For 2006, the results of the Huygens probe has been released in a series of articles for Nature Magazine. Please click the links below to read the PDF's of these articles.

• A soft solid surface on Titan as revealed by the Huygens Surface Science Package
• An overview of the descent and landing of the Huygens probe on Titan
• Complex organic matter in Titan's atmospheric aerosols from in situ pyrolysis and analysis
• Huygens Rediscovers Titan
• In situ measurements of the physical characteristics of Titan's environment
• Rain, winds and haze during the Huygens probe's descent to Titan's surface
• The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe
• The vertical profile of winds on Titan

For more information on the specific instruments used to collect data from Huygens - click here.

There are two key points as to why this is:

• Land shaping is similar to that on Earth
• Evidence of liquid methane is present
• Spectroscopy indicated Titan's crust to be a sandy material (possibly methane in origin)
• Hydrocarbon particles are present on Titan's surface

This image is the location of Huygens landing site:

Initial views as Huygens passed through the dense regions of the atmosphere. A defined coastline is present as are rivers carved by liquid methane. The white areas near the bottom are low clouds:

A bit closer to the surface, Huygens images what looks like mountains piercing what may be a methane ocean:

As Huygens descended, a view of what looks like a coastline was spied prior to landing:

This image is a true color rendition of Titan's surface:

And this image shows the dimensions of the objects in the above image:

And finally, a model of what we think the atmosphere of Titan is like compared to Earth (notice how much farther Titan's atmosphere extends):

Details of the Huygens mission can be found here:

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