History of Astronomy |
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Page 24
... attraction . In the year 134 B.C. Hipparchus observed a new star . This upset every notion about the permanence of the fixed stars . He then set to work to catalogue all the principal stars so as to know if any others appeared or ...
... attraction . In the year 134 B.C. Hipparchus observed a new star . This upset every notion about the permanence of the fixed stars . He then set to work to catalogue all the principal stars so as to know if any others appeared or ...
Page 34
... attraction of the sun . To correct for these irreg- ularities Copernicus introduced epicycle on epi- cycle in the lunar orbit . This is in its main features the system pro- pounded by Copernicus . But attention must , to state the case ...
... attraction of the sun . To correct for these irreg- ularities Copernicus introduced epicycle on epi- cycle in the lunar orbit . This is in its main features the system pro- pounded by Copernicus . But attention must , to state the case ...
Page 56
... attracted to the earth's centre , not because it is the centre of the universe , but because it is the centre of the ... attraction . Kepler had been appointed Imperial Astrono- mer with a handsome salary ( on paper ) , a frac- tion of ...
... attracted to the earth's centre , not because it is the centre of the universe , but because it is the centre of the ... attraction . Kepler had been appointed Imperial Astrono- mer with a handsome salary ( on paper ) , a frac- tion of ...
Page 65
... attraction for both of them fol- low the same law as to distance as is given by the planetary motions round the sun ? It has been stated that in this way the first conception of universal gravitation arose.1 66 1 The writer inherited ...
... attraction for both of them fol- low the same law as to distance as is given by the planetary motions round the sun ? It has been stated that in this way the first conception of universal gravitation arose.1 66 1 The writer inherited ...
Page 67
... attraction by the separate particles of a sphere of uniform density ( or one composed of concentric spherical shells , each of uniform den- sity ) , acts as if the whole mass were collected at the centre , he was able to express the ...
... attraction by the separate particles of a sphere of uniform density ( or one composed of concentric spherical shells , each of uniform den- sity ) , acts as if the whole mass were collected at the centre , he was able to express the ...
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Common terms and phrases
accurate Airy ancient astron Astronomer Royal astronomical units bright calculations Cape catalogue centre century Chaldæans Chinese comet Copernicus diameter discovered discovery earth Egyptian epicycles equatorial error excentric explain fact fixed stars Galileo Greenwich Halley heavenly bodies heavens heliometer Hipparchus History of Astronomy instruments JOHANNES KEPLER John Herschel Jupiter Jupiter's Kepler Laplace Lick Observatory light line of apses line of sight lunar Mars mathematical mean distance mean motion measured ment Mercury meteor miles a second moon moon's nebulæ Newton observations Observatory orbit parallax period photographic physical planet planetary pole position predicted proper motion proved Ptolemy R. S. Phil records refractor retrograde retrograde motion revolving round ring rotation satellites Saturn seems showing Sir William Herschel Sirius solar eclipse solar system spectra spectroscope spectrum sphere spots stellar sun-spot supposed tables telescope theory tion Trans Tycho Brahe universal gravitation Uranus velocity Venus Verrier
Popular passages
Page 67 - that every particle of matter in the universe attracts every other particle, with a force whose direction is that of the line joining the two, and whose magnitude is directly as the product of their masses, and inversely as the square of their distances from each other.
Page 26 - So he sate and cunningly guided the craft with the helm, nor did sleep fall upon his eyelids, as he viewed the Pleiads and Bootes, that setteth late, and the Bear, which they likewise call the Wain, which turneth ever in one place, and keepeth watch upon Orion, and alone hath no part, in the baths of Ocean. This star, Calypso, the fair goddess, bade him to keep ever on the left as he traversed the deep.
Page 53 - The third, viz. that the squares of the periodic times are proportional to the cubes of the mean distances...
Page 79 - Wherefore if according to what we have already said it should return again about the year 1758, candid posterity will not refuse to acknowledge that this was first discovered by an Englishman.
Page 122 - ... They have not been regarded as so successful as his geometrical analysis of the observed phenomena. It is only just to add that he himself did not attach equal weight to them ; for in answer to objections urged by Lalande to his theory that the spots are depressions, Wilson wrote thus in 1783 : — ' Whether their first production and subsequent numberless changes depend upon the eructation of elastic vapours from below, or upon eddies or whirlpools commencing at the surface, or upon the dissolving...
Page 51 - He then said boldly that it was impossible that so good an observer as Tycho could be wrong by eight minutes* and added, " out of these eight minutes we will construct a new theory that will explain the motions of all the planets.