U 334
15:12 to 15:44
-17° to -28°
Lib, Sco

FEATURED OBJECTS: NGC 5903, NGC 5898, NGC 5897.

NGC 5903
ESO514-G004
RA 15:18:36
Dec -24°04.1'
Galaxy

Discovered in 1784 by William Herschel (H III-139) "Two, nearly parallel 7' distant, Both vF, not vS, R." The two objects are NGC 5898 and NGC 5903.

h: "B, R, pgbM, 20 arcseconds." On a second occassion he called it "pF, R, gpmbM, 30 arcseconds."

Sandage (1975, Astrophysical Journal, 202, 563-582) notes that this galaxy is a member of the NGC 5898 Pair. Members include NGC 5898, NGC 5903 & ESO 514-G 3.

NGC 5898
ESO514-G002
RA 15:18:13
Dec -24°05.8'
Galaxy

Discovered in 1784 by William Herschel (H III-138) "Two, nearly parallel 7' distant, Both vF, not vS, R." The two objects are NGC 5898 and NGC 5903.

h: "pB, R, pgbM, 15 arcseconds."

Sandage (1975, Astrophysical Journal, 202, 563-582) notes that this galaxy is a member of the NGC 5898 Pair. Members include NGC 5898, NGC 5903 & ESO 514-G 3.

NGC 5897
Ben 68
ESO582-SC002, GCL-33, H 19
RA 15:17:24
Dec -21°01.0'
Globular cluster

On a cloudy night in April, 1784, William Herschel was sweeping with his 18.7-inch f/13 speculum telescope. In his Journal he wrote: "The moon is very bright, but in pursuit of the nebulous stratum I look in hopes of seeing some of the brighter nebulae in it." Herschel recorded VI.8 as "a very close, compressed cluster of stars 8' or 9' in diameter, extremely rich, of an irregular round figure, a little extended. The stars are so small as hardly to be visible, and so accumulated in the middle as to look nebulous." Because of the uncertainty in the recorded position, Dreyer has concluded this is the same object as VI.19, which was first recorded on March 10, 1785; it is described as a "beautiful large cluster of the most minute and most compressed stars of different sizes. 6 or 7' diameter, irregularly round, faint, red colour."

h: "globular, pF, v irr R, vgbM, all resolved into stars 12..16th mag, diam 5' to 5.5'."

Houston calls this globular "a big, splashy affair .. its 8.5 mag disk is more than 10' across and a 10-inch will resolve some stars. In the 1940's I viewed it from Louisiana with a 6-inch reflector at 25x and noted it as 'bright and mottled.' " He notes that this cluster is of mag 9 or 10, with a diameter of about 7'.

Tom Lorenzin: "10M; 8.5' extent; large and little-compressed with little, if any, central brightness; unresolved in 8-in. except for few 13M to 13.5M stars which dot the central region."

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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