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To explain the
structure of the atom, the Danish physicist Niels
Bohr developed in 1913 a hypothesis known as the Bohr
theory of the atom. He assumed that electrons move in
definite orbits at a considerable distance from the
nucleus. The number of such electrons equals the
atomic number of the atom: hydrogen has a single
orbital electron, helium has 2, and uranium has 92.
Bohr was able to use his model of the atom to explain
the spectrum of the simplest atom, hydrogen.

Bohr's ideas were
developed further to explain the chemical properties
of the elements. It was realized that the electrons'
orbits are grouped together into "shells", each of
which has an upper limit to the number of electrons
that it can accommodate. The first shell is complete
when it contains two electrons, the second can hold
up to eight, and successive shells hold still larger
numbers. The seventh shell is not filled in any
naturally occurring atom. The "last" electrons, those
which are outermost or added last to the atom's
structure, determine the chemical behavior of the
atom.
The inert, or noble, gases
(helium, neon, argon, krypton, xenon, and radon) all
have completely filled outer shells. They do not
enter into chemical combinations in nature, although
the three heaviest inert gases (krypton, xenon, and
radon) have formed chemical compounds in the
laboratory. On the other hand, the outermost shells
of such elements as lithium, sodium, and potassium
contain only one electron. These elements combine
readily with other elements (transferring their
outermost electrons to them) to form a great many
chemical compounds. Correspondingly, such elements as
fluorine, chlorine, and bromine lack only one
electron to acquire a filled outermost shell. They
too combine readily with other elements, receiving
electrons from them.
Atomic shells do not
necessarily fill up with electrons in consecutive
order. The electrons of the first 18 elements in the
periodic table are added in a regular manner, each
shell being filled to a designated limit before a new
shell is started. From the 19th element onwards, the
outermost shell is started before the previous shell
is completely filled. A regularity is still
maintained, however, as electrons fill successive
shells in a repetitive back-and-forth pattern. The
result is the regular repetition of chemical
properties for atoms of increasing atomic weight that
corresponds to the arrangement of the elements in the
periodic table.
It is still convenient to
visualize the electrons as Rutherford and Bohr did
originally, as moving about the nucleus of an atom
much as if they were planets moving about the Sun.
This view is much simpler than that held by
present-day physicists, however. It is now known that
it is impossible to pinpoint the precise position of
an electron in the atom's space without disturbing
its predicted location at some future time. This
uncertainty is expressed by attributing to the atom a
cloud-like form, in which the electron's position is
defined in terms of the probability of finding it at
some distance from the nucleus. The
"probability-cloud" view of the atom has superseded
the solar-system model.
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