*Bhāskara the teacher*) was an Indian mathematician and astronomer of 12th century AD.

He is refered as Bhāskara II to avoid confusion with Bhāskara I (of 7th century AD).

He was born near Vijjadavida (Bijapur in modern Karnataka) and lived between 1114-1185 AD.

He represented the peaks of mathematical knowledge in the 12th century and was the head of the astronomical observatory at Ujjain, the leading mathematical centre of ancient India.

Bhaskara II’s family belonged to Deshastha Brahmin community, which served as court scholars at Kings forts.

He learned Mathematics from his father Maheswara, an astrologer.

He imparted his knowledge of mathematics to his son Lokasamudra, whose son had started a school to study the works of his grand father in 1207 AD.

Bhaskara II’s family belonged to Deshastha Brahmin community, which served as court scholars at Kings forts.

He learned Mathematics from his father Maheswara, an astrologer.

He imparted his knowledge of mathematics to his son Lokasamudra, whose son had started a school to study the works of his grand father in 1207 AD.

His main work Siddhānta Shiromani, (Sanskrit for “

These four sections deal with arithmetic, algebra, mathematics of the planets, and spheres respectively. He also wrote another treatise named

Bhāskara’s work on calculus predates

He is particularly known in the discovery of the principles of differential calculus and its application to astronomical problems and computations. While Newton and Leibniz have been credited with differential and integral calculus, there is strong evidence to suggest that

*Crown of treatises,*“) is divided into four parts called*Lilāvati(beautiful woman, named after his daughter Lilavati), Bijaganita, Grahaganita (mathematics of planets)*and*Golādhyāya (study of sphere/earth)*.These four sections deal with arithmetic, algebra, mathematics of the planets, and spheres respectively. He also wrote another treatise named

*Karna Kautoohala*.Bhāskara’s work on calculus predates

*Newton*and*Leibniz*by over half a millennium.He is particularly known in the discovery of the principles of differential calculus and its application to astronomical problems and computations. While Newton and Leibniz have been credited with differential and integral calculus, there is strong evidence to suggest that

*Bhāskara*was a pioneer in some of the principles of differential calculus. He was perhaps the first to conceive the differential coefficient and differential calculus.
Lilavati (meaning a beautiful woman) is based on Arithmetic. It is believed that Bhaskara named this book after his daughter Lilavati. Many of the problems in this book are addressed to his daughter. For example “Oh Lilavati, intelligent girl, if you understand addition & subtraction, tell me the sum of the amounts 2, 5, 32, 193, 18, 10 & 100, as well as [the remainder of] those when subtracted from 10000.” The book contains thirteen chapters, mainly definitions, arithmetical terms, interest computation, arithmetical & geometric progressions. Many of the methods in the book on computing numbers such as multiplications, squares & progressions were based on common objects like kings & elephants, which a common man could understand.

*Bijaganita*is on Algebra & contains 12 chapters.

“

*A positive number has two square-roots (a negative root & a positive root)*“. This was published in this text for the very first time. It contains concepts of positive & negative numbers, zero, the ‘

*unknown*‘ (includes determining unknown quantities), surds, simple equations & quadratic equations.

Bhaskara was the first to introduce the concept of

Also the fact that if any finite number is added to infinity then the sum is infinity. He developed a proof of the Pythogorean theorem by calculating the same area in two different ways & then cancelling out two terms to get a

He is also known for his calculation of the time required (365.2588 days) by the Earth to orbit the Sun which differs from the modern day calculation of 365.2563 days, by just 3.5 minutes!

The law of Gravitation had been proved by Bhaskara 500 years before it was rediscovered by Newton.

**Infinity**:*If any finite number is divided by zero, the result is infinity*.Also the fact that if any finite number is added to infinity then the sum is infinity. He developed a proof of the Pythogorean theorem by calculating the same area in two different ways & then cancelling out two terms to get a

^{2}+ b^{2}= c^{2}.He is also known for his calculation of the time required (365.2588 days) by the Earth to orbit the Sun which differs from the modern day calculation of 365.2563 days, by just 3.5 minutes!

The law of Gravitation had been proved by Bhaskara 500 years before it was rediscovered by Newton.

### Bhaskaracharya’s contributions

**Mathematics**

Some of Bhaskara’s contributions to mathematics include the following:

A proof of the Pythagorean theorem by calculating the same area in two different ways and then canceling out terms to get a

^{2}+ b

^{2}= c

^{2}.

In Lilavati, solutions of quadratic, cubic and quartic indeterminate equations are explained.

Solutions of indeterminate quadratic equations (of the type ax

^{2}+ b = y

^{2}).

Integer solutions of linear and quadratic indeterminate equations (Kuttaka). The rules he gives are (in effect) the same as those given by the Renaissance European mathematicians of the 17th century

A cyclic Chakravala method for solving indeterminate equations of the form ax

^{2}+ bx + c = y. The solution to this equation was traditionally attributed to William Brouncker in 1657, though his method was more difficult than the chakravala method.

The first general method for finding the solutions of the problem x

^{2}− ny

^{2}= 1 (so-called “

*Pell’s equation*“) was given by Bhaskara II.

Solutions of Diophantine equations of the second order, such as 61x

^{2}+ 1 = y

^{2}. This very equation was posed as a problem in 1657 by the French mathematician Pierre de Fermat, but its solution was unknown in Europe until the time of Euler in the 18th century.

Solved quadratic equations with more than one unknown, and found negative and irrational solutions.

Preliminary concept of mathematical analysis.

Preliminary concept of infinitesimal calculus, along with notable contributions towards integral calculus.

Conceived differential calculus, after discovering the derivative and differential coefficient.

Stated Rolle’s theorem, a special case of one of the most important theorems in analysis, the mean value theorem. Traces of the general mean value theorem are also found in his works.

Calculated the derivatives of trigonometric functions and formulae. (See Calculus section below.)

In Siddhanta Shiromani, Bhaskara developed spherical trigonometry along with a number of other trigonometric results. (See Trigonometry section below.)

**Arithmetic**

Bhaskara’s arithmetic text Leelavati covers the topics of definitions, arithmetical terms, interest computation, arithmetical and geometrical progressions, plane geometry, solid geometry, the shadow of the gnomon, methods to solve indeterminate equations, and combinations.

Lilavati is divided into 13 chapters and covers many branches of mathematics, arithmetic, algebra, geometry, and a little trigonometry and mensuration. More specifically the contents include:

Definitions.

Properties of zero (including division, and rules of operations with zero).

Further extensive numerical work, including use of negative numbers and surds.

Estimation of π.

Arithmetical terms, methods of multiplication, and squaring.

Inverse rule of three, and rules of 3, 5, 7, 9, and 11.

Problems involving interest and interest computation.

Indeterminate equations (Kuttaka), integer solutions (first and second order). His contributions to this topic are particularly important, since the rules he gives are (in effect) the same as those given by the renaissance European mathematicians of the 17th century, yet his work was of the 12th century. Bhaskara’s method of solving was an improvement of the methods found in the work of Aryabhata and subsequent mathematicians.

His work is outstanding for its systemisation, improved methods and the new topics that he has introduced. Furthermore the Lilavati contained excellent recreative problems and it is thought that Bhaskara’s intention may have be.

**Algebra**

His Bijaganita (

*“Algebra”*) was a work in twelve chapters. It was the first text to recognize that a positive number has two square roots (a positive and negative square root).

His work Bijaganita is effectively a treatise on algebra and contains the following topics:

Positive and negative numbers.

Zero.

The ‘unknown’ (includes determining unknown quantities).

Determining unknown quantities.

Surds (includes evaluating surds).

Kuttaka (for solving indeterminate equations and Diophantine equations).

Simple equations (indeterminate of second, third and fourth degree).

Simple equations with more than one unknown.

Indeterminate quadratic equations (of the type ax

^{2}+ b = y

^{2}).

Solutions of indeterminate equations of the second, third and fourth degree.

Quadratic equations.

Quadratic equations with more than one unknown.

Operations with products of several unknowns.

Bhaskara derived a cyclic, chakravala method for solving indeterminate quadratic equations of the form ax

^{2}+ bx + c = y.

Bhaskara’s method for finding the solutions of the problem Nx

^{2}+ 1 = y

^{2}(the so-called “

*Pell’s equation*“) is of considerable importance.

**Trigonometry**

The Siddhanta Shiromani (written in 1150) demonstrates Bhaskara’s knowledge of trigonometry, including the sine table and relationships between different trigonometric functions. He also discovered spherical trigonometry, along with other interesting trigonometrical results. In particular Bhaskara seemed more interested in trigonometry for its own sake than his predecessors who saw it only as a tool for calculation. Among the many interesting results given by Bhaskara, discoveries first found in his works include the now well known results for sin(a + b) and sin(a – b)

**Calculus**

His work, the Siddhanta Shiromani, is an astronomical treatise and contains many theories not found in earlier works. Preliminary concepts of infinitesimal calculus and mathematical analysis, along with a number of results in trigonometry, differential calculus and integral calculus that are found in the work are of particular interest.

Evidence suggests Bhaskara was acquainted with some ideas of differential calculus. It seems, however, that he did not understand the utility of his researches, and thus historians of mathematics generally neglect this achievement. Bhaskara also goes deeper into the ‘

*differential calculus*‘ and suggests the differential coefficient vanishes at an extremum value of the function, indicating knowledge of the concept of ‘

*infinitesimals*‘.

There is evidence of an early form of Rolle’s theorem in his work

- If f (a) = f (b) = 0, then f ‘ (x) = 0 for some x with a<x<b then
- He gave the result that if x =(approx) y then sin(y) – sin(x) =(approx) (y-x) cos(y), thereby finding the derivative of sine, although he never developed the notion of derivatives.

Bhaskara uses this result to work out the position angle of the ecliptic, a quantity required for accurately predicting the time of an eclipse.

In computing the instantaneous motion of a planet, the time interval between successive positions of the planets was no greater than a truti, or a 1⁄33750 of a second, and his measure of velocity was expressed in this infinitesimal unit of time.

He was aware that when a variable attains the maximum value, its differential vanishes.

He also showed that when a planet is at its farthest from the earth, or at its closest, the equation of the centre (measure of how far a planet is from the position in which it is predicted to be, by assuming it is to move uniformly) vanishes. He therefore concluded that for some intermediate position the differential of the equation of the centre is equal to zero.

In this result, there are traces of the general mean value theorem, one of the most important theorems in analysis, which today is usually derived from Rolle’s theorem. The mean value theorem was later found by Parameshvara in the 15th century in the Lilavati Bhasya, a commentary on Bhaskara’s Lilavati.

Madhava (1340–1425) and the Kerala School mathematicians (including Parameshvara) from the 14th century to the 16th century expanded on Bhaskara’s work and further advanced the development of calculus in India.

In computing the instantaneous motion of a planet, the time interval between successive positions of the planets was no greater than a truti, or a 1⁄33750 of a second, and his measure of velocity was expressed in this infinitesimal unit of time.

He was aware that when a variable attains the maximum value, its differential vanishes.

He also showed that when a planet is at its farthest from the earth, or at its closest, the equation of the centre (measure of how far a planet is from the position in which it is predicted to be, by assuming it is to move uniformly) vanishes. He therefore concluded that for some intermediate position the differential of the equation of the centre is equal to zero.

In this result, there are traces of the general mean value theorem, one of the most important theorems in analysis, which today is usually derived from Rolle’s theorem. The mean value theorem was later found by Parameshvara in the 15th century in the Lilavati Bhasya, a commentary on Bhaskara’s Lilavati.

Madhava (1340–1425) and the Kerala School mathematicians (including Parameshvara) from the 14th century to the 16th century expanded on Bhaskara’s work and further advanced the development of calculus in India.

**Astronomy**

Using an astronomical model developed by Brahmagupta in the 7th century, Bhaskara accurately defined many astronomical quantities, including, for example, the length of the sidereal year, the time that is required for the Earth to orbit the Sun, as 365.2588 days which is same as in Suryasiddhanta. The modern accepted measurement is 365.2563 days, a difference of just 3.5 minutes !

His mathematical astronomy text Siddhanta Shiromani is written in two parts: the first part on mathematical astronomy and the second part on the sphere.

The twelve chapters of the first part cover topics such as:

Mean longitudes of the planets.

True longitudes of the planets.

The three problems of diurnal rotation.

Syzygies.

Lunar eclipses.

Solar eclipses.

Latitudes of the planets.

Sunrise equation

The Moon’s crescent.

Conjunctions of the planets with each other.

Conjunctions of the planets with the fixed stars.

The paths of the Sun and Moon.

The second part contains thirteen chapters on the sphere. It covers topics such as:

Praise of study of the sphere.

Nature of the sphere.

Cosmography and geography.

Planetary mean motion.

Eccentric epicyclic model of the planets.

The armillary sphere.

Spherical trigonometry.

Ellipse calculations.

First visibilities of the planets.

Calculating the lunar crescent.

Astronomical instruments.

The seasons.

Problems of astronomical calculations.

His mathematical astronomy text Siddhanta Shiromani is written in two parts: the first part on mathematical astronomy and the second part on the sphere.

The twelve chapters of the first part cover topics such as:

Mean longitudes of the planets.

True longitudes of the planets.

The three problems of diurnal rotation.

Syzygies.

Lunar eclipses.

Solar eclipses.

Latitudes of the planets.

Sunrise equation

The Moon’s crescent.

Conjunctions of the planets with each other.

Conjunctions of the planets with the fixed stars.

The paths of the Sun and Moon.

The second part contains thirteen chapters on the sphere. It covers topics such as:

Praise of study of the sphere.

Nature of the sphere.

Cosmography and geography.

Planetary mean motion.

Eccentric epicyclic model of the planets.

The armillary sphere.

Spherical trigonometry.

Ellipse calculations.

First visibilities of the planets.

Calculating the lunar crescent.

Astronomical instruments.

The seasons.

Problems of astronomical calculations.

**Engineering**

The earliest reference to a perpetual motion machine date back to 1150, when Bhāskara II described a wheel that he claimed would run forever.

Bhāskara II used a measuring device known as Yasti-yantra. This device could vary from a simple stick to V-shaped staffs designed specifically for determining angles with the help of a calibrated scale.

Bhāskara II used a measuring device known as Yasti-yantra. This device could vary from a simple stick to V-shaped staffs designed specifically for determining angles with the help of a calibrated scale.

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