Armillary Spheres in China

  • Jiang Xiaoyuan
Reference work entry
DOI: https://doi.org/10.1007/978-1-4020-4425-0_8446

The equatorial armillary sphere was a traditional Chinese astronomical instrument used to observe celestial bodies in an equatorial coordinate system. Its origin is still not very clear. Astronomer Luoxia Hong (ca. 100 BCE) of the Western Han Dynasty was probably the first maker of this instrument which possessed a very basic form.

The early equatorial armilla was composed of two layers: the outside layer included a meridian circle, equatorial circle, and vertical circle – all three of these were fixed. The inside layer included a polar axis, right ascension circle, and sighting tube. The right ascension circle could rotate around the polar axis, and the sighting tube could rotate in the right ascension circle freely so it could point to everywhere in the sky.

In the Tang Dynasty (AD 618–907), a third layer was added to the equatorial armillary which included an ecliptic (the band of the zodiac through which the Sun apparently moves in its yearly course) circle and a circle of the...

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References

  1. Study Group for the History of Chinese Astronomy. Zhong Guo Tian Wen Xue Shi (The History of Chinese Astronomy). Beijing: Science Press, 1981.Google Scholar
  2. Wei Zheng, Linghu Defen. Sui Shu (The History of Sui Dynasty). Vol. 19. Beijing: Zhonghua Press, 1973.Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg New York 2008

Authors and Affiliations

  • Jiang Xiaoyuan

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