Titan
A journey to Saturn and its moons
The Cassini-Huygens mission
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Titan: moon with an atmosphere

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  • Blick unter den Schleier der Titan%2dAtmosphäre

    Titan - Saturn's moon with hydrocarbon lakes under a dense atmosphere

    At 5150 kilometres across, Titan is the second-largest moon in the Solar System and one of the most mysterious. An atmosphere surrounds many planets. Titan, however, is the only moon in the Solar System with a significant gaseous envelope. The atmosphere is a brownish-orange and so dense that the moon’s surface cannot be seen at visible light wavelengths. Only by using what are known as 'atmospheric windows' – narrow wavelength bands in the near and middle infrared is analysis of the surface possible. This technique is used by the infrared spectrometer VIMS (Visible and Infrared Mapping Spectrometer) on the Cassini space probe, which has been analysing the Saturnian system since July 2004. Because of the distance of Titan from the Sun, its surface temperature is about minus 180 degrees Celsius.



    The picture shows a superposition of VIMS images of Titan in three different infrared wavelengths: 1.3 microns (thousandths of a millimetre, blue),) 2 microns (green) and 5 microns (red). The circular structure in the middle is probably an older impact basin. Titan's equatorial latitudes are most likely dry areas, without extensive 'water'. The numerous liquid bodies in the northern hemisphere, one of which is described in this web article, the Kraken Mare, are probably part of an active fluid circulation. These lakes are fed by liquid hydrocarbons that a drainage system carries out of the surrounding valleys. The drainage system, in turn, is fed by methane and ethane precipitation. Many scientists suspect that the nitrogen atmosphere of Titan exhibits strong similarities with the primitive atmosphere of the Earth.

First discovered in 1655 by the Dutch astronomer Christiaan Huygens, Titan is the largest of the 53 moons of Saturn we know to exist. With a diameter of 5150 kilometres, Titan is the second largest moon in the entire Solar System second only to Jupiter’s moon Ganymede with a diameter of 5262 kilometres.

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 to 300 metres 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 flybys 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.

Last modified:
07/07/2011 17:48:11

Contacts

 

Elke Heinemann
Deutsches Zentrum für Luft- und Raumfahrt (DLR) - German Aerospace Center

Tel.: +49 2203 601-2867

Fax: +49 2203 601-3249
Ulrich Köhler
Deutsches Zentrum für Luft- und Raumfahrt (DLR) - German Aerospace Center

Tel.: +49 30 67055-215

Fax: +49 30 67055-402