Shadows are cast by Daphnis and the moon's attendant edge waves in this Cassini image taken about a month and a half before the Saturn's August 2009 equinox.
Daphnis (8 kilometers, 5 miles across) appears as a tiny bright dot in the Keeler Gap of the A ring near the center of the image. The moon has an inclined orbit and its gravitational pull perturbs the orbits of the particles of the A ring forming the Keeler Gap's edge and sculpts the edge into waves having both horizontal (radial) and out-of-plane components. Material on the inner edge of the gap orbits faster than the moon so that the waves there lead the moon in its orbit. Material on the outer edge moves slower than the moon, so waves there trail the moon. See PIA11656 to learn more about this process.
The Encke Gap of the A ring, wider than the Keeler Gap, can be seen on the left of the image. The thin F ring is on the far right. Numerous background stars are visible elongated by the motion of the spacecraft during the exposure.
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 southern, unilluminated side of the rings from about 53 degrees above the ringplane.
The image was taken in visible light with the Cassini spacecraft narrow-angle camera on June 28, 2009. The view was acquired at a distance of approximately 1.5 million kilometers (932,000 miles) from Daphnis and at a Sun-Daphnis-spacecraft, or phase, angle of 74 degrees. Image scale is 9 kilometers (6 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.