Abstract
Imagine a star pair orbiting round their common centre of gravity in 30 days = 2592000 sec. in a virtual circle (eccentricity of the orbital ellipses are very small, nearly zero). The heavier one is like Rigel, having a mass of 65×10 30 k.g.km. It is expected that it will be 20400 (or more) times brighter than the Sun, in accordance with the "Mass Luminosity Law", and more for Characteristic II. effect of Chapter-I, Art.12. Since the distance between the centre of gravities of the two stars will be only 6.09879 A.U. Its companion is as massive as Sun 1.984×10 30 k.g. The orbiting velocity of the heavier star will be only 6 553.821203 metres/sec. (equation 2 of Chapter-1, Para 8) around their common centre of gravity.
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