The three spot detections in the movie were obtained by Cassini's ultraviolet imaging spectrograph at 8 p.m. and 9:20 p.m. PST on Aug. 25, 2008, and 1:02 a.m. PST on Aug. 26 (3 a.m., 4:20 a.m. and 8:02 a.m. UTC on Aug. 26), a period of time spanning five hours and two minutes. The footprint moved according to changes in the position of Enceladus. In the image, the colors represent how bright the extreme ultraviolet emissions are. The lowest emission areas (one to two extreme ultraviolet counts per pixel) are in black/blue. The brightest emission areas (500 to 1,000 extreme ultraviolet counts per pixel) are in yellow/white.
italian movie download Ultraviolet
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Credit: NASA's Goddard Space Flight Center/CI Lab Download Options 3840x2160 jpeg (2.8 MB)
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Right click images to download them if they automatically display in your browser. This illustration shows the hot, dense, expanding cloud of debris stripped from the neutron stars just before they collided. This cloud produces the kilonova's visible and infrared light. Within this neutron-rich debris, large quantities of some of the universe's heaviest elements were forged, including hundreds of Earth masses of gold and platinum. Credit: NASA's Goddard Space Flight Center/CI Lab Download Options 3840x2160 quicktime (888.0 MB) 59.94 fps ProRes version for Video Editors
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Right click movies to download them if they automatically play in your browser. After the neutron stars merged, the remains of the jets that produced the gamma-ray burst continue expanding into space, as shown in this illustration. After nine days, the jet directed toward us had spread laterally enough that observers could detect its X-ray emission.Credit: NASA's Goddard Space Flight Center/CI Lab Download Options 3840x2160 mpeg-4 (178.2 MB) 29.97 fps
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Right click movies to download them if they automatically play in your browser. This animation shows the shrinking orbit and explosive merging of two neutron stars, immediately followed by the eruption of powerful jets (orange) and then expanding shock waves where the jets plow into surrounding material (pink structures at the tip of each jet). The animation then shows the kilonova, the neutron-rich debris of the explosion (depicted by the expanding and flattened blue spheres) powered by the decay of newly forged radioactive elements. The jets emit gamma rays, the shock wave glows in X-rays and the kilonova produces ultraviolet light.Credit: NASA's Goddard Space Flight Center/CI LabMusic: "Exploding Skies" from Killer TracksComplete transcript available. 2ff7e9595c
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