
Saturn's largest moon, often used as a reference for size in exomoon studies.Titan is Saturn's largest moon and the second-largest moon in the solar system, after Jupiter's Ganymede. It is a world of thick orange haze, liquid methane and ethane lakes, and a nitrogen-rich atmosphere—the only moon with a substantial atmosphere. Titan serves as a natural laboratory for prebiotic chemistry and is a prime target in the search for life beyond Earth. In exomoon studies, Titan is often used as a reference point for size and mass, since it is large enough to be a planet if it orbited the sun directly.
Titan was discovered by Christiaan Huygens in 1655. The first close-up observations were made by the Voyager probes in 1980-1981, and the Cassini-Huygens mission (2004-2017) provided detailed maps and landed the Huygens probe on its surface in 2005.
Titan's atmosphere is primarily nitrogen (about 95%) with methane (about 5%). Solar ultraviolet light breaks down methane, leading to complex organic molecules that form the characteristic orange haze. The surface is hidden from visible light but was mapped by the Cassini spacecraft using radar. Titan's surface has rivers, lakes, and seas of liquid hydrocarbons, with a hydrological cycle based on methane instead of water. Its interior likely contains a subsurface ocean of liquid water beneath an icy crust.
Titan is a key analog for studying atmospheric chemistry and the potential for life in exotic environments. Its data informs models of planetary atmospheres and guides the design of future missions, such as NASA's Dragonfly rotorcraft, which will explore Titan's surface in the 2030s.
Titan's surface pressure is about 1.5 times that of Earth, so a person would not need a pressure suit—only a warm jacket and an oxygen mask.
























