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Alpha Rays in Matter



An atomic bulldozer, strongly ionizing along a very short path

The wake of an alpha particle
An alpha particle is some 7300 times heavier than an electron. It undergoes practically no change in direction when it ionises other atoms. It leaves behind it, strewn around its straight path, a wake of ejected electrons and ionised atoms. Occasionally, when the electron is released at great speed, it too develops the ability to ionise. Finally, alpha particles do sometimes collide with other atomic nuclei, resulting in a deflection at large angles. These collisions are very rare, but were what allowed Ernest Rutherford to deduce the existence of the nucleus.
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Alpha particles are simultaneously the most dangerous form of radiation for living matter and the easiest to protect oneself from.

A very short trajectory !
Because of their great ability to ionise, the trajectory of alpha particles through matter is very short. In a dense medium such as water, even those energetic alpha particles emitted by polonium 212 can barely travel 90 microns - less than a tenth of a millimetre. A sheet of paper or the thickness of an item of clothing is more than enough to render them harmless. The inset shows that inside a ‘cloud chamber’ saturated with water vapor, the range of alpha particles does not exceed a few centimetres. It is very easy to protect against alpha when the source is external.
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An alpha particle ejected from a nucleus is travelling at a speed greater than the fastest of man-made rockets. This speed, which can reach 9,600 kilometres per second for an alpha particle with 2 MeV of energy, is nonetheless much smaller than that of light - almost 300,000 kilometres per second. An alpha particle is also much heavier than the atomic electrons it bumps into, with a mass ratio of around 8000:1!

An alpha particle en route is like an atomic bulldozer, unperturbed by the electrons it rips away from the atoms met along its travel path. Travelling in a straight line, and at a comparatively low velocity (compared to electrons), it can force large numbers of atoms to give up their electrons in a process known as ionisation.

The alpha decays caused by the trace amounts of uranium found in blocks of granite will never escape the confines of the rock. Those particles emitted by atoms at the surface, however, will be stopped by the thickness of a sheet of paper, a pair of trousers or a glove.

A well defined range
This historic photograph shows the trajectories of 9 MeV alpha emitted from a radioactive source of thorium-C (polonium-212) inside a Wilson cloud chamber. The ‘shaving-brush’ aspect is due to the fact that alpha, issued with the same energy, have a well defined range and travel no farther than 11.5 cm in the chamber. The curve on the right illustrates the same effect is a different way : the percentage of alpha particles crossing a given thickness of matter, remains at 100% before falling sharply to 0 when this range is reached.
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The only time an alpha particle is dangerous is if it attaches itself inside living matter. Contact with the skin is not enough, as the epidermis is thick enough for the radiation to be absorbed entirely within the 'dead' layers of skin. Real risks arise from the inhalation of radioactive aerosols which come to rest on the cells of the lungs. When an alpha emitter finds itself inside an organ it can cause considerable damage, as the living cells absorb the brunt of the energy over very short distances.

Alpha particles, which carry a positive electric charge of +2, are repulsed by the nuclei of other atoms. They do not have in general enough energy to enter in contact with target nuclei and induce nuclear reactions (*).

However they can approach these nuclei and bounce back at large angles. These rare collisions have played an important part in the history of nuclear physics. It was by observing alpha particles travelling through a thin sheet of gold, and noting that they occasionally collided with large, unseen bodies, that between 1909 and 1911 Geiger, Marsden and Rutherford were able to deduce the existence of atomic nuclei.

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