Liouville's Eq. applied to debris in space

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Discussion Overview

The discussion centers on the application of Liouville's Equation to calculate the probability of collisions between spacecraft and debris fragments in space. Participants explore the potential of using initial states of debris to determine phase space density functions and predict the density of debris in real space over time, focusing on gravitational accelerations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests using Liouville's Equation to model the probability of collisions with space debris, questioning if this approach has been previously explored or if there are reasons it may not be viable.
  • Another participant references a book on mathematically modeling space debris but notes it does not mention Liouville's Equation or phase-space evolution.
  • A different participant expresses interest in the referenced book but highlights their focus on short-lived debris, which may differ from the more evenly dispersed orbital debris, suggesting that the proposed approach might be more applicable in their context.
  • One participant posts a message to increase visibility of the thread, indicating a desire for more engagement on the topic.

Areas of Agreement / Disagreement

Participants have not reached a consensus on the viability of using Liouville's Equation for this application. There are differing views on the relevance of existing literature and the applicability of the approach to different types of debris.

Contextual Notes

There are limitations regarding the assumptions made about the types of debris being considered, particularly the differences between short-lived debris and orbital debris. The discussion also reflects uncertainty about prior work in this area.

Who May Find This Useful

Researchers and practitioners interested in space debris modeling, collision probability assessments, and the application of Liouville's Equation in astrophysical contexts may find this discussion relevant.

belliott4488
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A colleague of mine has suggested using Liouville's Equation in order to calculate the probability of collision between spacecraft and debris fragments produced by collisions in space. The application would be to take the known initial states of all the debris fragments, to determine the phase space density function, and then to propagate that using Liouville's Eq. Our hope is that we could use this to predict the density of debris fragments in real space as a function of time this way. We are considering only gravitational accelerations right now.

If this approach makes sense, it would surprise me that it hasn't been done before. Does anyone know of any work that has been done along these lines? Or, is there a reason why such an approach will not work?
 
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jackiefrost said:
Here's an interesting book dealing with mathematically modeling space debris, though there is no mention of using Liouville or evolution in phase-space -http://books.google.com/books?hl=en...LWqE&sig=8E3yf9yJyvTnYlsZaCTbl02-1O0#PPP1,M1"
Thanks - that looks like a book I should probably have on my shelf.

On a cursory look, however, it appears to deal with the big issue in this area, i.e. orbital debris. As it happens, I am in the business of looking at debris that is very short-lived, i.e. with less than orbital velocities. That is part of the reason I think this approach might work, even if it might not in the case of orbital debris, which is dispersed more evenly.
 
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Sorry, this is just to bump this thread back up, since I posted it late Friday afternoon, so it's probably been buried by Monday AM, and I wanted to be sure people who browse the forums during working hours see it ...
 

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