sponsored by psychohistorian.org


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.


log in to manage your observing lists























Full database:

Entire DOCdb database of 18,816 objects.



NGC 1535 (2,850 of 18,816)


oc gc pln bn dn gx gxcl ast aka lost




finder chart

altitude today

altitude (year)


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

Cleopatra's Eye

NGC 1535, HD 26847, PK 206-40 1, PN VV' 25, PN VV 19, PN G206.4-40.5, Bennett 22, Cleopatra's Eye, IV 26, h 2618, GC 826

RA: 04h 14m 15.76s
Dec: −12° 44′ 22″

Con: Eridanus
Ch: MSA:306, U2:268, SA:11


(reference key)

Type: planetary nebula

Mag: B=11.6, V=10.553

Size: ?
PA: ?

Image gallery

Sketches  (2)

Select a sketch and click the button to view

Photos  (1)

Select a photo and click the button to view


Modern catalogues give it a magnitude of 9.6 with a 18 arcsecond diameter. The Vorontsov-Velyaminov description classifies it as exhibiting ring structure. The central star is of magnitude 11.6.

Historical observations

William Herschel (c.1784)

Synonyms: H IV-026

William Herschel discovered it on February 1, 1785 with his newly completed 18.7-inch f/13 speculum telescope. He called it "a very bright, planetary nebula, about half a minute in diameter, but the edges are not very well defined. It is perfectly round, or perhaps a very little elliptical, and all over of an uniform brightness: with higher powers it becomes proportionally magnified." and also as "vB, perfectly round or very little elliptical. Planetary but ill defined disk. Second observation, resolvable on the borders, and is probably a very compressed cluster of stars at an immense distance."

John Herschel

It was also observed by John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "Bright; small; round; first pretty suddenly, then very gradually brighter in the middle; 20 arcsec across. A mottled disc, but so hazy at the borders that I have no doubt of its being a very distant and highly compressed globular cluster. It is not a planetary nebula, though a near approach to one: does not bear magnifying. A power of 320 is of no use. A very remarkable and interesting object."

Lassell, W. (1854)

Lassell, W. (1854) Observations of the nebula of Orion, made at Valletta, with the twenty-foot equatorial. Memoirs R.A.S., 23, 53-62.

Lassell, W. (1866)

Bibcode: [1866MmRAS..36....1L]

Sketched and described.

NGC/IC Dreyer (1888, 1895, 1908)

It is described in the NGC as "planetary nebula, very bright, small, round, pretty suddenly then very suddenly brighter in the middle, resolvable."

Webb, T.W. (1893)

In the 5th edition of Webb's Celestial Objects for Common Telescopes it is described as "planetary, bright and round, with low powers of 3.7-inch, but not bearing magnifying. Lassell has described it as the most interesting and extraordinary object of the kind he had ever seen; an 11th mag star standing in the centre of a circular nebula, itself placed centrally upon a larger and fainter circle of hazy light. D'Arrest did not see this, but thought nucleus excentric, edges resolvable, and colour light blue, as E. of Rosse, who makes nucleus granular. Huggins finds the spectrum though, like that of several other nebulae, deficient at the red end, not gaseous."

Burnham, S.W. (1894)

Burnham, S. W. () "Measures of planetary nebulae with the 36-inch equatorial of the Lick Observatory", Pub. Lick Obs., vol 2, p159-167. "Besides the central star, there are other fainter stars within the nebula .The most prominent of these is near the northern edge of the circular disc. ... This nebula is H IV.26 It has been drawn by d'Arrest and by Lassell (Memoirs RAS, vols 23 and 36). The 14.5mag star [PA 324° 16.17arcsec] does not seem to have been seen by these observers."

Stewart, D. (1908) Ann.Harv.Coll.Obs., 60 (6)

Table IV: Not seen, but poss. a pB, R, neb. spot at 10.0m, -12°47'.

Published comments

Helwan Obs. Bulletin No 21 (1920)

!! vB, pS, R, planetary. B central star surrounded by two slightly irregular rings, the inner one being much the denser. The appearance If gaseous 'shells', rather than rings, is caused by both rings being brighter on their outer edges, especially the inner ring.

Doig, P. (1925)

Doig, P. (1925) Notes on the nebulae and clusters in Webb's 'Celestial Objects for Common Telescopes' (Sixth edition, Vol.ii). Part I. M.N.R.A.S., 35(5), 159.

Sulentic & Tifft (1973)

The RNGC (Sulentic and Tifft 1973) notes that this is a planetary nebula.

Sanford (1989) Observing the Constellations

Sanford notes that it is "half an arcminute in diameter and of 9th magnitude, bluish in colour. An 11th magnitude central star is visible in larger instruments."

James, Andrew (1998+)

From: "Neat Southern Planetaries - VII."

NGC 1535 / HD 26847/ VV 19/ Herschel IV 26 / PK206-40.1 (04144-1245) (Eridanus) is the most northern planetary that we will discuss in this series. Positioned in an attractive field, this slightly ovoid planetary is easily visible in a 7.5cm., and as a 'star' even in the telescope finder! Sir William Herschel discovered this object in 1785, and placed in his object Class IV; "Stars with burs [Nebulous disks; bur(r)s is now archaic], with milky chevelure [French for 'hair'], with short rays, remarkable shapes, etc." To find it, I used the red 2.8 magnitude Gamma ( ) Eridani (03580-1330), some 4.0O SWW of the planetary. Simply move 18'min.arc. north and then 4.0O west to find the field. Within the field, using a medium magnification, to the south-east is an 2'min.arc. trapezium of 11.4 to 12.3 magnitude stars. At medium magnification in a 15cm. the oval becomes apparent, estimated to be along about position angle 145O. The image bears reasonable magnification, however, I saw little improvement to any visual features in the Celestron-8. Rev. Thomas Webb, in 'Celestial Objects for Common Telescopes' pg.127 states;

"Planetary bright with low power in 3.7" [9.4cm.] but not bearing magnification. [Lalande] has described it as the most interesting and extraordinary object he has ever seen... D'Arrest...thought [that the] nucleus excentric, edges resolvable, and colour light blue, as Earl of Rosse, who makes the nucleus granular."

I suspected a hint of mottling toward the centre, and an O-III did little to improve this. According to the "Webb Society Deep Sky Observer Handbook: Volume 2 - Planetary and Gaseous Nebulae." pg.58, a 42cm. (16.5") telescope will see;

"Blue irregularity round nebula; 351X star surrounded by dark mottling enclosed by a bright ring in slightly elongated shell."

To quote from the apt description of NGC 1535 in AOST2; "In an effective field of scattered stars this bright pale blue planetary nebula stands out conspicuously." or as Burnham's states "[A]..pale bluish disc..."

The photographic magnitude is stated as 9.6, while the visual magnitude is 10.55 and the 'B' magnitude is 11.6. Visually, it subtends an angle some 21.0"sec.arc. Some sources, like Sky Catalogue 2000.0 claims a size of 18"sec.arc. and 44"sec.arc., while Burnham's states 20"x17"sec.arc. Classed as '4+2c', to me this is a bit confusing - Ring structure, with a smooth disk and traces of ring structure. For a 25cm. or less this doesn't describe the object adequately. I could only assumed this meant a ring with a inner ring-like disk. If the Webb Society's description is correct, a 30cm. or 40cm. should be able to see this inner ring. Figure 3 shows an overexposed image of the nearby 5'min.arc. field. while insert shows the telescopic image using a 30cm.

The white dwarf PNN (HD 26847) is an O5 star of magnitude 12.1, but it is invisible for telescopes below 25cm. I am certain the star is particularly difficult to see in poor seeing because it merges into the planetary's nebulosity. Californian Jack Marling in an article in June's 1986 S&T (pg, 633) claims in a 50cm. (17.5"); "The 12th magnitude star is easy to see." David Frew also claims to have easily seen the PNN using a direct-vision prism, that reveals a stellar 'streak' within the planetary. I attempted this with a C8, and admit I could not see it, though others might have some better luck. Spectrally the white dwarf is stated as '?npe' - suspected nebulous lines and a peculiar spectra.

Radial Velocities were first measured in 1952, at a small 1.2kms-1. By 1993, the latest measure is about 3.2kms-1. The distance of 2.14 kiloparsecs was first proposed by Cahn and Kaler in 1971. More recent estimates suggest a closer 1.65 kiloparsecs.

A good 'honest to god' planetary!

Photo index

Photo Index by Jim Lucyk: Sky&Tel. 6/86 p632.

Terzian, Y. (1980)

Terzian Y (1980) Q.J. R.astr.Soc vol 21, p82-92 [09.16.1] notes that this planetary shows multiple shell structure.

Modern observations

Hartung, E.J. (1968) Astron.Obj.South.Tel

Hartung writes: "In an effective field of scattered stars this bright pale blue planetary nebula stands out conspicuously; it is about 30 arcsec across and well defined with fairly even light. No central star is visible..."

Walter Scott Houston

Houston notes that this 9th mag nebula lies in Eridanus. With a magnification of 100 on a 4-inch refractor, he did not need averted vision to see it.

Houston calls it a "bright planetary nebula .. which swims like a celestial jellyfish. Its 9th mag oval disk is about three-quarters arc minute long and surrounds a 12th mag central star."

Steve Coe

Steve Coe, observing with a 13" f/5.6, notes: "Bright, pretty large, round, easy to spot at 100X. Going to 180X shows two concentric rings, one bright near the center, the other ring dimmer and larger that forms the outer edge of this planetary. The central star is easy at high power and the nebula is light blue at all powers."

Steve Gottlieb

04 14.3 -12 44 17.5: very bright, fairly small, high surface brightness, mag 12.5 central star visible, blue color. This planetary has a double shell structure with inner shell slightly elongated and a faint rounder outer shell. Small dark gaps are visible around the central star.

13: at 360x the central star visible surrounded by two shells; a bright annular inner shell and a fainter outer halo.

8: bright, greenish, fairly small, round.

Ancient City Astron.Club (1980)

Listed by the Herschel Club, described as "small, circular, almost stellar, definite blue tint noticed. 6-inch, 40x."

Mullaney, J

Mullaney writes: "This is a small pale blue-green planetary in Eridanus .. shining at about 9th mag and measuring 44 arcseconds by 18 arcseconds, NGC 1535 has a faint central star and disk structure that can be glimpsed in an 8-inch or larger telescope."

Layton, Chuck (IAAC)

Observer: Chuck Layton Your skills: Intermediate (some years) Date/time of observation: 1 Feb 98 0330 UT Location of site: Roy, WA (Lat 47 N, Elev 200ft) Site classification: Suburban Sky darkness: 6 1-10 Scale (10 best) Seeing: 8 1-10 Scale (10 best) Moon presence: Minor - crescent or far from object Instrument: 8" f/6 Newtonian Eq. Magnification: 38X, 177X Filter(s): none Object(s): NGC 1535 Category: Planetary nebula Class: 4 + 2c Constellation: Eri Data: mag 9.4 size 20" x 17" Position: RA 04:14 DEC -12:44 Description:

Another relatively easy to locate planetary neb. Large enough at low power to differentiate from nearby stars. At high power the central star is hard to serperate from the small angular bight portion of nebulosity. Surrounding this central section was a "seperate", dimmer oval of gas, uniform in bightness, with a slight extention to the SW. This gave the appearance of a small bright nebula floating on top of a larger dimmer one. Interesting to observe.

Shortly after this observation the clouds closed in again. Living in the Pacific NW sure makes you appreciate ANY clear night sky!!!

Marling, J.B. (1986)

Marling, J.B. (1986) In pursuit of planetaries. Sky&Telescope, Jun, 631.

Medkeff, Jeff (IAAC)

Observer: Jeff Medkeff; Your skills: Advanced (many years); Date/time of observation: Oct 4, 1997; Location of site: Rockland Observatory, Sierra Vista, Arizona (Lat +31.5, Elev 4550 ft.); Site classification: Rural; Sky darkness: 6 Limiting magnitude; Seeing: 6 1-10 Seeing Scale (10 best); Moon presence: None - moon not in sky; Instrument: 4.5" f/7 Dob; Magnification: 32 53 68; Object(s): NGC 1535

NGC 1535 pn in Eridanus. Small. Very bright, takes magnification well. No hint of annular appearance. [I later learned that this pn is often called the "Strawberry Nebula", allegedly because of its strong red color. Subsequent observations do not show color with the 4.5".]

Clarke, W.P. (1992)

William P. Clarke (San Diego, California, USA) writes in The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: "A small round ghostly patch with a central star and blurred outer edge (21-inch f/20, x140)." In Report No. 11, January 1993, he writes: "The bright inner disc is easily visible and is about 20 arcseconds in diameter. The outer disc is hazy and gradually fades away; it is about twice the diameter of the inner disc. This shell structure is very much like that of NGC 2392. Contrast greatly improved with an OIII filter. (21-inch, x350)"

Gramer, Lew (IAAC)

Observer: Lew Gramer; Your skills: Intermediate (some years); Date/time of observation: 9/10 Feb 1999 04:00 UT; Location of site: MIT Haystack Obs., Westford, MA, USA (Lat 43N, Elev 30m); Site classification: Exurban; Sky darkness: 6.6 Limiting magnitude; Seeing: 4 1-10 Seeing Scale (10 best); Moon presence: None - moon not in sky; Instrument: 17.5" f/4.5 dob reflector; Magnification: 55x, 225x; Filter(s): None, OIII; Object(s): NGC 1535

Description: After Steve Clougherty & I finished setting up the ATMs of Boston 17.5" Club scope, we had to wait out a brief threat of cloud-over. As bands of cirrus and cirrocumulus obligingly dissolved or swept off to the S, we began this evening's observing in earnest. First target was the bright n1535 in Eri, easily found by sweeping ENE of gamma Eri just about exactly 4o, stopping just a wide field E of a beautiful equilateral trio of mag 9 late spectral-type stars.

At lowest power n1535 was distinctly non-stellar, with a yellowish coloring. Jumping immediately to 9mm (225x), the bright, seemingly smooth face of the nebula became more yellow-green, with a fairly obvious irregularity to the N, either the edge of a lobe of nebu- losity or perhaps a dark obstruction. Also, the face showed a non- symmetric flattening on the W, probably indicating more structure. The central star was neither strikingly obvious nor very difficult once looked for. Surprisingly, even without any filter there was a hint of a faint outer halo, or at least of much fainter nebulosity surrounding the central disk. This "second tier" of the nebula (if it was not in fact the actual halo) was only subtle, and was best seen to the ESE of the center. Finally, with the idea of enhancing this outer haze, we blinked the view at 225x with an OIII filter. Strangely, the central star was neither more nor less visible than it had been. But suddenly, the annular (ring-like) nature of n1535 became apparent, with just the suggestion of irregularities in the inner darkened area to averted vision. As expected, the outer halo could be clearly seen to SE, but now actually showed up as brighter and more elongated W of the disc, reaching out to perhaps twice the radius of the bright inner disk, roughly per cataloged sizes.

[amastro] NGC1535 in the 36"

Last night (11-10-99) I viewed NGC1535 with a 16", and was taking time to compare it with various photos and images (DSS, Doug Snyder's, Vickers). Not terribly impressive in the 16" and none of the images available made me salavate. However, I was feeling energetic, so I cranked up the 36" (suffering from truss sag...and therefor collimation) and used a 12mm Nagler.(that's 390X for those who can count). The following are excerps from my notes, partially readible between slobber spots:


I'm not sure at what aperture the transition takes place at, but NGC1535 takes on a whole different view in a 36".......the central star is bright and has a bluish tinge to it, with an inner circle distincly dark grey and with a very distinct circlular boundry. An outer shell surrounds the inner and presents a hint of copper copper. This, too, has its own boundry, but is subtley more diffuse and lighter than the inner shell. All the images that I had available to me, paled in comparison to the visual image. Obviously not true with most objects, but true in this case with what was available.

I would be interested in hearing from any members of the group that have instruments in the 20" - 30" size, as to their visual views relative to prints or digital images. I would guess that NGC1535 becomes a different animal somewhere in that aperture range. Neal


I just revisited this object, this time with my 25" f/5. The view in my 16" previously was good, but the 25" at 300x really displayed this object as quite knotty, with a very bright, blue central star. I selected it to view at the recent Virginia Association of Astronomical Societies meeting this past Saturday. Unfortunately I didn't get too much chance to study it as there was always a long line. A stunning planetary nebula, as is N1501 in Camelopardalis. To see is N1501 in a 25" at 1,000x is awesome. Planetaries are often forgiving of less-than-ideal seeing conditions. Put lots of power to them and enjoy. Kent Blackwell

Tom Lorenzin

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "9M; 20" diameter; 11.5M center star; distinct bluish discus!."

Brian Skiff

= PK206-40 1 = HD 26847 = BD-13 842

PK: three *s 2'.5 W.

6cm - vis as m9 * 20' E of equilateral triangle of *s on AE.

7cm - just discernable from a * @ 30x. 75x: circ spot that seems to have sharp center w/averted vis. no other details, too sm! BS, 26Nov1992, Anderson Mesa.

15cm - fairly br well-def ellipse w/distinctly *-like point at center. 20" long. good object. HM/BS, 15Oct1971, FtL.

- evenly br inner circle and incompl narrower outer shell. cen * perhaps. greenish. HM.

25cm - br & vlg. 180x: cen * seen. br well-def core 20" across w/fntr halo 35" across. creamy blue.

30cm - neat! elong pa10, 25"x18". has two distinct zones @ 220x: 12"x8" inner zone around sparkling cen *; br fuzzy halo fades pretty abruptly at its outer edge. 440x: inner `core' has definite br edge, and sfc of core is mottled w/holes. three m13.5-14.2 *s 1' W. one of the neater pn's. CBL.

Paul Alsing

82-inch at McDonald - Observing Report

[amastro] posting, Sat Nov 25, 2006

82" telescope, McDonald Observatory near Fort Davis, Texas, USA

f/13.7, 35mm Televue Panoptic (5' fov, 812x)

Bright dual-shelled PNe, both shells aqua in color. The bright inner shell has a ropey, intricate outer edge, while the dimmer outer shell is featureless and has a nice sharp outer edge. Bright central star. Very dramatic at this aperture.

Contemporary observations

Magda Streicher

(no date)

12-inch f/10 SCT (EP: 2-inch 32mm SW 95x 42' fov; 2-inch 14mm UW 218x 23' fov)

Small, bright and well defined round planetary nebula with a definite blue hue and sharp edges. The northern portion is well defined where as the southern side appears fuzzy. With higher magnification (218x) it appears cloudy at the edges. The central star can be seen with averted vision. This planetary is outstanding against the background stars. The two galaxies NGC 1538 & IC 2048 are situated 27' arc minutes to the south outside the field of view. Discovered by William Herschel in 1785. He stated that it is a remarkable and interesting object.

1997 July 4

Location: Pietersburg South 23o 53. East 29o 28.

Sky conditions: Clear.

Date: 4 Julie 1997.

Field of view: 52.7 arc minutes.

ASSA-DSO - Report J

NGC 1535 P/n Mag 10 size 42

Small, bright, well defined, round planetary nebula with a definite blue even colour, and sharp edges. Beautiful object.

Auke Slotegraaf

2007 April 15

Sutherland (Ouberg Quarry)

11x80 tripod mounted binoculars

Conditions: NELM: fainter than 6.0 at the S.pole

Appears stellar in binoculars, like a 9.5mag star.

Tom Bryant

2008-01-04 21:30:00

Observing site: Little Tycho Observatory

Telescope: C-8

[4h 14m 12s, -12° 44' 0"] A pastel blue planetary nebula, looking like an out of focus star in the 24.5. The sky was becoming cloudy, a clear sky might have shown more detail.

Richard Ford

2012 February 19, Sun


Instrument:12-Inch Dobsonian Reflector Telescope.


Sky Conditions:The fainter parts of the Milky Way are barely visible.

Transparency Of the Sky:Haziness only visible on the horizon.

Seeing:Atmosphere stable with little interference.

This planetary nebula is seen as a bluish oval disk at high magnification and is well defined.At low magnification this nebula looks like a fuzzy out of focus star.

It measures 1'*0.3'.

Challenge Rating:Difficult.

Carol Botha

2011 - 12 - 07

Location:Betty's Bay

Time: 21:50

Telescope: 12” Dobsonian – f4,9. Eyepiece 15mm. FOV- 36’

Sky conditions: Seeing 3/5 (intermittent high cloud cover)

Actual dimensions: 0.7' x 0.7'(Cartes Du Ciel)

Object description:

Planetary nebula in Eridanus

Very dim disk. Hazy bluish colour. With higher magnification seeing conditions did not reveal a central star .

Arc of dim stars just W of the nebula. Four stars in diamond shape to SW. a line of two bright , two dimmer stars to N. Four stars in kite formation to E

Now that I realize I’ve found the eye of Cleopatra I will have to set up a meeting in really dark skies with good seeing.

Favourite lists

Lacaille's catalogue

The Messier objects

Dunlop's catalogue

The Bennett objects

The Caldwell list

Named DSOs

Object search

First search phrase


Second search phrase

Type of object to include:

open cluster
globular cluster
planetary nebula
bright nebula
dark nebula
galaxy cluster
asterism & stars

The Bug Report

DOCdb is still in beta-release.

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

> Bug Report


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

> Contact us


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.