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Caldwell 84 — Globular Cluster in Centaurus

NGC 5286

Globular Cluster Excellent (68/100)
Magnitude 7.6m GlobularCluster Centaurus Visible
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About C84

Description

NGC 5286 is a bright globular cluster in Centaurus, about 35,900 light-years away. It is a moderately concentrated cluster spanning about 9 arcminutes with an integrated magnitude of 7.6, located near the star M Centauri.

Observing Tips

Visible as a bright, round glow in a 4-inch telescope. An 8-inch scope begins to resolve the outer halo into individual stars. Located conveniently near the naked-eye star M Centauri for easy finding. Best in spring and summer from southern locations.

History

Discovered by James Dunlop on May 7, 1826 from Australia. The cluster has been studied for its multiple stellar populations, which hint at a complex formation history.

Fun Facts

NGC 5286 may be another example of a globular cluster that originated as the nucleus of a small dwarf galaxy, based on its chemical abundance patterns that differ from typical Milky Way globulars.

Observe

1Properties

Magnitude 7.6
Angular Size 6.6′
Distance 36,100 ly
Globular Cluster [Distance: 36100 ly]

Position & Identifiers

RA 13h 46m 26.9s
Dec -51° 22' 26.4"
Constellation Centaurus
Catalog C84
Also known as NGC 5286
Physical size
16 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 Mar – May (peak: Apr)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

C84 · 6.6′ 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 C84 [Fe/H] = -1.69

[Fe/H] = -1.69 — these stars formed from gas about 49× 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 7.2′ half 0.7′ core 0.28′

Shapley-Sawyer class V — moderately concentrated core.

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Light Travel Time Machine

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Relativistic Travel

Community Photos (1)

Credit: Own work. License: CC BY-SA 3.0. (Wikimedia Commons)

Credit: Own work. License: CC BY-SA 3.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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