CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Beneath the Haze
[For trouble viewing the images/movies on this page, go here]
Beneath the Haze
PIA 10444

Avg Rating: 8.08/10

Full Size 1014x1014:
PNG 742 KB
  Swirling clouds drift like phantoms in Saturn's murky depths.

The camera filter used for this image captures light at wavelengths where atmospheric gases like methane are fairly transparent, allowing for detailed views of deep cloud features. Other filters (see PIA09859) use light that is strongly absorbed by methane gas; the light bounces off the high clouds, making them visible, but gets absorbed before it reaches the low clouds. The use of such filters allows Cassini's cameras to probe Saturn's atmosphere at different depths.

The view looks toward a region 22 degrees north of Saturn's equator. North is up.

The image was taken with the Cassini spacecraft narrow-angle camera on June 20, 2008 using a spectral filter sensitive to wavelengths of infrared light centered at 750 nanometers. The view was obtained at a distance of approximately 1.2 million kilometers (774,000 miles) from Saturn. Image scale is 7 kilometers (4 miles) per pixel.

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, and

Credit: NASA/JPL/Space Science Institute
Released: August 11, 2008 (PIA 10444)
Image/Caption Information

Want to add a comment?   Login (for Alliance Members) ... or ... Join the CICLOPS Alliance!