Interstitial compound
An interstitial compound, or interstitial alloy, is a compound that is formed when an atom with a small enough radius sits in an interstitial “hole” in a metal lattice. Examples of small atoms are hydrogen, boron, carbon and nitrogen. The compounds are industrially important. They are neither typically ionic nor covalent. History. The idea of interstitial compounds was started in the late 1930s and they are often called Hagg phases after Hägg. Transition metals generally crystallise in either the hexagonal close packed or face centered cubic structures, both of which can be considered to be made up of  layers of hexagonally close packed atoms. In both of these very similar lattices there are two sorts of interstice, or hole: It was suggested by early workers that: These were not viewed as compounds, but rather as solutions, of say carbon, in the metal lattice, with a limiting upper “concentration” of the smaller atom that was determined by the number of interstices available. Current. A more detailed knowledge of the structures of metals, and binary and ternary phases of metals and non metals shows that: One example is the solubility of carbon in iron. The form of pure iron stable  between 910 °C and 1390 °C, γ-iron, forms a solid solution with carbon termed austenite which is also known as steel.