The Gases of the Atmosphere: The History of Their DiscoveryRamsay, William
History
The Gases of the Atmosphere: The History of Their Discovery
Ramsay, William
Air; Argon; Chemistry -- History
Molecules, on this supposition, may consist of single atoms, or they
may consist of pairs of such atoms, joined in some fashion like the
bulged ends of a dumb-bell; or lastly, they may consist of greater
numbers of atoms arranged in some different manner, the arrangement
depending on their relative size and attraction for each other. It must
be clearly understood, however, that such mental pictures are not to
be taken as actually representing the true constitution of matter, but
merely as attempts to picture such forms as will allow of our drawing
conclusions regarding their behaviour from known configurations of
large masses.
The molecules of gases are imagined to be in a state of continual
motion, up and down, backwards and forwards, and from side to side.
It is true that they must also move in directions which cannot be
described by any of these expressions, but such other directions may be
conceived as partaking more or less of motions in the three directions
specified; _i.e._ in being resolvable into these. To these motions
have been applied the term “degrees of freedom.” Such motions through
space, in which the molecule is transported from one position in space
to another, form three of the possible six degrees of freedom which a
molecule may possess, and the molecules are said to possess “energy
of translation” in virtue of this motion. The other three consist in
rotations in three planes at right angles to each other.
Now, it can be shown that the product of pressure and volume of a gas,
_pv_, is equal to ⅔rds of the energy of translation of all molecules
of the gas, or
_pv_ = ⅔(NR),
where N stands for the number of molecules in unit volume, and R for
their energy of translation; inasmuch as a pressure diminishing a
volume is of the nature of work, or energy. For one gram of air at O°
C. and 76 cms. pressure (normal temperature and pressure), the pressure
(_p_), measured in grams per square centimetre, is 1033, and the volume
(_v_) is 773·3 cubic centimetres; and the raising of the temperature
through 1°, as was shown before, requires 2927 gram-centimetres of
work. Further, since the product of pressure into volume is equal to
⅔rds of the energy due to motion, or the translational energy of the
gas,
NR = 3/2_pv_ = 3/2 × 2927 = 4391 gram-centimetres.
Dividing this number by 42,380, the mechanical equivalent of heat,
or the number of gram-centimetres corresponding to one calory, the
quotient is 0·1040 calory. If the energy of the air were due to the
translational motion of its molecules, we should expect this number,
0·1040, to stand for the specific heat of air at constant volume; but
it has been found equal to 0·1683, as already shown.
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