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Johann Heinrich Lambert

Johann Heinrich Lambert is a mathematics topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Johann Heinrich Lambert rather than just read about it. In short: Johann Heinrich Lambert (German: [ˈlambɛʁt]; French: Jean-Henri Lambert; 26 or 28 August 1728 – 25 September 1777) was an Alsatian polymath from the Republic of Mulhouse—then an associate of the Swiss Confederacy—who made fundamental contributions to mathematics, physics (particularly optics), philosophy, astronomy, and map projections. Biography Lambert was born in 1728 into a Huguenot family in the city-state of M…

Johann Heinrich Lambert — main illustration
Johann Heinrich Lambert — illustration

Key takeaways

  • Johann Heinrich Lambert belongs to mathematics; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Johann Heinrich Lambert to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Johann Heinrich Lambert from memory before moving on to harder problems.

Reference excerpt

Johann Heinrich Lambert (German: [ˈlambɛʁt]; French: Jean-Henri Lambert; 26 or 28 August 1728 – 25 September 1777) was an Alsatian polymath from the Republic of Mulhouse—then an associate of the Swiss Confederacy—who made fundamental contributions to mathematics, physics (particularly optics), philosophy, astronomy, and map projections.

Biography Lambert was born in 1728 into a Huguenot family in the city-state of Mulhouse (in modern-day Alsace, France), which was allied to the Swiss Confederacy. His family had fled from Lorraine following the Thirty Years War. Historical sources differ on his exact date of birth, citing either 26 or 28 August. Forced to leave school at age twelve due to financial constraints, Lambert pursued an exhaustive course of self-study during his free time while maintaining various jobs. In his youth, he worked as an assistant to his father (a tailor), a clerk at a local ironworks, a private tutor, and a secretary to the editor of the Basler Zeitung. At age twenty, he secured a position as private tutor to the sons of Count Salis in Chur, Switzerland. Between 1756 and 1758, Lambert traveled extensively across Europe with his pupils, affording him the opportunity to connect with established mathematicians and intellectuals throughout the German states, the Netherlands, France, and the Italian states. Upon returning to Chur, he published his first major treatises on optics and cosmology and began seeking a formal academic appointment. Following several short-term positions, Lambert's growing reputation earned him an invitation in 1763 to join the Prussian Academy of Sciences in Berlin. Supported by Frederick II of Prussia and working alongside Leonhard Euler, he spent his remaining years in this intellectually stimulating and financially secure environment, producing a prolific volume of work until his death in 1777.

Work

Mathematics

Lambert was the first to systematize and popularize the use of hyperbolic functions into trigonometry. He credits the previous works of Vincenzo Riccati and Daviet de Foncenex. Lambert developed exponential expressions and identities and introduced the modern notation. Lambert also made conjectures about non-Euclidean space. Lambert is credited with the first proof that π is irrational using a generalized continued fraction for the function tan x. Euler believed the conjecture but could not prove that π was irrational, and it is speculated that Aryabhata also believed this, in 500 CE. Lambert also devised theorems about 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 added up to less than π (radians), or 180°. The defect (amount of shortfall) increases with area. The larger the triangle's area, the smaller the sum of the angles and hence the larger the defect C△ = π — (α + β + γ). That is, the area of a hyperbolic triangle (multiplied by a constant C) is equal to π (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 by definition negative). 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 the area of the triangle's being expressed in terms of the lengths of its sides, as in Euclidean 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 (of a spherical Earth). 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 p77). In 1772, Lambert published 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)). Lambert did not give names to any of his projections but they are now known as:

Lambert conformal conic Transverse Mercator Lambert azimuthal equal area Lagrange projection Lambert cylindrical equal area Transverse cylindrical equal area Lambert conical equal area The first three of these are of great importance. Further details may be found at map projections and in several texts.

Physics Lambert invented the first practical hygrometer. In 1760, he published a book on photometry, the Photometria. From the assumption that light travels in straight lines, he showed that 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 results were supported by experiments involving the visual comparison of illuminations and used for the calculation of illumination. In Photometria Lambert also cited a law of light absorption, formulated earlier by Pierre Bouguer he is mistakenly credited for (the Beer–Lambert law) and introduced the term albedo. Lambertian reflectance is named after him. He wrote a classic work on perspective and contributed to geometrical optics. The non-SI unit of luminance, lambert, is named in recognition of his work in establishing the study of photometry. Lambert was also a pioneer in the development of three-dimensional colour models. Late in life, he published a description of a triangular colour pyramid (Farbenpyramide), which shows a total of 107 colours on six different levels, variously combining red, yellow and blue pigments, and with an increasing amount of white to provide the vertical component. His investigations were built on the earlier theoretical proposals of Tobias Mayer, greatly extending these early ideas. Lambert was assisted in this project by the court painter Benjamin Calau.

… excerpt ends here. Continue reading the full article.

Illustrations

Johann Heinrich Lambert illustration
Johann Heinrich Lambert: Illustration from De ichnographica campi published in Acta Eruditorum, 1763
Illustration from De ichnographica campi published in Acta Eruditorum, 1763
Johann Heinrich Lambert: La perspective affranchie de l'embarras du plan géometral, French edition, 1759
La perspective affranchie de l'embarras du plan géometral, French edition, 1759
Johann Heinrich Lambert illustration
Johann Heinrich Lambert illustration

Worked examples

Example 1 — a first encounter with Johann Heinrich Lambert

Start with the simplest possible case. Write down what Johann Heinrich Lambert claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In mathematics, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Johann Heinrich Lambert before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Johann Heinrich Lambert ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Johann Heinrich Lambert

In research
Johann Heinrich Lambert appears in mathematics research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Johann Heinrich Lambert in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Johann Heinrich Lambert is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1728 births, 1777 deaths, 18th-century German astronomers, so understanding it makes those chapters shorter.
In everyday life
Look for Johann Heinrich Lambert outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Johann Heinrich Lambert in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Johann Heinrich Lambert means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Johann Heinrich Lambert out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Johann Heinrich Lambert in simple terms?

Johann Heinrich Lambert (German: [ˈlambɛʁt]; French: Jean-Henri Lambert; 26 or 28 August 1728 – 25 September 1777) was an Alsatian polymath from the Republic of Mulhouse—then an associate of the Swiss Confederacy—who made fundamental contributions to mathematics, physics (particularly optics), phil…

Why does Johann Heinrich Lambert matter?

Because it connects several mathematics ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Johann Heinrich Lambert?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Johann Heinrich Lambert.

Tags

  • 1728 births
  • 1777 deaths
  • 18th-century German astronomers
  • 18th-century German male writers
  • 18th-century German mathematicians
  • 18th-century German philosophers
  • 18th-century Swiss astronomers
  • 18th-century Swiss mathematicians
  • 18th-century Swiss philosophers
  • 18th-century Swiss writers
  • Hyperbolic geometers
  • Members of the Prussian Academy of Sciences

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