madchemist said:
I welcome all thoughts and ideas...
Let's take Newton's second law: ##\vec F = m\vec a## and consider a mass at centre of a planet. The mass is at rest, so there no acceleration and, therefore, no "force".
But, the ##\vec F## in Newton's second law is
net external force. You can crush an object by applying a uniform force to all sides. The (centre of mass of the) object does not accelerate in the sense of Newton's second law because there is no net force. But, the object is subject to a crushing pressure.
Let's take an non-gravitational analogy. We have a line of blocks (perhaps 11 blocks) and we apply an inward force to each end block. There are no
external forces applied to any other block. But, there is still pressure on the centre block because of the external force on the end blocks.
Now, we apply an additional (external) inward force to the second block from each end. The internal pressure on the middle block increases.
Finally, we imagine an external force on each block except the centre one, decreasing linearly perhaps towards the centre. There is no external force on the middle block, but it is still under pressure according to the sum of the external forces on the other blocks.
The pressure on the centre block is a consequence of Newton's second and third laws. The forces on each block must be balanced (zero acceleration and Newton's second law). And, each block has an equal and opposite normal force with each of its neighbours. If you specify the external forces, you can easily calculate the force on both sides of each block. And, the centre block is under the greatest pressure.
The situation for a large mass under gravity is the spherical equivalent of this.
Note that a perfect large shell of zero thickness would be an unstable equilibrium. But, any deviation from perfection would lead to the shell's collapse under the mutual gravitational attraction of its constituent particles. Likewise, for any material, there would be a maximum size of hollow sphere before the pressure on the inner part of the sphere becomes too great and the sphere collapses under its own gravity.