Bright spokes and the shadow of a moon grace Saturn's B ring in this Cassini spacecraft image.
Spokes are radial markings scientists continue to study, and they can be seen here stretching from the far left to upper right of the image. Spokes appear bright when they are viewed at phase, or Sun-Saturn-spacecraft, angles higher than about 45 degrees. This image was taken at a phase angle of 50 degrees. See PIA11144 and PIA08288 to learn more.
The moon Mimas is not shown here, but its shadow appears on the rings near the top of the image. The novel illumination geometry that accompanies equinox lowers the sun's angle to the ringplane, significantly darkens the rings, and causes out-of-plane structures to look anomalously bright and cast shadows across the rings. These scenes are possible only during the few months before and after Saturn's equinox, which occurs only once in about 15 Earth years. Before and after equinox, Cassini's cameras have spotted not only the predictable shadows of some of Saturn's moons (see PIA11657), but also the shadows of newly revealed vertical structures in the rings themselves (see PIA11665).
This view looks toward the northern, sunlit side of the rings from about 9 degrees above the ringplane. The image was taken using a compression scheme that reduces the image file size on the spacecraft's data recorder, resulting in the rings' slightly pixelated appearance.
The image was taken in visible light with the Cassini spacecraft wide-angle camera on Jan. 11, 2010. The view was acquired at a distance of approximately 611,000 kilometers (380,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 50 degrees. Image scale is 66 kilometers (41 miles) per pixel.
Photo credit: NASA/JPL/Space Science Institute
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