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Johann Heinrich Lambert

 
Scientist: Johann Heinrich Lambert

German mathematician, physicist, astronomer, and philosopher (1728–1777)

Lambert, the son of a poor tailor from Mulhouse (now in France), was largely self-educated. He spent the early part of his life in various occupations, including teaching and bookkeeping, and followed his scientific interests in his spare time. In 1764 he moved to Berlin where he attracted the notice of Frederick the Great and became a member of the Berlin Academy.

Lambert contributed to numerous branches of science and learning generally. His main mathematical achievement was to prove that ‘π’ is irrational. He did this by use of continued fractions and published the proof in 1768. He also studied the hyperbolic functions and introduced their use into trigonometry. Lambert did some remarkable work in non-Euclidean geometry, but this remained totally unknown until the end of the 19th century when it was published.

In addition to mathematics Lambert was an astronomer of note. The suggestion that there might be further galaxies beyond our own was first made by him and this was subsequently confirmed observationally by William Herschel. Lambert was the first to invent an accurate way of measuring light intensities and the lambert, a measurement of light intensity, was named for him.

In his philosophical ideas Lambert largely developed the ideas of the great German rationalist philosopher Gottfried Leibniz and his chief philosophical work, Neues Organon (New Organon), was published in 1764.

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Philosophy Dictionary: Johann Heinrich Lambert
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Lambert, Johann Heinrich (1728-77) German mathematician and cosmologist. Largely self-taught, Lambert became one of the most distinguished German scientists and mathematicians of the eighteenth century. Philosophically he attempted to ally rationalism in metaphysics with the mathematical treatment of reasoning and logic, continuing the tradition of Leibniz. He was much admired by Kant.

 
Columbia Encyclopedia: Johann Heinrich Lambert
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Lambert, Johann Heinrich ('hän hīn'rĭkh läm'bĕrt), 1728-77, German-French philosopher and scientist, b. Alsace. He developed many basic concepts in mathematics, including that of the hyperbolic functions in trigonometry. In physics he achieved valuable results in work on the measurement of the intensity of light (the metric unit of brightness in the cgs system is named for him), degrees of heat, and humidity. In his philosophical work Neues Organon (1764) he pointed out the importance of beginning with experience and using the analytical method to investigate any theory of knowledge. His correspondence with Kant is of great philosophical significance. His other important books are Photometria (1760) and Pyrometrie (1779).
Wikipedia: Johann Heinrich Lambert
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Johann Heinrich Lambert

Johann Heinrich Lambert (1728-1777)
Born 26 August 1728(1728-08-26)
Mülhausen, Alsace, France
Died 25 September 1777 (aged 49)
Berlin, Prussia
Residence Germany
Nationality German
Fields Mathematician, physicist and astronomer
Known for Irrationality of π
Lambert-Beer-Bouguer Law
Religious stance Huguenot

Johann Heinrich Lambert (August 26, 1728September 25, 1777), was a Swiss mathematician, physicist and astronomer.

Contents

Biography

He was born in Mülhausen (now Mulhouse, Alsace, France; then an exclave of Switzerland).

His father was a poor tailor, so Johann had to struggle to gain an education. He first worked as a clerk in an ironworks, then gained a position in a newspaper office.

The editor recommended him as a private tutor to a family, which gave him access to a good library and provided enough leisure time in which to explore it.

In 1759 he moved to Augsburg, then in 1763 he dwelt in Berlin. In the final decade of his life he gained the sponsorship of Frederick II of Prussia, and passed the rest of his life in reasonable comfort. He died in Berlin, Prussia (today Germany).

Work

Mathematics

Lambert studied light intensity and was the first to introduce hyperbolic functions into trigonometry. Also, he made conjectures regarding non-Euclidean space. Lambert is credited with the first proof that π is irrational in 1768[1] and of several map projections in 1772, such as the Lambert cylindrical equal-area projection[2][3]. Lambert also devised theorems regarding conic sections that made the calculation of the orbits of comets simpler. The first practical hygrometer and photometer were invented by Lambert.

Lambert devised a formula for the relationship between the angles and the area of hyperbolic triangles. These are triangles drawn on a concave surface, as on a saddle, instead of the usual flat Euclidean surface. Lambert showed that the angles cannot add up to π (radians), or 180°. The amount of shortfall, called defect, is proportional to the area. The larger the triangle's area, the smaller the sum of the angles and hence the larger the defect CΔ = π — (α + β + γ). That is, the area of a hyperbolic triangle (multiplied by a constant C) is equal to π (in radians), or 180°, minus the sum of the angles α, β, and γ. Here C denotes, in the present sense, the negative of the curvature of the surface (taking the negative is necessary as the curvature of a saddle surface is defined to be negative in the first place). As the triangle gets larger or smaller, the angles change in a way that forbids the existence of similar hyperbolic triangles, as only triangles that have the same angles will have the same area. Hence, instead of expressing the area of the triangle in terms of the lengths of its sides, as in Euclid's geometry, the area of Lambert's hyperbolic triangle can be expressed in terms of its angles.

Philosophy

In his main philosophical work, New Organon (1764), Lambert studied the rules for distinguishing subjective from objective appearances. This connects with his work in the science of optics. In 1760, he published a book on light reflection in Latin, the Photometria, in which the word albedo was introduced and the Beer–Lambert law was formulated that describes the way in which light is absorbed. Lambert also wrote a classic work on perspective and also contributed to geometrical optics.

Astronomy

Lambert also developed a theory of the generation of the universe that was similar to the nebular hypothesis that Thomas Wright and Immanuel Kant had (independently) developed. Wright published his account in An Original Theory or New Hypothesis of the Universe (1750), Kant in Allgemeine Naturgeschichte und Theorie des Himmels, published anonymously in 1755. Shortly afterward, Lambert published his own version of the nebular hypothesis of the origin of the solar system in Cosmologische Briefe über die Einrichtung des Weltbaues (1761). Lambert hypothesized that the stars near the sun were part of a group which travelled together through the Milky Way, and that there were many such groupings (star systems) throughout the galaxy. The former was later confirmed by Sir William Herschel.

Notes

  1. ^ Lambert, Johann Heinrich (1761), "Mémoire sur quelques propriétés remarquables des quantités transcendentes circulaires et logarithmiques", Histoire de l'Académie, (Berlin) XVII: 265–322, 1768 
  2. ^ Mulcahy, Karen. "Cylindrical Projections". City University of New York. http://www.geo.hunter.cuny.edu/mp/cylind.html. Retrieved 2007-03-30. 
  3. ^ Lambert, Johann Heinrich (1772). "Anmerkungen und Zusätze zur Entwerfung der Land- und Himmelscharten. Von J. H. Lambert (1772.) Hrsg. von A. Wangerin. Mit 21 Textfiguren." (xml). W. Engelmann, reprint 1894. http://name.umdl.umich.edu/ABR2581.0001.001. Retrieved 2007-04-10. 

References

  • A Short Account of the History of Mathematics, W. W. Rouse Ball, 1908.
  • Asimov's Biographical Encyclopedia of Science and Technology, Isaac Asimov, Doubleday & Co., Inc., 1972, ISBN 0-385-17771-2.

See also

External links


 
 

 

Copyrights:

Scientist. A Dictionary of Scientists. Copyright © Market House Books Ltd 1993, 1999, 2003. All rights reserved.  Read more
Philosophy Dictionary. The Oxford Dictionary of Philosophy. Copyright © 1994, 1996, 2005 by Oxford University Press. All rights reserved.  Read more
Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2003, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/ Read more
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