
Saturns Dynamic Aurora #1

by Science Source
Title
Saturns Dynamic Aurora #1
Artist
Science Source
Medium
Photograph - Photograph
Description
These images reveal the dynamic nature of Saturn's auroras. Viewing the planet's southern polar region for several days, NASA's Hubble Space Telescope snapped a series of photographs of the aurora dancing in the sky. The snapshots show that Saturn's auroras differ in character from day to day, as they do on Earth, moving around on some days and remaining stationary on others. But compared with Earth, where auroral storms develop in about 10 minutes and may last for a few hours, Saturn's auroral displays always appear bright and may last for several days. The observations, made by Hubble and the Cassini spacecraft, while enroute to the planet, suggest that Saturn's auroral storms are driven mainly by the pressure of the solar wind rather than by the Sun's magnetic field. The aurora's strong brightening on January 28, 2004 corresponds with the recent arrival of a large disturbance in the solar wind. The image shows that when Saturn's auroras become brighter (and thus more powerful), the ring of light encircling the pole shrinks in diameter. Astronomers combined ultraviolet images of Saturn's southern polar region with visible-light images of the planet and its rings to make this picture. The auroral display appears blue because of the glow of ultraviolet light. In reality, the aurora would appear red to an observer at Saturn because of the presence of glowing hydrogen in the atmosphere. The ultraviolet images were taken on January 24, 26, and 28, 2004 by Hubble's Space Telescope Imaging Spectrograph. The visible-light images were acquired using the telescope's Advanced Camera for Surveys on March 22, 2004.
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December 2nd, 2015
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