How Do Gravitational Forces Affect the Speed of Two Approaching Masses?

AI Thread Summary
The discussion focuses on calculating the speeds of two masses, M1 and M2, as they approach each other due to gravitational forces. Participants emphasize using energy conservation principles to relate gravitational potential energy and kinetic energy, noting that the initial potential energy is zero when the masses are infinitely apart. The importance of conservation of momentum is also highlighted, as it is necessary to solve for both velocities accurately. There is debate over the relevance of the mass ratio M1 to M2, with some arguing that the approximation M1>>M2 is not applicable in this scenario. Overall, the conversation stresses the need for a comprehensive approach that combines energy and momentum conservation to determine the speeds of both masses.
NAkid
Messages
70
Reaction score
0

Homework Statement


Two particles of masses M1 = 81000 kg and M2 = 9400 kg are initially at rest an infinite distance apart. As a result of the gravitational force the two masses move towards each other. Calculate the speed of mass M1 and mass M2 when their separation distance is 26.5 km.


Homework Equations





The Attempt at a Solution


I think you have to use energy-conservation equations here for each mass

1/2mv1^2 - (GM1M2)/R = 1/2mv2^2 - (GM1M2)/R

so, for mass M1, v1=0 and (GM1M2)/R on the left = 0 because R = infinite. then you get

1/2m1v2^2 = (GM1M2)/R --and solve for v2, but this doesn't seem to be correct..
 
Physics news on Phys.org
Lets say that the 2 masses were infinitely separated. The potential energy of the system would be 0J. However, an attractive force acts on them and they are brought closer together, in which the separation between them 26.5 km. Because it is an attractive force, the potential energy of the system is negative. What you do is find the change in potential energy. The initial value is 0J and the final value would be when they are the given distance apart. Using -dU = dK (d being delta, U being gravitational potential energy, and K being kinetic energy), you would solve for the kinetic energy of each mass. From that, you solve for velocity.
 
isn't that basically what i did? calculated the changes to solve for velocity?
 
Hint:

M1>>M2
 
physixguru said:
Hint:

M1>>M2

M1 / M2 <10 so I don't think you can say that.


-GM1M2/r is the potential energy of BOTH the masses.

At the start, potential and kinetic energy is 0. at a distance r the total energy is:

(1/2)m_1v_1^2 + (1/2)m_2v_2^2 - Gm_1m_2/r

This won't allow you to calculate v_1 and v_2 by itself. You also need conservation of momentum.
 
kamerling said:
M1 / M2 <10 so I don't think you can say that.


-GM1M2/r is the potential energy of BOTH the masses.

At the start, potential and kinetic energy is 0. at a distance r the total energy is:

(1/2)m_1v_1^2 + (1/2)m_2v_2^2 - Gm_1m_2/r

This won't allow you to calculate v_1 and v_2 by itself. You also need conservation of momentum.

I never told him to ignore the masses.

DID I?
 
physixguru said:
I never told him to ignore the masses.

DID I?

Well I didn't think you said that. I just don't think that M1>>M2 is either true or helpful.
 
kamerling said:
Well I didn't think you said that. I just don't think that M1>>M2 is either true or helpful.

It is helpful for sure, especially when energy consideration comes into play.
 
physixguru said:
It is helpful for sure, especially when energy consideration comes into play.
It is not helpful for this problem. First, the approximation m1>>m2 is incorrect here, as m2 > m1/10. Second, the approximation implicitly makes the velocity of the larger mass zero, and the problem asks for both v1 and v2.

kamerling said:
-GM1M2/r is the potential energy of BOTH the masses.

At the start, potential and kinetic energy is 0. at a distance r the total energy is:

(1/2)m_1v_1^2 + (1/2)m_2v_2^2 - Gm_1m_2/r

This won't allow you to calculate v_1 and v_2 by itself. You also need conservation of momentum.

This, on the other hand, is very good advice.
 
Back
Top