CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Small Wonders
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This montage of views from NASA's Cassini spacecraft shows three of Saturn's small ring moons: Atlas, Daphnis and Pan at the same scale for ease of comparison.

Two differences between Atlas and Pan are obvious in this montage. Pan's equatorial band is much thinner and more sharply defined, and the central mass of Atlas (the part underneath the smooth equatorial band) appears to be smaller than that of Pan.

Images of Atlas and Pan taken using infrared, green and ultraviolet spectral filters were combined to create enhanced-color views (Figure A), which highlight subtle color differences across the moons' surfaces at wavelengths not visible to human eyes. (The Daphnis image in figure A was colored using the same green filter image for all three color channels, adjusted to have a realistic appearance next to the other two moons.)

A version of the montage using only monochrome images is also provided (Figure B).

All of these images were taken using the Cassini spacecraft narrow-angle camera. The images of Atlas were acquired on April 12, 2017, at a distance of 10,000 miles (16,000 kilometers) and at a sun-moon-spacecraft angle (or phase angle) of 37 degrees. The images of Pan were taken on March 7, 2017, at a distance of 16,000 miles (26,000 kilometers) and a phase angle of 21 degrees. The Daphnis image was obtained on Jan. 16, 2017, at a distance of 17,000 miles (28,000 kilometers) and at a phase angle of 71 degrees. All images are oriented so that north is up.

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 http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

Credit: NASA/JPL-Caltech/SSI
Released: June 28, 2017 (PIA 21449)
Image/Caption Information
  Small Wonders
PIA 21449

Avg Rating: 9.71/10

Figure A Full Size 800x1200:
JPEG 265 KB
PNG 3.8 MB
TIFF 3.8 MB

 

Small Wonders
PIA 21449

Avg Rating: 10/10

Figure B Full Size 800x1200:
JPEG 173 KB
PNG 1.9 MB
TIFF 1.3 MB


Alliance Member Comments
J.M.Hoomans (Sep 14, 2017 at 11:11 AM):
Intriguing:

Atlas is saucer-shaped because it's most likely gathering particles from Saturns' rings: this process allows Atlas to grow over time (same thing happened probably to Iapetus: it has the same ridge along its equator).

Ergo: Saturn rings probably act like an accretion disk :-)
XRumerTest (Jul 18, 2017 at 2:45 PM):
Hello. And Bye.
XRumerTest (Jul 11, 2017 at 3:08 PM):
Hello. And Bye.

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