Than you for useful information.
This is not so easy to estimate necessary precision.
Let I just write final purpose of these questions:
There is physical value Φ – gravitational potential
http://en.wikipedia.org/wiki/Gravitational_potential
Lets introduce another similar physical value.
Lets mark it for now like Θ and describe it like so:
Θ = g*r
where g is total gravitational acceleration and
r is radius of curvature of gravitational force.
This r can be found like so.
See picture:
http://www.part.lt/img/d653dc3bc9e1aa48d6c4bc6ad672b3cc965.png
(if link will not work just copy paste it to your browser)
Lets consider some point in space (black dot)
Then let's take some very close point (gray point) and find where vectors of gravitational
forces intersects (red point)
Now we have, r is distance between black and red points.
Φ almost equals to Θ outside our planet.
But inside they may differ a lot.
For example at the center of the planet Θ will be almost 0
The reason/target of previous questions was how to calculate or measure the difference
between Φ and Θ at Mariana Trench or at some other places where it is measurable difference.
Or maybe better I need to look for differences at some places in space?
Maybe at the points where Earth's and Sun's gravitational forces becomes equivalent?