Titan (moon)

**Titan** (Ancient Greek: *Τῑτάν*) is Saturn's moon. It was found by Christiaan Huygens on 25 March 1655. Titan is a unique moon: it is the Solar System’s only moon to have an atmosphere.

Titan is the largest moon of Saturn and the second largest in the Solar System. It orbits 1,221,865&nbsp;km away from Saturn.

## Discovery
Titan was discovered on 25 March 1655 by Christiaan Huygens, an astronomer from the Netherlands. Earlier, in 1610, Galileo Galilei had discovered four of Jupiter's moons. This inspired Huygens: he also wanted to discover new moons. Because Huygens had also improved the telescopes of the time, making them a lot better, he thought he might be able to discover a new moon.

Christiaan and his brother, Constantijn, started to build their own telescopes in 1650. Using the first telescope he ever built, Christiaan Huygens was able to see Titan. At first he called it "Luna Saturni", which means "Saturn's moon" (he did not know there was more than one). Through the years, lots of other moons have been discovered and today the moon is known as "Titan" or as "Saturn VI". The name "Titan", and all the names of Saturn's other moons, are from the Greek legends.

## Structure 
Titan is the only moon in the Solar System that has a thick atmosphere (the gases that surround a planet or moon).

At its centre, Titan has a rocky core that is about 3400&nbsp;km thick. This core is made up of silicates and metals. The gravity (the force that keeps everything attached to the ground) is a lot weaker than here on earth. If you could jump one meter high on the Earth, you would be able to jump seven meters high on Titan.

## Movement  
It takes Titan 15 days and 22 hours to orbit (travel) around Saturn. This is almost the same time it takes Saturn to rotate or spin around its own axis - one full spin. This is known as "synchronous rotation", which means that the same side of Titan is always pointed to Saturn.

The path in which Titan moves, its orbit, is very close to a circle, but not quite. We use the word "eccentricity" to describe the path that a moon or planet travels in. An image with an eccentricity of 0 (zero) has a path that is a perfect circle. If the eccentricity is more than 0, the path is less round (see image below). Titan's eccentricity is 0.028, very close to zero.

## Cassini-Huygens mission
On July 1, 2004, the Cassini-Huygens probe entered into orbit around Saturn. On December 25, 2004, the Huygens probe separated from the Cassini probe and started to move towards Titan. It landed on Titan's surface on January 14, 2005. It landed on a dry surface, but it confirmed that large bodies of liquid exist on the moon. The Cassini probe continued to gain data of Titan and a number of the icy moons. It found evidence that the moon Enceladus had water erupting from its geysers. Cassini also proved in July, 2006 that Titan contained hydrocarbon lakes, located near its north pole. In March, 2007, it discovered a large hydrocarbon lake the size of the Caspian Sea near its north pole. The lake of liquid methane has been named Kraken Mare. In 2009, Nasa showed a photograph showing the sunlight reflecting off the surface of the lake. This was the first ever picture of liquid on another world.

In 2012 researchers at NASA discovered that Titan is giving off a faint glow of light. This is believed to be caused by complex chemical reactions occurring in Titan's atmosphere. This kind of light is called an airglow.

## Related pages
* Lakes of Titan
* Shangri-La (Titan)

## Further reading 
* 

## References