Hello Larry,  I was the one that put "dust bunnies" in the discussion mix 
whilst discussion space weathering color changes to meteoroids.  

I was using it generically and did not limit it to particles which were neutral 
in charge and gravitationaly emplaced. I was thinking in terms that there are 
particles that are magnetic/polarized/ionized and are buzzing about the 
asteroid on or near the surface.  I am comfortable that TC3 was not likely a 
major dust collector.

We are in further agreement that the quality of the spectral measurements have 
yet to be explained/validated publicly.  Given "chondridic pallesite" 
proclaimations by novice but "credentialed" researchers in the past I'd like to 
know that more than a few novice eyes were looking over the researchers work.

Someone asked earlier about nanodiamond formation re: Carbonaceous Chondrites.  
I wanted to point out for listeners that Urelites and some CCs already contain 
nanodiamonds and impact is not necessary for nanodiamond to be found on the 
terrain.

Elton


--- On Wed, 3/25/09, lebof...@lpl.arizona.edu <lebof...@lpl.arizona.edu> wrote:

> From: lebof...@lpl.arizona.edu <lebof...@lpl.arizona.edu>
> Subject: Re: [meteorite-list] One of the best of the 2008 TC3 articles
> To: cyna...@charter.net
> Cc: meteorite-list@meteoritecentral.com
> Date: Wednesday, March 25, 2009, 7:24 PM
> Hi everone:
> 
> As someone who has studied asteroids, this is great news.
> 
> Only two comments:
> 
> 1. I am a little concerned with the classification of the
> "asteroid" as F. The spectral range is not perfect and I wonder what the 
> uncertainty of the spectrum is (might be very poor quality at the longer 
> wavelengths).

> 2. I do not think that 2008 TC 3 was "dusty." It
> was tumbling in space and spinning once ever 50 to 100 seconds. An object 
> this size is not going to have a dusty surface!
> 
> my two cents
> 
> Larry

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