In celestial navigation the Moon is close enough to Earth that its observed altitude is affected by parallax β the apparent shift caused by the observerβs position on the rotating globe. The amount of shift depends on the Moonβs horizontal parallax (HP), the observerβs latitude (Ο) and the azimuth of the Moon at the moment of the sight.
The parallax correction is added to the raw observed altitude (Ho) to obtain a parallaxβfree altitude that can be used with the sight reduction tables. Because the Moon moves quickly, this correction is usually the largest of any celestial body.
The correction formula is derived from spherical trigonometry and can be expressed as:
HP = horizontal parallax of the Moon (Β°)
phi = observer latitude (Β°)
Az = azimuth of the Moon (Β°)
What is parallax correction in celestial navigation?
How does the Moon’s horizontal parallax affect observations?
What factors are considered in calculating parallax correction?
Why is it important to correct for parallax when observing the Moon?
How do I use this calculator to get the parallax correction?
Results are for informational purposes only and do not constitute professional advice.
