Does Titan Have Oily Oceans?

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SUMMARY

Titan, Saturn's largest moon, is believed to have a surface covered with lakes or oceans of methane or ethane, as indicated by recent radar research. The Huygens probe, developed by the European Space Agency, is equipped with a robotic laboratory to analyze Titan's atmosphere and surface. Designed to float and transmit data even if it lands in liquid, the probe will begin its descent in January 2005, following the Cassini orbiter's arrival in July 2004. The probe's successful landing and data transmission will provide critical insights into Titan's unique environment.

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  • Understanding of planetary science and celestial bodies
  • Familiarity with the Huygens probe and its mission objectives
  • Knowledge of radar research techniques in planetary exploration
  • Basic principles of atmospheric science related to Titan's environment
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  • Research the Huygens probe's scientific instruments and their functions
  • Explore the composition and characteristics of Titan's atmosphere
  • Learn about the Cassini mission and its contributions to Saturn exploration
  • Investigate the implications of methane and ethane lakes on Titan's geology
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Astronomers, planetary scientists, and space exploration enthusiasts interested in the study of Titan and the Huygens probe's findings.

Ivan Seeking
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We should find out soon. :smile:

If the Huygens probe lands on one of these 'oceans' will it affect the ability of the probe to send back useful data? Or could the probe sink without trace?
 
It was built with the assumption (hope?) that it might land in liquid. It's set up to float, right itself and send data from there.
 
Cassini arrives at Saturn in July 2004. I can't wait! (well, I suppose I have been waiting patiently for the past 6 years...a few more months should be ok)

from NASA's site...(emphasis mine)
http://saturn.jpl.nasa.gov/cassini/MoreInfo/faq.shtml#faq8
The Huygens probe, supplied by the European Space Agency, carries a well-equipped robotic laboratory that it will use to scrutinize the clouds, atmosphere, and surface of Saturn's moon Titan. As the 2.7-meter-diameter (8.9-foot) probe enters the atmosphere it will begin taking measurements in the haze layer above the cloud tops. As it descends -- first on a main parachute and later on a drogue chute for stability -- various instruments will measure the temperature, pressure, density, and energy balance in the atmosphere.
As the Huygens probe breaks through the cloud deck, a camera will capture pictures of the Titan panorama. Instruments will also be used to study properties of Titan's surface remotely -- and perhaps directly, should the probe survive the landing.

Many scientists theorize that Titan may be covered by lakes or oceans of methane or ethane, so the Huygens probe is designed to function even if it lands in liquid. If the battery-powered probe survives its landing, it will relay measurements from Titan's surface until the Cassini orbiter flies beyond the horizon and out of radio contact.

Guess I got to wait until Jan 2005 before we find out about Titan though (according to the BBC article in the OP).
 
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