To find the binding energy (\( BE \)) of a nucleus, we use the equation:
\[
BE = \Delta m \cdot c^2,
\]
where \( \Delta m \) is the mass defect and \( c \) is the speed of light.
For the helium nucleus, the mass defect is:
\[
\Delta m = (2m_p + 2m_n) - m_{\text{He}},
\]
where:
- \( m_p = 1.0073 \, \text{u} \) is the mass of a proton,
- \( m_n = 1.0087 \, \text{u} \) is the mass of a neutron,
- \( m_{\text{He}} = 4.0015 \, \text{u} \) is the mass of the helium nucleus.
Substitute the values for the protons and neutrons:
\[
\Delta m = (2 \cdot 1.0073 + 2 \cdot 1.0087) - 4.0015 = 4.0310 - 4.0015 = 0.0295 \, \text{u}.
\]
Now, to convert the mass defect into energy, we use the conversion factor \( 1 \, \text{u} = 931.5 \, \text{MeV/c}^2 \):
\[
BE = 0.0295 \cdot 931.5 = 28.4 \, \text{MeV}.
\]
Final Answer:
\[
\boxed{28.4 \, \text{MeV}}.
\]