Click on the image for full resolution movie
Radar Shows Evidence of Seas
(Half Resolution)
This movie, comprised of several detailed images taken by Cassini's radar
instrument, shows bodies of liquid near Titan's north pole. These images
show that many of the features commonly associated with lakes on Earth,
such as islands, bays, inlets and channels, are also present on this cold
Saturnian moon. They offer strong evidence that larger bodies seen in
infrared images are, in fact, seas. These seas are most likely liquid
methane and ethane.
For more than two decades, scientists have debated whether liquids on
Titan exist, and if so, where they would be located. Pre-Cassini
observations from the 1980s indicated that something on Titan's surface
must be re-supplying the methane to its atmosphere. A global ocean was
once hypothesized. Subsequently, disconnected lakes or seas were
predicted. The discovery of numerous lakes near Titan's north pole by the
Cassini radar instrument in July 2006 has confirmed the latter idea, and
indicates an apparent preference during the current season for liquids to
be located near the north pole.
These new observations of the north polar area show how extensive and
widespread these lakes are, and reveal at least one body of liquid that
might rightly be called a sea. These seas cover an area about 100,000
square kilometers (about 39,000 square miles), larger than the largest
Great Lake, Lake Superior, near the U.S. and Canadian border, whose area
is 82,000 square kilometers (about 32,000 square miles). Analysis of the
data indicates that the bodies of liquid may be tens of meters in depth.
This high-definition video offers a trip through the north polar area just
as Cassini radar saw it. It combines radar swaths seen on several Titan
passes: July 22, 2006 (T16); Sept. 23, 2006 (T18); Oct. 9, 2006 (T19); and
Feb. 22, 2007 (T25), respectively. The mosaic reveals the extent of the
lakes, their shapes and interconnections. The areas believed to be
composed of liquids are shown in blue as an aid to interpretation.
The movie begins with an illustration of the relative orbits of Titan and
Cassini, both circling Saturn. The spacecraft is seen approaching the
planet with a nodding motion as its antenna scans the moon's surface,
turning to keep its target in sight. The animation shows all radar swaths,
and zooms in for a close look at the many complex shapes the lakes take.
Some features that resemble lakes with no liquid may be remnants that have
already dried as the northern winter fades into spring.
The resolution of the radar data varies from several kilometers to as
fine as 300 meters (984 feet). The coverage shown in the video spans from
50 degrees north latitude, almost to the pole, where a small triangular
gap in coverage misses the exact pole.
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/home/index.cfm.
