QuantumDefect
- 64
- 0
I was wondering if any of you could explain how Newton derived his Law of Gravitation: F=G*m_1*m_2/r^2 ? If this question is to vague tell me, thanks guys.
Adrian Baker said:Newton relied heavily on Keplar's three laws of Planetary motion. These were deduced from the data that Tycho Brahe obtained over many years. These laws seemed to be correct, but didn't explain WHY objects orbited as they did.
Newton devised laws of circular motion and realized that the same force that made things fall down on Earth, was responsiple for the Centripetal force that keep the planets in orbit. This was his 'Eureka' moment - realising that the two forces were one and the same.
Newton then showed mathematically that the gravitational force between two objects was proportional to their masses and inversely proportional to the square of the distances between them.
To get a value for the constant 'G' he estimated the density of planet Earth and from that estimated its mass.
Clever chap...!
Adrian Baker said:Yes, Cavendish was the first to calculate the Earths mass (and big 'G'), but as Integral points out above - do you really thing Newton wouldn't have tried to estimate its value?
Adrian Baker said:It isn't that hard to make an estimate of the Earth's mass is it? The Earth is mosly made of rock and it must be Iron rich due to it having a magnetic field. Estimate the proportions of each, measure the density of an average rock, add a bit for the iron rich core and then use the Earths dimensions to work out its mass. From this you get big 'G'.