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By a process of logic that I will not attempt to describe, 
Newton deduced that the force  F  between two objects with 
masses  m  and  M  separated by a distance  r  
was given by 
   | 
(10.3) | 
 
where  
 m
kg
s-2  
is the Universal Gravitational Constant.  
Actually, Newton didn't know the value of G; 
he only postulated that it was universal - 
i.e. that it was the same constant of proportionality 
for every pair of masses in this universe.  
The actual determination of the value of G 
was first done by Cavendish 
in an experiment to be described below.  
We should also express this equation in vector form 
to emphasize that the force on either mass acts in the 
direction of the other mass:  
if  
  denotes 
the force acting on mass  m2  
due to its gravitational attraction by mass  m1  then 
   | 
(10.4) | 
 
where  
  
is a unit vector in the direction of 
 
,  
the vector distance from m1 to m2, 
and  r12  is the scalar magnitude of 
.
Note that the reaction force  
  
on m1 due to m2 is obtained by interchanging the labels 
``1'' and ``2'' which ensures that it is equal and opposite 
because  
  by definition.  
 
 
 
 
   
 Next: Weighing the Earth
 Up: Celestial Mechanics
 Previous: Kepler's Laws of Planetary Motion
Jess H. Brewer 
1998-10-08