{ "count": 110, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Boulder%22", "previous": null, "results": [ { "id": 5629, "url": "https://svs.gsfc.nasa.gov/5629/", "result_type": "Visualization", "release_date": "2026-03-26T13:00:00-04:00", "title": "Arctic Sea Ice Maximum 2026", "description": "Arctic sea ice maximum extent 2026, still image || arctic_sea_ice_max_2026_print_print.jpg (1024x576) [157.5 KB] || arctic_sea_ice_max_2026_print.png (3840x2160) [6.2 MB] || arctic_sea_ice_max_2026_print_searchweb.png (320x180) [79.9 KB] || arctic_sea_ice_max_2026_print_web.png (320x180) [79.9 KB] || arctic_sea_ice_max_2026_print_thm.png (80x40) [6.2 KB] || ", "hits": 797 }, { "id": 5583, "url": "https://svs.gsfc.nasa.gov/5583/", "result_type": "Visualization", "release_date": "2025-09-17T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2025", "description": "Animation of Arctic sea ice from its maximum extent, March 22 2025, to its minimum, September 10, 2025, 4K version || sea_ice_2025_min_2160p60.2820_print.jpg (1024x576) [154.9 KB] || sea_ice_2025_min_2160p60.2820_searchweb.png (320x180) [74.1 KB] || sea_ice_2025_min_2160p60.2820_thm.png (80x40) [6.0 KB] || 3840x2160_16x9_60p (3840x2160) [3200 Item(s)] || sea_ice_2025_min_2160p60_p60.mp4 (3840x2160) [107.4 MB] || sea_ice_2025_min_2160p60_p60.mp4.hwshow [194 bytes] || ", "hits": 739 }, { "id": 14841, "url": "https://svs.gsfc.nasa.gov/14841/", "result_type": "Produced Video", "release_date": "2025-05-12T09:00:00-04:00", "title": "Carruthers Geocorona Observatory Assembly & Testing at BAE Systems", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ", "hits": 63 }, { "id": 14830, "url": "https://svs.gsfc.nasa.gov/14830/", "result_type": "Produced Video", "release_date": "2025-04-23T09:00:00-04:00", "title": "Carruthers Geocorona Observatory Images", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ", "hits": 92 }, { "id": 5522, "url": "https://svs.gsfc.nasa.gov/5522/", "result_type": "Visualization", "release_date": "2025-03-27T12:00:00-04:00", "title": "Arctic Sea Ice Maximum 2025", "description": "Arctic sea ice maximum extent 2025, still image || arctic_sea_ice_max_2025.png (3840x2160) [6.2 MB] || arctic_sea_ice_max_2025_print.jpg (1024x576) [150.6 KB] || arctic_sea_ice_max_2025_web.png (320x180) [73.6 KB] || arctic_sea_ice_max_2025_searchweb.png (320x180) [73.6 KB] || arctic_sea_ice_max_2025_thm.png [5.9 KB] || ", "hits": 359 }, { "id": 5521, "url": "https://svs.gsfc.nasa.gov/5521/", "result_type": "Visualization", "release_date": "2025-03-27T09:15:00-04:00", "title": "Sea Ice Extent 1978-2025", "description": "A graph of sea ice extent from 1978-2025 showing Arctic ice, Antarctic ice, and total sea ice.", "hits": 1172 }, { "id": 14784, "url": "https://svs.gsfc.nasa.gov/14784/", "result_type": "Produced Video", "release_date": "2025-02-13T14:00:00-05:00", "title": "PUNCH Mission Media Teleconference", "description": "NASA held a media teleconference at 2 p.m. EST on Tuesday, February 4, to share information about the agency’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, which is targeted to launch no earlier than Thursday, February 27, 2025.The agency’s PUNCH mission is a constellation of four small satellites. When they arrive in low Earth orbit, the satellites will make global, 3D observations of the Sun’s outer atmosphere, the corona, and help NASA learn how the mass and energy there become solar wind. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission will share a ride to space with NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) space telescope on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.The Southwest Research Institute in Boulder, Colorado, leads the PUNCH mission. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington.To learn more about PUNCH, please visit: nasa.gov/punch || ", "hits": 84 }, { "id": 14773, "url": "https://svs.gsfc.nasa.gov/14773/", "result_type": "Produced Video", "release_date": "2025-02-04T10:00:00-05:00", "title": "NASA's PUNCH Mission", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun’s corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.Watch the video to learn how imaging the Sun’s corona and the solar wind together will help scientists better understand the entire inner heliosphere — Sun, solar wind, and Earth — as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate.For more information visit science.nasa.gov/mission/punch || ", "hits": 84 }, { "id": 14776, "url": "https://svs.gsfc.nasa.gov/14776/", "result_type": "Produced Video", "release_date": "2025-01-30T14:00:00-05:00", "title": "PUNCH Satellites Integration and Testing", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 62 }, { "id": 14770, "url": "https://svs.gsfc.nasa.gov/14770/", "result_type": "Produced Video", "release_date": "2025-01-24T09:00:00-05:00", "title": "PUNCH Satellites Test Operations at Vandenberg Space Force Base", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 53 }, { "id": 14768, "url": "https://svs.gsfc.nasa.gov/14768/", "result_type": "Produced Video", "release_date": "2025-01-23T17:00:00-05:00", "title": "PUNCH Satellites Solar Array Deployment Test", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 71 }, { "id": 14767, "url": "https://svs.gsfc.nasa.gov/14767/", "result_type": "Produced Video", "release_date": "2025-01-23T16:00:00-05:00", "title": "PUNCH Satellites Arrival at Vandenberg Space Force Base", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 58 }, { "id": 14765, "url": "https://svs.gsfc.nasa.gov/14765/", "result_type": "Produced Video", "release_date": "2025-01-23T15:00:00-05:00", "title": "PUNCH Assembly and Testing", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 66 }, { "id": 5382, "url": "https://svs.gsfc.nasa.gov/5382/", "result_type": "Visualization", "release_date": "2024-09-24T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2024", "description": "Animation of Arctic sea ice maximum extent, March 14 2024, to its minimum, September 11, 2024 || sea_ice_2024_min_2160p60.2608_print.jpg (1024x576) [152.6 KB] || sea_ice_2024_min_2160p60.2608_searchweb.png (320x180) [74.6 KB] || sea_ice_2024_min_2160p60.2608_thm.png (80x40) [6.0 KB] || sea_ice_2024_min_1080p60.mp4 (1920x1080) [38.2 MB] || sea_ice_min_2024 [0 Item(s)] || sea_ice_2024_min_2160p60.mp4 (3840x2160) [106.6 MB] || antarctic_arctic_seaice_comp_5x3.hwshow || ", "hits": 458 }, { "id": 14690, "url": "https://svs.gsfc.nasa.gov/14690/", "result_type": "Produced Video", "release_date": "2024-09-23T14:00:00-04:00", "title": "Ten Years at Mars with NASA’s MAVEN Mission", "description": "During its first decade at Mars, MAVEN has helped to explain how the Red Planet evolved from warm and wet into the cold, dry world we see today. Complete transcript available.Universal Production Music: “Executive Deceit” by Samuel Karl Bohn [PRS], Chalk Music [PRS]; “Quasar” by Ross Stephen Gilmartin [PRS], Chappell Recorded Music Library Ltd [PRS]; “Modular Odyssey” and “Synthology” by Laetitia Frenod [SACEM], Koka Media [SACEM]Watch this video on the NASA Goddard YouTube channel. || MAVEN-10th-Anniversary-Preview_print.jpg (1024x576) [160.7 KB] || MAVEN-10th-Anniversary-Preview.jpg (1280x720) [622.5 KB] || MAVEN-10th-Anniversary-Preview.png (1280x720) [1.2 MB] || MAVEN-10th-Anniversary-Preview_searchweb.png (320x180) [80.6 KB] || MAVEN-10th-Anniversary-Preview_thm.png (80x40) [6.3 KB] || 14690_MAVEN_10th_Anniversary_720.mp4 (1280x720) [92.2 MB] || 14690_MAVEN_10th_Anniversary_1080.mp4 (1920x1080) [516.6 MB] || Maven10thAnniversaryCaptionsV3.en_US.srt [8.9 KB] || Maven10thAnniversaryCaptionsV3.en_US.vtt [8.5 KB] || 14690_MAVEN_10th_Anniversary_4K.mp4 (3840x2160) [6.3 GB] || 14690_MAVEN_10th_Anniversary_ProRes.mov (3840x2160) [36.5 GB] || ", "hits": 60 }, { "id": 14640, "url": "https://svs.gsfc.nasa.gov/14640/", "result_type": "Produced Video", "release_date": "2024-08-13T08:00:00-04:00", "title": "Touching the Sun with Solar Stones", "description": "In August 2024, the Heliophysics Big Year theme is Kids and Education. In collaboration with NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission and the Colorado School for the Deaf and Blind, Creative Technology and Design students at the ATLAS Institute at University of Colorado Boulder have developed tactile representations of what many scholars believe to be the earliest known record of solar observations. Titled “Solar Stones,” the exhibit displays two famous petroglyphs, or rock carvings, found in Chaco Culture National Historical Park located in northwestern New Mexico. One petroglyph is believed to represent a total solar eclipse occurring on July 11, 1097, and the other a solar marker that indicates the annual equinoxes and solstices. The project is on display at Fiske Planetarium located on the University of Colorado Boulder campus.The Heliophysics Big Year is a global celebration of the Sun’s influence on Earth and the entire solar system. From Oct. 14, 2023, to Dec. 24, 2024, we are challenging you to participate in as many Sun-related activities as you can.For each month from October 2023 to December 2024, the Heliophysics Big Year will celebrate under a theme, sharing opportunities to participate in many solar science events from watching eclipses to joining citizen science projects. During the Heliophysics Big Year, participation isn’t limited to science – NASA invites everyone to celebrate the Sun with activities including dance, fashion, sustainability, and more. || ", "hits": 76 }, { "id": 5200, "url": "https://svs.gsfc.nasa.gov/5200/", "result_type": "Visualization", "release_date": "2023-12-11T12:00:00-05:00", "title": "Mars Disappearing Solar Wind: MAVEN Visualizations", "description": "This data visualization depicts a period of decreased solar wind at Mars that occurred on December 25, 2022, causing the planet’s magnetosphere to expand outward. Ion velocity and density data collected by the MAVEN spacecraft is presented using a color-mapped satellite orbit tail and vectors along MAVEN’s orbit. || maven_solar_wind_comp.02715_print.jpg (1024x576) [84.4 KB] || maven_solar_wind_comp.02715_searchweb.png (320x180) [47.3 KB] || maven_solar_wind_comp.02715_thm.png (80x40) [4.3 KB] || maven_solar_wind_comp (3840x2160) [0 Item(s)] || maven_solar_wind_comp_2160p60.mp4 (3840x2160) [187.6 MB] || maven_solar_wind_comp_prores.mov (3840x2160) [10.1 GB] || ", "hits": 287 }, { "id": 14477, "url": "https://svs.gsfc.nasa.gov/14477/", "result_type": "Produced Video", "release_date": "2023-12-11T12:00:00-05:00", "title": "The Day the Solar Wind Disappeared from Mars", "description": "Learn about the “disappearance” of the solar wind at Mars that was witnessed by MAVEN – an event last seen nearly a quarter-century ago at Earth.Complete transcript available.Universal Production Music: “Space Museum” by Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]; “Currents and Crime Scenes” by Dylan Matthew Love and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || MAVEN_Solar_Wind_Disappear_V4_print.jpg (1024x576) [142.7 KB] || MAVEN_Solar_Wind_Disappear_V4.jpg (1280x720) [459.3 KB] || MAVEN_Solar_Wind_Disappear_V4.png (1280x720) [800.2 KB] || MAVEN_Solar_Wind_Disappear_V4_searchweb.png (320x180) [69.9 KB] || MAVEN_Solar_Wind_Disappear_V4_thm.png (80x40) [6.5 KB] || 14477_MAVEN_Solar_Wind_Disappear_720.mp4 (1280x720) [43.4 MB] || 14477_MAVEN_Solar_Wind_Disappear_1080.mp4 (1920x1080) [243.1 MB] || MavenSolarWindCaptionsV2.en_US.srt [3.8 KB] || MavenSolarWindCaptionsV2.en_US.vtt [3.6 KB] || 14477_MAVEN_Solar_Wind_Disappear_4K.mp4 (3840x2160) [3.0 GB] || 14477_MAVEN_Solar_Wind_Disappear_ProRes.mov (3840x2160) [20.7 GB] || ", "hits": 156 }, { "id": 5162, "url": "https://svs.gsfc.nasa.gov/5162/", "result_type": "Visualization", "release_date": "2023-09-25T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2023", "description": "Animation of Arctic sea ice maximum extent, March 6 2023, to its minimum, September 19, 2023 || arctic_sea_ice_2023_min_2160p60.2820_print.jpg (1024x576) [138.6 KB] || arctic_sea_ice_min_2023 (3840x2160) [0 Item(s)] || arctic_sea_ice_2023_min_2160p60_p60.mp4 (3840x2160) [107.4 MB] || ", "hits": 137 }, { "id": 14362, "url": "https://svs.gsfc.nasa.gov/14362/", "result_type": "Produced Video", "release_date": "2023-06-13T12:00:00-04:00", "title": "High Above Down Under Series", "description": "Around a different star, Earth may never have developed life at all. So what makes a star friendly to life? We joined two rocket teams as they traveled to the remote Northern Territory of Australia to capture light from our closest stellar neighbors to help reveal the answer. Follow their journey in the 6-part video series High Above Down Under. Episodes released weekly starting June 27, 2023. || ", "hits": 58 }, { "id": 5030, "url": "https://svs.gsfc.nasa.gov/5030/", "result_type": "Visualization", "release_date": "2022-09-22T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2022", "description": "Arctic Sea Ice Minimum 2022, Animation || sea_ice_2022_min_1080p60.03100_print.jpg (1024x576) [125.6 KB] || sea_ice_2022_min_1080p60.03100_searchweb.png (180x320) [71.7 KB] || sea_ice_2022_min_1080p60.03100_thm.png (80x40) [6.2 KB] || full (1920x1080) [0 Item(s)] || sea_ice_2022_min_1080p60.mp4 (1920x1080) [31.1 MB] || sea_ice_2022_min_1080p60.webm (1920x1080) [7.1 MB] || sea_ice_2022_min_1080p60.hwshow [89 bytes] || ", "hits": 81 }, { "id": 14204, "url": "https://svs.gsfc.nasa.gov/14204/", "result_type": "Produced Video", "release_date": "2022-08-31T09:00:00-04:00", "title": "Mars Patchy Proton Aurora", "description": "NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission and the United Arab Emirates’ Emirates Mars Mission (EMM) have released joint observations of dynamic proton aurora events at Mars. Remote auroral observations by EMM paired with in-situ plasma observations made by MAVEN open new avenues for understanding the Martian atmosphere. This collaboration was made possible by recent data-sharing between the two missions and highlights the value of multi-point observations in space.Learn more about this discovery by MAVEN and EMM. || ", "hits": 85 }, { "id": 14164, "url": "https://svs.gsfc.nasa.gov/14164/", "result_type": "Produced Video", "release_date": "2022-06-07T19:00:00-04:00", "title": "Australia Sounding Rocket Campaign Press Kit", "description": "NASA will launch three suborbital sounding rockets in June and July 2022 from the Arnhem Space Center in Australia’s Northern Territory to conduct astrophysics studies that can only be done from the Southern Hemisphere. The three missions will focus on α Centauri A and B, two of the three-star α Centauri system that are the closest stars to our Sun, and X-rays emanating from the interstellar medium, clouds of gases and particles between stars.The three sounding rocket night-time missions will be launched between June 26 and July 12 on two-stage Black Brant IX sounding rockets, from the Arnhem Space Center, which is owned and operated by Equatorial Launch Australia or ELA. The Arnhem Space Center is a commercial space launch facility, located on the Dhupuma Plateau near Nhulunbuy. The NASA missions will be the first launches from Arnhem.Learn more: Australia Sounding Rocket Fact SheetWatch more: Sounding Rockets: Cutting Edge Science, 15 Minutes at a TimeWhat Is a Sounding Rocket?Riding Along with a NASA Sounding Rocket || ", "hits": 71 }, { "id": 31171, "url": "https://svs.gsfc.nasa.gov/31171/", "result_type": "Hyperwall Visual", "release_date": "2021-12-14T00:00:00-05:00", "title": "How do we know for sure about Atmospheric Aerosols?", "description": "Dr. Brent Holben explains how NASA's program of global ground-based sun photometers measure aerosols at the surface and why those measurements are so vital to understanding the Earth's processes at the 2021 United Nations Climate Change Conference. Also available on YouTube || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_print.jpg (1024x576) [112.3 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_searchweb.png (320x180) [81.8 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_thm.png (80x40) [7.0 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.mp4 (1280x720) [135.7 MB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.webm (1280x720) [110.7 MB] || AERONET-COP26-talk2021.en_US.srt [19.2 KB] || AERONET-COP26-talk2021.en_US.vtt [19.0 KB] || ", "hits": 70 }, { "id": 13944, "url": "https://svs.gsfc.nasa.gov/13944/", "result_type": "Produced Video", "release_date": "2021-10-14T14:00:00-04:00", "title": "Lucy L-2 Engineering Briefing", "description": "NASA will hold a virtual media briefing at 3 p.m. EDT Thursday, October 14th, to preview the engineering behind the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun. The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Lucy engineering briefing participants include:• Joan Salute, associate director for flight programs, Planetary Science Division, NASA Headquarters.• Katie Oakman, Lucy structures and mechanisms lead, Lockheed Martin Space.• Jessica Lounsbury, Lucy project systems engineer, Goddard.• Coralie Adam, deputy navigation team chief, KinetX Aerospace.Over its 12-year primary mission, Lucy will explore a record-breaking number of asteroids. The spacecraft will fly by one asteroid in the solar system’s main belt and seven Trojan asteroids. Lucy’s path will circle back to Earth three times for gravity assists, which will make it the first spacecraft ever to return to our planet’s vicinity from the outer solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida. Lucy’s principal investigator is based out of the Boulder, Colorado, branch of Southwest Research Institute (SwRI), headquartered in San Antonio, Texas. NASA’s Goddard Space Flight Center in Greenbelt, Maryland provides overall mission management, systems engineering, and safety and mission assurance. Lockheed Martin Space in Littleton, Colorado, built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the agency’s Science Mission Directorate in Washington. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida. || ", "hits": 22 }, { "id": 13946, "url": "https://svs.gsfc.nasa.gov/13946/", "result_type": "Produced Video", "release_date": "2021-10-01T15:00:00-04:00", "title": "Landsat 9 Launch Footage", "description": "Video showing the countdown and launch of Landsat 9, on Monday, Sept 27, 2021. The satellite launched at 2:12pm EDT, from Vandenberg Space Force Base in California, riding on and Atlas V rocket. || L9_launch_footage_print.jpg (1280x720) [232.9 KB] || L9_launch_footage_print_searchweb.png (320x180) [70.4 KB] || L9_launch_footage_print_thm.png (80x40) [5.3 KB] || L9_launch_footage.mp4 (1280x720) [42.0 MB] || L9_launch_footage.webm (1280x720) [6.7 MB] || L9_launch_footage-captions.en_US.srt [1.0 KB] || L9_launch_footage-captions.en_US.vtt [997 bytes] || ", "hits": 85 }, { "id": 13933, "url": "https://svs.gsfc.nasa.gov/13933/", "result_type": "Produced Video", "release_date": "2021-09-28T13:00:00-04:00", "title": "Lucy L-20 Briefing", "description": "NASA will hold a virtual media briefing at 2 p.m. EDT Tuesday, Sept. 28, to preview the launch of the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun.The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Participants in Tuesday's briefing will include:• Alana Johnson, Senior Communications Specialist, NASA Planetary Science Division• Lori Glaze, director of NASA's Planetary Science Division at NASA Headquarters in Washington.• Hal Levison, Lucy Principal Investigator, Southwest Research Institute in Boulder, Colorado.• Keith Noll, Lucy Project Scientist, NASA’s Goddard Space Flight Center in Greenbelt, Maryland. • Rich Lipe, Lockheed Marin Spacecraft Program Manager, Denver, Colorado. • Donya Douglas-Bradshaw, Lucy Project Manager, NASA Goddard Space Flight Center in Greenbelt, Maryland.Over its 12-year primary mission, Lucy will explore a record number of asteroids in separate orbits around the Sun. The spacecraft will fly by one asteroid in the solar system’s main belt, located between the orbits of Mars and Jupiter, followed by seven Trojans. In addition, Lucy’s path will circle back to Earth three times for gravity assists, making it the first spacecraft ever to travel out to the distance of Jupiter and return to the vicinity of Earth.The Lucy mission is named after the fossilized skeleton of an early hominin (pre-human ancestor) discovered in Ethiopia in 1974 and named “Lucy” by the team of paleoanthropologists who discovered it. Just as the Lucy fossil provided unique insights into humanity’s evolution, the Lucy mission promises to revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida.Southwest Research Institute is the home institution of the principal investigator. NASA Goddard Space provides overall mission management, systems engineering, plus safety and mission assurance. Lockheed Martin Space built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the Science Mission Directorate. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida.For more information about Lucy, visit: http://www.nasa.gov/lucy || ", "hits": 29 }, { "id": 4941, "url": "https://svs.gsfc.nasa.gov/4941/", "result_type": "Visualization", "release_date": "2021-09-22T11:00:00-04:00", "title": "Arctic Sea Ice Minimum 2021", "description": "Arctic Sea Ice Minimum 2021, Animation || sea_ice_2021_min_1080p60.02820_print.jpg (1024x576) [162.7 KB] || sea_ice_2021_min_1080p60.02820_searchweb.png (320x180) [82.1 KB] || sea_ice_2021_min_1080p60.02820_thm.png (80x40) [14.7 KB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || sea_ice_2021_min_1080p60.mp4 (1920x1080) [41.3 MB] || sea_ice_2021_min_1080p60.webm (1920x1080) [7.6 MB] || ", "hits": 44 }, { "id": 13932, "url": "https://svs.gsfc.nasa.gov/13932/", "result_type": "Produced Video", "release_date": "2021-09-15T10:00:00-04:00", "title": "Riding Along With a NASA Sounding Rocket (2021)", "description": "On Sept. 9, 2021, a sounding rocket launched from the White Sands Missile Range in New Mexico, carrying a copy of the Extreme Ultraviolet Variability Experiment, or EVE. This flight was used to calibrate the identical version of EVE that has flown in space since 2010 aboard NASA’s Solar Dynamics Observatory (SDO). Over the years, the space-based EVE has become degraded by intense sunlight, so scientists fly periodic calibration missions to keep EVE’s measurements sharp. || ", "hits": 52 }, { "id": 13919, "url": "https://svs.gsfc.nasa.gov/13919/", "result_type": "Produced Video", "release_date": "2021-08-31T10:00:00-04:00", "title": "Landsat 9 L-16 Press Briefing Graphics", "description": "Officials from NASA and the U.S. Geological Survey (USGS) discussed the upcoming launch of the Landsat 9 satellite during a media briefing at 10 a.m. EDT Tuesday, Aug. 31.The Landsat 9 launch is targeted for no earlier than Thursday, Sept. 23, 2021.The media briefing will air live on NASA TV, the NASA app, and the agency’s website.Data from Landsat 9 will add to nearly 50 years of free and publicly available data from the Landsat program. The Landsat program is the longest-running enterprise for acquisition of satellite imagery of Earth. It is a joint NASA/USGS program. Researchers harmonize Landsat data to detect the footprint of human activities and measure the effects of climate change on land over decades.Once fully operational in orbit, Landsat 9 will replace Landsat 7 and join its sister satellite, Landsat 8, in continuing to collect data from across the planet every eight days. This calibrated data will continue the Landsat program’s critical role in monitoring land use and helping decision-makers manage essential resources including crops, water resources, and forests.Briefing participants, in speaking order, are:•Karen St. Germain, director of NASA's Earth Science Division•Del Jenstrom, Landsat 9 project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland•Jeff Masek, Landsat 9 project scientist at Goddard•David Applegate, acting director of USGS•Birgit Peterson, geographer at USGS•Inbal Becker-Reshef, director of NASA’s Harvest food security and agriculture program.NASA manages the Landsat 9 mission. Goddard teams also built and tested one of the two instruments on Landsat 9, the Thermal Infrared Sensor 2 (TIRS-2) instrument. TIRS-2 will use thermal imaging to make measurements that are used to calculate soil moisture and detect the health of plants.The USGS Earth Resources Observation and Science Center in Sioux Falls, South Dakota, will operate the mission and manage the ground system, including maintaining the Landsat archive. Ball Aerospace in Boulder, Colorado, built and tested the Operational Land Imager 2 (OLI-2) instrument, another imaging sensor that provides data in the visible, near infrared, and shortwave infrared portions of the spectrum. United Launch Alliance is the rocket provider for Landsat 9’s launch. Northrop Grumman in Gilbert, Arizona, built the Landsat 9 spacecraft, integrated it with instruments, and tested the observatory.For more information:Media AdvisoryLandsat Video Resourceshttps://landsat.gsfc.nasa.gov/https://www.usgs.gov/landsat || ", "hits": 50 }, { "id": 4908, "url": "https://svs.gsfc.nasa.gov/4908/", "result_type": "Visualization", "release_date": "2021-06-30T11:00:00-04:00", "title": "Climate Drivers", "description": "Data visualization of human and natural drivers of climate change for the period 1850-2018, showcasing data products from NASA's GISS Model E 2.1-G and observations.Dr. Gavin Schmidt uses this visual to explain NASA's role in tracking and predicting climate at the 2021 COP26 conference - https://www.youtube.com/watch?v=CCAcKuJaJOg. || ClimateDrivers_3840x2160_30fps_923_print.jpg (1024x576) [106.7 KB] || ClimateDrivers_3840x2160_30fps_923_searchweb.png (320x180) [44.7 KB] || ClimateDrivers_3840x2160_30fps_923_thm.png (80x40) [4.9 KB] || ClimateDrivers_1080p30.mp4 (1920x1080) [13.2 MB] || ClimateDrivers_1080p30.webm (1920x1080) [3.6 MB] || Composite (3840x2160) [0 Item(s)] || ClimateDrivers_3840x2160p30.mp4 (3840x2160) [36.1 MB] || ClimateDrivers_3840x2160_30fps_923.tif (3840x2160) [31.7 MB] || ClimateDrivers_1080p30.mp4.hwshow || ", "hits": 280 }, { "id": 13849, "url": "https://svs.gsfc.nasa.gov/13849/", "result_type": "Produced Video", "release_date": "2021-05-04T11:00:00-04:00", "title": "NASA’s OSIRIS-REx Begins its Journey Home with a Bounty of Asteroid Sample Live Shots", "description": "Associated b-roll will be added by Friday May 7 by 5:00 p.m. EDT || OREX_banner_new.jpg (4800x1670) [6.8 MB] || OREX_banner_new_print.jpg (1024x356) [357.6 KB] || OREX_banner_new_searchweb.png (320x180) [109.2 KB] || OREX_banner_new_thm.png (80x40) [11.1 KB] || ", "hits": 38 }, { "id": 4896, "url": "https://svs.gsfc.nasa.gov/4896/", "result_type": "Visualization", "release_date": "2021-04-19T09:30:00-04:00", "title": "Dust Reduction - Intertropical Convergence Zone (ITCZ) Movement", "description": "This visualization depicts the northern trend of the Intertropical Convergence Zone (ITCZ). A horizontal black line indicates the current ITCZ centroid for the longitudinal extents of the study region, which moves with GPCP precipitation data. The northernmost extent of the ITCZ is indicated with a thin white line for each year. The bold white line represents the northernmost overall extent. The grey box represents the study region used to calculate the ITCZ centroid. A region of dust optical depth data is shown in orange off the coast of Africa. || itcz_movement_dust_01.2410_print.jpg (1024x576) [108.8 KB] || itcz_movement_dust_01.2410_searchweb.png (320x180) [72.8 KB] || itcz_movement_dust_01.2410_thm.png (80x40) [6.4 KB] || itcz_movement_dust_1080p30.mp4 (1920x1080) [34.7 MB] || itcz_movement_dust_1080p60.mp4 (1920x1080) [38.1 MB] || itcz_movement_dust_1080p30.webm (1920x1080) [6.0 MB] || ITCZ_movement_with_dust (3840x2160) [0 Item(s)] || itcz_movement_dust_2160p30.mp4 (3840x2160) [104.0 MB] || itcz_movement_dust_2160p60.mp4 (3840x2160) [114.1 MB] || itcz_movement_dust_1080p30.mp4.hwshow [192 bytes] || ", "hits": 127 }, { "id": 13837, "url": "https://svs.gsfc.nasa.gov/13837/", "result_type": "Produced Video", "release_date": "2021-04-15T14:00:00-04:00", "title": "OSIRIS-REx Leaves its Mark on Asteroid Bennu", "description": "New images taken by the OSIRIS-REx spacecraft on April 7, 2021 show how the spacecraft's Touch-and-Go (TAG) sample acquisition event impacted the surface of asteroid Bennu.Music is \"Go for Launch\" by David Scott Butler of Universal Production MusicWatch this video on the NASA Goddard YouTube channel. || 13837thumbnail.jpg (1440x810) [550.3 KB] || 13837_OSIRISREx_Flyover.00241_searchweb.png (320x180) [77.1 KB] || 13837_OSIRISREx_Flyover.00241_thm.png (80x40) [3.5 KB] || 13837_OSIRISREx_Flyover_facebook_720.mp4 (1280x720) [90.3 MB] || 13837_OSIRISREx_Flyover_twitter_720.mp4 (1280x720) [16.5 MB] || 13837_OSIRISREx_Flyover.mp4 (3840x2160) [97.6 MB] || 13837_caption.en_US.srt [1.8 KB] || 13837_caption.en_US.vtt [1.7 KB] || 13837_OSIRISREx_Flyover.webm (3840x2160) [30.2 MB] || ", "hits": 46 }, { "id": 13803, "url": "https://svs.gsfc.nasa.gov/13803/", "result_type": "Produced Video", "release_date": "2021-02-08T06:00:00-05:00", "title": "Destination Mars! On February 18 NASA’s Newest and Most Ambitious Rover Lands on the Red Planet", "description": "Click here for Mars 2020 Perseverance Rover press kit.Quick link to cut B-ROLL for the LIVE SHOTSQuick link to canned interview with KEITH COMEAUXQuick link to PROMO for Spanish language show || MARS_landing_copy_print.jpg (1024x524) [309.4 KB] || MARS_landing_copy.jpg (2099x1075) [773.4 KB] || MARS_landing_copy_searchweb.png (320x180) [82.3 KB] || MARS_landing_copy_thm.png (80x40) [23.8 KB] || ", "hits": 57 }, { "id": 20324, "url": "https://svs.gsfc.nasa.gov/20324/", "result_type": "Animation", "release_date": "2020-10-20T00:00:00-04:00", "title": "OSIRIS-REx \"What If?\" Scenarios: Animations", "description": "\"Wave Off\" Scenario || OSIRIS-RExWaveOffThumbnail_print.jpg (1024x576) [195.3 KB] || OSIRIS-RExWaveOffThumbnail.jpg (3840x2160) [3.2 MB] || OSIRIS-RExWaveOffThumbnail_searchweb.png (320x180) [97.1 KB] || OSIRIS-RExWaveOffThumbnail_thm.png (80x40) [5.5 KB] || P_OREx_0620_What_If_Sc1 (3840x2160) [0 Item(s)] || P_ORex_0620_What_If_Sc1.mp4 (3840x2160) [46.0 MB] || P_ORex_0620_What_If_Sc1.webm (3840x2160) [12.2 MB] || P_ORex_0620_What_If_Sc1.mov (3840x2160) [3.9 GB] || ", "hits": 27 }, { "id": 13738, "url": "https://svs.gsfc.nasa.gov/13738/", "result_type": "Produced Video", "release_date": "2020-10-19T11:30:00-04:00", "title": "OSIRIS-REx Science and Engineering Briefing", "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ", "hits": 63 }, { "id": 13731, "url": "https://svs.gsfc.nasa.gov/13731/", "result_type": "Produced Video", "release_date": "2020-10-14T21:00:00-04:00", "title": "OSIRIS-REx Live Shots: NASA Will Make U.S. History Next Week Snagging Samples From An Asteroid For Return To Earth", "description": "Quick link to the OSIRIS-REx team cheering after a successful TAG maneuver on Tuesday, Oct 20Quick link to B-ROLL for the live shotsClick here for OSIRIS-REx PRESS KITClick here for Latest releaseLatest release in Spanish.OSIRIS-REx poster COLLECTABLESWhy Bennu? 10 Reasons***NASA's OSIRIS-REx spacecraft is going Asteroid Hunting. Listen now to NASA's \"Curious Universe\" podcast that takes you inside the daring mission || OREX_banner_new.jpg (4800x1670) [6.8 MB] || OREX_banner_new_print.jpg (1024x356) [357.6 KB] || OREX_banner_new_searchweb.png (320x180) [109.2 KB] || OREX_banner_new_thm.png (80x40) [11.1 KB] || ", "hits": 35 }, { "id": 4863, "url": "https://svs.gsfc.nasa.gov/4863/", "result_type": "Visualization", "release_date": "2020-10-08T14:00:00-04:00", "title": "Tour of Asteroid Bennu – Visualizations", "description": "This first shot of the sequence begins with OSIRIS-REx’s arrival at the asteroid Bennu. A low resolution view of the asteroid is presented and thermal inertia data fades in, representing our initial understanding of the asteroid. The asteroid then spins quickly to serve as a transition to the second shot in the sequence. || bennu_tour_shot_01.1870_print.jpg (1024x576) [22.9 KB] || bennu_tour_shot_01 (1920x1080) [0 Item(s)] || bennu_tour_shot_01_1080p30.mp4 (1920x1080) [11.9 MB] || bennu_tour_shot_01_1080p30.webm (1920x1080) [7.7 MB] || 4863_Bennu_Tour_Shot_1.mov (1920x1080) [681.5 MB] || bennu_tour_shot_01 (3840x2160) [0 Item(s)] || bennu_tour_shot_01_2160p30.mp4 (3840x2160) [44.0 MB] || bennu_tour_shot_01_1080p30.mp4.hwshow || ", "hits": 54 }, { "id": 13724, "url": "https://svs.gsfc.nasa.gov/13724/", "result_type": "Produced Video", "release_date": "2020-09-24T14:25:00-04:00", "title": "OSIRIS-REx: Countdown to TAG", "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ", "hits": 78 }, { "id": 4860, "url": "https://svs.gsfc.nasa.gov/4860/", "result_type": "Visualization", "release_date": "2020-09-21T13:20:00-04:00", "title": "Arctic Sea Ice Minimum 2020", "description": "Animation of Arctic sea ice extent from the Mar. 5, 2020 maximum to the Sept. 15, 2020 minimum, 30-year average extents in yellow || arctic_sea_ice_min_2020.1410_print.jpg (1024x576) [135.2 KB] || arctic_sea_ice_min_2020.1410_print_searchweb.png (320x180) [72.1 KB] || arctic_sea_ice_min_2020.1410_print_thm.png (80x40) [6.3 KB] || yellow_average (1920x1080) [0 Item(s)] || arctic_sea_ice_min_2020_1080p30_y.mp4 (1920x1080) [29.3 MB] || arctic_sea_ice_min_2020_1080p30_y.webm (1920x1080) [6.3 MB] || ", "hits": 89 }, { "id": 13714, "url": "https://svs.gsfc.nasa.gov/13714/", "result_type": "Produced Video", "release_date": "2020-09-15T13:00:00-04:00", "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means", "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ", "hits": 208 }, { "id": 4834, "url": "https://svs.gsfc.nasa.gov/4834/", "result_type": "Visualization", "release_date": "2020-08-31T11:00:00-04:00", "title": "First Global Survey of Glacial Lakes Shows 30-Years of Dramatic Growth", "description": "Data visualization featuring the glacier rich region of the Himalayas, along with many of Earth’s highest peaks. The visualization sequence starts with a wide view of the Tibetan plateau and moves along a hiking path highlighting Mt. Everest, Mt. Lhotse, Mt Nuptse, the Everest Base Camp, the Khumbhu glacier, all the way to Imja Lake. Moving to a top-down view of Imja Lake, a time series of Landsat data unveils its dramatic growth for the period 1989-2019.This video is also available on our YouTube channel. || imja_final_4k.4600_print.jpg (1024x576) [114.8 KB] || imja_final_4k.4600_searchweb.png (320x180) [101.5 KB] || imja_final_4k.4600_web.png (320x180) [101.5 KB] || imja_final_4k.4600_thm.png (80x40) [7.5 KB] || imja_final_HD_1080p60.mp4 (1920x1080) [72.9 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || imja_final_HD_1080p60.webm (1920x1080) [19.7 MB] || with_cities (3840x2160) [0 Item(s)] || captions_silent.30013.en_US.srt [43 bytes] || imja_final_4k_2160p60.mp4 (3840x2160) [215.1 MB] || imja_final_2160p60_prores.mov (3840x2160) [16.9 GB] || ", "hits": 133 }, { "id": 4730, "url": "https://svs.gsfc.nasa.gov/4730/", "result_type": "Visualization", "release_date": "2020-05-25T11:00:00-04:00", "title": "MAVEN – Mars Electric Current Systems", "description": "The current systems formed around Mars as a result of a solar wind driven convective electric field(Note: These frame sets were converted to the sRGB color space on 6/16/2020)This video is also available on our YouTube channel. || ideal_currents_1080.00600_print.jpg (1024x576) [71.1 KB] || ideal_currents_1080.00600_searchweb.png (320x180) [21.7 KB] || ideal_currents_1080.00600_thm.png (80x40) [2.0 KB] || ideal_currents_1080p30.mp4 (1920x1080) [74.0 MB] || ideal_currents_1080.webm (1920x1080) [9.9 MB] || ideal_curr (1920x1080) [0 Item(s)] || ideal_curr (3840x2160) [0 Item(s)] || captions_silent.25991.en_US.srt [43 bytes] || ideal_currents_4k_2160p30.mp4 (3840x2160) [170.1 MB] || idealized_currents_prores.mov (1920x1080) [2.9 GB] || Mars_idealized_currents_4k_prores.mov (3840x2160) [3.5 GB] || ideal_currents_1080p30.mp4.hwshow || ", "hits": 182 }, { "id": 13625, "url": "https://svs.gsfc.nasa.gov/13625/", "result_type": "Produced Video", "release_date": "2020-05-25T11:00:00-04:00", "title": "First Map of Mars Electric Currents", "description": "MAVEN data have enabled the first map of the electric current systems (blue and red arrows) that shape the induced magnetic field surrounding Mars.Credit: NASA/Goddard/MAVEN/CU Boulder/SVSUniversal Production Music: “A Lucid Dream” and “Shimmer Oscillations” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MarsElectricCurrentsPreview6_print.jpg (1024x576) [305.8 KB] || MarsElectricCurrentsPreview6.jpg (1920x1080) [853.6 KB] || MarsElectricCurrentsPreview6_searchweb.png (320x180) [50.6 KB] || MarsElectricCurrentsPreview6_thm.png (80x40) [5.3 KB] || 13625_Mars_Electric_Currents_Twitter.mp4 (1280x720) [63.8 MB] || 13625_Mars_Electric_Currents_Facebook.mp4 (1920x1080) [359.1 MB] || 13625_Mars_Electric_Currents_YouTube.webm (3840x2160) [91.7 MB] || 13625_Mars_Electric_Currents_Captions.en_US.srt [7.2 KB] || 13625_Mars_Electric_Currents_Captions.en_US.vtt [6.8 KB] || 13625_Mars_Electric_Currents_YouTube.mp4 (3840x2160) [2.8 GB] || 13625_Mars_Electric_Currents_MASTER.mov (3840x2160) [14.2 GB] || 13625_Mars_Electric_Currents_Facebook.mp4.hwshow [134 bytes] || ", "hits": 102 }, { "id": 4824, "url": "https://svs.gsfc.nasa.gov/4824/", "result_type": "Visualization", "release_date": "2020-05-25T00:00:00-04:00", "title": "MAVEN Observes Solar Particle Velocities and the Induced Magnetic Field", "description": "MAVEN orbits Mars and measures solar particle velocities and variations in the solar wind’s magnetic field. || maven_vels_magField.03000_print.jpg (1024x576) [92.5 KB] || maven_vels_magField.03000_searchweb.png (320x180) [63.5 KB] || maven_vels_magField.03000_thm.png (80x40) [4.2 KB] || maven_vels_magField_1080p30.mp4 (1920x1080) [83.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || maven_vels_magField_1080p30.webm (1920x1080) [19.0 MB] || 4824_MAVEN_Solar_Wind_Data_1080_30p.mov (1920x1080) [2.6 GB] || maven_vels_magField_1080p30.mp4.hwshow [193 bytes] || ", "hits": 94 }, { "id": 4825, "url": "https://svs.gsfc.nasa.gov/4825/", "result_type": "Visualization", "release_date": "2020-05-25T00:00:00-04:00", "title": "MAVEN – Mars and Solar Wind Simulation", "description": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded. || maven_cme44.03600_print.jpg (1024x512) [253.9 KB] || maven_cme44.03600_searchweb.png (320x180) [92.7 KB] || maven_cme44.03600_thm.png (80x40) [5.2 KB] || 1920x1080_16x9_30p (2048x1024) [0 Item(s)] || maven_cme44_1024p30.webm (2048x1024) [5.9 MB] || maven_cme44_1024p30.mp4 (2048x1024) [195.1 MB] || maven_cme44_1024p30.mp4.hwshow [58 bytes] || ", "hits": 65 }, { "id": 13610, "url": "https://svs.gsfc.nasa.gov/13610/", "result_type": "Produced Video", "release_date": "2020-05-18T00:00:00-04:00", "title": "Snow Scientists Dig Deep in Grand Mesa", "description": "Music: \"Storm Chasers,\" \"Black Coffee,\" \"From Small Beginnings,\" Universal Production MusicComplete transcript available. || SnowEx2020_thumb_print.jpg (1024x569) [77.1 KB] || SnowEx2020_thumb.png (2970x1652) [3.2 MB] || SnowEx2020_thumb_searchweb.png (320x180) [67.2 KB] || SnowEx2020_thumb_thm.png (80x40) [7.9 KB] || SnowEx_Wrap_v2.webm (1920x1080) [34.2 MB] || SnowEx_Wrap_v2.mp4 (1920x1080) [322.6 MB] || SnowEx2020_YouTube.mp4 (1920x1080) [509.7 MB] || SnowEx2020.en_US.srt [6.2 KB] || SnowEx2020.en_US.vtt [6.3 KB] || SnowEx2020_prores.mov (1920x1080) [4.3 GB] || ", "hits": 36 }, { "id": 4795, "url": "https://svs.gsfc.nasa.gov/4795/", "result_type": "Animation", "release_date": "2020-02-26T16:00:00-05:00", "title": "OSIRIS-REx – Global Model of Asteroid Bennu", "description": "Looping animation of asteroid Bennu rotating. This 3D model of Bennu was created using 20cm resolution laser altimetry data and imagery taken by OSIRIS-REx. || Bennu_spin_full_20cm.1000_print.jpg (1024x576) [82.7 KB] || Bennu_spin_full_20cm.1000_searchweb.png (320x180) [17.4 KB] || Bennu_spin_full_20cm.1000_thm.png (80x40) [1.5 KB] || Bennu_spin_full_20cm_1080p30.webm (1920x1080) [14.4 MB] || Bennu_spin_full_20cm_1080p30.mp4 (1920x1080) [111.9 MB] || Bennu_GlobalSpin_20cm (3840x2160) [0 Item(s)] || Bennu_spin_full_20cm_2160p30.mp4 (3840x2160) [351.8 MB] || 4771_20cm_Bennu_Global_Spin.mov (3840x2160) [8.1 GB] || Bennu_spin_full_20cm_1080p30.mp4.hwshow [194 bytes] || ", "hits": 116 }, { "id": 13482, "url": "https://svs.gsfc.nasa.gov/13482/", "result_type": "Produced Video", "release_date": "2020-01-13T10:00:00-05:00", "title": "Lucy Mission Overview: Journey to Explore the Trojan Asteroids", "description": "An overview of the Lucy Mission and its targets, the Trojan Asteroids. This overview features interviews with Hal Levison (Principal Investigator) and Cathy Olkin (Deputy Principal Investigator) from the Southwest Research Institute in Boulder, Colorado. Music is \"Life Choices\" by Universal Production Music. || LUCY_OVERVIEW_MASTER.00035_print.jpg (1024x576) [157.1 KB] || LUCY_THUMB.jpg (3840x2160) [1.4 MB] || LUCY_OVERVIEW_MASTER.00035_searchweb.png (320x180) [88.7 KB] || LUCY_OVERVIEW_MASTER.00035_thm.png (80x40) [6.2 KB] || LUCY_OVERVIEW_MASTER_VX-310983.webm (960x540) [73.8 MB] || LUCY_OVERVIEW_MASTER_VX-310983_facebook_720.mp4 (1280x720) [252.2 MB] || LUCY_OVERVIEW_MASTER_VX-310983_twitter_720.mp4 (1280x720) [41.4 MB] || LUCY_MASTER_SMALLERSIZE.mp4 (3840x2160) [263.2 MB] || Lucy_Subtitles.en_US.srt [5.0 KB] || Lucy_Subtitles.en_US.vtt [5.0 KB] || LUCY_OVERVIEW_MASTER.mov (3840x2160) [13.1 GB] || ", "hits": 75 }, { "id": 4755, "url": "https://svs.gsfc.nasa.gov/4755/", "result_type": "Visualization", "release_date": "2019-12-12T14:00:00-05:00", "title": "Mars Upper Level Winds Observed by MAVEN - Visualizations", "description": "MAVEN observes upper level Martian winds over the course of about two years. || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_print.jpg (1024x576) [42.9 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_searchweb.png (320x180) [49.1 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_thm.png (80x40) [4.0 KB] || maven_upper_winds_campaigns_1080p60.mp4 (1920x1080) [51.0 MB] || maven_upper_winds_campaigns_1080p30.mp4 (1920x1080) [46.4 MB] || maven_upper_winds.0104_cam_mainShape_190909182423_beauty_1080p30.webm (1920x1080) [9.6 MB] || campaigns (3840x2160) [0 Item(s)] || maven_upper_winds_campaigns_2160p60.mp4 (3840x2160) [162.2 MB] || maven_upper_winds_campaigns_2160p30.mp4 (3840x2160) [146.8 MB] || 4755_MAVEN_Wind_Currents_Full.mov (3840x2160) [9.7 GB] || maven_upper_winds_campaigns_1080p30.mp4.hwshow [201 bytes] || ", "hits": 49 }, { "id": 13485, "url": "https://svs.gsfc.nasa.gov/13485/", "result_type": "Produced Video", "release_date": "2019-12-12T14:00:00-05:00", "title": "Mars Wind Currents Reveal a Surprising Feature", "description": "By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below.Credit: NASA/Goddard/MAVEN/CU Boulder/University of MichiganUniversal Production Music: “Glacial Shifts” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13485_Mars_Upper_Winds_MASTER_facebook_720.mp4 (1280x720) [216.5 MB] || 13485_MarsUpperWinds_Preview_print.jpg (1024x576) [77.9 KB] || 13485_MarsUpperWinds_Preview.jpg (3840x2160) [399.6 KB] || 13485_MarsUpperWinds_Preview_searchweb.png (320x180) [57.6 KB] || 13485_MarsUpperWinds_Preview_thm.png (80x40) [4.8 KB] || TWITTER_720_13485_Mars_Upper_Winds_MASTER_twitter_720.mp4 (1280x720) [37.3 MB] || 13485_Mars_Upper_Winds_MASTER.webm (960x540) [78.1 MB] || 13485_Mars_Upper_Winds_Captions.en_US.srt [4.2 KB] || 13485_Mars_Upper_Winds_Captions.en_US.vtt [4.2 KB] || CH28_13485_Mars_Upper_Winds_MASTER_ch28.mov (1280x720) [1.8 GB] || 13485_Mars_Upper_Winds_YouTube.mp4 (3840x2160) [2.0 GB] || 13485_Mars_Upper_Winds_MASTER.mov (3840x2160) [19.2 GB] || ", "hits": 92 }, { "id": 20302, "url": "https://svs.gsfc.nasa.gov/20302/", "result_type": "Animation", "release_date": "2019-12-12T14:00:00-05:00", "title": "Mars Wind Currents Reveal a Surprising Feature - Animations", "description": "By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below. || 20302_MarsUpperWinds_Preview_print.jpg (1024x576) [131.1 KB] || 20302_MarsUpperWinds_Preview.jpg (3840x2160) [676.6 KB] || 20302_MarsUpperWinds_Preview_searchweb.png (320x180) [86.0 KB] || 20302_MarsUpperWinds_Preview_thm.png (80x40) [6.4 KB] || TWITTER_720_MAVEN_Mars_Terrain_Winds_twitter_720.mp4 (1280x720) [16.4 MB] || MAVEN_Mars_Terrain_Winds.webm (960x540) [39.0 MB] || YOUTUBE_1080_MAVEN_Mars_Terrain_Winds_youtube_1080.mp4 (1920x1080) [135.6 MB] || FACEBOOK_720_MAVEN_Mars_Terrain_Winds_facebook_720.mp4 (1280x720) [104.1 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4 (3840x2160) [595.8 MB] || MAVEN_Mars_Terrain_Winds.mov (3840x2160) [10.6 GB] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4.hwshow [143 bytes] || ", "hits": 60 }, { "id": 4762, "url": "https://svs.gsfc.nasa.gov/4762/", "result_type": "Visualization", "release_date": "2019-12-10T17:30:00-05:00", "title": "GOLD Instrument observes the July 2019 Total Solar Eclipse", "description": "Comparative visualizations of Earth in visible light and the ultraviolet emission of oxygen recombining from ions. The Appleton anomaly is faintly visible above and below the equator on the nightside of the Earth. This version presents the path of the solar eclipse but variations are available in the popup menu to the right. || GOLDEclipse201907.O5S+VIS_path_UHD3840.00192_print.jpg (1024x576) [68.5 KB] || GOLDEclipse201907.O5S+VIS_path_UHD3840.00192_searchweb.png (320x180) [59.6 KB] || GOLDEclipse201907.O5S+VIS_path_UHD3840.00192_thm.png (80x40) [5.4 KB] || GOLDEclipse201907.O5S+VIS_path_HD1080i_p5.webm (1920x1080) [4.7 MB] || Eclipse2019.O5S_VIS_path (1920x1080) [0 Item(s)] || GOLDEclipse201907.O5S+VIS_path_HD1080i_p5.mp4 (1920x1080) [19.8 MB] || Eclipse2019.O5S_VIS_nopath (1920x1080) [0 Item(s)] || GOLDEclipse201907.O5S+VIS_nopath_HD1080i_p5.mp4 (1920x1080) [20.0 MB] || Eclipse2019.O5S_VIS_nopath (3840x2160) [0 Item(s)] || GOLDEclipse201907.O5S+VIS_nopath_UHD3840_2160p5.mp4 (3840x2160) [64.3 MB] || Eclipse2019.O5S_VIS_path (3840x2160) [0 Item(s)] || GOLDEclipse201907.O5S+VIS_path_UHD3840_2160p5.mp4 (3840x2160) [63.4 MB] || ", "hits": 35 }, { "id": 13502, "url": "https://svs.gsfc.nasa.gov/13502/", "result_type": "Produced Video", "release_date": "2019-12-10T17:00:00-05:00", "title": "AGU 2019 — Postcards from the edge of space: New images, new phenomena, and new insights", "description": "In a Dec. 10 press event at the fall meeting of the American Geophysical Union in San Francisco, California, three scientists presented new images of the ionosphere, the dynamic region where Earth’s atmosphere meets space. Home to astronauts and everyday technology like radio and GPS, the ionosphere constantly responds to changes from space above and Earth below.The collection of images presented include the first images from NASA’s ICON, new science results from NASA’s GOLD, and observations of a fleeting, never-before-studied aurora. Together, they bring color to invisible processes that have widespread implications for the part of space that is closest to home.SPEAKERS:• Jennifer Briggs, Pepperdine University, Malibu, California, United States• Richard Eastes, University of Colorado Boulder, Boulder, Colorado, United States• Thomas Immel, University of California Berkeley, Berkeley, California, United States || ", "hits": 79 }, { "id": 13329, "url": "https://svs.gsfc.nasa.gov/13329/", "result_type": "Produced Video", "release_date": "2019-09-27T12:45:00-04:00", "title": "OLI-2 ships to Northrop Grumman", "description": "The Operational Land Imager 2, or OLI-2, will detect visible and infrared light from Earth's surface, providing data on our changing planet. OLI-2 was built and tested at Ball Aerospace in Boulder, Colorado. Landsat 9, a partnership between NASA and the U.S. Geological Survey, is a series of satellites that began with Landsat 1 in 1972.Music: Bit Streaming, composed by David Edwards [ASCAP], published by Soundcast Music [SESAC] Complete transcript available. || 13329_OLI-2_Ships_still.jpg (1920x1080) [555.8 KB] || 13329_OLI-2_Ships_still_searchweb.png (320x180) [110.3 KB] || 13329_OLI-2_Ships_still_thm.png (80x40) [8.5 KB] || 13329_OLI-2_Ships_large.webm (1920x1080) [19.2 MB] || 13329_OLI-2_Ships_large.mp4 (1920x1080) [217.5 MB] || 13329_OLI-2_ships-captions.en_US.srt [1.4 KB] || 13329_OLI-2_ships-captions.en_US.vtt [1.4 KB] || 13329_OLI-2_Ships_MASTER.mov (1920x1080) [3.5 GB] || ", "hits": 29 }, { "id": 4757, "url": "https://svs.gsfc.nasa.gov/4757/", "result_type": "Visualization", "release_date": "2019-09-23T13:00:00-04:00", "title": "Arctic Sea Ice Minimum 2019", "description": "Arctic Sea Ice Minimum 2019, Animation || minimum_2019.1409_print.jpg (1024x576) [130.4 KB] || minimum_2019.1409_searchweb.png (320x180) [85.2 KB] || minimum_2019.1409_thm.png (80x40) [6.7 KB] || minimum_2019_1080p30.mp4 (1920x1080) [34.7 MB] || full (1920x1080) [0 Item(s)] || minimum_2019_1080p30.webm (1920x1080) [6.3 MB] || minimum_2019_1080p30.mp4.hwshow [186 bytes] || ", "hits": 24 }, { "id": 4733, "url": "https://svs.gsfc.nasa.gov/4733/", "result_type": "Visualization", "release_date": "2019-04-04T00:00:00-04:00", "title": "Hyperwall: Scouting the Apollo 11 Landing Site", "description": "This sequence of images from Apollo 10 looks west across southern Mare Tranquillitatis. The Apollo 11 landing site is circled in green. The bright crater at about 7 o'clock within the circle is West crater. Black and white, 70mm magazine R, AS10-31-4607 to 11. || apollo10_as10-31-4607_print.jpg (1024x345) [81.6 KB] || apollo10_as10-31-4607_searchweb.png (320x180) [47.4 KB] || apollo10_as10-31-4607_thm.png (80x40) [3.9 KB] || apollo10_as10-31-4607.tif (9600x3240) [13.8 MB] || apollo-10-photo-sequence-of-apollo-11-site.hwshow [237 bytes] || ", "hits": 188 }, { "id": 12658, "url": "https://svs.gsfc.nasa.gov/12658/", "result_type": "Produced Video", "release_date": "2018-12-10T13:50:00-05:00", "title": "OSIRIS-REx Arrives at Bennu -- 2018 AGU Press Conference", "description": "NASA’s OSIRIS-REx mission presented the science results gained during the spacecraft’s approach toward the asteroid Bennu at a press conference hosted during AGU’s Fall Meeting at 2 p.m. ET, Monday, Dec. 10.The Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft, which launched on Sept. 8, 2016, started asteroid science operations on Aug. 17, 2018, while still 1.4 million miles from the asteroid Bennu. Between that time and the spacecraft’s arrival at Bennu on Dec. 3, the mission made a number of discoveries about the asteroid. The mission represents a valuable opportunity to learn more about the origins of our solar system, the sources of water and organic molecules on Earth, and the hazards and resources in near-Earth space. The briefing participants are:Jeffrey Grossman, OSIRIS-REx program scientist at NASA HeadquartersDante Lauretta, OSIRIS-REx principal investigator at the University of Arizona, TucsonAmy Simon, OVIRS deputy instrument scientist at NASA Goddard Space Flight Center Michael Nolan, OSIRIS-REx science team chief at the University of Arizona, TucsonFor more information, go to nasa.gov/osiris-rex or asteroidmission.org. || ", "hits": 45 }, { "id": 30960, "url": "https://svs.gsfc.nasa.gov/30960/", "result_type": "Hyperwall Visual", "release_date": "2018-06-04T10:00:00-04:00", "title": "Eagle Nebula: M16 Wide", "description": "This series of images shows the environment around the Pillars of Creation, the Eagle Nebula, Messier 16. The images reveal the nebula in optical, X-ray, mid-infrared, and far-infrared light. || STScI-H-M16wide_1x-1920x1080.00001_print.jpg (1024x576) [163.7 KB] || STScI-H-M16wide_1x-1920x1080.00001_searchweb.png (320x180) [108.4 KB] || STScI-H-M16wide_1x-1920x1080.00001_thm.png (80x40) [6.9 KB] || STScI-H-M16wide_1x-1280x720.mp4 (1280x720) [8.5 MB] || STScI-H-M16wide_1x-1920x1080.mp4 (1920x1080) [17.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M16wide_1x-1920x1080.webm (1920x1080) [5.2 MB] || STScI-H-M16wide_1x-640x360.mp4 (640x360) [2.9 MB] || STScI-H-M16wide_1x-3840x2160.mp4 (3840x2160) [17.1 MB] || STScI-H-M16wide_1x-H265-3840x2160.mp4 (3840x2160) [7.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 201 }, { "id": 12825, "url": "https://svs.gsfc.nasa.gov/12825/", "result_type": "Infographic", "release_date": "2018-01-24T12:00:00-05:00", "title": "GOLD Resources", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. The more we know about the fundamental physics of this region of space, the more we can protect our assets there.Gathering observations from geostationary orbit above the Western Hemisphere, GOLD measures the temperature and composition of neutral gases in Earth’s thermosphere. This part of the atmosphere co-mingles with the ionosphere, which is made up of charged particles. Both the Sun from above and terrestrial weather from below can change the types, numbers, and characteristics of the particles found here — and GOLD helps track those changes.Activity in this region is responsible for a variety of key space weather events. GOLD scientists are particularly interested in the cause of dense, unpredictable bubbles of charged gas that appear over the equator and tropics, sometimes causing communication problems. As we discover the very nature of the Sun-Earth interaction in this region, the mission could ultimately lead to ways to improve forecasts of such space weather and mitigate its effects. || ", "hits": 99 }, { "id": 12817, "url": "https://svs.gsfc.nasa.gov/12817/", "result_type": "Produced Video", "release_date": "2018-01-05T13:00:00-05:00", "title": "Why NASA Is Exploring The Edge Of Our Planet", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, instrument launches aboard a commercial communications satellite in January 2018 to inspect the dynamic intermingling of space and Earth’s uppermost atmosphere. Together, GOLD and another NASA mission, Ionospheric Connection Explorer spacecraft, or ICON, will provide the most comprehensive of Earth’s upper atmosphere we’ve ever had.Above the ozone layer, the ionosphere is a part of Earth’s atmosphere where particles have been cooked into a sea of electrically-charged electrons and ions by the Sun’s radiation. The ionosphere is co-mingled with the very highest — and quite thin — layers of Earth’s neutral upper atmosphere, making this region an area that is constantly in flux undergoing the push-and-pull between Earth’s conditions and those in space. Increasingly, these layers of near-Earth space are part of the human domain, as it’s home not only to astronauts, but to radio signals used to guide airplanes and ships, and satellites that provide our communications and GPS systems. Understanding the fundamental processes that govern our upper atmosphere and ionosphere is crucial to improve situational awareness that helps protect astronauts, spacecraft and humans on the ground.GOLD, in geostationary orbit over the Western Hemisphere, will build up a full-disk view of the ionosphere and upper atmosphere every half hour, providing detailed large-scale measurements of related processes — a cadence which makes it the first mission to be able to monitor the true weather of the upper atmosphere. GOLD is also able to focus in on a tighter region and scan more quickly, to complement additional research plans as needed. || ", "hits": 63 }, { "id": 12820, "url": "https://svs.gsfc.nasa.gov/12820/", "result_type": "Produced Video", "release_date": "2018-01-04T00:00:00-05:00", "title": "Going for GOLD: Exploring the Interface to Space", "description": "Going for GOLD: Exploring the Interface to Space || 12820_GOLD_FB_Live.00001_print.jpg (1024x576) [125.3 KB] || 12820_GOLD_FB_Live.00001_searchweb.png (320x180) [84.7 KB] || 12820_GOLD_FB_Live.00001_thm.png (80x40) [6.6 KB] || 12820_GOLD_FB_Live.mp4 (1280x720) [5.1 GB] || 12820_GOLD_FB_Live.mov (1280x720) [41.9 GB] || 12820_GOLD_FB_Live.webm (960x540) [1.7 GB] || 12820_GOLD_FB_Live.en_US.srt [119.6 KB] || 12820_GOLD_FB_Live.en_US.vtt [112.9 KB] || ", "hits": 40 }, { "id": 12796, "url": "https://svs.gsfc.nasa.gov/12796/", "result_type": "Produced Video", "release_date": "2017-12-13T11:30:00-05:00", "title": "2017 AGU Habitability Press Conference", "description": "Spanning Disciplines to Search for Life Beyond EarthThe search for life beyond Earth is riding a surge of creativity and innovation. Following a gold rush of exoplanet discovery over the past two decades, it is time to tackle the next step: determining which of the known exoplanets are proper candidates for life. Scientists from NASA and two universities presented new results dedicated to this task in fields spanning astrophysics, Earth science, heliophysics and planetary science — demonstrating how a cross-disciplinary approach is essential to finding life on other worlds — at the fall meeting of the American Geophysical Union on Dec. 13, 2017, in New Orleans, Louisiana.PANELISTS:• Giada Arney, NASA’s Goddard Space Flight Center• Stephen Kane, University of California-Riverside• Katherine Garcia-Sage, NASA’s Goddard Space Flight Center/Catholic University of America• Dave Brain, University of Colorado-Boulder || ", "hits": 107 }, { "id": 12734, "url": "https://svs.gsfc.nasa.gov/12734/", "result_type": "Produced Video", "release_date": "2017-10-30T13:00:00-04:00", "title": "Arctic Update", "description": "Arctic Sea ice reached its minimum extent in September, 2017. || SeaIceMin2017_1920x1080_print_1024x576.jpg (1024x576) [161.5 KB] || SeaIceMin2017_1920x1080.tif (1920x1080) [3.3 MB] || ", "hits": 21 }, { "id": 4455, "url": "https://svs.gsfc.nasa.gov/4455/", "result_type": "Visualization", "release_date": "2017-09-19T15:00:00-04:00", "title": "Arctic Sea Ice from March to September 2017", "description": "In this visualization, the daily Arctic sea ice and seasonal land cover change progress through time, from this year’s wintertime maximum extent on March 7, 2017, through September 13, 2017 when the sea ice reached its annual minimum extent for the year. Over the water, Arctic sea ice changes from day to day showing a running 3-day minimum sea ice concentration in the region where the concentration is greater than 15%. The blueish white color of the sea ice is derived from a 3-day running minimum of the AMSR2 89 GHz brightness temperature. Over the terrain, monthly data from the seasonal Blue Marble Next Generation fades slowly from month to month. || SeaIceMin2017_1920x1080_print.jpg (1024x576) [161.8 KB] || SeaIceMin2017_1920x1080_searchweb.png (320x180) [98.0 KB] || SeaIceMin2017_1920x1080_thm.png (80x40) [6.7 KB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || SeaIceMin2017_30fps_1080p30.mp4 (1920x1080) [22.0 MB] || SeaIceMin2017_1920x1080.tif (1920x1080) [3.3 MB] || SeaIceMin2017_30fps_1080p30.webm (1920x1080) [1.5 MB] || SeaIceMin2017_30fps_1080p30.mp4.hwshow [193 bytes] || ", "hits": 42 }, { "id": 12179, "url": "https://svs.gsfc.nasa.gov/12179/", "result_type": "Produced Video", "release_date": "2017-07-25T09:30:00-04:00", "title": "NASA Jets Chase The Total Solar Eclipse", "description": "For most viewers, the Aug. 21, 2017, total solar eclipse will last less than two and half minutes. But for one team of NASA-funded scientists, the eclipse will last over seven minutes. Their secret? Following the shadow of the Moon in two retrofitted WB-57F jet planes. Amir Caspi of the Southwest Research Institute in Boulder, Colorado, and his team will use two of NASA’s WB-57F research jets to chase the darkness across America on Aug. 21. Taking observations from twin telescopes mounted on the noses of the planes, Caspi will capture the clearest images of the Sun’s outer atmosphere — the corona — to date and the first-ever thermal images of Mercury, revealing how temperature varies across the planet’s surface. || ", "hits": 56 }, { "id": 30884, "url": "https://svs.gsfc.nasa.gov/30884/", "result_type": "Hyperwall Visual", "release_date": "2017-06-23T00:00:00-04:00", "title": "CYGNSS First Light", "description": "The three maps on the right each show a single pass of the CYGNSS constellation, and the larger image on the left shows the full day's data combined into one image. || cygnss_1stlight_all_print.jpg (1024x574) [163.2 KB] || cygnss_1stlight_all.png (4104x2304) [27.1 MB] || cygnss_1stlight_all_searchweb.png (320x180) [60.9 KB] || cygnss_1stlight_all_thm.png (80x40) [5.6 KB] || ", "hits": 22 }, { "id": 12480, "url": "https://svs.gsfc.nasa.gov/12480/", "result_type": "Produced Video", "release_date": "2017-04-10T12:00:00-04:00", "title": "Shrinking Sea Ice", "description": "A combination of warmer-than-average temperatures, winds unfavorable to ice expansion, and a series of storms halted Arctic sea ice growth. || NPseaIce_MIN2016_til_Mar2017.8218_1024x576.jpg (1024x576) [148.2 KB] || NPseaIce_MIN2016_til_Mar2017.8218_print.jpg (1024x576) [161.6 KB] || NPseaIce_MIN2016_til_Mar2017.8218_thm.png (80x40) [6.5 KB] || NPseaIce_MIN2016_til_Mar2017.8218_1024x576_searchweb.png (320x180) [78.8 KB] || NPseaIce_MIN2016_til_Mar2017.8218.tif (1920x1080) [2.3 MB] || ", "hits": 140 }, { "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": 30 }, { "id": 12549, "url": "https://svs.gsfc.nasa.gov/12549/", "result_type": "Produced Video", "release_date": "2017-03-24T13:00:00-04:00", "title": "How a NASA Science Flight is No Ordinary Journey", "description": "A group of scientists and pilots conducted a series of science flights over Western Colorado for a new five-year NASA-led airborne mission called SnowEx.SnowEx is exploring better ways to measuring how much water is stored in snow-covered regions with the goal of eventually creating a future snow satellite mission. More accurate snow measurements will help scientists and decisions-makers better understand our world’s water supply and better predict floods and droughts. Data acquired from the SnowEx campaign will be stored at the National Snow and Ice Data Center in Boulder, Colorado, and will be available to anyone to order at no cost, as is the case with all NASA data.For more information:NASA's SnowEx Challenges the Sensing Techniques...'Until They Break'NASA: Snow Science in Support of Our Nation's Water Supply || ", "hits": 47 }, { "id": 4564, "url": "https://svs.gsfc.nasa.gov/4564/", "result_type": "Visualization", "release_date": "2017-03-22T12:00:00-04:00", "title": "Arctic Daily Sea Ice Concentration from Arctic Minimum 2016 to Arctic Maximum 2017", "description": "This movie begins at Arctic Minimum on September 10, 2016 and shows daily sea ice concentration until the Arctic maximum on March 7, 2017. The 2017 Arctic maximum was 14.42 million square kilometers (5.57 million square miles). The average maximum (1981-2010) is 15.64 million square kilometers. || print_Arctic_Max_2017_March07.8218_print.jpg (1024x576) [138.6 KB] || print_Arctic_Max_2017_March07.8218_searchweb.png (320x180) [75.7 KB] || print_Arctic_Max_2017_March07.8218_thm.png (80x40) [6.2 KB] || NorthPole_seaIce_MIN2016_til_Max2017_1080p30.mp4 (1920x1080) [14.8 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || NorthPole_seaIce_MIN2016_til_Max2017_1080p30.webm (1920x1080) [3.9 MB] || print_Arctic_Max_2017_March07.8218.tif (3840x2160) [10.4 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || NorthPole_seaIce_MIN2016_til_Max2017_1080p30.mp4.hwshow [210 bytes] || ", "hits": 41 }, { "id": 12496, "url": "https://svs.gsfc.nasa.gov/12496/", "result_type": "B-Roll", "release_date": "2017-02-22T17:00:00-05:00", "title": "SnowEx Field Campaign: 4K B-roll From The P-3 Orion Aircraft", "description": "SnowEx is a NASA led multi-year research campaign to improve measurements of how much snow is on the ground at any given time and how much liquid water is contained in that snow.Five aircraft with a total of ten different sensors will participate in the SnowEx campaign. From a base of operations at Peterson Air Force Base, Colorado Springs, SnowEx will deploy a P-3 Orion aircraft operated by the Scientific Development Squadron ONE (VXS-1), based at Naval Air Station Patuxent River, Maryland. A King Air plane will fly out of Grand Junction, Colorado, while high-altitude NASA jets will fly from Johnson Space Center in Houston.The planes will carry passive and active microwave sensors that are good at measuring snow-water equivalent in dry snow, but are less optimal for measuring snow forests or light snow cover. The campaign will also deploy an airborne laser instrument to measure snow depth, and airborne sensors to measure surface temperature and reflected light from snow.Data acquired from the SnowEx campaign will be stored at the National Snow and Ice Data Center in Boulder, Colorado, and will be available to anyone to order at no cost, as is the case with all NASA data.For more information: https://www.nasa.gov/earthexpeditions || ", "hits": 41 }, { "id": 12511, "url": "https://svs.gsfc.nasa.gov/12511/", "result_type": "Produced Video", "release_date": "2017-02-16T10:00:00-05:00", "title": "NASA Investigates Water Supply in Snow", "description": "This February, a NASA-led research campaign called SnowEx kicked off in Colorado. The 5-year study will advance global measurements of how much snow is on the ground at any given time and how much liquid water is contained in that snow. The amount of water in snow plays a huge role in water availability for drinking water, agriculture, and hydropower.Teams of 50 researchers are stationed at Grand Mesa and Senator Beck Basin over a three-week period to measure snow using a variety of snow-sensing instruments and techniques. Ground measurements will allow the team to validate the remotely sensed measurements acquired by multiple sensors on the various aircraft.Data acquired from the SnowEx campaign will be stored at the National Snow and Ice Data Center in Boulder, Colorado, and will be available to anyone to order at no cost, as is the case with all NASA data. For more information: https://www.nasa.gov/earthexpeditions/ || ", "hits": 36 }, { "id": 12489, "url": "https://svs.gsfc.nasa.gov/12489/", "result_type": "B-Roll", "release_date": "2017-02-14T02:00:00-05:00", "title": "SnowEx Field Campaign: B-roll From The P-3 Orion Aircraft", "description": "SnowEx is a NASA led multi-year research campaign to improve measurements of how much snow is on the ground at any given time and how much liquid water is contained in that snow.Five aircraft with a total of ten different sensors will participate in the SnowEx campaign. From a base of operations at Peterson Air Force Base, Colorado Springs, SnowEx will deploy a P-3 Orion aircraft operated by the Scientific Development Squadron ONE (VXS-1), based at Naval Air Station Patuxent River, Maryland. A King Air plane will fly out of Grand Junction, Colorado, while high-altitude NASA jets will fly from Johnson Space Center in Houston. The planes will carry passive and active microwave sensors that are good at measuring snow-water equivalent in dry snow, but are less optimal for measuring snow forests or light snow cover. The campaign will also deploy an airborne laser instrument to measure snow depth, and airborne sensors to measure surface temperature and reflected light from snow.Data acquired from the SnowEx campaign will be stored at the National Snow and Ice Data Center in Boulder, Colorado, and will be available to anyone to order at no cost, as is the case with all NASA data.For more information: https://www.nasa.gov/earthexpeditions || ", "hits": 43 }, { "id": 12490, "url": "https://svs.gsfc.nasa.gov/12490/", "result_type": "B-Roll", "release_date": "2017-02-13T00:00:00-05:00", "title": "SnowEx Field Campaign: B-roll From Grand Mesa", "description": "SnowEx is a NASA led multi-year research campaign to improve measurements of how much snow is on the ground at any given time and how much liquid water is contained in that snow.Starting in February, teams of 50 researchers are stationed at Grand Mesa and Senator Beck Basin over a three-week period to measure snow using a variety of snow-sensing instruments and techniques.Ground measurements will allow the team to validate the remotely-sensed measurements acquired by the multiple sensors on the various aircraft.Data acquired from the SnowEx campaign will be stored at the National Snow and Ice Data Center in Boulder, Colorado, and will be available to anyone to order at no cost, as is the case with all NASA data. For more information: https://www.nasa.gov/earthexpeditions/ || ", "hits": 33 }, { "id": 12457, "url": "https://svs.gsfc.nasa.gov/12457/", "result_type": "Produced Video", "release_date": "2016-12-14T12:00:00-05:00", "title": "AGU Ionosphere Press Conference", "description": "The ionosphere is a layer of charged particles in Earth’s atmosphere that extends from about 50 to 360 miles above the surface of Earth. Processes in the ionosphere also create bright swaths of color in the sky, known as airglow. Credit: NASA GSFC || AGUIonosphereV4_1.jpg (1280x960) [109.7 KB] || ", "hits": 50 }, { "id": 30814, "url": "https://svs.gsfc.nasa.gov/30814/", "result_type": "Hyperwall Visual", "release_date": "2016-10-05T00:00:00-04:00", "title": "The Color Wonderland of Mawrth Vallis", "description": "The Color Wonderland of Mawrth Vallis || PIA21029_print.jpg (1024x640) [380.8 KB] || PIA21029_searchweb.png (320x180) [127.2 KB] || PIA21029_thm.png (80x40) [8.0 KB] || PIA21029.tif (2880x1800) [14.8 MB] || Mawrth_Vallis30814.key [15.5 MB] || Mawrth_Vallis30814.pptx [14.1 MB] || the-color-wonderland-of-mawrth-vallis.hwshow [213 bytes] || ", "hits": 34 }, { "id": 12379, "url": "https://svs.gsfc.nasa.gov/12379/", "result_type": "Produced Video", "release_date": "2016-09-28T10:00:00-04:00", "title": "Space Radiation Highlights", "description": "A collection of space radiation highlights featuring:NASA's Van Allen ProbesNASA's CubeSats || ", "hits": 80 }, { "id": 12292, "url": "https://svs.gsfc.nasa.gov/12292/", "result_type": "Produced Video", "release_date": "2016-06-24T15:00:00-04:00", "title": "Solar Highlights of 2016/2017", "description": "A collection of solar highlights featuring:- NASA's Solar Dynamics Observatory (SDO)- NASA's Interface Region Imaging Spectrograph (IRIS) mission- ESA/NASA's Solar and Heliospheric Observatory (SOHO)- NASA's Solar TErrestrial RElations Observatory (STEREO) mission || ", "hits": 126 }, { "id": 4302, "url": "https://svs.gsfc.nasa.gov/4302/", "result_type": "Visualization", "release_date": "2015-12-08T20:00:00-05:00", "title": "Apollo 17 Landing Site", "description": "Apollo 17, crewed by Eugene Cernan, Ronald Evans, and Harrison Schmitt, was the final Apollo mission to the Moon. The Lunar Module Challenger landed in the Taurus-Littrow valley on December 11, 1972 and remained there for 75 hours. The landing site is a relatively flat spot among low mountains at the southeastern edge of Mare Serenitatis.The images here are designed for display on NASA's hyperwall. They help tell the story of Apollo 17's exploration of the Taurus-Littrow site using data and imaging from Lunar Reconnaissance Orbiter (LRO) and photographs taken by the astronauts. LRO's detailed and comprehensive remote sensing capabilities have fostered a reinterpretation of the geology of the site. || ", "hits": 429 }, { "id": 4370, "url": "https://svs.gsfc.nasa.gov/4370/", "result_type": "Visualization", "release_date": "2015-11-05T14:00:00-05:00", "title": "Solar Wind Strips the Martian Atmosphere", "description": "Scientists have long suspected the solar wind of stripping the Martian upper atmosphere into space, turning Mars from a blue world to a red one. Now, NASA's MAVEN orbiter is observing this process in action, providing significant data on solar wind erosion at Mars.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.This video is also available on our YouTube channel. || MarsAtmoLossExplainPreview.jpg (1920x1080) [993.6 KB] || APPLE_TV_4370_MAVEN_Mars_Atmo_Loss_appletv_subtitles.m4v (1280x720) [53.7 MB] || WEBM_4370_MAVEN_Mars_Atmo_Loss_APR.webm (960x540) [44.7 MB] || 4370_MAVEN_Mars_Atmo_Loss_appletv.m4v (1280x720) [53.7 MB] || NASA_TV_4370_MAVEN_Mars_Atmo_Loss.mpeg (1280x720) [369.5 MB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.srt [2.3 KB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.vtt [2.3 KB] || LARGE_MP4_4370_MAVEN_Mars_Atmo_Loss_large.mp4 (3840x2160) [111.3 MB] || YOUTUBE_HQ_4370_MAVEN_Mars_Atmo_Loss_youtube_hq.mov (3840x2160) [2.2 GB] || 4370_MAVEN_Mars_Atmo_Loss_APR.mov (3840x2160) [5.9 GB] || ", "hits": 313 }, { "id": 4385, "url": "https://svs.gsfc.nasa.gov/4385/", "result_type": "Visualization", "release_date": "2015-10-09T17:00:00-04:00", "title": "Zooming In: Remote Sensing the Earth", "description": "This gallery was created for Earth Science Week 2015 and beyond. It includes a quick start guide for educators and first-hand stories (blogs) for learners of all ages by NASA visualizers, scientists and educators. We hope that your understanding and use of NASA's visualizations will only increase as your appreciation grows for the beauty of the science they portray, and the communicative power they hold. Read all the blogs and find educational resources for all ages at: the Earth Science Week 2015 page.Observing something without coming in contact with it is called remote sensing. Think about that. Every living animal uses remote sensing. A spider keeps its eight eyes fixed on a fly, watches its movements. A dolphin sends out sounds to locate a school of fish. A tiger uses its Jacobson's organ to smell a mate. Humans listen to cicadas' loud noises coming from the trees. These are all examples of remote sensing. And, more than likely, all of these animals are analyzing the data they are receiving. I used these particular examples to show that there are different methods of receiving this data. The spider uses sight. The dolphin uses echolocation. The tiger uses smell. The human uses sound. I remember the first time I flew in an airplane. I was about 12 years old and was lucky enough to get a window seat. It was amazing to look down and try to identify things on the ground. I didn't realize it at the time but I was remotely sensing Earth! I could almost imagine how a bird must see the land when it's flying high in the sky. Since I cannot fly all the time like birds do, I can use another tool — Google Earth — to get the same experience. I can look at my computer screen, and identify the differences between urban and natural areas and between fields and forests. NASA creates the most amazing remotely-sensed images of space and the planets. I have always been fascinated by space and space exploration. In 1969, as I listened on my radio to the broadcast of the moon landing, I wondered what it would be like to walk on the moon and to look further out into space. Now, space telescopes, such as Hubble, provide scientists with hundreds of thousands of images for understanding our universe. Images of outer space are fascinating, but I am most excited about images of Earth. NASA and the U.S. Geological Survey have created an amazing collection of satellite images, called Earth as Art. Sometimes these almost look like art from a museum. These images are not only pleasing to look at; they can also tell us valuable information. || ", "hits": 37 }, { "id": 11978, "url": "https://svs.gsfc.nasa.gov/11978/", "result_type": "Produced Video", "release_date": "2015-08-26T11:00:00-04:00", "title": "Sea Level Rise Briefing - August 26, 2015", "description": "Seas around the world have risen an average of nearly 3 inches since 1992, with some locations rising more than 9 inches due to natural variation, according to the latest satellite measurements from NASA and its partners. An intensive research effort now underway, aided by NASA observations and analysis, points to an unavoidable rise of several feet in the future. Members of NASA’s new interdisciplinary Sea Level Change Team will discuss recent findings and new agency research efforts during a media teleconference on Aug. 26, 2015, at 12:30 p.m. EDT The question scientists are grappling with is how quickly will seas rise?Participating in the briefing:* Michael Freilich, director of NASA’s Earth Science Division at the agency’s headquarters in Washington* Steve Nerem, lead for NASA’s Sea Level Change Team at the University of Colorado in Boulder* Eric Rignot, glaciologist at the University of California, Irvine and NASA's Jet Propulsion Labratory (JPL) in Pasadena, California* Josh Willis, climate scientist at NASA’s JPLFor more information:Rising SeasPress Release: NASA Science Zeros in on Ocean Rise: How Much? How Soon?Sea Level Rise Video Resources || ", "hits": 18 }, { "id": 4328, "url": "https://svs.gsfc.nasa.gov/4328/", "result_type": "Visualization", "release_date": "2015-08-25T00:00:00-04:00", "title": "Greenland's Glaciers as seen by RadarSat", "description": "An animation up the Greenland's Sermilik Fjord to the calving front of the Helheim Glacier, showing the glacier front's change between 2000 to 2013This video is also available on our YouTube channel. || Helheim_radarsat_4k.0800_print.jpg (1024x576) [242.6 KB] || Helheim_radarsat_4k.0800_searchweb.png (180x320) [121.8 KB] || Helheim_radarsat_4k.0800_web.png (320x180) [121.8 KB] || Helheim_radarsat_4k.0800_thm.png (80x40) [7.6 KB] || Helheim_radarsat_4k_1080p30.mp4 (1920x1080) [84.5 MB] || Helheim_radarsat_4k_720p30.mp4 (1280x720) [43.3 MB] || Helheim_radarsat_4k_2160p30.webm (3840x2160) [16.2 MB] || Helheim (3840x2160) [256.0 KB] || Helheim_radarsat_4k_2160p30.mp4 (3840x2160) [225.6 MB] || ", "hits": 54 }, { "id": 4308, "url": "https://svs.gsfc.nasa.gov/4308/", "result_type": "Visualization", "release_date": "2015-08-08T00:00:00-04:00", "title": "SIGGRAPH Daily 2015: How did we tile Greenland?", "description": "This narrated animation shown as a Daily at SIGGRAPH 2015 describes a method of automatically mapping of 87 gigapixels of data over Greenland. For complete transcript, click here.This video is also available on our YouTube channel. || Radarsat_Daily.2178_print.jpg (1024x576) [186.4 KB] || Radarsat_Daily.2178_thm.png (80x40) [7.1 KB] || Radarsat_Daily.2178_searchweb.png (180x320) [106.4 KB] || 1920x1080_16x9_30p (1920x1080) [256.0 KB] || 4308_Tiling_Greenland_appletv_subtitles.m4v (1280x720) [47.1 MB] || 4308_Tiling_Greenland_VX-70360.webm (1280x720) [9.0 MB] || 1280x720_16x9_30p (1280x720) [256.0 KB] || 4308_Tiling_Greenland_H264_1080p.mp4 (1920x1080) [133.1 MB] || 4308_Tiling_Greenland_prores.mov (1920x1080) [1.5 GB] || 4308_Tiling_Greenland_1280x720.wmv (1280x720) [37.5 MB] || 4308_Tiling_Greenland_VX-70360.mpeg (1280x720) [366.2 MB] || 4308_Tiling_Greenland_appletv.m4v (1280x720) [47.0 MB] || 4308_Tiling_Greenland_youtube_hq.mov (1280x720) [161.9 MB] || 4308_Tiling_Greenland_H264_1080p.mov (1920x1080) [133.1 MB] || 4308_Tiling_Greenland.en_US.srt [2.0 KB] || 4308_Tiling_Greenland.en_US.vtt [1.9 KB] || 4308_Tiling_Greenland_ipod_sm.mp4 (320x240) [21.1 MB] || ", "hits": 29 }, { "id": 11815, "url": "https://svs.gsfc.nasa.gov/11815/", "result_type": "Produced Video", "release_date": "2015-03-19T14:00:00-04:00", "title": "Instagram: 2015 Arctic Sea Ice Maximum Extent Is Lowest On Record", "description": "The sea ice cap of the Arctic appeared to reach its annual maximum winter extent on February 25, according to data from the NASA-supported National Snow and Ice Data Center (NSIDC) at the University of Colorado, Boulder. At 5.61 million square miles (14.54 million square kilometers), this year’s maximum extent was the smallest on the satellite record and also one of the earliest.Arctic sea ice, frozen seawater floating on top of the Arctic Ocean and its neighboring seas, is in constant change: it grows in the fall and winter, reaching its annual maximum between late February and early April, and then it shrinks in the spring and summer until it hits its annual minimum extent in September. The past decades have seen a downward trend in Arctic sea ice extent during both the growing and melting season, though the decline is steeper in the latter.This year’s maximum was reached 15 days earlier than the 1981 to 2010 average date of March 12, according to NSIDC. Only in 1996 did it occur earlier, on February 24. However, the sun is just beginning to rise on the Arctic Ocean and a late spurt of ice growth is still possible, though unlikely.If the maximum were to remain at 5.61 million square miles, it would be 50,000 square miles below the previous lowest wintertime extent, reached in 2011 at 5.66 million square miles — in percentages, that’s less than a 1 percent difference between the two record low maximums. In comparison, the swings between record lows for the Arctic summertime minimum extent have been much wider: the lowest minimum extent on record, in 2012, was 1.31 million square miles, about 300,000 square miles, or 18.6 percent smaller than the previous record low one, which happened in 2007 and clocked at 1.61 million square miles.A record low sea ice maximum extent does not necessarily lead to a record low summertime minimum extent.“The winter maximum gives you a head start, but the minimum is so much more dependent on what happens in the summer that it seems to wash out anything that happens in the winter,” said Walt Meier, a sea ice scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “If the summer is cool, the melt rate will slow down. And the opposite is true, too: even if you start from a fairly high point, warm summer conditions make ice melt fast. This was highlighted by 2012, when we had one of the later maximums on record and extent was near-normal early in the melt season, but still the 2012 minimum was by far the lowest minimum we’ve seen.”The main player in the wintertime maximum extent is the seasonal ice at the edges of the ice pack. This type of ice is thin and at the mercy of which direction the wind blows: warm winds from the south compact the ice northward and also bring heat that makes the ice melt, while cold winds from the north allow more sea ice to form and spread the ice edge southward.“Scientifically, the yearly maximum extent is not as interesting as the minimum. It is highly influenced by weather and we’re looking at the loss of thin, seasonal ice that is going to melt anyway in the summer and won’t become part of the permanent ice cover,” Meier said. “With the summertime minimum, when the extent decreases it’s because we’re losing the thick ice component, and that is a better indicator of warming temperatures.” || ", "hits": 21 }, { "id": 11816, "url": "https://svs.gsfc.nasa.gov/11816/", "result_type": "Produced Video", "release_date": "2015-03-19T13:00:00-04:00", "title": "Arctic Sea Ice Sets New Record Winter Low", "description": "This short video shows the bulk of the Arctic sea ice freeze cycle from October through this year’s apparent winter maximum on Feb. 25th. || Arctic_sea_ice_max_2015_vo_youtube_hq_print.jpg (1024x576) [142.2 KB] || Arctic_sea_ice_max_2015_vo_youtube_hq_searchweb.png (320x180) [88.0 KB] || Arctic_sea_ice_max_2015_vo_youtube_hq_web.png (320x180) [88.0 KB] || Arctic_sea_ice_max_2015_vo_youtube_hq_thm.png (80x40) [6.6 KB] || Arctic_sea_ice_max_2015_vo_youtube_hq.mov (1280x720) [21.0 MB] || Arctic_sea_ice_max_2015_vo_prores.mov (1280x720) [893.4 MB] || Arctic_sea_ice_max_2015_vo_appletv.m4v (960x540) [22.8 MB] || Arctic_sea_ice_max_2015_vo_appletv_subtitles.m4v (960x540) [22.8 MB] || Arctic_sea_ice_max_2015_vo_nasaportal.mov (640x360) [18.9 MB] || Arctic_sea_ice_max_2015_vo_720x480.wmv (720x480) [18.4 MB] || Arctic_sea_ice_max_2015_vo_720x480.webm (720x480) [6.3 MB] || Arctic_Sea_Ice_Record.en_US.srt [1.2 KB] || Arctic_sea_ice_max_2015_vo_ipod_sm.mp4 (320x240) [4.4 MB] || ", "hits": 26 }, { "id": 40415, "url": "https://svs.gsfc.nasa.gov/gallery/whats-newwith-earth-today/", "result_type": "Gallery", "release_date": "2015-01-04T00:00:00-05:00", "title": "What's New with Earth Today", "description": "Explore the latest visualizations of NASA's Earth Observing satellites and the data they collect. NASA researchers are constantly tracking remote-sensing data and modeling processes to better understand our home planet.", "hits": 188 }, { "id": 4247, "url": "https://svs.gsfc.nasa.gov/4247/", "result_type": "Visualization", "release_date": "2014-12-17T00:00:00-05:00", "title": "Greenland Survey Areas", "description": "This animation starts with an overview of the Earth looking down upon North America. It then zooms into Greenland taking up most of the frame, and slowly dissolves in the research areas of interest. This animation ends where the following 4 animations pick up, so they can be composited together, if desired. || greenland_all_locs.jpg (1920x1080) [356.3 KB] || greenland_slow.1339_print.jpg (1024x576) [107.2 KB] || greenland_slow.1339_searchweb.png (320x180) [72.8 KB] || greenland_slow.1339_thm.png (80x40) [5.7 KB] || greenland_zoom_in_1080.mp4 (1920x1080) [5.2 MB] || Zoom_in (1920x1080) [32.0 KB] || greenland_zoom_in_1080.webm (1920x1080) [1.3 MB] || ", "hits": 11 }, { "id": 11432, "url": "https://svs.gsfc.nasa.gov/11432/", "result_type": "Produced Video", "release_date": "2013-12-09T17:28:00-05:00", "title": "Briefing Materials: Taking Landsat to the Extreme", "description": "At 2:30pm (PST) on Monday, Dec. 9, 2013, there was be a press conference as part of the American Geophysical Union Fall Meeting.What is the coldest place in the world? It is a high ridge in Antarctica on the East Antarctic Plateau where temperatures in several hollows can dip below minus 133.6° Fahrenheit (minus 92° Celsius) on a clear winter night – colder than the previous recorded low temperature.Scientists at the National Snow and Ice Data Center made the discovery while analyzing the most detailed global surface temperature maps to date, developed with data from remote sensing satellites including the MODIS sensor on NASA's Aqua satellite, and the TIRS sensor on Landsat 8, a joint project of NASA and the U.S. Geological Survey (USGS).The researchers analyzed 32 years of data from several satellite instruments that have mapped Antarctica's surface temperature. Near a high ridge that runs from Dome Arugs to Dome Fuji, the scientists found clusters of pockets that have plummeted to record low temperatures dozens of times. The lowest temperature the satellites detected – minus 136° F (minus 93.2° C), on Aug. 10, 2010.The new record is several degrees colder than the previous low of minus 128.6° F (minus 89.2° C), set in 1983 at the Russian Vostok Research Station in East Antarctica. The coldest permanently inhabited place on Earth is northeastern Siberia, where temperatures dropped to a bone-chilling 90 degrees below zero F (minus 67.8° C) in the towns of Verkhoyansk (in 1892) and Oimekon (in 1933).Related feature story: http://www.nasa.gov/content/goddard/nasa-usgs-landsat-8-satellite-pinpoints-coldest-spots-on-earthBriefing SpeakersTed Scambos, National Snow and Ice Data Center (NSIDC), Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado Boulder, Boulder, Colorado, USA;Jim Irons, Landsat 8 Project Scientist, NASA's Goddard Space Flight Center, Greenbelt, Maryland.Presenter 1: Ted Scambos || ", "hits": 110 }, { "id": 40152, "url": "https://svs.gsfc.nasa.gov/gallery/maven/", "result_type": "Gallery", "release_date": "2013-11-01T00:00:00-04:00", "title": "MAVEN", "description": "NASA's Mars Atmosphere and Volatile Evolution (MAVEN) is the first mission devoted to understanding the Martian upper atmosphere. Today Mars is cold and dry, but ancient Mars was warm, wet, and possibly hospitable to life. Scientists think that the loss of Mars' early atmosphere caused the planet to dry up, and MAVEN is testing this hypothesis by observing present-day interactions of the Martian atmosphere with the solar wind. Learn more about MAVEN from\n NASA and CU Boulder.", "hits": 122 }, { "id": 3886, "url": "https://svs.gsfc.nasa.gov/3886/", "result_type": "Visualization", "release_date": "2013-05-16T14:00:00-04:00", "title": "Regional Rates of Glacier Loss for 2003 to 2009", "description": "In the image below, global glacial mass loss and area are summarized by regions. The area of the red circles corresponds to the annual glacial mass loss from 2003 to 2009. Glacier mass change estimates are determined from a combination of satellite altimetry (ICESat), satellite gravimetry (GRACE) and in situ field observations as determined by Gardner et al. Light orange halos surrounding red circles show the 95% confidence interval in mass change estimates, but can only be seen in regions with large uncertainties.The area of the green/blue circles depicts total glacier area for each region with the tidewater basin fractions [TW] shown separately in blue. The geographic locations of all glaciers, evident primarily in mountainous regions and high latitudes, are shown in yellow with their area increased to improve visibility. || ", "hits": 35 }, { "id": 11086, "url": "https://svs.gsfc.nasa.gov/11086/", "result_type": "Produced Video", "release_date": "2012-09-27T12:00:00-04:00", "title": "Simulations Uncover 'Flashy' Secrets of Merging Black Holes", "description": "According to Einstein, whenever massive objects interact, they produce gravitational waves — distortions in the very fabric of space and time — that ripple outward across the universe at the speed of light. While astronomers have found indirect evidence of these disturbances, the waves have so far eluded direct detection. Ground-based observatories designed to find them are on the verge of achieving greater sensitivities, and many scientists think that this discovery is just a few years away. Catching gravitational waves from some of the strongest sources — colliding black holes with millions of times the sun's mass — will take a little longer. These waves undulate so slowly that they won't be detectable by ground-based facilities. Instead, scientists will need much larger space-based instruments, such as the proposed Laser Interferometer Space Antenna, which was endorsed as a high-priority future project by the astronomical community. A team that includes astrophysicists at NASA's Goddard Space Flight Center in Greenbelt, Md., is looking forward to that day by using computational models to explore the mergers of supersized black holes. Their most recent work investigates what kind of \"flash\" might be seen by telescopes when astronomers ultimately find gravitational signals from such an event. To explore the problem, a team led by Bruno Giacomazzo at the University of Colorado, Boulder, and including Baker developed computer simulations that for the first time show what happens in the magnetized gas (also called a plasma) in the last stages of a black hole merger. In the turbulent environment near the merging black holes, the magnetic field intensifies as it becomes twisted and compressed. The team suggests that running the simulation for additional orbits would result in even greater amplification. The most interesting outcome of the magnetic simulation is the development of a funnel-like structure — a cleared-out zone that extends up out of the accretion disk near the merged black hole. The most important aspect of the study is the brightness of the merger's flash. The team finds that the magnetic model produces beamed emission that is some 10,000 times brighter than those seen in previous studies, which took the simplifying step of ignoring plasma effects in the merging disks. || ", "hits": 149 }, { "id": 11053, "url": "https://svs.gsfc.nasa.gov/11053/", "result_type": "B-Roll", "release_date": "2012-07-30T00:00:00-04:00", "title": "MAVEN Broadcast-Quality Spacecraft and Instrument Footage", "description": "This page contains broadcast-quality footage of the MAVEN spacecraft and science instruments. The MAVEN bus was built at Lockheed Martin Space Systems in Littleton, Colorado. MAVEN's science instruments were built at the Space Sciences Laboratory (SSL) at the University of California, Berkeley; at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado, Boulder; and at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Launch operations were conducted at the Kennedy Space Center on Cape Canaveral, Florida. MAVEN was launched on November 18, 2013 and arrived at Mars on September 21, 2014 EDT. || ", "hits": 46 }, { "id": 10952, "url": "https://svs.gsfc.nasa.gov/10952/", "result_type": "Produced Video", "release_date": "2012-04-17T00:00:00-04:00", "title": "The Biggest Losers", "description": "Giant ice sheets cover Antarctica and Greenland, holding 99 percent of the world's freshwater ice. But the ice sheets are giving up this water, as glaciers accelerate their journey to the sea and warmer air and ocean currents melt the ice. Orbiting 300 miles above Earth, NASA's twin GRACE (Gravity Recovery and Climate Experiment) satellites measure precisely how much these ice reservoirs are contributing to sea level rise. Measurements show Antarctica and Greenland are shedding roughly 385 billion tons of ice each year—that's more than 10 times the annual ice losses from Himalayan glaciers. This is causing global ocean waters to rise by about 0.04 inches each year. Watch the visualization below to see how the ice masses covering Greenland and Antarctica changed from 2003 to 2010. || ", "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": 121 }, { "id": 10920, "url": "https://svs.gsfc.nasa.gov/10920/", "result_type": "Produced Video", "release_date": "2012-03-08T00:00:00-05:00", "title": "Retreating Glaciers And Groundwater", "description": "The glacier-covered Himalayas are among the most hostile places on Earth, yet just south of the mountains, India's rapidly growing cities bustle with activity. Despite this contrast, human impact has altered the water and ice inventory of both regions, as measured by NASA's Gravity Recovery and Climate Experiment (GRACE) satellites. Driven by climate change, Himalayan glaciers are losing about 4 billion tons of ice each year—a large volume, but nowhere near previous higher estimates. Meanwhile, a burst of economic and population growth has drastically depleted groundwater reserves in northern India by an average of 35 billion tons annually. The visualization below provides a detailed look at the change in groundwater levels and ice-capped glaciers from 2003 to 2010 on a map of the region, where yellow dots mark the location of individual glaciers. || ", "hits": 44 }, { "id": 10892, "url": "https://svs.gsfc.nasa.gov/10892/", "result_type": "Produced Video", "release_date": "2012-02-23T00:00:00-05:00", "title": "Goodbye, Glaciers", "description": "While previous studies have focused on Antarctica's and Greenland's massive ice sheets, this year scientists offered the first detailed estimate of how much all the world's ice deposits are melting and contributing to sea level rise. Using data from NASA's twin GRACE satellites, researchers concluded that Earth has lost a total of 4.3 trillion tons of ice between 2003 and 2010. Greenland and Antarctica lost the bulk of the ice, but nearly a quarter of the losses came from glaciers in Alaska, Canada and Patagonia. The total melting during this period added about half an inch to global sea levels—enough to cover the United States with a layer of water one-and-a-half feet thick. GRACE's inventory of North and South America is shown on a rotating globe in the visualization below, where yellow dots mark the location of individual glaciers and areas with greatest ice loss are shaded purple and blue. || ", "hits": 43 }, { "id": 3906, "url": "https://svs.gsfc.nasa.gov/3906/", "result_type": "Visualization", "release_date": "2012-02-07T12:40:00-05:00", "title": "Global Mass Balance from GRACE", "description": "In the first comprehensive satellite study of its kind, a University of Colorado Boulder-led team used NASA data to calculate how much Earth's melting land ice is adding to global sea level rise.Using satellite measurements from the NASA/German Aerospace Center Gravity Recovery and Climate Experiment (GRACE), the researchers measured ice loss in all of Earth's land ice between 2003 and 2010, with particular emphasis on glaciers and ice caps outside of Greenland and Antarctica. The total global ice mass lost from Greenland, Antarctica and all Earth's glaciers and ice caps over the period studied was about 4.3 trillion tons (1,000 cubic miles), adding about 12 millimeters (0.5 inches) to global sea level. That's enough ice to cover the United States 1.5 feet (0.5 meters) deep.About a quarter of the average annual ice loss came from glaciers and ice caps outside of Greenland and Antarctica (about 148 billion tons, or 39 cubic miles), while ice loss from Greenland and Antarctica and their peripheral ice caps and glaciers averaged roughly 385 billion tons (100 cubic miles) a year. Results of the study are published online Feb. 8 in the journal Nature.\"Earth is losing a huge amount of ice to the ocean annually, and these new results will help us answer important questions in terms of both sea rise and how the planet's cold regions are responding to global change,\" said University of Colorado Boulder physics professor John Wahr, who helped lead the study.\"The strength of GRACE is it sees all the mass in the system, even though its resolution isn't high enough to allow us to determine separate contributions from each individual glacier,\" said Wahr, also a fellow at the University of Colorado-headquartered Cooperative Institute for Research in Environmental Sciences. Traditional estimates of Earth's ice caps and glaciers have been made using ground measurements from relatively few glaciers to infer what all the world's unmonitored glaciers were doing. Only a few hundred of the roughly 200,000 glaciers worldwide have been monitored for longer than a decade.One unexpected study result from GRACE was that the estimated ice loss from high Asian mountain ranges like the Himalaya, the Pamir and the Tien Shan was only about 4 billion tons of ice annually. Some previous ground-based estimates of ice loss in these high Asian mountains have ranged up to 50 billion tons annually, Wahr said.\"The GRACE results in this region really were a surprise,\" said Wahr. \"One possible explanation is that previous estimates were based on measurements taken primarily from some of the lower, more accessible glaciers in Asia and were extrapolated to infer the behavior of higher glaciers. But unlike the lower glaciers, most of the high glaciers are located in very cold environments, and require greater amounts of atmospheric warming before local temperatures rise enough to cause significant melting. This makes it difficult to use low-elevation, ground-based measurements to estimate results from the entire system.\"\"This study finds that the world's small glaciers and ice caps in places like Alaska, South America and the Himalayas contribute about 0.4 millimeters (.02 inches) per year to sea level rise,\" said Tom Wagner, cryosphere program scientist at NASA Headquarters in Washington. \"While this is lower than previous estimates, it confirms that ice is being lost from around the globe, with just a few areas in precarious balance. The results sharpen our view of land ice melting, which poses the biggest, most threatening factor in future sea level rise.\"Launched in 2002, the twin GRACE satellites track changes in Earth's gravity field by noting minute changes in gravitational pull caused by regional variations in Earth's mass, which for periods of months to years is typically due to movements of water on Earth's surface. It does this by measuring changes in the distance between its two identical spacecraft to one-hundredth the width of a human hair. The spacecraft, developed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., are in the same orbit approximately 220 kilometers (137 miles) apart. || ", "hits": 23 } ] }