||It has been suggested that Barycentric coordinates (astronomy) be merged into this article. (Discuss) Proposed since June 2015.|
The barycenter (from the Greek βαρύκεντρον) is the center of mass of two or more bodies which are orbiting each other, and is the point around which both of them orbit. It is an important concept in the fields of astronomy, astrophysics, and the like.
In the case where one of the two objects is much larger and more massive than the other, the barycenter will be located within the larger object. Rather than appearing to orbit it will simply be seen to "wobble" slightly. This is the case for the Moon and Earth, where the barycenter is located on average 4,671 km from Earth's center, well within the planet's radius of 6,378 km. When the two bodies are of similar masses (or at least the mass ratio is less extreme), however, the barycenter will be located outside of either of them and both bodies will follow an orbit around it. This is the case for Pluto and Charon, Jupiter and the Sun, and many binary asteroids and binary stars.
In geometry, the term "barycenter" is a synonym for centroid, the geometric center of a two-dimensional shape.
The distance from the center of a body (thought of as a point-mass) to the barycenter in a simple two-body case can be calculated as follows:
- r1 is the distance from body 1 to the barycenter
- rtot is the distance between the two bodies
- m1 and m2 are the masses of the two bodies.
Two bodies with similar mass orbiting around a common barycenter with elliptic orbits.
|Wikimedia Commons has media related to barycenter animations.|