Galilean Satellites:
The satellites discovered by Galileo with his small telescope form a
small, `mini' solar system around Jupiter. They each have special
characteristics related to their formation process, but have the
following traits in common:
1) all orbit Jupiter
2) they all are tidally locked to Jupiter
3) they all have radii larger than our Moon
4) the inner moons have densities higher than outer moons (implies that
Jupiter was much warmer in the past, such that the moons formed near
Jupiter have less of the volatile elements such as CO2 and
H2O)
Io:
Io is the innermost world, closest to Jupiter and can be classified as one of the
most unusual moons in our solar system. Its unique properties include:
Europa:
Europa is the next world out from Io and is considered a strong
candidate to find primitive life. Its characteristics are:
- icy world with high albedo, smooth surface with only a few
hills/mountains and craters, meaning the surface is young and renewing
itself
- large long cracks on the surface, due to ice plate tectonics floating
on water mantle
- visible surface is actually H2O ice mixed with rock (dirty
icefield) about 100 km thick

Ganymede:
Ganymede is much less dense than Europa or Io. Its interesting
characteristics are:
- very diversified surface with dark regions, valleys, mountains,
evidence of past tectonic activity and lots of vertical relief
- low mean density implies a very deep ice mantle, about 1000 km
thick
- white craters and rims =
impact exposes mantle ice
- ghost craters = smoothed by ice flow
- thin oxygen atmosphere, possible aurora at its poles (magnetic
field?)
Callisto:
Callisto is the outermost of the 4 primary satellites:
- similar surface to Ganymede but with 10 times more cratering,
which means less tectonic activity, cooler interior
- little vertical relief = craters destroyed landscape = weak surface
material (low density)
- large impact basins
Summary of Galilean Moons:
- mini-Solar System model where the closer moons are rocky, high density
and the outer moons are icy, low density
- geological activity decreases with distance from Jupiter, due to the
decreasing tidal friction from Jupiter on interior of moons - this has a
marked influence on the appearance of their surfaces
- little or no atmospheres
- high icy component to crust of all moons

Titan:
Titan is the largest satellite of Saturn, unique in its methane
atmosphere:
- detected to have spectral lines of methane in 1944
- surface mapped in IR
- heavy atmosphere (1.4 times the Earth's) with structure in the form of
haze - reddish color from organic molecules formed by breakdown of CH4 by
cosmic rays
- composition of atmosphere is 90% N2, 7% CH4, 2%
Ar and traces of ethane, acetylene, ethylene, propane and hydrogen cyanide
(i.e. smog)
- the temperature and pressures are near the triple point of methane
(CH4) -> methane rain, snow, ice, clouds, rivers, etc.
- Earth's environment is near the triple point of water - water
serves as the solvent for organic chemicals to interact = life. Titan
is an excellent place to search for new forms of life based on methane
as a solvent