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NGC 6543

4-8 inch Telescope • Planetary Nebulae Detailed NGC 6543 finder map.

Finder map for NGC 6543

Its striking appearance and the popular name ‘Cat’s Eye Nebula’ have made it one of the most famous and recognizable deep-sky objects, frequently featured in books, documentaries, and popular science articles. Circumpolar for many northern latitudes, best observed when high in the sky. Very low or not visible for most southern hemisphere observers. Detecting the nebula as distinctly non-stellar and noticing its tiny, high–surface-brightness disk against the surrounding star field. The famous internal structure, faint outer halo, and central star are revealed only with large telescopes or imaging and lie beyond typical binocular views.

NGC 6543 finder optic view.

Finder scope & binocular view of NGC 6543

PropertyValue
Common namesCat’s Eye Nebula, Caldwell 6
Catalog namesC 6, NGC 6543, PGC 2921944, PK 096+29.1, PN G096.4+29.9
TypeEvolved Star
SubtypePlanetary Nebula
Coordinates17h 58m 33.40s, +66° 37’ 58.75”
SeasonMay - July
Best monthMid-June
Beginner friendlyNo
Visual rewardModerate
Filters requiredOIII, UHC
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude8.1
Size0.33 arcminutes x 0.33 arcminutes
ConstellationDraco

Observation Notes

Naked Eye

Not visible to the naked eye.

Binoculars

Appears as a star-like object with no obvious nebulosity. Its planetary nature is not apparent in binoculars.

Small Telescope

In a 5–6 inch telescope, appears as a small, bright, distinctly non-stellar disk with a noticeable blue-green color. An O-III filter greatly enhances contrast against surrounding stars.

Medium Telescope

The nebula’s oval disk is obvious, and the blue-green coloration is vivid. Under steady seeing and high magnification, the central star may be glimpsed with averted vision. Subtle internal brightness variations can be detected, though fine structure remains elusive.

Large Telescope

Reveals increased texture and uneven brightness across the nebula, with brighter regions and a more complex appearance at high magnification. The central star is more readily visible under good conditions. The extremely faint outer halo can be detected by experienced observers under very dark skies with patience and averted vision.