A couple questions about gravity

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Discussion Overview

The discussion revolves around the implications of gravitational force as described by the equation f=g*m1m2/d^2. Participants explore the conditions under which objects can orbit each other, become gravitationally bound, or exhibit noticeable attraction. The conversation includes theoretical considerations and practical examples, such as the gravitational interaction between binary stars and everyday objects like cars.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants express uncertainty about the meaning of calculated gravitational force and what it implies for orbital mechanics and gravitational binding.
  • There is a question about the specific force required for one object to orbit another, with a request for ballpark estimates.
  • Participants discuss the gravitational attraction between two cars in space, with differing views on whether they are massive enough to exert noticeable force on each other.
  • One participant suggests that while cars do exert a gravitational force, it may be too weak to observe without sensitive instruments.
  • Another participant proposes a criterion for visibility of gravitational attraction, suggesting that an acceleration of 0.001 m/s² could be a threshold for noticeable movement.

Areas of Agreement / Disagreement

Participants generally agree that gravitational forces exist between all masses, but there is disagreement regarding the practical implications of these forces, particularly in terms of visibility and the conditions necessary for observable attraction.

Contextual Notes

Participants acknowledge that there is no definitive answer to the questions posed about gravitational force and observable attraction, and that estimates may vary based on assumptions about mass and distance.

fezmaster
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So I understand the equation f=g*m1m2/d^2 and I understand how to use it, but I'm unsure what my results actually mean. Once I have calculated the force, I don't know what the strength implies. How much force do I need for one object to orbit another? How much is so much that the objects become 'attached' to one another (like we are to the earth)? How much is too little?

Also, if we look at binary stars, they are both attracted to each other with a similar force due to their masses. What strength is required for this to happen? If I were to put two cars in space, they certainly wouldn't be massive enough to pull at each other. But how big/close together would two objects have to be in order for this to happen?
 
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fezmaster said:
So I understand the equation f=g*m1m2/d^2 and I understand how to use it, but I'm unsure what my results actually mean. Once I have calculated the force, I don't know what the strength implies. How much force do I need for one object to orbit another? How much is so much that the objects become 'attached' to one another (like we are to the earth)? How much is too little?

Do you have a basic knowledge of second-order partial differential equations? You should probably get some before attempting to solve this.

Also, if we look at binary stars, they are both attracted to each other with a similar force due to their masses. What strength is required for this to happen? If I were to put two cars in space, they certainly wouldn't be massive enough to pull at each other. But how big/close together would two objects have to be in order for this to happen?

Same, but two cars actually are massive enough to pull at each other, just rather weakly. There's also a good chance they'll be gravitationally bound (assuming that's what you mean.)
 
I believe that I understand it... Unless there's something fundamental that I'm missing, but I'm not sure what that would be. I just wondered how much force is required for one object to orbit another. I understand that there's no set answer to this question, but I was just hoping for some sort of ballpark estimate.

And I do understand that the cars would pull at each other with a little amount of force. I'm just unsure how much force would be enough that you could actually observe them being mutually attracted towards each other.
 
fezmaster said:
If I were to put two cars in space, they certainly wouldn't be massive enough to pull at each other.

That's not true. The equation which you already know tells you the force of attraction between them. Perhaps you mean that a person could spend a long time watching them and not notice their acceleration toward one another. That's just a matter of being able to notice movement. The hour hand of a clock is moving but it doesn't look like it.
 
mikelepore said:
That's not true. The equation which you already know tells you the force of attraction between them. Perhaps you mean that a person could spend a long time watching them and not notice their acceleration toward one another. That's just a matter of being able to notice movement. The hour hand of a clock is moving but it doesn't look like it.
Yes, I made an error when I wrote it out. I meant visibly pull at each other (just with our eyes)
 
As for what is noticably visible, maybe we can estimate that it's just barely visible if, during a period of time of one second, an object goes from being at rest to having a speed of 1 millimeter per second. If so, that would be an acceleration of a=0.001 m/s^2. Whatever "a" you want to use, solve F=ma to get the necessary values of force and mass.
 

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