The Prutenic Tables (Tabulae prutenicae from Prutenia meaning "Prussia", Prutenische oder Preußische Tafeln), were an ephemeris (astronomical tables) by the astronomer Erasmus Reinhold published in 1551 (reprinted in 1562, 1571 & 1585). They are sometimes called the Prussian Tables after Albert I, Duke of Prussia, who supported Reinhold and financed the printing. Reinhold calculated this new set of astronomical tables based on Nicolaus Copernicus' De revolutionibus orbium coelestium, the epochal exposition of Copernican heliocentrism published in 1543. Throughout his explanatory canons, Reinhold used as his paradigm the position of Saturn at the birth of the Duke, on 17 May 1490. With these tables, Reinhold intended to replace the Alfonsine Tables; he added redundant tables to his new tables so that compilers of almanacs familiar with the older Alfonsine Tables could perform all the steps in an analogous manner.
Several tables based on the Alfonsine Tables were published after the publication of the Prussian Tables. Copernicus's heliocentric claims were slow to be accepted by all European astronomers. Rather, the Prussian Tables became popular in German speaking countries for nationalistic and confessional reasons, and it is through these tables that Copernicus's reputation was established as a skilled mathematician or an astronomer on a par with Ptolemy, and helped to disseminate the Copernicus' methods of calculating the positions of astronomical objects throughout the Holy Roman Empire. They eventually replaced the Alfonsine tables, which astronomers and astrologers had used for 300 years.
The Alfonsine tables in Table of the Stars by Regiomontanus also were used by sailors and sea explores during the fourteenth and fifteenth centuries.
Christopher Clavius used Reinhold's Prutenic Tables and Copernicus' work as a basis for the calendar reform instituted under Pope Gregory XIII.
Decades later, in Prague, Johannes Kepler compiled the Rudolphine Tables, based on Tycho Brahe's lifetime of astronomical observations, which were the most extensive and accurate observations until his time.