Yaʿqūb ibn Ṭāriq | |
|---|---|
یعقوب ابن طارق | |
| Born | fl. 8th century |
| Died | c. 796 |
| Academic work | |
| Era | Islamic Golden Age |
| Main interests | Astronomer andmathematician |
Yaʿqūb ibn Ṭāriq (Persian:یعقوب ابن طارق; referred to by some sources asYaʿqūb;[1] diedc. 796) was aPersian astronomer and mathematician who lived inBaghdad.

Yaʿqūb ibn Ṭāriq was active inBaghdad as anastronomer during the rule of the secondAbbasid caliph,al-Manṣūr (r. 754–775).[2][3] He seems not to have been aware ofPtolemaic astronomy,[2] and used aZoroastrian calendar, which consisted of 12 months of 30 days each, with any remaining days being added after the eighth month,Ābān.[2]
Yaʿqūb ibn Ṭāriq'streatiseTarkīb al‐aflāk dealt withcosmography (the placement and sizes of the heavenly bodies).[4] The estimations of their sizes and distances inTarkīb al‐aflāk were tabulated in the 11th century by the polymathal-Bīrūnī, in hiswork on India. According to al-Bīrūnī, Yaʿqūb ibn Ṭāriq gave theradius of the Earth as 1,050farsakhs, the diameter of theMoon andMercury as 5,000farsakhs (4.8 Earth radii), and the diameter of the other heavenly bodies (Venus, the Sun, Mars, Jupiter, and Saturn) as 20,000farsakhs (19.0 Earth radii).[5] He wrote that each of the planets had six associated spheres, that the Sun possessed two spheres, and the Moon three. He also spoke of planetaryepicycles and speeds.[6] His values for thelongitudes andapogees of celestial objects originated from aPersian set of astronomical tables, theZīǧ aš-šāh written byYazdegerd III, although he used methods originating from the work ofIndian astronomers to calculate thelunar phases.[1]
The ChristianastrologerIbn Hibintā mentioned Yaʿqūb, noting that he used the positions of the Sun and the stars to determine thelatitude of places.[7]
Works ascribed to Yaʿqūb ibn Ṭāriq include:[4]
An astrological work,Al‐maqālāt ("The Chapters"), is ascribed to Yaʿqūb ibn Ṭāriq by an unreliable source.[4]
Yaʿqūb ibn Ṭāriq'szij, written in around 770, was based on aSanskrit work,[4] thought to be similar to theBrāhmasphuṭasiddhānta. It was brought to the court ofal-Mansūr, the thirdcaliph of theFatimid Caliphate, fromSindh,[9] reportedly by the Sindhi astronomerKankah.[10]