EGU Blogs

Photo of the Week #50

This week’s photo is brought to you from outer space! Indeed, this a beautiful cut section of a meteorite that fell in northwest Australia and was found in 1892 (ignore the label behind it). It is an iron-nickel meteorite and is composed entirely of metal. This crazy cross-hatching, which is most commonly found in such iron-nickel meteorites, is called a Widmanstätten pattern.

Widmanstätten patterns, also known as Thomson patterns, are revealed only when the meteorite is cut, polished and acid etched. The patterns formed when the meteorite cooled and only do so if the meteorite cooled very slowly i.e. over millions of years.

First, when the meteorite is hot the entire thing is mono-crystalline and is formed of an Fe-Ni phase called taenite. However, as a it cools another phase develops called kamacite (low Ni) which grows within the existing taneite (high Ni) lattice resulting in the Widmanstätten pattern.

Iron meteorite found in Roeburne, Hammersley Range, NW Australia. This piece is exhibited in the Museum Reich der Kristalle, Munich, Germany.by Konstantinos Kourtidis

Iron meteorite found in Roeburne, Hammersley Range, NW Australia. This piece is exhibited in the Museum Reich der Kristalle, Munich, Germany by Konstantinos Kourtidis

Matt Herod is a Ph.D Candidate in the Department of Earth Sciences at the University of Ottawa in Ontario, Canada. His research focuses on the geochemistry of iodine and the radioactive isotope iodine-129. His work involves characterizing the cycle and sources of 129I in the Canadian Arctic and applying this to long term radioactive waste disposal and the effect of Fukushima fallout. His project includes field work and lab work at the André E. Lalonde 3MV AMS Laboratory. Matt blogs about any topic in geology that interests him, and attempts to make these topics understandable to everyone. Tweets as @GeoHerod.