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Caldwell 93 — Globular Cluster in Pavo

NGC 6752

Globular Cluster Showpiece (91/100)
Magnitude 5.4m GlobularCluster Pavo Visible
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About C93

Description

NGC 6752 is the third-brightest globular cluster in the sky (after Omega Centauri and 47 Tucanae), located about 13,000 light-years away in Pavo. At magnitude 5.4, it is visible to the naked eye and spans 20 arcminutes.

Observing Tips

A superb globular visible to the naked eye from dark sites. Binoculars show a bright, granular ball. Any telescope resolves the outer regions into streams of individual stars. A 6-inch scope provides a stunning view at 80-120x. Best from southern locations in summer and autumn.

History

Discovered by James Dunlop on June 30, 1826 from Australia. It is one of the nearest globular clusters and has been the subject of intensive study, including Hubble observations of its white dwarf population.

Fun Facts

NGC 6752 has undergone core collapse, resulting in an extremely dense center. Millisecond pulsars discovered in its core are among the fastest-spinning objects known. The cluster also contains one of the first known planetary systems in a globular cluster — a pulsar with a planet-mass companion.

Observe

1Properties

Magnitude 5.4
Angular Size 13.2′
Distance 13,000 ly
Globular Cluster [Distance: 13000 ly]

Position & Identifiers

RA 19h 10m 52.1s
Dec -59° 59' 06.0"
Constellation Pavo
Catalog C93
Also known as NGC 6752
Physical size
14 light-years across — tens of light-years across — wider than the solar neighbourhood

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

3Visibility

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Best season Jun – Aug (peak: Jul)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C93 · 13.2′ 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 M71 NGC 6441 C93 [Fe/H] = -1.54

[Fe/H] = -1.54 — these stars formed from gas about 35× poorer in iron than the Sun.

7Concentration class

I II III IV V VI VII VIII IX X XI XII Dense (I) Loose (XII) I Core / half-light / tidal tidal 53.8′ half 1.9′ core 0.17′

Shapley-Sawyer class I — extremely centrally concentrated core.

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Light Travel Time Machine

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Relativistic Travel

Community Photos (1)

Credit: en:NASA, en:STScI, en:WikiSky. License: Public domain. (Wikimedia Commons)

Credit: en:NASA, en:STScI, en:WikiSky. License: Public domain. (Wikimedia Commons)

Skybred Mar 2, 2026

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