U 307
00:48 to 01:20
-17° to -28°
Cet, Scl

A PORTION OF THE BELLY of the sea creature is shown on chart 307. A bright globular cluster and two spectacular galaxies are also depicted. The South Galactic Pole - one of the points around which our Milky Way galaxy appears to rotate - may be found near the lower right-hand corner.

The splendid pair NGC 288 and NGC 253 is an almost unique conjunction of bright galaxy and bright globular cluster, the other being Omega Centauri and Centaurus A.

FEATURED OBJECTS: NGC 288.

NGC 288
Ben 5
RA 00:52:46
Dec -26° 35.4'
Globular cluster

Discovered in 1785 by William Herschel (H VI-020) with an 18.7-inch f/13 speculum telescope. He called it "cB, iR, 8 or 9' diameter, a great many of the stars visible, so that there can remain no doubt but that it is a cluster of vS stars."

h: "globular cluster; bright; large; round; gradually brighter in the middle; all resolved into stars 12..16 mag; 5' diameter."

Houston notes that this "8th mag ball of stars about a quarter of a degree in diameter lies about two degrees southeast of NGC 253. Steve Gottlieb of Albany, California, reports that his 13-inch Dobsonian at 166x resolved some 40 to 50 stars against a background of hazy light." In 1976 Houston wrote: " . . binoculars were sufficient to distinguish NGC 288, which I make to be 12' in diameter and of visual magnitude 7.0. In a pair of 5-inch 20power binoculars, it was possible to see individual stars around the edge of the cluster. With a 12.5-inch f/8 the cluster could be resolved almost to its centre. Only the regularity of the star pattern indicated that NGC 288 was a globular cluster. ."

William P. Clarke (San Diego, California, USA) writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: "A large, irregular-looking globular with no core. Many tiny stars resolved. (10-inch, x48)."

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "8M; 14' diameter; easily resolved at 100x into compressed glitter of 12M and dimmer stars; 1.75 degrees SE of N253; S Galactic Pole is 40' to SW (don't look for it!)."

Steve Coe, observing with a 17.5" f/4.5 at 100X, notes: "Pretty faint, large, not much brighter in the middle, irregularly round, 40 stars resolved at 135X. It can be seen in a pair of 10X50 binoculars as a dim, small spot. Even this low surface brightness globular cluster is a welcome as a break in all these galaxies.

11x80: A delicate, round puffy globular cluster, some 8 arcmin across, amongst the stars of a parallelogram. (exurban skies, seeing 7, transparency 7, sky darkness 6, lim.mag. at south pole 6.0 (naked eye)) [AS]

10-inch f/5 Newtonian: At 30x the 10-inch shows this as a considerably bright, very large unresolved cluster, presenting a surface which does not even appear mottled. The higher contrast at 120x shows it clearly composed of pretty evenly scattered, very small stars. At times it appears somewhat elongated, but this is doubtful.. (suburban skies) [AS]

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"Deepsky Observers Companion" (http://www.global.co.za/~auke) Copyright 1998 Auke Slotegraaf. All rights reserved. Uranometria 2000.0 copyright (c) 1987-1996 Willmann-Bell, Inc. Page last updated 1998 March 01