Universal gravitation’s problem -- Balancing gravitational forces from 2 masses

In summary, the problem of balancing gravitational forces from two masses involves determining the point at which the gravitational pulls of both masses are equal and opposite, resulting in a state of equilibrium. This requires calculating the gravitational force exerted by each mass using Newton's law of universal gravitation and setting them equal to solve for the distance from each mass where this balance occurs. Understanding this concept is crucial in fields like astrophysics and orbital mechanics.
  • #1
Riccardo Finessi
1
0
Homework Statement
I have this problem that I’ll must have done for tomorrow but I can’t figure it out, I have done an attempt but dosean’t take anywhere, can anyone help me figure it out


Two particles are on the x-axis. Particle 1 has mass m and is at the origin of the axis, while particle 2 has mass 2m and its position is x = +L. Between these two particles there is a third particle.
At what position on the x-axis would the third particle have to be for the magnitude of the gravitational attractive force acting on both particles 1 and 2 to double? Express your answer in terms of L.


result:0,414L
Relevant Equations
F=G m1 m2 / d*2
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Last edited:
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  • #2
Welcome to PF.

What is "t" in your equations? Time?
 
  • #3
Welcome to PF!

When posting your work, we ask that you type your work (using Latex if possible), rather than posting images of your work. More guidelines for posting questions about homework problems can be found here.

It's a little hard to follow your work in the image. There are no words to describe your train of thought. However, I think your work is ok up to the following

1715622246482.png
 
  • #4
With a small sketch things become easier:

1715645968120.png

In number 1 you have $$
F={G\,m_1m_2\over L^2}
$$so in number 2 you want $$
{G\,m_1m_3\over x^2L^2}={G\,m_1m_2\over L^2}\quad\Rightarrow \quad
m_2 = {m_3\over x^2} \quad \Rightarrow \quad m_1 = {m_3\over 2x^2}
$$Then in number 3 you require $$
{G\,m_2m_3\over (1-x^2)L^2} = {G\,m_1m_2\over L^2}\quad\Rightarrow \quad m_1 = {m_3\over (1-x)^2}
$$this way it's easy to see your
1715687608177.png
was still correct, as @TSny replied.

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FAQ: Universal gravitation’s problem -- Balancing gravitational forces from 2 masses

What is universal gravitation?

Universal gravitation is a fundamental physical law that describes the attraction between two masses. Formulated by Sir Isaac Newton, it states that every point mass attracts every other point mass in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The formula is given by F = G(m1*m2)/r², where F is the gravitational force, G is the gravitational constant, m1 and m2 are the masses, and r is the distance between their centers.

How do you calculate gravitational force between two masses?

To calculate the gravitational force between two masses, you can use Newton's law of universal gravitation. The formula is F = G(m1*m2)/r². Here, F is the gravitational force, G is the gravitational constant (approximately 6.674 × 10^-11 N(m/kg)²), m1 and m2 are the masses of the two objects, and r is the distance between the centers of the two masses. By substituting the values of the masses and the distance into the formula, you can find the gravitational force acting between them.

What is the balancing point between two masses?

The balancing point, or equilibrium point, between two masses occurs at a location where the gravitational forces exerted by both masses on a third mass are equal in magnitude but opposite in direction. To find this point, you can set the gravitational forces equal to each other and solve for the position. If m1 is the mass of the first object, m2 is the mass of the second object, and d is the distance between them, the position x from m1 where the third mass would balance can be found using the equation m1/(d-x) = m2/x, where d-x is the distance from m1 to the balancing point and x is the distance from m2 to the balancing point.

What happens if the two masses are equal?

If the two masses are equal, the balancing point is located exactly halfway between them. This is because the gravitational forces exerted by both masses will be the same at that midpoint, resulting in a net force of zero on a third mass placed there. Mathematically, if m1 = m2, the distance x from either mass to the balancing point will be d/2, where d is the total distance between the two masses.

Can gravitational balance points exist outside the two masses?

Yes, gravitational balance points can exist outside the two masses, particularly if the masses are significantly different. In such cases, a third mass can be placed at a distance beyond the lighter mass, where the gravitational pull from the heavier mass can balance the gravitational pull from the lighter

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