We've looked closely at the terrestrial planets (the inner, rocky
ones). The Gas Giants (Jupiter, Saturn, Uranus & Neptune) don't seem
much like planets for life to form on. But how about their moons?
Titan is the fifteenth of Saturn's known satellites and the largest. Discovered in 1655 by Dutch physicist and astronomer, Christiaan Huygens. The orangy haze seen in the picture to the left is due to Titan's thick atmosphere, and we have no direct images of the surface.
Titan's low density
Earth has a dense iron rich core, giving it its high density. Even the
Moon has a significantly higher density, 3 x water, and is made
mostly of silicate rock (little iron). Titan's low density suggests
it contains a lot of frozen water, methane, carbon dioxide and ammonia.
Probably the dominant ice is water ice. Water ices are common and ubiquitous all over the outer solar system, in Jupiter, on the icy rings of Saturn and are the predominant ice found in Comets.
Titan's interior is primarily composed of ice existing in different phases. The drawing to the left shows a plausible description of the differing phases of ice in Titan's interior, becoming more densely packed as one moves towards the interior. At mid-depths in Titan, high pressures may allow for liquid water. Deep inside Titan are found the heavier, rocky and metal elements such as silicates and iron, which form the core of Titan.