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Inner B-Ring "Terminus" and Spiral Corrugation
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Caption NASA:"This mosaic of Cassini images, part of a larger mosaic of images captured just hours before exact Equinox at Saturn, shows that the "Spiral Corrugation" in the Planet’s Inner Rings continues right up to the inner B-Ring: an unexpected result that scientists are working to understand.
The inner B-Ring boundary is visible on the right. The C-Ring’s Maxwell Gap, demarcated by two bright arcs in this view, is on the left.
The larger mosaic shows a gently undulating pattern stretching from the D-Ring to inner B-Ring (see PIA11670).
An earlier mosaic, captured in June, showed the corrugation extending only as far as the middle of the C-Ring (see PIA11664).
The periodic brightness variations in this corrugation are most likely caused by the changing slopes in the rippled Ring-Plane, much like the corrugations of a tin roof. Although previous Cassini observations (see PIA08325) had revealed corrugations in the D-Ring extending over 500 miles (about 800 Km), this image now shows these features extending beyond their origin in the D-Ring for 11.000 miles (approx. 17.000 Km) into the C-Ring.
This new imagery supports earlier evidence that something happened in the early 1980s to generate this feature.
In 2006, imaging scientists speculated that a collision with a comet or asteroid may have disturbed the D-Ring. That explanation seems less likely now that this new image shows the effect spread over a much broader radial range, extending completely across the C-Ring, and scientists are continuing to investigate the cause of this disturbance.
Whatever created the corrugation apparently tilted a vast region of the Inner Rings relative to Saturn’s gravitational field in a relatively short period of time during the early 1980s.
In the intervening years, the natural tendency for inclined orbits to systematically and slowly wobble at different rates, depending on their distance from Saturn, has created a tightly wound spiral corrugation in the Ring-Plane.
This view and others like it are only possible around the time of Saturn’s Equinox which occurs every half-Saturn-year (equivalent to about 15 Earth years). Exact Equinox is when the Sun is directly overhead at the Equator. The illumination geometry that accompanies equinox lowers the Sun’s angle to the Ring-Plane, significantly darkens the Rings and causes out-of-plane structures to cast long shadows across the Rings.
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 southern side of the Rings from about 4° below the Ring-Plane. Background stars are visible shining through the Rings, and the image has not been cleaned to remove Cosmic Rays, which struck the camera’s detector during the exposures.
The image was taken in Visible Light with the Cassini Spacecraft narrow-angle camera on Aug. 10, 2009. The view was acquired at a distance of approx. 888.000 Km (about 552.000 miles) from Saturn and at a Sun-Saturn-Spacecraft, or Phase, Angle of 157°.
Image scale is roughly 5 Km (a little more than 3 miles) per pixel".
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