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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Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of JyesthadevaVolume II - Astronom

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Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of Jyesthadeva978-93-86279-37-8

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Computation of Planets number of .-s moved per day is the same for all planets. For planets which move along smaller orbits, the circle would be completed in a shorter time. For those which move along larger orbits, the circle would be completed only in a longer period. For instance, the Moon would have completely moved

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The Fifteen Problemsd by solid lines in Figure 10.1. Three more circles which are referred to later in the chapter are indicated by dashed lines. In Table 10.1, the second column gives the names of the circles in Sanskrit. The third column gives their modern equivalents. In the last column we have listed the poles (vis

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Gnomonic Shadowd spread in a circle and flow forth on all the sides uniformly. That is the indication for a level surface. On this surface draw a circle (in the following manner): Take a rod slightly bent at both ends and, with one end of the rod fixed at the centre, rotate the other end on all sides (so that a ci

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