NEA 051 Iron Meteorite - 70.0g - Stunning Pattern - From The Core Of An Asteroid!

Presented here is a genuine specimen of NEA 051, a recently classified IIIAB iron meteorite recovered from the deserts of Libya. This extraordinary extraterrestrial metal represents a fragment of an ancient planetary body that formed during the earliest history of our Solar System, more than 4.5 billion years ago. 

IIIAB irons are valued by collectors and researchers for their distinctive metallic structure and importance in understanding the formation and evolution of asteroid cores.  When cut and professionally prepared, NEA 051 reveals the classic crystalline architecture expected from iron meteorites, including a striking Widmanstätten pattern — the interlocking growth structure of kamacite and taenite crystals formed during extremely slow cooling inside its parent asteroid.

Friendly Reminder: iron meteorites are going to exhibit signs of rust.  It’s solid nickel/iron! This is a normal occurrence with iron meteorites. At some point in its life with you, it will need to be cared for.  Please see our care guide on our FAQ for further details on how to keep rust at bay.  Remember, you can always send the meteorite back to us at any time you feel necessary and we will re-stabilize the stone and bring it back to perfection, which is at a minimum cost ($30-$50 depending upon the size of the stone). 

About Iron Meteorites:

Iron meteorites consist almost entirely of nickel and iron and are thought to originate from the cores of ancient, differentiated asteroids. In the early solar system, these large asteroids underwent internal melting, causing heavier elements like iron and nickel to sink toward their centers—much like the Earth’s own core. Over time, catastrophic collisions shattered these bodies, sending fragments hurtling through space until some eventually landed on Earth as meteorites.

One of the most striking features of iron meteorites is the Widmanstätten pattern—a distinctive interlocking crystalline structure of nickel-iron alloys that can be revealed through careful acid etching. This process requires expert preparation, including stabilization, slicing, and polishing, as even slight errors can damage the specimen. The pattern itself is often called the meteorite’s “thumbprint” because it is entirely unique and cannot be replicated in laboratory conditions. Its formation requires incredibly slow cooling—about one degree Celsius every 10,000 years—making it a visual testament to the vast timescales and processes that shaped our solar system.