Visit NASA's Home Page Jet Propulsion Laboratory California Institute of Technology View the NASA Portal Click to search JPL Visit JPL Home Page Proceed to JPL's Earth Page Proceed to JPL's Solar System Page Proceed to JPL's Stars & Galaxies Page Proceed to JPL's Technology Page Proceed to JPL's People and Facilities Photojournal Home Page View the Photojournal Image Gallery
Top navigation bar

PIA08110: Titan Viewed by Cassini’s Radar
Target Name: Titan
Is a satellite of: Saturn
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
Product Size: 2538 samples x 1900 lines
Produced By: JPL
Primary Data Set: Cassini
Full-Res TIFF: PIA08110.tif (14.48 MB)
Full-Res JPEG: PIA08110.jpg (222.9 kB)

Click on the image to download a moderately sized image in JPEG format (possibly reduced in size from original).

Original Caption Released with Image:

This set of images show the areas mapped so far on Saturn’s moon Titan by the Cassini Radar Mapper using its Synthetic Aperture Radar imaging mode and the location of the upcoming Oct. 28, 2005, Titan flyby. Labels represent the approximate central longitude of each globe.

The radar swaths are superimposed on a false-color image made from observations by NASA’s Hubble Space Telescope. The top image shows radar swaths from the first Titan flyby, on Oct. 26, 2004, (northernmost) and the second radar pass of Titan, on Feb. 15, 2005 (near-equatorial). The Oct. 26 swath is about 4,500 kilometers long (2,800 miles), extending from 133 degrees west longitude and 32 degrees north latitude through 12 degrees west and 29 degrees north. The February swath is centered at approximately 30 degrees north and 70 degrees west. The spatial resolution of the radar images ranges from about 300 meters (980 feet) per pixel to about 1.5 kilometers (0.93 miles) per pixel.

The middle globe shows the radar swath acquired during the third radar pass, on Sept. 7, 2005, close to Titan's south pole. The swath is centered at 12 degrees west and 51 degrees south, with similar spatial resolution to the previous two.

These first three radar passes revealed a variety of geologic features, including impact craters, wind-blown deposits, channels, and cryovolcanic features.

The third globe at the bottom shows the location of the radar swath for the upcoming Oct. 28 flyby. The location of the Huygens landing site is marked in red. The overlap between the Huygens data and the radar data will give new clues to the nature of the surface seen by the Huygens probe, which landed on Titan in January 2005.

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 was designed, developed and assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the United States and several European countries.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov .


Image Credit:
NASA/JPL


Latest Images Search Methods Animations Spacecraft & Telescopes Related Links Privacy/Copyright Image Use Policy Feedback Frequently Asked Questions Photojournal Home Page First Gov Freedom of Information Act NASA Home Page Webmaster
Bottom navigation bar