To convert from m^3*s^-2*kg^-1 to cm^3*s^2*g^-1, we need to use the conversion factor of 1 m = 100 cm and 1 kg = 1000 g. This means that we can multiply the given value of G by (100 cm)^3/(1 m)^3 and (1000 g)/(1 kg) to get the equivalent value in cm^3*s^2*g^-1.
The value of G in cm^3*s^2*g^-1 is 6.67x10^-8.
G, also known as the gravitational constant, is a fundamental physical constant that relates the strength of the gravitational force between two objects to their masses and the distance between them. The units of m^3*s^-2*kg^-1 represent the proportionality constant in the equation for gravitational force, F = G*(m1*m2)/r^2, where m1 and m2 are the masses of the objects and r is the distance between them.
Yes, G can be expressed in different unit systems, but the most commonly used unit system for G is the SI (International System of Units) system, which uses meters, kilograms, and seconds as base units. However, it is important to note that the value of G may vary depending on the unit system used, so it is essential to use the correct unit conversion when working with this constant.
G is a very small and difficult constant to measure, as it requires very precise and sensitive equipment. It is typically determined through experiments involving the motion of celestial bodies, such as planets and stars. The most accurate and recent value of G was determined by the Cavendish experiment in 1798, which measured the gravitational force between two small lead spheres.