The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
It is very difficult for one to conceive how such a delicate structure,
as the system of rings appears to be, can keep together in equilibrium
and avoid destruction from the powerful attraction of the planet on one
side and the disturbing influence of the satellites on the other. To
explain it, several hypotheses have been advanced. The rings were first
supposed to be solid, and upon this supposition Laplace determined the
necessary conditions for their equilibrium; the most important of which
require that the cross section of the rings should be an ellipse of
irregular curvature, and having its major axis directed towards the
centre of the planet, and also that the system should rotate upon an
axis perpendicular to the plane of the rings. This theory was superseded
by another, which supposed the rings to be fluid. This one was soon
rejected for a third, assuming the system to be composed of vapors or
gases; and more recently, all these theories were considered untenable,
and replaced by a fourth, which supposes the system of rings to be made
up of a congregation of innumerable small, independent bodies, revolving
around Saturn in concentric zones. Naturally, such a divergence of
opinion can only result from our comparative ignorance of the subject,
and sufficiently indicates our inability to explain the phenomena; and
it must be admitted that, so far, nothing is certainly known about this
strange system. We shall probably remain in the same uncertainty until
the rotation of the rings is ascertained by direct observations. It is
pretty certain, however, that none of these theories account for the
observed phenomena in their details, although a partial explanation may
be obtained by borrowing something from each hypothesis.
It has been conjectured, and a theory has been advanced, that the
breadth of the whole ring system is gradually increasing inwards, and
that it will come in contact with the planet in about 2,150 years; but
the question seems to have been settled in the negative by the elaborate
measurements of the English observers. It is likely that the increase is
only in the defining power of the instruments.
COMETS
PLATE XI
Among the celestial phenomena, none are more interesting than those
mysterious apparitions from the depths which unexpectedly display their
strange forms in our familiar constellations, through which they wander
for a time, until they disappear like phantoms.
A comet, with its luminous diffused head, whence proceeds a long vapory
appendage gradually fading away in the sky, presents an extraordinary
aspect, which may well astonish and deeply impress the observer.
Although these visitors from infinite space do not now inspire dread, as
in by-gone times, yet, owing to the mystery in which the phenomenon is
still involved, the apparition of a large comet, even in our days, never
fails to create a profound sensation, and in some cases that unconscious
fear which results from the unknown.
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