Longomontanus's ASTRONOMIA DANICA in China

@article{Hashimoto1987LongomontanussAD,
  title={Longomontanus's ASTRONOMIA DANICA in China},
  author={Keizo Hashimoto},
  journal={Journal for the History of Astronomy},
  year={1987},
  volume={18},
  pages={110 - 95}
}
  • K. Hashimoto
  • Published 1 May 1987
  • Physics
  • Journal for the History of Astronomy
Many authors have so far worked on the Ch'ung-Chen Li-Shu (a, 1629-35) and its revised version, the Hsi-Yang Hsin-Fa Li-Shu (b, 1645), which can be regarded as an encyclopaedic work based on the astronomical knowledge introduced from the West (the chiefeditor was the Chinese high scholar-official, Hsu Kuang-Ch'i (c, 1562-1633). It is now well known that this work was based essentially on the Tychonic world system. However, as far as the theories of lunar and planetary motions as well as the… 
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References

SHOWING 1-5 OF 5 REFERENCES

How Copernicanism Took Root in Denmark and Norway

During the period 1578–1590 when at Hveen Tycho Brahe laid the foundations of modern observational astronomy, the chair of mathematics, including astronomy, at the University of Copenhagen was held

Galileo in China

The Geoheliocentric Mathematical Hypothesis in Sixteenth-Century Planetary Theory

It has become generally accepted that the earliest geoheliocentric representation of the planets' motions in which the majority of the planets orbited about the Sun appeared in 1588. For in this year

234-47) on the one hand, and Chiao-Shih L-Chih, chap. I (HFSS, chap. 64)

  • Astronomiae pars optica (Gesammelte Werke, ii
  • 1939

Professor Nathan Sivin has suggested that to some extent Longomontanus may have influenced the compilation of the Ch'ung-Chen Li-Shu (see his

  • Studia Copernicana
  • 1973