Sadr's astronomical work represents an ongoing revision of Ptolemaic astronomy. In that context, he undertook to correct the works of two of his predecessors, namely Nasir al-Din al-Tusi and Qutb al-Din al-Shirazi. The models of the last two were developed in their two respective works, the Tadhkira and the Tuhfa. Sadr took it upon himself to solve the problems they did not tackle, and to supply answers to the subtleties they did not address.
