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Details of Dark Senkyo



Category: Moons > Titan

The low albedo feature known as Senkyo is visible through the haze of Titan's atmosphere

Details of Dark Senkyo
December 2, 2009
Full-Res: PIA11636

The low albedo feature known as Senkyo is visible through the haze of Titan's atmosphere.

See Saturn's View of Titan to learn about this area that appears dark near the moon's equator. This view looks toward Saturn-facing side of Titan (5,150 kilometers, or 3,200 miles across) and is centered on terrain at 1 degree south latitude, 345 degrees west longitude. North on Titan is up and rotated 10 degrees to the right.

The image was taken with the Cassini spacecraft narrow-angle camera on Oct. 12, 2009 using a spectral filter sensitive to wavelengths of near-infrared light centered at 938 nanometers. The view was acquired at a distance of approximately 296,000 kilometers (184,000 miles) from Titan and at a Sun-Titan-spacecraft, or phase, angle of 11 degrees. Image scale is 2 kilometers (about 1 mile) per pixel.

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.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Credit: NASA/JPL/Space Science Institute




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