Lakes of Titan

, methane and nitrogen. Coloured in blue and brown. Photographs Kraken Mare, the large lake at the lower left, is twice as large as can be seen here.]]

The **lakes of Titan**, a moon of Saturn, are made of liquid methane. The lakes were found by the *Cassini-Huygens* space probe. The larger lakes are known as **maria** (seas) and the smaller ones as **lacūs** (lakes).

It was possible that there were seas of liquid methane on Titan and first suggested after reading Voyager 1 and Voyager 2 information that showed Titan to have a thick atmosphere, capable of supporting lakes, but exact evidence was not found until 1995 when pictures from the Hubble telescope and other telescopes had already shown some proof of liquid methane possibly in lakes or planet-wide oceans, similar to oceans on Earth.

The *Cassini* mission proved there are liquid lakes on Titan, but not at first. When the probe arrived in the Saturnian system in 2004, scientists hoped that hydrocarbon lakes or oceans might be seen in reflected sunlight from the surface, but no reflections were found.

Scientists still believed that liquid ethane and methane would be found near Titan's poles, where they expected to find lots of liquid. A possible shoreline was also identified at the pole in radar images. As the Huygens-Cassini probe flew by on July 22, 2006, its radar took pictures of the northern part of the planet (which was in its winter), a number of large, smooth areas were found on the surface near the northern pole. Based on this data, scientists announced "definitive evidence of lakes filled with methane on Saturn's moon Titan" in January 2007. The *Cassini–Huygens* team decided that the smooth areas are the hydrocarbon lakes they had been searching for, the first lakes found off Earth. Some valleys appear to have rivers.

 and Lake Superior.]]
The *Cassini-Huygens* probe flew by in February, 2007, taking radar and camera pictures of some large areas near the north pole that may be large areas of liquid methane and/or ethane, including one sea larger than 100,000&nbsp;km² (larger than Lake Superior), and another area similar in size to the Caspian Sea. Pictures taken near Titan's southern pole in October 2007 showed similar, but far smaller, areas that look like lakes.
''' landing, showing hills, rivers and beaches.]]

The Cassini-Huygens probe, flew very close to Titan in December 2007, and took infrared pictures of the chemicals on the surface and found a lake called Ontario Lacus near the south pole. Scientists studying the infrared pictures decided that one or more of the large lakes in the pictures of Saturn's moon Titan does hold liquid and that the liquid is made of hydrocarbons. They have also found ethane on Titan.  This mission proves Titan to be the only other planet known to have liquid on its surface. The lakes make Titan a very important planet for studying weather science. Liquids, gases and temperatures are at play on Titan.  This should help the science of weather forecasting.

Lakes were not found near the center of Titan which was studied on January 14, 2005. A part of the Huygens-Cassini probe landed there. The pictures taken by the probe as it fell showed no open areas of liquid, but showed rivers that had dried. It was at first thought that dark areas near the center of Titan could be a lake of a liquid or tar-like substance, but the probe landed on the dark area, and it is solid without any liquid. A device known as a penetrometer studied the surface as the probe landed and seemed to find wet clay. Scientists believe that the penetrometer may have landed on a large pebble, and they say that the surface is similar to sand made of ice. Pictures taken after the probe landed show a  large flat area covered in pebbles. The pebbles may be made of water ice and are partly rounded, which indicates fluids.

On February 13, 2008, scientists said that Titans polar lakes contain "hundreds of times more natural gas and other hydrocarbons than all the known natural gas on Earth." The desert near the center of the planet are not liquid but do have more organics than Earth. In June 2008, *Cassini*'s Visible and Infrared Mapping Spectrometer confirmed the presence of liquid ethane beyond doubt in a lake in Titan's southern hemisphere.

Predictions of Titan's clouds are that during in a Saturnian year, liquid moves from the equator to the poles, in clouds, and falls as rain.

## Names of Titans lakes and seas
Titanian *maria* (large hydrocarbon seas) are named after sea monsters of Earth.

Areas named *Lacus* are believed to be methane lakes. They are named after lakes on Earth.

## Related pages
*Solar system

## References