File:PIA17184 rot180 inset PIA14658 rot38.jpg

Summary

The large image, of the south polar jets of <a href="https://en.wikipedia.org/wiki/Saturn" class="extiw" title="w:Saturn">Saturn</a>'s moon <a href="https://en.wikipedia.org/wiki/Enceladus_(moon)" class="extiw" title="w:Enceladus (moon)">Enceladus</a>, is NASA/JPL image PIA17184, rotated 180 degrees. The inset image, of the entire moon, is image PIA14658 rotated 38 degrees counterclockwise.

Original caption for PIA17184:

This <a href="https://en.wikipedia.org/wiki/Cassini-Huygens" class="extiw" title="w:Cassini-Huygens">Cassini</a> narrow-angle camera image -- one of those acquired in the survey conducted by the Cassini imaging science team of the geyser basin at the south pole of Enceladus -- was taken as Cassini was looking across the moon's south pole. At the time, the spacecraft was essentially in the moon's equatorial plane. The image scale is 1280 feet (390 meters) per pixel and the sun-Enceladus-spacecraft, or phase, angle is 162.5 degrees.

The image was taken through the clear filter of the narrow angle camera on November 30, 2010, 1.4 years after southern autumnal equinox. The shadow of the body of Enceladus on the lower portions of the jets is clearly seen.

In an annotated version of the image, the colored lines represent the projection of Enceladus' shadow on a plane normal to the branch of the Cairo fracture (yellow line), normal to the Baghdad fracture (blue line) and normal to the Damascus fracture (pink line).

Post-equinox images like this, clearly showing the different projected locations of the intersection between the shadow and the curtain of jets from each fracture, were useful for scientists in checking the triangulated positions of the geysers, as described in a paper by Porco, DiNino, and Nimmo, and published in the online version of the Astronomical Journal in July 2014: <a rel="nofollow" class="external free" href="http://dx.doi.org/10.1088/0004-6256/148/3/45">http://dx.doi.org/10.1088/0004-6256/148/3/45</a>.

A companion paper, by Nimmo et al. is available at: <a rel="nofollow" class="external free" href="http://dx.doi.org/10.1088/0004-6256/148/3/46">http://dx.doi.org/10.1088/0004-6256/148/3/46</a>.

The Cassini Solstice 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 Solstice Mission visit <a rel="nofollow" class="external free" href="http://ciclops.org">http://ciclops.org</a>, <a rel="nofollow" class="external free" href="http://www.nasa.gov/cassini">http://www.nasa.gov/cassini</a> and <a rel="nofollow" class="external free" href="http://saturn.jpl.nasa.gov">http://saturn.jpl.nasa.gov</a>.

Original caption for PIA14658:

Like a proud peacock displaying his tail, Enceladus shows off its beautiful plume to Cassini's cameras.

Enceladus (313 miles, 504 kilometers across) is seen here illuminated by light reflected off of Saturn.

This view looks toward the Saturn-facing side of Enceladus. North on Enceladus is up and rotated 45 degrees to the right. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Jan. 18, 2013.

The view was acquired at a distance of approximately 483,000 miles (777,000 kilometers) from Enceladus and at a Sun-Enceladus-spacecraft, or phase, angle of 173 degrees. Image scale is 3 miles (5 kilometers) per pixel.

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