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[[File:Pure iron phase diagram (EN).svg|thumb|right|400px|Low-pressure [[phase diagram]] of pure iron.]]
[[File:Pure iron phase diagram (EN).svg|thumb|right|400px|Low-pressure [[phase diagram]] of pure iron.]]
[[File:Steel pd.svg|thumb|right|340px|Iron-carbon [[eutectic system|euctectic]] phase diagram, showing various forms of Fe<sub>x</sub>C<sub>y</sub> substances.]]
[[File:Steel pd.svg|thumb|right|340px|Iron-carbon [[eutectic system|eutectic]] phase diagram, showing various forms of Fe<sub>x</sub>C<sub>y</sub> substances.]]





Revision as of 21:21, 9 February 2012

Low-pressure phase diagram of pure iron.
Iron-carbon eutectic phase diagram, showing various forms of FexCy substances.


Iron represents perhaps the best-known example for allotropy in a metal. At atmospheric pressure, there are three allotropic forms of iron: [[ferrite (iron) | alpha iron (α) a.k.a. ferrite, gamma iron (γ) a.k.a. austenite, and delta iron (δ). At very high pressure, a fourth form exists, called epsilon iron (ε) hexaferrum. Some controversial experimental evidence exists for another high-pressure form that is stable at very high pressures and temperatures.[1]

The phases of iron at atmospheric pressure are important because of the differences in soluability of carbon, forming different types of steel. The high-pressure phases of iron are important as models for the solid parts of planetary cores. The inner core of the Earth is generally assumed to consist essentially of a crystaline iron-nickel alloy with ε structure.[2][3][4] The outer core surrounding the solid inner core is believed to be composed of liquid iron mixed with nickel and trace amounts of lighter elements.


Standard pressure allotropes

Delta iron (δ-Fe)

As molten iron cools down, it crystallizes at 1,538 °C (2,800 °F) into its δ allotrope, which has a body-centered cubic (BCC) crystal structure.[5]

Gamma iron / Austenite(γ-Fe)

As the iron cools further to 1,394 °C its crystal structure changes to a face centered cubic (FCC) crystaline structure. In this form it is called gamma iron (γ-Fe) or Austenite. γ-iron can dissolve considerably more carbon (as much as 2.04% by mass at 1,146°C). This γ form of carbon saturation is exhibited in stainless steel.

Beta iron (β-Fe)

Beta ferrite (β-Fe) and beta iron (β-iron) are obsolete terms for the paramagnetic form of ferrite (α-Fe).[6][7] The primary phase of low-carbon or mild steel and most cast irons at room temperature is ferromagnetic ferrite (α-Fe). As iron or ferritic steel is heated above the critical temperature A2 or Curie temperature of 771°C (1044K or 1420°F),[8] the random thermal agitation of the atoms exceeds the oriented magnetic moment of the unpaired electron spins in the 3d shell.[9] The A2 forms the low-temperature boundary of the beta iron field in the phase diagram in Figure 1. Beta ferrite is crystallographically identical to alpha ferrite, except for magnetic domains and the expanded body-centered cubic lattice parameter as a function of temperature, and is therefore of only minor importance in steel heat treating. For this reason, the beta “phase” is not usually considered a distinct phase but merely the high-temperature end of the alpha phase field.


Alpha iron / Ferrite (α-Fe)

At 912 °C (1,674 °F) the crystal structure again becomes BCC as α-iron is formed. The substance assumes a paramagnetic property. α-iron can dissolve only a small concentration of carbon (no more than 0.021% by mass at 910 °C).

at 770 °C (1,418 °F), the Curie point (TC), the iron is a fairly soft metal and becomes ferromagnetic. As the iron passes through the Curie temperature there is no change in crystalline structure, but there is a change in the magnetic properties as the magnetic domains become aligned. This is the stable form of iron at room temperature.

High pressure allotropes

Epsilon iron / Hexaferrum (ε-Fe)

At pressures above approximately 10 GPa and temperatures of a few hundred kelvin or less, α-iron changes into a hexagonal close-packed (hcp) structure, which is also known as ε-iron or hexaferrum.[10]; the higher-temperature γ-phase also changes into ε-iron, but does so at a higher pressure. Antiferromagnetism in alloys of epsilon-Fe with Mn, Os and Ru has been observed.[11]

Experimental high temperature and pressure

An alternate stable form, if it exists, may appear at pressures of at least 50 GPa and temperatures of at least 1,500 K; it has been thought to have an orthorhombic or a double hcp structure.[1] as of December 2011, recent and ongoing experiments are being conducted on high-pressure and Superdense carbon allotropes.

See also

References

  1. ^ a b Boehler, Reinhard (2000). "High-pressure experiments and the phase diagram of lower mantle and core materials". Review of Geophysics. 38. American Geophysical Union: 221–245. Bibcode:2000RvGeo..38..221B. doi:10.1029/1998RG000053.
  2. ^ Cohen, Ronald. "Crystal at the Center of the Earth". Retrieved 2007-02-05. {{cite web}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  3. ^ Lars Stixrude and R. E. Cohen, "High-Pressure Elasticity of Iron and Anisotropy of Earth's Inner Core", Science 31 March 1995: Vol. 267. no. 5206, pp. 1972 - 1975 DOI: 10.1126/science.267.5206.1972
  4. ^ BBC News, "What is at the centre of the Earth?
  5. ^ Metals Handbook, Vol. 8 Metallography, Structures and Phase Diagrams (8th ed.). Metals Park, Ohio: ASM International. 1973.
  6. ^ D.K. Bullens et al., Steel and Its Heat Treatment, Vol. I, Fourth Ed., J. Wiley & Sons Inc., 1938, p 86.
  7. ^ S.H. Avner, Introduction to Physical Metallurgy, 2nd Ed., McGraw-Hill, 1974, p 225.
  8. ^ ASM Handbook, Vol. 3: Alloy Phase Diagrams, ASM International, 1992, p 2.210 and 4.9, ISBN 0-87170-381-5.
  9. ^ B.D. Cullity & C.D. Graham, Introduction to Magnetic Materials, Second Ed., IEEE Inc., 2009, p 91, ISBN 978-0-471-47741-9.
  10. ^ Template:Cite article
  11. ^ Template:Cite article