Math 2.0

Astronomy and astrophysics Definition

Hour angle

Builds on Equatorial coordinate systemCelestial sphere

Definition

Fix an observer on the Earth and a direction uu 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 uu is the half great circle from the north celestial pole through uu to the south celestial pole. The hour angle HH of uu is the angle along the celestial equator from the local meridian to the hour circle of uu, measured westward. It is given in hours, with 1h=15∘1^{\mathrm h} = 15^\circ, either in [0h,24h)[0^{\mathrm h}, 24^{\mathrm h}) or in (−12h,12h](-12^{\mathrm h}, 12^{\mathrm h}].

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: H=LST−αH = \mathrm{LST} - \alpha. Example: a star on the meridian has H=0H = 0; six sidereal hours later it has H=6hH = 6^{\mathrm h}. Non-example: right ascension is counted eastward from the March equinox; it is fixed for a star, while HH grows with time. A negative hour angle means the object has not yet reached the meridian.

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  1. Celestial sphere concept
  2. Equatorial coordinate system concept
  3. Hour angle definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Hour_angle
About this page
TagTYE6885WXJ
URIm2://TYE6885WXJ
Kinddefinition
WritingW0 stub
MSC85A04
DefinesHour angle
UsesEquatorial coordinate system, Celestial sphere
Changed3 November 2026

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