History of Astronomy |
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No one recognises more than the mathematical astronomer this feebleness of the
human intellect , and no one is more ... of the logical process called mathematics
, which even now has not solved directly the problem of only three bodies .
No one recognises more than the mathematical astronomer this feebleness of the
human intellect , and no one is more ... of the logical process called mathematics
, which even now has not solved directly the problem of only three bodies .
Page 55
But improved mathematical methods have always succeeded in the end , and so
the seeming doubt has been converted into a surer conviction of the universality
of the law . Having once established the law , Newton proceeded to trace some ...
But improved mathematical methods have always succeeded in the end , and so
the seeming doubt has been converted into a surer conviction of the universality
of the law . Having once established the law , Newton proceeded to trace some ...
Page 58
When Newton applied his law of gravitation to an explanation of the tides he
started a new field for the application of mathematics to physical problems ; and
there can be little doubt that , if he could have been furnished with complete tidal
...
When Newton applied his law of gravitation to an explanation of the tides he
started a new field for the application of mathematics to physical problems ; and
there can be little doubt that , if he could have been furnished with complete tidal
...
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Contents
ANCIENT GREEK ASTRONOMY | 3 |
GALILEO AND THE TELESCOPENOTIONS OF GRAVITY | 46 |
NEWTONS SUCCESSORS HALLEY EULER | 60 |
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Common terms and phrases
accepted accurate ancient appear astronomers attraction bodies bright calculations called catalogue cause centre century Chinese circle comet compared complete Copernicus determined diameter direction discovered discovery distance earth eclipse effect elements enabled epicycles equal error explain fact fixed follow force four Galileo gave give given gravitation heavens held Herschel increased interesting Jupiter Kepler knowledge known later light lunar Mars mass mathematical mean measured method miles moon moon's motion move nebulæ Newton noted noticed object observations Observatory opposition orbit original parallax pass period photographic physical planet planetary pole position predicted progress proper motion proved records researches revolve ring rotation round Royal satellites seems seen showed solar system spectroscope spectrum stars studied sun's supposed surface tables telescope theory tion trace true Tycho Brahe UNIVERSITY