CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Titan Polar Maps - June 2015
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Titan Polar Maps - June 2015
PIA 19657

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Titan Polar Maps - June 2015
PIA 19657

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Titan Polar Maps - June 2015
PIA 19657

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Titan Polar Maps - June 2015
PIA 19657

South Pole Unlabeled Full Size 1966x1966:
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South Pole Unlabeled Half Size 983x983:
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  The northern and southern hemispheres of Titan are seen in these polar stereographic maps, assembled in 2015 using the best-available images of the giant Saturnian moon from NASA's Cassini mission. The images were taken by Cassini's imaging cameras using a spectral filter centered at 938 nanometers, allowing researchers to examine variations in albedo (or inherent brightness) across the surface of Titan. These maps utilize imaging data collected through Cassini's flyby on April 7, 2014, known as "T100".

Titan's north pole was not well illuminated early in Cassini's mission, because it was winter in the northern hemisphere when the spacecraft arrived at Saturn. Cassini has been better able to observe northern latitudes in more recent years due to seasonal changes in solar illumination. Compared to the previous version of Cassini's north polar map (see PIA11146), this map provides much more detail and fills in a large area of missing data. The imaging data in these maps complement Cassini synthetic aperture radar (SAR) mapping of Titan's north pole PIA17655.

These two maps show the contrasting character of terrains near Titan’s poles especially well. The north polar region is heavily dotted with hydrocarbon lakes and seas. The dark feature that extends from the mid to lower-right quadrant of the northern map is Titan’s largest sea, Kraken Mare. At about 150,000 square miles (400,000 square kilometers), Kraken Mare is roughly the size of the Caspian Sea on Earth. Titan’s second largest sea, Ligeia Mare (49,000 square miles or 126,000 square kilometers) is seen just above Kraken Mare. Very near the north pole of Titan is another large sea, Punga Mare (about 240 miles or 380 kilometers across).

The uniform gray area in the northern hemisphere indicates a gap in the imaging coverage of Titan's surface, to date. The missing data will be imaged by Cassini during flybys on December 15, 2016 and March 5, 2017.

Lakes are also seen in the southern hemisphere map, but they are much less common than in the north polar region. Only a lakes have been confirmed in the south. The dark, footprint-shaped feature at 180 degrees west is Ontario Lacus; a smaller lake named Crveno Lacus can be seen as a very dark spot just above Ontario. The dark-albedo area seen at the top of the southern hemisphere map (at 0 degrees west) is an area called Mezzoramia.

Each map is centered on one of the poles, and surface coverage extends southward to 60 degrees latitude. Grid lines indicate latitude in 10-degree increments and longitude in 30-degree increments. The scale in the full-size versions of these maps is 4,600 feet (1,400 meters) per pixel. The mean radius of Titan used for projection of these maps is 1,600 miles (2,575 kilometers).

The Cassini Solstice Mission is a joint United States and European endeavor. 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 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 Solstice Mission visit, and

Credit: NASA/JPL-Caltech/SSI
Released: October 9, 2015 (Happy 75th Birthday, John) (PIA 19657)
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