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Messier 23 — Open Cluster in Sagittarius

NGC 6494

Open Cluster Showpiece (79/100)
Magnitude 5.5m OpenCluster Sagittarius Visible
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About M23

Description

M23 is a large, rich open star cluster in the constellation Sagittarius, located about 2,150 light-years from Earth. It contains roughly 150 stars spread across about 15 light-years of space. At magnitude 5.5 with an apparent diameter of about 27 arcminutes (nearly the size of the full Moon), it is a bright and impressive cluster. M23 is estimated to be about 300 million years old. Its brightest stars are blue-white main sequence stars of spectral type B9, with several notable red and orange giants adding color contrast.

Observing Tips

Located about 5 degrees northwest of M24 (the Small Sagittarius Star Cloud). At magnitude 5.5, it can be glimpsed with the naked eye under dark skies. Binoculars reveal a beautiful, large, rich cluster of dozens of stars. A telescope at 40-75x provides an outstanding view, resolving the cluster into a rich field of stars with arcs and chains. The cluster is large enough that too much magnification breaks up its visual impact. Best observed from July through September.

History

Discovered by Charles Messier on June 20, 1764. He described it as a cluster of small stars without any nebulosity. Admiral Smyth later described it as a 'splendid cluster' and noted the beautiful arcs and festoons of stars visible in moderate telescopes.

Fun Facts

M23 is one of the finest open clusters in Sagittarius for visual observation, though it is often overlooked in favor of the surrounding nebulae. Its stars form attractive curved chains and arcs that have delighted observers since the 18th century. The cluster lies in the rich Sagittarius Milky Way but is actually a foreground object, much closer to us than the dense star clouds behind it.

Observe

1Properties

Magnitude 5.5
Angular Size 16.8′
Distance 2,150 ly
Open Cluster [Distance: 2150 ly]

Position & Identifiers

RA 17h 56m 48.0s
Dec -19° 00' 60.0"
Constellation Sagittarius
Catalog M23
Also known as NGC 6494
Physical size
12 light-years across — about 1.4× the Sun-to-Sirius distance

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

Easy on Seestar S50
At 150mm under B5 skies you should resolve about 263 of 718 members.

3Visibility

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Best season May – Jul (peak: Jun)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

M23 · 16.8′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Pleiades M67 NGC 188 M23 380 Myr

Open clusters span more than four orders of magnitude in age — from newborn OB associations to ancient, metal-rich survivors.

7 Colour-Magnitude Diagram

A cluster's colour-magnitude diagram reveals its age: the bluer the turn-off point where the main sequence bends into red giants, the younger the cluster.

Loading member data…

Each point is a Gaia-DR3 member. Colour encodes spectral type; size reflects membership probability.

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8 Classification Decoder

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9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Chuck Ayoub. License: CC0. (Wikimedia Commons)

Credit: Chuck Ayoub. License: CC0. (Wikimedia Commons)

Skybred Feb 28, 2026

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