sponsored by psychohistorian.org

DOCdb

Deep Sky Observer's Companion – the online database

 

Welcome, guest!

If you've already registered, please log in,

or register an observer profile for added functionality.

List:

log in to manage your observing lists

 browse:

 

 position:

 

 next:

 

 options:

summary

rename

prune

trim

remove

close

copy

combine

plan

bookmark

load

new

delete

marathon

favourite!

Full database:

Entire DOCdb database of 18,816 objects.

 browse:

 position:

NGC 7129 (16,847 of 18,816)

 next:

oc gc pln bn dn gx gxcl ast aka lost

Object:

list

bookmark

finder chart

altitude today

altitude (year)

 search:

½°, , in DOCdb


Warning: date(): It is not safe to rely on the system's timezone settings. You are *required* to use the date.timezone setting or the date_default_timezone_set() function. In case you used any of those methods and you are still getting this warning, you most likely misspelled the timezone identifier. We selected the timezone 'UTC' for now, but please set date.timezone to select your timezone. in /home/yivumoo/public_html/show_object.php on line 167

show browsing

Small Cluster Nebula

NGC 7129, Ced 196, DG 176, Cl Collinder 441, C 2140+658, Small Cluster Nebula, IV 75, h 2131, GC 4702

RA: 21h 42m 56s
Dec: +66° 06′ 12″

Con: Cepheus
Ch: MSA:1060, U2:33, SA:3

Ref: SIMBAD, Collinder (1931), DAML02, Archinal&Hynes (2003)

(reference key)

Type: open cluster, 42pn

Mag: B=?, V=11.5

Size: 8′ x 6′
PA: ?

History and Accurate Positions for the NGC/IC Objects (Corwin 2004)

NGC 7129 is a diffuse nebula enveloping three pretty bright stars. Both Herschels described it the same, and JH measured the position angles and distances of the two flanking stars with respect to the brightest, more central southern one, BD +65 1638. His mean position for the nebula, adopted in GC and NGC, is for that star.

Bigourdan apparently did not read JH's 1833 description before he examined the area in the 1884, 1889, and 1895. Bigourdan applied NGC 7129 only to the patch of nebulosity to the northwest of JH's star C, the northeastern of the three stars. He also found a "new" nebula in 1895 around JH's star A, the south-central of the three. This now carries the number IC 5134 (which see). Another "nova" from Bigourdan, NGC 7133 (which see), was apparently an illusion as there is nothing near his place but faint stars.

Historical observations

William Herschel (c.1784)

Synonyms: H IV-075

Discovered in 1794 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it "three stars about 9m involved in nebulosity. The whole takes up a space of about 1.5' diameter; other stars of the same size are free from nebulosity."

NGC/IC Dreyer (1888, 1895, 1908)

"remarkable, considerably faint, pretty large, gradually brighter in the middle, triple star involved."

Published comments

Cederblad, S. (1946) [VII/231]

Ced 196 (NGC 7129)

Position (1900): RA 22 40.7, Dec + 65 39

Star: Anon (Mp=10.5, V=10.3, SpT=B6)

Spectrum of nebula: continuous spectrum (inferred from sp.t. of illuminating star)

Classification: Neb associated with mainly one star (which may be multiple) - star surrounded by a neb envelope with conspicuous structure (eg. IC 5146)

Size: 7.5'x7'

Notes: "NGC 7129 = GC 4702 = h 2131 = H IV 75. Disc. 1792. (114, 194, 196, 208, 216, 217, 304, 366, 486, 549, 578, 608, 615 Pl 9, 631). R. The cluster contains the BD stars: +65 1631, 1633, 1635-1638, which are not in the HD catalogue. NGC 7133 is probably a part of this nebula. Alternative Class: A. 1."

Dorschner & Gürtler (1963)

Untersuchungen uber Reflexionsnebel.

DG 176 = NGC 7129, Ced 196

Pos (1950.0) 21:41.9, +65:53

Size: 8x6 (blue), 5x5 (red).

Lynds, B.T. (1965)

(Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae notes that this isolated nebula is very bright, equally prominent on the red and blue POSS plates and has a maximum size of 2' x 2'.

Bernes, C. (1977)

Bernes, C. (1977) A catalogue of bright nebulosities in opaque dust clouds.

describes it as a reflection nebula, very bright on the blue plates, measuring 4' x 5'. The associated open cluster spans 2.7', contains 10 stars and has an integrated magnitude of 12.0. The cluster appears more like a star field concentration, and has a medium range in the brightness of the member stars.

Sulentic & Tifft (1973)

The RNGC (Sulentic and Tifft 1973) notes that this is a 11.5 mag cluster associated with nebulosity.

Lynds, B.T. (1962)

Lynds, B.T. (1962) Catalogue of dark nebulae. Astrophys.J.Suppl.Ser. 7, 1-52. [also: computer datafile: VII/7A]

Photo index

by Jim Lucyk: Vehrenberg's Atlas of Galactic Neb-2 p126.

Modern observations

Rajanen, Petteri (1992)

(Kauppi, Tampere, Finland) observing with a 8-inch f/5, writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: "Observed with a Lumicon Deep-Sky filter. The associated cluster is very poor but bright, the surrounding nebula being of rather high surface brightness. Brightest portion is on NE side, with sharp edges. Clearly seen without filter. Overall shape somewhat rectangular."

Tom Lorenzin

Lorenzin, in the e-version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "11.5M; Nebulosity surrounds four 10.5M stars; 5th star to NE = 12.5M; all 5 embedded in soft glow; two S-most aligned N-S; two N-most aligned WNW-ESE; nebulosity greatest around N-most, brighter pair; includes DIF NEB N7133; 20' NW of cluster N7142."

Brian Skiff

NGC 7129 & N7133

6cm - -29 seen as two dbl *s w/neb. brtst part of neb is around & N of Nrn pair. -33 is just NE, 1' diam, a faint splotch w/o *s.

15cm - consp neb oval elong E-W, 3'x2', overlying four *s in diamond, brtst is m8 on S. neb brtst nr vf * or knot on N side. a few other brtr *s in 15' area, hardly a cl. no neb around two *s NW of main grp. SW 15' is poor wkly concen cl of rel br *s. is there ID problem here in L&S, RNGC, etc? BS, 8Sep1991, Anderson Mesa.

25cm - nebulous cl w/four br *s & several fntr ones. neb around two cen *s, 4'x2'. fairly hisfcbr.

30cm - two pairs: Srn one in pa0, Nrn pair in pa110. neb is vbr around Ern member of Nrn pair & perhaps that * has f comp. neb mostly N of this pair w/two more *s inv, one vf. 2' irreg diam, bears magnification well. -33 is inv w/one * on its S side. 1' diam, fntr than -29.

Favourite lists

Lacaille's catalogue

The Messier objects

Dunlop's catalogue

The Bennett objects

The Caldwell list

Named DSOs

Object search

First search phrase

    and

Second search phrase

Type of object to include:

open cluster
globular cluster
planetary nebula
bright nebula
dark nebula
galaxy
galaxy cluster
asterism & stars
unverified/lost
nova

The Bug Report

DOCdb is still in beta-release.

Known issues, feature requests, and updates on bug fixes, are here:

> Bug Report

Feedback

Found a bug? Have a comment or suggestion to improve DOCdb? Please let us know!

> Contact us

Help!

DOCdb is a free online resource that exists to promote deep sky observing.

You could help by sharing your observations, writing an article, digitizing and proof-reading historical material, and more.

> Find out more

Everything on DOCdb.net is © 2004-2010 by Auke Slotegraaf, unless stated otherwise or if you can prove you have divine permission to use it. Before using material published here, please consult the Creative Commons Attribution-Non-Commercial-Share Alike 2.5 License. Some material on DOCdb is copyright the individual authors. If in doubt, don't reproduce. And that goes for having children, too. Please note that the recommended browser for DOCdb is Firefox 3.x. You may also get good results with K-Meleon. Good luck if you're using IE. A successful experience with other browsers, including Opera and Safari, may vary.