Saturn's rings - A photometric study of ring C

Statistics – Computation

Scientific paper

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Astronomical Photometry, Optical Properties, Saturn Rings, Luminous Intensity, Photographic Recording, Point Sources, Ring Structures

Scientific paper

A simple computational procedure is proposed for determining the true photometric profile of ring C using the spread function obtained from the satellite Dione and also slightly overexposed photographs of Saturn. No trace of a faint additional ring between ring C and the disk was found. The decreasing part, toward the planet, of the recorded photometric profile of ring C exhibits a slight depression tentatively attributed to a new division.

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