{ "count": 69, "next": null, "previous": null, "results": [ { "id": 31376, "url": "https://svs.gsfc.nasa.gov/31376/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "SPHEREx All Sky Map 2025", "description": "Two passes of an all-sky mosaic image from NASAs SPHEREx space telescope, the first showing dust and gas and the second showing stars and galaxies.", "hits": 470 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 712 }, { "id": 14947, "url": "https://svs.gsfc.nasa.gov/14947/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Webb Spectrum and Image Animations", "description": "These are animated versions of James Webb Space Telescope imagery and spectra. The spectra visualizations were created by the Space Telescope Science Institute and then animated at NASA's Goddard Space Flight Center. || ", "hits": 459 }, { "id": 14933, "url": "https://svs.gsfc.nasa.gov/14933/", "result_type": "Produced Video", "release_date": "2025-12-04T09:00:00-05:00", "title": "XRISM Finds Elemental Bounty in Supernova Remnant", "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ", "hits": 342 }, { "id": 60001, "url": "https://svs.gsfc.nasa.gov/60001/", "result_type": "Produced Video", "release_date": "2025-09-11T15:00:00-04:00", "title": "NASA Mapping Critical Minerals", "description": "The Geological Earth Mapping Experiment (GEMx) is a joint effort between NASA and the U.S. Geological Survey (USGS) to advance our knowledge of critical mineral resources in the Western United States. In September 2023, NASA aircraft began supporting an effort to find and map critical mineral deposits in Western regions of the U.S. Identifying these minerals could help improve environmental processes for mining and geological activities, enhance national security, and boost the economy.", "hits": 247 }, { "id": 14868, "url": "https://svs.gsfc.nasa.gov/14868/", "result_type": "Produced Video", "release_date": "2025-07-23T00:00:00-04:00", "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail", "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ", "hits": 103 }, { "id": 14867, "url": "https://svs.gsfc.nasa.gov/14867/", "result_type": "Produced Video", "release_date": "2025-07-15T14:00:00-04:00", "title": "GEMx Animations", "description": "Conceptual animation illustrating the ER-2 aircraft collecting spectroscopic mineral data over the American West. || GEMxThumbnail.png (1948x1052) [1.5 MB] || GEMxThumbnail_print.jpg (1024x553) [118.0 KB] || GEMxThumbnail_searchweb.png (320x180) [55.7 KB] || GEMxThumbnail_thm.png (80x40) [8.2 KB] || GEMx_Interface_1080p.mov (1920x1080) [37.6 MB] || GEMx_Interface_4k.mp4 (3840x2160) [36.0 MB] || GEMx_Interface_ProRes.mov (3840x2160) [4.1 GB] || ", "hits": 66 }, { "id": 14861, "url": "https://svs.gsfc.nasa.gov/14861/", "result_type": "Produced Video", "release_date": "2025-07-07T10:00:00-04:00", "title": "NASA's Habitable Worlds Observatory Will Search For Life", "description": "No description available.", "hits": 509 }, { "id": 14851, "url": "https://svs.gsfc.nasa.gov/14851/", "result_type": "Produced Video", "release_date": "2025-06-04T14:00:00-04:00", "title": "GEMx Illustrations", "description": "Conceptual illustration depicting the ER-2 aircraft and the AVIRIS instrument searching for critical minerals as part of the GEMx campaign. || GEMx_Illustration_withTEXT_vFinal.png (3840x2160) [17.0 MB] || GEMx_Illustration_withTEXT_vFinal_print.jpg (1024x576) [287.6 KB] || GEMx_Illustration_withTEXT_vFinal_searchweb.png (320x180) [123.2 KB] || GEMx_Illustration_withTEXT_vFinal_thm.png (80x40) [8.2 KB] || ", "hits": 28 }, { "id": 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": 106 }, { "id": 14801, "url": "https://svs.gsfc.nasa.gov/14801/", "result_type": "Produced Video", "release_date": "2025-05-27T20:53:00-04:00", "title": "Astrophysics Explainer Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to explainer videos.", "hits": 62 }, { "id": 14838, "url": "https://svs.gsfc.nasa.gov/14838/", "result_type": "Produced Video", "release_date": "2025-05-14T00:00:00-04:00", "title": "NASA FireSense (Fort Stewart-Hunter Army Airfield, Georgia)", "description": "On April 14th-20th, 2025, NASA’s FireSense project led a multi-agency prescribed burn research operation at Fort Stewart-Hunter Army Field, Georgia, in partnership with the U.S. Department of War (DoW). The DoW led the prescribed burn activities, while NASA FireSense coordinated field and airborne sampling with academic and agency partners, including the DoW Strategic Environmental Research and Development Program (SERDP) and DoW Environmental Security Technology Certification Program (ESTCP). The campaign targeted vegetation, fire, and smoke measurements, and aims to enhance understanding of fire behavior and smoke dynamics in order to provide actionable information to practitioners.NASA FireSense Website || ", "hits": 91 }, { "id": 14820, "url": "https://svs.gsfc.nasa.gov/14820/", "result_type": "Infographic", "release_date": "2025-04-24T12:00:00-04:00", "title": "Roman's Core Surveys Infographics", "description": "NASA’s Nancy Grace Roman Space Telescope’s three main observing programs, highlighted in this infographic, will enable astronomers to view the universe as never before, revealing billions of cosmic objects strewn across enormous swaths of space-time.Credit: NASA’s Goddard Space Flight Center || Roman_CoreSurveys_Infographic_print.jpg (1024x640) [155.3 KB] || Roman_CoreSurveys_Infographic.png (8000x5000) [28.6 MB] || Roman_CoreSurveys_Infographic.jpg (8000x5000) [2.5 MB] || Roman_CoreSurveys_Infographic_Half.jpg (4000x2500) [1.3 MB] || Roman_CoreSurveys_Infographic_searchweb.png (320x180) [72.9 KB] || Roman_CoreSurveys_Infographic_thm.png [6.6 KB] || ", "hits": 350 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 655 }, { "id": 14581, "url": "https://svs.gsfc.nasa.gov/14581/", "result_type": "Produced Video", "release_date": "2024-05-23T10:00:00-04:00", "title": "Gliese 12 b: An Intriguing World Sized Between Earth and Venus", "description": "Gliese 12 b’s estimated size may be as large as Earth or slightly smaller — comparable to Venus in our solar system. This artist’s concept compares Earth with different possible Gliese 12 b interpretations, from no atmosphere to a thick Venus-like one. Follow-up observations with NASA’s James Webb Space Telescope will help determine just how much atmosphere the planet retains as well as its composition.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Alt text: Illustration of Earth compared to various models of Gliese 12 b Image description: At left, against a black background, floats an artist's concept of a nearly half-illuminated Earth, with clouds, blue oceans, and land areas rendered in green, tan, brown, and white. At right are three similarly illuminated planets, slightly smaller than Earth and each representing a possible interpretation of Gliese 12 b. The version on the left has a surface of blotchy reddish and brownish features and no atmosphere. The middle version has the same surface texture partly obscured by a hazy atmosphere. And the rightmost and smallest version of the planet has a thick, Venus-like atmosphere that obscures the surface completely. || Gl12b_Earth_Comparison_ac.jpg (3840x2160) [935.8 KB] || Gl12b_Earth_Comparison_ac_print.jpg (1024x576) [126.0 KB] || Gl12b_Earth_Comparison.jpg (3840x2160) [929.5 KB] || Gl12b_Earth_Comparison_ac_searchweb.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_web.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_thm.png (80x40) [9.8 KB] || Gl12b_Earth_Comparison.tif (3840x2160) [6.4 MB] || ", "hits": 459 }, { "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": 146 }, { "id": 14463, "url": "https://svs.gsfc.nasa.gov/14463/", "result_type": "Produced Video", "release_date": "2024-04-30T11:00:00-04:00", "title": "XRISM Mission Captures Unmatched Data With Just 36 Pixels", "description": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XRISM_36_Pixels_Still.jpg (1920x1080) [959.9 KB] || XRISM_36_Pixels_Still_searchweb.png (320x180) [94.7 KB] || XRISM_36_Pixels_Still_thm.png (80x40) [7.0 KB] || 14463_XRISM_36Pixels_Good.mp4 (1920x1080) [148.9 MB] || 14463_XRISM_36Pixels_Best.mp4 (1920x1080) [514.8 MB] || 14463_XRISM_36Pixels_Captions.en_US.srt [4.6 KB] || 14463_XRISM_36Pixels_Captions.en_US.vtt [4.4 KB] || 14463_XRISM_36Pixels_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || ", "hits": 79 }, { "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": 161 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 335 }, { "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": 292 }, { "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": 379 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 1099 }, { "id": 14389, "url": "https://svs.gsfc.nasa.gov/14389/", "result_type": "Produced Video", "release_date": "2023-08-01T13:00:00-04:00", "title": "XRISM Additional Images", "description": "The XRISM spacecraft during acoustic testing at JAXA's Tsukuba Space Center in December 2022. These and other tests confirm that the spacecraft can withstand the severe vibrations and sounds of its rocket launch.Credit: JAXA || XRISM_Acoustic_12_23_22.jpg (2832x4240) [6.9 MB] || ", "hits": 62 }, { "id": 40456, "url": "https://svs.gsfc.nasa.gov/gallery/xrism/", "result_type": "Gallery", "release_date": "2023-02-03T00:00:00-05:00", "title": "XRISM", "description": "XRISM (X-ray Imaging and Spectroscopy Mission) is a JAXA/NASA collaborative mission with ESA participation. It launched from Japan in September of 2023 and is investigating the X-ray sky using high-resolution spectroscopy and imaging.", "hits": 300 }, { "id": 20374, "url": "https://svs.gsfc.nasa.gov/20374/", "result_type": "Animation", "release_date": "2022-12-12T00:00:00-05:00", "title": "XRISM Beauty Shots", "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ", "hits": 54 }, { "id": 14244, "url": "https://svs.gsfc.nasa.gov/14244/", "result_type": "Produced Video", "release_date": "2022-11-25T00:00:00-05:00", "title": "XRISM Resolve Animation", "description": "This animation illustrates how the microcalorimeter array at the heart of XRISM's revolutionary Resolve soft X-ray spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to 50 millikelvins, just above absolute zero, detects this minute temperature change.Credit: NASA's Goddard Space Flight Center || XRISM_Calorimeter-STILL_print.jpg (1024x576) [64.0 KB] || XRISM_Calorimeter-STILL.jpg (3840x2160) [716.3 KB] || XRISM_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL_thm.png (80x40) [5.5 KB] || XRISM_Calorimeter-STILL_web.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || 3840x2160_16x9_60p (3840x2160) [64.0 KB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || ", "hits": 151 }, { "id": 14136, "url": "https://svs.gsfc.nasa.gov/14136/", "result_type": "Produced Video", "release_date": "2022-04-20T00:00:00-04:00", "title": "Webb Instrument Overview", "description": "A look at the instruments on the Webb Telescope. || Webb_Instruments-Thumbnail-2.jpg (1920x1080) [1.3 MB] || Webb_Instruments-Thumbnail-2_print.jpg (1024x576) [676.3 KB] || Webb_Instruments-Thumbnail-2_searchweb.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_web.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_thm.png (80x40) [13.8 KB] || WEBB_Instrument_Package-closecap.en_US.srt [4.9 KB] || WEBB_Instrument_Package.webm (4096x2160) [68.8 MB] || WEBB_Instrument_Package.mp4 (4096x2160) [276.0 MB] || ", "hits": 19 }, { "id": 14074, "url": "https://svs.gsfc.nasa.gov/14074/", "result_type": "Produced Video", "release_date": "2022-03-22T10:00:00-04:00", "title": "The Roman Space Telescope's High Latitude Survey Pointing Scheme", "description": "The sequence and layout of the Roman Space Telescope's High Latitude Spectroscopic Survey tiling pattern.Credit: NASA's Goddard Space Flight Center || Roman_HLSS_Pointing_Scheme_Still_print.jpg (1024x576) [119.5 KB] || Roman_HLSS_Pointing_Scheme_Still.jpg (3840x2160) [1.1 MB] || Roman_HLSS_Pointing_Scheme_Still_searchweb.png (320x180) [53.3 KB] || Roman_HLSS_Pointing_Scheme_Still_thm.png (80x40) [5.1 KB] || Roman_HLSS_Pointing_Scheme_FINAL_4k.mp4 (3840x2160) [25.1 MB] || Roman_HLSS_Pointing_Scheme_FINAL_4k.webm (3840x2160) [9.1 MB] || Roman_HLSS_Pointing_Scheme_FINAL_ProRes_3840x2160_5994.mov (3840x2160) [1.7 GB] || ", "hits": 130 }, { "id": 14111, "url": "https://svs.gsfc.nasa.gov/14111/", "result_type": "Produced Video", "release_date": "2022-02-28T07:00:00-05:00", "title": "Webb's Mid-Infrared Instrument (MIRI) Light Path Animation", "description": "The spectrograph light path inside the Mid Infrared Instrument (MIRI) on the Webb Telescope. Versions with labels and without labels.Credit: European Space Agency || MIRI_SPECTRO_v2.00030_print.jpg (1024x576) [40.5 KB] || MIRI_SPECTRO_v2.00030_searchweb.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_web.png (320x180) [21.1 KB] || MIRI_SPECTRO_v2.00030_thm.png (80x40) [2.1 KB] || MIRI_SPECTRO_v2.mp4 (1920x1080) [156.3 MB] || MIRI_SPECTRO_labels_v3.mp4 (1920x1080) [177.9 MB] || MIRI_SPECTRO_v2.webm (1920x1080) [9.0 MB] || ", "hits": 67 }, { "id": 14112, "url": "https://svs.gsfc.nasa.gov/14112/", "result_type": "Produced Video", "release_date": "2022-02-28T07:00:00-05:00", "title": "Webb's Near Infrared Spectrograph (NIRSpec) Instrument Light Path Animation", "description": "Animation of the light path inside the Near Infrared Spectrometer (NIRSpec) on the Webb Telescope. Showing simulated data.Credit: European Space Agency || NIRSPEC_IFU_with_graph_v3.00030_print.jpg (1024x576) [39.9 KB] || NIRSPEC_IFU_with_graph_v3.00030_searchweb.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_web.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_thm.png (80x40) [2.1 KB] || NIRSPEC_IFU_with_graph_v3.mp4 (1920x1080) [311.7 MB] || NIRSPEC_IFU_with_graph_v3.webm (1920x1080) [12.7 MB] || ", "hits": 62 }, { "id": 14014, "url": "https://svs.gsfc.nasa.gov/14014/", "result_type": "Produced Video", "release_date": "2022-01-26T00:00:00-05:00", "title": "Elements of Webb: Elements Seeking Elements Ep12", "description": "Elements of Webb EP12: Seeking Elements || 12-Seeking_-_Dark.jpg (1920x1080) [795.3 KB] || 12-Seeking_-_Dark_print.jpg (1024x576) [315.1 KB] || 12-Seeking_-_Dark_searchweb.png (320x180) [73.2 KB] || 12-Seeking_-_Dark_web.png (320x180) [73.2 KB] || 12-Seeking_-_Dark_thm.png (80x40) [6.5 KB] || 12_-_Seeking_Elements_ProRes.mov (1920x1080) [4.9 GB] || 12_-_Seeking_Elements.mp4 (1920x1080) [391.3 MB] || 12_-_Seeking_Elements.webm (1920x1080) [41.3 MB] || 12_-_Seeking_Elements.en_US.srt [6.2 KB] || 12_-_Seeking_Elements.en_US.vtt [6.1 KB] || ", "hits": 24 }, { "id": 14076, "url": "https://svs.gsfc.nasa.gov/14076/", "result_type": "Produced Video", "release_date": "2022-01-19T10:55:00-05:00", "title": "HUBBLE FINDS A BLACK HOLE IGNITING STAR FORMATION IN A DWARF GALAXY", "description": "Black holes are often described as the monsters of the universe—tearing apart stars, consuming anything that comes too close, and holding light captive. Detailed evidence from NASA's Hubble Space Telescope, however, shows a black hole in a new light: fostering, rather than suppressing, star formation. Hubble imaging and spectroscopy of the dwarf starburst galaxy Henize 2-10 clearly show a gas outflow stretching from the black hole to a bright star birth region like an umbilical cord, triggering the already dense cloud into forming clusters of stars. Astronomers have previously debated that a dwarf galaxy could have a black hole analogous to the supermassive black holes in larger galaxies. Further study of dwarf galaxies, which have remained small over cosmic time, may shed light on the question of how the first seeds of supermassive black holes formed and evolved over the history of the universe. For more information, visit https://nasa.gov/hubble. Music Credits: “Champagne Age” by Damon Bradley [BMI] via Network Production Music Publishing [BMI] and Universal Production Music || ", "hits": 85 }, { "id": 14011, "url": "https://svs.gsfc.nasa.gov/14011/", "result_type": "Produced Video", "release_date": "2022-01-05T00:00:00-05:00", "title": "Elements of Webb: Helium Ep 09", "description": "Elements of Webb EP09: Helium || 9-Helium_-_Dark.jpg (1920x1080) [681.7 KB] || Helium_-_Dark.jpg (1920x1080) [681.7 KB] || 9-Helium_-_Dark_print.jpg (1024x576) [287.9 KB] || 9-Helium_-_Dark_searchweb.png (320x180) [75.4 KB] || 9-Helium_-_Dark_web.png (320x180) [75.4 KB] || 9-Helium_-_Dark_thm.png (80x40) [7.1 KB] || 9-Elements-Helium_ProRes.mov (1920x1080) [3.7 GB] || 9-Elements-Helium.mp4 (1920x1080) [288.4 MB] || 9-Elements-Helium.webm (1920x1080) [30.3 MB] || 9-Elements-Helium.en_US.srt [5.1 KB] || 9-Elements-Helium.en_US.vtt [5.1 KB] || ", "hits": 24 }, { "id": 14010, "url": "https://svs.gsfc.nasa.gov/14010/", "result_type": "Produced Video", "release_date": "2021-12-29T00:00:00-05:00", "title": "Elements of Webb: Silicon Ep08", "description": "Elements of Webb EP07: Silicon || Silicon__-_Dark.jpg (1920x1080) [577.3 KB] || 8-Silicon__-_Dark.jpg (1920x1080) [577.3 KB] || Silicon__-_Dark_print.jpg (1024x576) [279.3 KB] || Silicon__-_Dark_searchweb.png (320x180) [76.0 KB] || Silicon__-_Dark_web.png (320x180) [76.0 KB] || Silicon__-_Dark_thm.png (80x40) [7.0 KB] || 8-Elements-Silicon_ProRes.mov (1920x1080) [1.8 GB] || 8-Elements-Silicon.mp4 (1920x1080) [132.1 MB] || 8-Elements-Silicon.webm (1920x1080) [14.1 MB] || 8-Elements-Silicon.en_US.srt [2.3 KB] || 8-Elements-Silicon.en_US.vtt [2.3 KB] || ", "hits": 35 }, { "id": 14043, "url": "https://svs.gsfc.nasa.gov/14043/", "result_type": "Produced Video", "release_date": "2021-12-13T14:00:00-05:00", "title": "Tour 2022: NASA's Upcoming Earth Missions", "description": "NASA has a unique view of our planet from space. NASA’s fleet of Earth-observing satellites provide high quality data on different parts of Earth’s interconnected environment from air quality to sea ice. Take a tour of missions launching in 2022, including SWOT, TROPICS, EMIT, and JPSS-2. || ", "hits": 35 }, { "id": 14001, "url": "https://svs.gsfc.nasa.gov/14001/", "result_type": "Infographic", "release_date": "2021-11-09T10:00:00-05:00", "title": "Roman Space Telescope High Latitude Wide Area Survey", "description": "This illustration compares the relative sizes of the areas of sky covered by two surveys: Roman’s High Latitude Wide Area Survey, outlined in blue, and the largest mosaic led by Hubble, the Cosmological Evolution Survey (COSMOS), shown in red. In current plans, the Roman survey will be more than 1,000 times broader than Hubble’s. Roman will also explore more distant realms of space than most other telescopes have probed in previous efforts to study why the expansion of the universe is speeding up. Credit: NASA's Goddard Space Flight Center || Roman_HLS_FINAL_1080.png (2160x1080) [9.8 MB] || Roman_HLS_FINAL_1080.jpg (2160x1080) [800.5 KB] || Roman_HLS_FINAL_1080_print.jpg (1024x512) [224.7 KB] || Roman_HLS_Final_Full.jpg (8000x4000) [3.8 MB] || Roman_HLS_FINAL_Half.png (4000x2000) [31.6 MB] || Roman_HLS_FINAL_Half.jpg (4000x2000) [1.7 MB] || Roman_HLS_FINAL_Full.png (8000x4000) [114.3 MB] || Roman_HLS_FINAL_1080_searchweb.png (320x180) [90.3 KB] || Roman_HLS_FINAL_1080_thm.png (80x40) [6.9 KB] || ", "hits": 110 }, { "id": 13804, "url": "https://svs.gsfc.nasa.gov/13804/", "result_type": "Produced Video", "release_date": "2021-02-16T09:55:00-05:00", "title": "Hubble’s Servicing Mission 2", "description": "The Second Servicing Mission, launched February 11, 1997, greatly improved Hubble's productivity. The installation of new instruments extended Hubble's wavelength range into the near infrared for imaging and spectroscopy, allowing us to probe the most distant reaches of the universe. The replacement of failed or degraded spacecraft components increased efficiency and performance.A seven-member STS-82 crew took part in this mission. Four astronauts conducted the planned spacewalks: Mark Lee, Gregory Harbaugh, Steven Smith and Joseph Tanner were part of the extravehicular activity crew. Kenneth Bowersox was the commander, Scott Horowitz was the pilot, and Steven Hawley was the Remote Manipulator System Operator.For more information, visit https://nasa.gov/hubble. Music Credits: \"Cristal Delight\" by Fred Dubois [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Paradigm” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Temporal Kinetics” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music.“Drive to Succeed” by Stephen Daniel Lemaire [ASCAP] via El Murmullo Sarao [SGAE], Universal Sarao [SGAE] and Universal Production Music.Motion Graphics Template Media Credits:Lower Thirds Auto Self Resizing by cayman via Motion Array || ", "hits": 29 }, { "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": 63 }, { "id": 13606, "url": "https://svs.gsfc.nasa.gov/13606/", "result_type": "Produced Video", "release_date": "2020-05-20T11:00:00-04:00", "title": "A New Portrait of the Cosmos is Coming", "description": "Welcome to NASA's upcoming infrared survey mission, taking a wider view of the cosmos.Credit: NASA's Goddard Space Flight CenterMusic: \"The Decision (alternate)\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Trailer_still_1_print.jpg (1024x576) [181.5 KB] || Trailer_still_1.jpg (3840x2160) [2.0 MB] || Trailer_still_1_searchweb.png (180x320) [104.8 KB] || Trailer_still_1_thm.png (80x40) [7.9 KB] || Roman_Space_Telescope_Trailer_ProRes_1920x1080_2997.mov (1920x1080) [797.0 MB] || Roman_Space_Telescope_Trailer_Best_1080.mp4 (1920x1080) [281.5 MB] || Roman_Space_Telescope_Trailer_1080.mp4 (1920x1080) [132.9 MB] || Roman_Space_Telescope_Trailer_1080.webm (1920x1080) [7.2 MB] || Roman_Trailer_SRT_Captions.en_US.srt [740 bytes] || Roman_Trailer_SRT_Captions.en_US.vtt [753 bytes] || ", "hits": 66 }, { "id": 13597, "url": "https://svs.gsfc.nasa.gov/13597/", "result_type": "Produced Video", "release_date": "2020-04-27T12:00:00-04:00", "title": "Animation of the NIRSpec Instrument", "description": "Turntable animation of the James Webb Space Telescope NIRSpec instrument. || NIRSPEC_TT.00001_print.jpg (1024x576) [32.2 KB] || NIRSPEC_TT.00001_searchweb.png (180x320) [29.8 KB] || NIRSPEC_TT.00001_thm.png (80x40) [2.2 KB] || NIRSPEC_TT.mov (3840x2160) [396.3 MB] || NIRSPEC_TT.mp4 (3840x2160) [14.6 MB] || NIRSPEC_TT.webm (3840x2160) [1.9 MB] || ", "hits": 71 }, { "id": 13595, "url": "https://svs.gsfc.nasa.gov/13595/", "result_type": "Produced Video", "release_date": "2020-04-27T11:00:00-04:00", "title": "FGS/NIRISS Turntable Animation", "description": "A turntable animation of the James Webb Space Telescope FGS/NIRISS instruments || FGS_tt.00001_print.jpg (1024x576) [27.3 KB] || FGS_tt.00001_searchweb.png (180x320) [19.3 KB] || FGS_tt.00001_thm.png (80x40) [2.2 KB] || FGS_tt.mov (3840x2160) [270.6 MB] || FGS_tt.mp4 (3840x2160) [14.9 MB] || FGS_tt.webm (3840x2160) [1.7 MB] || ", "hits": 88 }, { "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": 66 }, { "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": 99 }, { "id": 13784, "url": "https://svs.gsfc.nasa.gov/13784/", "result_type": "Produced Video", "release_date": "2019-11-13T00:00:00-05:00", "title": "Seasonal Variations in Oxygen at Gale Crater", "description": "For the first time in the history of space exploration, scientists have measured the seasonal changes in the gases that fill the air directly above the surface of Gale Crater on Mars. As a result, they noticed something baffling: oxygen, the gas many Earth creatures use to breathe, behaves in a way that so far scientists cannot explain through any known chemical processes. || ", "hits": 248 }, { "id": 12916, "url": "https://svs.gsfc.nasa.gov/12916/", "result_type": "Produced Video", "release_date": "2018-12-11T14:00:00-05:00", "title": "50th Anniversary of NASA's OAO 2 Mission", "description": "“Seas of Infinity” (1968), full-length version scanned from 16mm color film and color corrected; run time 14:25. Original description: The film opens with an explanation of the electromagnetic spectrum. The limited capabilities of skyhook balloons and sounding rockets are used to illustrate the need for orbiting observatories. Reviews the planning, development, launching and function of the Orbiting Astronomical Observatory, a series of orbiting telescopes which are being used to study our solar system and the stars beyond. Features comments by the following leading scientists on the potential of this advancement in astronomy: Dr. Arthur Code, Wisconsin telescopes; Dr. James Kupperian, Goddard Flight Center using Cassegrain designs; Dr. Fred Whipple on the ultraviolet light sky mapping project; and Dr. Donald Morton on the Princeton OAO ultraviolet spectroscopy project. The film has scenes of the assembly of the OAO. The OAO will be launched by an Atlas-Centaur. Credit: NASAComplete transcript available. || Seas_Of_Infinity_OAO2_Color_Corrected.22261_print.jpg (1024x768) [40.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_searchweb.png (320x180) [42.3 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_thm.png (80x40) [4.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.mp4 (640x480) [136.1 MB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.srt [16.6 KB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.vtt [16.6 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.webm (640x480) [110.9 MB] || ", "hits": 82 }, { "id": 12966, "url": "https://svs.gsfc.nasa.gov/12966/", "result_type": "Produced Video", "release_date": "2018-06-06T00:00:00-04:00", "title": "Measuring the Atmosphere on ATom's Final Flight Around the World", "description": "NASA's Atmospheric Tomography (ATom) mission team just finished their final trip around the world, taking atmospheric samples from all over our home planet. Flying in NASA's DC-8 plane, the scientists and engineers collected their samples during four different trips, one for each season, to see how the atmosphere changed across fall, winter, spring and summer. || ", "hits": 25 }, { "id": 12850, "url": "https://svs.gsfc.nasa.gov/12850/", "result_type": "Produced Video", "release_date": "2018-03-28T13:00:00-04:00", "title": "NASA's New Planet Hunter: TESS", "description": "Watch an overview of the TESS mission.Music: \"Drive to Succeed\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Still_B1_00812_print.jpg (1024x576) [56.9 KB] || TESS_Still_B1_00812.png (3840x2160) [5.6 MB] || TESS_Still_B1_00812_searchweb.png (320x180) [53.1 KB] || TESS_Still_B1_00812_thm.png (80x40) [4.8 KB] || 12850_TESS_Overview_1080.webm (1920x1080) [34.9 MB] || 12850_TESS_Overview_1080.m4v (1920x1080) [321.6 MB] || TESS_Overview_SRT_Captions.en_US.srt [5.8 KB] || TESS_Overview_SRT_Captions.en_US.vtt [5.8 KB] || 12850_TESS_Overview_4K_Good_H264.mov (3840x2160) [931.4 MB] || 12850_TESS_Overview_4K_Best_H264.m4v (3840x2160) [1.5 GB] || 12850_TESS_Overview.mp4 (3840x2160) [1.6 GB] || 12850_TESS_Overview_YOUTUBE.mov (3840x2160) [3.2 GB] || 12850_TESS_Overview_Prores_3840x2160_2997.mov (3840x2160) [17.2 GB] || ", "hits": 245 }, { "id": 12804, "url": "https://svs.gsfc.nasa.gov/12804/", "result_type": "Produced Video", "release_date": "2018-03-15T07:00:00-04:00", "title": "SEEC AAS Hyperwall Presentation January 2018", "description": "This animation illustrates the Kepler-186 system, whose fifth world is the first Earth-sized exoplanet to be found orbiting within its star’s habitable zone. The animation closes with a simulated image from a coronagraph showing how such a planet might appear when directly imaged.Credit: NASA/Ames/SETI Institute/JPL-Caltech || Kepler186_Coronagraph_Combined_LongPause.01270_print.jpg (1024x576) [35.2 KB] || Kepler186_Coronagraph_Combined_LongPause.webm (1920x1080) [14.0 MB] || Kepler186_Coronagraph_Combined_LongPause.mov (1920x1080) [180.7 MB] || ", "hits": 35 }, { "id": 12844, "url": "https://svs.gsfc.nasa.gov/12844/", "result_type": "Produced Video", "release_date": "2018-02-05T11:00:00-05:00", "title": "Hubble Observes Atmospheres of TRAPPIST-1 Exoplanets in the Habitable Zone", "description": "Astronomers using the Hubble Space Telescope have conducted the first spectroscopic survey of Earth-sized planets in the TRAPPIST-1 system's habitable zone. Hubble reveals that at least the inner five planets do not seem to contain puffy, hydrogen-rich atmospheres similar to gaseous planets such as Neptune. This means the atmospheres may be more shallow and rich in heavier gases like carbon dioxide, methane, and oxygen.Find the full story and press release at hubblesite.org.Read the joint Hubble and Spitzer findings on nasa.gov.The science paper is available from Nature Astronomy. || ", "hits": 171 }, { "id": 12805, "url": "https://svs.gsfc.nasa.gov/12805/", "result_type": "Produced Video", "release_date": "2018-01-07T00:00:00-05:00", "title": "TESS AAS Hyperwall Presentation January 2018", "description": "Venus transits the Sun on June 5, 2012 as observed by the Solar Dynamics Observatory in 171 Angstrom light.Credit: NASA/SDO || Venus_Transit_SDO_1080.00049_print.jpg (1024x576) [158.1 KB] || Venus_Transit_SDO_1080.mov (1920x1080) [62.9 MB] || Venus_Transit_SDO_1080.webm (1920x1080) [1.0 MB] || ", "hits": 34 }, { "id": 12709, "url": "https://svs.gsfc.nasa.gov/12709/", "result_type": "Produced Video", "release_date": "2017-09-12T10:00:00-04:00", "title": "Cassini's Infrared Saturn", "description": "Since arriving at Saturn in 2004, Cassini has used its Composite Infrared Spectrometer (CIRS) to study the ringed planet and its moons in heat radiation. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Particle Waves,\" \"Odyssey,\" \"Solaris,\" \"Expansive,\"\"Horizon Ahead,\" \"Ion Bridge,\" \"Outer Space\" || CassiniCIRSpreviewShort.jpg (1920x1080) [591.6 KB] || CassiniCIRSpreviewShort_searchweb.png (320x180) [125.9 KB] || CassiniCIRSpreviewShort_thm.png (80x40) [8.4 KB] || 12709_Cassini_CIRS_Short_TWTR.mp4 (1280x720) [102.0 MB] || WEBM-12709_Cassini_CIRS_Short_APR.webm (960x540) [191.9 MB] || 12709_Cassini_CIRS_Short_FB.mp4 (1280x720) [574.1 MB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.srt [10.3 KB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.vtt [10.3 KB] || 12709_Cassini_CIRS_Short_YT.mp4 (1920x1080) [1.2 GB] || 12709_Cassini_CIRS_Short_APR.mov (1920x1080) [6.0 GB] || 12709_Cassini_CIRS_Short_YT.hwshow [96 bytes] || ", "hits": 55 }, { "id": 20267, "url": "https://svs.gsfc.nasa.gov/20267/", "result_type": "Animation", "release_date": "2017-04-26T00:00:00-04:00", "title": "Neutron Star Animations", "description": "The Neutron star Interior Composition Explorer (NICER) mission will study neutron stars, the densest known objects in the cosmos. These neutron star animations and graphics highlight some of their unique characteristics.For more information about NICER visit: nasa.gov/nicer. || ", "hits": 557 }, { "id": 12319, "url": "https://svs.gsfc.nasa.gov/12319/", "result_type": "Produced Video", "release_date": "2016-07-20T12:55:00-04:00", "title": "Hubble Makes First Measurements of Earth-Sized Exoplanet Atmospheres", "description": "Watch this video on the NASA.gov Video YouTube channel.Music credit: \"Feels Good\" by Louise Dowd and Stephen William Cornish, Atmosphere Music Ltd, Killer Tracks Production Music || Hubble_Trappist_thumbnail_print.jpg (1024x574) [103.5 KB] || Hubble_Trappist_thumbnail.png (2105x1182) [2.6 MB] || Hubble_Trappist_thumbnail_searchweb.png (320x180) [87.3 KB] || Hubble_Trappist_thumbnail_thm.png (80x40) [7.2 KB] || Hubble_TRAPPIST_final.mov (1920x1080) [2.2 GB] || Hubble_TRAPPIST_final.mp4 (1920x1080) [174.3 MB] || Hubble_TRAPPIST_final.webm (1920x1080) [19.4 MB] || Hubble_TRAPPIST_final.en_US.srt [3.4 KB] || Hubble_TRAPPIST_final.en_US.vtt [3.4 KB] || ", "hits": 86 }, { "id": 11992, "url": "https://svs.gsfc.nasa.gov/11992/", "result_type": "Produced Video", "release_date": "2015-09-02T11:00:00-04:00", "title": "Mapping Mars' Upper Atmosphere", "description": "Principal Investigator Bruce Jakosky talks about MAVEN’s science observations at Mars.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Bruce_Jakosky_G2015-007_thumbnail.png (1920x1080) [1.8 MB] || Bruce_Jakosky_G2015-007_thumbnail_print.jpg (1024x576) [100.6 KB] || Bruce_Jakosky_G2015-007_thumbnail_searchweb.png (320x180) [90.5 KB] || Bruce_Jakosky_G2015-007_thumbnail_thm.png (80x40) [7.2 KB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv.m4v (1280x720) [123.4 MB] || WEBM_G2015-007_MAVEN_Early_Sci_MASTER.webm (960x540) [101.9 MB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv_subtitles.m4v (1280x720) [123.5 MB] || NASA_TV_G2015-007_MAVEN_Early_Sci_MASTER.mpeg (1280x720) [846.9 MB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.srt [4.1 KB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.vtt [4.2 KB] || G2015-007_MAVEN_Early_Sci_MASTER_H264.mov (1920x1080) [1.7 GB] || NASA_PODCAST_G2015-007_MAVEN_Early_Sci_MASTER_ipod_sm.mp4 (320x240) [44.1 MB] || PRORES_B-ROLL_G2015-007_MAVEN_Early_Sci_MASTER_prores.mov (1280x720) [3.4 GB] || G2015-007_MAVEN_Early_Sci_MASTER.mov (1920x1080) [6.5 GB] || ", "hits": 59 }, { "id": 20223, "url": "https://svs.gsfc.nasa.gov/20223/", "result_type": "Animation", "release_date": "2015-09-02T11:00:00-04:00", "title": "MAVEN Stellar Occultation", "description": "NASA's Mars Atmosphere and Volatile Evolution mission (MAVEN) is the first spacecraft specifically designed to study the upper atmosphere of Mars. MAVEN's goal is to determine how Mars lost its thick early atmosphere, and with it, its once hospitable climate.While previous Mars orbiters have peered down at the planet's surface, MAVEN is spending part of its time gazing at the stars, observing the Martian atmosphere through a series of stellar occultations. As Mars rolls beneath MAVEN, due to the spacecraft's own orbital motion, background stars rise and set behind the planet. Their light dims as it passes through the tenuous atmosphere, with specific gases absorbing specific wavelengths. MAVEN uses its Imaging Ultraviolet Spectrograph to break apart this light and see which wavelengths are absorbed, allowing it to determine atmospheric composition at varying altitudes. || ", "hits": 78 }, { "id": 4318, "url": "https://svs.gsfc.nasa.gov/4318/", "result_type": "Visualization", "release_date": "2015-06-26T14:00:00-04:00", "title": "A Slice of Light: How IRIS Observes the Sun", "description": "Short version of the IRIS visualization with windowed SJI imagery. || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_print.jpg (1024x576) [122.9 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_searchweb.png (320x180) [95.6 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_thm.png (80x40) [7.6 KB] || SDO304IRISspectraWin4_1080p.mp4 (1920x1080) [22.3 MB] || Windowed.short (1920x1080) [128.0 KB] || SDO304IRISspectraWin4_1080p.webm (1920x1080) [4.3 MB] || ", "hits": 75 }, { "id": 11553, "url": "https://svs.gsfc.nasa.gov/11553/", "result_type": "Produced Video", "release_date": "2014-05-30T13:00:00-04:00", "title": "WFIRST: Uncovering the Mysteries of the Universe", "description": "The Wide-Field Infrared Survey Telescope (WFIRST) is an upcoming space telescope designed to perform wide-field imaging and spectroscopy of the infrared sky. One of WFIRST’s objectives will be looking for clues about dark energy—the mysterious force that is accelerating the expansion of the universe. Another objective of the mission will be finding and studying exoplanets. WFIRST uses the same 2.4 meter telescope size as Hubble, but with 18 cutting-edge fourth-generation image sensors compared to Hubble's single first-generation sensor. As a result, each WFIRST image will cover over 200 times as much as a Hubble Wide Field Camera 3/IR image and be 300 megapixels in size. Hubble images reveal thousands of galaxies; a single WFIRST image will uncover millions.To help uncover the mystery of dark energy, WFIRST will make incredibly precise measurements of the universe. These measurements, like the distance and position of galaxies, can be compared to other measurements—such as the cosmic microwave background from the WMAP mission—to determine how dark energy has changed over time. WFIRST can also measure the slight distortions in light from distant galaxies as it passes more nearby mass concentrations. These data will build a three dimensional picture of how mass is distributed throughout the universe, and provide independent confirmation of its structure.Because WFIRST has such a large and sensitive field of view, it can find thousands of new exoplanets through a process called microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the gravitational \"attraction\" of the foreground star. This \"lens\" star is then a virtual magnifying glass, amplifying the brightness of the background source star. If the lens star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. For closer planets, WFIRST will open a new era of direct observation. Currently only a handful of planets are observable in light reflected off of them, and they are all large planets close to their stars. WFIRST will be able to detect planets as small as Neptune, and as far from their stars as Saturn is from the sun. This is possible thanks to newly developed coronagraphs, which block the bright light from the star to make the planet more visible. || ", "hits": 159 }, { "id": 11402, "url": "https://svs.gsfc.nasa.gov/11402/", "result_type": "Produced Video", "release_date": "2014-04-09T14:00:00-04:00", "title": "Webb Telescope's NIRSpec Instrument Arrives at NASA Goddard Space Flight Center - Video Snap Shot", "description": "The Webb Telescope's Near-Infrared Spectrograph (NIRSpec) instrument arrives at NASA Goddard Space Flight Center on September 20, 2013. NIRSpec is a near infrared multi-object dispersive spectrograph capable of simultaneously observing more than 100 sources over a field-of-view (FOV) larger than 3' x 3'. The NIRSpec will be the first spectrograph in space that has this capability. Targets in the Field of View are normally selected by opening groups of shutters in a micro-shutter array (MSA) to form multiple apertures.NIRSpec will address all of the four main JWST science themes, and much more. It will enable large spectroscopic surveys of faint galaxies at high redshift, obtain sensitive spectra of transiting exoplanets and image line emission from protoplanetary disks and protostars. NIRSpec is being built for the European Space Agency (ESA) by the Airbus Group. || ", "hits": 22 }, { "id": 11520, "url": "https://svs.gsfc.nasa.gov/11520/", "result_type": "B-Roll", "release_date": "2014-04-08T12:00:00-04:00", "title": "NIRSpec Instrument Gets Integrated into Webb's ISIM - B-ROLL", "description": "Engineers install the Near Infrared Spectrometer (NIRSpec) onto the Webb Telescope's Integrated Science Instrument Module (ISIM) in NASA Goddard Space Flight Center cleanroom. This delicate procedure took place during March 24 and March 25, 2014 in preparation for the cryogenic test of a fully integrated ISIM structure to occur this summer. The Near-Infrared Spectrograph (NIRSpec) is a near infrared multi-object dispersive spectrograph capable of simultaneously observing more than 100 sources over a field-of-view (FOV) larger than 3' x 3'. The NIRSpec will be the first spectrograph in space that has this capability. Targets in the Field of View are normally selected by opening groups of shutters in a micro-shutter array (MSA) to form multiple apertures. The microshutters are arranged in a waffle-like grid that contains more than 62000 shutters with each cell measuring 100 µm x 200 µm. Sweeping a magnet across the surface of the MSA opens all operable shutters. Individual shutters may then be addressed and closed electronically. NIRSpec is also capable of Fixed-slit and Integral-field spectroscopy and provides medium-resolution spectroscopy over a wavelength range of 1 - 5 µm and lower-resolution spectroscopy from 0.6 - 5 µm.NIRSpec will address all of the four main JWST science themes, and much more. It will enable large spectroscopic surveys of faint galaxies at high redshift, obtain sensitive spectra of transiting exoplanets and image line emission from protoplanetary disks and protostars. NIRSpec is being built for the European Space Agency (ESA) by the Airbus Group with Dr. Pierre Ferruit guiding its development as the ESA JWST Project Scientist. Peter Jakobsen, the NIRSpec Instrument PI, retired in December 2011. || ", "hits": 16 }, { "id": 11510, "url": "https://svs.gsfc.nasa.gov/11510/", "result_type": "Produced Video", "release_date": "2014-04-08T11:00:00-04:00", "title": "NIRSpec Instrument Gets Integrated into Webb's ISIM", "description": "Engineers install the Near Infrared Spectrometer (NIRSpec) onto the Webb Telescope's Integrated Science Instrument Module (ISIM) in NASA Goddard Space Flight Center cleanroom. This delicate procedure took place during March 24 and March 25, 2014 in preparation for the cryogenic test of a fully integrated ISIM structure to occur this summer. The Near-Infrared Spectrograph (NIRSpec) is a near infrared multi-object dispersive spectrograph capable of simultaneously observing more than 100 sources over a field-of-view (FOV) larger than 3' x 3'. The NIRSpec will be the first spectrograph in space that has this capability. Targets in the Field of View are normally selected by opening groups of shutters in a micro-shutter array (MSA) to form multiple apertures. The microshutters are arranged in a waffle-like grid that contains more than 62000 shutters with each cell measuring 100 µm x 200 µm. Sweeping a magnet across the surface of the MSA opens all operable shutters. Individual shutters may then be addressed and closed electronically. NIRSpec is also capable of Fixed-slit and Integral-field spectroscopy and provides medium-resolution spectroscopy over a wavelength range of 1 - 5 µm and lower-resolution spectroscopy from 0.6 - 5 µm.NIRSpec will address all of the four main JWST science themes, and much more. It will enable large spectroscopic surveys of faint galaxies at high redshift, obtain sensitive spectra of transiting exoplanets and image line emission from protoplanetary disks and protostars. NIRSpec is being built for the European Space Agency (ESA) by the Airbus Group with Dr. Pierre Ferruit guiding its development as the ESA JWST Project Scientist. Peter Jakobsen, the NIRSpec Instrument PI, retired in December 2011. || ", "hits": 15 }, { "id": 11428, "url": "https://svs.gsfc.nasa.gov/11428/", "result_type": "Produced Video", "release_date": "2013-12-03T12:00:00-05:00", "title": "Alien Atmospheres", "description": "Since the early 1990's, astronomers have known that extrasolar planets, or \"exoplanets,\" orbit stars light-years beyond our own solar system. Although most exoplanets are too distant to be directly imaged, detailed studies have been made of their size, composition, and even atmospheric makeup - but how? By observing periodic variations in the parent star's brightness and color, astronomers can indirectly determine an exoplanet's distance from its star, its size, and its mass. But to truly understand an exoplanet astronomers must study its atmosphere, and they do so by splitting apart the parent star's light during a planetary transit. || ", "hits": 328 }, { "id": 11339, "url": "https://svs.gsfc.nasa.gov/11339/", "result_type": "Produced Video", "release_date": "2013-09-30T12:00:00-04:00", "title": "Propylene on Titan", "description": "With a thick atmosphere, clouds, a rain cycle and giant lakes, Saturn's large moon Titan is a surprisingly Earthlike place. But unlike on Earth, Titan's surface is far too cold for liquid water - instead, Titan's clouds, rain, and lakes consist of liquid hydrocarbons like methane and ethane (which exist as gases here on Earth). When these hydrocarbons evaporate and encounter ultraviolet radiation in Titan's upper atmosphere, some of the molecules are broken apart and reassembled into longer hydrocarbons like ethylene and propane.NASA's Voyager 1 spacecraft first revealed the presence of several species of atmospheric hydrocarbons when it flew by Titan in 1980, but one molecule was curiously missing - propylene, the main ingredient in plastic number 5. Now, thanks to NASA's Cassini spacecraft, scientists have detected propylene on Titan for the first time, solving a long-standing mystery about the solar system's most Earthlike moon. || ", "hits": 129 }, { "id": 11220, "url": "https://svs.gsfc.nasa.gov/11220/", "result_type": "Produced Video", "release_date": "2013-03-11T00:00:00-04:00", "title": "FGS/NIRISS Installation into the ISIM Structure", "description": "Time Lapse of FGS/NIRISS Installation into the ISIM Structure on February 28, 2013 in the NASA Goddard Space Flight Center clean room.NASA and Canadian Space Agency (CSA) engineers install the Fine Guidance Sensor (FGS) / Near-InfraRed Imager and Slitless Spectrograph (NIRISS) instrument package onto the Webb Telescope's Integrated Science Instrument Module (ISIM). The FGS/NIRISS was built by the Canadian Space Agency and delivered to NASA Goddard in July of 2012. The Fine Guidance Sensor (FGS) allows Webb to point precisely, so that it can obtain high-quality images. The Near Infrared Imager and Slitless Spectrograph part of the FGS/NIRISS will be used to investigate the following science objectives: first light detection, exoplanet detection and characterization, and exoplanet transit spectroscopy. It has a wavelength range of 0.8 to 5.0 microns, and is a specialized instrument with three main modes, each of which addresses a separate wavelength range. || ", "hits": 21 }, { "id": 20193, "url": "https://svs.gsfc.nasa.gov/20193/", "result_type": "Animation", "release_date": "2012-12-03T12:00:00-05:00", "title": "Curiosity Rover Shakes, Bakes, and Tastes Mars with SAM", "description": "NASA's Curiosity rover analyzed its first solid sample of Mars with a variety of instruments, including the Sample Analysis at Mars (SAM) instrument suite. Developed at NASA's Goddard Space Flight Center in Greenbelt, Md., SAM is a portable chemistry lab tucked inside the Curiosity rover. SAM examines the chemistry of samples it ingests, checking particularly for chemistry relevant to whether an environment can support or could have supported life. Learn more about how SAM processes samples by watching this video! || ", "hits": 37 }, { "id": 11089, "url": "https://svs.gsfc.nasa.gov/11089/", "result_type": "Produced Video", "release_date": "2012-10-18T14:00:00-04:00", "title": "IRIS Launch, Deploy and Beauty Passes", "description": "Understanding the interface between the photosphere and corona remains a fundamental challenge in solar and heliospheric science. The Interface Region Imaging Spectrograph (IRIS) mission opens a window of discovery into this crucial region by tracing the flow of energy and plasma through the chromosphere and transition region into the corona using spectrometry and imaging. IRIS is designed to provide significant new information to increase our understanding of energy transport into the corona and solar wind and provide an archetype for all stellar atmospheres. The unique instrument capabilities, coupled with state of the art 3-D modeling, will fill a large gap in our knowledge of this dynamic region of the solar atmosphere. The mission will extend the scientific output of existing heliophysics spacecraft that follow the effects of energy release processes from the sun to Earth.IRIS will provide key insights into all these processes, and thereby advance our understanding of the solar drivers of space weather from the corona to the far heliosphere, by combining high-resolution imaging and spectroscopy for the entire chromosphere and adjacent regions. IRIS will resolve in space, time, and wavelength the dynamic geometry from the chromosphere to the low-temperature corona to shed much-needed light on the physics of this magnetic interface region. || ", "hits": 24 }, { "id": 40122, "url": "https://svs.gsfc.nasa.gov/gallery/mars/", "result_type": "Gallery", "release_date": "2012-06-28T00:00:00-04:00", "title": "Mars Missions and Science", "description": "This multimedia gallery assembles and organizes Mars content on the Scientific Visualization Studio website. Highlights of NASA Goddard Space Flight Center’s animations, visualizations, videos, images and graphics relating to Mars science and missions can be found here.", "hits": 274 }, { "id": 10799, "url": "https://svs.gsfc.nasa.gov/10799/", "result_type": "Produced Video", "release_date": "2011-06-30T00:00:00-04:00", "title": "MicroSpec: Revolutionary Instrument on a Chip", "description": "Scientists may finally get a glimpse at our adolescent universe from a revolutionary new technology being developed at NASA's Goddard Space Flight Center. An instrument on a chip. This new, potentially game-changing instrument, called MicroSpec, is a far-infrared spectrometer that will be 10,000 times more sensitive and infinitely smaller than it's predecessor. || ", "hits": 38 }, { "id": 10360, "url": "https://svs.gsfc.nasa.gov/10360/", "result_type": "Produced Video", "release_date": "2009-01-15T00:00:00-05:00", "title": "Mars Methane Spectroscopy", "description": "Conceptual animation demonstrating the process of spectroscopy. The first animation demonstrates the general concept of visible-light spectroscopy by which white light is separated into its component wavelengths (colors) using a prism. The second animation demonstrates how this idea is applied to the discovery of methane in Mars' atmosphere. Because it absorbs specific wavelengths of electromagnetic energy, methane has a 'fingerprint' that can be seen as missing lines on the resulting spectograph. || Mars_Methane_Spectroscopy_mpgLG.00715_print.jpg (1024x576) [54.5 KB] || Mars_Methane_Spectroscopy_mpgLG_web.png (320x180) [60.4 KB] || Mars_Methane_Spectroscopy_mpgLG_thm.png (80x40) [6.9 KB] || Mars_Methane_Spectroscopy_h264fullres.webmhd.webm (960x540) [2.9 MB] || Mars_Methane_Spectroscopy_h264fullres.mov (1280x720) [9.7 MB] || Mars_Methane_Spectroscopy_prores.mov (1280x720) [140.3 MB] || Mars_Methane_Spectroscopy_YouTube.mov (1280x720) [6.8 MB] || Mars_Methane_Spectroscopy_ipodLG.m4v (640x360) [3.6 MB] || Mars_Methane_Spectroscopy_mpgLG.mpg (640x360) [6.2 MB] || Mars_Methane_Spectroscopy_ipodSM.m4v (320x180) [1017.7 KB] || Mars_Methane_Spectroscopy_mp4SM.mp4 (320x240) [658.4 KB] || Mars_Methane_Spectroscopy_mpgSM.mpg (512x288) [4.2 MB] || ", "hits": 44 }, { "id": 40116, "url": "https://svs.gsfc.nasa.gov/gallery/jwst/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "James Webb Space Telescope", "description": "The James Webb Space Telescope (sometimes called JWST) is a large, infrared-optimized space telescope. The observatory launched into space on an Ariane 5 rocket from the Guiana Space Centre in Kourou, French Guiana on December 25, 2021. After launch, the observatory was successfully unfolded and is being readied for science. \n\nWebb will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy. Webb will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System. Webb's instruments are designed to work primarily in the infrared range of the electromagnetic spectrum, with some capability in the visible range.\n\nWebb has a large primary mirror, 6.5 meters (21.3 feet) in diameter and a sunshield the size of a tennis court. Both the mirror and sunshade are too large to fit onto the Ariane 5 rocket fully open, so both were folded which meant they needed to be unfolded in space. \n\nWebb is currently in its operational orbit about 1.5 million km (1 million miles) from the Earth at a location known as Lagrange Point 2 (L2).\n\nThe James Webb Space Telescope was named after the NASA Administrator who crafted the Apollo program, and who was a staunch supporter of space science.", "hits": 836 } ] }