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| The '''vertical circle''' is an ] used to measure angles in ], which name is derived from the mathematical concept of the ] from ]. It is a device for measuring astronomical angles, which can be rotated in altitude and azimuth and is similar in design to the ]. It consists of a ] (in ] occasionally also with a ]), which is mounted on a horizontal tilting axis and is supported by a stable ] mount. The angular movements around the tilting and standing axes are measured with large, finely divided circles and a reading ]. | The '''vertical circle''' is an ] used to measure angles in ], which name is derived from the mathematical concept of the ] from ]. It is a device for measuring astronomical angles, which can be rotated in altitude and azimuth and is similar in design to the ]. It consists of a ] (in ] occasionally also with a ]), which is mounted on a horizontal tilting axis and is supported by a stable ] mount. The angular movements around the tilting and standing axes are measured with large, finely divided circles and a reading ].<ref>{{cite book |last=Chauvenet |first=William |author-link=William Chauvenet |date=1863 |title=A Manual of Spherical and Practical Astronomy |volume=II: Theory and use of astronomical instruments |url=https://books.google.de/books?id=AVI8pz41ia8C&pg=PA315 |location=Philadelphia |publisher=J.B. Lippincott & Co. |page=315 |quote=Chapter VII. The Altitude and Azimuth Instrument. Sometimes the horizontal circle is reduced to small and designed simply as a finder or to set the instrument approximately at a given azimuth while the vertical is made of unusually large dimensions and is intended for most refined astronomical measurement. The instrument is then known simply as a ''vertical circle''. Such is the ERTEL Vertical Circle of the Pulkova Observatory, the telescope of which has a focal length of 77 inches, and its vertical circle a diameter of 43 inches.}}</ref> | ||
| 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. | 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. | ||
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Revision as of 00:34, 19 December 2024
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.
See also
References
- Chauvenet, William (1863). A Manual of Spherical and Practical Astronomy. Vol. II: Theory and use of astronomical instruments. Philadelphia: J.B. Lippincott & Co. p. 315.
Chapter VII. The Altitude and Azimuth Instrument. Sometimes the horizontal circle is reduced to small and designed simply as a finder or to set the instrument approximately at a given azimuth while the vertical is made of unusually large dimensions and is intended for most refined astronomical measurement. The instrument is then known simply as a vertical circle. Such is the ERTEL Vertical Circle of the Pulkova Observatory, the telescope of which has a focal length of 77 inches, and its vertical circle a diameter of 43 inches.