The gravitational constant in Newton's equations is primarily a scalar constant derived from experimental measurements, rather than a tensor. It serves as a conversion factor between energy units and the curvature of space-time, linking the stress-energy tensor to gravitational effects. The gravitational constant has specific units of m^3 s^{-2} kg^{-1}, which facilitate dimensional analysis in gravitational equations. These units reflect its role in expressing force, as seen in the equation F_g = G(m_1 m_2)/r^2. Understanding its nature is crucial for grasping the relationship between gravity and the geometry of space-time.