1. Start with Newton's Law of Gravitation: \(F = G \frac{m_1 m_2}{r^2}\).
2. Rearrange to solve for G: \(G = \frac{F r^2}{m_1 m_2}\).
3. Substitute the SI units for each term:
F (Force) \(\rightarrow\) N (Newton)
r (distance) \(\rightarrow\) m (meter), so \(r^2 \rightarrow m^2\)
\(m_1, m_2\) (mass) \(\rightarrow\) kg (kilogram), so \(m_1 m_2 \rightarrow kg^2\)
4. Unit of G = \(\frac{\text{N} \cdot \text{m}^2}{\text{kg}^2} = \text{Nm}^2\text{kg}^{-2}\).