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Original animation: HERE
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Credit: NASA's Goddard Space Flight Center/CI Lab", "items": [ { "id": 273812, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436693, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/HMXB_Cam1_00611.png", "filename": "HMXB_Cam1_00611.png", "media_type": "Image", "alt_text": "Illustration of a pulsar orbiting a massive star, forming a high-mass X-ray binary.Credit: NASA's Goddard Space Flight Center/CI Lab", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 273813, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436694, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/HMXB_Cam1_00611_print.jpg", "filename": "HMXB_Cam1_00611_print.jpg", "media_type": "Image", "alt_text": "Illustration of a pulsar orbiting a massive star, forming a high-mass X-ray binary.Credit: NASA's Goddard Space Flight Center/CI Lab", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 439365, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335375, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335375", "widget": "Single image", "title": "", "caption": "", "description": "Illustration of a binary system where a pulsar is slowly evaporating its stellar companion.
Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "items": [ { "id": 273815, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436696, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/BW_topX_00038-1080_print.jpg", "filename": "BW_topX_00038-1080_print.jpg", "media_type": "Image", "alt_text": "Illustration of a binary system where a pulsar is slowly evaporating its stellar companion.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 273814, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436695, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/BW_topX_00038-1080.tif", "filename": "BW_topX_00038-1080.tif", "media_type": "Image", "alt_text": "Illustration of a binary system where a pulsar is slowly evaporating its stellar companion.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439366, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335376, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335376", "widget": "Single image", "title": "", "caption": "", "description": "Multiwavelength image of supernova remnant IC 443.
Credit: NASA/DOE/Fermi LAT Collaboration, NOAO/AURA/NSF, JPL-Caltech/UCLA", "items": [ { "id": 273816, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436697, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/SNR_graphic.jpg", "filename": "SNR_graphic.jpg", "media_type": "Image", "alt_text": "Multiwavelength image of supernova remnant IC 443.Credit: NASA/DOE/Fermi LAT Collaboration, NOAO/AURA/NSF, JPL-Caltech/UCLA", "width": 800, "height": 450, "pixels": 360000 } }, { "id": 439367, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335377, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335377", "widget": "Single image", "title": "", "caption": "", "description": "Multiwavelength image of galaxy M82.
Credit:NASA/JPL-Caltech/STScI/CXC/UofA/ESA/AURA/JHU", "items": [ { "id": 273817, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436698, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/SBG_M82_Multi-Spectrum_1080.jpg", "filename": "SBG_M82_Multi-Spectrum_1080.jpg", "media_type": "Image", "alt_text": "Multiwavelength image of galaxy M82.Credit:NASA/JPL-Caltech/STScI/CXC/UofA/ESA/AURA/JHU", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439368, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335378, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335378", "widget": "Single image", "title": "", "caption": "", "description": "Globular clusters are ancient groupings of stars that orbit our galaxy. This view of globular cluster NGC 6624 was imaged by the NASA's Hubble Space Telescope. The cluster is 27,000 light-years away and lies farther than the center of our galaxy in the constellation Sagittarius.
Credit: NASA/ESA/I. King, Univ. of Calif., Berkeley/Wikisky.org", "items": [ { "id": 273818, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436699, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/GC_NGC_6634_1080.jpg", "filename": "GC_NGC_6634_1080.jpg", "media_type": "Image", "alt_text": "Globular clusters are ancient groupings of stars that orbit our galaxy. This view of globular cluster NGC 6624 was imaged by the NASA's Hubble Space Telescope. The cluster is 27,000 light-years away and lies farther than the center of our galaxy in the constellation Sagittarius.Credit: NASA/ESA/I. King, Univ. of Calif., Berkeley/Wikisky.org", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439369, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335379, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335379", "widget": "Single image", "title": "", "caption": "", "description": "Chandra and Hubble image of the Crab Nebula's central region, where the pulsar is located.
Credit: NASA/HST/CXC/ASU/J. Hester et al.", "items": [ { "id": 273819, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436700, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/PWN_Chandra_Hubble-crab_CLOSE_1080.jpg", "filename": "PWN_Chandra_Hubble-crab_CLOSE_1080.jpg", "media_type": "Image", "alt_text": "Chandra and Hubble image of the Crab Nebula's central region, where the pulsar is located.Credit: NASA/HST/CXC/ASU/J. Hester et al.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439370, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335380, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335380", "widget": "Single image", "title": "", "caption": "", "description": "This image is a view of the Sun captured by NASA’s Solar Dynamics Observatory on Oct. 7, 2010, while partially obscured by the Moon. A close look at the crisp horizon of the Moon against the Sun shows the outline of lunar mountains. A model of the Moon from NASA’s Lunar Reconnaissance Orbiter has been inserted into the picture, showing how perfectly the Moon's true topology fits into the shadow observed by SDO.
Credit: NASA/SDO/LRO/GSFC", "items": [ { "id": 273820, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436701, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Sun_Moon_1080.jpg", "filename": "Sun_Moon_1080.jpg", "media_type": "Image", "alt_text": "This image is a view of the Sun captured by NASA’s Solar Dynamics Observatory on Oct. 7, 2010, while partially obscured by the Moon. A close look at the crisp horizon of the Moon against the Sun shows the outline of lunar mountains. A model of the Moon from NASA’s Lunar Reconnaissance Orbiter has been inserted into the picture, showing how perfectly the Moon's true topology fits into the shadow observed by SDO.Credit: NASA/SDO/LRO/GSFC", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439371, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335381, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335381", "widget": "Single image", "title": "", "caption": "", "description": "Illustration of a pulsar producing narrow radio beams (green), which do not intersect Earth, and broad gamma ray emission (magenta) that does.
Credit: NASA/Fermi/Cruz deWilde", "items": [ { "id": 273821, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436702, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/pulsar_1920x1080_0759.png", "filename": "pulsar_1920x1080_0759.png", "media_type": "Image", "alt_text": "Illustration of a pulsar producing narrow radio beams (green), which do not intersect Earth, and broad gamma ray emission (magenta) that does.Credit: NASA/Fermi/Cruz deWilde", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 273822, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436703, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/pulsar_1920x1080_0759_print.jpg", "filename": "pulsar_1920x1080_0759_print.jpg", "media_type": "Image", "alt_text": "Illustration of a pulsar producing narrow radio beams (green), which do not intersect Earth, and broad gamma ray emission (magenta) that does.Credit: NASA/Fermi/Cruz deWilde", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 439372, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335382, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335382", "widget": "Single image", "title": "", "caption": "", "description": "Illustration of a binary system where a pulsar is slowly destroying its small binary companion.
Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "items": [ { "id": 273823, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436704, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Cruz_deWilde-bwPulsar_persp.01094-bigjpg.jpg", "filename": "Cruz_deWilde-bwPulsar_persp.01094-bigjpg.jpg", "media_type": "Image", "alt_text": "Illustration of a binary system where a pulsar is slowly destroying its small binary companion.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 335383, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335383", "widget": "Single image", "title": "", "caption": "", "description": "Image of a portion of the Large Magellanic Cloud with Fermi gamma-ray imagery showing bright sources centered on the Tarantuala Nebula.
Credit: C. Smith, S. Points, the MCELS Team, NOAO/AURA/NSF and NASA/DOE/Fermi LAT Collaboration", "items": [ { "id": 273824, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436705, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/LMC_Pulsar_Multi.jpg", "filename": "LMC_Pulsar_Multi.jpg", "media_type": "Image", "alt_text": "Image of a portion of the Large Magellanic Cloud with Fermi gamma-ray imagery showing bright sources centered on the Tarantuala Nebula.Credit: C. Smith, S. Points, the MCELS Team, NOAO/AURA/NSF and NASA/DOE/Fermi LAT Collaboration", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439373, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335384, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335384", "widget": "Single image", "title": "", "caption": "", "description": "Fermi data from the center of the Milky Way superimposed over a visible light image of the same region.
Credit: NASA Goddard/A. Mellinger (Central Michigan Univ.) and T. Linden (Univ. of Chicago)", "items": [ { "id": 273825, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436706, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Dark_Matter_Final_Frame.png", "filename": "Dark_Matter_Final_Frame.png", "media_type": "Image", "alt_text": "Fermi data from the center of the Milky Way superimposed over a visible light image of the same region.Credit: NASA Goddard/A. Mellinger (Central Michigan Univ.) and T. Linden (Univ. of Chicago)", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 273826, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436707, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Dark_Matter_Final_Frame_print.jpg", "filename": "Dark_Matter_Final_Frame_print.jpg", "media_type": "Image", "alt_text": "Fermi data from the center of the Milky Way superimposed over a visible light image of the same region.Credit: NASA Goddard/A. Mellinger (Central Michigan Univ.) and T. Linden (Univ. of Chicago)", "width": 1024, "height": 576, "pixels": 589824 } } ], "extra_data": {} }, { "id": 335385, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335385", "widget": "Single image", "title": "", "caption": "", "description": "Illustration of one possible model for the dramatic changes observed from J1023. The two stars of AY Sextantis orbit closely enough that a stream of gas flows from the sun-like star toward the pulsar. The pulsar's rapid rotation and intense magnetic field produce both the radio beam and the high-energy wind, which is eroding its companion. When the radio beam (green) is detectable, the pulsar wind holds back the companion's gas stream, preventing it from approaching too closely.
Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "items": [ { "id": 273827, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436708, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Transformer_pulsar_gif_Still_2.png", "filename": "Transformer_pulsar_gif_Still_2.png", "media_type": "Image", "alt_text": "Illustration of one possible model for the dramatic changes observed from J1023. The two stars of AY Sextantis orbit closely enough that a stream of gas flows from the sun-like star toward the pulsar. The pulsar's rapid rotation and intense magnetic field produce both the radio beam and the high-energy wind, which is eroding its companion. When the radio beam (green) is detectable, the pulsar wind holds back the companion's gas stream, preventing it from approaching too closely.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 273828, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436709, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Transformer_pulsar_gif_Still_2_print.jpg", "filename": "Transformer_pulsar_gif_Still_2_print.jpg", "media_type": "Image", "alt_text": "Illustration of one possible model for the dramatic changes observed from J1023. The two stars of AY Sextantis orbit closely enough that a stream of gas flows from the sun-like star toward the pulsar. The pulsar's rapid rotation and intense magnetic field produce both the radio beam and the high-energy wind, which is eroding its companion. When the radio beam (green) is detectable, the pulsar wind holds back the companion's gas stream, preventing it from approaching too closely.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 439374, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335386, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335386", "widget": "Single image", "title": "", "caption": "", "description": "The white dwarf star in V407 Cygni, shown here in an artist's concept, went nova in 2010. Scientists think the outburst primarily emitted gamma rays (magenta) as the blast wave plowed through the gas-rich environment near the system's red giant star.
Credit: NASA's Goddard Space Flight Center/S. Wiessinger", "items": [ { "id": 273829, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436710, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/V407_Cyg_Nova_Final_1080crop.jpg", "filename": "V407_Cyg_Nova_Final_1080crop.jpg", "media_type": "Image", "alt_text": "The white dwarf star in V407 Cygni, shown here in an artist's concept, went nova in 2010. Scientists think the outburst primarily emitted gamma rays (magenta) as the blast wave plowed through the gas-rich environment near the system's red giant star. Credit: NASA's Goddard Space Flight Center/S. Wiessinger", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439375, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335387, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335387", "widget": "Single image", "title": "", "caption": "", "description": "Illustration of a binary system where a pulsar is slowly destroying its small binary companion.
Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "items": [ { "id": 273830, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 436711, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/Cruz_deWilde-bwPulsar_pulsarCam.00300-close.jpg", "filename": "Cruz_deWilde-bwPulsar_pulsarCam.00300-close.jpg", "media_type": "Image", "alt_text": "Illustration of a binary system where a pulsar is slowly destroying its small binary companion.Credit: NASA's Goddard Space Flight Center/Cruz deWilde", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 439376, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1101024, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012101/fermi-1-13-SplashScreen.hwshow", "filename": "fermi-1-13-SplashScreen.hwshow", "media_type": "HyperwallShow", "alt_text": "", "width": 0, "height": 0, "pixels": null } } ], "extra_data": {} }, { "id": 335388, "url": "https://svs.gsfc.nasa.gov/12101/#media_group_335388", "widget": "Single image", "title": "", "caption": "", "description": "The Fermi logo.
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