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Ephemeriden

Ephemeriden erlauben die Berechnung der Standorte von Sonne, Mond und Planeten
TODO: Ptolemäischen Planetentafeln
ca: 1080: Toledaner Tafeln
1252: Alfonsinische Tafeln
1551: Prutenische Tafeln
1627 (Druck): Rudolfinische Tafeln
JPL Horizons
XEphem

TODO

Johannes Stöffler (der Nachfolger von Regiomontanus), war der erfolgreichste Ephemeridenproduzent seiner Zeit
Stoefller was born in 1452. When late in life he became professor of mathematics at T~ibingen, he already enjoyed a virtual monopoly with the ephemerides prepared by himself and Jacob Pflaum; these had continued through 1531 those of Regiomontanus. At Tübingen he extended his calculations to 1551, and these were published there posthumously in 1531.
Johannes Stadius
At about the same time that Stoeffler died (1530), Johannes Stadius was born (1527). In the 1560s Stadius taught mathematics at Louvain, and later he worked in Paris. Stadius was the first computer to adopt the Copernican parameters for a major ephemeris. His own tables were, in effect, the successors to Stoeffler's, and their users included Tycho Brahe.
[…]
the error patterns of Stadius closely resemble those of Maestlin, Magini, Origanus, and others who followed the Copernican parameters
[…]
In the Regiomontanus and Stoeftler ephemerides, the error in longitude for Mars is sometimes as large as 5°
[…]
However, in 1625, the Copernican errors for Mars reached nearly 5°
1457 beobachtete Georg von Peuerbach eine Eklipse und bemerkte, dass sie 8 Minuten früher begonnen hatte, wie von den Alfonsinischen Tafeln vorausgesagt. Daraufhin berechnete er seine eigenen Ephemeriden, die Tabulae Eclipsum.

See also

Ephemeriden Texte
Swiss Ephemeris
Tools/Software for Astronomy

Index