The Determination of the Equator-Point for Observing Star Declinations
The deolinations of the stars are by definition reckoned from the celestial equator. However this great circle is not marked on the sky; therefore, instead of dejclinations, the polar distances of the stars are measured, as the position of the pole can be found by observing a star in upper and lower...
Published in: | International Astronomical Union Colloquium |
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Main Author: | |
Format: | Article in Journal/Newspaper |
Language: | English |
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Cambridge University Press (CUP)
1975
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Subjects: | |
Online Access: | http://dx.doi.org/10.1017/s0252921100051125 |