#  A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z   

 Home

 Calculations
 Contacts
 Conversions
 Help
 Links
 Subjects


Lagrangian Points

In a system of two large bodies (Sun-Earth or Earth-Moon), these are the points where a small third body will keep a fixed position relative to the other two.

Named for French astronomer Louis Lagrange (1736-1813) who first studied them and who showed there existed 5 such points. In the Sun-Earth system only two are important, both on the Earth-Sun line--the L1 point 236 Earth radii sunward of Earth, and the L2 point at a similar distance on the night side. The L1 point is a good "early warning" outpost intercepting shocks and particles emitted by the Sun and its vicinity has been occupied by several spacecraft.

Altogether five Lagrangian points exist in the Earth-Sun or Earth-Moon system.

See also: Earth, Sun.

Previous PageView links to and from this pageNext Page

Subjects:
Mathematics
Science & Engineering Encyclopaedia Version 2.4 © 2001-2010 Dirac Delta Consultants Limited