CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Go Huygens!
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These two maps illustrate the planned imaging coverage for the Descent Imager/Spectral Radiometer, or DISR, onboard the European Space Agency's Huygens probe during the probe's descent toward Titan's surface on January 14, 2005.

The colored lines delineate regions that will be imaged at different resolutions as the probe descends. On each map, the site where Huygens is predicted to land is marked with a yellow dot. This area is in a boundary between dark and bright regions.

These maps were made from the images taken by the Orbiter's cameras on October 26, 2004, at image scales of 4 to 6 kilometers (2.5 to 3.7 miles) per pixel. The images were obtained using a narrow band filter centered at 938 nanometers - a near-infrared wavelength (invisible to the human eye) at which light can penetrate Titan's atmosphere to reach the surface and return through the atmosphere to be detected by the camera. The images have been processed to enhance surface details. Only brightness variations on Titan's surface are seen; the illumination is such that there is no shading due to topographic variations.

For about two hours, the probe will fall by parachute from an altitude of 160 kilometers (99 miles) to Titan's surface. During the descent the DISR and five other science instruments will send data about the moon's atmosphere and surface back to the Cassini spacecraft for relay to Earth. The DISR will take pictures as the probe slowly spins, and some these will be made into panoramic views of Titan's surface.

The first map (PIA#06172) shows expected coverage by the DISR side-looking imager and two downward-looking imagers - one providing medium-resolution and the other high-resolution coverage. The planned coverage by the medium- and high-resolution imagers is the subject of the second map (PIA#06173).

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 Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. 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-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.

Credit: NASA/JPL/Space Science Institute
Released: January 11, 2005 (PIA 06172, 06173)
Image/Caption Information
  Go Huygens!
PIA 06172

Avg Rating: 5/10

Full Size 1500 x 1620:
JPEG 236 KB
PNG 564 KB
TIFF 1.6 MB

Half Size 750 x 810:
JPEG 86 KB
PNG 240 KB
TIFF 505 KB

 

Go Huygens!
PIA 06173

Avg Rating: 7/10

Full Size 1500 x 1620:
JPEG 228 KB
PNG 496 KB
TIFF 1.5 MB

Half Size 750 x 810:
JPEG 82 KB
PNG 219 KB
TIFF 499 KB



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