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.
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 ; the viewer combines them as and .
Procedure
- Start in the bonding state at Å (the measured H–H length) and rotate the cloud to see the sausage-shaped σ orbital enclosing both nuclei.
- Switch to the antibonding state at the same and locate the nodal plane halfway between the nuclei.
- Slide down to 0.3 Å and up to 3.0 Å in both states; note where density piles up or collapses between the nuclei.
- 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 the two nuclei nearly merge and the σ cloud looks like the 1s orbital of He; at large 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 – Å.
Explanation
Molecular orbital theory combines atomic orbitals into wavefunctions spread over the whole molecule. For the two 1s orbitals add in phase to give (electron density between the nuclei screens their repulsion and binds the molecule) or out of phase to give (a nodal plane leaves density outside, so filling it weakens the bond). The energy gap between σ and σ* shrinks as 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
Virtual experiment: a simplified model to build intuition. It does not replace real lab work or safety training; never repeat chemistry at home without supervision.