Geometry
Civil, nautical and astronomical twilight use the Sun’s center at roughly −6°, −12° and −18° altitude. These geometric conventions make planning repeatable.
Move the Sun below the horizon and connect the −6°, −12° and −18° twilight boundaries to practical changes in sky brightness. These are geometric definitions, not fixed exposure recipes.
Civil twilight ends at −6°, nautical twilight at −12°, and astronomical twilight at −18° solar elevation. The boundaries describe solar geometry; actual sky brightness also depends on atmosphere and local conditions.
Watch the histogram and foreground, not just the clock. As twilight fades, shutter time usually lengthens and the balance between sky, artificial light and foreground changes quickly.
Use solar altitude to choose the kind of light you want, then meter the real scene. For faint Milky Way work, −18° is a useful darkness boundary, but Moon and light pollution can still dominate.
Move from −4° to −10° to −19°. Notice how the planning question changes from balancing twilight to protecting faint night-sky contrast.
Twilight thresholds follow NOAA definitions. Atmospheric refraction, aerosols, clouds, Moon, airglow and light pollution are not modeled in this teaching view.
Civil, nautical and astronomical twilight use the Sun’s center at roughly −6°, −12° and −18° altitude. These geometric conventions make planning repeatable.
Real sky brightness does not jump at those angles. Aerosols, humidity, clouds, elevation and light pollution change how quickly the sky darkens and how color develops.
Higher twilight can retain landscape detail and color; deeper twilight increases contrast for faint stars. The useful point depends on whether your subject is foreground, Moon, bright stars or faint Milky Way structure.
Use solar altitude to predict the phase, then judge the real sky. Check histogram, foreground readability, Moon altitude and local light dome before deciding exposure strategy.