00:01
We're given that the radius of a hydrogen atom is about a tenth of a nanometer.
00:07
So the volume of a hydrogen atom is 4 3rds pi r cubed.
00:14
So for gas, pressure is 1 atmosphere, the temperature is 0 degrees c, which is 273 kelvin.
00:31
So we can get n over v, which is kind of the number density of molecules in the gas, is p over rt.
00:47
So let's not confuse this r, the ideal gas constant, with rh, the radius of the hydrogen atoms.
00:57
So the volume of molecules is the number of moles times avogadro's number times the volume of an individual hydrogen atom.
01:06
So if i take that and divide by v, i get this, and then i've got my little n over v thing, so that's p over rt.
01:35
We know that the ideal gas constant is 0 .821 liter atmospheres per mole degree kelvin.
01:43
So we need to have that form of the ideal gas constant because our pressure is in atmospheres...