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Contact Binary
AE Phe binary
Image from Steve Bowers
AE Phoenicis, a W Ursae Majoris contact binary 165 ly from Sol
A co-orbiting pair of stars whose inner atmospheres or surfaces touch, often called a W Ursae Majoris binary, after the system of the same name 162 ly from Sol. In most contact binaries one component is larger than the other. In this kind of system both stars fill their respective Roche Lobes; many contact binaries in fact exceed the equipotential boundary defined by the Roche Lobes, and become so-called overcontact binaries with a common gaseous envelope.

A contact binary pair can have a system of planets in orbit around it, but the innermost planet must orbit no closer than 3.5 times the separation of the two stars.

Most W Ursae Majoris binaries have strong magnetic fields due to the disrupted nature of the component stars; this can make any planetary system associated with such stars an extreme environment.

TY Men binary
Image from Steve Bowers
TY Mensae, a hot contact binary 569 ly from Sol

Celestia Information

To download these starsThe models used to make the images on this page are available for the Celestia Space simulation program from this link; models and data copyright Andrew Tribick
 
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Appears in Topics
Astronomy
 
Development Notes
Text by M. Alan Kazlev
Initially published on 24 September 2001.

 
 
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