Triquetrum (astronomy)

Triquetrum of Copernicus

The triquetrum (derived from the Latin tri- ["three"] and quetrum ["cornered"]) was the medieval name for an ancient astronomical instrument first described by Ptolemy (c. 90 – c. 168) in the Almagest (V. 12). Also known as Parallactic Rulers, it was used for determining altitudes of heavenly bodies. Ptolemy calls it a "parallactic instrument" and seems to have used it to determine the zenith distance and parallax of the Moon.[1][2][self-published source?]

  1. ^ Kelley, D., Milone, E., (2005), Exploring Ancient Skies: An Encyclopedic Survey of Archaeoastronomy, pages 77-79. Birkhäuser.
  2. ^ Gassendi, P., Thill, O., (2002) The Life of Copernicus (1473-1543), pages 118-120. Xulon Press.