|In situ availability:||abundant|
|melting point:|| 1811K,|
|boiling point:|| 3134K,|
|N/A ← N/A → N/A|
|Mn ← Fe → Co|
|Tc ← Ru → Rh|
|Atomic radius (pm):||140|
|Bohr radius (pm):||156|
|Covalent radius (pm):||125|
|Van der Waals radius (pm):|
|ionic radius (pm):||(+3) 55|
|1st ion potential (eV):||7.90|
| 1s2 |
3s2 3p6 3d6
|Electrons Per Shell|
|2, 8, 14, 2|
|Oxidation states:||2, 3|
|Crystal structure:||Body centered cubic|
Iron is a Transition Metal in group 8.
It has a Body centered cubic crystalline structure.
This element has 4 stable isotopes: 54, 56, 57, and 58.
 Lunar Iron Use/Production
Lunar iron is present both in metallic form and as oxides. Metallic iron is found virtually everywhere on the moon, alloyed with nickel in tiny particles dispersed in the regolith, the remnants of pulverized nickel-iron meteorites. Iron oxides are found predominately on the maria, where they can make up nearly 15% of the regolith by weight. Due to this abundance of both free iron and iron oxides, as well as the fact that iron oxides require less energy to reduce than any other oxide found in the lunar surface, iron is considered to be the easiest metal to obtain on Luna.
Due to this ease of acquirement, lunar iron could become a workhorse metal for lunar construction. Iron could be alloyed with carbon extracted from the lunar regolith to produce steel. Other important alloying elements include titanium, chromium, nickel, and manganese, all of which are available from lunar sources.
Metalic iron is strongly attracted to magnetic fields, and can be easily separated from the lunar regolith by magnetic processes. Many iron oxides can also be extracted from the regolith using magnetic separation, including Ilmenite(FeTiO3), hematite (Fe2O3), and magnetite (FeO.Fe2O3). These oxides generally have much weaker attraction to magnetic fields than metallic iron, enabling separation of the two after gathering.