Binary black hole

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Computer simulation of the black hole merger GW150914. The background is distorted as the intense gravity from the merger causes gravitational lensing.

A Binary Black Hole (often abbreviated BBH), are two black holes in close orbit around each other. The two black holes will eventually merge into one releasing a large amount of gravitational waves.

Discovery[change | change source]

For years the existence of binary black holes was only theoretical. Proving they exist was a challenge due to the nature of black holes. Although if two black holes were to ever merge this would cause a significant amount of gravitational waves to be released. The existence of binary black holes (and gravitational waves themselves) was proven when on September 2015, LIGO detected GW150914.[1]

  1. Castelvecchi, Davide; Witze, Alexandra (2016-02-11). "Einstein's gravitational waves found at last". Nature. doi:10.1038/nature.2016.19361. ISSN 1476-4687.