Deriving Orbital Motion from Collisions in Travel along Chords

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Homework Help Overview

The problem involves a body of mass m traveling along chords within a circle of radius r, reflecting perfectly upon collision. The goal is to derive the radial momentum change per collision, expressed as Δp = mvsinθ, where θ is the angle between the tangent and the chord.

Discussion Character

  • Exploratory, Assumption checking

Approaches and Questions Raised

  • Participants discuss the calculation of momentum change and question the assumptions regarding conservation of momentum in the radial direction. There is an exploration of the implications of the mass of the circle and the isolation of the system.

Discussion Status

Some participants express agreement with the derived momentum change, while others raise concerns about the assumptions made in the calculations. The discussion is ongoing, with various interpretations of the problem being explored.

Contextual Notes

Participants note that the problem lacks clarity regarding the physical properties of the circle, such as its mass and whether the system is isolated from the environment. There is also mention of a potential connection to kinetic theory of gases, suggesting a consideration of the circle's mass as effectively infinite.

LucidLunatic
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Homework Statement



Inscribe N chords of equal length within a circle of radius r. A body of mass m travels at constant speed v along the chords and is perfectly reflected in each collision with the circle (there is no momentum change tangent to the circle). Show that the radial momentum change per collision is Δp =mvsinθ, where θ is the angle between tangent and chord.

Homework Equations


Δpr = pr1-pr0

The Attempt at a Solution


We can write
p0 = mvsinθ \hat{r} + mvcosθ\hat{\theta}
p1 = -mvsinθ \hat{r} + mvcosθ\hat{\theta}

therefore Δp = -2mvsinθ.

This seems like a fairly simple problem, so I'm not sure where I'm going wrong. The later steps of this problem then show that the net centripetal force obeys F = mv^2/r as N→∞, but that depends on getting the correct answer here. What am I missing? Note: this is me going through problems in a book, not an actual homework assignment.
 
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LucidLunatic said:

Homework Statement



Inscribe N chords of equal length within a circle of radius r. A body of mass m travels at constant speed v along the chords and is perfectly reflected in each collision with the circle (there is no momentum change tangent to the circle). Show that the radial momentum change per collision is Δp =mvsinθ, where θ is the angle between tangent and chord.


Homework Equations


Δpr = pr1-pr0


The Attempt at a Solution


We can write
p0 = mvsinθ \hat{r} + mvcosθ\hat{\theta}
p1 = -mvsinθ \hat{r} + mvcosθ\hat{\theta}

therefore Δp = -2mvsinθ.

This seems like a fairly simple problem, so I'm not sure where I'm going wrong. The later steps of this problem then show that the net centripetal force obeys F = mv^2/r as N→∞, but that depends on getting the correct answer here. What am I missing? Note: this is me going through problems in a book, not an actual homework assignment.
I agree with your Δp (except the sign depends on how you care to define +ve direction), and from it I obtain F = mv2/r.
 
Dumb EE's observation:

The above calculatios (posts 1 and 2) were made under the assumption that the radial component of momentum is also conserved. But that is not stated.

Let M = mass of circle and V be its + radial velocity after collision. Then if the system is isolated form the environment (e.g. on a frictionless horizontal plane):

Assume MV = +3mv sinθ
the answer would be correct, since then for the radial direction

p1 = +mv sinθ
p2 = -mv sinθ + MV = -mv sinθ + 3mv sinθ = 2mv sinθ
so that p2 - p1 = 2mv sinθ - mv sinθ = mv sinθ.

In other words the problem has no solution unless the physical aspects of the circle are defined:

circle's mass
system isolated form the environment or not?
etc.

Comments?
 
rude man said:
Dumb EE's observation:

The above calculatios (posts 1 and 2) were made under the assumption that the radial component of momentum is also conserved. But that is not stated.

Let M = mass of circle and V be its + radial velocity after collision. Then if the system is isolated form the environment (e.g. on a frictionless horizontal plane):

Assume MV = +3mv sinθ
the answer would be correct, since then for the radial direction

p1 = +mv sinθ
p2 = -mv sinθ + MV = -mv sinθ + 3mv sinθ = 2mv sinθ
so that p2 - p1 = 2mv sinθ - mv sinθ = mv sinθ.

In other words the problem has no solution unless the physical aspects of the circle are defined:

circle's mass
system isolated form the environment or not?
etc.

Comments?
I presumed the exercise related to kinetic theory of gases, so the mass of the circle is effectively infinite.
 
haruspex said:
I presumed the exercise related to kinetic theory of gases, so the mass of the circle is effectively infinite.

I agree, that makes sense.
 

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