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.
He published a two-volume work on the restricted three-body problem.
- "[Observatoire de la Côte d’Azur] Décès de Michel Hénon, Astronome à l'Observatoire de la Côte d'Azur". Oca.eu. 2011-03-18. Retrieved 2013-06-12.[permanent dead link]
- Hénon's publications (a partial list from NASA Astrophysics Data System).
- A discussion of Hénon's equation, contains further links.