{ "count": 799, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Infrared%22", "previous": null, "results": [ { "id": 31376, "url": "https://svs.gsfc.nasa.gov/31376/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "SPHEREx All Sky Map 2025", "description": "Two passes of an all-sky mosaic image from NASAs SPHEREx space telescope, the first showing dust and gas and the second showing stars and galaxies.", "hits": 470 }, { "id": 31374, "url": "https://svs.gsfc.nasa.gov/31374/", "result_type": "Visualization", "release_date": "2026-03-26T10:59:59-04:00", "title": "Aurora Mosaic from the Geomagnetic Storm of November 11-13, 2025", "description": "A mosaic of Day/Night Band (DNB) images from the the Visible Infrared Imaging Radiometer (VIIRS) on the NOAA-20/JPSS-1 satellite showing a ring of bright auroral light extending south past 50N latitude.", "hits": 361 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 712 }, { "id": 31373, "url": "https://svs.gsfc.nasa.gov/31373/", "result_type": "Hyperwall Visual", "release_date": "2026-03-24T16:59:59-04:00", "title": "The JWST Advanced Deep Extragalactic Survey (JADES), JADES-GS-z13-1 (NIRCam Close-Up)Untitled", "description": "This image of JADES GS-z13-1 (the red dot at center), imaged with NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) as part of the JWST Advanced Deep Extragalactic Survey (JADES) program.", "hits": 470 }, { "id": 31371, "url": "https://svs.gsfc.nasa.gov/31371/", "result_type": "Hyperwall Visual", "release_date": "2026-03-10T06:59:59-04:00", "title": "Exposed Cranium", "description": "This video compares infrared views of the PMR 1 “Exposed Cranium” nebula taken by NASA’s retired Spitzer Space Telescope, as well as NASA’s James Webb Space Telecope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument).No description available.", "hits": 66 }, { "id": 14969, "url": "https://svs.gsfc.nasa.gov/14969/", "result_type": "Produced Video", "release_date": "2026-03-05T11:00:00-05:00", "title": "Introducing NASA's Roman Space Telescope", "description": "Named after NASA’s first chief astronomer, the ‘mother of the Hubble Space Telescope,’ the Nancy Grace Roman Space Telescope will have a field of view at least 100 times larger than Hubble's, potentially measuring light from a billion galaxies in its lifetime. This observatory will also be able to block starlight to directly see exoplanets and planet-forming disks, complete a statistical census of planetary systems in our galaxy, and settle essential questions in the areas of dark energy, dark matter, and infrared astrophysics.Music credit: “Fire,” by Frederick Helmut Wiedmann [GMR], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_RomanShortOverview3.jpg (1280x720) [222.3 KB] || YTframe_RomanShortOverview3_searchweb.png (320x180) [80.5 KB] || YTframe_RomanShortOverview3_thm.png (80x40) [9.6 KB] || 14969_Roman_Short_Overview_Good.mp4 (1920x1080) [109.7 MB] || 14969_Roman_Short_Overview_Best.mp4 (1920x1080) [215.6 MB] || 14969_Roman_Short_Overview_YT.mp4 (1920x1080) [523.0 MB] || 14969RomanShortOverviewCaptions.en_US.srt [2.1 KB] || 14969RomanShortOverviewCaptions.en_US.vtt [2.0 KB] || 14969_Roman_Short_Overview_ProRes_1920x1080_29.97.mov (1920x1080) [1.4 GB] || ", "hits": 535 }, { "id": 31369, "url": "https://svs.gsfc.nasa.gov/31369/", "result_type": "Hyperwall Visual", "release_date": "2026-03-02T18:59:59-05:00", "title": "Zoom into the Cats Paw Nebula", "description": "This zoom-in video shows the location of the Cat’s Paw Nebula on the sky. It begins with a ground-based photo by the late astrophotographer Akira Fujii, then shows views from the Digitized Sky Survey. Honeing in on the European Southern Observatory image of the Cat’s Paw Nebula in visible light. The video continues to zoom in on a section of the Cat’s Paw, which gradually transitions to the stunning image captured by NASA’s James Webb Space Telescope in near-infrared light.", "hits": 104 }, { "id": 14982, "url": "https://svs.gsfc.nasa.gov/14982/", "result_type": "Produced Video", "release_date": "2026-02-27T11:00:00-05:00", "title": "Deserts of Africa and the Middle East", "description": "Deserts of North Africa and the Middle East || Africa-Asia_HYPERWALL_PRINT.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_Thumb.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_Thumb.png (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_SearchWeb.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_1080.webm (1920x1080) [21.4 MB] || Africa-Asia_HYPERWALL_1080.mp4 (1920x1080) [222.6 MB] || Africa-Asia_HYPERWALL_6K.webm (5760x3240) [7.2 MB] || Africa-MiddleEast_HYPERWALL_4K.mp4 (3840x2160) [1.1 GB] || Africa-Asia_HYPERWALL_6K.mp4 (5760x3240) [5.0 GB] || ", "hits": 180 }, { "id": 14966, "url": "https://svs.gsfc.nasa.gov/14966/", "result_type": "Produced Video", "release_date": "2026-02-14T00:00:00-05:00", "title": "SPHEREx Spacecraft and Observing Animations", "description": "SPHEREx is a small, highly-capable astronomy satellite mission that will map out the entire sky in 102 colors of infrared light from its vantage point in a low-Earth orbit. The spacecraft bus is powered by Sun-facing, rectangular solar panels.The white, conical Sun shield keeps the inner telescope components at a cool temperature that enables the detectors to operate with high sensitivity. The Sun shields are faded out at the end of the sequence to provide an unobstructed view of the telescope components.Credit: NASA/JPL-CaltechWatch this video on the JPLraw YouTube channel.JPL Page || SPHEREx_SurveyAnimationShot1_Stlll.jpg (3840x2160) [658.9 KB] || SPHEREx_SurveyAnimationShot1_Stlll_searchweb.png (320x180) [63.1 KB] || SPHEREx_SurveyAnimationShot1_Stlll_thm.png (80x40) [4.5 KB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422.mov (1920x1080) [703.6 MB] || SPHEREx_Shot1_Caption.en_US.srt [49 bytes] || SPHEREx_Shot1_Caption.en_US.vtt [59 bytes] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_4K.mp4 (3840x2160) [154.7 MB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422_4K.mov (3840x2160) [2.0 GB] || ", "hits": 234 }, { "id": 31363, "url": "https://svs.gsfc.nasa.gov/31363/", "result_type": "Hyperwall Visual", "release_date": "2026-02-09T18:59:59-05:00", "title": "Observatory Comparison (Hubble/Spitzer/Webb)", "description": "This video compares images of the Helix Nebula from three NASA observatories: Hubble’s image in visible light, Spitzer’s infrared view, and Webb’s high-resolution near-infrared look.No description available.\r\n\r\nmore info: https://science.nasa.gov/asset/webb/observatory-comparison-hubble-spitzer-webb/", "hits": 394 }, { "id": 14955, "url": "https://svs.gsfc.nasa.gov/14955/", "result_type": "Produced Video", "release_date": "2026-01-27T09:00:00-05:00", "title": "NASA Tests LISA Development Units", "description": "A prototype charge management device for the future LISA (Laser Interferometer Space Antenna) mission sits on a lab bench at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The device will reduce the buildup of electric charge on the gold-platinum test masses that float freely inside each of the three LISA spacecraft. The University of Florida in Gainesville and Fibertek Inc. in McNair, Virginia, are developing the device. Credit: NASA/Dennis HenryAlt text: An instrument rests on a lab bench.Image description: A silver box with red and black connector caps on one side rests on a white lab bench with a blue mat on top. Three black cables connect to the box and another yellow cable curls around it. || GSFC_20250602_LISA_006584.jpg (8098x5399) [11.3 MB] || ", "hits": 278 }, { "id": 31362, "url": "https://svs.gsfc.nasa.gov/31362/", "result_type": "Hyperwall Visual", "release_date": "2026-01-22T18:59:59-05:00", "title": "Circinus Galaxy Zoom", "description": "This shows the location of the Circinus galaxy on the sky. It begins with a ground-based photo of the constellation Circinus. The video closes in on the Circinus galaxy, using views from the Digitized Sky Survey and the Dark Energy Survey Camera. Continueing with an image of the galaxy from NASA’s Hubble Space Telescope, zooms in even more to the image of the galaxy’s core from NASA’s James Webb Space Telescope in near-infrared light.", "hits": 56 }, { "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": 353 }, { "id": 14942, "url": "https://svs.gsfc.nasa.gov/14942/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Roman and Webb Comparison Graphics from Far and Wide", "description": "This page contains individual animation clips from the Far and Wide series. These clips all focus on the relationship between the Nancy Grace Roman and James Webb space telescopes: how they are different and how they will work together. These animations may be useful in presentations and other video products. || ", "hits": 198 }, { "id": 14943, "url": "https://svs.gsfc.nasa.gov/14943/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Additional Graphics", "description": "This page houses animation clips from the Far and Wide video series, which may be useful in presentations or other video products. || ", "hits": 147 }, { "id": 14947, "url": "https://svs.gsfc.nasa.gov/14947/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Webb Spectrum and Image Animations", "description": "These are animated versions of James Webb Space Telescope imagery and spectra. The spectra visualizations were created by the Space Telescope Science Institute and then animated at NASA's Goddard Space Flight Center. || ", "hits": 459 }, { "id": 14945, "url": "https://svs.gsfc.nasa.gov/14945/", "result_type": "Produced Video", "release_date": "2026-01-09T09:00:00-05:00", "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars", "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ", "hits": 463 }, { "id": 14937, "url": "https://svs.gsfc.nasa.gov/14937/", "result_type": "Produced Video", "release_date": "2025-12-23T11:00:00-05:00", "title": "NASA's Roman Space Telescope: Widening Our Gaze", "description": "The NASA Astrophysics fleet of spacecraft has an impressive range of capabilities. What is the next step in exploring the cosmos? The Nancy Grace Roman Space Telescope, NASA’s upcoming flagship mission, will take Hubble’s resolution and widen its infrared view to more than 100 times the coverage in every single image. Roman is a survey telescope that can peer through the Milky Way’s obscuring dust, and see faint, distant galaxies. Roman’s rigid design allows it to scan large regions of sky very quickly. Hubble would take 1,000 years to observe what Roman can see in one. Roman’s 18 4k x 4k detectors create 300-megapixel images covering an area of sky slightly larger than the full Moon. Roman will also look at the same regions of space repeatedly over time, allowing astronomers to see changes and observe temporary events like supernovae. Roman’s surveys of deep space and the center of our Milky Way galaxy will find thousands of new exoplanets, survey millions of galaxies, help us understand dark matter and dark energy, and learn more about the evolution of the universe. || ", "hits": 356 }, { "id": 14930, "url": "https://svs.gsfc.nasa.gov/14930/", "result_type": "Infographic", "release_date": "2025-12-18T10:00:00-05:00", "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles", "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel", "hits": 140 }, { "id": 14917, "url": "https://svs.gsfc.nasa.gov/14917/", "result_type": "Infographic", "release_date": "2025-12-12T10:00:00-05:00", "title": "Roman Galactic Plane Survey", "description": "No description available.", "hits": 226 }, { "id": 14916, "url": "https://svs.gsfc.nasa.gov/14916/", "result_type": "Produced Video", "release_date": "2025-12-08T09:30:00-05:00", "title": "Black Hole Eats Star: The Longest GRB Ever Seen", "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ", "hits": 603 }, { "id": 14933, "url": "https://svs.gsfc.nasa.gov/14933/", "result_type": "Produced Video", "release_date": "2025-12-04T09:00:00-05:00", "title": "XRISM Finds Elemental Bounty in Supernova Remnant", "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ", "hits": 342 }, { "id": 31358, "url": "https://svs.gsfc.nasa.gov/31358/", "result_type": "Hyperwall Visual", "release_date": "2025-11-12T18:59:59-05:00", "title": "Sagittarius B2 | NIRCam MIRI Filter comparison", "description": "NIRCam filters capture near-infrared light,the images tend to show stars more prominently with features like diffraction spikes, as stars are brighter at shorter wavelengths. MIRI (Mid-Infrared Instrument) Saggitarious A in unprecedented detail, including glowing cosmic dust heated by very young massive stars. The reddest area on the right half of MIRI’s image, known as Sagittarius B2 North, is one of the most molecularly rich regions known, but astronomers have never seen it with such clarity.", "hits": 77 }, { "id": 5557, "url": "https://svs.gsfc.nasa.gov/5557/", "result_type": "Visualization", "release_date": "2025-09-08T16:30:00-04:00", "title": "Daily Visualizations of the Largest Wildfires in the United States: 2025", "description": "Wildland fires pose significant threats to ecosystems, property, and human lives. Leveraging NASA’s satellite data, advanced models, visualization capacity and computing power, we analyze fire events, monitor how weather conditions impact fires and how regional air quality affects communities. Through this webpage we offer daily updated visualizations of the two largest active wildfires events in the continental United States throughout fire season.", "hits": 0 }, { "id": 31356, "url": "https://svs.gsfc.nasa.gov/31356/", "result_type": "Animation", "release_date": "2025-08-30T01:59:59-04:00", "title": "Cosmic Caverns in the Cat’s Paw Nebula", "description": "This visualization explores a subset of toe bean-reminiscent structures within a section of the Cat’s Paw Nebula, a massive, local star-forming region located approximately 4,000 light-years away in the constellation Scorpius.", "hits": 52 }, { "id": 14878, "url": "https://svs.gsfc.nasa.gov/14878/", "result_type": "Produced Video", "release_date": "2025-07-31T11:00:00-04:00", "title": "Installing the Roman Space Telescope Lower Instrument Sun Shade", "description": "Technicians have successfully installed two sunshields onto NASA’s Nancy Grace Roman Space Telescope’s inner segment. Along with the observatory’s Solar Array Sun Shield and Deployable Aperture Cover, the panels (together called the Lower Instrument Sun Shade), will play a critical role in keeping Roman’s instruments cool and stable as the mission explores the infrared universe. || ", "hits": 75 }, { "id": 14868, "url": "https://svs.gsfc.nasa.gov/14868/", "result_type": "Produced Video", "release_date": "2025-07-23T00:00:00-04:00", "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail", "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ", "hits": 103 }, { "id": 14867, "url": "https://svs.gsfc.nasa.gov/14867/", "result_type": "Produced Video", "release_date": "2025-07-15T14:00:00-04:00", "title": "GEMx Animations", "description": "Conceptual animation illustrating the ER-2 aircraft collecting spectroscopic mineral data over the American West. || GEMxThumbnail.png (1948x1052) [1.5 MB] || GEMxThumbnail_print.jpg (1024x553) [118.0 KB] || GEMxThumbnail_searchweb.png (320x180) [55.7 KB] || GEMxThumbnail_thm.png (80x40) [8.2 KB] || GEMx_Interface_1080p.mov (1920x1080) [37.6 MB] || GEMx_Interface_4k.mp4 (3840x2160) [36.0 MB] || GEMx_Interface_ProRes.mov (3840x2160) [4.1 GB] || ", "hits": 66 }, { "id": 14866, "url": "https://svs.gsfc.nasa.gov/14866/", "result_type": "Produced Video", "release_date": "2025-07-15T00:00:00-04:00", "title": "Cosmic Desktop & Phone Wallpapers", "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||", "hits": 31825 }, { "id": 14859, "url": "https://svs.gsfc.nasa.gov/14859/", "result_type": "Produced Video", "release_date": "2025-06-21T00:00:00-04:00", "title": "Webb Stellarium", "description": "Stellarium is an installation video designed for the Goddard Space Flight Center visitor center. It is playing temporarily in the room designed for Solarium, and installation built around Sun footage from the Solar Dynamics Observatory (SDO).\r\n\r\nStellarium sources James Webb Space Telescope imagery processed and provided by the Space Telescope Science Institute and available here.", "hits": 101 }, { "id": 14857, "url": "https://svs.gsfc.nasa.gov/14857/", "result_type": "Produced Video", "release_date": "2025-06-11T14:10:00-04:00", "title": "NASA’s Webb Reveals Galaxy Population Driving Cosmic Renovation", "description": "Symbols mark the locations of young, low-mass galaxies bursting with new stars when the universe was about 800 million years old. Using a filter sensitive to such galaxies, NASA’s James Webb Space Telescope imaged them with the help of a natural gravitational lens created by the massive galaxy cluster Abell 2744. In all, 83 young galaxies were found, but only the 20 shown here (white diamonds) were selected for deeper study. The inset zooms into one of the galaxies. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025Alt text: Animation showing the locations of young, low-mass, starburst galaxies around galaxy cluster Abell 2744.Image description:White and yellow galaxies of various sizes and shapes appear against the blackness of space. Two bright stars in our own galaxy display prominent six-spike diffraction patterns with bluish rays, visible at center left and lower left. Then 20 white diamonds sweep across the image. One diamond enlarges to reveal an image of a young, low-mass, star-forming galaxy. It looks like a green oval against a red and green checked background. The enlarged image then shrinks back, and the diamonds sweep away. The sequence loops. || Pandora_stamp_60pct.gif (600x600) [961.0 KB] || ", "hits": 270 }, { "id": 14851, "url": "https://svs.gsfc.nasa.gov/14851/", "result_type": "Produced Video", "release_date": "2025-06-04T14:00:00-04:00", "title": "GEMx Illustrations", "description": "Conceptual illustration depicting the ER-2 aircraft and the AVIRIS instrument searching for critical minerals as part of the GEMx campaign. || GEMx_Illustration_withTEXT_vFinal.png (3840x2160) [17.0 MB] || GEMx_Illustration_withTEXT_vFinal_print.jpg (1024x576) [287.6 KB] || GEMx_Illustration_withTEXT_vFinal_searchweb.png (320x180) [123.2 KB] || GEMx_Illustration_withTEXT_vFinal_thm.png (80x40) [8.2 KB] || ", "hits": 28 }, { "id": 31349, "url": "https://svs.gsfc.nasa.gov/31349/", "result_type": "Hyperwall Visual", "release_date": "2025-05-28T18:59:59-04:00", "title": "Juno images, 2024 - early 2025", "description": "Several recent images from the JunoCam and Jovian Infrared Auroral Mapper (JIRAM) instruments show volcanic hot spots on IO, polar storms and Jupiter's moon Amalthea.", "hits": 434 }, { "id": 14798, "url": "https://svs.gsfc.nasa.gov/14798/", "result_type": "Produced Video", "release_date": "2025-05-27T20:56:00-04:00", "title": "Astrophysics Multiwavelength Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos that show multiwavelength content.", "hits": 184 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 486 }, { "id": 14842, "url": "https://svs.gsfc.nasa.gov/14842/", "result_type": "B-Roll", "release_date": "2025-05-19T00:00:00-04:00", "title": "Roman Space Telescope's Outer Shell Passes Thermal Test - Drone Footage", "description": "The outer portion of the Nancy Grace Roman Space Telescope recently passed a major milestone: thermal cycling. Drone footage captures its emergence from the test facility and return to the clean room. The Roman Space Telescope is a NASA observatory designed to perform wide-field imaging and surveys of the near-infrared sky. || ", "hits": 82 }, { "id": 31346, "url": "https://svs.gsfc.nasa.gov/31346/", "result_type": "Hyperwall Visual", "release_date": "2025-05-13T13:59:59-04:00", "title": "Planetary Nebula NGC 1514: WISE vs Webb Images", "description": "Two infrared views of NGC 1514. Starting with an observation from NASA’s Wide-field Infrared Survey Explorer (WISE). Ending with a more refined image from NASA's James Webb Space Telescope.", "hits": 74 }, { "id": 14839, "url": "https://svs.gsfc.nasa.gov/14839/", "result_type": "Produced Video", "release_date": "2025-05-12T08:00:00-04:00", "title": "Webb Captures Jupiter’s Aurora", "description": "NASA’s James Webb Space Telescope has captured a spectacular light show on Jupiter — an enormous display of auroras unlike anything seen on Earth. These infrared observations reveal unexpected activity in Jupiter’s atmosphere, challenging what scientists thought they knew about the planet’s magnetic field and particle interactions. Combined with ultraviolet data from Hubble, the results have raised surprising new questions about Jupiter’s extreme environment.For more information, visit https://nasa.gov/webbCredit:Producer: Paul MorrisWriter: Thaddeus CesariNarrator: Professor Jonathan NicholsImages: NASA, ESA, CSA, STSciMusic Credit:\"Zero Gravity\" by Brice Davoli [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music || ", "hits": 102 }, { "id": 14834, "url": "https://svs.gsfc.nasa.gov/14834/", "result_type": "Produced Video", "release_date": "2025-05-12T00:00:00-04:00", "title": "Cosmic Dawn: The Untold Story of the James Webb Space Telescope", "description": "For more than three decades, NASA and an international team of scientists and engineers pushed the limits of technology, innovation, and perseverance to build and launch the James Webb Space Telescope, the most powerful space observatory ever created. Cosmic Dawn brings audiences behind the scenes with the Webb film crew, and never-before-heard testimonies revealing the real story of how this telescope overcame all odds. ||", "hits": 313 }, { "id": 31344, "url": "https://svs.gsfc.nasa.gov/31344/", "result_type": "Animation", "release_date": "2025-05-05T18:59:59-04:00", "title": "Herbig-Haro 49/50 Stellar Jets", "description": "This visualization examines the three-dimensional structure of Herbig-Haro 49/50 (HH 49/50) as seen in near- and mid-infrared light by the James Webb Space Telescope. The spiral galaxy has a prominent central bulge. The bulge also shows hints of “side lobes” suggesting that this could be a barred spiral galaxy. Reddish clumps show the locations of warm dust and groups of forming stars.Examining in three dimensions helps understand how young stars form and the environment around them.", "hits": 97 }, { "id": 20398, "url": "https://svs.gsfc.nasa.gov/20398/", "result_type": "Animation", "release_date": "2025-03-19T11:00:00-04:00", "title": "Habitable Worlds Observatory (HWO) EAC 2 Design Animations", "description": "Animations and stills of design concept EAC 2 for the Habitable Worlds Observatory", "hits": 89 }, { "id": 14783, "url": "https://svs.gsfc.nasa.gov/14783/", "result_type": "Produced Video", "release_date": "2025-02-13T12:00:00-05:00", "title": "NASA Interview Opportunity: Two Missions, One Rocket: One Shared Goal", "description": "Assocated cut b-roll will be posted by 5 p.m. EST on Monday, Feb 24. || SPHEREx_PUNCH_Live_Shots_Banner.jpg (1800x720) [495.3 KB] || SPHEREx_PUNCH_Live_Shots_Banner_print.jpg (1024x409) [260.6 KB] || SPHEREx_PUNCH_Live_Shots_Banner_searchweb.png (320x180) [111.2 KB] || SPHEREx_PUNCH_Live_Shots_Banner_thm.png [8.0 KB] || ", "hits": 58 }, { "id": 5481, "url": "https://svs.gsfc.nasa.gov/5481/", "result_type": "Visualization", "release_date": "2025-02-09T00:00:00-05:00", "title": "Science on a Sphere: VIIRS Global Fires", "description": "VIIRS Fires for Science on a Sphere || fires_SoaS_no_gaps.0001_print.jpg (1024x512) [100.3 KB] || fires_SoaS_no_gaps.0001_searchweb.png (320x180) [43.4 KB] || fires_SoaS_no_gaps (4096x2048) [1490 Item(s)] || fires_SoaS_no_gaps.0001_thm.png [5.0 KB] || fires_SoaS_no_gaps_2048p30.mp4 (4096x2048) [58.3 MB] || Colorbar || colorbar_frp3.png (1920x960) [92.5 KB] || colorbar_frp3_print.jpg (1024x512) [23.5 KB] ||", "hits": 163 }, { "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": 45 }, { "id": 14759, "url": "https://svs.gsfc.nasa.gov/14759/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman's Wide Field Instrument added to the Mirror Assembly", "description": "B-roll footage slowed from 60 frames per second and 30 frames per second of the Wide Field Instrument (WFI) installation. || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_print.jpg (1024x576) [202.4 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_searchweb.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_web.png (320x180) [103.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly_ProRes.mov (3840x2160) [35.6 MB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.03840_thm.png [6.9 KB] || 1_-_14759_-_Footage_Romans_Wide_Field_Instrument_added_to_Mirror_Assembly.mp4 (3840x2160) [3.8 GB] || ", "hits": 60 }, { "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": 48 }, { "id": 14754, "url": "https://svs.gsfc.nasa.gov/14754/", "result_type": "Produced Video", "release_date": "2025-01-16T10:14:00-05:00", "title": "NASA’s Pandora Mission Closer To Probing Alien Atmospheres", "description": "Basic overview of NASA's Pandora mission, which will revolutionize the study of exoplanet atmospheres.", "hits": 125 }, { "id": 14738, "url": "https://svs.gsfc.nasa.gov/14738/", "result_type": "Produced Video", "release_date": "2024-12-20T10:00:00-05:00", "title": "What Are Gamma-ray Bursts?", "description": "Watch to learn more about gamma-ray bursts, the most powerful explosions in the cosmos. They first came to the attention of astronomers in the 1970s when new satellites detected this surprising phenomenon. Over decades, scientists have found that these blasts could be detected somewhere in the sky almost every day, and that they were both extremely distant — the closest known is over 100 million light-years away — and enormously powerful. Gamma-ray bursts are now linked to the explosive deaths of massive stars and to mergers of compact objects, like neutron stars and black holes, but many puzzles remain. Credit: NASA’s Goddard Space Flight CenterMusic: “Time Science,” Steve Fawcett [ASCAP] and Katherine F Martin [BMI], Universal Production Music Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_ASD_GRB.jpg (1280x720) [221.2 KB] || YTframe_ASD_GRB_searchweb.png (320x180) [81.7 KB] || YTframe_ASD_GRB_thm.png (80x40) [9.6 KB] || 14738_GRBexplainer_Small.mp4 (1920x1080) [117.7 MB] || 14738_GRBexplainer_Best.mp4 (1920x1080) [526.7 MB] || 14738GRBexplainerCaptions.en_US.srt [4.4 KB] || 14738GRBexplainerCaptions.en_US.vtt [4.2 KB] || 14738_GRBexplainer_ProRes_1920x1080_2997.mov (1920x1080) [2.9 GB] || ", "hits": 345 }, { "id": 5217, "url": "https://svs.gsfc.nasa.gov/5217/", "result_type": "Visualization", "release_date": "2024-12-09T10:00:00-05:00", "title": "Northern California Fires in September 2020", "description": "This visualization shows the lightning over California on August 16 and 17, 2020 that caused 38 separate fires to ignite. These eventually combined into the August Complex fire, the first recorded gigafire in California history, which burned until November 12 consuming 1,614 square miles (4,180 square kilometers). As the lightning fades, a series of images shows the smoke emanating from the fires on September 8 of that year. The visible smoke is followed by a series showing the Aerosol Optical Depth (a unitless quantitative metric of how much smoke is present in the atmosphere) as the smoke particles were transported across the Western US and Canada over a 10 day period. || geoxo_fires_v049_2024-02-21_0939.04321_print.jpg (1024x576) [185.9 KB] || geoxo_fires_v049_2024-02-21_0939.04321_searchweb.png (320x180) [78.6 KB] || geoxo_fires_v049_2024-02-21_0939.04321_thm.png (80x40) [5.6 KB] || geoxo_fires_v049_2024-02-21_0939_p30_1080p30.mp4 (1920x1080) [101.5 MB] || geoxo_fires_v049_2024-02-21_0939_1080p60.mp4 (1920x1080) [110.3 MB] || composite (3840x2160) [0 Item(s)] || composite (3840x2160) [0 Item(s)] || geoxo_fires_v049_2024-02-21_0939_2160p60.mp4 (3840x2160) [333.3 MB] || geoxo_fires_v049_2024-02-21_0939_p30_2160p30.mp4 (3840x2160) [322.9 MB] || geoxo_fires_v049_2024-02-21_0939_p30_2160p30.mp4.hwshow || ", "hits": 95 }, { "id": 14728, "url": "https://svs.gsfc.nasa.gov/14728/", "result_type": "B-Roll", "release_date": "2024-12-06T12:00:00-05:00", "title": "Geological Earth Mapping Experiment (GEMx) B-roll", "description": "The Geological Earth Mapping Experiment (GEMx) is a joint campaign between NASA and the U.S. Geological Survey (USGS) to map portions of the southwest United States for critical minerals using advanced airborne imaging. Spectral data from hundreds of wavelengths of reflected light can provide new information about Earth’s surface and atmosphere to help scientists understand Earth’s geology and biology, as well as the effects of climate change. The research project will use NASA’s Airborne Visible/Infrared Imaging Spectrometer (AVIRIS), the Modified Daedalus Wildfire scanning spectrometer (MASTER), and other airborne spectrocopic instruments flown on NASA’s ER-2 and Gulfstream V aircraft to collect the measurements over the country’s arid and semi-arid regions, including parts of California, Nevada, Arizona, and New Mexico.GEMx VISIONS PortalGEMx Campaign Information || ", "hits": 28 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 655 }, { "id": 14650, "url": "https://svs.gsfc.nasa.gov/14650/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Infrared Detector and Spectrometer", "description": "EXCITE (EXoplanet Climate Infrared TElescope) is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during long-duration scientific balloon trips over Antarctica.These images, taken in July 2024, show Peter Nagler and Nat DeNigris preparing EXCITE’s infrared detector and installing it into the mission’s spectrometer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. At the time, the EXCITE team was gearing up for a test flight in Fort Sumner, New Mexico. || ", "hits": 42 }, { "id": 14725, "url": "https://svs.gsfc.nasa.gov/14725/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Payload Prep", "description": "In August 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both Arctic and Antarctic, with the latter offering longer duration flights optimum for observing planets for their entire orbit. || ", "hits": 71 }, { "id": 14726, "url": "https://svs.gsfc.nasa.gov/14726/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Launch and Recovery", "description": "On August 31, 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both the north and south poles, although flights over Antarctica allow for longer-duration flights at a latitude optimum for observing planets for their entire orbit. || ", "hits": 110 }, { "id": 14715, "url": "https://svs.gsfc.nasa.gov/14715/", "result_type": "Produced Video", "release_date": "2024-11-18T00:00:00-05:00", "title": "COBE Celebrates 35th Launch Anniversary", "description": "Technicians work on the COBE (Cosmic Background Explorer) spacecraft in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission launched into an Earth orbit in 1989 to make an all-sky map of the cosmic microwave background, the oldest light in the universe. The conical silver shield protects the scientific instruments from direct radiation from the Sun and Earth, isolates them from radio-frequency interference from the spacecraft transmitters and terrestrial sources, and provides thermal isolation for a dewar containing liquid helium coolant.Credit: NASA/COBE Science Team || COBE_in_gfsc_clean_room_1.jpg (1629x1600) [552.8 KB] || ", "hits": 212 }, { "id": 31323, "url": "https://svs.gsfc.nasa.gov/31323/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GOES East vs GMAO – Global GeoColor Imagery", "description": "gmao-plot-all-colorbars-goes-east-vs-gmao_print.jpg (1024x576) [168.6 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao.png (3840x2160) [6.9 MB] || gmao-plot-all-colorbars-goes-east-vs-gmao_searchweb.png (320x180) [78.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_thm.png (80x40) [6.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_1080p30.mp4 (1920x1080) [12.9 MB] ||", "hits": 49 }, { "id": 5389, "url": "https://svs.gsfc.nasa.gov/5389/", "result_type": "Visualization", "release_date": "2024-11-14T00:00:00-05:00", "title": "Tracking methane with EMIT and AVIRIS-3", "description": "Methane plumes can now be detected using the airborne AVIRIS-3 spectrometer in addition to EMIT on the International Space Station.", "hits": 153 }, { "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": 184 }, { "id": 20395, "url": "https://svs.gsfc.nasa.gov/20395/", "result_type": "Animation", "release_date": "2024-11-12T15:00:00-05:00", "title": "Habitable Worlds Observatory Additional Spacecraft Designs", "description": "The Habitable Worlds Observatory is early in its development. Many designs are under consideration. These artist's concept animations show some of the options.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": 301 }, { "id": 14716, "url": "https://svs.gsfc.nasa.gov/14716/", "result_type": "Produced Video", "release_date": "2024-11-07T13:00:00-05:00", "title": "Hurricane Helene’s Gravity Waves Revealed by NASA’s AWE", "description": "On Sept. 26, 2024, Hurricane Helene slammed into the Gulf Coast of Florida, inducing storm surges and widespread destruction on the land below. At the same time, NASA’s Atmospheric Waves Experiment (AWE), which is mounted on the outside of the International Space Station, recorded enormous swells that the hurricane produced in the atmosphere roughly 55 miles above the ground.These massive ripples through the upper atmosphere, known as atmospheric gravity waves, appear in AWE’s images as concentric bands extending away from northern Florida.Visit this page to learn more. || ", "hits": 90 }, { "id": 31319, "url": "https://svs.gsfc.nasa.gov/31319/", "result_type": "Hyperwall Visual", "release_date": "2024-10-23T00:00:00-04:00", "title": "2025 NASA Science Calendar", "description": "Images from the 2025 NASA Science Calendar", "hits": 124 }, { "id": 14698, "url": "https://svs.gsfc.nasa.gov/14698/", "result_type": "Produced Video", "release_date": "2024-10-22T11:00:00-04:00", "title": "NASA Reveals LISA Engineering Development Unit Telescope", "description": "NASA has revealed the first look at a full-scale prototype for six telescopes that will enable, in the next decade, the space-based detection of gravitational waves — ripples in space-time caused by merging black holes and other cosmic sources.The LISA (Laser Interferometer Space Antenna) mission is led by ESA (European Space Agency) in partnership with NASA to detect gravitational waves by using lasers to measure precise distances — down to picometers, or trillionths of a meter — between a trio of spacecraft distributed in a vast configuration larger than the Sun. Each side of the triangular array will measure nearly 1.6 million miles, or 2.5 million kilometers.Twin telescopes aboard each spacecraft will both transmit and receive infrared laser beams to track their companions, and NASA is supplying all six of them to the LISA mission. The prototype, called the Engineering Development Unit Telescope, will provide guidance as engineers and scientists work toward building the flight hardware.In May, the prototype, which was manufactured and assembled by L3Harris Technologies in Rochester, New York, arrived at NASA's Goddard Space Flight Center in Greenbelt, Maryland. The primary mirror is coated in gold to better reflect the infrared lasers and to reduce heat loss from a surface exposed to cold space since the telescope will operate best when close to room temperature. The prototype is made entirely from an amber-colored glass-ceramic called Zerodur, manufactured by Schott in Mainz, Germany. The material is widely used for telescope mirrors and other applications requiring high precision because its shape changes very little over a wide range of temperatures. || ", "hits": 99 }, { "id": 14681, "url": "https://svs.gsfc.nasa.gov/14681/", "result_type": "Produced Video", "release_date": "2024-10-01T11:00:00-04:00", "title": "Launch Your Creativity with Space Crafts", "description": "In honor of the completion of our Nancy Grace Roman Space Telescope’s spacecraft — the vehicle that will maneuver the observatory to its place in space and enable it to function once there — we’re bringing you some space crafts you can complete at home! || ", "hits": 78 }, { "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": 309 }, { "id": 5373, "url": "https://svs.gsfc.nasa.gov/5373/", "result_type": "Visualization", "release_date": "2024-09-03T13:00:00-04:00", "title": "PREFIRE First Light", "description": "Visualization emphasizing two passes of PREFIRE over Greenland. Information about the rates of atmospheric emission can be derived from the change in emission at the intersection of the passes. || prefire_first_light_FINAL_2160p30.00450_print.jpg (1024x576) [224.8 KB] || prefire_first_light_FINAL_2160p30.00450_thm.png (80x40) [6.3 KB] || prefire_first_light_FINAL_2160p30.00450_searchweb.png (320x180) [78.7 KB] || prefire_first_light_FINAL [0 Item(s)] || prefire_first_light_FINAL_1080p30.mp4 (1920x1080) [47.2 MB] || prefire_first_light_FINAL_4K [0 Item(s)] || prefire_first_light_FINAL_2160p30.mp4 (3840x2160) [133.7 MB] || prefire_first_light_FINAL_2160p30.mp4.hwshow [199 bytes] || ", "hits": 73 }, { "id": 14658, "url": "https://svs.gsfc.nasa.gov/14658/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible Light || PRINT.jpg (1920x1080) [298.3 KB] || THUMB.jpg (1920x1080) [298.3 KB] || SEARCH.jpg (320x180) [27.0 KB] || Flight_Through_the_Orion_Nebula_in_Visible_Light_Dome_Version.mp4 (1920x1080) [225.5 MB] || 3840x3840_1x1_60p [0 Item(s)] || ", "hits": 159 }, { "id": 14661, "url": "https://svs.gsfc.nasa.gov/14661/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Infrared Light || PRINT.jpg (1920x1080) [206.5 KB] || THUMB.jpg (1920x1080) [206.5 KB] || SEARCH.jpg (320x180) [22.2 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.1 MB] || ", "hits": 68 }, { "id": 14662, "url": "https://svs.gsfc.nasa.gov/14662/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible and Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible and Infrared Light || PRINT.jpg (1920x1080) [159.4 KB] || THUMB.jpg (1920x1080) [159.4 KB] || SEARCH.jpg (320x180) [18.5 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Visible_and_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.3 MB] || ", "hits": 155 }, { "id": 31304, "url": "https://svs.gsfc.nasa.gov/31304/", "result_type": "Hyperwall Visual", "release_date": "2024-08-06T00:00:00-04:00", "title": "Take a Cosmic Road Trip this Summer with Chandra and Webb", "description": "Images combining data from NASA’s Chandra and Webb telescopes, of a cloud complex, a region of star formation, a spiral galaxy, and a galaxy cluster. || chandrawebb3-hw_print.jpg (1024x576) [176.0 KB] || chandrawebb3-hw_searchweb.png (320x180) [65.0 KB] || chandrawebb3-hw_thm.png (80x40) [6.0 KB] || chandrawebb3-hw.tif (5760x3240) [53.4 MB] || take-a-cosmic-road-trip-this-summer-with-chandra-and-webb.hwshow [311 bytes] || ", "hits": 67 }, { "id": 14603, "url": "https://svs.gsfc.nasa.gov/14603/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "NICER Hardware and Patch Kit", "description": "This video shows different components of NICER (Neutron star Interior Composition Explorer). The damaged thermal shield is a flight spare used during the patch testing process.0:00 A NICER patch slowly rotates counterclockwise. 0:14 A top-down view of the same patch, still rotating. 0:21 Another side view of the patch rotating. A gloved hand enters from the right-hand side, picks up the patch, and turns it on its side. The patch begins rotating again, so the tab on the bottom becomes visible. 1:03 A gloved hand slowly tilts a damaged thermal shield. 1:41 The thermal shield rests in a container that slowly rotates. 2:08 A gloved hand rotates a NICER X-ray concentrator. 2:30The camera moves past the X-ray concentrator. 2:52 A hand places a NICER sunshade on the table. 2:58 The sunshade rotates counterclockwise. 3:00 The sunshade rotates on its side.Credit:NASA/Sophia Roberts and Scott Wiessinger || Studio_Shoot_Single_Components.00001_print.jpg (1024x540) [16.9 KB] || Studio_Shoot_Single_Components.00001_searchweb.png (320x180) [23.1 KB] || Studio_Shoot_Single_Components.00001_thm.png (80x40) [2.1 KB] || Studio_Shoot_Single_Components.mp4 (4096x2160) [1.9 GB] || Studio_Shoot_Single_Components.mov (4096x2160) [12.7 GB] || ", "hits": 31 }, { "id": 31299, "url": "https://svs.gsfc.nasa.gov/31299/", "result_type": "Hyperwall Visual", "release_date": "2024-07-24T00:00:00-04:00", "title": "The Penguin and the Egg (Interacting Galaxies Arp 142)", "description": "ARP 142 as seen by Hubble vs. Webb || penguin-and-the-egg_print.jpg (1024x576) [59.0 KB] || penguin-and-the-egg.png (3840x2160) [4.6 MB] || penguin-and-the-egg_searchweb.png (320x180) [30.6 KB] || penguin-and-the-egg_thm.png (80x40) [2.5 KB] || penguin-and-the-egg_1080p.mp4 (1920x1080) [10.1 MB] || penguin-and-the-egg_1080p.webm (1920x1080) [1.5 MB] || penguin-and-the-egg_4k.mp4 (3840x2160) [31.2 MB] || the-penguin-and-the-egg-4k.hwshow [292 bytes] || the-penguin-and-the-egg-1080p.hwshow [301 bytes] || ", "hits": 93 }, { "id": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 331 }, { "id": 31290, "url": "https://svs.gsfc.nasa.gov/31290/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb and Hubble's Views of Spiral Galaxy NGC 628", "description": "animated comparison || NGC_628-HST_Webb-1080p.00001_print.jpg (1024x576) [334.0 KB] || NGC_628-HST_Webb-1080p.mp4 (1920x1080) [58.7 MB] || NGC_628-HST_Webb-4k.mp4 (3840x2160) [221.7 MB] || webb-and-hubbles-views-of-spiral-galaxy-ngc-628-4k-movie.hwshow [350 bytes] || ", "hits": 402 }, { "id": 31291, "url": "https://svs.gsfc.nasa.gov/31291/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb Identifies Tiniest Free-Floating Brown Dwarf", "description": "This image from the NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope shows the central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs: objects too small to be stars but larger than most planets. They found three brown dwarfs that are less than eight times the mass of Jupiter. The smallest weighs just three to four times Jupiter, challenging theories for star formation.The wispy curtains filling the image are interstellar material reflecting the light from the cluster’s stars – what is known as a reflection nebula. The material also includes carbon-containing molecules known as polycyclic aromatic hydrocarbons, or PAHs. The bright star closest to the center of the frame is actually a pair of type B stars in a binary system, which are the most massive stars in the cluster. Winds from these stars may help sculpt the large loop seen on the right side of the field of view. || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_print.jpg (1024x1372) [393.6 KB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam.png (3788x5077) [24.7 MB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam-hw.png (3840x2160) [4.8 MB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_searchweb.png (320x180) [111.1 KB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_thm.png (80x40) [14.4 KB] || webb-identifies-tiniest-free-floating-brown-dwarf-nircam.hwshow [364 bytes] || ", "hits": 143 }, { "id": 31292, "url": "https://svs.gsfc.nasa.gov/31292/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb Probes an Extreme Starburst Galaxy", "description": "Starburst galaxy M82 was observed by the Hubble Space Telescope in 2006, which showed the galaxy’s edge-on spiral disk, shredded clouds, and hot hydrogen gas. The James Webb Space Telescope has observed M82’s core, capturing in unprecedented detail the structure of the galactic wind and characterizing individual stars and star clusters.The Webb image is from the telescope’s NIRCam (Near-Infrared Camera) instrument. The red filaments trace the shape of the cool component of the galactic wind via polycyclic aromatic hydrocarbons (PAHs). PAHs are very small dust grains that survive in cooler temperatures but are destroyed in hot conditions. The structure of the emission is similar to that of the ionized gas, suggesting PAHs may be replenished from cooler molecular material as it is ionized. || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_print.jpg (1024x576) [178.7 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw.png (3840x2160) [10.9 MB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_searchweb.png (320x180) [74.1 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_thm.png (80x40) [5.4 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset.png (16260x7030) [87.9 MB] || webb-probes-an-extreme-starburst-galaxy-hst-v-webb.hwshow [356 bytes] || ", "hits": 54 }, { "id": 31293, "url": "https://svs.gsfc.nasa.gov/31293/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Hubble Telescopes Affirm Universe's Expansion Rate", "description": "This image of NGC 5468, a galaxy located about 130 million light-years from Earth, combines data from the Hubble and James Webb space telescopes. This is the farthest galaxy in which Hubble has identified Cepheid variable stars. These are important milepost markers for measuring the expansion rate of the universe. The distance calculated from Cepheids has been cross-correlated with a type Ia supernova in the galaxy. Type Ia supernovae are so bright they are used to measure cosmic distances far beyond the range of the Cepheids, extending measurements of the universe's expansion rate deeper into space.CreditsNASA, ESA, CSA, STScI, Adam G. Riess (JHU, STScI) || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_print.jpg (1024x576) [160.4 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb.png (3214x3233) [16.1 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw.png (3840x2160) [7.7 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_searchweb.png (320x180) [58.9 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_thm.png (80x40) [8.5 KB] || webb-hubble-telescopes-affirm-universes-expansion-rate.hwshow [366 bytes] || ", "hits": 287 }, { "id": 31285, "url": "https://svs.gsfc.nasa.gov/31285/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "The Webb Space Telescope Studies the \"Cosmic Cliffs\" in NGC 3324", "description": "The seemingly three-dimensional “Cosmic Cliffs” showcases Webb’s capabilities to peer through obscuring dust and shed new light on how stars form. Webb reveals emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. This landscape of “mountains” and “valleys” is actually the edge of a nearby stellar nursery called NGC 3324 at the northwest corner of the Carina Nebula.So-called mountains — some towering about 7 light-years high — are speckled with glittering, young stars imaged in infrared light. A cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located above the area shown in this image. The blistering, ultraviolet radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Dramatic pillars rise above the glowing wall of gas, resisting this radiation. The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation.Objects in the earliest, rapid phases of star formation are difficult to capture, but Webb’s extreme sensitivity, spatial resolution and imaging capability can chronicle these elusive events. || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_print.jpg (1024x593) [318.7 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution.png (3840x2224) [10.2 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png (14575x8441) [113.7 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_searchweb.png (320x180) [116.3 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_thm.png (80x40) [13.5 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png.dzi [179 bytes] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png_files [4.0 KB] || the-webb-space-telescope-studies-the-cosmic-cliffs-in-ngc-3324-still.hwshow [430 bytes] || ", "hits": 374 }, { "id": 31287, "url": "https://svs.gsfc.nasa.gov/31287/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "Webb and Hubble Combine to Create Most Colorful View of Universe", "description": "This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope. To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies that could be described as one of the most colorful views of the universe ever created.MACS0416 is a galaxy cluster located about 4.3 billion light-years from Earth, meaning that light we see now left the cluster shortly after the formation of our solar system. This cluster magnifies the light from more distant background galaxies through gravitational lensing. As a result, the research team has been able to identify magnified supernovae and even very highly magnified individual stars.Those colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amount of dust, as detected by Webb. The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes.In this image, blue represents data at wavelengths of 0.435 and 0.606 microns (Hubble filters F435W and F606W); cyan is 0.814, 0.9, and 1.05 microns (Hubble filters F814W, and F105W and Webb filter F090W); green is 1.15, 1.25, 1.4, 1.5, and 1.6 microns (Hubble filters F125W, F140W, and F160W, and Webb filters F115W and F150W); yellow is 2.00 and 2.77 microns (Webb filters F200W, and F277W); orange is 3.56 microns (Webb filter F356W); and red represents data at 4.1 and 4.44 microns (Webb filters F410M and F444W). || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_print.jpg (1024x949) [349.8 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite.png (4457x4133) [34.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite-hw.png (3840x2160) [9.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_searchweb.png (320x180) [105.9 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_thm.png (80x40) [13.0 KB] || webb-and-hubble-combine-to-create-most-colorful-view-of-universe-composite-image.hwshow [394 bytes] || ", "hits": 256 }, { "id": 31289, "url": "https://svs.gsfc.nasa.gov/31289/", "result_type": "Hyperwall Visual", "release_date": "2024-06-07T00:00:00-04:00", "title": "Webb Depicts Staggering Structure in 19 Nearby Spiral Galaxies", "description": "Collection of 19 face-on spiral galaxies from the James Webb Space Telescope in near- and mid-infrared light || STScI-01HM9N7MFNS25D041H5YFKHE0J_print.jpg (1024x1024) [652.8 KB] || STScI-01HM9N7MFNS25D041H5YFKHE0J.png (4500x4500) [31.7 MB] || STScI-01HM9N7MFNS25D041H5YFKHE0J_searchweb.png (320x180) [119.4 KB] || STScI-01HM9N7MFNS25D041H5YFKHE0J_thm.png (80x40) [15.0 KB] || webb-depicts-staggering-structure-in-19-nearby-spiral-galaxies.hwshow [71 bytes] || ", "hits": 261 }, { "id": 31286, "url": "https://svs.gsfc.nasa.gov/31286/", "result_type": "Hyperwall Visual", "release_date": "2024-05-28T00:00:00-04:00", "title": "Webb Space Telescope Studies the Pillars of Creation", "description": "Webb MIRI ImageNASA’s James Webb Space Telescope’s mid-infrared view of the Pillars of Creation strikes a chilling tone. Thousands of stars that exist in this region disappear – and seemingly endless layers of gas and dust become the centerpiece.The detection of dust by Webb’s Mid-Infrared Instrument (MIRI) is extremely important – dust is a major ingredient for star formation. Many stars are actively forming in these dense blue-gray pillars. When knots of gas and dust with sufficient mass form in these regions, they begin to collapse under their own gravitational attraction, slowly heat up – and eventually form new stars.Although the stars appear missing, they aren’t. Stars typically do not emit much mid-infrared light. Instead, they are easiest to detect in ultraviolet, visible, and near-infrared light. In this MIRI view, two types of stars can be identified. The stars at the end of the thick, dusty pillars have recently eroded the material surrounding them. They show up in red because their atmospheres are still enshrouded in cloaks of dust. In contrast, blue tones indicate stars that are older and have shed most of their gas and dust.Mid-infrared light also details dense regions of gas and dust. The red region toward the top, which forms a delicate V shape, is where the dust is both diffuse and cooler. And although it may seem like the scene clears toward the bottom left of this view, the darkest gray areas are where densest and coolest regions of dust lie. Notice that there are many fewer stars and no background galaxies popping into view.Webb’s mid-infrared data will help researchers determine exactly how much dust is in this region – and what it’s made of. These details will make models of the Pillars of Creation far more precise. Over time, we will begin to more clearly understand how stars form and burst out of these dusty clouds over millions of years. || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars.png (1987x1817) [4.1 MB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_print.jpg (1024x576) [125.2 KB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres.png (3840x2160) [4.3 MB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_searchweb.png (320x180) [65.3 KB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_thm.png (80x40) [7.3 KB] || webb-space-telescope-studies-the-pillars-of-creation.hwshow [368 bytes] || ", "hits": 352 }, { "id": 31284, "url": "https://svs.gsfc.nasa.gov/31284/", "result_type": "Hyperwall Visual", "release_date": "2024-05-27T00:00:00-04:00", "title": "The Webb Space Telescope Studies the Southern Ring Nebula", "description": "Webb Space Telescope NIRCam image || southern-ring-nebula_00433_print.jpg (1024x576) [198.6 KB] || southern-ring-nebula_00433.png (3840x2160) [8.6 MB] || NGC_3132_webb_NIRCam-STScI-01G8GZQ3ZFJRD8YF8YZWMAXCE3.png (4833x4501) [21.3 MB] || southern-ring-nebula_00433_searchweb.png (320x180) [90.4 KB] || southern-ring-nebula_00433_thm.png (80x40) [6.2 KB] || the-webb-space-telescope-studies-the-southern-ring-nebula-nircam-view.hwshow [274 bytes] || ", "hits": 148 }, { "id": 14594, "url": "https://svs.gsfc.nasa.gov/14594/", "result_type": "Animation", "release_date": "2024-05-17T00:00:00-04:00", "title": "Habitable Worlds Observatory Beauty Pass Animations and Stills", "description": "Artist's concept of one design for the proposed Habitable Worlds Observatory. Still image includes option with transparent background. || S8.jpg (3840x2160) [685.1 KB] || S8_alpha_00000.png (3840x2160) [1.5 MB] || S8.png (3840x2160) [4.9 MB] || S8_searchweb.png (320x180) [67.8 KB] || S8_thm.png (80x40) [4.4 KB] || AC1_BeautyPass_4K_V2.mp4 [68.5 MB] || AC1_BeautyPass_4K_V2.mov [1.0 GB] || ", "hits": 84 }, { "id": 14591, "url": "https://svs.gsfc.nasa.gov/14591/", "result_type": "Produced Video", "release_date": "2024-05-16T12:00:00-04:00", "title": "Quickshot: Twin NASA Spacecraft Headed To Ends Of The Earth Launching May 22", "description": "Scroll down page to see pre-recorded soundbites available for download + animations of the satellites.Check out 5 Things to Know About NASA’s Tiny Twin Polar Satellites ! || Screenshot_2024-05-14_at_4.19.48_PM.png (3360x844) [4.6 MB] || Screenshot_2024-05-14_at_4.19.48_PM_print.jpg (1024x257) [95.7 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_print.jpg (1024x257) [53.8 KB] || Screenshot_2024-05-14_at_4.19.48_PM_web.png (320x80) [53.4 KB] || Screenshot_2024-05-14_at_4.19.48_PM_thm.png (80x40) [10.8 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_searchweb.png (320x180) [94.5 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_thm.png (80x40) [10.3 KB] || ", "hits": 32 }, { "id": 5257, "url": "https://svs.gsfc.nasa.gov/5257/", "result_type": "Visualization", "release_date": "2024-04-12T00:00:00-04:00", "title": "04/08/24 Total Solar Eclipse: NOAA GOES-East True Color Imagery", "description": "A true color view of the Earth from GOES-16 (GOES-East) from 2024/04/08 15:00 UTC to 2024/04/08 20:30 UTC. This view of the Americas captures the passage of the total solar eclipse over North America on 04/08/2024. || PR_WorldView_geostationary_east_2160x2160_en.00200_print.jpg (1024x1024) [322.2 KB] || PR_WorldView_geostationary_east_2160x2160_en.00200_searchweb.png (320x180) [126.2 KB] || PR_WorldView_geostationary_east_2160x2160_en.00200_thm.png (80x40) [8.2 KB] || PR_WorldView_geostationary_east_2160x2160_en.mp4 (2160x2160) [48 bytes] || ", "hits": 72 }, { "id": 14521, "url": "https://svs.gsfc.nasa.gov/14521/", "result_type": "Produced Video", "release_date": "2024-03-12T10:00:00-04:00", "title": "Using Infrared to Survey Our Galaxy’s Far Side", "description": "Observatories with smaller views of space have provided exquisite images of other galaxies, revealing complex structures. But studying our own galaxy’s anatomy is surprisingly difficult. The plane of the Milky Way covers such a large area on the sky that studying it in detail can take a very long time. Astronomers also must peer through thick dust that obscures distant starlight. Infrared light can pass through that dust and is a key tool for learning about the far side of our galaxy.Credit: NASA's Goddard Space Flight CenterMusic: \"Time Shift Equalibrium\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || GalacticPlaneIR_Split_Still.jpg (1920x1080) [430.6 KB] || GalacticPlaneIR_Split_Still_searchweb.png (320x180) [103.4 KB] || GalacticPlaneIR_Split_Still_thm.png (80x40) [7.6 KB] || 14521_Galactic_Plane_Infrared_good.mp4 (1920x1080) [51.0 MB] || 14521_GalacticPlaneIR_SRT_Captions.en_US.srt [1.0 KB] || 14521_GalacticPlaneIR_SRT_Captions.en_US.vtt [1.0 KB] || 14521_Galactic_Plane_Infrared_ProRes_1920x1080_30.mov (1920x1080) [923.1 MB] || 14521_Galactic_Plane_Infrared_Best.mp4 (1920x1080) [106.4 MB] || ", "hits": 132 }, { "id": 5234, "url": "https://svs.gsfc.nasa.gov/5234/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "AIRS Global Carbon Dioxide (CO₂) measurements (2002-October 2023)", "description": "Data visualization showing the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft over a 20 year timespan.", "hits": 176 }, { "id": 5113, "url": "https://svs.gsfc.nasa.gov/5113/", "result_type": "Visualization", "release_date": "2024-03-01T14:00:00-05:00", "title": "Active Fires As Observed by VIIRS, 2024-Present", "description": "This animated visualization uses a moving five-day window of VIIRS measurments of fire radiative power (FRP), to present a view of fire intensities around the globe. || fires_frp_VIIRS.892_print.jpg (1024x512) [71.9 KB] || fires_frp_VIIRS.892_searchweb.png (320x180) [37.8 KB] || fires_frp_VIIRS.892_web.png (320x160) [33.5 KB] || fires_frp_VIIRS.892_thm.png (80x40) [4.3 KB] || fires_frp_VIIRS_2048p30.mp4 (4096x2048) [46.5 MB] || EIC (4096x2048) [824 Item(s)] || VIIRS_fires_latest.exr [7.0 MB] || ", "hits": 235 }, { "id": 31274, "url": "https://svs.gsfc.nasa.gov/31274/", "result_type": "Hyperwall Visual", "release_date": "2024-02-01T00:00:00-05:00", "title": "The Creation of Pillars", "description": "A Hyperwall ready version of the Space Telescope Science Institute video originally published at www.youtube.com/watch?v=Slx91ASCiXwA behind the scenes look at producing a scientific visualization of the famous Pillars of Creation in the Eagle Nebula.The AstroViz Project of NASA's Universe of Learning is creating an exploration into the iconic Pillars of Creation in the Eagle Nebula. This production reel provides a peek into the underlying science, the 2D image processing, and the development of 3D volumetric models of these star-forming wonders using visible and infrared data from the Hubble and Webb Space Telescopes. || ", "hits": 101 }, { "id": 31273, "url": "https://svs.gsfc.nasa.gov/31273/", "result_type": "Hyperwall Visual", "release_date": "2024-01-31T00:00:00-05:00", "title": "NASA Telescopes Chase Down \"Green Monster\" in Star's Debris", "description": "Animations of images originally published at https://chandra.harvard.edu/photo/2024/casa/ and https://www.nasa.gov/image-article/nasa-telescopes-chase-down-green-monster-in-stars-debris/.Astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure called the “Green Monster”. Composite images from Chandra, Webb, Hubble, NuSTAR, and Spitzer reveal where elements such as silicon, iron, and titanium are located. Comparing where certain elements are with the location of the blast wave, researchers conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it. || ", "hits": 32 }, { "id": 31271, "url": "https://svs.gsfc.nasa.gov/31271/", "result_type": "Hyperwall Visual", "release_date": "2024-01-26T00:00:00-05:00", "title": "Webb Views the Outer Planets", "description": "Images by Webb’s Near-Infrared Camera (NIRCam) show Jupiter, Saturn, Uranus, and Neptune. || ", "hits": 210 }, { "id": 14727, "url": "https://svs.gsfc.nasa.gov/14727/", "result_type": "Produced Video", "release_date": "2024-01-22T00:00:00-05:00", "title": "Fort Sumner, New Mexico: 2024 Drone Views", "description": "This clip contains various shots of the NASA payload processing facility at Fort Sumner as well as general views of the surrounding area, acquired Aug. 23, 2024. Credit: NASA/Francis ReddyVideo playback is at half speed (30 fps). 0:00 A slow, early morning approach to the staging facility as its doors open, revealing the EXCITE (EXoplanet Climate Infrared TElescope) payload. 0:45 The camera descends, with the rising sun moving behind the staging facility. 0:58 A closer, lower approach to the EXCITE payload. 1:10 A higher, more distant arc that starts by showing the low sun and the NASA sign on the staging facility, moving north. 1:41 A slow ascent looking toward EXCITE and the morning sun. 1:28 Hovering as the doors close on EXCITE. 03:20 Overview flying back across the airport revealing various vehicles and structures. 4:41 Similar, but at higher altitude and flying in a different direction. || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.00001_print.jpg (1024x576) [139.0 KB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.webm (3840x2160) [67.5 MB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.mp4 (3840x2160) [2.9 GB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility_ProRes.mov (3840x2160) [22.1 GB] || ", "hits": 54 }, { "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": 256 }, { "id": 5185, "url": "https://svs.gsfc.nasa.gov/5185/", "result_type": "Visualization", "release_date": "2023-12-07T15:00:00-05:00", "title": "PACE orbit with Ocean Color Instrument (OCI) data", "description": "PACE orbiting Earth with Ocean Color Instrument (OCI) swath revealed below || pace_orbit_swath.45_OCIonly_2023-10-27_1527.08000_print.jpg (1024x576) [73.1 KB] || pace_orbit_swath.45_OCIonly_2023-10-27_1527.08000_searchweb.png (320x180) [34.6 KB] || pace_orbit_swath.45_OCIonly_2023-10-27_1527.08000_thm.png (80x40) [3.5 KB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || pace_orbit_swath.45_OCIonly_2023-10-27_1527_2160p60.mp4 (3840x2160) [24.0 MB] || ", "hits": 57 }, { "id": 5177, "url": "https://svs.gsfc.nasa.gov/5177/", "result_type": "Visualization", "release_date": "2023-12-07T00:00:00-05:00", "title": "Polarimetry Data (HARP) and PACE orbit", "description": "This visualization begins with a view of several HARP sample data swaths depicting total radiance and polarized radiance with feature callouts. The camera then pulls back to reveal the PACE spacecraft orbit HARP2 instrument swath (shown in orange). || pace_polarimetry.02020_print.jpg (1024x576) [141.8 KB] || pace_polarimetry.02020_searchweb.png (320x180) [70.1 KB] || pace_polarimetry.02020_thm.png (80x40) [5.3 KB] || pace_polarimetry_1080p60.mp4 (1920x1080) [43.4 MB] || pace_polarimetry (3840x2160) [512.0 KB] || pace_polarimetry_2160p30.mp4 (3840x2160) [118.7 MB] || pace_polarimetry_2160p60.mp4 (3840x2160) [126.6 MB] || pace_polarimetry_prores.mov (3840x2160) [6.8 GB] || ", "hits": 48 }, { "id": 14452, "url": "https://svs.gsfc.nasa.gov/14452/", "result_type": "Produced Video", "release_date": "2023-11-08T00:00:00-05:00", "title": "Roman's Galactic Bulge Time Domain Survey Graphics", "description": "For the Galactic Bulge Time Domain Survey, Roman will aim its expansive view at the center of our galaxy and observe a two-square-degree region in infrared wavelengths that cut through the obscuring dust to reveal millions of stars. || Galactic_Bulge_Survey_Intro_ProRes_3840x2160_2997.00177_print.jpg (1024x576) [78.6 KB] || Galactic_Bulge_Survey_Intro_ProRes_3840x2160_2997.00177_searchweb.png (320x180) [59.3 KB] || Galactic_Bulge_Survey_Intro_ProRes_3840x2160_2997.00177_thm.png (80x40) [4.6 KB] || Galactic_Bulge_Survey_Intro_1080.mp4 (1920x1080) [25.1 MB] || Galactic_Bulge_Survey_Intro_1080.webm (1920x1080) [2.3 MB] || Galactic_Bulge_Survey_Intro_4k.mp4 (3840x2160) [33.3 MB] || Galactic_Bulge_Survey_Intro_ProRes_3840x2160_2997.mov (3840x2160) [1.4 GB] || ", "hits": 158 }, { "id": 14438, "url": "https://svs.gsfc.nasa.gov/14438/", "result_type": "Produced Video", "release_date": "2023-10-24T10:00:00-04:00", "title": "Why NASA's Roman Mission Will Study Milky Way's Flickering Lights", "description": "Watch this video to learn about time-domain astronomy and how time will be a key element in the Nancy Grace Roman Space Telescope's galactic bulge survey.Music: \"Elapsing Time\" and \"Beyond Truth\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_TDA-GBS_Still.jpg (1920x1080) [716.0 KB] || Roman_TDA-GBS_Still_print.jpg (1024x576) [206.4 KB] || Roman_TDA-GBS_Still_searchweb.png (320x180) [95.5 KB] || Roman_TDA-GBS_Still_thm.png (80x40) [7.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Sub100.mp4 (1920x1080) [91.9 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.webm (1920x1080) [32.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.mp4 (1920x1080) [215.7 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Best.mp4 (1920x1080) [744.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Captions.en_US.srt [6.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || ", "hits": 86 }, { "id": 5173, "url": "https://svs.gsfc.nasa.gov/5173/", "result_type": "Visualization", "release_date": "2023-10-10T00:00:00-04:00", "title": "Earth's Radiation Balance, 2000-2023", "description": "A plotted view of planetary heat uptake since the beginning of the CERES data record showing an oscillating, monthly mean (yellow) and twelve-month running average (red line). These data show how much energy is added (absorbed) by Earth during the CERES period. || planetary_heat_anomaly.1800_print.jpg (1024x576) [69.7 KB] || planetary_heat_anomaly.1800_searchweb.png (320x180) [21.2 KB] || planetary_heat_anomaly.1800_thm.png (80x40) [3.0 KB] || phu_2023 (3840x2160) [0 Item(s)] || planetary_heat_anomaly_2160p60.mp4 (3840x2160) [4.2 MB] || ", "hits": 358 }, { "id": 14402, "url": "https://svs.gsfc.nasa.gov/14402/", "result_type": "Produced Video", "release_date": "2023-09-20T13:00:00-04:00", "title": "Simulated Gravitational Wave All-Sky Image", "description": "Watch as gravitational waves from a simulated population of compact binary systems combine into a synthetic map of the entire sky. Such systems contain white dwarfs, neutron stars, or black holes in tight orbits. Maps like this using real data will be possible once space-based gravitational wave observatories become active in the next decade. The center of our Milky Way galaxy lies at the center of this all-sky view, with the galactic plane extending across the middle. Brighter spots indicate sources with stronger signals and lighter colors indicate those with higher frequencies. Larger colored patches show sources whose positions are less well known. The inset shows the frequency and strength of the gravitational signal, as well as the sensitivity limit for LISA (Laser Interferometer Space Antenna), an observatory now being designed by ESA (European Space Agency) in collaboration with NASA for launch in the 2030s.Credit: NASA’s Goddard Space Flight CenterMusic: \"Shadowless\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || LISA_AllSky_withInset_Still.jpg (2985x1497) [795.1 KB] || LISA_AllSky_1080.mp4 (1920x1080) [22.8 MB] || LISA_AllSky_1080.webm (1920x1080) [2.5 MB] || LISA_AllSky_4k.mp4 (3840x2160) [60.4 MB] || LISA_AllSky_SRT_Captions.en_US.srt [205 bytes] || LISA_AllSky_SRT_Captions.en_US.vtt [218 bytes] || LISA_AllSky_ProRes_3840x2160_30.mov (3840x2160) [992.4 MB] || ", "hits": 85 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 342 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 335 } ] }