المرجع الالكتروني للمعلوماتية
المرجع الألكتروني للمعلوماتية

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Ulugh Beg  
  
1894   02:01 صباحاً   date: 25-10-2015
Author : J B J Delambre
Book or Source : Histoire de l,astronomie du moyen âge
Page and Part : ...


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Date: 22-10-2015 2152
Date: 23-10-2015 1992
Date: 22-10-2015 1391

Born: 1393 in Soltaniyeh, Timurid, Persia (now Iran)
Died: 27 October 1449 in Samarkand, Timurid empire

 

Ulugh Beg was the grandson of the conqueror Timur, who is often known as Tamerlane (from Timur-I-Leng meaning Timur the Lame, a title of contempt used by his Persian enemies). Although in this archive we are primarily interested in Ulugh Beg's achievements in mathematics and astronomy, we need to examine the history of the area since it had such a major impact on Ulugh Beg's life.

Timur, Ulugh Beg's grandfather, came from the Turkic Barlas tribe which was a Mongol tribe that was living in Transoxania, today essentially Uzbekistan. He united several Turko-Mongol tribes under his leadership and set out on a conquest, with his armies of mounted archers, of the area now occupied by Iran, Iraq, and eastern Turkey.

Shortly after his grandson Ulugh Beg was born, Timur invaded India and by 1399 he had taken control of Delhi. Timur continued his conquests by extending his empire to the west from 1399 to 1402, winning victories over the Egyptian Mamluks in Syria and the Ottomans in a battle near Ankara. Timur died in 1405 leading his armies into China.

After Timur's death his empire was disputed among his sons. Ulugh Beg's father Shah Rukh was the fourth son of Timur and, by 1407, he had gained overall control of most of the empire, including Iran and Turkistan regaining control of Samarkand. Samarkand had been the capital of Timur's empire but, although his grandson Ulugh Beg had been brought up at Timur's court, he was seldom in that city. When Timur was not on one of his military campaigns he moved with his army from place to place and his court, including his grandson Ulugh Beg, travelled with him.

In 1409 Shah Rukh decided to make Herat in Khorasan (today in western Afghanistan) his new capital. Shah Rukh ruled there making it a trading and cultural centre. He founded a library there and became a patron of the arts. However Shah Rukh did not give up Samarkand, rather he decided to give it to his son Ulugh Beg who was more interested in making the city a cultural centre than he was in politics or military conquest. Although Ulugh Beg was only sixteen years old when his father put him in control of Samarkand, he became his father's deputy and he became ruler of the Mawaraunnahr region.

Ulugh Beg was primarily a scientist, in particular a mathematician and an astronomer. However, he certainly did not neglect the arts, writing poetry and history and studying the Qur'an. In 1417, to push forward the study of astronomy, Ulugh Beg began building a madrasah which is a centre for higher education. The madrasah, fronting the Rigestan Square in Samarkand, was completed in 1420 and Ulugh Beg then began to appoint the best scientists he could find to positions there as lecturers.

Ulugh Beg invited al-Kashi to join his madrasah in Samarkand, as well as around sixty other scientists including Qadi Zada. There is little doubt that, other than Ulugh Beg himself, al-Kashi was the leading astronomer and mathematician at Samarkand. Letters which al-Kashi wrote to his father have survived. These were written from Samarkand and give a wonderful description of the scientific life there. The contents of one of these letters has only recently been published, see [5].

In the letters al-Kashi praises the mathematical abilities of Ulugh Beg but of the other scientists in Samarkand, only Qadi Zada earned his respect. Ulugh Beg led scientific meetings where problems in astronomy were freely discussed. Usually these problems were too difficult for all except al-Kashi and the letters confirm that al-Kashi was the closest collaborator of Ulugh Beg at his madrasah in Samarkand.

In addition to the madrasah, Ulugh Beg built an observatory at Samarkand, the construction of this beginning in 1428. The Observatory, which was circular in shape, had three levels. It was over 50 metres in diameter and 35 metres high. The director of the Observatory was Ali-Kudschi, a Muslim astronomer. Al-Kashi and other mathematicians and astronomers appointed to the madrasah also worked at Ulugh Beg's Observatory.

Among the instruments specially constructed for the Observatory was a quadrant so large that part of the ground had to be removed to allow it to fit in the Observatory. There was also a marble sextant, a triquetram and an armillary sphere. The achievements of the scientists at the Observatory, working there under Ulugh Beg's direction and in collaboration with him, are discussed in detail in [4]. This excellent book records the main achievements which include the following: methods for giving accurate approximate solutions of cubic equations; work with the binomial theorem; Ulugh Beg's accurate tables of sines and tangents correct to eight decimal places; formulae of spherical trigonometry; and of particular importance, Ulugh Beg's Catalogue of the stars, the first comprehensive stellar catalogue since that of Ptolemy.

This star catalogue, the Zij-i Sultani, set the standard for such works up to the seventeenth century. Published in 1437, it gives the positions of 992 stars. The catalogue was the results of a combined effort by a number of people working at the Observatory including Ulugh Beg, al-Kashi, and Qadi Zada. As well as tables of observations made at the Observatory, the work contained calendar calculations and results in trigonometry.

The trogonometric results include tables of sines and tangents given at 1° intervals. These tables display a high degree of accuracy, being correct to at least 8 decimal places. The calculation is built on an accurate determination of sin 1° which Ulugh Beg solved by showing it to be the solution of a cubic equation which he then solved by numerical methods. He obtained

sin 1° = 0.017452406437283571

The correct approximation is

sin 1° = 0.017452406437283512820

which shows the remarkable accuracy which Ulugh Beg achieved.

Observations made at the Observatory brought to light a number of errors in the computations of Ptolemy which had been accepted without question up to that time. Data from his Observatory allowed Ulugh Beg to calculate the length of the year as 365 days 5 hours 49 minutes 15 seconds, a fairly accurate value. He produced data relating to the Sun, the Moon and the planets. His data for the movements of the planets over a year is, like so much of his work, very accurate [1]:-

... the difference between Ulugh Beg's data and that of modern times relationg to [Saturn, Jupiter, Mars, Venus] falls within the limits of two to five seconds.

Ulugh Beg's politics were not up to his science and, after his father's death in 1447, he was unable to retain power despite being an only son. He was eventually put to death at Samarkand at the instigation of his own son 'Abd al-Latif. His tomb was discovered in 1941 in the mausoleum built by Timur in Samarkand. It was discovered that Ulugh Beg had been buired in his clothes which is known to indicate that he was considered a martyr. The injuries inflicted on him were evident when his body was examined [1]:-

... the third cervical vertebra was severed by a sharp instrument in such a way that the main portion of the body and an arc of that vertebra were cut cleanly; the blow, struck from the left, also cut through the right corner of the lower jaw and its lower edge.


 

  1. T N Kari-Niazov, Biography in Dictionary of Scientific Biography (New York 1970-1990). 
    http://www.encyclopedia.com/topic/Ulugh-Beg.aspx
  2. Biography in Encyclopaedia Britannica. 
    http://www.britannica.com/eb/article-9074183/Ulugh-Beg

Books:

  1. J B J Delambre, Histoire de l'astronomie du moyen âge (Paris, 1819).
  2. T N Kary-Nijazov, The Ulugh Beg school of astronomy (Russian) (Tashkent, 1967).

Articles:

  1. M Bagheri, A newly found letter of al-Kashi on scientific life in Samarkand, Historia Math. 24 (3) (1997), 241-256.
  2. M S Bulatov, Ulugh Beg's observatory in Samarkand (Russian), Istor.-Astronom. Issled. 18 (1986), 199-216.
  3. H Hobden, Ulugh Beg and his Observatory in Samarkand, Astronomy Now 2 (1988), 32-36.
  4. T N Kary-Nijazov, Ulugh Beg and Subah Jai Singh (Russian), in 1966 Phys. Math. Sci. in the East 'Nauka' (Moscow, 1966), 247-255.
  5. V Lutsky, Ulugh Beigh's ancient star atlas, Astromony and Space 1 (1972), 342-344.
  6. M Shevchenko, An analysis of errors in the star catalogues of Ptolemy and Ulugh Beg, J. Hist. Astronom. 21 (2) (1990), 187-201.
  7. A U Usmanov, A short survey of the history of the development of astronomy in the medieval East up to the age of Ulugh Beg (Russian), Questions on the history of mathematics and astronomy I, Trudy Samarkand. Gos. Univ. (N.S.) Vyp. 229 (1972), 60-97.

 




الجبر أحد الفروع الرئيسية في الرياضيات، حيث إن التمكن من الرياضيات يعتمد على الفهم السليم للجبر. ويستخدم المهندسون والعلماء الجبر يومياً، وتعول المشاريع التجارية والصناعية على الجبر لحل الكثير من المعضلات التي تتعرض لها. ونظراً لأهمية الجبر في الحياة العصرية فإنه يدرّس في المدارس والجامعات في جميع أنحاء العالم. ويُعجب الكثير من الدارسين للجبر بقدرته وفائدته الكبيرتين، إذ باستخدام الجبر يمكن للمرء أن يحل كثيرًا من المسائل التي يتعذر حلها باستخدام الحساب فقط.وجاء اسمه من كتاب عالم الرياضيات والفلك والرحالة محمد بن موسى الخورازمي.


يعتبر علم المثلثات Trigonometry علماً عربياً ، فرياضيو العرب فضلوا علم المثلثات عن علم الفلك كأنهما علمين متداخلين ، ونظموه تنظيماً فيه لكثير من الدقة ، وقد كان اليونان يستعملون وتر CORDE ضعف القوسي قياس الزوايا ، فاستعاض رياضيو العرب عن الوتر بالجيب SINUS فأنت هذه الاستعاضة إلى تسهيل كثير من الاعمال الرياضية.

تعتبر المعادلات التفاضلية خير وسيلة لوصف معظم المـسائل الهندسـية والرياضـية والعلمية على حد سواء، إذ يتضح ذلك جليا في وصف عمليات انتقال الحرارة، جريان الموائـع، الحركة الموجية، الدوائر الإلكترونية فضلاً عن استخدامها في مسائل الهياكل الإنشائية والوصف الرياضي للتفاعلات الكيميائية.
ففي في الرياضيات, يطلق اسم المعادلات التفاضلية على المعادلات التي تحوي مشتقات و تفاضلات لبعض الدوال الرياضية و تظهر فيها بشكل متغيرات المعادلة . و يكون الهدف من حل هذه المعادلات هو إيجاد هذه الدوال الرياضية التي تحقق مشتقات هذه المعادلات.