The Composition of Icy moons


This drawing illustrates the general composition of icy moons.
Composition is generally determined by detailed measurements of the spectra of an object. Spectral measurements of the surfaces of some of these moons reveal the presence not only of ice but of several different kinds of snow (crushed ice).

The interior composition can be guessed from density mass of these moons, and so determined the densities to be about 1.2 (refer to the reference information for exact measurements of the icy moons). This density which is closer to that of ice than rock, so most of these moons must be made of ice.

The fact that they are made primarily of ice suggests a certain path for their evolution.


The Composition of Icy moons


This drawing illustrates the general composition of icy moons.
When the Voyager missions flew by some the icy moons, they took the spectra of the surface. The spectra matched that of ice and also several different kinds of snow (crushed ice).

The Voyager spacecraft could not measure the interior of the moons, however. Instead they measured the density. The density of iron or rock is between 3 and 5. The density of ice is 1. Voyager measured the densities to be about 1.2 (refer to the reference information for exact measurements of the icy moons), which is closer to that of ice than rock, so most of these moons must be made out of ice.

The fact that they are made primarily of ice suggests a certain path for their evolution.


The Composition of Icy moons


This drawing illustrates the general composition of icy moons.
Not only ice but several different kinds of snow (crushed ice) have been found on the surfaces of these moons.

Scientists can only guess what the inside is made of, but when the Voyager missions flew by some the icy moons, measurements were made that showed that the inside of the moons might also made of ice.

The fact that the major moons are made primarily of ice suggests a certain path for the evolution of these bodies.



Last modified April 9, 1997 by the Windows Team

The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). © The Regents of the University of Michigan. Windows to the Universe® is a registered trademark of UCAR. All Rights Reserved. Site policies and disclaimer