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HENRY KATER (1777-1835)

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Originally appearing in Volume V15, Page 695 of the 1911 Encyclopedia Britannica.
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HENRY See also:KATER (1777-1835)  , See also:English physicist of See also:German descent, was See also:born at See also:Bristol on the 16th of See also:April 1777 . At first he purposed to study See also:law; but this he abandoned on his See also:father's See also:death in 1794, and entered the See also:army, obtaining a See also:commission in the 12th See also:regiment of See also:foot, then stationed in See also:India, where he rendered valuable assistance in the See also:great trigonometrical survey . Failing See also:health obliged him to return to See also:England; and in 1808, being then a See also:lieutenant, he entered on a distinguished student career in the See also:senior See also:department of the Royal Military See also:College at See also:Sandhurst . Shortly after he was promoted to the See also:rank of See also:captain . In 1814 he retired on See also:half-pay, and devoted the See also:remainder of his See also:life to scientific See also:research . He died at See also:London on the 26th of April 1835 . His first important contribution to scientific knowledge was the comparison of the merits of the Cassegrainian and Gregorian telescopes, from which (Phil . Trans., 1813 and 1814) he deduced that the See also:illuminating See also:power of the former exceeded that of the latter in the proportion of 5 : 2 . This inferiority of the Gregorian he explained as being probably due to the mutual interference of the rays as they crossed at the See also:principal See also:focus before reflection at the second See also:mirror . His most valuable See also:work was the determination of the length of the second's pendulum, first at London and subsequently at various stations throughout the See also:country (Phil . Trans., 1818, 1819) . In these researches he skilfully took See also:advantage of the well-known See also:property of See also:reciprocity between the centres of suspension and oscillation of an oscillating See also:body, so as to determine experimentally the precise position of the centre of oscillation; the distance between these centres was then the length of the ideal See also:simple pendulum having the same See also:time of oscillation .

As the inventor of the floating collimator, See also:

Kater rendered a great service to See also:practical See also:astronomy (Phil . Trans., 1825, 1828) . He also published See also:memoirs (Phil . Trans., 1821, 1831) on See also:British See also:standards of length and See also:mass; and in 1832 he published an See also:account of his labours in verifying the See also:Russian standards of length . For his services to See also:Russia in this respect he received in 1814 the decoration of the See also:order of St . See also:Anne; and the same See also:year he was elected a See also:fellow of the Royal Society . His See also:attention was also turned to the subject of See also:compass needles, his Bakerian lecture " On the Best See also:Kind of See also:Steel and See also:Form for a Compass See also:Needle" (Phil . Trans., 1821) containing the results of many experiments . The See also:treatise on " See also:Mechanics " in See also:Lardner's Cyclopaedia was partly written by him; and his See also:interest in more purely astronomical questions was evidenced by two communications to the Astronomical Society's Memoirs for 1831–1833—the one on an observation of See also:Saturn's See also:outer See also:ring, the other on a method of determining See also:longitude by means of lunar eclipses .

End of Article: HENRY KATER (1777-1835)
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