Net gravitational force of zero?

In summary, the question asks for the position along the x-axis between two spherical planets with identical masses M, located at the origin and position x = +d, where a person would experience a net gravitational force of zero. The formula Fg = (Gm1m2) / r^2 is used to calculate the force between the two planets, but the error is that the force on the person must be calculated, resulting in two equations. The solution for the first part of the problem is x = d/2, but for the second part where the mass at the origin changes to 4M, the answer will be different. The balance point occurs at the location where the two masses are equidistant from the person.
  • #1
tquiva
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Homework Statement


Imagine two spherical planets fixed on the x-axis, one with mass M at the origin, and the other with identical mass M at the position x = +d. (Assume that d is much greater than the radius of either planet.) At what position along the x-axis between the two masses could you position yourself so that you would experience a net gravitational force of zero?


Homework Equations


Fg = (Gm1m2) / r^2


The Attempt at a Solution


I know that
Fg = (Gm1m2) / r^2
and since both masses are identical, then
Fg = (GMM) / d^2 = (GM^2)/ d^2

I've tried plugging in numerous values for d in which both would cancel out, but I can't seem to find a value. Could someone please help me? Any help would be greatly appreciated...
 
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  • #2
tquiva said:
and since both masses are identical, then
Fg = (GMM) / d^2 = (GM^2)/ d^2

I've tried plugging in numerous values for d in which both would cancel out, but I can't seem to find a value.

Hopefully it is pretty obvious that plugging values into that particular equation is never going to get you a result of 0 for the force, not for any finite value of d. The error here is that you are calculating the force that each planet exerts on the other planet. What you need to calculate is the force that each planet exerts on you. This means there will be two equations, one for the force of planet 1 on you, and other for the force of planet 2 on you. Let's say that we're calling the planet that is at the origin 'planet 1.' Let's say also, for the sake of argument, that you are located a distance 'x' from the origin. This means that 'x' is your distance from planet 1. What is your distance from planet 2? Draw a picture.

You want to solve for the location 'x' that results in the force from planet 1 on you cancelling out the force from planet 2 on you. Remember that force has a direction, and in the case of gravity, the force always points towards the object that is causing it. This means that one of the forces will point to the right (which we could call the 'positive' direction), and the other force will point to the left (which we could call the 'negative' direction). Therefore, the forces will have opposite signs, so if you find x such that their magnitudes are equal, then they will cancel exactly.
 
  • #3
I finally came up with my value for x, which is x = d/2. However, part II of my problem asks for the same question except the mass at origin changes to 4M. I did the math, and it seems that it does not matter if both masses change, since the masses cancel out in the equation. So if I want a net gravitational force of zero with mass 4M, the value for x is also d/2 as in part I of the problem. Am I correct?
 
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  • #4
tquiva said:
I finally came up with my value for x, which is x = d/2. However, part II of my problem asks for the same question except the mass at origin changes to 4M. I did the math, and it seems that it does not matter if both masses change, since the masses cancel out in the equation. So if I want a net gravitational force of zero with mass 4M, the value for x is also d/2 as in part I of the problem. Am I correct?

Well, which one is it? Do both masses change, or just the one at the origin? If only one of the masses changes, then the answer will be different.

Intuitively, if both masses are the same, the balance point occurs at the location where they are equidistant from you. Makes sense, right? If the two masses are different, then the balance point will be closer to the lighter mass and farther from the heavier mass. Again, this makes sense, right?
 
  • #5
yes it does now.
thank you very much
 

FAQ: Net gravitational force of zero?

What is the concept of "Net gravitational force of zero"?

The net gravitational force of zero refers to a scenario in which the total gravitational force acting on an object is equal to zero. This can occur when the gravitational forces from multiple sources cancel each other out.

How is the net gravitational force of zero calculated?

The net gravitational force of zero is calculated by adding up all the individual gravitational forces acting on an object and determining if they cancel each other out. This can be done using vector addition and taking into account the direction and magnitude of each force.

What are some examples of objects with a net gravitational force of zero?

One example is a satellite in a circular orbit around the Earth. The gravitational force from the Earth is balanced by the centrifugal force from the satellite's orbit, resulting in a net gravitational force of zero. Another example is a person standing on a scale in an elevator that is accelerating downwards at the same rate as the force of gravity, resulting in a net gravitational force of zero and no change in weight.

Can the net gravitational force of zero ever change?

Yes, the net gravitational force of zero can change if the individual gravitational forces acting on an object change. For example, if the satellite in a circular orbit around the Earth moves closer or further away from the Earth, the net gravitational force of zero will change.

What are the implications of a net gravitational force of zero?

If an object experiences a net gravitational force of zero, it will not accelerate or change its motion. This can be useful in certain scenarios, such as in stable orbits or when objects are in free fall. It also allows for the study of the effects of gravity on objects without the interference of other forces.

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