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For this reason, for many years astronomers considered the possibility that hydrocarbon lakes and seas might exist on this fantastic moon-world. Data that finally arrived courtesy of the joint NASA and European Space Agency's (ESA's) Cassini-Huygens mission lived up to their expectations. Since arriving at the Saturn system in 2004, the Cassini spacecraft has revealed more than 620,000 square miles of Titan's long-hidden, bewildering surface--and it has shown that almost two percent of Titan's entire surface is covered in liquid.
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The research proposes that the shoreline surrounding Ligeia Mare is possibly porous and may be saturated with liquid hydrocarbons. The data span a period running from local winter to spring, and the astronomers expected that--in a way similar to seasides on Earth--the surrounding solid terrains on Titan would warm much more rapidly than the sea.
In the tragicomedy that characterizes human relationships, it has been said that the closer we get to someone, the weirder that person gets. Earth's Moon is our planet's closest neighbor in Space--mysterious, bewitching, bothersome, and bewildering, it has successfully hidden many of its secrets from the prying eyes of curious observers. In July 2017, using satellite data, a team of astronomers announced that they have, for the first time, detected widespread water hidden within ancient explosive volcanic material on Earth's nearest and dearest companion world. This discovery indicates that the interior of Earth's Moon contains large quantities of indigenous water that has finally been revealed in numerous volcanic deposits distributed across the lunar surface--and these ancient deposits contain unusually high amounts of imprisoned water compared with surrounding terrains. The discovery of water in these ancient lunar deposits, which are believed to be composed of glass beads created in the explosive fiery eruption of magma shooting out from the deep interior of the Moon, strengthens the theory that the lunar mantle is surprisingly water-rich.
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Very long ago, when our Solar System was young, Earth's Moon possessed active volcanoes. However, today, the lunar volcanoes are dormant and have not erupted for millions of years.
According to this theory, the Saturn system began with a family of several relatively large moons, analogous to the four large Galilean moons of Jupiter--Io, Europa, Ganymede, and Callisto. However, strange and violent things happened in the Saturn system that drove its large moons onto a collision course with destiny. According to the theory, there were a few dramatic moon mergers, forming the Titan that we now know--but there was also a sufficiently large quantity of moon-stuff left over from the collisions to create the icy mid-sized satellites--Mimas, Iapetus, Enceladus, Tethys, Dione, and Rhea!
"Our model explains the diversity of these ice-rich moons and the evidence for their very active geology and dynamics. It also explains a puzzling fact about Titan, in that a giant impact would give it a high orbital eccentricity," Asphaug continued to explain to the press on October 18, 2012.