| November 2005
Cassini Mission Update:
Larry Esposito—This mosaic of 15 Cassini
images of the F ring shows how Prometheus
creates a gore (dark channel) in the ring once every 14.7
hours as it approaches and recedes from the
F ring on its eccentric orbit. The individual
images have been processed to make the
ring appear as if it has been straightened,
making it easier to see the ring’s structure. The
mosaic shows a region 147,000 kilometers
(91,000 miles) along the ring (horizontal direction
in the image); this represents about
60 degrees of longitude around the ring. The
region seen here is about 1,500 kilometers
(900 miles) across (vertical direction). The
first and last images in the mosaic were taken
approximately 2.5 hours apart. Each dark
channel, or “gore”, is clearly visible across
more than 1,000 kilometers (600 miles) of
the ring and is due to the gravitational effect
of Prometheus (102 kilometers, 63 miles
across), even though the moon does not
enter the F ring. The channels have different
tilts because the ring particles closer to
Prometheus (overexposed, stretched, and
just visible at the bottom right of the image)
move slower with respect to the moon than
those farther away. This causes the channels
to shear with time, their slopes becoming
greater, and gives the overall visual impression
of drapes of ring material. The channels
at right are the youngest and have near-vertical
slopes while those at the left are the
oldest and have near-horizontal slopes.
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