The Celestial Meridian, Upper Culmination, and Lower Culmination

The line that runs across the sky through the celestial north pole, the celestial south pole, and your zenith, and all the way around the celestial sphere, is called the celestial meridian. The celestial poles divide it into two parts. The part corresponding to your longitude is the upper meridian. The other part of the celestial meridian lies on the opposite side of the celestial sphere. This is the lower meridian. Stars that are on the celestial meridian and on its upper meridian part are also at their upper culmination, meaning they are at their highest point above the horizon. Celestial bodies that are on the lower meridian are at their lower culmination. Note that when you are close enough to the Earth's poles, or when observing stars near the poles, you can see the same celestial body both at its upper and lower culmination. The clearest example is the summer Sun in the Arctic, which north of the Arctic Circle does not set below the horizon during midsummer. At its lowest point it is at lower culmination on the lower meridian, and at midday it is at its highest point on the upper meridian.

 


Hamburg VII 2026