Āryabhaṭa or Aryabhatt (Devanāgarī: आर्यभट) (476 – 550 CE) is the first of the great mathematician-astronomers of the classical age of Indian mathematics and Indian astronomy. Born in 476 CE in Kusumpur, Bihar — Aryabhatt's intellectual brilliance remapped the boundaries of mathematics and astronomy. In 499 CE, at the age of 23, he wrote a text on astronomy and an unparallel treatise on mathematics called Aryabhatiyam. He formulated the process of calculating the motion of planets and the time of eclipses. Aryabhatt was the first to proclaim that the earth is round, it rotates on its axis, orbits the sun and is suspended in space - 1000 years before Copernicus published his heliocentric theory. He is also acknowledged for calculating p (Pi) to four decimal places: 3.1416 and the sine table in trigonometry. Centuries later, in 825 CE, the Arab mathematician, Mohammed Ibna Musa credited the value of Pi to the Indians, "This value has been given by the Hindus." And above all, his most spectacular contribution was the concept of zero without which modern computer technology would have been non-existent. Aryabhatt was a colossus in the field of mathematics.
Date of Aryabhata
When sixty times sixty years and three quarters of the yugas (of this yuga) had elapsed, twenty three years had then passed since my birth.
In Aryabhata's system of measuring time, 3600 of the Kali era corresponds to mean noon at Ujjain, on March 21, 499 CE (Sunday). So Aryabhata was born in 476 CE. All other authors known by name are later to Aryabhata I, and mention his theories while refuting them or correcting them. The dates for Varahamihira have been verified also by independent techniques.
Aryabhata's major contributions
Propounded the view that earth was round
Aryabhata compared the Earth to a Kadamba flower as explained in the following quotes.
Gola 6: The globe of the Earth stands (supportless) in space at the centre of the celestial sphere….The Earth is circular on all sides.
Gola 7: Just as the bulb of a Kadamba flower is surrounded by blossoms on all sides, so also is the globe of the Earth surrounded by all creatures whether living on land or in water.
(The very term Gola means sphere or round. Vatesvara, explicitly mentions a popular belief about the Earth being supported on the back of a turtle, and points out its deficiencies, "What does the turtle rest upon, etc". But no other reputed astronomer seems to have taken such possibilities seriously enough even to contest them.)
Propounded in the 5th Century CE that the Earth rotates and not the celestial sphere
Gola 9: Just as a man in a moving boat sees the stationary objects on the land moving in the opposite direction, so also the stationary stars are seen by a person at Lanka as moving exactly towards the West. (Lanka is an imaginary point on the equator at which the Meridian of Ujjayini intersects the Equator. Ujjayini is the modern-day Ujjain. Thus, Aryabhata's Lanka is below the current-day Lanka. The Meridian of Ujjayini is was later copied by instituting the Meridian of Greenwich. )
Gola 10: It only appears to an observer at Lanka as if the celestial sphere and the asterisms and planets move to the West…to cause their rising and setting.
(This view is rejected by later authors, like Varahamihira, Brahmagupta etc. on the grounds that if it is the Earth that rotates, then clothes on a line will fly, and the falcon, which rises high in the sky will not be able to find its way back. Others say, the tops of trees will be destroyed, the ocean will invade the land etc.)
Worked out the duration of the day at the poles
Gola 16: The gods living in the north at the Meru mountain (north pole) see one half of the Bhagola (celestial sphere with its centre at the centre of the earth) as revolving from left to right (i.e., clockwise); the demons living in the south at Badvâmukha (south pole) see the other half rotating from right to left (i.e., anti-clockwise).
Gola 17: The gods (at the north pole) see the sun after sunrise for half a solar year; so do the demons (at the south pole). Those living on the moon see the sun for half a lunar month; the humans here see it for half a civil day.
(Wooden and iron models were used to demonstrate the spheres. Bhagola is the celestial sphere centred at the centre of the earth, while Khagola is the sphere centred on the observer. The principal circles of the Bhagola are the celestial equator, the ecliptic etc., while the principal circles of the Khagola are the horizon, the meridian, the prime vertical etc. For the related concepts of spherical astronomy, consult any text on spherical astronomy.)
Given an accurate value of pi (p)
Rational approximation to pi
Ganita 10: 104 multiplied by 8 and added to 62000 is the approximate circumference of a circle whose diameter is 20,000.
That is, pi = 62832/20000 = 3.1416. This value of pi was widely used in the Arabic world. In Europe, this value is cited by Simon Stevin in his book on navigation, The Haven Finding Art, as the value known to the "ancients" which he states (correctly) as far superior to any value known to the Greeks. Unlike what current-day historians would have us believe, Egypt does not mean Greece to Simon Stevin. In any case Aryabhata's value is better than that of Ptolemy (3.141666), who lived in Alexandria, in Egypt. Simon Stevin, a Dutch mathematician, astronomer and navigator, introduced the decimal system in Europe, c. 1580, and gives a table of sine values like Aryabhata, correcting the earlier table given by Nunes. Better values of pi were subsequently obtained in Europe using the "Gregory" series for the arctangent, and faster convergent methods, all of which are found in works of the Aryabhata school, which were imported into Europe in the 16th and 17th c. (Gregory does not claim originality.) The Sanskrit term for approximate is asanna, a term also used in the sulba sutra. The Chinese had a better value of pi than Aryabhata, just as al Kashi had a more accurate value of pi than Nîlkantha. However, none of those values had the potential of the calculus, and neither Chinese nor al Kashi had equally accurate sine values. (Ptolemy does not even mention sines.) The Chinese value may well have been a fluke, while al-Kashi's value was based on extremely laborious computation. Neither had the future potential or the sweep that Aryabhata's approximation techniques had. These techniques were later developed by his school into the "Taylor" series for arctangent, the sine and the cosine.
Aryabhata is also known as Aryabhata I to distinguish him from the later mathematician of the same name who lived about 400 years later. Al-Biruni has not helped in understanding Aryabhata's life, for he seemed to believe that there were two different mathematicians called Aryabhata living at the same time. He therefore created a confusion of two different Aryabhatas which was not clarified until 1926 when B Datta showed that al-Biruni's two Aryabhatas were one and the same person.
We know the year of Aryabhata's birth since he tells us that he was twenty-three years of age when he wrote Aryabhatiya which he finished in 499. We have given Kusumapura, thought to be close to Pataliputra (which was refounded as Patna in Bihar in 1541), as the place of Aryabhata's birth but this is far from certain, as is even the location of Kusumapura itself. As Parameswaran writes in:-
… no final verdict can be given regarding the locations of Asmakajanapada and Kusumapura.
We do know that Aryabhata wrote Aryabhatiya in Kusumapura at the time when Pataliputra was the capital of the Gupta empire and a major centre of learning, but there have been numerous other places proposed by historians as his birthplace. Some conjecture that he was born in south India, perhaps Kerala, Tamil Nadu or Andhra Pradesh, while others conjecture that he was born in the north-east of India, perhaps in Bengal. In  it is claimed that Aryabhata was born in the Asmaka region of the Vakataka dynasty in South India although the author accepted that he lived most of his life in Kusumapura in the Gupta empire of the north. However, giving Asmaka as Aryabhata's birthplace rests on a comment made by Nilakantha Somayaji in the late 15th century. It is now thought by most historians that Nilakantha confused Aryabhata with Bhaskara I who was a later commentator on the Aryabhatiya.
We should note that Kusumapura became one of the two major mathematical centres of India, the other being Ujjain. Both are in the north but Kusumapura (assuming it to be close to Pataliputra) is on the Ganges and is the more northerly. Pataliputra, being the capital of the Gupta empire at the time of Aryabhata, was the centre of a communications network which allowed learning from other parts of the world to reach it easily, and also allowed the mathematical and astronomical advances made by Aryabhata and his school to reach across India and also eventually into the Islamic world.
As to the texts written by Aryabhata only one has survived. However Jha claims that:-
… Aryabhata was an author of at least three astronomical texts and wrote some free stanzas as well.
The surviving text is Aryabhata's masterpiece the Aryabhatiya which is a small astronomical treatise written in 118 verses giving a summary of Hindu mathematics up to that time. Its mathematical section contains 33 verses giving 66 mathematical rules without proof. The Aryabhatiya contains an introduction of 10 verses, followed by a section on mathematics with, as we just mentioned, 33 verses, then a section of 25 verses on the reckoning of time and planetary models, with the final section of 50 verses being on the sphere and eclipses.
There is a difficulty with this layout which is discussed in detail by van der Waerden. Van der Waerden suggests that in fact the 10 verse Introduction was written later than the other three sections. One reason for believing that the two parts were not intended as a whole is that the first section has a different meter to the remaining three sections. However, the problems do not stop there. We said that the first section had ten verses and indeed Aryabhata titles the section Set of ten giti stanzas. But it in fact contains eleven giti stanzas and two arya stanzas. Van der Waerden suggests that three verses have been added and he identifies a small number of verses in the remaining sections which he argues have also been added by a member of Aryabhata's school at Kusumapura.
The mathematical part of the Aryabhatiya covers arithmetic, algebra, plane trigonometry and spherical trigonometry. It also contains continued fractions, quadratic equations, sums of power series and a table of sines. Let us examine some of these in a little more detail.
First we look at the system for representing numbers which Aryabhata invented and used in the Aryabhatiya. It consists of giving numerical values to the 33 consonants of the Indian alphabet to represent 1, 2, 3, … , 25, 30, 40, 50, 60, 70, 80, 90, 100. The higher numbers are denoted by these consonants followed by a vowel to obtain 100, 10000, …. In fact the system allows numbers up to 1018to be represented with an alphabetical notation. Ifrah in  argues that Aryabhata was also familiar with numeral symbols and the place-value system. He writes:-
… it is extremely likely that Aryabhata knew the sign for zero and the numerals of the place value system. This supposition is based on the following two facts: first, the invention of his alphabetical counting system would have been impossible without zero or the place-value system; secondly, he carries out calculations on square and cubic roots which are impossible if the numbers in question are not written according to the place-value system and zero.
Next we look briefly at some algebra contained in the Aryabhatiya. This work is the first we are aware of which examines integer solutions to equations of the form by = ax + c and by = ax - c, where a, b, c are integers. The problem arose from studying the problem in astronomy of determining the periods of the planets. Aryabhata uses the kuttaka method to solve problems of this type. The word kuttaka means "to pulverise" and the method consisted of breaking the problem down into new problems where the coefficients became smaller and smaller with each step. The method here is essentially the use of the Euclidean algorithm to find the highest common factor of a and b but is also related to continued fractions.
Aryabhata gave an accurate approximation for π. He wrote in the Aryabhatiya the following:-
Add four to one hundred, multiply by eight and then add sixty-two thousand. the result is approximately the circumference of a circle of diameter twenty thousand. By this rule the relation of the circumference to diameter is given.
This gives π = 62832/20000 = 3.1416 which is a surprisingly accurate value. In fact π = 3.14159265 correct to 8 places. If obtaining a value this accurate is surprising, it is perhaps even more surprising that Aryabhata does not use his accurate value for π but prefers to use √10 = 3.1622 in practice. Aryabhata does not explain how he found this accurate value but, for example, Ahmad considers this value as an approximation to half the perimeter of a regular polygon of 256 sides inscribed in the unit circle. However, in  Bruins shows that this result cannot be obtained from the doubling of the number of sides. Another interesting paper discussing this accurate value of π by Aryabhata is  where Jha writes:-
Aryabhata I's value of π is a very close approximation to the modern value and the most accurate among those of the ancients. There are reasons to believe that Aryabhata devised a particular method for finding this value. It is shown with sufficient grounds that Aryabhata himself used it, and several later Indian mathematicians and even the Arabs adopted it. The conjecture that Aryabhata's value of π is of Greek origin is critically examined and is found to be without foundation. Aryabhata discovered this value independently and also realised that π is an irrational number. He had the Indian background, no doubt, but excelled all his predecessors in evaluating π. Thus the credit of discovering this exact value of π may be ascribed to the celebrated mathematician, Aryabhata I.
We now look at the trigonometry contained in Aryabhata's treatise. He gave a table of sines calculating the approximate values at intervals of 90degrees/24 = 3degrees 45'. In order to do this he used a formula for sin(n+1)x - sin nx in terms of sin nx and sin (n-1)x. He also introduced the versine (versin = 1 - cosine) into trigonometry.
Other rules given by Aryabhata include that for summing the first n integers, the squares of these integers and also their cubes. Aryabhata gives formulae for the areas of a triangle and of a circle which are correct, but the formulae for the volumes of a sphere and of a pyramid are claimed to be wrong by most historians. For example Ganitanand in  describes as "mathematical lapses" the fact that Aryabhata gives the incorrect formula V = Ah/2 for the volume of a pyramid with height h and triangular base of area A. He also appears to give an incorrect expression for the volume of a sphere. However, as is often the case, nothing is as straightforward as it appears and Elfering (see for example ) argues that this is not an error but rather the result of an incorrect translation.
This relates to verses 6, 7, and 10 of the second section of the Aryabhatiya and in  Elfering produces a translation which yields the correct answer for both the volume of a pyramid and for a sphere. However, in his translation Elfering translates two technical terms in a different way to the meaning which they usually have. Without some supporting evidence that these technical terms have been used with these different meanings in other places it would still appear that Aryabhata did indeed give the incorrect formulae for these volumes.
We have looked at the mathematics contained in the Aryabhatiya but this is an astronomy text so we should say a little regarding the astronomy which it contains. Aryabhata gives a systematic treatment of the position of the planets in space. He gave the circumference of the earth as 4 967 yojanas and its diameter as 1 5811/24 yojanas. Since 1 yojana = 5 miles this gives the circumference as 24 835 miles, which is an excellent approximation to the currently accepted value of 24 902 miles. He believed that the apparent rotation of the heavens was due to the axial rotation of the Earth. This is a quite remarkable view of the nature of the solar system which later commentators could not bring themselves to follow and most changed the text to save Aryabhata from what they thought were stupid errors!
Aryabhata gives the radius of the planetary orbits in terms of the radius of the Earth/Sun orbit as essentially their periods of rotation around the Sun. He believes that the Moon and planets shine by reflected sunlight, incredibly he believes that the orbits of the planets are ellipses. He correctly explains the causes of eclipses of the Sun and the Moon. The Indian belief up to that time was that eclipses were caused by a demon called Rahu. His value for the length of the year at 365 days 6 hours 12 minutes 30 seconds is an overestimate since the true value is less than 365 days 6 hours.
Bhaskara I who wrote a commentary on the Aryabhatiya about 100 years later wrote of Aryabhata:-
Aryabhata is the master who, after reaching the furthest shores and plumbing the inmost depths of the sea of ultimate knowledge of mathematics, kinematics and spherics, handed over the three sciences to the learned world.
Rate this post: