Calculating Gravitational Attraction Between Two Masses in Empty Space

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The discussion centers on calculating the time it takes for two 1 kg masses, initially 1 meter apart, to attract each other gravitationally in empty space. Participants explore using gravitational force equations and conservation of energy to derive the time, with initial calculations suggesting a range of 20 to 417,904 seconds. There is debate over the accuracy of these methods, particularly regarding the use of constant acceleration versus integrating the changing gravitational force as the masses approach each other. Some participants propose using known results from orbital mechanics, leading to a derived time of approximately 26.7 hours based on Kepler's laws. The complexity of the problem highlights the nuances of gravitational attraction and the mathematical challenges involved in solving it.
  • #31
schroder said:
I will make one final attempt to explain about gravitational potential enrgy, even though I expect you will not agree. This may be a bit long, but I hope it is worth your while to read through it with an open mind. First, I believe it is useful to point out where our disagreement is; in other words, let us agree on what points we disagree on.

You are saying that gravitational potential is negative, and is expressed dimensionally as:
-GMm/R
Obviously, as R goes to zero, GPE will go to infinity. (I agree with this)

We also agree that Total energy is conserved. That is, the total energy remains unchanged in any process. We all agree this is true.
As r goes to 0, the GPE approaches negative infinity.

In a conservative system, that is, one in which only conservative forces are acting, the total energy is the sum of the PE and KE. When KE is zero, all of the energy is PE and vice versa. This can be seen in a simple pendulum. The gravitational system we are discussing here is a conservative system and we are starting out with zero KE and some fixed amount of PE. For the purpose of this discussion, let us say we are starting out with 100 Joules of PE, which must be equal to the total energy as KE is zero to start with. The number does not matter, as long as we agree it must remain constant throughout at 100 Joules, never more and never less. I think we are in agreement up to this point, but please correct me if I am mistaken.
You would be wise to use a negative number for the initial PE (using r = ∞ as your zero point for PE), and thus the total energy. Then you would be less tempted to associate KE with that total energy.

Now the distance decreases from the starting distance of 1 meter. The PE must increase in Magnitude, according to the math, and is always Negative so it is decreasing. At the same time, the KE must increase, in order for the total energy to remain constant at 100 J.


Now we get into the area where we disagree: According to you, the PE increases to a Negative infinite value, so the KE must increase to a positive infinite value and thay add according to sign convention and the total remains constant.

I disagree right away, because what you are saying means that the KE is going to infinity, which means, according to KE = 1/2 MV^2 that velocity must also be going to infinity. What this clearly says is that the two spheres will come together at infinite velocity and infinite KE!
But it's true! If two point masses under the influence of Newtonian gravity alone approach each other, they will end up going infinitely fast as they approach each other. Realize that this is just an exercise--not realizable in practice.
In other words, under the weak force of gravity, we would have for all intents and purposes a nuclear explosion caused by two spheres coming together in such a way. In fact, if I jump in the air, and return to earth, I should land with infinite energy at an infinite velocity using the exact same mathematics. Obviously, by common sense alone, this is wrong!
Obviously, there are other factors that distinguish this case from the ideal case of two colliding point masses: You are not a point mass and other forces are involved. Two spheres coming together is quite different than two point masses colliding.

But I will not base my disagreement on common sense alone. Here is my explanation, and I hope you will take the time to read and try to understand what I am saying. Yes, PE is always negative, and it does increase towards negative infinity as radius goes toward zero. The plot is a hyperbola. But this hyperbola is so not very useful at small values of radius since all PE are very close to negative infinity. It would not be useful at all for calculating the PE of gravity at the surface of the earth, for example. So physicists have linearized the gravitational potential and potential energy to make it more useful for everyday experience, which includes our consideration of two bodies separated by only one meter. The method of linearization is this:
PE2 – PE1 = - GM/(R + h) – ( - GM/R ) this is the Difference between two potentials where h is the difference in R.

Now we need to do a bit of algebraic simplification: = GM ( 1/R – 1/(R + h)
By LCD we get: = GMh/R(R + h) the final step is to drop the h as it is insignificant to the R.
And we have finally, GMh/R^2 which is gravitational acceleration multiplied by h and is
Gravitational potential and reduces to gh. For GPE just multiply by m and we have our familiar
Mgh. Which is the familiar linearized form of GPE. This is much more useful than using the more general form –GMm/R^2. And, because it is a difference in potential energy,, it is usually treated as a positive number. Although sign convention can be followed if the problem calls for it.

What this all boils down to for the case at hand of two 1 kg spheres at a distance of 1 meter:

g’ = Gmm/R^2 = G = 6.67 E-11 m/s^2
GPE (initial) = mg’h = G = 6.67 E-11 Joules
Total energy = PE (initial) = 6.67 E-11 Joules and is Constant
KE = (Total energy – PE ) at all times
At a distance of zero meters, when the spheres are touching, PE = mg’h and is also zero.
Thus KE is equal to 6.67 E -11 Joules and is shared equally by the two spheres.
Each sphere has 3.335 E-11 Joules of KE which = 1/2 MV^2
So Max possible velocity = 8.167 E-6 m/s which is considerably less than infinity!
Sorry, but this "linearization" is nonsense as applied to the problem at hand. Of course, near the surface of the Earth we "linearize" gravity and use mgh for local changes in GPE.

The two spheres will pull together very slowly, by your own calculation, in a time of 28 hours.
At no time will velocity be infinite of KE be infinite. The KE cannot exceed the total energy that the system started with!
The system started out with negative energy. Are you saying that the KE energy must be negative? :rolleyes:
I sense that as a mathematical purist you may have trouble accepting this, but I assure you that such linearizations are done in physics all the time. I recommend Physics by K.R. Atkins for more such examples.
Please scan in the pages where Atkins does this particular example.
 
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  • #32
Doc Al said:
As r goes to 0, the GPE approaches negative infinity.


You would be wise to use a negative number for the initial PE (using r = ∞ as your zero point for PE), and thus the total energy. Then you would be less tempted to associate KE with that total energy.
But it's true! If two point masses under the influence of Newtonian gravity alone approach each other, they will end up going infinitely fast as they approach each other. Realize that this is just an exercise--not realizable in practice.

Obviously, there are other factors that distinguish this case from the ideal case of two colliding point masses: You are not a point mass and other forces are involved. Two spheres coming together is quite different than two point masses colliding.


Sorry, but this "linearization" is nonsense as applied to the problem at hand. Of course, near the surface of the Earth we "linearize" gravity and use mgh for local changes in GPE.


The system started out with negative energy. Are you saying that the KE energy must be negative? :rolleyes:

Please scan in the pages where Atkins does this particular example.

I think it would be even wiser to stick with the problem as stated : two 1 kg masses starting out (stationary) at a distance of 1 meter. The PE and indeed the total energy they possesses is based on that distance and not on infinity. When you calculate the PE of a rock held at 1 meter above the ground, you do not reference it to infinity? The linearization I am using here is valid for a distance of 1 meter. It takes about 27 hours for them to cover 1 meter. Do you really think their velocity is approaching infinity? When that tool bag floated away from the astronaut in space, would it have come back to her at infinite velocity and infinite energy? I am not the one talking nonsense here!
 
  • #33
schroder said:
<incorrect mathematical and physical reasoning snipped> I am not the one talking nonsense here!

Actually you are.

Maybe putting some numbers into the equations will help you: For simplicity let's use a system of units where G=m_1=m_2=1 and so the potential energy is just U=\frac{-1}{r}...at r=1 let's say that the two masses are at rest so that the kinetic energy K=v^2 of each particle is zero. Then the total energy is initially E=K+U=0+1=1 and since energy is conserved you require that at all times t, you have U(t)+K(t)=1\implies K(t)=1-U(t)

Now at some time after the objects are released, they will be much closer together...let's say at t=1, we have r=\frac{1}{1000000000}=10^{-9} (that is VERY close together). Clearly U(t=1)=-10^9 and so K(t)=1-(-10^9)=10^9+1\approx 10^9. You see as the objects get closer, their kinetic energy gets larger and larger (of course in the real world there are other forces at work which will repel the objects once they get close enough to each other).
 
  • #34
You are saying that they are accelerating from rest to approaching infinite velocity and infinite kinetic energy, over a distance of one meter. And yet, we have shown it takes 27 hours to cover that distance. I would call what you are saying "nonsense"!
 
  • #35
schroder said:
You are saying that they are accelerating from rest to approaching infinite velocity and infinite kinetic energy, over a distance of one meter. And yet, we have shown it takes 27 hours to cover that distance.
Yes.
I would call what you are saying "nonsense"!

Then you would be wrong again.

Think of it this way...at r=1/2, U=-2 and so E=1 and hence v=1...that means that over the first half of their journey (distance wise), the particles have been slowly accelerating up to a speed of 1. In that first half, most of the time necessary for the entire journey has passed...it isn't until they get very very close together that they start to accelerate to enormous speeds and by that time most of the 27 hours has already passed.

It's sort of like driving most of the way from LA to New York at 1km/h and then switching on a jet pack when you reach Washington...you'll get from Washington to New York very quickly, but your entire journey will take considerably longer.
 
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  • #36
schroder said:
I think it would be even wiser to stick with the problem as stated : two 1 kg masses starting out (stationary) at a distance of 1 meter.
I did. Of course you must realize for the exercise that these are point masses, not macroscopic objects.
The PE and indeed the total energy they possesses is based on that distance and not on infinity.
All measures of PE depend upon a reference point. When talking about the gravitational PE between two point masses (or astronomical bodies), the natural reference point is to take PE = 0 when they are infinitely far apart. You earlier agreed that the gravitational PE between two bodies is given by -GMm/R; that relationship assumes a reference point at infinity.
When you calculate the PE of a rock held at 1 meter above the ground, you do not reference it to infinity?
Not generally, because you are talking about Earth gravity and you are only concerned about small changes in position compared to the distance to the Earth's center. But if you were to move that rock to a height equal to the Earth's radius, you'd certainly use the more general expression. Or perhaps you want to calculate the escape velocity of that rock, again you'd use the more general expression.

In raising the rock a mere 1 m above the Earth's surface, you are only changing the distance to the Earth's center by 1 part in about 6,400,000. That's a realm where you can treat the force of gravity as being constant. Not so when the bodies are going from 1m to "contact". Just to get to within a mm of each other changes the distance between them by a factor of 1000!
The linearization I am using here is valid for a distance of 1 meter.
Nope. As explained above, over this range the force is wildly nonlinear.
It takes about 27 hours for them to cover 1 meter. Do you really think their velocity is approaching infinity? When that tool bag floated away from the astronaut in space, would it have come back to her at infinite velocity and infinite energy? I am not the one talking nonsense here!
Again, you are confusing your common sense experience with ordinary objects with this exercise in Newtonian gravity involving point masses.
 
  • #37
schroder said:
In other words, under the weak force of gravity, we would have for all intents and purposes a nuclear explosion caused by two spheres coming together in such a way. In fact, if I jump in the air, and return to earth, I should land with infinite energy at an infinite velocity using the exact same mathematics. Obviously, by common sense alone, this is wrong!
Without involving general relativity, you know from special relativity that as kinetic energy goes to infinity, the speed approaches c (the speed of light), not infinity. Even so, we are also assuming that these are point masses, which, from our experience, also do not exist in reality. They would really collide at some point before r = 0.

Anyway, let's do some specific calculations. For simplicity I'll pick my units such that Gm2 = 1, so U = -1/2r.

Initially, the masses are not moving, so the kinetic energy is K = 0. Since the distance between the masses is 2r = 1, the potential energy is U = -1. Thus the total energy is E = -1.

Now remember, total energy is conserved, so E = -1 always. Now let's say the distance between the masses is now 0.1. The potential energy is U = -1/0.1 = -10, so kinetic energy is K = E - U = (-1) - (-10) = 9. If the distance is 0.001, U = -1000, so K = E - U = 999. It should be clear that K increases without bound, as long as r is allowed to go to zero.

The value of E does not in any way limit the value of K. In this particular example this is most apparent, since E is negative, but K must always be nonnegative.

Remember that potential energy is always measured relative to some reference point, so we can make, in our calculations, total energy to be any value we like. Kinetic energy, however, is absolute.

If you're still having trouble understanding what's going on, I suggest that it would be more productive to talk to a physicist in person.

Denton said:
Adrian, if you have the time could you explain a little better how you integrated the (1/r - 1/r0). Namely how you obtained <br /> r = r_0 \cos^2 \theta

It's one of the usual trigonometric substitutions, although in a slightly unusual form. I wanted to have 1/r = (1/r_0) \sec^2 \theta. Once you have that, the rest is straightforward:
<br /> \begin{align*}<br /> \int_0^{r_0} \left( \frac{1}{r} - \frac{1}{r_0} \right)^{-1/2} dr<br /> &amp;= \int_{\pi/2}^0 \left( \frac{1}{r_0 \cos^2 \theta} - \frac{1}{r_0} \right)^{-1/2}<br /> \frac{dr}{d\theta} \,d\theta \\<br /> &amp;= r_0^{1/2} \int_{\pi/2}^0 (\sec^2 \theta - 1)^{-1/2}<br /> (-2r_0 \sin \theta \cos \theta) \,d\theta \\<br /> &amp;= r_0^{3/2} \int_0^{\pi/2} 2 (\tan^2 \theta)^{-1/2} \sin<br /> \theta \cos \theta \,d\theta \\<br /> &amp;= r_0^{3/2} \int_0^{\pi/2} 2 \cos^2 \theta \,d\theta \\<br /> &amp;= \frac{\pi}{2} r_0^{3/2}.<br /> \end{align*}<br />
 
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  • #38
gabbagabbahey said:
Yes.


Then you would be wrong again.

Think of it this way...at r=1/2, U=-2 and so E=1 and hence v=1...that means that over the first half of their journey (distance wise), the particles have been slowly accelerating up to a speed of 1. In that first half, most of the time necessary for the entire journey has passed...it isn't until they get very very close together that they start to accelerate to enormous speeds and by that time most of the 27 hours has already passed.

It's sort of like driving most of the way from LA to New York at 1km/h and then switching on a jet pack when you reach Washington...you'll get from Washington to New York very quickly, but your entire journey will take considerably longer.



What you, as well as others here, are doing, is taking that hyperbolic acceleration curve, which approaches asymptotes at a radious of infinity and PE of zero, and other asymptote of radius zero and PE infinity, and you are applying that entire curve to a distance of one meter! It has long ago been established that you cannot do that. On the earth’s surface, for near Earth objects we linearize that curve to get mgh. And for two objects ( I don’t give a damn whether they are “point sources” or spheres as it makes no difference in the analysis ) at a distance of one meter you also must linearize that curve. It is ridiculous in the extreme to have two objects starting from rest at a distance of one meter accelerating to infinite velocity under the extremely weak force of gravity! If gravity were that powerful, nothing would ever float away in space, like that astronaut’s tool kit, but it would be stuck to her like the most powerful magnet imaginable. For once, think about what you are saying instead of blindly applying the math! LINEARIZE over short distances. Get a good physics book and READ IT!
 
  • #39
Don't you find it odd that everyone else is disagreeing with you?

schroder said:
It is ridiculous in the extreme to have two objects starting from rest at a distance of one meter accelerating to infinite velocity under the extremely weak force of gravity!
This doesn't ever happen in reality because point masses aren't real.

Why are you talking about linearization? Why use an approximation? The exact solution has already been given.

Alright, so let's say kinetic energy doesn't increase without bound. What value will it approach as r goes to zero? (It won't be the total energy, since we've already established that total energy is negative; using our gauge choice for the potential energy, U = -Gm2/2r, so that E = -Gm2/2r0.) Where is your math?
 
  • #40
adriank said:
Don't you find it odd that everyone else is disagreeing with you?


This doesn't ever happen in reality because point masses aren't real.

Why are you talking about linearization? Why use an approximation? The exact solution has already been given.

Alright, so let's say kinetic energy doesn't increase without bound. What value will it approach as r goes to zero? (It won't be the total energy, since we've already established that total energy is negative; using our gauge choice for the potential energy, U = -Gm2/2r, so that E = -Gm2/2r0.) Where is your math?

I don't find that at all odd, on THIS forum, where at least one of the so-called "mentors" firmly believes in DDWFTTFW! So why should I be surprised at this?

I have already, several times, calculated the MAX velocity that is reached. You can find that a couple of posts on up. IF that max velocity was constant (it isn't) but IF it were, it would take 17 hours to pull them together. IF the acceleration was constant (it isn't) it would take 34 hours. By integration, we all agree total time is around 27 hours. Each sphere or "point mass" take you pick covers a half meter in 27 hours starting from rest. And somehow you are saying and actually believing, that they approach infinite velocity! That is one HELL of an acceleration curve over one meter and all under the force of gravity! THat makes sense to you? The problem comes from applying that acceleration curver over the distance of one meter. THAT is why it must be linearized.
They may as well draw that staright line through my name right now, as this physics forum never admits they are wrong they just delete posts and ban people. I have had enough of this. Incidently, I am a degreed engineer in both civils engineering and EE and have been a team leader on advanced R+D for satellite communications as well as deep space probes. I know what I am talking about.
 
  • #41
Gravity is inversely proportional to r^2. With pointlike masses, as r approaches zero, G approaches infinity. From the classical mechanics viewpoint, anyway.
That's why I hate equations, they never make any sense. Just take it easy, schroder ;)
 
  • #42
schroder: Clearly you don't know what your talking about, and throwing credentials around will get you nowhere if you can't make sense.

I'll now respond to your post where you gave the maximum speed, which I really didn't read fully before.
So physicists have linearized the gravitational potential and potential energy to make it more useful for everyday experience, which includes our consideration of two bodies separated by only one meter.
Do you understand that linearization is an approximation? It's just nonsense to use an approximation to claim that an exact solution is wrong! You won't get the correct time to collision that way, either.
By LCD we get: = GMh/R(R + h) the final step is to drop the h as it is insignificant to the R.
Assuming I'm interpreting what you mean by h, that is far from insignificant compared to R! That isn't valid. The amount the masses move is comparable (actually equal!) to the distance between them.
At a distance of zero meters, when the spheres are touching, PE = mg’h and is also zero.
That only works for variations in height that are very small compared to the distance between the masses, so that g' is effectively constant. That's only a first-order approximation of the actual potential energy, U = U0 - GMm/r2. You really should know this. Your problem there is that the gravitational acceleration is not constant. You even admitted earlier that potential energy does indeed go to negative infinity.

Prove to me that, given your solution, energy is conserved. If you can't do that, then there's a problem with your argument, isn't there?
The problem comes from applying that acceleration curve over the distance of one meter.
There is no problem.
If you continue to insist that you are correct, I will consider you to be trolling and ignore you.
 
  • #43
One more thing: I will find the velocity in terms of r directly. Recall from my initial post that

-\frac{dr}{\sqrt{\frac{Gm}{2} \left( \frac{1}{r} - \frac{1}{r_0} \right) }} = dt,

or equivalently,

-\sqrt{\frac{2}{Gm}} \left( \frac{1}{r&#039;} - \frac{1}{r_0} \right)^{-1/2} dr&#039; = dt&#039;,

where I changed r to r' and t to t' so I could use r and t inside the limits of integrals.

I integrate this to find the time required to reach any particular position. At t' = 0, r' = r0, and at t' = t, r' = r, so

-\sqrt{\frac{2}{Gm}} \int_{r_0}^{r} \left( \frac{1}{r&#039;} - \frac{1}{r_0} \right)^{-\frac12} \,dr&#039; = \int_0^t dt&#039; = t.

I make the substitution r&#039; = r_0 \cos^2 \theta, so \theta = \arccos \sqrt{r&#039;/r_0}:

\begin{align*}<br /> t &amp;= \sqrt{\frac{2}{Gm}} \int_{0}^{\arccos \sqrt{r/r_0}} \left( \frac{1}{r_0 \cos^2 \theta} - \frac{1}{r_0} \right)^{-\frac12} 2r_0 \sin \theta \cos \theta \,d\theta<br /> \\<br /> &amp;= \sqrt{\frac{2r_0^3}{Gm}} \int_{0}^{\arccos \sqrt{r/r_0}} 2 \cos^2 \theta \,d\theta<br /> \\<br /> &amp;= \sqrt{\frac{2r_0^3}{Gm}} \left[ \theta + \sin \theta \cos \theta \right]_{0}^{\arccos \sqrt{r/r_0}}<br /> \\<br /> &amp;= \sqrt{\frac{2r_0^3}{Gm}} \left( \arccos \sqrt{\frac{r}{r_0}} + \sqrt{1 - \frac{r}{r_0}}\sqrt{\frac{r}{r_0}} \right).<br /> \end{align*}

I can differentiate this to obtain the velocity:

\begin{align*}<br /> \frac{1}{v} &amp;= \frac{dt}{dr} = -\sqrt{\frac{2r}{Gm (1 - r/r_0)}}<br /> \\<br /> v &amp;= -\sqrt{\frac{Gm}{2r} \left( 1 - \frac{r}{r_0} \right)} = -\sqrt{\frac{Gm}{2r_0} \left( \frac{r_0 - r}{r} \right)}.<br /> \end{align*}

I plot that below.

http://img56.imageshack.us/img56/1972/graveo8.png

It's pretty apparent from both the equation and the graph that as r goes to 0, v goes to negative infinity.

Remember that I've been using purely classical mechanics here, so the kinetic energy of one of the masses is mv^2/2. Let's see if this expression for velocity conserves energy:

\begin{align*}<br /> E &amp;= U + K = -\frac{Gm^2}{2r} + 2 \left( \frac12 mv^2 \right)<br /> \\<br /> &amp;= -\frac{Gm^2}{2r} + m \frac{Gm}{2r_0} \left( \frac{r_0 - r}{r} \right)<br /> \\<br /> &amp;= -\frac{Gm^2}{2r} + \frac{Gm^2}{2r} - \frac{Gm^2}{2r_0}<br /> \\<br /> &amp;= -\frac{Gm^2}{2r_0}.<br /> \end{align*}

This is what was desired. Note that I have made no approximations or unjustified steps anywhere. This is exact.
 
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  • #44
schroder said:
What you, as well as others here, are doing, is taking that hyperbolic acceleration curve, which approaches asymptotes at a radious of infinity and PE of zero, and other asymptote of radius zero and PE infinity, and you are applying that entire curve to a distance of one meter! It has long ago been established that you cannot do that.
Kind of silly for you to keep insisting this, when not only can you do it, it's been done for you right in this thread.
On the earth’s surface, for near Earth objects we linearize that curve to get mgh.
Yes, because h << radius of the earth!
And for two objects ( I don’t give a damn whether they are “point sources” or spheres as it makes no difference in the analysis ) at a distance of one meter you also must linearize that curve.
Still comically wrong! And why even attempt a linear approximation when you can solve it exactly?
It is ridiculous in the extreme to have two objects starting from rest at a distance of one meter accelerating to infinite velocity under the extremely weak force of gravity!
Please give me an estimate of the gravitational force between two 1 kg point masses that are 10-12 m apart?
If gravity were that powerful, nothing would ever float away in space, like that astronaut’s tool kit, but it would be stuck to her like the most powerful magnet imaginable.
Still not relevant. Again, such examples have nothing to do with idealized point masses.
For once, think about what you are saying instead of blindly applying the math! LINEARIZE over short distances.
This is getting comical. You linearize as an approximation, and only when Δx << x. That is far from applicable to this elementary exercise.
Get a good physics book and READ IT!
:rolleyes:

Again let me remind you that this is just an exercise in applying Newtonian gravity to idealized point masses in Newtonian mechanics: There are no real point masses that are only subject to Newtonian gravity, and Newtonian mechanics breaks down at small distances and high speeds.
 
  • #45
schroder said:
What you, as well as others here, are doing, is taking that hyperbolic acceleration curve, which approaches asymptotes at a radious of infinity and PE of zero, and other asymptote of radius zero and PE infinity, and you are applying that entire curve to a distance of one meter!
Yes. And the reason we are doing that is because (in the context of Newtonian gravity) it is the correct approach.

It has long ago been established that you cannot do that.
Your definition of established clearly differs greatly from the definition that reasonable people use.

On the earth’s surface, for near Earth objects we linearize that curve to get mgh. And for two objects ( I don’t give a damn whether they are “point sources” or spheres as it makes no difference in the analysis ) at a distance of one meter you also must linearize that curve. It is ridiculous in the extreme to have two objects starting from rest at a distance of one meter accelerating to infinite velocity under the extremely weak force of gravity! If gravity were that powerful, nothing would ever float away in space, like that astronaut’s tool kit, but it would be stuck to her like the most powerful magnet imaginable. For once, think about what you are saying instead of blindly applying the math! LINEARIZE over short distances.

This is complete and utter nonsense. The reason you linearize gravity near the surface of the Earth is because your PE and hence acceleration due to gravity are vary slowly over reasonable height distances. This (as Doc Al has already pointed out to you) is because the radius of the Earth is MUCH larger than normal height distances and so R+h \approx R. In the case of these two particles which are subject only to each others gravity, there is no large Earth that they sit on. 'R' is zero and so a change of one meter in h changes the PE and the acceleration GREATLY.


Get a good physics book and READ IT!

Get a less defective brain and use it.
 
  • #46
Doc Al said:
Kind of silly for you to keep insisting this, when not only can you do it, it's been done for you right in this thread.

Yes, because h << radius of the earth!

Still comically wrong! And why even attempt a linear approximation when you can solve it exactly?

Please give me an estimate of the gravitational force between two 1 kg point masses that are 10-12 m apart?

Still not relevant. Again, such examples have nothing to do with idealized point masses.

This is getting comical. You linearize as an approximation, and only when Δx << x. That is far from applicable to this elementary exercise.

:rolleyes:

Again let me remind you that this is just an exercise in applying Newtonian gravity to idealized point masses in Newtonian mechanics: There are no real point masses that are only subject to Newtonian gravity, and Newtonian mechanics breaks down at small distances and high speeds.


Let me remind you, that until you entered this thread, in post number 31, there was NO mention of idealized “point masses” The only thing mentioned was two 1 kg masses and “time for two bodies to converge in space”. Read the thread and tell me where and when “point masses” entered the discussion. Until you made it an “exercise” in abstract mathematical concepts that have absolutely NO bearing on the physical world, this was a PHYSICS question. And in PHYSICS, there is such a thing as the conservation of mechanical energy in a conservative system. THAT is what this system is, or was, until you decided to change the subject entirely.
In the context of physics, in the real world, the TOTAL amount of energy in such a conservative SUSTEM, with two stationary masses, is determined by the gravitational PE BETWEEN the two masses over the distance between them. ALL the energy is PE at the start and during the transit over the distance the energy is converted to KE, until at the point of contact ALL of the energy is KE and PE is zero. Tell me how much PE there is between two masses that are in contact with each other, when the distance is zero. I will give you the answer without the need for any integration; the PE is zero, NOT infinity. The only thing that is comical about this is the way you are blindly applying abstract mathematical concepts to what is a practical real world physics problem and coming up with comical answers. There are NO “point particles” there is NO infinite energy and there is NO infinite velocity except in your abstract math which has no application to the real physical universe. I am done with this joke of a physics forum. This is a sad reflection on the state of physics education in the USA today.
 
  • #47
schroder said:
I am done with this joke of a physics forum. This is a sad reflection on the state of physics education in the USA today.
Your woefully inadequate ability to comprehend simple physical reasoning is the only sad reflection on the state of physics education.

This thread is done. If the OP would like to discuss this further they are more than welcome to PM me and I'll re-open the thread.
 
  • #48
schroder said:
Let me remind you, that until you entered this thread, in post number 31, there was NO mention of idealized “point masses”
Right. I was the one who made explicit the assumption that everyone--including you--was making. If you weren't making such an assumption, tell me how big those two objects were and how far apart they were when they touched?
The only thing mentioned was two 1 kg masses and “time for two bodies to converge in space”. Read the thread and tell me where and when “point masses” entered the discussion. Until you made it an “exercise” in abstract mathematical concepts that have absolutely NO bearing on the physical world, this was a PHYSICS question. And in PHYSICS, there is such a thing as the conservation of mechanical energy in a conservative system. THAT is what this system is, or was, until you decided to change the subject entirely.
Get a clue: I and everyone else agree that mechanical energy is conserved in this system.
In the context of physics, in the real world, the TOTAL amount of energy in such a conservative SUSTEM, with two stationary masses, is determined by the gravitational PE BETWEEN the two masses over the distance between them. ALL the energy is PE at the start and during the transit over the distance the energy is converted to KE, until at the point of contact ALL of the energy is KE and PE is zero.
Still comically wrong. You might have squeaked by in your civil engineering classes with such a shoddy understanding, but clearly you never took a serious course in classical mechanics.

Just for review: Conservation of mechanical energy means that PEi + KEi = PEf + KEf, not that KEf = PEi. (That latter is only true in certain simple cases.)
Tell me how much PE there is between two masses that are in contact with each other, when the distance is zero.
Two macroscopic masses? Easy: How big are they? How far apart are their centers?
I will give you the answer without the need for any integration; the PE is zero, NOT infinity.
It's easy to get the wrong answer with no calculation at all!
Don't confuse macroscopic objects with point masses. (Of course, that's just one of your confusions.) In any case, the PE is not zero!
The only thing that is comical about this is the way you are blindly applying abstract mathematical concepts to what is a practical real world physics problem and coming up with comical answers. There are NO “point particles” there is NO infinite energy and there is NO infinite velocity except in your abstract math which has no application to the real physical universe.
Note that the "real world" problem of two macroscopic objects (let's say two perfect spheres, for simplicity) being attracted by gravity alone is solved in exactly the same way as for two point masses! The only difference is that you don't go from r = 1 m to r= 0, you go from r = 1 m to r = D (the distance between the centers on contact). In both problems the PE is given by -GMm/r; it is most certainly not zero.
I am done with this joke of a physics forum. This is a sad reflection on the state of physics education in the USA today.
My thoughts exactly! :wink:
 

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