Music Library: UPM_NM288_30_Unveiling_Courage_Main_Track_367199 || RAVEN.png (1920x1080) [2.4 MB] || RAVEN_print.jpg (1024x576) [85.7 KB] || RAVEN_searchweb.png (320x180) [81.9 KB] || RAVEN_web.png (320x180) [81.9 KB] || RAVEN_thm.png (80x40) [5.7 KB] || Raven_Teaser_FINAL.mov (1920x1080) [2.0 GB] || Raven_Teaser_FINAL.mp4 (1920x1080) [106.2 MB] || Raven_Teaser_FINAL_appletv.m4v (1280x720) [32.9 MB] || Raven_Teaser_FINAL_youtube_hq.mov (1920x1080) [355.3 MB] || Raven_Teaser_FINAL.webmhd.webm (1080x606) [14.2 MB] || Raven_Teaser_FINAL_large.mp4 (1920x1080) [75.5 MB] || Raven_Teaser_FINAL_appletv_subtitles.m4v (1280x720) [32.9 MB] || Raven_Teaser_FINAL.en_US.srt [1.4 KB] || Raven_Teaser_FINAL.en_US.vtt [1.4 KB] || ", "hits": 20 }, { "id": 12502, "url": "https://svs.gsfc.nasa.gov/12502/", "result_type": "Produced Video", "release_date": "2017-02-13T11:00:00-05:00", "title": "Coming soon: The latest Tracking and Data Relay Satellite, TDRS-M", "description": "TDRS-M will be the 12th satellite the TDRS team has launched since 1983. || TDRS_M_Teaser_FINAL.02143_print.jpg (1024x576) [31.6 KB] || TDRS_M_Teaser_FINAL.02143_searchweb.png (320x180) [42.2 KB] || TDRS_M_Teaser_FINAL.02143_thm.png (80x40) [3.8 KB] || TDRS_M_Teaser_FINAL.mov (1920x1080) [1.3 GB] || TDRS_M_Teaser_FINAL_youtube_hq.mov (1920x1080) [144.6 MB] || TDRS_M_Teaser_FINAL.mp4 (1920x1080) [74.7 MB] || TDRS_M_Teaser_FINAL_appletv_subtitles.m4v (1280x720) [24.8 MB] || TDRS_M_Teaser_FINAL_appletv.m4v (1280x720) [24.8 MB] || TDRS_M_Teaser_FINAL.webmhd.webm (1080x606) [6.9 MB] || TDRS_M_Teaser_FINAL.en_US.srt [308 bytes] || TDRS_M_Teaser_FINAL.en_US.vtt [294 bytes] || ", "hits": 33 }, { "id": 12347, "url": "https://svs.gsfc.nasa.gov/12347/", "result_type": "Produced Video", "release_date": "2016-08-23T00:00:00-04:00", "title": "OSIRIS-REx Interview Clips", "description": "This resource page contains broadcast-quality interview clips about the OSIRIS-REx mission. Clips are available for download in both Apple ProRes and H.264 versions. || ", "hits": 31 }, { "id": 12309, "url": "https://svs.gsfc.nasa.gov/12309/", "result_type": "Produced Video", "release_date": "2016-07-25T10:00:00-04:00", "title": "OSIRIS-REx Technology: OVIRS", "description": "OSIRIS-REx will use its visible and infrared spectrometer (OVIRS) to study the chemical composition of Bennu, a near-Earth asteroid that may hold clues to the origins of life.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || OvirsPreview3.jpg (1920x1080) [859.9 KB] || OvirsPreview3_searchweb.png (320x180) [122.7 KB] || OvirsPreview3_thm.png (80x40) [8.7 KB] || 12309_OVIRS_Profile_APR.mov (1920x1080) [8.7 GB] || 12309_OVIRS_Profile_large.mp4 (1920x1080) [340.1 MB] || 12309_OVIRS_Profile_H264.mp4 (1280x720) [340.6 MB] || 12309_OVIRS_Profile_appletv.m4v (1280x720) [169.3 MB] || 12309_OVIRS_Profile.webm (960x540) [135.6 MB] || 12309_OVIRS_Profile_appletv_subtitles.m4v (1280x720) [169.4 MB] || 12309_OVIRS_Profile_APR_Output.en_US.srt [7.0 KB] || 12309_OVIRS_Profile_APR_Output.en_US.vtt [7.0 KB] || 12309_OVIRS_Profile_ipod_sm.mp4 (320x240) [58.3 MB] || ", "hits": 156 }, { "id": 12264, "url": "https://svs.gsfc.nasa.gov/12264/", "result_type": "Produced Video", "release_date": "2016-06-07T09:30:00-04:00", "title": "LISA Pathfinder Spaceflight Experiment a Rousing Success", "description": "The LISA Pathfinder mission is an ESA-led effort to demonstrate technologies for a future gravitational wave observatory in space. NASA Goddard astrophysicist Ira Thorpe, a member of the team, discusses the mission and its spectacular results so far. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || LPF_Still.png (1920x1080) [3.1 MB] || LPF_Still_print.jpg (1024x576) [110.1 KB] || LPF_Still_searchweb.png (320x180) [98.0 KB] || LPF_Still_thm.png (80x40) [9.8 KB] || 12264_LISA_Pathfinder_Final_ProRes_1920x1080_2997.mov (1920x1080) [3.6 GB] || YOUTUBE_HQ_12264_LISA_Pathfinder_Final_youtube_hq.mov (1920x1080) [1.2 GB] || 12264_LISA_Pathfinder_Final-HD_1080p.mov (1920x1080) [409.0 MB] || 12264_LISA_Pathfinder_Final-Apple_Devices_HD_Best.m4v (1920x1080) [272.7 MB] || 12264_LISA_Pathfinder_Final_appletv.m4v (1280x720) [138.6 MB] || 12264_LISA_Pathfinder_Final_large.mp4 (1920x1080) [278.0 MB] || 12264_LISA_Pathfinder_Final_appletv_subtitles.m4v (1280x720) [138.7 MB] || 12264_LISA_Pathfinder_Final_appletv.webm (1280x720) [24.4 MB] || 12264_LISA_Pathfinder_SRT_Captions.en_US.srt [5.6 KB] || 12264_LISA_Pathfinder_SRT_Captions.en_US.vtt [5.6 KB] || ", "hits": 67 }, { "id": 12019, "url": "https://svs.gsfc.nasa.gov/12019/", "result_type": "Produced Video", "release_date": "2016-01-07T14:15:00-05:00", "title": "NASA's Fermi Mission Sharpens its High-energy View", "description": "Tour the best view of the high-energy gamma-ray sky yet seen. This video highlights the plane of our galaxy and identifies objects producing gamma rays with energies greater than 1 TeV. Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here.Credit: NASA's Goddard Space Flight Center || 2FHL_Still_print.jpg (1024x576) [66.4 KB] || 2FHL_Still.png (3840x2160) [19.0 MB] || 2FHL_Still_searchweb.png (320x180) [55.9 KB] || 2FHL_Still_thm.png (80x40) [5.5 KB] || 12019_2FHL_H264_Good_1920x1080_2997.mov (1920x1080) [39.6 MB] || 12019_2FHL_H264_Good_1920x1080_2997.webm (1920x1080) [9.9 MB] || 12019_2FHL_3840x2160_FINAL_appletv.m4v (1280x720) [49.2 MB] || 12019_2FHL_3840x2160_FINAL_appletv_subtitles.m4v (1280x720) [49.3 MB] || 12019_2FHL_SRT_Captions.en_US.srt [330 bytes] || 12019_2FHL_SRT_Captions.en_US.vtt [343 bytes] || 12019_2FHL_3840x2160_2997_20mbps.mp4 (3840x2160) [190.4 MB] || 12019_2FHL_3840x2160_2997_40mbps.mp4 (3840x2160) [371.2 MB] || 12019_2FHL_3840x2160_FINAL_lowres.mp4 (480x272) [13.0 MB] || NASA_PODCAST_12019_2FHL_3840x2160_FINAL_ipod_sm.mp4 (320x240) [17.8 MB] || 12019_2FHL_ProRes_3840x2160_2997.mov (3840x2160) [3.8 GB] || ", "hits": 37 }, { "id": 12065, "url": "https://svs.gsfc.nasa.gov/12065/", "result_type": "Produced Video", "release_date": "2015-11-18T10:00:00-05:00", "title": "Lesley Ott: Carbon and Climate Soundbite", "description": "Lesley Ott, research meteorologist in the Global Modeling and Assimilation Center at NASA's Goddard Space Flight Center, discusses how NASA is working to understand the global carbon cycle. Dr. Ott made these points on a media telecon in advance of the United Nations COP-21 climate meeting in Paris, 2015.For complete transcript, click here.Music credit: Piano Dreams by Jon Wygens || Lesley_Ott_Poster-no_text.jpg (1280x720) [219.6 KB] || Lesley_Ott_Poster-no_text_searchweb.png (320x180) [82.4 KB] || Lesley_Ott_Poster-no_text_thm.png (80x40) [17.1 KB] || Lesley_Ott_MASTER_prores.mov (1280x720) [596.5 MB] || Lesley_Ott_MASTER_youtube_hq.mov (1280x720) [137.3 MB] || Lesley_Ott_MASTER_appletv.m4v (1280x720) [20.8 MB] || Lesley_Ott_Carbon_Climate.mp4 (1280x720) [41.2 MB] || Lesley_Ott_MASTER.mpeg (1280x720) [140.0 MB] || Lesley_Ott_MASTER.webm (960x540) [16.7 MB] || Lesley_Ott_MASTER_appletv_subtitles.m4v (1280x720) [20.9 MB] || 12065_Lesley_Ott-captions.en_US.srt [953 bytes] || 12065_Lesley_Ott-captions.en_US.vtt [963 bytes] || Lesley_Ott_MASTER_ipod_sm.mp4 (320x240) [7.2 MB] || ", "hits": 17 }, { "id": 12035, "url": "https://svs.gsfc.nasa.gov/12035/", "result_type": "Produced Video", "release_date": "2015-10-28T11:00:00-04:00", "title": "Brazil’s Extreme Drought Seen From Space", "description": "Empty water reservoirs, severe water rationing, and electrical blackouts are the new status quo in major cities across southeastern Brazil where the worst drought in 35 years has desiccated the region. A new NASA study estimates that the region has lost an average of 15 trillion gallons of water per year from 2012 to 2015. Eastern Brazil as a whole has lost on average 28 trillion gallons of water per year over the same time period.Augusto Getirana, a hydrologist at NASA's Goddard Space Flight Center, in Greenbelt, Maryland, analyzed the amount of water stored in aquifers and rivers across Brazil from 2002 to 2015, interested in understanding the depth of the current drought.A new data visualization of 13 years of GRACE data shows the distribution of water across Brazil. Blues indicate increases in water, mostly occurring in the western regions of Brazil in the rainforest. Meanwhile red and orange shows where water stores have declined, occurring mainly in the north and southeast. At the beginning of the data collection, in 2002, Brazil was just coming out of a drought that began in 2000. A wet period followed until 2012 when dry conditions set in again due to a lack of precipitation and higher than usual temperatures, according to supplemental data.Southeastern Brazil was hardest hit by drought conditions, said Getirana. To make matters worse, Brazil relies on rivers that feed into reservoirs and dams that generate about 75 percent of the electrical power for the country. By September 2014, for example, the Cantareira reservoir system that provides water for 8.8 million people in São Paulo's metro region reported that it was filled to 10.7 percent of its total capacity, a situation that has led to major water rationing.Research: Extreme water deficit in Brazil detected from space.Journal: Hydrometeorology, October 27, 2015.Link to paper: http://journals.ametsoc.org/doi/abs/10.1175/JHM-D-15-0096.1Here is the YouTube video.Additional footage from: Itaipu Binacional Files. || ", "hits": 41 }, { "id": 10171, "url": "https://svs.gsfc.nasa.gov/10171/", "result_type": "Produced Video", "release_date": "2014-11-20T14:00:00-05:00", "title": "Swift: A Decade of Game-Changing Astrophysics", "description": "Scientists participating in NASA's Swift mission discuss the spacecraft, the science, and recall their personal experiences as members of the team.Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Swift_Interview_Still_print.jpg (1024x576) [160.8 KB] || Swift_Interview_Still.png (2560x1440) [4.1 MB] || Swift_Interview_Still_web.jpg (180x320) [21.2 KB] || Swift_Interview_Still_thm.png (80x40) [9.1 KB] || Swift_Interview_Still_web.png (320x180) [95.3 KB] || Swift_Interview_Still_searchweb.png (180x320) [95.3 KB] || Swift_10_Interviews_MPEG4_1280X720_2997.mp4 (1280x720) [149.1 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.webmhd.webm (960x540) [98.0 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.m4v (960x540) [257.7 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv_subtitles.m4v (960x540) [257.5 MB] || G2014-067_Swift_10_Interviews_FINAL_1280x720.wmv (1280x720) [292.3 MB] || Swift_10_Interviews_H264_Good_1280x720_2997.mov (1280x720) [551.2 MB] || Swift_10_Interviews_H264_640x360_2997_iPhone.m4v (640x360) [94.6 MB] || G2014-067_Swift_10_Interviews.en_US.srt [11.7 KB] || G2014-067_Swift_10_Interviews.en_US.vtt [11.7 KB] || G2014-067_Swift_10_Interviews_FINAL_ipod_lg.m4v (640x360) [102.9 MB] || G2014-067_Swift_10_Interviews_FINAL_ipod_sm.mp4 (320x240) [51.9 MB] || Swift_10_Interviews_H264_Best_1280x720_5994.mov (1280x720) [3.9 GB] || Swift_10_Interviews_ProRes_1280x720_5994.mov (1280x720) [8.7 GB] || ", "hits": 68 }, { "id": 11668, "url": "https://svs.gsfc.nasa.gov/11668/", "result_type": "Produced Video", "release_date": "2014-10-23T07:00:00-04:00", "title": "Vital Signs: Taking the Pulse of Our Planet", "description": "Our planet is a beautiful and awesome place. In a new video, join NASA scientists on a 40-minute visual tour of Earth from space, presented at the IMAX Theater at National Air and Space Museum in Washington, D.C. on September 10. “Vital Signs: Taking the Pulse of Our Planet\" was the theme for NASA’s Goddard Space Flight Center's fifteenth installment of its annual lecture and reception sponsored by the Maryland Space Business Roundtable. Earth is a complex, dynamic system we do not yet fully understand. Like the human body, the Earth system comprises diverse components that interact in complex ways.On this global tour, scientists lead the viewer through Earth’s water cycle, forests and frozen regions as seen through the eyes of NASA’s Earth observing satellite fleet. They share a story of how we can make life better today and into the future.NASA's Earth science program aims to develop a greater understanding of Earth's system and its response to natural or human-induced changes, and to improve predictions of climate, weather and natural disasters. || ", "hits": 31 }, { "id": 11531, "url": "https://svs.gsfc.nasa.gov/11531/", "result_type": "Produced Video", "release_date": "2014-09-30T14:00:00-04:00", "title": "Swift Catches Mega Flares from a Mini Star", "description": "On April 23, NASA's Swift satellite detected the strongest, hottest, and longest-lasting sequence of stellar flares ever seen from a nearby red dwarf star. The initial blast from this record-setting series of explosions was as much as 10,000 times more powerful than the largest solar flare ever recorded. At its peak, the flare reached temperatures of 360 million degrees Fahrenheit (200 million Celsius), more than 12 times hotter than the center of the sun. The \"superflare\" came from one of the stars in a close binary system known as DG Canum Venaticorum, or DG CVn for short, located about 60 light-years away. Both stars are dim red dwarfs with masses and sizes about one-third of our sun's. They orbit each other at about three times Earth's average distance from the sun, which is too close for Swift to determine which star erupted. At 5:07 p.m. EDT on April 23, the rising tide of X-rays from DG CVn's superflare triggered Swift's Burst Alert Telescope (BAT). Swift turned to observe the source in greater detail with other instruments and, at the same time, notified astronomers around the globe that a powerful outburst was in progress.For about three minutes after the BAT trigger, the superflare's X-ray brightness was greater than the combined luminosity of both stars at all wavelengths under normal conditions.The largest solar explosions are classified as extraordinary, or X class, solar flares based on their X-ray emission. The biggest flare ever seen from the sun occurred in November 2003 and is rated as X 45. But if the flare on DG CVn were viewed from a planet the same distance as Earth is from the sun and measured the same way, it would have been ranked 10,000 times greater, at about X 100,000. How can a star just a third the size of the sun produce such a giant eruption? The key factor is its rapid spin, a crucial ingredient for amplifying magnetic fields. The flaring star in DG CVn rotates in under a day, about 30 or more times faster than our sun. The sun also rotated much faster in its youth and may well have produced superflares of its own, but, fortunately for us, it no longer appears capable of doing so. || ", "hits": 118 }, { "id": 11216, "url": "https://svs.gsfc.nasa.gov/11216/", "result_type": "Produced Video", "release_date": "2014-02-20T11:00:00-05:00", "title": "Black Widow Pulsars Consume Their Mates", "description": "Black widow spiders and their Australian cousins, known as redbacks, are notorious for an unsettling tendency to kill and devour their male partners. Astronomers have noted similar behavior among two rare breeds of binary system that contain rapidly spinning neutron stars, also known as pulsars. The essential features of black widow and redback binaries are that they place a normal but very low-mass star in close proximity to a millisecond pulsar, which has disastrous consequences for the star. Black widow systems contain stars that are both physically smaller and of much lower mass than those found in redbacks.So far, astronomers have found at least 18 black widows and nine redbacks within the Milky Way, and additional members of each class have been discovered within the dense globular star clusters that orbit our galaxy. One black widow system, named PSR J1311-3430 and discovered in 2012, sets the record for the tightest orbit of its class and contains one of the heaviest neutron stars known. The pulsar's featherweight companion, which is only a dozen or so times the mass of Jupiter and just 60 percent of its size, completes an orbit every 93 minutes – less time than it takes to watch most movies. The side of the star facing the pulsar is heated to more than 21,000 degrees Fahrenheit (nearly 12,000 C), or more than twice as hot as the sun's surface. Recent studies allow a range of values extending down to 2 solar masses for the pulsar, making it one of the most massive neutron stars known. Watch the video to learn more about this system and its discovery from some of the scientists involved. || ", "hits": 68 }, { "id": 11457, "url": "https://svs.gsfc.nasa.gov/11457/", "result_type": "Produced Video", "release_date": "2014-01-21T11:00:00-05:00", "title": "GPM: Meet the Team", "description": "This is a series of short profiles that showcase the systems engineers and designers who helped develop, build, and test the Global Precipitation Measurement (GPM) Core Observatory spacecraft. || ", "hits": 27 }, { "id": 11311, "url": "https://svs.gsfc.nasa.gov/11311/", "result_type": "Produced Video", "release_date": "2013-08-21T13:00:00-04:00", "title": "Highlights of Fermi's First Five Years", "description": "This compilation summarizes the wide range of science from the first five years of NASA's Fermi Gamma-ray Space Telescope. Fermi is a NASA observatory designed to reveal the high-energy universe in never-before-seen detail. Launched in 2008, Fermi continues to give astronomers a unique tool for exploring high-energy processes associated with solar flares, spinning neutron stars, outbursts from black holes, exploding stars, supernova remnants and energetic particles to gain insight into how the universe works. Fermi detects gamma rays, the most powerful form of light, with energies thousands to billions of times greater than the visible spectrum.The mission has discovered pulsars, proved that supernova remnants can accelerate particles to near the speed of light, monitored eruptions of black holes in distant galaxies, and found giant bubbles linked to the central black hole in our own galaxy. From blazars to thunderstorms, from dark matter to supernova remnants, catch the highlights of NASA Fermi’s first five years in space.View all the Fermi-related media from the last 5 years in the Fermi Gallery.For more information about Fermi, visit NASA's Fermi webpage. || ", "hits": 36 }, { "id": 11229, "url": "https://svs.gsfc.nasa.gov/11229/", "result_type": "Produced Video", "release_date": "2013-04-30T11:00:00-04:00", "title": "When Fermi Dodged a 1.5-ton Bullet", "description": "NASA scientists don't often learn that their spacecraft is at risk of crashing into another satellite. But when Julie McEnery, the project scientist for NASA's Fermi Gamma-ray Space Telescope, checked her email on March 29, 2012, she found herself facing this precise situation. While Fermi is in fine shape today, continuing its mission to map the highest-energy light in the universe, the story of how it sidestepped a potential disaster offers a glimpse at an underappreciated aspect of managing a space mission: orbital traffic control. As McEnery worked through her inbox, an automatically generated report arrived from NASA's Robotic Conjunction Assessment Risk Analysis (CARA) team based at NASA's Goddard Space Flight Center in Greenbelt, Md. On scanning the document, she discovered that Fermi was just one week away from an unusually close encounter with Cosmos 1805, a dead Cold-War era spy satellite. The two objects, speeding around Earth at thousands of miles an hour in nearly perpendicular orbits, were expected to miss each other by a mere 700 feet.Although the forecast indicated a close call, satellite operators have learned the hard way that they can't be too careful. The uncertainties in predicting spacecraft positions a week into the future can be much larger than the distances forecast for their closest approach. With a speed relative to Fermi of 27,000 mph, a direct hit by the 3,100-pound Cosmos 1805 would release as much energy as two and a half tons of high explosives, destroying both spacecraft. The update on Friday, March 30, indicated that the satellites would occupy the same point in space within 30 milliseconds of each other. Fermi would have to move out of the way if the threat failed to recede. Because Fermi's thrusters were designed to de-orbit the satellite at the end of its mission, they had never before been used or tested, adding a new source of anxiety for the team.By Tuesday, April 3, the close approach was certain, and all plans were in place for firing Fermi's thrusters. The maneuver was performed by the spacecraft based on previously developed procedures. Fermi fired all thrusters for one second and was back doing science within the hour.Watch this video on YouTube. || ", "hits": 64 }, { "id": 10988, "url": "https://svs.gsfc.nasa.gov/10988/", "result_type": "Produced Video", "release_date": "2013-02-08T12:00:00-05:00", "title": "Robotic Refueling Mission", "description": "Robotic refueling is challenging. Before a satellite leaves the ground, technicians fill its fuel tank through a valve that's then triple-sealed and covered with a protective blanket&mdashdesigned never to be accessed again. RRM paves the way for a future robotic servicing mission by demonstrating that a remote-controlled robot can overcome these obstacles to service and refuel a satellite on orbit. A joint effort between NASA and the Canadian Space Agency (CSA), this mission will use the station's robotic arm known as Dextre to conduct these experiments. Normally employed for maintenance of the orbiting superstructure, Dextre becomes experimental hardware in RRM, pushing the limits of robotic teleoperation. It's a first step to making routine robotic servicing on orbit a reality. || ", "hits": 150 }, { "id": 11137, "url": "https://svs.gsfc.nasa.gov/11137/", "result_type": "Produced Video", "release_date": "2013-01-17T12:00:00-05:00", "title": "NASA Beams Mona Lisa to Lunar Reconnaissance Orbiter at the Moon", "description": "As part of the first demonstration of laser communication with a satellite at the moon, scientists with NASA's Lunar Reconnaissance Orbiter (LRO) beamed an image of the Mona Lisa to the spacecraft from Earth.The iconic image traveled nearly 240,000 miles in digital form from the Next Generation Satellite Laser Ranging (NGSLR) Station at NASA's Goddard Space Flight Center in Greenbelt, MD, to the Lunar Orbiter Laser Altimeter (LOLA) instrument on the spacecraft. By transmitting the image piggyback on laser pulses that are routinely sent to track LOLA's position, the team achieved simultaneous laser communication and tracking.To learn more about how it happened, watch the video below! || ", "hits": 48 }, { "id": 20193, "url": "https://svs.gsfc.nasa.gov/20193/", "result_type": "Animation", "release_date": "2012-12-03T12:00:00-05:00", "title": "Curiosity Rover Shakes, Bakes, and Tastes Mars with SAM", "description": "NASA's Curiosity rover analyzed its first solid sample of Mars with a variety of instruments, including the Sample Analysis at Mars (SAM) instrument suite. Developed at NASA's Goddard Space Flight Center in Greenbelt, Md., SAM is a portable chemistry lab tucked inside the Curiosity rover. SAM examines the chemistry of samples it ingests, checking particularly for chemistry relevant to whether an environment can support or could have supported life. Learn more about how SAM processes samples by watching this video! || ", "hits": 37 }, { "id": 11087, "url": "https://svs.gsfc.nasa.gov/11087/", "result_type": "Produced Video", "release_date": "2012-10-19T12:00:00-04:00", "title": "Astronomers Uncover a Surprising Trend in Galaxy Evolution", "description": "A comprehensive study of hundreds of galaxies observed by the Keck telescopes in Hawaii and NASA's Hubble Space Telescope has revealed an unexpected pattern of change that extends back 8 billion years, or more than half the age of the universe.\"Astronomers thought disk galaxies in the nearby universe had settled into their present form by about 8 billion years ago, with little additional development since,\" said Susan Kassin, an astronomer at NASA's Goddard Space Flight Center in Greenbelt, Md., and the study's lead researcher. \"The trend we've observed instead shows the opposite, that galaxies were steadily changing over this time period.\"Today, star-forming galaxies take the form of orderly disk-shaped systems, such as the Andromeda Galaxy or the Milky Way, where rotation dominates over other internal motions. The most distant blue galaxies in the study tend to be very different, exhibiting disorganized motions in multiple directions. There is a steady shift toward greater organization to the present time as the disorganized motions dissipate and rotation speeds increase. These galaxies are gradually settling into well-behaved disks.Blue galaxies — their color indicates stars are forming within them — show less disorganized motions and ever-faster rotation speeds the closer they are observed to the present. This trend holds true for galaxies of all masses, but the most massive systems always show the highest level of organization.Researchers say the distant blue galaxies they studied are gradually transforming into rotating disk galaxies like our own Milky Way.Watch this video on YouTube. || ", "hits": 104 }, { "id": 11036, "url": "https://svs.gsfc.nasa.gov/11036/", "result_type": "Produced Video", "release_date": "2012-09-11T00:00:00-04:00", "title": "Laser Comm: That's a Bright Idea", "description": "Laser light made records obsolete. NASA is on the verge of doing the same thing with space based communications. Before the end of the decade, the Laser Communication Relay Demonstration (LCRD) mission will revolutionize the way we move tons of data from orbit to ground and all around the solar system. || ", "hits": 42 }, { "id": 11051, "url": "https://svs.gsfc.nasa.gov/11051/", "result_type": "Produced Video", "release_date": "2012-07-23T10:00:00-04:00", "title": "Landsat—From the Archives", "description": "The Landsat program is the longest continuous global record of Earth observations from space — ever. On July 23, 1972 NASA launched the first satellite in this program, then known as ERTS, the Earth Resources Technology Satellite and later renamed Landsat 1. In honor of that history, NASA edited together selections of an archive video from 1973 about the ERTS launch.Featured in this 1973 video was a senior geologist at NASA, Nicholas Short, and at Dartmouth College, Robert Simpson and David Lindgren. NASA and the U.S. Department of the Interior through the U.S. Geological Survey (USGS) jointly manage Landsat, and the USGS preserves a nearly 50-year archive of Landsat data that is freely available over the Internet. The next Landsat satellite, known as Landsat 9, is scheduled for launch in 2021.For more information about Landsat visit www.nasa.gov/landsat, or landsat.usgs.govTo watch the entire 23-minute long NASA archive video of the ERTS Launch, go here. || ", "hits": 108 }, { "id": 11045, "url": "https://svs.gsfc.nasa.gov/11045/", "result_type": "Produced Video", "release_date": "2012-07-18T09:00:00-04:00", "title": "The Mars Chamber", "description": "The Mars chamber is a box—about the size of a refrigerator—that re-creates the temperatures, pressures, and atmosphere of the Martian surface, essentially creating a Mars environment on Earth!Scientists and engineers use this chamber to test experiments on the Sample Analysis at Mars (SAM) instrument suite—a fully functioning chemistry lab about the Curiosity Mars rover.By re-creating Mars on Earth and using an exact duplicate of SAM, scientists can \"pre-run\" experiments on SAM to make sure everything will work properly on the Mars rover. Learn more about the Mars chamber by watching this video! || ", "hits": 64 }, { "id": 11017, "url": "https://svs.gsfc.nasa.gov/11017/", "result_type": "Produced Video", "release_date": "2012-06-29T13:00:00-04:00", "title": "Sample Analysis at Mars (SAM) Employee Profiles", "description": "These videos give an inside perspective on what it's like to work on the Sample Analysis at Mars (SAM) suite of instruments! Learn more about the people who work on SAM here. || a010206_sam_dan_carrigan_1280_thm.png (80x40) [15.4 KB] || a010206_sam_dan_carrigan_1280_web.png (320x180) [241.0 KB] || ", "hits": 15 }, { "id": 11018, "url": "https://svs.gsfc.nasa.gov/11018/", "result_type": "Produced Video", "release_date": "2012-06-29T13:00:00-04:00", "title": "Sample Analysis at Mars (SAM) Overview", "description": "This video gives a short overview of the Sample Analysis at Mars (SAM) suite of instruments inside the Curiosity Rover. || ", "hits": 87 }, { "id": 11020, "url": "https://svs.gsfc.nasa.gov/11020/", "result_type": "Produced Video", "release_date": "2012-06-29T13:00:00-04:00", "title": "Sample Analysis at Mars (SAM) Teaser Trailer", "description": "This video is a short teaser trailer for the Sample Analysis at Mars (SAM) instrument suite installed in the Mars Science Laboratory (Curiosity) rover. || a010206_sam_trailer_ipod_lg_thm.png (80x40) [13.4 KB] || a010206_sam_trailer_ipod_lg_web.png (320x180) [169.7 KB] || ", "hits": 12 }, { "id": 11021, "url": "https://svs.gsfc.nasa.gov/11021/", "result_type": "B-Roll", "release_date": "2012-06-29T13:00:00-04:00", "title": "Sample Analysis at Mars (SAM): Broadcast-Quality B-roll", "description": "Below are broadcast-quality b-roll clips of integration, testing, and fabrication of instruments on board the Sample Analysis at Mars (SAM) suite of instruments. || ", "hits": 29 }, { "id": 11022, "url": "https://svs.gsfc.nasa.gov/11022/", "result_type": "Produced Video", "release_date": "2012-06-29T13:00:00-04:00", "title": "Sample Analysis at Mars (SAM): Interview Clips", "description": "This section contains interviews with various Sample Analysis at Mars (SAM) personnel, including Paul Mahaffy, SAM Principal Investigator. || a010206_Pamela_Conrad_sound_bites_ipod_lg_thm.png (80x40) [11.7 KB] || a010206_Pamela_Conrad_sound_bites_ipod_lg_web.png (320x180) [176.1 KB] || ", "hits": 21 }, { "id": 11008, "url": "https://svs.gsfc.nasa.gov/11008/", "result_type": "Produced Video", "release_date": "2012-06-21T16:00:00-04:00", "title": "WMAP—From the Archives", "description": "On June 20, 2012, Dr. Charles Bennett and the WMAP team were awarded the Gruber Cosmology Prize. The Wilkinson Microwave Anisotropy Probe (WMAP) was built and launched by NASA to measure a remnant of the early universe - its oldest light. The conditions of the early times are imprinted on this light. It is the result of what happened earlier, and a backlight for the later development of the universe. This light lost energy as the universe expanded over 13.7 billion years, so WMAP now sees the light as microwaves. By making accurate measurements of microwave patterns, WMAP has answered many longstanding questions about the universe's age, composition and development.This video from Goddard's tape archive features Dr. Bennett after the first results were announced in 2003. || ", "hits": 108 }, { "id": 10964, "url": "https://svs.gsfc.nasa.gov/10964/", "result_type": "Produced Video", "release_date": "2012-06-21T09:00:00-04:00", "title": "Using Quasars to Measure the Earth: A Brief History of VLBI", "description": "VLBI, or Very Long Baseline Interferometry, is a technique that uses multiple radio telescopes to very precisely measure the Earth's orientation. It was originally invented back in the 1960s to take better pictures of quasars, but scientists soon found out that if you threw the process in reverse, you could measure how the ground beneath the telescopes moves around, how long days really are, and how the Earth wobbles on its axis as it revolves around the sun! Learn more about VLBI here!This video is presented in both stereoscopic 3D and standard 2D versions. The labels below will help you pick which video is right for your display! || ", "hits": 51 }, { "id": 11007, "url": "https://svs.gsfc.nasa.gov/11007/", "result_type": "Produced Video", "release_date": "2012-06-20T15:00:00-04:00", "title": "Space Shuttle Discovery Comes to Dulles", "description": "On April 17, 2012 the space shuttle Discovery hitched a ride on the back of a 747 jumbo jet especially designed as a space shuttle transport. It landed at Dulles Airport in Washington, DC, and the process to deliver Discovery to its new home at the Steven F. Udvar-Hazy Center got under way. Through the eyes of a veteran NASA tour guide and aficionado, DJ Emmanuel, we get a behind-the-scenes view of what it was like to be there on such an historic and exciting day! || ", "hits": 36 }, { "id": 10941, "url": "https://svs.gsfc.nasa.gov/10941/", "result_type": "Produced Video", "release_date": "2012-04-24T10:00:00-04:00", "title": "Space Weather FAQ Interviews", "description": "NASA scientists answer some frequently asked questions about the sun, space weather, and the effects on Earth. Each video is one or more scientists responding to the question above it. The videos are available as ProRes files for broadcast use and have had minor audio equalizing and color correction applied.The scientists interviewed are:Dr. Holly Gilbert, NASA HeliophysicistDr. Alex Young, NASA HeliophysicistDr. Phil Chamberlin, NASA Research Heliophysicist and SDO Deputy Project ScientistThere are also two short videos created with this interview content. They are available here.Additional responses to these questions are available upon specific request.For space weather-related footage, animations, and features, visit the Space Weather gallery. || ", "hits": 23 }, { "id": 10959, "url": "https://svs.gsfc.nasa.gov/10959/", "result_type": "Produced Video", "release_date": "2012-04-24T10:00:00-04:00", "title": "NASA Scientists Answer Top Space Weather Questions", "description": "NASA scientists answer some common questions about the sun, space weather, and how they affect the Earth. This is a two-part series.Part One addresses:1. What is space weather?2. What are coronal mass ejections?3. What are solar flares?4. What are solar energetic particles?5. What causes flares and CMEs?Part Two addresses:1. Do all flares and CMEs affect the Earth?2. What happens when a flare or CME hits the Earth?3. How quickly can we feel the effects of space weather?4. Why are there more flares and CMEs happening now?For more information about all these questions and more, visit NASA's Space Weather FAQ.For individual interview responses to frequently asked space weather questions, go here. || ", "hits": 75 }, { "id": 10929, "url": "https://svs.gsfc.nasa.gov/10929/", "result_type": "Produced Video", "release_date": "2012-03-14T10:00:00-04:00", "title": "A Narrated Tour of the Moon", "description": "Although the moon has remained largely unchanged during human history, our understanding of it and how it has evolved over time has evolved dramatically. Thanks to new measurements, we have new and unprecedented views of its surface, along with new insight into how it and other rocky planets in our solar system came to look the way they do. See some of the sights and learn more about the moon here! || ", "hits": 141 }, { "id": 10930, "url": "https://svs.gsfc.nasa.gov/10930/", "result_type": "Produced Video", "release_date": "2012-03-14T10:00:00-04:00", "title": "Evolution of the Moon", "description": "From year to year, the moon never seems to change. Craters and other formations appear to be permanent now, but the moon didn't always look like this. Thanks to NASA's Lunar Reconnaissance Orbiter, we now have a better look at some of the moon's history. Learn more in this video!This entry contains the Evolution of the Moon video in mutliple formats, including stereoscopic 3D in both side-by-side and individual left/right channel versions. It also includes a narrated and non-narrated version. Each individual video is labeled to make it easier to find the version that works for you! || ", "hits": 278 }, { "id": 10910, "url": "https://svs.gsfc.nasa.gov/10910/", "result_type": "Produced Video", "release_date": "2012-02-23T14:00:00-05:00", "title": "Looking Down a Well: A Brief History of Geodesy", "description": "Geodesy is a field of study that deals with the measurement and representation of the Earth, and it all started when a clever human named Eratosthenes discovered that you could measure the circumference of the Earth by looking down a well. Over time, the field of geodesy has expanded and evolved dramatically, and NASA uses technology like radio telescopes, ground surveys, and satellites to contribute! Learn more about geodesy in this video! || ", "hits": 85 }, { "id": 10915, "url": "https://svs.gsfc.nasa.gov/10915/", "result_type": "Produced Video", "release_date": "2012-02-20T11:00:00-05:00", "title": "NASA Spacecraft Reveals Recent Geological Activity on the Moon", "description": "New images acquired by NASA's Lunar Reconnaissance Orbiter (LRO) spacecraft show that the moon's crust is being slightly stretched, forming small valleys - at least in some small areas. High-resolution images obtained by the Lunar Reconnaissance Orbiter Camera (LROC) provide evidence that these valleys are very young, suggesting the moon has experienced relatively recent geologic activity. || ", "hits": 107 }, { "id": 10861, "url": "https://svs.gsfc.nasa.gov/10861/", "result_type": "Produced Video", "release_date": "2011-11-03T14:00:00-04:00", "title": "Fermi Pulsar Interactive Videos", "description": "These videos originally accompanied a Fermi Pulsar Interactive. That interactive is now available here. || ", "hits": 172 }, { "id": 10818, "url": "https://svs.gsfc.nasa.gov/10818/", "result_type": "Produced Video", "release_date": "2011-09-06T10:00:00-04:00", "title": "New LRO Images Offer Sharper Views of Apollo 12, 14, and 17 Sites", "description": "NASA's Lunar Reconnaissance Orbiter (LRO) has captured the sharpest images ever taken from space of the Apollo 12, 14 and 17 sites, revealing the twists and turns of the paths made when the astronauts explored these areas. || ", "hits": 7091 }, { "id": 10784, "url": "https://svs.gsfc.nasa.gov/10784/", "result_type": "Produced Video", "release_date": "2011-07-27T08:00:00-04:00", "title": "Revealing the Old Man in the Sun", "description": "When one moves through 11 SDO images taken at the same time, and shown in order from the lowest temperature material being imaged to the highest, a funny thing thing happens: the features of a face in the sun begin to appear. The movie underscores the fact that images taken at different wavelengths do reveal different features. The images also start at the sun's surface and gradually move out to the sun's upper corona. Enjoy the show! || ", "hits": 34 }, { "id": 10782, "url": "https://svs.gsfc.nasa.gov/10782/", "result_type": "Produced Video", "release_date": "2011-07-22T09:00:00-04:00", "title": "The How-To Guide to Satellites: Putting it Together", "description": "Building satellites isn't easy. They're complex, expensive, and not to mention hard to make! This is why whenever NASA makes a new satellite—like the MAVEN mission to Mars—its scientists and engineers do everything they can to make sure it's done right.Now, putting a satellite together is nothing like putting together, say, an office chair. A single bolt can take hours to install, and you can't even imagine how complex the electronics are! Find out more about the whole process in this video! || ", "hits": 12 }, { "id": 10745, "url": "https://svs.gsfc.nasa.gov/10745/", "result_type": "Produced Video", "release_date": "2011-06-07T09:00:00-04:00", "title": "SDO Catches Surf Waves on the Sun", "description": "Scientists have spotted the iconic surfer's wave rolling through the atmosphere of the sun. This makes for more than just a nice photo-op: the waves hold clues as to how energy moves through that atmosphere, known as the corona. Since scientists know how these kinds of waves — initiated by a Kelvin-Helmholtz instability if you're being technical — disperse energy in the water, they can use this information to better understand the corona. This in turn, may help solve an enduring mystery of why the corona is thousands of times hotter than originally expected.Kelvin-Helmholtz instabilities occur when two fluids of different densities or different speeds flow by each other. In the case of ocean waves, that's the dense water and the lighter air. As they flow past each other, slight ripples can be quickly amplified into the giant waves loved by surfers. In the case of the solar atmosphere, which is made of a very hot and electrically charged gas called plasma, the two flows come from an expanse of plasma erupting off the sun's surface as it passes by plasma that is not erupting. The difference in flow speeds and densities across this boundary sparks the instability that builds into the waves. In order to confirm this description, the team developed a computer model to see what takes place in the region. Their model showed that these conditions could indeed lead to giant surfing waves rolling through the corona. Seeing the big waves suggests they can cascade down to smaller forms of turbulence too. Scientists believe that the friction created by turbulence — the simple rolling of material over and around itself — could help add heating energy to the corona. The analogy is the way froth at the top of a surfing wave provides friction that will heat up the wave. || ", "hits": 25 }, { "id": 10554, "url": "https://svs.gsfc.nasa.gov/10554/", "result_type": "Produced Video", "release_date": "2010-05-24T00:00:00-04:00", "title": "NASA Develops Enhanced Search and Rescue Technologies", "description": "The Search and Rescue Mission Office at the NASA Goddard Space Flight Center, in collaboration with NOAA, Coast Guard, Air Force, and other U.S. agency partners, has developed new technology that will more quickly identify the locations of people in distress and reduce the risk to rescuers. Called the Distress Alerting Satellite System (DASS), this next-generation search and rescue system reduces search times from hours to a few minutes. When it goes online, DASS will be able to almost instantaneously detect and locate distress signals generated by 406 MHz beacons installed on aircraft and vessels or carried by individuals, greatly enhancing the international community's ability to rescue people in distress. || ", "hits": 64 }, { "id": 10560, "url": "https://svs.gsfc.nasa.gov/10560/", "result_type": "Produced Video", "release_date": "2010-01-26T00:00:00-05:00", "title": "Interview Segments with Key Glory Personnel", "description": "The Glory team is comprised of dedicated and highly skilled scientists and engineers. The following interview segments provide comments on the mission from key Glory personnel. Glory is a remote-sensing Earth-orbiting observatory designed to achieve two separate mission objectives. One is to collect data on the chemical, microphysical, and optical properties of aerosols, along with their spatial and temporal distributions. Glory's second mission objective is to continue collection of total solar irradiance data for the long-term climate record. Glory accomplishes these objectives by deploying two instruments aboard a low earth orbit satellite: the Aerosol Polarimetry Sensor (APS) and the Total Irradiance Monitor (TIM). Scientists are working to better understand exactly how and why Earth's climate changes, and the Glory mission will provide significant contributions toward this critical endeavor. || ", "hits": 22 }, { "id": 10433, "url": "https://svs.gsfc.nasa.gov/10433/", "result_type": "Produced Video", "release_date": "2009-05-14T00:00:00-04:00", "title": "LRO Interview: Craig Tooley, Project Manager", "description": "Craig Tooley is the Project Manager for the Lunar Reconnaissance Orbiter (LRO) mission. The following soundbites from Tooley give information about the LRO mission's objectives and importance. || LRO_invu_Tooley_ipod.00078_print.jpg (1024x576) [70.0 KB] || LRO_invu_Tooley_ipod_web.png (320x180) [149.5 KB] || LRO_invu_Tooley_ipod_thm.png (80x40) [11.7 KB] || LRO_invu_Tooley_fullres.webmhd.webm (960x540) [51.0 MB] || LRO_invu_Tooley_fullres.mov (1280x720) [136.3 MB] || LRO_invu_Tooley_prores.mov (1280x720) [3.6 GB] || LRO_invu_Tooley_ipod.m4v (640x360) [43.8 MB] || ", "hits": 13 }, { "id": 10429, "url": "https://svs.gsfc.nasa.gov/10429/", "result_type": "Produced Video", "release_date": "2009-04-29T00:00:00-04:00", "title": "LRO Interview: John Keller, Deputy Project Scientist", "description": "John Keller is the Deputy Project Scientist for the Lunar Reconnaissance Orbiter (LRO) mission. The following soundbites from Keller give information about the LRO mission's objectives and importance. || LRO_invu_Keller_ipod.00352_print.jpg (1024x576) [85.5 KB] || LRO_invu_Keller_ipod_web.png (320x180) [186.1 KB] || LRO_invu_Keller_ipod_thm.png (80x40) [16.0 KB] || LRO_invu_Keller_fullres.webmhd.webm (960x540) [53.1 MB] || LRO_invu_Keller_fullres.mov (1280x720) [146.6 MB] || LRO_invu_Keller_prores.mov (1280x720) [3.7 GB] || LRO_invu_Keller_ipod.m4v (640x360) [43.5 MB] || LRO_invu_Keller_svs.mpg (512x288) [35.1 MB] || ", "hits": 16 }, { "id": 10430, "url": "https://svs.gsfc.nasa.gov/10430/", "result_type": "Produced Video", "release_date": "2009-04-29T00:00:00-04:00", "title": "LRO Interview: Cathy Peddie, Deputy Project Manager", "description": "For more from Cathy Peddie, see entry #10257: Return with LRO. || ", "hits": 33 }, { "id": 10378, "url": "https://svs.gsfc.nasa.gov/10378/", "result_type": "Produced Video", "release_date": "2009-03-24T00:00:00-04:00", "title": "LRO Interview: Rich Vondrak, Project Scientist", "description": "Rich Vondrak is the Project Scientist for the Lunar Reconnaissance Orbiter (LRO) mission. The following soundbites from Vondrak give information about the LRO mission's objectives and importance. || Vondrak_01_intro_640x360.04097_print.jpg (1024x576) [58.3 KB] || Vondrak_01_intro_640x360_web.png (320x180) [170.3 KB] || Vondrak_01_intro_640x360_thm.png (80x40) [16.3 KB] || LRO_invu_Vondrak_fullres.webmhd.webm (960x540) [47.8 MB] || LRO_invu_Vondrak_fullres.mov (1280x720) [142.0 MB] || LRO_invu_Vondrak_prores.mov (1280x720) [3.6 GB] || LRO_invu_Vondrak_ipod.m4v (640x360) [42.6 MB] || LRO_invu_Vondrak_svs.mpg (512x288) [34.1 MB] || ", "hits": 15 }, { "id": 10376, "url": "https://svs.gsfc.nasa.gov/10376/", "result_type": "Produced Video", "release_date": "2009-02-17T12:00:00-05:00", "title": "LRO's Team Spirit with Joanne Baker", "description": "The Lunar Reconnaissance Orbiter (LRO) is the first step to future missions to the Moon, Mars, and beyond. But a lot has to happen before we get there and one woman on the LRO team played a key role in 'putting it together.' || Joanne_Baker_Profile.01252_print.jpg (1024x576) [56.3 KB] || Joanne_Baker_Profile_web.png (320x180) [240.1 KB] || Joanne_Baker_Profile_thm.png (80x40) [16.3 KB] || Joanne_Baker_Profile_AppleTV.webmhd.webm (960x540) [30.2 MB] || Joanne_Baker_Profile_AppleTV.m4v (960x540) [57.0 MB] || Joanne_Baker_Profile.mov (1280x720) [82.9 MB] || Joanne_Baker_Profile.mpg (640x360) [31.5 MB] || Joanne_Baker_Profile_ipod.m4v (640x360) [26.2 MB] || Joanne_Baker_Profile.m4v (320x180) [11.8 MB] || Joanne_Baker_Profile.mp4 (320x240) [6.2 MB] || Joanne_Baker_Profile_SVSsmall.mpg (512x288) [21.1 MB] || Joanne_Baker_Profile.wmv (346x260) [19.4 MB] || ", "hits": 20 } ] }