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Murky World

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ March 9, 2007
Straining to make out the surface of Titan through its murky atmosphere, NASA's Cassini spacecraft's wide angle camera manages to exploit one of the infrared spectral windows where the particulate smog is transparent enough for a peek.

Straining to make out the surface of Titan through its murky atmosphere, the Cassini spacecraft's wide angle camera manages to exploit one of the infrared spectral windows where the particulate smog is transparent enough for a peek.

The Senkyo region is visible in the north, while Mezzoramia lies to the south in this view of Titan (5,150 kilometers, or 3,200 miles across). (See the December 2006 Map of Titan at PIA08346.)

The image was taken with the Cassini spacecraft wide-angle camera using a spectral filter sensitive to wavelengths of infrared light centered at 939 nanometers. The image was taken on Jan. 29, 2007 at a distance of approximately 79,000 kilometers (49,000 miles) from Titan. Image scale is 5 kilometers (3 miles) per pixel.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov/home/index.cfm. The Cassini imaging team homepage is at http://ciclops.org.

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Mission
Target
  • Titan
Spacecraft
  • Cassini Orbiter
Instrument
  • Imaging Science Subsystem - Wide Angle
Credit
NASA/JPL/Space Science Institute

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