Iron is an ancient metal that became the basis of our civilization. It is usually used in the form of steel which contains 0.5% and 1% carbon. World steel production in 1 year equals the production of all other metals combined in 10 years. It is a transition metal, that is, it is less reactive than the typical metals but more reactive than the less-typical metals. It occurs as an alloy with nickel in meteorites.
Physical Properties
Iron exists in several allotropic forms:
α-Iron: Magnetic and stable to 768°C, crystallizes in a body-centered cubic. It dissolves very little carbon (0.025% at 721°C).
β-Iron: It is a form stable between 768°C and 910°C. It is alpha iron that has lost its magnetism. It does not dissolve carbon.
γ-Iron: This form is stable between 910°C and 1,390°C, crystallizes in face-centered cubic. It is nonmagnetic and dissolves 2% carbon at 1,102°C. Carbon in solution forms a hard carbide.
δ-Iron: It is nonmagnetic and stable between 1,391°C and the melting point...
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Habashi F et al (1997) Iron. In: Habashi F (ed) Handbook of extractive metallurgy. Wiley, Weinheim, pp 29–268
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Habashi, F. (2013). Iron, Physical and Chemical Properties. In: Kretsinger, R.H., Uversky, V.N., Permyakov, E.A. (eds) Encyclopedia of Metalloproteins. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-1533-6_417
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DOI: https://doi.org/10.1007/978-1-4614-1533-6_417
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