Distance from sun to earth= 1.5 x10^11m

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SUMMARY

The discussion focuses on calculating the point between Earth and the Sun where the gravitational forces exerted by both bodies on an object are equal, resulting in a net gravitational force of zero. The masses used are Me = 5.98 x 1024 kg for Earth and Ms = 2 x 1030 kg for the Sun, with a distance of 1.5 x 1011 m between them. The user attempted to solve the problem using the gravitational force equation F = Gm1m2/r2 but arrived at an incorrect distance of 1.49 x 1011 m, indicating a misunderstanding of the problem's requirements.

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Littlemin5
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Please help!

1. Homework Statement
Find the point between Earth and the Sun at which an object an be placed so that the net gravitatinal force exerted by Earth an the sun on this object is zero.

Me=5.98 x 10^24kg
Ms=2 x 10^30kg
Distance from sun to earth= 1.5 x10^11m

2. Homework Equations

F=Gm1m2/r^2 --> not sure if this is right?

3. The Attempt at a Solution

So I tried to manipulate the situation and thought I could do:
When x equals the distance from the sun.

(G(Ms)) / x^2 = (G(Me))/ (d-x)^2

When I plugged in the numbers though I got 1.49x10^11m as my answer. I don't feel like this is right because it's pretty much the full distance between them. Is this not the way to do it, and if not how do I go about doig this problem?
 
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I have not done this one in a while, but I believe that you may need to take the radii of the bodies into account. Since in that formula for Gravitational force, r is the distance between the centers.
 

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