Prob Regarding Gravitational Force

In summary: Your name]In summary, we are trying to find the magnitude of the initial acceleration of the third sphere, released from rest at one corner of an equilateral triangle with sides of 1.2m and two spheres with a known mass of 2.8kg each at the other two corners. By using Newton's second law, F=ma, and calculating the net gravitational force on the third sphere from the other two spheres using F=G(m1m2/r^2), we can solve for the magnitude of the initial acceleration using the equation a = (2Gm1m2sin60)/(mr^2).
  • #1
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Homework Statement


Three uniform spheres are located at the corners of an equilateral triangle. each side of the triangle has a length of 1.2m. two of the spheres have a mass of 2.8kg each. the third sphere(mass unknown) is released from rest. considering only the gravitational forces that the spheres exert on each other, what is the magnitude of the initial acceleration of the third sphere?



Homework Equations


F=G(m1m2/r2)


The Attempt at a Solution


I oriented the triangle so the two spheres with a known mass are along the y-axis, therefore the x-component of the forces cancel via symmetry and we're left w/ the y-component which is (2Gm1m2sin60)/r2
Am i doing this right so far?
 
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  • #2




Yes, you are on the right track. To find the magnitude of the initial acceleration of the third sphere, you can use Newton's second law, F=ma, where F is the net force acting on the third sphere and m is its mass. In this case, the net force is the sum of the gravitational forces exerted by the other two spheres, which you have correctly calculated using the equation F=G(m1m2/r^2). As you mentioned, the x-components of these forces will cancel out, leaving only the y-component. Therefore, you can set up the equation F=ma as follows:

(2Gm1m2sin60)/r^2 = ma

Now, you can solve for the magnitude of the initial acceleration, a, by dividing both sides by the mass of the third sphere, m. This will give you:

a = (2Gm1m2sin60)/(mr^2)

Since you know the values for m1, m2, and r, you can plug them into the equation to find the numerical value for the initial acceleration. Remember to use the appropriate units for mass (kg) and distance (m) to get the correct units for acceleration (m/s^2).

I hope this helps! Let me know if you have any further questions.

 

1. What is gravitational force?

Gravitational force is a natural phenomenon by which objects with mass are attracted to one another. It is one of the four fundamental forces of nature and is responsible for the interactions between planets, stars, and other celestial bodies.

2. How does gravitational force affect objects?

Gravitational force affects objects by pulling them towards one another. The strength of this force depends on the mass of the objects and the distance between them. Objects with larger mass will have a stronger gravitational force between them.

3. What is the equation for calculating gravitational force?

The equation for calculating gravitational force is F = G(m1m2)/d^2, where F is the force, G is the gravitational constant, m1 and m2 are the masses of the two objects, and d is the distance between them. This equation was discovered by Sir Isaac Newton.

4. How does the distance between two objects affect gravitational force?

The distance between two objects directly affects the gravitational force between them. As the distance increases, the gravitational force decreases. This is known as the inverse-square law, where the force is inversely proportional to the square of the distance between the objects.

5. What is the difference between gravitational force and weight?

Gravitational force is the attraction between two objects with mass, while weight is the measurement of the force of gravity on an object. Weight can change depending on the gravitational force acting on an object, while gravitational force remains constant between two objects.

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