retort was almost red hot, the red matter
began gradually to decrease in bulk, and in a few minutes after it
disappeared altogether; at the same time 41-1/2 grains of running
mercury were collected in the recipient, and 7 or 8 cubical inches of
elastic fluid, greatly more capable of supporting both respiration and
combustion than atmospherical air, were collected in the bell-glass.

A part of this air being put into a glass tube of about an inch
diameter, showed the following properties: A taper burned in it with a
dazzling splendour, and charcoal, instead of consuming quietly as it
does in common air, burnt with a flame, attended with a decrepitating
noise, like phosphorus, and threw out such a brilliant light that the
eyes could hardly endure it. This species of air was discovered almost
at the same time by Mr Priestley, Mr Scheele, and myself. Mr Priestley
gave it the name of _dephlogisticated air_, Mr Scheele called it
_empyreal air_. At first I named it _highly respirable air_, to which
has since been substituted the term of _vital air_. We shall presently
see what we ought to think of these denominations.

In reflecting upon the circumstances of this experiment, we readily
perceive, that the mercury, during its calcination, absorbs the
salubrious and respirable part of the air, or, to speak more strictly,
the base of this respirable part; that the remaining air is a species of
mephitis, incapable of supporting combustion or respiration; and
consequently that atmospheric air is composed of two elastic fluids of
different and opposite qualities. As a proof of this important truth, if
we recombine these two elastic fluids, which we have separately obtained
in the above experiment, viz. the 42 cubical inches of mephitis, with
the 8 cubical inches of respirable air, we reproduce an air precisely
similar to that of the atmosphere, and possessing nearly the same power
of supporting combustion and respiration, and of contributing to the
calcination of metals.

Although this experiment furnishes us with a very simple means of
obtaining the two principal elastic fluids which compose our atmosphere,
separate from each other, yet it does not give us an exact idea of the
proportion in which these two enter into its composition: For the
attraction of mercury to the respirable part of the air, or rather to
its base, is not sufficiently strong to overcome all the circumstances
which oppose this union. These obstacles are the m