Pallasites
Modern meteoriticists use the term "pallasite" to describe a
certain structural class of stony-iron meteorites that contains abundant
silicate inclusions in a nickel-iron matrix. Usually, the silicates are
large olivine crystals, often of gem quality. These peridots make the
pallasites some of the most attractive meteorites known, and cut and
polished pallasite slices are highly coveted among meteorite collectors.
Sometimes pallasites and pallasitic peridots are used in jewelry, making
them the only genuine cosmic gemstones on Earth.
Based on their origin and formation history, the pallasites are
regarded as samples of core/mantle boundary material from differentiated
asteroids, inferring that a close relationship exists to the iron
meteorites. Upon etching, larger metal portions of polished slices display
typical Widmanstätten figures. In addition to this, pallasites display
chemical, elemental, and isotopic trends that link them to specific
chemical groups of iron meteorites, linking their origin to a common
parent body. Hence, they are classified into three distinct groups or
grouplets, similar to the chemical groups of the iron meteorites: (1) the
main group pallasites, (2) the Eagle Station grouplet, and (3) the
pyroxene grouplet.
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Imilac
Found in 1822 in Chile
TKW 920 Kg
Main group pallasite
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Imilac 01
translucent slice with crust
27gr
SOLD
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Imilac 02
slice with crust
36.27gr
SOLD
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Imilac 03
end cut with fresh exterior
36.87gr
SOLD
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Imilac 04
perfect complete individual
27.41gr
$550
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Imilac 05
individual with open window
20.50gr
$350
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Imilac 06
perfect quality thin slice
6.87gr
SOLD
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Imilac 07
perfect quality thin slice
9.7gr
Sold
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Imilac 08
perfect quality thin slice
10.37gr
SOLD
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