- #1
Tiiba
- 54
- 0
I'm trying to understand the chemistry of stars. At what point do molecules really end?
I guess there would be no one temperature where every molecule of hydrogen breaks apart in unison, but there should be an equation that says: if a diatomic gas is held together by 100 kJ/mol, at a temperature of 5000 kelvin it will be mostly individual atoms.
So, is there? I can't find anything.
(And if it's a complex situation for real gases, is there a formula that would make the same prediction for two hard spheres held together by a rubber band, or some other idealization?)
I guess there would be no one temperature where every molecule of hydrogen breaks apart in unison, but there should be an equation that says: if a diatomic gas is held together by 100 kJ/mol, at a temperature of 5000 kelvin it will be mostly individual atoms.
So, is there? I can't find anything.
(And if it's a complex situation for real gases, is there a formula that would make the same prediction for two hard spheres held together by a rubber band, or some other idealization?)