Appearance move to sidebar hide Coordinates: 19h 53m 46.11s, +18° 46′ 42.3″ From Wikipedia, the free encyclopedia Globular cluster in the constellation Sagitta
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Messier 71
The globular cluster Messier 71 by the Hubble Space Telescope.
Observation data (J2000 epoch)
Class
X-XI
Constellation
Sagitta
Right ascension
19h 53m 46.49s[1]
Declination
+18° 46′ 45.1″[1]
Distance
13.0 kly (4.0 kpc)[2]
Apparent magnitude (V)
8.2[3]
Apparent dimensions (V)
7.2'
Physical characteristics
Mass
1.7×104[4] M☉
Radius
13 ly[5]
Metallicity
[Fe/H] = –0.78[6] dex
Estimated age
9-10 Gyr
Other designations
M71, NGC 6838, Cr 409, GCl 115[7]
See also: Globular cluster, List of globular clusters
Messier 71 (also known as M71, NGC 6838, or the Angelfish Cluster) is a globular cluster in the small northern constellation Sagitta. It was discovered by Philippe Loys de Chéseaux in 1745 and included by Charles Messier in his catalog of non-comet-like objects in 1780. It was also noted by Koehler at Dresden around 1775.[8] Messier 71 is also known as NGC 6839, though this identification is very uncertain.[9]
This star cluster is about 13,000 light years away from Earth and spans 27 light-years (8 pc). The irregular variable star Z Sagittae is a member.[10]
The M71 globular cluster at the center is surrounded by a dense Milky Way star field.
M71 was for many decades thought (until the 1970s) 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 (chart of temperature versus luminosity) which is characteristic of a globular cluster. The shortness of the branch explains the lack of RR Lyrae variables and is due to the globular's relatively young age of 9–10 billion years. Taking in many or only late series (Population I) stars explains relatively its stars. Hence today M71 is designated as a very loosely concentrated globular cluster, much like M68 in Hydra. M71 has a mass of about 53,000 M☉ and a luminosity of around 19,000 L☉.[11]
Map showing location of M71 Wikimedia Commons has media related to Messier 71.
See also
[edit]
List of Messier objects
NGC 6366
NGC 6342
References
[edit]
^ abGoldsbury, Ryan; et al. (December 2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters", The Astronomical Journal, 140 (6): 1830–1837, arXiv:1008.2755, Bibcode:2010AJ....140.1830G, doi:10.1088/0004-6256/140/6/1830, S2CID 119183070.
^Hessels, J. W. T.; et al. (November 2007), "A 1.4 GHz Arecibo Survey for Pulsars in Globular Clusters", The Astrophysical Journal, 670 (1): 363–378, arXiv:0707.1602, Bibcode:2007ApJ...670..363H, doi:10.1086/521780, S2CID 16914232.
^"Messier 71". SEDS Messier Catalog. Retrieved 30 April 2022.
^Marks, Michael; Kroupa, Pavel (August 2010), "Initial conditions for globular clusters and assembly of the old globular cluster population of the Milky Way", Monthly Notices of the Royal Astronomical Society, 406 (3): 2000–2012, arXiv:1004.2255, Bibcode:2010MNRAS.406.2000M, doi:10.1111/j.1365-2966.2010.16813.x, S2CID 118652005. Mass is from MPD on Table 1.
19h 53m 46.11s, +18° 46′ 42.3″ From Wikipedia, the free encyclopedia Globular cluster in the constellation Sagitta 
Wikimedia Commons has media related to Messier 71. 
Retrieved from "https://en.wikipedia.org/w/index.php?title=Messier_71&oldid=1328050422" Categories: 
19h 53m 46.11s, +18° 46′ 42.3″ From Wikipedia, the free encyclopedia Globular cluster in the constellation Sagitta 
The globular cluster Messier 71 by the Hubble Space Telescope.
Wikimedia Commons has media related to Messier 71. 
Till Credner and Sven Kohle, Calar Alto Observatory. 
M71 in visible light by the NOAO. 
M71 in infrared by the survey 2MASS. 
M71 in visible light by the survey DSS. 
Astronomy
Stars
Outer space
