Primary and Secondary Structures - Meteorites
New England Meteoritical Services


 

Cloudy taenite-rimmed plessite and kamacite

Listing of Structures
Back...Next
Meteorite, Grant, IIIAB, Iron

 
{short description of image}

 
Figure 1. Scale bar 1.2 mm.
Meteorite, Grant, IIIAB Iron
 

Cloudy taenite is a high-nickel (Ni), secondary structure found in iron meteorites, distinguished by its unique appearance and composition. It emerges after the initial crystallization of primary metallic phases, forming through the gradual diffusion of nickel and iron atoms. This slow process creates fine intergrowths of taenite with another Ni-rich phase, often tetrataenite (containing 49% to 57% Ni, sometimes referred to as "clear" taenite). The result is a submicroscopic, two-phase mixture that gives cloudy taenite its characteristic "cloudy" texture, typically with a nickel content of 30% to 40%.

Taenite rims, enriched in high-Ni tetrataenite, can also develop around existing structures like kamacite lamellae or plessite fields. These rims form through nucleation and growth during the slow cooling of the meteorite, driven by the differing stabilities of iron-nickel phases at various temperatures. In prepared specimens, such as those of the Grant meteorite, these rims often appear as bright metallic borders encircling plessitic fields and kamacite, highlighting the presence of tetrataenite.

 
 
Listing of Structures