Sound Of Rigel ( Orion Star System - By Fibonacci Cosmic Power Chord - 432 Ratio Binaural )

The star system of which Rigel is a part has at least four components. Rigel (sometimes called Rigel A to distinguish from the other components) has a visual companion, which is likely a close triple-star system. A fainter star at a wider separation might be a fifth component of the Rigel system. Component B is a double-lined spectroscopic binary system, which shows two sets of spectral lines combined within its single stellar spectrum. Periodic changes observed in relative positions of these lines indicate an orbital period of days. The two spectroscopic components Rigel Ba and Rigel Bb cannot be resolved in optical telescopes but are known to both be hot stars of spectral type around B9. This spectroscopic binary, together with the close visual component Rigel C, is likely a physical triple-star system although Rigel C cannot be detected in the spectrum, which is inconsistent with its observed brightness Rigel B has a time period of days from the formula f=1/T frequency equals one