U 329
12:32 to 13:04
-17° to -28°
Crv, Hya, Vir

A GALAXY-RICH REGIONin Corvus and Virgo, with many 'faint fuzzies' on display. Breaking the mould is the bright globular cluster NGC 4590.

FEATURED OBJECTS: NGC 4830, NGC 4763, NGC 4590.

NGC 4830
ESO575-G037
RA 12:57:26
Dec -19°41.5'
Galaxy

NGC 4763
MCG-03-33-013
RA 12:53:25
Dec -17°00.3'
Galaxy

NGC 4590
Bennett 51, Messier 68
ESO506-SC030, GCL-20
RA 12:39:27
Dec -26°44.5'
Globular cluster

In the Philosophical Transactions, 1814, William Herschel described it as "a beautiful cluster of stars, extremely rich, and so compressed that most of the stars are blended together; it is near 3' broad and about 4' long, but chiefly round, and there are very few scattered stars about. This oval cluster is also approaching to the globular form, and the central compression is carried to a high degree. The insulation is likewise so far advanced that it admits of an accurate description of the contour. The clusters of this class are beautiful, but can hardly be seen to any advantage without a 20 feet telescope." In the Philosophical Transactions, 1818, William Herschel wrote: "1786, 1789, 1790, 20 feet telescope. A cluster of very compressed small stars, about 3' broad and 4' long. The stars are so compressed, that most of them are blended together."

h: "globular, irregularly round, gbM, diam in RA = 12..15 seconds. All clearly resolved into stars 12th mag; very loose and ragged at the borders."

Hartung notes: "Faint outliers may be detected with 10.5cm. It is very rich, broadly concentrated to a central region about 2' across and the outlying stars show evidence of a spiral pattern 5' - 6' across. 15cm resolves this cluster clearly though faintly."

Houston includes this globular in his Hydra Hysteria. He calls it "beautiful" and notes that "individual stars should be easily visible in a 6-inch scope." In 1972 he called it one of two globulars worth-while looking up in Hydra (the other being NGC 5694). He notes that it shines at 8th mag: "since its stars are 12th mag and fainter, a large scope is needed to discern them. Visually, M68 appears about 3' in diameter. Observing with a 6-inch refractor, Smyth described this globular as oval, pale and mottled."

Donald J. Ware: "This rather bright globular cluster is about 8-10' in diameter and is very compact, showing a bright, granulated core and many stars resolved around its edges."

Steve Coe (1992, The Deep-Sky Observer, Webb Society, Issue 1) observing with a 17.5-inch f/4.5 at 100x notes: "pB, rich, compressed, seen in finder. Resolved at all powers. 'Kidney-shaped' with streamers on one side. About 50 stars resolved at 165x. Many stars at the limit of the 17.5-inch, averted vision makes it grow. At 300x the core has about 10 stars resolved and the central area is very grainy. Entire cluster looks like a garden sprinkler, with eF stars seen as a set of curved chains that exit the main body and swirl around."
Sentinel 13" 8/10-- bright, large, extremely rich, extrememly compressed, bright middle, irregularly round, stars 13th mag and less. Easy in 11X80, very comet-like in finder. 330X--20 stars resolved, several nice chains, curved edges are ragged at high power.

Tom Lorenzin: "8M; 9' diameter; well resolved into glitter of 13M stars; 33' to SW lies bright DBL ST ADS 8612."

10x50: "faint, small, round glow. Almost stellar core. Near a rather bright star." (suburban skies) [DC]

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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 April 05