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|  | | | | | | Titan’s surface organics surpass oil reserves on Earth
13 February 2008
| An artist's imagination of hydrocarbon pools, icy and rocky terrain on the surface of Saturn's largest moon Titan.
Credits: Steven Hobbs | |  |  | |
| | | | | This movie, comprised of several detailed images taken by Cassini's radar instrument, shows bodies of liquid near Titan's north pole. The 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 sq km, larger than Lake Superior, near the U.S. and Canadian border, whose area is 82 000 sq km. Analysis of the data indicates that the bodies of liquid may be tens of metres 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: 22 July 2006 (T16); 23 September 2006 (T18); 9 October 2006 (T19) and 22 February 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 kilometres to as fine as 300 m. The coverage shown in the video spans from 50º north, almost to the pole, where a small triangular gap in coverage misses the exact pole.
Credits: NASA/JPL | | | | |
| | | | | This image, taken by Cassini's radar instrument, shows bodies of liquid near Titan's north pole. The 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 sq km, larger than Lake Superior, near the U.S. and Canadian border, whose area is 82 000 sq km. Analysis of the data indicates that the bodies of liquid may be tens of metres in depth.
The resolution of the radar data varies from several kilometres to as fine as 300 m.
Credits: NASA/JPL | | | | |
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