This is an old revision of this page, as edited by Gunnar.Kaestle (talk | contribs) at 20:56, 18 December 2024 (Excerpt from vertical circle, see Talk:Vertical_circle#one_article_per_concept). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Revision as of 20:56, 18 December 2024 by Gunnar.Kaestle (talk | contribs) (Excerpt from vertical circle, see Talk:Vertical_circle#one_article_per_concept)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)
The vertical circle is an optical instrument used to measure angles in astronomy, which name is derived from the mathematical concept of the vertical circle from spherical trigonometry. It is a device for measuring astronomical angles, which can be rotated in altitude and azimuth and is similar in design to the meridian circle. It consists of a telescope (in astronomical geodesy occasionally also with a reflecting telescope), which is mounted on a horizontal tilting axis and is supported by a stable altazimuth mount. The angular movements around the tilting and standing axes are measured with large, finely divided circles and a reading microscope.
Instruments like this were more common in 19th century observatories and were important for locating and recording coordinates in the cosmos, and observatories often had various other instruments for certain functions as well as advanced clocks of the period. The popularly known example in the observatories, was the Great Refractors which became larger and larger and came to have a dominating effect to the point that observatories were moved simply to have better conditions for their biggest telescope, in the modern style where observatories often have one instrument only in a remote location on the Earth or even in outer space. However, in the 19th century it was more basic with observatories often making recording of coordinates of different items and to determine the shape of the Earth and times.