The gravitational force between two masses is measured by the gravitational constant, or G, which is a fundamental constant in physics. It makes an appearance in Newton’s law of universal gravitation and has a value of roughly 6.674 × 10⁻¹¹ N•m²/kg².
Gravitational constant is important because, its calculate the gravitational force between objects requires knowledge of the gravitational constant. It is utilised in equations explaining planetary motion, galaxy structure, and Einstein’s general theory of relativity. It also enables scientists to forecast how masses interact as a result of gravity.
It measured by Henry Cavendish and used a torsion balance experiment in 1798 to determine the gravitational constant for the first time. The minute force of attraction between lead spheres was measured by him. Although increasingly sophisticated methods are used in modern research, the inadequacy of gravitational forces makes measuring G difficult.
The relative weakness of gravity in relation to other fundamental forces in nature, such as electromagnetic, is reflected in the tiny value of G. When it comes to large things like planets, stars, and black holes, gravity becomes important despite its weakness.
The gravitational constant is represented in units of N•m²/kg² (newton meter squared per kilogram squared). These units ensure that the force of gravity calculated by using Newton’s law has the correct dimensions (newtons).
From Earthly objects to the motion of galaxies, the gravitational constant aids in explaining how gravity behaves on all scales. It plays a vital role in models of the creation and growth of the universe and is necessary to understand phenomena like gravitational waves and black holes.
Current data indicate that G remains constant in both space and time. However, certain physics models suggest that G could change over outer space timeframes or in harsh environments. This theory is being tested in ongoing research, but so far, no visible differences have been found.