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Contact Binary

28 October 2015

A contact binary star occurs when two stars are close enough that their outer layers are in contact with each other. Often this can occur when one member of a close binary system enters a red giant stage and swells to the point where it is in contact with the companion star. Such systems can create novae, and perhaps supernovae. But recently we’ve discovered1 a contact binary consisting of two O-type stars.

Currently the two stars orbit each other about once a day, as seen in the artist video above. But their eventual fate is still unknown. Stars of this size typically have a cosmically short lifetime of about 5 million years. It’s possible that they merge into a single, fast-rotating star. Such a supermassive could end its life with a long duration gamma ray burst. But it’s also possible that the stars remain a stable binary throughout their lifetime. If that’s the case, then each would end their lives as supernovae, and produce a black hole. This could create a close black hole binary.

Such a black hole binary would be a boon for astronomers trying to detect gravitational waves, since close binary black holes would create the strongest consistent signal.


  1. Almeida, L. A., et al. “Discovery of the massive overcontact binary VFTS 352: evidence for enhanced internal mixing.” The Astrophysical Journal 812.2 (2015): 102. ↩︎