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NGC 6397 — Globular Cluster in Ara

Globular Cluster Showpiece (86/100)
Magnitude 5.7m GlobularCluster Ara Visible
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About NGC 6397

Description

NGC 6397 is one of the nearest globular clusters to Earth, at about 7,800 light-years away in Ara. At magnitude 5.7, it is visible to the naked eye from dark sites. It has an unusual core-collapsed structure, meaning its center has become extremely dense.

Observing Tips

A superb target visible to the naked eye as a fuzzy star. Binoculars show a granular ball. Any telescope resolves it into a beautiful field of stars. Notable for its lack of a bright concentrated core — a hallmark of core collapse. Best in summer from southern locations.

History

Discovered by Nicolas Louis de Lacaille in 1751 from South Africa. It is one of the two nearest globular clusters (along with M4) and has been extensively studied by the Hubble Space Telescope.

Fun Facts

NGC 6397 has undergone core collapse, a gravitational process where the most massive stars sink to the center, creating an extremely dense core. Hubble images revealed a population of faint blue stars in its core — helium-core white dwarfs in binary systems.

Observe

1Properties

Magnitude 5.7
Angular Size 15.3′
glob. cl. , B, vL, Ri, st 13

Position & Identifiers

RA 17h 40m 42.0s
Dec -53° 40' 00.0"
Constellation Ara
Catalog NGC 6397
Physical size
13 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 May – Jul (peak: Jun)

4 Eyepiece View

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50x TFOV: 1.0° Lim. mag: 13.6
N E

NGC 6397 · 15.3′ 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 NGC 6397 [Fe/H] = -2.02

[Fe/H] = -2.02 — these stars formed from gas about 105× 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 15.8′ half 2.9′ core 0.05′

Shapley-Sawyer class I — extremely centrally concentrated core.

Explore

8 Classification Decoder

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