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NGC 6826

4-8 inch Telescope • Planetary Nebulae Detailed NGC 6826 finder map.

Finder map for NGC 6826

A famous and beloved object in the amateur astronomy community, often used as a showpiece to demonstrate the quirks of human vision and the utility of nebula filters. Best observed when high in the sky to reduce atmospheric extinction and improve contrast. The primary visual challenge is experiencing the famous “blinking” effect, which becomes apparent when alternating between direct and averted vision as the bright central star dominates the view. Much fainter structural features such as low-ionization knots detected in images lie beyond the visual reach of 4–8 inch telescopes.

NGC 6826 finder optic view.

Finder scope & binocular view of NGC 6826

PropertyValue
Common namesBlinking Planetary Nebula, Blinking Nebula
Catalog namesC 15, NGC 6826, PGC 2906369, PK 083+12.1, PN G083.5+12.7
TypeEvolved Star
SubtypePlanetary Nebula
Coordinates19h 44m 48.15s, +50° 31’ 30.25”
SeasonJune - August
Best monthMid-July
Beginner friendlyYes
Visual rewardModerate
Filters requiredOIII, UHC
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude8.8
Size0.6 arcminutes x 0.6 arcminutes
ConstellationCygnus

Observation Notes

Naked Eye

Not visible.

Binoculars

In very dark, transparent skies, large binoculars (around 70 mm or larger) may show it as a faint, star-like point; it does not appear nebular at binocular magnifications.

Small Telescope

In 4–6 inch apertures, appears as a slightly out-of-focus “star” with a noticeable greenish tint. The characteristic blinking effect is readily apparent, and at higher magnification the object resolves into a tiny, fuzzy disk.

Medium Telescope

With 8–12 inches, the blinking effect is very pronounced. The small disk is clearly defined, the central star is sharp and bright, and the green coloration is often obvious. An O-III filter enhances the nebular disk while dimming the central star, increasing contrast.

Large Telescope

In apertures of roughly 14 inches and larger, high magnification and good seeing reveal subtle unevenness or a slightly annular appearance within the disk, while the central star remains prominent. Under excellent conditions, the extremely faint outer halo may be suspected with averted vision; an O-III filter enhances the nebular shell and suppresses the central star.