India is a land of great diversity. This diversity is seen not only in its culture but also in the advancements that the country has made in the field of science and mathematics. Our textbooks and journals often attribute groundbreaking scientific ideas to foreign 'geniuses,' while many of these discoveries actually have their origins here in India. As a result, we are neglecting the Indian roots and contributions that formed the foundations of most of those theories.
The term 'foreign' is inappropriate in the context of science, as scientific discoveries, regardless of where they originate, have a global impact and contribute to the collective knowledge of humanity, without assigning exclusive credit to any one country or individual.
The purpose of this blog is to highlight the significant advancements in science and mathematics made in India, which have often been overshadowed or credited to other countries or scientists.
In this blog we will be discussing about the Kerala School of Astronomy and Mathematics.
बकुलाधिष्ठितथ्वेना
विहारो यो विष्यथे
ग्रुहानमणि सोयं स्याथ
निजनमणि माधव |
-Madhava (13th sloka, Venuroham)
Astronomical and mathematical development in India is not well known after 10th century AD and many important works that prove the presence of many great astronomers and mathematicians of Kerala remain little known in the field of history of science. One such great astronomer-mathematician was Madhava of Sangamagrama. Sangamagrama Madhava’s work Venuaroham was used for the computation of the true longitude of the moon. Sangamagrama Madhava was one of the great geniuses of the time before Kepler and Newton.
Sangamagrama Madhava and his school were known to the western world through a series of papers published by Charles Whish in 1834 in the journal called Transactions of Asiatic Society of Great Britain and Ireland. In his series of papers, Whish showed that works of Newton, Leibnitz, Gregory and others (who lived during 17th -18th century) were just rediscoveries of the mathematics contributed by the Kerala School.
While Europe was divided in modeling solar system to geocentric and heliocentric systems even in the 17th century, an astronomer-mathematician from Kerala during the 16th century described observational studies as geocentric which can be transformed into a mathematical model with the Sun as the centre.
Neelakanda Somayaji, born in present day Malappuram district of Kerala, a 16th century astronomer-mathematician belonging to a long guru-sishyaparampara chain of five hundred years of length, described in his work, Tantra Sangraha, the subject of observational astronomy along with necessary mathematical techniques.
Neelakanda also made a significant contribution by revising Aryabhata's model for the interior planets, Mercury and Venus. His modifications provided a more precise calculation of the equation of the center for these planets, surpassing existing models in Islamic and European astronomy prior to Johannes Kepler, who emerged 130 years later. This provides a significant insight into the groundbreaking contributions of Indian scientists, demonstrating their achievements in comparison to global advancements at that time.
In his work, Aryabhatiyabhasya, Neelakanda devised a computational scheme for planetary motion that outperformed later models, including Tycho Brahe's. His approach suggested a heliocentric system where Mercury, Venus, Mars, Jupiter, and Saturn orbited the Sun, which itself circled the Earth.
MADHAVA'S ANOMAMLISTIC CYCLES
The fundamental lunar cycles in relation to the Earth are the Synodic cycle (refer my blog on the Moon), which has a period of 29.5 days (New Moon to New Moon) and the Anomalistic cycle (perigee to perigee) which is 27 days 13hrs 18min 34.45s (about 27.5 days). Anomalistic cycles from a zero period will end at cycle number, days, hours, minutes, seconds respectively as follows:
1, 27,13 18 34.45
2, 55, 02,37, 08.90
3, 82, 15, 55, 43.35
4, 110, 05, 14, 17.79
5, 137, 18, 32, 52.24
6, 165, 07, 51, 36.69
7, 192, 21, 10, 01.14
8, 220, 10, 38, 35.59
9, 247, 23, 47, 10.04
D1: After 6,460 days, the first Dhruva cycle completes.
- S1 (Chandravakya at D1): 0 degrees. This means that at the end of the first Dhruva cycle, the Moon is at 0 degrees in its orbit, marking the start of the next cycle.
D2: After 3,411 days, the second Dhruva cycle completes.
- S2 (Chandravakya at D2): 28 degrees. This means that when the second cycle ends, the Moon is at 28 degrees in its orbit.
D3: After 362 days, the third Dhruva cycle completes.
- S3 (Chandravakya at D3): 56 degrees. At the end of this third cycle, the Moon is positioned at 56 degrees in its orbit.
D4: After 4,158 days, the fourth Dhruva cycle completes.
- S4 (Chandravakya at D4): 83 degrees. The Moon's position at the end of the fourth cycle is 83 degrees.
D5: After 1,109 days, the fifth Dhruva cycle completes.
- S5 (Chandravakya at D5): 111 degrees. At the conclusion of the fifth cycle, the Moon is at 111 degrees in its orbit.
D6: After 4,905 days, the sixth Dhruva cycle completes.
- S6 (Chandravakya at D6): 138 degrees. The Moon is positioned at 138 degrees at the end of the sixth cycle.
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