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NGC 281

4-8 inch Telescope • Star Forming Regions

NGC 281 (NGC281)

Image: Chuck Ayoub

NGC 281 finder map.

Finder map for NGC 281

Widely known by its modern nickname, the “Pacman Nebula,” derived from its resemblance in photographs to the iconic video game character. It is a familiar object in modern amateur astronomy, particularly in astrophotography. Best observed from the Northern Hemisphere, where it reaches high altitude. From the Southern Hemisphere it remains very low on the northern horizon and is difficult to observe, becoming inaccessible from far-southern latitudes. The main visual challenge is detecting the nebula’s faint, diffuse glow against the background sky, which demands dark, transparent conditions and the use of a nebula filter. The small dark globules and finer structural details seen in images lie beyond reliable visual detection in 4–8 inch telescopes.

NGC 281 finder optic view.

Finder scope & binocular view of NGC 281

PropertyValue
Common namesPacman Nebula, Sh2-184
Catalog namesNGC 281, SH 2-184, LBN 616, Ced 3
TypeInterstellar Medium
SubtypeHII Region
Coordinates0h 52m 25.10s, +56° 33’ 54.00”
SeasonSeptember - November
Best monthOctober
Beginner friendlyNo
Visual rewardModerate
Filters requiredUHC
LP toleranceLow
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude-
Size35.0 arcminutes x 30.0 arcminutes
ConstellationCassiopeia

Observation Notes

Naked Eye

Not visible.

Binoculars

The nebulosity is not visible; under exceptionally dark skies the central star cluster may be suspected as a very faint, non-stellar patch, but no nebulous glow is seen.

Small Telescope

In 4–6 inch apertures under dark skies, the IC 1590 cluster is visible. With a UHC or O-III filter, a very faint, large, diffuse glow from the surrounding nebula can be detected, though contrast remains low.

Medium Telescope

With 8–12 inches and a suitable nebular filter, the nebulosity becomes more apparent as a broad, uneven glow, and the characteristic dark bay forming the “Pacman mouth” can be discerned as a contrast feature. Additional stars in the central cluster are resolved.

Large Telescope

In apertures of roughly 14 inches and larger under excellent conditions, the nebula shows increased contrast with subtle texture and brightness variations across its extent. Very small dark features may be suspected as tiny notches against the brighter background, but these impressions are delicate and seeing-dependent rather than clearly defined structures.

Observing NGC 281 from your latitude

From mid-northern latitudes (~40°N), NGC 281 reaches a maximum altitude of about 73° above the northern horizon and is circumpolar — it never sets, staying above the horizon all night, best placed October - December.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)87°Circumpolar (24h)
50°N (≈ London, Prague, Vancouver)83°Circumpolar (24h)
40°N (≈ Madrid, New York, Beijing)73°Circumpolar (24h)
30°N (≈ Cairo, Houston, Delhi)63°20h 28m
20°N (≈ Honolulu, Mexico City, Mumbai)53°16h 38m
10°N (≈ Chennai, Bangalore, Bangkok)43°14h 13m
(≈ Quito, Nairobi, Singapore)33°12h 8m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)13°7h 43m
35°S (≈ Sydney, Cape Town, Buenos Aires)Below horizonNever rises
45°S (≈ Christchurch, Hobart, Puerto Montt)Below horizonNever rises

Altitudes and durations are geometric, computed for each latitude, independent of date. Set your location below for tonight's exact rise, transit, and set times.

Visibility from New York
Circumpolar: this object never sets from New York.
Altitude
Azimuth
Max Altitude
74.1°
Rises
CP
Sets
CP
Transit
06:19 AM
NGC 281: RA 0h 52m 25.10s, Dec +56° 33' 54.00"
Computed for the night of July 13–14, 2026 (New York).