An Introduction to the History of ScienceLibby, Walter
History
An Introduction to the History of Science
Libby, Walter
Science -- History
In his _Celestial Mechanics_ (1825) Laplace states that, according to
Herschel's observations, Saturn's rotation is slightly quicker than that
of its rings. This seemed a confirmation of the hypothesis of the
_Exposition du Système du Monde_.
When Laplace presented the first edition of this earlier work to
Napoleon, the First Consul said: "Newton has spoken of God in his book.
I have already gone through yours, and I have not found that name in it
a single time." To this Laplace is said to have replied: "First Citizen
Consul, I have not had need of that hypothesis." The astronomer did not,
however, profess atheism; like Kant he felt competent to explain on
mechanical principles the development of the solar system from the point
at which he undertook it. In his later years he desired that the
misleading anecdote should be suppressed. So far was he from
self-sufficiency and dogmatism that his last utterance proclaimed the
limitations of even the greatest intellects: "What we know is little
enough, what we don't know is immense" (_Ce que nous connaissons est peu
de chose, ce que nous ignorons est immense_).
Sir William Herschel's observations, extended over many years, confirmed
both the nebular hypothesis and the theory of the systematic arrangement
of the stars. He made use of telescopes 20 and 40 feet in focal length,
and of 18.7 and 48 inches aperture, and was thereby enabled, as Humboldt
said, to sink a plummet amid the fixed stars, or, in his own phrase, to
gauge the heavens. _The Construction of the Heavens_ was always the
ultimate object of his observations. In a contribution on this subject
submitted to the Royal Society in 1787 he announced the discovery of 466
new nebulæ and clusters of stars. The sidereal heavens are not to be
regarded as the concave surface of a sphere, from the center of which
the observer might be supposed to look, but rather as resembling a rich
extent of ground or chains of mountains in which the geologist discovers
many strata consisting of various materials. The Milky Way is one
stratum and in it our sun is placed, though perhaps not in the very
center of its thickness.
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