Atomic Orbitals Lab

Visualize hydrogen atom wave functions in real time. Select quantum numbers to see orbital shapes as 2D density plots, radial probability distributions, and energy level diagrams. Explore how n, ℓ, and m determine the size, shape, and orientation of electron orbitals.

Guided Experiment: Exploring Quantum Numbers

How do the quantum numbers n, ℓ, and m affect the shape, size, and energy of hydrogen orbitals? What patterns do you expect for node counts?

Write your hypothesis in the Lab Report panel, then click Next.

1s Orbital(n=1, ℓ=0, m=0)
Low
Mid
High
(|ψ|² density)

Controls

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Orbital Properties

Orbital
1s
Energy
Quantum Numbers
Nodes
Radial: 0
Angular: 0
Total: 0

Data Table

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#nmOrbitalEnergy (eV)Radial NodesAngular NodesTotal Nodes
0 / 500
0 / 500
0 / 500

Reference Guide

Quantum Numbers

Three quantum numbers describe each orbital in the hydrogen atom.

n=1,2,3,=0,1,,n1m=,,+n = 1,2,3,\ldots \quad \ell = 0,1,\ldots,n{-}1 \quad m = -\ell,\ldots,+\ell

The principal number n sets the energy and overall size. The angular momentum number ℓ sets the orbital shape (s, p, d, f). The magnetic number m sets the orientation.

Hydrogen Wave Function

The wave function separates into radial and angular parts.

ψnm(r,θ,ϕ)=Rn(r)Ym(θ,ϕ)\psi_{n\ell m}(r,\theta,\phi) = R_{n\ell}(r) \cdot Y_{\ell}^{m}(\theta,\phi)

The probability density |ψ|² gives the likelihood of finding the electron at each point. Bright regions in the heatmap show where the electron is most likely found.

Radial Probability Distribution

The radial probability gives the likelihood of finding the electron at distance r from the nucleus, summed over all angles.

P(r)=r2Rn(r)2P(r) = r^2 |R_{n\ell}(r)|^2

Radial nodes (where P(r) = 0) are points where the radial wave function changes sign. The number of radial nodes is n − ℓ − 1.

Energy Levels and Spectral Lines

In hydrogen, the energy depends only on the principal quantum number n. All subshells with the same n have the same energy (they are degenerate).

En=13.6 eVn2E_n = -\frac{13.6 \text{ eV}}{n^2}

The ground state (n = 1) has E = −13.6 eV. As n increases, levels get closer together, converging to 0 eV at ionization.