History of Astronomy |
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Page 24
The only object ever aimed at in those days was to prepare tables for predicting
the places of the planets . It was not a mechanical problem ; there was no notion
of a governing law of forces . From this time onwards all interest in astronomy ...
The only object ever aimed at in those days was to prepare tables for predicting
the places of the planets . It was not a mechanical problem ; there was no notion
of a governing law of forces . From this time onwards all interest in astronomy ...
Page 57
Grant has shown the values of some of these as given by observation in the
tables of Meyer and more modern tables , and has compared them with the
values assigned by Newton from his theory ; and the comparison is very
remarkable .
Grant has shown the values of some of these as given by observation in the
tables of Meyer and more modern tables , and has compared them with the
values assigned by Newton from his theory ; and the comparison is very
remarkable .
Page 68
In 1790 Delambre , using all these observations , prepared tables for computing
its position . These worked well enough for a time , but at last the differences
between the calculated and observed longitudes of the planet became serious .
In 1790 Delambre , using all these observations , prepared tables for computing
its position . These worked well enough for a time , but at last the differences
between the calculated and observed longitudes of the planet became serious .
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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