{ "count": 64, "next": null, "previous": null, "results": [ { "id": 14859, "url": "https://svs.gsfc.nasa.gov/14859/", "result_type": "Produced Video", "release_date": "2025-06-21T00:00:00-04:00", "title": "Webb Stellarium", "description": "Stellarium is an installation video designed for the Goddard Space Flight Center visitor center. It is playing temporarily in the room designed for Solarium, and installation built around Sun footage from the Solar Dynamics Observatory (SDO).\r\n\r\nStellarium sources James Webb Space Telescope imagery processed and provided by the Space Telescope Science Institute and available here.", "hits": 101 }, { "id": 14757, "url": "https://svs.gsfc.nasa.gov/14757/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman Space Telescope's Coronagraph Instrument Integration into the Instrument Carrier", "description": "The Coronagraph, one of two science instruments, finds it home in NASA's Nancy Grace Roman Telescope Instrument Carrier.Designed and built by NASA’s Jet Propulsion Laboratory, the Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars (exoplanets). Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet. The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star. || ", "hits": 64 }, { "id": 14759, "url": "https://svs.gsfc.nasa.gov/14759/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman's Wide Field Instrument added to the Mirror Assembly", "description": "B-roll footage slowed from 60 frames per second and 30 frames per second of the Wide Field Instrument (WFI) installation. || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_print.jpg (1024x576) [202.4 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_searchweb.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_web.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly_ProRes.mov (3840x2160) [35.6 MB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_thm.png [6.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.mp4 (3840x2160) [3.8 GB] || ", "hits": 63 }, { "id": 14678, "url": "https://svs.gsfc.nasa.gov/14678/", "result_type": "Produced Video", "release_date": "2025-01-07T00:00:00-05:00", "title": "Astronauts Practice NICER Repair", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague practiced a repair for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station. The training exercise took place in the (NBL) Neutral Buoyancy Laboratory at NASA’s Johnson Space Center in Houston.Before any spacewalk, astronauts rehearse activities in the NBL to simulate — as much as possible — the conditions under which they’ll complete the task in space.In May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the instrument. The damage allows sunlight to reach the detectors during the station’s daytime, saturating sensors and interfering with NICER’s X-ray measurements. The damage does not impact nighttime observations.The NICER team developed a plan to cover the largest areas of damage using five patches, each shaped like a piece of pie, to be inserted into the instrument’s sunshades and locked in place. || ", "hits": 74 }, { "id": 14602, "url": "https://svs.gsfc.nasa.gov/14602/", "result_type": "Produced Video", "release_date": "2024-06-17T06:00:00-04:00", "title": "NOAA Interview Opportunity: Ready to GOES! NOAA’s Latest GOES Weather Satellite Ready To Launch Next Week!", "description": "Join a NOAA expert on June 25, 2024 to celebrate the launch of the next and final installment of the GOES weather satellite series!From Earth weather to space weather, NOAA’s fleet of geostationary satellites play an important role in our everyday lives. And on June 25th, the fourth and final installation of the GOES-R series is set to launch from NASA’s Kennedy Space Center. As the final satellite in NOAA’s GOES-R (Geostationary Operational Environmental Satellites) series, GOES-U will continue to provide fast, clear and reliable weather-tracking information. GOES-U will provide real-time data for monitoring severe weather, hurricanes, wildfires, floods, fog and even lightning. Not only that, GOES-U carries a suite of instruments, including the first operational compact coronagraph, to monitor the Sun and warn us of approaching space weather hazards. A coronagraph is an instrument that blocks out the bright disk of the Sun so that researchers can see our star’s fainter outer atmosphere where much of the solar activity originates. This new coronagraph will better detect and characterize coronal mass ejections. The GOES series of weather satellites are parked in a geostationary orbit at points over the equator and rotate at the same speed as the Earth. The fixed location provides continuous coverage of weather conditions across the Western hemisphere. Once in orbit GOES-U will be renamed GOES-19. After an on-orbit check out to ensure its instruments and systems are working properly, GOES-19 will go into service as GOES-East, replacing GOES-16. In this location, GOES-19 will watch over most of North America, including the contiguous United States and Mexico, as well as Central and South America, the Caribbean, and the Atlantic Ocean to the west coast of Africa.* Live interviews are available June 25, 2024, between 6 a.m. - 1 p.m. EDT* Click here to request an interview: https://forms.gle/ny5wyq2mP52hQcyu7* Requests sent via the above form will have scheduling priority. Please do not email requests.* Find out more about GOES and other NOAA missions here @NOAASatellites and https://www.nesdis.noaa.gov/goes-uSuggested Anchor Intro:The nation’s most advanced fleet of weather satellites is about to get an update. Later today the fourth and final installation of NOAA’s GOES-R series will launch from NASA’s Kennedy Space Center. The new satellite, named GOES-U, will join the fleet that helps keep us safe here on the ground and in space. Welcome NOAA expert XX live from Cape Canaveral where GOES-U will launch in just a few hours.Suggested Questions:1. What is the GOES-U mission and why is it important? 2. GOES-U is the final installment in the series and we hear it has a new instrument on board that will be focused on space weather from the Sun. Can you tell us about this new instrument? 3. Here in our area, we’re particularly concerned about ______. How will GOES-U help forecasters better predict these types of extremes? [stations choice]: Wildfire and smoke monitoring and tracking Hurricane & storm tracking Lightning trackingFlooding4. What are you most excited about with the GOES-U launch?5. How can viewers watch the launch today and keep up to date on this mission? Questions for longer interviews: 6. What's next after GOES-U? What does NOAA have planned?7. Once GOES-U is launched, where will it be positioned in orbit?8. What is a geostationary orbit, and why is it used for the GOES satellites? || ", "hits": 33 }, { "id": 14494, "url": "https://svs.gsfc.nasa.gov/14494/", "result_type": "Produced Video", "release_date": "2024-01-08T10:00:00-05:00", "title": "Atmospheric Waves Experiment (AWE) Installation", "description": "On Saturday, Nov. 18, at 2 p.m. EST, installation of NASA’s Atmospheric Waves Experiment (AWE) was completed on the International Space Station.By remotely controlling the Canadarm2 robotic arm, engineers first extracted AWE from SpaceX’s Dragon cargo spacecraft a couple days after it arrived at the station on Nov. 11. Then, on Saturday, using the Canadarm2 robotic arm again, engineers completed AWE’s installation onto the EXPRESS Logistics Carrier 1, a platform designed to support external payloads mounted to the International Space Station.AWE is led by Ludger Scherliess at Utah State University in Logan, and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Utah State University’s Space Dynamics Laboratory built the AWE instrument and provides the mission operations center.To learn more visit science.nasa.gov/mission/awe || ", "hits": 83 }, { "id": 14440, "url": "https://svs.gsfc.nasa.gov/14440/", "result_type": "Produced Video", "release_date": "2023-10-25T08:00:00-04:00", "title": "Atmospheric Waves Experiment (AWE) Media Resources", "description": "From its unique vantage point on the International Space Station, NASA’s Atmospheric Waves Experiment (AWE) will look directly down into Earth’s atmosphere to study how gravity waves travel through the upper atmosphere. Data collected by AWE will enable scientists to determine the physics and characteristics of atmospheric gravity waves and how terrestrial weather influences the ionosphere, which can affect communication with satellites.AWE is led by Michael Taylor at Utah State University in Logan, and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Utah State University’s Space Dynamics Laboratory built the AWE instrument and will provide the mission operations center.Visit https://science.nasa.gov/mission/awe/ to learn more. Watch AWE launch aboard NASA's SpaceX Cargo Dragon. Download isolated launch views of NASA's SpaceX CRS-29 mission. || ", "hits": 89 }, { "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": 79 }, { "id": 13804, "url": "https://svs.gsfc.nasa.gov/13804/", "result_type": "Produced Video", "release_date": "2021-02-16T09:55:00-05:00", "title": "Hubble’s Servicing Mission 2", "description": "The Second Servicing Mission, launched February 11, 1997, greatly improved Hubble's productivity. The installation of new instruments extended Hubble's wavelength range into the near infrared for imaging and spectroscopy, allowing us to probe the most distant reaches of the universe. The replacement of failed or degraded spacecraft components increased efficiency and performance.A seven-member STS-82 crew took part in this mission. Four astronauts conducted the planned spacewalks: Mark Lee, Gregory Harbaugh, Steven Smith and Joseph Tanner were part of the extravehicular activity crew. Kenneth Bowersox was the commander, Scott Horowitz was the pilot, and Steven Hawley was the Remote Manipulator System Operator.For more information, visit https://nasa.gov/hubble. Music Credits: \"Cristal Delight\" by Fred Dubois [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Paradigm” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Temporal Kinetics” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Drive to Succeed” by Stephen Daniel Lemaire [ASCAP] via El Murmullo Sarao [SGAE], Universal Sarao [SGAE] and Universal Production Music.Motion Graphics Template Media Credits:Lower Thirds Auto Self Resizing by cayman via Motion Array || ", "hits": 26 }, { "id": 40414, "url": "https://svs.gsfc.nasa.gov/gallery/webb-arapp-media/", "result_type": "Gallery", "release_date": "2020-04-02T00:00:00-04:00", "title": "Webb AR App Media", "description": "Backend video content to support the Webb AR app!", "hits": 113 }, { "id": 13434, "url": "https://svs.gsfc.nasa.gov/13434/", "result_type": "Produced Video", "release_date": "2019-12-09T14:00:00-05:00", "title": "Operation IceBridge - Thule, Greenland Landscape", "description": "Thule, Greenland has been one of the major hubs of Operation IceBridge since the mission began in 2009. The Thule Air Base, located 750 miles north of the Arctic circle, has been a critical hub of IceBridge Arctic flights during the course of the mission. || ", "hits": 61 }, { "id": 40388, "url": "https://svs.gsfc.nasa.gov/gallery/nasaearth-science/", "result_type": "Gallery", "release_date": "2019-09-13T10:53:37-04:00", "title": "NASA Earth Science", "description": "NASA’s Earth Science Division (ESD) missions help us to understand our planet’s interconnected systems, from a global scale down to minute processes. Working in concert with a satellite network of international partners, ESD can measure precipitation around the world, and it can employ its own constellation of small satellites to look into the eye of a hurricane. ESD technology can track dust storms across continents and mosquito habitats across cities.\n\nFor more information:\nhttps://science.nasa.gov/earth-science", "hits": 209 }, { "id": 12971, "url": "https://svs.gsfc.nasa.gov/12971/", "result_type": "Produced Video", "release_date": "2018-10-19T13:00:00-04:00", "title": "Unboxing a New NASA Spacecraft", "description": "Go behind the scenes as we unbox NASA’s Ionospheric Connection Explorer, or ICON, after its arrival at Vandenberg Air Force Base in California. Northrop Grumman engineer Steve Turek and NASA EDGE’s Chris Giersch walk us through the whole process of unboxing a spacecraft – from the instrument that records every tiny bump on its journey to the special crane used to lift the spacecraft to its new home.ICON launches in fall 2018 from NASA's Kennedy Space Center in Florida to study Earth’s interface to space. Read more about the ICON mission: nasa.gov/icon || ", "hits": 26 }, { "id": 13082, "url": "https://svs.gsfc.nasa.gov/13082/", "result_type": "Produced Video", "release_date": "2018-10-04T11:00:00-04:00", "title": "Hubble Archive - Servicing Mission 1, STS-61", "description": "Shortly after the Hubble Space Telescope was deployed in 1990, the observatory's primary mirror was discovered to have an aberration that affected the clarity of the telescope's early images. Fortunately, Hubble, orbiting 353 miles (569 km) above the surface of the Earth, was the first telescope designed to be visited in space by astronauts to perform repairs, replace parts, and update its technology with new instruments. Servicing Mission 1, launched in December 1993, was the first opportunity to conduct planned maintenance on the telescope. In addition, new instruments were installed and the optics of the flaw in Hubble's primary mirror was corrected. || ", "hits": 86 }, { "id": 30979, "url": "https://svs.gsfc.nasa.gov/30979/", "result_type": "Hyperwall Visual", "release_date": "2018-07-31T00:00:00-04:00", "title": "ECOSTRESS Installation and First Data", "description": "The first light image from ECOSTRESS, showing the Nile river valley. || ecostress_first_light_PIA22590.png (1920x1080) [1.3 MB] || ecostress_first_light_PIA22590_print.jpg (1024x576) [99.0 KB] || ecostress_first_light_PIA22590_searchweb.png (320x180) [55.4 KB] || ecostress_first_light_PIA22590_thm.png (80x40) [4.5 KB] || ecostress_first_light_PIA22590.hwshow [228 bytes] || ", "hits": 72 }, { "id": 13011, "url": "https://svs.gsfc.nasa.gov/13011/", "result_type": "Produced Video", "release_date": "2018-07-25T00:00:00-04:00", "title": "Sounds of the Sun", "description": "An illustration of a sunspot inspired by imagery from NASA's Solar Dynamics Observatory (SDO). || sunspot.gif (1280x720) [1.5 MB] || sunspot_searchweb.png (320x180) [95.7 KB] || ", "hits": 257 }, { "id": 12997, "url": "https://svs.gsfc.nasa.gov/12997/", "result_type": "Produced Video", "release_date": "2018-07-12T15:00:00-04:00", "title": "Parker Solar Probe Beauty Images", "description": "Still ImageParker Solar Probe sits in a clean room on July 6, 2018, at Astrotech Space Operations in Titusville, Florida, after the installation of its heat shield.Credit: NASA/Johns Hopkins APL/Ed Whitman || 5D1_9384_print.jpg (1024x774) [479.3 KB] || 5D1_9384.jpg (3840x2903) [6.6 MB] || 5D1_9384_searchweb.png (320x180) [88.4 KB] || 5D1_9384_web.png (320x241) [114.7 KB] || 5D1_9384_thm.png (80x40) [6.8 KB] || ", "hits": 108 }, { "id": 12979, "url": "https://svs.gsfc.nasa.gov/12979/", "result_type": "Produced Video", "release_date": "2018-06-06T15:00:00-04:00", "title": "Power Up: Solar Arrays Installed on NASA’s Mission to Touch the Sun", "description": "NASA’s Parker Solar Probe depends on the Sun, not just as an object of scientific investigation, but also for the power that drives its instruments and systems. On Thursday, May 31, 2018, the spacecraft’s solar arrays were installed and tested. These arrays will power all of the spacecraft’s systems, including the suites of scientific instruments studying the solar wind and the Sun’s corona as well as the Solar Array Cooling System (SACS) that will protect the arrays from the extreme heat at the Sun. “Unlike solar-powered missions that operate far from the Sun and are focused only on generating power from it, we need to manage the power generated along with the substantial heat that comes from being so close to the Sun,” said Andy Driesman, project manager from the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland. “When we’re out around the orbit of Venus, we fully extend the arrays to get the power we need. But when we’re near the Sun, we tuck the arrays back until only a small wing is exposed, and that portion is enough to provide needed electrical power.”The solar arrays are cooled by a gallon of water that circulates through tubes in the arrays and into large radiators at the top of the spacecraft. They are just over three and a half feet (1.12 meters) long and nearly two and a half feet (0.69 meters) wide. Mounted on motorized arms, the arrays will retract almost all of their surface behind the Thermal Protection System – the heat shield – when the spacecraft is close to the Sun. The solar array installation marks some of the final preparation and testing of Parker Solar Probe leading up to the mission’s July 31 launch date. || ", "hits": 41 }, { "id": 12841, "url": "https://svs.gsfc.nasa.gov/12841/", "result_type": "Produced Video", "release_date": "2018-01-30T15:00:00-05:00", "title": "Parker Solar Probe: Solar60 Series", "description": "Parker Solar Probe Enters Thermal Vacuum ChamberNASA's Parker Solar Probe Deputy Lead Mechanical Engineer Felipe Ruiz and Lead Thermal Engineer Jack Ercol - both from Johns Hopkins Applied Physics Lab - take us through the process of preparing the spacecraft for space environment testing. The Thermal Protection System (TPS) simulator placed on the spacecraft is to provide accurate simulation conditions during testing. Learn more here. Credit: NASA/Johns Hopkins APL/Lee HobsonWatch this video on the Johns Hopkins APL YouTube channel. || 1800101Solar6001PSPTVacV31080p.00037_print.jpg (1024x576) [194.3 KB] || 1800101Solar6001PSPTVacV31080p.00037_searchweb.png (320x180) [112.2 KB] || 1800101Solar6001PSPTVacV31080p.00037_web.png (320x180) [112.2 KB] || 1800101Solar6001PSPTVacV31080p.00037_thm.png (80x40) [7.6 KB] || 1800101Solar6001PSPTVacV31080p.mp4 (1920x1080) [189.9 MB] || 1800101Solar6001PSPTVacV31080p.webm (1920x1080) [12.1 MB] || Solar60_1captions.en_US.srt [1.7 KB] || Solar60_1captions.en_US.vtt [1.7 KB] || ", "hits": 24 }, { "id": 12726, "url": "https://svs.gsfc.nasa.gov/12726/", "result_type": "Produced Video", "release_date": "2017-09-22T18:00:00-04:00", "title": "Parker Solar Probe: Testing and Integration", "description": "Main flight harness installation.Credit: NASA/JHUAPL || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_print.jpg (1024x576) [120.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_searchweb.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_web.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_thm.png (80x40) [5.6 KB] || 12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1920x1080) [2.9 GB] || PRORES_B-ROLL-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1280x720) [1.5 GB] || YOUTUBE_1080-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_youtube_1080.mp4 (1920x1080) [373.7 MB] || APPLE_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_appletv.m4v (1280x720) [117.9 MB] || NASA_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072.mpeg (1280x720) [697.9 MB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.mp4 (1920x1080) [209.3 MB] || 17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_1080p.mp4 (1920x1080) [408.5 MB] || LARGE_MP4-12726_ParkerSolarProbe_blanketing_17-08-01-08_SPP_Timelapse_17-00_large.webm (1280x720) [15.6 MB] || NASA_PODCAST-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_ipod_sm.mp4 (320x240) [38.5 MB] || ", "hits": 128 }, { "id": 12662, "url": "https://svs.gsfc.nasa.gov/12662/", "result_type": "Produced Video", "release_date": "2017-08-03T13:00:00-04:00", "title": "TESS Camera Mounting Photos", "description": "TESS cameras being mounted onto the camera plate at Orbital ATK in Dulles, Va. prior to installation onto spacecraft. || TESS_Camera_3_Install_-_026.jpg (3229x3840) [2.3 MB] || TESS_Camera_3_Install_-_026_thm.png (80x40) [7.6 KB] || TESS cameras being mounted to the camera plate at Orbital ATK in Dulles, Va. before installation onto the spacecraft. || ", "hits": 20 }, { "id": 12316, "url": "https://svs.gsfc.nasa.gov/12316/", "result_type": "Produced Video", "release_date": "2017-08-03T11:00:00-04:00", "title": "TESS Camera Mounting Timelapse", "description": "A timelapse of TESS cameras being mounted to the camera plate before installation onto spacecraft. || TESS_B-Roll_-_Camera3_Mount-ProRes.00001_print.jpg (1024x576) [167.3 KB] || TESS_B-Roll_-_Camera3_Mount-ProRes.00001_searchweb.png (320x180) [103.9 KB] || TESS_B-Roll_-_Camera3_Mount-ProRes.00001_web.png (320x180) [103.9 KB] || TESS_B-Roll_-_Camera3_Mount-ProRes.00001_thm.png (80x40) [7.3 KB] || TESS_B-Roll_-_Camera3_Mount-ProRes.mov (1920x1080) [1.0 GB] || TESS_B-Roll_-_Camera3_Mount-ProRes.webm (1920x1080) [8.1 MB] || ", "hits": 29 }, { "id": 12668, "url": "https://svs.gsfc.nasa.gov/12668/", "result_type": "Produced Video", "release_date": "2017-07-17T13:00:00-04:00", "title": "NICER in Space", "description": "Several cameras on the International Space Station (ISS) have eyes on NICER. Since arriving to the space station on June 5 – aboard SpaceX’s eleventh cargo resupply mission – NICER underwent robotic installation on ExPRESS Logistics Carrier 2, initial deployment, precise point tests and more. This video shows segments of NICER’s time in space. Scientists and engineers will continue to watch NICER, using these cameras, throughout the mission’s science operations. || ", "hits": 41 }, { "id": 12430, "url": "https://svs.gsfc.nasa.gov/12430/", "result_type": "B-Roll", "release_date": "2017-02-16T15:00:00-05:00", "title": "Webb Telescope First Golden Mirror Installation 4K B-Roll", "description": "4K B-roll footage of the Webb Telescope's first flight mirror being installed onto the backplane at GSFC. || Screen_Shot_2016-11-29_at_4.05.32_PM.png (1920x1080) [4.3 MB] || Screen_Shot_2016-11-29_at_4.05.32_PM_print.jpg (1024x576) [198.2 KB] || Screen_Shot_2016-11-29_at_4.05.32_PM_searchweb.png (320x180) [129.2 KB] || Screen_Shot_2016-11-29_at_4.05.32_PM_thm.png (80x40) [8.4 KB] || First_Mirror_Install_4K_B-Roll_Master.mov (3840x2160) [16.7 GB] || First_Mirror_Install_4K_B-Roll_Master.mp4 (3840x2160) [134.3 MB] || First_Mirror_Install_4K_B-Roll_Master.webm (3840x2160) [24.2 MB] || First_Mirror_Install_4K_B-Roll_Master.wmv [0 bytes] || ", "hits": 27 }, { "id": 12431, "url": "https://svs.gsfc.nasa.gov/12431/", "result_type": "B-Roll", "release_date": "2017-02-16T15:00:00-05:00", "title": "Webb Telescope's 18th Golden Mirror Installation 4K B-Roll", "description": "4K B-roll footage of the 18th golden mirror being installed to the backplane structure of the Webb Telescope. || Screen_Shot_2016-11-30_at_1.46.14_PM_print.jpg (1024x570) [199.9 KB] || Screen_Shot_2016-11-30_at_1.46.14_PM_searchweb.png (320x180) [125.4 KB] || Screen_Shot_2016-11-30_at_1.46.14_PM_print_thm.png (80x40) [8.5 KB] || 18th_Mirror_Install_4K_B-roll_Master.mov (3840x2160) [54.5 MB] || 18th_Mirror_Install_4K_B-roll_Master.mp4 (3840x2160) [147.7 MB] || 18th_Mirror_Install_4K_B-roll_Master.webm (3840x2160) [200.2 KB] || 18th_Mirror_Install_4K_B-roll_Master.wmv [0 bytes] || ", "hits": 16 }, { "id": 12446, "url": "https://svs.gsfc.nasa.gov/12446/", "result_type": "B-Roll", "release_date": "2017-02-16T15:00:00-05:00", "title": "ISIM Installation 4K B-Roll", "description": "4K b-roll footage of the Integrated Science Instrument Module being installed into the James Webb Space Telescope's Optical Telescope Element. || Screen_Shot_2016-12-06_at_2.15.16_PM_print.jpg (1024x575) [170.7 KB] || Screen_Shot_2016-12-06_at_2.15.16_PM_searchweb.png (320x180) [116.4 KB] || Screen_Shot_2016-12-06_at_2.15.16_PM_thm.png (80x40) [8.0 KB] || ISIM_Instillation_4K_B-Roll_Master_.mov (3840x2160) [14.1 GB] || ISIM_Instillation_4K_B-Roll_Master_.mp4 (3840x2160) [122.2 MB] || ISIM_Instillation_4K_B-Roll_Master_.webm (3840x2160) [21.1 MB] || ISIM_Instillation_4K_B-Roll_Master_.wmv [0 bytes] || ", "hits": 24 }, { "id": 12331, "url": "https://svs.gsfc.nasa.gov/12331/", "result_type": "Produced Video", "release_date": "2016-08-01T00:00:00-04:00", "title": "Hubble Traveling Exhibit", "description": "Hubble's \"New Views of the Universe\" traveling exhibit immerses visitors in the magnificence and mystery of the Hubble mission and introduces the James Webb Space Telescope. If you are considering hosting the exhibit, you may explore the different sections of the installation in these videos. If you are currently hosting the exhibit, you are welcome to share this short promotional video. A special thank you to the Buffalo State University Planetarium, Buffalo, NY and its students for supporting the production of this video.For more information, visit nasa.gov/content/the-hubble-traveling-exhibit || ", "hits": 20 }, { "id": 12295, "url": "https://svs.gsfc.nasa.gov/12295/", "result_type": "Produced Video", "release_date": "2016-06-27T15:00:00-04:00", "title": "Reflections on JWST", "description": "Reflections on NASA's James Webb Space Telescope's gold-coated mirrors || Photo_print.jpg (1024x574) [116.0 KB] || Photo.png (4508x2530) [10.9 MB] || Photo_searchweb.png (320x180) [95.9 KB] || Photo_web.png (320x179) [96.0 KB] || Photo_thm.png (80x40) [9.9 KB] || Reflections_on_JWST_May_4_2016.mp4 (1920x1080) [143.1 MB] || Reflections_on_JWST_May_4_2016.webm (1920x1080) [10.4 MB] || ", "hits": 20 }, { "id": 12273, "url": "https://svs.gsfc.nasa.gov/12273/", "result_type": "Produced Video", "release_date": "2016-06-07T09:00:00-04:00", "title": "Webb Telescope's Science Instrument Installation Time Lapse", "description": "Time Lapse video of the science instrument package installation into the Webb Telescope. || ISIM_Install_timelapse-IMAGE_ONLY.00001_print.jpg (1024x576) [212.2 KB] || ISIM_Install_timelapse-IMAGE_ONLY.00001_searchweb.png (180x320) [122.0 KB] || ISIM_Install_timelapse-IMAGE_ONLY.00001_web.png (320x180) [122.0 KB] || ISIM_Install_timelapse-IMAGE_ONLY.00001_thm.png (80x40) [7.7 KB] || ISIM_Install_timelapse_5-19-2016-h264.mp4 (1920x1080) [52.3 MB] || ISIM_Install_timelapse-5-19-2016-ProRes-master.webm (1920x1080) [10.3 MB] || ISIM_Install_timelapse_5-19-2016-closecap-srt.en_US.srt [937 bytes] || ISIM_Install_timelapse_5-19-2016-closecap-srt.en_US.vtt [950 bytes] || ISIM_Install_timelapse-5-19-2016-ProRes-master.mov (1920x1080) [1.4 GB] || ISIM_Install_timelapse_5-19-2016-h264.mp4.hwshow [90 bytes] || ", "hits": 28 }, { "id": 12212, "url": "https://svs.gsfc.nasa.gov/12212/", "result_type": "Produced Video", "release_date": "2016-04-14T14:00:00-04:00", "title": "JWST Secondary Mirror Installation", "description": "NASA's James Webb Space Telescope Secondary Mirror Installed || Secondary_Mirror_Installation.png (1914x1073) [2.6 MB] || Secondary_Mirror_Installation_print.jpg (1024x574) [125.2 KB] || Secondary_Mirror_Installation_searchweb.png (320x180) [112.5 KB] || Secondary_Mirror_Installation_web.png (320x179) [112.0 KB] || Secondary_Mirror_Installation_thm.png (80x40) [13.5 KB] || Secondary_Mirror_Installation.mp4 (1280x720) [288.6 MB] || Secondary_Mirror_Installation_59.94_Sequence.mov (1920x1080) [181.1 MB] || Secondary_Mirror_Installation_29.97_Sequence.mov (1920x1080) [180.3 MB] || Secondary_Mirror_Installation.webm (1280x720) [18.8 MB] || ", "hits": 32 }, { "id": 12187, "url": "https://svs.gsfc.nasa.gov/12187/", "result_type": "B-Roll", "release_date": "2016-04-01T00:00:00-04:00", "title": "Webb's Heart Endures Its Last Cryogenic Test B-Roll", "description": "B-roll footage of engineers at NASA Goddard Space Flight Center lifting the Webb Telescope's ISIM along with it's instruments, out of the Speace Environment Simulator after completing its last cryogenic test before integration into the telescope. || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_print.jpg (1024x576) [179.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_searchweb.png (180x320) [110.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_web.png (320x180) [110.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_thm.png (80x40) [7.4 KB] || ISIM_Completes_Last_Cryo_Test-B-ROLL-h264.mov (1280x720) [384.0 MB] || ISIM_Completes_Last_Cryo_Test-B_ROLL-ProREs-master.mov (1920x1080) [6.6 GB] || ISIM_Completes_Last_Cryo_Test-B-ROLL-h264.webm (1280x720) [51.7 MB] || ", "hits": 31 }, { "id": 12186, "url": "https://svs.gsfc.nasa.gov/12186/", "result_type": "Produced Video", "release_date": "2016-03-29T10:00:00-04:00", "title": "Webb's Heart Endures Its Last Cryogenic Test Before Installation Into the Telescope", "description": "A produced video showing engineers at NASA Goddard Space Flight Center lifting the Webb Telescope's instruments and their support structure out of the Space Environment Simulator after completing it's last cryogenic test before installation into the telescope || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_print.jpg (1024x576) [179.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_searchweb.png (180x320) [110.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_web.png (320x180) [110.4 KB] || ISIM_Completes_Last_Cryo_Test-IMAGE-ONLY.00001_thm.png (80x40) [7.4 KB] || ISIM_Completes_Last_Cryo_Test-VSS-2-2016-h264.mov (1280x720) [90.3 MB] || ISIM_Completes_Last_Cryo_Test_VSS-2-2016-ProRes_master.mov (1920x1080) [1.5 GB] || ISIM_Completes_Last_Cryo_Test-VSS-2-2016-h264.webm (1280x720) [12.0 MB] || ISIM_Completes_Last_Cryo_Test-VSS-closecap-srt.en_US.srt [954 bytes] || ISIM_Completes_Last_Cryo_Test-VSS-closecap-srt.en_US.vtt [967 bytes] || ", "hits": 30 }, { "id": 40297, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall29-mar2016/", "result_type": "Gallery", "release_date": "2016-03-29T00:00:00-04:00", "title": "Hyperwall 29 Mar 2016", "description": "Content for the March 2016 Hyperwall Content News mailing list", "hits": 6 }, { "id": 12120, "url": "https://svs.gsfc.nasa.gov/12120/", "result_type": "Produced Video", "release_date": "2016-02-22T14:00:00-05:00", "title": "NASA Goddard Spectrometer Launches on Hitomi Observatory", "description": "An artist's rendering of Hitomi in orbit.Credit: JAXA || Astro_h_art.jpg (3179x4500) [2.5 MB] || Astro_h_art_searchweb.png (180x320) [102.0 KB] || Astro_h_art_thm.png (80x40) [6.9 KB] || ", "hits": 39 }, { "id": 12146, "url": "https://svs.gsfc.nasa.gov/12146/", "result_type": "Produced Video", "release_date": "2016-02-09T11:00:00-05:00", "title": "Building The Next Hubble", "description": "Scientists and engineers finish installing the primary mirrors on NASA's next-generation space observatory. || cf-1024.jpg (1024x576) [96.4 KB] || cf-1280.jpg (1280x720) [128.6 KB] || cf-1920.jpg (1920x1080) [203.0 KB] || cf-1024_print.jpg (1024x576) [92.9 KB] || cf-1024_searchweb.png (320x180) [30.7 KB] || cf-1024_web.png (320x180) [30.7 KB] || cf-1024_thm.png (80x40) [3.4 KB] || ", "hits": 32 }, { "id": 12150, "url": "https://svs.gsfc.nasa.gov/12150/", "result_type": "B-Roll", "release_date": "2016-02-09T11:00:00-05:00", "title": "Webb Final Primary Mirror Installation B-roll", "description": "Raw footage of Webb's 18th and final mirror segment installation at NASA Goddard Space Flight Center. Part 1 of 2. || Webb_18th_Mirror_Instalation_B-roll-part_1-image_only_print.jpg (1024x576) [112.1 KB] || Webb_18th_Mirror_Instalation_B-roll-part_1-image_only_searchweb.png (320x180) [91.9 KB] || Webb_18th_Mirror_Instalation_B-roll-part_1-image_only_web.png (320x180) [91.9 KB] || Webb_18th_Mirror_Instalation_B-roll-part_1-image_only_thm.png (80x40) [7.0 KB] || Webb_18th_Mirror_Instalation_B-roll-part_1.mov (1920x1080) [5.2 GB] || Webb_18th_Mirror_Instalation_B-roll-part_1-h264.mov (1280x720) [309.4 MB] || Webb_18th_Mirror_Instalation_B-roll-part_1-h264.webm (1280x720) [40.0 MB] || ", "hits": 20 }, { "id": 12148, "url": "https://svs.gsfc.nasa.gov/12148/", "result_type": "Produced Video", "release_date": "2016-02-09T10:00:00-05:00", "title": "JWST Primary Mirror Installation Complete", "description": "Webb's 18th Mirror is Installed at Goodard Space Flight Center || Screen_Shot_2016-02-08_at_3.59.00_PM.png (1586x975) [2.5 MB] || Screen_Shot_2016-02-08_at_3.59.00_PM_print.jpg (1024x629) [164.9 KB] || Screen_Shot_2016-02-08_at_3.59.00_PM_searchweb.png (320x180) [124.2 KB] || Screen_Shot_2016-02-08_at_3.59.00_PM_web.png (320x196) [135.0 KB] || Screen_Shot_2016-02-08_at_3.59.00_PM_thm.png (80x40) [10.6 KB] || JWST_18_Mirror_Installation_Snapshot_h264.mov (1280x720) [2.0 GB] || JWST_18_Mirror_Installation_Snapshot_ProRes.mov (1280x720) [1.8 GB] || JWST_18_Mirror_Installation_Snapshot_h264.webm (1280x720) [13.3 MB] || JWST_Primary_Mirror_Complete_Snapshot_h264.mov (1280x720) [215.3 MB] || JWST_18_Mirror_Installation_Snapshot_h264_GoogOut.en_US.srt [376 bytes] || JWST_18_Mirror_Installation_Snapshot_h264_GoogOut.en_US.vtt [389 bytes] || ", "hits": 37 }, { "id": 12149, "url": "https://svs.gsfc.nasa.gov/12149/", "result_type": "B-Roll", "release_date": "2016-02-08T16:00:00-05:00", "title": "Webb Mirror Installation B-roll 2", "description": "Raw video of Webb Telescope mirror installation at NASA Goddard Space Flight Center || JWST_Mirror_Install_B-roll-image_only_print.jpg (1024x576) [172.3 KB] || JWST_Mirror_Install_B-roll-image_only_searchweb.png (320x180) [109.8 KB] || JWST_Mirror_Install_B-roll-image_only_web.png (180x320) [109.8 KB] || JWST_Mirror_Install_B-roll-image_only_thm.png (80x40) [7.5 KB] || JWST_Mirror_Install_B-roll_Part_2-ProRes-Master.mov (1920x1080) [9.6 GB] || JWST_Mirror_Install_B-roll_Part_2-h264.mov (1280x720) [589.0 MB] || JWST_Mirror_Install_B-roll_Part_2-h264.webm (1280x720) [67.7 MB] || ", "hits": 37 }, { "id": 12145, "url": "https://svs.gsfc.nasa.gov/12145/", "result_type": "Produced Video", "release_date": "2016-02-05T14:00:00-05:00", "title": "Webb Primary Mirror Installation Time Lapse", "description": "Time lapse video showing the installation of all 18 mirror segments of the Webb Telescope at the NASA Goddard Space Flight Center. || OTE-timelaspe-image.jpg (1920x1080) [1.3 MB] || OTE-timelaspe-image_print.jpg (1024x576) [647.9 KB] || OTE-timelaspe-image_searchweb.png (180x320) [149.2 KB] || OTE-timelaspe-image_web.png (320x180) [149.2 KB] || OTE-timelaspe-image_thm.png (80x40) [31.2 KB] || Webb_Mirror_Install_timelapse-quicktime.mov (1280x720) [82.6 MB] || Webb_Mirror_Install_timelapse-quicktime.webm (1280x720) [9.1 MB] || Webb_Mirror_Install_timelapse12145.key [87.1 MB] || Webb_Mirror_Install_timelapse12145.pptx [84.4 MB] || Webb_Mirror_Install_timelapse.mov (1920x1080) [1.4 GB] || webb-primary-mirror-installation-time-lapse.hwshow [343 bytes] || ", "hits": 48 }, { "id": 12115, "url": "https://svs.gsfc.nasa.gov/12115/", "result_type": "Produced Video", "release_date": "2016-01-04T16:00:00-05:00", "title": "Sen. Barbara Mikulski Visit To Goddard Jan. 6, 2016", "description": "B-roll of includes: Senator Mikulski views the James Webb Space Telescope being assembled in a clean room at Goddard. Webb project manager Bill Oches talked to the Senator about the progress being made with the installation of its 18 primary mirrors. The James Webb Space Telescope is the scientific successor to NASA's Hubble Space Telescope. Next Senator Mikulski participated in a ribbon cutting to officially open the new Robotic Operations Center (ROC) developed by the Satellite Servicing Capabilities Office. Goddard Center director Chris Scolese and Satellite Servicing Capabilities Office (SSCO) Associate Director Frank Cepollina stood next to the Senator as she cut the ribbon. SSCO Deputy Project Manager Ben Reed showed Mikulski around the ROC where they saw a demonstration of the robotic technology. || mikulski_sitting.png (1964x1296) [3.5 MB] || mikulski_sitting_print.jpg (1024x675) [131.9 KB] || Screen_Shot_2016-01-04_at_5.02.53_PM_searchweb.png (320x180) [111.0 KB] || mikulski_sitting_web.png (320x211) [123.8 KB] || mikulski_sitting_thm.png (80x40) [11.0 KB] || GSFC_Mikulski_Broll.mov (1280x720) [4.7 GB] || WEBM_GSFC_Mikulski_Broll.webm (960x540) [129.9 MB] || ", "hits": 20 }, { "id": 12528, "url": "https://svs.gsfc.nasa.gov/12528/", "result_type": "Produced Video", "release_date": "2015-12-23T00:00:00-05:00", "title": "NICER Lift Time-lapse", "description": "The Neutron star Interior Composition Explorer (NICER) box-shaped X-ray Timing Instrument (XTI) is lifted and integrated at NASA's Goddard Space Flight Center in Greenbelt, Maryland.The time-lapse shows the XTI, with attached flight electronics and the payload's pointing system, being lifted and joined to the flight Adapter Plate, NICER's connection to the International Space Station-provided hardware for installation on station. || ", "hits": 30 }, { "id": 12092, "url": "https://svs.gsfc.nasa.gov/12092/", "result_type": "Produced Video", "release_date": "2015-12-03T11:00:00-05:00", "title": "NASA’s Webb Space Telescope Receives First Mirror Installation", "description": "Produced Video showing engineers in the NASA Goddard Space Flight Center cleanroom placing the first mirror on the Webb Telescope. || VSS-Webb_Telescope_First_Mirror-image_only_print.jpg (1024x576) [209.6 KB] || VSS-Webb_Telescope_First_Mirror-image_only_searchweb.png (320x180) [117.2 KB] || VSS-Webb_Telescope_First_Mirror-image_only_web.png (180x320) [117.2 KB] || VSS-Webb_Telescope_First_Mirror-image_only_thm.png (80x40) [7.9 KB] || VSS-Webb_Telescope_First_Mirror_Installation-h264.mov (1280x720) [70.8 MB] || VSS-Webb_Telescope_First_Mirror_Installation-ProRes-master.mov (1920x1080) [1.1 GB] || VSS-Webb_Telescope_First_Mirror_Installation-h264.webm (1280x720) [8.9 MB] || VSS-Webb_Telescope_First_Mirror_Installation-srt-ccaption.en_US.srt [1017 bytes] || VSS-Webb_Telescope_First_Mirror_Installation-srt-ccaption.en_US.vtt [1.0 KB] || ", "hits": 46 }, { "id": 12090, "url": "https://svs.gsfc.nasa.gov/12090/", "result_type": "Produced Video", "release_date": "2015-11-30T14:00:00-05:00", "title": "James Webb Space Telescope: Ready for Mirror Assembly", "description": "Produced video showing engineers in the NASA Goddard Space Flight Center cleanroom lifting the Webb Telescope telescope structure into the assembly stand in preparation for installation of the primary mirror segments. || Telescope_Structure_Lift_to_Assembly_stand-image_only_print.jpg (1024x576) [184.9 KB] || Telescope_Structure_Lift_to_Assembly_stand-image_only_searchweb.png (320x180) [118.9 KB] || Telescope_Structure_Lift_to_Assembly_stand-image_only_web.png (180x320) [118.9 KB] || Telescope_Structure_Lift_to_Assembly_stand-image_only_thm.png (80x40) [7.8 KB] || Telescope_Structure_Lift_to_Assembly_stand-h264.mov (1280x720) [81.5 MB] || Telescope_Structure_Lift_to_Assembly_stand-master.mov (1920x1080) [1.2 GB] || Telescope_Structure_Lift_to_Assembly_stand-h264.webm (1280x720) [10.3 MB] || ", "hits": 34 }, { "id": 40110, "url": "https://svs.gsfc.nasa.gov/gallery/astro-galaxy/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Galaxy Listing", "description": "No description available.", "hits": 123 }, { "id": 40111, "url": "https://svs.gsfc.nasa.gov/gallery/astro-star/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Star Listing", "description": "No description available.", "hits": 176 }, { "id": 11887, "url": "https://svs.gsfc.nasa.gov/11887/", "result_type": "Produced Video", "release_date": "2015-06-03T14:00:00-04:00", "title": "JWST Pathfinder Backplane Mirror Placement GSFC", "description": "Backplane Pathfinder Mirror Placement || Screen_Shot_2015-06-03_at_11.07.44_AM.png (1273x713) [972.9 KB] || Screen_Shot_2015-06-03_at_11.07.44_AM_print.jpg (1024x573) [136.0 KB] || Screen_Shot_2015-06-03_at_11.07.44_AM_searchweb.png (320x180) [96.8 KB] || Screen_Shot_2015-06-03_at_11.07.44_AM_web.png (320x179) [96.4 KB] || Screen_Shot_2015-06-03_at_11.07.44_AM_thm.png (80x40) [9.9 KB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_youtube_hq.mov (1280x720) [91.8 MB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_prores.mov (1280x720) [1.8 GB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_1280x720.wmv (1280x720) [61.2 MB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_appletv.m4v (960x540) [51.1 MB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_youtube_hq.webm (1280x720) [13.3 MB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_ipod_lg.m4v (640x360) [20.0 MB] || Backplane_Pathfinder_EDU_Mirror_Placement_only-ITAR_cleared_ipod_sm.mp4 (320x240) [10.1 MB] || ", "hits": 21 }, { "id": 11787, "url": "https://svs.gsfc.nasa.gov/11787/", "result_type": "Produced Video", "release_date": "2015-02-26T13:25:00-05:00", "title": "CATS Up and Running on the Space Station", "description": "The Cloud-Aerosol Tranpsort System (CATS) was installed on the International Space Station on January 22, 2015. Data from CATS will help scientists model the structure of dust plumes and other atmospheric features, which can travel far distances and impact air quality. Climate scientists will also use the CATS data, along with data from other Earth-observing instruments, to look at trends and interactions in clouds and aerosols over time.For complete transcript, click here. || G2015-025_CATS_Install_MASTER_nasaportal_print.jpg (1024x576) [71.8 KB] || G2015-025_CATS_Install_MASTER_nasaportal_searchweb.png (320x180) [68.8 KB] || G2015-025_CATS_Install_MASTER_nasaportal_web.png (320x180) [68.8 KB] || G2015-025_CATS_Install_MASTER_nasaportal_thm.png (80x40) [5.6 KB] || G2015-025_CATS_Install_MASTER_prores.mov (1280x720) [1.7 GB] || G2015-025_CATS_Install_MASTER_youtube_hq.mov (1280x720) [72.1 MB] || G2015-025_CATS_Install_MASTER_appletv.m4v (960x540) [45.3 MB] || G2015-025_CATS_Install_MASTER.webm (960x540) [51.8 MB] || G2015-025_CATS_Install_MASTER_1280x720.wmv (1280x720) [54.2 MB] || G2015-025_CATS_Install_MASTER_appletv_subtitles.m4v (960x540) [45.2 MB] || G2015-025_CATS_Install_MASTER_nasaportal.mov (640x360) [43.3 MB] || G2015-025_CATS_Install_MASTER_ipod_lg.m4v (640x360) [18.4 MB] || G2015-025_CATS_Install-captions.en_US.srt [109 bytes] || G2015-025_CATS_Install-captions.en_US.vtt [122 bytes] || G2015-025_CATS_Install_MASTER_ipod_sm.mp4 (320x240) [9.9 MB] || ", "hits": 12 }, { "id": 11788, "url": "https://svs.gsfc.nasa.gov/11788/", "result_type": "Produced Video", "release_date": "2015-02-26T13:00:00-05:00", "title": "Earth Right Now Briefing - February 26, 2015", "description": "Over the past 12 months NASA has added five missions to its orbiting Earth-observing fleet – the biggest one-year increase in more than a decade. NASA scientists will discuss early observations from the new missions and their current status during a media teleconference at 2 p.m. EST Thursday, Feb. 26. New views of global carbon dioxide, rain and snowfall, ocean winds, and aerosol particles in the atmosphere will be presented during the briefing. The teleconference panelists are:Peg Luce, deputy director of the Earth Science Division in NASA’s Science Mission Directorate, Headquarters, WashingtonGail Skofronick-Jackson, GPM project scientist, NASA’s Goddard Space Flight Center, Greenbelt, MarylandRalph Basilio, Orbiting Carbon Observatory-2 project manager, NASA’s Jet Propulsion Laboratory, Pasadena, CaliforniaBryan Stiles, ISS-RapidScat science processing lead, NASA’s Jet Propulsion LaboratoryMatthew McGill, Cloud Aerosol Transport System (CATS) principal investigator, NASA’s Goddard Space Flight CenterNASA Releases First Global Rainfall and Snowfall Map from New Mission.Africa, from a CATS point of view.New NASA Earth Science Mission Expand View of Our Home Planet. || ", "hits": 36 }, { "id": 11777, "url": "https://svs.gsfc.nasa.gov/11777/", "result_type": "Produced Video", "release_date": "2015-02-13T16:00:00-05:00", "title": "JWST NIRSpec Microshutters Assembly Unit Gets Replaced", "description": "JWST NIRSpec Microshutters Assembly Unit gets replaced. || NIRSpec-MSA-change-out-broll_1-13-2015_youtube_hq_print.jpg (1024x576) [200.3 KB] || NIRSpec-MSA-change-out-broll_1-13-2015_youtube_hq_searchweb.png (320x180) [120.1 KB] || NIRSpec-MSA-change-out-broll_1-13-2015_youtube_hq_web.png (320x180) [120.1 KB] || NIRSpec-MSA-change-out-broll_1-13-2015_youtube_hq_thm.png (80x40) [8.0 KB] || NIRSpec-MSA-change-out-broll_1-13-2015_prores.mov (1280x720) [7.6 GB] || NIRSpec-MSA-change-out-broll_1-13-2015_appletv.m4v (960x540) [217.5 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_youtube_hq.mov (1280x720) [479.6 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_1280x720.wmv (1280x720) [265.1 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_appletv.webm (960x540) [56.8 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_nasaportal.mov (640x360) [218.8 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_ipod_lg.m4v (640x360) [84.9 MB] || NIRSpec-MSA-change-out-broll_1-13-2015_ipod_sm.mp4 (320x240) [45.0 MB] || ", "hits": 26 }, { "id": 11745, "url": "https://svs.gsfc.nasa.gov/11745/", "result_type": "Produced Video", "release_date": "2015-02-05T00:00:00-05:00", "title": "Solarium - Resource Page", "description": "A child looks up at Solarium at the Goddard Visitor Center in Greenbelt, Maryland.Photo Credit: NASA's Goddard Space Flight Center || E_LowAngle_304_crop_print.jpg (1024x677) [110.0 KB] || E_LowAngle_304_crop.png (3938x2604) [11.3 MB] || E_LowAngle_304_crop.jpg (3938x2604) [1.8 MB] || E_LowAngle_304_crop_web.png (320x211) [82.5 KB] || ", "hits": 49 }, { "id": 11487, "url": "https://svs.gsfc.nasa.gov/11487/", "result_type": "Produced Video", "release_date": "2014-02-20T12:00:00-05:00", "title": "GPM: Countdown to Launch", "description": "GPM is a joint mission between NASA and the Japan Aerospace Exploration Agency (JAXA). The Core Observatory will link data from a constellation of current and planned satellites to produce next-generation global measurements of rainfall and snowfall from space.The GPM mission is the first coordinated international satellite network to provide near real-time observations of rain and snow every three hours anywhere on the globe. The GPM Core Observatory anchors this network by providing observations on all types of precipitation. The observatory's data acts as the measuring stick by which partner observations can be combined into a unified data set. The data will be used by scientists to study climate change, freshwater resources, floods and droughts, and hurricane formation and tracking. || ", "hits": 31 }, { "id": 11314, "url": "https://svs.gsfc.nasa.gov/11314/", "result_type": "Produced Video", "release_date": "2013-07-25T13:55:00-04:00", "title": "IRIS First Light", "description": "The images and video on this page are from the IRIS first light media teleconference on July 25, 2013.For supporting media resources, please click here.On July 17, 2013 at 11:14 pm PDT (2:14 pm EDT) the IRIS Lockheed Martin instrument team successfully opened the door on NASA’s Interface Region Imaging Spectrograph, which launched June 27, 2013, aboard a Pegasus XL rocket from Vandenberg Air Force Base, Calif.As the telescope door opened, IRIS’s single instrument began to observe the sun for the first time. Designed to research the interface region in more detail than has ever been done before, IRIS’s instrument is a combination of an ultraviolet telescope and a spectrograph. The telescope provides high-resolution images, capturing data on about 1 percent of the sun at a time. The images can resolve very fine features, as small as 150 miles across. While the telescope can look at only one wavelength of light at a time, the spectrograph collects information about many wavelengths of light at once. The instrument then splits the sun’s light into its various wavelengths and measures how much of any given wavelength is present. Analysis of the spectral lines can also provide velocity, temperature and density information, key information when trying to track how energy and heat moves through the region. || ", "hits": 55 }, { "id": 11286, "url": "https://svs.gsfc.nasa.gov/11286/", "result_type": "Produced Video", "release_date": "2013-06-04T12:00:00-04:00", "title": "IRIS L-14 Media Briefing", "description": "Lying just above the sun's surface is an enigmatic region of the solar atmosphere called the interface region. A relatively thin region, just 3,000 to 6,000 miles thick, it pulses with movement: zones of different temperature and density are scattered throughout, while energy and heat course through the solar material. Understanding how the energy travels through this region – energy that helps heat the upper layer of the atmosphere, the corona, to temperatures of 1,000,000 kelvins, some thousand times hotter than the sun’s surface itself – is the goal of NASA's Interface Region Imaging Spectrograph, or IRIS, scheduled to launch on June 26, 2013 from California's Vandenberg Air Force Base. Scientists wish to understand the interface region in exquisite detail, since energy flowing through this region has an effect on so many aspects of near-Earth space. For one thing, despite the intense amount of energy deposited into the interface region, only a fraction leaksthrough, but this fraction drives the solar wind, the constant stream of particles that flows out to fill the entire solar system. The interface region is also the source of most of the sun's ultraviolet emission, which impacts both the near-Earth space environment and Earth's climate. IRIS's capabilities are uniquely tailored to unravel the interface region by providing both high-resolution images and a kind of data known as spectra, which can see many wavelengths at once. For its high-resolution images, IRIS will capture data on about one percent of the sun at a time. While these are relatively small snapshots, IRIS will be able to see very fine features, as small as 150 miles across. || ", "hits": 61 }, { "id": 11220, "url": "https://svs.gsfc.nasa.gov/11220/", "result_type": "Produced Video", "release_date": "2013-03-11T00:00:00-04:00", "title": "FGS/NIRISS Installation into the ISIM Structure", "description": "Time Lapse of FGS/NIRISS Installation into the ISIM Structure on February 28, 2013 in the NASA Goddard Space Flight Center clean room.NASA and Canadian Space Agency (CSA) engineers install the Fine Guidance Sensor (FGS) / Near-InfraRed Imager and Slitless Spectrograph (NIRISS) instrument package onto the Webb Telescope's Integrated Science Instrument Module (ISIM). The FGS/NIRISS was built by the Canadian Space Agency and delivered to NASA Goddard in July of 2012. The Fine Guidance Sensor (FGS) allows Webb to point precisely, so that it can obtain high-quality images. The Near Infrared Imager and Slitless Spectrograph part of the FGS/NIRISS will be used to investigate the following science objectives: first light detection, exoplanet detection and characterization, and exoplanet transit spectroscopy. It has a wavelength range of 0.8 to 5.0 microns, and is a specialized instrument with three main modes, each of which addresses a separate wavelength range. || ", "hits": 13 }, { "id": 11200, "url": "https://svs.gsfc.nasa.gov/11200/", "result_type": "Produced Video", "release_date": "2013-01-30T20:48:00-05:00", "title": "TDRS-K Video File", "description": "NASA is preparing to launch the first in a series of three third generation advanced Tracking and Data Relay Satellites, known as TDRS-K. This latest addition to the fleet of seven will augment a space communications network that provides the critical path for high data-rate communication to the International Space Station, Hubble Space Telescope, past shuttle missions and a host of other spacecraft. It has been 10 years since NASA last launched a TDRS. This launch is the beginning of a welcome replenishment to the space network, which has served numerous national and international space missions since 1983. || ", "hits": 81 }, { "id": 11058, "url": "https://svs.gsfc.nasa.gov/11058/", "result_type": "Produced Video", "release_date": "2012-08-02T00:00:00-04:00", "title": "Cruising With Curiosity", "description": "The Mars of today is desolate and cold, but has the planet ever been hospitable enough for life? NASA sent its Curiosity rover there to find out. Using a suite of instruments, Curiosity will explore the planet's habitability, past and present. Part of its payload consists of a trio of chemistry tools called SAM, short for Sample Analysis at Mars. SAM's job is to analyze samples scooped or drilled from the surface and \"sniff\" the Martian air for chemical clues about the environment. Roughly the size of a microwave oven, SAM can do the work of an entire chemistry lab and is the most advanced instrument of its kind ever sent to another planet. Watch the videos to learn more about SAM and see it in action. || ", "hits": 24 }, { "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": 39 }, { "id": 10232, "url": "https://svs.gsfc.nasa.gov/10232/", "result_type": "Produced Video", "release_date": "2008-08-22T00:00:00-04:00", "title": "HST SM4 COS Installation EVA", "description": "Cosmic Origins Spectrograph (COS) will be the most sensitive ultraviolet spectrograph ever flown on Hubble. COS will probe the \"cosmic web\" - the large-scale structure of the universe whose form is determined by the gravity of dark matter and is traced by galaxies and intergalactic gas. COS will explore how the \"cosmic web\" evolved from ancient times. COS will also sample the chemical content and physical state of gas in distant galaxy halos, providing important insight into the building process of early galaxies and the production of elements heavier than hydrogen and helium over cosmic time. Required to accomplish these goals is the extraordinary sensitivity of COS's far-ultraviolet channel—a factor more than 30 times greater than that of previous spectroscopic instruments for the detection of extremely low light levels. A two-fold enhancement will be offered by COS's near-ultraviolet channel. To install the COS instrument into the Hubble Space Telescope, he Servicing Mission 4 astronauts will remove the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument (installed during Servicing Mission 1 in 1993, to correct for Hubble's spherical aberration) and then install COS in its place. || ", "hits": 35 }, { "id": 10233, "url": "https://svs.gsfc.nasa.gov/10233/", "result_type": "Produced Video", "release_date": "2008-08-22T00:00:00-04:00", "title": "HST SM4 WFC3 Installation EVA", "description": "Wide Field Camera 3 (WFC3) will have a broad range of inquiry, from early and distant galaxies beyond Hubble's current reach, to more nearby galaxies with \"stories to tell\" about their star formation histories, to the planets in our solar system. Along the way, \"dark energy\" will be seriously probed by WFC3. The instrument's key feature is its ability to span the electromagnetic spectrum from the near ultraviolet through the optical (to which our eyes are sensitive), and into the near infrared. WFC3 is the only Hubble instrument with this \"panchromatic\" capability. WFC3's strengths complement those of the Advanced Camera for Surveys (ACS) should it be repaired. Working together these two instruments could create the greatest era in the spectacular history of Hubble imaging. The Servicing Mission 4 astronauts will remove the Wide Field Planetary Camera 2 (WFPC2) installed during Servicing Mission 1 in 1993 and install the WFC3 in its place. || ", "hits": 11 }, { "id": 10328, "url": "https://svs.gsfc.nasa.gov/10328/", "result_type": "Produced Video", "release_date": "2008-08-22T00:00:00-04:00", "title": "Fine Guidance Sensor Installation EVA Animation", "description": "Hubble uses three Fine Guidance Sensors for steady pointing and measurement. Astronauts will exchange one of these optical sensors with a refurbished unit that has enhanced, on-orbit alignment capability during Hubble Space Telescope Servicing Mission 4. || ", "hits": 11 }, { "id": 10330, "url": "https://svs.gsfc.nasa.gov/10330/", "result_type": "Produced Video", "release_date": "2008-08-22T00:00:00-04:00", "title": "New Outer Blanket Layer (NOBL) Installation EVA Animation", "description": "A NOBL consists of stainless steel panels covered with a protective Multi-Layer Insulation (MLI) thermal coating. These panels fit over existing, degraded insulation on Hubble's exterior surface, to control Hubble's internal temperature. The NOBL will be permanently mounted. || ", "hits": 40 }, { "id": 10321, "url": "https://svs.gsfc.nasa.gov/10321/", "result_type": "Produced Video", "release_date": "2008-08-01T00:00:00-04:00", "title": "HST SM4 Resource Reel v2.0", "description": "1. Hubble Space Telescope Service Mission 4 Animation: A collection of several animations showing the Hubble Space Telescope orbiting Earth and in space shuttle Atlantis cargo bay. All animations depict the Hubble Space Telescope in its current (July 2008) configuration. || 1-resource-hstsm4animation-resourcereelreference_MPEG-100852_print.jpg (1024x768) [98.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_web.png (320x240) [107.6 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_thm.png (80x40) [16.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_searchweb.png (320x180) [85.3 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.webmhd.webm (960x540) [12.8 MB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.mpg (320x240) [63.5 MB] || ", "hits": 31 }, { "id": 10318, "url": "https://svs.gsfc.nasa.gov/10318/", "result_type": "Produced Video", "release_date": "2008-07-26T00:00:00-04:00", "title": "HST SM4 Extended Resource Reel v2.0", "description": "Full HD Resource ReelThis resource reel includes all the clips shown below on this page. || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.00001_print.jpg (1024x576) [99.1 KB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.mov (1280x720) [57.2 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.mp4 (1280x720) [4.1 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.webm (1280x720) [454.7 MB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.webm [0 bytes] || ", "hits": 57 }, { "id": 40116, "url": "https://svs.gsfc.nasa.gov/gallery/jwst/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "James Webb Space Telescope", "description": "The James Webb Space Telescope (sometimes called JWST) is a large, infrared-optimized space telescope. The observatory launched into space on an Ariane 5 rocket from the Guiana Space Centre in Kourou, French Guiana on December 25, 2021. After launch, the observatory was successfully unfolded and is being readied for science. \n\nWebb will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy. Webb will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System. Webb's instruments are designed to work primarily in the infrared range of the electromagnetic spectrum, with some capability in the visible range.\n\nWebb has a large primary mirror, 6.5 meters (21.3 feet) in diameter and a sunshield the size of a tennis court. Both the mirror and sunshade are too large to fit onto the Ariane 5 rocket fully open, so both were folded which meant they needed to be unfolded in space. \n\nWebb is currently in its operational orbit about 1.5 million km (1 million miles) from the Earth at a location known as Lagrange Point 2 (L2).\n\nThe James Webb Space Telescope was named after the NASA Administrator who crafted the Apollo program, and who was a staunch supporter of space science.", "hits": 911 } ] }