An atomic emission spectrum of hydrogen shows three wavelengths: 121.5 nm, 102.6 nm, and 97.23 nm. Assign these wavelengths to transitions in the hydrogen atom.

Key Concepts

Atomic Emission Spectrum

An atomic emission spectrum is a spectrum of the electromagnetic radiation emitted by a substance when its atoms transition from a higher energy state to a lower energy state. Each element has a unique emission spectrum, which can be used to identify the element and its electronic transitions. In hydrogen, these transitions correspond to specific wavelengths that can be observed in the ultraviolet region of the spectrum.

Energy Levels in Hydrogen Atom

The hydrogen atom has quantized energy levels, which are defined by the principal quantum number (n). Electrons can occupy these discrete energy levels, and when they absorb energy, they can jump to a higher level. When they return to a lower energy level, they emit energy in the form of light at specific wavelengths, which correspond to the differences in energy between the levels.

Balmer and Lyman Series

The Balmer and Lyman series are sets of spectral lines corresponding to electron transitions in the hydrogen atom. The Lyman series involves transitions to the n=1 level and emits ultraviolet light, while the Balmer series involves transitions to the n=2 level and emits visible light. The wavelengths provided in the question correspond to transitions in the Lyman series, specifically from n=2 to n=1 and n=3 to n=1.