Decoding the Hydrogen Spectrum
The hydrogen emission spectrum is one of the most beautiful and foundational concepts in quantum mechanics. It provides direct evidence for the quantized nature of energy levels in an atom. In this problem, we are diving deep into the Balmer series, which is the only series of hydrogen that falls in the visible region of the electromagnetic spectrum.
Let's break down the given statements one by one to see which ones hold true.
Statement I
Convergence of Spectral Lines
The wave number of any spectral line in the hydrogen spectrum is given by the Rydberg formula:
uˉ=λ1=RH(n121−n221)
As we look at transitions from higher and higher energy levels (i.e., as n2 increases), the energy difference between consecutive levels becomes smaller and smaller. For example, the gap between n=3 and n=4 is much larger than the gap between n=10 and n=11.
Because the energy levels crowd together near the ionization limit (n→∞), the energy of the emitted photons approaches a maximum limit. Since energy is inversely proportional to wavelength (E=λhc), the wavelength approaches a minimum limit. This causes the spectral lines to bunch up or converge at the shorter wavelength (higher frequency) end of the series. Thus, Statement I is absolutely correct.
Statement II
The Balmer Series Definition
By definition, the spectral series are named based on the lower energy level (n1) to which the electron transitions:
- Lyman series: n1=1
- Balmer series: n1=2
- Paschen series: n1=3
Since the question specifically mentions the Balmer series, the integer n1 must be exactly 2. Statement II is correct.
Statement III
The Longest Wavelength
We know that the energy of a photon is given by E=λhc. This tells us that energy and wavelength are inversely related.
To find the longest wavelength (λmax), we need the transition that releases the minimum energy. In the Balmer series, the electron falls to n1=2. The smallest possible energy jump to n=2 is from the immediately adjacent higher level, which is n2=3.
Therefore, the line with the longest wavelength corresponds to the transition from n2=3 to n1=2 (often called the Hα line). Statement III is correct.
Statement IV
Ionisation Energy
Ionisation energy is defined as the energy required to completely remove an electron from the atom in its ground state. For hydrogen, the ground state is n1=1. The electron must be taken to n2=∞.
The wave number corresponding to the ionisation energy would be:
This transition belongs to the Lyman series, not the Balmer series. The Balmer series only gives us information about transitions ending at n=2. We cannot directly calculate the ionisation energy from the Balmer series lines alone without knowing the energy gap between n=1 and n=2. Thus, Statement IV is incorrect.
Final Conclusion
Statements I, II, and III are correct, while Statement IV is incorrect. This makes option (d) the right choice. Understanding these fundamental definitions is crucial for mastering atomic structure!