NGC 6522

NGC 6522
32 inch telescope NGC 6528 (lower left) and NGC 6522 (upper right)
Observation data (J2000 epoch)
Constellation	Sagittarius
Right ascension	18^h 3^m 34.1^s[1]
Declination	−30° 2′ 2.3″[1]
Distance	25.1 kly (7.7 kpc)[2]
Apparent magnitude (V)	10.5
Apparent dimensions (V)	2'
Physical characteristics
Mass	3.00×10^5[2] M☉
Metallicity	${\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}$ = –1.34[2] dex
Estimated age	12.0 Gyr[3]

NGC 6522 is a globular cluster in the constellation Sagittarius. It is apparent magnitude 10.5, and diameter 2 arc seconds, and class VI with stars 16th magnitude and dimmer. It was discovered by William Herschel on June 24, 1784. It is centered in a region of the sky known as Baade's Window.^[1]

NGC 6522 is possibly the oldest star cluster in the Milky Way,^[4] with an age of more than 12 billion years.^[5]

References

1. "SIMBAD Astronomical Database". Results for NGC 6522. Retrieved 2011-03-13.
2. Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal, 742 (1): 51, arXiv:1108.4402, Bibcode:2011ApJ...742...51B, doi:10.1088/0004-637X/742/1/51.
3. Koleva, M.; et al. (April 2008), "Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting", Monthly Notices of the Royal Astronomical Society, 385 (4): 1998–2010, arXiv:0801.0871, Bibcode:2008MNRAS.385.1998K, doi:10.1111/j.1365-2966.2008.12908.x
4. "VLT-FLAMES Analysis of 8 giants in the Bulge Metal-poor Globular Cluster NGC 6522: Oldest Cluster in the Galaxy?" by B. Barbuy et al., 2009
5. "The universe's first stars were whirling dervishes", New Scientist by David Shiga, 30 April 2011, p. 20. "Imprints of fast-rotating massive stars in the Galactic Bulge" by Cristina Chiappini et al., Nature 472, pp. 454–457 (28 April 2011).

External links

• NGC6522, Galactic Globular Clusters Database page