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

PIA08346: Map of Titan - December 2006
Target Name: Titan
Is a satellite of: Saturn
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem
Product Size: 8748 samples x 4860 lines
Produced By: Cassini Imaging Team
Primary Data Set: Cassini
Full-Res TIFF: PIA08346.tif (127.5 MB)
Full-Res JPEG: PIA08346.jpg (2.144 MB)

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

Original Caption Released with Image:

Click here for poster version of PIA08346 Map of Titan - December 2006
Annotated Version

This global digital map of Titan was created using data taken by the Cassini spacecraft Imaging Science Subsystem (ISS).

The data here consist of images taken using a filter centered at 938 nanometers, allowing researchers to examine albedo (or inherent brightness) variations across the surface of Titan. Due to the scattering of light by Titan's dense atmosphere, no topographic shading is visible in these images.

The map is an equidistant projection and has a scale of 2 kilometers (1.25 miles) per pixel. Equidistant projections preserve distances on a body, with some distortion of area and direction. Actual resolution varies greatly across the map, with the best coverage (close to the map scale) near the center and edges of the map and the worst coverage on the trailing hemisphere (centered around 270 degrees west longitude).

Coverage should improve in some of the poorly covered areas starting in February 2007, when northern Belet, Adiri, and Dilmun will be imaged. Imaging coverage in the northern polar region, currently blank on this map, will improve over the next few years, as Titan approaches vernal equinox in August 2009.

The mean radius of Titan used for projection of this map is 2,575 kilometers (1,600 miles). Until a control network is created for Titan, the satellite is assumed to be spherical.

The named features are designated by the International Astronomical Union. (A "facula" on Titan is a bright spot; a "macula" is a dark spot.)

This map demonstrates how our knowledge of Titan's surface has been vastly improved since Cassini arrived and began mapping the outsize moon. See PIA06086 for an earlier Cassini map of Titan.

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/home/index.cfm. The Cassini imaging team homepage is at http://ciclops.org.


Image Credit:
NASA/JPL/Space Science Institute


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