In Newtonian physics, it is a well known equation that F=Gm1m2/d2. Substituting, we receive ma=Gm1m2/d2, so a=dv/dt=Gm/d2. My question is, how do we integrate this to find what the velocity is at a given moment or at a given distance?
By chain rule, we have
a=dv/dt=(dx/dt)(dv/dx)=vdv/dx
Thus
vdv/dx=-Gm/x2
Separating variables and integrate to give v in terms of x. The
result is
v2-v02=2Gm(1/x-1/x0)
and thus we can use the fact that v=dx/dt to separate variables and
integrate again to give t in terms of x. Unfortunately, this
usually does not give a nice formula.
Hope this helps.
Kerwin
Kerwin is right...
This is a constantly asked CSYS / A-Level Mechanics question. You
change the variable from time to displacement as indicated.
Neil M
Sorry, but what does the v or x with a zero under it mean. I am
fairly unacquainted with physics notatation. Also, when you label
the distance traveled as x, the d in my equation represents the
distance from the earth (or whatever body we are dealing with). So,
how do you derive that the distance from the earth is equivalent to
the distance the object has traveled.
Unless of course, it is meant that v=-dx/dt, as the more a body
moves, the closer it is to earth. Anyway, you accounted for this in
your second line of math but I am not sure that you differentiated
with this in mind as I do not know what v0 indicates.
Thanks though,
Brad
Brad,
Sorry for the confusion caused.
v0 denotes the initial speed,
and similarly,
x0 denotes the initial separation of the centres of
mass.
The equation of motion is
a=dv/dt=-Gm/x2
where x denotes the separation of centres of mass.
Kerwin
I have attempted another integration of this. I would like to
know if this makes sense
We start with the equation
v.dv/dx=-Gm/x2
v.dv=(-Gm/x2)dx
Integrating both terms
Gm/x=v2/2
Therefore
v=sqrt(2Gm/x)
This is of course assuming that the object was dropped from
"infinite height". I am fairly sure that this is right, but when I
try to integrate with v=-dx/dt, I end up with nonsense.
Hi Brad,
It is worth knowing that the integrated form of your equation,
i.e.
½v2 = Gm/x + C
is actually a statement of the law of conservation of energy. In
your equation presumably m is the mass of the object which is
attracting the object you're considering. Suppose we let the object
you are considering (which has position vector x) have mass M. Now
multiply both sides of the equation by M and re-arrange.
½Mv2 - GmM/x = CM = constant
The first term is the kinetic energy. The second term is what we
call the gravitational potential energy. The statement says that
the sum of gravitational and kinetic energies are constant.
The formula -GMm/x for GPE is useful generally. You might like to
try to show how to derive the approximation mgdh for small dh.
In fact you can use it to find the escape velocity very easily.
Remember the total energy of an object free-falling stays constant.
So what minimum total energy does a body need to get to an infinite
distance of its attractor? Supposing it starts at a distance r,
therefore what KE does it need? So what is the escape velocity? You
can use this to calculate the Schwarzchild radius of a black hole
of known mass.
Actually you can do this with forces too, but it seems slightly
more straightforward this way.
Yours,
Michael