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Re: Building the Solar System: A look at element classification.
Hello to everyone on this list! I have been gone a while, so let
me introduce myself to those new to the list. My name is Frank Stroik,
and I am at the University of Wyoming Geological Museum, and Department of
Geology and Geophysics. I am student/researcher, studying Geochemistry,
and Petrology.
I would like to discuss what makes up meteorites, Planets,
Asteroids, Comets, Moons, and space dust. All the above planetary bodies
are made up of elements, as we all know, but what properties do these
elements have, and why are they found the way they are.
This answer will provide insight into why Chondrites for example, are
composed of
primarly two minerals, Pyroxene, and Olivine, and not, say, Quartz, or
Corundum. Also we begin to understand why elements become distributed in
planetary bodies, and why they bond to each other in certain ways.
It is my hope that we will be able to start a journey that never
ends, one that leads us closer to understanding the Solar System we
inhabit, and the Universe it is in. I will post additions to this line of
thought periodicaly throughout the next few weeks, in hopes that you
will learn and be enlightened by learning how to build a Solar System,
from the smallest elements, to the largest Jovian planets.
Let us begin by looking at Goldschmidts classification of
elements. V.M. Goldschmidt was a geochemist from the early 1920's who
became interested in why elemements work the way they do in nature. He
was, in my view, the founder of the science of geochemistry, and
cosmochemistry. He describes geochemistry as thus: " The primary purpose
of geochemistry is on the one hand to determine quantitatively the
composition of the Earth and it's parts, and on the other to discover the
laws which control the distribution of the individual elements. To solve
these problems, the geochemist requires a comprehensive collection of
anaylitical data on terrestrial materials,such as rocks, waters, and the
atmosphere; he also uses meteorites, astrophysical data on the
composition of other cosmic bodies, and geophysical data on the nature of
the Earth's interior" (Mason 1958).
From the above concepts he developed a classification system to
define the elements, and put them into perspective from a scientific
point of view. The basic concept is this: elements want to bond in
certain manners which can be predicted. From this ability to predict the
arrangements of elements, we can see how elements are arranged, and thus
provide us with a window into what type of environment the specimen in
hand formed. It is important to know these patterns, as it will help you
understand why meteorites are the way they are, and what the environment
was like in which they formed.
Goldschmidt postulated that the three main phases of meteorites
Stone, Stony iron, and Iron represent the differentiation of the Earth
(Brownlow 1979). In doing this he began to realize that meteorites can be
used as primary models to help explain the geochemical behavior of
elements on all planetary bodies. It must be said, that this
classification is excellent in allowing to us to predict the what
elements will be found where, it is not a useful tool to define environments
of formation in the absolute, rather it guides us in our thinking about
the larger picture of Solar System composition.
The classification is as follows:
1. Siderophile(Metal Loving) Elements: Those elements that tend to
concentrate in metallic iron, such as Ni,and Co.
2. Chalcophile(Sulfur loving) Elements: These tend to concentrate in
sulfide phases such as troilite in iron meteorites. Examples are Zn, and Cd.
3.Lithophile(rock loving) Elements: These elements tend to concentrate in
silcate materials(igneous rocks, meteorites ect.). Some examples are, Na,
K, and Ca.
4. Atmophile(gas loving) Elements: These tend to be found in our
atmosphere such as N and Ar.
Above based on Henderson(1982 pp 76).
The above gives us a foundation to build our understanding of the
Solar System, and allows us to expect certain elements to availible in
certain portions of meteorites, and the Earth. We have seen a pattern
formed, we must now decipher it. Here we will stop, as I will prepare the
next piece of the puzzle to present to you. Below I have constructed a
rough chart that shows siderophile, chalcophile, lithophile, and
atmophile elements. If there are questions please let me know.
Siderophile Chalcophile Lithophile Atmophile
C,P,Fe,Co Cr, S, Mn, Si, Mg, Na H, C, N,
Ni,Ge,Ir Ag, Zn, Se K, Ca, Cl O, I, Br
References:
Brownlow, Aurthur H. Geochemistry. Prentice Hall Inc Englewood
Cliffs NJ, 498 pp, 1979
Henderson, Paul. Inorganic Geochemistry. Pergammon Press 353 pp,1982
Mason, Brian. Principles of Geochemistry. John Wiley & Sons,
INC, New York. 310pp, 1958
Frank Stroik
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