Retain horizon-grazing cases instead of forcing a visibility label
A fixed celestial direction traces a daily circle around a celestial pole as Earth rotates. Depending on latitude and declination, that circle can cross the horizon, stay entirely above it or stay entirely below it. Circumpolar describes the observer-dependent geometry, not a special physical type of star.
Learning outcome: At latitude 60°, compare declinations−60°,−30°,0°,30° and 60°. Retain both extrema and note the two grazing boundaries. Change latitude without changing declination and explain which evidence belongs to the observer.
Starting recap
Keep celestial and local frames, solar and sidereal time, phase and eclipse geometry, and source rendering versus direct observation distinct.
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Try
At latitude 60° and declination 30°, the lower culmination touches altitude 0° and upper culmination reaches 60°. The model labels grazing, with the path above the horizon except at the limiting touch. At declination 60° the lower altitude is 30° and the source is strictly circumpolar.
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Why should a source that just touches the horizon be treated differently from a robustly circumpolar one?
Experiment
At latitude 60°, compare declinations−60°,−30°,0°,30° and 60°. Retain both extrema and note the two grazing boundaries. Change latitude without changing declination and explain which evidence belongs to the observer.
Separate rising/setting from circumpolar and horizon-grazing cases
Worked teaching model · synthetic values · Spherical geometric horizon, point source and fixed declination. sin h = sinφ sinδ + cosφ cosδ cosH. Extremes at H 0 and 180°. Equality with horizon is recorded as grazing, not silently classified as always strictly above/below. No atmospheric refraction or terrain.
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The same celestial declination can rise and set for one latitude yet remain circumpolar for another.
A geometric grazing case is not robust real visibility: refraction, terrain, finite disk and coordinate uncertainty can change it. Sidereal hours here describe the rotation fraction, not a civil clock timetable.
Boundary classification: A limiting culmination touches the geometric horizon.
| Quantity | Value | Unit |
|---|---|---|
| Upper culmination altitude | 60.00000 | degrees |
| Lower culmination altitude | -1.272222e-14 | degrees |
| Geometric hours above horizon per rotation | 24.00000 | sidereal hours |
| Visibility class | 2 | −1 never / 0 rises and sets / 1 circumpolar / 2 grazes |
Use the supplied screen-based records and diagrams. No direct Sun viewing, instrument aiming or outdoor observation is required or requested.
The same celestial declination can rise and set for one latitude yet remain circumpolar for another.
A geometric grazing case is not robust real visibility: refraction, terrain, finite disk and coordinate uncertainty can change it. Sidereal hours here describe the rotation fraction, not a civil clock timetable.
Captures preserve recipes and replay their calculated results. They are synthetic model evidence, not physical measurements.
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At the equator, how long is a fixed δ+60° point direction above the ideal horizon, and what are its extrema?
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