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NGC 2392

4-8 inch Telescope • Planetary Nebulae Detailed NGC 2392 finder map.

Finder map for NGC 2392

NGC 2392 is widely known by the traditional nickname “Eskimo Nebula” (also sometimes called the “Clownface Nebula”), making it a popular outreach target and a frequent subject in amateur astronomy literature and astrophotography. Best observed when high in the sky to reduce atmospheric extinction and improve contrast, which is important for this compact planetary nebula. The visual challenge lies in distinguishing the bright inner shell from the fainter surrounding envelope using moderate to high magnification, and in glimpsing the central star against the bright nebulosity. Much finer filamentary structure in the extended halo seen in images lies beyond the visual reach of 4–8 inch telescopes.

NGC 2392 finder optic view.

Finder scope & binocular view of NGC 2392

PropertyValue
Common namesEskimo Nebula, Clown-faced Nebula, Lion Nebula
Catalog namesC 39, NGC 2392, PK 197+17.1, PN G197.8+17.3
TypeEvolved Star
SubtypePlanetary Nebula
Coordinates7h 29m 10.77s, +20° 54’ 42.47”
SeasonDecember - February
Best monthMid-January
Beginner friendlyYes
Visual rewardHigh
Filters requiredOIII, UHC
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude9.1
Size0.9 arcminutes x 0.9 arcminutes
ConstellationGemini

Observation Notes

Naked Eye

Not visible.

Binoculars

Appears stellar and indistinguishable from a faint star, with no nebulous character.

Small Telescope

In 4–6 inch apertures, appears at low power as a slightly fuzzy, bluish-green star. At higher magnification (100× or more), its small, round disk becomes apparent. An O-III filter helps the nebula stand out by suppressing surrounding stars.

Medium Telescope

With 8–12 inches, the bright inner region is clearly defined, and the central star, near magnitude 10.5, may be glimpsed intermittently during moments of steady seeing. The nebula responds very well to an O-III filter, which markedly improves contrast.

Large Telescope

In apertures of roughly 14 inches and larger under dark skies, careful high-magnification viewing can reveal a brighter inner shell surrounded by a much fainter, diffuse outer envelope. Subtle textural impressions within the inner region may be suspected under excellent seeing, but all fine structure remains low contrast and seeing-dependent.