The atom and the Bohr theory of its structure : $b an elementary presentationHolst, Helge
Science
The atom and the Bohr theory of its structure : $b an elementary presentation
Holst, Helge
Atomic theory
There is no doubt that the process which takes place in the emission
of radiation from the radioactive elements is a _transformation of
the element_, an explosion of the atoms accompanied by the emission
either of double-charged helium atoms or of electrons, and the forming
of the atoms of a new element. The energy of the rays is an internal
atomic energy, freed by these transformations. The element uranium,
with the greatest of all known atomic weights (238), passes, by several
intermediate steps, into radium with atomic weight 226; from radium
there comes, after a series of steps, lead, or, in any case, an element
which, in all its chemical properties, behaves like lead. We shall go
no further into this subject, merely remarking that the transformations
are quite independent of the chemical combinations into which the
radioactive elements have entered, and of all external influences.
When α-particles from radium are sent against a screen with a coating
of especially prepared zinc sulphide, on this screen, in the dark,
there can be seen a characteristic light phenomenon, the so-called
scintillation, which consists of many flashes of light. Each individual
flash means that an α-particle, a helium atom, has hit the screen. In
this bombardment by atoms the individual atom-projectiles are made
visible in a manner similar to that in which the individual raindrops
which fall on the surface of a body of water are made visible by the
wave rings which spread from the places where the drops meet the water.
This flash of light was the first effect of the individual atom to
be available for investigation and observation. The incredibility of
anything so small as an atom producing a visible effect is lessened
when, instead of paying attention merely to the small size or mass of
the atom, its kinetic energy is considered; this energy is proportional
to the square of the velocity, which is here of overwhelming magnitude.
For the most rapid α-particles the velocity is 2·26 × 10⁹ cm. per
second; their kinetic energy is then about ⁴/₃₀ of the kinetic
energy of a weight of one milligram of a substance at a velocity of
one centimetre per second. This energy may seem very small, but, at
least, it is not a magnitude of “inconceivable minuteness,” and it is
sufficient under the conditions given above to produce a visible light
effect. We must here also consider the extreme sensitiveness of the eye.
[Illustration: FIG. 19.—Photograph of paths described
by α-particles (positive helium ions) emitted from a radioactive
substance.]
More practical methods of revealing the effects of the individual
α-particles and of counting them are founded on their very strong
ionization power. By strengthening the ionization power of α-particles,
Rutherford and Geiger were able to make the air in a so-called
ionization chamber so good a conductor that an individual α-particle
caused a deflection in an electrical apparatus, an electrometre.
Public-domain text, read in full here on John Shaqi.
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