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Messier 19

File:M19-Cluster.png · Wikimedia Commons · See Wikimedia Commons

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Messier 19

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Also known as M19

globular cluster

AI overview

Messier 19 is a dense, spherical collection of hundreds of thousands of old stars held together by gravity, located about 28,000 light-years away in the constellation Ophiuchus. It matters to astronomers because studying such globular clusters helps us understand the age and history of our galaxy, as these clusters are among the oldest objects in the Milky Way.

AI-generated from the Wikipedia summary — may contain errors.

Wikidata facts

Distance from Earth
28700
Radius
70
Image
Messier 19 Hubble WikiSky.jpg
Show 13 more facts
Commons category
Messier 19
catalog code
[KPS2012] MWSC 2519
metallicity
-1.76
time of discovery or invention
1764-06-05
Commons gallery
Messier 19
apparent magnitude
5.801
radial velocity
135.0
absolute magnitude
-9.13
spectral class
VIII
right ascension
255.657042
declination
-26.267944
right ascension component of proper motion
-2.86
declination component of proper motion
-0.45
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Article

Messier 19 or M19 (also designated NGC 6273) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier on June 5, 1764 and added to his catalogue of comet-like objects that same year. It was resolved into individual stars by William Herschel in 1784. His son, John Herschel, described it as "a superb cluster resolvable into countless stars". The cluster is located 4.5° WSW of Theta Ophiuchi and is just visible as a fuzzy point of light using 50 mm (2.0 in) binoculars. Using a telescope with a 25.4 cm (10.0 in) aperture, the cluster shows an oval appearance with a 3′ × 4′ core and a 5′ × 7′ halo.

M19 is one of the most oblate of the known globular clusters. This flattening may not accurately reflect the physical shape of the cluster because the emitted light is being strongly absorbed along the eastern edge. This is the result of extinction caused by intervening gas and dust. When viewed in the infrared, the cluster shows almost no flattening. It lies at a distance of about 28.7 kly (8.8 kpc) from the Solar System, and is quite near to the Galactic Center at only about 6.5 kly (2.0 kpc) away.

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