Messier 72

Source: Wikipedia, the free encyclopedia.
Distance
54.57 ± 1.17 kly (16.73 ± 0.36 kpc)[3]
Apparent magnitude (V)9.3[4]
Apparent dimensions (V)6.6'
Physical characteristics
Mass1.68×105[5] M
Metallicity = –1.48 ± 0.03
Gyr[6]
Other designationsNGC 6981, GCl 118[7]
See also: Globular cluster, List of globular clusters

Messier 72 (also known as M72 or NGC 6981) is a

southern constellation of Aquarius
.

Observational history and guide

M72 was discovered by astronomer Pierre Méchain in 1780.[a] His countryman Charles Messier looked for it 36 days later, and included it in his catalog.[8] Both opted for the then-dominant of the competing terms for such objects, considering it a faint nebula rather than a cluster. With a larger instrument, astronomer John Herschel called it a bright "cluster of stars of a round figure". Astronomer Harlow Shapley noted a similarity to Messier 4 and 12.[9]

It is visible in

diameter, meaning a broad spread; and small parts scarcer in stars to the south and east.[10]

Properties

Based upon a 2011 census of variable stars, the cluster is 54.57 ± 1.17 kly (16.73 ± 0.36 kpc) away from the Sun.[3] It has an estimated combined mass of 168,000[5] solar masses (M) and is around 9.5 billion years old. The core region has a density of stars that is radiating 2.26 times solar luminosity (L) per cubic parsec.[6] There are 43 identified variable stars in the cluster.[3]

Map showing location of M72

See also

  • List of Messier objects

References and footnotes

  1. ^ on August 29

External links