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Caldwell 106 — Globular Cluster in Tucana

NGC 104

Globular Cluster Showpiece (96/100)
Magnitude 4.0m GlobularCluster Tucana Visible
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About 47 Tucanae

Description

47 Tucanae (NGC 104) is the second-brightest globular cluster in the sky (after Omega Centauri), located about 13,000 light-years away in Tucana. At magnitude 4.0, it is easily visible to the naked eye and spans 31 arcminutes, appearing projected near the Small Magellanic Cloud.

Observing Tips

One of the greatest deep-sky showpieces. Visible to the naked eye as a fuzzy star near the SMC. Binoculars show a large, bright, granular ball. Any telescope resolves it beautifully into thousands of stars. The dense, blazing core is unforgettable. Best from southern latitudes year-round.

History

First noted by Nicolas Louis de Lacaille in 1751. It has been observed by every major space telescope and is one of the most studied stellar systems in astronomy. It was designated "47 Tucanae" in Johann Bode's star catalog as if it were a star.

Fun Facts

47 Tucanae contains at least 25 millisecond pulsars, over 300 X-ray sources, and numerous blue stragglers. Despite a dense search, no planets have been found around its stars, suggesting that the crowded environment may prevent planet formation or survival.

Observe

1Properties

Magnitude 4.0
Angular Size 31.8′
Distance 13,400 ly
Globular Cluster [Distance: 13400 ly]

Position & Identifiers

RA 00h 24m 05.8s
Dec -72° 04' 51.6"
Constellation Tucana
Catalog C106
Also known as NGC 104
Physical size
27 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 Aug – Oct (peak: Sep)

4 Eyepiece View

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30x TFOV: 1.7° Lim. mag: 13.6
N E

47 Tucanae · 31.8′ 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 NGC 6441 47 Tucanae [Fe/H] = -0.72

[Fe/H] = -0.72 — these stars formed from gas about 5.2× poorer in iron than the Sun.

7Concentration class

I II III IV V VI VII VIII IX X XI XII Dense (I) Loose (XII) II Core / half-light / tidal tidal 42.3′ half 3.2′ core 0.36′

Shapley-Sawyer class II — extremely centrally concentrated core.

Explore

8 Classification Decoder

Discover

9

Light Travel Time Machine

10

Relativistic Travel

Community Photos (1)

Credit: Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy). License: CC BY 4.0. (Wikimedia Commons)

Credit: Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration Acknowledgment: J. Mack (STScI) and G. Piotto (University of Padova, Italy). License: CC BY 4.0. (Wikimedia Commons)

Skybred Mar 2, 2026

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