Titan: moon with an atmosphere
Voyager 2 image of Titan
First discovered in 1655 by the Dutch astronomer Christiaan Huygens, Titan is the largest of the 47 moons of Saturn we know to exist. With a diameter of 5150 km, Titan is the second largest moon in the entire Solar System – second only to Jupiter’s moon Ganymede with a diameter of 5262 km.
Titan is the only moon in the whole Solar System to have an atmosphere, making it a particularly interesting and intriguing research prospect for scientists. Because this atmosphere has an aerosol layer (a layer of tiny suspended particles of hydrocarbons) at a height of 200 m – 300 m and a high proportion of methane in its nitrogen atmosphere, it is impenetrable to telescopes and cameras. Together with distant Pluto, Titan is the last major body in the Solar System about whose surface we know virtually nothing. And we’re talking about a surface area the same size as Africa, Asia and Europe put together.
To researchers, this Saturnian moon is like a trip back in time to our planet’s past that could give them a glimpse of a primitive Earth. Titan and the Earth are the only bodies in our Solar System whose atmospheres are composed principally of nitrogen; in the case of Titan, the proportion of nitrogen is ten times greater than that of our own atmosphere here on Earth. Scientists believe that the atmosphere of Titan might be similar to Earth’s early atmosphere. By exploring Titan, they hope to find clues as to how the ‘primitive’ Earth could have developed into a planet on which life could form.
A cold, dark world
Titan is approximately 1500 million kilometres away from the Sun. This huge distance from the Sun, combined with its nebulous atmosphere, mean that a person walking about on Titan would have to make do with roughly one thousandth of the daylight we have on Earth. For this reason, solar radiation does little to warm up Titan: the average surface temperature is minus 179 degrees Celsius. It is possible that Titan could have preserved many of the chemical components that preceded the formation of life on Earth by deep-freezing them. Perhaps this Saturnian moon has a ‘hydrological’ cycle like we do on Earth with clouds, rain, rivers and oceans, but with ethane and methane taking the place of water. Researchers are faced with a whole range of questions. To come closer to answering them, the Cassini orbiter will perform 45 fly-bys of Titan at distances of as little as 950 km. One high point of the Cassini-Huygens mission was the landing of the Huygens probe on the mysterious moon on 14 January 2005.