Joseph von Fraunhofer

This page was last edited on 7 December 2017, at 21:01.

Joseph Ritter von Fraunhofer (6 March 1787 – 7 June 1826) was a Bavarian physicist and optical lens manufacturer. He made optical glass and achromatic telescope objective lenses, invented the spectroscope, and developed diffraction grating. He also discovered and studied the dark absorption lines in the spectrum of the sun now known as Fraunhofer lines.

Joseph von Fraunhofer
Joseph v Fraunhofer.jpg
Born 6 March 1787
Straubing, Electorate of Bavaria
Died 7 June 1826 (aged 39)
Munich, German Confederation

Biography

Joseph Fraunhofer was born in Straubing, in the Electorate of Bavaria, to Franz Xaver Fraunhofer and Maria Anna Frohlich.[1] He was orphaned at the age of 11 and 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 Prince-Elector Maximilian 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, Utzschneider and Georg von Reichenbach brought Fraunhofer into their Institute at Benediktbeuern, a secularised Benedictine monastery devoted to glass making. There he discovered how to make the world's finest optical glass for that time and invented precise methods for measuring dispersion.

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

His illustrious career eventually earned him an honorary doctorate from the University of Erlangen in 1822. In 1824, Fraunhofer was appointed an Knight of the Order of Merit of the Bavarian Crown by King Maximilian I, through which he was raised into personal nobility (with the title "Ritter von", i.e. knight). The same year, he was also made an honorary citizen of Munich.

Like many glassmakers of his era, he was poisoned by heavy metal vapors, resulting in his premature death. Fraunhofer died 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 during the time period was to polish the spherical surfaces of large object glasses accurately. Fraunhofer invented the 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, which he always found to be injured by flaws and irregularities of various sorts.[4]

In 1811, he constructed a new kind of furnace, and during his second melting session when he melted a large quantity of glass, he found that he could produce flint glass, which, when taken from the bottom of a vessel containing roughly 224 pounds 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 which tended to cause irregular refraction. In the thicker and larger glasses, there would be even 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]

It was thought that the cause that prevented the accurate determination of power of a given medium to refract rays of light and separate the different colors which they contain was chiefly due to the colors of the spectrum having 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 debunk 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 spectroscope.JPG
Fraunhofer demonstrating the spectroscope.

Thus in 1814, Fraunhofer invented the spectroscope. In the course of his experiments, he discovered a 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 orange as the line produced by the orange of fire light led him to the discovery of 574 dark fixed lines in the solar spectrum. Today, 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".[11]

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 to Dorpat Observatory), and the Bessel Heliometer (delivered posthumously), which were both used to collect data for stellar parallax. The firm's successor, Merz und Mahler, made a telescope for the New Berlin Observatory, which confirmed the existence of the major planet Neptune. Possibly the last telescope objective made by Fraunhofer was supplied for a transit telescope at the City Observatory, Edinburgh,[12] the telescope itself being completed by Repsold of Hamburg after Fraunhofer's death.

Works

See also

Notes

  1. ^ Hockey, Thomas (2009). The Biographical Encyclopedia of Astronomers. Springer Publishing. ISBN 978-0-387-31022-0. Retrieved August 22, 2012.
  2. ^ Ralf Kern: Wissenschaftliche Instrumente in ihrer Zeit. Band 4: Perfektion von Optik und Mechanik. Cologne, 2010. 355-356.
  3. ^ a b c "Fraunhofer, Joseph von (1787 - 1826)". plicht.de. Retrieved 26 March 2011. (in English)
  4. ^ a b c d e Wikisource-logo.svg This article incorporates text from a publication now in the public domainRines, George Edwin, ed. (1920). "Fraunhofer, Joseph von". Encyclopedia Americana.
  5. ^ See:
  6. ^ See:
    • Gustav Kirchhoff (1859) "Ueber die Fraunhofer'schen Linien" (On Fraunhofer's lines), Monatsbericht der Königlichen Preussische Akademie der Wissenschaften zu Berlin (Monthly report of the Royal Prussian Academy of Sciences in Berlin), 662-665.
    • Gustav Kirchhoff (1859) "Ueber das Sonnenspektrum" (On the sun's spectrum), Verhandlungen des naturhistorisch-medizinischen Vereins zu Heidelberg (Proceedings of the Natural History / Medical Association in Heidelberg), 1 (7) : 251-255.
  7. ^ William Hyde Wollaston (1802) "A method of examining refractive and dispersive powers, by prismatic reflection," Philosophical Transactions of the Royal Society, 92: 365-380; see especially p. 378.
  8. ^ See:
  9. ^ Parker AR (March 2005). "A geological history of reflecting optics". Journal of the Royal Society, Interface. 2 (2): 1–17. doi:10.1098/rsif.2004.0026. PMC 1578258Freely accessible. PMID 16849159.
  10. ^ Fraunhofer (1814-1815), pages 220-221 : Original : Ich habe auch mit derselben Vorrichtung Versuche mit dem Lichte einiger Fixsterne erster Grösse gemachte. Da aber das Licht dieser Sterne noch vielmal schwächer ist, als das der Venus, so ist natürlich auch die Helligkeit des Farbenbildes vielmal geringer. Demohngeachtet habe ich, ohne Täuschung, im Farbenbilde vom Lichte des Sirius drey breite Streifen gesehen, die mit jenen vom Sonnenlichte keine Aehnlichkeit zu haben scheinen; einer dieser Streifen ist im Grünen, und zwey im Blauen. Auch im Farbenbilde vom Lichte anderer Fixsterne erster Grösse erkennt man Streifen; doch scheinen diese Sterne, in Beziehung auf die Streifen, unter sich verschieden zu seyn. Translation : With the same device [i.e., spectroscope], I've also made some experiments on the light of some stars of the first magnitude. Since the light of these stars is many times weaker than that of Venus, so naturally, the brightness of the spectrum is also many times less. Notwithstanding, I have seen -- without any illusion -- three broad stripes in the spectrum of Sirius, which seem to have no similarity to those of sunlight; one of these stripes is in the green, and two in the blue. Also, in the spectrum of the light of other fixed stars of the first magnitude, one detects stripes; yet these stars, in regard to the stripes, seem to differ among themselves.
  11. ^ Prismatic and Diffraction Spectra: Memoirs (1899) Tr. & Ed. J. S. Ames p. 10
  12. ^ A Guide to Edinburgh's Popular Observatory, Astronomical Society of Edinburgh
  13. ^ Tr. Brief outline of the life-story of Dr. Joseph von Fraunhofer

References

  • I. Bernard Cohen; Henry Crew; Joseph von Fraunhofer; De Witt Bristol Brace (1981). The Wave theory, light and spectra. Ayer Publishing. ISBN 0-405-13867-9.
  • Aller, Lawrence H. (1991). Atoms, Stars and Nebulae, 3rd ed. Cambridge University Press. ISBN 0-521-32512-9.
  • Klaus Hentschel: Mapping the spectrum. Techniques of visual representation in research and teaching. Oxford Univ. Press, Oxford 2002.
  • 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

This page is based on a Wikipedia article written by authors (here).
Text is available under the CC BY-SA 3.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.