{ "count": 109, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&people=Jeanette+Kazmierczak", "previous": null, "results": [ { "id": 14980, "url": "https://svs.gsfc.nasa.gov/14980/", "result_type": "Produced Video", "release_date": "2026-02-26T12:00:00-05:00", "title": "Prototype ComPair-2 Gamma-Ray Detectors Complete Thermal Vacuum Testing", "description": "Prototype gamma-ray detectors for the ComPair-2 mission rests in a thermal vacuum chamber after testing in June 2025 at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The ComPair-2 team tested the detectors’ performance at hot and cold temperatures over the course of a week and the overall survivability of the layer itself. Credit: NASA/Sophia RobertsAlt text: A piece of equipment sits inside a chamber in a lab. Image description: A cylindrical metal chamber at the center of the image has its door swung all the way open. Inside are silver-wrapped ComPair-2 detectors attached to many copper-colored wires. The chamber is in a lab with white walls and has tubes, wires, and other pieces of equipment attached. || ComPair2_TVAC-1-small.jpg (4096x2732) [3.2 MB] || ComPair2_TVAC-1.jpg (8192x5464) [30.6 MB] || ", "hits": 356 }, { "id": 14955, "url": "https://svs.gsfc.nasa.gov/14955/", "result_type": "Produced Video", "release_date": "2026-01-27T09:00:00-05:00", "title": "NASA Tests LISA Development Units", "description": "A prototype charge management device for the future LISA (Laser Interferometer Space Antenna) mission sits on a lab bench at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The device will reduce the buildup of electric charge on the gold-platinum test masses that float freely inside each of the three LISA spacecraft. The University of Florida in Gainesville and Fibertek Inc. in McNair, Virginia, are developing the device. Credit: NASA/Dennis HenryAlt text: An instrument rests on a lab bench.Image description: A silver box with red and black connector caps on one side rests on a white lab bench with a blue mat on top. Three black cables connect to the box and another yellow cable curls around it. || GSFC_20250602_LISA_006584.jpg (8098x5399) [11.3 MB] || ", "hits": 355 }, { "id": 14945, "url": "https://svs.gsfc.nasa.gov/14945/", "result_type": "Produced Video", "release_date": "2026-01-09T09:00:00-05:00", "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars", "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ", "hits": 351 }, { "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": 269 }, { "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": 343 }, { "id": 14922, "url": "https://svs.gsfc.nasa.gov/14922/", "result_type": "Produced Video", "release_date": "2025-12-01T14:00:00-05:00", "title": "Anatomy of an Active Galactic Nucleus", "description": "An active galactic nucleus, or AGN, is a supermassive black hole at the center of a galaxy that is consuming surrounding matter. Although the black hole itself is not visible, the structures around it emit light across many wavelengths. The artist’s concepts here highlight distinct structures that can accompany an AGN — the photon ring, accretion disk, corona, dusty torus, and relativistic jets. || ", "hits": 386 }, { "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": 196 }, { "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": 458 }, { "id": 14906, "url": "https://svs.gsfc.nasa.gov/14906/", "result_type": "Produced Video", "release_date": "2025-09-30T15:00:00-04:00", "title": "Evolution of a Sun-Like Star", "description": "As a star ages, its spin and the number and sizes of its spots decreases as shown in this animation of a Sun-like star. Star spots are tied to local magnetic fields that have been amplified by the star’s rotation, so the phenomena are connected.A version without labels is available for download.Credit: NASA’s Goddard Space Flight Center || ThreeStars_Still.jpg (3840x2160) [586.8 KB] || ThreeStars_Still.png (3840x2160) [3.4 MB] || ThreeStars_Still_searchweb.png (320x180) [65.9 KB] || ThreeStars_Still_thm.png (80x40) [6.3 KB] || 14906_ThreeStars_NoText_1080.mp4 (1920x1080) [53.6 MB] || 14906_ThreeStars_1080.mp4 (1920x1080) [53.8 MB] || 14906_ThreeStars_4k.mp4 (3840x2160) [178.6 MB] || 14906_ThreeStars_NoText_4k.mp4 (3840x2160) [178.3 MB] || 14906_ThreeStars_NoText_ProRes_3840x2160_2997.mov (3840x2160) [1.8 GB] || 14906_ThreeStars_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || ", "hits": 273 }, { "id": 14883, "url": "https://svs.gsfc.nasa.gov/14883/", "result_type": "Produced Video", "release_date": "2025-08-25T11:00:00-04:00", "title": "Mapping Stellar ‘Polka Dots’", "description": "Watch to learn how a new tool uses data from exoplanets, worlds beyond our solar system, to tell us about their polka-dotted stars.Credit: NASA’s Goddard Space Flight CenterMusic: “Whimsical Whirlwinds,” Claire Leona Batchelor [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Get the vertical version of this video [here](https://svs.gsfc.nasa.gov/14797/){target=_blank}. || PolkaDotStars_Thumbnail.jpg (1920x1080) [145.7 KB] || PolkaDotStars_Thumbnail_print.jpg (1024x576) [59.8 KB] || PolkaDotStars_Thumbnail_searchweb.png (320x180) [33.1 KB] || PolkaDotStars_Thumbnail_thm.png (80x40) [3.1 KB] || 14883_MappingStellarPolkaDots_Low.mp4 (1920x1080) [74.2 MB] || 14883_MappingStellarPolkaDots.mp4 (1920x1080) [262.9 MB] || MappingStellarPolkaDotsCaptions.en_US.srt [1.4 KB] || 14883_MappingStellarPolkaDots_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 143 }, { "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": 87 }, { "id": 14792, "url": "https://svs.gsfc.nasa.gov/14792/", "result_type": "Produced Video", "release_date": "2025-05-27T20:57:00-04:00", "title": "Astrophysics Missions Vertical Video", "description": "This page collects vertical videos related to specific Astrophysics missions and their hardware or capabilities.", "hits": 100 }, { "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": 3359 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 323 }, { "id": 14819, "url": "https://svs.gsfc.nasa.gov/14819/", "result_type": "Produced Video", "release_date": "2025-05-06T10:45:00-04:00", "title": "NASA's NICER Studies Recurring Cosmic Crashes", "description": "Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" by Lee Groves [PRS] and Peter Geogre Marett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_thumbnail_NICER_QPE.jpg (1280x720) [225.7 KB] || YTframe_thumbnail_NICER_QPE_searchweb.png (320x180) [95.5 KB] || YTframe_thumbnail_NICER_QPE_thm.png [8.7 KB] || 14819_NICER_QPE_Good.mp4 (1920x1080) [70.6 MB] || 14819_NICER_QPE_Best.mp4 (1920x1080) [172.3 MB] || 14819_NICER_QPE_Captions.en_US.srt [2.8 KB] || 14819_NICER_QPE_Captions.en_US.vtt [2.7 KB] || 14819_NICER_QPE_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ", "hits": 155 }, { "id": 14809, "url": "https://svs.gsfc.nasa.gov/14809/", "result_type": "Produced Video", "release_date": "2025-03-24T00:00:00-04:00", "title": "Testing AstroPix, A New Gamma-Ray Detector", "description": "An AstroPix detector board rests inside a protective tray in a lab at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The squares in the center are silicon pixel gamma-ray sensors. There are two more under the rectangular copper bus bar, which carries data from the sensors to rest of the A-STEP system. The detector connects to a high-power voltage board and other electronics. Credit: NASA/Sophia RobertsAlt text: Electronic components rest on a lab tableImage description: What looks like a large computer chip — an AstroPix detector — rests inside a white tray on a blue lab bench. The detector is green and has two reflective squares in the middle with a long copper rectangle at right parallel to them. Black wires attached to the bottom of the chip connect it to other pieces of equipment and circuit boards on the lab bench. || ASTEP_Chips3.jpg (8192x5464) [32.7 MB] || ASTEP_Chips3_half.jpg (4096x2732) [3.1 MB] || ASTEP_Chips3_half_searchweb.png (320x180) [109.8 KB] || ASTEP_Chips3_half_thm.png [11.5 KB] || ", "hits": 84 }, { "id": 14794, "url": "https://svs.gsfc.nasa.gov/14794/", "result_type": "Produced Video", "release_date": "2025-03-11T00:00:00-04:00", "title": "Developing NASA’s ComPair-2 Detectors", "description": "ComPair-2 will host a gamma-ray tracker with 10 layers, each with 380 silicon detectors, like the engineering test unit shown here. This trial version allows the mission team to test the electronics, measure how well the detectors work together, and develop assembly procedures for each layer. Credit: NASA/Sophia RobertsAlt text: Scientific hardware on a table Image description: A square piece of scientific hardware rests on a table on top of a silver cover. The hardware has a white board on the bottom with a silver peg at each corner. Inside the pegs is a black square with orange and green electronic components. The green runs along the bottom of the square and takes up the left corner of the black square. The orange electronic components run in 20 stripes along the black square. The orange is interspersed with black. || ComPair2-3_print.jpg (1024x683) [631.9 KB] || ComPair2-3.jpg (8192x5464) [29.1 MB] || ComPair2-3_searchweb.png (320x180) [124.5 KB] || ComPair2-3_web.png (320x213) [137.6 KB] || ComPair2-3_thm.png [28.0 KB] || ", "hits": 64 }, { "id": 14786, "url": "https://svs.gsfc.nasa.gov/14786/", "result_type": "Animation", "release_date": "2025-02-20T00:00:00-05:00", "title": "Swift Spacecraft Animations: 2025", "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || ", "hits": 102 }, { "id": 14680, "url": "https://svs.gsfc.nasa.gov/14680/", "result_type": "Produced Video", "release_date": "2025-01-09T00:00:00-05:00", "title": "Astronauts Prepare for NICER Repair Training", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague participated in a training exercise at the NBL (Neutral Buoyancy Laboratory) at NASA’s Johnson Space Center in Houston. They were rehearsing activities related to repairing NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.Before any spacewalk, astronauts practice and refine procedures in the NBL to simulate — as closely as possible on Earth — the conditions under which they’ll complete the task in space.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s X-ray measurements during orbital daytime.The NICER team developed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 60 }, { "id": 14678, "url": "https://svs.gsfc.nasa.gov/14678/", "result_type": "Produced Video", "release_date": "2025-01-07T00:00:00-05:00", "title": "Astronauts Practice NICER Repair", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague practiced a repair for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station. The training exercise took place in the (NBL) Neutral Buoyancy Laboratory at NASA’s Johnson Space Center in Houston.Before any spacewalk, astronauts rehearse activities in the NBL to simulate — as much as possible — the conditions under which they’ll complete the task in space.In May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the instrument. The damage allows sunlight to reach the detectors during the station’s daytime, saturating sensors and interfering with NICER’s X-ray measurements. The damage does not impact nighttime observations.The NICER team developed a plan to cover the largest areas of damage using five patches, each shaped like a piece of pie, to be inserted into the instrument’s sunshades and locked in place. || ", "hits": 73 }, { "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": 350 }, { "id": 14679, "url": "https://svs.gsfc.nasa.gov/14679/", "result_type": "Produced Video", "release_date": "2024-12-13T00:00:00-05:00", "title": "NICER Caddy Preparation", "description": "In Spring 2024, scientists and engineers at NASA prepared and packed a patch kit for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s measurements during orbital daytime.The NICER team designed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 51 }, { "id": 14650, "url": "https://svs.gsfc.nasa.gov/14650/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Infrared Detector and Spectrometer", "description": "EXCITE (EXoplanet Climate Infrared TElescope) is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during long-duration scientific balloon trips over Antarctica.These images, taken in July 2024, show Peter Nagler and Nat DeNigris preparing EXCITE’s infrared detector and installing it into the mission’s spectrometer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. At the time, the EXCITE team was gearing up for a test flight in Fort Sumner, New Mexico. || ", "hits": 57 }, { "id": 14725, "url": "https://svs.gsfc.nasa.gov/14725/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Payload Prep", "description": "In August 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both Arctic and Antarctic, with the latter offering longer duration flights optimum for observing planets for their entire orbit. || ", "hits": 88 }, { "id": 14726, "url": "https://svs.gsfc.nasa.gov/14726/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Launch and Recovery", "description": "On August 31, 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both the north and south poles, although flights over Antarctica allow for longer-duration flights at a latitude optimum for observing planets for their entire orbit. || ", "hits": 129 }, { "id": 14721, "url": "https://svs.gsfc.nasa.gov/14721/", "result_type": "Produced Video", "release_date": "2024-11-20T10:00:00-05:00", "title": "What's In A Name? NASA's Swift Mission", "description": "Watch to learn how NASA’s Neil Gehrels Swift Observatory got its name.Credit: NASA’s Goddard Space Flight CenterMusic: “In a Conundrum,” Pip Heywood [PRS], Universal Production Music“Spinning Particles,” Christian Telford [ASCAP] and Koichi Sanchez-Imahashi [ASCAP], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Swift_Name_20_Thumbnail2.jpg (1280x720) [308.5 KB] || Swift_Name_20_Thumbnail2_searchweb.png (320x180) [103.9 KB] || Swift_Name_20_Thumbnail2_thm.png (80x40) [9.3 KB] || 14721_Swift20_WhatsInAName_Good.mp4 (1920x1080) [199.2 MB] || 14721_Swift20_WhatsInAName_Best.mp4 (1920x1080) [883.1 MB] || 14721_Swift20_WhatsInAName_Captions.en_US.srt [3.7 KB] || 14721_Swift20_WhatsInAName_Captions.en_US.vtt [3.5 KB] || 14721_Swift20_WhatsInAName_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || ", "hits": 95 }, { "id": 14719, "url": "https://svs.gsfc.nasa.gov/14719/", "result_type": "Visualization", "release_date": "2024-11-13T09:00:00-05:00", "title": "Swift Studies Gas-Churning Monster Black Holes", "description": "Watch as a gas cloud encounters two supermassive black holes. The complex interplay of gravitational and frictional forces causes the cloud to condense and heat. Some of the gas is ejected from the system with each orbit of the black holes.Credit: F. Goicovic et al. 2016Music: \"Forgotten Fortunes,\" Magnum Opus [ASCAP] , Universal Production MusicComplete transcript available. || Sim_Video_Still.jpg (3840x2160) [744.6 KB] || Sim_Video_Still_searchweb.png (320x180) [37.6 KB] || Sim_Video_Still_thm.png (80x40) [3.4 KB] || BH_Binary_TD_Sim_1080_Final.mp4 (1920x1080) [38.5 MB] || BH_Binary_TD_Sim_4k_Final.mp4 (3840x2160) [45.5 MB] || BH_Binary_TD_Sim_4k_Final_best.mp4 (3840x2160) [67.9 MB] || 14719_BinaryBHTDE_Captions.en_US.srt [57 bytes] || 14719_BinaryBHTDE_Captions.en_US.vtt [67 bytes] || BH_Binary_TD_Sim_4k_Final_ProRes.mov (3840x2160) [1.5 GB] || ", "hits": 184 }, { "id": 14705, "url": "https://svs.gsfc.nasa.gov/14705/", "result_type": "Produced Video", "release_date": "2024-10-21T14:00:00-04:00", "title": "A-STEP’s AstroPix Detectors Get Ready for Flight", "description": "Scientists and engineers at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, have been preparing a new gamma-ray detector called AstroPix for an upcoming rocket payload called A-STEP (AstroPix Sounding Rocket Technology dEmonstration Payload).Each detector contains four silicon sensors, and each sensor incorporates 1,225 pixels. A-STEP will carry a three-detector stack to the edge of space on the SubTEC-10 sounding rocket, which will launch in 2025 from NASA’s Wallops Flight Facility in Virginia. The flight’s primary goal is to successfully operate the detectors, with a secondary goal of measuring the rate of impacts from cosmic rays, high-energy particles from space. || ", "hits": 83 }, { "id": 14603, "url": "https://svs.gsfc.nasa.gov/14603/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "NICER Hardware and Patch Kit", "description": "This video shows different components of NICER (Neutron star Interior Composition Explorer). The damaged thermal shield is a flight spare used during the patch testing process.0:00 A NICER patch slowly rotates counterclockwise. 0:14 A top-down view of the same patch, still rotating. 0:21 Another side view of the patch rotating. A gloved hand enters from the right-hand side, picks up the patch, and turns it on its side. The patch begins rotating again, so the tab on the bottom becomes visible. 1:03 A gloved hand slowly tilts a damaged thermal shield. 1:41 The thermal shield rests in a container that slowly rotates. 2:08 A gloved hand rotates a NICER X-ray concentrator. 2:30The camera moves past the X-ray concentrator. 2:52 A hand places a NICER sunshade on the table. 2:58 The sunshade rotates counterclockwise. 3:00 The sunshade rotates on its side.Credit:NASA/Sophia Roberts and Scott Wiessinger || Studio_Shoot_Single_Components.00001_print.jpg (1024x540) [16.9 KB] || Studio_Shoot_Single_Components.00001_searchweb.png (320x180) [23.1 KB] || Studio_Shoot_Single_Components.00001_thm.png (80x40) [2.1 KB] || Studio_Shoot_Single_Components.mp4 (4096x2160) [1.9 GB] || Studio_Shoot_Single_Components.mov (4096x2160) [12.7 GB] || ", "hits": 62 }, { "id": 14609, "url": "https://svs.gsfc.nasa.gov/14609/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "Anodizing NICER’s Patches", "description": "This video shows engineering technician Katrina Harvey anodizing NICER’s patches at the Plating Laboratory at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.0:00 One of the NICER patch bodies hangs from a spiky stick by a wire. 0:05 Patch lids attached to a similar stick are seen submerged in a dark blue liquid. 0:07 Harvey lifts the lids and one patch body from a chemical bath and submerges them in a container of deionized water. 0:24 Several lids have been dyed black. 0:29 Harvey submerges the black lids into a chemical bath covered with white plastic balls. 0:42 Harvey lifts undyed patch bodies from a deionized water rinse. 0:47 Harvey lifts patch bodies from a chemical bath covered in white plastic balls and dunks them in deionized water. 1:07 A wider view of Harvey as she works on the patch bodies in the plating lab. 1:24 The patch bodies are shown submerged in a blue liquid. 1:28 A pan across patch bodies submerged in blue liquid. 1:34 Harvey lifts the patch bodies on their individual wires out of a well where nozzles spray them with deionized water. She then dunks them several times in a container of black dye. 1:54 She adds more patch bodies to the black dye. 2:22 She hangs the dyed bodies in a well where nozzles spray them with deionized water. 2:35 Harvey sprays the patches with deionized water. 2:40 Keith Gendreau (NASA), Steve Kenyon (NASA), and Isiah Holt (NASA) cluster together, looking at one of the dyed NICER patch bodies. 2:48 Harvey rinses dyed patch bodies. 2:58 Harvey holds several dyed patch bodies still on their wires. She lifts them and starts walking through the lab. 3:18 Gendreau and Kenyon help remove plugs from holes in the patch bodies. These protected screw threads during the anodizing process. 3:32: Someone dries one of the patch bodies with compressed air. 3:42 The dyed patch bodies rest on a table. 3:58 Close-ups of various features of the lab, like labels, knobs, readouts, buttons, clamps, and wires.Credit:NASA/Sophia Roberts and Scott Wiessinger || Anondizing_Patches_at_4k.00001_print.jpg (1024x576) [72.4 KB] || Anondizing_Patches_at_4k.00001_searchweb.png (320x180) [61.0 KB] || Anondizing_Patches_at_4k.00001_thm.png (80x40) [5.0 KB] || Anondizing_Patches_at_4k.webm (3840x2160) [99.1 MB] || Anondizing_Patches_at_4k.mp4 (3840x2160) [2.5 GB] || Anondizing_Patches_at_4k_ProRes.mov (3840x2160) [18.3 GB] || ", "hits": 53 }, { "id": 14610, "url": "https://svs.gsfc.nasa.gov/14610/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "Machining NICER’s Patches", "description": "This video shows Richard Koenecke, an engineer at NASA’s Goddard Space Flight Center, creating the body of one of the NICER (Neutron star Interior Composition Explorer) patches.0:00 Two blocks of aluminum sit on a counter in front of a laptop that displays the schematics for the NICER patches. 0:06 Koenecke puts one block on the bed of a saw littered with metal shavings and then trims the block. 0:23 Koenecke sands down the block’s rough edges. 0:30 Koenecke walks into another part of his workshop. 0:37 Koenecke preps the machining chamber. 0:49 Inside the chamber, the machine starts to carve out the shape of the patch. Fluid sprayed from the nozzles above the tool helps cool the metal. 0:56 Koenecke looks into the chamber. 0:59 The chamber is shown at different angles. 1:15 Koenecke walking up to the chamber window. 1:22 Inside the chamber, the patch’s shape is now visible amidst a sea of aluminum shavings. 1:25 The cutting tool refines the shape of the patch. 1:40 Koenecke looks at a computer readout for the machining chamber. 1:45 Inside the chamber, the cutting tool lowers to hollow out the patch. 1:56 Koenecke holds and turns a block of the aluminum. 2:45 Koenecke’s dog Sara guards his shop on the Eastern Shore. 2:53 Koenecke sands a block of aluminum. 3:01 He closes the doors to the machining chamber and adjusts the settings on a computer screen. 3:10 Numbers change on the chamber’s computer screen. 3:31 Koenecke holds and turns the fully machined patch body. 3:51 In slow motion, Koenecke walking through his shop. 4:25 In slow motion, Koenecke holds the patch in close-up shots.Credit: NASA/Sophia Roberts and Scott Wiessinger || Machine_Shop_B-roll_-_Part_1.03720_print.jpg (1024x576) [111.0 KB] || Machine_Shop_B-roll_-_Part_1.03720_searchweb.png (320x180) [82.6 KB] || Machine_Shop_B-roll_-_Part_1.03720_thm.png (80x40) [6.8 KB] || Machine_Shop_B-roll_-_Part_1.webm (3840x2160) [74.7 MB] || Machine_Shop_B-roll_-_Part_1.mp4 (3840x2160) [2.5 GB] || Machine_Shop_B-roll_-_Part_1_ProRes.mov (3840x2160) [18.0 GB] || ", "hits": 61 }, { "id": 14608, "url": "https://svs.gsfc.nasa.gov/14608/", "result_type": "Produced Video", "release_date": "2024-06-24T13:00:00-04:00", "title": "BurstCube Deploys from International Space Station", "description": "The shoebox-sized BurstCube and SNOOPI (Signals of Opportunity P-band Investigation) satellites entered low-Earth orbit from the International Space Station on April 18, 2024.BurstCube will study gamma-ray bursts, the universe’s most powerful explosions. SNOOPI will demonstrate technology for measuring soil moisture. These CubeSats launched to the space station aboard SpaceX’s 30th Commercial Resupply Services mission on March 21, 2024 || ", "hits": 78 }, { "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": 117 }, { "id": 14522, "url": "https://svs.gsfc.nasa.gov/14522/", "result_type": "Produced Video", "release_date": "2024-04-16T12:00:00-04:00", "title": "Fermi Sees No Gamma Rays from Nearby Supernova", "description": "Even when it doesn’t detect gamma rays, NASA’s Fermi Gamma-ray Space Telescope helps astronomers learn more about the universe.Credit: NASA’s Goddard Space Flight CenterMusic: \"Trial\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Fermi_Missing_GR_Still.jpg (1920x1080) [757.8 KB] || Fermi_Missing_GR_Still_searchweb.png (320x180) [86.6 KB] || Fermi_Missing_GR_Still_thm.png (80x40) [6.5 KB] || 14522_Fermi_Missing_GammaRays_Captions.en_US.srt [3.4 KB] || 14522_Fermi_Missing_GammaRays_Captions.en_US.vtt [3.2 KB] || 14522_Fermi_Missing_GammaRays_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 14522_Fermi_Missing_GammaRays_Good.mp4 (1920x1080) [110.3 MB] || 14522_Fermi_Missing_GammaRays_Best.mp4 (1920x1080) [382.1 MB] || ", "hits": 146 }, { "id": 14727, "url": "https://svs.gsfc.nasa.gov/14727/", "result_type": "Produced Video", "release_date": "2024-01-22T00:00:00-05:00", "title": "Fort Sumner, New Mexico: 2024 Drone Views", "description": "This clip contains various shots of the NASA payload processing facility at Fort Sumner as well as general views of the surrounding area, acquired Aug. 23, 2024. Credit: NASA/Francis ReddyVideo playback is at half speed (30 fps). 0:00 A slow, early morning approach to the staging facility as its doors open, revealing the EXCITE (EXoplanet Climate Infrared TElescope) payload. 0:45 The camera descends, with the rising sun moving behind the staging facility. 0:58 A closer, lower approach to the EXCITE payload. 1:10 A higher, more distant arc that starts by showing the low sun and the NASA sign on the staging facility, moving north. 1:41 A slow ascent looking toward EXCITE and the morning sun. 1:28 Hovering as the doors close on EXCITE. 03:20 Overview flying back across the airport revealing various vehicles and structures. 4:41 Similar, but at higher altitude and flying in a different direction. || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.00001_print.jpg (1024x576) [139.0 KB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.webm (3840x2160) [67.5 MB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.mp4 (3840x2160) [2.9 GB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility_ProRes.mov (3840x2160) [22.1 GB] || ", "hits": 49 }, { "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": 129 }, { "id": 14492, "url": "https://svs.gsfc.nasa.gov/14492/", "result_type": "Produced Video", "release_date": "2024-01-05T08:50:00-05:00", "title": "XRISM Reveals Its First Look at X-ray Cosmos", "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ", "hits": 150 }, { "id": 14487, "url": "https://svs.gsfc.nasa.gov/14487/", "result_type": "Produced Video", "release_date": "2023-12-18T13:00:00-05:00", "title": "BurstCube Completes Magnetic Calibration", "description": "BurstCube is a mission developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. It is expected to launch in March 2024. This CubeSat will detect short gamma-ray bursts, brief flashes of the highest-energy form of light. Dense stellar remnants called neutron stars create these bursts when they collide with other neutron stars or black holes. Short gamma-ray bursts, which last less than 2 seconds, are important sources for gravitational wave discoveries and multimessenger astronomy. BurstCube will use Earth’s magnetic field to orientate itself as it scans the sky. To do so, the mission team had to map the spacecraft’s own magnetic field using a special facility at NASA’s Wallops Flight Facility in Virginia. The magnetic calibration chamber generates a known magnetic field that cancels out Earth’s. The team's measurements of BurstCube’s field in the chamber will help figure out where the satellite is pointing once in space, so scientists can locate gamma-ray bursts and tell other observatories where to look. || ", "hits": 94 }, { "id": 14488, "url": "https://svs.gsfc.nasa.gov/14488/", "result_type": "Produced Video", "release_date": "2023-12-18T11:00:00-05:00", "title": "BurstCube Gets Its Solar Panels", "description": "Engineers work on the BurstCube mission’s solar panels in this video. The first shot pans across the spacecraft as it rests on a table, panels unfolded. The second shot starts close to the spacecraft, then pulls back. The third shot shows NASA engineers Julie Cox and Kate Gasaway attaching one of the panels. The fourth shot shows one of the unattached panels sitting on a piece of foil on a blue tabletop. The fifth shot is a wider view of the unattached panel with Cox in view. The sixth and seventh shots show Cox and Gasaway attaching the second panel to the other side of the spacecraft, from the side and above, respectively. The final shot shows a test deployment of the solar panels. Credit: NASA/Sophia Roberts || BurstCube_Solar_Panel_Install_4k.00060_print.jpg (1024x540) [110.8 KB] || BurstCube_Solar_Panel_Install_4k.00060_searchweb.png (320x180) [65.1 KB] || BurstCube_Solar_Panel_Install_4k.00060_thm.png (80x40) [5.4 KB] || BurstCube_Solar_Panel_Install_4k.webm (4096x2160) [28.3 MB] || BurstCube_Solar_Panel_Install_Clips4k_ProRes.mov (4096x2160) [7.6 GB] || BurstCube_Solar_Panel_Install_4k.mp4 (4096x2160) [1.0 GB] || ", "hits": 80 }, { "id": 14489, "url": "https://svs.gsfc.nasa.gov/14489/", "result_type": "Produced Video", "release_date": "2023-12-18T11:00:00-05:00", "title": "BurstCube Completes Thermal Vacuum Testing", "description": "BurstCube is a mission developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The spacecraft is slated for takeoff in March 2024 from NASA’s Kennedy Space Center in Florida aboard a resupply mission to the International Space Station. This CubeSat will detect short gamma-ray bursts, brief flashes of the highest-energy form of light. Dense stellar remnants called neutron stars create these bursts when they collide with other neutron stars or black holes. Short gamma-ray bursts, which last less than 2 seconds, are important sources for gravitational wave discoveries and multimessenger astronomy. As BurstCube orbits, it will experience major temperature swings every 90 minutes as it passes in and out of daylight. The team evaluated how the spacecraft will operate in these new conditions using a thermal vacuum chamber at Goddard, shown in these images and video, where temperatures ranged from minus 4 to 113 degrees Fahrenheit (minus 20 to 45 Celsius). || ", "hits": 82 }, { "id": 14490, "url": "https://svs.gsfc.nasa.gov/14490/", "result_type": "Produced Video", "release_date": "2023-12-18T11:00:00-05:00", "title": "BurstCube Completes an Open-Sky Test", "description": "This video shows engineers conducting an open-sky test of the BurstCube satellite’s GPS at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The first shot shows Benjamin Nold (NASA) and Justin Clavette (SSAI) sitting around the spacecraft on a rooftop while Kate Gasaway (NASA) works in the background. The second shot shows Gasaway and Clavette looking at a laptop in the background, with BurstCube in the foreground. The third shot shows birds landing on an antenna on the rooftop. The fourth shot shows Clavette and Nold crouched next to the BurstCube satellite. The fifth shot shows Gasaway typing on the laptop. The sixth shot is a closer view of Gasaway and Clavette looking at the laptop. The eighth shot shows some of the electronics used to monitor the spacecraft. The ninth shot shows the data readout from the spacecraft on the laptop. The final shots show birds flying over the rooftop. Credit: NASA/Sophia Roberts || Open_Air_test_4k.01440_print.jpg (1024x540) [103.1 KB] || Open_Air_test_4k.01440_searchweb.png (320x180) [74.5 KB] || Open_Air_test_4k.01440_web.png (320x168) [70.2 KB] || Open_Air_test_4k.01440_thm.png (80x40) [5.8 KB] || Open_Air_test_4k.webm (4096x2160) [27.4 MB] || Open_Air_test_4k.mp4 (4096x2160) [891.4 MB] || BurstCube_Open_Air_test_4k_ProRes.mov (4096x2160) [6.5 GB] || ", "hits": 78 }, { "id": 14408, "url": "https://svs.gsfc.nasa.gov/14408/", "result_type": "Produced Video", "release_date": "2023-09-07T11:00:00-04:00", "title": "Swift Spots a Snacking Black Hole Using a New Trick", "description": "Watch to learn how an update to NASA’s Neil Gehrels Swift Observatory allowed it to catch a supersized black hole in a distant galaxy munching repeatedly on a circling star. Credit: NASA’s Goddard Space Flight CenterMusic: \"Teapot Waltz\" by Benjamin Parsons from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Repeating_TDE_Still.jpg (1920x1080) [446.8 KB] || Repeating_TDE_Still_searchweb.png (320x180) [63.3 KB] || Repeating_TDE_Still_thm.png (80x40) [4.6 KB] || 14408_Repeating_TDE_sub100.mp4 (1920x1080) [89.7 MB] || Repeating_TDE_SRT_Captions.en_US.srt [1.7 KB] || Repeating_TDE_SRT_Captions.en_US.vtt [1.6 KB] || 14408_Repeating_TDE_ProRes_1920x1080_2997.mov (1920x1080) [1.2 GB] || 14408_Repeating_TDE_1080.mp4 (1920x1080) [186.2 MB] || ", "hits": 132 }, { "id": 14405, "url": "https://svs.gsfc.nasa.gov/14405/", "result_type": "Produced Video", "release_date": "2023-08-25T10:00:00-04:00", "title": "XRISM: Exploring the Hidden X-ray Cosmos", "description": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim || YTframe_XRISM_Exploring_XrayCosmos.jpg (1280x720) [668.5 KB] || YTframe_XRISM_Exploring_XrayCosmos_searchweb.png (320x180) [100.3 KB] || YTframe_XRISM_Exploring_XrayCosmos_thm.png (80x40) [7.6 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.srt [7.8 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.vtt [7.4 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mov (3840x2160) [21.6 GB] || ", "hits": 273 }, { "id": 12956, "url": "https://svs.gsfc.nasa.gov/12956/", "result_type": "Produced Video", "release_date": "2023-08-15T10:00:00-04:00", "title": "Spectroscopy, Explained", "description": "Video producer Sophia Roberts explains the basic principles behind spectroscopy, the science of reading light to determine the size, distance, spin and chemical composition of distant objects in space. Complete transcript available.Music Credits:Universal Production MusicOxygenate the Idea – by Amon Turner, Banksman, Eben StoneJungle Bounce – by Siddharth NadkarniSilent Patient – by Paul Reeves Background Story - by Peter LarsenData Dynamism – by Florian Moenks and Aron Wright Watch this video on the NASA Goddard YouTube channel. || Spectroscopy,_Explained_Thumbnail.jpg (3840x2160) [2.2 MB] || Spectroscopy,_Explained_Thumbnail_searchweb.png (320x180) [75.1 KB] || Spectroscopy,_Explained_Thumbnail_thm.png (80x40) [6.3 KB] || Spectroscopy,_Explained_Final_1080.mp4 (1920x1080) [412.9 MB] || SpectroscopyExplainedAdjustedCaptions.en_US.srt [11.1 KB] || SpectroscopyExplainedAdjustedCaptions.en_US.vtt [10.5 KB] || Spectroscopy_Explained.webm (3840x2160) [125.6 MB] || Spectroscopy_Explained.mp4 (3840x2160) [1.1 GB] || Spectroscopy,_Explained_Final_Best_4k.mp4 (3840x2160) [2.5 GB] || Spectroscopy,_Explained_Final_ProRes.mov (3840x2160) [43.3 GB] || ", "hits": 354 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 82 }, { "id": 14372, "url": "https://svs.gsfc.nasa.gov/14372/", "result_type": "B-Roll", "release_date": "2023-07-20T10:00:00-04:00", "title": "ComPair Thermal Vacuum Photos", "description": "Team members work on the ComPair balloon instrument before it begins testing in a thermal vacuum chamber at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. ComPair project manager Regina Caputo (front right), graduate student Nicholas Kirschner (George Washington University, left), and research scientist Nicholas Cannady (University of Maryland Baltimore County, rear) examine ComPair's various components to determine what needs to be “harnessed,” or connected via cable to power systems and the onboard computer.Credit: NASA/Scott Wiessinger || ComPair_TVac_IMG_2141.png (5319x3546) [30.9 MB] || ComPair_TVac_IMG_2141.jpg (5319x3546) [6.0 MB] || ComPair_TVac_IMG_2141_half.jpg (2659x1773) [1.4 MB] || ", "hits": 78 }, { "id": 14354, "url": "https://svs.gsfc.nasa.gov/14354/", "result_type": "B-Roll", "release_date": "2023-05-25T00:00:00-04:00", "title": "ComPair Gamma-Ray Balloon Mission", "description": "Carolyn Kierans, principal investigator for the ComPair balloon mission at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, works on the instrument in this video. First, she assembles a layer of the tracker, which is housed in an aluminum casing. Next, she shows one of the tracker’s silicon detectors. Then she takes the lid off the tracker.Credit: NASA/Sophia Roberts || Unassembled_Parts_of_ComPair.01740_print.jpg (1024x540) [148.3 KB] || Unassembled_Parts_of_ComPair.01740_searchweb.png (320x180) [94.0 KB] || Unassembled_Parts_of_ComPair.01740_thm.png (80x40) [7.0 KB] || Unassembled_Parts_of_ComPair.webm (4096x2160) [18.2 MB] || Unassembled_Parts_of_ComPair.mp4 (4096x2160) [570.8 MB] || ", "hits": 44 }, { "id": 14282, "url": "https://svs.gsfc.nasa.gov/14282/", "result_type": "Produced Video", "release_date": "2023-05-17T11:00:00-04:00", "title": "Spitzer, TESS Find Potential Earth-Size World Covered in Volcanoes", "description": "LP 791-18 d, illustrated here in an artist's concept, is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system. Astronomers discovered and studied the planet using data from NASA’s Spitzer Space Telescope and TESS (Transiting Exoplanet Survey Satellite) along with many other observatories.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || LP79118d_BeautyShot.jpg (2048x1152) [130.9 KB] || LP79118d_Temperate_Earth_BeautyShot_Full.jpg (5760x3240) [2.2 MB] || LP79118d_Temperate_Earth_BeautyShot_Full.png (5760x3240) [12.4 MB] || LP79118d_BeautyShot_searchweb.png (320x180) [59.9 KB] || LP79118d_BeautyShot_thm.png (80x40) [5.1 KB] || ", "hits": 112 }, { "id": 14309, "url": "https://svs.gsfc.nasa.gov/14309/", "result_type": "Produced Video", "release_date": "2023-03-15T11:00:00-04:00", "title": "Fermi Captures Dynamic Gamma-ray Sky", "description": "Watch a cosmic gamma-ray fireworks show in this animation using just a year of data from the Large Area Telescope (LAT) aboard NASA’s Fermi Gamma-ray Space Telescope. Each object’s magenta circle grows as it brightens and shrinks as it dims. The yellow circle represents the Sun following its apparent annual path across the sky. The animation shows a subset of the LAT gamma-ray records now available for more than 1,500 objects in a new, continually updated repository. Over 90% of these sources are a type of galaxy called a blazar, powered by the activity of a supermassive black hole.Credit: NASA’s Marshall Space Flight Center/Daniel Kocevski || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_ProRes_3840x2160.mov (3840x2160) [170.3 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1600.gif (1600x900) [6.5 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1050.gif (1050x590) [3.2 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark.gif (800x450) [2.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.mp4 (3840x2160) [12.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.webm (3840x2160) [1.9 MB] || ", "hits": 105 }, { "id": 14281, "url": "https://svs.gsfc.nasa.gov/14281/", "result_type": "Produced Video", "release_date": "2023-01-26T11:00:00-05:00", "title": "Fermi Spots Gamma-ray Eclipsing 'Spider Systems'", "description": "An orbiting star begins to eclipse its partner, a rapidly rotating, superdense stellar remnant called a pulsar, in this illustration. The pulsar emits multiwavelength beams of light that rotate in and out of view and produces outflows that heat the star’s facing side, blowing away material and eroding its partner.Credit: NASA/Sonoma State University, Aurore Simonnet || GamRayEclipseG22.jpg (1800x1200) [1.1 MB] || GamRayEclipseG22_searchweb.png (320x180) [70.2 KB] || GamRayEclipseG22_thm.png (80x40) [6.8 KB] || ", "hits": 80 }, { "id": 14264, "url": "https://svs.gsfc.nasa.gov/14264/", "result_type": "Produced Video", "release_date": "2023-01-10T13:00:00-05:00", "title": "TESS Finds System’s Second Earth-Size World", "description": "Watch to learn about TOI 700 e, a newly discovered Earth-size planet with an Earth-size sibling. Credit: NASA/JPL-Caltech/Robert Hurt/NASA’s Goddard Space Flight CenterMusic Credit: Dream Box by Carl David HarmsWatch this video on the NASA Goddard YouTube channel. || Title_Card_TOI700_e.jpg (1920x1080) [1.2 MB] || Second_Habitable_World_in_TOI700.00250_print.jpg (1024x576) [50.0 KB] || Second_Habitable_World_in_TOI700.00250_searchweb.png (320x180) [50.3 KB] || Second_Habitable_World_in_TOI700.00250_thm.png (80x40) [3.4 KB] || Second_Habitable_World_in_TOI700.mp4 (1920x1080) [69.1 MB] || Second_Habitable_World_in_TOI700.webm (1920x1080) [7.7 MB] || Second_Habitable_World_in_TOI700_ProRes.mov (1920x1080) [948.8 MB] || Second_Habitable_World_in_TOI700.en_US.srt [1.1 KB] || Second_Habitable_World_in_TOI700.en_US.vtt [1.1 KB] || ", "hits": 322 }, { "id": 14255, "url": "https://svs.gsfc.nasa.gov/14255/", "result_type": "Produced Video", "release_date": "2022-12-07T11:00:00-05:00", "title": "NASA’s Fermi, Swift Capture Revolutionary Gamma-Ray Burst", "description": "Watch to learn how an event called GRB 211211A rocked scientists’s understanding of gamma-ray bursts – the most powerful explosions in the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic Credits: \"Finished Plate\" by Airglo and \"Binary Fission\" by Tom KaneWatch this video on the NASA Goddard YouTube channel. || Title_Card_Revolutionary_GRB.jpg (1920x1080) [1.5 MB] || Title_Card_Revolutionary_GRB_searchweb.png (320x180) [100.7 KB] || Title_Card_Revolutionary_GRB_thm.png (80x40) [7.3 KB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.mp4 (1920x1080) [171.9 MB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst_ProRes.mov (1920x1080) [2.2 GB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.webm (1920x1080) [18.4 MB] || Long_GRB_Captions.en_US.srt [2.8 KB] || Long_GRB_Captions.en_US.vtt [2.8 KB] || ", "hits": 125 }, { "id": 14167, "url": "https://svs.gsfc.nasa.gov/14167/", "result_type": "Produced Video", "release_date": "2022-10-31T11:00:00-04:00", "title": "BurstCube Integration", "description": "BurstCube is a mission under development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. This CubeSat will detect short gamma-ray bursts, which are important sources for gravitational wave discoveries and multimessenger astronomy. The satellite is expected to launch in March 2024. || ", "hits": 52 }, { "id": 20371, "url": "https://svs.gsfc.nasa.gov/20371/", "result_type": "Animation", "release_date": "2022-10-28T14:00:00-04:00", "title": "BurstCube Animations", "description": "BurstCube is a mission under development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. This CubeSat will detect short gamma-ray bursts, which are important sources for gravitational wave discoveries and multimessenger astronomy. The satellite is expected to launch in 2023. || ", "hits": 51 }, { "id": 14146, "url": "https://svs.gsfc.nasa.gov/14146/", "result_type": "Produced Video", "release_date": "2022-05-04T00:00:00-04:00", "title": "Black Hole Desktop & Phone Wallpapers", "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ", "hits": 3981 }, { "id": 20367, "url": "https://svs.gsfc.nasa.gov/20367/", "result_type": "Animation", "release_date": "2022-04-28T00:00:00-04:00", "title": "Gravitational Wave", "description": "Two black holes orbit around each other and generate space-time ripples called gravitational waves in this animation. As the black holes get closer, the waves increase in frequency. Eventually, the event horizons merge into a peanut-shaped object, generating one very high-frequency wave. Within a rotation, the black holes merge completely. One lower-frequency wave, called the ring down, ripples out after the merger.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || A_Gravitational_Wave_ProRes.00450_print.jpg (1024x576) [119.9 KB] || A_Gravitational_Wave_ProRes.00450_searchweb.png (320x180) [78.6 KB] || A_Gravitational_Wave_ProRes.00450_thm.png (80x40) [6.8 KB] || A_Gravitational_Wave_ProRes.mov (3840x2160) [2.2 GB] || A_Gravitational_Wave_h264.mp4 (3840x2160) [40.4 MB] || A_Gravitational_Wave (3840x2160) [128.0 KB] || A_Gravitational_Wave_ProRes.webm (3840x2160) [15.0 MB] || ", "hits": 231 }, { "id": 14130, "url": "https://svs.gsfc.nasa.gov/14130/", "result_type": "Produced Video", "release_date": "2022-04-07T14:00:00-04:00", "title": "Fermi Searches for Gravitational Waves From Monster Black Holes", "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ", "hits": 103 }, { "id": 14099, "url": "https://svs.gsfc.nasa.gov/14099/", "result_type": "Produced Video", "release_date": "2022-02-28T00:00:00-05:00", "title": "Black Hole Week Assets", "description": "This page will introduce you to the world, characters, colors, and fonts of Black Hole Week. NASA celebrated Black Hole Week in 2019, 2021 and May, 2022.The world of Black Hole Week is bold, colorful, and a bit retro. It's also populated by a fun bunch of characters, including a little blue explorer (called the \"Traveler\") and their black hole friends. Below, you'll find tons of helpful images, GIFs, and other materials to get you going if you want to join in!If you are having trouble downloading the ZIP or AI files, please contact Barb Mattson: barb.mattson@nasa.gov || ", "hits": 265 }, { "id": 14000, "url": "https://svs.gsfc.nasa.gov/14000/", "result_type": "Produced Video", "release_date": "2021-11-26T10:00:00-05:00", "title": "Supercomputer Simulations Test Star-destroying Black Holes", "description": "Watch eight model stars stretch and deform as they approach a virtual black hole 1 million times the mass of the Sun. The black hole’s gravity rips some stars apart into a stream of gas, a phenomenon called a tidal disruption event. Others manage to withstand their close encounters. These simulations show that destruction and survival depend on the stars’ initial densities. Yellow represents the greatest densities, blue the least dense. Credit: NASA's Goddard Space Flight Center/Taeho Ryu (MPA)Music: \"Lava Flow Instrumental\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14000_TDE_Simulation_Still.jpg (1920x1080) [205.0 KB] || 14000_TDE_Simulation_Still_searchweb.png (320x180) [42.8 KB] || 14000_TDE_Simulation_Still_thm.png (80x40) [4.9 KB] || 14000_TDE_Simulation_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 14000_TDE_Simulation_Best_1080.mp4 (1920x1080) [357.4 MB] || 14000_TDE_Simulation_1080.mp4 (1920x1080) [164.7 MB] || 14000_TDE_Simulation_1080.webm (1920x1080) [17.6 MB] || 14000_TDE_Simulation_SRT_Captions.en_US.srt [2.7 KB] || 14000_TDE_Simulation_SRT_Captions.en_US.vtt [2.7 KB] || ", "hits": 131 }, { "id": 13876, "url": "https://svs.gsfc.nasa.gov/13876/", "result_type": "Produced Video", "release_date": "2021-07-12T10:00:00-04:00", "title": "TESS Finds Related Stars Have Young Exoplanets", "description": "Stellar siblings over 130 light-years away host two systems of teenage planets. Watch to learn how NASA’s Transiting Exoplanet Survey Satellite discovered these young worlds and what they might tell us about the evolution of planetary systems everywhere, including our own.Music Credit: \"Building Ideas\" from Universal Production MusicCredit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || tess_stellar_siblings_label.jpg (1920x1080) [572.8 KB] || stellar_siblings_still_01.jpg (1920x1080) [536.3 KB] || stellar_siblings_still_01_print.jpg (1024x576) [179.0 KB] || stellar_siblings_still_01_searchweb.png (320x180) [57.0 KB] || stellar_siblings_still_01_web.png (320x180) [57.0 KB] || stellar_siblings_still_01_thm.png (80x40) [4.7 KB] || TESS_stellar_siblings_HQ.mp4 (1920x1080) [286.2 MB] || TESS_stellar_siblings_LQ.mp4 (1920x1080) [150.7 MB] || TESS_stellar_siblings_prores.mov (1920x1080) [1.6 GB] || TESS_stellar_siblings_LQ.webm (1920x1080) [16.0 MB] || TESS_stellar_siblings_prores.en_US.srt [2.0 KB] || TESS_stellar_siblings_prores.en_US.vtt [2.0 KB] || ", "hits": 122 }, { "id": 13832, "url": "https://svs.gsfc.nasa.gov/13832/", "result_type": "Produced Video", "release_date": "2021-04-17T11:00:00-04:00", "title": "NASA’s NICER Tests Matter’s Limits", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) is helping physicists peer into the hearts of neutron stars, the remains of massive stars that exploded in supernovae. Scientists want to explore the nature of matter inside these objects, where it exists on the verge of collapsing into black holes. To do so, scientists need precise measurements of neutron stars’ masses and sizes, which NICER and other efforts are now making possible.Credit: NASA’s Goddard Space Flight CenterMusic: \"Question Time\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Video_title_card_2.jpg (1920x1080) [206.4 KB] || Video_title_card_2_searchweb.png (320x180) [54.8 KB] || Video_title_card_2_thm.png (80x40) [5.7 KB] || 13832_NICER_TestsMattersLimits_Best_1080.webm (1920x1080) [28.5 MB] || 13832_NICER_TestsMattersLimits_1080.mp4 (1920x1080) [187.8 MB] || 13832_NICER_TestsMattersLimits_Best_1080.mp4 (1920x1080) [650.1 MB] || 13832_NICER_TestsMattersLimits_SRT_Captions.en_US.srt [4.7 KB] || 13832_NICER_TestsMattersLimits_SRT_Captions.en_US.vtt [4.8 KB] || 13832_NICER_TestsMattersLimits_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || ", "hits": 433 }, { "id": 13834, "url": "https://svs.gsfc.nasa.gov/13834/", "result_type": "Produced Video", "release_date": "2021-04-12T10:00:00-04:00", "title": "NASA's Field Guide to Black Holes", "description": "Thinking about doing some black hole watching the next time you’re on an intergalactic vacation, but you’re not quite sure where to start? Well, look no further! This series of videos shows you everything you need to know. With topics ranging from basic black holes, to fancy black holes, to giant black holes and their companions, you’ll be more than ready for your next adventure.In addition to the videos, you can also download a printable guide that has even more information.Note: While these videos can be shared in their entirety without permission, their music has been licensed and may not be excised or remixed in other products. || ", "hits": 122 }, { "id": 13806, "url": "https://svs.gsfc.nasa.gov/13806/", "result_type": "Produced Video", "release_date": "2021-03-12T11:00:00-05:00", "title": "Scientists Build a Detailed Image of U Mon Binary", "description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ", "hits": 45 }, { "id": 13805, "url": "https://svs.gsfc.nasa.gov/13805/", "result_type": "Produced Video", "release_date": "2021-02-22T11:00:00-05:00", "title": "Swift Links Neutrino to Star-destroying Black Hole", "description": "Watch how a monster black hole ripping apart a star may have launched a ghost particle toward Earth. Astronomers have long predicted that tidal disruption events could produce high-energy neutrinos, nearly massless particles from outside our galaxy traveling close to the speed of light. One recent event, named AT2019dsg, provides the first proof this prediction is true but has challenged scientists’ assumptions of where and when these elusive particles might form during these destructive outbursts. Credit: NASA’s Goddard Space Flight CenterMusic: \"Diagnostic Report\" from Universal Production MusicComplete transcript available. || AT2019dsg_prores_still.jpg (1920x1080) [299.2 KB] || AT2019dsg_prores_still_print.jpg (1024x576) [119.5 KB] || AT2019dsg_prores_still_searchweb.png (180x320) [42.6 KB] || AT2019dsg_prores_still_web.png (320x180) [42.6 KB] || AT2019dsg_prores_still_thm.png (80x40) [4.1 KB] || AT2019dsg_HQ.mp4 (1920x1080) [347.5 MB] || AT2019dsg_LQ.mp4 (1920x1080) [191.3 MB] || AT2019dsg_prores.mov (1920x1080) [1.7 GB] || AT2019dsg_LQ.webm (1920x1080) [21.5 MB] || AT2019dsg_LQ.en_US.srt [3.7 KB] || AT2019dsg_LQ.en_US.vtt [3.7 KB] || ", "hits": 203 }, { "id": 13798, "url": "https://svs.gsfc.nasa.gov/13798/", "result_type": "Produced Video", "release_date": "2021-01-12T12:15:00-05:00", "title": "Swift, TESS Catch Eruptions from an Active Galaxy", "description": "Watch as a monster black hole partially consumes an orbiting giant star. In this illustration, the gas pulled from the star collides with the black hole’s debris disk and causes a flare. Astronomers have named this repeating event ASASSN-14ko. The flares are the most predictable and frequent yet seen from an active galaxy. Credit: NASA’s Goddard Space Flight CenterMusic: \"Ruminations\" from Universal Production MusicComplete transcript available. || periodic_AGN_still.jpg (1920x1080) [512.8 KB] || periodic_AGN_still_print.jpg (1024x576) [229.4 KB] || periodic_AGN_still_searchweb.png (320x180) [77.1 KB] || periodic_AGN_still_web.png (320x180) [77.1 KB] || periodic_AGN_still_thm.png (80x40) [6.3 KB] || periodic_AGN_HQ.mp4 (1920x1080) [230.6 MB] || periodic_AGN_LQ.mp4 (1920x1080) [123.5 MB] || periodic_AGN_prores.mov (1920x1080) [1.3 GB] || periodic_AGN_LQ.webm (1920x1080) [13.2 MB] || periodic_AGN_prores.mov.en_US.srt [1.6 KB] || periodic_AGN_prores.mov.en_US.vtt [1.6 KB] || ", "hits": 98 }, { "id": 13636, "url": "https://svs.gsfc.nasa.gov/13636/", "result_type": "Produced Video", "release_date": "2020-09-30T10:00:00-04:00", "title": "Join the Hunt for New Worlds Through Planet Patrol", "description": "Want to hunt the skies for uncharted worlds from home? Join Planet Patrol! Watch to learn how you can collaborate with professional astronomers and analyze images from NASA's Transiting Exoplanet Survey Satellite (TESS) on your own. You'll answer questions about each TESS image and help scientists figure out if they contain signals from new worlds or planetary imposters.Credit: NASA's Goddard Space Flight Center/Conceptual Image LabMusic: \"A Wonderful Loaf\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Planet_Patrol_Still-logo_print.jpg (1024x576) [111.4 KB] || Planet_Patrol_Still-logo.jpg (3840x2160) [1.1 MB] || Planet_Patrol_Still-logo_searchweb.png (320x180) [61.9 KB] || Planet_Patrol_Still-logo_thm.png (80x40) [9.8 KB] || 13636_Planet_Patrol_Best_1080.mp4 (1920x1080) [100.9 MB] || 13636_Planet_Patrol_1080.mp4 (1920x1080) [39.6 MB] || 13636_Planet_Patrol_Best_1080.webm (1920x1080) [7.9 MB] || 13636_Planet_Patrol_ProRes_3840x2160_2997.mov (3840x2160) [3.6 GB] || 13636_Planet_Patrol_4k.mp4 (3840x2160) [114.2 MB] || 13636_Planet_Patrol_SRT_Captions.en_US.srt [878 bytes] || 13636_Planet_Patrol_SRT_Captions.en_US.vtt [890 bytes] || ", "hits": 43 }, { "id": 13708, "url": "https://svs.gsfc.nasa.gov/13708/", "result_type": "Produced Video", "release_date": "2020-09-16T11:00:00-04:00", "title": "Potential Giant World Circles a Tiny Star", "description": "Watch to learn how a possible giant planet may have survived its tiny star’s chaotic history. Jupiter-size WD 1856 b is nearly seven times larger than the white dwarf it orbits every day and a half. Astronomers discovered it using data from NASA’s Transiting Exoplanet Survey Satellite and now-retired Spitzer Space Telescope.Credit: NASA/JPL-Caltech/NASA's Goddard Space Flight CenterMusic: \"Titanium\" from Killer Tracks.Complete transcript available. || wd_1856_still.jpg (1920x1080) [306.2 KB] || wd_1856_still_print.jpg (1024x576) [106.2 KB] || wd_1856_still_searchweb.png (320x180) [46.5 KB] || wd_1856_still_web.png (320x180) [46.5 KB] || wd_1856_still_thm.png (80x40) [4.2 KB] || WD_1856_HQ.mp4 (1920x1080) [279.8 MB] || WD_1856_LQ.mp4 (1920x1080) [146.4 MB] || WD_1856_prores.mov (1920x1080) [1.5 GB] || WD_1856_LQ.webm (1920x1080) [17.1 MB] || WD_1856_prores.en_US.srt [3.0 KB] || WD_1856_prores.en_US.vtt [2.9 KB] || ", "hits": 165 }, { "id": 13696, "url": "https://svs.gsfc.nasa.gov/13696/", "result_type": "Produced Video", "release_date": "2020-08-25T11:00:00-04:00", "title": "Young Active Galaxy with ‘TIE Fighter’ Shape", "description": "This illustration shows two views of the active galaxy TXS 0128+554, located around 500 million light-years away. Left: The galaxy’s central jets appear as they would if we viewed them both at the same angle. The black hole, embedded in a disk of dust and gas, launches a pair of particle jets traveling at nearly the speed of light. Scientists think gamma rays (magenta) detected by NASA’s Fermi Gamma-ray Space Telescope originate from the base of these jets. As the jets collide with material surrounding the galaxy, they form identical lobes seen at radio wavelengths (orange). The jets experienced two distinct bouts of activity, which created the gap between the lobes and the black hole. Right: The galaxy appears in its actual orientation, with its jets tipped out of our line of sight by about 50 degrees.Credit: NASA’s Goddard Space Flight Center || TXS0128_Side-by-Side_FInal.jpg (7680x2160) [1.8 MB] || TXS0128_Side-by-Side_FInal_Half.jpg (3840x1080) [601.5 KB] || TXS0128_Side-by-Side_FInal_print.jpg (1024x288) [45.4 KB] || TXS0128_Side-by-Side_FInal.jpg.dzi (7680x2160) [178 bytes] || TXS0128_Side-by-Side_FInal.jpg_files (1x1) [4.0 KB] || ", "hits": 90 }, { "id": 13280, "url": "https://svs.gsfc.nasa.gov/13280/", "result_type": "Produced Video", "release_date": "2020-08-19T00:00:00-04:00", "title": "Assembling XRISM's X-ray Mirrors", "description": "Team members Lawrence Lozipone of Stinger Ghaffarian Technologies, Inc. and Yang Soong, a researcher at the University of Maryland, College Park, work with flight mirrors for the X-ray Imaging and Spectroscopy Mission (XRISM). Nested aluminum mirror segments – 1,624 of them for each X-ray Mirror Assembly – focus the incoming X-rays for the satellite's science instruments. Credit: NASA's Goddard Space Flight Center || XRISM_Cleanroom_B-roll_1080Still.jpg (1920x1080) [727.5 KB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.mov (1920x1080) [7.0 GB] || XRISM_Cleanroom_B-roll_1080.mp4 (1920x1080) [991.6 MB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.webm (1920x1080) [52.0 MB] || ", "hits": 130 }, { "id": 13605, "url": "https://svs.gsfc.nasa.gov/13605/", "result_type": "Produced Video", "release_date": "2020-05-13T11:00:00-04:00", "title": "TESS Aids Breakthrough in Puzzling Stellar Flashes", "description": "Watch the pulsations of a Delta Scuti star! In this illustration, the star changes in brightness when internal sound waves at different frequencies cause parts of the star to expand and contract. In one pattern, the whole star expands and contracts, while in a second, opposite hemispheres swell and shrink out of sync. In reality, a single star exhibits many pulsation patterns that can tell astronomers about its age, composition and internal structure. The exact light variations astronomers observe also depend on how the star's spin axis angles toward us. Delta Scuti stars spin so rapidly they flatten into ovals, which jumbles these signals and makes them harder to decode. Now, thanks to NASA's Transiting Exoplanet Survey Satellite, astronomers are deciphering some of them.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || Exterior_still.jpg (1920x1080) [460.3 KB] || 13605_Delta_Scuti_Pulsation_ProRes_1920x1080_2997.mov (1920x1080) [523.3 MB] || 13605_Delta_Scuti_Pulsation.mp4 (1920x1080) [36.1 MB] || 13605_Delta_Scuti_Pulsation.webm (1920x1080) [3.6 MB] || ", "hits": 84 }, { "id": 13570, "url": "https://svs.gsfc.nasa.gov/13570/", "result_type": "Produced Video", "release_date": "2020-04-27T11:00:00-04:00", "title": "Swift Tracks Water from Interstellar Visitor Borisov", "description": "Watch how NASA’s Neil Gehrels Swift Observatory tracked water production by interstellar comet 2I/Borisov as it sped through the solar system. On average, Borisov produced enough water to fill a standard bathtub in 10 seconds. It shares many traits with solar system comets, which may mean that comets form similarly in different planetary systems.Credit: NASA’s Goddard Space Flight CenterMusic: \"Mesmeric Thoughts\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Swift_Comet_Still.jpg (1920x1080) [599.5 KB] || Swift_Comet_Still_searchweb.png (320x180) [94.6 KB] || Swift_Comet_Still_thm.png (80x40) [6.0 KB] || 13570_Swift_Interstellar_Comet.webm (1920x1080) [17.2 MB] || 13570_Swift_Interstellar_Comet_SRT_Captions.en_US.vtt [2.1 KB] || 13570_Swift_Interstellar_Comet_SRT_Captions.en_US.srt [2.1 KB] || 13570_Swift_Interstellar_Comet_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || 13570_Swift_Interstellar_Comet_Best_1080.mp4 (1920x1080) [375.4 MB] || 13570_Swift_Interstellar_Comet.mp4 (1920x1080) [159.3 MB] || ", "hits": 65 }, { "id": 13590, "url": "https://svs.gsfc.nasa.gov/13590/", "result_type": "Produced Video", "release_date": "2020-04-23T10:00:00-04:00", "title": "Build Your Own Fermi Satellite", "description": "With a printer, scissors, glue and wooden skewers, you can make your own replica of the Fermi spacecraft. Grab the files to make your own here: https://go.nasa/papermodels Credit: NASA's Goddard Space Flight CenterMusic Credit: \"Bahama Beats\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || PaperModelFermi_ProRes_1920x1080_2997.02354_print.jpg (1024x576) [169.3 KB] || PaperModelFermi_ProRes_1920x1080_2997.02354_searchweb.png (320x180) [109.7 KB] || PaperModelFermi_ProRes_1920x1080_2997.02354_thm.png (80x40) [6.6 KB] || PaperModelFermi_Best.mp4 (1920x1080) [256.9 MB] || PaperModelFermi_ProRes_1920x1080_2997.mov (1920x1080) [1.5 GB] || PaperModelFermi_Good.mp4 (1920x1080) [109.9 MB] || PaperModelFermi_Best.webm (1920x1080) [12.1 MB] || PaperModelFermi_SRT_Captions.en_US.srt [1.3 KB] || PaperModelFermi_SRT_Captions.en_US.vtt [1.4 KB] || ", "hits": 75 }, { "id": 13556, "url": "https://svs.gsfc.nasa.gov/13556/", "result_type": "Produced Video", "release_date": "2020-02-14T03:00:00-05:00", "title": "Astrophysics Valentines", "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ", "hits": 182 }, { "id": 13197, "url": "https://svs.gsfc.nasa.gov/13197/", "result_type": "Produced Video", "release_date": "2020-02-11T09:00:00-05:00", "title": "Gravitational Wave Simulations of Merging Black Holes: 1080 and 8k Resolutions", "description": "This visualization shows gravitational waves emitted by two black holes (black spheres) of nearly equal mass as they spiral together and merge. Yellow structures near the black holes illustrate the strong curvature of space-time in the region. Orange ripples represent distortions of space-time caused by the rapidly orbiting masses. These distortions spread out and weaken, ultimately becoming gravitational waves (purple). The merger timescale depends on the masses of the black holes. For a system containing black holes with about 30 times the sun’s mass, similar to the one detected by LIGO in 2015, the orbital period at the start of the movie is just 65 milliseconds, with the black holes moving at about 15 percent the speed of light. Space-time distortions radiate away orbital energy and cause the binary to contract quickly. As the two black holes near each other, they merge into a single black hole that settles into its \"ringdown\" phase, where the final gravitational waves are emitted. For the 2015 LIGO detection, these events played out in little more than a quarter of a second. This simulation was performed on the Pleiades supercomputer at NASA's Ames Research Center. Fixed view.Credit: NASA/Bernard J. Kelly (Goddard and Univ. of Maryland Baltimore County), Chris Henze (Ames) and Tim Sandstrom (CSC Government Solutions LLC)Watch this video on the NASAgovVideo YouTube channel. || Merger_Fixed_Still.png (1920x1080) [1.2 MB] || Merger_Fixed_Still_print.jpg (1024x576) [59.6 KB] || BH_merger_fixed_camera_close_H264_YouTube_720p.mp4 (1280x720) [65.5 MB] || BH_merger_fixed_camera_close_H264_YouTube_1080p.mp4 (1920x1080) [65.2 MB] || BH_merger_fixed_camera_close_H264_YouTube_720p.webm (1280x720) [3.9 MB] || BH_merger_fixed_camera_close_ProRes_1920x1080.mov (1920x1080) [1.1 GB] || ", "hits": 341 }, { "id": 13531, "url": "https://svs.gsfc.nasa.gov/13531/", "result_type": "Produced Video", "release_date": "2020-01-31T00:00:00-05:00", "title": "XRISM: Calorimeter Spectrometer Insert and Mirror Tests", "description": "XRISM team members pose with the XRISM Calorimeter Spectrometer Insert in a NASA Goddard clean room. From left to right, they are Bryan James, Mike Sampson, Tomomi Watanabe, Pete Barfknecht, Scott Porter, and Sinclair Douglas.Credit: Larry Gilbert/NASA || GSFC_20191101__2020-2568_07.jpg (3000x1995) [3.6 MB] || GSFC_20191101__2020-2568_07_searchweb.png (320x180) [111.9 KB] || GSFC_20191101__2020-2568_07_thm.png (80x40) [7.7 KB] || ", "hits": 92 }, { "id": 13530, "url": "https://svs.gsfc.nasa.gov/13530/", "result_type": "Produced Video", "release_date": "2020-01-30T00:00:00-05:00", "title": "Mirror Quadrants for XRISM", "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ", "hits": 117 }, { "id": 13526, "url": "https://svs.gsfc.nasa.gov/13526/", "result_type": "Infographic", "release_date": "2020-01-24T10:00:00-05:00", "title": "What Makes an Exoplanet Habitable?", "description": "Explore this infographic to learn more about the many different factors that make a planet potentially habitable. Complete text transcript available.Machine readable version available.Credit: NASA Goddard Space Flight Center || Infographic_24x70_inset.jpg (1920x1080) [201.2 KB] || Habitability_Infographic_CROP_print.jpg (1024x702) [120.2 KB] || Habitability_Infographic_CROP.png (6667x4573) [1.7 MB] || Habitability_Infographic_FULL_24x70_2024Update.png (6667x19500) [5.4 MB] || Habitability_Infographic_CROP_searchweb.png (320x180) [47.0 KB] || Habitability_Infographic_CROP_thm.png (80x40) [5.7 KB] || ", "hits": 417 }, { "id": 13496, "url": "https://svs.gsfc.nasa.gov/13496/", "result_type": "Produced Video", "release_date": "2020-01-06T19:15:00-05:00", "title": "TESS Mission’s First Earth-size World in Star’s Habitable-zone", "description": "Take a tour through TOI 700, a planetary system 100 light-years away in the constellation Dorado. One of the system’s residents is TOI 700 d, the first Earth-size habitable-zone planet discovered by NASA’s Transiting Exoplanet Survey Satellite. Credit: NASA’s Goddard Space Flight Center.Music: \"Family Tree\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TOI_700d.jpg (1920x1080) [397.4 KB] || TOI_700d_print.jpg (1024x576) [128.3 KB] || TOI_700d_searchweb.png (320x180) [65.8 KB] || TOI_700d_thm.png (80x40) [5.5 KB] || 13496_TOI700_Earth-size_1080.webm (1920x1080) [25.7 MB] || 13496_TOI700_Earth-size_1080.mp4 (1920x1080) [229.2 MB] || 13496_TOI700_Earth-size_1080_Best.mp4 (1920x1080) [394.2 MB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.srt [4.4 KB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.vtt [4.4 KB] || 13496_TOI700_Earth-size_ProRes_1920x1080.mov (1920x1080) [2.7 GB] || ", "hits": 364 }, { "id": 13510, "url": "https://svs.gsfc.nasa.gov/13510/", "result_type": "Produced Video", "release_date": "2020-01-06T19:15:00-05:00", "title": "TESS Satellite Discovered Its First World Orbiting Two Stars", "description": "NASA’s Transiting Exoplanet Survey Satellite found its first circumbinary planet, a world orbiting two stars 1,300 light-years away. Watch to learn more about this Saturn-size world called TOI 1338 b.Credit: NASA's Goddard Space Flight CenterMusic: \"Albatross\" from Universal Production Music.Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || TOI_1338b_video_still.jpg (1920x1080) [389.2 KB] || TOI_1338b_video_still_print.jpg (1024x576) [128.2 KB] || TOI_1338b_video_still_searchweb.png (320x180) [75.4 KB] || TOI_1338b_video_still_web.png (320x180) [75.4 KB] || TOI_1338b_video_still_thm.png (80x40) [7.0 KB] || TOI_1338b_video_HQ.mp4 (1920x1080) [200.1 MB] || TOI_1338b_video_LQ.mp4 (1920x1080) [107.2 MB] || TOI_1338b_video_prores.mov (1920x1080) [1.0 GB] || TOI_1338b_video_LQ.webm (1920x1080) [12.1 MB] || TOI_1338b_video.en_US.srt [2.0 KB] || TOI_1338b_video.en_US.vtt [2.0 KB] || ", "hits": 266 }, { "id": 13240, "url": "https://svs.gsfc.nasa.gov/13240/", "result_type": "Produced Video", "release_date": "2019-12-12T11:00:00-05:00", "title": "NASA’s NICER Sizes Up a Pulsar, Reveals First-ever Surface Map", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) has expanded our understanding of pulsars, the dense, spinning corpses of exploded stars. Pulsar J0030+0451 (J0030 for short), located 1,100 light-years away in the constellation Pisces, now has the most precise and reliable measurements of both a pulsar’s mass and size to date. The shapes and locations of its hot spots challenge textbook depictions of these incredible objects. Music: \"Uncertain Ahead\" and \"Flowing Cityscape\" (underscore). Both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Two_NS_Model_Still.jpg (1920x1080) [308.5 KB] || Two_NS_Model_Still_print.jpg (1024x576) [140.4 KB] || Two_NS_Model_Still_searchweb.png (320x180) [87.0 KB] || Two_NS_Model_Still_thm.png (80x40) [8.0 KB] || 13240_NICER_J0030_MassRadius_1080.webm (1920x1080) [33.5 MB] || 13240_NICER_J0030_MassRadius_1080.mp4 (1920x1080) [301.1 MB] || 13240_NICER_J0030_MassRadius_Best_1080.mp4 (1920x1080) [804.5 MB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.srt [5.9 KB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.vtt [5.9 KB] || 13240_NICER_J0030_MassRadius_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || ", "hits": 200 }, { "id": 13267, "url": "https://svs.gsfc.nasa.gov/13267/", "result_type": "Produced Video", "release_date": "2019-11-05T13:00:00-05:00", "title": "TESS Southern Hemisphere Sector Images", "description": "Sector 1.The Transiting Exoplanet Survey Satellite (TESS) observed this strip of stars and galaxies in the southern sky from July 25, 2018, to August 22, 2018. TESS captured this individual image during one 30-minute period on 2018-08-07 at 04:59:42 UTC. The Large and Small Magellanic Clouds appear on the right-hand side. || TESS_Sector_1.png (16774x4272) [75.1 MB] || TESS_Sector_1.jpeg (16774x4272) [27.6 MB] || TESS_Sector_1_halfsize.jpeg (8387x2136) [9.7 MB] || TESS_Sector_1_halfsize.png (8387x2136) [9.7 MB] || ", "hits": 101 }, { "id": 13321, "url": "https://svs.gsfc.nasa.gov/13321/", "result_type": "Produced Video", "release_date": "2019-09-26T12:00:00-04:00", "title": "Rare Black Hole Event Seen by Satellites and Ground-based Telescopes Live Shots", "description": "B-roll package that corresponds to the following:SUGGESTED QUESTIONSWhat is a black hole and what did NASA and its partners discover?How does a black hole destroy a star?How did NASA and other observatories work together to capture this moment?What new things did we learn from this catastrophic event?How far away is this black hole? Could our Sun be eaten by a black hole?Black holes are black right? How do scientists study something that can’t be seen?Where can we learn more?QUESTIONS FOR LONGER INTERVIEWS:How does a planet-hunting mission help us learn about black holes?How did the scientists involved first learn about the event?What is #BlackHoleWeek?QUICK LINKS TO VIDEO AND AUDIOClick for downloadable AUDIO SOUNDBITE with NASA Scientist Knicole Colon.Click for downloadable soundbites with NASA Scientist Knicole ColonClick for downloadable soundbites with NASA Scientist Brad CenkoClick for downloadable soundbites with Carnegie astronomer Tom Holoien. || b_roll_slate.png (1280x720) [336.8 KB] || Rare_Black_Hole_Event_Broll_720p.webm (1280x720) [37.1 MB] || Rare_Black_Hole_Event_Broll_720p.mp4 (1280x720) [677.9 MB] || ", "hits": 120 }, { "id": 13237, "url": "https://svs.gsfc.nasa.gov/13237/", "result_type": "Produced Video", "release_date": "2019-09-26T11:00:00-04:00", "title": "TESS Catches Its First Star-destroying Black Hole", "description": "When a star strays too close to a black hole, intense tides break it apart into a stream of gas. The tail of the stream escapes the system, while the rest of it swings back around, surrounding the black hole with a disk of debris. This video includes images of a tidal disruption event called ASASSN-19bt taken by NASA’s Transiting Exoplanet Survey Satellite (TESS) and Swift missions, as well as an animation showing how the event unfolded. Credit: NASA’s Goddard Space Flight CenterMusic: \"Games Show Sphere 03\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_TDE_Still_print.jpg (1024x576) [87.3 KB] || TESS_TDE_Still.jpg (3840x2160) [629.6 KB] || TESS_TDE_Still_searchweb.png (320x180) [68.3 KB] || TESS_TDE_Still_thm.png (80x40) [5.3 KB] || 13237_TESS_TDE_ProRes_1920x1080.mov (1920x1080) [1.6 GB] || 13237_TESS_TDE_1080_Best.mp4 (1920x1080) [380.2 MB] || 13237_TESS_TDE_1080.mp4 (1920x1080) [125.6 MB] || 13237_TESS_TDE_1080_Best.webm (1920x1080) [12.6 MB] || 13237_TESS_TDE_SRT_Captions.en_US.srt [2.2 KB] || 13237_TESS_TDE_SRT_Captions.en_US.vtt [2.2 KB] || ", "hits": 152 }, { "id": 13324, "url": "https://svs.gsfc.nasa.gov/13324/", "result_type": "Produced Video", "release_date": "2019-09-25T09:00:00-04:00", "title": "Black Hole Safety: Desktop & Phone Wallpaper", "description": "So you’ve planned your trip to a black hole, you’ve packed your bags, and you’ve even watched the pre-flight safety video. If you haven’t yet watched the video, however, we highly recommend you click the image below. Don’t worry, we’ll wait.Now then, want to make black hole travel an even bigger part of your daily life? Wishing that black holes actually WERE portals to dimensions filled with unicorns and space potatoes? Download these phone and desktop wallpapers to fill your screens. || ", "hits": 125 }, { "id": 13322, "url": "https://svs.gsfc.nasa.gov/13322/", "result_type": "Animation", "release_date": "2019-09-23T10:00:00-04:00", "title": "NASA's Guide To Black Hole Safety", "description": "Have you ever thought about visiting a black hole? We sure hope not. However, if you're absolutely convinced that a black hole is your ideal vacation spot, watch this video before you blast off to learn more about them and (more importantly) how to stay safe.You can also download a handy safety brochure, watch short clips to learn different things about black holes, and even get some short glimpses into the lives of black holes and the explorers that want to visit them. || ", "hits": 542 }, { "id": 13323, "url": "https://svs.gsfc.nasa.gov/13323/", "result_type": "Produced Video", "release_date": "2019-09-23T10:00:00-04:00", "title": "Black Hole Travel Postcards", "description": "Wish you were here! Now, you can send your friends postcards from one of the most extreme vacation spots in the universe—or at least convince them you've gone even though you stayed safe at home. || ", "hits": 124 }, { "id": 13260, "url": "https://svs.gsfc.nasa.gov/13260/", "result_type": "Produced Video", "release_date": "2019-07-22T00:00:00-04:00", "title": "How the Sun Warps Starlight", "description": "This illustration shows how the Sun's gravity bends the path of light from a distant star, changing its apparent location in the sky. The effect is highly exaggerated here. From Earth, the apparent deflection would appear to be no more than the width of a dime seen at 1.25 miles away. || Sun_Gravitational_Lensing_Still.jpg (1920x1080) [259.6 KB] || Sun_Gravitational_Lensing_Still_print.jpg (1024x576) [79.3 KB] || Sun_Gravitational_Lensing_Still_searchweb.png (320x180) [63.1 KB] || Sun_Gravitational_Lensing_Still_thm.png (80x40) [4.7 KB] || Sun_Gravitational_Lensing_FINAL_ProRes_1920x1080.mov (1920x1080) [243.6 MB] || Sun_Gravitational_Lensing_FINAL_Best.mp4 (1920x1080) [26.8 MB] || Sun_Gravitational_Lensing_FINAL_Good.mp4 (1920x1080) [16.1 MB] || Sun_Gravitational_Lensing_FINAL_Small.mp4 (1280x720) [5.9 MB] || Sun_Gravitational_Lensing_FINAL_Small.webm (1280x720) [1.6 MB] || ", "hits": 612 }, { "id": 13223, "url": "https://svs.gsfc.nasa.gov/13223/", "result_type": "Produced Video", "release_date": "2019-06-27T09:00:00-04:00", "title": "TESS Discovers Its Tiniest World To Date", "description": "NASA’s Transiting Exoplanet Survey Satellite has confirmed the tiniest planet in its catalog so far — one of three discovered around a bright, nearby star called L 98-59. As shown in the illustrations in this video, all could occupy the “Venus zone,” the range of distances from the star where a Venus-like atmosphere is possible. The outermost planet also has the potential for a Neptune-like atmosphere. Credit: NASA’s Goddard Space Flight CenterMusic: \"Autumn Rush\" from Killer TracksComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || tess_smallest_planet_preview.jpg (1920x1080) [288.5 KB] || tess_smallest_planet_preview_print.jpg (1024x576) [118.1 KB] || tess_smallest_planet_preview_searchweb.png (320x180) [53.2 KB] || tess_smallest_planet_preview_web.png (320x180) [53.2 KB] || tess_smallest_planet_preview_thm.png (80x40) [5.5 KB] || tess_smallest_planet_HQ.mp4 (1920x1080) [245.9 MB] || tess_smallest_planet_LQ.mp4 (1920x1080) [190.0 MB] || tess_smallest_planet_prores.mov (1920x1080) [1.3 GB] || tess_smallest_planet_HQ.webm (1920x1080) [14.8 MB] || tess_smallest_planet.en_US.srt [1.9 KB] || tess_smallest_planet.en_US.vtt [1.9 KB] || ", "hits": 172 }, { "id": 13199, "url": "https://svs.gsfc.nasa.gov/13199/", "result_type": "Produced Video", "release_date": "2019-06-24T13:00:00-04:00", "title": "XMM-Newton Anniversary Products", "description": "Scientists reflect on XMM-Newton’s 20th anniversary. The mission, led by ESA (European Space Agency), has dramatically improved our understanding of the cosmos thanks to detailed X-ray observations. NASA funded two of its three instruments, including the Optical/UV Monitor Telescope, which made XMM-Newton one of the first multiwavelength observatories in space.Music: \"Passionate Research\" and \"Wondrous Planet\" both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XMM_Still1.jpg (1280x720) [553.6 KB] || XMM_Still1_print.jpg (1024x576) [451.3 KB] || XMM_20th_Anniversary_ProRes_1280x720_2997.mov (1280x720) [3.1 GB] || XMM_20th_Anniversary_Best_720.mp4 (1280x720) [891.1 MB] || XMM_20th_Anniversary_Good_720.mp4 (1280x720) [251.9 MB] || XMM_20th_Anniversary_Best_720.webm (1280x720) [52.7 MB] || XMM_20th_Anniversary_SRT_Captions.en_US.srt [9.6 KB] || XMM_20th_Anniversary_SRT_Captions.en_US.vtt [9.6 KB] || ", "hits": 70 }, { "id": 13220, "url": "https://svs.gsfc.nasa.gov/13220/", "result_type": "Produced Video", "release_date": "2019-06-13T11:00:00-04:00", "title": "Ten Years of High-Energy Gamma-ray Bursts", "description": "Green dots show the locations of 186 gamma-ray bursts observed by the Large Area Telescope (LAT) on NASA’s Fermi satellite during its first decade. Some noteworthy bursts are highlighted and labeled. Background: Constructed from nine years of LAT data, this map shows how the gamma-ray sky appears at energies above 10 billion electron volts. The plane of our Milky Way galaxy runs along the middle of the plot. Brighter colors indicate brighter gamma-ray sources.Credit: NASA/DOE/Fermi LAT Collaboration || Fermi_LAT_GRBs.jpg (5991x2994) [2.1 MB] || ", "hits": 139 }, { "id": 13156, "url": "https://svs.gsfc.nasa.gov/13156/", "result_type": "Produced Video", "release_date": "2019-03-19T12:00:00-04:00", "title": "NASA’s Fermi Satellite Clocks a ‘Cannonball’ Pulsar", "description": "New radio observations combined with 10 years of data from NASA’s Fermi Gamma-ray Space Telescope have revealed a runaway pulsar that escaped the blast wave of the supernova that formed it. Credit: NASA’s Goddard Space Flight CenterMusic: \"Forensic Scientist\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available.See the bottom of the page for a version without on-screen text. || CTA1_Still.jpg (1920x1080) [291.7 KB] || CTA1_Still_print.jpg (1024x576) [137.4 KB] || CTA1_Still_searchweb.png (320x180) [86.6 KB] || CTA1_Still_thm.png (80x40) [7.2 KB] || 13156_CTB1_Cannonball_Pulsar_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 13156_CTB1_Cannonball_Pulsar_Best.mov (1920x1080) [727.8 MB] || 13156_CTB1_Cannonball_Pulsar_Good.mp4 (1920x1080) [400.9 MB] || 13156_CTB1_Cannonball_Pulsar.mp4 (1920x1080) [147.3 MB] || 13156_CTB1_Cannonball_Pulsar.m4v (1920x1080) [144.6 MB] || 13156_CTB1_Cannonball_Pulsar_ProRes_1920x1080_2997.webm (1920x1080) [15.7 MB] || 13156_CTB1_Cannonball_Pulsar_SRT_Captions.en_US.srt [1.9 KB] || 13156_CTB1_Cannonball_Pulsar_SRT_Captions.en_US.vtt [1.9 KB] || ", "hits": 93 }, { "id": 13147, "url": "https://svs.gsfc.nasa.gov/13147/", "result_type": "Produced Video", "release_date": "2019-02-19T00:00:00-05:00", "title": "Volunteer Discovers Record-Setting White Dwarf Star", "description": "In this illustration, an asteroid (bottom left) breaks apart under the powerful gravity of LSPM J0207+3331, the oldest, coldest white dwarf known to be surrounded by a ring of dusty debris. Scientists think the system’s infrared signal is best explained by two distinct rings composed of dust supplied by crumbling asteroids.Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || White_Dwarf_Disk_FINAL_1080.png (1920x1080) [11.5 MB] || White_Dwarf_Disk_FINAL_1080.jpg (1920x1080) [372.7 KB] || White_Dwarf_Disk_FINAL_1080_print.jpg (1024x576) [98.1 KB] || White_Dwarf_Disk_FINAL_4k.png (3840x2160) [48.9 MB] || White_Dwarf_Disk_FINAL_4k.jpg (3840x2160) [1.2 MB] || White_Dwarf_Disk_FINAL_1080_searchweb.png (320x180) [52.9 KB] || White_Dwarf_Disk_FINAL_1080_thm.png (80x40) [4.3 KB] || ", "hits": 190 }, { "id": 12854, "url": "https://svs.gsfc.nasa.gov/12854/", "result_type": "Produced Video", "release_date": "2019-01-30T12:30:00-05:00", "title": "NICER Charts the Area Around a New Black Hole", "description": "Watch how X-ray echoes, mapped by NASA’s Neutron star Interior Composition Explorer (NICER) revealed changes to the corona of black hole MAXI J1820+070.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" from Killer TracksComplete transcript available. || Black_Hole_Corona_Still.jpg (1920x1080) [317.0 KB] || Black_Hole_Corona_Still_print.jpg (1024x576) [109.5 KB] || Black_Hole_Corona_Still_searchweb.png (320x180) [87.9 KB] || Black_Hole_Corona_Still_thm.png (80x40) [6.6 KB] || 12854_Black_Hole_Corona_ProRes_1920x1080.mov (1920x1080) [3.3 GB] || 12854_Black_Hole_Corona_1080p.mov (1920x1080) [515.0 MB] || 12854_Black_Hole_Corona.mp4 (1920x1080) [335.5 MB] || 12854_Black_Hole_Corona_small.mp4 (1920x1080) [135.2 MB] || 12854_Black_Hole_Corona_ProRes_1920x1080.webm (1920x1080) [26.7 MB] || 12854_Black_Hole_Corona_SRT_Captions.en_US.srt [4.5 KB] || 12854_Black_Hole_Corona_SRT_Captions.en_US.vtt [4.5 KB] || ", "hits": 110 }, { "id": 12855, "url": "https://svs.gsfc.nasa.gov/12855/", "result_type": "Produced Video", "release_date": "2019-01-10T13:00:00-05:00", "title": "Mysterious ‘Cow’ Blast Studied with NASA Telescopes", "description": "Watch what scientists think happens when a black hole tears apart a hot, dense white dwarf star. A team working with observations from NASA’s Neil Gehrels Swift Observatory suggest this process explains a mysterious outburst known as AT2018cow. Credit: NASA's Goddard Space Flight CenterMusic: \"Curious Events\" from Killer TracksWatch this video on the JPL YouTube channel.Complete transcript available. || AT2018COW_Labeled_Still_3_print.jpg (1024x576) [66.0 KB] || AT2018COW_Labeled_Still_3.jpg (3840x2160) [494.0 KB] || AT2018COW_Labeled_Still_3_searchweb.png (320x180) [56.8 KB] || AT2018COW_Labeled_Still_3_thm.png (80x40) [5.5 KB] || AT2018COW_Labeled_Music_Intro_3_1080.mp4 (1920x1080) [116.5 MB] || AT2018COW_Labeled_Music_Intro_3_1080p.mov (1920x1080) [161.2 MB] || AT2018COW_Labeled_Music_Intro_3_1080.webm (1920x1080) [13.2 MB] || AT2018COW_Labeled_Music_Intro_3_ProRes_3840x2160.mov (3840x2160) [4.7 GB] || AT2018COW_Labeled_Music_Intro_3_4k.mp4 (3840x2160) [436.5 MB] || AT2018COW_Labeled_Music_Intro_3_4K.mov (3840x2160) [241.6 MB] || AT2018COW_SRT_Captions.en_US.srt [1.2 KB] || AT2018COW_SRT_Captions.en_US.vtt [1.3 KB] || ", "hits": 122 }, { "id": 13104, "url": "https://svs.gsfc.nasa.gov/13104/", "result_type": "Produced Video", "release_date": "2018-11-29T14:00:00-05:00", "title": "Tracing the History of Starlight with NASA's Fermi Mission", "description": "Gamma rays from distant galaxies called blazars interact with starlight as they travel across the universe. As shown in this video, those reaching the Fermi Gamma-ray Space Telescope can help scientists learn about the history of star formation throughout the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic: \"Inducing Waves\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || blazarEBL_Fog2-still.jpg (1920x1080) [165.1 KB] || blazarEBL_Fog2-still_print.jpg (1024x576) [53.5 KB] || blazarEBL_Fog2-still_searchweb.png (320x180) [50.2 KB] || blazarEBL_Fog2-still_thm.png (80x40) [4.5 KB] || 13104_Starlight_History_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || 13104_Starlight_History_1080p.mov (1920x1080) [205.4 MB] || 13104_Starlight_History_1080.mp4 (1920x1080) [138.8 MB] || 13104_Starlight_History_1080.m4v (1920x1080) [135.4 MB] || 13104_Starlight_History_1080.webm (1920x1080) [14.4 MB] || 13104_Starlight_History_SRT_Captions.en_US.srt [2.3 KB] || 13104_Starlight_History_SRT_Captions.en_US.vtt [2.2 KB] || ", "hits": 166 }, { "id": 13097, "url": "https://svs.gsfc.nasa.gov/13097/", "result_type": "Produced Video", "release_date": "2018-10-17T12:30:00-04:00", "title": "Fermi Scientists Introduce Gamma-ray Constellations", "description": "Scientists with NASA’s Fermi Gamma-ray Space Telescope devised a set of constellations for the high-energy sky to highlight the mission’s 10th year of operations. Characters from modern myths, like the Hulk and the time-warping TARDIS from “Doctor Who,” represent one source of inspiration. Others include scientific concepts and tools, like the Fermi Satellite, and famous landmarks in countries contributing to the development and operation of Fermi. The mission has mapped about 3,000 gamma-ray sources -- 10 times the number known before its launch and comparable to the number of bright stars in the traditional constellations. The background shows the gamma-ray sky as mapped by Fermi. The prominent reddish band is the plane of our own galaxy, the Milky Way; brighter colors indicate brighter gamma-ray sources. Credit: NASA || GR_Constellations-NorthFermi_FullSize_FInal.gif (1920x930) [4.4 MB] || ", "hits": 76 }, { "id": 13058, "url": "https://svs.gsfc.nasa.gov/13058/", "result_type": "Produced Video", "release_date": "2018-10-10T11:00:00-04:00", "title": "Simulations Create New Insights Into Pulsars", "description": "Explore a new “pulsar in a box” computer simulation that tracks the fate of electrons (blue) and their antimatter kin, positrons (red), as they interact with powerful magnetic and electric fields around a neutron star. Lighter colors indicate higher particle energies. Each particle seen in this visualization actually represents trillions of electrons or positrons. Better knowledge of the particle environment around neutron stars will help astronomers understand how they produce precisely timed radio and gamma-ray pulses.Credit: NASA’s Goddard Space Flight CenterMusic: \"Reaching for the Horizon\" and \"Leaving Earth\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Pulsar_Still_1_print.jpg (1024x576) [436.1 KB] || Pulsar_Still_1.jpg (3840x2160) [4.5 MB] || Pulsar_Still_1_searchweb.png (320x180) [134.5 KB] || Pulsar_Still_1_thm.png (80x40) [9.1 KB] || 13058_Pulsar_Particle_Simulation_1080.webm (1920x1080) [25.8 MB] || 13058_Pulsar_Particle_Simulation_1080.mp4 (1920x1080) [208.0 MB] || 13058_Pulsar_Particle_Simulation_H264_1080.mov (1920x1080) [313.3 MB] || 13058_Pulsar_Particle_Simulation_SRT_Captions.en_US.srt [3.7 KB] || 13058_Pulsar_Particle_Simulation_SRT_Captions.en_US.vtt [3.6 KB] || 13058_Pulsar_Particle_Simulation_2160.mp4 (3840x2160) [523.3 MB] || 13058_Pulsar_Particle_Simulation_ProRes_3840x2160_2997.mov (3840x2160) [10.6 GB] || ", "hits": 188 }, { "id": 13043, "url": "https://svs.gsfc.nasa.gov/13043/", "result_type": "Produced Video", "release_date": "2018-10-02T10:50:00-04:00", "title": "New Simulation Sheds Light on Spiraling Supermassive Black Holes", "description": "Gas glows brightly in this computer simulation of supermassive black holes only 40 orbits from merging. Models like this may eventually help scientists pinpoint real examples of these powerful binary systems. Credit: NASA's Goddard Space Flight Center/Scott Noble; simulation data, d'Ascoli et al. 2018Music: \"Games Show Sphere 01\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SMBH_Sim_Still_1.jpg (1920x1080) [333.8 KB] || SMBH_Sim_Still_1_print.jpg (1024x576) [138.8 KB] || SMBH_Sim_Still_1_searchweb.png (320x180) [69.3 KB] || SMBH_Sim_Still_1_thm.png (80x40) [6.4 KB] || 13043_SMBH_Simulation_1080.webm (1920x1080) [17.4 MB] || 13043_SMBH_Simulation_1080.mp4 (1920x1080) [202.8 MB] || SMBH_SRT_Captions.en_US.srt [2.0 KB] || SMBH_SRT_Captions.en_US.vtt [1.9 KB] || 13043_SMBH_Simulation_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || ", "hits": 301 }, { "id": 13086, "url": "https://svs.gsfc.nasa.gov/13086/", "result_type": "Produced Video", "release_date": "2018-10-02T10:50:00-04:00", "title": "Supermassive Black Hole Binary Simulation Visualizations in 4k", "description": "Simulation of the light emitted by a supermassive black hole binary system where the surrounding gas is optically thin (transparent). Viewed from 0 degrees inclination, or directly above the plane of the disk. The emitted light represents all wavelengths.Credit: NASA's Goddard Space Flight Center/Scott Noble; simulation data, d'Ascoli et al. 2018 || image-000-_000150_print.jpg (1024x576) [33.9 KB] || image-000-_000150.png (3840x2160) [5.1 MB] || 0Degrees (3840x2160) [0 Item(s)] || SMBH_Sim_Thin0_4kFull.mp4 (3840x2160) [15.0 MB] || SMBH_Sim_Thin0_4kFull.webm (3840x2160) [2.2 MB] || SMBH_Sim_Thin0_4kFull.mov (3840x2160) [427.6 MB] || ", "hits": 425 }, { "id": 13069, "url": "https://svs.gsfc.nasa.gov/13069/", "result_type": "Produced Video", "release_date": "2018-09-17T13:00:00-04:00", "title": "NASA’s TESS Releases First Science Image", "description": "The Transiting Exoplanet Survey Satellite (TESS) took this snapshot of the Large Magellanic Cloud (right) and the bright star R Doradus (left) with just a single detector of one of its cameras on Tuesday, Aug. 7. The frame is part of a swath of the southern sky TESS captured in its “first light” science image as part of its initial round of data collection.Credit: NASA/MIT/TESS || TESSFLleadimagefeature.jpg (987x1019) [839.4 KB] || ", "hits": 135 } ] }