Newton's gravitational constant (G) serves as a fundamental reference in physics, allowing comparisons across different gravitational situations. It is derived from the law of gravitational acceleration, expressed as g = GM/r², which can be reformulated to highlight the relationship between various masses and distances. The constant G remains consistent regardless of the chosen reference values for mass (M0) and distance (r0), although its units may vary based on these choices. This underscores the arbitrary nature of the reference situation in determining G's value. Ultimately, G represents a universal relationship that holds true across different physical contexts.