Optical microscopy, transmission electron microscopy, and electron diffract
ion were used to study the structural state of a coarse (type IIB) Sikhote
Alin octahedrite. During its destruction in the atmosphere and after fallin
g to the Earth, the Sikhote Alin meteorite underwent an impact. Traces of d
eformation such as uniformly distributed dislocations, dislocation loops, c
ellular dislocation substructure, Neumann bands, deformation microtwins, lo
calized shear bands, fine fragmented structure, serrated boundaries of micr
ofragments, broken branching dislocation boundaries, and microcracks were f
ound in the meteorite microstructure. The formation of these defects in the
meteorite samples depends on the intensity of impact action. No traces of
the reversible alpha --> epsilon --> alpha phase transformation were found
in the microstructure of the meteorite samples. Upon the shock loading duri
ng the fall, the pressure affecting the Sikhote Alin meteorite did not exce
ed 12 GPa. The degree of true local deformation could reach 4-5. Fine oxide
and hydroxide precipitates caused by the oxidizing action of atmosphere du
ring a long period of the meteorite exposure at the Earth surface were foun
d in the surface layers of the meteorite material.