The binding energy (\( BE \)) of a nucleus is calculated using the equation \( BE = \Delta m \cdot c^2 \), where \( \Delta m \) is the mass defect and \( c \) is the speed of light. For a helium nucleus, the mass defect (\( \Delta m \)) is determined by subtracting the nucleus's mass from the combined mass of its constituent protons and neutrons: \( \Delta m = (2m_p + 2m_n) - m_{\text{He}} \). The given values are: \( m_p = 1.0073 \, \text{u} \) (proton mass), \( m_n = 1.0087 \, \text{u} \) (neutron mass), and \( m_{\text{He}} = 4.0015 \, \text{u} \) (helium nucleus mass). Substituting these values yields \( \Delta m = (2 \cdot 1.0073 + 2 \cdot 1.0087) - 4.0015 = 4.0310 - 4.0015 = 0.0295 \, \text{u} \). To convert this mass defect to energy, we use the conversion factor \( 1 \, \text{u} = 931.5 \, \text{MeV/c}^2 \), resulting in a binding energy of \( BE = 0.0295 \cdot 931.5 = 28.4 \, \text{MeV} \). Final Answer: \[ \boxed{28.4 \, \text{MeV}} \]