Universal gravitation previous exam problem

In summary, the conversation is discussing a problem with understanding the gravity equation and determining the separation between two objects. The expert provides clarification on the meaning of "r" in the equation and gives examples to help the student understand. They also mention a potential mistake in the student's approach to finding the answer.
  • #1
Mikecarlson
3
0

Homework Statement


I'm having trouble with this problem attached. Any help would be appreciated.


Homework Equations





The Attempt at a Solution

 

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  • #2
You have the basic idea - but the r in the gravity equation is the separation between the two objects, not their distance from the origin.

So if one object is at x1=4m from the origin, and the other is at x2=6m, in the same direction, then how far apart are they?
if one is at x1=4m and the other at x2=x, in the same direction, then how far apart are they?
 
  • #3
Simon Bridge said:
You have the basic idea - but the r in the gravity equation is the separation between the two objects, not their distance from the origin.

So if one object is at x1=4m from the origin, and the other is at x2=6m, in the same direction, then how far apart are they? 2m
if one is at x1=4m and the other at x2=x, in the same direction, then how far apart are they?x-4

So, are you saying object 1 and two are not 4 units apart?
 
  • #4
The answer key has an answer of 4.98M. I have tried a few different ways to get that answer and have yet to figure it out. can you tell me if that answer is actually correct?

Thanks
 
  • #5
Objects 1 and 2 are 4 units apart - that that's not the only separation that counts.
What is the separation between object 3 and 2?

The secret is to write the whole thing out in symbolic form first - then simplify the equation.
 
  • #6
There is something else to worry about: you write an expression for |F| which is correct, but then you work it out to |F|+|F|=0 and there is a little thing you missed there.

The numerical value you found somewhere is totally unimportant, but correct.
 

Related to Universal gravitation previous exam problem

1. What is universal gravitation?

Universal gravitation is a fundamental force of nature that describes the attraction between all objects with mass in the universe. It is responsible for the movement of planets, stars, and galaxies.

2. Who discovered universal gravitation?

Sir Isaac Newton is credited with discovering universal gravitation in the 17th century. He developed the theory of gravity and published his findings in his famous work, "Principia Mathematica."

3. How does universal gravitation work?

Universal gravitation states that every object in the universe attracts every other object with a force that is directly proportional to their masses and inversely proportional to the square of the distance between them. This means that the larger the mass of an object, the stronger its gravitational pull will be.

4. What is the formula for universal gravitation?

The formula for universal gravitation is F = G (m1m2)/r^2, where F is the force of gravity, G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between them.

5. How does universal gravitation relate to orbits?

Universal gravitation is responsible for the orbits of planets around the sun and moons around planets. The gravitational force between the two objects keeps them in orbit and maintains their stability.

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