- always an attractive force,
- proportional to the mass of each object
- proportional to 1/ r², where r is their distance apart.
These last two requirements can be summarised as:
Gravitational force F= Gm₁m₂/r²
where m₁ and m₂ are masses of the two objects
The constant of proportionality,G, in the above equation, is called the universal constant of gravitation.
G can be given units of Nm²kg¯². The value of G is 6.67 x 10¯¹¹ Nm²kg¯².
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