The Anatomy of a Diatomic Molecule
Imagine you are observing a single molecule of Hydrogen Chloride (HCl) floating in a gaseous state. It is not just sitting still; it is performing a complex, energetic dance.
The problem explicitly tells us that this molecule is exhibiting translational, rotational, and vibrational motions.
This is a crucial piece of information because it dictates how the molecule stores its thermal energy.
Counting the Degrees of Freedom
To understand the energy of the molecule, we first need to count its degrees of freedom (f). Think of degrees of freedom as the independent ways a molecule can move and store energy.
For a diatomic molecule like HCl:
1. It can move in 3-dimensional space (x, y, z axes), giving it 3 translational degrees of freedom.
2. It can rotate around two independent axes perpendicular to the bond connecting the atoms, giving it 2 rotational degrees of freedom.
3. Because the problem specifies vibrational motion, the atoms can oscillate back and forth along the bond. This contributes 2 vibrational degrees of freedom (one for kinetic energy and one for potential energy).
Adding these up, we get the total degrees of freedom:
The Law of Equipartition of Energy
Now, we bring in a powerful principle from statistical mechanics: the Law of Equipartition of Energy.
This law states that in thermal equilibrium, every single degree of freedom contributes an equal amount of average energy to the molecule, specifically 21kBT, where kB is the Boltzmann constant and T is the absolute temperature.
Since our HCl molecule has 7 degrees of freedom, its total average thermal energy (E) is:
Bridging the Microscopic and Macroscopic
We also know from the kinetic theory of gases that the total kinetic energy of a molecule can be expressed macroscopically using its root mean square velocity (vrms).
The formula for this kinetic energy is:
The problem states that the rms velocity is vˉ. So, we can write:
The Final Calculation
We now have two different expressions for the same total energy of the molecule. Let's equate them to find the temperature T:
Notice how beautifully the 21 on both sides cancels out!
Finally, we isolate T by dividing both sides by 7kB:
And there we have it! The temperature of the gas is directly related to the mass of the molecule, the square of its rms velocity, and inversely proportional to its degrees of freedom. This perfectly matches option (b).