Authors: Adham Ahmed Mohamed Ahmed
E=mc^2 we could take this relation to celestial systems to know the energy of a system. to do this we can make the difference between mass of the star and mass of planet's difference as in this relation (m1-m2)c^2 where m1 is the mass of a the star and m2 is the mass of the planet and one of the c is equal to orbit speed + gravitational pull at one sec and the other c or the other speed of light is multiplied by the difference between the masses and that is equal to the quantity of time in seconds that the system is at existence
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[v1] 2018-10-02 12:42:47
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