Primary and Secondary Structures - Meteorites
New England Meteoritical Services


 

Comb plessite

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Meteorite - Carbo, IID Iron
Plessite is a fine-grained mixture of kamacite and taenite, often containing minor amounts of schreibersite and tetrataenite. Rather than being a simple mineral, plessite is a complex term describing the diverse structural patterns that frequently form between kamacite and taenite lamellae. This two-phase mixture represents the final stage of development from retained taenite during the primary cooling process.

Plessite fields are visually striking and are typically bordered by a continuous taenite rim. Larger plessitic fields, known as comb plessites, develop under extremely slow primary cooling conditions and exhibit a distinctive structure resembling the teeth of a comb.

The Carbo meteorite, classified as a IID iron, provides an example of this phenomenon. Its primary cooling rate is estimated to have been between 10°C and 20°C per million years. In this context, plessitic fields are regarded as secondary structures, with their alignment closely tied to the host Widmanstätten pattern.

 
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Figure 1. Scale bar 900 µm.
 
Comb plessite, Carbo, Iron, IID.
 
 
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