Menu

Caldwell 108 — Globular Cluster in Musca

NGC 4372

Globular Cluster Showpiece (77/100)
Magnitude 7.8m GlobularCluster Musca Visible
Star Map
+ List + Plan Star Hop

About C108

Description

NGC 4372 is a large, sparse globular cluster in Musca, about 18,900 light-years away. It spans about 19 arcminutes and appears partially obscured by the nearby dark nebula known as the Dark Doodad, creating a striking visual contrast.

Observing Tips

Visible as a faint, large, granular glow in a 6-inch telescope. Its sparse nature makes resolution relatively easy. The Dark Doodad nebula nearby adds visual interest to the field. Best from southern latitudes in autumn.

History

Discovered by James Dunlop on April 4, 1826 from Australia. The cluster is notable for its low concentration and large angular size, making it an easy target for resolution.

Fun Facts

The Dark Doodad, a narrow dark nebula about 3 degrees long, passes near NGC 4372 and makes for one of the more photogenic pairings of a globular cluster with a dark nebula in the southern sky.

Observe

1Properties

Magnitude 7.8
Angular Size 12.0′
Distance 18,900 ly
Globular Cluster [Distance: 18900 ly]

Position & Identifiers

RA 12h 25m 45.4s
Dec -72° 39' 32.4"
Constellation Musca
Catalog C108
Also known as NGC 4372
Physical size
43 light-years across — about 5.0× the Sun-to-Sirius distance

2How easy to spot?

Sign in and configure your equipment and default location to see a personalized row.
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

3Visibility

Set a location in User Settings to see visibility data.

Best season Feb – Apr (peak: Mar)

4 Eyepiece View

Log in to set your own equipment
125x TFOV: 0.4° Lim. mag: 13.6
N E

C108 · 12.0′ diameter · N up, E left

5 Best Magnification

6Metallicity

-2.5 -2.0 -1.5 -1.0 -0.5 0.0 Ancient halo Disc / bulge M3 M71 NGC 6441 C108 [Fe/H] = -2.17

[Fe/H] = -2.17 — these stars formed from gas about 148× poorer in iron than the Sun.

7Concentration class

I II III IV V VI VII VIII IX X XI XII Dense (I) Loose (XII) V Core / half-light / tidal tidal 34.9′ half 3.9′ core 1.75′

Shapley-Sawyer class V — moderately concentrated core.

Explore

8 Classification Decoder

Discover

9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Donald Pelletier. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: Donald Pelletier. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Mar 2, 2026

}