Triquetrum (astronomy)

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Triquetrum of Copernicus

The triquetrum (derived from the Latin tri- ["three"] and quetrum ["cornered"]) was the medieval name for an ancient

zenith distance and parallax of the Moon.[1][2][self-published source?
]

Design

The triquetrum performed the same function as the

celestial object could be calculated.[1][3]

Use

The triquetrum was one of the most popular astronomical instruments until the invention of the telescope, it could measure angles with a better precision than the

Copernicus describes its use in the fourth book of the De revolutionibus orbium coelestium (1543) under the heading "Instrumenti parallactici constructio."[2] The instrument was also used by Tycho Brahe[4]
in the same century.

See also

Notes

  1. ^ a b Kelley, D., Milone, E., (2005), Exploring Ancient Skies: An Encyclopedic Survey of Archaeoastronomy, pages 77-79. Birkhäuser.
  2. ^ a b c Gassendi, P., Thill, O., (2002) The Life of Copernicus (1473-1543), pages 118-120. Xulon Press.
  3. ^ Krebs, R., (2004), Groundbreaking Scientific Experiments, Inventions, and Discoveries of the Middle Ages and the Renaissance, page 225. Greenwood Publishing Group.
  4. ^ Christianson, J., (2000), On Tycho's Island: Tycho Brahe and His Assistants, 1570-1601, pages 73-75. Cambridge University Press.

External links