What Is the Orbit Radius of Two Equal-Mass Particles?

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Homework Help Overview

The discussion revolves around two equal-mass particles orbiting each other in circular orbits, focusing on determining the radius of their orbits. The context includes concepts from gravitational physics and orbital mechanics.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants explore various equations related to energy, tangential velocity, and angular momentum to find the orbit radius. There are attempts to derive relationships between parameters, including velocity and radius, while questioning the necessity of knowing specific values to solve the problem.

Discussion Status

The discussion is ongoing, with participants sharing different equations and expressing uncertainty about the correct approach. Some have proposed relationships between variables, while others emphasize the need for additional information, such as velocity, to proceed further.

Contextual Notes

There is mention of a previous thread that did not yield a resolution, indicating potential complexity in the problem. Participants are also grappling with the implications of varying parameters on the orbit radius.

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1. Two particles of equal mass are orbiting each other in circular orbits. What is the radius at which they orbit?


Energy = T + U = 0 (for circular orbits)

T = 1/2 m v^2

U = -(Gm*m)/r + [L^2] / [2(mu)r^2]

period=[2 pi r] / vt

vt is tangential velocity
L is angular momentum
mu is a constant
G is the gravitational constant
r is the radius from one particle to the center of their rotation

I have attempted to solve for R by plugging those equations in and simplifying, but I do not believe my answer is correct (it would require a lot of skill to represent it with mere type here). I must calculate the radius in order to find the time it takes for the two to collide if they were stopped in their orbits and fell towards each other. So any help calculating the velocity?
 
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I actually figured out that r = (mu tau^2 / 4pi^2)^1/3

The problem I have now is figuring out how long it takes until they collide.
 
scratch that, i have no idea. back to square one.
 
Let's go back to the first question, ok? Do you know v? Otherwise there's no answer, they could orbit at any r with appropriate v.
 
Use the centripetal force equation to get r=mG/(4v^2).
You have to know v or some other parameter to find r.
 

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