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See also:FRIEDRICH WILHELM See also:BESSEL (1784-1846)
, See also:German astronomer, was See also:born at See also:Minden on the 22nd of See also:July 1784
.
Placed at the See also:age of fifteen in a counting-See also:house at See also:Bremen, he was impelled by his See also:desire to obtain a situation as See also:supercargo on a See also:foreign voyage to study See also:navigation, See also:mathematics and finally See also:astronomy
.
In 1804 he calculated the See also:orbit of See also:Halley's See also:comet from observations made in 1607 by See also:
In Tabulae Regiomontanae (1830), he definitively established the See also:uniform See also:system of reduction still in use
.
During the years 1821-1833, he observed all stars to the ninth magnitude in zones extending from-r5° to +45° dec., and thus raised the number of those accurately determined to about 50,000
.
He corrected the length of the seconds' pendulum in 1826, in a discussion re-published by H
.
Bruns in 1889; measured an arc of the See also:meridian in See also:East Prussia in 1831-1832; and deduced for the See also:earth in 1841 an See also:ellipticity of T4-g
.
His ascertainment in 1838 (See also:Asir
.
Nach., Nos
.
365-366) of a parallaxof 0"•31 for 61 Cygni was the first See also:authentic result of the See also:kind published
.
He announced in 1844 the binary See also:character of Sirius and Procyon from their disturbed proper motions; and was preparing to attack the problem solved later by the See also:discovery of See also:Neptune, when fatal illness intervened
.
He died at Konigsberg on the 17th of See also: L . See also:Busch appeared in vol . 24 of the same See also:series . Especial See also:attention should be directed to his Astronomische Untersuchungen (2 Vo1S . 1841—1842), Populare Vorlesungen (1848), edited by H . C . See also:Schumacher, and to the important collection entitled Abhandlungen (4 vols . 1875-1882), issued by R . Engelmann at See also:Leipzig . His See also:minor See also:treatises numbered over 350 . In pure mathematics he enlarged the resources of See also:analysis by the invention of Bessel's Functions . He made some preliminary use of these expressions in 1817, in a See also:paper on See also:Kepler's Problem (Transactions See also:Berlin .See also:Academy, 1816-1817, p . 49), and fully See also:developed them seven years later, for the purposes of a See also:research into planetary perturbations (Ibid . 1824, pp . 1-52) . See also H . Durege, Bessels Leben and Wirken (See also:Zurich, 1860; J . F . See also:Encke, Geddchtnissrede auf Bessel (Berlin, 1846) ; C . T . Anger, Erinnerung an Bessels Leben and Wirken (See also:Danzig, 1845) ; Astronomische Nachrichten, See also:xxiv . 49, 331 (1846); Monthly Notices,See also:Roy . Astr . Society, vii . 199 (1847) ; Allgemeine deutsche Biographie, Ii . 558-567 . |
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