22. Titanium

Name: Titanium
Symbol: Ti
Atomic Number: 22
Atomic Mass: 47.867 amu
Melting Point: 1660.0 °C (1933.15 °K, 3020.0 °F)
Boiling Point: 3287.0 °C (3560.15 °K, 5948.6 °F)
Number of Protons/Electrons: 22
Number of Neutrons: 26
Classification: Transition Metal
Crystal Structure: Hexagonal
Density(293 K): 4.54 g/cm3
Color: silverish

Titanium, when pure, is a lustrous, white metal.

Titanium minerals are quite common. The metal has a low density, good strength, is easily fabricated, and has excellent corrosion resistance. The metal burns in air and is the only element that burns in nitrogen. It is marvellous in fireworks.

Titanium is resistant to dilute sulphuric and hydrochloric acid, most organic acids, damp chlorine gas, and chloride solutions. Titanium metal is considered to be physiologically inert.

Titanium is present in meteorites and in the sun. Some lunar rocks contain high concentrations of the dioxide, TiO2. Titanium oxide bands are prominent in the spectra of M-type stars.

Titanium (Latin Titans, Earth or the first sons of Gaia) was discovered in England by Reverend William Gregor in 1791. He recognized the presence of a new element in ilmenite, and named it menachite. At around the same time, Franz Joseph Muller also produced a similar substance, but could not identify it. The element was independently rediscovered several years later by German chemist Martin Heinrich Klaproth in rutile ore. Klaproth confirmed it as a new element and in 1795 he named it for the Latin word for Earth (also the name for the Titans of Greek mythology).

The metal has always been difficult to extract from its various ores. Pure metallic titanium (99.9%) was first prepared in 1910 by Matthew A. Hunter by heating TiCl4 with sodium in a steel bomb at 700-800°C. Titanium metal was not used outside the laboratory until 1946 when William Justin Kroll proved that titanium could be commercially produced by reducing titanium tetrachloride with magnesium in the Kroll process (which is the method still used today).

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Non-metals H, C, N, O, P, S, Se
Halogens F, Cl, Br, I, At
Alkali metals Li, Na, K, Rb, Cs, Fr
Alkaline Earth Be, Mg, Ca, Sr, Ba, Ra
Transition metals Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Y, Zr, Nb, Mo, Tc, Ru, Rh, Pd, Ag, Cd, Hf, Ta, W, Re, Os, Ir, Pt, Au, Hg, Rf, Db, Sg, Bh, Hs, Mt, Ds, Rg, Uub
Metalloids B, Si, Ge, As, Sb, Te, Po
Other metals Al, Ga, In, Sn, Tl, Pb, Bi
Rare Earth Lu, Lr, La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Ac, Th, Pa, U, Np, Pu, Am, Cm, Bk, Cf, Es, Fm, Md, No
Noble gases He, Ne, Ar, Kr, Xe, Rn

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