CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Enceladus Polar Maps - February 2010
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Enceladus Polar Maps - February 2010
PIA 12565

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North Pole Labeled Full Size 10154x10154:
JPEG 11.9 MB
PNG 31.6 MB
TIFF 38.8 MB

Quarter Size 2539x2539:
JPEG 1.5 MB
PNG 3.8 MB
TIFF 4.0 MB

 

Avg Rating: 10/10

North Pole Unlabeled Full Size 9166x9166:
JPEG 13.4 MB
PNG 27.3 MB
TIFF 44.1 MB

 

Enceladus Polar Maps - February 2010
PIA 12566

Avg Rating: 10/10

South Pole Labeled Full Size 10154x10154:
JPEG 13.0 MB
PNG 32.7 MB
TIFF 40.4 MB

Quarter Size 2539x2539:
JPEG 1.7 MB
PNG 4.3 MB
TIFF 4.2 MB

 

Avg Rating: 10/10

South Pole Unlabeled Full Size 9166x9166:
JPEG 14.8 MB
PNG 29.3 MB
TIFF 47.0 MB
  The northern and southern hemispheres of Enceladus are seen in these polar stereographic maps, mosaicked from the best-available Cassini and Voyager clear-filter images.

Each map is centered on one of the poles and surface coverage extends to the equator. Grid lines show latitude and longitude in 30-degree increments. The scale in the full-size versions of these maps is 110 meters (360 feet) per pixel. These maps are updated versions of those released in October 2009 (see PIA11678 and PIA11679).

These two maps show that the character of terrains near the north pole differs strongly from those near the south pole. Terrain near the north pole is among the most heavily cratered and oldest on the surface of Enceladus. The northern hemisphere map shows that a broad band of cratered terrain extends from the equator on the Saturn-facing side (centered on 0 degrees longitude), over the pole and to the equator on the anti-Saturn side (centered on 180 degrees longitude). Terrains near the equator and mid-latitudes on the leading (90 degrees west longitude) and trailing (270 degrees west longitude) sides of Enceladus are much less heavily cratered and are characterized by intense zones of fracturing and faulting.

As seen in the southern hemisphere map, the band of cratered terrain at 0 and 180 degrees longitude extends southward from the equator. However, poleward of about 55 degrees south latitude, the cratered terrain is interrupted and replaced by a conspicuously fractured circumpolar terrain that is nearly devoid of impact craters. In contrast to the very old north polar terrains, the south circumpolar terrains are among the youngest on the surface of Enceladus.

Within the south circumpolar region is a group of prominent parallel "stripes" made up of fractures that are delineated by relatively dark albedo markings flanking the sides of each fracture.

An interesting property of the parallel fracture system is that each appears to turn back at its westernmost segment as if it has been "bent" or "folded" into a hook-like curve. Similar patterns of folded or kinked fractures can be found throughout the region -- a unique feature of the south polar terrain.

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.

For more information about the Cassini Equinox Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

Credit: NASA/JPL/Space Science Institute
Released: February 17, 2010 (PIA 12565, 12566)
Image/Caption Information



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