On the calculation of the Moon’s latitude in Indian astronomy

IF 0.1 Q4 HISTORY & PHILOSOPHY OF SCIENCE
Anil Narayanan
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Abstract

The latitude algorithm of Indian astronomy has been a long-standing puzzle. All interpretations of the algorithm by various authorities of the past have failed to produce a reasonably accurate result for the latitude of the heavenly bodies. In this paper we examine the latitude algorithm of the Moon in detail. It is determined that a central cause for the failure is a misinterpretation of the mean-max parameter as specified in ancient texts such as the Sūryasiddhānta. In addition, there appears to be a missing sub-algorithm for the calculation of maximum latitude, a key component in the overall latitude algorithm. After a detailed analysis, we provide a conjecture of what the missing algorithm for the Moon’s maximum latitude may have been like and why it was possibly expunged from the Sūryasiddhānta.

Abstract Image

关于印度天文学中月球纬度的计算
印度天文学的纬度算法是一个长期存在的难题。过去各种权威对该算法的解释都未能得出合理准确的天体纬度结果。在本文中,我们详细研究了月球的纬度算法。结果发现,失败的一个主要原因是对《苏利亚悉达论》(Sūryasiddhānta)等古籍中规定的平均-最大参数的误读。此外,最大纬度的计算似乎缺少一个子算法,而最大纬度是整个纬度算法的关键组成部分。经过详细分析,我们猜测了缺失的月球最大纬度算法可能是怎样的,以及为什么它可能被从 Sūryasiddhānta 中删除。
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来源期刊
INDIAN JOURNAL OF HISTORY OF SCIENCE
INDIAN JOURNAL OF HISTORY OF SCIENCE HISTORY & PHILOSOPHY OF SCIENCE-
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