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 5068 (11,297 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

NGC 5068

NGC 5068, ESO 576-29, LEDA 46400, MCG-03-34-046, SGC 131613-2046.6, Bennett 59a, II 312, GC 3482

RA: 13h 18m 55.2s
Dec: −21° 02′ 21″

Con: Virgo
Ch: MSA:867, U2:330, SA:21

Ref: SIMBAD

(reference key)

Type: galaxy, Sd

Mag: B=10.53, V=9.9

Size: 7.079′ x 6.309′
PA: 110°

Historical observations

William Herschel (c.1784)

Synonyms: H II-312

Discovered in 1785 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it "F, L, iR, vgbM."

Published comments

Helwan Obs. Bulletin No 38 (1935)

F, 6'x3', E 30deg, irr.spiral with pF N 1' long, E, 150deg, undisticnt whirls and very many stell.condenastions and some absorptions.

de Vaucouleurs, G. (1975)

de Vaucouleurs, G. (1975) Nearby groups of galaxies. In: Kuiper, G. (ed) Stars and Stellar Systems. Volume 9: Galaxies and the Universe. Chapter 14, p557.

5. The nearer groups within 10 megaparsecs

G4. NGC 5128 Group

Brightest members: 5236,5128,4945,5102,5068,5253.

Several large southern galaxies having low velocities may form a loose group or chain centred on NGC 5128, 4945, 5102, 5236 and NGC 5253 and possibly NGC 5068. Two (NGC 5102 and perhaps NGC 5128=CenA) are lenticulars, three are late-type spirals Sc-Scd and one (NGC 5253) is peculiar, possibly an I0 irregular (the BGC classificaion Imp is incorrect). The overall length of the chain is 30° = 2.1Mpc or 20° = 1.4 Mpc (excluding NGC 5068 which has the highest velocity). ... Even if this chain does not form a physical (bound) group, it is useful to obtain some estimate of the distance of NGC 5128.

Sulentic & Tifft (1973)

The RNGC (Sulentic and Tifft 1973) notes that this is a 11.0 mag galaxy. Their coded description reads SBC,VDIF,BM TOBAR,PD KNOTTY.

Sandage & Tammann (1975)

Sandage, A. & Tammann, G. A. (1975) Steps toward the Hubble constant. V - The Hubble constant from nearby galaxies and the regularity of the local velocity field. ApJ, 196, 313-328. [1975ApJ...196..313S]

Sandage and Tammann (1975, Astrophysical Journal, 196, 313-328) includes this galaxy in the NGC 5128 Group. Members include NGC 4945, NGC 5068, NGC 5102, NGC 5128 & NGC 5236.

Schmidt, K.-H. et al. (1993)

Schmidt K.-H., Priebe A. & Boller T. (1993) Nearby galaxies. Revised machine-readable version of the catalogue. Astron. Nachr., 314, 371. [1993AN....314..371S]

Other names: "UA345,E576-29". Inclination: (face-on, in degrees) 22 Total photoelectric blue mag 10.7 Total colour index .67 Logarithm of the angular diameter D25 (arcminutes) 1.86 Blue photographic magnitude 10.39 This galaxy is included in a sample of galaxies with velocity less than 500km/s with respect to the centroid of the Local Group. [Nearby Galaxies. Schmidt K.-H., Priebe A., Boller T. (Astron. Nachr. 314, 371 (1993))]

Ryder & Dopita (1993)

Included in the CCD-atlas of Ryder S.D. & Dopita M.A. (1993) "An H-alpha Atlas of Nearby Southern Spiral Galaxies" Astrophys.J.Suppl. 88, 415. They note: "Here is yet another example of how lopsided the H II region distribution in late-type spirals can be, even those exhibiting well-organized spiral structure. A number of giant H II region complexes to the west are visible even in blue light photographs, but only two such objects are found in the eastern arms."

Modern observations

Tom Lorenzin

Tom Lorenzin, in the e-version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "11.6M; 6' x 5.5' extent; fairly large, faint, not quite round fuzz ball with brighter center; !good supernova prospect! EL GAL N5087 (12.4M; 50" x 30" extent) small, centerless fuzzy patch 30' to NE with 9M star 7' to NW."

Contemporary observations

Magda Streicher

1997 May 14

Location: Campsite Farm. (South 23 16 East 29 26)

Sky conditions: clear.

Instrument: Meade 8 inch (Super wide-angle 18mm eyepiece.

Date: 14 May 1979.

ASSA-DSO - Report H

This is a real faint, roundish structure with no hint of a core. Gaseous structure, like cottonwool. A few faint stars to the edge of the field.

This is a really faint, large roundish structure with a very dim small nucleus. Busy extended gaseous surroundings. A few faint stars to the edge of the field.

1997 June 06

Date: 7 6 1997

Real faint. Hint of core. Very hazy few faint stars to edge. Roundish, backround bare. Looks gasious.

(no date)

8-inch f/10 SCT (EP: 1.25-inch 26mm SP 77x 41' fov; 1.25-inch 18mm SW 111x 36' fov)

This is a really faint, large round puff of light, with a very soft small nucleus. Very hazy outer envelope can be detected with careful observation. Busy extended gaseous surroundings. Few stars surround this galaxy, which is situated in a bare star-field.

Richard Ford

2015, April, 19th

Location:Perdeberg.

Time:3:02am.

Sky Conditions:The fainter parts of the Milky Way are barely visible.Haziness only visible on the horizon.Atmosphere stable with little interference.

Instrument:12-inch Dobsonian.

This galaxy has a circular patch of faint light which looks like an out of focus mist in the dark and that the galactic nucleus of this galaxy is strongly condensed.Around the regions of this galaxy there are plenty of dark regions being noticed.This galaxy measures 9.1'x 7'.Chart No:464,NSOG,Vol.2.

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.