Homework #2
SOLUTION
You can find information that you can use for this homework problem at the "Chemicool" web site (linked to the course schedule as Web database on the elements). Continue your answers on the back if you need more room.
Whether an element or compound will be abundant in a solar system body depends very much on the element or compound's volatility. An indication of a material's volatility can be obtained from its boiling point, that is, the temperature (at 1-atmosphere pressure) at which the material has its liquid and vapor phase in equilibrium. The opposite of a volatile element or compound is a refractory element or compound -- this would be an element or compound that forms a vapor phase only at very high temperatures.
1. This table gives the relative
amounts of elements in the Sun. List the first three noble
(inert) gases, and for each,
give
its abundance in the Sun, relative to silicon:
element:
Helium
number per Si atom:
2162
element:
Neon
number per Si atom:
3.5
element:
Argon
number per Si atom: 0.1
Pure
hydrogen is a gas at 1-atmosphere pressure and room temperature.
It
boils at 20 K (much lower temperature than room temperature, 300 K),
and so it is very volatile.
6. Hydrogen atoms can combine with oxygen atoms to form H2O
molecules (water). Is water more or less volatile than pure
hydrogen?
Is water more or less volatile than pure oxygen? Explain your
answers.
Hydrogen
boils at 20 K, and oxygen boils at 90 K (they are both cryogens).
In contrast, water boils at 100 Centigrade, or 373 K, so it's a lot
less volatile than the elements of which it is composed. This
tells us that volatile elements can be a lot less volatile when they
are in chemical compounds. Similarly, Earth's rocks contain
significant amounts of oxygen, a volatile element by itself.