The Bortle scale: how dark is your sky?

The Bortle scale describes how bright the night sky is at a place, from class 1 (a pristine dark sky far from any city) to class 9 (an inner-city sky). It was proposed by the amateur astronomer John E. Bortle in 2001 and is now the usual way to say how much light pollution a site has.

The 9 classes at a glance

ClassSkyWhat you seeFaintest stars (naked eye)
1Excellent dark skyThe Milky Way casts faint shadows; the zodiacal light is obvious≈ 7.6–8.0
2Typical truly dark siteDetailed Milky Way, clouds are black holes in the sky≈ 7.1–7.5
3Rural skyMilky Way still rich; some glow on the horizon≈ 6.6–7.0
4Rural / suburban transitionMilky Way visible but without detail near the horizon≈ 6.1–6.5
5Suburban skyMilky Way faint, washed out near the horizon≈ 5.6–6.0
6Bright suburban skyMilky Way only overhead, if at all≈ 5.1–5.5
7Suburban / urban transitionSky grey-orange, Milky Way invisible≈ 4.6–5.0
8City skyOnly bright constellations are recognisable≈ 4.1–4.5
9Inner-city skyMoon, planets and a few bright stars≈ 4.0 at best

What it means for observing

The Moon, planets and double stars are fine even from a city (classes 7–9). Bright star clusters need class 5–6 or darker. Galaxies, nebulae and the Milky Way really need class 4 or better — moving from class 7 to class 3 can show you ten times more stars.

How NightSkyCast estimates the class

We estimate the Bortle class for every point from NASA satellite images of night lights (VIIRS Black Marble): each lit area adds brightness that fades with distance. It is an estimate, not a measurement — for exact values astronomers use a sky quality meter (SQM).

How to find a darker sky

Open the sky map, turn on the light pollution layer and look for green and dark-blue areas 30–60 km from your town, away from the glow of big cities. Tap a spot to see its class and tonight’s forecast — a dark site is only useful on a clear, moonless night.

Open map

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