How Does Angular Momentum Conservation Affect Asteroid Collision Dynamics?

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Angular momentum conservation plays a crucial role in asteroid collision dynamics, particularly when a minor asteroid collides with a major one and becomes embedded. Before the collision, both linear and angular momentum are conserved, allowing for the calculation of post-collision velocities and angular velocities. After the collision, the combined system moves as a single rigid body, with the minor asteroid contributing to the overall moment of inertia. The discussion highlights the importance of correctly determining the linear velocity of the center of mass and the angular velocity, especially in the context of centripetal forces acting on the embedded asteroid. Overall, the conversation emphasizes the complexities of applying conservation laws in inelastic collisions involving extended bodies.
  • #151
erobz said:
The theory we were laboring under there was updated 5 posts later. Have you properly updated the linear momentum equation?
Sorry, we had said that the linear momentum conservation equation was not necessary for the purpose of force calculation, so we did not update it. Our discussion on it ended there, so this is our final equation. How should it be modified?
 
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  • #152
Hak said:
Sorry, we had said that the linear momentum conservation equation was not necessary for the purpose of force calculation, so we did not update it. Our discussion on it ended there, so this is our final equation. How should it be modified?
What is the linear velocity of the imbedded asteroid in the ground frame just after impact?
 
  • #153
erobz said:
What is the linear velocity of the imbedded asteroid in the ground frame just after impact?
We had said ##V = v' + \omega d##, but it doesn't fit with what I said in post #149
 
  • #154
Hak said:
We had said ##V = v' + \omega d##, but it doesn't fit with what I said in post #149
What is the angular momentum of the little asteroid with respect to the center mass before impact?
 
  • #155
erobz said:
What is the angular momentum of the little asteroid with respect to the center mass before impact?
Isn't it ##L = mvd##?
 
  • #156
Hak said:
Isn't it ##L = mvd##?
Yeah
 
  • #157
erobz said:
Yeah
Okay, but I can't hit the nail on the head. In post #149 I said that I arrived at the same angular momentum conservation equation by a different method, which involves a different linear momentum conservation equation, isn't that right?
 
  • #158
Hak said:
Okay, but I can't hit the nail on the head. In post #149 I said that I arrived at the same angular momentum conservation equation by a different method, which involves a different linear momentum conservation equation, isn't that right?
We don't arrive at the same angular momentum by linear momentum arguments.

Angular momentum is not dependent on the linear momentum here, but the linear momentum is dependent on the angular momentum.
 
  • #159
erobz said:
We don't arrive at the same angular momentum by linear momentum arguments.

Angular momentum is not dependent on the linear momentum here, but the linear momentum is dependent on the angular momentum.
So why is my expression in post #149 incorrect?
 
  • #160
I believe the equation should be:

$$ mv = M v' + m(v' + \omega d)$$

where ## \omega = \frac{mvd}{I_{com}}##
 
  • #161
erobz said:
I believe the equation should be:

$$ mv = M v' + m(v' + \omega d)$$

where ## \omega = \frac{mvd}{I_{com}}##
Okay, so far so good, but I'm talking about something else. I am saying that calculating angular momentum with respect to the center of the larger sphere, and not with respect to the center of mass of the system, leads to a different equation of conservation of linear momentum. What you expressed just now is a different procedure from mine in post #149, that's what we used yesterday.
 
  • #163
Hak said:
Okay, so far so good, but I'm talking about something else. I am saying that calculating angular momentum with respect to the center of the larger sphere, and not with respect to the center of mass of the system, leads to a different equation of conservation of linear momentum. What you expressed just now is a different procedure from mine in post #149, that's what we used yesterday.
Maybe now that I'm looking at it, the mass ##M## is rotating about the center of mass too after the collision albeit with smaller radius and in opposite direction.

##v'## is the combined center of mass velocity...

So perhaps it should be:

$$ mv = M( v' - \omega ( R-d) ) + m( v' + \omega d ) $$

Or do we also need to adjust the referencing the center of mass velocity before the collision too like:

$$ \frac{m}{M+m}v = M( v' -\omega ( R-d) ) + m( v' + \omega d ) $$
 
  • #164
Hak said:
@PeroK, @kuruman, @haruspex, @Chestermiller What do you think about it?
Linear momentum and angular momentum are conserved separately. The point about which you choose to measure angular momentum does not affect the linear momentum calculation.
 
  • #165
erobz said:
Maybe now that I'm looking at it, the mass ##M## is rotating about the center of mass too after the collision albeit with smaller radius.

##v'## is the combined center of mass velocity?

So perhaps it should be:

$$ mv = M( v' + \omega ( R-d) ) + m( v' + \omega d ) $$

Or do we also need to adjust the referencing the center of mass velocity before the collision too like:

$$ \frac{m}{M+m}v = M( v' + \omega ( R-d) ) + m( v' + \omega d ) $$
I am struggling to understand this process. The velocity ##v'## is the velocity of the center of mass of the largest sphere, I think. Could you explain these steps better?
 
  • #166
PeroK said:
Linear momentum and angular momentum are conserved separately. The point about which you choose to measure angular momentum does not affect the linear momentum calculation.
Ok, but I can't find the error in post #149. Could you help me in that regard?
 
  • #167
Hak said:
I am struggling to understand this process. The velocity ##v'## is the velocity of the center of mass of the largest sphere, I think. Could you explain these steps better?
I think ##v'## actually needs to be the velocity of the center of mass. Before collision are looking at ##v_{cm} = \frac{m}{M+m}v##, and after the collision we are looking at ##v_{cm} = v'##.
 
  • #168
erobz said:
Before collision are looking at ##v_{cm} = \frac{m}{M+m}v##, and after the collision we are looking at ##v_{cm} = v'##.
Why?
 
  • #169
Hak said:
Why?
The rotation of each mass ( ##M## and ##m##) about the center of mass the instant after collision has me speculating.
 
  • #170
erobz said:
The rotation of each mass ( ##M## and ##m##) about the center of mass the instant after collision has me speculating.
Yes, but I cannot understand such assumptions. From where do you derive this velocity ##v_{cm}##, and under what assumptions do you place it as the initial velocity? Could it not be, more simply, ##mv = (M+m) v_{cm}##?
 
  • #171
I don't know, I'm getting confused. You might be correct and we only need to look at the change in center of mass velocity before and after collision, not the velocities of each component mass...
 
  • #172
erobz said:
I don't know, I'm probably confused. You might be correct and we only need to look at the change in center of mass velocity before and after collision, not the velocities of each component mass...so:

$$ \frac{m^2}{m+M}v = ( M+m)v'$$

?

Although the problem is solved, this point is interesting, isn't it? I can't understand the ##(M+m)## factor in the denominator, I'm more confused than you are. What do you say, let's wait for some input from the other members, like @kuruman, @haruspex, @PeroK, @Chestermiller, or maybe others who haven't participated in the thread?
 
  • #173
Hak said:
Although the problem is solved, this point is interesting, isn't it? I can't understand the ##(M+m)## factor in the denominator, I'm more confused than you are. What do you say, let's wait for some input from the other members, like @kuruman, @haruspex, @PeroK, @Chestermiller, or maybe others who haven't participated in the thread?
Considering the apparent source and level of this problem, I agree with @haruspex's determination.
 
  • #174
Hak said:
Although the problem is solved, this point is interesting, isn't it? I can't understand the ##(M+m)## factor in the denominator, I'm more confused than you are. What do you say, let's wait for some input from the other members, like @kuruman, @haruspex, @PeroK, @Chestermiller, or maybe others who haven't participated in the thread?
I deleted that equation. It might be correct, but I'm not sure. So I didn't want to stir the pot with it ( but you are very quick on the draw).

As for that factor in the denominator it would have came from this idea:

1695645885499.png


to calculate the velocity of the system center of mass:

$$ v_{cm} = \frac{mv+ M\cdot 0}{m+M} = \frac{m}{M+m}v$$
 
  • #175
Chestermiller said:
Considering the apparent source and level of this problem, I agree with @haruspex's determination.
What is "@haruspex's determination"?
 
  • #176
erobz said:
I deleted that equation. It might be correct, but I'm not sure. So I didn't want to stir the pot with it ( but you are very quick on the draw).

As for that factor in the denominator it would have came from this idea:

View attachment 332540

to calculate the velocity of the system center of mass:

$$ v_{cm} = \frac{mv+ M\cdot 0}{m+M} = \frac{m}{M+m}v$$
The problem is that all the assumptions made are worthy of attention and make sense, so as far as I can tell, they could all be correct. Unfortunately, I do not have much experience (I am only a student), so I cannot know for sure which of them is the correct answer. Anyway, I don't want to be presumptuous, I just try to learn by asking questions.
 
  • #177
Hak said:
The problem is that all the assumptions made are worthy of attention and make sense, so as far as I can tell, they could all be correct. Unfortunately, I do not have much experience (I am only a student), so I cannot know for sure which of them is the correct answer. Anyway, I don't want to be presumptuous, I just try to learn by asking questions.
Its possible... the same way @kuruman and I had different approaches to the moment of inertia that appeared to be different on inspection, but were in fact the same.

$$ mv = M( v' - \omega ( R-d) ) + m( v' + \omega d ) \tag{1} $$

This equation (1) seems like its keeping track of all the individual mass center momentums

$$( M+m) \frac{m}{m+M}v = ( M+m )v' \tag{2} $$

This equation (2) seems like forget about that and just focus on the change in center of mass momentum.

Both of them make sense to me, and for some reason I decided to mix them...which I think was wrong.

The second is easy to solve. The first one is obviously more work, but I ( we) should probably try it to see if they yield to each other.

EDIT: fixed equation 2 to make it correct.
 
Last edited:
  • #178
Linear momentum conservation throughout a collision between two masses means one thing and one thing only: The momentum of the center of mass of the two-mass system is the same before the collision as it is after the collision. Since linear momentum is a vector, this means that both its magnitude and direction do not change. We can find the velocity of the center of mass using the definition $$V_{cm}=\frac{mv_{\text{before}}+MV_{\text{before}}}{m+M}.$$ Before the collision, ##v_{\text{before}}=v## and ##V_{\text{before}}=0## so that $$V_{cm}=\frac{mv}{m+M}$$ and that's all there is. Note that after the collision, the CM is the only point that moves in a straight line with velocity ##V_{cm}## while all other points rotate about it with angular velocity ##\omega.## This means that the linear momentum of any mass element ##dm## away from the CM is not conserved.

As for conserving angular momentum about point O, the center of the planet, one needs to also consider the orbital angular moment about O after the collision.
##L_{\text{before}}=mvR##
##L_{\text{after}}=L_{\text{about CM}}+L_{\text{of cm}}##
Now
##L_{\text{about cm}}=I_{cm}~\omega## which is the same as before.
##L_{\text{of cm}}=(M+m)V_{cm}(R-d)## because the cm is at distance ##(R-d)## from point O.
Angular momentum conservation about point O demands that $$\begin{align}
& L_{\text{before}} = L_{\text{after}} \nonumber \\
&mvR=I_{cm}~\omega+(M+m)V_{cm}(R-d) \nonumber \\
& mvR=I_{cm}~\omega+\cancel{(M+m)}\frac{mv}{\cancel{M+m}}(R-d) \nonumber \\
& \cancel{mvR}=I_{cm}~\omega+mv(\cancel{R}-d) \nonumber \\
& 0=I_{cm}~\omega -mvd \nonumber \\
& mvd=I_{cm}~\omega. \nonumber
\end{align} $$ Surprise, surprise!
 
  • #179
kuruman said:
Linear momentum conservation throughout a collision between two masses means one thing and one thing only: The momentum of the center of mass of the two-mass system is the same before the collision as it is after the collision. Since linear momentum is a vector, this means that both its magnitude and direction do not change. We can find the velocity of the center of mass using the definition $$V_{cm}=\frac{mv_{\text{before}}+MV_{\text{before}}}{m+M}.$$ Before the collision, ##v_{\text{before}}=v## and ##V_{\text{before}}=0## so that $$V_{cm}=\frac{mv}{m+M}$$ and that's all there is. Note that after the collision, the CM is the only point that moves in a straight line with velocity ##V_{cm}##, while all other points rotate about it with angular velocity ##\omega.## This means that the linear momentum of any mass element ##dm## away from the CM is not conserved.

As for conserving angular momentum about point O, the center of the planet, one needs to also consider the orbital angular moment about O after the collision.
##L_{\text{before}}=mvR##
##L_{\text{after}}=##L_{\text{about CM}}+##L_{\text{of cm}}##
Now
##L_{\text{about cm}}=I_{cm}~\omega## which is the same as before.
##L_{\text{of cm}}=(M+m)V_{cm}(R-d)## because the cm is at distance ##(R-d)## from point O.
Angular momentum conservation about point O demands that $$\begin{align}
& L_{\text{before}} = L_{\text{after}} \nonumber \\
&mvR=I_{cm}~\omega+(M+m)V_{cm}(R-d) \nonumber \\
& mvR=I_{cm}~\omega+\cancel{(M+m)}\frac{mv}{\cancel{M+m}}(R-d) \nonumber \\
& \cancel{mvR}=I_{cm}~\omega+mv(\cancel{R}-d) \nonumber \\
& 0=I_{cm}~\omega -mvd \nonumber \\
& mvd=I_{cm}~\omega. \nonumber
\end{align} $$ Surprise, surprise!
I don't know if you noticed, but it is roughly the same procedure as mine in post #149. The equation I arrived at is the same.
 
  • #180
erobz said:
Its possible... the same way @kuruman and I had different approaches to the moment of inertia that appeared to be different on inspection, but were in fact the same.
This equation (1) seems like its keeping track of all the individual mass center momentums
This equation (2) seems like forget about that and just focus on the change in center of mass momentum.

Both of them make sense to me, and for some reason I decided to mix them...which I think was wrong.

The second is easy to solve. The first one is obviously more work, but I ( we) should probably try it to see if they yield to each other.
Equation (2) gives:

$$v' = \left(\frac{m}{m+M} \right)^2 v$$.

This equation has a power of 2 to the exponent over the expression of ##v_{cm}## that I had calculated and that @kuruman also calculated.

Equation (1) gives:

$$v' = \left(\frac{m}{m+M}\right) v + \frac{10 m^2 M}{(M+m)^2 (2M + 7m)}v$$.

This expression, in my opinion, has an awkward term on the right hand side. Most interestingly, if you change a minus sign to a plus sign in only one of the two round brackets referring to ##m## and ##M##, you get the expression:

$$v' = \left(\frac{m}{m+M} \right) v$$, that is, the same as before.

How can this be explained?
 

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