» Newton's Law of Universal Gravitation

Newton's Law of Universal Gravitation states that two point masses attract each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them:

$$F_{1}=F_{2}=G\frac{m_{1}m_{2}}{r^{2}}$$


where,

Gβ€” gravitational constant,
m1β€” mass of the first object,
m2β€” mass of the second object,
rβ€” separation between the masses.

Gravitational Constant

Gravitational constant (symbol G, also known as the universal gravitational constant, Newton's gravitational constant, or Cavendish's gravitational constant) is a physics constant that characterizes the strength of the gravitational force. Its value is:

$$G=6.67430(15) \times 10^{-11} \frac{N\times m^{2}}{kg^{-2}}$$


The first indirect measurement of the gravitational constant is attributed to Henry Cavendish in 1798.


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FAQ

What does Newton's law of universal gravitation describe?

It describes the attractive force between two masses.

What is the gravitational constant?

It is the constant G in the gravitation formula that sets the strength of the force.

How does distance affect gravity?

The force decreases with the square of the distance between the objects.