CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Anthe's Faint Arc
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Anthe's Faint Arc
PIA 11100

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  Cassini images reveal the existence of a faint arc of material orbiting with Saturn's small moon Anthe.

The moon is moving in a counterclockwise direction in this perspective, and is about to reach the ansa -- the point of maximum elongation -- as seen by the viewer, in its curving path around Saturn. In this image, most of the visible material in the arc lies ahead of Anthe (2 kilometers, 1 mile across) in its orbit. However, over time the moon drifts slowly back and forth with respect to the arc. Also ahead of the moon is a dark channel where the arc appears split into two strands, and these then merge farther around the orbital path.

The arc extends over about 20 degrees in longitude (about 5.5 percent of Anthe's orbit) and appears to be associated with a gravitational resonance caused by Mimas. Micrometeoroid impacts on Anthe are the likely source of the arc material.

The orbit of Anthe lies between the larger moons Mimas and Enceladus. Anthe shares this region with two other small moons, Pallene (4 kilometers, 3 mile across) and Methone (3 kilometers, 2 mile across). Methone also possesses an arc (see PIA11102), while Pallene is known to orbit within a faint, complete ring of its own (see PIA08328).

Cassini imaging scientists believe the process that maintains the Anthe and Methone arcs is similar to that which maintains the arc in the G ring (see PIA08327).

This view looks toward the unilluminated side of the rings from about 3 degrees above the ringplane. The view has been rotated so that Saturn's north pole would point upward.

The general brightness of the image (along with the faint horizontal and vertical banding pattern) results from the long exposure time of 32 seconds required to capture the extremely faint ring arc and the processing needed to enhance its visibility (which also enhances the digital background noise in the image). The image was digitally processed to remove most of the background noise. The long exposure also produced star trails in the background.

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 4, 2008. The view was acquired at a distance of approximately 1.2 million kilometers (746,000 miles) from Anthe and at a Sun-Anthe-spacecraft, or phase, angle of 23 degrees. Image scale is 7 kilometers (4 miles) per pixel.

The Cassini Equinox Mission is a joint United States and European endeavor. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini Equinox Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

Credit: NASA/JPL/Space Science Institute
Released: September 5, 2008 (PIA 11100)
Image/Caption Information


Alliance Member Comments
Crystal (Sep 10, 2008 at 1:42 AM):
Sergio,

There seems to be an explanation here.

http://ciclops.org/view.php?id=5152
Sergio (Sep 7, 2008 at 4:26 PM):
Why this image is so noisy after a digital clean-up process ?
Could be possible to see the "darks" of the CCDs ?
I knew that in the deep space the environmental operational conditions are the best possible for CCDs, aren't they ?
The temperature is the coldest that it can be ever obtainable for the CCDs, the background is the darker that one could only hope to see in a whole life... Can you tell me something ?
Thanks in advance for any precious information about.
However is a great image.

PS
Do you have published a collection of "darks" somewhere on the site, just to play with "cleaning" mathematics ?

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