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Joseph von Fraunhofer

Joseph von Fraunhofer
Born (1787-03-06)6 March 1787
Straubing, Bavaria
Died 7 June 1826(1826-06-07) (aged 39)

Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.

He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.

Contents

  • Early life 1
  • Career 2
    • Early career 2.1
    • 1990s 2.2
    • 2000s 2.3
    • 2010s 2.4
  • Business activities 3
  • Personal life 4
    • Relationships and children 4.1
    • Religious views 4.2
  • Political views 5
  • Military interests 6
  • Controversy 7
    • Comments at playoffs 7.1
  • Cultural references 8
  • Filmography 9
  • Discography 10
  • Awards and honors 11
  • See also 12
  • References 13
  • External links 14

Biography

Fraunhofer was born in Straubing, Bavaria, to Franz Xaver Fraunhofer and Maria Anna Frohlich.[1] He became an orphan at the age of 11, and he started working as an apprentice to a harsh glassmaker named Philipp Anton Weichelsberger. In 1801, the workshop in which he was working collapsed and he was buried in the rubble. The rescue operation was led by Maximilian IV Joseph, Prince Elector of Bavaria (the future Maximilian I Joseph). The prince entered Fraunhofer's life, providing him with books and forcing his employer to allow the young Fraunhofer time to study.

Joseph Utzschneider was also at the site of the disaster, a fact which turned out to be important. With the money given to him by the Prince upon his rescue and the support he received from Utzschneider, Fraunhofer was able to continue his education alongside his practical training.[2] In 1806 Utzscheider and Benediktbeuern, a secularised Benedictine monastery devoted to glass making. There he discovered how to make the world's finest optical glass and invented incredibly precise methods for measuring dispersion.

It was at the Institute that Fraunhofer met Pierre Louis Guinand, a Swiss glass technician, who Utzschneider had introduce Fraunhofer to the secrets of glass making.[3] In 1809 the mechanical part of the Optical Institute was chiefly under Fraunhofer's direction, and that same year he became one of the members of the firm.[4] In 1814, Guinand left the firm, as did Reichenbach, and Fraunhofer became a partner in the firm,[3] the name being changed to Utzschneider und Fraunhofer. In 1818, he became the director of the Optical Institute. Due to the fine optical instruments he had developed, Bavaria overtook England as the centre of the optics industry. Even the likes of Michael Faraday were unable to produce glass that could rival Fraunhofer's.

His illustrious career eventually earned him an honorary doctorate from the University of Erlangen in 1822. In 1824, he was awarded the Merit Order of the Bavarian Crown (through which he was ennobled), and made an honorary citizen of Munich. Like many glassmakers of his era who were poisoned by heavy metal vapours, Fraunhofer died young, in 1826 at the age of 39. His most valuable glassmaking recipes are thought to have gone to the grave with him.

Invention and scientific research

One of the most difficult operations of practical optics was to polish the spherical surfaces of large object glasses accurately. Fraunhofer invented a machine which rendered the surface more accurately than traditional grinding. He also invented other grinding and polishing machines, and introduced many improvements into the manufacture of the different kinds of glass used for optical instruments, and which he found to be always injured by flaws and irregularities of various sorts.[4]

In 1811 he constructed a new kind of furnace, and on the second occasion when he melted a large quantity found that he could produce flint glass, which, taken from the bottom of a vessel containing two hundredweight of glass, had the same refractive power as glass taken from the surface. He found that the English crown glass and the German table glass both contained defects occasioning irregular refraction. In the thicker and larger glasses, there would be more of such defects, so that in larger telescopes this kind of glass would not be fit for object glasses. Fraunhofer therefore made his own crown glass.[4]

The cause which had hitherto prevented the accurate determination of the power of a given medium to refract the rays of light and separate the different colors which they contain was chiefly the circumstance that the colors of the spectrum have no precise limits, and that the transition from one to another is gradual and not immediate; hence, the angle of refraction could not be accurately measured. To obviate this, Fraunhofer made a series of experiments for the purpose of producing homogeneous light artificially, and unable to effect his object in a direct way, he did so by means of lamps and prisms.[4]

Fraunhofer demonstrating the spectroscope.

Thus in 1814, Fraunhofer invented the spectroscope. In the course of his experiments he discovered the bright fixed line which appears in the orange color of the spectrum when it is produced by the light of fire. This line enabled him afterward to determine the absolute power of refraction in different substances. Experiments to ascertain whether the solar spectrum contained the same bright line in the orange as that produced by the light of fire led him to the discovery of 574 dark fixed lines in the solar spectrum; millions of such fixed absorption lines are now known.[4][5]

These dark fixed lines were later shown to be atomic absorption lines, as explained by Kirchhoff and Bunsen in 1859.[6] These lines are still called Fraunhofer lines in his honor; his discovery had gone far beyond the half-dozen apparent divisions in the solar spectrum that had previously been noted by Wollaston in 1802.[7]

Fraunhofer also developed a diffraction grating in 1821, which occurred after James Gregory discovered the principles of diffraction grating and after American astronomer David Rittenhouse invented the first man-made diffraction grating in 1785.[8][9] Fraunhofer found out that the spectra of Sirius and other first-magnitude stars differed from the sun and from each other, thus founding stellar spectroscopy.[10]

Ultimately, however, his primary passion was still practical optics, once noting that "In all my experiments I could, owing to lack of time, pay attention to only those matters which appeared to have a bearing upon practical optics".

Telescopes and optical instruments

Fraunhofer produced various optical instruments including microscopes for his firm.[3] This included the Fraunhofer Dorpat Refractor used by Struve (delivered 1824), and the Bessel Repsold of Hamburg after Fraunhofer's death.

See also

Further reading

  • Prismatic and diffraction spectra: memoirs. By Joseph von Fraunhofer, William Hyde Wollaston. American Book Co., 1899.
  • Kurzer Umriß der Lebens-Geschichte des Herrn Dr. Joseph von Fraunhofer.[12] By Joseph von Utzschneider. Rösl, 1826.

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References

  • I. Bernard Cohen, Henry Crew, Joseph von Fraunhofer, De Witt Bristol Brace (1981). The Wave theory, light and spectra. Ayer Publishing.  
  • Aller, Lawrence H. (1991). Atoms, Stars and Nebulae, 3rd ed.  
  • Jackson, Myles W. (2000). Spectrum of Belief: Joseph von Fraunhofer and the Craft of Precision Optics. MIT Press.  (German translation: Fraunhofers Spektren: Die Präzisionsoptik als Handwerkskunst, Wallstein Verlag, 2009.)
  • Ralf Kern: Wissenschaftliche Instrumente in ihrer Zeit. Band 4: Perfektion von Optik und Mechanik. Cologne, 2010.

External links

  • Biography of Joseph von Fraunhofer
  • Catholic Encyclopedia article on Joseph von Fraunhofer
  • Fraunhofer.de Joseph von Fraunhofer
  • microscope by Utzschneider and Fraunhofer in Munich, made in 1820
  • telescope by Utzschneider and Fraunhofer
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