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- Q2051578 subject Q7238070.
- Q2051578 abstract "In spherical astronomy, the parallactic angle is the angle between the great circle through a celestial object and the zenith, and the hour circle of the object. It is usually denoted q. In the triangle zenith—object—celestial pole, the parallactic angle will be the angle at the celestial object. Despite its name, this angle is unrelated with parallax. The parallactic angle is zero when the object crosses the meridian.".
- Q2051578 wikiPageWikiLink Q1061971.
- Q2051578 wikiPageWikiLink Q1129343.
- Q2051578 wikiPageWikiLink Q1195520.
- Q2051578 wikiPageWikiLink Q120200.
- Q2051578 wikiPageWikiLink Q1205231.
- Q2051578 wikiPageWikiLink Q1399772.
- Q2051578 wikiPageWikiLink Q146657.
- Q2051578 wikiPageWikiLink Q148901.
- Q2051578 wikiPageWikiLink Q165074.
- Q2051578 wikiPageWikiLink Q2105737.
- Q2051578 wikiPageWikiLink Q218673.
- Q2051578 wikiPageWikiLink Q23718.
- Q2051578 wikiPageWikiLink Q3380435.
- Q2051578 wikiPageWikiLink Q4213.
- Q2051578 wikiPageWikiLink Q43261.
- Q2051578 wikiPageWikiLink Q677971.
- Q2051578 wikiPageWikiLink Q6999.
- Q2051578 wikiPageWikiLink Q7238070.
- Q2051578 wikiPageWikiLink Q82806.
- Q2051578 wikiPageWikiLink Q934.
- Q2051578 comment "In spherical astronomy, the parallactic angle is the angle between the great circle through a celestial object and the zenith, and the hour circle of the object. It is usually denoted q. In the triangle zenith—object—celestial pole, the parallactic angle will be the angle at the celestial object. Despite its name, this angle is unrelated with parallax. The parallactic angle is zero when the object crosses the meridian.".
- Q2051578 label "Parallactic angle".