Calculating two masses colliding

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In summary, the conversation discusses the method for calculating the time it takes for two masses in space to collide due to the force of gravity. The speaker explains their approach of integrating the formula a = GM / R^2 between the two points corresponding to the distances between the masses and using the acceleration formula T = sqrt (2S / a) to find the time. However, they are unsure if their method is correct and asks for confirmation or correction. The listener suggests a different approach using conservation of energy and separating the variables to find the time.
  • #1
Denton
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I have been wondering for a long time now on how to calculate the time taken for two masses in space to collide by force of gravity.

Now what I've basically done was integrate the formula a = GM / R^2 between the two points corresponding to the distances appart from the masses (assuming the masses are equal.) And with the acceleration, T = sqrt ( 2S / a ) (S being the distance between masses).

And I've gotten values of, say two 1 tonne masses at a distance of 1 Km would take approx 70 years to collide with each other.

Now I've got no idea whether I've gotten it right, or I am way off. It seems like a fair answer (then again they only weigh one tonne).

Can anyone confirm my working is correct and or what I am doing wrong. Thanks

-Denton.
 
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  • #2
Denton said:
I have been wondering for a long time now on how to calculate the time taken for two masses in space to collide by force of gravity.

Now what I've basically done was integrate the formula a = GM / R^2 between the two points corresponding to the distances appart from the masses (assuming the masses are equal.) And with the acceleration, T = sqrt ( 2S / a ) (S being the distance between masses).
HOW did you integrate that? That's the crucial point and you don't say. You can't just integrate the two sides independently- the right is a function of R and the left side is a derivative with respect to t.

And I've gotten values of, say two 1 tonne masses at a distance of 1 Km would take approx 70 years to collide with each other.

Now I've got no idea whether I've gotten it right, or I am way off. It seems like a fair answer (then again they only weigh one tonne).

Can anyone confirm my working is correct and or what I am doing wrong. Thanks

-Denton.
Again, I can't say what you are doing wrong because you don't say what you did! Simply saying you "integrated" an equation doesn't help since I don't know how you tried to itegrate it.

Here's how I would do that problem: First I'm going to put it in the "center of mass" system. Since the two objects have the same mass that will be the point exactly half way between them. If r is the distance from each mass, the distance between the two masses is 2r so we have, for each mass, [itex]dr^2/dt^2= -GM/4r^2[/itex]. Since the independent variable "t" does not appear in that explicitely, we can reduce the order of the equation by letting v= dr/dt. By the chain rule, [itex]dr^2/dt^2= dv/dt= (dv/dr)(dr/dt)= v(dv/dr)[/itex] so the equation becomes [itex]v(dv/dr)= -GM/r^2[/itex] for v as a function of r. We can write that as [itex]vdv= -(GM/4r^2)dr[/itex] and NOW integrate the left side with respect to v and the right side with respect to r. We get [itex](1/2)v^2= GM/4r+ C[/itex]. (If you move the "GM/4r" to the left side and multiply by M, you might recognize that as "conservation of energy".) If, initially, v= 0 and r= R, C= -GM/4R and we have [itex]v= dr/dt= \sqrt{GM/4r- GM/4R}= (\sqrt{GM}/2)\sqrt{1/r- 1/R}= (\sqrt{GM}/2R)\sqrt{(R-r)/r}[/itex]. That can be separted as [itex]\sqrt{r/(R-r)}dr= \sqrt{GM/2R}dt[/itex]. I don't have time now to complete that but if what you did is not like that, it's probable that your result is wrong.
 
  • #3


Hello Denton,

Thank you for your question. Calculating the time for two masses to collide due to gravity can be a complex problem, so it's great that you are thinking about it.

From your description, it seems like you have used the equation for Newton's Law of Gravitation, which states that the force of gravity between two masses is equal to the product of their masses divided by the square of the distance between them. This is a good starting point for calculating the acceleration of the masses towards each other.

However, there are a few things to consider when using this equation. Firstly, it assumes that the masses are point masses, which means they have no size or volume. In reality, all objects have a size and shape, which can affect the calculation. Secondly, the equation assumes that there are no other external forces acting on the masses, which may not be the case in space. Finally, the equation only gives us the magnitude of the force, not the direction. To get the direction, we need to use vector calculus, which can be quite complex.

With all that being said, your approach of using the equation for acceleration and then using it to calculate the time taken for the masses to collide is a valid method. However, it would be helpful to show your calculations and assumptions, so that we can verify if your answer is correct. Also, keep in mind that your answer may change depending on the masses and distances involved.

In summary, your approach seems reasonable, but it would be helpful to see your calculations and assumptions to confirm if your answer is correct. Keep exploring and asking questions, as that is the essence of science. Good luck!
 

1. How do I calculate the momentum of two masses colliding?

To calculate the momentum of two masses colliding, you will need to know the mass and velocity of each object. The formula for momentum is mass multiplied by velocity (p = mv). You can calculate the individual momentums of each object before the collision and then add them together to find the total momentum of the system.

2. What is the conservation of momentum?

The conservation of momentum states that in a closed system, the total momentum before a collision is equal to the total momentum after the collision. This means that the total momentum of the two masses colliding will remain constant, regardless of any changes in velocity or direction.

3. How do I calculate the velocity of the objects after the collision?

To calculate the velocity of the objects after the collision, you can use the conservation of momentum equation: m1v1 + m2v2 = m1v1' + m2v2'. Here, m1 and m2 are the masses of the two objects, v1 and v2 are their velocities before the collision, and v1' and v2' are their velocities after the collision.

4. What is an elastic collision?

An elastic collision is a type of collision in which the total kinetic energy of the system is conserved. This means that the objects involved will bounce off each other without any loss of energy. In other words, the total kinetic energy before the collision is equal to the total kinetic energy after the collision.

5. What is an inelastic collision?

An inelastic collision is a type of collision in which the total kinetic energy of the system is not conserved. This means that some energy is lost during the collision, usually in the form of heat or sound. In an inelastic collision, the objects involved will stick together or deform upon impact.

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