CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Titan's Changing Seasons
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Titan's Changing Seasons
PIA 12586

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  Cassini records Titan's seasonal hemispheric dichotomy, with the moon's northern half appearing slightly lighter than the southern half in this image.

See PIA11603 to learn more about this change on Titan.

This view looks toward the trailing hemisphere of Titan (5150 kilometers, 3200 miles across). North on Titan is up and rotated 12 degrees to the right.

The image was taken with the Cassini spacecraft narrow-angle camera on Feb. 16, 2010 using a spectral filter sensitive to wavelengths of near-infrared light centered at 889 nanometers. The view was obtained at a distance of approximately 1.1 million kilometers (684,000 miles) from Titan and at a Sun-Titan-spacecraft, or phase, angle of 28 degrees. 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: March 10, 2010 (PIA 12586)
Image/Caption Information

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