Credit: NASA/JIm Grossmann", "items": [ { "id": 273834, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436715, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_2_Instruments_5760_print.jpg", "filename": "Fermi_Hyperwall_2_2_Instruments_5760_print.jpg", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi Gamma-ray Space Telescope with instruments labeled.Credit: NASA/JIm Grossmann", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273833, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436714, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_2_Instruments_5760.png", "filename": "Fermi_Hyperwall_2_2_Instruments_5760.png", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi Gamma-ray Space Telescope with instruments labeled.Credit: NASA/JIm Grossmann", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 439378, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101025, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/fermi-2-2-Instruments.hwshow", "filename": "fermi-2-2-Instruments.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335391, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335391", "widget": "Basic text with HTML", "title": "", "caption": "", "description": "For additional Fermi hyperwall visuals please check the second hyperwall page
", "items": [], "extra_data": {} }, { "id": 335393, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335393", "widget": "Video player", "title": "", "caption": "", "description": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears.
Credit: NASA's Goddard Space Flight Center", "items": [ { "id": 273840, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436717, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/frame-001216_print.jpg", "filename": "frame-001216_print.jpg", "media_type": "Image", "alt_text": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA's Goddard Space Flight Center", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273838, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436721, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/GRB_mkII-HD_1080p.webm", "filename": "GRB_mkII-HD_1080p.webm", "media_type": "Movie", "alt_text": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA's Goddard Space Flight Center", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 273839, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436720, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/GRB_mkII-HD_1080p.mov", "filename": "GRB_mkII-HD_1080p.mov", "media_type": "Movie", "alt_text": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. 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These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA's Goddard Space Flight Center", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 273837, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436718, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/GRB_4k_mkII-4K.mov", "filename": "GRB_4k_mkII-4K.mov", "media_type": "Movie", "alt_text": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA's Goddard Space Flight Center", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 273835, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436719, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/GRB_4k_mkII_ProRes.mov", "filename": "GRB_4k_mkII_ProRes.mov", "media_type": "Movie", "alt_text": "Gamma-ray bursts are the most luminous explosions in the cosmos. Astronomers think most occur when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA's Goddard Space Flight Center", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 335394, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335394", "widget": "Single image", "title": "", "caption": "", "description": "Up-resed, UHD-resolution artist's conception of an active galactic nucleus.
Original animation: HERE
Credit: NASA's Goddard Space Flight Center/CI Lab", "items": [ { "id": 273842, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436722, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/AGN_00526_print.jpg", "filename": "AGN_00526_print.jpg", "media_type": "Image", "alt_text": "Up-resed, UHD-resolution artist's conception of an active galactic nucleus.Original animation: HERECredit: NASA's Goddard Space Flight Center/CI Lab", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273841, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436723, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/frames/3840x2160_16x9_30p/AGN/", "filename": "AGN", "media_type": "Frames", "alt_text": "Up-resed, UHD-resolution artist's conception of an active galactic nucleus.Original animation: HERECredit: NASA's Goddard Space Flight Center/CI Lab", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 335395, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335395", "widget": "Single image", "title": "", "caption": "", "description": "Up-resed, UHD resolution artist's conception that tracks several gamma rays through space and time, from their emission in the jet of a distant blazar to their arrival in Fermi's Large Area Telescope (LAT). During their journey, the number of randomly moving ultraviolet and optical photons (blue) increases as more and more stars are born in the universe. Eventually, one of the gamma rays encounters a photon of starlight and the gamma ray transforms into an electron and a positron. The remaining gamma-ray photons arrive at Fermi, interact with tungsten plates in the LAT, and produce the electrons and positrons whose paths through the detector allows astronomers to backtrack the gamma rays to their source.
Original animation: HERE
Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "items": [ { "id": 273844, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436725, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/blazarFinal_cdewilde.01847_print.jpg", "filename": "blazarFinal_cdewilde.01847_print.jpg", "media_type": "Image", "alt_text": "Up-resed, UHD resolution artist's conception that tracks several gamma rays through space and time, from their emission in the jet of a distant blazar to their arrival in Fermi's Large Area Telescope (LAT). During their journey, the number of randomly moving ultraviolet and optical photons (blue) increases as more and more stars are born in the universe. Eventually, one of the gamma rays encounters a photon of starlight and the gamma ray transforms into an electron and a positron. The remaining gamma-ray photons arrive at Fermi, interact with tungsten plates in the LAT, and produce the electrons and positrons whose paths through the detector allows astronomers to backtrack the gamma rays to their source.Original animation: HERECredit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273843, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436724, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/frames/3840x2160_16x9_60p/EBL/", "filename": "EBL", "media_type": "Frames", "alt_text": "Up-resed, UHD resolution artist's conception that tracks several gamma rays through space and time, from their emission in the jet of a distant blazar to their arrival in Fermi's Large Area Telescope (LAT). During their journey, the number of randomly moving ultraviolet and optical photons (blue) increases as more and more stars are born in the universe. Eventually, one of the gamma rays encounters a photon of starlight and the gamma ray transforms into an electron and a positron. The remaining gamma-ray photons arrive at Fermi, interact with tungsten plates in the LAT, and produce the electrons and positrons whose paths through the detector allows astronomers to backtrack the gamma rays to their source.Original animation: HERECredit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 335396, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335396", "widget": "Single image", "title": "", "caption": "", "description": "UHD-resolution sequence of the Centaurus A radio galaxy and a radio image of the central black hole's jet.
Original animation: HERE
Credit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray); NASA/TANAMI/Müller et al. (jet)", "items": [ { "id": 273846, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436726, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/frame-001117_print.jpg", "filename": "frame-001117_print.jpg", "media_type": "Image", "alt_text": "UHD-resolution sequence of the Centaurus A radio galaxy and a radio image of the central black hole's jet.Original animation: HERECredit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray); NASA/TANAMI/Müller et al. (jet)", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273845, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436727, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/frames/3840x2160_16x9_30p/Radio/", "filename": "Radio", "media_type": "Frames", "alt_text": "UHD-resolution sequence of the Centaurus A radio galaxy and a radio image of the central black hole's jet.Original animation: HERECredit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray); NASA/TANAMI/Müller et al. (jet)", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 335397, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335397", "widget": "Single image", "title": "", "caption": "", "description": "Composite image of Centaurus A in radio, optical and gamma-ray light.
Credit: Capella Observatory (optical), with radio data from Ilana Feain, Tim Cornwell, and Ron Ekers (CSIRO/ATNF), R. Morganti (ASTRON), and N. Junkes (MPIfR).", "items": [ { "id": 273848, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436729, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/437997main_CenA_radio_optical_gamma_composite_labeled_print.jpg", "filename": "437997main_CenA_radio_optical_gamma_composite_labeled_print.jpg", "media_type": "Image", "alt_text": "Composite image of Centaurus A in radio, optical and gamma-ray light.Credit: Capella Observatory (optical), with radio data from Ilana Feain, Tim Cornwell, and Ron Ekers (CSIRO/ATNF), R. Morganti (ASTRON), and N. Junkes (MPIfR).", "width": 1024, "height": 1340, "pixels": 1372160 } }, { "id": 273847, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436728, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/437997main_CenA_radio_optical_gamma_composite_labeled.jpg", "filename": "437997main_CenA_radio_optical_gamma_composite_labeled.jpg", "media_type": "Image", "alt_text": "Composite image of Centaurus A in radio, optical and gamma-ray light.Credit: Capella Observatory (optical), with radio data from Ilana Feain, Tim Cornwell, and Ron Ekers (CSIRO/ATNF), R. Morganti (ASTRON), and N. Junkes (MPIfR).", "width": 1963, "height": 2570, "pixels": 5044910 } }, { "id": 439379, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101026, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/fermi-5x3-radio.hwshow", "filename": "fermi-5x3-radio.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335398, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335398", "widget": "Single image", "title": "", "caption": "", "description": "Various images of the Large Magellanic Cloud, a dwarf galaxy that houses several bright gamma-ray pulsars.
Credits, (clockwise from right):
NASA/JPL-Caltech/M. Meixner (STScI), the SAGE Legacy Team and NASA/DOE/Fermi LAT Collaboration
C. Smith, S. Points, the MCELS Team, NOAO/AURA/NSF and NASA/DOE/Fermi LAT Collaboration
NASA/DOE/Fermi LAT Collaboration
Axel Mellinger, Central Michigan University", "items": [ { "id": 273850, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436731, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_8_Dwarf_5760_print.jpg", "filename": "Fermi_Hyperwall_2_8_Dwarf_5760_print.jpg", "media_type": "Image", "alt_text": "Various images of the Large Magellanic Cloud, a dwarf galaxy that houses several bright gamma-ray pulsars.Credits, (clockwise from right): NASA/JPL-Caltech/M. Meixner (STScI), the SAGE Legacy Team and NASA/DOE/Fermi LAT Collaboration C. Smith, S. Points, the MCELS Team, NOAO/AURA/NSF and NASA/DOE/Fermi LAT CollaborationNASA/DOE/Fermi LAT CollaborationAxel Mellinger, Central Michigan University", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273849, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436730, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_8_Dwarf_5760.png", "filename": "Fermi_Hyperwall_2_8_Dwarf_5760.png", "media_type": "Image", "alt_text": "Various images of the Large Magellanic Cloud, a dwarf galaxy that houses several bright gamma-ray pulsars.Credits, (clockwise from right): NASA/JPL-Caltech/M. Meixner (STScI), the SAGE Legacy Team and NASA/DOE/Fermi LAT Collaboration C. Smith, S. Points, the MCELS Team, NOAO/AURA/NSF and NASA/DOE/Fermi LAT CollaborationNASA/DOE/Fermi LAT CollaborationAxel Mellinger, Central Michigan University", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 439380, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101027, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/fermi-2-8-Dwarf.hwshow", "filename": "fermi-2-8-Dwarf.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335399, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335399", "widget": "Single image", "title": "", "caption": "", "description": "3x3 hyperwall-resolution image of the Fermi bubbles.
Credit: NASA/DOE/Fermi LAT Collaboration", "items": [ { "id": 273852, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436733, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_9_BubblesTemp_5k_print.jpg", "filename": "Fermi_Hyperwall_2_9_BubblesTemp_5k_print.jpg", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi bubbles.Credit: NASA/DOE/Fermi LAT Collaboration", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273851, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436732, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_9_BubblesTemp_5k.png", "filename": "Fermi_Hyperwall_2_9_BubblesTemp_5k.png", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi bubbles.Credit: NASA/DOE/Fermi LAT Collaboration", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 273853, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436734, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_9_BubblesTemp_5k_searchweb.png", "filename": "Fermi_Hyperwall_2_9_BubblesTemp_5k_searchweb.png", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi bubbles.Credit: NASA/DOE/Fermi LAT Collaboration", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 273854, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436735, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_9_BubblesTemp_5k_thm.png", "filename": "Fermi_Hyperwall_2_9_BubblesTemp_5k_thm.png", "media_type": "Image", "alt_text": "3x3 hyperwall-resolution image of the Fermi bubbles.Credit: NASA/DOE/Fermi LAT Collaboration", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 439381, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101028, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/fermi-2-9-Bubbles.hwshow", "filename": "fermi-2-9-Bubbles.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335400, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335400", "widget": "Single image", "title": "", "caption": "", "description": "Illustrations of a white dwarf star going nova in a binary with a red giant, and a white dwarf star going nova in a more classic binary with a sun-like star.
Credit: NASA's Goddard Space Flight Center/S. Wiessinger", "items": [ { "id": 273856, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436737, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_10_Novae_5k_print.jpg", "filename": "Fermi_Hyperwall_2_10_Novae_5k_print.jpg", "media_type": "Image", "alt_text": "Illustrations of a white dwarf star going nova in a binary with a red giant, and a white dwarf star going nova in a more classic binary with a sun-like star.Credit: NASA's Goddard Space Flight Center/S. Wiessinger", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273855, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436736, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/Fermi_Hyperwall_2_10_Novae_5k.png", "filename": "Fermi_Hyperwall_2_10_Novae_5k.png", "media_type": "Image", "alt_text": "Illustrations of a white dwarf star going nova in a binary with a red giant, and a white dwarf star going nova in a more classic binary with a sun-like star.Credit: NASA's Goddard Space Flight Center/S. Wiessinger", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 439382, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101029, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012102/fermi-2-10-Novae.hwshow", "filename": "fermi-2-10-Novae.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335401, "url": "https://svs.gsfc.nasa.gov/12102/#media_group_335401", "widget": "Single image", "title": "", "caption": "", "description": "Up-resed, UHD-resolution illustration of a so-called \"black widow\" pulsar binary.
Original animation: HERE
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Original animation: HERE
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