Primary and Secondary Structures - Meteorites
New England Meteoritical Services


 

Mosaic aggregates in a hexahedrite

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Meteorite - Santo Antônio do Descoberto, IIAB Iron
 
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Figure 1. Scale bar 150 µm.
Meteorite - Santo Antônio do Descoberto, IIAB Iron
Irregular troilite, daubreelite and metal mosaic aggregates. Note the abundance of Neumann lines.

Hexahedrites are a category of iron meteorites with low nickel content, primarily made up of the nickel-iron alloy kamacite. Compared to octahedrites, they contain less nickel, with concentrations typically below 5.8% and seldom dropping under 5.3%. Their name derives from the cubic (hexahedron) shape of the kamacite crystals.

Unlike octahedrites, hexahedrites lack a Widmanstätten pattern. Instead, they often exhibit Neumann lines, which are signs of impact shock that occurred after the initial cooling of the taenite-kamacite mix.

The mosaic aggregates found in hexahedrites emerge from rapid cooling and reheating events experienced during their journey through space and entry into Earth’s atmosphere. These aggregates are composed of irregularly shaped kamacite grains, oriented in different directions, giving them a mosaic-like texture.

Their structure forms through a transformation process: alpha-iron shifts to gamma-iron and then reverts to alpha-iron when heated above 750°C, followed by swift cooling. These features are considered secondary structures.
 
 
 
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Figure 2. Scale bar 100 µm.
Meteorite - Santo Antônio do Descoberto, IIAB iron
Mosaic aggregates.
 
 
 
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Figure 3. Scale bar 30 µ.
Meteorite - Santo Antônio do Descoberto, IIAB iron
Irregular troilite, daubreelite and metal mosaic aggregates.
 
 
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