{ "count": 99, "next": null, "previous": null, "results": [ { "id": 3335, "url": "https://svs.gsfc.nasa.gov/3335/", "result_type": "Visualization", "release_date": "2025-12-31T00:00:00-05:00", "title": "Meteor Crater Topography", "description": "The Earth and Mars are two planets which evolved very differently. By studying locations on Earth whose environment might be similar with that of Mars, scientists are able to theorize about 'the red planet' as well. Meteor Crater is one such study site in the Colorado Plateau, 73 km east of Flagstaff, Arizona. After the meteorite hit the surface of the Arizona desert thousands of years ago, some of the rocks were pushed up along the edge to form a rim around the crater. High resolution (2 m) digital elevation of the site, collected by aerial overflights of the region, is shown here overlain with a natural color IKONOS image. || ", "hits": 150 }, { "id": 14735, "url": "https://svs.gsfc.nasa.gov/14735/", "result_type": "Produced Video", "release_date": "2024-12-16T10:00:00-05:00", "title": "DAVINCI: Venus' Alpha Regio", "description": "Vertical video for sharing on social media platforms.Music is \"Eternal Sapphire\" by Brice Davoli and \"Beyond our Imagination\" by Timothy James Cornick and Matthew Jacob Loveridge of Universal Production Music. || DAVINCI_REEL_THUMB.jpg (1080x1920) [328.4 KB] || DAVINCI_REEL_1.02082_searchweb.png (320x180) [64.8 KB] || DAVINCI_REEL_1.02082_thm.png (80x40) [4.3 KB] || DAVINCI_REEL_1.mp4 (1080x1920) [162.8 MB] || DAVINCI_REEL_1.en_US.srt [3.1 KB] || DAVINCI_REEL_1.en_US.vtt [2.9 KB] || ", "hits": 77 }, { "id": 14582, "url": "https://svs.gsfc.nasa.gov/14582/", "result_type": "Produced Video", "release_date": "2024-05-14T10:00:00-04:00", "title": "DAVINCI Drop Testing at UTTR", "description": "The DAVINCI Project is led by NASA GSFC with primary partners at Lockheed Martin as well as from NASA’s JPL, JHU’s APL, Malin Space Science Systems, NASA’s LaRC, NASA ARC, University of Michigan, and Kinetx.The PI, Deputy PI’s and Program management team are at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The artwork shown here was developed for the DAVINCI team by CI Labs and the SVS. Special data analysis by the PI and Project Science team led by Dr. Jim Garvin, Dr. Stephanie Getty, and Dr. Giada Areny with Dr. Natasha Johnson and Dr. Erika Kohler is included. NASA Langley (LaRC) partners include Dr. S. Dutta and his team who developed the probe aerodynamic drop test experiment for the DAVINCI project. Narration is by Dr. Jim Garvin, PI for the DAVINCI mission to Venus. The DAVINCI Project acknowledges the continuing support of NASA’s Discovery Program, with DAVINCI Program Executive Andrea Riley and Program scientist Nick Lang, and Mission Manager Kevin Sykes. Music is \"Great Secrets\" by Thomas Alexander Farnon of Universal Production Music. || DAVINCI_REEL_THUMB.jpg (1080x1920) [584.4 KB] || DAVINCI_UTTR.01191_searchweb.png (320x180) [71.8 KB] || DAVINCI_UTTR.01191_thm.png (80x40) [6.4 KB] || DAVINCI_UTTR.en_US.srt [2.5 KB] || DAVINCI_UTTR.en_US.vtt [2.3 KB] || DAVINCI_UTTR.mp4 [30.7 MB] || ", "hits": 151 }, { "id": 14505, "url": "https://svs.gsfc.nasa.gov/14505/", "result_type": "Produced Video", "release_date": "2024-01-19T17:00:00-05:00", "title": "Goddard Year In Review 2023", "description": "From our home planet to the farthest reaches of the universe, review top highlights over 2023 from NASA’s Goddard Space Flight Center, the agency’s scientific nerve center. Download a PDF of Goddard’s 2023 year in review booklet at: https://www.nasa.gov/goddard/annual-reports/An interactive version may be browsed at: https://issuu.com/nasagsfc/stacks Goddard is NASA’s premiere space flight complex and home to the nation’s largest organization of scientists, engineers, and technologists who build spacecraft, instruments, and new technology to study Earth, the Sun, our solar system, and the universe. Universal Production Music \"Info Bed Underscore\" \"World Wide Instrumental\" \"Nanotech Instrumental\" \"The Big Rush Instrumental\" \"Unsmiling Seriousness Underscore\" || Goddard_Year_in_Review_Thumbnail.png (1280x720) [1.0 MB] || Goddard_Year_in_Review_Thumbnail_print.jpg (1024x576) [144.4 KB] || Goddard_Year_in_Review_Thumbnail_searchweb.png (320x180) [86.6 KB] || Goddard_Year_in_Review_Thumbnail_thm.png (80x40) [6.4 KB] || GoddardYearInReview2023.en_US.srt [14.5 KB] || GoddardYearInReview2023.en_US.vtt [13.8 KB] || 2023_Goddard_Year_in_Review.webm (3840x2160) [258.1 MB] || Goddard_Year_in_Review_2023_1080.mp4 (1920x1080) [2.5 GB] || 2023_Goddard_Year_in_Review.mp4 (3840x2160) [1.9 GB] || Goddard_Year_in_Review_2023_1080.mov (1920x1080) [16.8 GB] || 2023_Goddard_Year_in_Review.mov (3840x2160) [59.3 GB] || ", "hits": 172 }, { "id": 14415, "url": "https://svs.gsfc.nasa.gov/14415/", "result_type": "Produced Video", "release_date": "2023-09-24T18:00:00-04:00", "title": "OSIRIS-REx Sample Return Broadcast and Landing Highlights", "description": "This page includes multimedia from the OSIRIS-REx sample return broadcast.It will be updated periodically with additional b-roll footage. Date: 9/24/2023 || ", "hits": 182 }, { "id": 14346, "url": "https://svs.gsfc.nasa.gov/14346/", "result_type": "Produced Video", "release_date": "2023-05-30T10:00:00-04:00", "title": "Skywatchers Delight! Venus Will Dazzle In The Night Sky Next Weekend! NASA’s Upcoming DAVINCI Mission Will Take The Plunge into Venus’s Hellish Atmosphere Live Shots", "description": "Quick link to EDITED BROLL for the live shotsQuick link to pre-recorded interview with DR. JIM GARVIN / DAVINCI Principal InvestigatorAdditional still images of Venus from NASA's Magellan and Mariner missions. Credit: NASA/JPLLearn more about VENUS here!!Quick link to pre-recorded interview with MATT GARRISONQuick link to pre-recorded interview with DR LINDSAY HAYS || VENUS.jpeg (1800x720) [220.3 KB] || VENUS_print.jpg (1024x409) [85.9 KB] || VENUS_searchweb.png (320x180) [64.2 KB] || VENUS_thm.png (80x40) [7.4 KB] || ", "hits": 218 }, { "id": 14298, "url": "https://svs.gsfc.nasa.gov/14298/", "result_type": "Produced Video", "release_date": "2023-03-01T09:00:00-05:00", "title": "NASA Prepares to Explore Venus with DAVINCI", "description": "Overview of NASA's DAVINCI Mission.Music is \"Blackened Skies\" by Enrico Cacace and Lorenzo Castellarin of Universal Production Music. || 14298_venus.jpg (1920x1080) [947.8 KB] || DAVINCI_Highlight_14298.04780_searchweb.png (320x180) [79.4 KB] || DAVINCI_Highlight_14298.04780_thm.png (80x40) [5.6 KB] || DAVINCI_Highlight_14298.mp4 (1920x1080) [787.1 MB] || DAVINCI_Highlight_14298.webm (1920x1080) [24.7 MB] || DAVINCI_Highlight_14298.en_US.srt [3.9 KB] || DAVINCI_Highlight_14298.en_US.vtt [3.7 KB] || ", "hits": 77 }, { "id": 14261, "url": "https://svs.gsfc.nasa.gov/14261/", "result_type": "Produced Video", "release_date": "2023-01-19T16:00:00-05:00", "title": "Leaders in Lidar", "description": "In this series, we dive into the legacy of Goddard's lead role in developing laser altimetry, which has revolutionized the way we map our planet, the Moon and other planets. Each chapter looks at the successes and failures of these lidar instruments, beginning with the Mars Observer Laser Altimeter in the late 1980s, through the current generation of laser altimeters on ICESat-2 and GEDI. Through dozens of interviews and archival footage, the history, challenges and legacy of lidar are uncovered. || ", "hits": 144 }, { "id": 14212, "url": "https://svs.gsfc.nasa.gov/14212/", "result_type": "Produced Video", "release_date": "2022-09-20T07:00:00-04:00", "title": "Exploring Venus with DAVINCI", "description": "Watch this video on the NASA Solar System Instagram.Music is \"Arise\" from Jose Tomas Novoa Espinosa and Sebastian Felipe Olivares de Simone of Universal Production Music. || davinci_reel_still_thumb.jpg (2160x3840) [1.3 MB] || davinci_reel_1.00148_searchweb.png (320x180) [22.5 KB] || davinci_reel_1.00148_thm.png (80x40) [2.4 KB] || davinci_reel_1.mp4 (2160x3840) [414.3 MB] || davinci_reel_caption.en_US.srt [1.7 KB] || davinci_reel_caption.en_US.vtt [1.6 KB] || davinci_reel_1.webm (2160x3840) [16.7 MB] || ", "hits": 75 }, { "id": 14214, "url": "https://svs.gsfc.nasa.gov/14214/", "result_type": "Produced Video", "release_date": "2022-09-20T00:00:00-04:00", "title": "How NASA Sees the Life Cycle of Volcanic Island Hunga Tonga-Hunga Ha’apai", "description": "Complete transcript available. || HHTH_Final.00001_print.jpg (1024x576) [78.9 KB] || Thumbnail.png (2838x1588) [5.2 MB] || HHTH_Final.00001_searchweb.png (320x180) [66.5 KB] || HHTH_Final.00001_thm.png (80x40) [5.0 KB] || HHTH_Final.webm (1920x1080) [43.1 MB] || HHTH_Final.mp4 (1920x1080) [779.2 MB] || HHTH_Audio_otter_ai.en_US.srt [7.7 KB] || HHTH_Audio_otter_ai.en_US.vtt [7.7 KB] || ", "hits": 210 }, { "id": 14140, "url": "https://svs.gsfc.nasa.gov/14140/", "result_type": "Produced Video", "release_date": "2022-04-21T00:00:00-04:00", "title": "The Final Day of the Cretaceous: Recent Discoveries by the Tanis research team led by Robert DePalma", "description": "Scientific_Colloquium_DePalma_Final.00001_print.jpg (1024x576) [73.9 KB] || Scientific_Colloquium_DePalma_Final.00001_searchweb.png (320x180) [43.2 KB] || Scientific_Colloquium_DePalma_Final.00001_thm.png (80x40) [4.1 KB] || Scientific_Colloquium_DePalma_Final.mp4 (1920x1080) [12.1 GB] || Scientific_Colloquium_DePalma_Final.webm (1920x1080) [678.8 MB] || Scientific_Colloquium_DePalma_prores.mov (1920x1080) [62.1 GB] || Scientific_Colloquium_DePalma.en_US.srt [178.3 KB] || Scientific_Colloquium_DePalma.en_US.vtt [167.9 KB] || ", "hits": 244 }, { "id": 20351, "url": "https://svs.gsfc.nasa.gov/20351/", "result_type": "Animation", "release_date": "2021-11-09T10:00:00-05:00", "title": "The DAVINCI Mission to Venus", "description": "DAVINCI the Movie || DaVinci1021cut422HQ.00130_print.jpg (1024x438) [75.7 KB] || DaVinci1021cut422HQ.00130_searchweb.png (180x320) [61.3 KB] || DaVinci1021cut422HQ.00130_thm.png (80x40) [5.3 KB] || DaVinci1021cut1080h264.mp4 (1920x820) [208.7 MB] || DaVinci1021cut720422HQ.mov (1682x720) [3.5 GB] || DaVinci1021cut720h264.mp4 (1280x548) [133.2 MB] || DaVinci1021cut720h264.webm (1280x548) [22.0 MB] || DaVinci1021cut422HQ.mov (5045x2160) [20.3 GB] || DaVinci1021cut1080422HQ.mov (2523x1080) [5.6 GB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.srt [3.8 KB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.vtt [3.6 KB] || ", "hits": 158 }, { "id": 13972, "url": "https://svs.gsfc.nasa.gov/13972/", "result_type": "Produced Video", "release_date": "2021-10-20T13:00:00-04:00", "title": "Ten Mysteries of Venus", "description": "Ten mysteries of our sister planet, Venus.Music is \"Spring into Life\" by Oliver Worth of Univeral Production Music.Watch this video on the NASA Goddard YouTube channel. || 13972_mysteriesvenusthumb.jpg (1920x1080) [385.7 KB] || 13972_venusmysteries.01764_searchweb.png (320x180) [65.7 KB] || 13972_venusmysteries.01764_thm.png (80x40) [4.6 KB] || 13972_venusmysteries.mp4 (1920x1080) [299.0 MB] || 13972_venusmysteries_twitter_720.mp4 (1280x720) [53.1 MB] || 13972_venusmysteries_facebook_720.mp4 (1280x720) [317.0 MB] || 13972_venusmysteries_twitter_720.webm (1280x720) [32.1 MB] || 13972_venusmysteries_caption.en_US.srt [6.3 KB] || 13972_venusmysteries_caption.en_US.vtt [5.9 KB] || ", "hits": 323 }, { "id": 13904, "url": "https://svs.gsfc.nasa.gov/13904/", "result_type": "Produced Video", "release_date": "2021-08-05T09:55:00-04:00", "title": "We Asked NASA Scientists and Astronauts \"What is your Favorite Hubble Image?\"", "description": "Over the years, Hubble video producer Paul Morris has had the amazing opportunity to interview some of the brightest minds in astrophysics, and some of the coolest astronauts and people in the world.As a rule, he always asked every single person this one question. Every single time:“What is your favorite Hubble image?”He began to see a pattern in their answers. For more information, visit https://nasa.gov/hubble. Additional Visualizations:Time Lapse of Sun Setting: Pond 5Diatom Movement: Credit: Brenden SeahHubble: Galaxies Across Space and Time: Credit: NASA, ESA and F. Summers (STScI)Music Credits: \"’Children’s Games’ Piece for orchestra\" by Georges Bizet [DP] via Koka Media [SACEM], and Universal Production Music.“Horn Romp” by Oded Fried-Gaon [ACUM] via 10 Miles [ACUM], and Universal Production Music.“Ever Onward” by Joel Goodman [ASCAP] via Medley Lane Music [ASCAP], and Universal Production Music.“Saving Earth” by Enrico Cacace [BMI] and Lorenzo Castellarin [BMI] via Atmosphere Music Ltd. [PRS], and Universal Production Music.“Solaris Planet” by Matthew Nicholson [PRS] and Shin Suzuma [PRS] via Ninja Tune Production Music [PRS], and Universal Production Music.“Dream of Stars” by Magnum Opus [ASCAP] via Sound Pocket Music [PRS], and Universal Production Music.“The Moldau (Exc. My Country)” by Bedrich Smetana [PD] via Koka Media [SACEM], and Universal Production Music. || ", "hits": 301 }, { "id": 13887, "url": "https://svs.gsfc.nasa.gov/13887/", "result_type": "Produced Video", "release_date": "2021-07-27T10:00:00-04:00", "title": "DAVINCI Probe's Eye View", "description": "An overview of the DAVINCI mission through the eyes of the descent probe.Music is \"Mountains of Hokkaido\" by Natalie Holt and Yoann Le Dantec of Universal Production Music || 13887_DAVINCI_PEVAA.02257_print.jpg (1024x576) [101.1 KB] || 13887_thumbnail.jpg (1920x1080) [157.6 KB] || 13887_DAVINCI_PEVAA.02257_searchweb.png (320x180) [69.3 KB] || 13887_DAVINCI_PEVAA.02257_thm.png (80x40) [5.1 KB] || 13887_DAVINCI_PEVAA.mp4 (1920x1080) [177.3 MB] || 13887_DAVINCI_PEVAA_twitter_720.mp4 (1280x720) [32.7 MB] || 13887_DAVINCI_PEVAA_facebook_720.mp4 (1280x720) [190.4 MB] || 13887_DAVINCI_PEVAA.webm (960x540) [47.1 MB] || 13877_DAVINCI_PEVAA_caption.en_US.srt [2.9 KB] || 13877_DAVINCI_PEVAA_caption.en_US.vtt [2.8 KB] || ", "hits": 54 }, { "id": 13878, "url": "https://svs.gsfc.nasa.gov/13878/", "result_type": "Produced Video", "release_date": "2021-07-09T14:00:00-04:00", "title": "Quickshot: Skywatchers Delight! July 12-13 Venus and Mars Will Appear Extra Close To Each Other In Night Sky", "description": "Quick link to associated B-ROLLQuick link to soundbites with Giada Arney / DAVINCI Deputy Principal InvestigatorQuick link to soundbites with Jim Garvin / DAVINCI Principal Investigator || venus.banner3-final.jpg (926x179) [50.5 KB] || venus.banner3-final_print.jpg (1024x197) [50.0 KB] || venus.banner3-final_searchweb.png (320x180) [112.6 KB] || venus.banner3-final_thm.png (80x40) [9.1 KB] || ", "hits": 86 }, { "id": 13640, "url": "https://svs.gsfc.nasa.gov/13640/", "result_type": "Produced Video", "release_date": "2020-07-21T10:00:00-04:00", "title": "Venus in a Minute", "description": "“Venus in a Minute” – a vision for exploration of our mysterious sister planet in response to National Academy of Sciences Decadal priorities that will provide a new window on the evolution of planets in our solar system and beyond. Music Credit: \"Save us All\" by Alec Michael Harrison via Universal Production Music || venus_thumb.jpg (3840x2160) [197.9 KB] || 13640_VIAM_MASTER.01625_searchweb.png (320x180) [26.7 KB] || 13640_VIAM_MASTER.01625_thm.png (80x40) [2.9 KB] || VIAM_MASTER_13640_facebook_720.mp4 (1280x720) [88.2 MB] || VIAM_MASTER_13640_twitter_720.mp4 (1280x720) [15.2 MB] || VIAM_MASTER_13640.webm (960x540) [33.1 MB] || VIAM_MASTER_13640.mp4 (3840x2160) [87.9 MB] || VIAM_caption.en_US.srt [1.5 KB] || VIAM_caption.en_US.vtt [1.5 KB] || ", "hits": 344 }, { "id": 13584, "url": "https://svs.gsfc.nasa.gov/13584/", "result_type": "Produced Video", "release_date": "2020-04-23T10:00:00-04:00", "title": "Venus: Forgotten Sister Planet or Our Next Frontier?", "description": "Dr. James B. Garvin (NASA Goddard Chief Scientist) tells the story of Venus, from early humans to today’s spacecraft, illuminating what may soon be possible and discussing the possibilities for discovery as rich as any in the universe. He believes that deciphering the story which Venus is waiting to tell us will not be easy, but in the words of a US President at the dawn of the space age, we will explore not because it is easy, but because it is “hard”. By exploring our neglected sister (Venus), we will never wait to wonder. Her secrets will inspire and catalyze new understanding of our home world, and impact our destiny as spacefaring people. || venusthumb.jpg (1920x1080) [222.7 KB] || GarvinVenuslecture2.00100_searchweb.png (320x180) [93.8 KB] || GarvinVenuslecture2.00100_thm.png (80x40) [6.9 KB] || GarvinVenuslecture2.mp4 (1920x1080) [583.9 MB] || GarvinVenuslecture2.webm (1920x1080) [250.7 MB] || TWITTER_720_GarvinVenuslecture2_twitter_720.mp4 (1280x720) [268.5 MB] || FACEBOOK_720_GarvinVenuslecture2_facebook_720.mp4 (1280x720) [398.3 MB] || GarvinVenuslecture2.en_US.srt [61.6 KB] || GarvinVenuslecture2.en_US.vtt [58.0 KB] || ", "hits": 59 }, { "id": 13301, "url": "https://svs.gsfc.nasa.gov/13301/", "result_type": "Produced Video", "release_date": "2019-08-29T12:00:00-04:00", "title": "Photon Phriday", "description": "Photon Phriday is a weekly look at what ICESat-2 is measuring as it orbits the Earth. || ", "hits": 148 }, { "id": 13258, "url": "https://svs.gsfc.nasa.gov/13258/", "result_type": "Produced Video", "release_date": "2019-07-15T09:55:00-04:00", "title": "Hubble and Going Forward to the Moon", "description": "We are going forward to the Moon by 2024, but did you know that back in 2005, Dr. Jim Garvin and his team of scientists pointed the Hubble Space Telescope at our nearest celestial neighbor for a very important reason? The Hubble team used the telescope’s powerful instruments to work as a prospector for the Moon’s surface, searching for resources that would help future human-led missions mine and utilize those materials to “live off the land” of the Moon. Hubble’s lunar research led the way for future missions, such as the Lunar Reconnaissance Orbiter, helping men and women to go forward to the Moon by 2024!For more information, visit https://nasa.gov/hubble.Credit: NASA's Goddard Space Flight Center/Paul Morris.Music credits: \"Tracer\" by Max Cameron Concors [ASCAP]; Killer Tracks Production Music. “Insights” by Axel Coon [GEMA], Ralf Goebel [GEMA] Killer Tracks Production Music. “Transitions” by Ben Niblett [PRS], Jon Cotton [PRS] Killer Tracks Production Music. “Interstellar Spacecraft” by JC Lemay [SACEM] Killer Tracks Production Music. || ", "hits": 49 }, { "id": 13184, "url": "https://svs.gsfc.nasa.gov/13184/", "result_type": "Produced Video", "release_date": "2019-04-29T00:00:00-04:00", "title": "Goddard at 60", "description": "On July 29, 1958, President Eisenhower signed the National Aeronautics and Space Act, establishing the National Aeronautics and Space Administration. When it began operations on October 1, 1958, NASA consisted mainly of the four laboratories and some 80 employees of the government's 46-year-old research agency, the National Advisory Committee for Aeronautics (NACA). Goddard Space Flight Center was established on May 1, 1959 as NASA's first space flight center.In celebration of its 60th year, we look back at the innovations and scientific impacts the women and men of Goddard have made throughout its history. || ", "hits": 177 }, { "id": 13191, "url": "https://svs.gsfc.nasa.gov/13191/", "result_type": "Produced Video", "release_date": "2019-04-22T00:00:00-04:00", "title": "NASA Science Live: Our Weird Home (Episode 03)", "description": "NASA Science Live: Our Wierd Home (Episode 03)Program Aired April 22, 2019 || 13191_NSL_Ep03_youtube_720.00476_print.jpg (1024x576) [80.4 KB] || 13191_NSL_Ep03_youtube_720.00476_searchweb.png (320x180) [79.0 KB] || 13191_NSL_Ep03_youtube_720.00476_thm.png (80x40) [5.7 KB] || 13191_NSL_Ep03_lowres.mp4 (1280x720) [551.2 MB] || 13191_NSL_Ep03_youtube_720.mp4 (1280x720) [3.1 GB] || 13191_NSL_Ep03.mov (1280x720) [20.7 GB] || 13191_NSL_Ep03.webm (960x540) [817.8 MB] || 13191_NSL_Ep03.en_US.srt [46.9 KB] || 13191_NSL_Ep03.en_US.vtt [44.2 KB] || ", "hits": 128 }, { "id": 4726, "url": "https://svs.gsfc.nasa.gov/4726/", "result_type": "Visualization", "release_date": "2019-03-27T00:00:00-04:00", "title": "New Island forms in Tonga (Updated)", "description": "This visualization shows the evolution Tonga's new island between January 2015 and March 2018. || Tonga_evolutn.1300_print.jpg (1024x576) [129.1 KB] || Tonga_evolutn.1300_searchweb.png (320x180) [84.2 KB] || Tonga_evolutn.1300_web.png (320x180) [84.2 KB] || Tonga_evolutn_Wcredits_1080p30.mp4 (1920x1080) [43.0 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4 (1920x1080) [17.9 MB] || Tonga_evolutn_Wcredits_1080p30.webm (1920x1080) [5.8 MB] || Tonga_evolutn_Wcredits_2160p30_h265.mp4 (3840x2160) [50.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Tonga_evolutn_Wcredits_2160p30.mp4 (3840x2160) [140.4 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4.hwshow || ", "hits": 180 }, { "id": 13070, "url": "https://svs.gsfc.nasa.gov/13070/", "result_type": "Produced Video", "release_date": "2018-09-21T00:00:00-04:00", "title": "500th Anniversary of Humanity's First Circumnavigation of Earth", "description": "From Magellan to the UniverseMusic Credit: Killer TracksTrack Titles:(1) GTP56_Stunt_Kite(2) ICON023_Anything_is_Possible(3) ATMOS402_Spiralling_Spheres || 13070_Magellans_500th_Anniversary.00103_print.jpg (1024x576) [92.0 KB] || 13070_Magellans_500th_Anniversary.00103_searchweb.png (320x180) [89.7 KB] || 13070_Magellans_500th_Anniversary.00103_thm.png (80x40) [6.6 KB] || 13070_Magellans_500th_Anniversary.mov (1920x1080) [5.1 GB] || 13070_Magellans_500th_Anniversary.mp4 (1920x1080) [624.6 MB] || 13070_Magellans_500th_Anniversary.webm (960x540) [160.3 MB] || 13070_Magellans_500th_Anniversary_CC.en_US.srt [9.6 KB] || 13070_Magellans_500th_Anniversary_CC.en_US.vtt [9.6 KB] || ", "hits": 40 }, { "id": 20283, "url": "https://svs.gsfc.nasa.gov/20283/", "result_type": "Animation", "release_date": "2018-08-07T15:00:00-04:00", "title": "CURIOSITY MARDI Sidewalk imaging", "description": "CURIOSITY MARDI Sidewalk imaging || MarsSidewalkAPRHQv2.00001_print.jpg (1024x576) [157.8 KB] || MarsSidewalkAPRHQv2.00001_searchweb.png (320x180) [104.3 KB] || MarsSidewalkAPRHQv2.00001_thm.png (80x40) [5.8 KB] || MarsSidewalkAPRHQv2.webm (1920x1080) [8.6 MB] || MarsSidewalkV2 (1920x1080) [0 Item(s)] || MarsSidewalkAPRHQv2.mov (1920x1080) [1.2 GB] || MarsSidewalk720pv2.h264.mov (1280x720) [1.2 GB] || MarsSidewalk1080v2.h264.mov (1920x1080) [2.5 GB] || curiosity-mardi-sidewalk-imaging.hwshow [189 bytes] || ", "hits": 16 }, { "id": 4635, "url": "https://svs.gsfc.nasa.gov/4635/", "result_type": "Visualization", "release_date": "2018-06-15T11:00:00-04:00", "title": "Visualizations of Hunga Tonga Hunga Ha'apai and the Martian Landscape", "description": "In early 2015, a volcanic eruption in the Kingdom of Tonga created a new island informally known as Hunga Tonga Hunga Ha'apai (HTHH). The subsequent evolution of the new island was previously described in \"The Birth of a New Island\" available here. Below are additional visualizations, including an updated view of the island's appearance in March 2018 as well as some visualizations of the martian surface. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.The complete visualization of \"Using Earth to understand how water may have affected volcanoes on Mars\" is available here.Learn more about the evolution of Earth's newest island and how it could reveal new information about the presence of water on Mars: https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL076621 || ", "hits": 147 }, { "id": 12932, "url": "https://svs.gsfc.nasa.gov/12932/", "result_type": "Produced Video", "release_date": "2018-06-08T14:00:00-04:00", "title": "Using Earth to Understand How Water May Have Affected Volcanoes on Mars", "description": "This scientific data visualization shows the evolution of the newly-erupted island in the Kingdom of Tonga. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.Learn more about the evolution of Earth's newest island and how it could reveal new infomration about the presence of water on Mars: Monitoring and Modeling the Rapid Evolution of EArth's Newest Volcanic Island: Hunga Tonga Hunga Ha'apai (Tonga) Using High Spatial Resolution Satellite Observations Authors: J.B. Garvin, D.A. Slayback, V. Ferrini, J. Frawley, C. Giguere, G.R. Asrar, K. AndersonPages: 3445-3452 l First Published: 26 March 2018- Volumetric erosion for new hydromagmatic island is approximately 0.0026km3/year- Demostrated first meter-scale documentation of landscapes and topography for a new volcanic island over its initial stages of evolution (approximately 3 years)- Satellite-based measurements of news island predict lifetime of up to approximately 42 years || ", "hits": 140 }, { "id": 12784, "url": "https://svs.gsfc.nasa.gov/12784/", "result_type": "Produced Video", "release_date": "2018-05-21T12:00:00-04:00", "title": "Martian Clues on a Baby Island", "description": "A young volcanic island on Earth may hold clues to former islands on Mars. || Tonga_v60_vis.0780_16x9.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_16x9_print.jpg (1024x576) [123.6 KB] || Tonga_v60_vis.0780_16x9_searchweb.png (320x180) [96.3 KB] || Tonga_v60_vis.0780_16x9_thm.png (80x40) [7.7 KB] || ", "hits": 29 }, { "id": 12800, "url": "https://svs.gsfc.nasa.gov/12800/", "result_type": "Produced Video", "release_date": "2017-12-11T16:00:00-05:00", "title": "The Birth of a New Island: Press Materials", "description": "Music: Fountain by Mailcoat Sheppard; Data Visions by Pike; Guilty Curiosity by Brice Davoli; Concerning Nymphs by Hammond Roberts. Complete transcript available. || NewTongaIsland_Long_print.jpg (1024x573) [107.5 KB] || NewTongaIsland_Long.png (2552x1429) [3.6 MB] || NewTongaIsland_Long_searchweb.png (320x180) [99.0 KB] || NewTongaIsland_Long_thm.png (80x40) [7.8 KB] || FACEBOOK_720_NewTongaIsland_Long_facebook_720.webm (1280x720) [43.3 MB] || TWITTER_720_NewTongaIsland_Long_twitter_720.mp4 (1280x720) [96.7 MB] || NewTongaIsland_Long_large.mp4 (1920x1080) [404.5 MB] || FACEBOOK_720_NewTongaIsland_Long_facebook_720.mp4 (1280x720) [504.5 MB] || YOUTUBE_720_NewTongaIsland_Long_youtube_720.mp4 (1280x720) [660.6 MB] || YOUTUBE_1080_NewTongaIsland_Long_youtube_1080.mp4 (1920x1080) [694.2 MB] || TongaNewIslandCaptions.en_US.srt [7.9 KB] || TongaNewIslandCaptions.en_US.vtt [7.8 KB] || CH28_NewTongaIsland_Long_ch28.mov (1280x720) [3.7 GB] || NewTongaIsland_Long.mov (1920x1080) [10.5 GB] || ", "hits": 95 }, { "id": 4602, "url": "https://svs.gsfc.nasa.gov/4602/", "result_type": "Visualization", "release_date": "2017-12-11T10:00:00-05:00", "title": "New island forms in Tonga", "description": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel. || Tonga_v60_vis.0780_print.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_searchweb.png (320x180) [76.8 KB] || Tonga_v60_vis.0780_thm.png (80x40) [6.0 KB] || new_island_vis (1920x1080) [0 Item(s)] || Tonga_v60_vis_1080p30.mp4 (1920x1080) [33.3 MB] || Tonga_v60_vis_1080p30.webm (1920x1080) [5.1 MB] || Tonga_4k_final2_1080p30.mp4 (1920x1080) [34.3 MB] || new_island_vis (3840x2160) [0 Item(s)] || Tonga_4k_final2_2160p30.mp4 (3840x2160) [52.0 MB] || Tonga_v60_vis_1080p30.mp4.hwshow [187 bytes] || ", "hits": 48 }, { "id": 12533, "url": "https://svs.gsfc.nasa.gov/12533/", "result_type": "Produced Video", "release_date": "2017-05-18T11:00:00-04:00", "title": "Science Comes Alive at NASA Goddard", "description": "Science Comes Alive at NASA Goddard TRT: 3:35Music Credit: Killer TracksOld River [CM099]Mainframe Disturbance [ICON007]Never Lost Combat [KOK2425]Simple Logic [CM099]Shout [CM116]Hope for Change [NYB120]Illuminating [KT332]Breaking the Atmosphere [ICON013]Chop It Up [KT332] || 12533_At_NASA_Goddard_Promo_w_Title_youtube_hq.00001_print.jpg (1024x576) [25.3 KB] || 12533_At_NASA_Goddard_Promo_w_Title_appletv.m4v (1280x720) [139.9 MB] || 12533_At_NASA_Goddard_Promo_w_Title.webm (960x540) [106.0 MB] || 12533_At_NASA_Goddard_Promo_w_Title_appletv_subtitles.m4v (1280x720) [140.0 MB] || 12533_At_NASA_Goddard_Promo_LONG_w_Title.en_US.srt [5.1 KB] || 12533_At_NASA_Goddard_Promo_LONG_w_Title.en_US.vtt [4.9 KB] || 12533_At_NASA_Goddard_Promo_w_Title_youtube_hq.mov (1920x1080) [1.5 GB] || 12533_At_NASA_Goddard_Promo_w_Title_prores.mov (1280x720) [3.6 GB] || 12533_At_NASA_Goddard_Promo_w_Title.mov (1920x1080) [6.8 GB] || ", "hits": 128 }, { "id": 12558, "url": "https://svs.gsfc.nasa.gov/12558/", "result_type": "Produced Video", "release_date": "2017-04-04T10:00:00-04:00", "title": "Goddard Helicopter Simulation of Venus Descent Imaging for Science", "description": "Venus Descent Imaging Proposal || RoadToVenus_Final_1080p.00132_print.jpg (1024x576) [64.2 KB] || RoadToVenus_Final_1080p.00132_searchweb.png (320x180) [55.4 KB] || RoadToVenus_Final_1080p.00132_web.png (320x180) [55.4 KB] || RoadToVenus_Final_1080p.00132_thm.png (80x40) [4.5 KB] || RoadToVenus_Final_1080p.mov (1920x1080) [2.5 GB] || RoadToVenus_Final_720p.mov (1280x720) [1.3 GB] || RoadToVenus_Final_720p.mp4 (1280x720) [257.0 MB] || RoadToVenus_Final_1080p.mp4 (1920x1080) [287.2 MB] || RoadToVenus_Final_1080p.webmhd.webm (1080x606) [41.0 MB] || RoadToVenus_Final.mov (2704x1520) [4.8 GB] || RoadToVenus.en_US.srt [5.0 KB] || RoadToVenus.en_US.vtt [5.0 KB] || ", "hits": 50 }, { "id": 12042, "url": "https://svs.gsfc.nasa.gov/12042/", "result_type": "Produced Video", "release_date": "2015-11-05T14:00:00-05:00", "title": "MAVEN Results Live Shot Page", "description": "Interview with MAVEN Principal Investigator Dr. Bruce Jakosky || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_print.jpg (1024x576) [109.3 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_searchweb.png (320x180) [93.0 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_thm.png (80x40) [6.5 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq.mov (1280x720) [649.6 MB] || Bruce_Jakosky_MAVEN_LS_Canned.mov (1280x720) [2.1 GB] || WEBM_Bruce_Jakosky_MAVEN_LS_Canned.webm (960x540) [89.8 MB] || Bruce_Jakosky_MAVEN_LS_Canned.en_US.srt [4.7 KB] || Bruce_Jakosky_MAVEN_LS_Canned.en_US.vtt [4.5 KB] || ", "hits": 146 }, { "id": 11792, "url": "https://svs.gsfc.nasa.gov/11792/", "result_type": "Produced Video", "release_date": "2015-03-03T00:00:00-05:00", "title": "Inspiring Women in Science", "description": "Favorite ScienceWoman - Katrina's CutThis is a video Katrina edited of everyone talking about their favorite #ScienceWoman.For complete transcript, click here. || Favorite_ScienceWoman_Katrinas_cut_youtube_hq.00527_print.jpg (1024x576) [110.3 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_print.jpg (1024x576) [118.6 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_thm.png (80x40) [6.1 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_web.png (320x180) [85.7 KB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq_searchweb.png (320x180) [85.7 KB] || Favorite_ScienceWoman_Katrinas_cut_1280x720.wmv (1280x720) [161.3 MB] || Favorite_ScienceWoman_Katrinas_cut_appletv_subtitles.m4v (960x540) [133.2 MB] || Favorite_ScienceWoman_Katrinas_cut_youtube_hq.mov (1280x720) [148.5 MB] || Favorite_ScienceWoman_Katrinas_cut_appletv.m4v (960x540) [133.3 MB] || Favorite_ScienceWoman_Katrinas_cut_prores.mov (1280x720) [4.8 GB] || Favorite_ScienceWoman_Katrinas_cut_720x480.webm (720x480) [35.5 MB] || Favorite_ScienceWoman_Katrinas_cut_720x480.wmv (720x480) [104.4 MB] || Favorite_ScienceWoman_Katrinas_cut_ipod_lg.m4v (640x360) [53.1 MB] || Favorite_ScienceWoman.en_US.srt [6.5 KB] || Favorite_ScienceWoman.en_US.vtt [6.5 KB] || Favorite_ScienceWoman_Katrinas_cut_nasaportal.mov (640x360) [127.5 MB] || Favorite_ScienceWoman_Katrinas_cut_ipod_sm.mp4 (320x240) [28.5 MB] || ", "hits": 138 }, { "id": 11662, "url": "https://svs.gsfc.nasa.gov/11662/", "result_type": "Produced Video", "release_date": "2014-09-19T21:05:00-04:00", "title": "MAVEN Arrives at Mars Live Shot 2014", "description": "The Mars Atmosphere Volatile Evolution mission, or MAVEN, is NASA's newest mission to Mars. After a 10 month journey, it's arriving at the Red Planet on Sunday, September 21, where it will study the planet's upper atmosphere. MAVEN will help determine why Mars has lost the majority of its atmosphere over the past four billion years, giving us information on how the Mars climate has evolved over time. This will also help us understand the evolution of other planets, including Earth. || ", "hits": 43 }, { "id": 11494, "url": "https://svs.gsfc.nasa.gov/11494/", "result_type": "Produced Video", "release_date": "2014-03-24T06:00:00-04:00", "title": "Jim Garvin's Top \"Pics\" - LROC Images", "description": "In this video series, NASA Scientist Jim Garvin highlights his favorite pictures taken throughout the solar system. This episode focuses on images taken by LROC – the Lunar Reconnaissance Orbiter Camera. Jim explains which pictures made his “top 5” list. || ", "hits": 35 }, { "id": 11408, "url": "https://svs.gsfc.nasa.gov/11408/", "result_type": "Produced Video", "release_date": "2013-11-13T00:00:00-05:00", "title": "Mars MAVEN mission live shots Nov. 13, 2013", "description": "Broll and interview with Dr. Jim Garvin previewing the upcoming launch of NASA's newest mission to Mars, the Mars Atmosphere and Volatile Evoution or MAVEN set to launch Monday, Nov. 18th. || ", "hits": 26 }, { "id": 11374, "url": "https://svs.gsfc.nasa.gov/11374/", "result_type": "Produced Video", "release_date": "2013-11-05T00:00:00-05:00", "title": "Craterology", "description": "To better understand how Earth evolved, scientists are pointing cameras toward impact craters on the moon. Impact craters are giant surface depressions that form in the aftermath of collisions by asteroids, meteoroids and comets. Exposure to wind, water and geologic activity slowly degrades impact craters found on Earth. But by knowing how a crater has changed over time, scientists can piece together clues of what conditions were like on the planet long ago. Now, NASA’s Lunar Reconnaissance Orbiter spacecraft is collecting images of impact craters on the moon’s surface. Unlike on Earth, these craters aren’t prone to weathering because the moon has practically no atmosphere. As a result, some have remained untouched since the day they were born. Scientists will use the images to determine how natural disasters and the climates of Earth’s past have shaped how its craters look today. Watch the video to learn more. || ", "hits": 63 }, { "id": 10792, "url": "https://svs.gsfc.nasa.gov/10792/", "result_type": "Produced Video", "release_date": "2012-11-05T14:00:00-05:00", "title": "NASA's Planetary CSI: Crater Science Investigations", "description": "If you want to learn more about the history of Earth and other rocky planets in the solar system, craters are a great place to look. Now, thanks to LRO's LROC instrument, we can take a much closer look at Linn? Crater on the moon—a pristine crater that's great to use to compare with other craters! || ", "hits": 104 }, { "id": 10904, "url": "https://svs.gsfc.nasa.gov/10904/", "result_type": "Produced Video", "release_date": "2012-02-14T00:00:00-05:00", "title": "Love's Terrain", "description": "Over centuries, the planet second closest to the sun was known by many names: Ishtar, Ouaiti, Hesperus, Aphrodite. But just as with the heart's memory one name prevails. In honor of Valentine's Day, homage is paid to the celestial sphere that personifies the mythological goddess of love and beauty—Venus. Of all the planets in our solar system Venus is nearest in size to Earth, though its dry rocky landscape is much hotter. Processed images of the surface using data collected by instruments onboard NASA's Magellan spacecraft reveal vast plains intermixed with sloping highlands and ancient volcanoes. These features are highlighted on a rotating globe of Venus in the color-coded visualization below, where high elevation terrain is shaded yellow and red with low elevation regions tinted blue and green. Black gaps represent areas of the planet uncharted during the first mapping cycle made by Magellan, which surveyed Venus over a period of four years beginning in 1990. || ", "hits": 498 }, { "id": 3874, "url": "https://svs.gsfc.nasa.gov/3874/", "result_type": "Visualization", "release_date": "2011-10-27T06:00:00-04:00", "title": "Tour of the Moon", "description": "Using elevation and image data returned by Lunar Reconnaissance Orbiter (LRO), this animation takes the viewer on a virtual tour of the Moon. The tour visits a number of interesting sites chosen to illustrate a wide variety of lunar terrain features. Some are on the near side and are familiar to both professional and amateur observers on Earth, while others can only be seen clearly from space. Some are large and old (Orientale, South Pole-Aitken), others are smaller and younger (Tycho, Aristarchus). Constantly shadowed areas near the poles are hard to photograph but easier to measure with altimetry, while several of the Apollo landing sites, all relatively near the equator, have been imaged at resolutions as high as 25 centimeters (10 inches) per pixel.The shape of the terrain in this animation is based primarily on data from LRO's laser altimeter (LOLA), supplemented by stereo image data from its wide angle camera (LROC WAC) and from Japan's Kaguya mission. The global surface color is from Clementine. || ", "hits": 260 }, { "id": 10749, "url": "https://svs.gsfc.nasa.gov/10749/", "result_type": "Produced Video", "release_date": "2011-05-01T00:00:00-04:00", "title": "Goddard Virtual Tour", "description": "Goddard Chief Scientist Jim Garvin takes us on a tour of the life of a spacecraft, from the idea to the collection of data in orbit. Each segment looks at a different phase of the spacecraft and its place in Goddard Space Flight Center: Idea, Design, Construction, Testing, Launch, Operations, and Scientific Analysis. These videos were produced in support of the Goddard Virtual Tour web interactive feature. || ", "hits": 50 }, { "id": 10618, "url": "https://svs.gsfc.nasa.gov/10618/", "result_type": "Produced Video", "release_date": "2010-08-16T00:00:00-04:00", "title": "The Inner Solar System: Discovering Earth's Neighborhood w/ Dr. James Garvin", "description": "Chief Scientist of Goddard Space Flight Center, Dr. James Garvin, takes us on a journey of Earth, the moon, and our neighboring planets. Why does space matter? Why is exploring our closest neighbors significant? Where will human venture to next? In this studio lecture, Dr. Garvin answers these questions and discusses what NASA has learned about our inner solar system. || ", "hits": 30 }, { "id": 3731, "url": "https://svs.gsfc.nasa.gov/3731/", "result_type": "Visualization", "release_date": "2010-06-21T00:00:00-04:00", "title": "LOLA: Lunar Topography in Natural Color", "description": "This animation is a brief tour of several prominent features of the Moon's terrain: Tycho crater, the south pole, and the South Pole-Aitken basin. It is match-moved to a companion piece showing the terrain elevations in false color.This is an update of animation 3594, which was produced before the launch of Lunar Reconnaissance Orbiter. Except for the Tycho crater inset, the elevation map in this updated version is based entirely on early results of the Lunar Orbiter Laser Altimeter onboard LRO.The surface appearance is derived from photographs taken by the Clementine spacecraft. Although it shows the visible surface in natural color, this animation does not depict realistic sunlight and shadows. This is especially significant near the poles, where certain parts of the terrain can be in permanent shadow and would never be fully visible in the manner depicted here. || ", "hits": 376 }, { "id": 3728, "url": "https://svs.gsfc.nasa.gov/3728/", "result_type": "Visualization", "release_date": "2010-06-17T00:00:00-04:00", "title": "Magellan: Venus False-Color Terrain", "description": "This animation is a brief tour of the global terrain of the planet Venus as revealed by radar onboard the Magellan spacecraft. The height of the terrain is color-coded, with blues and greens representing low altitudes and reds representing high altitudes. Highlighted are two large \"continents,\" or highlands, Aphrodite Terra and Ishtar Terra; the Maxwell Montes mountain range; and Maat Mons, a large, currently dormant volcano.Magellan arrived at Venus in August of 1990 and spent four years there collecting data. The elevation map used here was created with data collected during the first mapping cycle. Many of the coverage gaps, represented here by black pixels, were filled in during later mapping cycles. || ", "hits": 464 }, { "id": 3727, "url": "https://svs.gsfc.nasa.gov/3727/", "result_type": "Visualization", "release_date": "2010-06-11T00:00:00-04:00", "title": "LOLA Lunar Topography in False Color", "description": "This animation is a brief tour of several prominent features of the Moon's terrain: Tycho crater, the south pole, and the South Pole-Aitken basin. The height of the terrain is color-coded, with blues and greens representing low altitudes and reds representing high altitudes. The view is match-moved to a companion piece showing the Moon in natural colors.This is an update of animation 3582, which was produced before the launch of Lunar Reconnaissance Orbiter. Except for the Tycho crater inset, the elevation map in this updated version is based entirely on early results of the Lunar Orbiter Laser Altimeter onboard LRO. These results already represent a substantial improvement in our knowledge of the Moon's topography. || ", "hits": 304 }, { "id": 10444, "url": "https://svs.gsfc.nasa.gov/10444/", "result_type": "Produced Video", "release_date": "2009-06-23T00:00:00-04:00", "title": "LRO Enters Lunar Orbit (full live event)", "description": "This entry is the full one hour program that was produced live during the orbit insertion event. To see just a short portion of highlights from the event, see entry #10445 || ", "hits": 75 }, { "id": 10445, "url": "https://svs.gsfc.nasa.gov/10445/", "result_type": "Produced Video", "release_date": "2009-06-23T00:00:00-04:00", "title": "LRO Enters Lunar Orbit (Highlights)", "description": "After a four and a half day journey from the Earth, the Lunar Reconnaissance Orbiter, or LRO, successfully entered orbit around the moon. Engineers at NASA's Goddard Space Flight Center in Greenbelt, Md., confirmed the spacecraft's lunar orbit insertion at 6:27 a.m. EDT Tuesday, June 23, 2009.During transit to the moon, engineers performed a mid-course correction to get the spacecraft in the proper position to reach its lunar destination. Since the moon is always moving, the spacecraft shot for a target point ahead of the moon. When close to the moon, LRO used its rocket motor to slow down until the gravity of the moon caught the spacecraft in lunar orbit.To see the full one hour video produced live during the orbit insertion burns, visit entry #10444 || ", "hits": 24 }, { "id": 10443, "url": "https://svs.gsfc.nasa.gov/10443/", "result_type": "Produced Video", "release_date": "2009-06-17T00:00:00-04:00", "title": "Lunar Reconnaissance Orbiter (LRO) Launch Videos", "description": "The videos on this page were shot during the week of the LRO/LCROSS launch (June 15-19, 2009) at Kennedy Space Center.For more views of the LRO/LCROSS launch, including footage from inside the Missions Operations Control Room at Goddard and individual camera feeds of the launch from Kennedy, check out entry #10469. || ", "hits": 138 }, { "id": 3582, "url": "https://svs.gsfc.nasa.gov/3582/", "result_type": "Visualization", "release_date": "2009-04-17T00:00:00-04:00", "title": "Lunar Topography in False Color", "description": "An updated version of this animation is available here.This animation is a brief tour of several prominent features of the Moon's terrain: Tycho crater, the south pole, and the South Pole-Aitken basin. The height of the terrain is color-coded, with blues and greens representing low altitudes and reds representing high altitudes. The view is match-moved to a companion piece showing the Moon in natural colors.The elevation map comprises low-resolution data from a number of sources, including the Clementine and JAXA/SELENE spacecraft, combined with high-resolution insets for Tycho and the region near the south pole. One of the goals of the Lunar Reconnaissance Orbiter mission is the creation of a high-resolution elevation map of the entire surface of the Moon. || ", "hits": 73 }, { "id": 3594, "url": "https://svs.gsfc.nasa.gov/3594/", "result_type": "Visualization", "release_date": "2009-04-17T00:00:00-04:00", "title": "Lunar Topography in Natural Color", "description": "An updated version of this animation is available here.This animation is a brief tour of several prominent features of the Moon's terrain: Tycho crater, the south pole, and the South Pole-Aitken basin. It is match-moved to a companion piece showing the terrain elevations in false color.The surface appearance is derived from photographs taken by the Clementine spacecraft. Although it shows the visible surface in natural color, this animation does not depict realistic sunlight and shadows. This is especially significant near the poles, where certain parts of the terrain can be in permanent shadow and would never be fully visible in the manner depicted here. || ", "hits": 98 }, { "id": 10400, "url": "https://svs.gsfc.nasa.gov/10400/", "result_type": "Produced Video", "release_date": "2009-03-04T00:00:00-05:00", "title": "50 Years of Goddard", "description": "Pioneer rocket scientist Robert H. Goddard once said, 'It is difficult to say what is impossible, for the dream of yesterday is the hope of today and the reality of tomorrow.' Fifty years after its inception, NASA's Goddard Space Flight Center continues to live by these words, advancing science and engineering to new limits once thought impossible as it explores of the Earth, the sun, the solar system, and the universe. || ", "hits": 223 }, { "id": 10343, "url": "https://svs.gsfc.nasa.gov/10343/", "result_type": "Produced Video", "release_date": "2009-01-14T00:00:00-05:00", "title": "Up to the Challenge", "description": "In October 2008, Goddard hosted The Discovery Channel's 'Young Scientist Challenge.' The challenge brought ten middle school student finalists from across the country to vie for the title of 'America's Top Young Scientist' and a chance to win a U.S. Savings Bond. Five teacher finalists contended for recognition as 'America's Top Science Teacher.' NASA scientists and educators helped design the activities, which both tested the communication skills of the students and celebrated 50 years of NASA space science.For complete transcript, click here. || DYSChallenge_1280x72002412_print.jpg (1024x576) [139.7 KB] || DYSChallenge_1280x720_web.png (320x180) [208.4 KB] || DYSChallenge_1280x720_thm.png (80x40) [17.4 KB] || DYSChallenge_1280x720.webmhd.webm (960x540) [45.1 MB] || DYSChallenge_1280x720.mp4 (1280x720) [90.9 MB] || DYSChallenge_ipod_640x480.m4v (640x360) [34.4 MB] || DYSChallenge_640x360.mpg (640x360) [41.7 MB] || DYSChallenge_youtube_640x480.mov (640x480) [40.0 MB] || DYSChallenge_320x240.mp4 (320x240) [13.2 MB] || DYSChallenge_ipod_320x240.m4v (320x180) [15.6 MB] || DYSChallenge_512x288.mpg (512x288) [27.9 MB] || ", "hits": 118 }, { "id": 20169, "url": "https://svs.gsfc.nasa.gov/20169/", "result_type": "Animation", "release_date": "2008-07-22T12:00:00-04:00", "title": "LEX / Boomerang Mission", "description": "LEX is one of the candidates for inclusion in the LRO mission - LEX will sample the lunar soil as well as search for signs of water. || ", "hits": 13 }, { "id": 10192, "url": "https://svs.gsfc.nasa.gov/10192/", "result_type": "Produced Video", "release_date": "2008-03-31T12:00:00-04:00", "title": "Venus: Long Time, No See", "description": "The last U.S. spacecraft mission to Venus was in 1989 with the launch of Magellan. Even though Magellan spent the next five years radar mapping the surface and gathering high resolution gravity data, much remains a mystery about our so-called sister planet. Did Venus experience a run-a-way greenhouse effect at some point in its history? Why is the surface pressure 90 times greater on Venus then on Earth? Why is the planet so hot? These are only a few of the question that must be answered if we are to learn more about Venus's past and possibly Earth's future. || ", "hits": 36 }, { "id": 3443, "url": "https://svs.gsfc.nasa.gov/3443/", "result_type": "Visualization", "release_date": "2007-08-27T00:00:00-04:00", "title": "Clementine Lunar South Pole", "description": "NASA's next moon mission, the Lunar Reconaissance Orbiter (LRO), will pave the way for future lunar missions by taking high resolution data of the entire lunar body. This animation zooms into one region of high interest, the lunar south pole, as seen by the 1994 Clementine mission. The possibility of frozen water is one of many reasons NASA is interested in this potential landing site. However, many of the craters in this area where frozen water sources are most likely to be found are in constant shadow which inhibited Clementine's ability to see into these craters. These shadows are the very dark areas at the poles center as seen in this animation, and one of the moon's secrets on which LRO should shed some light. || ", "hits": 199 }, { "id": 3444, "url": "https://svs.gsfc.nasa.gov/3444/", "result_type": "Visualization", "release_date": "2007-08-27T00:00:00-04:00", "title": "Clementine Moon Spin", "description": "This animation rotates around a virtual moon showing Clementine data. The first frame and last frame of the animation match up to allow continuous cycling of the rotation. || ", "hits": 198 }, { "id": 3380, "url": "https://svs.gsfc.nasa.gov/3380/", "result_type": "Visualization", "release_date": "2006-11-14T12:00:00-05:00", "title": "Great Zoom into Chicago, IL: The Adler Planetarium", "description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the Adler Planetarium. The Adler Planetarium and Astronomy Museum in Chicago, Illinois was built in 1930 by philanthropist Max Adler. It is located on the shore of Lake Michigan near the Shedd Aquarium, the Field Museum of Natural History, and Soldier Field. || ", "hits": 73 }, { "id": 3381, "url": "https://svs.gsfc.nasa.gov/3381/", "result_type": "Visualization", "release_date": "2006-11-14T12:00:00-05:00", "title": "Great Zoom out of Chicago, IL: The Adler Planetarium", "description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the Adler Planetarium. The Adler Planetarium and Astronomy Museum in Chicago, Illinois was built in 1930 by philanthropist Max Adler. It is located on the shore of Lake Michigan near the Shedd Aquarium, the Field Museum of Natural History, and Soldier Field. || ", "hits": 20 }, { "id": 3334, "url": "https://svs.gsfc.nasa.gov/3334/", "result_type": "Visualization", "release_date": "2006-02-07T00:00:00-05:00", "title": "Zoom to the Meteor Crater, Arizona", "description": "The Earth and Mars are two planets which evolved very differently. By studying locations on Earth whose environment might be similar with that of Mars, scientists are able to theorize about 'the red planet' as well. Meteor Crater is one such study site in the Colorado Plateau, 73 km east of Flagstaff, Arizona. This terrestrial impact crater, 1.2 km in diameter and 185 m deep, is clearly visible in satellite imagery. || ", "hits": 53 }, { "id": 3274, "url": "https://svs.gsfc.nasa.gov/3274/", "result_type": "Visualization", "release_date": "2005-10-18T00:00:00-04:00", "title": "Hubble Space Telescope Looks at the Moon to Prospect for Resources (Apollo 17 Landing Region)", "description": "The Hubble Space Telescope looked at specific areas of the moon prospecting for important minerals that may aid future sustained human presence on the moon. Initial analysis of the data indicate the likely presence of titanium and iron oxides. These minerals can be sources of oxygen, essential for human exploration.This visualization starts with a view of the moon as seen from Earth using a USGS Apollo derived artist rendered texture (airbrushed). The camera then zooms into the Apollo 17 landing region using Clementine data (the outer area after the camera pauses), high resolution HST data (the inner area), and Apollo 17 derived topgraphy.Exposure Time: 2.5 minutesFilters: F250W (250nm), F344N (344nm), F502N (502nm), F658N (658nm)Data from these multiple filters were used to produce the mosaic Apollo 17 landing site image. || ", "hits": 208 }, { "id": 3275, "url": "https://svs.gsfc.nasa.gov/3275/", "result_type": "Visualization", "release_date": "2005-10-18T00:00:00-04:00", "title": "Hubble Space Telescope Looks at the Moon to Prospect for Resources (Aristarchus Crater - gray)", "description": "My edit: The Hubble Space Telescope was used to gather high resolution multi spectral data of the moon's Aristarchus Crater in order to investigate the possibility of potential oxygen producing minerals on the surface. Identifying such minerals could aid in planning future sustained human missions on the moon. Initial analysis of the data indicate the likely presence of titanium and iron oxides. Both these minerals could be used as oxygen sources essential for human exploration.This visualization starts with a view of the moon as seen from Earth using a USGS Apollo derived artist rendered texture (airbrushed). The camera then zooms into the Aristarchus Crater region. Simulated topography derived from Clementine data is used for relief and high resolution HST data is used for the area of interest. After investigating Aristarchus Crater, the camera then moves over to Schroter's Valley for a brief investigation.This visualization is match rendered with id 3275 so that the color version can be dissolved in or out as needed.Exposure Time: 2.5 minutesFilters: F250W (250nm), F344N (344nm), F502N (502nm), F658N (658nm) || ", "hits": 170 }, { "id": 3276, "url": "https://svs.gsfc.nasa.gov/3276/", "result_type": "Visualization", "release_date": "2005-10-17T00:00:00-04:00", "title": "Hubble Space Telescope Looks at the Moon to Prospect for Resources (Aristarchus Crater - color)", "description": "The Hubble Space Telescope looked at specific areas of the moon prospecting for important minerals that may aid future sustained human presence on the moon. Initial analysis of the data indicate the likely presence of titanium and iron oxides. These minerals can be sources of oxygen, essential for human exploration. This visualization starts with a view of the moon as seen from Earth using a USGS Apollo derived artist rendered texture (airbrushed). The camera then zooms into the Aristarchus crater region. Clementine derived simulated topography is shown around the outside and HST color imagery is shown filling most of the view. The camera then flies into the crater site using using simulated topgraphy and then over to Schroter's Valley. This visualization is match rendered with animation 3274 so that the color version can be dissolved in or out as needed. The colors are from these HST filter bands: RED = 502/250 nm ratio, GREEN = 502 nm (green), BLUE = 250/502 nm ratio. In the image, blues are—in principle—higher in ilmenite. || ", "hits": 30 }, { "id": 3042, "url": "https://svs.gsfc.nasa.gov/3042/", "result_type": "Visualization", "release_date": "2004-11-01T12:00:00-05:00", "title": "Lunar Beauty Shot", "description": "This is a beauty shot animation flying over the surface of the moon created in support of a series of live interviews about the 2004 lunar eclipse.Scales are not accurate in this visualization. The Earth is about 3 times larger than it would actually appear. The source of the moon texture is unknown; it is thought to be a composite from several missions. The Earth texture was captured as the Galileo spacecraft swung by the Earth in 1990 for a gravity assist on its way to Jupiter. || ", "hits": 25 }, { "id": 2882, "url": "https://svs.gsfc.nasa.gov/2882/", "result_type": "Visualization", "release_date": "2004-05-02T12:00:00-04:00", "title": "Zoom down to the Gale Crater on Mars", "description": "This is a zoom down to the Gale Crater on MARS as seen by Viking and the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC). These images show a very large area of sedimentation inside the Gale Crater. The origin of the sedimentary material remains unanswered. Studying these layers of rocks could answer many questions about the history of MARS. || ", "hits": 138 }, { "id": 2864, "url": "https://svs.gsfc.nasa.gov/2864/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Final Composite", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, still dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is 10km. high compared to Olympus Mons at 23km. This post-produced animation composite was created using various elements from animations #2865 through #2872. || ", "hits": 298 }, { "id": 2865, "url": "https://svs.gsfc.nasa.gov/2865/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: True Color Earth", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, still dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing Earth in its true color beauty. This animation is match-framed to animations #2864 through #2872. || ", "hits": 56 }, { "id": 2866, "url": "https://svs.gsfc.nasa.gov/2866/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Earth with Elevation Color Map", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing a bare Earth (no oceans) via an elevation color map. This color map is the same one used to map Mars in Animation #2868. Instead of using sea level as zero (i.e., yellow) we use Earth's mean elevation which is approximately 1 km. below sea level. We then map the higher elevations in greens, reds, and white at the highest peaks, and blue and purple are used for the low lying areas. This animation is match-framed to animations #2864 through #2872. || ", "hits": 65 }, { "id": 2867, "url": "https://svs.gsfc.nasa.gov/2867/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Elevation color-mapped Earth with True Color Land", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison. It shows ocean bathymetry via an elevation color map (greens, blues, and purples indicate deeper ocean depths respectively) along with true color land (everything above sea level). This animation is match-framed to animations #2864 through #2872. || ", "hits": 321 }, { "id": 2868, "url": "https://svs.gsfc.nasa.gov/2868/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: True Color Mars", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing Mars in it's true color beauty. The beginning of this animation is match-framed to animations #2864 through #2872. || ", "hits": 537 }, { "id": 2869, "url": "https://svs.gsfc.nasa.gov/2869/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Elevation Color-Mapped Mars", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison. It shows Mars' differing terrain via an elevation color map. Yellow indicates the mean elevation. Green, blue, and purple are low lying areas. Red, brown, and white are the highest elevations. This animation is match-framed to animations #2864 through #2872 and uses the same color map as animation #2866. || ", "hits": 487 }, { "id": 2870, "url": "https://svs.gsfc.nasa.gov/2870/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: True Color Olympus Mons over Elevation Color-Mapped Earth Bathymetry with True Color Land Features", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, Olympus Mons obstructs the view of Mauna Loa, but gives the viewer a good perspective of the overall size of this giant volcano. This animation is match-framed to animations #2864 through #2872. || ", "hits": 264 }, { "id": 2871, "url": "https://svs.gsfc.nasa.gov/2871/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Transparent Olympus Mons over Elevation Color-Mapped Earth with True Color Land", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, a transparent Olympus Mons is juxtaposed over Mauna Loa, allowing the viewer to better see the size differences between these land masses. This animation is match-framed to animations #2864 through #2872. || ", "hits": 152 }, { "id": 2872, "url": "https://svs.gsfc.nasa.gov/2872/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Earth-Mars Volcano Comparisons: Mars Inside a Transparent Earth", "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation not only shows the relative size differences between Mauna Loa and Olympus Mons, but also shows the size difference between these 2 planets. The equatorial radius of Mars is approximately 3397 km. compared to Earth's equatorial radius of 6378.1 km. This animation is match-framed to animations #2864 through #2872. || ", "hits": 175 }, { "id": 2873, "url": "https://svs.gsfc.nasa.gov/2873/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Great Zoom into Don Juan Pond, Antarctica (treatment #1)", "description": "Antarctica is the coldest and most remote continent on Earth. It is also home to one of the most Mars-like places that scientists can study without actually traveling to the fourth planet. In this sequence we plunge from space down to a remarkably detailed view of a unique part of the Dry Valleys. By studying this place researchers think they might gain insight into how life on Mars might either survive now or have developed in the past. It is called the Don Juan Pond, and it's one of the saltiest, coldest bodies of water on Earth.The zoom passes through four different resolution data sets including data from Terra, Landsat, and IKONOS. || ", "hits": 265 }, { "id": 2874, "url": "https://svs.gsfc.nasa.gov/2874/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Great Zoom into Don Juan Pond, Antarctica (treatment #2)", "description": "Antarctica is the coldest and most remote continent on Earth. It is also home to one of the most Mars-like places that scientists can study without actually traveling to the fourth planet. In this sequence we plunge from space down to a remarkably detailed view of a unique part of the Dry Valleys. By studying this place researchers think they might gain insight into how life on Mars might either survive now or have developed in the past. It is called the Don Juan Pond, and it's one of the saltiest, coldest bodies of water on Earth.The zoom passes through four different resolution data sets including data from Terra, Landsat, and IKONOS. This treatment uses an IKONOS inset that's enhanced to show detail. || ", "hits": 91 }, { "id": 2875, "url": "https://svs.gsfc.nasa.gov/2875/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Great Zoom into Don Juan Pond, Antarctica (treatment #2 North)", "description": "Antarctica is the coldest and most remote continent on Earth. It is also home to one of the most Mars-like places that scientists can study without actually traveling to the fourth planet. In this sequence we plunge from space down to a remarkably detailed view of a unique part of the Dry Valleys. By studying this place researchers think they might gain insight into how life on Mars might either survive now or have developed in the past. It is called the Don Juan Pond, and its one of the saltiest, coldest bodies of water on Earth. Treatment #2 uses an IKONOS inset that's enhanced to show detail. This portion of the visualization is intended to follow Great Zoom into Don Juan Pond, Antarctica (treatment #2 - found in animation 2874) and moves in close to traverses the top edge of the valley surrounding it. We see the crinkled folds and dug out rivulets and gullies eroded into the landscape. These gullies are similar to features on Mars that have been photographed by orbiting spacecraft. They serve as signs of surface erosion and are analogous to the kinds of tell-tales that Mars experts are want to study more thoroughly for signs of a wetter Martian past. || ", "hits": 25 }, { "id": 2876, "url": "https://svs.gsfc.nasa.gov/2876/", "result_type": "Visualization", "release_date": "2004-04-22T12:00:00-04:00", "title": "Great Zoom into Don Juan Pond, Antarctica (Treatment #2 South)", "description": "Antarctica is the coldest and most remote continent on Earth. It is also home to one of the most Mars-like places that scientists can study without actually traveling to the fourth planet. In this sequence we plunge from space down to a remarkably detailed view of a unique part of the Dry Valleys. By studying this place, researchers think they might gain insight into how life on Mars might either survive now or have developed in the past. This place is called the Don Juan Pond, and it's one of the saltiest, coldest bodies of water on Earth. Treatment #2 uses an IKONOS inset that's enhanced to show detail. This portion of the visualization is intended to follow animation 2874, 'Great Zoom into Don Juan Pond, Antarctica (treatment #2)' and moves in close to circumnavigate a portion of the lower edge of the valley. Textured, folded gully formations appear in the rocky surface. Then the camera slides down the valley slope and stops above the actual pond of sub-freezing water at the base. || ", "hits": 39 }, { "id": 2880, "url": "https://svs.gsfc.nasa.gov/2880/", "result_type": "Visualization", "release_date": "2004-04-01T12:00:00-05:00", "title": "Great Zoom into Distributary Fan, Mars", "description": "This is a Great Zoom into the so-called Distributary Fan on Mars. It is located just northeast of Holden Crater. As seen from Martian orbit by the Mars Orbiter Camera (MOC) flying on the Mars Global Surveyor (MGS) spacecraft, this dramatic visualization shows us where liquid water likely flowed across the Martian surface sometime in the planet's past. || ", "hits": 167 }, { "id": 2447, "url": "https://svs.gsfc.nasa.gov/2447/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Smoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts). A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 18 }, { "id": 2448, "url": "https://svs.gsfc.nasa.gov/2448/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Unsmoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts). A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 8 }, { "id": 2449, "url": "https://svs.gsfc.nasa.gov/2449/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flat, Viking True Color)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 22 }, { "id": 2450, "url": "https://svs.gsfc.nasa.gov/2450/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Smoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 26 }, { "id": 2451, "url": "https://svs.gsfc.nasa.gov/2451/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Unsmoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 11 }, { "id": 2452, "url": "https://svs.gsfc.nasa.gov/2452/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Viking True Color)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 135 }, { "id": 2453, "url": "https://svs.gsfc.nasa.gov/2453/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Smoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 16 }, { "id": 2454, "url": "https://svs.gsfc.nasa.gov/2454/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Unsmoothed)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 12 }, { "id": 2455, "url": "https://svs.gsfc.nasa.gov/2455/", "result_type": "Visualization", "release_date": "2002-05-31T12:00:00-04:00", "title": "Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Viking True Color)", "description": "Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data. || ", "hits": 147 }, { "id": 2427, "url": "https://svs.gsfc.nasa.gov/2427/", "result_type": "Visualization", "release_date": "2002-04-16T12:00:00-04:00", "title": "MOLA-based Flyover of Hellas Transitioning to Utopia Planitia", "description": "MOLA-based animations showing Martian topography as both color and elevation. The exaggeration is 3x. This was created for a talk James Garvin will give on The Hill in late April 2002. || ", "hits": 16 }, { "id": 2428, "url": "https://svs.gsfc.nasa.gov/2428/", "result_type": "Visualization", "release_date": "2002-04-16T12:00:00-04:00", "title": "MOLA-based Flyover of Tharsis Volcanos", "description": "MOLA-based animations showing Martian topography as both color and elevation. The exaggeration is 3x. This was created for a talk James Garvin will give on The Hill in late April 2002. || ", "hits": 21 }, { "id": 2429, "url": "https://svs.gsfc.nasa.gov/2429/", "result_type": "Visualization", "release_date": "2002-04-16T12:00:00-04:00", "title": "MOLA-based Flyover of Gusev Crater", "description": "MOLA-based animations showing Martian topography as both color and elevation. The exaggeration is 3x. This was created for a talk James Garvin will give on The Hill in late April 2002. || ", "hits": 21 }, { "id": 2430, "url": "https://svs.gsfc.nasa.gov/2430/", "result_type": "Visualization", "release_date": "2002-04-16T12:00:00-04:00", "title": "MOLA-based Flyover of Korolev Crater", "description": "MOLA-based animations showing Martian topography as both color and elevation. The exaggeration is 3x. This was created for a talk James Garvin will give on The Hill in late April 2002. || ", "hits": 9 }, { "id": 356, "url": "https://svs.gsfc.nasa.gov/356/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "High Slow Fly around Pole", "description": "Slow spin around Mars north pole || a000356.00010_print.png (720x480) [404.0 KB] || a000356_thm.png (80x40) [3.4 KB] || a000356_pre.jpg (320x238) [5.2 KB] || a000356_pre_searchweb.jpg (320x180) [34.8 KB] || a000356.webmhd.webm (960x540) [7.3 MB] || a000356.dv (720x480) [175.3 MB] || a000356.mp4 (640x480) [10.0 MB] || a000356.mpg (352x240) [5.6 MB] || ", "hits": 53 }, { "id": 357, "url": "https://svs.gsfc.nasa.gov/357/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Mars: Fly Straight over Pole", "description": "Fly over Mars north pole || a000357.00010_print.png (720x480) [394.2 KB] || a000357_pre.jpg (320x238) [5.5 KB] || a000357.webmhd.webm (960x540) [5.4 MB] || a000357.dv (720x480) [175.2 MB] || a000357.mp4 (640x480) [10.0 MB] || a000357.mpg (352x240) [5.6 MB] || ", "hits": 54 }, { "id": 358, "url": "https://svs.gsfc.nasa.gov/358/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Fly up to Sasquatch Crater view one", "description": "Fly up to Mars north poles Sasquatch Crater || a000358.00010_print.png (720x480) [389.8 KB] || a000358_thm.png (80x40) [3.9 KB] || a000358_pre.jpg (320x238) [5.0 KB] || a000358_pre_searchweb.jpg (320x180) [32.6 KB] || a000358.webmhd.webm (960x540) [7.0 MB] || a000358.dv (720x480) [175.2 MB] || a000358.mp4 (640x480) [10.0 MB] || a000358.mpg (352x240) [5.6 MB] || ", "hits": 64 }, { "id": 359, "url": "https://svs.gsfc.nasa.gov/359/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Fly up to Sasquatch Crater view two", "description": "Fly up to Mars north poles Sasquatch Crater || a000359.00010_print.png (720x480) [388.4 KB] || a000359_thm.png (80x40) [3.9 KB] || a000359_pre.jpg (320x238) [5.0 KB] || a000359_pre_searchweb.jpg (320x180) [32.6 KB] || a000359.webmhd.webm (960x540) [5.3 MB] || a000359.dv (720x480) [175.2 MB] || a000359.mp4 (640x480) [9.8 MB] || a000359.mpg (352x240) [5.4 MB] || ", "hits": 43 }, { "id": 360, "url": "https://svs.gsfc.nasa.gov/360/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Fly up to Dunes- thought to cover ice", "description": "Fly up to Mars north pole spinning around dunes area || a000360.00010_print.png (720x480) [389.3 KB] || a000360_thm.png (80x40) [4.0 KB] || a000360_pre.jpg (320x238) [5.0 KB] || a000360_pre_searchweb.jpg (320x180) [33.0 KB] || a000360.webmhd.webm (960x540) [6.1 MB] || a000360.dv (720x480) [175.2 MB] || a000360.mp4 (640x480) [10.0 MB] || a000360.mpg (352x240) [5.2 MB] || ", "hits": 153 }, { "id": 361, "url": "https://svs.gsfc.nasa.gov/361/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Fly over of Mars Mesa, Tounge, Dunes, Sasquatch Crater", "description": "Fly over of Mesa, Tounge, Dunes, Sasquatch Crater Based on MOLA data for topography and Viking data for color. Exaggeration is about 300x || Fly up to and around Mars north pole || a000361.00010_print.png (720x480) [402.7 KB] || a000361_pre.jpg (320x238) [5.5 KB] || a000361.webmhd.webm (960x540) [5.9 MB] || a000361.dv (720x480) [232.5 MB] || a000361.mp4 (640x480) [13.3 MB] || a000361.mpg (352x240) [7.8 MB] || ", "hits": 44 }, { "id": 362, "url": "https://svs.gsfc.nasa.gov/362/", "result_type": "Visualization", "release_date": "1998-12-02T12:00:00-05:00", "title": "Mars North Polar Fly In From Above And Tilt", "description": "Mars north pole flyover from above || a000362.00010_print.png (720x480) [416.8 KB] || a000362_thm.png (80x40) [4.4 KB] || a000362_pre.jpg (320x238) [6.0 KB] || a000362_pre_searchweb.jpg (320x180) [44.3 KB] || a000362.webmhd.webm (960x540) [6.8 MB] || a000362.dv (720x480) [175.3 MB] || a000362.mp4 (640x480) [10.1 MB] || a000362.mpg (352x240) [5.5 MB] || ", "hits": 57 } ] }