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M92

4-8 inch Telescope • Globular Clusters Detailed

M92

Image: ESA/Hubble & NASA

M92 finder map.

Finder map for M92

A classic ‘showpiece’ object for amateur astronomers, often viewed alongside its brighter neighbor M13. It serves as a textbook example of a dense, old globular cluster. Best observed when high in the sky to reduce atmospheric extinction and take advantage of steadier seeing for resolving stars. The main challenge is resolving stars as deeply toward the cluster’s intensely condensed core as possible. In 4–8 inch telescopes, the outer regions are well resolved, while the core remains only partially resolved, and the faint outer halo can be difficult to trace under less-than-ideal skies.

M92 finder optic view.

Finder scope & binocular view of M92

PropertyValue
Common namesMessier 92, Hercules Globular Cluster
Catalog namesM 92, NGC 6341, Mel 168
TypeStellar Cluster
SubtypeGlobular Cluster
Coordinates17h 17m 07.39s, +43° 08’ 09.40”
SeasonMay - July
Best monthMid-June
Beginner friendlyYes
Visual rewardHigh
Filters requiredNone
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude6.5
Size14.0 arcminutes x 14.0 arcminutes
ConstellationHercules

Observation Notes

Naked Eye

Generally not visible; under pristine, very dark skies a few experienced observers report a barely perceptible, diffuse suspicion with averted vision, but naked-eye detection is rare and uncertain.

Binoculars

Easily visible as a small, bright, circular, fuzzy patch of light that is clearly non-stellar but unresolved.

Small Telescope

In 4–6 inch apertures, appears as a bright, compact globular with a strongly condensed core surrounded by a grainy halo. Under excellent conditions, a few of the brightest peripheral stars may be suspected with averted vision, while the core remains unresolved.

Medium Telescope

With 8–12 inches, numerous stars resolve around the outer regions, producing a finely sparkling appearance, while the core remains an intensely bright, unresolved mass.

Large Telescope

In apertures of roughly 14 inches and larger, stars are resolved well inward from the halo toward the center, giving the cluster a rich, densely packed appearance. The core remains extremely concentrated and only partially resolved, emphasizing stellar density rather than open structure.

Observing M92 from your latitude

From mid-northern latitudes (~40°N), M92 reaches a maximum altitude of about 87° above the northern horizon and stays above the horizon for about 19h 8m, best placed June - August.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)73°Circumpolar (24h)
50°N (≈ London, Prague, Vancouver)83°Circumpolar (24h)
40°N (≈ Madrid, New York, Beijing)87°19h 8m
30°N (≈ Cairo, Houston, Delhi)77°16h 31m
20°N (≈ Honolulu, Mexico City, Mumbai)67°14h 47m
10°N (≈ Chennai, Bangalore, Bangkok)57°13h 22m
(≈ Quito, Nairobi, Singapore)47°12h 6m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)27°9h 27m
35°S (≈ Sydney, Cape Town, Buenos Aires)12°6h 42m
45°S (≈ Christchurch, Hobart, Puerto Montt)3h 7m

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

From New York tonight, M92 rises at 01:04 PM, is highest in the sky at 10:45 PM (88° above the horizon), and sets at 08:25 AM.

Altitude
Azimuth
Max Altitude
87.6°
Rises
01:04 PM
Sets
08:25 AM
Transit
10:45 PM
M92: RA 17h 17m 07.39s, Dec +43° 08' 09.40"
Computed for the night of July 13–14, 2026 (New York).