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NGC 6302

10+ inch Telescope • Challenging Planetaries NGC 6302 finder map.

Finder map for NGC 6302

Its dramatic butterfly-like appearance in astrophotography has made it one of the most famous planetary nebulae in outreach and popular media, often used to illustrate the late stages of stellar evolution. This striking morphology, however, is far more apparent in images than at the eyepiece. Well placed for Southern Hemisphere observers. From mid- to high-northern latitudes it remains low on the southern horizon and requires exceptionally clear conditions. At the eyepiece, the nebula appears compact and irregular, with hints of asymmetry rather than a clearly defined butterfly shape. Tracing the faint extensions and internal structure requires large apertures, high magnification, and excellent seeing. The central star is extremely difficult and effectively beyond reach for most amateur telescopes.

NGC 6302 finder optic view.

Finder scope & binocular view of NGC 6302

PropertyValue
Common namesBug Nebula, Butterfly Nebula
Catalog namesC 69, NGC 6302, SH 2-6, RCW 124, Ced 139, …
TypeEvolved Star
SubtypePlanetary Nebula
Coordinates17h 13m 44.50s, -37° 06’ 11.16”
SeasonMay - July
Best monthMid-June
Beginner friendlyYes
Visual rewardHigh
Filters requiredOIII, UHC
LP toleranceHigh
Minimum equipmentMedium telescope
Optimal equipmentLarge telescope
Magnitude9.6
Size1.48 arcminutes x 1.48 arcminutes
ConstellationScorpius

Observation Notes

Naked Eye

Not visible.

Binoculars

Not visible.

Small Telescope

Very difficult. Appears as a tiny, high–surface-brightness object that is nearly stellar and easily overlooked. An O-III filter is strongly recommended to confirm its non-stellar nature, where it may show a slight elongation rather than a clean disk.

Medium Telescope

With an O-III filter and steady seeing, the nebula shows a distinctly non-stellar, elongated form. A brighter central bar may be apparent, but the full bipolar or “bow-tie” structure is subtle and not sharply defined.

Large Telescope

Under dark skies with an O-III filter, the nebula becomes strikingly irregular and strongly elongated. The opposing lobes are clearly suggested rather than crisply outlined, and brightness variations across the nebula give a strong impression of complex structure. Even in large apertures, details remain delicate rather than sharply resolved.