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  2. Lagrange point - Wikipedia

    en.wikipedia.org/wiki/Lagrange_point

    The three collinear Lagrange points (L 1, L 2, L 3) were discovered by the Swiss mathematician Leonhard Euler around 1750, a decade before the Italian-born Joseph-Louis Lagrange discovered the remaining two.

  3. Joseph-Louis Lagrange - Wikipedia

    en.wikipedia.org/wiki/Joseph-Louis_Lagrange

    Joseph-Louis Lagrange [a] (born Giuseppe Luigi Lagrangia [5] [b] or Giuseppe Ludovico De la Grange Tournier; [6] [c] 25 January 1736 – 10 April 1813), also reported as Giuseppe Luigi Lagrange [7] or Lagrangia, [8] was an Italian mathematician, physicist and astronomer, later naturalized French.

  4. History of group theory - Wikipedia

    en.wikipedia.org/wiki/History_of_group_theory

    Lagrange's goal (1770, 1771) was to understand why equations of third and fourth degree admit formulas for solutions, and a key object was the group of permutations of the roots. On this was built the theory of substitutions. [10]

  5. Celestial mechanics - Wikipedia

    en.wikipedia.org/wiki/Celestial_mechanics

    After Newton, Joseph-Louis Lagrange attempted to solve the three-body problem in 1772, analyzed the stability of planetary orbits, and discovered the existence of the Lagrange points. Lagrange also reformulated the principles of classical mechanics, emphasizing energy more than force, and developing a method to use a single polar coordinate ...

  6. Timeline of gravitational physics and relativity - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_gravitational...

    1765 – Leonhard Euler discovers the first three Lagrange points. [18] [19] 1767 – Leonhard Euler solves Euler's restricted three-body problem. [20] 1772 – Joseph-Louis Lagrange discovers the two remaining Lagrange points. [21] 1796 – Pierre-Simon de Laplace independently introduces the nebular hypothesis. [17]

  7. Three-body problem - Wikipedia

    en.wikipedia.org/wiki/Three-body_problem

    In the special case of the circular restricted three-body problem, these solutions, viewed in a frame rotating with the primaries, become points called Lagrangian points and labeled L 1, L 2, L 3, L 4, and L 5, with L 4 and L 5 being symmetric instances of Lagrange's solution.

  8. Euler–Lagrange equation - Wikipedia

    en.wikipedia.org/wiki/Euler–Lagrange_equation

    In the calculus of variations and classical mechanics, the Euler–Lagrange equations [1] are a system of second-order ordinary differential equations whose solutions are stationary points of the given action functional. The equations were discovered in the 1750s by Swiss mathematician Leonhard Euler and Italian mathematician Joseph-Louis Lagrange.

  9. Sophie Germain - Wikipedia

    en.wikipedia.org/wiki/Sophie_Germain

    Marie-Sophie Germain (French: [maʁi sɔfi ʒɛʁmɛ̃]; 1 April 1776 – 27 June 1831) was a French mathematician, physicist, and philosopher.Despite initial opposition from her parents and difficulties presented by society, she gained education from books in her father's library, including ones by Euler, and from correspondence with famous mathematicians such as Lagrange, Legendre, and Gauss ...