103. Lawrencium

Name: Lawrencium
Symbol: Lr
Atomic Number: 103
Atomic Mass: (262.0) amu
Melting Point: Unknown
Boiling Point: Unknown
Number of Protons/Electrons: 103
Number of Neutrons: 159
Classification: Rare Earth
Crystal Structure: Unknown
Density(293 K): Unknown
Color: Unknown

Lawrencium is a synthetic "rare earth metal" which does not occur in the environment.

Lawrencium was discovered by Albert Ghiorso, Torbjorn Sikkeland, Almon Larsh and Robert M. Latimer on February 14, 1961 at the Berkeley Radiation Laboratory (now called Lawrence Berkeley National Laboratory) on the University of California, Berkeley campus. It was produced by bombarding a 3 milligram target composed of three isotopes of californium with boron-10 and B-11 ions in the Heavy Ion Linear Accelerator (HILAC).

The transmutation nuclei became electrically charged, recoiled with a helium atmosphere and were collected on a thin copper conveyor tape. This tape was then moved in order to place the collected atoms in front of a series of solid-state detectors. The Berkeley team reported that the isotope 103-257 was detected in this manner and decayed by emitting an 8.6 MeV alpha particle with a half-life of 4.2 seconds.

In 1967, researchers in Dubna, Russia reported that they were not able to confirm an alpha emitter with a half-life of 4.2 seconds as 103-257. This assignment has since been changed to Lr-258 or Lr-259. Eleven isotopes of element 103 have been synthesized with Lr-262 being the longest lived with a half-life of 216 minutes (it decays into nobelium-256). The isotopes of lawrencium decay via alpha emission, spontaneous fission and electron capture (in order or most to least common types).

The origin of the name, preferred by the American Chemical Society, is in reference to Ernest O. Lawrence, inventor of the cyclotron. The symbol Lw was originally used but in 1963 it was changed to Lr. In August 1997 the International Union of Pure and Applied Chemistry (IUPAC) ratified the name lawrencium and symbol Lr during a meeting in Geneva.

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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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