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Level Abundances

One Atom vs. Many Atoms

When an atom is by itself, in isolation, its orbitals behave differently than when in packed tightly with other atoms. For example, the energy levels of a single carbon atom are slightly different than a diamond. Similarly, hydrogen gas (H2) is a tiny bit different than a simple H atom. The difference in energy levels, however, is not much in that case. The Hydrogen Atom Simulator showed just one H atom.

Astronomically one H atom is never observed. Rather, only vast numbers of Hydrogen atoms together are observed. Often they atoms (or H2 molecules) are on average far enough apart so that the orbitals aren't significantly altered. Another way of saying that is the density is “low”. But even when the density is low (which we will assume here), there are the occasional collisions between the atoms. When they collide some of the energy goes into them bouncing off of each other and some of it can go into exciting electrons. How frequently collisions occur and how much energy typically goes to exciting the atom depends on how fast the low density cloud of hydrogen atoms are moving on average. A way to measure the average speed of the atoms with respect to each other is temperature.

Thermal Distribution

To the right is shown a histogram of 1025 Hydrogen atoms. The density of the atoms is low so that their energy levels are very close to what we see for a single atom. The temperature can be varied from 3000 K to 30,000 K (a range which includes the surface temperature of almost all stars). Experiment with the slider.

this page is mirrored from astro.unl.edu — 19 July 2014