Astronomy and astrophysics Definition
Hour angle
Definition
Fix an observer on the Earth and a direction on the celestial sphere, not at a celestial pole. The local meridian is the half great circle from the north celestial pole through the zenith to the south celestial pole. The hour circle of is the half great circle from the north celestial pole through to the south celestial pole. The hour angle of is the angle along the celestial equator from the local meridian to the hour circle of , measured westward. It is given in hours, with , either in or in .
Remarks
The hour angle uses the celestial equator of the equatorial coordinate system, but counts from a meridian that turns with the Earth. So it equals the local sidereal time minus the right ascension: . Example: a star on the meridian has ; six sidereal hours later it has . Non-example: right ascension is counted eastward from the March equinox; it is fixed for a star, while grows with time. A negative hour angle means the object has not yet reached the meridian.
Reading path
To understand this page from the ground up, read these 3 pages in order. The foundations come first.
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- no evidence level
- Celestial sphere concept
- Equatorial coordinate system concept
- Hour angle definition
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About this page
| Tag | TYE6885WXJ |
|---|---|
| URI | m2://TYE6885WXJ |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A04 |
| Defines | Hour angle |
| Uses | Equatorial coordinate system, Celestial sphere |
| Changed | 3 November 2026 |
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