{ "count": 14, "next": null, "previous": null, "results": [ { "id": 14891, "url": "https://svs.gsfc.nasa.gov/14891/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Roman and Webb's Overlapping Roles in Understanding Our Universe", "description": "The four Roman/Webb Far and Wide videos that detail the differences between the two missions, why we need both, what they will do and how they will work together.", "hits": 224 }, { "id": 14943, "url": "https://svs.gsfc.nasa.gov/14943/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Additional Graphics", "description": "This page houses animation clips from the Far and Wide video series, which may be useful in presentations or other video products. || ", "hits": 64 }, { "id": 14598, "url": "https://svs.gsfc.nasa.gov/14598/", "result_type": "Produced Video", "release_date": "2024-06-07T00:00:00-04:00", "title": "Cruising the Cosmic Web (Dome Version)", "description": "Cruising the Cosmic Web || PRINT.jpg (1920x1080) [250.5 KB] || THUMB.jpg (1920x1080) [250.5 KB] || SEARCH.jpg (320x180) [20.0 KB] || Cruising_the_Cosmic_Web,_V2_Dome_Version.mp4 (1280x720) [36.0 MB] || 1024x1024_1x1_30p [256.0 KB] || 2200x2200_1x1_30p [256.0 KB] || ", "hits": 475 }, { "id": 14323, "url": "https://svs.gsfc.nasa.gov/14323/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Echoes of the Big Bang\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Complete list of footage usedHERE. Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_print.jpg (1024x576) [73.5 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2.jpg (3840x2160) [511.8 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_searchweb.png (320x180) [40.4 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_thm.png (80x40) [5.4 KB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.webm (1920x1080) [130.2 MB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.mp4 (1920x1080) [1.7 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_50mbps.mp4 (1920x1080) [4.1 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_ProRes_1920x1080_2997.mov (1920x1080) [14.7 GB] || ", "hits": 78 }, { "id": 40461, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles7-echoesofthe-big-bang/", "result_type": "Gallery", "release_date": "2023-03-27T00:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "NASA studies the makeup and workings of the universe, from the smallest particles of matter and energy to its large-scale structure and evolution. Scientists look far back in space and time to learn the full cosmic history of stars and galaxies. They tease out details of the environments around black holes and observe the most powerful explosions since the big bang. NASA is discovering numerous planets beyond our solar system, decoding how planetary systems form, and learning how environments hospitable for life develop.\n\nWant to know more?\nNASA Universe Webb Space Telescope images Hubble Space Telescope", "hits": 38 }, { "id": 14055, "url": "https://svs.gsfc.nasa.gov/14055/", "result_type": "Produced Video", "release_date": "2021-12-20T22:00:00-05:00", "title": "Parker Solar Probe's WISPR Images Inside The Sun's Atmosphere", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. As Parker Solar Probe flew through the corona, its WISPR instrument captured images.The Wide-Field Imager for Parker Solar Probe (WISPR) is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment.To image the solar atmosphere, WISPR uses the heat shield to block most of the Sun’s light, which would otherwise obscure the much fainter corona. Specially designed baffles and occulters reflect and absorb the residual stray light that has been reflected or diffracted off the edge of the heat shield or other parts of the spacecraft.WISPR uses two cameras with radiation-hardened Active Pixel Sensor CMOS detectors. These detectors are used in place of traditional CCDs because they are lighter and use less power. They are also less susceptible to effects of radiation damage from cosmic rays and other high-energy particles, which are a big concern close to the Sun. The camera’s lenses are made of a radiation hard BK7, a common type of glass used for space telescopes, which is also sufficiently hardened against the impacts of dust.WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, D.C. (principal investigator Russell Howard), which will also develop the observing program. || ", "hits": 284 }, { "id": 13035, "url": "https://svs.gsfc.nasa.gov/13035/", "result_type": "Produced Video", "release_date": "2018-08-08T16:00:00-04:00", "title": "Parker Solar Probe Instruments", "description": "SWEAPThe Solar Wind Electrons Alphas and Protons investigation, or SWEAP, gathers observations using two complementary instruments: the Solar Probe Cup, or SPC, and the Solar Probe Analyzers, or SPAN. The instruments count the most abundant particles in the solar wind — electrons, protons and helium ions — and measure such properties as velocity, density, and temperature to improve our understanding of the solar wind and coronal plasma. SWEAP was built mainly at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and at the Space Sciences Laboratory at the University of California, Berkeley. The institutions jointly operate the instrument. The principal investigator is Justin Kasper from the University of Michigan. || SWEAP.00001_print.jpg (1024x581) [151.9 KB] || SWEAP_thumb.png (2560x1448) [4.7 MB] || SWEAP.00001_searchweb.png (320x180) [86.1 KB] || SWEAP.00001_web.png (320x181) [86.8 KB] || SWEAP.00001_thm.png (80x40) [5.6 KB] || SWEAP.webm (1902x1080) [21.8 MB] || SWEAP.mp4 (1902x1080) [195.4 MB] || SWEAP.en_US.srt [3.8 KB] || SWEAP.en_US.vtt [3.8 KB] || ", "hits": 157 }, { "id": 10232, "url": "https://svs.gsfc.nasa.gov/10232/", "result_type": "Produced Video", "release_date": "2008-08-22T00:00:00-04:00", "title": "HST SM4 COS Installation EVA", "description": "Cosmic Origins Spectrograph (COS) will be the most sensitive ultraviolet spectrograph ever flown on Hubble. COS will probe the \"cosmic web\" - the large-scale structure of the universe whose form is determined by the gravity of dark matter and is traced by galaxies and intergalactic gas. COS will explore how the \"cosmic web\" evolved from ancient times. COS will also sample the chemical content and physical state of gas in distant galaxy halos, providing important insight into the building process of early galaxies and the production of elements heavier than hydrogen and helium over cosmic time. Required to accomplish these goals is the extraordinary sensitivity of COS's far-ultraviolet channel—a factor more than 30 times greater than that of previous spectroscopic instruments for the detection of extremely low light levels. A two-fold enhancement will be offered by COS's near-ultraviolet channel. To install the COS instrument into the Hubble Space Telescope, he Servicing Mission 4 astronauts will remove the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument (installed during Servicing Mission 1 in 1993, to correct for Hubble's spherical aberration) and then install COS in its place. || ", "hits": 18 }, { "id": 10321, "url": "https://svs.gsfc.nasa.gov/10321/", "result_type": "Produced Video", "release_date": "2008-08-01T00:00:00-04:00", "title": "HST SM4 Resource Reel v2.0", "description": "1. Hubble Space Telescope Service Mission 4 Animation: A collection of several animations showing the Hubble Space Telescope orbiting Earth and in space shuttle Atlantis cargo bay. All animations depict the Hubble Space Telescope in its current (July 2008) configuration. || 1-resource-hstsm4animation-resourcereelreference_MPEG-100852_print.jpg (1024x768) [98.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_web.png (320x240) [107.6 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_thm.png (80x40) [16.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_searchweb.png (320x180) [85.3 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.webmhd.webm (960x540) [12.8 MB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.mpg (320x240) [63.5 MB] || ", "hits": 21 }, { "id": 10318, "url": "https://svs.gsfc.nasa.gov/10318/", "result_type": "Produced Video", "release_date": "2008-07-26T00:00:00-04:00", "title": "HST SM4 Extended Resource Reel v2.0", "description": "Full HD Resource ReelThis resource reel includes all the clips shown below on this page. || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.00001_print.jpg (1024x576) [99.1 KB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.mov (1280x720) [57.2 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.mp4 (1280x720) [4.1 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.webm (1280x720) [454.7 MB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.webm [0 bytes] || ", "hits": 45 }, { "id": 10217, "url": "https://svs.gsfc.nasa.gov/10217/", "result_type": "Produced Video", "release_date": "2008-05-20T00:00:00-04:00", "title": "HST Zoom-Way-Out", "description": "An animation of the Hubble Space Telescope in orbit where the camera zooms out to show how tiny Hubble is in relation to Earth and then how small Earth is in relation to space. Companion animation is Cosmic Origins Spectrograph: Large Scale Structure of the Universe. || ", "hits": 22 }, { "id": 10223, "url": "https://svs.gsfc.nasa.gov/10223/", "result_type": "Produced Video", "release_date": "2008-05-20T00:00:00-04:00", "title": "Cosmic Origins Spectrograph: Large Scale Structure of the Universe", "description": "The Cosmic Origins Spectrograph (COS) instrument will be placed in the Hubble Space Telescope during Service Mission 4. It's primary science objectives are the study of the origins of large scale structure in the Universe, the formation and evolution of galaxies, the origin of stellar and planetary systems, and the cold interstellar medium. This animation zooms out from our Milky Way galaxy to show the cosmic web, or large scale structure of the Universe. || ", "hits": 90 }, { "id": 10118, "url": "https://svs.gsfc.nasa.gov/10118/", "result_type": "Produced Video", "release_date": "2007-07-30T00:00:00-04:00", "title": "Journey Through the Cosmic Web: Cosmic Cruising 2", "description": "This animation flies through the cosmic web of the early universe. At the end, we see the Hubble Space Telescope collecting data points.Launched in 1990, the Hubble Space Telescope (HST) has revolutionized astronomy by providing unprecedented views of the Universe. Hubble's spectral range extends from the ultraviolet, through the visible, and into the near-infrared. NASA will fly a servicing mission in 2008 to bring two new science instruments to Hubble - the Cosmic Origins Spectrograph and the Wide Field Camera 3. New gyros and batteries will extend Hubble's life through 2013. || ", "hits": 1953 }, { "id": 7, "url": "https://svs.gsfc.nasa.gov/7/", "result_type": "Visualization", "release_date": "1990-07-10T12:00:00-04:00", "title": "Stellar Wind Disruption by an Orbiting Neutron Star: Neutron Star Close-up", "description": "A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own. The high luminosity of the massive star drives a strong wind from its surface. The neutron star crashes through this wind at over 300 kilometers per second. The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star. The large scale structure seen in the accretion wake is powered by the release of gravitational potential energy near the surface of the neutron star.The numerical simulations depicted here were computed using the Cray X-MP 48 at the National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign. || ", "hits": 56 } ] }