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Physical Chemistry

Electronic Transition

Definition and meaning of Electronic Transition in chemistry.
An electronic transition is the movement of an electron between two fixed energy levels. These specific energy levels exist inside an atom or a molecule. The jump happens when the particle absorbs or releases a tiny packet of light called a photon.

In more detail

Electrons cannot simply exist anywhere they want around an atomic nucleus. They must sit in specific orbitals that have exact energy values. An electron can only jump if a photon exactly matches the energy gap between two orbitals.

Chemists calculate this required energy using the formula ΔE = hν = hc/λ. This strict rule explains why glowing gases produce sharp lines of color instead of a continuous rainbow. Molecules experience several common types of electron jumps when they absorb light.

These specific types include the σ→σ*, n→σ*, π→π*, and n→π* transitions. Each specific jump requires a different amount of photon energy to succeed. Quantum physics uses strict selection rules to predict if a jump will occur.

These selection rules look at the electron spin and the overall orbital symmetry. Jumps that follow all the selection rules are called allowed transitions. Allowed transitions happen almost instantly and absorb or release light very strongly.

Jumps that break the selection rules are given the label of forbidden transitions. Forbidden transitions are highly unlikely, so they happen slowly and show weak light interactions. This slow release of trapped light energy causes the lingering glow seen in phosphorescent materials.

Key facts

Field
Physical Chemistry
Governing equation
ΔE = hν = hc/λ
Common molecular types
σ→σ*, n→σ*, π→π*, n→π*
Underlies
UV-Vis and atomic emission or absorption spectroscopy
Driven by
The exact absorption or emission of a single photon
Example
Consider a simple hydrogen atom that has gained some extra energy. An excited electron might fall from the n=3 energy level down to the n=2 level. This specific downward jump releases a photon with a wavelength of exactly 656 nanometers. We see this exact photon as a bright red line in the atomic emission spectrum of hydrogen. This glowing red line is part of a famous group of visible lines called the Balmer series.

Frequently asked questions

What determines the energy needed for an electronic transition?

The energy gap between the starting and ending orbitals determines the exact requirement. An electron will only move if a photon perfectly matches that exact energy difference.

Why are some electronic transitions called forbidden?

Quantum selection rules make certain transitions highly improbable based on electron spin and orbital shape. These jumps are not truly impossible, but they happen very slowly and appear very weak.

How do electronic transitions explain the colors of neon lights?

Different atomic gases have completely unique sets of energy levels for their bound electrons. When the excited electrons fall back down, they release specific colors of light that create the glow.

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