Lecture 17
Titan and the Galilean Satellites
(chapter 8)




Titan is Saturn's moon, and is almost as large as Mercury--Titan's diameter is 5150 km.  In many ways Titan is like a planet.
 
 
 

The nature of Titan
 

Titan has a very thick atmosphere (second only to Venus) which obscures the surface.  Such thick cloud cover and atmosphere might signal significant greenhouse warming.  The presence of a greenhouse effect would mean thatTitan may be warmer than would be expected for a satellite at its distance from the Sun.

For some of the best ground based images of Titan taken by Professor Close click here

Saturn is located 9.5 A.U. from the Sun--->Saturn's moon should have a surface temp of below 100 K--->water would only exist as ice and there would be no biological activity--->of no interest.

BUT Titan's possible greenhouse means warmer surface temperatures and possible liquid water.

Voyager (1982) spacecraft flyby has gave scientists the first good data on Titan (see below for more info from the recent Cassini mission).

Voyager discoveries:

1.  Titan's mass and radius determined and then used to calculate its density:

    1.9 g.cm3

whereas the Earth's density=5.2 g/cm3 and the Moon's density=3.3 g/cm3

Such a density means that Titan is very light.
 

2.  Considering the density value of Titan, it is most likely Titan is composed of mainly ICE.  More than half of its volume must be ice.

Remember: the density of water=1 g/cm3.
 

3.  Titan's atmosphere consists of mainly N2.
 

4.  Temperature on the surface of Titan=94 K.

Temperature 40 km above the surface=70 K.

Temperature rises again at higher altitudes.  This atmospheric temperature profile is similar to the Earth's.

*Such a relatively low surface temperature (94 K) rules out the presence of a strong greenhouse.

BUT even at fairly low temps, organic molecules are involved in chemical processes and for this reason Titan makes for an interesting natural laboratory.

Why does Titan have such thick clouds?

Titan's atmosphere is predominantly N2, but also contains small amounts of methane (CH4).  It has been theorized that Titan has global scale oceans of methane which continually resupply the Titan atmosphere with the small amounts of methane observed.  Further, it has been thought that the evaporation of methane in the atmosphere has condensed into clouds, creating Titan's thick cloud cover.  However, observations tell us Titan's atmosphere is not saturated with methane so the clouds cannot consist of methane.

Another hypothesis given to explain Titan's thick clouds is that the global oceans that may be present consist of ethane and nitrogen as well as methane.  This would fit well with the chemical compounds observed in the atmosphere BUT observations contradict the presence of any such global oceans.

Instead, it is more likely that the ethane-methane mixture does not reside at the surface in large open bodies of liquid.  Rather, it percolates up through the cracks and pores in the surface ice.  Then, it evaporates into the atmosphere helping to create the thick cloud cover.
 

Water on Titan


Titan exobiology

For all the most up to date news about Titan from the Cassini-Huygens spacecraft click here


The Galilean satellites

The Jupiter system is composed of:

Jupiter-----------Io--------------Europa--------------Ganymede----------------Callisto
 

Jupiter has a source of energy like our Sun.  However, while the Sun's energy is nuclear in nature, Jupiter's  energy is given off during gravitational contraction of the planet as it cools.

Both Io and Europa are similar in size to the Moon.

Io--->r=1815 km
Europa--->r=1569 km
Moon--->r=1738 km

Ganymede and Callisto are both similar in size to Titan.

Ganymede--->r=2631 km
Callisto--->r=2400 km
Titan--->r=2575 km

The Galilean satellites--water ice, liquid water and tidal heating



Io density=3.55 g/cm3
--very similar to the Moon (density=3.34 g/cm3)

This density value tells us that Io probably has an iron core.

There appears to be no ice on Io.


Europa density=3.01 g/cm3

Combine this value with an observed highly reflective surface and it can be concluded that the surface of Europa is composed of pure water ice.

The water abundance of Europa is a little more than 15%.


Ganymede density=1.93 g/cm3
Callisto density=1.83 g/cm3

Probably 50-57% and 52-58% of Ganymede and Callisto respectively are made up of ice.


Scientists find both Io and Europa interesting because they experience tidal heating.

*The entire surface of Io appears to be volcanic.
 

Focus on Io


Question: Could there be hidden water?

Possibly---and therefore exobiological activity could exist.
 

**However, it seems despite the active volcanism, there is neither water nor life on Io.
 

Focus on Europa

1.  Could be evenly distributed throughout Europa's interior like hydrated silicates--minerals that contain water bound in their structure.  These are common on Earth, e.g. clay.

OR

2.  Could be on the surface in the form of an ocean of liquid water covered with ice.

This is idea of a sub-surface ocean of liquid water is now quite popular. For more information on Europa click here for a start

It has not been possible to prove (2).  But we do know there is abundant water ice on the surface and it may be present beneath the surface too.
 
 

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