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Revision as of 01:58, 13 January 2025 editKrishnachandranvn (talk | contribs)Extended confirmed users, Pending changes reviewers12,309 edits Created page with '{{italic title}} '''Grahalāghavaṃ''' is a Sanskrit treatise on astronomy composed by Gaṇeśa Daivajna (c. 1507-1554), a sixteenth century astronomer, astrologer, and mathematician from western India, probably from the Indian state of Maharashtra. It is a work in the genre of the ''karaṇa'' text in the sense that it is in the form of a handbook or manual for the computation of the positions of the planets. Of all the ancient and medieval ''k...'  Revision as of 01:59, 13 January 2025 edit undoKrishnachandranvn (talk | contribs)Extended confirmed users, Pending changes reviewers12,309 editsNo edit summaryNext edit →
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'''Grahalāghavaṃ''' is a Sanskrit treatise on astronomy composed by ] (c. 1507-1554), a sixteenth century astronomer, astrologer, and mathematician from western India, probably from the Indian state of ]. It is a work in the genre of the ''karaṇa'' text in the sense that it is in the form of a handbook or manual for the computation of the positions of the planets. Of all the ancient and medieval ''karaṇa'' texts on astronomy, ''Grahalāghavaṃ'' is the most popular among the '']'' makers of most parts of India.It is also considered to be the most comprehensive, exhuastive and easy to use ''karaṇa'' text on astronomy.<ref name="S1">{{cite journal |last1=Balachandra Rao S. and S. K. Uma |title=Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes |journal=Indian Journal of History of Science |date=2006 |volume=41 |issue=1 Supplement |pages=S1-S88 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol41_1_11_Supplement_Grahalaghavam.pdf |access-date=11 January 2025}}</ref> The popularity of this work is attested by the large number of commentaries (at least 14 in number) on it and also by the large number of modern editions (at least 23 in number) of the book.<ref name="Sahana">{{cite book |last1=Sahana Cidambi |title=The first three chapters of the Grahalaghva of Ganesa Daivajna |date=2022 |publisher=Department of Mathematics and Statistics, University of Canterbury |location=New Zealand |url=https://ir.canterbury.ac.nz/bitstreams/6d4403fe-69ba-4946-8fcc-d1d93b7702e9/download |access-date=12 January 2025}}</ref> The work is divided into sixteen chapters and covers all the commonly discussed topics in such texts including planetary positions, timekeeping and calendar construction, eclipses, heliacal rising and settings, planetary conjunctions, and the ''mahāpāta''-s.<ref name="Sahana"/> '''Grahalāghavaṃ''' is a Sanskrit treatise on astronomy composed by ] (c. 1507-1554), a sixteenth century astronomer, astrologer, and mathematician from western India, probably from the Indian state of ]. It is a work in the genre of the ''karaṇa'' text in the sense that it is in the form of a handbook or manual for the computation of the positions of the planets. Of all the ancient and medieval ''karaṇa'' texts on astronomy, ''Grahalāghavaṃ'' is the most popular among the '']'' makers of most parts of India.It is also considered to be the most comprehensive, exhuastive and easy to use ''karaṇa'' text on astronomy.<ref name="S1">{{cite journal |last1=Balachandra Rao S. and S. K. Uma |title=Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes |journal=Indian Journal of History of Science |date=2006 |volume=41 |issue=1 Supplement |pages=S1-S88 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol41_1_11_Supplement_Grahalaghavam.pdf |access-date=11 January 2025}}</ref> The popularity of this work is attested by the large number of commentaries (at least 14 in number) on it and also by the large number of modern editions (at least 23 in number) of the book.<ref name="Sahana">{{cite book |last1=Sahana Cidambi |title=The first three chapters of the Grahalaghva of Ganesa Daivajna |date=2022 |publisher=Department of Mathematics and Statistics, University of Canterbury |location=New Zealand |url=https://ir.canterbury.ac.nz/bitstreams/6d4403fe-69ba-4946-8fcc-d1d93b7702e9/download |access-date=12 January 2025}}</ref> The work is divided into sixteen chapters and covers all the commonly discussed topics in such texts including planetary positions, timekeeping and calendar construction, eclipses, heliacal rising and settings, planetary conjunctions, and the ''mahāpāta''-s.<ref name="Sahana"/>


The most striking features of the work that made it highly popular include its use of an ingenious method to reduce the traditional method of computations involving 'astronomical numbers' to smaller numbers and its meticulous and careful avoidance of the use of the trigonometrical sines by replacing them with simpler, still acceptably accurate, algebraic expressions.<ref name=S1/> The former is effected by introducing the concept of a new cycle called a ''cakra'', a period consisting of 4016 days which is approximately 11 years. Traditional computations make use the concept of ''ahargaṇa'' which is the number of civil days elapsed since the ] which falls on 17/18 February 3102 BCE. The traditional ''ahargaṇa'' is a huge number. For example, the ''ahargaṇa'' corresponding to 1 January 2025 is 1872211. The ''ahargaṇa'' as modified in ''Grahalāghavaṃ'' is the remainder number of days after completing full ''cakra''-s of 4016 days each since the beginning of the epoch. Thus the modified ''ahargaṇa'' corresponding to 1 January 2025 would be 755, a number less than 4016. To avoid the use of trigonometrical sines, ''Grahalāghavaṃ'' uses several approximations to the sine function. For example, in the context of computing the true longitudes of celestial objects, approximation formulas based on the following approximation to the sine function (known as the ]) is used<ref name="S1">{{cite journal |last1=Balachandra Rao S. and S. K. Uma |title=Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes |journal=Indian Journal of History of Science |date=2006 |volume=41 |issue=1 Supplement |pages=S56-S65 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol41_1_11_Supplement_Grahalaghavam.pdf |access-date=11 January 2025}}</ref>: The most striking features of the work that made it highly popular include its use of an ingenious method to reduce the traditional method of computations involving 'astronomical numbers' to smaller numbers and its meticulous and careful avoidance of the use of the trigonometrical sines by replacing them with simpler, still acceptably accurate, algebraic expressions.<ref name=S1/> The former is effected by introducing the concept of a new cycle called a ''cakra'', a period consisting of 4016 days which is approximately 11 years. Traditional computations make use the concept of ''ahargaṇa'' which is the number of civil days elapsed since the ] which falls on 17/18 February 3102 BCE. The traditional ''ahargaṇa'' is a huge number. For example, the ''ahargaṇa'' corresponding to 1 January 2025 is 1872211. The ''ahargaṇa'' as modified in ''Grahalāghavaṃ'' is the remainder number of days after completing full ''cakra''-s of 4016 days each since the beginning of the epoch. Thus the modified ''ahargaṇa'' corresponding to 1 January 2025 would be 755, a number less than 4016. To avoid the use of trigonometrical sines, ''Grahalāghavaṃ'' uses several approximations to the sine function. For example, in the context of computing the true longitudes of celestial objects, approximation formulas based on the following approximation to the sine function (known as the ]) is used<ref>{{cite journal |last1=Balachandra Rao S. and S. K. Uma |title=Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes |journal=Indian Journal of History of Science |date=2006 |volume=41 |issue=1 Supplement |pages=S56-S65 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol41_1_11_Supplement_Grahalaghavam.pdf |access-date=11 January 2025}}</ref>:
:: <math>\sin x^\circ \approx \frac{4x(180 - x)}{40500 - x(180 - x)}.</math> :: <math>\sin x^\circ \approx \frac{4x(180 - x)}{40500 - x(180 - x)}.</math>
In the context of the computation of eclipses, the following approximation is used<ref>{{cite journal |last1=S. Balachandra Rao, S.K. Uma and Padmaja Venugopal |title=Lunar eclipse computation in Indian astronomy with special reference to ''Grahalaghava'' |journal=Indian Journal of History of Science |date=2003 |volume=38 |issue=3 |pages=255-271 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol38_3_4_SBRao.pdf |access-date=13 January 2025}}</ref>: In the context of the computation of eclipses, the following approximation is used<ref>{{cite journal |last1=S. Balachandra Rao, S.K. Uma and Padmaja Venugopal |title=Lunar eclipse computation in Indian astronomy with special reference to ''Grahalaghava'' |journal=Indian Journal of History of Science |date=2003 |volume=38 |issue=3 |pages=255-271 |url=https://cahc.jainuniversity.ac.in/assets/ijhs/Vol38_3_4_SBRao.pdf |access-date=13 January 2025}}</ref>:

Revision as of 01:59, 13 January 2025

Grahalāghavaṃ is a Sanskrit treatise on astronomy composed by Gaṇeśa Daivajna (c. 1507-1554), a sixteenth century astronomer, astrologer, and mathematician from western India, probably from the Indian state of Maharashtra. It is a work in the genre of the karaṇa text in the sense that it is in the form of a handbook or manual for the computation of the positions of the planets. Of all the ancient and medieval karaṇa texts on astronomy, Grahalāghavaṃ is the most popular among the pañcāṅgaṃ makers of most parts of India.It is also considered to be the most comprehensive, exhuastive and easy to use karaṇa text on astronomy. The popularity of this work is attested by the large number of commentaries (at least 14 in number) on it and also by the large number of modern editions (at least 23 in number) of the book. The work is divided into sixteen chapters and covers all the commonly discussed topics in such texts including planetary positions, timekeeping and calendar construction, eclipses, heliacal rising and settings, planetary conjunctions, and the mahāpāta-s.

The most striking features of the work that made it highly popular include its use of an ingenious method to reduce the traditional method of computations involving 'astronomical numbers' to smaller numbers and its meticulous and careful avoidance of the use of the trigonometrical sines by replacing them with simpler, still acceptably accurate, algebraic expressions. The former is effected by introducing the concept of a new cycle called a cakra, a period consisting of 4016 days which is approximately 11 years. Traditional computations make use the concept of ahargaṇa which is the number of civil days elapsed since the kali epoch which falls on 17/18 February 3102 BCE. The traditional ahargaṇa is a huge number. For example, the ahargaṇa corresponding to 1 January 2025 is 1872211. The ahargaṇa as modified in Grahalāghavaṃ is the remainder number of days after completing full cakra-s of 4016 days each since the beginning of the epoch. Thus the modified ahargaṇa corresponding to 1 January 2025 would be 755, a number less than 4016. To avoid the use of trigonometrical sines, Grahalāghavaṃ uses several approximations to the sine function. For example, in the context of computing the true longitudes of celestial objects, approximation formulas based on the following approximation to the sine function (known as the Bhāskara I's sine approximation formula) is used:

sin x 4 x ( 180 x ) 40500 x ( 180 x ) . {\displaystyle \sin x^{\circ }\approx {\frac {4x(180-x)}{40500-x(180-x)}}.}

In the context of the computation of eclipses, the following approximation is used:

When x {\displaystyle x} is small, sin x 3 175 x . {\displaystyle \sin x^{\circ }\approx {\frac {3}{175}}x.} It may be noted that this is an approximation to the well known result sin θ θ {\displaystyle \sin \theta \approx \theta } when θ {\displaystyle \theta } is in radians and is small.

Full texts

Full text of the work with commentaries in Sanskrit and with English translation are available at the following sources:

  • Kapilesvara Sasthri (1948). The Grahalaghava of Ganesa Daivajnja with Sanskrit Commentary by Visvanatha Daivajnja. Benares City: Jayakrishna das Haridas Gupta. Retrieved 12 January 2025.
  • For an English translation of the full text of Grahalāghavaṃ see: Rao, S. Balachandra & S. K. Uma, Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes, IJHS 41.1 (2006) Supplement pp. S1-88; 41.2 (2006) Supplement pp. S89-183; 41.3 (2006) Supplement pp. S185-315; 41.4 (2006) Supplement pp. S317-415.

References

  1. ^ Balachandra Rao S. and S. K. Uma (2006). "Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes" (PDF). Indian Journal of History of Science. 41 (1 Supplement): S1 – S88. Retrieved 11 January 2025.
  2. ^ Sahana Cidambi (2022). The first three chapters of the Grahalaghva of Ganesa Daivajna. New Zealand: Department of Mathematics and Statistics, University of Canterbury. Retrieved 12 January 2025.
  3. Balachandra Rao S. and S. K. Uma (2006). "Grahalaghavam of Ganesa Daivajna – an English Exposition, Mathematical Explanation and Notes" (PDF). Indian Journal of History of Science. 41 (1 Supplement): S56 – S65. Retrieved 11 January 2025.
  4. S. Balachandra Rao, S.K. Uma and Padmaja Venugopal (2003). "Lunar eclipse computation in Indian astronomy with special reference to Grahalaghava" (PDF). Indian Journal of History of Science. 38 (3): 255–271. Retrieved 13 January 2025.
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