The magnitude of the force of gravity between two bodies is proportional to the product of their masses:
F=Gfracm1m2r2
This doesn't change depending on which body you're applying the force to, i.e. if you interchange the masses. The magnitude is the same.
What does change is the direction of the force. Force is a vector quantity, denoted as vecF or mathbfF. If we write the equation for gravity using proper vector notation, we have
mathbfF=Gfracm1m2|mathbfr1−mathbfr2|2fracmathbfr1−mathbfr2|mathbfr1−mathbfr2|
Here, the positions of the objects are represented by vectors, mathbfr1 and mathbfr2. Additionally, |mathbfx| denotes the norm of a vector mathbfx - its magnitude.
Now, if you interchange the masses, the direction of the force changes, although |mathbfr1−mathbfr2|=|mathbfr2−mathbfr1|, because this refers to the magnitude of the vectors. So the force applied on one object is the opposite of the force applied on the other object. This is Newton's third law.
The acceleration is more interesting. The force on object 1 due to gravity is
F1=m1g1
Here,
g1=fracGm2r2
where m2 is the other mass. This should tell you that g1neqg2, except when m1=m2.
I'm not an expert in general relativity, but I do know that it describes how spacetime curves due to the presence of one body. The solution to the Einstein Field Equations, the metric, is different for different bodies, because one piece of it, the stress-energy tensor, is different for objects of different mass/energy/etc.
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