The Hydrogen Spectrum
When an electron in a hydrogen atom jumps from a higher energy level to a lower one, it emits a photon. The energy, wavelength, and wave number of this photon can be precisely calculated using the Rydberg formula. This formula is a cornerstone of atomic physics, elegantly connecting the discrete energy levels of an atom to the observable spectral lines.
The Rydberg Formula
The Rydberg formula for the wave number $\bar{
u}$ is given by:
Here, RH is the Rydberg constant, Z is the atomic number, ni is the initial energy level, and nf is the final energy level.
For our specific problem, we are dealing with atomic hydrogen, so Z=1. The electron is falling from the 8th orbit, meaning ni=8, and it lands in some final orbit nf=n. Substituting these values into our formula, we get:
Unveiling the Straight Line
Let's expand this expression to see its mathematical structure more clearly. By distributing the Rydberg constant RH inside the bracket, we separate the variable part from the constant part:
Now, take a close look at this equation. Does it remind you of something from coordinate geometry? It perfectly matches the standard equation of a straight line:
In our case, the y-axis represents the wave number $\bar{
u}$, and the x-axis represents the variable n21.
The Final Verdict
By comparing the two equations, we can easily identify the slope and the y-intercept of our plot. The slope m is the coefficient of our x-variable, which is simply the Rydberg constant RH. The y-intercept c is the constant term, which is −64RH.
Therefore, if we plot the wave number $\bar{
u}$ against n21, we will obtain a straight line with a positive slope equal to RH. This elegant linear relationship is a direct consequence of the quantized nature of atomic energy levels!