Hi Carl-

For the most part, breakup characteristics don't correlate well with either size or material. I think it's largely a matter of the bulk properties of the meteoroid- how monolithic versus faulted it is- and any material can exist on a wide range between those extremes.

For the most part, I'd say if there's any "sweet-spot", it is largely determined by the same factors that have been seen as key for a long time- a shallow entry angle, low entry speed, and low altitude terminal explosion all bode well for meteorite production. Of course, larger bodies have more material, and might well be expected to yield more meteorites under equivalent entry conditions. But that's a very broad generalization. I think that the nature of the terminal explosion of Chelyabinsk resulted in such tiny fragmentation that something in excess of 99% of the initial mass was lost. A somewhat stronger body of the same size might have survived a little longer, slowing enough that the disruption would be less violent, and a lot more could survive. Consider that Sikhote-Alin was a smaller body, but much more material survived to the ground- both because it was materially stronger, and because it didn't explode until it was much lower.

Chris

*******************************
Chris L Peterson
Cloudbait Observatory
http://www.cloudbait.com

On 2/27/2013 10:42 AM, Carl Agee wrote:
Hi Chris,

Do you have any references you could point me to for how break-up
scales with size-mass-physical properties etc. of meteoroids. I am
interested in knowing the "sweet-spot" for yielding meteorites on the
ground. In other words, when is a meteoroid too small or too big to
produce significant large pieces of surviving material? It seems like
Chelyabinsk is outside the sweet spot as it apparently produced mostly
fragments even though it had large mass. On the other hand much bigger
masses may also survive. Is it bimodal?

Thanks,

Carl Agee


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