The Story of Creation as Told By Theology and By ScienceAckland, T. S. (Thomas Suter)
Religion
The Story of Creation as Told By Theology and By Science
Ackland, T. S. (Thomas Suter)
Bible and science; Creation; Religion and science
When these facts are duly weighed, there seems to be a reasonable
probability that this process is the one which was actually
employed in the formation of the solar system. The remarkable
manner in which the theory adapts itself to the Mosaic account,
and the fact that that account records special interferences of
the Creator exactly at the points where the theory shows that such
interferences would be necessary, give rise to a very strong
presumption in its favour. We have in it also a clear illustration
of the combination of general laws of nature with special
interferences of Creative Power--the law of gravitation was called
into action, and the work would proceed steadily under that law
for a considerable period, till matters were ripe for a farther
stage in the progress, and then the special interference would
take place, in this instance the imparting the motion of rotation,
and the work would again proceed under the natural law. All this
while, however, the work would be one, and performed by one power,
the only difference being in the direct or indirect action of that
power.
The only point an reference to the first day which remains to be
inquired into is the extent to which the work had proceeded at its
close. As the commencement of the second day's work implies that
at that time the earth had an independent existence, we may
conclude that the first day's work comprehended the casting off of
the several successive rings, and the condensation of those rings,
or some of them, into the corresponding planets and satellites.
These would probably still retain their intense heat, in virtue of
which they would be luminous.
Many of the multiple stars may not improbably present to us much
the same appearance as the solar system then presented. In many
cases we have one large star, with one or more very minute
attendants. Such a star is Orionis, a tolerably conspicuous star,
which has two companions invisible to the naked eye, but visible
with moderate telescopic power. (A telescope of 2.1 inches
aperture, by Cooke, shows them well.) Five more companions are
visible in a 4-inch telescope. In the large telescope at Harvard
no less than 35 minute stars have been seen in apparent connexion
with the brilliant star Vega. In all these cases it is true that
the distances and periods of the companion stars are very much
greater than in the case of the earth; but then our telescopes
will only enable us to discern the more distant companions. Any
small companion stars holding positions corresponding to those of
the four interior planets, would be lost in the light of the
primary star; and if, as is suspected, all the heavenly bodies are
subject to some resistance, however small, from the medium in
which they move, this resistance would in the course of ages
diminish the mean distance, and with it the periodic time of the
companion stars.
Public-domain text, read in full here on John Shaqi.
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