13 Feb '15 16:58>2 edits
Well, I hope I'm not boring you with all this, but I found two things:
(1) An analytic way to solve this equation for velocity as a function of the radius (An analytic solution for position as a function of time is a whole other ball game).
(2) From the first result above, I found the way I approximated the position does not produce a good model. So throw it out.
Starting with a form of Equation (6) again:
d²r/dt² = a - G*M/r² ...6'
Making the following substitutions:
dv/dt = d²r/dt² ...7
v= dr/dt ...8 → dt = dr/v ...8'
Sub ...7 & ...8' → ...6'
d²r/dt² = a - G*M/r² → dv/dt = a - G*M/r² → v*dv = a*dr - G*M/r²*dr ...9
Then integrate (9) with the initial conditions v= v_o, and r_o = R
⌠v*dv = a⌠dr - G*M⌠1/r²*dr
½*v²- ½*v_o² = a(r - R) - G*M(1/r - 1/R) →
v = √{2*[a(r - R) - G*M(1/r - 1/R) + ½*v_o²]} ...10
v: velocity
a: acceleration (in your example 11.76 m/s², but it can be anything now as long as the units are consistent)
v_o: initial velocity ( if you assume it starts from rest at the surface that whole last term "½*v_o²" under the square root drops out)
R: radius of the Earth
M: mass of the Earth
G: gravitational constant
You can use equation (10) to predict the velocity as a function of distance of the body from the center of the earth.
Have fun!
(1) An analytic way to solve this equation for velocity as a function of the radius (An analytic solution for position as a function of time is a whole other ball game).
(2) From the first result above, I found the way I approximated the position does not produce a good model. So throw it out.
Starting with a form of Equation (6) again:
d²r/dt² = a - G*M/r² ...6'
Making the following substitutions:
dv/dt = d²r/dt² ...7
v= dr/dt ...8 → dt = dr/v ...8'
Sub ...7 & ...8' → ...6'
d²r/dt² = a - G*M/r² → dv/dt = a - G*M/r² → v*dv = a*dr - G*M/r²*dr ...9
Then integrate (9) with the initial conditions v= v_o, and r_o = R
⌠v*dv = a⌠dr - G*M⌠1/r²*dr
½*v²- ½*v_o² = a(r - R) - G*M(1/r - 1/R) →
v = √{2*[a(r - R) - G*M(1/r - 1/R) + ½*v_o²]} ...10
v: velocity
a: acceleration (in your example 11.76 m/s², but it can be anything now as long as the units are consistent)
v_o: initial velocity ( if you assume it starts from rest at the surface that whole last term "½*v_o²" under the square root drops out)
R: radius of the Earth
M: mass of the Earth
G: gravitational constant
You can use equation (10) to predict the velocity as a function of distance of the body from the center of the earth.
Have fun!