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NGC 6210

4-8 inch Telescope • Planetary Nebulae Detailed NGC 6210 finder map.

Finder map for NGC 6210

Best observed when high in the sky to reduce atmospheric extinction and improve contrast. Its northern declination favors Northern Hemisphere observers. The main visual challenge is confirming its non-stellar nature at moderate to high magnification and detecting subtle elongation or asymmetry in the nebula’s shape. Much finer internal structures such as jets and filaments seen in images lie beyond the visual reach of 4–8 inch telescopes.

NGC 6210 finder optic view.

Finder scope & binocular view of NGC 6210

PropertyValue
Common namesTurtle Nebula
Catalog namesNGC 6210, PGC 1693983, PK 043+37.1, PN G043.1+37.7
TypeEvolved Star
SubtypePlanetary Nebula
Coordinates16h 44m 29.52s, +23° 47’ 59.42”
SeasonMay - July
Best monthJune
Beginner friendlyMarginal
Visual rewardModerate
Filters requiredOIII, UHC
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude8.8
Size0.35 arcminutes x 0.35 arcminutes
ConstellationHercules

Observation Notes

Naked Eye

Not visible.

Binoculars

Not visible as a nebula; at best may appear stellar in very large binoculars under exceptionally dark skies.

Small Telescope

In 4–6 inch apertures, appears at higher magnification (100× or more) as a small, bright, distinctly non-stellar object resembling a slightly fuzzy, out-of-focus star. A bluish-green tint may be noticeable under good conditions.

Medium Telescope

With 8–12 inches, the nebula resolves into a small disk with a slightly irregular or boxy outline. The blue-green coloration is often apparent, and the object responds well to increased magnification.

Large Telescope

In apertures of roughly 14 inches and larger, high magnification under steady seeing may reveal subtle unevenness or mottling in surface brightness across the disk. Any internal jet-like features are an extreme visual challenge and, if suspected at all, appear only as fleeting contrast effects rather than distinct structures.