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Caldwell 107 — Globular Cluster in Apus

NGC 6101

Globular Cluster Good (59/100)
Magnitude 9.3m GlobularCluster Apus Visible
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About C107

Description

NGC 6101 is a loose, sparse globular cluster in Apus, about 47,600 light-years away. It spans about 11 arcminutes and shines at magnitude 9.3, making it one of the fainter Caldwell globulars.

Observing Tips

A small, faint glow in a 6-inch telescope. An 8-inch scope begins to resolve a few outer stars. Its sparse nature means it never looks as impressive as the more concentrated globulars. Best from southern latitudes in winter.

History

Discovered by James Dunlop on June 1, 1826 from Australia. It is one of the least concentrated globular clusters known.

Fun Facts

NGC 6101 has one of the lowest central concentrations of any globular cluster. Studies suggest it may contain an intermediate-mass black hole that has gravitationally stirred the cluster, pushing stars outward and preventing core collapse.

Observe

1Properties

Magnitude 9.3
Angular Size 4.5′
Distance 49,900 ly
Globular Cluster [Distance: 49900 ly]

Position & Identifiers

RA 16h 27m 04.1s
Dec -72° 12' 07.2"
Constellation Apus
Catalog C107
Also known as NGC 6101
Physical size
31 light-years across — about 3.6× the Sun-to-Sirius distance

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Medium+ Medium
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

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Best season Apr – Jun (peak: May)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C107 · 4.5′ 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 M92 M3 M71 NGC 6441 C107 [Fe/H] = -1.98

[Fe/H] = -1.98 — these stars formed from gas about 95× poorer in iron than the Sun.

7Concentration class

I II III IV V VI VII VIII IX X XI XII Dense (I) Loose (XII) IX Core / half-light / tidal tidal 6.1′ half 1.1′ core 0.97′

Shapley-Sawyer class IX — diffuse profile with a loose outer envelope.

Explore

8 Classification Decoder

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9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: NASA - Hubble Space Telescope. License: Public domain. (Wikimedia Commons)

Credit: NASA - Hubble Space Telescope. License: Public domain. (Wikimedia Commons)

Skybred Mar 2, 2026

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