How Does Angular Momentum Conservation Affect Asteroid Collision Dynamics?

In summary, the conservation of angular momentum plays a crucial role in asteroid collision dynamics by dictating the rotational and translational motion of colliding bodies. When asteroids collide, their angular momentum before the impact must equal the angular momentum after the impact, influencing their post-collision trajectories and spins. This principle helps scientists predict the outcomes of collisions, including changes in rotation rates and orbital paths, which are vital for understanding the behavior of asteroids in space and assessing potential threats to Earth.
  • #106
Note that I used ##R## instead of ##d## in calculating ##\omega##, so I'll have to redo my calculation.
 
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  • #107
Hak said:
the previous calculations regarding Icm and conservation of momentum are wrong.
Not wrong enough to matter. ##I_{cm}\approx \frac 25MR^2##, ##I_{cm}\omega\approx mvR##.
 
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  • #108
haruspex said:
Not wrong enough to matter. ##I_{cm}\approx \frac 25MR^2##, ##I_{cm}\omega\approx mvR##.
Yes, if ##m \ll M##.
 
  • #109
PeroK said:
Note that I used ##R## instead of ##d## in calculating ##\omega##, so I'll have to redo my calculation.
Okay, I am waiting for a response. I didn't understand what result there is in Kleppner and Kolenkow....
 
  • #110
erobz said:
If it was meant to be a small asteroid hitting a still planetary sized body where ##m \ll M## then we can tell without doing any calculation though that ##F \approx 0##. by your own result as ##\frac{m}{M} \approx 0## , giving ##\omega \approx 0##?
m/M is supposed to be small compared to unity, not approach zero absolutely. It can't be eliminated when it stands alone.
 
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  • #111
Hak said:
Yes, if ##m \ll M##.
So what's your problem?
 
  • #112
Chestermiller said:
So what's your problem?
None, I had not noticed this aspect before @haruspex's message.
 
  • #113
When I don't use ##m \ll M ## and plug in ##M= 9m## I get:

$$ I_{com} = \frac{9}{2}m R^2 $$

$$ \omega = \frac{v}{5R} $$

$$F = \frac{9mv^2}{250 R}$$
 
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  • #114
erobz said:
When I don't use ##m \ll M ## and plug in ##M= 9m## I get:

$$ I_{com} = \frac{9}{2}m R^2 $$

$$ \omega = \frac{v}{5R} $$

$$F = \frac{9mv^2}{250 R}$$
That's what I get now.
 
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  • #115
PeroK said:
That's what I get now.
Yes, that should be right. So, is my generic result in post #101 correct?
 
  • #116
Chestermiller said:
m/M is supposed to be small compared to unity, not approach zero absolutely. It can't be eliminated when it stands alone.
I'd like to see the maths. There is a term in ##\frac {m^2v}{M}## in the final calculation for ##F##. I don't know how to handle that if we have ##m \ll M##.
 
  • #117
PeroK said:
I'd like to see the maths. There is a term in ##\frac {m^2v}{M}## in the final calculation for ##F##. I don't know how to handle that if we have ##m \ll M##.
Where is this term? I can't see it.
 
  • #118
PS it's not like the calculations are particularly complicated without the simplification. And, ultimately, the force per unit mass on ##m## is proportional to ##\frac m M##.
 
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  • #119
I am missing the utility in the approximation ##m \ll M ## that is being talked about, given that a person like me can solve it without.
 
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  • #120
PeroK said:
PS it's not like the calculations are particularly complicated without the simplification. And, ultimately, the force per unit mass on ##m## is proportional to ##\frac m M##.
Excuse me, but I cannot see what you are saying. Could you check my result in post #101 and tell me where I am wrong? Thank you very much.
 
  • #121
Hak said:
Excuse me, but I cannot see what you are saying. Could you check my result in post #101 and tell me where I am wrong? Thank you very much.
Yes, that looks right to me.
 
  • #122
PeroK said:
Yes, that looks right to me.
Okay, but how to make my equation for force per unit mass visibly proportional to ##\frac{m}{M}##? In the case where ## m \ll M##, how would such an equation become?
 
  • #123
Hak said:
Okay, but how to make my equation for force per unit mass visibly proportional to ##\frac{m}{M}##? In the case where ## m \ll M##, how would such an equation become?
That's with the simplifications using ##\frac m M \ll 1##. There's a discussion about whether that's a valid approximation to make in this case.
 
  • #124
PeroK said:
That's with the simplifications using ##\frac m M \ll 1##. There's a discussion about whether that's a valid approximation to make in this case.
Sorry to bother you, but I didn't understand very well, I understood only partially.
 
  • #125
Hak said:
Sorry to bother you, but I didn't understand very well, I understood only partially.
Don't worry about it. The thread has 125 posts already!
 
  • #126
PeroK said:
Don't worry about it. The thread has 125 posts already!
So?
 
  • #127
Hak said:
Okay, but how to make my equation for force per unit mass visibly proportional to ##\frac{m}{M}##? In the case where ## m \ll M##, how would such an equation become?
Not sure what you are asking. You have established ##\omega\approx\frac{5mv}{2MR}## and ##F\approx mR\omega^2##. Put those together.
 
  • #128
Just for the record.

My expression in post#55 for finding the moment of inertia of the composite mass is $$\frac{2}{5}MR^2+md^2=I_{cm}+(M+m)(R-d)^2.$$ If one replaces ##d=\dfrac{MR}{M+m}## and solves for ##I_{cm}##, one gets $$I_{cm}=\frac{2}{5}MR^2+\frac{Mm}{M+m}R^2.$$ @erobz 's expression for ##I_{cm}## in post#62 is $$I_{cm} = \frac{2}{5}MR^2 + M(R-d)^2 + md^2.$$
If one replaces ##d=\dfrac{MR}{M+m}## and solves for ##I_{cm}##, one gets $$I_{cm}=\frac{2}{5}MR^2+\frac{Mm}{M+m}R^2.$$Just because the expressions look different doesn't mean that they are different. Folks who are interested in expansions should note that $$I_{cm}\approx\frac{2}{5}MR^2\left(1+\frac{\cancel{7}5m}{2M}\right).$$

Edited to fix error in the approximate expression. See posts #208 and #231
 
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  • #129
haruspex said:
Not sure what you are asking. You have established ##\omega\approx\frac{5mv}{2MR}## and ##F\approx mR\omega^2##. Put those together.
Thank you, I understand now. So, the force ##F## is not approximate to ##0## when ## m \ll m## as was said previously, right?
 
  • #130
Okay, so what we have is the full calculation giving:
$$F = \frac{25mv^2}{4R}\bigg [\frac 1 {1 +\mu} \bigg ] \bigg [\frac{\mu}{1 + \frac{7\mu}{2}} \bigg ]^2 \approx \frac{25mv^2}{4R}\big [\mu^2 -8\mu^3 \big ]$$Where ##\mu = \frac m M##

Whereas, if we make the simplifications earlier in the calculation, we get:
$$F \approx \frac{25mv^2}{4R}\big [\mu^2 \big ]$$These are the same up to the second order in ##\mu##. But, there is a factor of ##8## in the third order term.

With ##\mu = 0.01## there is still an 8% difference. That seems quite significant. You need ##\mu = 0.001## for the early simplifications to give only a 1% error.

I'm not sure what conclusion to draw.
 
  • #131
Actually, my conclusion is that the question should be explicit about giving an answer to the first significant order of ##\frac m M##. Also, it seems pointless to calculate the centripetal force on ##m##. Calculating ##\omega## would make much more sense.
 
  • #132
PeroK said:
The idea is that I have got a formula for ##F## in terms of ##m, M, v, R##. If I post that formula, then I've given you the answer. But, if I plug ##M = 9m## into that formula and simplify, then that gives you something to check. It also gives the others something to check and they can confirm whether I've got it right or not. I think it's right, but we all make mistakes.
It's right unless I made the same mistake as you.
 
  • #133
kuruman said:
It's right unless I I made the same mistake as you.
But, not really a mistake. I unwittingly made the simplification ##d \approx R##. Which is significant if we take ##\mu = 0.1##, which is too large for the simplifications to be valid.
 
  • #134
Could you please explain the simplifications you have made? How did you come to such conclusions in retrospect?
 
  • #135
Hak said:
Could you please explain the simplifications you have made? How did you come to such conclusions in retrospect?
Just do what @haruspex suggested.
 
  • #136
PeroK said:
Just do what @haruspex suggested.
I did, but I didn't understand the percentages you set up.
 
  • #137
Hak said:
I did, but I didn't understand the percentages you set up.
Just plug in the numbers!
 
  • #138
PeroK said:
But, not really a mistake. I unwittingly made the simplification ##d \approx R##. Which is significant if we take ##\mu = 0.1##, which is too large for the simplifications to be valid.
Funny thing, I did too. My corrected exact value for ##\omega## when ##M=9m## is $$\omega =\frac{1}{5}\frac{v}{R}.$$It turns out that no approximation is needed if one uses the simplified moment of inertia in post#128.

(Original expression edited to add missing factor of 5 in the numerator.)
 
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  • #139
kuruman said:
Funny thing, I did too. My corrected exact value for ##\omega## when ##M=9m## is $$\omega =\frac{1}{25}\frac{v}{R}.$$It turns out that no approximation is needed if one uses the simplified moment of inertia in post#128.
Sorry to bother you again, could you explain this assumption better? Thank you for your patience, sorry again.
 
  • #140
It's not an assumption. I am following @PeroK's lead in post#95. I derived an expression for ##\omega## that I think is correct, I plugged in ##M=9m## and simplified. This allows for other users to check their answers against mine without anyone giving the answer away which is against our rules.
 
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