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NGC 6960

4-8 inch Telescope • Supernova Remnants NGC 6960 finder map.

Finder map for NGC 6960

Popularly known as the ‘Witch’s Broom Nebula’ due to its evocative shape. It is a classic and highly sought-after target for amateur astronomers and astrophotographers. Best viewed when high in the sky (above 40° altitude) to minimize atmospheric extinction, which is critical due to its low surface brightness. Its very low surface brightness makes it highly sensitive to light pollution. The nebula’s large angular extent means it is best explored with low magnification and wide-field eyepieces, often by sweeping along its length rather than viewing it all at once.

NGC 6960 finder optic view.

Finder scope & binocular view of NGC 6960

PropertyValue
Common namesWitch’s Broom Nebula, Western Veil Nebula, Filamentary Nebula
Catalog namesC 34, NGC 6960, LBN 191, PGC 3517684, Ced 182a
TypeInterstellar Medium
Subtype-
Coordinates20h 45m 38.00s, +30° 42’ 30.00”
SeasonJuly - September
Best monthAugust
Beginner friendlyMarginal
Visual rewardModerate
Filters requiredOIII, UHC
LP toleranceLow
Minimum equipmentBinoculars
Optimal equipmentMedium telescope
Magnitude7.0
Size70.0 arcminutes x 6.0 arcminutes
ConstellationCygnus

Observation Notes

Naked Eye

Not visible.

Binoculars

Extremely difficult; even from pristine dark-sky sites it is usually invisible. Some observers report fleeting, uncertain hints by holding a UHC or O-III filter over a binocular eyepiece, but detection is marginal and not reliable.

Small Telescope

In 4–6 inch apertures under dark skies, an O-III or UHC filter is essential. At low power, appears as a very faint, elongated wisp of nebulosity running near the star 52 Cygni, with low contrast against the background.

Medium Telescope

With 8–12 inches and an O-III filter, the filament becomes easier to follow, and the characteristic broom-like form is more apparent. The nebula shows increased contrast and length, but detail remains subtle and diffuse.

Large Telescope

In apertures of roughly 14 inches and larger under excellent conditions, the filament breaks into finer, thread-like strands with faint extensions visible using averted vision. The structure remains delicate and contrast-limited, appearing as overlapping wisps rather than sharply defined or truly three-dimensional features.