The Anatomy of a Diatomic Molecule
Imagine a diatomic gas molecule, like oxygen (O2) or nitrogen (N2). It looks like a tiny dumbbell flying through space. To understand its energy, we need to know all the independent ways it can move—these are called its degrees of freedom (f).
First, it can translate (move in a straight line) along the x, y, and z axes. This gives us 3 translational degrees of freedom (ftrans=3).
But it doesn't just fly straight; it tumbles! It can rotate end-over-end in two independent ways (imagine spinning a baton). We don't count rotation along its own internuclear axis because the atoms are essentially point masses, and the moment of inertia is negligible. So, that gives us 2 rotational degrees of freedom (frot=2).
Adding them up, the total degrees of freedom for our diatomic molecule is:
The Law of Equipartition of Energy
Now, let's talk about how this molecule stores thermal energy. The Law of Equipartition of Energy is a beautiful principle that states that every active degree of freedom contributes exactly 21RT to the internal energy per mole of the gas.
Since our gas has 5 degrees of freedom, the total internal energy U for μ moles is given by:
In our specific problem, we are dealing with exactly 1 mole of gas (μ=1). Substituting our values, we get:
Half the problem is solved! We now know the internal energy.
The Magic Ratio
Gamma (γ)
Next, we need to find γ, which is the ratio of molar specific heat at constant pressure (Cp) to the molar specific heat at constant volume (CV).
There is a direct, incredibly useful relationship between γ and the degrees of freedom f:
Let's plug in our value of f=5:
Taking the lowest common multiple, we get:
And there we have it! The internal energy is 25RT, and the ratio of specific heats γ is 57. This perfectly matches option (c). Always remember that the atomicity of the gas (monoatomic, diatomic, polyatomic) dictates the degrees of freedom, which in turn dictates all its thermodynamic properties!