{ "count": 195, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=Solid+Earth", "previous": null, "results": [ { "id": 31394, "url": "https://svs.gsfc.nasa.gov/31394/", "result_type": "Hyperwall Visual", "release_date": "2026-05-06T12:00:00-04:00", "title": "NASA Studies Fire in Microgravity", "description": "Images from studies of fire's behavior in microgravity aboard the ISS.", "hits": 333 }, { "id": 14979, "url": "https://svs.gsfc.nasa.gov/14979/", "result_type": "Produced Video", "release_date": "2026-03-26T14:00:00-04:00", "title": "Early Testing of Aerogel and Silicon Detectors for TIGERISS", "description": "Nick Cannady, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, examines a block of silica aerogel in May 2025. Cannady uses the light weight material in detectors for the upcoming TIGERISS (Trans-Iron Galactic Element Recorder for the International Space Station) mission, which is designed to study high-speed charged particles called cosmic rays.Credit: NASA/Scott WiessingerAlt text: A man studies a transparent block of aerogel.Image description: A man with glasses wearing a blue checkered shirt examines a block of transparent material resting on a table. He is leaning and rests his right hand on the table. The block glows faintly blue. The table is gray with evenly spaced rows of holes. || Tigeriss-Aerogel__Nick_Cannady-3.jpg (6393x4718) [17.4 MB] || Tigeriss-AerogelNick_Cannady-3-small.jpg (3196x2359) [1.6 MB] || ", "hits": 210 }, { "id": 5625, "url": "https://svs.gsfc.nasa.gov/5625/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami", "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.", "hits": 713 }, { "id": 5626, "url": "https://svs.gsfc.nasa.gov/5626/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)", "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.", "hits": 229 }, { "id": 5572, "url": "https://svs.gsfc.nasa.gov/5572/", "result_type": "Visualization", "release_date": "2025-08-08T14:00:02-04:00", "title": "GEOS Aerosols", "description": "Aerosols are tiny solid or liquid particles that float in the atmosphere and can travel long distances, affecting air quality and visibility far from their sources. This visualization covers the period from August 1 to September 14, 2024, and is based on NASA's Goddard Earth Observing System (GEOS) model, which delivers realistic, high-resolution weather and aerosol data that enable customized environmental prediction and advances in AI research.", "hits": 626 }, { "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": 60 }, { "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": 50 }, { "id": 5552, "url": "https://svs.gsfc.nasa.gov/5552/", "result_type": "Visualization", "release_date": "2025-06-23T09:00:00-04:00", "title": "Science On A Sphere: Aerosols in the Air", "description": "NASA merges observations, advanced models and computing power to monitor aerosols in the atmosphere. Aerosols are tiny invisible solid or liquid particles that float in the atmosphere and can travel long distances affecting air quality and visibility far from their source. These particles come from natural and human sources and include black carbon (orange/red), sea salt (cyan), dust (magenta) and sulfates (green).", "hits": 589 }, { "id": 14772, "url": "https://svs.gsfc.nasa.gov/14772/", "result_type": "B-Roll", "release_date": "2025-01-29T11:00:00-05:00", "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics", "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ", "hits": 699 }, { "id": 14774, "url": "https://svs.gsfc.nasa.gov/14774/", "result_type": "Produced Video", "release_date": "2025-01-29T11:00:00-05:00", "title": "NASA Finds Ingredients of Life in Fragments of Lost World", "description": "Scientists studying the Bennu samples have discovered evidence of a wet, salty environment from 4.5 billion years ago that created the molecular building blocks of life.Complete transcript available.Universal Production Music: “Future Tense” by Gresby Race Nash [PRS]; “Take Off” by Nicholas Smith [PRS]; “Big Decision” by Gresby Race Nash [PRS]; “Waiting for the Answer” by Gresby Race Nash [PRS]Watch this video on the NASA Goddard YouTube channel. || 14774-Bennu-Organics-Thumbnail-V4_print.jpg (1024x576) [395.9 KB] || 14774-Bennu-Organics-Thumbnail-V4.jpg (1280x720) [1.2 MB] || 14774-Bennu-Organics-Thumbnail-V4.png (1280x720) [1.8 MB] || 14774-Bennu-Organics-Thumbnail-V4_searchweb.png (320x180) [120.2 KB] || 14774-Bennu-Organics-Thumbnail-V4_thm.png [8.3 KB] || 14774_OSIRIS-REx_Bennu_Organics_720.mp4 (1280x720) [66.1 MB] || 14774_OSIRIS-REx_Bennu_Organics_1080.mp4 (1920x1080) [370.5 MB] || BennuOrganicsCaptions.en_US.srt [6.4 KB] || BennuOrganicsCaptions.en_US.vtt [6.0 KB] || 14774_OSIRIS-REx_Bennu_Organics_4K.mp4 (3840x2160) [2.3 GB] || 14774_OSIRIS-REx_Bennu_Organics_ProRes.mov (3840x2160) [14.5 GB] || ", "hits": 481 }, { "id": 31241, "url": "https://svs.gsfc.nasa.gov/31241/", "result_type": "Hyperwall Visual", "release_date": "2024-09-23T00:00:00-04:00", "title": "East African Rift Valley Volcanoes", "description": "Volcanic, tectonic, erosional and sedimentary landforms are all evident in this elevation model image of a region along the East African Rift at Lake Kivu. The area shown covers parts of Congo, Rwanda and Uganda.Lake Kivu, in the lower left of the image, lies within the East African Rift, an elongated tectonic pull-apart depression in Earth's crust. The rift extends to the northeast as a smooth lava- and sediment-filled trough. Two volcanic complexes are seen in the rift. The one closer to the lake is the Nyiragongo volcano, which erupted in January 2002, sending lava toward the lake shore and through the city of Goma. East of the rift, even more volcanoes are seen. These are the Virunga volcano chain, which is the home of the endangered mountain gorillas. Note that the terrain surrounding the volcanoes is much smoother than the eroding mountains that cover most of this view, such that topography alone is a good indicator of the extent of the lava flows.Elevation data used in this image was acquired by the Shuttle Radar Topography Mission aboard Space Shuttle Endeavour, launched on Feb. 11, 2000. The mission used the same radar instrument that comprised the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) that flew twice on Endeavour in 1994. || ", "hits": 243 }, { "id": 14652, "url": "https://svs.gsfc.nasa.gov/14652/", "result_type": "Produced Video", "release_date": "2024-08-15T17:00:00-04:00", "title": "Exploring Volcanoes with NASA’s GEODES Team", "description": "Enjoy this music video of NASA’s GEODES team exploring lunar-like landscapes.Complete transcript available.Music credit: “Aerial” by Ben Cosgrove” and \"Volcano\" by Ben Cosgrove. Used with permission from the artist.Watch this video on the NASA Goddard YouTube channel. || ExploringVolcanoes_Thumbnail_print.jpg (1024x576) [185.0 KB] || ExploringVolcanoes_Thumbnail.png (1280x720) [1.2 MB] || ExploringVolcanoes_Thumbnail_searchweb.png (320x180) [106.5 KB] || ExploringVolcanoes_Thumbnail_thm.png (80x40) [8.4 KB] || ExploringVolcanoes_720.mp4 (1280x720) [67.0 MB] || EXPLORING_VOLCANOES_Captions_Final.en_US.srt [2.1 KB] || EXPLORING_VOLCANOES_Captions_Final.en_US.vtt [2.0 KB] || ExploringVolcanoes.mp4 (1920x1080) [471.1 MB] || ", "hits": 42 }, { "id": 14576, "url": "https://svs.gsfc.nasa.gov/14576/", "result_type": "Visualization", "release_date": "2024-05-06T13:00:00-04:00", "title": "NASA Black Hole Visualization Takes Viewers Beyond the Brink", "description": "In this flight toward a supermassive black hole, labels highlight many of the fascinating features produced by the effects of general relativity along the way. This supercomputer visualization tracks a camera as it approaches, briefly orbits, and then crosses the event horizon — the point of no return — of a supersized black hole similar in mass to the one at the center of our galaxy. Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. PowellMusic: “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music“Memories” from Digital Juice“Path Finder,” Eric Jacobsen [TONO] and Lorenzo Castellarin [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14576_BHPlunge_Explain_Still.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail_searchweb.png (180x320) [85.0 KB] || 14576_PageThumbnail_thm.png (80x40) [9.6 KB] || 14576_BHPlunge_Explainer_1080.mp4 (1920x1080) [319.5 MB] || 14576_BHPlunge_Explainer_Captions.en_US.srt [2.5 KB] || 14576_BHPlunge_Explainer_Captions.en_US.vtt [2.4 KB] || 14576_BHPlunge_Explainer_4k.mp4 (3840x2160) [1.5 GB] || 14576_BHPlunge_Explainer_4kYouTube.mp4 (3840x2160) [3.0 GB] || 14576_BHPlunge_Explainer_ProRes_3840x2160_2997.mov (3840x2160) [12.8 GB] || ", "hits": 2166 }, { "id": 14574, "url": "https://svs.gsfc.nasa.gov/14574/", "result_type": "Produced Video", "release_date": "2024-05-06T10:00:00-04:00", "title": "Black Hole Week 2024 Poster and Media", "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.", "hits": 183 }, { "id": 31277, "url": "https://svs.gsfc.nasa.gov/31277/", "result_type": "Hyperwall Visual", "release_date": "2024-04-12T00:00:00-04:00", "title": "Gravity waves from Hunga Tonga Eruption", "description": "Gravity waves caused by the Hunga Tonga-Hunga Ha′apai volcanic eruption can be seen in Geostationary satellite data by taking the difference between subsequent images. Global images are acquired every 10 minutes by the GOES and Himawari weather satellite imagers. Calculating the difference between two subsequent images reveals circular gravity waves spreading out from the eruption center. || ", "hits": 166 }, { "id": 5157, "url": "https://svs.gsfc.nasa.gov/5157/", "result_type": "Visualization", "release_date": "2023-11-28T09:20:00-05:00", "title": "Fermi Catalog of Gamma-ray Pulsars", "description": "A visualization of the 294 pulsars in the Fermi gamma-ray pulsar catalog. The visualization starts with a full-sky Hammer projection view of the catalog. Different types of pulsars are indicated by different markers. The pulsar markers oscillate in size according to the object's pulsation frequency at actual speed. Millisecond pulsars are just shown as solid markers. The map then morphs into the full 3D view of the pulsar distribution, and we then fly out to give a top down view showing the distribution of gamma-ray pulsars in our galaxy. || pulsar3DMap_2160p30.00200_print.jpg (1024x576) [174.0 KB] || pulsar3DMap_2160p30.00200_searchweb.png (320x180) [72.3 KB] || pulsar3DMap_2160p30.00200_thm.png (80x40) [5.4 KB] || full (3840x2160) [0 Item(s)] || pulsar3DMap_2160p30.mp4 (3840x2160) [240.8 MB] || ", "hits": 239 }, { "id": 4948, "url": "https://svs.gsfc.nasa.gov/4948/", "result_type": "Visualization", "release_date": "2023-09-13T10:00:00-04:00", "title": "Reforestation in Kigoma region of Tanzania: 2005 - 2014", "description": "This visualization begins by showing the location of the village of Kigalye, south of the Gombe National Park in Tanzania. The topography of that region is draped with a satellite image taken on May 14, 2005. As we fly up the valley between Kigalye and the park, scars from deforestation cover much of the landscape. || habitat_reforestation_4k_60fps_2005.1000_print.jpg (1024x576) [290.7 KB] || habitat_reforestation_4k_30fps_2005_1080p30.webmhd.webm (1080x606) [10.0 MB] || habitat_reforestation_4k_30fps_2005_1080p30.mp4 (1920x1080) [49.6 MB] || habitat_reforestation_4k_60fps_2005_1080p60.mp4 (1920x1080) [52.8 MB] || Yr_2005 (3840x2160) [0 Item(s)] || Yr_2005 (3840x2160) [0 Item(s)] || habitat_reforestation_2005_2160p30.mp4 (3840x2160) [151.6 MB] || habitat_reforestation_2005_2160p60.mp4 (3840x2160) [152.5 MB] || ", "hits": 51 }, { "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": 947 }, { "id": 31199, "url": "https://svs.gsfc.nasa.gov/31199/", "result_type": "Hyperwall Visual", "release_date": "2022-10-31T00:00:00-04:00", "title": "Earth Surface Mineral Dust Source Investigation (EMIT) for hyperwall", "description": "Animation showing location of EMIT on the ISS || emit_on_iss_print.jpg (1024x576) [93.5 KB] || emit_on_iss.png (3840x2160) [3.2 MB] || emit_on_iss_searchweb.png (320x180) [67.7 KB] || emit_on_iss_thm.png (80x40) [6.1 KB] || emit_on_iss_1080p60.mp4 (1920x1080) [10.8 MB] || emit_on_iss_1080p60.webm (1920x1080) [3.0 MB] || emit_on_iss_2160p60.mp4 (3840x2160) [28.3 MB] || emit_on_iss.hwshow [198 bytes] || Images and videos prepared for hyperwall for EMIT. || ", "hits": 36 }, { "id": 14214, "url": "https://svs.gsfc.nasa.gov/14214/", "result_type": "Produced Video", "release_date": "2022-09-20T00:00:00-04:00", "title": "How NASA Sees the Life Cycle of Volcanic Island Hunga Tonga-Hunga Ha’apai", "description": "Complete transcript available. || HHTH_Final.00001_print.jpg (1024x576) [78.9 KB] || Thumbnail.png (2838x1588) [5.2 MB] || HHTH_Final.00001_searchweb.png (320x180) [66.5 KB] || HHTH_Final.00001_thm.png (80x40) [5.0 KB] || HHTH_Final.webm (1920x1080) [43.1 MB] || HHTH_Final.mp4 (1920x1080) [779.2 MB] || HHTH_Audio_otter_ai.en_US.srt [7.7 KB] || HHTH_Audio_otter_ai.en_US.vtt [7.7 KB] || ", "hits": 148 }, { "id": 5023, "url": "https://svs.gsfc.nasa.gov/5023/", "result_type": "Visualization", "release_date": "2022-09-19T09:30:00-04:00", "title": "Lunar Polar Wander", "description": "The wandering path of the lunar South Pole is shown over a period from 4.25 billion years ago to the present.This video can also be viewed on the SVS YouTube channel. || tpw.0750_print.jpg (1024x576) [250.9 KB] || tpw.0750_searchweb.png (320x180) [109.2 KB] || tpw.0750_thm.png (80x40) [7.6 KB] || tpw_1080p30.mp4 (1920x1080) [46.9 MB] || tpw_720p30.mp4 (1280x720) [22.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || tpw_720p30.webm (1280x720) [5.6 MB] || tpw_360p30.mp4 (640x360) [8.1 MB] || tpw_1080p30.mp4.hwshow [177 bytes] || ", "hits": 104 }, { "id": 20362, "url": "https://svs.gsfc.nasa.gov/20362/", "result_type": "Animation", "release_date": "2022-07-07T15:20:00-04:00", "title": "Gravity on the Moon vs. Asteroid Bennu: Animation", "description": "The lunar surface is better at resisting impacts than the loose surface of asteroid Bennu – thanks to the Moon’s much stronger gravity. || OREX-MoonvsBennuMograph-ProRes.00240_print.jpg (1024x576) [74.2 KB] || OREX-MoonvsBennuMograph-ProRes.00240_searchweb.png (320x180) [60.3 KB] || OREX-MoonvsBennuMograph-ProRes.00240_thm.png (80x40) [4.3 KB] || OREX-MoonvsBennuMograph-ProRes_1080.mp4 (1920x1080) [58.2 MB] || 3840x2160_16x9_30p (3840x2160) [128.0 KB] || OREX-MoonvsBennuMograph-ProRes.webm (3840x2160) [8.7 MB] || OREX-MoonvsBennuMograph-ProRes.mov (3840x2160) [3.2 GB] || OREX-MoonvsBennuMograph-ProRes_4K.mp4 (3840x2160) [238.1 MB] || ", "hits": 225 }, { "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": 6753 }, { "id": 4983, "url": "https://svs.gsfc.nasa.gov/4983/", "result_type": "Visualization", "release_date": "2022-04-11T12:00:00-04:00", "title": "Global Carbon Dioxide 2020-2021 for Hyperwalls", "description": "This webpage provides a wide aspect ratio version of: Global Carbon Dioxide 2020-2021, released on November 2, 2021. This version has been created for wide aspect ratio display systems with resolution up to 9600x3240. It is recommended to use content from this version for display systems with 16:9 aspect ratio. || ", "hits": 85 }, { "id": 14121, "url": "https://svs.gsfc.nasa.gov/14121/", "result_type": "Produced Video", "release_date": "2022-03-29T11:00:00-04:00", "title": "The Geocenter of the Earth Is Changing (And Why That Matters)", "description": "Stock Footage: Pond5Universal Production Music: Kinda Frantic by Steve Rucker [ASCAP]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com is obtained through permission and may not be excised or remixed in other products. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.htmlComplete transcript available. || 14121_Geodesy.jpg (1920x1080) [538.3 KB] || 14121_Geodesy_searchweb.png (320x180) [94.1 KB] || 14121_Geodesy_thm.png (80x40) [5.9 KB] || 14121_Geocenter.mp4 (1920x1080) [252.5 MB] || 14121_Geocenter_TWITTER.mp4 (1280x720) [65.3 MB] || 14121_Geocenter_TWITTER.webm (1280x720) [26.6 MB] || 14121_Geocenter.webm (1920x1080) [26.9 MB] || 14121_Geocenter_en.us.en_US.srt [5.3 KB] || 14121_Geocenter_en.us.en_US.vtt [5.1 KB] || ", "hits": 165 }, { "id": 4917, "url": "https://svs.gsfc.nasa.gov/4917/", "result_type": "Visualization", "release_date": "2021-11-29T11:00:00-05:00", "title": "ICON Snaps a Peek at the Ionospheric Dynamo", "description": "Visualization of ICON in Earth orbit, camera ahead of the spacecraft looking back on spacecraft and limb of Earth. Magenta curves are lines of Earth's geomagnetic field. Field-of-view (FOV) of MIGHTI imagers (green frustums) and the longitudinal wind vectors (green arrows) it measures are shown. MIGHTI imagers FOV eventually fades out. Vertical plasma speed (red arrows) is measured at the spacecraft. Magnetic field lines turn yellow as measurements of winds by MIGHT provide a connection to influence the plasma velocity measured at the spacecraft, redirecting the plasma flow from upward to downward. || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_print.jpg (1024x576) [135.0 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_searchweb.png (320x180) [79.4 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_thm.png (80x40) [5.7 KB] || ICONSyncView+x (1920x1080) [0 Item(s)] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4 (1920x1080) [36.4 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.webm (1920x1080) [5.1 MB] || ICONSyncView+x (3840x2160) [0 Item(s)] || ICONDataView.ICONSyncView+x.2160p30.mp4 (3840x2160) [114.3 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4.hwshow || ", "hits": 69 }, { "id": 4949, "url": "https://svs.gsfc.nasa.gov/4949/", "result_type": "Visualization", "release_date": "2021-11-02T00:00:00-04:00", "title": "Global Carbon Dioxide 2020-2021", "description": "Data visualization featuring volumetric carbon dioxide on a global scale for the period June 1, 2020 - July 31, 2021.Coming soon to our YouTube channel. || CO2Volumetric_1024x576_02582_print.jpg (1024x576) [90.6 KB] || CO2Volumetric_1024x576_02582.png (1024x576) [569.1 KB] || CO2Volumetric_1024x576_02582_searchweb.png (180x320) [60.0 KB] || CO2Volumetric_1024x576_02582_thm.png (80x40) [5.1 KB] || CO2Volumetric_1920x1080p30.mp4 (1920x1080) [65.3 MB] || CO2Volumetric_1920x1080p30.webm (1920x1080) [13.3 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || CO2Volumetric_3840x2160_30fps_02582.exr (3840x2160) [63.3 MB] || CO2Volumetric_3840x2160_30fps_02582.tif (3840x2160) [44.5 MB] || captions_silent.31831.en_US.srt [43 bytes] || CO2Volumetric_3840x2160p30.mp4 (3840x2160) [931.2 MB] || ", "hits": 146 }, { "id": 4920, "url": "https://svs.gsfc.nasa.gov/4920/", "result_type": "Visualization", "release_date": "2021-08-04T17:00:00-04:00", "title": "Earth System Observatory", "description": "An animated graphic showing the areas of focus for NASA's Earth System Observatory. || EarthSystemObservatory_9.00001_print.jpg (1024x576) [158.4 KB] || EarthSystemObservatory_9.00001_searchweb.png (320x180) [72.0 KB] || EarthSystemObservatory_9.00001_web.png (320x180) [72.0 KB] || EarthSystemObservatory_9.00001_thm.png (80x40) [6.4 KB] || EarthSystemObservatory_9.mp4 (1920x1080) [44.9 MB] || EarthSystemObservatory_9.webm (1920x1080) [4.6 MB] || EarthSystemObservatory_4K_9.mp4 (3840x2160) [47.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || EarthSystemObservatory_9.mp4.hwshow [220 bytes] || earth-system-observatory-4k-movie.hwshow [329 bytes] || ", "hits": 161 }, { "id": 13874, "url": "https://svs.gsfc.nasa.gov/13874/", "result_type": "Produced Video", "release_date": "2021-07-09T10:42:00-04:00", "title": "SPEXone: Dutch Instrument Arrives for PACE Mission", "description": "Aerosols are small solid or liquid particles suspended in the air that affect climate change directly throuhg interaction with solar radiation. Aerosols affect climate indirectly by changing the micro-and macro- physical properties of clouds. Scientists who study climate change rely on detailed data to properly characterize the the amount of radiative forcing that aerosols cause. SPEXone is a new instrument designed to pursue that data with superb accuracy. It's a polarimeter, intended to measure the intensity, Degree of Linear Polarization (DoLP) and Angle of Linear Polarization (AoLP) of sunlight reflected back from Earth's atmosphere, land surface, and ocean. Built by engineers at The Netherlands Institute for Space Research (SRON) and Airbus Defence and Space Netherlands (Airbus DS NL), SPEXone will fly on the PACE spacecraft as one of that mission's suite of sensors. || ", "hits": 24 }, { "id": 13873, "url": "https://svs.gsfc.nasa.gov/13873/", "result_type": "Produced Video", "release_date": "2021-07-01T00:00:00-04:00", "title": "Periodic Table of the Elements: Origins of the Elements", "description": "The periodic table organizes all the known elements by atomic number, which is the number of protons in each atom of the element. This version of the table, which draws on data compiled by astronomer Jennifer Johnson from Ohio State University, shows our current understanding of how each element found on Earth was originally produced. Most of them ultimately have cosmic origins. Some elements were created with the birth of the universe, while others were made during the lives or deaths of stars. The Nancy Grace Roman Space Telescope will help us understand the cosmic era when stars first began forming. The mission will help scientists learn more about how elements were created and distributed throughout galaxies.The related Tumblr post is here. || ", "hits": 2174 }, { "id": 13836, "url": "https://svs.gsfc.nasa.gov/13836/", "result_type": "Produced Video", "release_date": "2021-04-12T10:40:00-04:00", "title": "Delta-X Media Day", "description": "Music: Circles of Life and Building Ideas by Todd James Carlin Baker [DPRS]Complete transcript available. || Delta-X_Final_4_12_W_Broll.00001_print.jpg (1024x576) [301.9 KB] || Delta-X_Final_4_12_W_Broll.00001_searchweb.png (320x180) [106.2 KB] || Delta-X_Final_4_12_W_Broll.00001_thm.png (80x40) [6.8 KB] || Delta-X_Final_4_12_W_Broll.webm (1920x1080) [26.8 MB] || DeltaX.en_US.srt [4.5 KB] || DeltaX.en_US.vtt [4.5 KB] || Delta-X_Final_4_12_W_Broll.mp4 (1920x1080) [487.7 MB] || ", "hits": 19 }, { "id": 4893, "url": "https://svs.gsfc.nasa.gov/4893/", "result_type": "Visualization", "release_date": "2021-04-01T10:00:00-04:00", "title": "Shadows near the Moon's South Pole", "description": "This video shows the movement of shadows near the Moon's South Pole, over the course of two lunar days, which is approximately two months on Earth. The visualization was created from data gathered by the Lunar Reconnaissance Orbiter spacecraft.Music Provided by Universal Production Music: “Two Horizons” – Anthony d’AmarioWatch this video on the NASA Goddard YouTube channel. || ShadowsMoonSouthPole_Thumbnail1.jpg (1920x1080) [381.7 KB] || ShadowsMoonSouthPole_Thumbnail1_print.jpg (1024x576) [133.0 KB] || ShadowsMoonSouthPole_YouTubeHD.webm (1920x1080) [10.8 MB] || ShadowsMoonSouthPole_YouTubeHD.mp4 (1920x1080) [157.1 MB] || ShadowsMoonSouthPole_FacebookHD.mp4 (1920x1080) [118.7 MB] || ShadowsMoonSouthPole_CAPTIONS.en_US.srt [1.3 KB] || ShadowsMoonSouthPole_CAPTIONS.en_US.vtt [1.3 KB] || ShadowsMoonSouthPole_MASTER.mov (1920x1080) [1.3 GB] || ShadowsMoonSouthPole_FacebookHD.mp4.hwshow || ", "hits": 328 }, { "id": 13739, "url": "https://svs.gsfc.nasa.gov/13739/", "result_type": "Produced Video", "release_date": "2020-11-05T10:00:00-05:00", "title": "Rising Waters: Our Dynamic Earth", "description": "Universal Production Music: \"Patisserie Pressure\" by Benjamin James Parsons [PRS]Complete transcript available.This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com and Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.htmlNotes on Footage: Provided by Artbeats: 00:00-00:03; 00:08-00:15; 01:02-01:09; 01:48-01:52; 01:58-02:02Stock: 1:29 – 1:33 provided by Razvan25/Pond5 || Card_Title.jpg (1920x1080) [1003.9 KB] || Card_Title_print.jpg (1024x576) [348.9 KB] || Card_Title_searchweb.png (320x180) [102.1 KB] || Card_Title_web.png (320x180) [102.1 KB] || Card_Title_thm.png (80x40) [7.2 KB] || 13739_SLR_Subsidence.mov (1920x1080) [1.8 GB] || 13739_SLR_Subsidence.mp4 (1920x1080) [245.2 MB] || 13739_SLR_Subsidence_lowres.mp4 (1280x720) [42.2 MB] || 13739_SLR_Subsidence_lowres.webm (1280x720) [17.1 MB] || SLR_captions.en_US.srt [2.6 KB] || SLR_captions.en_US.vtt [2.6 KB] || ", "hits": 38 }, { "id": 13721, "url": "https://svs.gsfc.nasa.gov/13721/", "result_type": "Produced Video", "release_date": "2020-09-22T11:45:00-04:00", "title": "International Observe the Moon Night live shots", "description": "Quick link to associated B-ROLL for interviews.Quick link to canned interview with Andrea Jones NASA Public Engagement / Director, International Observe the Moon NightClick here to find out more about this year's International Observe the Moon night || observe-moon-night.png (1920x1080) [552.9 KB] || observe-moon-night_print.jpg (1024x576) [71.6 KB] || observe-moon-night_searchweb.png (320x180) [47.3 KB] || observe-moon-night_thm.png (80x40) [5.2 KB] || ", "hits": 83 }, { "id": 13688, "url": "https://svs.gsfc.nasa.gov/13688/", "result_type": "Produced Video", "release_date": "2020-08-17T11:45:00-04:00", "title": "NASA Explores Earth's Magnetic \"Dent\"", "description": "Music: \"Now We Wait\" by Kamal David Kamruddin [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com and Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.Complete transcript available. || South_Atlantic_Anomaly_Still_2.jpg (1920x1080) [346.0 KB] || South_Atlantic_Anomaly_Still_2_print.jpg (1024x576) [139.2 KB] || South_Atlantic_Anomaly_Still_2_searchweb.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_web.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_thm.png (80x40) [4.8 KB] || 13688_South_Atlantic_Anomaly_Fine.mov (1920x1080) [2.6 GB] || 13688_South_Atlantic_Anomaly_Fine.webm (960x540) [65.7 MB] || 13688_South_Atlantic_Anomaly_Fine.mp4 (1920x1080) [292.9 MB] || 13688_South_Atlantic_Anomaly_Fine_lowres.mp4 (1280x720) [52.3 MB] || SAA.en_US.srt [3.5 KB] || SAA.en_US.vtt [3.5 KB] || ", "hits": 232 }, { "id": 4840, "url": "https://svs.gsfc.nasa.gov/4840/", "result_type": "Visualization", "release_date": "2020-08-17T11:00:00-04:00", "title": "South Atlantic Anomaly: 2015 through 2025", "description": "South Atlantic Anomaly from 2015 through 2025 showing the geomagnetic intensity at the Earth's surface and the core-mantle boundary. There are versions that include the dates and colorbars and versions without the date and colorbat.This video is also available on our YouTube channel. || saa_intensity_comp2160_p60.4898_print.jpg (1024x576) [58.0 KB] || saa_intensity_comp2160_p60.4898_print_searchweb.png (320x180) [49.9 KB] || saa_intensity_comp2160_p60.4898_print_thm.png (80x40) [3.8 KB] || saa_intensity_comp_1080p30.mp4 (1920x1080) [31.9 MB] || saa_intensity_comp_1080p60.mp4 (1920x1080) [34.4 MB] || saa_intensity_dataOnly_1080_p30.mp4 (1920x1080) [29.3 MB] || saa_intensity_dataOnly_1080_p60.mp4 (1920x1080) [31.3 MB] || saa_intensity_dataOnly_1080_p30.webm (1920x1080) [9.1 MB] || dataOnly (1920x1080) [0 Item(s)] || saa_intensity_comp2160_p30.mp4 (3840x2160) [86.1 MB] || saa_intensity_comp2160_p60.mp4 (3840x2160) [93.1 MB] || comp (3840x2160) [0 Item(s)] || captions_silent.29860.en_US.srt [43 bytes] || saa_intensity_dataOnly_1080_p30.mp4.hwshow [197 bytes] || ", "hits": 1771 }, { "id": 13661, "url": "https://svs.gsfc.nasa.gov/13661/", "result_type": "Produced Video", "release_date": "2020-07-10T09:50:00-04:00", "title": "NASA Missions Spot Comet NEOWISE", "description": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO || wide.00250_print.jpg (1024x576) [164.4 KB] || wide.mp4 (3840x2160) [72.2 MB] || wide.webm (3840x2160) [6.2 MB] || ", "hits": 75 }, { "id": 13623, "url": "https://svs.gsfc.nasa.gov/13623/", "result_type": "Produced Video", "release_date": "2020-06-17T10:00:00-04:00", "title": "Four of Our Favorite SOHO-discovered Comets", "description": "Karl Battams, manager of NASA's citizen science Sungrazer Project, talks about his four favorite comets that SOHO has observed.Music: \"Inducing Waves\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_print.jpg (1024x576) [155.4 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_searchweb.png (320x180) [72.1 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_thm.png (80x40) [5.3 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.mov (1920x1080) [3.1 GB] || 13623_SOHO4FavoriteComets_1080.mp4 (1920x1080) [245.9 MB] || 13623_SOHO4FavoriteComets_Good_1080.mp4 (1920x1080) [128.8 MB] || 13623_SOHO4FavoriteComets_1080.webm (1920x1080) [27.2 MB] || SOHO_4000Comets_SRT_Captions.en_US.srt [4.8 KB] || SOHO_4000Comets_SRT_Captions.en_US.vtt [4.8 KB] || ", "hits": 36 }, { "id": 13565, "url": "https://svs.gsfc.nasa.gov/13565/", "result_type": "Produced Video", "release_date": "2020-02-27T15:00:00-05:00", "title": "Asteroid Bennu: Selecting Site Nightingale", "description": "After a year of studying asteroid Bennu, the OSIRIS-REx mission chose a location called “Nightingale” as the primary sample collection site.Universal Production Music: “Extreme Measures” by John Sands and Marc Ferrari, “Ice Echoes” by Dominik Luke Marsden Johnson, “Look at the Mirror” by Jonathan FigoliWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Bennu20cmGlobalPreviewV3_print.jpg (1024x576) [150.9 KB] || Bennu20cmGlobalPreviewV3.jpg (3840x2160) [2.4 MB] || Bennu20cmGlobalPreviewV3_web.png (320x180) [19.5 KB] || Bennu20cmGlobalPreviewV3_searchweb.png (320x180) [19.5 KB] || Bennu20cmGlobalPreviewV3_thm.png (80x40) [2.1 KB] || TWITTER_720_13565_Bennu_Nightingale_MASTER_twitter_720.mp4 (1280x720) [42.3 MB] || 13565_Bennu_Nightingale_MASTER.webm (960x540) [96.1 MB] || FACEBOOK_720_13565_Bennu_Nightingale_MASTER_facebook_720.mp4 (1280x720) [252.3 MB] || YOUTUBE_1080_13565_Bennu_Nightingale_MASTER_youtube_1080.mp4 (1920x1080) [319.9 MB] || 13565_Bennu_Nightingale_CAPTIONS.en_US.srt [5.3 KB] || 13565_Bennu_Nightingale_CAPTIONS.en_US.vtt [5.3 KB] || 13565_Bennu_Nightingale_MASTER.mp4 (3840x2160) [4.8 GB] || 13565_Bennu_Nightingale_MASTER.mov (3840x2160) [13.4 GB] || ", "hits": 43 }, { "id": 4778, "url": "https://svs.gsfc.nasa.gov/4778/", "result_type": "Visualization", "release_date": "2020-01-23T09:00:00-05:00", "title": "Earth Versus Proxima Centauri b Rotation Rates", "description": "Earth spins on its axis every 24 hours. Proxima B is tidally locked and therefore always faces it's star, much like how the moon has one side that always faces Earth. || near_evb.00333_print.jpg (1024x576) [88.2 KB] || near_evb.00333_searchweb.png (320x180) [55.2 KB] || near_evb.00333_thm.png (80x40) [5.5 KB] || Composite (1920x1080) [0 Item(s)] || near_evb_1080p30_2.webm (1920x1080) [72.6 MB] || near_evb_1080p30_2.mp4 (1920x1080) [367.4 MB] || ", "hits": 527 }, { "id": 13421, "url": "https://svs.gsfc.nasa.gov/13421/", "result_type": "Produced Video", "release_date": "2019-12-19T06:55:00-05:00", "title": "Hubble Archive - Servicing Mission 3A, STS-103", "description": "Hubble's third servicing mission, Servicing Mission 3A, launched on December 19, 1999 on Space Shuttle Discovery as part of the STS-103 mission.What was originally conceived as a mission of preventive maintenance turned more urgent on November 13, 1999, when the fourth of six gyros failed and Hubble temporarily closed its eyes on the universe. Unable to conduct science without three working gyros, Hubble entered a state of dormancy called safe mode. Essentially, Hubble \"went to sleep\" while it waited for help.NASA decided to split the Third Servicing Mission (SM3) into two parts, SM3A and SM3B, after the third of Hubble's six gyroscopes failed. In accordance with NASA's flight rules, a \"call-up\" mission was quickly approved and developed and executed in a record 7 months.The Hubble team left the telescope far more fit and capable than ever before. The new, improved, and upgraded equipment included six fresh gyroscopes, six battery voltage/temperature improvement kits, a faster, more powerful, main computer, a next-generation solid state data recorder, a new transmitter, an enhanced fine guidance sensor, and new insulation. || ", "hits": 61 }, { "id": 13502, "url": "https://svs.gsfc.nasa.gov/13502/", "result_type": "Produced Video", "release_date": "2019-12-10T17:00:00-05:00", "title": "AGU 2019 — Postcards from the edge of space: New images, new phenomena, and new insights", "description": "In a Dec. 10 press event at the fall meeting of the American Geophysical Union in San Francisco, California, three scientists presented new images of the ionosphere, the dynamic region where Earth’s atmosphere meets space. Home to astronauts and everyday technology like radio and GPS, the ionosphere constantly responds to changes from space above and Earth below.The collection of images presented include the first images from NASA’s ICON, new science results from NASA’s GOLD, and observations of a fleeting, never-before-studied aurora. Together, they bring color to invisible processes that have widespread implications for the part of space that is closest to home.SPEAKERS:• Jennifer Briggs, Pepperdine University, Malibu, California, United States• Richard Eastes, University of Colorado Boulder, Boulder, Colorado, United States• Thomas Immel, University of California Berkeley, Berkeley, California, United States || ", "hits": 60 }, { "id": 40388, "url": "https://svs.gsfc.nasa.gov/gallery/nasaearth-science/", "result_type": "Gallery", "release_date": "2019-09-13T10:53:37-04:00", "title": "NASA Earth Science", "description": "NASA’s Earth Science Division (ESD) missions help us to understand our planet’s interconnected systems, from a global scale down to minute processes. Working in concert with a satellite network of international partners, ESD can measure precipitation around the world, and it can employ its own constellation of small satellites to look into the eye of a hurricane. ESD technology can track dust storms across continents and mosquito habitats across cities.\n\nFor more information:\nhttps://science.nasa.gov/earth-science", "hits": 230 }, { "id": 13227, "url": "https://svs.gsfc.nasa.gov/13227/", "result_type": "Produced Video", "release_date": "2019-06-12T11:00:00-04:00", "title": "NASA Follows Changing Freshwater from Space", "description": "When we look into the vastness of space, our home planet stands out in many ways. One of the most crucial is the presence of abundant, accessible freshwater -- as a liquid, solid and gas. Water helps make our planet habitable. The first question NASA researchers studying freshwater on Earth ask is: Where is the water? As it constantly cycles between water vapor, rain and snow, and reservoirs above and below ground, water is tracked by a fleet of NASA satellites. Heat travels with that water, as energy from the Sun drives freshwater’s transformations between vapor, liquid water, and ice. As our planet warms due to greenhouse gases, scientists have a second pressing question: How is climate change affecting the distribution of water? || ", "hits": 67 }, { "id": 4714, "url": "https://svs.gsfc.nasa.gov/4714/", "result_type": "Visualization", "release_date": "2019-05-13T11:00:00-04:00", "title": "Lee Lincoln Scarp at the Apollo 17 Landing Site", "description": "An animated view of Lee Lincoln scarp from above and from near ground level. This visualization is created from Lunar Reconnaissance Orbiter photographs and elevation mapping. The scarp is at the western end of the Taurus-Littrow valley, landing site of Apollo 17, and was explored by the astronauts on their second moonwalk. || scarp.0510_print.jpg (1024x576) [101.8 KB] || scarp.0510_searchweb.png (320x180) [63.7 KB] || scarp.0510_thm.png (80x40) [5.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || scarp_1080p30.mp4 (1920x1080) [15.7 MB] || scarp_720p30.mp4 (1280x720) [8.7 MB] || scarp_720p30.webm (1280x720) [3.5 MB] || scarp_1080p30_prores.mov (1920x1080) [657.9 MB] || scarp_360p30.mp4 (640x360) [3.3 MB] || scarp_1080p30.mp4.hwshow || ", "hits": 75 }, { "id": 13078, "url": "https://svs.gsfc.nasa.gov/13078/", "result_type": "Produced Video", "release_date": "2019-04-15T11:00:00-04:00", "title": "Water Released from Moon During Meteor Showers", "description": "Data from the LADEE spacecraft reveal that the lunar surface is periodically releasing water.Music provided by Killer Tracks: Virtual MemoryComplete transcript available. Watch this video on the NASA Goddard YouTube channel. || LADEE_Moon_Earth_Preview_V4_print.jpg (1024x576) [181.9 KB] || LADEE_Moon_Earth_Preview_V4.jpg (1280x720) [281.6 KB] || LADEE_Moon_Earth_Preview_V4_searchweb.png (180x320) [46.5 KB] || LADEE_Moon_Earth_Preview_V4_thm.png (80x40) [3.9 KB] || TWITTER_720_13078_LADEE_Water_Short_MASTER_twitter_720.mp4 (1280x720) [21.1 MB] || 13078_LADEE_Water_Short_MASTER.webm (960x540) [48.9 MB] || YOUTUBE_1080_13078_LADEE_Water_Short_MASTER_youtube_1080.mp4 (1920x1080) [176.0 MB] || FACEBOOK_720_13078_LADEE_Water_Short_MASTER_facebook_720.mp4 (1280x720) [134.7 MB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.srt [2.6 KB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.vtt [2.6 KB] || 13078_LADEE_Water_Short_MASTER.mp4 (3840x2160) [940.5 MB] || 13078_LADEE_Water_Short_MASTER.mov (3840x2160) [5.5 GB] || ", "hits": 82 }, { "id": 30977, "url": "https://svs.gsfc.nasa.gov/30977/", "result_type": "Hyperwall Visual", "release_date": "2019-03-29T00:00:00-04:00", "title": "Nighttime Views of the 2018 Kilauea Eruption", "description": "An animation of Landsat-8 truecolor and nighttime imagery shows the prograssion of the East Rift Zone eruption. || kilauea_2018_east_rift_zone_20180712_print.jpg (1024x576) [70.6 KB] || kilauea_2018_east_rift_zone_20180712.png (3840x2160) [1.8 MB] || kilauea_2018_east_rift_zone_20180712_searchweb.png (320x180) [45.1 KB] || kilauea_2018_east_rift_zone_20180712_thm.png (80x40) [3.8 KB] || kilauea_2018_east_rift_zone_720p.mp4 (1280x720) [2.7 MB] || kilauea_2018_east_rift_zone_720p.webm (1280x720) [1.9 MB] || ", "hits": 217 }, { "id": 4726, "url": "https://svs.gsfc.nasa.gov/4726/", "result_type": "Visualization", "release_date": "2019-03-27T00:00:00-04:00", "title": "New Island forms in Tonga (Updated)", "description": "This visualization shows the evolution Tonga's new island between January 2015 and March 2018. || Tonga_evolutn.1300_print.jpg (1024x576) [129.1 KB] || Tonga_evolutn.1300_searchweb.png (320x180) [84.2 KB] || Tonga_evolutn.1300_web.png (320x180) [84.2 KB] || Tonga_evolutn_Wcredits_1080p30.mp4 (1920x1080) [43.0 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4 (1920x1080) [17.9 MB] || Tonga_evolutn_Wcredits_1080p30.webm (1920x1080) [5.8 MB] || Tonga_evolutn_Wcredits_2160p30_h265.mp4 (3840x2160) [50.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Tonga_evolutn_Wcredits_2160p30.mp4 (3840x2160) [140.4 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4.hwshow || ", "hits": 218 }, { "id": 4708, "url": "https://svs.gsfc.nasa.gov/4708/", "result_type": "Visualization", "release_date": "2019-02-07T00:00:00-05:00", "title": "Moon Sheds Light on Earth's Impact History", "description": "Diviner rock abundance data is overlaid on the lunar globe. Based on this data, the circled craters are less than one billion years old. || ra.0600_print.jpg (1024x576) [110.8 KB] || ra.0600_searchweb.png (320x180) [69.3 KB] || ra.0600_thm.png (80x40) [4.8 KB] || moon_rock_abundance_1080p30.mp4 (1920x1080) [12.4 MB] || moon_rock_abundance_720p30.mp4 (1280x720) [5.2 MB] || ra_comp (1920x1080) [0 Item(s)] || moon_globe (1920x1080) [0 Item(s)] || ra_globe (1920x1080) [0 Item(s)] || moon_rock_abundance_720p30.webm (1280x720) [2.4 MB] || moon_rock_abundance_1080p30.mov (1920x1080) [390.2 MB] || moon_rock_abundance_360p30.mp4 (640x360) [1.5 MB] || moon_rock_abundance_1080p30.mp4.hwshow [193 bytes] || ", "hits": 135 }, { "id": 12166, "url": "https://svs.gsfc.nasa.gov/12166/", "result_type": "Produced Video", "release_date": "2018-12-03T00:00:00-05:00", "title": "OSIRIS-REx Mission Arrives at Asteroid Bennu", "description": "OSIRIS-REx mission team members capture the excitement of arriving at asteroid Bennu. Music provided by Killer Tracks: Distant Echoes, Game Show Sphere 9Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 12166_Bennu_Arrival_Preview_print.jpg (1024x576) [101.3 KB] || 12166_Bennu_Arrival_Preview.jpg (1920x1080) [319.2 KB] || 12166_Bennu_Arrival_Preview_searchweb.png (320x180) [45.2 KB] || 12166_Bennu_Arrival_Preview_thm.png (80x40) [4.1 KB] || FACEBOOK_720_12166_OSIRIS-REx_Arrival_Bennu_MASTER_facebook_720.mp4 (1280x720) [473.9 MB] || TWITTER_720_12166_OSIRIS-REx_Arrival_Bennu_MASTER_twitter_720.mp4 (1280x720) [74.9 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.webm (960x540) [174.0 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.mov (3840x2160) [25.0 GB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER.mp4 (3840x2160) [5.7 GB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small.mp4 (3840x2160) [490.1 MB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small_Output.en_US.srt [11.2 KB] || 12166_OSIRIS-REx_Arrival_Bennu_MASTER_small_Output.en_US.vtt [11.2 KB] || ", "hits": 66 }, { "id": 30996, "url": "https://svs.gsfc.nasa.gov/30996/", "result_type": "Hyperwall Visual", "release_date": "2018-10-03T00:00:00-04:00", "title": "GRACE-FO First Light", "description": "The Gravity Recovery and Climate Experiment Follow-on (GRACE-FO) mission, launched on May 22, 2018 is a successor to the original 2002 GRACE mission, which monitored Earth's gravity by measuring the distance between two satllites following each other in orbit around Earth. In addition to carrying on the original series of measurements made by a microwave ranging system, the GRACE FO mission will test a new laser ranging interferometer, which will provide higher precision distance measurements.These two images show the first data from the Microwave Ranging Instrument and the Laser Ranging Interferometer (LRI) instrument onboard GRACE FO. The raw data for both instruments is a plot of inter-spacecraft distance, which changes as the spacecraft pass over varying mass distribution caused by features on Earth such as large mountain ranges.The Gravity Recovery and Climate Experiment Follow-on (GRACE-FO) mission is a partnership between NASA and the German Research Centre for Geosciences (GFZ). || ", "hits": 29 }, { "id": 30988, "url": "https://svs.gsfc.nasa.gov/30988/", "result_type": "Hyperwall Visual", "release_date": "2018-08-29T00:00:00-04:00", "title": "Earth System Diagram", "description": "Diagram showing parts of the Earth system. || earth_system_diagram_print.jpg (1024x574) [115.6 KB] || earth_system_diagram.png (4104x2304) [1.2 MB] || earth_system_diagram_searchweb.png (320x180) [63.5 KB] || earth_system_diagram_thm.png (80x40) [6.6 KB] || earth_system_diagram.hwshow [208 bytes] || ", "hits": 515 }, { "id": 4670, "url": "https://svs.gsfc.nasa.gov/4670/", "result_type": "Visualization", "release_date": "2018-08-01T09:00:00-04:00", "title": "Geothermal Heat Flux Reveals the Iceland Hotspot Track underneath Greenland", "description": "This visualization shows the Greenland geothermal heat flux map, the track of the Iceland hotspot through Greenland, and the plate tectonic motion of Greenland over the hotspot during the past 100 million years.This video is also on the NASA YouTube channel. || hotspot.0240_print.jpg (1024x576) [157.4 KB] || hotspot.0240_searchweb.png (320x180) [100.2 KB] || hotspot.0240_thm.png (80x40) [7.9 KB] || hotspot_1080p30.mp4 (1920x1080) [17.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || hotspot_720p30.mp4 (1280x720) [8.7 MB] || hotspot_720p30.webm (1280x720) [3.0 MB] || hotspot_360p30.mp4 (640x360) [3.4 MB] || hotspot_1080p30.mp4.hwshow [181 bytes] || ", "hits": 158 }, { "id": 13025, "url": "https://svs.gsfc.nasa.gov/13025/", "result_type": "Produced Video", "release_date": "2018-08-01T09:00:00-04:00", "title": "NASA Scientist Reveals Greenland's Geologic Past", "description": "A new map of Greenland's geothermal heat flux is helping to reveal the path of the North American tectonic plate over geologic time. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks: \"Valfri\" by James Alexander Dorman || FACEBOOK_720_13025_Greenland_Hotspot_MASTER_facebook_720.mp4 (1280x720) [173.9 MB] || Greenland_Tectonic_Preview_print.jpg (1024x576) [383.0 KB] || Greenland_Tectonic_Preview.jpg (3840x2160) [3.0 MB] || Greenland_Tectonic_Preview_searchweb.png (320x180) [136.6 KB] || Greenland_Tectonic_Preview_thm.png (80x40) [8.8 KB] || TWITTER_720_13025_Greenland_Hotspot_MASTER_twitter_720.mp4 (1280x720) [28.6 MB] || 13025_Greenland_Hotspot_MASTER.webm (960x540) [53.0 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080.mp4 (1920x1080) [228.2 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.srt [2.5 KB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.vtt [2.5 KB] || YOUTUBE_4K_13025_Greenland_Hotspot_MASTER_youtube_4k.mp4 (3840x2160) [543.3 MB] || 13025_Greenland_Hotspot_MASTER_youtube_hq.mov (3840x2160) [1.3 GB] || 13025_Greenland_Hotspot_MASTER.mov (3840x2160) [6.3 GB] || ", "hits": 72 }, { "id": 4635, "url": "https://svs.gsfc.nasa.gov/4635/", "result_type": "Visualization", "release_date": "2018-06-15T11:00:00-04:00", "title": "Visualizations of Hunga Tonga Hunga Ha'apai and the Martian Landscape", "description": "In early 2015, a volcanic eruption in the Kingdom of Tonga created a new island informally known as Hunga Tonga Hunga Ha'apai (HTHH). The subsequent evolution of the new island was previously described in \"The Birth of a New Island\" available here. Below are additional visualizations, including an updated view of the island's appearance in March 2018 as well as some visualizations of the martian surface. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.The complete visualization of \"Using Earth to understand how water may have affected volcanoes on Mars\" is available here.Learn more about the evolution of Earth's newest island and how it could reveal new information about the presence of water on Mars: https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL076621 || ", "hits": 51 }, { "id": 30962, "url": "https://svs.gsfc.nasa.gov/30962/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Sulfur Dioxide Leaks from Kilauea", "description": "This series of images, created using data from the Ozone Mapping Profiler Suite (OMPS) sensor on the Suomi National Polar-orbiting Partnership (NPP) satellite, shows elevated concentrations of sulfur dioxide from Hawaii's Kilauea volcano on May 5, 2018. || hawaii_omp_so2.png (1920x1080) [299.9 KB] || hawaii_omp_so2_print.jpg (1024x576) [49.1 KB] || hawaii_omp_so2_searchweb.png (320x180) [31.7 KB] || hawaii_omp_so2_thm.png (80x40) [3.7 KB] || sulfur-dioxide-leaks-from-kilauea-data.hwshow [290 bytes] || ", "hits": 47 }, { "id": 30964, "url": "https://svs.gsfc.nasa.gov/30964/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Kilauea Continues to Erupt", "description": "On May 14, 2018, at 10:41 AM local time (20:41 Universal Time), the Operational Land Imager (OLI) on Landsat 8 acquired a natural-color image of Hawaii’s Kilauea volcano. || kilauea_continues_print.jpg (1024x682) [280.7 KB] || kilauea_continues.png (4860x3240) [26.3 MB] || kilauea_continues_searchweb.png (320x180) [123.7 KB] || kilauea_continues_thm.png (80x40) [8.0 KB] || kilauea-continues-to-erupt.hwshow [284 bytes] || ", "hits": 70 }, { "id": 30965, "url": "https://svs.gsfc.nasa.gov/30965/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "The Infrared Glow of Kilauea’s Lava Flows", "description": "The Operational Land Imager (OLI) on Landsat 8 acquired the data for this false-color view of the lava flow as it appeared on the night of May 23, 2018. || IR_leilani_print.jpg (1024x574) [95.3 KB] || IR_leilani.png (4104x2304) [3.5 MB] || IR_leilani_searchweb.png (320x180) [44.9 KB] || IR_leilani_thm.png (80x40) [2.7 KB] || the-infrared-glow-of-kilaueas-lava-flows.hwshow [284 bytes] || ", "hits": 43 }, { "id": 30973, "url": "https://svs.gsfc.nasa.gov/30973/", "result_type": "Hyperwall Visual", "release_date": "2018-05-27T00:00:00-04:00", "title": "Aoba (Ambae) Volcano Eruption, Vanuatu", "description": "Activity for Aoba (Ambae) volcano has increased in recent months and is now in a minor eruption state. A restricted area of risk which is 3km around the active vent has been established as the volcano began to become more active in March and early April 2018. At that time the volcano began to emit more and sustained volcanic ash or/ and gases. Vanuatu’s Council of Ministers has declared a state of emergency on Ambae due to the heavy ash fall which has contaminated water and food supplies for the island’s nearly 11,000 inhabitants, who are in the process of being evacuated from the island. || ", "hits": 46 }, { "id": 12784, "url": "https://svs.gsfc.nasa.gov/12784/", "result_type": "Produced Video", "release_date": "2018-05-21T12:00:00-04:00", "title": "Martian Clues on a Baby Island", "description": "A young volcanic island on Earth may hold clues to former islands on Mars. || Tonga_v60_vis.0780_16x9.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_16x9_print.jpg (1024x576) [123.6 KB] || Tonga_v60_vis.0780_16x9_searchweb.png (320x180) [96.3 KB] || Tonga_v60_vis.0780_16x9_thm.png (80x40) [7.7 KB] || ", "hits": 27 }, { "id": 12880, "url": "https://svs.gsfc.nasa.gov/12880/", "result_type": "Produced Video", "release_date": "2018-03-05T00:00:00-05:00", "title": "Cosmic Designs and The Planets", "description": "Greetings and welcome to “Cosmic Designs” a performance by the National Philharmonic presented in partnership with NASA’s Goddard Space Flight Center.“Cosmic Designs” is a voyage that blends together science and art. The pursuit of knowledge and the creative drive for artistic expression are inherent to the human condition. The melding of NASA imagery and symphonic music we present here showcases the imagination that underpins both and highlights how inspiring the combination can be. || CD_Intro_Image_print.jpg (1024x567) [135.2 KB] || CD_Intro_Image.png (2918x1618) [5.8 MB] || CD_Intro_Image_searchweb.png (320x180) [103.7 KB] || CD_Intro_Image_web.png (320x177) [101.8 KB] || CD_Intro_Image_thm.png (80x40) [7.6 KB] || 1.CosmicDesigns_Title_1080.mov (1920x1080) [1.0 GB] || 1.CosmicDesigns_Title_1080.mp4 (1920x1080) [35.9 MB] || 1.CosmicDesigns_Title_1080.webm (1920x1080) [3.3 MB] || 1.CosmicDesigns_Title_4K.mov (3840x2160) [4.3 GB] || 1.CosmicDesigns_Title_4K.mp4 (3840x2160) [55.1 MB] || ", "hits": 176 }, { "id": 12861, "url": "https://svs.gsfc.nasa.gov/12861/", "result_type": "Produced Video", "release_date": "2018-02-14T09:00:00-05:00", "title": "NASA Valentines", "description": "Download our collection of valentines, featuring science visualizations and imagery from NASA missions.Want more NASA valentines? Visit https://mars.nasa.gov/free-holiday-ecard/love-valentine/#Send-A-Card ||", "hits": 135 }, { "id": 4602, "url": "https://svs.gsfc.nasa.gov/4602/", "result_type": "Visualization", "release_date": "2017-12-11T10:00:00-05:00", "title": "New island forms in Tonga", "description": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel. || Tonga_v60_vis.0780_print.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_searchweb.png (320x180) [76.8 KB] || Tonga_v60_vis.0780_thm.png (80x40) [6.0 KB] || new_island_vis (1920x1080) [0 Item(s)] || Tonga_v60_vis_1080p30.mp4 (1920x1080) [33.3 MB] || Tonga_v60_vis_1080p30.webm (1920x1080) [5.1 MB] || Tonga_4k_final2_1080p30.mp4 (1920x1080) [34.3 MB] || new_island_vis (3840x2160) [0 Item(s)] || Tonga_4k_final2_2160p30.mp4 (3840x2160) [52.0 MB] || Tonga_v60_vis_1080p30.mp4.hwshow [187 bytes] || ", "hits": 75 }, { "id": 30910, "url": "https://svs.gsfc.nasa.gov/30910/", "result_type": "Hyperwall Visual", "release_date": "2017-11-13T00:00:00-05:00", "title": "Simulation of Aerosols During the 2017 North Atlantic Hurricane Season", "description": "This animation shows the effects of hurricanes on dust, smoke, and sea salt. || plot_aerosols-northamerica_F517R06K-GEOS_06KM-REPLAY-20170915_1200_print.jpg (1024x567) [160.5 KB] || plot_aerosols-northamerica_F517R06K-GEOS_06KM-REPLAY-20170915_1200.png (5760x3190) [18.1 MB] || plot_aerosols-northamerica_F517R06K-GEOS_06KM-REPLAY-20170915_1200_searchweb.png (320x180) [108.2 KB] || plot_aerosols-northamerica_F517R06K-GEOS_06KM-REPLAY-20170915_1200_thm.png (80x40) [8.2 KB] || plot_aerosols-northamerica_720p.webm (1280x720) [35.3 MB] || plot_aerosols-northamerica_720p.mp4 (1280x720) [191.7 MB] || plot_aerosols-northamerica_1080p.mp4 (1920x1080) [369.7 MB] || ", "hits": 44 }, { "id": 3458, "url": "https://svs.gsfc.nasa.gov/3458/", "result_type": "Visualization", "release_date": "2017-10-01T00:00:00-04:00", "title": "Destination Asteroid", "description": "Not far from Earth, dark bodies of rock circle the sun in lonely orbits. These near Earth objects, or NEOs, are asteroids found outside the traditional belt between Mars and Jupiter. Protected from the gravitational tugs and tumbles that affect objects found closer to the gas giant, these asteroids may contain clues about the origins of the solar system. That's why experts from NASA and The University of Arizona want to send a research vehicle to collect a sample. That's OSIRIS. Once approved, the OSIRIS vehicle would leave Earth on a multi-year mission to map and collect samples from a particular NEO called RQ-36.In DESTINATION: ASTEROID, we look behind the scenes as a team of government scientists demonstrates for a visiting group of reporters how the mission will work. This short film explores the basics of the mission, including scientific goals, technical design plans, and a timeline of planned events. Imagination and invention meet in this spirited paean to NASA's legacy for great feats of exploration and discovery. Join us as we set our navigation systems to DESTINATION: ASTEROID. || ", "hits": 39 }, { "id": 4560, "url": "https://svs.gsfc.nasa.gov/4560/", "result_type": "Visualization", "release_date": "2017-03-31T09:00:00-04:00", "title": "Alfvén Waves - Basic", "description": "Alfven waves represented by undulation in the magnetic field vector. || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_print.jpg (1024x576) [158.5 KB] || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_thm.png (80x40) [4.6 KB] || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_web.png (320x180) [71.9 KB] || WavesOnly (1920x1080) [128.0 KB] || AlfvenWaveBasic_staticXwide.HD1080i_p30.mp4 (1920x1080) [34.0 MB] || AlfvenWaveBasic_staticXwide.HD1080i_p30.webm (1920x1080) [4.9 MB] || ", "hits": 476 }, { "id": 4561, "url": "https://svs.gsfc.nasa.gov/4561/", "result_type": "Visualization", "release_date": "2017-03-31T09:00:00-04:00", "title": "Alfvén Waves - Kinetic", "description": "Kinetic Alfven waves represented by undulation in the magnetic field vector. || AlfvenWaveKinetic_staticXwide_inertial.HD1080i.0300_print.jpg (1024x576) [155.7 KB] || WavesOnly (1920x1080) [128.0 KB] || AlfvenWaveKinetic_staticXwide.HD1080i_p30.mp4 (1920x1080) [37.9 MB] || AlfvenWaveKinetic_staticXwide.HD1080i_p30.webm (1920x1080) [4.9 MB] || ", "hits": 157 }, { "id": 40323, "url": "https://svs.gsfc.nasa.gov/gallery/applied-science/", "result_type": "Gallery", "release_date": "2017-03-30T00:00:00-04:00", "title": "Applied Science", "description": "Discovering innovative and practical uses of Earth observations\n\nappliedsciences.nasa.gov", "hits": 62 }, { "id": 4555, "url": "https://svs.gsfc.nasa.gov/4555/", "result_type": "Visualization", "release_date": "2017-02-23T00:00:00-05:00", "title": "California Gets Slammed Again", "description": "California has been experiencing a drought since 2012, but the first months of 2017 have brought some relief in the form of torrential rains. These rains have been brought to California in a series of atmospheric rivers, long narrow channels of water vapor in the atmosphere that reach from tropical latitudes to the coast of California. These channels bring rainfall to the state when they are disrupted by atmospheric conditions over California's eastern mountains. This visualization of atmospheric water vapor and precipitation during the first three weeks of February clearly show the successive atmospheric rivers and the resulting rainfall. || ", "hits": 26 }, { "id": 12425, "url": "https://svs.gsfc.nasa.gov/12425/", "result_type": "Produced Video", "release_date": "2016-12-15T13:00:00-05:00", "title": "Microlensing Study: Most Common Outer Planets Likely Neptune-mass", "description": "A new statistical study of planets found by the gravitational microlensing technique suggests that Neptune-mass planets may be the most common worlds in the outer reaches of planetary systems. Credit: NASA's Goddard Space Flight CenterMusic: \"Hurricanes Wrap My Heart\" from Stockmusic.netWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MOA_II_Still_print.jpg (1024x576) [117.4 KB] || MOA_II_Still.png (3356x1888) [8.3 MB] || 12425_Microlensing_Neptunes_ProRes_1920x1080_2997.mov (1920x1080) [3.3 GB] || 12425_Microlensing_Neptunes_FINAL_youtube_hq.mov (1920x1080) [821.9 MB] || 12425_Microlensing_Neptunes_H264_Good_1080.mov (1920x1080) [369.1 MB] || 12425_Microlensing_Neptunes_FINAL_HD.wmv (1920x1080) [167.7 MB] || 12425_Microlensing_Neptunes_H264_1080.m4v (1920x1080) [246.3 MB] || 12425_Microlensing_Neptunes_FINAL_appletv.m4v (1280x720) [124.2 MB] || 12425_Microlensing_Neptunes_Compatible_540.m4v (960x540) [94.7 MB] || 12425_Microlensing_Neptunes_ProRes_1920x1080_2997.webm (1920x1080) [24.6 MB] || 12425_Microlensing_Neptunes_FINAL_appletv_subtitles.m4v (1280x720) [124.4 MB] || Microlensing_Neptunes_SRT_Captions.en_US.srt [4.5 KB] || Microlensing_Neptunes_SRT_Captions.en_US.vtt [4.5 KB] || 12425_Microlensing_Neptunes_FINAL_ipod_sm.mp4 (320x240) [42.6 MB] || ", "hits": 155 }, { "id": 12456, "url": "https://svs.gsfc.nasa.gov/12456/", "result_type": "Produced Video", "release_date": "2016-12-12T18:45:00-05:00", "title": "Tracking Ocean Heat With Magnetic Fields", "description": "As Earth warms, much of the extra heat is stored in the planet’s ocean – but monitoring the magnitude of that heat content is a difficult task. A surprising feature of the tides could help, however. Scientists at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, are developing a new way to use satellite observations of magnetic fields to measure heat stored in the ocean.Music: War Torn by Brad Smith [BMI] Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12456-ocean-heat-AGU-web.jpg (1920x1080) [354.1 KB] || 12456-ocean-heat-AGU-web_searchweb.png (320x180) [122.0 KB] || 12456-ocean-heat-AGU-web_thm.png (80x40) [7.7 KB] || 12456-ocean-heat-APR_VX-680579_large.mp4 (1920x1080) [59.1 MB] || 12456-ocean-heat-APR_VX-680579_appletv.m4v (1280x720) [30.6 MB] || 12456-ocean-heat-AGU-720p.mp4 (1280x720) [59.5 MB] || 12456-ocean-heat-AGU.mp4 (1920x1080) [59.9 MB] || 12456-ocean-heat-APR_VX-680579.webm (960x540) [23.6 MB] || 12456-ocean-heat-APR_VX-680579_appletv_subtitles.m4v (1280x720) [30.7 MB] || 12456-ocean-heat-captions.en_US.srt [891 bytes] || 12456-ocean-heat-captions.en_US.vtt [904 bytes] || 12456-ocean-heat-APR_VX-680579_ipod_sm.mp4 (320x240) [10.9 MB] || 12456-ocean-heat-APR_VX-680579_prores.mov (1280x720) [791.2 MB] || 12456-ocean-heat-APR_VX-680579_youtube_hq.mov (1920x1080) [212.0 MB] || 12456-ocean-heat-APR_VX-680579.mpeg (1280x720) [196.6 MB] || ", "hits": 26 }, { "id": 12450, "url": "https://svs.gsfc.nasa.gov/12450/", "result_type": "Produced Video", "release_date": "2016-12-12T18:30:00-05:00", "title": "Ocean Tides and Magnetic Fields", "description": "Seawater is an electrical conductor, and therefore interacts with the magnetic field. As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along.Because the salty water is a good, but not great, conductor, the interaction is relatively weak. Scientists at NASA Goddard Space Flight Center are developing improved methods to isolate the signal from ocean tides and use that information to determine the heat content of the ocean.Music: \"Memory Of A Lifetime\" by J Ehrlich [SESAC], Jean-Christophe Beck [BMI]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12450-Tidal-Magnetic-Animation-APR_large.00545_print.jpg (1024x576) [189.1 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_searchweb.png (320x180) [93.6 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_thm.png (80x40) [5.8 KB] || 12450-Tidal-Magnetic-Animation-APR.webm (960x540) [26.5 MB] || 12450-Tidal-Magnetic-Animation-APR_prores.mov (1280x720) [989.0 MB] || 12450-Tidal-Magnetic-Animation-APR_large.mp4 (1920x1080) [66.1 MB] || 12450-Tidal-Magnetic-Animation-APR_youtube_hq.mov (1920x1080) [1.0 GB] || 12450-Tidal-Magnetic-Animation-APR_appletv.m4v (1280x720) [32.1 MB] || 12450-Tidal-Magnetic-Animation-APR_appletv_subtitles.m4v (1280x720) [32.2 MB] || 1920x1080_16x9_30p (1920x1080) [128.0 KB] || 12450-Tidal-Magnetic-Animation.en_US.srt [1.4 KB] || 12450-Tidal-Magnetic-Animation.en_US.vtt [1.4 KB] || 12450-Tidal-Magnetic-Animation-APR_ipod_sm.mp4 (320x240) [11.5 MB] || ", "hits": 424 }, { "id": 4505, "url": "https://svs.gsfc.nasa.gov/4505/", "result_type": "Visualization", "release_date": "2016-10-13T00:01:00-04:00", "title": "Gardening Rates on the Moon", "description": "After simulating the distant view of a new impact, the camera zooms up to the surface to show actual before/after images of a new 12-meter crater taken by the Lunar Reconnaissance Orbiter narrow-angle camera. (The impact that formed this crater wasn't seen from Earth, but a different one was.) || new_crater.0900_print.jpg (1024x576) [183.2 KB] || new_crater.0900_searchweb.png (320x180) [66.2 KB] || new_crater.0900_thm.png (80x40) [3.5 KB] || new_crater_1080p30.mp4 (1920x1080) [17.9 MB] || new_crater_720p30.mp4 (1280x720) [9.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || new_crater_720p30.webm (1280x720) [2.9 MB] || new_crater_360p30.mp4 (640x360) [3.0 MB] || new_crater_4505.key [19.1 MB] || new_crater_4505.pptx [18.8 MB] || gardening-moon-mp4.hwshow [204 bytes] || ", "hits": 230 }, { "id": 12716, "url": "https://svs.gsfc.nasa.gov/12716/", "result_type": "B-Roll", "release_date": "2016-09-08T20:30:00-04:00", "title": "OSIRIS-REx Launch Footage", "description": "On September 8, 2016, NASA's OSIRIS-REx spacecraft began its journey to near-Earth asteroid Bennu. Just as the sun began to set over Cape Canaveral, OSIRIS-REx made a picture-perfect liftoff at 7:05 pm EDT. It departed Space Launch Complex 41 aboard a United Launch Alliance Atlas V 411 rocket, cheered on by crowds of mission personnel and space enthusiasts. The launch sent OSIRIS-REx on a seven-year journey to asteroid Bennu and back.An excerpt of the launch broadcast appears at the top of this page. Raw camera feeds from Cape Canaveral and Kennedy Space Center appear below. These clips are intended as a video editor's resource, and are available for download in their original DVCPRO HD format. Launch commentary is provided by KSC host Mike Curie.Learn more about OSIRIS-REx from NASA and the University of Arizona. || ", "hits": 205 }, { "id": 20253, "url": "https://svs.gsfc.nasa.gov/20253/", "result_type": "Animation", "release_date": "2016-08-17T14:00:00-04:00", "title": "OSIRIS-REx Launch and Deployment Animations", "description": "OSIRIS-REx begins its journey to near-Earth asteroid Bennu from Space Launch Complex 41 on Cape Canaveral, aboard a United Launch Alliance Atlas V rocket. In addition to the launch vehicle's liquid-fueled main engine, its 411 configuration includes a strap-on solid rocket booster and a Centaur upper stage. When the launch window opens on the evening of September 8, 2016, the Atlas V will lift OSIRIS-REx above the Florida coastline and propel it eastward over the night side of Earth. Fifty-nine minutes later, OSIRIS-REx will separate from the Centaur upper stage, point its solar arrays at the rising sun, and embark on its nearly two-year cruise to Bennu. || ", "hits": 57 }, { "id": 12339, "url": "https://svs.gsfc.nasa.gov/12339/", "result_type": "Animation", "release_date": "2016-08-17T02:00:00-04:00", "title": "OSIRIS-REx L-14 Press Briefing Graphics", "description": "OSIRIS-REx is on a mission to study asteroid Bennu and return a sample to Earth. The graphics on this page were created to support the OSIRIS-REx L-14 press briefing at NASA headquarters on August 17, 2016. All videos are available for download in broadcast quality. The majority of the videos do not contain audio. Links to 4K-resolution versions appear at the bottom of the page.Watch the OSIRIS-REx L-14 press conference.Learn more about OSIRIS-REx from NASA and the University of Arizona. || ", "hits": 29 }, { "id": 4480, "url": "https://svs.gsfc.nasa.gov/4480/", "result_type": "Visualization", "release_date": "2016-08-15T14:00:00-04:00", "title": "Prompt Electron Acceleration in the Radiation Belts", "description": "Electrons gyrating along the lines of Earth's magnetic field make another orbit around Earth and strike the Van Allen Probe A AGAIN! || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_print.jpg (1024x576) [139.2 KB] || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_searchweb.png (320x180) [90.9 KB] || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_thm.png (80x40) [6.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || PromptAccel.HD1080i_p30.mp4 (1920x1080) [48.5 MB] || PromptAccel.HD1080i_p30.webm (1920x1080) [3.1 MB] || PromptAccel_EventCloseup_SlowOblique.HD1080i_720p30.mp4 (1280x720) [24.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || PromptAccel_EventCloseup_SlowOblique_2160p30.mp4 (3840x2160) [141.9 MB] || PromptAccel.HD1080i_p30.mp4.hwshow [189 bytes] || ", "hits": 222 }, { "id": 12302, "url": "https://svs.gsfc.nasa.gov/12302/", "result_type": "Produced Video", "release_date": "2016-07-13T00:00:00-04:00", "title": "Aerosol Optical Thickness, MODIS, 2000-2016", "description": "Aerosol optical depth from Terra/MODIS, 1-month composite.In the maps shown here, dark brown pixels show high aerosol concentrations, while tan pixels show lower concentrations, and light yellow areas show little or no aerosols. Black shows where the sensor could not make its measurement.Aerosol optical depth is the degree to which aerosols prevent the transmission of light by absorption or scattering of light. || MODIS_Aerosol_Optical_Depth_youtube_hq.00001_print.jpg (1024x512) [184.9 KB] || MODIS_Aerosol_Optical_Depth_youtube_hq.00001_searchweb.png (320x180) [92.7 KB] || MODIS_Aerosol_Optical_Depth_youtube_hq.00001_thm.png (80x40) [6.7 KB] || MODIS_Aerosol_Optical_Depth.webm (960x540) [42.2 MB] || 3600x1800_2x1_30p (3600x1800) [16.0 KB] || GSFC_20160713_MODIS_m12302_Aerosol.en_US.vtt [64 bytes] || MODIS_Aerosol_Optical_Depth_large.mp4 (3600x1800) [233.1 MB] || MODIS_Aerosol_Optical_Depth_youtube_hq.mov (3600x1800) [511.0 MB] || MODIS_Aerosol_Optical_Depth_prores720.mov (1280x720) [1.7 GB] || MODIS_Aerosol_Optical_Depth_prores.mov (3600x1800) [11.1 GB] || ", "hits": 199 }, { "id": 12291, "url": "https://svs.gsfc.nasa.gov/12291/", "result_type": "Produced Video", "release_date": "2016-06-28T11:00:00-04:00", "title": "Mission Juno", "description": "A NASA spacecraft en route to Jupiter will study the origin of the solar system’s largest planet. || cf-1024.jpg (1024x576) [149.3 KB] || cf-1024_print.jpg (1024x576) [155.4 KB] || cf-1024_searchweb.png (320x180) [87.4 KB] || cf-1024_web.png (320x180) [87.4 KB] || cf-1024_thm.png (80x40) [20.1 KB] || ", "hits": 74 }, { "id": 30730, "url": "https://svs.gsfc.nasa.gov/30730/", "result_type": "Hyperwall Visual", "release_date": "2015-12-16T12:00:00-05:00", "title": "High-Resolution Soil Moisture Maps", "description": "These maps combine data from the twin satellites of the Gravity Recovery and Climate Experiment (GRACE) with other satellite and ground-based measurements to model the relative amount of water stored at two different levels: at plant root level and underground. The wetness, or water content, of each layer is compared to the average between 1948 and 2009. The darkest red regions represent dry conditions that should occur only 2 percent of the time (about once every 50 years). All of the maps are experimental products funded by NASA’s Applied Sciences Program and developed by scientists at NASA’s Goddard Space Flight Center and the National Drought Mitigation Center. The maps do not attempt to represent human consumption of water; but rather, they show changes in water storage related to weather, climate, and seasonal patterns. || ", "hits": 105 }, { "id": 4376, "url": "https://svs.gsfc.nasa.gov/4376/", "result_type": "Visualization", "release_date": "2015-10-27T00:00:00-04:00", "title": "Antarctic Mass Change from GRACE derived Gravity Observations: Jan 2004 - Jun 2014", "description": "GRACE, NASA's Gravity Recovery and Climate Experiment, consists of twin co-orbiting satellites that fly in a near polar orbit separated by a distance of 220 km. GRACE precisely measures the distance between the two spacecraft in order to make detailed measurements of the Earth's gravitational field. Since its launch in 2002, GRACE has provided a continuous record of changes in the mass of the Earth's ice sheets.These animations show the change in the mass of the Antarctic Ice Sheet between January 2004 and June 2014 as measured by the pair of GRACE satellites. The 1-arc-deg NASA GSFC mascon solution data was resampled to a 5130 x 5130 data array using Kriging interpolation. A color scale was applied where blue values indicate an increase in the ice sheet mass while red shades indicate a decrease. In addition, a graph overlay shows the running total of the accumulated mass change in gigatons.Four separate animations are shown here: one of the full Antarctic Ice Sheet (above) and three of individual regional views (below) showing the regions of West Antarctica, the Antarctic Peninsula and East Antarctica. The time-series of each region is shown with a graph depicting the ice loss for the region alone. Note that the range on the color scale is different for each regional view in order to portray the most detail possible. Areas outside the region being shown are colored in a pale green to indicate that it is not included in the view. The floating ice shelves, shown in a lighter shade of green, are also not included.Technical Note: The glacial isostatic adjustment signal (Earth mass redistribution in response to historical ice loading) has been removed using the ICE-6G model (Peltier et al. 2015). || ", "hits": 32 }, { "id": 4325, "url": "https://svs.gsfc.nasa.gov/4325/", "result_type": "Visualization", "release_date": "2015-08-26T10:00:00-04:00", "title": "NASA GSFC MASCON Solution over Greenland from Jan 2004 - Jun 2014", "description": "Visualization of the mass change over Greenland from January 2004 through June 2014. The surface of Greenland shows the change in equivalent water height while the graph overlay shows the total accumulated change in gigatons. || GRACE_Greenland_wGraph_p30.1322_print.jpg (1024x576) [138.2 KB] || GRACE_Greenland_wGraph_p30.1322_searchweb.png (180x320) [84.6 KB] || GRACE_Greenland_wGraph_p30.1322_thm.png (80x40) [7.0 KB] || GRACE_Greenland_wGraph_p30_720p.webm (1280x720) [2.5 MB] || GRACE_Greenland_wGraph_p30_1080p.webm (1920x1080) [2.9 MB] || GRACE_Greenland_wGraph_p30_1080p.mp4 (1920x1080) [16.9 MB] || GRACE_Greenland_wGraph_p30_720p.mp4 (1280x720) [9.4 MB] || composite (1920x1080) [0 Item(s)] || composite (1920x1080) [0 Item(s)] || GRACE_Greenland_wGraph_p30_360p.mp4 (640x360) [3.4 MB] || MASCON_solution_greenland_4325.key [12.7 MB] || MASCON_solution_greenland_4325.pptx [10.1 MB] || ", "hits": 31 }, { "id": 4347, "url": "https://svs.gsfc.nasa.gov/4347/", "result_type": "Visualization", "release_date": "2015-08-26T10:00:00-04:00", "title": "NASA GSFC MASCON Solution over Antarctica from Jan 2004 - Jun 2014", "description": "Visualization of the mass change over the Antarctic Ice Sheet from January 2004 through June 2014. The color on the surface of the ice sheet shows the change in equivalent water height while the graph overlay shows the total accumulated change in gigatons. || GRACE_Antarctic_Wgraph_p30.2521_print.jpg (1024x576) [110.0 KB] || GRACE_Antarctic_Wgraph_p30.2521_searchweb.png (320x180) [71.0 KB] || GRACE_Antarctic_Wgraph_p30.2521_thm.png (80x40) [6.3 KB] || GRACE_Antarctic_Wgraph_p30_1080p.mp4 (1920x1080) [18.2 MB] || GRACE_Antarctic_Wgraph_p30_1080p.webm (1920x1080) [7.7 MB] || GRACE_Antarctic_Wgraph_p30_720p.mp4 (1280x720) [10.4 MB] || GRACE_Antarctic_Wgraph_p30_720p.webm (1280x720) [8.7 MB] || composite (1920x1080) [256.0 KB] || composite (1920x1080) [512.0 KB] || GRACE_Antarctic_Wgraph_p30_360p.mp4 (640x360) [3.8 MB] || MASCON_solution_antartica_4347.pptx [11.0 MB] || MASCON_solution_antartica_4347.key [13.6 MB] || ", "hits": 40 }, { "id": 11910, "url": "https://svs.gsfc.nasa.gov/11910/", "result_type": "Produced Video", "release_date": "2015-06-30T10:00:00-04:00", "title": "Studying an Asteroid on Earth", "description": "Project Scientist Jason Dworkin discusses the OSIRIS-REx mission to explore asteroid Bennu and return a sample to Earth.View transcript.Watch this video on the NASAexplorer YouTube channel. || OSIRIS_REx_Blue_Marble.png (1920x1080) [2.0 MB] || OSIRIS_REx_Blue_Marble_print.jpg (1024x576) [118.5 KB] || OSIRIS_REx_Blue_Marble_searchweb.png (320x180) [84.3 KB] || OSIRIS_REx_Blue_Marble_thm.png (80x40) [8.3 KB] || G2015-008_OREx_Astro_MASTER.mov (1280x720) [2.4 GB] || G2015-008_OREx_Astro_MASTER_youtube_hq.mov (1280x720) [118.8 MB] || G2015-008_OREx_Astro_MASTER_youtube_hq.webm (1280x720) [19.5 MB] || G2015-008_OREx_Astro_MASTER_appletv.m4v (960x540) [74.2 MB] || G2015-008_OREx_Astro_MASTER_1280x720.wmv (1280x720) [80.5 MB] || G2015-008_OREx_Astro_MASTER_appletv_subtitles.m4v (960x540) [74.1 MB] || G2015-008_OREx_Astro_MASTER_ipod_lg.m4v (640x360) [29.4 MB] || G2015-008_OREx_Astro_MASTER_youtube_hq.en_US.srt [3.2 KB] || G2015-008_OREx_Astro_MASTER_youtube_hq.en_US.vtt [3.2 KB] || G2015-008_OREx_Astro_MASTER_ipod_sm.mp4 (320x240) [15.8 MB] || ", "hits": 41 }, { "id": 4242, "url": "https://svs.gsfc.nasa.gov/4242/", "result_type": "Visualization", "release_date": "2015-03-17T14:00:00-04:00", "title": "March 17, 2013 Lunar Impact Forms a New Crater", "description": "Artist's conception of the March 17, 2013 lunar impact as seen from near the impact site in Mare Imbrium.This video is also available on our YouTube channel. || impactb.0172_print.jpg (1024x576) [43.7 KB] || impactb.0172_searchweb.png (320x180) [39.8 KB] || impactb.0172_thm.png (80x40) [3.6 KB] || from_moon_720p30.webmhd.webm (960x540) [249.9 KB] || from_moon_1080p30.mp4 (1920x1080) [629.5 KB] || from_moon_720p30.mp4 (1280x720) [298.3 KB] || from_moon (1920x1080) [0 Item(s)] || from_moon_360p30.mp4 (640x360) [100.4 KB] || from_moon_4242.key [2.8 MB] || from_moon_4242.pptx [390.9 KB] || ", "hits": 207 }, { "id": 40415, "url": "https://svs.gsfc.nasa.gov/gallery/whats-newwith-earth-today/", "result_type": "Gallery", "release_date": "2015-01-04T00:00:00-05:00", "title": "What's New with Earth Today", "description": "Explore the latest visualizations of NASA's Earth Observing satellites and the data they collect. NASA researchers are constantly tracking remote-sensing data and modeling processes to better understand our home planet.", "hits": 194 }, { "id": 30591, "url": "https://svs.gsfc.nasa.gov/30591/", "result_type": "Hyperwall Visual", "release_date": "2014-12-10T10:00:00-05:00", "title": "Simulated Clouds and Aerosols", "description": "GEOS-5 Model Visible || visible_1080_print.jpg (1024x576) [207.1 KB] || visible_1080_searchweb.png (180x320) [102.7 KB] || visible_1080_web.png (320x180) [102.7 KB] || visible_1080_thm.png (80x40) [7.7 KB] || visible (1920x1080) [0 Item(s)] || visible_1080.webm (1920x1080) [28.9 MB] || geos_visible_720p.mp4 (1280x720) [285.3 MB] || visible_1080.mp4 (1920x1080) [423.8 MB] || geos_visible_1080p.mp4 (1920x1080) [572.6 MB] || visible (5760x2881) [0 Item(s)] || geos_visible_2160p.mp4 (3840x2160) [1.8 GB] || ", "hits": 73 }, { "id": 10183, "url": "https://svs.gsfc.nasa.gov/10183/", "result_type": "Produced Video", "release_date": "2014-11-13T13:00:00-05:00", "title": "How Do Active Volcanoes Change Clouds?", "description": "NASA Goddard Space Flight Center scientist Andrew Sayer talks about how emissions from volcanoes can affect clouds.This video provides an overview of research published in the Journal of Atmospheric Chemistry and Physics Research:Systematic satellite observations of the impact of aerosols from passive volcanic degassing on local cloud propertiesJournal of Atmospheric Chemistry and Physics, October 9, 2014 || ", "hits": 56 }, { "id": 4217, "url": "https://svs.gsfc.nasa.gov/4217/", "result_type": "Visualization", "release_date": "2014-10-08T00:00:00-04:00", "title": "Coordinated Earth: Measuring Space in the Near-Earth Environment", "description": "When we operate satellites in space, they are often taking measurements along the locations of their travel. As with many measurements, they are only useful if they can be placed in the proper context - their relationship to other measurements at the same, and different, locations. To assemble these measurements within context, we also need to know where and when the measurements were taken, and to do that, we need to define a coordinate system.In three-dimensional space, we define a position with three numbers, relative to a point we define as the Origin of the coordinate system, defined as (0,0,0). Each number represents a distance from the origin along one of three directions. We usually defined these directions by axes, labelled X, Y, and Z, which are defined to be mutually perpendicular, each one is at right angles to the others.While all coordinate systems are equal, all coordinate systems are not equally convenient for a given problem of interest. Sometimes the data and mathematics we use for exploring different problems can be more complex in one coordinate system or another. To simplify this, we often define a number of different coordinate systems and ways to do transformations between them.In studying the space environment around Earth, we find five different coordinate systems of use. Geocentric (GEO): This is the coordinate system useful for measuring things close to Earth’s surface. The origin is chosen at the center of Earth. The x-axis points from the center of Earth through the Prime Meridian (by convention chosen as the meridian in Greenwich, London, UK (longitude = 0). The z-axis points towards the north geographic pole. Geocentric Earth Inertial (GEI): This coordinate system is fixed relative to the distant stars, so Earth rotates about the z-axis relative to it. The origin of this coordinate system is at the center of the Earth. The x-axis points to the first point in Aries (Wikipedia: Vernal Equinox) and the z-axis points to the north geographic & celestial pole. The direction of the celestial pole changes due to Earth’s rotational precession (Wikipedia). Geocentric Solar Ecliptic (GSE): The origin is at the center of the Earth. The x-axis is along the line between Earth and the Sun. The z-axis is the north ecliptic pole and is fixed in direction (but for slow changes due to Earth orbital changes). Solar Magnetic (SM): the origin is at the center of the Earth. The z-axis is chosen parallel to the Earth magnetic dipole axis. The y-axis is chosen to be perpendicular to the z-axis and the Earth-Sun line (pointing towards dusk). Geocentric Solar Magnetospheric (GSM): The origin is at the center of the Earth. The x-axis is defined as the Earth-Sun line (same as in GSE). The y-axis is defined to be perpendicular to the plane containing the x-axis and the magnetic dipole axis so the magnetic axis always lies in this plane.Similar coordinate systems are defined for the Sun and other planets of the Solar System.Development Note: This visualization was originally developed to test coordinate system transformations in the visualization framework.References:C. T. Russell. \"Geophysical coordinate transformations\". Cosmical Electrodynamics 2, 184-196 (1971). URL.M.A. Hapgood. \"Space Physics Coordinate Transformations: A User Guide\". Planetary & Space Science, 40, 711-717.(1992). URLSPENVIS Help Pages: Coordinate Systems and transformations || ", "hits": 184 }, { "id": 4205, "url": "https://svs.gsfc.nasa.gov/4205/", "result_type": "Visualization", "release_date": "2014-09-24T09:00:00-04:00", "title": "Earth Science Heads-up Display", "description": "On September 10, 2014, NASA's Earth Observing System (EOS) was celebrated in an evening event at the Smithsonian National Air and Space Museum in Washington DC. The title of this event was \"Vital Signs: Taking the Pulse of Our Planet\", and the speakers at this event included several Earth Scientists from Goddard Space Flight Center. This animation was used in the beginning of the event to illustrate the interconnectedness of the many Earth-based data sets that NASA has produced over the last decade or so. The animation simulates a view of the Earth from the International Space Station, over which interconnected data sets are displayed as if on a head-up display. || ", "hits": 34 }, { "id": 30503, "url": "https://svs.gsfc.nasa.gov/30503/", "result_type": "Hyperwall Visual", "release_date": "2014-05-13T00:00:00-04:00", "title": "Ocean Bottom Pressure from GRACE", "description": "The twin Gravity Recovery and Climate Experiment (GRACE) satellites, launched on March 17, 2002, have been making detailed measurements of Earth’s gravity field from space and revolutionizing investigations about Earth's ocean, water reservoirs, large-scale solid Earth changes, and ice cover.To aid in the interpretation of gravity change over the oceans, the GRACE Tellus project provides ocean bottom pressure maps derived from the GRACE satellite data. Ocean bottom pressure is the sum of the mass of the atmosphere and ocean in a \"cylinder\" above the seafloor. This visualization shows monthly changes in ocean bottom pressure data obtained by the GRACE satellites from November 2002 to January 2012. Purple and blue shades indicate regions with relatively low ocean bottom pressure, while red and white shades indicate regions with relatively high ocean bottom pressure. Scientists use these data to observe and monitor changes in deep ocean currents, which transport water and energy around the globe. || ", "hits": 48 }, { "id": 30476, "url": "https://svs.gsfc.nasa.gov/30476/", "result_type": "Hyperwall Visual", "release_date": "2013-11-01T15:00:00-04:00", "title": "Mount Etna", "description": "Twin volcanic plumes—one of ash, one of gas—rose from Sicily’s Mount Etna on the morning of October 26, 2013. L’Istituto Nazionale di Geofisica e Vulcanologia (INGV) Osservatorio Etneo (National Institute of Geophysics and Volcanology Etna Observatory) reported that Etna was experiencing its first paroxysm in six months. Multiple eruption columns are common at Etna, a result of complex plumbing within the volcano. The Northeast Crater, one of several on Etna’s summit, was emitting the ash column, while the New Southeast Crater was simultaneously venting mostly gas.This natural-color image collected by Landsat 8 shows the view from space at 11:38 a.m. local time. The towering, gas-rich plume cast a dark shadow over the lower, ash-rich plume and Etna’s northwestern flank. Relatively fresh lava flows (less than a century or so old) are dark gray; vegetation is green; and the tile-roofed buildings of Bronte and Biancavilla lend the towns an ochre hue. || ", "hits": 55 }, { "id": 30381, "url": "https://svs.gsfc.nasa.gov/30381/", "result_type": "Hyperwall Visual", "release_date": "2013-10-24T12:00:00-04:00", "title": "Monthly Aerosol Optical Thickness (Terra/MODIS)", "description": "Tiny solid and liquid particles suspended in the atmosphere are called aerosols. These particles are important to scientists because they represent an area of great uncertainty in their efforts to understand Earth's climate system. These maps show monthly aerosol optical thickness, derived using measurements from the Moderate Resolution Imaging Spectroradiometer (MODIS) sensor onboard NASA’s Terra satellite, from January 2005 to the present. Aerosol optical thickness is a measure of how much light the airborne particles prevent from traveling through the atmosphere. Aerosols absorb and scatter incoming sunlight, thus reducing visibility and increasing optical thickness. Dark orange pixels show high aerosol concentrations, while light orange pixels show lower concentrations, and light yellow areas show little or no aerosols. Black shows where the sensor could not make its measurement. An optical thickness of less than 0.1 (light yellow) indicates a crystal clear sky with maximum visibility, whereas a value of 1 (dark orange) indicates the presence of aerosols so dense that people would have difficulty seeing the sun. || ", "hits": 91 }, { "id": 30382, "url": "https://svs.gsfc.nasa.gov/30382/", "result_type": "Hyperwall Visual", "release_date": "2013-10-24T12:00:00-04:00", "title": "Monthly Aerosol Particle Radius (Terra/MODIS)", "description": "Tiny solid and liquid particles suspended in the atmosphere are called aerosols. These particles are important to scientists because they can affect climate, weather, and people's health. Using satellites scientists can tell whether a given plume of aerosols came from a natural source or were produced by human activities. Two important clues about aerosols' sources are particle size and location of the plume. Natural aerosols (such as dust and sea salts) tend to be larger than man-made aerosols (such as smoke and industrial pollution). These maps show monthly aerosol particle radius from January 2005 to the present, derived using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) sensor onboard NASA’s Terra satellite. Red areas show aerosol plumes made up of smaller particles. These red-colored plumes are over regions where we know humans produce pollution. Green areas show aerosol plumes made up of larger particles. These green-colored plumes are over regions where we know aerosols occur naturally. Yellow areas show plumes in which large and small aerosol particles are intermingling. Black shows where the satellite could not measure aerosols. Maps such as these allow scientists to estimate the location and size of aerosol particles present in the atmosphere. || ", "hits": 42 }, { "id": 30394, "url": "https://svs.gsfc.nasa.gov/30394/", "result_type": "Hyperwall Visual", "release_date": "2013-10-24T12:00:00-04:00", "title": "Monthly Aerosol Optical Thickness (Aqua/MODIS)", "description": "Tiny solid and liquid particles suspended in the atmosphere are called aerosols. These particles are important to scientists because they represent an area of great uncertainty in their efforts to understand Earth's climate system.These maps show monthly aerosol optical thickness, derived using measurements from the Moderate Resolution Imaging Spectroradiometer (MODIS) sensor onboard NASA’s Aqua satellite, from July 2002 to the present. Aerosol optical thickness is a measure of how much light the airborne particles prevent from traveling through the atmosphere. Aerosols absorb and scatter incoming sunlight, thus reducing visibility and increasing optical thickness. Dark orange pixels show high aerosol concentrations, while light orange pixels show lower concentrations, and light yellow areas show little or no aerosols. Black shows where the sensor could not make its measurement. An optical thickness of less than 0.1 (light yellow) indicates a crystal clear sky with maximum visibility, whereas a value of 1 (dark orange) indicates the presence of aerosols so dense that people would have difficulty seeing the sun. || ", "hits": 84 }, { "id": 30395, "url": "https://svs.gsfc.nasa.gov/30395/", "result_type": "Hyperwall Visual", "release_date": "2013-10-24T12:00:00-04:00", "title": "Monthly Aerosol Particle Radius (Aqua/MODIS)", "description": "Tiny solid and liquid particles suspended in the atmosphere are called aerosols. These particles are important to scientists because they can affect climate, weather, and people's health. Using satellites scientists can tell whether a given plume of aerosols came from a natural source or were produced by human activities. Two important clues about aerosols' sources are particle size and location of the plume. Natural aerosols (such as dust and sea salts) tend to be larger than man-made aerosols (such as smoke and industrial pollution). These maps show monthly aerosol particle radius from July 2002 to the present, derived using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) sensor onboard NASA’s Aqua satellite. Red areas show aerosol plumes made up of smaller particles. These red-colored plumes are over regions where we know humans produce pollution. Green areas show aerosol plumes made up of larger particles. These green-colored plumes are over regions where we know aerosols occur naturally. Yellow areas show plumes in which large and small aerosol particles are intermingling. Black shows where the satellite could not measure aerosols. Maps such as these allow scientists to estimate the location and size of aerosol particles present in the atmosphere. || ", "hits": 96 }, { "id": 30224, "url": "https://svs.gsfc.nasa.gov/30224/", "result_type": "Hyperwall Visual", "release_date": "2013-10-21T12:00:00-04:00", "title": "Loss of Ice on the Antarctic Peninsula", "description": "Land glacier extent and volume at the northern and southern margins of the Drake Passage have been in a state of dramatic demise since the early 1990s. Space gravity observations from the Gravity Recovery and Climate Experiment (GRACE) are combined with Global Positioning System bedrock uplift data to simultaneously solve for ice loss and for solid Earth glacial isostatic adjustment to Little Ice Age cryospheric loading. This image shows ice loss on the Antarctic peninsula between January 2003 and March 2010 derived from GRACE. The ice loss in the Graham Land section of the Antarctic peninsula is 32 ± 6 gigaton/year, while the total for the entire peninsula is 41.5 ± 9 gigaton/year. This ice loss corresponds to a global sea level rise of approximately 0.19 mm/year. || ", "hits": 64 }, { "id": 30307, "url": "https://svs.gsfc.nasa.gov/30307/", "result_type": "Hyperwall Visual", "release_date": "2013-10-21T12:00:00-04:00", "title": "Iceland Volcano Eruption Eyjafjallajökull", "description": "Iceland’s Eyjafjallajökull Volcano produced its second major ash plume of 2010 beginning on May 7. When the first ash eruption began on April 14, air travel across most of Europe was shut down, but by the time of the second eruption, forecasters were better prepared to predict the spread of volcanic ash. Despite some airport closures and flight cancellations, most air passengers completed their journeys with minimal delay.Among the key pieces of information that a computer model must have to predict the spread of ash is when the eruption happened, how much ash was ejected, and how high the plume got. The Multi-angle Imaging SpectroRadiometer (MISR) aboard NASA’s Terra satellite collected data on ash height when it passed just east of the Eyjafjallajökull Volcano mid-morning on May 7. || ", "hits": 39 }, { "id": 30308, "url": "https://svs.gsfc.nasa.gov/30308/", "result_type": "Hyperwall Visual", "release_date": "2013-10-21T12:00:00-04:00", "title": "Puyehue-Cordon Caulle Volcanic Complex, Chile", "description": "On June 4, 2011, a fissure opened in Chile's Puyehue-Cordón Caulle Volcanic Complex, sending ash 45,000 feet (14,000 meters) into the air. This image, taken on June 11, 2011, shows the path of the volcanic ash plume. Winds blowing from the west carried the plume downwind, across Argentina and eventually reaching the South Atlantic Ocean. Clear skies allow the snow-covered Andes Mountains to be seen just north and south of the erupting volcano. The opposite is true for areas downwind of the volcano beneath the highest concentrations of volcanic ash. It is hard for even the tiniest bit of sunlight to penetrate the thick plume as revealed by the dark shadow cast on the earth's surface directly south of the plume. The width of the plume increases with increasing distance from the volcano as particulates disperse in the atmosphere. The zigzag path of the plume over Argentina suggests shifts in wind direction. East of the Andes, heavier volcanic ash sediment has settled on the land below, blanketing large portions of Argentina. It appears that some of the settled ash has been picked up again, this time by surface winds that may eventually carry the sediment out to sea. A high resolution image acquired 6 weeks later shows ash covering the mountain slopes and pumice floating in lakes. || ", "hits": 43 }, { "id": 30171, "url": "https://svs.gsfc.nasa.gov/30171/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "Tohoku-oki Earthquake", "description": "Over 1200 permanent, geodetic GPS stations in the Japanese GEONET network recorded the motion of the Tohoku-Oki earthquake with 1-second resolution. This movie shows the displacements measured at each station. || ", "hits": 20 } ] }