sponsored by psychohistorian.org
RA: 18h 10m 18.38s
Dec: −31° 45′ 48.6″
Con: Sagittarius
Ch: MSA:1415, U2:377, SA:22
Ref: SIMBAD, Collinder (1931), SEDS
Type: globular cluster
Mag: B=12.39, V=11.29
Size: 4.2′
PA: ?
Discovered by Sir John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "globular, pB, irreg R, gmbM, composed of stars 16m, on a milky way ground of mixed L and vS stars." On a second occassion he called it "globular, pB, R, gbM, 80 arcseconds, resolvable or resolved in a field very full of milky way stars." His third observation was recorded as "globular, not vB, R, glbM, 2', resolved. The stars barely discernible."
Hinks, A. R. (1911) On the galactic distribution of gaseous nebulae and of star clusters. MNRAS, 71(8), 693-701.
List 6: "NGC numbers of clusters classed as globular, not in Bailey's catalogue"
Bailey, S.I. A catalogue of bright clusters and nebulae. Ann.Harv.Coll.Obs., 60(8), 199.
RA 18 10 18.4 (2000) Dec -31 45 49 Integrated V magnitude 9.26 Central surface brightness, V magnitudes per square arcsecond 17.08 Integrated spectral type F7- Central concentration, c = log(r_total/r_core); a 'c' denotes a core-collapsed cluster 2.50c: Core radius in arcmin .03. ["Catalog Of Parameters For Milky Way Globular Clusters", compiled by William E. Harris, McMaster University. (Revised: May 15, 1997; from http://www.physics.mcmaster.ca/Globular.html; Harris, W.E. 1996, AJ, 112, 1487) ]
The RNGC (Sulentic and Tifft 1973) notes that this is a globular cluster.
vS cl. about 1'x1'; probably should be classed as globular.
Confirms HOB 21.
A catalogue of star clusters shown on Franklin-Adams chart plates. Mem.R.A.S., 60(5), 175-186.
Steve Coe, observing with a 13" f/5.6, notes: "Pretty bright, pretty small, round and has a very bright middle. I could resolve 10 members at 220X."
30/04/93: I searched in vain for this cluster with the 6-inch f/8.6 Newtonian at 52x and 72x.
Observing site: Pinnacles overlook
Telescope: C-8
[18h 10m 18s, -31° 46' 0"] A small, very faint cluster, not granulated. It was not easy at 163x, and was almost invisible at 36x
Lacaille's catalogue
The Messier objects
Dunlop's catalogue
The Bennett objects
The Caldwell list
Named DSOs
DOCdb is still in beta-release.
Known issues, feature requests, and updates on bug fixes, are here:
Found a bug? Have a comment or suggestion to improve DOCdb? Please let us know!
DOCdb is a free online resource that exists to promote deep sky observing.
You could help by sharing your observations, writing an article, digitizing and proof-reading historical material, and more.
Everything on DOCdb.net is © 2004-2010 by Auke Slotegraaf, unless stated otherwise or if you can prove you have divine permission to use it. Before using material published here, please consult the Creative Commons Attribution-Non-Commercial-Share Alike 2.5 License. Some material on DOCdb is copyright the individual authors. If in doubt, don't reproduce. And that goes for having children, too. Please note that the recommended browser for DOCdb is Firefox 3.x. You may also get good results with K-Meleon. Good luck if you're using IE. A successful experience with other browsers, including Opera and Safari, may vary.