An Introduction to the History of ScienceLibby, Walter
History
An Introduction to the History of Science
Libby, Walter
Science -- History
Comets, now robbed of many of the terrors with which ancient
superstition endowed them, might, he says, seem to threaten catastrophe,
by colliding with the planets or by carrying off a satellite. But the
same hand which has cast the celestial spheres in space, has traced
their course in the heavens, and does not allow them to wander at
random to disturb and destroy each other. Lambert imagines that all
these bodies have exactly the volume, weight, position, direction, and
speed necessary for the avoidance of collisions. If we confess a Supreme
Ruler who brought order from chaos, and gave form to the universe; it
follows that this universe is a perfect work, the impress, picture,
reflex of its Creator's perfection. Nothing is left to blind chance.
Means are fitted to ends. There is order throughout, and in this order
the dust beneath our feet, the stars above our heads, atoms and worlds,
are alike comprehended.
Laplace in his statement of the nebular hypothesis made no mention of
Kant. He sets forth, in the _Exposition of the Solar System_, the
astronomical data that the theory is designed to explain: the movements
of the planets in the same direction and almost in the same plane; the
movements of the satellites in the same direction as those of the
planets; the rotation of these different bodies and of the sun in the
same direction as their projection, and in planes little different; the
small eccentricity of the orbits of planets and satellites; the great
eccentricity of the orbits of comets. How on the ground of these data
are we to arrive at the cause of the earliest movements of the planetary
system?
A fluid of immense extent must be assumed, embracing all these bodies.
It must have circulated about the sun like an atmosphere and, in virtue
of the excessive heat which was engendered, it may be assumed that this
atmosphere originally extended beyond the orbits of all the planets, and
was contracted by stages to its present form. In its primitive state
the sun resembled the nebulæ, which are to be observed through the
telescope, with fiery centers and cloudy periphery. One can imagine a
more and more diffuse state of the nebulous matter.
Planets were formed, in the plane of the equator and at the successive
limits of the nebulous atmosphere, by the condensation of the different
zones which it abandoned as it cooled and contracted. The force of
gravity and the centrifugal force sufficed to maintain in its orbit each
successive planet. From the cooling and contracting masses that were to
constitute the planets smaller zones and rings were formed. In the case
of Saturn there was such regularity in the rings that the annular form
was maintained; as a rule from the zones abandoned by the planet-mass
satellites resulted. Differences of temperature and density of the parts
of the original mass account for the eccentricity of orbits, and
deviations from the plane of the equator.
Public-domain text, read in full here on John Shaqi.
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