Newton's Gravitational Law and Heavenly Bodies Comments by Sherif Monem

Newton's Gravitational Law and Heavenly Bodies

Since there is no absolute scientific definition of distance between heavenly bodies or absolute scientific definition of distance between ultimately close objects then forward Newton's  law of gravity can not strictly be applied.

In addition there may be different gravitational paths to figure out the distance between two objects, as just there may be two or more paths or distances. Some may be main ways and the others are byways.

Very proximity electromagnetic laws will apply. Certain close distances both gravitational and electromagnetic forces will apply. Then from far away and approaching the object the stages are gravitational, mix gravitation and electromagnetic then electromagnetic dominant.

Sherif Monem modification of Newton's Law of gravity for two close bodies facing a third one

My Theory of Gravity

The Newton's law of gravity will not be accurate if there are two bodies m2 and m3  close to each other facing m1. My theory or hypothesis. The energy packets emitted from m1 will be shared by m2 and m3 since they are in the same direction.

If two bodies of mass m1 and m2 get two close together then the gravitational force between them will be reaching infinity. How this can happen? I theorize there will be some interaction of the gravitational forces and the electromagnetic and electrostatic properties of the body services'

Some reasoning can be given but no analytical analysis are available.

Newton's law of gravity

Image: decodedscience.com

Newton's law of gravitation - (physics) the law that states any two bodies attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. law of gravitation.

Mathematically, this translates into the force equation:

F_G = Gm₁m₂/r²

In this equation, the quantities are defined as:

• F_g = The force of gravity (typically in newtons)
• G = The gravitational constant, which adds the proper level of proportionality to the equation. The value of G is 6.67259 x 10^-11 N * m² / kg², although the value will change if other units are being used.
• m₁ & m₁ = The masses of the two particles (typically in kilograms)
• r = The straight-line distance between the two particles (typically in meters)