bksree said:
T
Since work is done by gravity each time, shouldn't its source (whatever that is) start running out of energy ? How is this physically manifest finally ?
Most of the potential energy has been there from the beginning. Every particle that makes up the Earth and everything around is some distance from the center of the earth, and energy would be released (work would be done) if that particle were to fall all the way to the center.
When something moves downwards (a boulder rolls into a valley, water flows downhill, we fill in a low spot in front yard) the gravitational energy that's released does some amount of work and eventually ends up as heat. However, that can only happen if there's a height difference somewhere. We need a high spot and a low spot so that something can move downwards from the higher spot to the lower spot - and every time that happens the high spot gets a bit lower, the low spot gets a bit higher, and we have less height difference to play with.
So the answer to your question is:
1) The Earth never "runs out" of gravitational potential energy, because every particle on the surface of the Earth is about 4000 miles from the center of the earth, and that's a long ways to fall.
2) We could, however, eventually run out of
usable gravitational potential energy (where "usable" means that it can be turned into work and kinetic energy). Once every low spot has been filled in and every high spot has been knocked down there are no longer any height differences, and without these height differences there's no possibility of moving downhill. The world would have to be a smooth and nearly perfect sphere.
3) However, the supply of usable gravitational potential energy is being continuously replenished: The movement of continental plates pushes up new mountains (imagine the amount of work done if we could drop the Himalaya mountains into the Marianas trench

); the sun heats water so that it evaporates and rises; we can use the chemical energy of our muscles to throw things into the air; and so forth.