davenn said:
I'm still concerned that you may think that 2 objects that are both much smaller mass that say the Earth, don't hit the ground at the same time ?
Me too.
There is a great temptation to look at these things from the point of view that says "Science got it wrong". I feel that is unhealthy because it neglects the basic authority of what is, in modern times, a very well justified body of work. In all matters Scientific, the actual numbers count and you have to take account of that before thinking that someone has found a loophole. Galilieo's (thought?) experiment shows that 'things fall down with the same acceleration'. That has been demonstrated to be true to greater and greater accuracy over the years.
What happens between bodies of near equal masses (planets etc.), follows the
exact same rules and the
same basic equations until General Relativity comes into it. You just have to look at the real (quantitative) consequences of that.
The attractive force between two masses m and M is always F = mMG/d
2. (G is the universal gravitational constant and
not g, d is the distance between the centres of mass of the two objects and both objects are actually heading for their
mutual centre of mass )The resulting acceleration of the two bodies will be F/m and F/M. Newton tells us that. Clearly the larger mass will accelerate less than the smaller mass. F/m is the same for any value of m and it
only depends on the 'other' mass M.
So why is it that that Earth seems to be different from the falling ball? Simply because the two accelerations are
so different and the Earth's surface accelerates so little, relative to the centre of mass of the two. One easily measurable effect of what happens between two no-dissimilar masses is the wobble of the Earth as the Moon orbits it. The Centre of mass of the two (the Barycentre) is about 4500km from the Earth's centre, which shows that the Earth
is pulled into 'an orbit' by the gravity of the Moon. There are no convenient stationary large masses up there to observe how they fall together so we have to imply things from orbiting objects but the centripetal acceleration of the Earth as it orbits round the barycentre is (2Πf)
2 r which comes to about
30μm/s2. How much less is the acceleration of the Earth when you drop a 1kg mass - or a 10kg - or a 1000kg? That's why we can say the Earth stays still for the Galileo experiments and why we can use g all over the place.