Calculation sequence
How this method is divided
- 01
The observer is placed at sea level at the supplied coordinates. Topocentric right ascension, declination, and distance include lunar parallax, light travel time, and aberration. Those coordinates are rotated to true-north azimuth and geometric altitude for the selected instant.
- 02
The page also shows a normally refracted altitude near the horizon and the next rise, set, and upper transit available for the location.
Working sheets
Two focused guides
Method selection
Where this method fits
- Location input is latitude and longitude for an ideal sea-level observer.
- Rise and set use an ideal horizon and a standard atmospheric-refraction convention.
- Use the eclipse finder for global shadow events, then inspect a contact instant here for local sky position.
Put the method to work
Use the working calculation
Evaluate another exact instant with the calculator described here, or return to the overview for the shared time conventions and supported era.
