I presume you mean you want a formula for an object falling through a distance large enough that you cannot just assume that the force due to gravity is constant:
[tex]ma= m\frac{dv}{dt}= -\frac{GMm}{r^2}[/tex]
We can, of course, immediately cancel the "m"s. Also, since v= dr/dt, we have, by the chain rule, that dv/dt= (dv/dr)(dr/dt)= v dv/dr. That is, we can change that equation in v, r, and t into an equation involving only v and r:
[tex]v\frac{dv}{dr}= - \frac{GM}{r^2}[/tex]
which is a "separable differential equation".
[tex]v dv= -GM \frac{dr}{r^2}[/itex] <br />
which can be integrated:<br />
[tex]\frac{1}{2}v^2= \frac{GM}{r}+ C[/itex]<br />
<br />
I doubt your calc prof would be all that disappointed. This is a technique, called "quadrature", for solving non-linear differential equations that is not normally taught in a calculus course. Notice, by the way, that that equation can be rewritten<br />
[tex]\frac{1}{2}mv^2- \frac{GmM}{r}= mC[/tex]<br />
and is basically "conservation of energy". <br />
<br />
If you take, as initial condition, that at t= 0, r(0)= R and v(0)= 0, an object falling from height R, we have <br />
[tex]\frac{1}{2}(0^2)= \frac{GM}{R}+ C[/tex]<br />
so C= -GM/R and <br />
[tex]\frac{1}{2}v^2= \frac{GM}{r}-\frac{GM}{R}[/tex]<br />
<br />
Now solve that for v:<br />
[tex]v^2= \frac{2GM}{r}- \frac{2GM}{R}[/tex]<br />
so <br />
[tex]v= \frac{dr}{dt}= -\sqrt{\frac{2GM}{r}- \frac{2GM}{R}}[/tex]<br />
(I took the negative root because I am taking "+" velocity upward.)<br />
<br />
Integrate<br />
[tex]\int\frac{dr}{\sqrt{\frac{1}{r}- \frac{1}{R}}}= \sqrt{GM}t[/tex]<br />
to find r as a function of t.<br />
<br />
Your calc prof would also not be too disappointed if you could not do that integral. It is not integrable in terms of elementary functions. It is a type of "elliptic" integral, so called because it arises in finding the length of an arc of an ellipse. Since the general motion in an "inverse square" gravity field is along an ellipse, that should not be too surprising.[/tex][/tex]