Media Information

 
 
 
Collection:
NASA Cassini-Huygens Collection
Title:
Saturn's Saucer Moons
Description:
Saturn's Saucer Moons
Full Description:
The highest resolution images of Pan and Atlas reveal distinctive "flying saucer" shapes created by prominent equatorial ridges not seen on the other small moons of Saturn.

From left to right: a view of Atlas' trailing hemisphere, with north up, at a spatial scale of about 1 kilometer (0.6 mile) per pixel; Atlas seen at about 250 meters (820 feet) per pixel from mid-southern latitudes, with the sub-Saturn hemisphere at the top and leading hemisphere to the left; Pan's trailing hemisphere seen at about 3 kilometers (2 miles) per pixel from low southern latitudes; an equatorial view, with Saturn in the background, of Pan's anti-Saturn hemisphere at about 1 kilometer (0.6 mile) per pixel.

On Atlas, the ridge extends 20 to 30 degrees in latitude on either side of the equator; on Pan, its latitudinal extent is 15 to 20 degrees. Atlas shows more asymmetry than Pan in having a more rounded ridge in the leading and sub-Saturn quadrants.

The heights of the ridges can be crudely estimated by assuming (ellipsoidal) shapes that lack ridges and vary smoothly cross the equator. Heights of Atlas' ridge range from about 3 kilometers (2 miles) at 270 degrees west longitude to 5 kilometers (3 miles) at 180 and 0 degrees. Pan's ridge reaches about 4 kilometers (2.5 miles) at 0 degrees west longitude, and is about 1.5 kilometers (0.9 mile) high over most of the rest of the equator.

The ridges represent about 27 percent of Atlas' volume and 10 percent of Pan's volume.

The images were acquired with the Cassini spacecraft narrow-angle camera between 2005 and 2007. Pan is 33 kilometers (20.5 miles) across at its equator and 21 kilometers (13 miles) across at its poles; Atlas is 39 kilometers (24 miles) across at its equator and 18 kilometers (11 miles) across at its poles.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. 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 and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.n…. The Cassini imaging team homepage is at http://ciclops.org.

*Credit:* NASA/JPL/Space Science Institute
Date:
December 6, 2007
Keywords:
gallery
Keywords:
images
Keywords:
Cassini
Keywords:
mission
Keywords:
Huygens
Keywords:
probe
Keywords:
Saturn
Keywords:
explore
Keywords:
videos
Keywords:
movies
Keywords:
Jupiter
Keywords:
flyby
Keywords:
spacecraft
Keywords:
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Keywords:
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Keywords:
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Keywords:
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Keywords:
mpeg
Keywords:
Quicktime
facet_what:
Saturn
facet_what:
Cassini
facet_what:
Jupiter
facet_what:
Cassini-Huygens
facet_what:
Huygens Probe
facet_what:
Cassini Orbiter
facet_what:
Atlas
facet_where:
Saturn
facet_where:
Jupiter
facet_where:
Jet Propulsion Laboratory
facet_where:
California
facet_where:
Washington
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_when:
December 6, 2007
facet_when_year:
2007
UID:
SPD-SATRN-2865
original url:

Saturn's Saucer Moons