History of Astronomy |
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Page 136
Since then we have the charts of Schröter, Beer and Mädler (1837), and of
Schmidt, of Athens (1878); and, above all, the photographic atlas by Loewy and
Puiseux. The details of the moon's surface require for their discussion a whole
book, ...
Since then we have the charts of Schröter, Beer and Mädler (1837), and of
Schmidt, of Athens (1878); and, above all, the photographic atlas by Loewy and
Puiseux. The details of the moon's surface require for their discussion a whole
book, ...
Page 146
... by the examination of photographic plates at the Lick Observatory in 1905,
since which time they have been continuously photographed, and their orbits
traced, at Greenwich. On examining these plates in 1908 Mr. Melotte detected the
...
... by the examination of photographic plates at the Lick Observatory in 1905,
since which time they have been continuously photographed, and their orbits
traced, at Greenwich. On examining these plates in 1908 Mr. Melotte detected the
...
Page 151
The discovery of Eros and the photographic attack upon its path have been
described in their relation to finding the sun's distance. A group of four asteroids
has lately been found, with a mean distance and period equal to that of Jupiter.
The discovery of Eros and the photographic attack upon its path have been
described in their relation to finding the sun's distance. A group of four asteroids
has lately been found, with a mean distance and period equal to that of Jupiter.
Page 164
When Huggins first applied the Döppler principle to measure velocities in the line
of sight,” the faintness of star spectra diminished the accuracy; but Vögel, in 1888,
overcame this to a great extent by long exposures of photographic plates.
When Huggins first applied the Döppler principle to measure velocities in the line
of sight,” the faintness of star spectra diminished the accuracy; but Vögel, in 1888,
overcame this to a great extent by long exposures of photographic plates.
Page 177
The result was such a display of sharp star images that he resolved on the Cape
Photographic Durchmusterung, which after fourteen years, By kind permission of
Sir David Gill. From this photograph originated all stellar chart-photography. with
...
The result was such a display of sharp star images that he resolved on the Cape
Photographic Durchmusterung, which after fourteen years, By kind permission of
Sir David Gill. From this photograph originated all stellar chart-photography. with
...
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accurate Airy ancient Astronomer Royal astronomical units bright calculations Cape catalogue centre century Chaldaeans 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 Huggins instruments JOHANNEs KEPLER John Herschel Jupiter Jupiter's Kepler Laplace Lick Observatory light line of apses line of sight lunar Mars mathematical mean distance measured ment Mercury meteor miles a second moon nebulae Newton º º 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.
Bibliographic information
| Title | History of Astronomy Hist. of sci. series History of the sciences |
| Author | George Forbes |
| Publisher | Putnam, 1909 |
| Original from | the University of California |
| Digitized | 29 Nov 2007 |
| Length | 200 pages |
| Export Citation | BiBTeX EndNote RefMan |