![]() © Ronald J. Maddalena 1998
|
The false-color
image to the left, created by the NRAO 140 FT telescope in Green Bank,
shows where one can find hydrogen atoms
toward Orion. The regions with the most atoms are red. The white
regions to the left is where we don't have observations with the 140 FT.
Most of the interstellar gas is hydrogen and most of the hydrogen is in the form of atoms. Thus, astronomers study atomic hydrogen to find out the properties of a good portion of the interstellar gas. Hydrogen can also be in the form of molecules or ions. If a region of gas is hot enough, molecules can be destroyed and then become atoms or ions. Or, if a region cools then molecules might form from the atoms. |
Start Here | Optical
| InfraRed | Molecules
| Atoms | Continuum | Mythology
Take the Test | Glossary | Credits
| Get
Help
© Ronald J. Maddalena 1998