--- On Thu, 8/14/08, mckinney trammell <[EMAIL PROTECTED]> wrote: vaca muerta 
eucrite--can anyone give any scientific info on this + pix? 

Here are the basic points.

All known mesosiderites come from a common parent/daughter which was a 
Vesta-like differentiated asteroid(having eucrite and diogenite material and 
possibly iron core (e.g Crust-Mantle-Core)  Since howardites are 
eucrite/diogenite/plus mixes some portion of regolith is likely incorporated in 
the overall petrology but too small for us to recognize as such.

This body was extensively disrupted by collision(s) which greatly mixed the 
strata: either a Vesta-like asteroid and it's a metallic core AND/OR some other 
massive iron body. 

A massive portion (if not the entire body) was essentially turned into 
something akin to an Impact Melt Breccia(IMB) but with achondrite materials.

On petrological study of Vaca Mutera specifically, what is commonly referred to 
as "eucrite" nodules are a wide ranging mix of eucrite and diogenite 
composition. They do NOT represent a different fall or named meteorite.

Owing to differential weathering: iron weathering faster than silicate, the 
clasts of "eucrite" character have been recovered as nodules in the VM strewn 
field.  They are also seen in sawed sections contained in classic meso 
"iron/silicate" masses. I don' have any statistcs or percentages but my swag is 
that they are probably less than 3-5% of this meteorite and would be rated as 
uncommon to rare. Perhaps others have better data.

I don't have a photo available but on a macro level the ones I have are fairly 
unremarkable; looking much like any other suspected meteorite: dark walnut-like 
without true fusion crust. I have been told that because of the random mix, 
their interiors contain a wide range of crystalline textures.

Regards,
Elton











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