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JOSEPH VON FRAUNHOFER (1787-1826)

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Originally appearing in Volume V11, Page 43 of the 1911 Encyclopedia Britannica.
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JOSEPH VON See also:FRAUNHOFER (1787-1826)  , See also:German optician and physicist, was See also:born at See also:Straubing in See also:Bavaria on the 6th of See also:March 1787, the son of a glazier who died in 1798 . He was apprenticed in 1799 to Weichselberger, a See also:glass-polisher and looking-glass maker . On the 21st of See also:July 18o1 he nearly lost his See also:life by the fall of the See also:house in which he lodged, and the elector of Bavaria, See also:Maximilian See also:Joseph, who was See also:present at his extrication from the ruins, gave him 18 ducats . With a portion of this sum he obtained See also:release from the last six months of his See also:apprenticeship, and with the See also:rest he See also:purchased a glass-polishing See also:machine . He now employed himself in making See also:optical glasses, and in See also:engraving on See also:metal, devoting his spare See also:time to the perusal of See also:works on See also:mathematics and See also:optics . In 18o6 he obtained the See also:place of optician in the mathematical See also:institute which in 1804 had been founded at See also:Munich by Joseph von Utzschneider, G . See also:Reichenbach and J . Liebherr; and in 1807 arrangements were made by Utzschneider for his instruction by See also:Pierre See also:Louis Guinand, a skilled optician, in the fabrication of See also:flint and See also:crown glass, in. which he soon became an See also:adept (see R . See also:Wolf, Gesch. der Wissensch. in Deutschl. bd. xvi. p . 586) . With Reichenbach and Utzschneider, See also:Fraunhofer established in 1809 an optical institute at Benedictbeuern, near Munich, of which he in 1818 became See also:sole manager . The institute was in 1819 removed to Munich, and on Fraunhofer's See also:death came under the direction of G .

Merz . Amongst the earliest See also:

mechanical contrivances of Fraunhofer was a machine for polishing mathematically See also:uniform spherical surfaces . He was the inventor of the See also:stage-See also:micrometer, and of a See also:form of See also:heliometer; and in 1816 he succeeded in constructing for the See also:microscope achromatic glasses of See also:long See also:focus, consisting of a single See also:lens, the constituent glasses of which were in juxtaposition, but not cemented together . The See also:great reflecting See also:telescope at Dorpat was manufactured by him, and so great was the skill he attained in the making of lenses for achromatic telescopes that, in a See also:letter to See also:Sir See also:David See also:Brewster, he expressed his willingness to furnish an achromatic glass of 18 in. See also:diameter . Fraunhofer is especially known for the researches, published in the Denkschriften der Miinchener Akademie for 1814-1815, by which he laid the See also:foundation of See also:solar and stellar See also:chemistry . The dark lines of the spectrum of sunlight, earliest noted by Dr W . H . See also:Wollaston (Phil . Trans., 1802, p . 378), were independently discovered, and, by means of the telescope of a See also:theodolite, between which and a distant slit admitting the See also:light a See also:prism was interposed, were for the first time carefully observed by Fraunhofer, and have on that See also:account been designated " Fraunhofer's lines." He constructed a See also:map of as many as 576 of these lines, the See also:principal of which he denoted by the letters of the See also:alphabet from A to G; and by ascertaining their refractive indices he determined that their relative positions are See also:constant, whether in spectra produced by the See also:direct rays of the See also:sun, or by the reflected light of the See also:moon and See also:planets . The spectra of the stars he obtained by using, outside the See also:object-glass of his telescope, a large prism, through which the light passed to be brought to a focus in front of the See also:eye-piece . He showed that in the spectra of the fixed stars many of the dark lines were different from those of the solar spectrum, whilst other well-known solar lines were wanting; and he concluded that it was not by any See also:action of the terrestrial See also:atmosphere upon the light passing through it that the lines were produced .

He further expressed the belief that the dark lines D of the solar spectrum coincide with the See also:

bright lines of the See also:sodium See also:flame . He was also the inventor of the diffraction grating . In 1823 he was appointed See also:conservator of the See also:physical See also:cabinet at Munich, and in the following See also:year he received from the See also:king of Bavaria the See also:civil See also:order of merit . He died at Munich on the 7th of See also:June 1826, and was buried near Reichenbach, whose decease had taken place eight years previously . On his See also:tomb is the inscription " Approximavit sidera." See J. von Utzschneider, Kurzer Umriss der Lebensgeschichte See also:des See also:Hearn Dr J. von Fraunhofer (Munich, 1826) ; and G .

End of Article: JOSEPH VON FRAUNHOFER (1787-1826)
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