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Messier 19 — Globular Cluster in Ophiuchus

NGC 6273

Globular Cluster Showpiece (80/100)
Magnitude 6.8m GlobularCluster Ophiuchus Visible
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About M19

Description

M19 is a globular cluster in the constellation Ophiuchus, located about 28,700 light-years from Earth. It is one of the most oblate (flattened) globular clusters known, with a noticeably elliptical appearance. M19 contains several hundred thousand stars and spans about 140 light-years in diameter. It lies only about 6,500 light-years from the galactic center, making it one of the innermost Milky Way globular clusters. Its proximity to the galactic center likely causes the tidal forces responsible for its elongated shape.

Observing Tips

Located about 8 degrees south-southeast of Antares. At magnitude 7.5, it is visible in binoculars as a small fuzzy spot. A 4-inch telescope shows a round to slightly oval glow with a brighter center. The elliptical shape becomes more apparent in 8-inch or larger telescopes at 150x or more. Star resolution is difficult due to its distance and compact nature — apertures of 10 inches or more are needed to resolve the outer fringes. Best observed from June through August.

History

Discovered by Charles Messier on June 5, 1764. He described it as a round nebula without stars. William Herschel was the first to note its slightly elliptical shape. The cluster's unusual oblateness has been studied extensively, with modern research attributing it to tidal forces from the galactic center.

Fun Facts

M19 is the most oblate globular cluster in the Messier catalog, with an ellipticity of about 0.22. Its flattened shape is thought to be caused by the strong tidal field near the galactic center. The cluster is one of the closest known globular clusters to the center of the Milky Way, orbiting in a region of intense gravitational forces.

Observe

1Properties

Magnitude 6.8
Angular Size 7.5′
Distance 28,700 ly
Globular Cluster [Distance: 28700 ly]

Position & Identifiers

RA 17h 02m 37.7s
Dec -26° 16' 04.6"
Constellation Ophiuchus
Catalog M19
Also known as NGC 6273
Physical size
22 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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125x TFOV: 0.4° Lim. mag: 13.6
N E

M19 · 7.5′ 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 M19 [Fe/H] = -1.74

[Fe/H] = -1.74 — these stars formed from gas about 55× poorer in iron than the Sun.

7Concentration class

I II III IV V VI VII VIII IX X XI XII Dense (I) Loose (XII) IV Core / half-light / tidal tidal 14.6′ half 1.3′ core 0.43′

Shapley-Sawyer class IV — moderately concentrated core.

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Community Photos (1)

Credit: Doug Williams, REU Program / NOIRLAB / NSF / AURA. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: Doug Williams, REU Program / NOIRLAB / NSF / AURA. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026

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