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This video features some of the scientists and engineers that work on Hubble, and how the Hubble Deep Field changed everything.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Compact galaxies in the Hubble Ultra Deep Field: Credit: ESA/Hubble (M. Kornmesser & L. L. Christensen)Pan of GOODS field containing distant dwarf galaxies forming stars at an incredible rate: Credit: NASA & ESAHubble: Galaxies Across Space and Time: Credit: NASA, ESA and F. Summers (STScI)Speedthrough of galaxies added to deep field image: Credit: NASA/CXC/SAO/K.Arcand; Sonification: @SYSTEMSounds (M. Russo, A. Santaguida)Music Credits: \"Earth’s Orbit\" by Andreas Andreas Bolldén [STIM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music.“Planetary Exploration” by Richard Andrew Canavan [PRS] via Sound Pocket Music [PRS], and Universal Production Music. || ", "release_date": "2021-08-02T09:55:00-04:00", "update_date": "2023-05-03T13:44:02.312765-04:00", "main_image": { "id": 377761, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013900/a013902/13902_DF_WIDE_PRINT.jpg", "filename": "13902_DF_WIDE_PRINT.jpg", "media_type": "Image", "alt_text": "Master VersionHorizontal version. 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Kornmesser (ESA/Hubble) || ", "release_date": "2021-05-07T09:55:00-04:00", "update_date": "2023-05-03T13:44:08.731110-04:00", "main_image": { "id": 378760, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013800/a013845/13845_GRAV_WIDE_PRINT.jpg", "filename": "13845_GRAV_WIDE_PRINT.jpg", "media_type": "Image", "alt_text": "Master VersionHorizontal version. This is for use on any YouTube or non-YouTube platform where you want to display the video horizontally.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 13713, "url": "https://svs.gsfc.nasa.gov/13713/", "page_type": "Produced Video", "title": "Hubble Makes Unexpected Dark Matter Discovery", "description": "Astronomers seem to have revealed a puzzling detail in the way dark matter behaves. 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About 80 percent of the matter in the universe is invisible to telescopes, yet its gravitational influence is manifest in the orbital speeds of stars around galaxies and in the motions of clusters of galaxies. Yet, despite decades of effort, no one knows what this \"dark matter\" really is. Many scientists think it's likely that the mystery will be solved with the discovery of new kinds of subatomic particles, types necessarily different from those composing atoms of the ordinary matter all around us. The search to detect and identify these particles is underway in experiments both around the globe and above it. Scientists working with data from NASA's Fermi Gamma-ray Space Telescope have looked for signals from some of these hypothetical particles by zeroing in on 10 small, faint galaxies that orbit our own. Although no signals have been detected, a novel analysis technique applied to two years of data from the observatory's Large Area Telescope (LAT) has essentially eliminated these particle candidates for the first time.WIMPs, or Weakly Interacting Massive Particles, represent a favored class of dark matter candidates. Some WIMPs may mutually annihilate when pairs of them interact, a process expected to produce gamma rays — the most energetic form of light — that the LAT is designed to detect. The team examined two years of LAT-detected gamma rays with energies in the range from 200 million to 100 billion electron volts (GeV) from 10 of the roughly two dozen dwarf galaxies known to orbit the Milky Way. Instead of analyzing the results for each galaxy separately, the scientists developed a statistical technique — they call it a \"joint likelihood analysis\" — that evaluates all of the galaxies at once without merging the data together. No gamma-ray signal consistent with the annihilations expected from four different types of commonly considered WIMP particles was found.For the first time, the results show that WIMP candidates within a specific range of masses and interaction rates cannot be dark matter. A paper detailing these results appeared in the Dec. 9, 2011, issue of Physical Review Letters. || ", "release_date": "2012-04-02T12:30:00-04:00", "update_date": "2023-11-14T00:18:38.335149-05:00", "main_image": { "id": 477680, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010900/a010943/test__left_00999.jpg", "filename": "test__left_00999.jpg", "media_type": "Image", "alt_text": "No one knows what dark matter is, but it constitutes 80 percent of the matter in our universe. By studying numerous dwarf galaxies — satellite systems that orbit our own Milky Way galaxy — NASA's Fermi Gamma-ray Space Telescope has produced some of the strongest limits yet on the nature of the hypothetical particles suspected of making up dark matter. Short, narrated video.Poster image, and dark matter simulations credit: Simulation: Wu, Hahn, Wechsler, Abel(KIPAC), Visualization: Kaehler (KIPAC)Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }