History of Astronomy |
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Page 113
SPECTRoscope Since the invention of the telescope no discovery has given so
great an impetus to astronomical physics as the spectroscope; and in giving us
information about the systems of stars and their proper motions it rivals the ...
SPECTRoscope Since the invention of the telescope no discovery has given so
great an impetus to astronomical physics as the spectroscope; and in giving us
information about the systems of stars and their proper motions it rivals the ...
Page 119
When Galileo directed his telescope to the heavens, when Secchi and Huggins
studied the chemistry of the stars by means of the spectroscope, and when
Warren De la Rue set up a photoheliograph at Kew, we see that a progress in the
same ...
When Galileo directed his telescope to the heavens, when Secchi and Huggins
studied the chemistry of the stars by means of the spectroscope, and when
Warren De la Rue set up a photoheliograph at Kew, we see that a progress in the
same ...
Page 120
Meanwhile the accumulation of facts has been prodigious, and the revelations of
the telescope and spectroscope entrancing. I 2. THE SUN One of Galileo's most
striking discoveries, when he pointed his telescope to the heavenly bodies, was ...
Meanwhile the accumulation of facts has been prodigious, and the revelations of
the telescope and spectroscope entrancing. I 2. THE SUN One of Galileo's most
striking discoveries, when he pointed his telescope to the heavenly bodies, was ...
Page 129
The spectroscope is placed with its slit in the focus of an equatorial telescope,
pointed to the sun, so that the circular image of the sun falls on the slit. At the
other end of the spectroscope is the photographic plate. Just in front of this plate
there ...
The spectroscope is placed with its slit in the focus of an equatorial telescope,
pointed to the sun, so that the circular image of the sun falls on the slit. At the
other end of the spectroscope is the photographic plate. Just in front of this plate
there ...
Page 130
... and nothing is more astonishing than to note the total want of resemblance in
the forms shown on the two. This mode of research promises to afford many new
and useful data. The spectroscope has revealed the fact that, broadly speaking, ...
... and nothing is more astonishing than to note the total want of resemblance in
the forms shown on the two. This mode of research promises to afford many new
and useful data. The spectroscope has revealed the fact that, broadly speaking, ...
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Common terms and phrases
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 |