Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10410
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dc.contributor.authorPAI, VENKETESWARA R.en_US
dc.date.accessioned2025-09-16T06:14:11Z-
dc.date.available2025-09-16T06:14:11Z-
dc.date.issued2025-08en_US
dc.identifier.citationIndian Journal of History of Science, 60, 121–134.en_US
dc.identifier.issn2454-9991en_US
dc.identifier.issn0019-5235en_US
dc.identifier.urihttps://doi.org/10.1007/s43539-025-00165-4en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10410-
dc.description.abstractIn modern astronomy, the expression for the longitude of the Moon has a large number of terms to include the effects of the Sun, planets etc. apart from the Earth. If the desired accuracy is an arc minute or so, it is sufficient to include only about 5 to 6 terms. The Moon-mnemonics (Candravākyas) are based on a simple epicycle model for the Moon (with only one correction to the mean longitude to obtain the true longitude). Moon’s longitude can be computed in a few simple steps using these vākyas This paper presents the details of the actual method for computing Moon’s longitude using vākyas in one of the texts, namely, Dṛkkaraṇa from medieval Kerala. It highlights the simplicity and ingenuity of the method in taking various corrections into account.en_US
dc.language.isoenen_US
dc.publisherSpringer Nature/Indian National Science Academy, New Delhi, Indiaen_US
dc.subjectVākya/mnemonics—en_US
dc.subjectTrue longitude of the Moonen_US
dc.subjectCandravākyasen_US
dc.subjectDṛkkaraṇaen_US
dc.titleObtaining the longitude of the moon through mnemonics – An example from a medieval Kerala text, Dṛkkaraṇaen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Humanities and Social Sciencesen_US
dc.identifier.sourcetitleIndian Journal of History of Scienceen_US
dc.publication.originofpublisherForeignen_US
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