{ "count": 97, "next": null, "previous": null, "results": [ { "id": 31381, "url": "https://svs.gsfc.nasa.gov/31381/", "result_type": "Hyperwall Visual", "release_date": "2026-03-31T11:51:59-04:00", "title": "NASA’S PUNCH Images Eruptions from the Sun", "description": "This video shows several coronal mass ejections (CMEs) erupting from the Sun’s surface from Oct. 21 to Nov. 12, 2025.", "hits": 1552 }, { "id": 14970, "url": "https://svs.gsfc.nasa.gov/14970/", "result_type": "Animation", "release_date": "2026-02-20T12:00:00-05:00", "title": "Roman Space Telescope Assembly Animation", "description": "This animation shows key systems assembling to form NASA's Nancy Grace Roman Space Telescope. It starts with the spacecraft bus and then adds the instrument carrier. Then the Coronagraph Instrument joins, followed by the mirror assembly and the Wide Field Instrument, completing the main half of the observatory. The outer portion, which contains the outer barrel assembly, solar array Sun shield, and deployable aperture cover, slides over the exposed mirror to complete the full observatory. This animation includes a version with a transparent alpha channel. || Roman_Assembly_Still.jpg (3840x2160) [377.3 KB] || Roman_Assembly_Still_searchweb.png (320x180) [18.8 KB] || Roman_Assembly_Still_thm.png (80x40) [2.3 KB] || Roman_Asssembly_1080.mp4 (1920x1080) [61.6 MB] || Roman_Asssembly_4k.mp4 (3840x2160) [308.1 MB] || Roman_Asssembly_ProRes_3840x2160_60.mov (3840x2160) [3.7 GB] || Roman_Asssembly_ProRes4444Alpha_3840x2160_60.mov (3840x2160) [7.1 GB] || ", "hits": 132 }, { "id": 14961, "url": "https://svs.gsfc.nasa.gov/14961/", "result_type": "Produced Video", "release_date": "2026-01-30T18:00:00-05:00", "title": "The Roman Space Telescope - Just Before Integration: Beauty Shots", "description": "The Roman Space Telescope team is preparing to join the two halves that will form the full observatory. Currently, Roman consists of the internal section, housing the mirror assembly and science instruments, and the outer portion, which includes the solar panels and deployable aperture cover.In this footage, team members inspect their work and take final looks before the mirror assembly disappears beneath the Outer Barrel Assembly. Once fully integrated, Roman will move on to its final environmental tests. || ", "hits": 160 }, { "id": 14891, "url": "https://svs.gsfc.nasa.gov/14891/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Roman and Webb's Overlapping Roles in Understanding Our Universe", "description": "The four Roman/Webb Far and Wide videos that detail the differences between the two missions, why we need both, what they will do and how they will work together.", "hits": 266 }, { "id": 5567, "url": "https://svs.gsfc.nasa.gov/5567/", "result_type": "Visualization", "release_date": "2025-07-21T18:59:59-04:00", "title": "New Missions to L1", "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.", "hits": 142 }, { "id": 14861, "url": "https://svs.gsfc.nasa.gov/14861/", "result_type": "Produced Video", "release_date": "2025-07-07T10:00:00-04:00", "title": "NASA's Habitable Worlds Observatory Will Search For Life", "description": "No description available.", "hits": 327 }, { "id": 31354, "url": "https://svs.gsfc.nasa.gov/31354/", "result_type": "Animation", "release_date": "2025-06-13T16:19:00-04:00", "title": "PUNCH", "description": "NASA’s PUNCH Releases Its First Images of Huge Eruptions from Sun", "hits": 182 }, { "id": 20400, "url": "https://svs.gsfc.nasa.gov/20400/", "result_type": "Animation", "release_date": "2025-04-07T00:00:00-04:00", "title": "Habitable Worlds Observatory Ultra-stable Telescope", "description": "HWO ultra stable animation || UltraStableTelescope_Prores.00877_print.jpg (1024x576) [74.6 KB] || UltraStableTelescope_Prores.00877_searchweb.png (320x180) [65.2 KB] || UltraStableTelescope_1080_h264.mov [59.2 MB] || UltraStableTelescope_Prores.00877_thm.png [4.3 KB] || UltraStableTelescope_UHD_h264.mov (3840x2160) [141.7 MB] || UltraStableTelescope_Prores.mov (3840x2160) [2.7 GB] ||", "hits": 142 }, { "id": 14788, "url": "https://svs.gsfc.nasa.gov/14788/", "result_type": "Produced Video", "release_date": "2025-03-03T00:00:00-05:00", "title": "Roman Vertical Video", "description": "This page collects all the vertically-formatted videos produced for the Nancy Grace Roman Space Telescope mission. ||", "hits": 133 }, { "id": 14779, "url": "https://svs.gsfc.nasa.gov/14779/", "result_type": "Produced Video", "release_date": "2025-02-11T09:00:00-05:00", "title": "NASA's Illuminate Series (2025)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 197 }, { "id": 14777, "url": "https://svs.gsfc.nasa.gov/14777/", "result_type": "Produced Video", "release_date": "2025-01-31T11:00:00-05:00", "title": "Coming Together : Roman's Internal Pieces are now Installed", "description": "NASA's Nancy Grace Roman Space Telescope is in the SCIPA configuation or the Spacecraft Integrated Payload Assembly. It includes the spacecraft bus, with all the support systems and electronics, the Wide Field Instrument, the Coronagraph Instrument, and the Optical Telescope Assembly, which is built around the 2.4 meter (7.9 foot) primary mirror. || ", "hits": 58 }, { "id": 14775, "url": "https://svs.gsfc.nasa.gov/14775/", "result_type": "Produced Video", "release_date": "2025-01-29T10:00:00-05:00", "title": "Roman Instrument Posters", "description": "NASA’s Roman Coronagraph Instrument will greatly advance our ability to directly image exoplanets, or planets and disks around other stars.Credit: NASA/JPLDigital version of poster with back panelPress version of poster with back panel. FOR PRINT || CGI_Digital_12x18.jpg (1837x2737) [1.1 MB] || CGI_Digital_12x18-1.jpg (3663x5475) [5.7 MB] || CGI_Digital_12x18-1.png (3663x5475) [39.5 MB] || ", "hits": 46 }, { "id": 14761, "url": "https://svs.gsfc.nasa.gov/14761/", "result_type": "Produced Video", "release_date": "2025-01-29T09:00:00-05:00", "title": "Roman Space Telescope's Instruments and Mirror attached to the Spacecraft Bus", "description": "NASA's Nancy Grace Roman Space Telescope is now in the formation of SCIPA (Spacecraft Integrated Payload Assembly). The footage captures the Integrated Payload Assembly, which contains the Mirror assembly, Instrument Carrier, and the two science instruments, the Wide Field Instrument and Coronagraph, along with the hexagonal Spacecraft bus, which houses electronics and the propulsion system. SCIPA includes all the primary internal parts of the telescope. This whole assembly will undergo further testing until integrated with the Outer Barrel assembly, deployable aperture cover, and solar panels. || ", "hits": 55 }, { "id": 14771, "url": "https://svs.gsfc.nasa.gov/14771/", "result_type": "Produced Video", "release_date": "2025-01-24T14:00:00-05:00", "title": "PUNCH Instruments", "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.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ", "hits": 85 }, { "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": 57 }, { "id": 14758, "url": "https://svs.gsfc.nasa.gov/14758/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman Space Telescope's Coronagraph Instrument Arrives to Goddard Space Flight Center", "description": "The first of two scientific instruments for NASA's Nancy Grace Roman Space Telescope has arrived to Goddard Space Flight Center.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": 53 }, { "id": 14760, "url": "https://svs.gsfc.nasa.gov/14760/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Mirror Assembly for Roman Space Telescope Arrives to NASA Goddard", "description": "This footage depicts the mirror assembly for the Nancy Grace Roman Space Telescope arriving at NASA's Goddard Space Flight Center. It is transported at night to accommodate the slow-moving specialized transport vehicle called the \"Chariot.\" Within hours of arriving, the lid of the Chariot was removed, and the lower portion was pushed into NASA's largest cleanroom for further unpacking.Designed and built by L3Harris Technologies in Rochester, New York, the assembly incorporates key optics (including the primary mirror) that were made available to NASA by the National Reconnaissance Office. The team at L3Harris then reshaped the mirror and built upon the inherited hardware to ensure it would meet Roman's specifications for expansive, sensitive infrared observations.Roman's primary mirror is 7.9 feet (2.4 meters) across. While it's the same size as the Hubble Space Telescope's main mirror, it is less than one-fourth the weight. Roman's mirror weighs only 410 pounds (186 kilograms) thanks to major improvements in technology.The newly resurfaced mirror sports a layer of silver less than 400 nanometers thick – about 200 times thinner than a human hair. The silver coating was specifically chosen for Roman because of how well it reflects near-infrared light. The primary mirror, in concert with other optics, will send light to Roman's two science instruments – the Wide Field Instrument and Coronagraph Instrument. The first is essentially a giant 300-megapixel camera that provides the same sharp resolution as Hubble across nearly 100 times the field of view. Using this instrument, scientists will be able to map the structure and distribution of invisible dark matter, study planetary systems around other stars, and explore how the universe evolved to its present state. || ", "hits": 27 }, { "id": 14746, "url": "https://svs.gsfc.nasa.gov/14746/", "result_type": "Produced Video", "release_date": "2025-01-14T13:00:00-05:00", "title": "Roman SCIPA Hyperwall Time-lapse", "description": "This 3x3-hyperwall-resolution time-lapse video of Roman shows the major integration steps of the key systems to form SCIPA, or the Spacecraft Integrated Payload Assembly. It includes the spacecraft bus, with all the support systems and electronics, the Wide Field Instrument, the Coronagraph Instrument, and the Optical Telescope Assembly, which is built around the 2.4 meter (7.9 foot) primary mirror. This sequence does not have sound and is available as video and frames.Credit: NASA's Goddard Space Flight Center || Roman_SCIPA_TL_Still.jpg (5760x3240) [8.6 MB] || Roman_SCIPA_TL_Still_searchweb.png (320x180) [126.8 KB] || Roman_SCIPA_TL_Still_thm.png [8.3 KB] || 5760x3240_16x9_30p (5760x3240) [17806 Item(s)] || Roman_SCIPA_TL_Still.jpg.dzi [178 bytes] || Roman_SCIPA_TL_Still.jpg_files [4.0 KB] || Roman_SCIPA_Time-lapse_D4.mp4 (5760x3240) [1.4 GB] || ", "hits": 58 }, { "id": 20394, "url": "https://svs.gsfc.nasa.gov/20394/", "result_type": "Animation", "release_date": "2024-11-12T15:00:00-05:00", "title": "Habitable Worlds Observatory (HWO) Animations and Stills", "description": "This page contains artist's concept computer renderings of a current possible design for the Habitable Worlds Observatory. HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ", "hits": 221 }, { "id": 20392, "url": "https://svs.gsfc.nasa.gov/20392/", "result_type": "Animation", "release_date": "2024-11-12T14:00:00-05:00", "title": "Space Weather and NOAA's Space Weather Follow On at Lagrange point 1 (SWFO-L1)", "description": "NOAA and Impacts of Space Weather || SWFO_0924_2MinVer_HD_v02.01800_print.jpg (1024x576) [187.1 KB] || SWFO_0924_2MinVer_HD_v02.01800_searchweb.png (180x320) [89.8 KB] || SWFO_0924_2MinVer_HD_v02.01800_thm.png (80x40) [6.3 KB] || SWFO_0924_2MinVer_FHD_v02.mp4 (1920x1080) [159.2 MB] || SWFO_0924_2MinVer_HD_v02.mp4 (1280x720) [157.5 MB] || SWFO_0924_2MinVer_SD_v02.mp4 (852x480) [156.8 MB] || SWFO_0924_2MinVer_4k_v02.mp4 (3840x2160) [231.9 MB] || SWFO_0924_2MinVer_4k_v02.mov (3840x2160) [15.8 GB] || ", "hits": 122 }, { "id": 14714, "url": "https://svs.gsfc.nasa.gov/14714/", "result_type": "B-Roll", "release_date": "2024-11-06T10:00:00-05:00", "title": "CODEX Heads to the Space Station for Install", "description": "On Nov. 4, 2024, the Coronal Diagnostic Experiment (CODEX) launched to space aboard NASA’s SpaceX CRS-31 – a commercial resupply mission of an uncrewed Dragon spacecraft headed for the International Space Station. Liftoff occurred at 9:29 p.m. EST.CODEX is a solar coronagraph that will be installed on the Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun’s outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contributions from Italy’s National Institute for Astrophysics (INAF).To learn more about the experiment, visit: https://science.nasa.gov/mission/codex/ || ", "hits": 75 }, { "id": 14693, "url": "https://svs.gsfc.nasa.gov/14693/", "result_type": "Produced Video", "release_date": "2024-10-02T12:00:00-04:00", "title": "NASA's Nancy Grace Roman Space Telescope: Systems, Assemble!", "description": "In September 2024, the Nancy Grace Roman Space Telescope passed a key milestone and was approved for the next stage of construction. Work on the main systems that will make up the final spacecraft is finishing, and the team at NASA’s Goddard Space Flight Center is ready to begin integration, the process of connecting them together. This video celebrates the effort to reach the final stages of assembly.Music: “The Call,” Torsti Juhani Spoof [BMI] Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Building_Roman_Main2.jpg (1280x720) [451.7 KB] || YTframe_Building_Roman_Main2_searchweb.png (320x180) [124.6 KB] || YTframe_Building_Roman_Main2_thm.png (80x40) [11.0 KB] || 14693_RomanSystemsAssemble_Good.mp4 (1920x1080) [234.1 MB] || 14693_RomanSystemsAssemble_Better.mp4 (1920x1080) [444.0 MB] || 14693RomanSystemsAssembleCaptions.en_US.srt [491 bytes] || 14693RomanSystemsAssembleCaptions.en_US.vtt [475 bytes] || 14693_RomanSystemsAssemble_YouTube.mp4 (1920x1080) [1012.1 MB] || 14693_RomanSystemsAssemble_ProRes1920x1080_2997.mov (1920x1080) [2.8 GB] || 14693_RomanSystemsAssemble_Better.hwshow [508 bytes] || ", "hits": 62 }, { "id": 40525, "url": "https://svs.gsfc.nasa.gov/gallery/habitable-worlds-observatory/", "result_type": "Gallery", "release_date": "2024-10-01T00:00:00-04:00", "title": "Habitable Worlds Observatory", "description": "The Habitable Worlds Observatory is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.\n\nHabitable Worlds will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.\n\nThis future space observatory will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter and the evolution of cosmic structure.\n\nThe Habitable Worlds Observatory will build on the technological foundations of the Hubble, Webb and Roman Space Telescopes, uniting government, industry, academia, and international partners.", "hits": 252 }, { "id": 14647, "url": "https://svs.gsfc.nasa.gov/14647/", "result_type": "B-Roll", "release_date": "2024-08-12T13:00:00-04:00", "title": "CODEX – Coronal Diagnostic Experiment", "description": "The Coronal Diagnostic Experiment (CODEX) is a solar coronagraph that will be installed on the International Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contribution from Italy's National Institute for Astrophysics (INAF).Learn more: https://science.nasa.gov/mission/codex/ || ", "hits": 82 }, { "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": 44 }, { "id": 14601, "url": "https://svs.gsfc.nasa.gov/14601/", "result_type": "Produced Video", "release_date": "2024-06-13T13:00:00-04:00", "title": "From GOES to GeoXO: Past Highlights to Future Horizons", "description": "When NOAA’s GOES-U satellite is launched in June of 2024, it will be the final satellite in a heralded NOAA satellite program and bridge to another future age of advanced satellite technology. For nearly 50 years, NOAA and NASA have partnered to develop and advance NOAA’s geostationary satellites as part of the most sophisticated weather-observing, environmental monitoring, and space weather monitoring satellite system in the world.The first GOES satellite, GOES-1 (SMS-3), was launched in October of 1975. As groundbreaking as it was, it had limited capabilities and viewed Earth only about ten percent of the time. Each generation since the launch of GOES-1 has improved significantly, bringing with new capabilities and instruments. The most recent, and last generation is the GOES-R series that first launched in 2016 with GOES-R or GOES-16. This series came with new instruments such as the Geostationary Lightning Mapper (GLM) and the Advanced Baseline Imager (ABI). GOES-U, the final satellite of the series, also has the Compact Coronagraph-1 (CCOR-1) to monitor the Sun’s corona.After GOES-U launches, its successor will be a series called Geostationary Extended Observations, or GeoXO. The first satellite in the series is expected to launch in the early 2030s. GeoXO will continue NOAA’s five decades of critical Earth-observing data. To learn more about GeoXO and its new state-of-the-art instruments, follow this link. || ", "hits": 48 }, { "id": 14573, "url": "https://svs.gsfc.nasa.gov/14573/", "result_type": "Produced Video", "release_date": "2024-04-25T10:00:00-04:00", "title": "Nancy Grace Roman Space Telescope Reaction Wheel and Thruster Animations", "description": "Beauty pass of Roman, coming over the top of the solar panels.Credit: NASA's Goddard Space Flight Center/CI Lab || RST_Beauty_S1_4K_60_ProRes.00458_print.jpg (1024x576) [164.9 KB] || RST_Beauty_S1_1080.mp4 [19.0 MB] || RST_Beauty_S1_4K_60.mp4 [92.2 MB] || RST_Beauty_S1_4K_60_ProRes.webm [10.4 MB] || RST_Beauty_S1_4K_60_ProRes.mov [2.0 GB] || ", "hits": 73 }, { "id": 14491, "url": "https://svs.gsfc.nasa.gov/14491/", "result_type": "Produced Video", "release_date": "2023-12-26T00:00:00-05:00", "title": "Roman Hardware Highlights", "description": "This video, covering the second half of 2025, opens with a person entering NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.The outside half of Roman, called OSD, contains the solar panels and protective layers. The Deployable Aperture Cover, which protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space. Then the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool.In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right, and forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as they anticipated.While these tests occur, Roman’s inside half, containing the mirrors, instruments and support equipment, move into Goddard’s largest thermal vacuum chamber, the SES (Space Environment Simulator). This 40-foot-tall chamber can simulate the vacuum of space and the wide temperature range that Roman will experience there: from -310° Fahrenheit (-190° C) to 302° Fahrenheit (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned both horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.Music credit: “Our Journey Begins,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_SummerFall2025_3.jpg (1280x720) [473.7 KB] || Roman_HH_Summer-Fall2025_10mbps.mp4 (1920x1080) [185.0 MB] || Roman_HH_Summer-Fall2025_25mbps.mp4 (1920x1080) [452.7 MB] || Roman_HH_Summer-Fall2025_YT.mp4 (1920x1080) [880.2 MB] || RomanHHLate2025Captions.en_US.srt [588 bytes] || RomanHHLate2025Captions.en_US.vtt [570 bytes] || Roman_HH_Summer-Fall2025_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || ", "hits": 205 }, { "id": 14422, "url": "https://svs.gsfc.nasa.gov/14422/", "result_type": "Produced Video", "release_date": "2023-10-06T00:00:00-04:00", "title": "Roman's Instrument Carrier Arrives", "description": "The Nancy Grace Roman Space Telescope's Instrument Carrier arrives at NASA's Goddard Space Flight Center. The workers remove the grid-like structure from the truck container that brought it and move it into a clean tent. Once there, engineers remove the protective wrapping and inspect the carbon fiber struts. The Instrument Carrier sits between the primary mirror and spacecraft bus and will hold Roman's Wide Field Instrument and Coronagraph technology demonstration.Music: \"Knowledge and Process\" from Universal Production MusicComplete transcript available. || Roman_Instrument_Carrier.jpg (1849x1004) [426.6 KB] || Roman_Instrument_Carrier_searchweb.png (320x180) [105.1 KB] || Roman_Instrument_Carrier_thm.png (80x40) [10.6 KB] || Roman_Instrument_Carrier_Arrival_Good.webm (1920x1080) [13.2 MB] || Roman_Instrument_Carrier_Arrival_Good.mp4 (1920x1080) [105.1 MB] || Roman_Instrument_Carrier_Arrival_Best.mp4 (1920x1080) [257.6 MB] || Roman_Instrument_Carrier_Arrival_Captions.en_US.srt [894 bytes] || Roman_Instrument_Carrier_Arrival_Captions.en_US.vtt [907 bytes] || Roman_Instrument_Carrier_Arrival_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 35 }, { "id": 40455, "url": "https://svs.gsfc.nasa.gov/gallery/spacecraft-animations/", "result_type": "Gallery", "release_date": "2023-01-24T00:00:00-05:00", "title": "Satellite Animations", "description": "A collection of spacecraft beauty pass animations for current missions.", "hits": 265 }, { "id": 14194, "url": "https://svs.gsfc.nasa.gov/14194/", "result_type": "Produced Video", "release_date": "2022-08-12T00:00:00-04:00", "title": "Roman Interactive Promo", "description": "Short promotional video for the Nancy Grace Roman Interactive.Music: \"Braniacs and Machines\" from Universal Production Music.Complete transcript available. || Interactive_zoom_STILL.jpg (1920x1080) [302.4 KB] || Interactive_zoom_STILL_searchweb.png (320x180) [85.1 KB] || Interactive_zoom_STILL_thm.png (80x40) [7.4 KB] || Interactive_Teaser_V3.mp4 (1920x1080) [33.5 MB] || Interactive_Teaser_V3.webm (1920x1080) [2.2 MB] || Roman_Interactive_Teaser_ProRes_1920x1080_24.mov (1920x1080) [252.7 MB] || Interactive_Teaser_SRT_Captions.en_US.srt [246 bytes] || Interactive_Teaser_SRT_Captions.en_US.vtt [259 bytes] || ", "hits": 61 }, { "id": 14181, "url": "https://svs.gsfc.nasa.gov/14181/", "result_type": "Produced Video", "release_date": "2022-08-04T13:00:00-04:00", "title": "Roman Interactive Stills", "description": "Right-side view of the Roman Space Telescope. Highlighted parts available under \"Download Options\" || ROMAN_interactive_Spacecraft_V009_R_Off_2080_print.jpg (1024x576) [57.5 KB] || ROMAN_interactive_V009_R_Roman_off_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080.png (2080x1170) [751.5 KB] || ROMAN_interactive_V009_R_Roman_on_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_V009_R_Roman_comms_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Comms_2080.png (2080x1170) [771.3 KB] || ROMAN_interactive_V009_R_Roman_support_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Support_2080.png (2080x1170) [768.7 KB] || ROMAN_interactive_V009_R_Roman_tele_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_Tele_2080.png (2080x1170) [776.8 KB] || ROMAN_interactive_V009_R_Roman_SP_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_SP_2080.png (2080x1170) [786.4 KB] || ROMAN_interactive_V009_R_Roman_WFI_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_WFI_2080.png (2080x1170) [772.1 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_searchweb.png (320x180) [26.4 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_thm.png (80x40) [3.0 KB] || ", "hits": 43 }, { "id": 14172, "url": "https://svs.gsfc.nasa.gov/14172/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Dominic Benford 2022 AAS Roman Hyperwall Talk", "description": "Static title card.Credit: NASA's Goddard Space Flight Center || dominic_benford_roman_title_slide_print.jpg (1024x576) [262.4 KB] || dominic_benford_roman_title_slide.png (3840x2160) [10.2 MB] || dominic_benford_roman_title_slide_searchweb.png (320x180) [113.1 KB] || dominic_benford_roman_title_slide_thm.png (80x40) [7.9 KB] || ", "hits": 25 }, { "id": 14174, "url": "https://svs.gsfc.nasa.gov/14174/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Rebekah Hounsell 2022 AAS Roman Hyperwall Talk", "description": "Title slide.Credit: NASA's Goddard Space Flight Center || rebekah_hounsell_roman_title_print.jpg (1024x576) [250.4 KB] || rebekah_hounsell_roman_title.png (3840x2160) [10.3 MB] || rebekah_hounsell_roman_title_searchweb.png (320x180) [111.8 KB] || rebekah_hounsell_roman_title_thm.png (80x40) [8.1 KB] || ", "hits": 44 }, { "id": 14175, "url": "https://svs.gsfc.nasa.gov/14175/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Expanding Our View (2022 STScI presentation)", "description": "Complete PowerPoint file with all slides and notes || PPT_still.jpg (3840x2160) [750.6 KB] || roman-expanding-our-view-presentation.pptx [76.2 MB] || Slide #1 – Onscreen before presentation begins and during introductionCredit: STScI, NASA || Slide1_print.jpg (1024x576) [98.1 KB] || Slide1.png (3840x2160) [3.4 MB] || Slide1.jpg (3840x2160) [750.6 KB] || Slide1_searchweb.png (320x180) [63.9 KB] || Slide1_thm.png (80x40) [5.6 KB] || ", "hits": 57 }, { "id": 13775, "url": "https://svs.gsfc.nasa.gov/13775/", "result_type": "Produced Video", "release_date": "2020-12-02T11:00:00-05:00", "title": "25 Years of Sun from ESA/NASA's SOHO", "description": "December 2, 1995 marks the 25th anniversary of the Solar and Heliospheric Observatory, or SOHO — a joint mission of the European Space Agency and NASA. Since its launch on that date, the mission has kept watch on the Sun. || ", "hits": 99 }, { "id": 13664, "url": "https://svs.gsfc.nasa.gov/13664/", "result_type": "Produced Video", "release_date": "2020-07-16T08:00:00-04:00", "title": "ESA and NASA Release First Images From Solar Orbiter Mission", "description": "Scientists from ESA (European Space Agency) and NASA will present the first images captured by Solar Orbiter, the joint ESA/NASA mission to study the Sun, during an online news briefing at 8 a.m. EDT Thursday, July 16. Launched on Feb. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun. The flyby captured the closest images ever taken of the Sun. During the briefing, mission experts will discuss what these closeup images reveal about our star, including what we can learn from Solar Orbiter’s new measurements of particles and magnetic fields flowing from the Sun.The briefing will stream live at:https://www.nasa.gov/solarorbiterfirstlight/Participants in the call include:•Daniel Müller – Solar Orbiter Project Scientist at ESA•Holly R. Gilbert – Solar Orbiter Project Scientist at NASA•José Luis Pellón Bailón – Solar Orbiter Deputy Spacecraft Operations Manager at ESA•David Berghmans – Principal investigator of the Extreme Ultraviolet Imager (EUI) at the Royal Observatory of Belgium•Sami Solanki – Principal investigator of the Polarimetric and Helioseismic Imager (PHI) and director of the Max Planck Institute for Solar System Research•Christopher J. Owen – Principal investigator of the Solar Wind Analyser (SWA) at Mullard Space Science Laboratory, University College London•ESA’s first light images•ESA press release •NASA feature story || ", "hits": 197 }, { "id": 13661, "url": "https://svs.gsfc.nasa.gov/13661/", "result_type": "Produced Video", "release_date": "2020-07-10T09:50:00-04:00", "title": "NASA Missions Spot Comet NEOWISE", "description": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO || wide.00250_print.jpg (1024x576) [164.4 KB] || wide.mp4 (3840x2160) [72.2 MB] || wide.webm (3840x2160) [6.2 MB] || ", "hits": 78 }, { "id": 13623, "url": "https://svs.gsfc.nasa.gov/13623/", "result_type": "Produced Video", "release_date": "2020-06-17T10:00:00-04:00", "title": "Four of Our Favorite SOHO-discovered Comets", "description": "Karl Battams, manager of NASA's citizen science Sungrazer Project, talks about his four favorite comets that SOHO has observed.Music: \"Inducing Waves\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_print.jpg (1024x576) [155.4 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_searchweb.png (320x180) [72.1 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_thm.png (80x40) [5.3 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.mov (1920x1080) [3.1 GB] || 13623_SOHO4FavoriteComets_1080.mp4 (1920x1080) [245.9 MB] || 13623_SOHO4FavoriteComets_Good_1080.mp4 (1920x1080) [128.8 MB] || 13623_SOHO4FavoriteComets_1080.webm (1920x1080) [27.2 MB] || SOHO_4000Comets_SRT_Captions.en_US.srt [4.8 KB] || SOHO_4000Comets_SRT_Captions.en_US.vtt [4.8 KB] || ", "hits": 76 }, { "id": 13325, "url": "https://svs.gsfc.nasa.gov/13325/", "result_type": "Produced Video", "release_date": "2019-09-24T13:00:00-04:00", "title": "The Nancy Grace Roman Space Telescope's Coronagraph Instrument", "description": "Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.Credit: NASA's Goddard Space Flight CenterMusic: \"Concept of Motion\" from Universe Production MusicComplete transcript available. || Roman_CGI_Still.jpg (1920x1080) [396.1 KB] || 13325_Roman_CGI_1080.mp4 (1920x1080) [96.8 MB] || 13325_Roman_CGI_Final_ProRes_1920x1080_2997.mov (1920x1080) [1.3 GB] || 13325_Roman_CGI_1080.webm (1920x1080) [13.9 MB] || Roman_CGI_SRT_Captions.en_US.srt [2.4 KB] || Roman_CGI_SRT_Captions.en_US.vtt [2.4 KB] || ", "hits": 139 }, { "id": 13296, "url": "https://svs.gsfc.nasa.gov/13296/", "result_type": "Produced Video", "release_date": "2019-09-02T00:00:00-04:00", "title": "Nancy Grace Roman Space Telescope 360 spacecraft animations PDR version", "description": "Animated 3D model of the Roman Space Telescope spacecraft rotated through 360 degrees in a neutral gray environment.Credit: NASA's Goddard Space Flight Center/CI Lab || WFIRST_TurntableRev01ProRes_3840x2160.00001_print.jpg (1024x576) [57.3 KB] || WFIRST_TurntableRev01ProRes_3840x2160.00001_searchweb.png (320x180) [44.6 KB] || WFIRST_TurntableRev01ProRes_3840x2160.00001_thm.png (80x40) [4.0 KB] || WFIRST_TurntableRev01_1080.mp4 (1920x1080) [36.9 MB] || WFIRST_TurntableRev01_1080.webm (1920x1080) [2.3 MB] || WFIRST_TurntableRev01_4k.mp4 (3840x2160) [133.0 MB] || WFIRST_TurntableRev01ProRes_3840x2160.mov (3840x2160) [1.1 GB] || ", "hits": 42 }, { "id": 13295, "url": "https://svs.gsfc.nasa.gov/13295/", "result_type": "Produced Video", "release_date": "2019-08-28T10:00:00-04:00", "title": "Take a Spin With NASA's Nancy Grace Roman Space Telescope", "description": "Learn more about the Roman Space Telescope spacecraft with this short tour of the main systems.Music: “Phenomenon\" from Above and Below Written and produced by Lars LeonhardCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Spacecraft_360STILL_1.jpg (1920x1080) [272.4 KB] || 13295_Roman_360_1080.mp4 (1920x1080) [219.9 MB] || 13295_Roman_360_Best_1080.mp4 (1920x1080) [807.1 MB] || 13295_Roman_360_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || 13295_Roman_360_1080.webm (1920x1080) [24.0 MB] || Roman_360_SRT_Captions.en_US.srt [4.3 KB] || Roman_360_SRT_Captions.en_US.vtt [4.3 KB] || ", "hits": 64 }, { "id": 13291, "url": "https://svs.gsfc.nasa.gov/13291/", "result_type": "Produced Video", "release_date": "2019-08-23T11:30:00-04:00", "title": "NASA’s New Solar Scope Is Ready For Balloon Flight", "description": "NASA and the Korea Astronomy and Space Science Institute, or KASI, are getting ready to test a new way to see the Sun, high over the New Mexico desert. A pearlescent balloon — large enough to hug a football field — is scheduled to take flight no earlier than Aug. 26, 2019, carrying beneath it a solar scope called BITSE. BITSE is a coronagraph, a kind of telescope that blocks the Sun’s bright face in order to reveal its dimmer atmosphere, called the corona. Short for Balloon-borne Investigation of Temperature and Speed of Electrons in the corona, BITSE seeks to explain how the Sun spits out the solar wind. || ", "hits": 40 }, { "id": 13235, "url": "https://svs.gsfc.nasa.gov/13235/", "result_type": "Produced Video", "release_date": "2019-06-26T09:50:00-04:00", "title": "NASA's Nancy Grace Roman Space Telescope's Wide Field Instrument", "description": "The Nancy Grace Roman Space Telescope is a next-generation space telescope that will survey the infrared universe from beyond the orbit of the Moon. The spacecraft's giant camera, the Wide Field Instrument (WFI), will be fundamental to this exploration. The WFI features the same angular resolution as Hubble but with 100 times the field of view. Data it gathers will enable scientists to discover new and uniquely detailed information about planetary systems around other stars. The WFI will also map how matter is structured and distributed throughout the cosmos, which should ultimately allow scientists to discover the fate of the universe. Watch this video to see a simplified version of how it works.Credit: NASA's Goddard Space Flight Center.Music\" \"Horizon Ahead\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || RomanWide_Field_Still.jpg (3840x2160) [827.1 KB] || 13235_WFI_Roman_1080.mp4 (1920x1080) [92.9 MB] || 13235_WFI_Roman_Best_1080.mp4 (1920x1080) [272.1 MB] || 13235_WFI_Roman_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || 13235_WFI_Roman_1080.webm (1920x1080) [13.2 MB] || WFI_Roman_SRT_Captions.en_US.srt [2.5 KB] || WFI_Roman_SRT_Captions.en_US.vtt [2.5 KB] || ", "hits": 71 }, { "id": 12927, "url": "https://svs.gsfc.nasa.gov/12927/", "result_type": "Produced Video", "release_date": "2018-04-16T12:00:00-04:00", "title": "Looking at the Corona with WISPR on Parker Solar Probe", "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere) and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun. || ", "hits": 128 }, { "id": 12804, "url": "https://svs.gsfc.nasa.gov/12804/", "result_type": "Produced Video", "release_date": "2018-03-15T07:00:00-04:00", "title": "SEEC AAS Hyperwall Presentation January 2018", "description": "This animation illustrates the Kepler-186 system, whose fifth world is the first Earth-sized exoplanet to be found orbiting within its star’s habitable zone. The animation closes with a simulated image from a coronagraph showing how such a planet might appear when directly imaged.Credit: NASA/Ames/SETI Institute/JPL-Caltech || Kepler186_Coronagraph_Combined_LongPause.01270_print.jpg (1024x576) [35.2 KB] || Kepler186_Coronagraph_Combined_LongPause.webm (1920x1080) [14.0 MB] || Kepler186_Coronagraph_Combined_LongPause.mov (1920x1080) [180.7 MB] || ", "hits": 28 }, { "id": 12805, "url": "https://svs.gsfc.nasa.gov/12805/", "result_type": "Produced Video", "release_date": "2018-01-07T00:00:00-05:00", "title": "TESS AAS Hyperwall Presentation January 2018", "description": "Venus transits the Sun on June 5, 2012 as observed by the Solar Dynamics Observatory in 171 Angstrom light.Credit: NASA/SDO || Venus_Transit_SDO_1080.00049_print.jpg (1024x576) [158.1 KB] || Venus_Transit_SDO_1080.mov (1920x1080) [62.9 MB] || Venus_Transit_SDO_1080.webm (1920x1080) [1.0 MB] || ", "hits": 34 }, { "id": 12238, "url": "https://svs.gsfc.nasa.gov/12238/", "result_type": "Produced Video", "release_date": "2017-12-22T13:00:00-05:00", "title": "WFIRST Will See the Big Picture of the Universe", "description": "Learn about the Wide Field Infrared Survey Telescope (WFIRST) mission.Music: \"We Dissolve in Stars\" and \"Climb the Ladder\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WFIRST_Beauty_still_print.jpg (1024x576) [97.2 KB] || WFIRST_Beauty_still.png (3840x2160) [36.5 MB] || WFIRST_Beauty_still.jpg (3840x2160) [988.6 KB] || WFIRST_Beauty_still_searchweb.png (320x180) [72.0 KB] || WFIRST_Beauty_still_thm.png (80x40) [5.1 KB] || YOUTUBE_1080_12238_WFIRST_Overview_V3_FINAL.mp4 (1920x1080) [845.8 MB] || 12238_WFIRST_Overview_V3_H264_1080p.mov (1920x1080) [759.1 MB] || 12238_WFIRST_Overview_V3_H264_1080_2997.m4v (1920x1080) [377.3 MB] || 12238_WFIRST_Overview_V3_H264_1080p.webm (1920x1080) [41.2 MB] || 12238_WFIRST_Overview_V3_ProRes_3840x2160_2997.mov (3840x2160) [19.3 GB] || YOUTUBE_HQ_12238_WFIRST_Overview_V3_FINAL_4k.mov (3840x2160) [6.5 GB] || 12238_WFIRST_Overview_V3_H264_4K.mov (3840x2160) [1.1 GB] || WFIRST_overview_SRT_Captions.en_US.srt [6.7 KB] || WFIRST_overview_SRT_Captions.en_US.vtt [6.4 KB] || ", "hits": 80 }, { "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": 134 }, { "id": 12687, "url": "https://svs.gsfc.nasa.gov/12687/", "result_type": "Produced Video", "release_date": "2017-08-15T12:00:00-04:00", "title": "NASA and ESA Spacecraft Track a Solar Storm Through Space", "description": "This animation follows the October 14, 2014 CME as it moves through the solar system and identifies a few of the NASA and ESA missions that observed it.Music: “Comely\" from FelicityWritten and produced by Lars LeonhardWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || CME_Solar_System_Still.jpg (3840x2160) [555.5 KB] || CME_Solar_System_Still_searchweb.png (320x180) [38.4 KB] || CME_Solar_System_Still_thm.png (80x40) [4.0 KB] || 12687_CME_Solar_System_1080p.mov (1920x1080) [90.8 MB] || 12687_CME_Solar_System_FINAL_appletv.m4v (1280x720) [71.7 MB] || 12687_CME_Solar_System_1080p.webm (1920x1080) [10.4 MB] || 12687_CME_Solar_System_FINAL_appletv_subtitles.m4v (1280x720) [71.7 MB] || FACEBOOK_720_12687_CME_Solar_System_FINAL_facebook_720.mp4 (1280x720) [158.9 MB] || 12687_CME_Solar_System_SRT_Captions.en_US.srt [1.2 KB] || 12687_CME_Solar_System_SRT_Captions.en_US.vtt [1.2 KB] || 12687_CME_Solar_System_-4K.mov (3840x2160) [287.7 MB] || 12687_CME_Solar_System_Apple_Devices_4K.m4v (3840x2160) [340.2 MB] || YOUTUBE_4K_12687_CME_Solar_System_FINAL_youtube_4k.mp4 (3840x2160) [627.2 MB] || 12687_CME_Solar_System_ProRes_3840x2160_2997.mov (3840x2160) [2.5 GB] || ", "hits": 82 }, { "id": 12636, "url": "https://svs.gsfc.nasa.gov/12636/", "result_type": "Produced Video", "release_date": "2017-08-07T00:00:00-04:00", "title": "2 Minutes, 6 Hands, 1 Chance", "description": "Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: Patisserie Pressure by Benjamin James Parsons || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_print.jpg (1024x576) [159.7 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_searchweb.png (320x180) [112.1 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_thm.png (80x40) [7.9 KB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.webm (1920x1080) [16.4 MB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv_subtitles.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.mp4 (1920x1080) [152.5 MB] || YOUTUBE_1080-12636_2Minutes6Hands1ChanceV6_youtube_1080.mp4 (1920x1080) [244.6 MB] || NASA_TV-12636_2Minutes6Hands1ChanceV6.mpeg (1280x720) [507.3 MB] || YOUTUBE_HQ-12636_2Minutes6Hands1ChanceV6_youtube_hq.mov (1920x1080) [672.4 MB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.srt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.vtt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.mp4 (320x240) [26.4 MB] || PRORES_B-ROLL-12636_2Minutes6Hands1ChanceV6_prores.mov (1280x720) [2.1 GB] || 12636_2Minutes6Hands1ChanceV6.mov (1920x1080) [4.0 GB] || ", "hits": 26 }, { "id": 12451, "url": "https://svs.gsfc.nasa.gov/12451/", "result_type": "Produced Video", "release_date": "2017-01-30T11:30:00-05:00", "title": "Fermi Sees Gamma Rays from Far Side Solar Flares", "description": "On three occasions, NASA's Fermi Gamma-ray Space Telescope has detected gamma rays from solar storms on the far side of the sun, emission the Earth-orbiting satellite shouldn't be able to detect. Particles accelerated by these eruptions somehow reach around to produce a gamma-ray glow on the side of the sun facing Earth and Fermi. Watch to learn more. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available.This illustration shows large magnetic structures extending high above the sun from the active region hosting the Sept. 1, 2014, solar blast. Left: Scientists think particles accelerated at the leading edge of the event's coronal mass ejection followed magnetic lines high above the sun. Right: Some of the particles followed similar magnetic structures rooted in the Earth-facing side of the sun. They rained down on the sun and interacted with the solar surface, producing gamma rays (magenta). The solar images shown here come from (left) STEREO B and (right) NASA's Solar Dynamics Observatory. Credit: NASA/STEREO and NASA/SDO || STEREO-SDO_Fermi_Still.jpg (1920x1080) [433.9 KB] || STEREO-SDO_Fermi_Still_searchweb.png (320x180) [101.1 KB] || STEREO-SDO_Fermi_Still_thm.png (80x40) [7.7 KB] || 12451_Fermi_Farside_Flares_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || 12451_Fermi_Farside_Flares_FINAL_youtube_hq.mov (1920x1080) [1.2 GB] || 12451_Fermi_Farside_Flares-H264_1080.mov (1920x1080) [286.5 MB] || 12451_Fermi_Farside_Flares-H264_Good_1080.m4v (1920x1080) [190.5 MB] || 12451_Fermi_Farside_Flares_FINAL_appletv.m4v (1280x720) [100.4 MB] || 12451_Fermi_Farside_Flares-H264_Compatible.m4v (960x540) [74.4 MB] || 12451_Fermi_Farside_Flares_FINAL_appletv_subtitles.m4v (1280x720) [100.5 MB] || 12451_Fermi_Farside_Flares-H264_Compatible.webm (960x540) [20.5 MB] || 12451_Fermi_Farside_Flares_SRT_Captions.en_US.srt [3.3 KB] || 12451_Fermi_Farside_Flares_SRT_Captions.en_US.vtt [3.3 KB] || ", "hits": 71 }, { "id": 12417, "url": "https://svs.gsfc.nasa.gov/12417/", "result_type": "Produced Video", "release_date": "2017-01-13T13:00:00-05:00", "title": "WFIRST 2017 AAS Hyperwall Presentation", "description": "New hyperwall resources for Neil Gehrels' 2017 AAS talk. Most visuals are 5760x3240 and designed for a 3x3 hyperwall with 1920x1080 screens. || ", "hits": 45 }, { "id": 12308, "url": "https://svs.gsfc.nasa.gov/12308/", "result_type": "Produced Video", "release_date": "2016-09-20T14:00:00-04:00", "title": "Hubble vs Roman Space Telescope Image Size Comparisons", "description": "The Nancy Grace Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics. The telescope has a primary mirror that is 2.4 meters in diameter (7.9 feet), and is the same size as the Hubble Space Telescope's primary mirror. The Roman Space Telescope will have two instruments, the Wide Field Instrument, and the Coronagraph Instrument.The Wide Field Instrument will have a field of view that is 100 times greater than the Hubble infrared instrument, capturing more of the sky with less observing time. As the primary instrument, the Wide Field Instrument will measure light from a billion galaxies over the course of the mission lifetime. It will perform a microlensing survey of the inner Milky Way to find ~2,600 exoplanets. || ", "hits": 146 }, { "id": 20243, "url": "https://svs.gsfc.nasa.gov/20243/", "result_type": "Animation", "release_date": "2016-09-20T14:00:00-04:00", "title": "Roman Space Telescope Coronagraph Animation", "description": "Animation illustrating how a planet can disappear in a star's bright light, and how a coronagraph can reveal it. || Coronagraph_Still_print.jpg (1024x576) [23.5 KB] || Coronagraph_Still.png (3840x2160) [4.8 MB] || Coronagraph_Still_searchweb.png (320x180) [32.9 KB] || Coronagraph_Still_thm.png (80x40) [3.2 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.mov (1920x1080) [28.1 MB] || 3840x2160_16x9_60p (3840x2160) [128.0 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_4K.mov (3840x2160) [47.0 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.webm (3840x2160) [3.3 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.key [29.9 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.pptx [29.6 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.mov (3840x2160) [2.4 GB] || ", "hits": 92 }, { "id": 20247, "url": "https://svs.gsfc.nasa.gov/20247/", "result_type": "Animation", "release_date": "2016-09-20T14:00:00-04:00", "title": "WFIRST MCR Spacecraft Animations", "description": "Articulated spin of spacecraft in \"warehouse\" setting with human silhouette for scale. || WFIRST_Turnaround_fr_01799.png (1920x1080) [3.1 MB] || WFIRST_Turnaround_fr_01799_print.jpg (1024x576) [84.1 KB] || WFIRST_Turn_ProResnoTxt_fr01799.png (3840x2160) [7.4 MB] || WFIRST_Turnaround_fr_01799_searchweb.png (320x180) [67.5 KB] || WFIRST_Turnaround_fr_01799_thm.png (80x40) [5.7 KB] || 360Articulated_bkgrnd (1920x1080) [0 Item(s)] || WFIRST_Turntable_Articulated_Bkgrnd_H264_1080p.webm (1920x1080) [7.0 MB] || WFIRST_Turntable_Articulated_Bkgrnd_H264_1080p.mov (1920x1080) [108.4 MB] || WFIRST_Turntable_Articulated_Bkgrnd_H264_4K.mov (3840x2160) [140.9 MB] || WFIRST_Turntable_Articulated_Bkgrnd_4k_ProRes.mov (3840x2160) [3.9 GB] || ", "hits": 28 }, { "id": 40305, "url": "https://svs.gsfc.nasa.gov/gallery/roman/", "result_type": "Gallery", "release_date": "2016-07-21T00:00:00-04:00", "title": "Nancy Grace Roman Space Telescope", "description": "Formerly known as WFIRST, the Wide Field Infrared Survey Telescope, the Roman Space Telescope is a NASA observatory designed to perform wide field imaging and surveys of the near infrared (NIR) sky. The current design of the mission makes use of an existing 2.4m telescope, which is the same size as the Hubble Space Telescope. The Roman Space Telescope is the top-ranked large space mission in the New Worlds, New Horizon Decadal Survey of Astronomy and Astrophysics. The Wide Field Instrument will provide a field of view of the sky that is 100 times larger than images provided by HST. The coronagraph will enable astronomers to detect and measure properties of planets in other solar systems.\nMore information about the Roman Space Telescope", "hits": 354 }, { "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": 145 }, { "id": 12147, "url": "https://svs.gsfc.nasa.gov/12147/", "result_type": "Produced Video", "release_date": "2016-03-03T10:00:00-05:00", "title": "2016 Eclipse", "description": "Solar scientists Natchimuthuk Gopalswamy, Nelson Reginal, Eric Christian, and Sarah Jaeggli discuss the 2016 eclipse and how it is great preparation for the 2017 eclipse.Complete transcript available. || eclipse_promo_thumb.jpg (1280x720) [53.1 KB] || eclipse_promo_thumb_searchweb.png (320x180) [69.9 KB] || eclipse_promo_thumb_thm.png (80x40) [12.8 KB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.mov (1920x1080) [534.5 MB] || PRORES_B-ROLL_12147_2016.eclipse_promo_V2_prores.mov (1280x720) [1.5 GB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv.m4v (1280x720) [63.3 MB] || NASA_TV_12147_2016.eclipse_promo_V2.mpeg (1280x720) [383.5 MB] || 12147_2016.eclipse_promo_V2.mov (1920x1080) [2.7 GB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.webm (1920x1080) [11.6 MB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv_subtitles.m4v (1280x720) [63.4 MB] || 12147_2016_eclipse_PROMO.en_US.srt [2.0 KB] || 12147_2016_eclipse_PROMO.en_US.vtt [2.0 KB] || NASA_PODCAST_12147_2016.eclipse_promo_V2_ipod_sm.mp4 (320x240) [21.4 MB] || ", "hits": 79 }, { "id": 12153, "url": "https://svs.gsfc.nasa.gov/12153/", "result_type": "Produced Video", "release_date": "2016-02-18T11:00:00-05:00", "title": "WFIRST: The Best of Both Worlds", "description": "With a view 100 times bigger than that of NASA’s Hubble Space Telescope, the Wide Field Infrared Survey Telescope WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life. Scientists participating in the mission discuss the spacecraft, the science, and its potential. Slated to launch in the mid-2020s, the observatory will operate at a gravitational balance point known as Earth-sun L2, which is located about 930,000 miles from Earth and directly opposite the sun.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WfirstAfta-PrintStill2_print.jpg (1024x576) [79.3 KB] || WfirstAfta-PrintStill2.png (3840x2160) [4.7 MB] || WfirstAfta-PrintStill2_searchweb.png (320x180) [59.2 KB] || WfirstAfta-PrintStill2_thm.png (80x40) [4.6 KB] || 12153_WFIRST_Best_Both_Worlds_ProRes_1280x720_5994.mov (1280x720) [3.1 GB] || 12153_WFIRST_Best_Both_Worlds_H264_Best_1280x720_5994.mov (1280x720) [1.7 GB] || 12153_WFIRST_Best_Both_Worlds_FINAL_youtube_hq.mov (1280x720) [671.5 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.mov (1280x720) [174.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv.m4v (1280x720) [122.3 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.webm (1280x720) [25.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv_subtitles.m4v (1280x720) [122.4 MB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.srt [4.6 KB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.vtt [4.4 KB] || NASA_PODCAST_12153_WFIRST_Best_Both_Worlds_FINAL_ipod_sm.mp4 (320x240) [41.6 MB] || ", "hits": 51 }, { "id": 4342, "url": "https://svs.gsfc.nasa.gov/4342/", "result_type": "Visualization", "release_date": "2015-09-15T10:00:00-04:00", "title": "Sixteen Comets Touring the Inner Solar System", "description": "This visualization presents a small sample of the 9 years of comets seen by SOHO from the perspective a an observer at a fixed point above the ecliptic plane with the Sun at the center. || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [109.1 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [72.2 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_thm.png (80x40) [4.3 KB] || SixteenComets-oblique.HD1080.webm (1920x1080) [11.3 MB] || SixteenComets-oblique.HD1080.mov (1920x1080) [109.2 MB] || Oblique (1920x1080) [512.0 KB] || SixteenComets-oblique_1080p30.mp4 (1920x1080) [64.2 MB] || ", "hits": 39 }, { "id": 4343, "url": "https://svs.gsfc.nasa.gov/4343/", "result_type": "Visualization", "release_date": "2015-09-15T10:00:00-04:00", "title": "Lots of Comets - Long trail version", "description": "This visualization presents 14 years of comets seen by SOHO from the perspective of an observer orbiting a fixed point above the ecliptic plane with the Sun at the center.This video is also available on our YouTube channel. || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [110.2 KB] || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [71.5 KB] || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_thm.png (80x40) [4.7 KB] || Orbit (1920x1080) [512.0 KB] || LotsaComets-orbit_1080p30.mp4 (1920x1080) [188.3 MB] || LotsaComets-orbit_1080p30.webm (1920x1080) [20.8 MB] || ", "hits": 53 }, { "id": 4344, "url": "https://svs.gsfc.nasa.gov/4344/", "result_type": "Visualization", "release_date": "2015-09-15T10:00:00-04:00", "title": "Lots of Comets - Short trail version", "description": "This visualization presents 14 years of comets seen by SOHO from the perspective of an observer at a fixed point above the ecliptic plane with the Sun at the center. || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [97.7 KB] || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [65.2 KB] || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_thm.png (80x40) [3.5 KB] || Oblique (1920x1080) [768.0 KB] || LotsaCometsST-oblique_1080p30.mp4 (1920x1080) [103.6 MB] || LotsaCometsST-oblique_1080p30.webm (1920x1080) [20.3 MB] || ", "hits": 25 }, { "id": 11975, "url": "https://svs.gsfc.nasa.gov/11975/", "result_type": "Produced Video", "release_date": "2015-09-15T10:00:00-04:00", "title": "3,000 Comets for SOHO", "description": "Karl Battams of the Naval Research Lab talks us through a visualization of the comets that SOHO has witnessed.Watch this video on the NASAexplorer YouTube channel. || sohocometsthumb.jpg (1280x720) [150.9 KB] || sohocometsthumb_print.jpg (1024x576) [157.3 KB] || sohocometsthumb_searchweb.png (320x180) [82.6 KB] || sohocometsthumb_web.png (320x180) [82.6 KB] || sohocometsthumb_thm.png (80x40) [11.5 KB] || G2015-069_3000SOHOcometsV2-H264_Good_1080_29.97.mov (1920x1080) [565.6 MB] || G2015-069_3000SOHOcometsV2-H264_Best_1920x1080_59.94.mov (1920x1080) [3.3 GB] || VX-71391.m4v (1280x720) [134.5 MB] || VX-71391.mov (1920x1080) [2.1 GB] || VX-71391.webm (960x540) [108.0 MB] || 3000SOHOcometsV2.en_US.srt [4.5 KB] || 3000SOHOcometsV2.en_US.vtt [4.5 KB] || VX-71391.mp4 (480x272) [35.9 MB] || ", "hits": 52 }, { "id": 11811, "url": "https://svs.gsfc.nasa.gov/11811/", "result_type": "Produced Video", "release_date": "2015-03-17T13:15:00-04:00", "title": "SOHO Observes March 14 Coronal Mass Ejection", "description": "The Joint ESA/NASA Solar and Heliospheric Observatory, or SOHO, captured this image series of a coronal mass ejection, or CME, on March 14, 2015. || JHV_movie_created_2015-03-17_19.37.12_print.jpg (1024x576) [73.7 KB] || JHV_movie_created_2015-03-17_19.37.12_searchweb.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12_web.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12.webm (1920x1080) [334.4 KB] || JHV_movie_created_2015-03-17_19.37.12.mp4 (1920x1080) [9.0 MB] || ", "hits": 61 }, { "id": 11737, "url": "https://svs.gsfc.nasa.gov/11737/", "result_type": "Produced Video", "release_date": "2015-02-05T11:00:00-05:00", "title": "Tracking Solar Eruptions", "description": "Explore how scientists trace the journey of material exploding from the sun. || c-1024.jpg (1024x576) [129.9 KB] || c-1920.jpg (1920x1080) [290.2 KB] || c-1280.jpg (1280x720) [181.0 KB] || c-1024_print.jpg (1024x576) [126.9 KB] || c-1024_searchweb.png (320x180) [78.3 KB] || c-1024_print_thm.png (80x40) [14.7 KB] || ", "hits": 70 }, { "id": 11558, "url": "https://svs.gsfc.nasa.gov/11558/", "result_type": "Produced Video", "release_date": "2014-09-24T10:00:00-04:00", "title": "NASA's Many Views of a Massive CME", "description": "On July 23, 2012, a massive cloud of solar material erupted off the sun's right side, zooming out into space. It soon passed one of NASA's Solar Terrestrial Relations Observatory, or STEREO, spacecraft, which clocked the CME as traveling between 1,800 and 2,200 miles per second as it left the sun. This was the fastest CME ever observed by STEREO. Two other observatories – NASA's Solar Dynamics Observatory and the joint European Space Agency/NASA Solar and Heliospheric Observatory — witnessed the eruption as well. The July 2012 CME didn't move toward Earth, but watching an unusually strong CME like this gives scientists an opportunity to observe how these events originate and travel through space. STEREO's unique viewpoint from the sides of the sun combined with the other two observatories watching from closer to Earth helped scientists create models of the entire July 2012 event. They learned that an earlier, smaller CME helped clear the path for the larger event, thus contributing to its unusual speed. Such data helps advance our understanding of what causes CMEs and improves modeling of similar CMEs that could be Earth-directed. || ", "hits": 110 }, { "id": 11651, "url": "https://svs.gsfc.nasa.gov/11651/", "result_type": "Produced Video", "release_date": "2014-09-11T08:00:00-04:00", "title": "September 10, 2014 X1.6 flare", "description": "The sun emitted a significant solar flare, peaking at 1:48 p.m. EDT on Sept. 10, 2014. NASA's Solar Dynamics Observatory captured images of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground. However — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel.This flare is classified as an X1.6 class flare. \"X-class\" denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. || ", "hits": 50 }, { "id": 4177, "url": "https://svs.gsfc.nasa.gov/4177/", "result_type": "Visualization", "release_date": "2014-07-23T00:00:00-04:00", "title": "As Seen by STEREO-A: The Carrington-Class CME of 2012", "description": "STEREO-A, at a position along Earth's orbit where it has an unobstructed view of the far side of the Sun, could clearly observe possibly the most powerful coronal mass ejection (CME) of solar cyle 24 on July 23, 2012. The visualizations on this page cover the entire day.We see the flare erupt in the lower right quadrant of the solar disk from a large active region. The material is launched into space in a direction towards STEREO-A. This creates the ring-like 'halo' CME visible in the STEREO-A coronagraph, COR-2 (blue circular image).As the CME expands beyond the field of view of the COR-2 imager, the high energy particles reach STEREO-A, creating the snow-like noise in the image. The particles also strike the HI-2 imager (blue square) brightening the image.The HI-1 imager has had 'bloom removal' enabled and filled with contents of the immediately previous HI-1 image, which creates a linear artifact above and below bright stars and planets. || ", "hits": 139 }, { "id": 4178, "url": "https://svs.gsfc.nasa.gov/4178/", "result_type": "Visualization", "release_date": "2014-07-23T00:00:00-04:00", "title": "As Seen by STEREO-B: The Carrington-Class CME of 2012", "description": "Like SDO, STEREO-B did not have a direct view of the coronal mass ejection (CME) launched by the sun on July 23, 2012. However, the active region involved was very close to the limb of the sun (lower left quadrant) and STEREO-B provided an excellent view of plasma launched in both ultraviolet light and the white-light coronagraph. || ", "hits": 67 }, { "id": 11493, "url": "https://svs.gsfc.nasa.gov/11493/", "result_type": "Produced Video", "release_date": "2014-02-25T00:00:00-05:00", "title": "NASA's SDO Provides Images of Significant Solar Flare", "description": "The sun emitted a significant solar flare, peaking at 7:49 p.m. EST on Feb. 24, 2014. NASA's Solar Dynamics Observatory, which keeps a constant watch on the sun, captured images of the event.This flare is classified as an X4.9-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. || ", "hits": 83 }, { "id": 11387, "url": "https://svs.gsfc.nasa.gov/11387/", "result_type": "Produced Video", "release_date": "2013-10-29T16:30:00-04:00", "title": "Five Days of Flares and CMEs", "description": "This movie shows 23 of the 26 M- and X-class flares on the sun between 18:00 UT Oct. 23 and 15:00 UT Oct. 28, 2013, as captured by NASA's Solar Dynamics Observatory. It also shows the coronal mass ejections — great clouds of solar material bursting off the sun into space — during that time as captured by the ESA/NASA Solar and Heliospheric Observatory. || ", "hits": 57 }, { "id": 30081, "url": "https://svs.gsfc.nasa.gov/30081/", "result_type": "Hyperwall Visual", "release_date": "2013-10-10T00:00:00-04:00", "title": "Stereo Captures Eruption and CME", "description": "On May 1, 2013, NASA's Solar Terrestrial Relations Observatory Ahead (STEREO-A) satellite along with its twin STEREO Behind (STEREO-B), observed an active region (right) of the sun erupt. This eruption, called a coronal mass ejection, or CME, sent plasma streaming out through the solar system. STEREO has an extreme ultraviolet camera similar to the Solar Dynamics Observatory (SDO) satellite, but it also has coronagraph telescopes like the European Space Agency/NASA Solar and Heliospheric Observatory (SOHO) where the bright sun is blocked by a disk so it does not overpower the fainter solar atmosphere. As a result, using its two inner coronagraphs, STEREO was able to track the CME from the solar surface out to 6.3 million miles. || ", "hits": 36 }, { "id": 30072, "url": "https://svs.gsfc.nasa.gov/30072/", "result_type": "Hyperwall Visual", "release_date": "2013-09-25T00:00:00-04:00", "title": "Heliophysics Fleet Captures Eruption and CME", "description": "On May 1, 2013, NASA's Solar Dynamics Observatory (SDO) watched as an active region (left) of the sun erupted with a huge cloud of solar material—a heated, charged gas called plasma. This eruption, called a coronal mass ejection, or CME, sent the plasma streaming out through the solar system. Viewing the sun in the extreme ultraviolet wavelength of 304 Ångström, SDO provided a beautiful view of the initial arc as it left the solar surface. In addition to the images captured by SDO the CME was also observed by the European Space Agency/NASA Solar and Heliospheric Observatory (SOHO). SOHO houses two overlapping Large Angle Spectrometric Coronagraph (LASCO) telescopes where the bright sun is blocked by a disk so it does not overpower the fainter solar atmosphere. Both LASCO telescopes, named C2 and C3, observed the CME. The LASCO C2 coronagraph shows the region out to about 2.5 million miles, while the LASCO C3 coronagraph expands even farther out to around 13.5 million miles. Both of these instruments show the CME as it expands and becomes fainter on its trip away from the sun. || ", "hits": 37 }, { "id": 10785, "url": "https://svs.gsfc.nasa.gov/10785/", "result_type": "Produced Video", "release_date": "2013-05-07T11:00:00-04:00", "title": "NASA's Heliophysics Fleet Captures May 1, 2013 Prominence Eruption and CME", "description": "On May 1, 2013, NASA's Solar Dynamics Observatory (SDO) watched as an active region just around the East limb (left edge) of the sun erupted with a huge cloud of solar material—a heated, charged gas called plasma. This eruption, called a coronal mass ejection, or CME, sent the plasma streaming out through the solar system. Viewing the sun in the extreme ultraviolet wavelength of 304 angstroms, SDO provided a beautiful view of the initial arc as it left the solar surface. Such eruptions soon leave SDO's field of view, but other satellites in NASA's Heliophysics fleet can pick them up, tracking such space weather to determine if they are headed toward Earth or spacecraft near other planets. With advance warning, many space assets can be put into safe mode and protect themselves from the effects of such particle radiation.In addition to the images captured by SDO, the May 1, 2013 CME was also observed by the ESA/NASA Solar and Heliospheric Observatory (SOHO). SOHO houses two overlapping coronagraphs—telescopes where the bright sun is blocked by a disk so it doesn't overpower the fainter solar atmosphere—and they both saw the CME continue outward. The LASCO C2 coronagraph shows the region out to about 2.5 million miles. The LASCO C3 coronagraph expands even farther out to around 13.5 million miles. Both of these instruments show the CME as it expands and becomes fainter on its trip away from the sun.NASA's Solar Terrestrial Relations Observatory (STEREO) Ahead satellite saw the eruption from a very different angle. It, along with its twin STEREO Behind, is orbiting at a similar distance as Earth. STEREO-A orbits slightly faster than Earth and STEREO-B orbits slightly slower. Currently, STEREO-A is more than two-thirds of the way to being directly behind the sun, and has a view of the far side of the sun. From this perspective, the CME came off the right side of the sun. STEREO has an extreme ultraviolet camera similar to SDO's, but it also has coronagraphs like SOHO. As a result, using its two inner coronagraphs, it was able to track the CME from the solar surface out to 6.3 million miles.Working together, such missions provide excellent coverage of a wide variety of solar events, a wealth of scientific data—and lots of beautiful imagery.Watch this video on YouTube. || ", "hits": 92 }, { "id": 11257, "url": "https://svs.gsfc.nasa.gov/11257/", "result_type": "Produced Video", "release_date": "2013-04-26T16:00:00-04:00", "title": "CMEs Galore", "description": "On April 20, 2013, at 2:54 a.m. EDT, the sun erupted with a coronal mass ejection (CME), a solar phenomenon that can send billions of tons of solar particles into space that can affect electronic systems in satellites. Experimental NASA research models show that the CME left the sun at 500 miles per second and is not Earth-directed. However, it may pass by NASA's Messenger and STEREO-A satellites, and their mission operators have been notified. There is, however, no particle radiation associated with this event, which is what would normally concern operators of interplanetary spacecraft since the particles can trip computer electronics on board. When warranted, NASA operators can put spacecraft into safe mode to protect the instruments from the solar material. The same region of the sun erupted with another coronal mass ejection (CME) at 3:54 a.m. on April 21, 2013. Experimental NASA research models show the CME left the sun at speeds of 550 miles per second. The models show that the CME will also pass by NASA's Messenger and the flank of the CME may graze STEREO-A.Another coronal mass ejection (CME) has erupted from the sun, headed toward Mercury and NASA's Messenger spacecraft. The CME began at 12:39 p.m. EDT on April 21, 2013. Experimental NASA research models show that the CME left the sun at 625 miles per second and that it will catch up to the CME from earlier on April 21 before the combined CMEs pass Messenger. There is also chance that the combined CMEs will give a glancing blow to STEREO-A. || ", "hits": 135 }, { "id": 11246, "url": "https://svs.gsfc.nasa.gov/11246/", "result_type": "Produced Video", "release_date": "2013-04-11T12:00:00-04:00", "title": "The Sun Emits a Mid-level Flare and CME", "description": "The sun emitted a mid-level flare, peaking at 3:16 a.m. EDT on April 11, 2013.Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel. This disrupts the radio signals for as long as the flare is ongoing, anywhere from minutes to hours.This flare is classified as an M6.5 flare, some ten times less powerful than the strongest flares, which are labeled X-class flares. M-class flares are the weakest flares that can still cause some space weather effects near Earth. This flare produced a radio blackout that has since subsided. The blackout was categorized as an R2 on a scale between R1 and R5 on NOAA's space weather scales.This is the strongest flare seen so far in 2013. Increased numbers of flares are quite common at the moment, since the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in late 2013. Humans have tracked this solar cycle continuously since it was discovered, and it is normal for there to be many flares a day during the sun's peak activity. || ", "hits": 65 }, { "id": 11225, "url": "https://svs.gsfc.nasa.gov/11225/", "result_type": "Produced Video", "release_date": "2013-03-18T08:00:00-04:00", "title": "Solar Storm Near Earth Caused by March 15, 2013 Fast CME", "description": "On March 15, 2013, at 2:54 a.m. EDT, the sun erupted with an Earth-directed coronal mass ejection (CME), a solar phenomenon that can send billions of tons of solar particles into space and can reach Earth one to three days later and affect electronic systems in satellites and on the ground. Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, show that the CME left the sun at speeds of around 900 miles per second, which is a fairly fast speed for CMEs. Historically, CMEs at this speed have caused mild to moderate effects at Earth.Update: On March 17, 2013, at 1:28 a.m. EDT, the coronal mass ejection (CME) from March 15 passed by NASA's Advanced Composition Explorer (ACE) as it approached Earth. Upon interacting with the giant magnetic bubble surrounding Earth, the magnetosphere, the CME caused a kind of solar storm known as a geomagnetic storm. The storm initially caused a mild storm rated on NOAA's geomagnetic storm scales as a G2 on a scale from G1 to G5, and subsequently subsided to a G1. In the past, storms of this strength have caused auroras near the poles but have not disrupted electrical systems on Earth or interfered with GPS or satellite-based communications systems. || ", "hits": 76 }, { "id": 11207, "url": "https://svs.gsfc.nasa.gov/11207/", "result_type": "Produced Video", "release_date": "2013-02-07T10:30:00-05:00", "title": "The Sun Produces Two CMEs", "description": "In the evening of Feb. 5, 2013, the sun erupted with two coronal mass ejections or CMEs that may glance near-Earth space. Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, show that the first CME began at 7 p.m. EST and left the sun at speeds of around 750 miles per second. The second CME began at 10:36 p.m. EST and left the sun at speeds of around 350 miles per second. Historically, CMEs of this speed and direction have been benign.Not to be confused with a solar flare, a CME is a solar phenomenon that can send solar particles into space and reach Earth one to three days later.Earth-directed CMEs can cause a space weather phenomenon called a geomagnetic storm, which occurs when they connect with the outside of the Earth's magnetic envelope, the magnetosphere, for an extended period of time. In the past, CMEs at this strength have had little effect. They may cause auroras near the poles but are unlikely to disrupt electrical systems on Earth or interfere with GPS or satellite-based communications systems. || ", "hits": 69 }, { "id": 11201, "url": "https://svs.gsfc.nasa.gov/11201/", "result_type": "Produced Video", "release_date": "2013-01-31T12:00:00-05:00", "title": "January 31, 2013 CME and Prominence Eruption", "description": "On Jan. 31, 2013 at 2:09am EST, the sun erupted with an Earth-directed coronal mass ejection or CME. Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, show that the CME left the sun at speeds of around 575 miles per second, which is a fairly typical speed for CMEs. Historically, CMEs at this speed are mild.Not to be confused with a solar flare, a CME is a solar phenomenon that can send solar particles into space and reach Earth one to three days later.Earth-directed CMEs can cause a space weather phenomenon called a geomagnetic storm, which occurs when they connect with the outside of the Earth's magnetic envelope, the magnetosphere, for an extended period of time. In the past, CME's such as this have caused auroras near the poles but didn't disrupt electrical systems on Earth or interfere with GPS or satellite-based communications systems. || ", "hits": 40 }, { "id": 3956, "url": "https://svs.gsfc.nasa.gov/3956/", "result_type": "Visualization", "release_date": "2012-09-20T00:00:00-04:00", "title": "Halloween Solar Storms - 2003", "description": "This is a 1024x1024 pixel version of solar storms providing a more complete view of the SOHO/LASCO/C3 field-of-view.Here is a view of the solar disk in 195 Å ultraviolet light (colored green in this movie) and the Sun's extended atmosphere, or corona, (blue and white in this movie). The corona is visible to the SOHO/LASCO coronagraph instruments, which block the bright disk of the Sun so the significantly fainter corona can be seen. In this movie, the inner coronagraph (designated C2) is combined with the outer coronagraph (C3). This movie covers a two week period in October and November 2003 which exhibited some of the largest solar activity events since the advent of space-based solar observing.As the movie plays, we can observe a number of features of the active Sun. Long streamers radiate outward from the Sun and wave gently due to their interaction with the solar wind. The bright white regions are visible due to their high density of free electrons which scatter the light from the photosphere towards the observer. Protons and other ionized atoms are there as well, but are not as visible since they do not interact with photons as strongly as electrons. Coronal Mass Ejections (CMEs) are occasionally observed launching from the Sun. Some of these launch particle events which can saturate the cameras with snow-like artifacts.Also visible in the coronagraphs are stars and planets. Stars are seen to drift slowly to the right, carried by the relative motion of the Sun and the Earth. The planet Mercury is visible as the bright point moving left of the Sun. The horizontal 'extension' in the image is called 'blooming' and is due to a charge leakage along the readout wires in the CCD imager in the camera. || ", "hits": 118 }, { "id": 10998, "url": "https://svs.gsfc.nasa.gov/10998/", "result_type": "Produced Video", "release_date": "2012-06-04T11:00:00-04:00", "title": "SOHO LASCO View of Approaching Venus Transit", "description": "The LASCO C2 and C3 coronographs on board the SOHO spacecraft have been watching the approach of Venus for its last solar transit until 2117.With coronagraphs, the Sun is being blocked by an occulting disk, seen here in blue, so that SOHO can observe the much fainter features in the Sun's corona. The actual size of the Sun is represented by the white disk. The transit of Venus begins tomorrow, June 5, at about 6pm Eastern Daylight Time, or about 10pm Universal Time. It will last approximately 6 hours. || ", "hits": 76 }, { "id": 10619, "url": "https://svs.gsfc.nasa.gov/10619/", "result_type": "Produced Video", "release_date": "2010-07-22T00:00:00-04:00", "title": "20 Years of Hubble Science", "description": "This video series focuses on two areas of science that the Hubble Space Telescope has helped advance: thee formation and evolution of galaxies and detection of extrasolar planets. || ", "hits": 50 }, { "id": 3566, "url": "https://svs.gsfc.nasa.gov/3566/", "result_type": "Visualization", "release_date": "2008-12-18T00:00:00-05:00", "title": "Multi-Sun Composition", "description": "This movie is a composition of multiple solar datasets synchronized in time. The time frame is late October and early November of 2003, the time of some record-breaking solar activity.The background of the movie shows the view of the wide-angle coronagraphs (blue/white), or LASCO instruments, aboard SOHO. They show streams of electrons outbound from the Sun, part of the solar atmosphere. The central green image is the Sun in ultraviolet light from the EIT instrument. Note that flashes of solar flares in the ultraviolet quickly propagate out from the Sun and are visible in LASCO. These events are coronal mass ejections, or CMEs.Overlaid on the upper left is a better view of the EIT ultraviolet image at a wavelength of 195 angstroms (19.5 nanometers).On the lower left, the orange movie is the EIT ultraviolet movie at 304 angstroms (30.4 nanometers).On the upper right is a solar magnetogram, taken by the MDI instrument. The white regions correspond to positive (north) magnetic flux and the dark regions to negative (south) magnetic flux.The colors for the sequences above are not real. They are chosen by convention since the properties recorded by the cameras are not visible to the human eye.The final image on the lower right is also from MDI. It is a combination of several optical wavelengths and is the best representation from SOHO of the Sun in visible light, as we would see it through ground-based telescopes.The movies that are part of this composition are also available individually on the SVS site: Halloween Solar Storms 2003: SOHO/EIT and SOHO/LASCOHalloween Solar Storms 2003: SOHO/EIT Ultraviolet, 195 angstromsHalloween Solar Storms 2003: SOHO/EIT Ultraviolet, 304 angstromsHalloween Solar Storms 2003: SOHO/MDI ContinuumHalloween Solar Storms 2003: SOHO/MDI Magnetograms || ", "hits": 30 }, { "id": 3504, "url": "https://svs.gsfc.nasa.gov/3504/", "result_type": "Visualization", "release_date": "2008-04-02T00:00:00-04:00", "title": "Halloween 2003 Solar Storms: SOHO/EIT and SOHO/LASCO", "description": "Here is a view of the solar disk in 195 Å ultraviolet light (colored green in this movie) and the Sun's extended atmosphere, or corona, (blue and white in this movie). The corona is visible to the SOHO/LASCO coronagraph instruments, which block the bright disk of the Sun so the significantly fainter corona can be seen. In this movie, the inner coronagraph (designated C2) is combined with the outer coronagraph (C3). This movie covers a two week period in October and November 2003 which exhibited some of the largest solar activity events since the advent of space-based solar observing.As the movie plays, we can observe a number of features of the active Sun. Long streamers radiate outward from the Sun and wave gently due to their interaction with the solar wind. The bright white regions are visible due to their high density of free electrons which scatter the light from the photosphere towards the observer. Protons and other ionized atoms are there as well, but are not as visible since they do not interact with photons as strongly as electrons. Coronal Mass Ejections (CMEs) are occasionally observed launching from the Sun. Some of these launch particle events which can saturate the cameras with snow-like artifacts.Also visible in the coronagraphs are stars and planets. Stars are seen to drift slowly to the right, carried by the relative motion of the Sun and the Earth. The planet Mercury is visible as the bright point moving left of the Sun. The horizontal 'extension' in the image is called 'blooming' and is due to a charge leakage along the readout wires in the CCD imager in the camera.This movie is part of a series of movies with matching cadence designed to play synchronously with each other. The other movies in this series are Halloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 195 angstromHalloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 304 angstromHalloween 2003 Solar Storms: SOHO/MDI Continuum Halloween 2003 Solar Storms: SOHO/MDI Magnetograms For more information, visit the SOHO project page.. || ", "hits": 55 }, { "id": 3431, "url": "https://svs.gsfc.nasa.gov/3431/", "result_type": "Visualization", "release_date": "2007-05-29T00:00:00-04:00", "title": "Coronal Mass Ejections (CME): Radio Quiet Variety", "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image. Moving material therefore appears white on the leading edge and dark behind it. The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis). A vertical white bar marks the time of the LASCO image.This CME shows no radio-loud emission between 0.2-1.0 MHz. || ", "hits": 20 }, { "id": 3432, "url": "https://svs.gsfc.nasa.gov/3432/", "result_type": "Visualization", "release_date": "2007-05-29T00:00:00-04:00", "title": "Coronal Mass Ejections (CME): Radio Loud Variety", "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image. Moving material therefore appears white on the leading edge and dark behind it. The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis). A vertical white bar marks the time of the LASCO image.The radio-loud emission of the CME is the yellow-orange band between 0.2-1.0 MHz. || ", "hits": 29 }, { "id": 3406, "url": "https://svs.gsfc.nasa.gov/3406/", "result_type": "Visualization", "release_date": "2007-03-01T00:00:00-05:00", "title": "STEREO Coronal Mass Ejection: From the EUVI to HI-2", "description": "This movie collects imagery from SOHO and STEREO-A of a coronal mass ejection (CME) during January of 2007. The instruments in this view, from left to right, are STEREO/HI-1, STEREO/HI-2, SOHO/LASCO/C3, SOHO/LASCO/C2, and STEREO/EUVI. The Heliospheric Imager, HI-2, shows some of the tail of comet McNaught. The dark trapezoidal shape on the left edge of the image in HI-2 is the Earth occulter which will block out the disk of the Earth when it moves into view (since the planet will appear so bright as to saturate the detectors). Due to ongoing work with the STEREO coronagraphs, COR1 and COR2, the SOHO/LASCO coronagraphs are used for this movie. The blue Sun in the center of the coronagraphs is STEREO/EUVI ultraviolet images.There is a 22 hour gap in the data coverage for HI-2 which creates the appearance of a jump in the playback.These are not standard images but are called 'running difference' images which highlight changes in the view. White pixels correspond to increases in brightness, while dark pixels reflect a decrease in brightness, with respect to the immediately previous image.'Running differencing' generates some unusual effects. For example, the mottled background is created by the motion of the stars through the field-of-view as the spacecraft pointing direction slowly changes (the Andromeda galaxy is the oblong 'smudge' near the upper left corner). The planets Venus (right edge of HI-2) and Mercury are visible (near center of HI-1), their column of pixels saturated due to their brightness.STEREO: Solar TErrestrial RElations ObservatorySOHO: SOlar Heliospheric ObservatoryLASCO: Large Angle and Spectrometric CoronagraphEUVI: Extreme UltraViolet Imager || ", "hits": 33 }, { "id": 3159, "url": "https://svs.gsfc.nasa.gov/3159/", "result_type": "Visualization", "release_date": "2005-05-24T12:00:00-04:00", "title": "SOHO/LASCO View of January 2005 Solar Events", "description": "The January 20 flare began just before 2 a.m. ET. A storm of energetic protons impacted Earth just 15 minutes later. These views of the flare are from the Solar and Heliospheric Observatory (SOHO). The proton storm near Earth causes `snow' in the images, obscuring the Sun as radiation swamps the cameras. The structure at the 1:30 position in the SOHO/LASCO/C3 data is the occulting disk pylon. || ", "hits": 31 }, { "id": 2961, "url": "https://svs.gsfc.nasa.gov/2961/", "result_type": "Visualization", "release_date": "2004-07-08T12:00:00-04:00", "title": "Halloween Solar Storms from SOHO/EIT and SOHO/LASCO", "description": "This movie is a combination of SOHO/EIT at 195 angstroms as well as the LASCO/C2 and C3 cameras. At this scale we can see the flashes from solar flares in SOHO/EIT (green) and the subsequent coronal mass ejections in SOHO/LASCO/C2 (red) and SOHO/LASCO/C3 (blue). This movie is synchronized to play with animation IDs 2960 and 2959. For more information on how X-ray solar flares are classified (B, C, M, X), visit SpaceWeather.com. || ", "hits": 31 }, { "id": 2950, "url": "https://svs.gsfc.nasa.gov/2950/", "result_type": "Visualization", "release_date": "2004-07-01T12:00:00-04:00", "title": "Building a 3-D Coronal Mass Ejection from 2-D Data", "description": "Using differences in polarization of light directly from the Sun vs. scattered from the CME electrons, it is possible to derive a distance of matter along the line-of-sight. This version is an early release of animation #2958. || ", "hits": 19 }, { "id": 2958, "url": "https://svs.gsfc.nasa.gov/2958/", "result_type": "Visualization", "release_date": "2004-07-01T12:00:00-04:00", "title": "Building a 3-D Coronal Mass Ejection from 2-D Data", "description": "Using differences in polarization of light directly from the Sun vs. scattered from the CME electrons, it is possible to derive a distance of matter along the line-of-sight. This version is an enhanced version of animation ID 2950 with a color table enhanced to show fainter regions of the CME. || ", "hits": 16 }, { "id": 2936, "url": "https://svs.gsfc.nasa.gov/2936/", "result_type": "Visualization", "release_date": "2004-05-23T12:00:00-04:00", "title": "The fastest CME of Cycle 23 overtakes another fast CME", "description": "On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft. || ", "hits": 78 }, { "id": 2509, "url": "https://svs.gsfc.nasa.gov/2509/", "result_type": "Visualization", "release_date": "2003-01-31T12:00:00-05:00", "title": "A Multi-Mission View of the AR9906 Solar Flare with Instrument Labels", "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from six hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, the instrument names appear in a color roughly matching the color used for the data, and black corresponds to no (current) instrument coverage. || ", "hits": 22 }, { "id": 2511, "url": "https://svs.gsfc.nasa.gov/2511/", "result_type": "Visualization", "release_date": "2003-01-31T12:00:00-05:00", "title": "A Multi-Mission View of the AR9906 Solar Flare without Instrument Labels", "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from 6 hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, black corresponds to no (current) instrument coverage (there used to be a LASCO C1 camera inside the ring of LASCO C2, but that instrument didn't recover after SOHO was temporarily 'lost' in 1998). || ", "hits": 16 }, { "id": 2553, "url": "https://svs.gsfc.nasa.gov/2553/", "result_type": "Visualization", "release_date": "2003-01-31T12:00:00-05:00", "title": "A Multi-Mission View of the AR9906 Solar Flare with Alternate Instrument Labels", "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from 6 hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, black corresponds to no (current) instrument coverage (there used to be a LASCO C1 camera inside the ring of LASCO C2, but that instrument didn't recover after SOHO was temporarily 'lost' in 1998). || ", "hits": 27 }, { "id": 40352, "url": "https://svs.gsfc.nasa.gov/gallery/exoplanets/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "Exoplanets", "description": "An exoplanet is a planet orbiting a star other than the Sun. Of particular interest are planets that may orbit in their star’s habitable zone, the distance from a star where temperatures allow liquid water to persist on a planet’s surface, given a suitable atmosphere. Since water is necessary for life as we know it, its presence is required for worlds to be considered capable of supporting life. Exoplanets can also teach us more about planets in the universe, such as the diversity of planets in the galaxy, how they interact with their host stars and with each other, and how common solar systems like ours really are.\n \nUsing a wide variety of methods, astronomers have discovered more than 3,700 exoplanets to date, largely thanks to NASA's Kepler/K2 mission.\n \nOther NASA missions also play a key role in detecting exoplanets. The Transiting Exoplanet Survey Satellite, which launched in April 2018, will monitor 200,000 of the brightest dwarf stars for transiting exoplanets. Future missions like the James Webb Space Telescope will be able to study these discovered planets in greater detail, helping determine their composition. \n \nResearchers in NASA Goddard Space Flight Center's Sellers Exoplanet Environments Collaboration are leveraging work across disciplines to better understand exoplanets. Areas like planet-star interactions, planetary formation, and even study of the Earth itself enable researchers to develop tools to learn more about how exoplanets evolve, and what ingredients are necessary to support life.", "hits": 557 } ] }