rewebster said:
I still think the energy required will be too much for the 'elevator' string--from the speed going up that's suggested of the packet, the pressure on the string to attain the added orbital velocity, the weight of the string in the Earth's gravity pulling it back to earth, the relation to the 'drag' effect in the Earth's atmosphere and that drag added in for the ascending packet, the tension pressure at and near the 'weighted end' to counter all these, any and all things passing through the atmosphere and orbiting, etc.
Calculating the
static characteristics of a space elevator is just math. Plug in the physical constants, turn the crank, and out pop required capabilities. No known material came close to having the required capabilities, not even close. Unobtainium was needed. The discovery of carbon nanotubes in the early 1990s changed everything. Carbon nanotubes (short strands of them, at least) have more than the requisite tensile strength. There are still many problems, but the material has changed from unobtainium to something real.
but I hope post 33 added to the OP 's question and solution
Back to post 33 then.
rewebster said:
If an object could somehow be placed at that altitude where geosynchronous orbits occur, the thrust required to set it into a geosynchronous orbit (around the planet), to me, would have to be quite a bit more than the energy required to provide an escape velocity (away from the planet).
Last item first: Escape velocity is a misnomer. It really should be escape speed. The direction of the velocity vector doesn't come into play when it comes to determine whether an object will escape the Earth's (or some other object's) gravity well. The only thing that matters is the magnitude of the velocity vector; i.e., speed.
An object in a circular orbit at some distance
r from some object with mass
M has speed given by
[tex]v^2 = \frac{GM}{r}[/tex]
Escape velocity, on the other hand, is determined by
[tex]v^2 = 2\,\frac{GM}{r}[/tex]
In other words, escape velocity is [itex]\surd 2[/itex] times circular orbit speed. Always. If some (small) object of mass
m is located some distance
r from a planet and has zero inertial velocity with respect to the planet, the energy needed to place the object into circular orbit is half of the energy needed to place the object on an escape trajectory.