History of Astronomy |
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Page 99
... Greenwich Ob- servatory , as first Astronomer Royal , in 1676 , with very poor instruments . In 1683 he put up a mural arc of 140 ° , and in 1689 a better one , seventy - nine inches radius . He conducted his measurements with great ...
... Greenwich Ob- servatory , as first Astronomer Royal , in 1676 , with very poor instruments . In 1683 he put up a mural arc of 140 ° , and in 1689 a better one , seventy - nine inches radius . He conducted his measurements with great ...
Page 101
... Greenwich star places have maintained the very highest accuracy . In George Biddell Airy , Seventh Astronomer Royal , ' commenced his Greenwich labours in 1835. His first and greatest reformation in the 1 Sir George Airy was very ...
... Greenwich star places have maintained the very highest accuracy . In George Biddell Airy , Seventh Astronomer Royal , ' commenced his Greenwich labours in 1835. His first and greatest reformation in the 1 Sir George Airy was very ...
Page 102
... Greenwich lunar observations have been a model and a standard for the whole world . Airy also undertook to superintend the reduc- tion of all Greenwich lunar observations from 1750 to 1830. 102 History of Astronomy.
... Greenwich lunar observations have been a model and a standard for the whole world . Airy also undertook to superintend the reduc- tion of all Greenwich lunar observations from 1750 to 1830. 102 History of Astronomy.
Page 103
George Forbes. tion of all Greenwich lunar observations from 1750 to 1830. The value of this laborious work , which was completed in 1848 , cannot be over- estimated . The demands of astronomy , especially in re- gard to small minor ...
George Forbes. tion of all Greenwich lunar observations from 1750 to 1830. The value of this laborious work , which was completed in 1848 , cannot be over- estimated . The demands of astronomy , especially in re- gard to small minor ...
Page 104
... Greenwich by the extensive use of photography and the establishment of large equatorials . From the point of view of instru- ments of precision , one of the most important new features is the astrographic equatorial , set up in 1892 and ...
... Greenwich by the extensive use of photography and the establishment of large equatorials . From the point of view of instru- ments of precision , one of the most important new features is the astrographic equatorial , set up in 1892 and ...
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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.