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 Olbersl--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 star,--Henderson's

measurements--Kirchhoff and Bunsen's perfection of the

spectroscope--Wonderful revelations of the spectroscope--Lord Kelvin's

estimate of the time that will be required for the earth to become

completely cooled--Alvan Clark's discovery of the companion star of

Sirius--The advent of the photographic film in astronomy--Dr. Huggins's

studies of nebulae--Sir Norman Lockyer's "cosmogonic guess,"--Croll's

pre-nebular theory.

A History of Science — Volume 3 · 第 2 / 13 章