History of Astronomy |
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Page 23
... and its ratio to that of the epicycle , the distance of the excentric3 from the
centre of the deferent , and the position of the line of apses , ' besides the
inclination and position. 2 lbid . . For definition see p . 22 . 3 For definition see p .
18 . possit .
... and its ratio to that of the epicycle , the distance of the excentric3 from the
centre of the deferent , and the position of the line of apses , ' besides the
inclination and position. 2 lbid . . For definition see p . 22 . 3 For definition see p .
18 . possit .
Page 68
Altogether , nineteen observations of Uranus ' s position , from the time of
Flamsteed , in 1690 , had been recorded . In 1790 Delambre , using all these
observations , prepared tables for computing its position . These worked well
enough for a ...
Altogether , nineteen observations of Uranus ' s position , from the time of
Flamsteed , in 1690 , had been recorded . In 1790 Delambre , using all these
observations , prepared tables for computing its position . These worked well
enough for a ...
Page 69
which as an undergraduate he had set himself — to see - whether the
disturbances of Uranus could be explained by assuming a certain orbit , and
position in that orbit , of a hypothetical planet even more distant than Uranus ,
Such an ...
which as an undergraduate he had set himself — to see - whether the
disturbances of Uranus could be explained by assuming a certain orbit , and
position in that orbit , of a hypothetical planet even more distant than Uranus ,
Such an ...
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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