Finding Balancing Point Between Earth and Sun

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SUMMARY

The discussion focuses on calculating the gravitational balance point between Earth and the Sun, utilizing Newton's law of gravitation. The masses involved 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 correct approach involves setting up the equation F = Gm1m2/r2 and solving for the distance from the Sun, leading to the conclusion that the balance point is approximately 1.49 x 1011 m from the Sun, indicating that the object must be significantly closer to the Sun than to Earth.

PREREQUISITES
  • Understanding of Newton's law of gravitation
  • Familiarity with gravitational force equations (F = Gm1m2/r2)
  • Basic knowledge of mass and distance measurements in astrophysics
  • Concept of gravitational dominance in celestial mechanics
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  • Learn about the implications of mass ratios in gravitational interactions
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Astronomy students, physics enthusiasts, and anyone interested in gravitational dynamics and celestial mechanics will benefit from this discussion.

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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

Homework Equations



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

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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Newton's law of gravitation is certainly right ;-)

Your method looks fine to me. Think about it intuitively. The sun is ridiculously huge, right? In fact, the sun is SO much more massive than anything else in the solar system, that it plays a dominant role over all of the gravitational interactions that occur. In this case, that means that your object has to be MOST of the way along the distance from the sun to the Earth before Earth's gravity starts to dominate. I mean, I think you can see from your numbers exactly how this result came about. The sun is more massive by six orders of magnitude (a factor of a million!)

Keep in mind also that the distance of the object from the Earth (1.5 - 1.49 hundred billion) is nothing to sneeze at (in human terms).

0.01 x 10^11 m = 10^9 m = 10^6 km

So out of the 150 million kilometres distance from here to the sun, the object has to travel a million kilometres away from Earth before the sun's gravity begins to dominate. That may only be a fraction of the distance to the sun, but it's still a million kilometres.
 
Last edited:


When you explain it like that then my answer makes more sense. Thanks so much though for clearing that all up!
 

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