Book Title: Jain Journal 1983 07
Author(s): Jain Bhawan Publication
Publisher: Jain Bhawan Publication

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Page 19
________________ JULY, 1983 Besides, from eq. No. (1) we have Da V1 = V1 S Vdt Now in vaiśvānara vithi (n=7), Dn is maximum (see table No. 4) D, S O Dn Vdt D, --minimum value (see table No. 4) Thus mean velocity of Venus is minimum in vaiśvānara vithi (fire lane). This result stands true also for actual physical situation as shown below: We know that instantaneous relative geocentric velocity of Venus, VVV-Vg............ 15 -3) Jain Education International where VvHeliocentric velocity of Venus during geocentric retrogression Vs Apparent velocity of the Sun Now as it is evident from fig. No. 2 that perigee (point of apparent maximum geocentric velocity) A of Sun lies in vaiśvānara vithi i.e. Vg in vaisvānara vithi lies in the neighbourhood of its maximum value ; and aphelion (point of minimum helocentric velocity) C of Venus lies very near to that i.e. Vy in vaiśvānara vithi lies in the neighbourhood of its minimum value. Thus in vaiśvānara vithi the various values of V(= Vv-Vs) would be smaller than its corresponding values in similar situations of Venus in any other vithi. Consequently mean velocity Vn of Venus will also mbe inimum in vaiśvānara vithi (for n=7). For Private & Personal Use Only www.jainelibrary.org

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