Water-Ammonia Ocean May Exist Beneath Saturnian Moon’s Surface
By Dee Chisamera
11:59, March 21st 2008
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Water-Ammonia Ocean May Exist Beneath Saturnian Moon’s Surface

NASA’s Cassini spacecraft is once again in the spotlight, as it uncovered evidence that points to the existence of an underground ocean on one of Saturn’s moons, namely Titan. Scientists believe the composition of the ocean could be water and ammonia, and will detail their findings in the March 21 issue of the journal Science.

The images that led scientists to such assumptions were taken with the help of Cassini’s radar observations on the moon’s rotation between 2004 and 2007. The geological features on the surface of Titan combined with its rotation and the mysterious displacement of some of these features in time led to the idea that there might be an ocean somewhere under the surface that is responsible for all the “movement.”

Ralph Lorenz, lead author of the paper, said that the organic dunes, lakes, channels and mountains point to a striking resemblance of Titan to our own planet. The radar images also gave scientists a glimpse on what could happen beneath the surface of Titan, and why not, even more hope that somewhere in the Universe life is possible to take shape.

Between October 2005 and May 2007, Cassini executed 19 passes over Titan, gathering detailed data on the surface of the moon and their precise location. The fact that the geological features changed location in such short periods of time got them thinking on the probable cause.

“We believe that about 100 kilometers (62 miles) beneath the ice and organic-rich surface is an internal ocean of liquid water mixed with ammonia,” concluded Bryan Stiles of NASA’s Jet Propulsion Laboratory in Pasadena, California, who also contributed to the paper.

The next Titan fly-by is set for March 25, when NASA’s Cassini spacecraft will get as close as 1,000 kilometers (620 miles) from the Saturn moon’s surface. The mission is to take a closer look at Titan’s upper atmosphere with the help of its Ion and Neutral Mass Spectrometer, while the spacecraft’s Visual and Infrared Mapping Spectrometer will take high-resolution images of Titan’s southeast quadrant.

Image credits: NASA



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