Titan surface
Photojournal: PIA21626
Source: NASA/JPL-Caltech/ASI
Published: August 11, 2017

During its final targeted flyby of Titan on April 22, 2017, Cassini's radar mapper got the mission’s last close look at the moon's surface.

On this 127th targeted pass by Titan (unintuitively named "T-126"), the radar was used to take two images of the surface, shown in Figure A at left and right. Both images are about 200 miles (300 kilometers) in width. Objects appear bright when they are tilted toward the spacecraft or have rough surfaces; smooth areas appear dark.

At left in Figure A are the same bright, hilly terrains and darker plains that Cassini imaged during its first radar pass of Titan, in 2004. Scientists do not see obvious evidence of changes in this terrain over the 13 years since the original observation.

At right, the radar looked once more for Titan's mysterious "magic island" (PIA20021) in a portion of one of the large hydrocarbon seas, Ligeia Mare. No "island" feature was observed during this pass. Scientists continue to work on what the transient feature might have been, with waves and bubbles being two possibilities.

In between the two parts of its imaging observation, the radar instrument switched to altimetry mode, in order to make a first-ever (and last-ever) measurement of the depths of some of the lakes that dot the north polar region. For the measurements, the spacecraft pointed its antenna straight down at the surface and the radar measured the time delay between echoes from the lakes’ surface and bottom.

Figure B shows a graph of the depths measured for eight small lakes at top, aligned with a radar image of the same area taken on a previous Cassini flyby of Titan. Although these data are still preliminary, all eight lakes are thought to be about the same depth (about 100 meters, which is about 328 feet). Scientists do not yet know if the lakes are connected by an underground system analogous to a water table or aquifer, but this is a possibility under investigation.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, DC. 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 https://saturn.jpl.nasa.gov.


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