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somewhat of the Arian or Unitarian persuasion--so, at least, it is
asserted by orthodox divines who understand these matters. He studied
theology more or less all his life, and towards the end was greatly
interested in questions of Biblical criticism and chronology. By some
ancient eclipse or other he altered the recognized system of dates a few
hundred years; and his book on the prophecies of Daniel and the
Revelation of St. John, wherein he identifies the beast with the Church
of Rome in quite the orthodox way, is still by some admired.
But in all these matters it is probable that he was a merely ordinary
man, with natural acumen and ability doubtless, but nothing in the least
superhuman. In science, the impression he makes upon me is only
expressible by the words inspired, superhuman.
And yet if one realizes his method of work, and the calm, uninterrupted
flow of all his earlier life, perhaps his achievements become more
intelligible. When asked how he made his discoveries, he replied: "By
always thinking unto them. I keep the subject constantly before me, and
wait till the first dawnings open slowly by little and little into a
full and clear light." That is the way--quiet, steady, continuous
thinking, uninterrupted and unharassed brooding. Much may be done under
those conditions. Much ought to be sacrificed to obtain those
conditions. All the best thinking work of the world has been thus
done.[18] Buffon said: "Genius is patience." So says Newton: "If I have
done the public any service this way, it is due to nothing but industry
and patient thought." Genius patience? No, it is not quite that, or,
rather, it is much more than that; but genius without patience is like
fire without fuel--it will soon burn itself out.
NOTES FOR LECTURE IX
The _Principia_ published 1687.
Newton died 1727.
THE LAW OF GRAVITATION.--Every particle of matter attracts every other
particle of matter with a force proportional to the mass of each and to
the inverse square of the distance between them.
SOME OF NEWTON'S DEDUCTIONS.
1. Kepler's second law (equable description of areas) proves that each
planet is acted on by a force directed towards the sun as a centre of
force.
2. Kepler's first law proves that this central force diminishes in the
same proportion as the square of the distance increases.
3. Kepler's third law proves that all the planets are acted on by the
same kind of force; of an
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