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Messier 70 — Globular Cluster in Sagittarius

NGC 6681

Globular Cluster Excellent (60/100)
Magnitude 7.9m GlobularCluster Sagittarius Visible
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About M70

Description

M70 (NGC 6681) is a globular cluster in the constellation Sagittarius, located approximately 29,300 light-years from Earth and about 5,000 light-years from the galactic center. At magnitude 7.9, it spans about 8 arcminutes, corresponding to a true diameter of roughly 68 light-years. M70 is classified as concentration class V, indicating moderate central concentration. The cluster has undergone core collapse — a gravitational process where the central stars become extremely densely packed as the core contracts under its own gravity. Only about 20% of known globular clusters have experienced core collapse, making M70 a member of an exclusive group. The cluster is moderately metal-poor with [Fe/H] = -1.51. M70 has a few dozen known variable stars and shares many physical characteristics with its neighbor M69, both in terms of distance and position near the galactic center. M70 lies in the rich Milky Way star fields toward the galactic bulge, surrounded by abundant field stars.

Observing Tips

Located in Sagittarius, roughly midway between Epsilon Sagittarii (Kaus Australis) and Zeta Sagittarii (Ascella), about 2 degrees east of M69. The two clusters can be observed in the same session with minimal repositioning. In binoculars, M70 appears as a faint, tiny, round haze — slightly fainter than M69. A 4-inch telescope at 100x shows a small, compact, unresolved glow with a bright center. An 8-inch telescope at 150-200x reveals a granular texture in the outer regions, though the core-collapsed center remains tight and stellar. Due to its southern declination, atmospheric conditions significantly affect the view from northern latitudes. Best observed from July through September under steady skies.

History

Discovered by Charles Messier on August 31, 1780, on the same night he found M69. Both clusters were described as faint nebulae without stars. William Herschel later resolved M70 into individual stars. The cluster gained a moment of fame in 1995 when Comet Hale-Bopp, one of the brightest comets of the 20th century, was discovered near M70 by Alan Hale and Thomas Bopp, who were independently observing the cluster and noticed the comet nearby.

Fun Facts

Comet Hale-Bopp was discovered on July 23, 1995, when two amateur astronomers independently spotted it while observing near M70 — making this modest globular cluster an unwitting landmark for one of the greatest comet discoveries in modern history. M70's core-collapsed state means its central stars are packed so densely that stellar encounters and collisions are far more frequent than in normal globulars.

Observe

1Properties

Magnitude 7.9
Angular Size 6.6′
Distance 29,400 ly
Globular Cluster [Distance: 29400 ly]

Position & Identifiers

RA 18h 43m 12.8s
Dec -32° 17' 31.6"
Constellation Sagittarius
Catalog M70
Also known as NGC 6681
Physical size
12 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

M70 · 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 M71 NGC 6441 M70 [Fe/H] = -1.62

[Fe/H] = -1.62 — these stars formed from gas about 42× 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 9.5′ half 0.7′ core 0.03′

Shapley-Sawyer class I — extremely centrally concentrated core.

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Community Photos (1)

Credit: ESA/Hubble & NASA. License: CC BY 4.0. (Wikimedia Commons)

Credit: ESA/Hubble & NASA. License: CC BY 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026

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