Objects falling towarda each other.

[E92M3]

Homework Statement

m1 and m2 only interact gravitationally. They are initially at rest and a distance L apart. They where then released. Where and when will they collide?

Homework Equations

F_g=G\frac{m_1m_2}{x^2}

The Attempt at a Solution

For the where part, my argument is that initially at the CM frame, the total momentum is zero, therefore, they must collide at the origin of the CM frame. I think this is not a good argument.

For the time part, I have no clue. I mechanics is really weak. Despite being a physics major I am not required to take any classical mechanics course to graduate.

 

[tiny-tim]

Hi E92M3!

For the where part, my argument is that initially at the CM frame, the total momentum is zero, therefore, they must collide at the origin of the CM frame. I think this is not a good argument.

It is an excellent agrument!

Have a mince pie! ​

For the time part, I have no clue. I mechanics is really weak. Despite being a physics major I am not required to take any classical mechanics course to graduate.

Stay with the CM frame.

Hints:

i] if the distance of mass 1 from the CM is x, the distance of mass 2 is … ?

ii] special trick: a = dv/dt = dv/dx dx/dt (chain rule) = v dv/dx.

 

[E92M3]

Stay with the CM frame.

Just to make sure, is this because the frame of the masses are accelerating and therefore not inertial frames so Newtons' laws don't apply?

i] if the distance of mass 1 from the CM is x, the distance of mass 2 is … ?

The distance of mass 2 from the origin of the CM frame is initially L-x. But since they both move towards the origin I don't know what it will be at a later time.

ii] special trick: a = dv/dt = dv/dx dx/dt (chain rule) = v dv/dx.

Well I can look at mass 2 (it is define to be the mass on the negative x-axis initially):
F_2=G\frac{m_1m_2}{(x_1-x_2)^2}
Here, x1 is the distance from the CM to m1 and x2 is the distance from the CM to m2. They are both functions of t.

Following the hint I can say:
a_2=G\frac{m_1}{(x_1-x_2)^2}=v_2\frac{dv_2}{dx_2}
Gm_1\int\frac{dx_2}{(x_1-x_2)^2}=\int v_2 dv_2
\frac{-Gm_1}{x_1-x_2}=\frac{v_2^2}{2}+C

At t=0, v2=0 and x2=x1-L:

\frac{-Gm_1}{L}=C
\frac{-Gm_1}{x_1-x_2}=\frac{v_2^2}{2}+\frac{-Gm_1}{L}

I'm kindda still stuck. This is a differential equation, but it is not one that I can solve readily.

 

[tiny-tim]

Hi E92M3!

Just to make sure, is this because the frame of the masses are accelerating and therefore not inertial frames so Newtons' laws don't apply?

No, it's because there are no external forces, so (Newton's first law) the CM has uniform velocity … which, in the CM frame, means it stays where it is.

Good ol' Newton's laws always apply (in an inertial frame).
​

(just to make it clear, "the CM frame" means the inertial frame in which, at one particular time, the CM is stationary: Newton's first law then tells you that it will always be stationary in that frame)

The distance of mass 2 from the origin of the CM frame is initially L-x. But since they both move towards the origin I don't know what it will be at a later time.

You're missing the point … the CM is stationary, so the ratio of the distances will always be m₁/m₂ …

so use that to write x₂ as a function of x₁ in the force equation.

 

[E92M3]

Hi E92M3!

You're missing the point … the CM is stationary, so the ratio of the distances will always be m₁/m₂ …

so use that to write x₂ as a function of x₁ in the force equation.

Ok, I think I'm in deep trouble. I am taking an astronomy course and final is in 3 days. While doing the past papers, I found out that I can do any of the classical mechanical questions.

Here's what I think,

m_1x_1=m_2x_2
therefore:
x_1=\frac{m_2}{m_1}x_2

Putting this into the force I get:
F_2=G\frac{m_1m_2}{x_2^2(\frac{m_2}{m_1}-1)^2}

Following the same procedure as I did before I get:
\frac{-Gm_1}{x_2(\frac{m_2}{m_1}-1)^2}=\frac{v_2^2}{2}-\frac{Gm_1}{(\frac{m_2}{m_1}-1)L}

Once again I ended up with a differential equation I can't solve.

 

[tiny-tim]

That's ok, except you need a + in the denominator, not a -, don't you?

Now write v = dx/dt = f(x), so dx/f(x) = dt, and integrate.

 

[E92M3]

Sorry, I am really not getting this. I guess of I want to keep the minus sign I need to write:
m_1x_1+m_2x_2=0
Since I defined x1 and x2 to be the vector pointing from the origin of the CM frame to the 2 masses. But I really don't know what to do next. I can modify this to be:
<br /> \frac{-Gm_1}{x_2(-\frac{m_2}{m_1}-1)^2}=\frac{v_2^2}{2}-\frac{Gm_1}{(-\frac{m_2}{m_1}-1)L}<br />

Am I correct here? Is my integral valid?
<br /> Gm_1\int\frac{dx_2}{(x_1-x_2)^2}=\int v_2 dv_2<br />

 

[tiny-tim]

Hi E92M3!

If we make x₁ and x₂ both positive, then r = x₁ + x₂ = (m₁ + m₂)x₂/m₁.

Am I correct here? Is my integral valid?
<br /> Gm_1\int\frac{dx_2}{(x_1-x_2)^2}=\int v_2 dv_2<br />

Where did dv come from?

The trick is to write v = dx/dt, the dx is then joined by the function of x on the other side (it'll be inside a √, because you started with v), while the dt goes to the other side, on its own.

 

[E92M3]

Wait what is r here? It seems like r is the separation between the two masses am I correct? Then how did you get this:r = x1 + x2 = (m1 + m2)x2/m1?

I got the dv from the chain rule:
a=\frac{dv}{dt}=\frac{dv}{dx}\frac{dx}{dt}=v\frac{dv}{dx}
<br /> a_2=G\frac{m_1}{(x_1-x_2)^2}=v_2\frac{dv_2}{dx_2}<br />

Then I integrated both sides:

<br /> <br /> Gm_1\int\frac{dx_2}{(x_1-x_2)^2}=\int v_2 dv_2<br /> <br />

And applied the initial condition that initially v=0 and they are separated by L to get the integration constant.

 

[tiny-tim]

ah, now I see it in full, it's ok

Wait what is r here? It seems like r is the separation between the two masses am I correct? Then how did you get this:r = x1 + x2 = (m1 + m2)x2/m1?

if x₁ and x₂ are both positive, then r = x₁ + x₂ = m₂x₂/m₁ + x₂

 

[E92M3]

Ok I set them both to positive then I get this after the integration:
<br /> <br /> \frac{-Gm_1}{x_2(\frac{m_2}{m_1}+1)^2}=\frac{v_2^2}{2}-\frac{Gm_1}{(\frac{m_2}{m_1}+1)^2L}<br /> <br />
This is not something I can solve though.

 

[tiny-tim]

As I said before …

The trick is to write v = dx/dt, the dx is then joined by the function of x on the other side (it'll be inside a √, because you started with v), while the dt goes to the other side, on its own.

 

[E92M3]

So... this?
<br /> <br /> <br /> \frac{-Gm_1}{x_2(\frac{m_2}{m_1}+1)^2}=\frac{v_2^2}{2}-\frac{Gm_1}{(\frac{m_2}{m_1}+1)^2L}<br /> <br /> <br />
<br /> <br /> <br /> \frac{Gm_1}{(\frac{m_2}{m_1}+1)^2L}-\frac{Gm_1}{x_2(\frac{m_2}{m_1}+1)^2}=\frac{v_2^2}{2}<br /> <br /> <br />
<br /> <br /> <br /> \sqrt{2}\sqrt{\frac{Gm_1}{(\frac{m_2}{m_1}+1)^2L}-\frac{Gm_1}{x_2(\frac{m_2}{m_1}+1)^2}}=v<br /> <br /> <br />
\sqrt{\frac{2Gm_1}{(\frac{m_2}{m_1}+1)^2}}\sqrt{\frac{1}{L}-\frac{1}{x_2}}=\frac{dx_2}{dt}
\sqrt{\frac{2Gm_1}{(\frac{m_2}{m_1}+1)^2}}\int dt=\int \frac{1}{\sqrt{\frac{1}{L}-\frac{1}{x_2}}} dx_2
t\sqrt{\frac{2Gm_1}{(\frac{m_2}{m_1}+1)^2}}=\int \sqrt{\frac{Lx_2}{x_2-L}} dx_2
This is not a form of integral that I recognize. I tried a few tricks but they don't really work.

 

[tiny-tim]

Hi E92M3!

(just got up :zzz: …)

This is not a form of integral that I recognize. I tried a few tricks but they don't really work.

Try a trig or hyperbolic trig substitution (if you like, substitute x = y² or y² + C first)

(btw, I think we missed a minus in the original equation … r'' = -F )

 

[E92M3]

Thanks!
I think I got:
t=\frac{\pi L^{3/2}}{2(\frac{m_2}{m_1}+1)^{3/2}\sqrt{2Gm_1}}
I think that this is the solution. I'm dead if the test consists of this king of question.

 

[tiny-tim]

… I think that this is the solution.

I'm not convinced …

I haven't worked it through, but I think it's going to involve an inverse trig …

if you want me to check it, you'd better write it out in full.

 

[E92M3]

well, the units worked out though. anyways:

F_2=\frac{Gm_1m_2}{(x_1+x_2)^2}
a_2=\frac{Gm_1}{(x_1+x_2)^2}=\frac{Gm_1}{x_2^2(\frac{m_2}{m_1}+1)^2}
note:
m_1x_1=m_2x_2
a=v\frac{dv}{dx}
\frac{Gm_1}{(\frac{m_2}{m_1}+1)^2}/int \frac{1}{x_2^2}dx_2=\int v_2 dv_2
I used the condition that their initial velocity is zero and the initial separation is L to solve for the integration constant.
\frac{Gm_1}{(\frac{m_2}{m_1}+1)^2} /left ( \frac{1}{L}-\frac{1}{x_2(\frac{m_2}{m_1}+1)} \right )=\frac{v_2^2}{2}
Now I set v=dx/dt then integrate:
\sqrt{\frac{2GM_1}{\frac{m_2}{m_1}+1}} \int dt= \int \sqrt{\frac{x_2L(\frac{m_2}{m_1}+1)}{x_2(\frac{m_2}{m_1}+1)-L}}dx_2
Now I let u=x2(m2/m1+1):
t=\frac{1}{(\frac{m_2}{m_1}+1)^{3/2}sqrt{2GM_1}} \int\sqrt{\frac{uL}{L-u}}
To find the limits of integration, u=x1+x2, then u is from L to 0. This allows me to flip the sign in the bottom.
t=\frac{1}{(\frac{m_2}{m_1}+1)^{3/2}\sqrt{2GM_1}} \int_0^L \sqrt{{\frac{uL}{u-L}}}=t=\frac{1}{(\frac{m_2}{m_1}+1)^{3/2}\sqrt{2GM_1}}\frac{\pi L^{3/2}}{2}

 

[tiny-tim]

… To find the limits of integration, u=x1+x2, then u is from L to 0. This allows me to flip the sign in the bottom.
t=\frac{1}{(\frac{m_2}{m_1}+1)^{3/2}\sqrt{2GM_1}} \int_0^L \sqrt{{\frac{uL}{u-L}}}=t=\frac{1}{(\frac{m_2}{m_1}+1)^{3/2}\sqrt{2GM_1}}\frac{\pi L^{3/2}}{2}

No, you can't just flip the sign and make negative square roots.

And I don't understand the last bit, are you saying ∫√(u/(L - u)) du is proportional to u^3/2 ?

Try u = y².