Titlebook: Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of Jyesthadeva; Volume II - Astronom K. V. Sarma,K. Ramasubramanian,M. S. Sriram Boo

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Computation of Planetsf all the planets is taken to be a constant. In other words, if . be the radius of the planetary orbit (usually given in .-s), and . be the sidereal time period, then . where . is a constant. Given ., the radius of the planetary orbit is determined, if the time period of a planet is known. The term

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