Newton's Law of Universal Gravitation
Every particle of matter attracts every other particle with a force directed along the line joining them. For two point masses m1 and m2 separated by a distance r, the magnitude of the attraction is
F=r2Gm1m2,
where G=6.67×10−11 N m2kg−2 is the universal gravitational constant. The force is attractive, acts along the line of centres, and obeys Newton's third law (equal and opposite on the two bodies). Its defining feature is the inverse-square dependence on separation.
Superposition. When several masses act on a body, the net gravitational force is the vector sum of the individual forces. For an extended body — a rod, ring or shell — the body is treated as a collection of point-mass elements and the contributions are integrated. For a uniform ring of mass M and radius R, the force on a point mass m placed on its axis at distance h from the centre is directed along the axis and has magnitude
F=(R2+h2)3/2GMmh,
because the components perpendicular to the axis cancel by symmetry while the axial components add. This axial formula is not a simple 1/h2 law: as h changes, the force scales as h/(R2+h2)3/2, so comparing the force at two axial positions (say h and 2h) means substituting into this expression rather than using the point-mass inverse square directly. Only when h≫R does the ring behave like a point mass and F→GMm/h2.
Newton's law of gravitation is one of the earliest topics in the NCERT Class 11 Physics chapter on Gravitation, and "universal law of gravitation formula and examples" or "gravitation class 11 important questions" are searched constantly by CBSE board and NEET/JEE Main aspirants. The extended-body superposition case shown here — finding the force due to a ring on an axial point mass — is a classic JEE Main gravitation numerical built directly on this NCERT Class 11 foundation.