The sun, the moon, the planets and the turn of the seasons — not in general, but over the exact spot you are standing on, on the exact date you name.
The sun's clock runs fast and slow against the one on your wall, and traces this figure over a year. The moon takes 29.53 days to come back to the same phase. Neither number is rounded for you here, and neither is looked up — both fall out of the same positions everything else on this page is read from.
Positions are read from NASA’s DE441 ephemeris and reduced to your horizon. Nothing is interpolated from a calendar and nothing is drawn from a table of typical years — the sky over you on 3 March 1974 is computed the same way as the sky over you tonight.
These are not pictures taken through a telescope and they are not stock. Each one is a surface evaluated at the moment named, lit from where the sun actually was, seen from where the observer actually is. Change the instant and the shadow moves — which is why the same machinery can draw a body as it will look on a night that has not happened yet.
Five small apps each take one piece of this sky. Every figure they show is computed on the spot for where you are standing.
The apps →Sun and moon times, phase and illumination, twilight bands, planet positions and visibility, eclipse and event dates, season instants, star rise and set — for any coordinate and any date, thousands of years either way. One request, one number, no interpretation attached.
Want it wired into something you already run, or built into software of your own? Ask for that instead. And if you have looked at this and concluded it could not be done — not at that span, that volume or that date — bring it here and let us give it a second thought.
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