Atomic and physical properties of a Ni nanocrystal inside a single wall
carbon nanotube; scale bar 5 nm Nickel is a silvery-white metal with a slight golden tinge that takes a high polish. It is one of only four elements that are
ferromagnetic at or near room temperature; the others are iron,
cobalt and
gadolinium. Its
Curie temperature is , meaning that bulk nickel is non-magnetic above this temperature.
Electron configuration dispute Nickel has two atomic
electron configurations, [Ar] 3d 4s and [Ar] 3d 4s, which are very close in energy; [Ar] denotes the complete
argon core structure. There is some disagreement on which configuration has the lower energy. also written [Ar] 3d 4s. This configuration agrees with the
Madelung energy ordering rule, which predicts that 4s is filled before 3d. It is supported by the experimental fact that the lowest energy state of the nickel atom is a 3d 4s energy level, specifically the 3d(F) 4s F,
J = 4 level. However, each of these two configurations splits into several energy levels due to
fine structure,
Isotopes The isotopes of nickel range in
atomic mass from () to (). Natural nickel is composed of five stable
isotopes, , , , and , of which is the most abundant (68.077%
natural abundance).
Nickel-62 has the highest
binding energy per nucleon of any
nuclide: 8.7946 MeV/nucleon. Its binding energy is greater than both iron-56| and iron-58|, more abundant nuclides often incorrectly cited as having the highest binding energy. Though this would seem to predict nickel as the most abundant heavy element in the universe, the high rate of
photodisintegration of nickel in stellar interiors causes iron to be by far the most abundant. At least 26 nickel
radioisotopes have been characterized; the most stable are with
half-life 76,000 years, (100 years), and (6 days). All other radioisotopes have half-lives less than 60 hours and most these have half-lives less than 30 seconds. This element also has one
meta state. Radioactive nickel-56 is produced by the
silicon burning process and later set free in large amounts in
type Ia supernovae. The shape of the
light curve of these supernovae at intermediate to late-times corresponds to the decay via
electron capture of to
cobalt-56 and ultimately to iron-56. Nickel-59 is a long-lived
cosmogenic radionuclide; half-life 76,000 years. has found many applications in
isotope geology. has been used to date the terrestrial age of
meteorites and to determine abundances of extraterrestrial dust in ice and
sediment. Nickel-78, with a half-life of 110 milliseconds, is believed an important isotope in
supernova nucleosynthesis of elements heavier than iron. Ni, discovered in 1999, is the most proton-rich heavy element isotope known. With 28
protons and 20
neutrons, Ni is "
doubly magic", as is Ni with 28 protons and 50 neutrons. Both are therefore unusually stable for nuclei with so large a
proton–neutron imbalance. Nickel-63 is a contaminant found in the support structure of nuclear reactors. It is produced through neutron capture by nickel-62. Small amounts have also been found near nuclear weapon test sites in the South Pacific.
Occurrence showing the two forms of nickel–iron, kamacite and taenite, in an octahedrite meteorite Nickel ores are classified as oxides or sulfides. Oxides include
laterite, where the principal mineral mixtures are nickeliferous
limonite, (Fe,Ni)O(OH), and
garnierite (a mixture of various hydrous nickel and nickel-rich silicates). Nickel sulfides commonly exist as solid solutions with iron in minerals such as
pentlandite and
pyrrhotite with the formula Fe9−xNixS8 and Fe7−xNixS6, respectively. Other common Ni-containing minerals are
millerite and the
arsenide niccolite. Identified land-based resources throughout the world averaging 1% nickel or greater comprise at least 130 million tons of nickel (about the double of known reserves). About 60% is in
laterites and 40% in sulfide deposits. On
geophysical evidence, most of the nickel on Earth is believed to be in Earth's
outer and
inner cores.
Kamacite and
taenite are naturally occurring
alloys of iron and nickel. For kamacite, the alloy is usually in the proportion of 90:10 to 95:5, though impurities (such as
cobalt or
carbon) may be present. Taenite is 20% to 65% nickel. Kamacite and taenite are also found in
nickel iron meteorites. Nickel is commonly found in
iron meteorites as the alloys
kamacite and
taenite. Nickel in meteorites was first detected in 1799 by
Joseph-Louis Proust, a French chemist who then worked in Spain. Proust analyzed samples of the meteorite from
Campo del Cielo (Argentina), which had been obtained in 1783 by Miguel Rubín de Celis, discovering the presence in them of nickel (about 10%) along with iron. == Compounds ==