Jump to content

Johann Heinrich Lambert: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
m Reverting possible vandalism by 187.74.184.199 to version by Yobot. False positive? Report it. Thanks, ClueBot NG. (1282436) (Bot)
added influences
Line 16: Line 16:
| doctoral_students = <!--please insert-->
| doctoral_students = <!--please insert-->
| known_for = [[Irrational number|Irrationality of]] [[pi|π]]</br>
| known_for = [[Irrational number|Irrationality of]] [[pi|π]]</br>
|influences = [[Aristotle]], [[Francis Bacon|Bacon]], [[Christian Wolff (philosopher)|Wolff]]
|influenced = [[Kant]], [[Mendelssohn]]
[[Beer-Lambert law|Lambert-Beer-Bouguer Law]]</br>
[[Beer-Lambert law|Lambert-Beer-Bouguer Law]]</br>
[[Transverse Mercator projection]]
[[Transverse Mercator projection]]

Revision as of 20:36, 18 October 2012

Johann Heinrich Lambert
Johann Heinrich Lambert (1728–1777)
Born(1728-08-26)26 August 1728
Republic of Mulhouse, Independent city-state (currently Alsace, France)
Died25 September 1777(1777-09-25) (aged 49)
Berlin, Prussia
NationalitySwiss
Known forIrrationality of π
Scientific career
FieldsMathematician, physicist and astronomer

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

Asteroid 187 Lamberta was named in his honour.

Biography

Lambert was born in 1728 in the city of Mulhouse (now in Alsace, France), at that time an exclave of Switzerland. Leaving school he continued to study in his free time whilst undertaking a series of jobs. These included assistant to his father (a tailor), a clerk at a nearby iron works, a private tutor, secretary to the editor of Basler Zeitung and, at the age of 20, private tutor to the sons of Count Salis in Chur. Travelling Europe with his charges (1756–1758) allowed him to meet established mathematicians in the German states, The Netherlands, France and the Italian states. On his return to Chur he published his first books (on optics and cosmology) and began to seek an academic post. After a few short posts he was rewarded (1764) by an invitation from Euler to a position at the Prussian Academy of Sciences in Berlin, where he gained the sponsorship of Frederick II of Prussia. In this stimulating, and financially stable, environment he worked prodigiously until his death in 1777.

Work

Mathematics

Lambert 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 (although it is speculated that Aryabhata was the first to hint at that, in 500 CE[1]).[2] Lambert also devised theorems regarding conic sections that made the calculation of the orbits of comets simpler.

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.

Map projection

Lambert was the first mathematician to address the general properties of map projections. In particular he was the first to discuss the properties of conformality and equal area preservation and to point out that they were mutually exclusive. (Snyder 1993[3] p77). In 1772 Lambert published[4][5] seven new map projections under the title Anmerkungen und Zusätze zur Entwerfung der Land- und Himmelscharten, (translated as Notes and Comments on the Composition of Terrestrial and Celestial Maps by Waldo Tobler (1972)[6]). Lambert did not give names to any of his projections but they are now known as:

  1. Lambert conformal conic
  2. Transverse Mercator
  3. Lambert azimuthal equal area
  4. Lagrange projection
  5. Lambert cylindrical equal area
  6. Transverse cylindrical equal area
  7. Lambert conical equal area

The first three of these are of great importance.[3] Further details may be found at map projections and in several texts.[3][7][8]

Physics

Lambert invented the first practical hygrometer. In 1760, he published a book on illumination, the Photometria, which was based on three assumptions, the illumination was proportional to the strength of the source, inversely proportional to the square of the distance of the illuminated surface and the sine of the angle of inclination of the light's direction to that of the surface. These assumptions were supported by experiments involving the visual comparison of illuminations and used for the calculation of illumination. In Photometria Lambert also formulated the law of light absorption—the Beer–Lambert law) and introduced the term albedo.[9] He wrote a classic work on perspective and contributed to geometrical optics. The photometric unit lambert is named in recognition of his work in establishing the study of photometry.

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 1765 he began corresponding with Immanuel Kant who intended to dedicate to him the Critique of Pure Reason but the work was delayed, appearing after his death.[10]

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.

Logic

Johann-Heinrich Lambert is the author of a treatise on logic, which he called Neues Organon, that is to say, the New Organon. The most recent edition of this work named after Aristotle's Organon was issued in 1990 by the Akademie-Verlag of Berlin. To say nothing of the fact that in it one has the first appearance of the term phenomenology, one can find therein a very pedagogical presentation of the various kinds of syllogism. In A System of Logic Ratiocinative and Inductive, John-Stuart Mill expresses his admiration for Johann Heinrich Lambert.

Notes

  1. ^ S. Balachandra Rao (1994/1998). Indian Mathematics and Astronomy: Some Landmarks. Jnana Deep Publications. ISBN 81-7371-205-0. {{cite book}}: Check date values in: |year= (help); Unknown parameter |address= ignored (|location= suggested) (help)CS1 maint: year (link)
  2. ^ Lambert, Johann Heinrich (1762). "Mémoire sur quelques propriétés remarquables des quantités transcendentes circulaires et logarithmiques". Histoire de l'Académie. XVII. Berlin (published 1768): 265–322.
  3. ^ a b c Snyder, John P. (1993). Flattening the Earth: Two Thousand Years of Map Projections. University of Chicago Press. ISBN 0-226-76747-7..
  4. ^ Lambert, Johann Heinrich. 1772. Ammerkungen und Zusatze zurder Land und Himmelscharten Entwerfung. In Beitrage zum Gebrauche der Mathematik in deren Anwendung, part 3, section 6).
  5. ^ 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. Retrieved 2007-04-10. {{cite web}}: Cite has empty unknown parameter: |coauthors= (help)
  6. ^ Tobler, Waldo R, Notes and Comments on the Composition of Terrestrial and Celestial Maps, 1972. (University of Michigan Press), reprinted (2010) by Esri: [1].
  7. ^ Snyder, John P. (1987). Map Projections - A Working Manual. U.S. Geological Survey Professional Paper 1395. United States Government Printing Office, Washington, D.C.This paper can be downloaded from USGS pages.
  8. ^ Mulcahy, Karen. "Cylindrical Projections". City University of New York. Retrieved 2007-03-30. {{cite web}}: Cite has empty unknown parameter: |coauthors= (help)
  9. ^ Mach, Ernst (2003). The Principles of Physical Optics. Dover. pp. 14–20. ISBN 0-486-49559-0.
  10. ^ O'Leary M., Revolutions of Geometry, London:Wiley, 2010, p.385

See also

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.
Wikimedia Commons has media related to Johann Heinrich Lambert.

Template:Persondata

Retrieved from "https://en.wikipedia.org/w/index.php?title=Johann_Heinrich_Lambert&oldid=518579391"