History of Science, a — Volume 3 by Henry Smith Williams;Edward Huntington Williams
page 2 of 354 (00%)
page 2 of 354 (00%)
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The work of Johannes Hevelius--Halley and Hevelius--Halley's
observation of the transit of Mercury, and his method of determining the parallax of the planets--Halley's observation of meteors--His inability to explain these bodies--The important work of James Bradley--Lacaille's measurement of the arc of the meridian--The determination of the question as to the exact shape of the earth--D'Alembert and his influence upon science- -Delambre's History of Astronomy--The astronomical work of Euler. CHAPTER II. THE PROGRESS OF MODERN ASTRONOMY The work of William Herschel--His discovery of Uranus--His discovery that the stars are suns--His conception of the universe--His deduction that gravitation has caused the grouping of the heavenly bodies--The nebula, hypothesis, --Immanuel Kant's conception of the formation of the world--Defects in Kant's conception--Laplace's final solution of the problem--His explanation in detail--Change in the mental attitude of the world since Bruno--Asteroids and satellites--Discoveries of Olbers1--The mathematical calculations of Adams and Leverrier--The discovery of the inner ring of Saturn--Clerk Maxwell's paper on the stability of Saturn's rings--Helmholtz's conception of the action of tidal friction--Professor G. H. Darwin's estimate of the consequences of tidal action--Comets and meteors--Bredichin's cometary theory--The final solution of the structure of comets--Newcomb's estimate of the amount of cometary dust swept up daily by the earth--The fixed stars--John Herschel's studies of double stars--Fraunhofer's perfection of the refracting telescope--Bessel's measurement of the parallax of a |
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