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Page 53
... that the sun ' s force on different planets ( besides depending as above on
distance ) is proportional to their masses . ... each of uniform density ) acts as if
the whole mass were collected at the centre , he was able to express the
meaning of ...
... that the sun ' s force on different planets ( besides depending as above on
distance ) is proportional to their masses . ... each of uniform density ) acts as if
the whole mass were collected at the centre , he was able to express the
meaning of ...
Page 56
By means of this principle he was able to compare the mass of the sun with the
masses of those planets that have moons , and also to compare the mass of our
moon with the mass of the earth . Thus Newton , after having established his
great ...
By means of this principle he was able to compare the mass of the sun with the
masses of those planets that have moons , and also to compare the mass of our
moon with the mass of the earth . Thus Newton , after having established his
great ...
Page 85
This led him to correct the mass of the moon , and to fix its ratio to the earth ' s
mass = 0 . 012240 . Another method of getting the distance from the sun is to
measure the velocity of the earth ' s orbital motion , giving the circumference
traversed ...
This led him to correct the mass of the moon , and to fix its ratio to the earth ' s
mass = 0 . 012240 . Another method of getting the distance from the sun is to
measure the velocity of the earth ' s orbital motion , giving the circumference
traversed ...
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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