Gravitational force of the Sun and Earth

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SUMMARY

The discussion focuses on calculating the gravitational force balance point between the Earth and the Sun, located at a distance R from the center of the Earth. The gravitational force is defined by the equation F = (G * m1 * m2) / R², where G is the gravitational constant, m1 is the mass of the Earth, and m2 is the mass of the Sun. Participants clarify that the distance R must be substituted into the equation to find the point where the gravitational forces from both bodies are equal. The correct approach involves setting up the equation with R and solving for it using algebraic methods.

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  • Understanding of gravitational force calculations using Newton's law of universal gravitation.
  • Familiarity with algebraic manipulation and solving quadratic equations.
  • Knowledge of the gravitational constant (G) and its significance in physics.
  • Basic understanding of the mass of celestial bodies, specifically the Earth and the Sun.
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  • Learn how to solve quadratic equations in physics contexts.
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  • Investigate the implications of gravitational forces in orbital mechanics.
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This discussion is beneficial for physics students, educators, and anyone interested in celestial mechanics and gravitational interactions between astronomical bodies.

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Homework Statement


Earth orbits around the sun at roughly 1.5x1011 m. Mass of Earth is 6x1024 kg. Mass of sun is 1.98892x1030 kg.

There is a point between the sun and the Earth at which the gravitational force by the sun equals that of Earth and the forces cancel each other out. How far is this point from the center of the earth? You will get a quadratic equation.


Homework Equations


I know the force between two bodies is calculated using F=(G*m1*m2)/R2


The Attempt at a Solution



Based on the above equation, I thought that this problem would be solved by setting that equation equal to itself. Basically F=F but with the R on the right side as an unknown, then solve for that R. but obviously this results in everything else cancelling out and the R I am left with is equal to the distance between the sun and the Earth (1.5x1011 m).
So I'm confused, I'm not sure what to do...
 
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This is an exercise in algebra more than anything else.
This magical point is at a distance R from the centre of the Earth and therefore at a distance of 1.5 x 10^11 - R from the centre of the sun.
Stick these in as your r^2 distances in the equation and you will get an equation that can be solved !
 
Last edited:
thank you very much. so does this mean my equation would be F=(G*m1*m2)/(1.5x1011 - R2) ? or is it [(G*m1*m2)/R2] = [(G*m1*m2)/(1.5x1011 - R2)

i having trouble figuring this out for some reason...
 

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