One good turn deserves another. I adore the consistent stream of imagery from the Saturnian system; these pictures offer us the ability to peer back in time, and to ponder what dynamic events have shaped these icy satellites as we view them today.

Continuing on the heels of the previous entry, the Cassini team has released another new look at Saturn’s moon Rhea, in false color — the second of its kind.

False color view of Rhea
Image Credit: NASA/JPL/Space Science Institute

Bright, wispy markings stretch across a region of darker terrain on Saturn’s moon Rhea. In this extreme false-color view, the roughly north-south fractures occur within strips of material (which appear greenish here) that are a different color from the surrounding cratered landscape.

To create the false-color view, ultraviolet, green and infrared images were combined into a single black and white picture that isolates and maps regional color differences. Most of the large-scale variations in brightness across the surface are removed by this process. This “color map” was then superimposed over a clear-filter image.

The origin of the color differences is not yet understood, but it may be caused by subtle differences in the surface composition or grain sizes making up the icy soil.

Wispy markings were seen on the trailing hemispheres of both Rhea and Dione in images taken by NASA’s Voyager spacecraft, and were hypothesized by some researchers to be the result of material extruded onto the surface by ice volcanism. Cassini’s earlier revelation of the braided fractures on Dione led to speculation that Rhea’s wisps might also be created by fractures.

This view shows terrain on the trailing hemisphere of Rhea (1,528 kilometers, or 949 miles across). North is up.

The image was taken using the Cassini spacecraft narrow-angle camera on Jan. 17, 2006, at a distance of approximately 245,000 kilometers (152,000 miles) from Rhea and at a Sun-Rhea-spacecraft, or phase, angle of 30 degrees. Image scale is 1 kilometer (4,771 feet) per pixel.

The possibility of past cryovolcanism on Rhea is tantalizing to say the least. Hopefully further study will provide additional evidence supporting the hypothesis.

For more imagery of Rhea, stop by NASA’s Planetary Photojournal.

-Added 24 February, 19:31 CST-

Today a second, similar false-color view was released:

Intense (false) color on Rhea
Image Credit: NASA/JPL/Space Science Institute

This view shows terrain on the trailing hemisphere of Rhea (1,528 kilometers, or 949 miles across). North is up.

The images were taken using the Cassini spacecraft narrow-angle camera on Jan. 18, 2006, at a distance of approximately 268,000 kilometers (166,000 miles) from Rhea and at a Sun-Rhea-spacecraft, or phase, angle of 115 degrees. Image scale is 2 kilometers (1.2 miles) per pixel.

Fantastic contrast is added to Rhea’s surface features by this enhanced view. Marvelous.

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