Observing
What still works under a bright sky
A city sky does not dim the Moon or the planets at all — they are bright enough to ignore it. What it takes is everything faint and extended, and no filter gives all of that back. This guide is about working with what is left.
By Jean-Benoit Buisson
What the city takes
Extended faint objects — galaxies, most nebulae, the fainter clusters. They are dim against a bright background, and contrast, not brightness, is what has been lost.
What it leaves
The Moon, the planets, double stars, the brighter clusters, and the Sun with the appropriate equipment and the maker’s instructions. All of these are contrast-independent in a way that a galaxy is not.
What a filter actually does
A narrowband filter passes the wavelengths where emission nebulae emit and blocks the rest. On those specific objects it works well. On a galaxy — which emits across the spectrum, like the sky glow — it removes as much object as background.
Aperture and the city
Resolution scales with aperture regardless of the sky, so planetary detail improves in a city exactly as it would elsewhere. This is why a folded catadioptric on a small mount is a good city instrument: long focal length, small footprint, and the targets that survive are the ones it is best at.