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Re: Equilibrated vs. Unequilibrated
- To: meteorite-list@meteoritecentral.com
- Subject: Re: Equilibrated vs. Unequilibrated
- From: Jeff Grossman <jgrossman@usgs.gov>
- Date: Thu, 25 Jun 1998 06:58:49 -0400
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- Resent-Date: Thu, 25 Jun 1998 08:03:14 -0400 (EDT)
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At 11:53 PM 6/24/98 EDT, you wrote:
>Hello Everyone,
>
>The May, 1998 issue of Meteorite! defines the above terms in the Ask the
>Geologist section but I must admit, after (re)reading it, I still have a hard
>grasping the concept as applied to meteorites (sorry Joel). Would someone
>more enlightened than myself please explain this using meteoritical examples?
>
>-Walter
>
Here's how these terms apply to chondrites. They refer to the effects
of thermal metamorphism (regardless of what causes it).
* Equilibrated chondrites generally have olivine, (Fe,Mg)2SiO4, that
is all one composition. Operationally, we define this as the standard
deviation of the Fe/(Fe+Mg) ratios of many olivine grains being less
than 5% relative. We believe that most chondrites started out with
more heteorogeneous olivine compositions, and that thermal metamorphism
caused diffusional Fe-Mg exchange between the grains until an
"equilibrium" value was attained. Chondrites with larger sigmas are
called "unequilibrated." H chondrites equilibrate to a different
Fe/(Fe+Mg) ratio in olivine and pyroxene than do L (and LL) chondrites,
which led to the old terms "bronzite-olivine chondrite" and "olivine-
hypersthene chondrite" for H and L. Highly unequilibrated ordinary
chondrites like Sharps (H3.4) and Chainpur (LL3.4) are hard to tell
apart by their mineralogy, since both have really wide ranges of
mineral compositions.
* Pyroxene does the same sort of thing as olivine, except that diffusion
is slower in this mineral, and equilibration may be incomplete
even in meteorites with fairly homogeneous olivine.
* Thermally metamorphosed meteorites may also have more "equilibrated"
textures. Extensive thermal annealing tends to coarsen grain-sizes, leading
to a blurring of chondrule outlines and the disappearance of fine-grained
matrix in high-petrologic type chondrites. A fully equilibrated
texture would have equant olivine and pyroxene grains meeting at 120-degree
triple-junctions (like the way tiled hexagons do). Textures like that
are generally only seen in primitive achondrites (closely related
to chondrites).
Most ordinary, enstatite, and R chondrites are "equilibrated" with respect
to olivine and pyroxene compositions. ~5% are unequilibrated.
Most carbonaceous chondrites are "unequilibrated." Only the rare
CK group has a significant number of metamorphosed members.
jeff