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Michel$501744$ - translation to Αγγλικά
![Dumonstier]]](https://commons.wikimedia.org/wiki/Special:FilePath/Montaigne-Dumonstier.jpg?width=200 "Dumonstier]]")
![Portrait of 1587 by [[Étienne Martellange]]](https://commons.wikimedia.org/wiki/Special:FilePath/Montaigne 1584 - Martellange.jpg?width=200 "Portrait of 1587 by [[Étienne Martellange]]")
![tower]] in which he wrote still stands](https://commons.wikimedia.org/wiki/Special:FilePath/St Michel de Montaigne Château01.jpg?width=200 "tower]] in which he wrote still stands")
![The Tour de Montaigne ([[Montaigne's tower]]), where Montaigne's library was located, remains mostly unchanged since the sixteenth century](https://commons.wikimedia.org/wiki/Special:FilePath/St Michel de Montaigne Tour03.jpg?width=200 "The Tour de Montaigne ([[Montaigne's tower]]), where Montaigne's library was located, remains mostly unchanged since the sixteenth century")
![First public demonstration in [[Annonay]], 4 June 1783](https://commons.wikimedia.org/wiki/Special:FilePath/Early flight 02562u (2).jpg?width=200 "First public demonstration in [[Annonay]], 4 June 1783")
![''Proposed Monument to Commemorate the Invention of the Balloon'' by [[Claude Michel]], c. 1784](https://commons.wikimedia.org/wiki/Special:FilePath/Model for a Proposed Monument to Commemorate the Invention of the Balloon MET DP248127.jpg?width=200 "''Proposed Monument to Commemorate the Invention of the Balloon'' by [[Claude Michel]], c. 1784")
![A model of the Montgolfier brothers' balloon at the [[London Science Museum]]](https://commons.wikimedia.org/wiki/Special:FilePath/Montgolfier Balloon.JPG?width=200 "A model of the Montgolfier brothers' balloon at the [[London Science Museum]]")
Βικιπαίδεια
Michel Hénon (French: [enɔ̃]; 23 July 1931, Paris – 7 April 2013, Nice) was a French mathematician and astronomer. He worked for a long time at the Nice Observatory.
In astronomy, Hénon is well known for his contributions to stellar dynamics. In the late 1960s and early 1970s he made important contributions on the dynamical evolution of star clusters, in particular globular clusters. He developed a numerical technique using Monte Carlo methods to follow the dynamical evolution of a spherical star cluster much faster than the so-called n-body methods.
In mathematics, he is well known for the Hénon map, a simple discrete dynamical system that exhibits chaotic behavior.
He published a two-volume work on the restricted three-body problem.
In 1978 he was awarded the Prix Jean Ricard.
