If it be a gaseous body, it must form part of the argon group, and, like its other members, be perfectly inert.
By studying the spectrum of the gas disengaged by a solution of salt of radium, Sir William Ramsay and Professor Soddy remarked that when the gas is radioactive there are first obtained rays of gases belonging to the argon family, then by degrees, as the activity disappears, the spectrum slowly changes, and finally presents the characteristic aspect of helium.
We know that the existence of this gas was first discovered by spectrum analysis in the sun.

Later its presence was noted in our atmosphere, and in a few minerals which happen to be the very ones from which radium has been obtained.

It might therefore have been the case that it pre-existed in the gases extracted from radium; but a remarkable experiment by M.Curie and Sir James Dewar seems to show convincingly that this cannot be so.

The spectrum of helium never appears at first in the gas proceeding from pure bromide of radium; but it shows itself, on the other hand, very distinctly, after the radioactive transformations undergone by the salt.
All these strange phenomena suggest bold hypotheses, but to construct them with any solidity they must be supported by the greatest possible number of facts.

Before admitting a definite explanation of the phenomena which have their seat in the curious substances discovered by them, M.and Madame Curie considered, with a great deal of reason, that they ought first to enrich our knowledge with the exact and precise facts relating to these bodies and to the effects produced by the radiations they emit.
Thus M.Curie particularly set himself to study the manner in which the radioactivity of the emanation is dissipated, and the radioactivity that this emanation can induce on all bodies.