{ "count": 515, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=dust", "previous": null, "results": [ { "id": 31395, "url": "https://svs.gsfc.nasa.gov/31395/", "result_type": "Hyperwall Visual", "release_date": "2026-05-30T18:59:59-04:00", "title": "Psyche Mission", "description": "Psyche is a NASA mission to study a metal-rich asteroid with the same name, located in the main asteroid belt between Mars and Jupiter. This is NASA’s first mission to study an asteroid that has more metal than rock or ice. No description available.", "hits": 212 }, { "id": 15042, "url": "https://svs.gsfc.nasa.gov/15042/", "result_type": "Produced Video", "release_date": "2026-05-21T11:00:00-04:00", "title": "How NASA Uses Light to Detect Waste From Mines", "description": "Tens of thousands of abandoned mines threaten waterways across the American West, but identifying which sites urgently need cleanup is slow and expensive. Now, NASA’s EMIT instrument can analyze the unique light signatures of mine waste from space to help focus remediation efforts where they're needed most.", "hits": 273 }, { "id": 15040, "url": "https://svs.gsfc.nasa.gov/15040/", "result_type": "Produced Video", "release_date": "2026-05-18T00:00:00-04:00", "title": "NASA Interview Opportunity: Catch Last Look at NASA’s Newest Space Telescope", "description": "Scroll down to cut associated b-roll. || final_final_studio_Catch_One_Last_Look_of_NASA’s_New_Space_Telescope_4_Large.jpeg (1280x640) [262.4 KB] || final_final_studio_Catch_One_Last_Look_of_NASA’s_New_Space_Telescope_4_Large_print.jpg (1024x512) [194.9 KB] || final_final_studio_Catch_One_Last_Look_of_NASA’s_New_Space_Telescope_4_Large_searchweb.png (320x180) [109.7 KB] || final_final_studio_Catch_One_Last_Look_of_NASA’s_New_Space_Telescope_4_Large_thm.png (80x40) [8.5 KB] || ", "hits": 244 }, { "id": 31393, "url": "https://svs.gsfc.nasa.gov/31393/", "result_type": "Hyperwall Visual", "release_date": "2026-05-05T06:59:59-04:00", "title": "Messier 101", "description": "A stunning view of M101, also known as the Pinwheel galaxy, one of the largest images Hubble has captured of a spiral galaxy. Assembled from 51 exposures taken over nearly ten years, this infrared and visible-light image measures 16,000 by 12,000 pixels. Ground-based images were used to fill in the portions of the galaxy. The heart of Messier 101, or the Pinwheel Galaxy, shines in this image that combines data from NASA’s Hubble Space Telescope and James Webb Space Telescope.", "hits": 262 }, { "id": 5599, "url": "https://svs.gsfc.nasa.gov/5599/", "result_type": "Visualization", "release_date": "2026-04-21T15:00:00-04:00", "title": "PACE Data Tour - Visualizations", "description": "A tour of PACE data products", "hits": 155 }, { "id": 15002, "url": "https://svs.gsfc.nasa.gov/15002/", "result_type": "Produced Video", "release_date": "2026-04-20T09:55:00-04:00", "title": "\"Cosmic Sea Slug\" Appears in Hubble’s 36th Birthday Image", "description": "NASA is celebrating the 36th anniversary of the Hubble Space Telescope with a stunning new look at the Trifid Nebula, a star-forming region about 5,000 light-years away. Powerful ultraviolet light from massive stars has carved out this glowing bubble, triggering new waves of star birth.First imaged in 1997, Hubble revisits this scene nearly 30 years later with sharper vision. The image reveals a structure nicknamed the “Cosmic Sea Slug,” including a jet from Herbig-Haro 399, showing how young stars actively shape their surroundings.Bright stars, dark dust, and glowing gas tell the story of stars forming and evolving. Over time, the nebula will fade, leaving only stars behind. For 36 years, Hubble has transformed how we see the universe, and it’s not done yet.Sit back and relax as Hubble Senior Project Scientist, Dr. Jennifer Wiseman takes us on a tour of this beautiful image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerScript: Claire Blome (STSci)Narrator: Dr. Jennifer WisemanMusic Credit:\"Hold Your Own\" by Tommy Evans [PRS] via Ninja Tune Production Music [PRS] and Universal Production Music || ", "hits": 161 }, { "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": 289 }, { "id": 31377, "url": "https://svs.gsfc.nasa.gov/31377/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "The Fluid Particles Experiment aboard the ISS", "description": "One of the experiments in the Microgravity Science Glovebox (MSG), observing how the particles cluster and form larger structures in microgravity.", "hits": 259 }, { "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": 166 }, { "id": 31372, "url": "https://svs.gsfc.nasa.gov/31372/", "result_type": "Hyperwall Visual", "release_date": "2026-03-17T18:59:59-04:00", "title": "Tour of the Serpens Nebula", "description": "This video tours the Serpens Nebula, a star-forming region that lies 1,300 light-years away from Earth. A new image of Serpens from NASA’s James Webb Space Telescope shows an intriguing group of aligned protostellar outflows within one region of the nebula. Protostellar outflows are formed when jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds. This region has several captivating features.", "hits": 55 }, { "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": 46 }, { "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": 307 }, { "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": 220 }, { "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": 164 }, { "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": 723 }, { "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": 244 }, { "id": 14905, "url": "https://svs.gsfc.nasa.gov/14905/", "result_type": "Produced Video", "release_date": "2025-11-28T09:00:00-05:00", "title": "Black Hole Environments, Explained", "description": "If light can’t escape black holes, how do we know where they are? The regions around them tell an incredible story. From blazing coronas and swirling accretion disks to powerful jets that stretch millions of miles, these extreme environments reveal black holes' secrets and how these mysterious objects shape the universe.Join host Sophia Roberts as she talks with researchers Jenna Cann and Cecilia Chirenti at NASA Goddard about how scientists study these mysterious structures, the challenges of observing the unseeable, and the discoveries that continue to change our understanding of black holes.Credit: NASA’s Goddard Space Flight CenterMusic credits from Universal Production Music:\"Breaking the Barrier,\" David Bertrand Holland\"Dust Spirals,\" Alexandre Prodhomme\"Miniature Universe,\" Geoffrey Wilkinson\"Urban Decay,\" Sarah Natasha Penelope Warne\"Solar Plexus,\" Brandon Seliga\"Polygraph,\" Eric Chevalier\"The Mischief Makers,\" Joaquim Badia\"Maelstrom Dream,\" Lucie Rose\"The Truth Will Out,\" Chris Dony and Beth Perry || 14905_-_BHE_Thumbnail.jpg (1280x720) [947.8 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.srt [15.7 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.vtt [14.8 KB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_1080.mp4 (1920x1080) [1.7 GB] || FINAL_-_14905_Black_Hole_Enviroments_Explained_4k.mp4 (3840x2160) [9.2 GB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_ProRes.mov (3840x2160) [39.3 GB] || ", "hits": 187 }, { "id": 14928, "url": "https://svs.gsfc.nasa.gov/14928/", "result_type": "Produced Video", "release_date": "2025-11-20T10:00:00-05:00", "title": "TESS Triples Size of Pleiades Star Cluster", "description": "These young, hot blue stars are members of the Pleiades open star cluster and reside about 430 light-years away in the northern constellation Taurus. The brightest stars are visible to the unaided eye during evenings from October to April. A new study finds the cluster to be triple the size previously thought — and shows that its stars are scattered across the night sky. The Schmidt telescope at the Palomar Observatory in California captured this color-composite image. Credit: NASA, ESA, and AURA/CaltechAlt text: Members of the Pleiades shine in blue. Image description: The Pleiades are shown in this image. Six of the stars, all blue-white, are larger than the others and have diffraction spikes and faint blue circles around them. Other, smaller blue stars are also scattered across the image. Patches of swirling blue dust surround some of the stars. || STScI-01EVVEYWX1TA3MGBK5F6EFQVGQ.jpg (4877x3513) [1.1 MB] || ", "hits": 607 }, { "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": 98 }, { "id": 14897, "url": "https://svs.gsfc.nasa.gov/14897/", "result_type": "Produced Video", "release_date": "2025-09-16T10:00:00-04:00", "title": "Our Interstellar Medium", "description": "Our Milky Way galaxy is home to more than 100 billion stars that are often separated by trillions of miles. The spaces in between, called the interstellar medium, aren't empty –– they're sprinkled with gas and dust that are both the seeds of new stars and the leftover crumbs from stars long dead. Studying the interstellar medium with observatories like NASA’s upcoming Nancy Grace Roman Space Telescope will reveal new insight into the galactic dust recycling system.Music Credit: Building Heroes by Enrico Cacace [BMI], Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Our_Interstellar_Medium_Thumbnail.jpg (1280x720) [658.8 KB] || Our_Interstellar_Medium_Thumbnail_searchweb.png (320x180) [105.7 KB] || Our_Interstellar_Medium_Thumbnail_thm.png (80x40) [7.3 KB] || Our_Interstellar_Medium.en_US.srt [1.1 KB] || Our_Interstellar_Medium.en_US.vtt [1.0 KB] || 14897_-_Our_Interstellar_Medium.mp4 (3840x2160) [651.7 MB] || 14897_-_Our_Interstellar_Medium_-_NO_TEXT.mov (3840x2160) [3.7 GB] || ", "hits": 442 }, { "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": 49 }, { "id": 14892, "url": "https://svs.gsfc.nasa.gov/14892/", "result_type": "Produced Video", "release_date": "2025-08-29T16:00:00-04:00", "title": "Solar Wind Animations", "description": "The Sun releases a constant stream of charged particles, called the solar wind. The solar wind originates in the outermost layer of the Sun’s atmosphere, the corona, when plasma is heated to a point that the Sun’s gravity can’t hold it down. When this plasma escapes – often reaching speeds of over one million miles per hour – it drags the Sun’s magnetic out across the solar system. When the solar wind encounters Earth, it is deflected by our planet's magnetic shield, causing most of the solar wind's energetic particles to flow around and beyond us. However, some of these high-energy particles can sneak past Earth’s natural magnetic defenses and produce hazardous conditions for satellites and astronauts, as well as power grids and infrastructure on Earth.Learn more about the solar wind: https://science.nasa.gov/sun/what-is-the-solar-wind/ || ", "hits": 869 }, { "id": 5572, "url": "https://svs.gsfc.nasa.gov/5572/", "result_type": "Visualization", "release_date": "2025-08-08T14:00:02-04:00", "title": "GEOS Aerosols", "description": "Aerosols are tiny solid or liquid particles that float in the atmosphere and can travel long distances, affecting air quality and visibility far from their sources. This visualization covers the period from August 1 to September 14, 2024, and is based on NASA's Goddard Earth Observing System (GEOS) model, which delivers realistic, high-resolution weather and aerosol data that enable customized environmental prediction and advances in AI research.", "hits": 565 }, { "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": 47 }, { "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": 12473 }, { "id": 5566, "url": "https://svs.gsfc.nasa.gov/5566/", "result_type": "Animation", "release_date": "2025-07-03T14:59:59-04:00", "title": "TEMPO Air Quality Monitoring: Three Example Cases", "description": "Three visualizations demonstrating the air quality monitoring capabilities of the TEMPO mission.", "hits": 169 }, { "id": 5552, "url": "https://svs.gsfc.nasa.gov/5552/", "result_type": "Visualization", "release_date": "2025-06-23T09:00:00-04:00", "title": "Science On A Sphere: Aerosols in the Air", "description": "NASA merges observations, advanced models and computing power to monitor aerosols in the atmosphere. Aerosols are tiny invisible solid or liquid particles that float in the atmosphere and can travel long distances affecting air quality and visibility far from their source. These particles come from natural and human sources and include black carbon (orange/red), sea salt (cyan), dust (magenta) and sulfates (green).", "hits": 523 }, { "id": 31355, "url": "https://svs.gsfc.nasa.gov/31355/", "result_type": "Hyperwall Visual", "release_date": "2025-06-17T00:00:00-04:00", "title": "Curiosity Postcard", "description": "Curiosity postcard", "hits": 67 }, { "id": 31353, "url": "https://svs.gsfc.nasa.gov/31353/", "result_type": "Animation", "release_date": "2025-06-09T18:59:59-04:00", "title": "Supermassive Black Holes", "description": "In this video NuSTAR (Nuclear Spectroscopic Telescope Array) lead scientist Peter Boorman explains how the NuSTAR penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)", "hits": 221 }, { "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": 160 }, { "id": 14793, "url": "https://svs.gsfc.nasa.gov/14793/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Black Holes Vertical Video", "description": "This page collects Astrophysics vertical videos with black-hole-related content", "hits": 1488 }, { "id": 14801, "url": "https://svs.gsfc.nasa.gov/14801/", "result_type": "Produced Video", "release_date": "2025-05-27T20:53:00-04:00", "title": "Astrophysics Explainer Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to explainer videos.", "hits": 47 }, { "id": 31348, "url": "https://svs.gsfc.nasa.gov/31348/", "result_type": "Hyperwall Visual", "release_date": "2025-05-21T18:59:59-04:00", "title": "Exploring the Cosmic Cliffs in 3D", "description": "In July 2022, NASA’s James Webb Space Telescope made history, revealing a breathtaking view of a region now nicknamed the Cosmic Cliffs. This glittering landscape, captured in incredible detail, is part of the nebula Gum 31 — a small piece of the vast Carina Nebula Complex", "hits": 455 }, { "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": 83 }, { "id": 14833, "url": "https://svs.gsfc.nasa.gov/14833/", "result_type": "Produced Video", "release_date": "2025-05-07T14:00:00-04:00", "title": "Exploring the Cosmic Cliffs in 3D", "description": "In July 2022, NASA’s James Webb Space Telescope made history, revealing a breathtaking view of a region now nicknamed the Cosmic Cliffs.This glittering landscape, captured in incredible detail, is part of the nebula Gum 31 — a small piece of the vast Carina Nebula Complex — where stars are born amid clouds of gas and dust.This visualization brings Webb’s iconic image to life — helping us imagine the true, three-dimensional structure of the universe… and our place within it.For more information, visit https://webb.nasa.gov/. Credit:Producer: Greg Bacon & Frank Summers (STScI), NASA’s Universe of Learning, NASA's Goddard Space Flight CenterVisualization: Greg Bacon, Ralf Crawford, Joseph DePasquale, Leah Hustak, Danielle Kirshenblat, Christian Nieves, Joseph Olmsted, Alyssa Pagan, & Frank Summers (STScI)Author of Original Release: Christine PulliamNarrator: Jacob PinterSupport/Editor for Shortened Version: Paul MorrisImages: NASA, ESA, CSA, STSciMusic Credit:\"One Way Journey\" by Timothy James Cormick [PRS], and Matthew Jacob Loveridge via BBC Production Music [PRS], and Universal Production Music. || ", "hits": 69 }, { "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": 77 }, { "id": 14830, "url": "https://svs.gsfc.nasa.gov/14830/", "result_type": "Produced Video", "release_date": "2025-04-23T09:00:00-04:00", "title": "Carruthers Geocorona Observatory Images", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ", "hits": 77 }, { "id": 14802, "url": "https://svs.gsfc.nasa.gov/14802/", "result_type": "Produced Video", "release_date": "2025-03-28T14:31:59-04:00", "title": "Earth to Space: A National Symphony Orchestra Concert", "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.", "hits": 115 }, { "id": 14781, "url": "https://svs.gsfc.nasa.gov/14781/", "result_type": "Produced Video", "release_date": "2025-02-25T13:00:00-05:00", "title": "NASA Interview Opportunities: Two Moon Deliveries with NASA Instruments Days from Landing", "description": "Associated cut b-roll will be added by 5 p.m. EST on Thursday, Feb. 27. || CLPS.jpeg (1800x720) [219.2 KB] || CLPS_print.jpg (1024x409) [94.0 KB] || CLPS_searchweb.png (320x180) [46.3 KB] || CLPS_thm.png [5.8 KB] || ", "hits": 119 }, { "id": 14772, "url": "https://svs.gsfc.nasa.gov/14772/", "result_type": "B-Roll", "release_date": "2025-01-29T11:00:00-05:00", "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics", "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ", "hits": 724 }, { "id": 14724, "url": "https://svs.gsfc.nasa.gov/14724/", "result_type": "Produced Video", "release_date": "2025-01-28T00:00:00-05:00", "title": "Significant Mission Milestones in OSIRIS-REx Journey to Bennu and Back", "description": "NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) capsule of rocks and dust collected from asteroid Bennu lands on Earth at, in a targeted area of the Department of Defense’s Utah Test and Training Range at 8:52 a.m. MDT (10:52 a.m. EDT) on Sunday. This video shows a compilation of spacecraft, airplane, and ground camera footage of the landing.Format: 1920 x 1080 px (HD) || OREX_LANDING_HD.00031_print.jpg (1024x576) [106.9 KB] || OREX_LANDING_HD.00031_searchweb.png (320x180) [45.2 KB] || OREX_LANDING_HD.00031_web.png (320x180) [45.2 KB] || OREX_LANDING_HD.00031_thm.png (80x40) [3.5 KB] || OREX_LANDING_HD.mp4 (1920x1080) [79.5 MB] || ", "hits": 65 }, { "id": 14763, "url": "https://svs.gsfc.nasa.gov/14763/", "result_type": "Produced Video", "release_date": "2025-01-24T17:00:00-05:00", "title": "Resource page: NASA to Brief Media on Asteroid Sample Mission Findings", "description": "Link to release: NASA’s Asteroid Bennu Sample Reveals Mix of Life’s IngredientsSee below for pre-recorded soundbites Associated b-roll for this story is linked at the bottom of the page and also on the following page: https://svs.gsfc.nasa.gov/14772/Click here for a link to a curated OSIRIS-REx image collection. || Screenshot_2025-01-24_at_5.13.10 PM.png (3094x986) [1.4 MB] || Screenshot_2025-01-24_at_5.13.10 PM_print.jpg (1024x326) [41.7 KB] || Screenshot_2025-01-24_at_5.13.10 PM_searchweb.png (320x180) [28.1 KB] || Screenshot_2025-01-24_at_5.13.10 PM_thm.png [5.9 KB] || ", "hits": 64 }, { "id": 14756, "url": "https://svs.gsfc.nasa.gov/14756/", "result_type": "Produced Video", "release_date": "2025-01-13T16:00:00-05:00", "title": "50 Years of GOES", "description": "Music:“Realms of the Sky” by Frederik Helmut Wiedmann [GMR]; Icon Trailer Music; Universal Production Music“Exoplanet” by Jeff Penny [ASCAP]; Emperia Musicworks; Universal Production Music“Solo Trip” by Nicholas Smith [PRS]; Ideal.e; Universal Production Music“Reaching the Skies” by Ben Hicks [ASCAP]; Emperia Musicworks; Universal Production Music“Aetherion” by Lincoln Dale Davis [BMI]; Emperia Musicworks; Universal Production MusicThis video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by FootageFirm.com, Sebolla74/Pond5 and danr13/Pond5 are obtained through permission and may not be excised or remixed in other products. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html || YouTubeThumbnail_GOES50th_GOESandEarth.jpg (1920x1080) [1.2 MB] || YouTubeThumbnail_GOES50th_GOESandEarth.png (1280x720) [1.5 MB] || 14756_GOES_50th_FINAL_UHD.00500_print.jpg (1024x576) [167.0 KB] || 14756_GOES_50th_FINAL_UHD.00500_searchweb.png (320x180) [95.9 KB] || 14756_GOES_50th_FINAL_UHD.00500_thm.png [7.4 KB] || 14756_GOES_50th_FINAL_1080.mp4 (1920x1080) [178.6 MB] || 14756_GOES_50th_FINAL_UHD.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_UHD.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_1080.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_1080.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_UHD.webm (3840x2160) [20.5 MB] || 14756_GOES_50th_FINAL_UHD.mp4 (3840x2160) [684.3 MB] || ", "hits": 72 }, { "id": 14748, "url": "https://svs.gsfc.nasa.gov/14748/", "result_type": "Produced Video", "release_date": "2025-01-08T09:00:00-05:00", "title": "WEBB Captures Fiery Star Formation", "description": "Dr. Michelle Thaller presents Webb’s stunning view of a young protostar, just 100,000 years old and cocooned in gas and dust.Webb reveals the protostar’s hourglass shape, vibrant blue and orange clouds, and spiraling accretion disk—key features of this early stage of star formation.A true marvel, this protostar offers insights into the origins of stars, unveiling a process billions of years in the making. What secrets will the universe reveal next?For more information, visit https://webb.nasa.gov/. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Thaddeus Cesari: ScriptDr. Michelle Thaller: NarratorMusic Credit:\"Looking to the Future\" by Carl David Harms [IMRO] via BBC Production Music [PRS], and Universal Production Music. || ", "hits": 34 }, { "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": 478 }, { "id": 14731, "url": "https://svs.gsfc.nasa.gov/14731/", "result_type": "Produced Video", "release_date": "2024-12-16T10:00:00-05:00", "title": "Hubble’s Inside the Image: Protoplanetary Disks", "description": "NASA's Hubble Space Telescope has captured stunning images of protoplanetary disks—dynamic, swirling structures of gas and dust surrounding young stars.In this video, Dr. Padi Boyd takes us on a journey through these remarkable objects, explaining how Hubble's observations are unraveling the mysteries of planet formation and providing a glimpse into the birthplaces of new solar systems.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. Christensen Exoplanet Animations: ESA/Hubble - M. Kornmesser & L. CalçadaMusic Credits:PREMIUM BEAT BY SHUTTERSTOCKThe Search by Northern Points\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music || ", "hits": 99 }, { "id": 5434, "url": "https://svs.gsfc.nasa.gov/5434/", "result_type": "Visualization", "release_date": "2024-12-10T10:00:00-05:00", "title": "Collecting Global Methane Emissions with EMIT", "description": "Animation that shows the data collection path of the EMIT instrument onboard the ISS. EMIT has a 75 kilometer swath width - which is relatively narrow, but you can see in this data visualization how it can get full global coverage over time. The violet dots are methane emission sources. || new_emit_v35_4K.0100_print.jpg (1024x576) [162.5 KB] || new_emit_v35_4K.0100_searchweb.png (320x180) [74.3 KB] || new_emit_v35_4K.0100_thm.png (80x40) [7.6 KB] || new_emit_v35_1080p30.mp4 (1920x1080) [28.2 MB] || new_emit_v35_4K_2160p30.mp4 (3840x2160) [86.9 MB] || 3840x2160_16x9_30p [0 Item(s)] || new_emit_v35_4K_2160p30.mp4.hwshow [189 bytes] || ", "hits": 336 }, { "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": 250 }, { "id": 14720, "url": "https://svs.gsfc.nasa.gov/14720/", "result_type": "Produced Video", "release_date": "2024-11-22T10:00:00-05:00", "title": "COBE All-Sky Map 360 Video With Narration", "description": "View the entire sky with the microwave eyes of NASA’s COBE (Cosmic Background Explorer) satellite in this immersive video. COBE took the first baby picture of the universe, revealing slight temperature variations when the cosmos was just 380,000 years old. This image shows the entire sky using four years of observations by COBE’s Differential Microwave Radiometer. The central plane of our galaxy runs across the middle, and its center is marked by a white X. Red indicates hotter regions, blue colder. The fluctuations are extremely faint, varying by only 1 part in 100,000 from the average temperature. They represent density variations in the early universe thought to have given rise to the structures we see today. After stripping away foreground emission arising from dust, hot gas, and charged particles interacting with magnetic fields in our galaxy, COBE data revealed tiny variations in the temperature of the cosmic microwave background — the oldest light in the universe — for the first time.(This video is formatted for 360-degree use.)Credit: NASA's Goddard Space Flight CenterMusic: “Meetings in Underwater Ruins,” Philippe Andre Vandenhende [SACEM], Olivier Louis Perrot [SACEM] and Idriss-El-Mehdi Bennani [SACEM], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Design_hybrid_COBE_360.jpg (1280x720) [235.1 KB] || YTframe_Design_hybrid_COBE_360_searchweb.png (320x180) [80.8 KB] || YTframe_Design_hybrid_COBE_360_thm.png (80x40) [9.2 KB] || 14720_COBE_360_Captions.en_US.srt [4.7 KB] || 14720_COBE_360_Captions.en_US.vtt [4.4 KB] || 14720_COBE_360_Narrated_Good.mp4 (8192x4096) [131.8 MB] || 14720_COBE_360_Narrated_Best.mp4 (8192x4096) [503.2 MB] || ", "hits": 337 }, { "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": 207 }, { "id": 31321, "url": "https://svs.gsfc.nasa.gov/31321/", "result_type": "Hyperwall Visual", "release_date": "2024-11-16T00:00:00-05:00", "title": "GMAO Africa Dust AQ", "description": "GMAO Africa Dust AQ 2024 run || 3840x2160_16x9_60p [0 Item(s)] || GMAO Africa Dust AQ || gmao-africa-dust-aq_print.jpg (1024x576) [172.3 KB] || gmao-africa-dust-aq.png (3840x2160) [4.5 MB] || gmao-africa-dust-aq_searchweb.png (320x180) [91.8 KB] || gmao-africa-dust-aq_thm.png (80x40) [7.0 KB] || gmao-africa-dust-aq_1080p60.mp4 (1920x1080) [14.5 MB] || gmao-africa-dust-aq_1080p60.webm (1920x1080) [2.2 MB] || gmao-africa-dust-aq_2160p60.mp4 (3840x2160) [46.8 MB] ||", "hits": 50 }, { "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": 258 }, { "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": 118 }, { "id": 5298, "url": "https://svs.gsfc.nasa.gov/5298/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "July mean Sargassum in the Atlantic: 2010 - 2023", "description": "This visualization shows the July mean Sargassum observed in the Atlantic Ocean by the MODIS instruments on NASA's TERRA and AQUA satellites from 2010 to 2023. Each square box of color represents an area 0.5 x 0.5 degrees, roughly 3025 square kilometers in size. The color represents the mean amount of Sargassum observed in that box during the month of July. Blue shades indicate that this area had on average less than 3 square kilomenters of Sargassum, while red indicates that the region had an average of 9 square kilometers or more. || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_print.jpg (1024x576) [156.7 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_searchweb.png (320x180) [77.0 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_thm.png (80x40) [6.5 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_30p_1080p30.mp4 (1920x1080) [6.4 MB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_30p_2160p30.mp4 (3840x2160) [21.4 MB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_2160p60.mp4 (3840x2160) [18.9 MB] || composite [0 Item(s)] || composite [0 Item(s)] || ", "hits": 206 }, { "id": 5299, "url": "https://svs.gsfc.nasa.gov/5299/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "Monthly mean Sargassum in the Atlantic: Jan 2018 - Dec 2023", "description": "This visualization shows the monthly mean Sargassum observed in the Atlantic Ocean by the MODIS instruments on NASA's TERRA and AQUA satellites from January 2018 through December 2023. Each square box of color represents an area 0.5 x 0.5 degrees, roughly 3025 square kilometers in size. The color represents the mean amount of Sargassum observed in that box during the month of July. Blue shades indicate that this area had on average less than 3 square kilomenters of Sargassum, while red indicates that the region had an average of 9 square kilometers or more. || sargassum_v30_monthly_4k_2024-05-28_1632.02876_print.jpg (1024x576) [152.7 KB] || sargassum_v30_monthly_4k_2024-05-28_1632.02876_searchweb.png (320x180) [75.7 KB] || sargassum_v30_monthly_4k_2024-05-28_1632.02876_thm.png (80x40) [6.4 KB] || sargassum_v30_monthly_4k_2024-05-28_1632_p30_1080p30.mp4 (1920x1080) [10.8 MB] || composite [0 Item(s)] || composite [0 Item(s)] || sargassum_v30_monthly_4k_2024-05-28_1632_p30_2160p30.mp4 (3840x2160) [31.5 MB] || sargassum_v30_monthly_4k_2024-05-28_1632_2160p60.mp4 (3840x2160) [31.8 MB] || ", "hits": 62 }, { "id": 5301, "url": "https://svs.gsfc.nasa.gov/5301/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "Atlantic Ocean Surface Drift Patterns from the Caribbean in 2010 and 2011", "description": "Simulated particle backtrack with windage and timelineThis visualization shows simulated particles released during 2010 and 2011 traced back in time to show their path based on the ocean surface velocities from Global HYCOM model with 1% windage applied. Simulated particles were released between December through April and tracked back in time. The gold balls under the timeline indicate the months when particles were released. Flow lines represent the movement of a particle over a 20-day period. Particles that venture above the 23 degree north latitude line (shown in red) during their lifespan are colored gold while particles that stayed south of it are colored green. || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_print.jpg (1024x576) [193.3 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_searchweb.png (320x180) [76.7 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_thm.png (80x40) [6.2 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_1080p60.mp4 (1920x1080) [52.6 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_1080p30.mp4 (1920x1080) [54.0 MB] || composite_wWind [0 Item(s)] || composite_wWind [0 Item(s)] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4 (3840x2160) [151.2 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_2160p30.mp4 (3840x2160) [158.8 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4.hwshow [226 bytes] || ", "hits": 64 }, { "id": 14673, "url": "https://svs.gsfc.nasa.gov/14673/", "result_type": "Produced Video", "release_date": "2024-09-09T09:55:00-04:00", "title": "NASA’s Hubble, Chandra Find Supermassive Black Hole Duo", "description": "The closest confirmed pair of supermassive black holes have been observed in tight proximity. These are located approximately 300 light-years apart and were detected using NASA’s Hubble Space Telescope and the Chandra X-ray Observatory. These black holes, buried deep within a pair of colliding galaxies, are fueled by infalling gas and dust, causing them to shine brightly as active galactic nuclei (AGN).For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerScott Wiessinger: Producer for Assorted AGN AnimationsMusic Credit:\"Drift\" by Alexandre Prodhomme [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music. || ", "hits": 49 }, { "id": 5360, "url": "https://svs.gsfc.nasa.gov/5360/", "result_type": "Visualization", "release_date": "2024-08-21T00:00:00-04:00", "title": "Global Methane Emissions", "description": "Spinning globe showing global methane emissions in magenta. || newemit_spinning_globe_v16.1440_print.jpg (1024x576) [73.5 KB] || newemit_spinning_globe_v16.1440_searchweb.png (320x180) [33.5 KB] || newemit_spinning_globe_v16.1440_thm.png (80x40) [5.6 KB] || newemit_spinning_globe_v16_1080p30.mp4 (1920x1080) [9.7 MB] || 1920x1080_16x9_30p [0 Item(s)] || ", "hits": 242 }, { "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": 89 }, { "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": 198 }, { "id": 5332, "url": "https://svs.gsfc.nasa.gov/5332/", "result_type": "Visualization", "release_date": "2024-07-18T00:00:00-04:00", "title": "NASA’s Greenhouse-Gas (GHG) Satellites", "description": "This visualization shows the orbits of the International Space Station (ISS) and Orbiting Carbon Observatory-2 (OCO-2) satellites. The ISS includes the EMIT and OCO-3 instruments. As the satellites orbit, their respective ground tracks are drawn on the Earth in white and orange to show how global coverage accumulates over time. || ghg_fleet.00915_print.jpg (1024x576) [84.4 KB] || ghg_fleet.00915_searchweb.png (320x180) [44.4 KB] || ghg_fleet.00915_thm.png (80x40) [3.1 KB] || ghg_fleet_1080p60.mp4 (1920x1080) [14.0 MB] || ghg_fleet [0 Item(s)] || ghg_fleet_2160p60.mp4 (3840x2160) [53.5 MB] || ghg_fleet_2160p60.mp4.hwshow [183 bytes] || ", "hits": 283 }, { "id": 14619, "url": "https://svs.gsfc.nasa.gov/14619/", "result_type": "Produced Video", "release_date": "2024-07-17T10:00:00-04:00", "title": "Black Hole with Accretion Disk Visualization", "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole surrounded by a rapidly-rotating disk of gas and dust. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The speed at which material, in what is known as an accretion disk, orbits the black hole increases with proximity. The orbital speed of material closest to the event horizon approaches the speed of light. This produces an effect known as “relativistic doppler beaming” which enhances the brightness of material moving towards us along our line of sight, and correspondingly dims the brightness of material moving away.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.The light from the orbiting material is likewise distorted, making the flat accretion disk appear to bend completely around the black hole’s shadow and have the disk behind the black hole appear to be both above and below it. Yet despite these strange visual distortions that change with viewing angle, the accretion disk itself physically remains flat.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance of a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ", "hits": 3900 }, { "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": 395 }, { "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": 552 }, { "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": 52 }, { "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": 428 }, { "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": 329 }, { "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": 361 }, { "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": 410 }, { "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": 183 }, { "id": 31283, "url": "https://svs.gsfc.nasa.gov/31283/", "result_type": "Hyperwall Visual", "release_date": "2024-05-22T00:00:00-04:00", "title": "Webb Space Telescope View of the Horsehead Nebula", "description": "Horsehead Nebula (Euclid, Hubble and Webb images) || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3.png (8983x3530) [35.2 MB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_print.jpg (1024x402) [143.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_searchweb.png (320x180) [90.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_thm.png (80x40) [15.8 KB] || ", "hits": 112 }, { "id": 5272, "url": "https://svs.gsfc.nasa.gov/5272/", "result_type": "Visualization", "release_date": "2024-05-21T08:00:00-04:00", "title": "Methane plumes detected by EMIT Space Mission", "description": "The Earth Surface Mineral Dust Source Investigation (EMIT) mission uses an imaging spectrometer to detect the unique pattern of reflected and absorbed light – called a spectral fingerprint – from various materials on Earth's surface and in its atmosphere. Perched on the International Space Station, EMIT was originally intended to map the prevalence of minerals in Earth's arid regions, such as the deserts of Africa and Australia. Scientists verified that EMIT could also detect the spectral fingerprints of methane and carbon dioxide which enables mapping of emissions from the energy, waste, and agriculture sectors. || ", "hits": 232 }, { "id": 14584, "url": "https://svs.gsfc.nasa.gov/14584/", "result_type": "Produced Video", "release_date": "2024-05-08T09:00:00-04:00", "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy", "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ", "hits": 112 }, { "id": 14577, "url": "https://svs.gsfc.nasa.gov/14577/", "result_type": "Produced Video", "release_date": "2024-05-03T09:55:00-04:00", "title": "Hubble’s Inside the Image: Herbig-Haro Jet HH 24", "description": "NASA's Hubble Space Telescope has photographed what looks like a cosmic, double-bladed lightsaber. In the center of the image, partially obscured by a dark, Jedi-like cloak of dust, a newborn star shoots twin jets out into space as a sort of birth announcement to the universe.In this video, Dr. Ken Carpenter explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe, even if it is far far away!For more information, visit https://nasa.gov/hubble. Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. Christensen Music Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music\"The Search\" by Northern Points via PREMIUM BEAT BY SHUTTERSTOCK || ", "hits": 46 }, { "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": 202 }, { "id": 31276, "url": "https://svs.gsfc.nasa.gov/31276/", "result_type": "Hyperwall Visual", "release_date": "2024-02-08T00:00:00-05:00", "title": "Curiosity's Hazcams Capture a Day on Mars", "description": "A hyperwall ready version of animation publised at https://photojournal.jpl.nasa.gov/catalog/PIA26209NASA's Curiosity Mars rover recorded two 25-frame videos showing the passage of 12 hours on Nov. 8, 2023, the 4,002nd Martian day, or sol, of the mission. The images were captured with Curiosity's front and rear Hazard-Avoidance Cameras, or Hazcams. A long series of images can be put together to create a video so that scientists can look for passing clouds or dust devils, which teach them more about the Martian environment. The perfect time for doing this type of work is when Curiosity is less active for long stretches, as it was during Mars solar conjunction. The lack of robotic arm motion and driving during conjunction allowed the Hazcams to image for 12 hours of a day for the first time. While these Hazcam videos didn't reveal any clouds or dust activity, they did capture the passage of time as the Sun rose and set. || ", "hits": 124 }, { "id": 14498, "url": "https://svs.gsfc.nasa.gov/14498/", "result_type": "Produced Video", "release_date": "2024-01-11T11:05:00-05:00", "title": "Finding A New Galactic 'Fossil'", "description": "Some 5 million years ago, a black hole eruption in the galaxy NGC 4945 set off a star-formation frenzy and shot a vast cloud of gas into intergalactic space. Watch and learn how two X-ray telescopes revealed the story.Music Credits: Universal Production Music\"Planetary Horizons\" by Jia Lee\"Eyes Peeled\" by Bard\"Sprinkle of Mischief\" by Ash and HaroldWatch this video on the NASA Goddard YouTube channel.Credit: NASA’s Goddard Space Flight Center", "hits": 101 }, { "id": 14493, "url": "https://svs.gsfc.nasa.gov/14493/", "result_type": "Produced Video", "release_date": "2024-01-05T09:55:00-05:00", "title": "Hubble’s Inside The Image: The Eagle Nebula", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of The Pillars of Creation.The Pillars of Creation in the Eagle Nebula, situated in the Serpens constellation, stand as celestial marvels. Composed of interstellar gas and dust, these towering structures captivate astronomers and stargazers alike. Shaped by the potent forces of stellar winds and radiation, the pillars, resembling cosmic sentinels, showcase vibrant hues. Functioning as crucibles for stellar birth, they facilitate the creation of new stars in a delicate dance of destruction and formation. The Pillars of Creation in the Eagle Nebula offer a captivating spectacle, inviting observers to contemplate the profound dynamics at play within our ever-evolving cosmic tapestry.In this video, Dr. Jennifer Wiseman explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationESA/Hubble (M. Kornmesser & L. L. Christensen) Light Echo AnimationNASA/ESA/Hubble - M. KornmesserMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music. || ", "hits": 79 }, { "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": 206 }, { "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": 95 }, { "id": 31244, "url": "https://svs.gsfc.nasa.gov/31244/", "result_type": "Hyperwall Visual", "release_date": "2023-09-25T00:00:00-04:00", "title": "OSIRIS-REx Tags Asteroid Bennu Videos", "description": "Touch-And-Go (TAG) sample collection || osiris-rex-tag_1000_print.jpg (1024x576) [124.1 KB] || osiris-rex-tag_1000_searchweb.png (320x180) [78.7 KB] || osiris-rex-tag_1000_thm.png (80x40) [5.0 KB] || osiris-rex-tag_1080p30.mp4 (1920x1080) [10.3 MB] || osiris-rex-tag_1080p30.webm (1920x1080) [1.4 MB] || osiris-rex-tag_2160p30.mp4 (3840x2160) [29.9 MB] || tag (3840x2160) [0 Item(s)] || ", "hits": 304 }, { "id": 14416, "url": "https://svs.gsfc.nasa.gov/14416/", "result_type": "B-Roll", "release_date": "2023-09-24T09:00:00-04:00", "title": "OSIRIS-REx Sample Return Broadcast Media", "description": "On September 24, 2023, NASA’s OSIRIS-REx spacecraft delivered a sample of the pristine asteroid Bennu to Earth. Its sample return capsule, containing rocks and dust collected from Bennu, touched down at the Department of Defense Utah Test and Training Range shortly before 9:00 am, Mountain Time. This page contains video packages and graphics that were broadcast by NASA during the event. View the OSIRIS-REx Sample Return Broadcast and Landing Highlights. || ", "hits": 181 }, { "id": 20378, "url": "https://svs.gsfc.nasa.gov/20378/", "result_type": "Animation", "release_date": "2023-09-19T18:00:00-04:00", "title": "Long Gamma-Ray Burst", "description": "Complete animation sequence.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GRB_Sequence_Still.jpg (3840x2160) [1.6 MB] || 20378_GRB_Sequence_1080.mp4 (1920x1080) [41.7 MB] || 20378_GRB_Sequence_4k.mp4 (3840x2160) [109.7 MB] || 20378_GRB_Sequence_ProRes_3840x2160_30.mov (3840x2160) [1.4 GB] || ", "hits": 458 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth 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": 252 }, { "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": 204 }, { "id": 5136, "url": "https://svs.gsfc.nasa.gov/5136/", "result_type": "Visualization", "release_date": "2023-08-22T00:00:00-04:00", "title": "STEREO-A Returns by Earth", "description": "The Solar Terrestrial Relations Observatory (STEREO) mission was launched on October 25, 2006, with the purpose of tracing the flow of energy and matter from the Sun to Earth. The STEREO mission began with two spacecraft: STEREO-A and STEREO-B. Each was launched into Sun-orbiting trajectories - STEREO-A moving ahead of Earth, and STEREO-B moving behind Earth (STEREO's Routes to Solar Orbits). In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) will pass Earth for the first time since its launch 17 years ago. Like race cars driving different speeds around a circular track, STEREO-A is traveling slightly faster than Earth around the Sun. After launch, STEREO-A pulled ahead of Earth and extended its lead a little bit more with each orbit. Now, STEREO-A’s lead is so great that it is catching up to Earth from behind and is about to “lap” Earth, having completed 18 circuits around the Sun while Earth completed just 17. || ", "hits": 154 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 973 }, { "id": 14385, "url": "https://svs.gsfc.nasa.gov/14385/", "result_type": "Produced Video", "release_date": "2023-07-20T10:00:00-04:00", "title": "OSIRIS-REx Returns – Teaser", "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Path of a Hero\" Caleb Jordan Swift of Universal Production Music. || OREX_PROMO_FINAL_SEP24.00867_print.jpg (1024x576) [182.9 KB] || OREX_PROMO_FINAL_SEP24.00867_searchweb.png (320x180) [75.6 KB] || OREX_PROMO_FINAL_SEP24.00867_thm.png (80x40) [6.1 KB] || OREX_PROMO_FINAL.en_US.srt [587 bytes] || OREX_PROMO_FINAL.en_US.vtt [565 bytes] || OREX_PROMO_14385.mp4 (3840x2160) [44.4 MB] || ", "hits": 112 }, { "id": 5104, "url": "https://svs.gsfc.nasa.gov/5104/", "result_type": "Visualization", "release_date": "2023-05-23T00:00:00-04:00", "title": "Two Decades of Changes in Nitrogen Dioxide and Fine Particulate Pollution in the U.S.", "description": "A data visualization of particulate matter 2.5 (PM2.5) data for the Washington DC region spanning 2000-2018 (annual averages). Higher values are represented with dark red and lower values are represented with bright yellow. This view uses the hybrid PM 2.5 color bar with a range of 5 to 20. || pm25_dc_annual.2018_print.jpg (1024x576) [216.4 KB] || pm25_dc_annual.2018_searchweb.png (320x180) [75.7 KB] || pm25_dc_annual.2018_thm.png (80x40) [6.2 KB] || pm25_dc_annual (3840x2160) [0 Item(s)] || pm25_dc_annual_2160p1.mp4 (3840x2160) [30.8 MB] || pm25_dc_annual_2160p60_prores.mov (3840x2160) [41.0 MB] || pm25_dc_annual_2160p1.webm (3840x2160) [1.9 MB] || ", "hits": 92 }, { "id": 14353, "url": "https://svs.gsfc.nasa.gov/14353/", "result_type": "Produced Video", "release_date": "2023-05-19T09:55:00-04:00", "title": "Sonification of V838 Monocerotis Light Echo", "description": "This data sonification of the star V838 Monocerotis, or V838 Mon, shows two Hubble images taken almost seven months apart. A pulse of light from the central star illuminates clouds of dust and gas surrounding V838 Mon. This star is located about 20,000 light-years away, at the outer edge of our Milky Way Galaxy. In this sonification, scientists mapped brightness to pitch and volume, and the surrounding stars are pitched to musical notes. Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ", "hits": 53 }, { "id": 14313, "url": "https://svs.gsfc.nasa.gov/14313/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 1: The Sun", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: \"The Sun\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Complete list of footage used HERE.Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_The_Sun_V2_print.jpg (1024x576) [103.2 KB] || Cosmic_Cycles_The_Sun_V2.jpg (3840x2160) [859.1 KB] || Cosmic_Cycles_The_Sun_V2_searchweb.png (320x180) [51.8 KB] || Cosmic_Cycles_The_Sun_V2_web.png (320x180) [51.8 KB] || Cosmic_Cycles_The_Sun_V2_thm.png (80x40) [5.6 KB] || Cosmic_Cycles-The_Sun_Online_50mbps.webm (1920x1080) [92.6 MB] || Cosmic_Cycles-The_Sun_Online_1080.mp4 (1920x1080) [1.5 GB] || Cosmic_Cycles-The_Sun_Online_50mbps.mp4 (1920x1080) [3.6 GB] || Cosmic_Cycles-The_Sun_Online_ProRes_1920x1080_2997.mov (1920x1080) [10.1 GB] || ", "hits": 104 }, { "id": 14318, "url": "https://svs.gsfc.nasa.gov/14318/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 2: Earth, Our Home", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Earth, Our Home\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Earth_Our_Home_V2_print.jpg (1024x576) [85.8 KB] || Cosmic_Cycles_Earth_Our_Home_V2.jpg (3840x2160) [715.2 KB] || Cosmic_Cycles_Earth_Our_Home_V2_searchweb.png (320x180) [48.3 KB] || Cosmic_Cycles_Earth_Our_Home_V2_thm.png (80x40) [5.7 KB] || CosmicCycles_Earth_With_Music_1080.webm (1920x1080) [100.5 MB] || CosmicCycles_Earth_With_Music_1080.mp4 (1920x1080) [1.3 GB] || CosmicCycles_Earth_With_Music_50mbps.mp4 (1920x1080) [4.0 GB] || CosmicCycles_Earth_With_Music_1920x1080_30fps.mov (1920x1080) [17.9 GB] || ", "hits": 50 }, { "id": 40463, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles2-earth-our-home/", "result_type": "Gallery", "release_date": "2023-05-01T00:00:00-04:00", "title": "Cosmic Cycles 2 Earth Our Home", "description": "Our home and the only planet we know of to possess life. In the years since we first managed to leave its atmosphere, our understanding of it has grown exponentially. NASA now observes and measures Earth with an unmatched fleet of spacecraft. Our influence on this incredibly complex and ever-changing sphere is both obvious and insignificant.", "hits": 19 }, { "id": 14334, "url": "https://svs.gsfc.nasa.gov/14334/", "result_type": "Produced Video", "release_date": "2023-04-20T09:55:00-04:00", "title": "Hubble's 33rd Anniversary: Dark Nebula is a Cauldron of Star Birth", "description": "NASA is celebrating the Hubble Space Telescope’s 33rd birthday with an ethereal image of a nearby star-forming region, NGC 1333.Located approximately 960 light-years away in the Perseus interstellar cloud, Hubble’s colorful view unveils glowing gasses and pitch-black dust stirred up, colliding, and blown around by several hundred forming stars within the dark cloud.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Dr. Jennifer Wiseman: NarrationMusic Credit:“Sensory Submersion” by Alessandro Rizzo [PRS ] and Elliot Greenway Ireland [PRS] via Pedigree Cuts [PRS] and Universal Production Music. || ", "hits": 45 }, { "id": 14317, "url": "https://svs.gsfc.nasa.gov/14317/", "result_type": "Produced Video", "release_date": "2023-03-28T13:50:00-04:00", "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst", "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ", "hits": 255 }, { "id": 40464, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles1-the-sun/", "result_type": "Gallery", "release_date": "2023-03-21T00:00:00-04:00", "title": "Cosmic Cycles 1: The Sun", "description": "Born from a swirling cloud of dust and gas some 4.6 billion years ago, our Sun seethes and boils like a living thing. It is the very center of our solar system, and large enough to encompass 1.3 million Earths. Explosions flash on its surface in colors of light beyond human vision and enormous loops of plasma stretch into space. The Sun’s influence extends out beyond the planets, creating a protective cocoon within the galaxy.\n\nWant to know more?\nSDO Gallery SDO website NASA Heliophysics Home Page", "hits": 70 }, { "id": 14288, "url": "https://svs.gsfc.nasa.gov/14288/", "result_type": "Produced Video", "release_date": "2023-03-03T09:55:00-05:00", "title": "Hubble’s Inside The Image: V838 Mon", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking image sequence of V838 Monocerotis (V838 Mon).Called a light echo, the expanding illumination of interstellar dust around the star has been revealing remarkable structures in the dusty cloud ever since the star suddenly brightened in January 2002. V838 Mon temporarily became 600,000 times brighter than our Sun, until it faded in April 2002. It was one of the brightest stars in the entire Milky Way. The reason for the eruption is still unclear.In this video, Dr. Padi Boyd explains this fascinating piece of history, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin FilmsVideo Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSFMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Moving Headlines” by Immersive Music (Via Shutterstock Music) || ", "hits": 57 }, { "id": 40455, "url": "https://svs.gsfc.nasa.gov/gallery/spacecraft-animations/", "result_type": "Gallery", "release_date": "2023-01-24T00:00:00-05:00", "title": "Satellite Animations", "description": "A collection of spacecraft beauty pass animations for current missions.", "hits": 289 }, { "id": 5060, "url": "https://svs.gsfc.nasa.gov/5060/", "result_type": "Visualization", "release_date": "2023-01-12T10:00:00-05:00", "title": "Global Temperature Anomalies from 1880 to 2022", "description": "This color-coded map in Robinson projection displays a progression of changing global surface temperature anomalies. Normal temperatures are shown in white. Higher than normal temperatures are shown in red and lower than normal temperatures are shown in blue. Normal temperatures are calculated over the 30 year baseline period 1951-1980. The final frame represents the 5 year global temperature anomalies from 2018-2022. || GISTEMP-2022-TemperatureAnomalyBothCelsiusFahrenheit.00899_print.jpg (1024x576) [145.3 KB] || GISTEMP-2022-TemperatureAnomalyBothCelsiusFahrenheit.00899_searchweb.png (180x320) [74.8 KB] || GISTEMP-2022-TemperatureAnomalyBothCelsiusFahrenheit.00899_thm.png (80x40) [6.3 KB] || GISTEMP-2022-TemperatureAnomalyBothCelsiusFahrenheit.mp4 (1920x1080) [57.8 MB] || celsius (1920x1080) [0 Item(s)] || celsius (3840x2160) [0 Item(s)] || ", "hits": 414 }, { "id": 14260, "url": "https://svs.gsfc.nasa.gov/14260/", "result_type": "Produced Video", "release_date": "2022-12-22T09:55:00-05:00", "title": "Sonification of RS Puppis", "description": "RS Puppis is a glittering star 200 times larger than our Sun and wreathed with dust reflecting starlight. Located about 6,500 light-years away, this star rhythmically brightens and dims over a six-week cycle. In this sonification, scientists represent data in the image as sound for a new, festive way of experiencing RS Puppis. Pitch is assigned based on direction from the center; as the circle travels inward, light closer to the top is high pitched, and light closer to the bottom is lower. Light toward the left is heard more in the left speaker and light toward the right is heard more in the right speaker. Additionally, brightness in the image is mapped to louder volume. Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ", "hits": 83 } ] }