{ "count": 66, "next": null, "previous": null, "results": [ { "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": 728 }, { "id": 40525, "url": "https://svs.gsfc.nasa.gov/gallery/habitable-worlds-observatory/", "result_type": "Gallery", "release_date": "2024-10-01T00:00:00-04:00", "title": "Habitable Worlds Observatory", "description": "The Habitable Worlds Observatory is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.\n\nHabitable Worlds will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.\n\nThis future space observatory will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter and the evolution of cosmic structure.\n\nThe Habitable Worlds Observatory will build on the technological foundations of the Hubble, Webb and Roman Space Telescopes, uniting government, industry, academia, and international partners.", "hits": 299 }, { "id": 12976, "url": "https://svs.gsfc.nasa.gov/12976/", "result_type": "Produced Video", "release_date": "2023-08-30T16:30:00-04:00", "title": "OSIRIS-REx L-30 Press Briefing Graphics", "description": "On Sept. 24, the OSIRIS-REx spacecraft will approach Earth and release a capsule containing samples of near-Earth asteroid Bennu. The Sample Return Capsule will streak into the atmosphere at 8:42 am MDT and land at the Department of Defense Utah Test and Training Range at 8:55 am.Touchdown will mark the end of a seven-year journey to explore asteroid Bennu, collect a sample from its surface, and deliver it to Earth. Scientists from around the world will study the sample over the coming decades to learn about the formation of the solar system and the delivery of organic molecules to early Earth.The week of Aug. 27, the OSIRIS-REx mission team gathered in Utah to test their landing and recovery plans. Their goal was to reduce the time to safely retrieve the capsule from the desert floor and transport it to a clean room on base, protecting the Bennu sample from earthly contaminants. On Wednesday, Aug. 30, NASA held a press briefing to discuss the test and to preview sample return. Presenter graphics are available below. Animations of OSIRIS-REx sample return are available here.Learn more about the drop test. Follow the journey to Bennu and back on NASA.gov and on Flickr. Watch a recording of the press briefing on YouTube. || ", "hits": 110 }, { "id": 14183, "url": "https://svs.gsfc.nasa.gov/14183/", "result_type": "Produced Video", "release_date": "2022-07-25T12:00:00-04:00", "title": "The James Webb Space Telescope First Images Press Conference July 12, 2022", "description": "Webb Telescope First Images media briefing - Scientists discuss more about the first images that have been taken by the James Webb Space Telescope, an answer questions from the public about the images following the broadcast at Goddard Space Flight Center in Greenbelt, MD on July 12th, 2022. || ", "hits": 74 }, { "id": 14122, "url": "https://svs.gsfc.nasa.gov/14122/", "result_type": "Produced Video", "release_date": "2022-03-23T00:00:00-04:00", "title": "The James Webb Space Telescope Mirror Alignment Press Conference Update", "description": "The press conference covering the latest updated on the James Webb Space Telescope and the mirror alignment. || ", "hits": 15 }, { "id": 14120, "url": "https://svs.gsfc.nasa.gov/14120/", "result_type": "Produced Video", "release_date": "2022-03-16T12:00:00-04:00", "title": "Tribute to Eugene Parker, Namesake of NASA’s Parker Solar Probe", "description": "Dr. Eugene N. Parker, visionary of heliophysics and namesake of NASA’s Parker Solar Probe, passed away on March 15, 2022. He was 94. As a young professor at the University of Chicago in the mid-1950s, Parker developed a mathematical theory that predicted the solar wind, the constant outflow of solar material from the Sun. Throughout his career, Parker revolutionized the field time and again, advancing ideas that addressed the fundamental questions about the workings of our Sun and stars throughout the universe.More information:• NASA Press Release• University of Chicago Press Release || ", "hits": 49 }, { "id": 14071, "url": "https://svs.gsfc.nasa.gov/14071/", "result_type": "Produced Video", "release_date": "2022-01-08T00:00:00-05:00", "title": "Webb Telescope Post-Deployment Media Briefing", "description": "Webb Telescope Post-Deployment Media Briefing || 14071_Webb_PostDeployment_Briefing.00001_print.jpg (1024x576) [86.4 KB] || 14071_Webb_PostDeployment_Briefing.00001_searchweb.png (320x180) [50.5 KB] || 14071_Webb_PostDeployment_Briefing.00001_thm.png (80x40) [4.7 KB] || 14071_Webb_PostDeployment_Briefing.mov (1280x720) [60.8 GB] || 14071_Webb_PostDeployment_Briefing.mp4 (1280x720) [6.1 GB] || 14071_Webb_PostDeployment_Briefing.webm (1280x720) [650.0 MB] || 14071_Webb_PostDeployment_Briefing.en_US.srt [138.0 KB] || 14071_Webb_PostDeployment_Briefing.en_US.vtt [129.7 KB] || ", "hits": 22 }, { "id": 13744, "url": "https://svs.gsfc.nasa.gov/13744/", "result_type": "Produced Video", "release_date": "2020-10-21T17:09:00-04:00", "title": "OSIRIS-REx Post-TAG Briefing", "description": "NASA is hosting a press briefing on Oct. 21 to unveil new videos of the OSIRIS-REx sample collection attempt.The Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) spacecraft unfurled its robotic arm on Oct. 20, and in a first for the agency, briefly touched an asteroid to collect dust and pebbles from the surface for delivery to Earth in 2023.This well-preserved, ancient asteroid, known as Bennu, is currently more than 200 million miles (321 million kilometers) from Earth. Bennu offers scientists a window into the early solar system as it was first taking shape billions of years ago and flinging ingredients that could have helped seed life on Earth. If the sample collection event, known as “Touch-And-Go” (TAG), provided enough of a sample, mission teams will command the spacecraft to begin stowing the precious primordial cargo to begin its journey back to Earth in March 2021. || ", "hits": 79 }, { "id": 13738, "url": "https://svs.gsfc.nasa.gov/13738/", "result_type": "Produced Video", "release_date": "2020-10-19T11:30:00-04:00", "title": "OSIRIS-REx Science and Engineering Briefing", "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ", "hits": 58 }, { "id": 13724, "url": "https://svs.gsfc.nasa.gov/13724/", "result_type": "Produced Video", "release_date": "2020-09-24T14:25:00-04:00", "title": "OSIRIS-REx: Countdown to TAG", "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ", "hits": 49 }, { "id": 13664, "url": "https://svs.gsfc.nasa.gov/13664/", "result_type": "Produced Video", "release_date": "2020-07-16T08:00:00-04:00", "title": "ESA and NASA Release First Images From Solar Orbiter Mission", "description": "Scientists from ESA (European Space Agency) and NASA will present the first images captured by Solar Orbiter, the joint ESA/NASA mission to study the Sun, during an online news briefing at 8 a.m. EDT Thursday, July 16. Launched on Feb. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun. The flyby captured the closest images ever taken of the Sun. During the briefing, mission experts will discuss what these closeup images reveal about our star, including what we can learn from Solar Orbiter’s new measurements of particles and magnetic fields flowing from the Sun.The briefing will stream live at:https://www.nasa.gov/solarorbiterfirstlight/Participants in the call include:•Daniel Müller – Solar Orbiter Project Scientist at ESA•Holly R. Gilbert – Solar Orbiter Project Scientist at NASA•José Luis Pellón Bailón – Solar Orbiter Deputy Spacecraft Operations Manager at ESA•David Berghmans – Principal investigator of the Extreme Ultraviolet Imager (EUI) at the Royal Observatory of Belgium•Sami Solanki – Principal investigator of the Polarimetric and Helioseismic Imager (PHI) and director of the Max Planck Institute for Solar System Research•Christopher J. Owen – Principal investigator of the Solar Wind Analyser (SWA) at Mullard Space Science Laboratory, University College London•ESA’s first light images•ESA press release •NASA feature story || ", "hits": 267 }, { "id": 40412, "url": "https://svs.gsfc.nasa.gov/gallery/van-allen-probes/", "result_type": "Gallery", "release_date": "2020-03-06T00:00:00-05:00", "title": "Van Allen Probes", "description": "Formally the Radiation Belt Storm Probes (RBSP)!", "hits": 42 }, { "id": 13535, "url": "https://svs.gsfc.nasa.gov/13535/", "result_type": "Produced Video", "release_date": "2020-02-07T14:30:00-05:00", "title": "Solar Orbiter Science Press Briefing", "description": "NASA and the European Space Agency (ESA) will present Solar Orbiter, the ESA/NASA mission to the Sun, during a science press briefing on Friday, Feb. 7. 2020, at 2.30 p.m. EST. Solar Orbiter will observe the Sun with high spatial resolution telescopes and capture observations in the environment directly surrounding the spacecraft to create a one-of-a-kind picture of how the Sun can affect the space environment throughout our solar system. The spacecraft also will provide the first-ever images of the Sun’s poles and the never-before-observed magnetic environment there, which helps drive the Sun’s 11-year solar cycle and its periodic outpouring of solar storms.The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:European Space Agency• Daniel Müller, Solar Orbiter Project Scientist• Günther Hasinger, Director of ScienceNASA• Nicky Fox, Heliophysics Division Director, NASA HQ• Thomas Zurbuchen, Associate Administrator for the Science Mission Directorate, NASA HQ || ", "hits": 52 }, { "id": 13489, "url": "https://svs.gsfc.nasa.gov/13489/", "result_type": "Produced Video", "release_date": "2019-12-12T14:00:00-05:00", "title": "OSIRIS-REx: X Marks the Spot - 2019 AGU Press Conference", "description": "Close-up images of the OSIRIS-REx sample site candidates on asteroid Bennu.Credit: NASA/Goddard/University of Arizona || Bennu_Site_Candidates_CloseUp_print.jpg (1024x575) [150.1 KB] || Bennu_Site_Candidates_CloseUp.png (7999x4499) [15.5 MB] || ", "hits": 35 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ", "hits": 109 }, { "id": 40372, "url": "https://svs.gsfc.nasa.gov/gallery/moonpole/", "result_type": "Gallery", "release_date": "2019-05-10T00:00:00-04:00", "title": "The Moon's South Pole", "description": "This is a collection of the media resources available on the Scientific Visualization Studio website related to the south pole of the Moon, an area of special interest for future exploration. It has been studied intensively by every instrument aboard Lunar Reconnaissance Orbiter (LRO). It includes cold, permanently shadowed craters that have collected water and other volatiles and shielded them from the Sun. Its rugged terrain also offers temperate high spots with persistent sunshine ideal for continuous solar power generation. More information and media are available at\nLRO Camera Images (search for south pole)\nLRO Diviner temperature measurements\nLyman-Alpha Map\n", "hits": 898 }, { "id": 13154, "url": "https://svs.gsfc.nasa.gov/13154/", "result_type": "Produced Video", "release_date": "2019-03-19T13:25:00-04:00", "title": "OSIRIS-REx LPSC Media Telecon", "description": "NASA hosted a media teleconference at 1:30 p.m. EDT Tuesday, March 19, to announce new science from the agency’s first mission to return to Earth an asteroid sample that may contain unaltered material from the very beginning of our solar system.The Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft launched Sept. 8, 2016, and began orbiting the asteroid Bennu on Dec. 31, 2018. Since its arrival at Bennu, the probe has been investigating the asteroid and searching for an ideal site for sample collection. Bennu is only slightly wider than the height of the Empire State Building and is the smallest body ever orbited by spacecraft. Studying Bennu with OSIRIS-REx will allow researchers to learn more about the origins of our solar system, the sources of water and organic molecules on Earth, and the hazards and resources in near-Earth space. The teleconference participants are:Lori Glaze, acting director, NASA’s Planetary Science Division, WashingtonDante Lauretta, OSIRIS-REx principal investigator, University of Arizona, TucsonCoralie Adam, OSIRIS-REx flight navigator, KinetX, Inc. Space Navigation and Flight Dynamics, Simi Valley, Calif.Rich Burns, OSIRIS-REx project manager, NASA’s Goddard Space Flight Center, Greenbelt, Md.For more information about the mission, go to nasa.gov/osirisrex or asteroidmission.org.Learn more about the big surprises at Bennu that were announced during this teleconference, and see images of the asteroid's particle plumes and its unexpectedly rugged surface. || ", "hits": 33 }, { "id": 13113, "url": "https://svs.gsfc.nasa.gov/13113/", "result_type": "Produced Video", "release_date": "2018-12-12T15:00:00-05:00", "title": "AGU 2018 - Expected Data and Scientific Discovery from NASA’s Parker Solar Probe", "description": "Animation of NASA's Parker Solar Probe in the solar wind. Credit: NASA/GSFC/CIL/Brian Monroe || 1_Nicky_ParkerBeautyPass_1.00200_print.jpg (1024x576) [34.0 KB] || 1_Nicky_ParkerBeautyPass_1.mp4 (1920x1080) [24.5 MB] || 1_Nicky_ParkerBeautyPass_1.webm (1920x1080) [2.4 MB] || ", "hits": 16 }, { "id": 12658, "url": "https://svs.gsfc.nasa.gov/12658/", "result_type": "Produced Video", "release_date": "2018-12-10T13:50:00-05:00", "title": "OSIRIS-REx Arrives at Bennu -- 2018 AGU Press Conference", "description": "NASA’s OSIRIS-REx mission presented the science results gained during the spacecraft’s approach toward the asteroid Bennu at a press conference hosted during AGU’s Fall Meeting at 2 p.m. ET, Monday, Dec. 10.The Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft, which launched on Sept. 8, 2016, started asteroid science operations on Aug. 17, 2018, while still 1.4 million miles from the asteroid Bennu. Between that time and the spacecraft’s arrival at Bennu on Dec. 3, the mission made a number of discoveries about the asteroid. The mission represents a valuable opportunity to learn more about the origins of our solar system, the sources of water and organic molecules on Earth, and the hazards and resources in near-Earth space. The briefing participants are:Jeffrey Grossman, OSIRIS-REx program scientist at NASA HeadquartersDante Lauretta, OSIRIS-REx principal investigator at the University of Arizona, TucsonAmy Simon, OVIRS deputy instrument scientist at NASA Goddard Space Flight Center Michael Nolan, OSIRIS-REx science team chief at the University of Arizona, TucsonFor more information, go to nasa.gov/osiris-rex or asteroidmission.org. || ", "hits": 47 }, { "id": 13083, "url": "https://svs.gsfc.nasa.gov/13083/", "result_type": "Produced Video", "release_date": "2018-10-04T11:00:00-04:00", "title": "Hubble Archive - Post-Deployment", "description": "Digitized tape of the press conference from June 27, 1990 where Ed Weiler and others explain the Hubble Space Telescope's spherical aberration problem and its impact to the science instruments. The aberration wouldn't much affect UV or IR observations, but the Wide Field Planetary Camera would be largely affected since it used visible wavelengths. TRT: 30:00Participants: Douglas Broome, HST Program Manager; Jean Olivier, Deputy Project Manager; Dr. Edward Weiler, HST Program Scientist at NASA HQ; Dr. Lennard A. Fisk, Associate Administrator Space Science and Applications at NASA HQ; Dr. Peter Stockman, Deputy Director of the Space Telescope Science InstituteLonger notes:Describing the initial spherical aberration problem with the Hubble Space Telescope’s primary mirror. Describe how they conclusively determined the nature of the problem. It affects one of their science objectives. Weiler: “We can still do important science.” UV capability and IR capability not impacted. Spatial resolution is about at ground-based resolution. Explains impacts to each of the instruments. HRS - will be able to do most of the science, just not in crowded fields, still excellent for planetary features, least impacted instrument FOS - UV science not impacted except on crowded fields, quasar absorption lines won’t be impacted because point sources, FOC - highest spatial resolution of the cameras, visible wavelengths will be ground-based resolution except maybe better for bright objects, HSP - won’t be able to do science with high signal to noise, but can do about half of proposed science esp in UV WFPC - probably no real science we can do with this because in visible Fine guidance sensors for astrometry - can do 100% of science we proposed, will be able to look at star’s wobble to find exoplanetsBiggest impact is loss of spatial resolution for WFPCInsurance policy - planned for maintenance program, are already building a second wide-field camera with a corrective mirror, think we can take out all the aberration and get back to original specification, 40% of science was going to be done with wide-field camera, developing NICMOS for near-IR capability that includes corrective opticsFor HRS and FOS, have STIS under development which would replace spectrographic capabilities Haven’t yet figured out how the problem occured; putting together a review boardDon’t know if the aberration is in the primary or secondary mirrorDidn’t test the two mirrors in combination because it would have been tremendously costly and difficult (hundreds of millions of dollars)Cuts off at endAudio missing from 11:10 - 11:20 || GSFC_19900627_HST_m001_thumbnail.jpg (720x484) [131.8 KB] || GSFC_19900627_HST_m001_thumbnail_searchweb.png (320x180) [145.5 KB] || GSFC_19900627_HST_m001_thumbnail_thm.png (80x40) [9.4 KB] || GSFC_19900627_HST_m001.mov (720x486) [12.5 GB] || GSFC_19900627_HST_m001.mp4 (720x484) [2.1 GB] || GSFC_19900627_HST_m001.webm [0 bytes] || ", "hits": 31 }, { "id": 40358, "url": "https://svs.gsfc.nasa.gov/gallery/sdopresentation-resources/", "result_type": "Gallery", "release_date": "2018-09-07T00:00:00-04:00", "title": "SDO: Presentation Resources", "description": "No description available.", "hits": 79 }, { "id": 13012, "url": "https://svs.gsfc.nasa.gov/13012/", "result_type": "Produced Video", "release_date": "2018-08-24T13:55:00-04:00", "title": "OSIRIS-REx Approach Media Telecon", "description": "Recorded audio from the OSIRIS-REx approach media teleconference on August 24, 2018, with accompanying presenter graphics. Individual graphics are available below.Watch this video on the NASA.gov Video YouTube channel. || OSIRIS-REx_TAG_preview.jpg (1920x1080) [380.4 KB] || OSIRIS-REx_Approach_Media_Telecon.webm (960x540) [427.4 MB] || TWITTER_720_OSIRIS-REx_Approach_Media_Telecon_twitter_720.mp4 (1280x720) [934.4 MB] || OSIRIS-REx_Approach_082418.wav [51.6 MB] || FACEBOOK_720_OSIRIS-REx_Approach_Media_Telecon_facebook_720.mp4 (1280x720) [1.7 GB] || OSIRIS-REx_Approach_Media_Telecon.mp4 (1920x1080) [4.0 GB] || ", "hits": 47 }, { "id": 13028, "url": "https://svs.gsfc.nasa.gov/13028/", "result_type": "Produced Video", "release_date": "2018-08-08T00:00:00-04:00", "title": "Parker Solar Probe Media Telecons", "description": "This is a resource page for the media teleconferences on August 8, 2018. || ", "hits": 50 }, { "id": 13003, "url": "https://svs.gsfc.nasa.gov/13003/", "result_type": "Produced Video", "release_date": "2018-07-20T12:30:00-04:00", "title": "Parker Solar Probe Science Briefing - Visual Resources", "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ", "hits": 51 }, { "id": 12994, "url": "https://svs.gsfc.nasa.gov/12994/", "result_type": "Produced Video", "release_date": "2018-07-12T11:00:00-04:00", "title": "NASA's Fermi Links Cosmic Neutrino to Monster Black Hole", "description": "The discovery of a high-energy neutrino on Sept. 22, 2017, sent astronomers on a chase to locate its source -- a supermassive black hole in a distant galaxy. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Hidden Tides\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Blazar.00590_print.jpg (1024x576) [61.2 KB] || Blazar.00590.png (3840x2160) [5.2 MB] || Blazar.00590.jpg (3840x2160) [536.3 KB] || Blazar.00590_searchweb.png (320x180) [46.6 KB] || Blazar.00590_thm.png (80x40) [4.6 KB] || 12994_Fermi_Blazar_Neutrino_1080p.webm (1920x1080) [17.1 MB] || 12994_Fermi_Blazar_Neutrino_1080.mp4 (1920x1080) [154.8 MB] || 12994_Fermi_Blazar_Neutrino_1080p.mov (1920x1080) [229.5 MB] || 12994_Fermi_Blazar_Neutrino_SRT_Captions.en_US.srt [2.8 KB] || 12994_Fermi_Blazar_Neutrino_SRT_Captions.en_US.vtt [2.7 KB] || 12994_Fermi_Blazar_Neutrino_H264_4k_2997.mp4 (3840x2160) [380.3 MB] || 12994_Fermi_Blazar_Neutrino_4K.mov (3840x2160) [445.0 MB] || 12994_Fermi_Blazar_Neutrino_ProRes_4k_2997.mov (3840x2160) [6.5 GB] || ", "hits": 124 }, { "id": 12818, "url": "https://svs.gsfc.nasa.gov/12818/", "result_type": "Produced Video", "release_date": "2018-01-10T00:00:00-05:00", "title": "Webb Telescope's Houston Highlights Time Lapse", "description": "A produced time-lapse video of activity in the NASA Johnson Space Center's Chamber A cleanroom from the arrival of the Webb Telescope's optical and instrument segment through to its roll out from the chamber after completing it's cryogenic testing. || Webb_at_JSC-IMAGE_ONLY.00001_print.jpg (1024x576) [179.0 KB] || Webb_at_JSC-IMAGE_ONLY.00001_searchweb.png (320x180) [99.6 KB] || Webb_at_JSC-IMAGE_ONLY.00001_web.png (320x180) [99.6 KB] || Webb_at_JSC-IMAGE_ONLY.00001_thm.png (80x40) [7.6 KB] || Webb_at_JSC_timelapse-90sec-music-ProRes.mov (1920x1080) [1.6 GB] || Webb_at_JSC_timelapse-90sec-music-h264.mp4 (1920x1080) [116.5 MB] || Webb_at_JSC_timelapse-90sec-music-h264.webm (1920x1080) [12.3 MB] || Webb_at_JSC_timelapse-90sec-music-h264.en_US.srt [251 bytes] || Webb_at_JSC_timelapse-90sec-music-h264.en_US.vtt [263 bytes] || ", "hits": 13 }, { "id": 12796, "url": "https://svs.gsfc.nasa.gov/12796/", "result_type": "Produced Video", "release_date": "2017-12-13T11:30:00-05:00", "title": "2017 AGU Habitability Press Conference", "description": "Spanning Disciplines to Search for Life Beyond EarthThe search for life beyond Earth is riding a surge of creativity and innovation. Following a gold rush of exoplanet discovery over the past two decades, it is time to tackle the next step: determining which of the known exoplanets are proper candidates for life. Scientists from NASA and two universities presented new results dedicated to this task in fields spanning astrophysics, Earth science, heliophysics and planetary science — demonstrating how a cross-disciplinary approach is essential to finding life on other worlds — at the fall meeting of the American Geophysical Union on Dec. 13, 2017, in New Orleans, Louisiana.PANELISTS:• Giada Arney, NASA’s Goddard Space Flight Center• Stephen Kane, University of California-Riverside• Katherine Garcia-Sage, NASA’s Goddard Space Flight Center/Catholic University of America• Dave Brain, University of Colorado-Boulder || ", "hits": 110 }, { "id": 12789, "url": "https://svs.gsfc.nasa.gov/12789/", "result_type": "Produced Video", "release_date": "2017-12-11T12:30:00-05:00", "title": "AGU Press Conference - Eclipse 2017: Studying the Sun-Earth Connection and More from the Moon’s Shadow", "description": "While people across North America took in the Aug. 21 eclipse, hundreds of citizen, student, and professional scientists were collecting scientific data. They gathered data with telescopes on the ground, balloons launched to the stratosphere, jets chasing the Moon’s shadow, and satellites far above Earth. In this panel, participants will share some of the initial results from a cross-section of these studies, in fields ranging from solar physics to Earth science to space biology. Panelists:•Lika Guhathakurta, NASA Headquarters/NASA Ames Research Center•Amir Caspi, Southwest Research Institute•Matt Penn, National Solar Observatory •Angela Des Jardins, Montana State University•Greg Earle, Virginia Tech •Jay Herman, NASA Goddard Space Flight Center/University of Maryland Baltimore County || ", "hits": 34 }, { "id": 12646, "url": "https://svs.gsfc.nasa.gov/12646/", "result_type": "Produced Video", "release_date": "2017-06-21T13:00:00-04:00", "title": "2017 Solar Eclipse Press Conference", "description": "For the first time in 99 years, a total solar eclipse will cross the entire nation Aug. 21. Representatives from NASA, other federal agencies, and science organizations, will provide important viewing safety, travel and science information during two briefings at the Newseum in Washington starting at 1 p.m. EDT Wednesday, June 21.The event will air live on NASA Television and stream on the agency’s website.Over the course of 100 minutes, 14 states across the United States will experience more than two minutes of darkness in the middle of the day. Additionally, a partial eclipse will be viewable across all of North America. The eclipse will provide a unique opportunity to study the sun, Earth, moon and their interaction because of the eclipse’s long path over land coast to coast. Scientists will be able to take ground-based and airborne observations over a period of an hour and a half to complement the wealth of data and images provided by space assets.The June 21 briefings are:Logistics Briefing: 1 to 2 p.m.Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate at the agency’s headquarters in WashingtonVanessa Griffin, director of the National Oceanic and Atmospheric Administration’s Office of Satellite and Product Operations in Suitland, MarylandBrian Carlstrom, deputy associate director of Natural Resource Stewardship and Science at the National Park Service in WashingtonMartin Knopp, associate administrator of the Office of Operations in the Federal Highway Administration at the U.S. Department of Transportation in WashingtonScience Briefing: 2:30 to 3:30 p.m.Thomas ZurbuchenAngela Des Jardins, principal investigator of the Eclipse Ballooning Project at Montana State University, BozemanAngela Speck, professor of astrophysics and director of astronomy at the University of Missouri, ColumbiaDave Boboltz, program director of solar physics in the Division of Astronomical Sciences at the National Science Foundation in Arlington, VirginiaLinda Shore, executive director of the Astronomical Society of the Pacific in San FranciscoMatt Penn, astronomer at the National Solar Observatory in Tucson, Arizona || ", "hits": 31 }, { "id": 12625, "url": "https://svs.gsfc.nasa.gov/12625/", "result_type": "Produced Video", "release_date": "2017-06-13T14:00:00-04:00", "title": "Rare Total Solar Eclipse Is Only Two Months Away Live Shots 6.21.17", "description": "B-roll for the live shots || eclipse_6_21_17_b-roll.00001_print.jpg (1024x576) [85.9 KB] || eclipse_6_21_17_b-roll.00001_web.png (320x180) [50.5 KB] || eclipse_6_21_17_b-roll.00001_thm.png (80x40) [5.5 KB] || eclipse_6_21_17_b-roll.00001_searchweb.png (320x180) [50.5 KB] || eclipse_6_21_17_b-roll.webm (1280x720) [40.3 MB] || eclipse_6_21_17_b-roll.mov (1280x720) [5.5 GB] || ", "hits": 36 }, { "id": 4574, "url": "https://svs.gsfc.nasa.gov/4574/", "result_type": "Visualization", "release_date": "2017-05-31T10:00:00-04:00", "title": "Temperature, Reflectance Point to Frost near the Moon's Poles", "description": "A view of the south pole of the Moon showing where reflectance and temperature data indicate the possible presence of surface water ice. Includes music and narration. Music by Killer Tracks: Full Charge - Zubin Thakkar. || 4574_LROMoonFrost_YouTube.00780_print.jpg (1024x576) [236.8 KB] || 4574_LROMoonFrost_YouTube.mp4 (1920x1080) [75.8 MB] || 4574_LROMoonFrost_Facebook.mp4 (1280x720) [65.4 MB] || 4574_LROMoonFrost_Twitter.mp4 (1280x720) [11.8 MB] || 4574_LROMoonFrost_Facebook.webm (1280x720) [5.2 MB] || 4574_LROMoonFrost_MASTER.mov (1920x1080) [639.4 MB] || 4574_LroMoonFrost_Captions.en_US.srt [761 bytes] || 4574_LroMoonFrost_Captions.en_US.vtt [774 bytes] || 4574_LROMoonFrost_YouTube.mp4.hwshow [191 bytes] || ", "hits": 137 }, { "id": 12414, "url": "https://svs.gsfc.nasa.gov/12414/", "result_type": "Produced Video", "release_date": "2016-12-14T17:30:00-05:00", "title": "AGU 2017 Eclipse Press Conference", "description": "Graphic depicting the geometry of a total solar eclipse. Credit: NASA || Eclipse_Geometry.png (1158x548) [180.5 KB] || ", "hits": 19 }, { "id": 12457, "url": "https://svs.gsfc.nasa.gov/12457/", "result_type": "Produced Video", "release_date": "2016-12-14T12:00:00-05:00", "title": "AGU Ionosphere Press Conference", "description": "The ionosphere is a layer of charged particles in Earth’s atmosphere that extends from about 50 to 360 miles above the surface of Earth. Processes in the ionosphere also create bright swaths of color in the sky, known as airglow. Credit: NASA GSFC || AGUIonosphereV4_1.jpg (1280x960) [109.7 KB] || ", "hits": 56 }, { "id": 12357, "url": "https://svs.gsfc.nasa.gov/12357/", "result_type": "Produced Video", "release_date": "2016-09-06T14:00:00-04:00", "title": "OSIRIS-REx L-2 Science Briefing Graphics", "description": "This page contains supporting graphics for the OSIRIS-REx L-2 science briefing from Kennedy Space Center on September 6, 2016. OSIRIS-REx is a NASA mission to explore asteroid Bennu and return a sample to Earth. The graphics on this page are available for download in broadcast resolution. These graphics do not include audio.Watch the OSIRIS-REx L-2 Science Briefing.To learn more, visit NASA's OSIRIS-REx website and asteroidmission.org. || ", "hits": 32 }, { "id": 12358, "url": "https://svs.gsfc.nasa.gov/12358/", "result_type": "Produced Video", "release_date": "2016-09-06T12:50:00-04:00", "title": "OSIRIS-REx L-2 Pre-Launch Briefing Graphics", "description": "Supporting graphics for the OSIRIS-REx L-2 pre-launch briefing at Kennedy Space Center on Sept. 6, 2016. || 1. Dante Lauretta - OSIRIS-REx Acronym || 0_Dante_All.00001_print.jpg (1024x576) [59.1 KB] || 0_Dante_All.00001_print_searchweb.png (320x180) [45.1 KB] || 0_Dante_All.00001_print_thm.png (80x40) [4.0 KB] || 0_Dante_All.webm (1280x720) [32.4 MB] || 0_Dante_All.mov (1280x720) [4.2 GB] || ", "hits": 34 }, { "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": 28 }, { "id": 11822, "url": "https://svs.gsfc.nasa.gov/11822/", "result_type": "Produced Video", "release_date": "2016-04-14T12:55:00-04:00", "title": "Hubble Memorable Moments", "description": "4. Hubble Memorable Moments: Comet ImpactIn July 1994, the Hubble Space Telescope was poised to use its newly fixed optics to observe one of the most impressive astronomical events of the century - the 21 fragments of Comet Shoemaker-Levy 9 impacting Jupiter. But these observations almost didn’t happen.Watch this video on the NASA Goddard YouTube channel. || Hubble_Memorable_Moments.png (1276x717) [1004.3 KB] || Hubble_Memorable_Moments_print.jpg (1024x575) [98.6 KB] || Hubble_Memorable_Moments_web.png (320x180) [78.1 KB] || Hubble_Memorable_Moments_thm.png (80x40) [7.7 KB] || mem.jpg (320x180) [9.8 KB] || HubbleMemorableMoments_CometImpact.webm (1280x720) [52.1 MB] || HubbleMemorableMoments_CometImpact.mp4 (1280x720) [763.6 MB] || HubbleMemorableMoments_CometImpact.en_US.srt [9.6 KB] || HubbleMemorableMoments_CometImpact.en_US.vtt [9.6 KB] || HubbleMemorableMoments_CometImpact.mov (1280x720) [6.4 GB] || ", "hits": 59 }, { "id": 12095, "url": "https://svs.gsfc.nasa.gov/12095/", "result_type": "Produced Video", "release_date": "2015-12-15T10:30:00-05:00", "title": "AGU El Nino Press Conference Release Materials", "description": "Forty percent of California's annual water supply comes in the form of atmospheric rivers, tendrils of moisture that travel from the Pacific Ocean and rain out when they move over the coast. New research on how El Niño affects atmospheric rivers headed for the California coast suggest that while the number of atmospheric rivers California receives (typically ten per year) will not change during an El Niño, they will be stronger, warmer, and thus wetter. || ", "hits": 20 }, { "id": 40110, "url": "https://svs.gsfc.nasa.gov/gallery/astro-galaxy/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Galaxy Listing", "description": "No description available.", "hits": 100 }, { "id": 40227, "url": "https://svs.gsfc.nasa.gov/gallery/suneclipse2017/", "result_type": "Gallery", "release_date": "2015-06-11T00:00:00-04:00", "title": "Solar Eclipse 2017", "description": "During the solar eclipse on August 21, 2017, the Moon's shadow will pass over all of North America. The path of the umbra, where the eclipse is total, stretches from Salem, Oregon to Charleston, South Carolina. This will be the first total solar eclipse visible in the contiguous United States in 38 years.\nDuring those brief moments when the moon completely blocks the sun’s bright face for 2 + minutes, day will turn into night, making visible the otherwise hidden solar corona, the sun’s outer atmosphere. Bright stars and planets will become visible as well. This is truly one of nature’s most awesome sights.\rThe eclipse provides a unique opportunity to study the sun, Earth, moon and their interaction because of the eclipse’s long path over land coast to coast. Scientists will be able to take ground-based and airborne observations over a period of an hour and a half to complement the wealth of data provided by NASA assets.\nVisit https://eclipse2017.nasa.gov for more information.", "hits": 241 }, { "id": 11637, "url": "https://svs.gsfc.nasa.gov/11637/", "result_type": "Produced Video", "release_date": "2014-09-08T10:15:00-04:00", "title": "CATS - New Remote-Sensing Instrument to Blaze a Trail on the International Space Station", "description": "The Cloud-Aerosol Transport System (CATS), a new instrument that will measure the character and worldwide distribution of the tiny particles that make up haze, dust, air pollutants, and smoke, will do more than gather data once it's deployed on the International Space Station in December. || ", "hits": 59 }, { "id": 11462, "url": "https://svs.gsfc.nasa.gov/11462/", "result_type": "Produced Video", "release_date": "2014-01-30T10:00:00-05:00", "title": "GPM L-30 Mission and Science Briefings", "description": "NASA held a series of media events Monday, Jan. 27, in advance of the February launch of the Global Precipitation Measurement (GPM) Core Observatory from Japan. The events were held at NASA’s Goddard Space Flight Center in Greenbelt, Md.GPM is an international satellite mission led by NASA and the Japan Aerospace Exploration Agency (JAXA) that will provide next-generation observations of rain and snow worldwide. GPM data also will contribute to climate research and the forecasting of extreme weather events such as floods and hurricanes.The GPM Core Observatory is scheduled to lift off Feb. 27, between 1:07 and 3:07 p.m. EST, from JAXA's Tanegashima Space Center in Japan.Media events include briefings on the GPM mission and science. Briefing panelists are: Steven Neeck, deputy associate director, flight program, Earth Science, NASA Headquarters, Washington Kinji Furukawa, GPM Dual-frequency Precipitation Radar deputy project manager, JAXA, Tsukuba Art Azarbarzin, GPM project manager, Goddard Ramesh Kakar, GPM program scientist, Headquarters Gail Skofronick-Jackson, GPM deputy project scientist, Goddard Riko Oki, GPM/DPR program scientist, JAXATo view on YouTube, click here for the Mission Briefing and the Science Briefing. || ", "hits": 19 }, { "id": 11432, "url": "https://svs.gsfc.nasa.gov/11432/", "result_type": "Produced Video", "release_date": "2013-12-09T17:28:00-05:00", "title": "Briefing Materials: Taking Landsat to the Extreme", "description": "At 2:30pm (PST) on Monday, Dec. 9, 2013, there was be a press conference as part of the American Geophysical Union Fall Meeting.What is the coldest place in the world? It is a high ridge in Antarctica on the East Antarctic Plateau where temperatures in several hollows can dip below minus 133.6° Fahrenheit (minus 92° Celsius) on a clear winter night – colder than the previous recorded low temperature.Scientists at the National Snow and Ice Data Center made the discovery while analyzing the most detailed global surface temperature maps to date, developed with data from remote sensing satellites including the MODIS sensor on NASA's Aqua satellite, and the TIRS sensor on Landsat 8, a joint project of NASA and the U.S. Geological Survey (USGS).The researchers analyzed 32 years of data from several satellite instruments that have mapped Antarctica's surface temperature. Near a high ridge that runs from Dome Arugs to Dome Fuji, the scientists found clusters of pockets that have plummeted to record low temperatures dozens of times. The lowest temperature the satellites detected – minus 136° F (minus 93.2° C), on Aug. 10, 2010.The new record is several degrees colder than the previous low of minus 128.6° F (minus 89.2° C), set in 1983 at the Russian Vostok Research Station in East Antarctica. The coldest permanently inhabited place on Earth is northeastern Siberia, where temperatures dropped to a bone-chilling 90 degrees below zero F (minus 67.8° C) in the towns of Verkhoyansk (in 1892) and Oimekon (in 1933).Related feature story: http://www.nasa.gov/content/goddard/nasa-usgs-landsat-8-satellite-pinpoints-coldest-spots-on-earthBriefing SpeakersTed Scambos, National Snow and Ice Data Center (NSIDC), Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado Boulder, Boulder, Colorado, USA;Jim Irons, Landsat 8 Project Scientist, NASA's Goddard Space Flight Center, Greenbelt, Maryland.Presenter 1: Ted Scambos || ", "hits": 126 }, { "id": 40152, "url": "https://svs.gsfc.nasa.gov/gallery/maven/", "result_type": "Gallery", "release_date": "2013-11-01T00:00:00-04:00", "title": "MAVEN", "description": "NASA's Mars Atmosphere and Volatile Evolution (MAVEN) is the first mission devoted to understanding the Martian upper atmosphere. Today Mars is cold and dry, but ancient Mars was warm, wet, and possibly hospitable to life. Scientists think that the loss of Mars' early atmosphere caused the planet to dry up, and MAVEN is testing this hypothesis by observing present-day interactions of the Martian atmosphere with the solar wind. Learn more about MAVEN from\n NASA and CU Boulder.", "hits": 122 }, { "id": 10874, "url": "https://svs.gsfc.nasa.gov/10874/", "result_type": "Produced Video", "release_date": "2013-04-17T16:00:00-04:00", "title": "Science in the Media Press Conference", "description": "This video supports the Science in the Media curriculum module, which culminates with students playing the role of reporters viewing this simulated press conference and writing a story about it. The findings discussed in the video are actual results from the Suzaku satellite.Science in the Media curriculum module here. || ", "hits": 40 }, { "id": 20195, "url": "https://svs.gsfc.nasa.gov/20195/", "result_type": "B-Roll", "release_date": "2012-12-03T12:00:00-05:00", "title": "AGU Press Conference 12/3/12 - Paul Mahaffy Multimedia", "description": "This page contains the media used by Sample Anylsis at Mars Principal Investigator Paul Mahaffy during the December 3, 2012 AGU Press Conference. || ", "hits": 9 }, { "id": 4011, "url": "https://svs.gsfc.nasa.gov/4011/", "result_type": "Visualization", "release_date": "2012-11-28T00:00:00-05:00", "title": "United States Active Fires 2012", "description": "Records maintained by the National Interagency Fire Center (NIFC) and NASA both indicate that 2012 was an extraordinary year for wildfires in the United States.NIFC statistics show that more than 9.1 million acres had burned as of November 30, 2012—the third highest total in a record that dates back to 1960. Also notable: despite the high number of acres burned in 2012, the total number of fires—55,505—was low, the least on the NIFC record. Average fire size in 2012 was the highest on the record.The visualizations depict fires that burned between January 1 and October 31, 2012, as detected by the MODIS instruments. The fires are displayed over MODIS' vegetation and snow cover data. Yellow and orange indicates fires that were more intense and had a larger area of active burning. Most of these intense fires occurred in the western United States, where lightning and human activity often sparks blazes that firefighters cannot contain. Many of the lower intensity fires shown in red were prescribed fires, lit for either agricultural or ecosystem management purposes.The Terra and Aqua Moderate Resolution Imaging Spectrometer (MODIS) can routinely detect both flaming and smoldering fires that are aproximately 1000 square meters in size. Under pristine and extremely rare observing conditions even smaller flaming fires that are aproximately 50 square meters can be detected. Each active fire location represents the center of a 1 km pixel that is flagged by the algorithm as containing a fire within the pixel. For more information on the fire data, see the MODIS Collection 5 Active Fire Product User's Guide. For more information on the algorithm, see Giglio, L., J. Descloitres, C. O. Justice, and Y. J. Kaufman. 2003. An enhanced contextual fire detection algorithm for MODIS. Remote Sensing of Environment, 87:273-282 || ", "hits": 33 }, { "id": 11027, "url": "https://svs.gsfc.nasa.gov/11027/", "result_type": "Produced Video", "release_date": "2012-08-09T14:00:00-04:00", "title": "RBSP L-14 Press Conference", "description": "The Radiation Belt Storm Probes mission is part of NASA's Living With a Star Geospace program to explore fundamental processes that operate throughout the solar system, in particular those that generate hazardous space weather effects near the Earth and phenomena that could affect solar system exploration.RBSP is designed to help us understand the sun's influence on the Earth and near-Earth space by studying the planet's radiation belts on various scales of space and time.Understanding the radiation belt environment and its variability has extremely important practical applications in the areas of spacecraft operations, spacecraft and spacecraft system design, mission planning, and astronaut safety.RBSP is scheduled to launch no earlier than 4:08 a.m. Thursday, Aug. 23 from Cape Canaveral Air Force Station in Florida. The twin probes will lift off on a United Launch Alliance Atlas V rocket.News conference panelists are:— Madhulika Guhathakurta, Living With a Star program scientist, NASA Headquarters, Washington— Mona Kessel, RBSP program scientist, NASA Headquarters— Barry Mauk, RBSP project scientist, Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md.— Rick Fitzgerald, RBSP project manager, APL, Laurel, Md. || ", "hits": 91 }, { "id": 11049, "url": "https://svs.gsfc.nasa.gov/11049/", "result_type": "Produced Video", "release_date": "2012-07-18T00:00:00-04:00", "title": "Landsat 40th Liveshot Roll-in Video", "description": "On Friday, July 20th, in advance of Landsat's 40th birthday and a live NASA press conference on Monday the 23rd, NASA scientists are available to discuss amazing & unprecedented images from space of your region. Cities grow, wildfires rage, rivers flood out of their beds and droughts shrink lakes and reservoirs — all captured by Landsat, the world's longest continuous record of Earth from space. Since 1972, Landsat satellites have been orbiting Earth, telling the story of soil moisture, urban spread, land use, assist disasters & recovery. Next year, the 8th Landsat satellite (LDCM) will be launched from California. The Landsat Data Continuity Mission (LDCM) will track food production and water resources, organize disaster recovery and monitor the impact of climate change.The following is broadcast quality video roll-ins in Apple ProRes 422, 1280x720, 59.94 fps. || ", "hits": 15 }, { "id": 40122, "url": "https://svs.gsfc.nasa.gov/gallery/mars/", "result_type": "Gallery", "release_date": "2012-06-28T00:00:00-04:00", "title": "Mars Missions and Science", "description": "This multimedia gallery assembles and organizes Mars content on the Scientific Visualization Studio website. Highlights of NASA Goddard Space Flight Center’s animations, visualizations, videos, images and graphics relating to Mars science and missions can be found here.", "hits": 206 }, { "id": 10908, "url": "https://svs.gsfc.nasa.gov/10908/", "result_type": "Produced Video", "release_date": "2012-05-10T09:00:00-04:00", "title": "IBEX: Observing the Sun's Horizon", "description": "The Interstellar Boundary Explorer, or IBEX, is the first mission designed to map the entire region of the boundary of our Solar System. As charged particles from the Sun, called the \"solar wind,\" flow outward well beyond the orbits of the planets, they collide with the material between the stars, called the \"interstellar medium\" (ISM). These interactions create energetic neutral atoms (ENAs), particles with no charge that move very quickly. This region emits no light that can be collected by conventional telescopes so, instead, IBEX measures the particles that happen to be traveling inward from the boundary. IBEX contains two detectors designed to collect and measure ENAs, providing data about the mass, location, direction of origin, and energy of these particles. From these data, maps of the boundary are created. IBEX's sole, focused science objective is to discover the nature of the interactions between the solar wind and the interstellar medium at the edge of our Solar System. || ", "hits": 66 }, { "id": 10966, "url": "https://svs.gsfc.nasa.gov/10966/", "result_type": "Produced Video", "release_date": "2012-04-20T08:00:00-04:00", "title": "SDO: Year 2", "description": "April 21, 2012 marks the two-year anniversary of the Solar Dynamics Observatory (SDO) First Light press conference, where NASA revealed the first images taken by the spacecraft. This video highlights just some of the amazing events witnessed in SDO's second year. || ", "hits": 63 }, { "id": 10905, "url": "https://svs.gsfc.nasa.gov/10905/", "result_type": "Produced Video", "release_date": "2012-01-31T13:00:00-05:00", "title": "Interstellar Neutral Atoms", "description": "Animation of the interstellar interaction with our Sun-one of billions of stars that orbits around the galaxy. As we zoom in through the galaxy we can see our heliosphere; then if we travel along with the interstellar material, we can see how only a very rare few are directed along precisely the right path to make the 30 year, 15 billion mile journey and enter IBEX's low energy sensor and be detected.For press release media associated with this animation, go: here. || ", "hits": 77 }, { "id": 10906, "url": "https://svs.gsfc.nasa.gov/10906/", "result_type": "Produced Video", "release_date": "2012-01-31T13:00:00-05:00", "title": "NASA's IBEX Spacecraft Reveals New Observations of Interstellar Matter", "description": "A great magnetic bubble surrounds the solar system as it cruises through the galaxy. The sun pumps the inside of the bubble full of solar particles that stream out to the edge until they collide with the material that fills the rest of the galaxy, at a complex boundary called the heliosheath. On the other side of the boundary, electrically charged particles from the galactic wind blow by, but rebound off the heliosheath, never to enter the solar system. Neutral particles, on the other hand, are a different story. They saunter across the boundary as if it weren't there, continuing on another 7.5 billion miles for 30 years until they get caught by the sun's gravity, and sling shot around the star. There, NASA's Interstellar Boundary Explorer lies in wait for them. Known as IBEX for short, this spacecraft methodically measures these samples of the mysterious neighborhood beyond our home. IBEX scans the entire sky once a year, and every February, its instruments point in the correct direction to intercept incoming neutral atoms. IBEX counted those atoms in 2009 and 2010 and has now captured the best and most complete glimpse of the material that lies so far outside our own system. The results? It's an alien environment out there: the material in that galactic wind doesn't look like the same stuff our solar system is made of.More than just helping to determine the distribution of elements in the galactic wind, these new measurements give clues about how and where our solar system formed, the forces that physically shape our solar system, and even the history of other stars in the Milky Way.In a series of science papers appearing in the Astrophysics Journal on January 31, 2012, scientists report that for every 20 neon atoms in the galactic wind, there are 74 oxygen atoms. In our own solar system, however, for every 20 neon atoms there are 111 oxygen atoms. That translates to more oxygen in any given slice of the solar system than in the local interstellar space. For media associated with this release, go to #10905 and #3900. || ", "hits": 153 }, { "id": 10809, "url": "https://svs.gsfc.nasa.gov/10809/", "result_type": "Produced Video", "release_date": "2011-08-18T13:00:00-04:00", "title": "NASA Spacecraft Track Solar Storms From Sun To Earth", "description": "NASA's STEREO spacecraft and new data processing techniques have succeeded in tracking space weather events from their origin in the Sun's ultrahot corona to impact with the Earth 93 million miles away, resolving a 40-year mystery about the structure of the structures that cause space weather: how the structures that impact the Earth relate to the corresponding structures in the solar corona.Despite many instruments that monitor the Sun and a fleet of near-earth probes, the connection between near-Earth disturbances and their counterparts on the Sun has been obscure, because CMEs and the solar wind evolve and change during the 93,000,000 mile journey from the Sun to the Earth.STEREO includes \"heliospheric imager\" cameras that monitor the sky at large angles from the Sun, but the starfield and galaxy are 1,000 times brighter than the faint rays of sunlight reflected by free-floating electron clouds inside CMEs and the solar wind; this has made direct imaging of these important structures difficult or impossible, and limited understanding of the connection between space storms and the coronal structures that cause them.Newly released imagery reveals absolute brightness of detailed features in a large geoeffective CME in late 2008, connecting the original magnetized structure in the Sun's corona to the intricate anatomy of an interplanetary storm as it impacted the Earth three days later. At the time the data were collected, in late 2008, STEREO-A was nearly 45 degrees ahead of the Earth in its orbit, affording a very clear view of the Earth-Sun line.For the press conference Visual 1, a visualization of the STEREO orbits and the 2008 CME, go here.For Visual 7, a CME and reconnection animation, go here.For Visual 8, footage of the October 2003 solar storms, go here. || ", "hits": 143 }, { "id": 10748, "url": "https://svs.gsfc.nasa.gov/10748/", "result_type": "Produced Video", "release_date": "2011-04-21T09:00:00-04:00", "title": "SDO: Year One", "description": "April 21, 2011 marks the one-year anniversary of the Solar Dynamics Observatory (SDO) First Light press conference, where NASA revealed the first images taken by the spacecraft.In the last year, the sun has gone from its quietest period in years to the activity marking the beginning of solar cycle 24. SDO has captured every moment with a level of detail never-before possible. The mission has returned unprecedented images of solar flares, eruptions of prominences, and the early stages of coronal mass ejections (CMEs). In this video are some of the most beautiful, interesting, and mesmerizing events seen by SDO during its first year.In the order they appear in the video the events are:1. Prominence Eruption from AIA in 304 Ångstroms on March 30, 20102. Cusp Flow from AIA in 171 Ångstroms on February 14, 20113. Prominence Eruption from AIA in 304 Ångstroms on February 25, 20114. Cusp Flow from AIA in 304 Ångstroms on February 14, 20115. Merging Sunspots from HMI in Continuum on October 24-28, 20106. Prominence Eruption and active region from AIA in 304 Ångstroms on April 30, 20107. Solar activity and plasma loops from AIA in 171 Ångstroms on March 4-8, 20118. Flowing plasma from AIA in 304 Ångstroms on April 19, 20109. Active regions from HMI in Magnetogram on March 10, 201110. Filament eruption from AIA in 304 Ångstroms on December 6, 201011. CME start from AIA in 211 Ångstroms on March 8, 201112. X2 flare from AIA in 304 Ångstroms on February 15, 2011 || ", "hits": 75 }, { "id": 10733, "url": "https://svs.gsfc.nasa.gov/10733/", "result_type": "Produced Video", "release_date": "2011-03-03T16:00:00-05:00", "title": "SDO First Light Media", "description": "A compilation of some of the videos and stills used during the SDO First Light press conference.There are more video and stills available. || ", "hits": 62 }, { "id": 40091, "url": "https://svs.gsfc.nasa.gov/gallery/stereoin-stereo/", "result_type": "Gallery", "release_date": "2011-02-01T00:00:00-05:00", "title": "STEREO in Stereo", "description": "A collection of media related to the STEREO mission which are configured for display by various stereo technologies.", "hits": 22 }, { "id": 40102, "url": "https://svs.gsfc.nasa.gov/gallery/astro-media-resources/", "result_type": "Gallery", "release_date": "2011-01-28T00:00:00-05:00", "title": "Astrophysics Media Resources", "description": "No description available.", "hits": 13 }, { "id": 10551, "url": "https://svs.gsfc.nasa.gov/10551/", "result_type": "Produced Video", "release_date": "2010-06-10T00:00:00-04:00", "title": "SDO First Light Press Conference", "description": "A unique NASA spacecraft launched February 11, 2010, called the Solar Dynamics Observatory, or SDO, has started delivering images of the sun that have astonished scientists. SDO is the most advanced spacecraft ever designed to study the sun and its dynamic behavior. The spacecraft can produce images with clarity ten times better than high definition television and provide more comprehensive science data faster than any solar observing spacecraft in history. The goal of the mission is to help scientists study solar activity to improve forecasts of how the sun affects Earth.On April 21, 2010, NASA held a live press conference at the Newseum in Washington D.C. to unveil the first images and videos from SDO—SDO's First Light.A version of the press conference with captioning is available. || ", "hits": 11 }, { "id": 40069, "url": "https://svs.gsfc.nasa.gov/gallery/sdofirst-light/", "result_type": "Gallery", "release_date": "2010-03-25T00:00:00-04:00", "title": "SDO First Light", "description": "These are \"First Light\" release movies for Solar Dynamics Observatory (SDO) from April 11, 2010. For more information about SDO, visit the SDO web site @ NASA.gov.", "hits": 79 }, { "id": 10483, "url": "https://svs.gsfc.nasa.gov/10483/", "result_type": "Produced Video", "release_date": "2009-10-17T00:00:00-04:00", "title": "LRO Early Results Press Conference Visuals", "description": "These are the visuals used to support the LRO Press Conference \"NASA's LRO Mission Mapping Lunar South Pole in Uprecedented Detail\" held on September 17, 2009 at Goddard Space Flight Center. || ", "hits": 45 }, { "id": 10528, "url": "https://svs.gsfc.nasa.gov/10528/", "result_type": "Produced Video", "release_date": "2009-09-17T00:00:00-04:00", "title": "LRO Early Results Press Conference", "description": "NASA showcased new images from the Lunar Reconnaissance Orbiter's seven instruments and provided updates about the topography of the moon's south pole during a news conference on September 17. NASA also provided an update about the spacecraft's status and mission plans. The briefing took place at NASA's Goddard Space Flight Center in Greenbelt, Md. (no transcript available) || LRO_1stResults_PressConf_ipod.00002_print.jpg (1024x576) [115.7 KB] || LRO_1stResults_PressConf_ipod_web.png (320x180) [138.1 KB] || LRO_1stResults_PressConf_ipod_thm.png (80x40) [16.1 KB] || LRO_1stResults_PC_appleTV.webmhd.webm (960x540) [499.4 MB] || LRO_1stResults_PC_appleTV.m4v (960x540) [1.4 GB] || LRO_1stResults_PressConf_ipod.m4v (640x360) [586.3 MB] || ", "hits": 19 }, { "id": 10249, "url": "https://svs.gsfc.nasa.gov/10249/", "result_type": "Produced Video", "release_date": "2009-05-14T00:00:00-04:00", "title": "LRO L-14 Press Conference Supporting Videos", "description": "LRO From Launch to OrbitThis video starts with LRO launch animation, shows the spacecraft's path to orbit, and ends with the spacecraft animated over the lunar surface. || LRO_L14_LaunchtoOrbit_50sec_ipod00702_print.jpg (1024x576) [91.7 KB] || LRO_L14_LaunchtoOrbit_50sec_ipod_web.png (320x180) [156.1 KB] || LRO_L14_LaunchtoOrbit_50sec_fullres.webmhd.webm (960x540) [11.4 MB] || LRO_L14_LaunchtoOrbit_50sec_fullres.mov (1280x720) [30.0 MB] || LRO_L14_LaunchtoOrbit_50sec_ipod.m4v (640x360) [8.8 MB] || LRO_L14_LaunchtoOrbit_50sec_svs.mpg (512x288) [7.6 MB] || LRO_L14_LaunchtoOrbit_50sec_portal.wmv (346x260) [7.1 MB] || LRO_L14_LaunchtoOrbit_50sec_fullres.mov.hwshow [218 bytes] || ", "hits": 16 }, { "id": 40056, "url": "https://svs.gsfc.nasa.gov/gallery/ionosphere/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "Ionosphere", "description": "No description available.", "hits": 20 }, { "id": 40352, "url": "https://svs.gsfc.nasa.gov/gallery/exoplanets/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "Exoplanets", "description": "An exoplanet is a planet orbiting a star other than the Sun. Of particular interest are planets that may orbit in their star’s habitable zone, the distance from a star where temperatures allow liquid water to persist on a planet’s surface, given a suitable atmosphere. Since water is necessary for life as we know it, its presence is required for worlds to be considered capable of supporting life. Exoplanets can also teach us more about planets in the universe, such as the diversity of planets in the galaxy, how they interact with their host stars and with each other, and how common solar systems like ours really are.\n \nUsing a wide variety of methods, astronomers have discovered more than 3,700 exoplanets to date, largely thanks to NASA's Kepler/K2 mission.\n \nOther NASA missions also play a key role in detecting exoplanets. The Transiting Exoplanet Survey Satellite, which launched in April 2018, will monitor 200,000 of the brightest dwarf stars for transiting exoplanets. Future missions like the James Webb Space Telescope will be able to study these discovered planets in greater detail, helping determine their composition. \n \nResearchers in NASA Goddard Space Flight Center's Sellers Exoplanet Environments Collaboration are leveraging work across disciplines to better understand exoplanets. Areas like planet-star interactions, planetary formation, and even study of the Earth itself enable researchers to develop tools to learn more about how exoplanets evolve, and what ingredients are necessary to support life.", "hits": 568 } ] }