NGC 1904 Bennett 34 Messier 79, ESO487-SC007, GCL-10 RA 05:24:10 Dec
-24°31.5' Globular cluster |
This globular cluster in Lepus was observed by
Mechain in 1780. The NGC description reads: "pretty large, extremely rich,
extremely compressed, clearly resolved into stars".
In the Philosophical Transactions, 1814,
William Herschel wrote "January 13, 1806. Large 10 feet Newtonian
telescope. The 79th of the Connoissance des Temps is a cluster of stars of a
globular construction, and certainly extremely rich. Towards the centre the
stars are extremely compressed, and even a good way from it. With 171 power the
diameter is a little less than 1/2 of the field, and with 220 a little more; the
field of one being 9' and of the other 8', a mean of both gives the diameter of
the cluster 2' 50 arcseconds, but I suppose that the lowness of the situation
prevents my seeing the thinly scattered stars, so that this cluster is probably
larges that it appears." In the Philosophical Transactions, 1818, William
Herschel wrote: "1783, 7 feet telescope. With 57 nebulous; with 86 a strong
suspicion of its being stars. 1799, 10 feet telescope. 300 power shows the stars
of it with difficulty. 1784, 20 feet telescope, a beautiful cluster of stars,
nearly 3' diameter. 1806, large 10 feet telescope. A globular cluster, the stars
of which are extremely compressed in the middle; with 171 and 220 the diameter
is 2' 50 seconds, but the lowness of the situation probably prevents my seeing
the whole of its extent."
Hartung notes that a 4-inch telescope "will
show the outlying stars faintly. It is bright, of moderate condensed type and
about 2.5' across with outliers extending considerably wider. Large apertures
show gleaming points right to the centre. It lies in a fine field..."
Tom Lorenzin: "8.4M; 7.5' diameter; rich,
compressed and faint; bright center, off center to S; DBL ST ADS3954 is 35' to
WSW."
Sanford notes that "in small telescopes,
it remains unresolved, but shows a few stars around the edges in an 8-inch. A
12-inch or larger will show the object richly resolved into a tight ball of
faint stars."
Steve Gottlieb, 17.5-inch: "40-50 stars
resolved mostly in halo or at the edge of the very mottled core. A string of
six stars is just E of center and a long string passes through the core. The
brightest mag 12.5 is N of the core"; 13-inch: "about 40 stars
resolved including a few over the core."; 8-inch: "small bright core,
few stars at edge and core, mottled. The outer halo is well resolved in
excellent conditions."
Steve Coe, observing with a 13" f/5.6,
notes: "Pretty bright, pretty large, round, very bright in the middle at
135X. Well resolved, with about 12 stars in the compressed central section and
another 50 stars in the outer portions. All against a very grainy backround.
Easily seen in the finder."
11x80: Observed this
globular quite low on horizon, soon after setting up so dark adaptation not
fully set in. It can be missed while sweeping, looking star-like. The nebulous
atmosphere, however, is evident with direct vision once located. It is neatly
flanked by two 8th mag stars due north/south. A slightly orange 5th mag star,
shown as double, lies over half a degree to the west-southwest, serving as a
convenient marker. (suburban skies) [AS]
13.1-inch f/4.4 Newtonian:
"Very large and very bright. Has a large nucleus, and is oval east-west.
Poor halo. In the southern portion of the edge seems to have a dark arc which
limits the nucleus. There are approximately 10 stars surrounding it in all
directions out to 3'." [229x, 14', sketched] (urban) [GG]
15.5-inch f/9 Newtonian: At
220x the cluster appears very bright and large. It is surrounded by a perimeter
of field-stars and there is a single star to the southwest. The definite nucleus
appears angular, with a straight edge running southwest to northeast. There is a
gradual decrease in brightness to the outer edge of this very charming cluster.
(suburban skies) [AS] |