Creator said:
Rusty on the math...
I am working on a problem and need the derivation of a free fall trajectory for an object at a distance above Earth where the change in acceleration is not negligible. How do I integrate the distance/ acceleration formula taking into account the change in g to get the total distance traveled.
The method and final formula...?
I'm looking for total distance after time t, trying to see how it scales as what power of t.
thanks.
Sidhartha23 and QuantumPion have argued back and forth but we haven't heard back from Creator so I am going to look at the specific case Creator asked about: An object falling from such a great height the we must use the general law for gravity: F= -GmM/r^2, rather than treating F as a constant, still satisfies "Force= mass times acceleration". Here "m" is the mass of the object, M is the mass of the Earth so we have ma= -GmM/r^2 or
a= \frac{dv}{dt}= -\frac{GM}{r^2}
We would like to integrate that but we need to integrate with respect to t and have "r" on the right. To fix that, we can use a method called "quadrature". By the chain rule, dv/dt= (dv/dr)(dr/dt)= v(dv/dr) becaues v, the speed, is dr/dt. Now we have
v\frac{dv}{dr}= -\frac{GM}{r^2}
which we can write, in "differential form" as
vdv= -\frac{GM}{r^2}dr= -GMr^{-2}dr
Integrating both sides,
\frac{1}{2}v^2= GMr^{-1}+ C
assuming that the object falls from a standstill at height R, v= 0, so 0= GMR^{-1}+ C, C= -GMR^{-1}.
From that,
v= \frac{dr}{dt}= \sqrt{2GMr^{-1}- 2GMR^{-1}}= \sqrt{2GM}\sqrt{r^{-1}- R^{-1}}
We can write that as
\frac{dr}{\sqrt{2GM}\sqrt{r^{-1}+ R^{-1}}}= dt
Integrating both sides of that will give t as a function of r which can then solved for r as a function of t. However, the left side cannot be integrated in terms of "elementary functions". It is an "elliptic integral" (the name, unsurprisingly, connected with the fact that planets move in ellipses around the sun). There used to be multi-volumes of tables of elliptic integrals.