Loading…
Loading contentLoading…
Loading contentFrom catalogue to eyepiece. This suite turns the platform's computed twilight, Moon, and planet data into a night's observing plan — what to see, when it is highest, and when the sky is truly dark — while the conditions that decide whether a session happens come only from connected providers, never invented.
The observing planners — tonight, visibility, target, Moon, planet, deep-sky, season, twilight, darkness, altitude, meridian-transit, equipment, astrophotography, and session — each built on the platform's real computed twilight, Moon, and planet data and its observing equipment, sites, and techniques.
14 entriesThe architecture-ready interfaces for the external conditions observing depends on — weather, seeing, transparency, cloud cover, and Bortle sky brightness. Each is wired into the planners and awaits a connected provider; no conditions are ever invented.
5 entriesHow high a target rides through the night — its altitude against time — so an observer can catch it near the meridian, above the murk of the horizon.
Plans an imaging session — the target's framing against the sensor, the Moon and darkness windows, and the capture technique — reusing the real camera, mount, and image-stacking entities.
The window of real darkness on a given night — after astronomical twilight ends and while the Moon is down. The hours that matter most for faint targets.
Plans a tour of galaxies, nebulae, and clusters by season, constellation, and difficulty, matched against the night's darkness and the target's altitude. The deep sky, night by night.
Matches targets to gear — which objects suit binoculars, a small refractor, or a large Dobsonian — using the platform's real equipment catalogue and the target's brightness and size.
When a target crosses the meridian — its highest, sharpest point in the sky — the ideal moment to observe or image it. Computed from its right ascension and the local sidereal time.
The Moon's phase, illumination, and rise and set for a chosen night — the single biggest factor in deep-sky observing. Computed, not assumed.
Which planets are visible tonight and where, from the platform's computed planetary positions and their altitudes through the night. Jupiter and Saturn to Mercury's fleeting apparitions.
What each season brings — the constellations overhead, the meteor showers, and the signature deep-sky objects — so a year of observing can be planned in advance.
Assembles a full observing session — an ordered list of targets timed to their best moments through a single night — from the visibility, altitude, and darkness plans. Exportable as a calendar or a printable plan.
Builds an observing list from the graph's real objects — stars, deep-sky objects, planets — and checks each against the night's visibility. A bridge from the catalogue to the eyepiece.
What is worth observing tonight from a given place, drawn together from the platform's computed twilight, Moon, and planet positions. The plan updates with the observer's clock and location, which stay on the device.
The civil, nautical, and astronomical twilight times for a given place and date — when true darkness begins and ends. Computed from the Sun's position.
When and whether a target clears the horizon and the twilight for a given night, from its coordinates and the observer's latitude. Built on the computed rise, set, and twilight times.
Each planner and integration is a first-class knowledge-graph entity resolved through the Scientific Data Engine. The planners reuse the computed live-sky data of the platform (twilight, the Moon, the planets) and its observing equipment, sites, and techniques — no ephemeris is re-implemented. The integrations are architecture-ready interfaces: weather, seeing, transparency, cloud, and Bortle data appear only from connected providers, never fabricated, following the same honesty envelope as the live-sky providers. The observing location stays on the device. See source quality.