Chemistry Labs
Undergraduate · 20 min

Bonding and antibonding orbitals of H₂

Build the molecular orbitals of the simplest molecule from two 1s atomic orbitals, then stretch and compress the bond to see how the bonding advantage disappears.

3D electron cloud of a σ molecular orbital of H₂: two nuclei inside a shared density for the bonding state, or two separated lobes with a node between them for the antibonding state.

Goal

Compare the σ bonding and σ* antibonding clouds, and find the bond length where overlap is strongest.

Apparatus and reagents

A pair of hydrogen 1s orbitals at distance RR; the viewer combines them as σ=12(1sa+1sb)\sigma = \frac{1}{\sqrt{2}}(1s_a + 1s_b) and σ∗=12(1sa−1sb)\sigma^{*} = \frac{1}{\sqrt{2}}(1s_a - 1s_b).

Procedure

  1. Start in the bonding state at R=0.74R = 0.74 Å (the measured H–H length) and rotate the cloud to see the sausage-shaped σ orbital enclosing both nuclei.
  2. Switch to the antibonding state at the same RR and locate the nodal plane halfway between the nuclei.
  3. Slide RR down to 0.3 Å and up to 3.0 Å in both states; note where density piles up or collapses between the nuclei.
  4. Estimate where the bonding cloud maximises density between the nuclei and compare with the equilibrium bond length.

What to observe

  • In the bonding state the cloud fills the internuclear region; in the antibonding state a nodal plane empties it completely.
  • At very short RR the two nuclei nearly merge and the σ cloud looks like the 1s orbital of He; at large RR the density splits back into two isolated atoms.
  • Density between the nuclei — hence the bond — is strongest near the middle of the slider range, around R≈0.7R \approx 0.7–0.80.8 Å.

Explanation

Molecular orbital theory combines atomic orbitals into wavefunctions spread over the whole molecule. For HX2\ce{H2} the two 1s orbitals add in phase to give σ\sigma (electron density between the nuclei screens their repulsion and binds the molecule) or out of phase to give σ∗\sigma^{*} (a nodal plane leaves density outside, so filling it weakens the bond). The energy gap between σ and σ* shrinks as RR grows — at dissociation both combinations cost the same energy. This LCAO picture is the simplest case solved by Hartree–Fock and by density-functional codes for real molecules.

Chemists behind it

Related topics

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