Scientists had already
spotted lakes of methane, a type of natural gas in Titan's poles, but so far
none had been found in its equatorial regions, which are mostly arid and vast
expanses of dunes.
"It was totally
unexpected, because the lakes are not stable in tropical latitudes," said
Caitlin Griffith of the University of Arizona, director of the team responsible
for the finding.
Thanks to the images
provided by the Cassini spacecraft orbiting Saturn since 2004, the team was
able to detect a black mark of 2,400 square kilometers, consisting of small
dark ovals, which constitute a set of small lakes and swamps, scattered
throughout the tropical surface of Titan. They said further analysis of the dark
spot suggest the presence a hydrocarbon lake about 2,400 square kilometers.
Also found evidence of four tropical lagoons near the lake.
Although in 2011 the
camera sensitive to infrared allowed Cassini incorporates signs of methane rain
on the dunes near the Ecuador of Titan, scientists do not believe that the
origin of the lakes is this. Griffith and his colleagues believe that Titan's
tropical lakes were formed by the existence of large underground reservoirs of
liquid methane during the last 10,000 years would have expelled this material
to the surface.
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