Messier 71 Globular Cluster in Constellation Sagitta Messier 71

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Messier 71 Globular Cluster in Constellation Sagitta Messier 71, also known as M71, NGC 6838, GCl 115 was discovered by Philippe Loys de Chéseaux in 1745 and included by Charles Messier in his catalog of comet-like objects in 1780. It was also noted by Koehler at Dresden around 1775. OBSERVATION DATA (J2000 EPOCH) Class X-XI Constellation Sagitta Right ascension 19h 53m 46.49s Declination +18° 46' 45.1" Distance 13.0 kly (4.0 kpc) Apparent magnitude (V) +6.1 Apparent dimensions (V) 7'.2 PHYSICAL CHARACTERISTICS Mass 1.7×104 M Radius 13 ly Metallicity [ Fe / H ] = –0.78[6] dex Estimated age 9-10 Gyr Messier 71 (also known as M71 or NGC 6838) is a globular cluster in the constellation Sagitta. It appears to be the only one in the constellation The star cluster is at a distance of about 12,000 light years away from Earth and spans some 27 light years across. The irregular variable star Z Sagittae is a member of this cluster. M71 was long thought to be a densely packed open cluster and was classified as such by leading astronomers in the field of star cluster research due to its lacking a dense central compression, and to its stars having more "metals" than is usual for an ancient globular cluster; furthermore, it lacks the RR Lyrae "cluster" variable stars that are common in most globulars. However, modern photometric photometry has detected a short "horizontal branch" in the H-R diagram of M71, which is characteristic of a globular cluster. The shortness of the branch explains the lacking of the RR Lyrae variables and is due to the globular's relatively young age of 9-10 billion years. The relative youth of this globular also explains the abundance of "metals" in its stars. Hence today M71 is designated as a very loosely concentrated globular cluster, much like M68 in Hydra. M71 has a luminosity of around 13,200 Suns. AK, with EarthSky and Wikipedia Notes Map showing location of M71.

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