Messier 10 (M10) is a rich, bright globular cluster located in the constellation Ophiuchus.
The cluster lies at a distance of 14,300 light years from Earth and has an apparent magnitude of 6.4. Its designation in the New General Catalogue is NGC 6254.
Messier 10 lies about 16,000 light years, or 5,000 parsecs, from the galactic centre. It takes roughly 140 million years to complete an orbit around the Milky Way Galaxy. It crosses the plane of the Milky Way’s disk every 53 million years.
M10 is moving away from the solar system at a velocity of 69 km/s. The cluster’s estimated mass is 200,000 solar masses.
The cluster was discovered by Charles Messier on May 29, 1764. Messier added it to his catalogue as object number 10, describing it as a “nebula, without stars, in the belt of Ophiuchus; near the 30th star of that constellation, of sixth magnitude, according to Flamsteed. This nebula is beautiful & round; one can only see it with difficulty in an ordinary telescope of 3-feet [FL].”
A decade later, German astronomer Johann Elert Bode provided a similar description, calling M10 a “nebulous patch without stars; very pale.” On August 14, 1774, he observed M10 and M12, another globular cluster in Ophiuchus that lies in the same field of view, and wrote:
On August 14 , I discovered in Ophiuchus two new nebulae not far from each other. One of them is situated south of 14, 16, 19 and 21 Oph near the western arm, the other below this one and eastward, closely west of 30 Oph. These nebulae appear very pale, and because of this, I found not very reliably the separation to Lambda as 6deg 7′, to the star 14 as 3deg 50′, and to 21 as 3deg 32′. The other one is separated from the 21st star by 5deg 32′, and by 1deg 4′ from the 30th.
It was not until German-born British astronomer William Herschel observed the cluster with a larger telescope that M10 was resolved into individual stars and recognised as a cluster. Herchel described the object as a “beautiful cluster of extremely compressed stars,“ adding that “it resembles the 53d [Messier 53]; and the most compressed part is about 3 or 4 minutes in diameter.”
American astronomer Harlow Shapley was the first to estimate an approximate distance to M10, but his estimation of 33,000 light years placed the cluster at twice the distance of the modern estimates.
Messier 10 has a spatial diameter of 83 light years, but small telescopes (3-inch) reveal about half the cluster’s size – roughly 8 to 9 minutes of arc – and its bright central region, which spans roughly 35 light years. 6-inch or 8-inch telescopes show the cluster extending across 15.1 arc minutes and reveal a large, bright central core. Meanwhile, deep images reveal M10 to span some 20 arc minutes of apparent sky and resolve stars across the entire area of the cluster.
The cluster is about two thirds the size of the full Moon, but its outer regions are very dim. With a visual magnitude of 6.4, even the cluster’s bright core is too faint to be seen without binoculars.
Messier 10 and Messier 12 can be found about half a fistwidth west of the bright star Beta Ophiuchi, also known as Cebalrai, with Messier 10 lying a bit lower in the sky, to the south of M12. M10 lies along the line from Cebalrai to Zeta Ophiuchi, the third brightest star in Ophiuchus. It is only a degree away from 30 Ophiuchi, an orange giant star with an apparent magnitude of 4.83.
The two clusters lie at an approximate distance of 2,000 light years from each other and are separated by 3 degrees in the sky. M10 appears brighter because it is about 2,000 light years closer to us than M12. The best time of year to observe the two clusters is in the months of May, June and July.
Messier 10 contains about 100,000 stars, with the core region consisting of 14 percent binary stars.
The cluster is classified as moderately metal-poor and there is evidence indicating that it is enriched by elements produced in Type II supernovae and the s-process (slow-neutron-capture process) in massive stars. The stars in M10 have only 3.5 percent of the heavy elements found in the Sun, pointing to an age of 11.4 billion years. This makes M10 one of the younger globular clusters known.
The central region of M10 contains many blue stragglers, stars formed 2-5 billion years ago that look younger than they are because they are bluer and more luminous than their neighbours. The phenomenon is believed to be a result of interactions between two or more stars in the dense, compact central regions of globular clusters. Four variable stars have been discovered in M10.
The cluster’s core will be the last part to survive and will likely be around for another 15 to 20 billion years. It will eventually be torn apart by gravitational forces of the Milky Way as it keeps passing through the galactic disk.
|Designations: Messier 10, M10, NGC 6254, GCl-49|
|Right ascension: 16h 57m 8.92s|
|Distance: 14,300 light years (4,400 parsecs)|
|Age: 11.39 billion years|
|Number of stars: 100,000|
|Apparent magnitude: +6.4|
|Apparent dimensions: 20′|
|Radius: 41.6 light years|
|Tidal radius: 19.3 arc minutes|