The dissociation energy of a molecule is the energy required to break it into its constituent neutral atoms.
For the hydrogen molecule ($H_2$), dissociation means splitting it into two hydrogen atoms (H).
The energy balance can be represented as:
$ \text{Energy}(H_2 \text{ molecule}) = 2 \times \text{Energy}(H \text{ atom}) - \text{Dissociation Energy} $
Rearranging the formula to find the dissociation energy ($D_{H_2}$):
$ D_{H_2} = 2 \times \text{Energy}(H \text{ atom}) - \text{Energy}(H_2 \text{ molecule}) $
We are given:
$ 2 \times E_H = 2 \times (-13.6 \text{ eV}) = -27.2 \text{ eV} $
$ D_{H_2} = (2 \times E_H) - E_{H_2} $ $ D_{H_2} = (-27.2 \text{ eV}) - (-31.7 \text{ eV}) $ $ D_{H_2} = -27.2 \text{ eV} + 31.7 \text{ eV} $
$ D_{H_2} = 4.5 \text{ eV} $
The calculated dissociation energy for the $H_2$ molecule is 4.5 eV.
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