Gravitational Force on three spheres

In summary: Components along the x and y axes? If so, remember that you're dealing with vectors, so you'll need to break the forces into components to do vector addition.
  • #1
TmrK
21
0

Homework Statement


Three uniform spheres are located at the corners of an equilateral triangle. Each side of the triangle has a length of 0.550 m. Two of the spheres have a mass of 2.85 kg 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/r^2
G=6.67x10^-11

The Attempt at a Solution


I took the first formula & wrote down two separate ones as

F= G*m1m3/r^2
F= G*m2m3/r^2

where m3 = the unknown mass.

Basically, I do not know how I would find the third "unknown mass" if the Force is not known.
 
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  • #2
TmrK said:
Basically, I do not know how I would find the third "unknown mass" if the Force is not known.
Hint: You are asked to find the acceleration, not the mass or force.

Just call the mass m3 and keep going.
 
  • #3
Before I reply, would I use the formula

[itex]\Sigma[/itex]F=ma

to solve for a, which would give me

a=[itex]\Sigma[/itex]F/m?

Here is my work:

[itex]\Sigma[/itex]F=[itex]\frac{6.67x10-11 N*2.85 kg*2.85 kg}{0.550m2}[/itex]

[itex]\Sigma[/itex]F=[itex]\frac{5.4177075x10-40}{.3025}[/itex]

[itex]\Sigma[/itex]F= 1.79x10-39

Then for solving for a,

a=[itex]\frac{1.79x10-39}{2.85}[/itex]

a=6.28x10-40
 
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  • #4
TmrK said:
Before I reply, would I use the formula

[itex]\Sigma[/itex]F=ma

to solve for a, which would give me

a=[itex]\Sigma[/itex]F/m?

Here is my work:

[itex]\Sigma[/itex]F=[itex]\frac{6.67x10-11 N*2.85 kg*2.85 kg}{0.550m2}[/itex]
This line is incorrect. Newton's second law says[tex]\sum_i {\vec{F}_3}_i = m_3 \vec{a}_3[/tex]where F3i are the individual forces acting on mass 3 and a3 is the acceleration of mass 3. In your original post, you have expressions for the magnitude of the two forces acting on mass 3. You need to use the geometry of the problem to figure out their directions, so you can calculate the vector sum of those two forces.

A good idea would be to draw a picture. Place the two known masses on the x-axis, centered around the origin, and place mass 3 at the appropriate spot on the y-axis.
 
  • #5
Okay, from what I understand, being that this is an equilateral triangle, each angle would be 60[itex]\circ[/itex]. Therefore, each sphere on the x-line is Fcos(60[itex]\circ[/itex]), and the third sphere on the y-line is Fsin(60[itex]\circ[/itex]).

I could then use F=Gm1m/r2 or F=Gm2m/r2 to find out the mass of the third sphere.

From there, I can use the force found out from Fsin(60[itex]\circ[/itex]) and the other two forces from cosine to find out the acceleration. Correct or did I go into another wrong route?
 
  • #6
TmrK said:
Okay, from what I understand, being that this is an equilateral triangle, each angle would be 60[itex]\circ[/itex]. Therefore, each sphere on the x-line is Fcos(60[itex]\circ[/itex]), and the third sphere on the y-line is Fsin(60[itex]\circ[/itex]).
I'm not sure what that's supposed to mean.
I could then use F=Gm1m/r2 or F=Gm2m/r2 to find out the mass of the third sphere.
No, you can't solve for m3. It turns out you don't need to know it because it will cancel out. So, as Doc Al suggested, just call it m3, write down your equations, and it will divide out.
From there, I can use the force found out from Fsin(60[itex]\circ[/itex]) and the other two forces from cosine to find out the acceleration. Correct or did I go into another wrong route?
Write down the two equations for the sums in the x and y directions.
 
  • #7
I mean 60 degrees. And the x & y equations would refer to the displacement equations, yes?

And to sum it all up, although I listed all of the equations, I would not know what to start out with and which equation to end with.
 
  • #8
I know what the 60∘ stood for. I don't understand what "each sphere on the x-line is Fcos(60∘), and the third sphere on the y-line is Fsin(60∘)" is supposed to mean.

There are two forces on the third sphere. Describe in words which way they point.
 
  • #9
What I mean is that since each of these spheres are in a position that makes up an equilateral triangle, the direction of these forces are 60 degrees north of east AND north of west. Come to think of it, when it comes to the direction of the third sphere on the top point of the triangle, if split in half one direction would be 30 degrees east of north and 30 degrees west of north (assuming the top of the triangle is in the positive y-coordinate range. The total force delivered by the third sphere on top of the triangle would be the total of the two separate force as mentioned earlier.
 
  • #10
Sorry if it seems I'm being pedantic here, but it's really hard to figure out what you mean when you use language so imprecisely. For example:
TmrK said:
What I mean is that since each of these spheres are in a position that makes up an equilateral triangle, the direction of these forces are 60 degrees north of east AND north of west.
Which forces? There are six forces in this problem, two forces on each of the three masses.
Come to think of it, when it comes to the direction of the third sphere on the top point of the triangle,
What do you mean by "direction of the third sphere"? Do you mean the direction of the forces on the third sphere?
The total force delivered by the third sphere on top of the triangle would be the total of the two separate force as mentioned earlier.
You mean the total or net force exerted on the third sphere, right? When you write "delivered by," it sounds like you're talking about the gravitational force on the other spheres due to their attraction to the third sphere.


Back to the problem, so I think what you've said is that there are two forces on the third sphere. One force — let's call it F1 — points downward and to the left, making a 30-degree angle with the y-axis, and the other force — we'll label this on F2 — points downward and to the right, making a 30-degree angle with the y-axis. So far, so good.

As you wrote in your first post, the magnitudes of the forces are
\begin{align*}
|\vec{F}_1| &= \frac{Gm_1m_3}{r_{13}^2} \\
|\vec{F}_2| &= \frac{Gm_2m_3}{r_{23}^2}
\end{align*}
where r13 = r23 = 0.550 m and m1=m2=2.85 kg.

Now you want to break these forces into horizontal and vertical components. Then using F=ma, you'll get the two equations:
\begin{align*}
\sum F_x &= F_{1_x} + F_{2_x} = m_3a_x \\
\sum F_y &= F_{1_y} + F_{2_y} = m_3a_y
\end{align*}
You need to plug in what you get for F1x, etc. One equation will let you solve for ax, and the other will let you solve for ay.
 
  • #11
So in short, I just need to find out what exactly is the magnitude of the forces before I can do anything else. But here's the problem: there is NOTHING given as to exactly on how much force there is between the spheres. That part is not given.
 
  • #12
No, that's not correct. I've essentially told you how to do the whole problem, including addressing the point you're bringing up yet again. I'll let you think about it for a while.
 
  • #13
Exactly how does m3 cancel out? And also, I realized that the force all along was G itself. Please tell me I've gone one step forward in the positive direction.
 
  • #14
TmrK said:
Exactly how does m3 cancel out?
The gravitational force on m3 is proportional to m3. Thus when you compute the acceleration of m3, the mass cancels.
And also, I realized that the force all along was G itself.
Not sure what you mean by that, since G is a constant.
 
  • #15
To find F, all I have to do is use G to replace as F, so really I'll be using G twice, yes?
 
  • #16
TmrK said:
To find F, all I have to do is use G to replace as F, so really I'll be using G twice, yes?
What do you mean by 'use G'? G is a constant that appears in the Newtonian formula for gravitational force. You cannot replace F by G. Or do you mean something else?
 
  • #17
Doc Al said:
What do you mean by 'use G'? G is a constant that appears in the Newtonian formula for gravitational force. You cannot replace F by G. Or do you mean something else?

Then if I really cannot use G again, then I would have to use all of the components to mind m3. However I can't being that there is no magnitude of the force mentioned at all. The problem alone I posted does not give me of what the magnitude of the forces are. Not one time is it even mentioned. So really, I cannot do anything if I don't have the magnitude of the force to work with.
 
  • #18
TmrK said:
Then if I really cannot use G again,
What are you talking about? G is just a constant. Whenever you calculate the gravitational force between two spheres you'll use G. So what?
then I would have to use all of the components to mind m3. However I can't being that there is no magnitude of the force mentioned at all. The problem alone I posted does not give me of what the magnitude of the forces are. Not one time is it even mentioned. So really, I cannot do anything if I don't have the magnitude of the force to work with.
You have everything needed to find the acceleration of m3. You have the mass of m1 and m2, and the distance between the spheres. You don't have a value for m3, but you don't need one.

To find the force between m1 and m3, use Newton's law of gravity. (The expression will be in terms of m3.)

To find the force between m2 and m3, use Newton's law of gravity. (The expression will be in terms of m3.)

Add up those force vectors to find the net force on m3. (The expression will be in terms of m3.)

Use Newton's 2nd law to find the acceleration of m3.
 

1. What is the formula for calculating gravitational force on three spheres?

The formula for calculating gravitational force on three spheres is F = G * (m1 * m2 * m3) / d^2, where G is the gravitational constant, m1, m2, and m3 are the masses of the three spheres, and d is the distance between the centers of the spheres.

2. How does the distance between the spheres affect the gravitational force?

The distance between the spheres has an inverse square relationship with the gravitational force. This means that as the distance increases, the force decreases and vice versa.

3. How does the mass of the spheres affect the gravitational force?

The mass of the spheres has a direct relationship with the gravitational force. This means that as the mass increases, the force also increases.

4. What is the role of the gravitational constant in calculating the force on three spheres?

The gravitational constant, denoted by G, is a constant value that helps to determine the strength of the gravitational force between objects. It is a fundamental constant in physics and its value is 6.674 x 10^-11 N*m^2/kg^2.

5. Can the gravitational force on three spheres ever be zero?

Yes, the gravitational force on three spheres can be zero if the distance between the spheres is infinite. This means that the spheres are so far apart that the force of gravity becomes negligible.

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