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HUYGENS, CHRISTIAAN (1629-1695)

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Originally appearing in Volume V14, Page 22 of the 1911 Encyclopedia Britannica.
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HUYGENS, CHRISTIAAN (1629-1695) , Dutch mathematician, mechanician, astronomer and physicist, was See also:born at the See also:Hague on the 14th of See also:April 1629. He was the second son of See also:Sir Constantijn Huygens. From his See also:father he received the rudiments of his See also:education, which was continued at See also:Leiden under A. Vinnius and F. See also:van Schooten, and completed in the juridical school of See also:Breda. His mathematical See also:bent, however, soon diverted him from legal studies, and the perusal of some of his earliest theorems enabled See also:Descartes to predict his future greatness. In 1649 he accompanied the See also:mission of See also:Henry, See also:count of See also:Nassau, to See also:Denmark, and in 1651 entered the lists of See also:science as an assailant of the unsound See also:system of quadratures adopted by See also:Gregory of St See also:Vincent. This first See also:essay (Exetasis quadraturae circuli, Leiden, 1651) was quickly succeeded by his Theoremata de quadratura hyperboles, ellipsis, et circuli; while, in a See also:treatise entitled De circuli magnitudine inventa, he made, three years later, the closest approximation so far obtained to the ratio of the circumference to the See also:diameter of a circle. Another class of subjects was now to engage his See also:attention. The improvement of the See also:telescope was justly regarded as a sine qua non for the See also:advancement of astronomical knowledge. But the difficulties interposed by spherical and See also:chromatic See also:aberration had arrested progress in that direction until, in 1655, Huygens, working with his See also:brother Constantijn, See also:hit upon a new method of grinding and polishing lenses. The immediate results of the clearer See also:definition obtained were the detection of a See also:satellite to See also:Saturn (the See also:sixth in See also:order of distance from its See also:primary), and the See also:resolution into their true See also:form of the abnormal appendages to that See also:planet. Each See also:discovery in turn was, according to the prevailing See also:custom, announced to the learned See also:world under the See also:veil of an See also:anagram—removed, in the See also:case of the first, by the publication, See also:early in 1656, of the little See also:tract De Saturni See also:luna observatio nova; but retained, as regards the second, until 1659, when in the Systema Saturnium the varying appearances of the so-called " triple planet " were clearly explained as the phases of a See also:ring inclined at an See also:angle of 28° to the See also:ecliptic.

Huygens was also in 1656 the first effective observer of the See also:

Orion nebula; he delineated the See also:bright region still known by his name, and detected the multiple See also:character of its nuclear See also:star. His application of the pendulum to regulate the See also:movement of clocks sprang from his experience of the need for an exact measure of See also:time in observing the heavens. The invention See also:dates from 1656; on the 16th of See also:June 1657 Huygens presented his first " pendulum-See also:clock " to the states-See also:general; and the Horologium, containing a description of the requisite mechanism, was published in 1658. His reputation now became See also:cosmopolitan. As early as 1655 the university of See also:Angers had distinguished him with an honorary degree of See also:doctor of See also:laws. In 1663, on the occasion of his second visit to See also:England, he was elected a See also:fellow of the Royal Society, and imparted to that See also:body in See also:January 1669 a clear and concise statement of the laws governing the collision of elastic bodies. Although these conclusions were arrived at independently, and, as it would seem, several years previous to their publication, they were in See also:great measure anticipated by the communications on the same subject of See also:John See also:Wallis and See also:Christopher See also:Wren, made respectively in See also:November and See also:December 1668. Huygens had before this time fixed his See also:abode in See also:France. In 1665 See also:Colbert made to him on behalf of See also:Louis XIV. an offertoo tempting to be refused, and between the following See also:year and 1681 his See also:residence in the philosophic seclusion of the Bibliotheque du Roi was only interrupted by two See also:short visits to his native See also:country. His magnum See also:opus dates from this See also:period. The Horologium oscillatorium, published with a See also:dedication to his royal See also:patron in 1673, contained See also:original discoveries sufficient to have furnished materials for See also:half a dozen striking disquisitions. His See also:solution of the celebrated problem of the "centre of oscillation " formed in itself an important event in the See also:history of See also:mechanics.

Assuming as an See also:

axiom that the centre of gravity of any number of interdependent bodies cannot rise higher than the point from which it See also:fell, he arrived, by anticipating in the particular case the general principle of the conservation of vis viva, at correct although not strictly demonstrated conclusions. His treatment of the subject was the first successful See also:attempt to See also:deal with the See also:dynamics of a system. The determination of the true relation between the length of a pendulum and the time of its oscillation; the invention of the theory of evolutes; the discovery, hence ensuing, that the See also:cycloid is its own evolute, and is strictly isochronous; the ingenious although practically inoperative See also:idea of correcting the " circular See also:error " of the pendulum by applying cycloidal cheeks to clocks—were all contained in this remarkable treatise. The theorems on the See also:composition of forces in circular See also:motion with which it concluded formed the true prelude to See also:Newton's Principia, and would alone suffice to establish the claim of Huygens to the highest See also:rank among See also:mechanical inventors. In 1681 he finally severed his See also:French connexions, and returned to See also:Holland. The harsher See also:measures which about that time began to be adopted towards his co-religionists in France are usually assigned as the See also:motive of this step. He now devoted himself during six years to the See also:production of lenses of enormous See also:focal distance, which, mounted on high poles, and connected with the See also:eye-piece by means of a See also:cord, formed what were called " aerial telescopes." Three of his See also:object-glasses, of respectively 123, 18o and 210 ft. focal length, are in the See also:possession of the Royal Society. He also succeeded in constructing an almost perfectly achromatic eye-piece, still known by his name. But his re-searches in See also:physical See also:optics constitute his See also:chief See also:title-See also:deed to See also:immortality. Although See also:Robert See also:Hooke in 1668 and Ignace Pardies in 1672 had adopted a vibratory See also:hypothesis of See also:light, the conception was a See also:mere floating possibility until Huygens provided it with a sure See also:foundation. His powerful scientific See also:imagination enabled him to realize that all the points of a See also:wave-front originate partial waves, the aggregate effect of which is to reconstitute the primary disturbance at the subsequent stages of its advance, thus accomplishing its See also:propagation; so that each primary undulation is the envelope of an indefinite number of secondary undulations. This resolution of the original wave is the well-known " Principle of Huygens," and by its means he was enabled to prove the fundamental laws of optics, and to assign the correct construction for the direction of the extra-See also:ordinary See also:ray in uniaxial crystals.

These investigations, together with his discovery of the " wonderful phenomenon " of polarization, are recorded in his Traite de la lumiere, published at Leiden in 1690, but composed in 1678. In the appended treatise Sur la Cause de la pesanteur, he rejected See also:

gravitation as a universal quality of See also:matter, although admitting the Newtonian theory of the planetary revolutions. From his views on centrifugal force he deduced the oblate figure of the See also:earth, estimating its See also:compression, however, at little more than one-half its actual amount. Huygens never married. He died at the Hague on the 8th of June 1695, bequeathing his See also:manuscripts to the university of Leiden, and his considerable See also:property to the sons of his younger brother. In character he was as estimable as he was brilliant in See also:intellect. Although, like most men of strong originative See also:power, he assimilated with difficulty the ideas of others, his tardiness sprang rather from inability to depart from the track of his own methods than from reluctance to acknowledge the merits of his competitors. In addition to the See also:works already mentioned, his Cosmotheoros— a See also:speculation concerning the inhabitants of the See also:planets—was printed posthumously at the Hague in 1698, and appeared almost simultaneously in an See also:English See also:translation. A See also:volume entitled See also:Opera posthuma (Leiden, 1703) contained his " Dioptrica," in which the ratio between the respective focal lengths of object-See also:glass and eye-glass is given as the measure of magnifying power, together with the shorter essays De vitris figurandis, De See also:corona et parheliis, &c. An early tract De ratiociniis in ludo aleae, printed in 16J7 with Schooten's Exercitationes mathematicae, is notable as one of the first formal See also:treatises on the theory of probabilities; nor should his investigations of the properties of the See also:cissoid, logarithmic and See also:catenary curves be See also:left unnoticed. His invention of the See also:spiral See also:watch-See also:spring was explained in the See also:Journal See also:des savants (Feb. 25, 1675).

An edition of his works was published by G. J. 's Gravesande, in four See also:

quarto volumes entitled Opera See also:varia (Leiden, 1724) and Opera reliqua (See also:Amsterdam, 1728). His scientific See also:correspondence was edited by P. J. Uylenbroek from manuscripts preserved at Leiden, with the title Christiana Hugenii aliorumque seculi X VII. virorum celebrium exercitationes mathematicae et philosophicae (the Hague, 1833). The publication of a monumental edition of the letters and works of Huygens was undertaken at the Hague by the Societe Hollandaise des Sciences, with the heading Euvres de See also:Christian Huygens (1888), &c. Ten quarto volumes, comprising the whole of his correspondence, had already been issued in 1905. A See also:biography of Huygens was prefixed to his Opera varia (1724); his Eloge in the character of a French academician was printed by J. A. N. See also:Condorcet in 1773.

Consult further: P. J. Uylenbroek, Oratio de fratribus Christiano atque Constantino Hugenio (See also:

Groningen, 1838); P. Harting, See also:Christie an Huygens in zijn See also:Leven en Werken geschetzt (Groningen, 1868) ; J. B. J. See also:Delambre, Hist. de l'astronomie moderne (ii. 549); J. E. See also:Montucla, Hist. des mathematiques (ii. 84, 412, 549) ; M. See also:Chasles, Apergu historique sur l'origine des melhodes en geometric, pp.

101-109; E. See also:

Duhring, Kritische Geschichte der allgemeinen Principien der Mechanik, Abschnitt (U. 120, 163, iii. 227) ; A. See also:Berry, A Short History of See also:Astronomy, p. zoo; R. See also:Wolf, Geschichte der Astronomic, passim; Houzeau, Bibliographie astronomique (ii. 169) ; F. Kaiser, Astr. Nach. (See also:xxv. 245, 1847) ; Tijdschrift voor de Wetenschappen (i. 7, 1848) ; Allgemeine deutsche Biographic (M.

B. Cantor) ; J. C. See also:

Poggendorff, Biog. lit. Handworterbuch. (A. M.

End of Article: HUYGENS, CHRISTIAAN (1629-1695)

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