NGC/IC Project Restoration Effort

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NGC3500

 

Basic Information


Location and Magnitude


Right Ascension: 11:1:51.3
Declination: +75:12:4
Constellation: DRA
Visual Magnitude: 13.5

Historic Information


Discoverer: Herschel W.
Year of discovery: 1801
Discovery aperture: 18.7

Observational


Summary description: vF, eF, D neb, v near (?? Place)
Sub-type: Sab

Corwin's Notes

===== NGC 3500 is given as a double nebula with one number in the NGC, while JH in GC assigns two numbers with a single position. In each catalogue, the position comes from WH's observations on the night of 2 April 1801 which suffer from large, systematic position errors (see NGC 3752 for more). Dreyer more or less sorted out the problems for his edition of WH's Scientific Papers, based on accurate positions measured on 30-inch reflector plates taken at Greenwich in 1910 or 1911 (see MNRAS 71, 509, 1911). Unfortunately, neither Dreyer nor the Greenwich observer(s) assign NGC numbers to all of the galaxies in that list (I have those listed in my note to NGC 3752). I've taken a bit of a liberty here, and have split out WH's two numbers, III 967 and III 968, giving the first to NGC 3465 (which see), and the second to NGC 3500 (this may not be correct; see the next paragraph). I follow Dreyer's lead on the first, but use NGC 3500 for the second where he does not. Looking at WH's original sweep 1096, I'm not totally convinced that this is the correct solution. In CH's fair copy of the sweep (in the Herschel Archive), we read for the observation Two, the 1st vF, vS. The 2nd eF and smaller than the first. It is a little more north and following, but very near to it. The phrase "but very near to it" has caught my attention. Given that the galaxies are nine arcminutes apart -- and NGC 3523 is actually closer (seven arcminutes) to NGC 3500 than is NGC 3465 -- I wonder if one of the asterisms in the area might not be a better candidate for one of WH's objects. I have my eye in particular on the double star at 11 01 24.0, +75 11 34 (J2000) -- but is this brighter than the galaxy as WH suggests? For now, I will just leave this as a possibility in a sweep with known problems.

Steve's Notes

===== NGC 3500 24" (5/25/14): at 280x appeared faint or fairly faint, fairly small, elongated 2:1 SW-NE, 0.6'x0.3', very small brighter core. Second of three in the KTG 34 triplet, with NGC 3465 9.0' W and NGC 3523 7.0' SE. This galaxy's redshift-based distance is ~150 million l.y., while the other two lie at 325 million l.y. 18" (3/30/05): very faint, small, elongated 2:1 SW-NE, 0.6'x0.3', low surface brightness. Smallest and faintest of a trio with NGC 3523 7.2' SE and NGC 3465 9' W. This galaxy is incorrectly listed as nonexistent in the RNGC and it is not identified as NGC 3500 in UGC, MCG or CGCG. 17.5" (4/25/98): extremely faint, small, elongated 2:1 SW-NE, 30"x20". Faintest of trio with NGC 3465 9' W and NGC 3523 7' SE. A pair of mag 12 stars [30" separation] is 6' preceding. Observation difficult due to very poor transparency.