Saturn's largest moon is the only planetary satellite in the Solar System with a dense atmosphere.
In the early 1980s, the Voyager 1 and 2 probes took the first close-ups of the permanent orange haze that hides Titan's surface.
In early 2005 the European Huygens probe parachuted through Titan's nitrogen-rich atmosphere and landed on the moon's surface while the Cassini spacecraft studied the moon from orbit. Images and other measurements from the craft show a world with riverbeds, liquid methane lakes and cryovolcanoes (ice volcanoes).
Photo: Titan with Saturn in the background taken by the Cassini probe (NASA/JPL/Space Science Institute)
Titan is the only moon with a dense atmosphere.
Titan has the basic ingredients for the precursors of life.
Saturn's moon Titan has a thick atmosphere of nitrogen and methane which, when combined with water and the Sun's energy, may form amino acids – the potential precursors to life on Earth.
The Cassini-Huygens probe finds ice volcanoes and methane rain on Titan.
The Cassini and Huygens probes found evidence of river channels and cryovolcanoes that erupt super-cold water mixed with ammonia on Titan.
The Huygens probe lands on Saturn's moon.
After a long journey fraught with technical problems, the Huygens probe managed to land on Saturn's moon Titan on 15 January 2005. The probe returned images and other data that showed scientists a surface covered with what may be riverbeds.
Researchers describe the Cassini-Huygens probe's design.
Researchers describe the Cassini-Huygens spacecraft's instruments and mission. They talk about the technical challenges they faced during the Huygens probe landing in 2005.
Saturn's moon intrigues scientists.
The Voyager 1 space probe, launched in 1977, photographed Saturn and its moons. Titan, with its thick, orange atmosphere, frustrated scientists eager to see the moon's surface.
Titan (or Saturn VI) is the largest moon of Saturn. It is the only natural satellite known to have a dense atmosphere, and the only object other than Earth where clear evidence of stable bodies of surface liquid has been found.
Titan is the sixth ellipsoidal moon from Saturn. Frequently described as a planet-like moon, Titan's diameter is 50% larger than Earth's natural satellite, the Moon, and it is 80% more massive. It is the second-largest moon in the Solar System, after Jupiter's moon Ganymede, and is larger by volume than the smallest planet, Mercury, although only 40% as massive. Discovered in 1655 by the Dutch astronomer Christiaan Huygens, Titan was the first known moon of Saturn, and the fifth known satellite of another planet.
Titan is primarily composed of water ice and rocky material. Much as with Venus before the Space Age, the dense opaque atmosphere prevented understanding of Titan's surface until new information accumulated when the Cassini–Huygens mission arrived in 2004, including the discovery of liquid hydrocarbon lakes in Titan's polar regions. The geologically young surface is generally smooth, with few impact craters, although mountains and several possible cryovolcanoes have been found.
The atmosphere of Titan is largely nitrogen; minor components lead to the formation of methane and ethane clouds and nitrogen-rich organic smog. The climate—including wind and rain—creates surface features similar to those of Earth, such as dunes, rivers, lakes, seas (probably of liquid methane and ethane), and deltas, and is dominated by seasonal weather patterns as on Earth. With its liquids (both surface and subsurface) and robust nitrogen atmosphere, Titan's methane cycle is viewed as an analogy to Earth's water cycle, although at a much lower temperature.