On the Connexion of the Physical SciencesSomerville, Mary
Science
On the Connexion of the Physical Sciences
Somerville, Mary
Physical sciences; Science
The equilibrium of the system, however, would be deranged if the planets
moved in a resisting medium (N. 78) sufficiently dense to diminish their
tangential velocity, for then both the excentricities and the major axes
of the orbits would vary with the time, so that the stability of the
system would be ultimately destroyed. The existence of an ethereal
medium is now proved; and, although it is so extremely rare that
hitherto its effects on the motions of the planets have been altogether
insensible, there can be no doubt that, in the immensity of time, it
will modify the forms of the planetary orbits, and may at last even
cause the destruction of our system, which in itself contains no
principle of decay, unless a rotatory motion from west to east has been
given to this medium by the bodies of the solar system, which have all
been revolving about the sun in that direction for unknown ages. This
rotation, which seems to be highly probable, may even have been coeval
with its creation. Such a vortex would have no effect on bodies moving
with it, but it would influence the motions of those revolving in a
contrary direction. It is possible that the disturbances experienced by
comets, which have already revealed the existence of this medium, may
also, in time, disclose its rotatory motion.
The form and position of the planetary orbits, and the motion of the
bodies in the same direction, together with the periodicity of the terms
in which the inequalities are expressed, assure us that the variations
of the system are confined within very narrow limits, and that, although
we do not know the extent of the limits, nor the period of that grand
cycle which probably embraces millions of years, yet they never will
exceed what is requisite for the stability and harmony of the whole; for
the preservation of which every circumstance is so beautifully and
wonderfully adapted.
The plane of the ecliptic itself, though assumed to be fixed at a given
epoch for the convenience of astronomical computation, is subject to a
minute secular variation of 45ʺ·7, occasioned by the reciprocal action
of the planets. But, as this is also periodical, and cannot exceed 2°
42ʹ, the terrestrial equator, which is inclined to it at an angle[2] of
23° 27ʹ 28ʺ·29, will never coincide with the plane of the ecliptic: so
there never can be perpetual spring (N. 79). The rotation of the earth
is uniform; therefore day and night, summer and winter, will continue
their vicissitudes while the system endures, or is undisturbed by
foreign causes.
Yonder starry sphere
Of planets and of fix’d, in all her wheels,
Resembles nearest mazes intricate,
Eccentric, intervolved, yet regular,
Then most, when most irregular they seem.
Public-domain text, read in full here on John Shaqi.
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