History of Astronomy |
From inside the book
Results 1-5 of 42
Page 7
... ever made in astronomical theory was the placing of the sun , moon , and planets at differ- ent distances from the earth instead of having same sun . 66 them stuck on the vault of heaven . It The Geometrical Period 7.
... ever made in astronomical theory was the placing of the sun , moon , and planets at differ- ent distances from the earth instead of having same sun . 66 them stuck on the vault of heaven . It The Geometrical Period 7.
Page 21
... distances from the earth , and their orbits , and the causes of their motions , he strongly objected to such a waste of valuable time . He dwelt on the contradictions and conflicting opinions of the physical philosophers , ...... and ...
... distances from the earth , and their orbits , and the causes of their motions , he strongly objected to such a waste of valuable time . He dwelt on the contradictions and conflicting opinions of the physical philosophers , ...... and ...
Page 23
... distance from the fixed earth . He called this point the excentric . The line from the earth to the " excentric " was called the line of apses . A circle having this centre I was called the equant , and he supposed that a radius drawn ...
... distance from the fixed earth . He called this point the excentric . The line from the earth to the " excentric " was called the line of apses . A circle having this centre I was called the equant , and he supposed that a radius drawn ...
Page 30
... distance of the excentric3 from the centre of the deferent , and the position of the line of apses , besides the inclination and position of the plane of the planet's orbit . The only object ever aimed at in those days was to prepare ...
... distance of the excentric3 from the centre of the deferent , and the position of the line of apses , besides the inclination and position of the plane of the planet's orbit . The only object ever aimed at in those days was to prepare ...
Page 36
... distance from the sun . The planets move in a similar way on epicycles , but their deferents have no geometrical or physical relation to the sun . The moon moves on an epicycle centred on a second epicycle , itself centred on a deferent ...
... distance from the sun . The planets move in a similar way on epicycles , but their deferents have no geometrical or physical relation to the sun . The moon moves on an epicycle centred on a second epicycle , itself centred on a deferent ...
Other editions - View all
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.