File:Saturns Northern Aurora in Motion.gif
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Saturns_Northern_Aurora_in_Motion.gif (352 × 288 pixels, file size: 5.77 MB, MIME type: image/gif, looped, 601 frames, 18 s)
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[edit]DescriptionSaturns Northern Aurora in Motion.gif |
English: An aurora, shining high above the northern part of Saturn, moves from the night side to the day side of the planet in this animation recorded by Cassini. These observations, taken over four days, represent the first visible-light video of Saturn's auroras. They show tall auroral curtains, rapidly changing over time when viewed at the limb, or edge, of the planet's northern hemisphere. The sequence of images also reveals that Saturn's auroral curtains, the sheet-like formations of light-emitting atmospheric molecules, stretch up along Saturn's magnetic field and reach heights of more than 1,200 kilometres above the planet's limb. These are the tallest known “northern lights” in the solar system. These auroral displays are created by charged particles from the magnetosphere that plunge into the planet's upper atmosphere and cause it to glow. The magnetosphere is the region of electrically charged particles that are trapped in the magnetic field of the planet. The auroral curtains shown in the animation reveal the paths that these charged particles take as they flow along lines of the magnetic field between the planet's magnetosphere and ionosphere. The day side of Saturn scatters light toward Cassini, creating the overexposed triangle at the centre of the left of the frame. Stars can be seen above the limb of the planet, trailing across the field of view. The images for the animation were captured in black and white, but the aurora in the animation is shown in a false orange colour to distinguish it from background noise in the images. The images were processed to remove cosmic ray hits, bad pixels and lens flare. On Earth, auroras often appear green, but scientists do not yet know the colour of auroras on Saturn. Auroras on Saturn, like those on Earth, appear mostly in the high latitudes near the planet's poles. The auroras can be seen moving with the planet's rotation along the curved path of about 74 degrees north latitude. They change shape and brightness in a manner similar to terrestrial auroras. The aurora curtains become particularly bright when they are projected edge-on to Cassini as they pass over the limb from the near (dark) side to the far (bright) side of Saturn. Near the end of the animation, a snake-shaped aurora footprint brightens abruptly and fades over about five frames. |
Date | |
Source | NASA Cassini |
Author | NASA Cassini |
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The animation consists of 472 images taken during an 81-hour period. Each image was obtained with a two- or three-minute exposure. These images were taken in visible light with the Cassini spacecraft's narrow-angle camera. The view was acquired at a distance of approximately 2.8 million kilometres from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 111 degrees. Image scale is 32 kilometres per pixel.
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[edit]Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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current | 12:39, 26 November 2009 | 352 × 288 (5.77 MB) | Originalwana (talk | contribs) | {{Information |Description={{en|1=An aurora, shining high above the northern part of Saturn, moves from the night side to the day side of the planet in this animation recorded by Cassini. These observations, taken over four d |
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