Venvaroha

From Wikipedia, the free encyclopedia
Jump to: navigation, search
Veṇvāroha
Author Madhava of Sangamagrama (c.1350 – c.1425)
Translator Malayalam commentary by Achyuta Pisharati (1550–1621)
Country India
Language Sanskrit
Subject Astronomy/Mathematics
Publisher Malayalam commentary edited by K.V. Sarma and printed by Sanskrit College, Thrippunithura, Kerala, India
Publication date
Original in 1403 CE. Malayalam commentary printed in 1956 CE.

Veṇvāroha is a work in Sanskrit composed by Mādhava (c.1350 – c.1425) of Sangamagrāma the founder of the Kerala school of astronomy and mathematics. It is a work in 74 verses describing methods for the computation of the true positions of the Moon at intervals of about half an hour for various days in an anomalistic cycle. This work is an elaboration of an earlier and shorter work of Mādhava himself titled Sphutacandrāpti.[1] Veṇvāroha is the most popular astronomical work of Mādhava.[2] It is dated 1403 CE. Acyuta Piṣārati (1550–1621), another prominent mathematician/astronomer of the Kerala school, has composed a Malayalam commentary on Veṇvāroha.[1] This astronomical treatise is of a type generally described as Karaṇa texts in India. Such works are characterized by the fact that they are compilations of computational methods of practical astronomy. The title Veṇvāroha literally means Bamboo Climbing and it is indicative of the computational procedure expounded in the text. The computational scheme is like climbing a bamboo tree, going up and up step by step at measured equal heights.

The novelty and ingenuity of the method attracted the attention of several of the followers of Mādhava and they composed similar texts thereby creating a genre of works in Indian mathematical tradition collectively referred to as ‘veṇvāroha texts’. These include Drik-veṇvārohakriya of unknown authorship of epoch 1695 and Veṇvārohastaka of Putuman Somāyaji.[3]

In the technical terminology of astronomy, he ingenuity introduced by Mādhava in Veṇvāroha can be explained thus: Mādhava has endeavored to compute the true longitude of the Moon by making use of the true motions rather than the epicyclic astronomy of the Aryabhatan tradition. He made use of the anomalistic revolutions for computing the true positions of the Moon using the successive true daily velocity specified in Candravākyas for easy memorization and use.[4]

Veṇvāroha has been studied from a modern perspective and the process is explained using the properties of periodic functions. [5]

See also[edit]

References[edit]

  1. ^ a b David Edwin Pingree (1981). Census of the exact sciences in Sanskrit, 4. Philadelphia: American Philosophical Society. p. 414. ISBN 0-87169-146-9. 
  2. ^ Helaine Selin, ed. (1997). "Article by R.C. Gupta". Encyclopaedia of the History of Science, Technology, and Medicine in Non-Westen Cultures. Springer. p. 522. ISBN 978-0-7923-4066-9. 
  3. ^ K.V. Sarma. "A survey of source materials". Indian national Academy of Science. Retrieved 21 March 2010. 
  4. ^ K. Chandra Hari. "Computation of the true moon by Madhava of Sangamagrama". Indian Journal of History of Science 38 (3): 251–253. Retrieved 21 March 2010. 
  5. ^ S. Madhavan (2012). "Veṇvāroha From a Modern Perspective". Indian Journal of History of Science 47 (4): 699–717. 

Further reading[edit]